---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21017'
abstract:
- lang: eng
  text: With the growing interest in blockchains, permissioned approaches to consensus
    have received increasing attention. Unfortunately, the BFT consensus algorithms
    that are the backbone of most of these blockchains scale poorly and offer limited
    throughput. In fact, many state-of-the-art BFT consensus algorithms require a
    single leader process to receive and validate votes from a quorum of processes
    and then broadcast the result, which is inherently non-scalable. Recent approaches
    avoid this bottleneck by using dissemination/aggregation trees to propagate values
    and collect and validate votes. However, the use of trees increases the round
    latency, which limits the throughput for deeper trees. In this paper we propose
    Kauri, a BFT communication abstraction that sustains high throughput as the system
    size grows by leveraging a novel pipelining technique to perform scalable dissemination
    and aggregation on trees. Furthermore, when the number of faults is moderate (arguably
    the most common case in practice), our construction is able to recover from faults
    in an optimal number of reconfiguration steps. We implemented and experimentally
    evaluated Kauri with up to 800 processes. Our results show that Kauri outperforms
    the throughput of state-of-the-art permissioned blockchain protocols, by up to
    58x without compromising latency. Interestingly, in some cases, the parallelization
    provided by Kauri can also decrease the latency.
acknowledgement: We thank the ACM TOCS Editors and the reviewers for their help in
  improving the manuscript. This work was partially supported by CAPES - Brazil (Coordenação
  de Aperfeiçoamento de Pessoal de Nível Superior) and byFundação para a Ciência e
  Tecnologia (FCT) under project UIDB/50021/2020 and grant 2020.05270.BD, and via
  project COSMOS (via the OE with ref. PTDC/EEI-COM/29271/2017, via the łPrograma
  Operacional Regional de Lisboa na sua componente FEDER” with ref. Lisboa-01-0145-FEDER-029271)
  and project Angainor with reference LISBOA-01-0145-FEDER-031456, grant agreement
  number 952226, and project GLOG, with reference LISBOA2030-FEDER-00771200, and project
  BIG (Enhancing the research and innovation potential of Tecnico through blockchain
  technologies and design Innovation for social Good), and project ScalableCosmosConsensus,
  and the Austrian Science Fund (FWF) SFB project SpyCoDe F8502 and the Vienna Science
  and Technology Fund (WWTF) project SCALE2 CT22-045
article_number: '3769423'
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Ray
  full_name: Neiheiser, Ray
  id: f09651b9-fec0-11ec-b5d8-934aff0e52a4
  last_name: Neiheiser
  orcid: 0000-0001-7227-8309
- first_name: Miguel
  full_name: Matos, Miguel
  last_name: Matos
- first_name: Luis
  full_name: Rodrigues, Luis
  last_name: Rodrigues
citation:
  ama: 'Neiheiser R, Matos M, Rodrigues L. Kauri: BFT consensus with pipelined tree-based
    dissemination and aggregation. <i>ACM Transactions on Computer Systems</i>. 2025.
    doi:<a href="https://doi.org/10.1145/3769423">10.1145/3769423</a>'
  apa: 'Neiheiser, R., Matos, M., &#38; Rodrigues, L. (2025). Kauri: BFT consensus
    with pipelined tree-based dissemination and aggregation. <i>ACM Transactions on
    Computer Systems</i>. Association for Computing Machinery. <a href="https://doi.org/10.1145/3769423">https://doi.org/10.1145/3769423</a>'
  chicago: 'Neiheiser, Ray, Miguel Matos, and Luis Rodrigues. “Kauri: BFT Consensus
    with Pipelined Tree-Based Dissemination and Aggregation.” <i>ACM Transactions
    on Computer Systems</i>. Association for Computing Machinery, 2025. <a href="https://doi.org/10.1145/3769423">https://doi.org/10.1145/3769423</a>.'
  ieee: 'R. Neiheiser, M. Matos, and L. Rodrigues, “Kauri: BFT consensus with pipelined
    tree-based dissemination and aggregation,” <i>ACM Transactions on Computer Systems</i>.
    Association for Computing Machinery, 2025.'
  ista: 'Neiheiser R, Matos M, Rodrigues L. 2025. Kauri: BFT consensus with pipelined
    tree-based dissemination and aggregation. ACM Transactions on Computer Systems.,
    3769423.'
  mla: 'Neiheiser, Ray, et al. “Kauri: BFT Consensus with Pipelined Tree-Based Dissemination
    and Aggregation.” <i>ACM Transactions on Computer Systems</i>, 3769423, Association
    for Computing Machinery, 2025, doi:<a href="https://doi.org/10.1145/3769423">10.1145/3769423</a>.'
  short: R. Neiheiser, M. Matos, L. Rodrigues, ACM Transactions on Computer Systems
    (2025).
corr_author: '1'
date_created: 2026-01-20T10:14:23Z
date_published: 2025-09-05T00:00:00Z
date_updated: 2026-06-18T18:28:26Z
day: '05'
ddc:
- '000'
department:
- _id: KrPi
doi: 10.1145/3769423
has_accepted_license: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1145/3769423
month: '09'
oa: 1
oa_version: Published Version
project:
- _id: 34a1b658-11ca-11ed-8bc3-c75229f0241e
  grant_number: F8502
  name: Interface Theory for Security and Privacy
- _id: 7bdd2f70-9f16-11ee-852c-b7950bc6d277
  grant_number: ICT22-045
  name: SeCure, privAte, and interoperabLe layEr 2
publication: ACM Transactions on Computer Systems
publication_identifier:
  eissn:
  - 1557-7333
  issn:
  - 0734-2071
publication_status: epub_ahead
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Kauri: BFT consensus with pipelined tree-based dissemination and aggregation'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '21020'
abstract:
- lang: eng
  text: "Runtime verification offers scalable solutions to improve the safety and
    reliability of systems. However, systems that require verification or monitoring
    by a third party to ensure compliance with a specification might contain sensitive
    information, causing privacy concerns when usual runtime verification approaches
    are used. Privacy is compromised if protected information about the system, or
    sensitive data that is processed by the system, is revealed. In addition, revealing
    the specification being monitored may undermine the essence of third-party verification.\r\nIn
    this work, we propose two novel protocols for the privacy-preserving runtime verification
    of systems against formal sequential specifications. In our first protocol, the
    monitor verifies whether the system satisfies the specification without learning
    anything else, though both parties are aware of the specification. Our second
    protocol ensures that the system remains oblivious to the monitored specification,
    while the monitor learns only whether the system satisfies the specification and
    nothing more. Our protocols adapt and improve existing techniques used in cryptography,
    and more specifically, multi-party computation.\r\nThe sequential specification
    defines the observation step of the monitor, whose granularity depends on the
    situation (e.g., banks may be monitored on a daily basis). Our protocols exchange
    a single message per observation step, after an initialisation phase. This design
    minimises communication overhead, enabling relatively lightweight privacy-preserving
    monitoring. We implement our approach for monitoring specifications described
    by register automata and evaluate it experimentally."
acknowledgement: This work is a part of projects VAMOS that has received fund-ing
  from the European Research Council (ERC), grant agreementNo 101020093 and the Austrian
  Science Fund (FWF) SFB projectSpyCoDe F8502.We thank anonymous reviewers for pointing
  us to related work [ 3] and for their valuable suggestions that improved this paper.
article_processing_charge: Yes (via OA deal)
arxiv: 1
author:
- first_name: Thomas A
  full_name: Henzinger, Thomas A
  id: 40876CD8-F248-11E8-B48F-1D18A9856A87
  last_name: Henzinger
  orcid: 0000-0002-2985-7724
- first_name: Mahyar
  full_name: Karimi, Mahyar
  id: 6e5417ba-5355-11ee-ae5a-94c2e510b26b
  last_name: Karimi
  orcid: 0009-0005-0820-1696
- first_name: K. S.
  full_name: Thejaswini, K. S.
  id: 3807fb92-fdc1-11ee-bb4a-b4d8a431c753
  last_name: Thejaswini
citation:
  ama: 'Henzinger TA, Karimi M, Thejaswini KS. Privacy-preserving runtime verification.
    In: <i>Proceedings of the 2025 ACM SIGSAC Conference on Computer and Communications
    Security</i>. Association for Computing Machinery; 2025:2774-2787. doi:<a href="https://doi.org/10.1145/3719027.3765137">10.1145/3719027.3765137</a>'
  apa: 'Henzinger, T. A., Karimi, M., &#38; Thejaswini, K. S. (2025). Privacy-preserving
    runtime verification. In <i>Proceedings of the 2025 ACM SIGSAC Conference on Computer
    and Communications Security</i> (pp. 2774–2787). Taipei, Taiwan: Association for
    Computing Machinery. <a href="https://doi.org/10.1145/3719027.3765137">https://doi.org/10.1145/3719027.3765137</a>'
  chicago: Henzinger, Thomas A, Mahyar Karimi, and K. S. Thejaswini. “Privacy-Preserving
    Runtime Verification.” In <i>Proceedings of the 2025 ACM SIGSAC Conference on
    Computer and Communications Security</i>, 2774–87. Association for Computing Machinery,
    2025. <a href="https://doi.org/10.1145/3719027.3765137">https://doi.org/10.1145/3719027.3765137</a>.
  ieee: T. A. Henzinger, M. Karimi, and K. S. Thejaswini, “Privacy-preserving runtime
    verification,” in <i>Proceedings of the 2025 ACM SIGSAC Conference on Computer
    and Communications Security</i>, Taipei, Taiwan, 2025, pp. 2774–2787.
  ista: 'Henzinger TA, Karimi M, Thejaswini KS. 2025. Privacy-preserving runtime verification.
    Proceedings of the 2025 ACM SIGSAC Conference on Computer and Communications Security.
    CCS: Conference on Computer and Communications Security, 2774–2787.'
  mla: Henzinger, Thomas A., et al. “Privacy-Preserving Runtime Verification.” <i>Proceedings
    of the 2025 ACM SIGSAC Conference on Computer and Communications Security</i>,
    Association for Computing Machinery, 2025, pp. 2774–87, doi:<a href="https://doi.org/10.1145/3719027.3765137">10.1145/3719027.3765137</a>.
  short: T.A. Henzinger, M. Karimi, K.S. Thejaswini, in:, Proceedings of the 2025
    ACM SIGSAC Conference on Computer and Communications Security, Association for
    Computing Machinery, 2025, pp. 2774–2787.
conference:
  end_date: 2025-10-17
  location: Taipei, Taiwan
  name: 'CCS: Conference on Computer and Communications Security'
  start_date: 2025-10-13
corr_author: '1'
date_created: 2026-01-20T10:17:10Z
date_published: 2025-11-22T00:00:00Z
date_updated: 2026-03-13T13:37:19Z
day: '22'
ddc:
- '000'
department:
- _id: ToHe
- _id: GradSch
doi: 10.1145/3719027.3765137
ec_funded: 1
external_id:
  arxiv:
  - '2505.09276'
file:
- access_level: open_access
  checksum: 615ffddab6c7285158c2953acec6fa6f
  content_type: application/pdf
  creator: dernst
  date_created: 2026-01-21T07:34:58Z
  date_updated: 2026-01-21T07:34:58Z
  file_id: '21024'
  file_name: 2025_CCS_HenzingerT.pdf
  file_size: 1241912
  relation: main_file
  success: 1
file_date_updated: 2026-01-21T07:34:58Z
has_accepted_license: '1'
language:
- iso: eng
month: '11'
oa: 1
oa_version: Published Version
page: 2774-2787
project:
- _id: 62781420-2b32-11ec-9570-8d9b63373d4d
  call_identifier: H2020
  grant_number: '101020093'
  name: Vigilant Algorithmic Monitoring of Software
- _id: 34a1b658-11ca-11ed-8bc3-c75229f0241e
  grant_number: F8502
  name: Interface Theory for Security and Privacy
publication: Proceedings of the 2025 ACM SIGSAC Conference on Computer and Communications
  Security
publication_identifier:
  isbn:
  - '9798400715259'
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
related_material:
  record:
  - id: '21401'
    relation: dissertation_contains
    status: public
scopus_import: '1'
status: public
title: Privacy-preserving runtime verification
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '21049'
abstract:
- lang: eng
  text: 'Post-hoc importance attribution methods are a popular tool for “explaining”
    Deep Neural Networks (DNNs) and are inherently based on the assumption that the
    explanations can be applied independently of how the models were trained. Contrarily,
    in this work we bring forward empirical evidence that challenges this very notion.
    Surprisingly, we discover a strong dependency on and demonstrate that the training
    details of a pre-trained model’s classification layer (<10% of model parameters)
    play a crucial role, much more than the pre-training scheme itself. This is of
    high practical relevance: (1) as techniques for pre-training models are becoming
    increasingly diverse, understanding the interplay between these techniques and
    attribution methods is critical; (2) it sheds light on an important yet overlooked
    assumption of post-hoc attribution methods which can drastically impact model
    explanations and how they are interpreted eventually. With this finding we also
    present simple yet effective adjustments to the classification layers, that can
    significantly enhance the quality of model explanations. We validate our findings
    across several visual pre-training frameworks (fully-supervised, self-supervised,
    contrastive vision-language training) and analyse how they impact explanations
    for a wide range of attribution methods on a diverse set of evaluation metrics.'
acknowledgement: "We sincerely thank Sukrut Rao and Yue Fan for their valuable feedback
  on the paper and insightful discussions throughout the project. Additionally, we
  appreciate Sukrut’s help\r\nwith some LATEX sorcery. This work was partially supported
  by ELSA Mobility Program1\r\nas part of the ELLIS2 exchange program to the Institute
  of Science and Technology Austria (ISTA), where a portion of this research was conducted."
article_processing_charge: No
arxiv: 1
author:
- first_name: Siddhartha
  full_name: Gairola, Siddhartha
  id: fb21489d-057c-11f1-b1b6-d68cd6ae64f5
  last_name: Gairola
- first_name: Moritz
  full_name: Böhle, Moritz
  last_name: Böhle
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
- first_name: Bernt
  full_name: Schiele, Bernt
  last_name: Schiele
citation:
  ama: 'Gairola S, Böhle M, Locatello F, Schiele B. How to probe: Simple yet effective
    techniques for improving post-hoc explanations. In: <i>13th International Conference
    on Learning Representations</i>. ICLR; 2025.'
  apa: 'Gairola, S., Böhle, M., Locatello, F., &#38; Schiele, B. (2025). How to probe:
    Simple yet effective techniques for improving post-hoc explanations. In <i>13th
    International Conference on Learning Representations</i>. Singapore: ICLR.'
  chicago: 'Gairola, Siddhartha, Moritz Böhle, Francesco Locatello, and Bernt Schiele.
    “How to Probe: Simple yet Effective Techniques for Improving Post-Hoc Explanations.”
    In <i>13th International Conference on Learning Representations</i>. ICLR, 2025.'
  ieee: 'S. Gairola, M. Böhle, F. Locatello, and B. Schiele, “How to probe: Simple
    yet effective techniques for improving post-hoc explanations,” in <i>13th International
    Conference on Learning Representations</i>, Singapore, 2025.'
  ista: 'Gairola S, Böhle M, Locatello F, Schiele B. 2025. How to probe: Simple yet
    effective techniques for improving post-hoc explanations. 13th International Conference
    on Learning Representations. ICLR: International Conference on Learning Representations.'
  mla: 'Gairola, Siddhartha, et al. “How to Probe: Simple yet Effective Techniques
    for Improving Post-Hoc Explanations.” <i>13th International Conference on Learning
    Representations</i>, ICLR, 2025.'
  short: S. Gairola, M. Böhle, F. Locatello, B. Schiele, in:, 13th International Conference
    on Learning Representations, ICLR, 2025.
conference:
  end_date: 2025-04-28
  location: Singapore
  name: 'ICLR: International Conference on Learning Representations'
  start_date: 2025-04-24
corr_author: '1'
date_created: 2026-01-27T12:48:35Z
date_published: 2025-01-22T00:00:00Z
date_updated: 2026-02-09T06:11:17Z
day: '22'
ddc:
- '000'
department:
- _id: FrLo
external_id:
  arxiv:
  - '2503.00641'
file:
- access_level: open_access
  checksum: 6c8dfe4291c41d5a2c2fd838105e10b9
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-09T06:06:14Z
  date_updated: 2026-02-09T06:06:14Z
  file_id: '21162'
  file_name: 2025_ICLR_Gairola.pdf
  file_size: 24386863
  relation: main_file
  success: 1
file_date_updated: 2026-02-09T06:06:14Z
has_accepted_license: '1'
language:
- iso: eng
month: '01'
oa: 1
oa_version: Published Version
publication: 13th International Conference on Learning Representations
publication_status: published
publisher: ICLR
quality_controlled: '1'
related_material:
  link:
  - relation: software
    url: https://github.com/sidgairo18/how-to-probe
status: public
title: 'How to probe: Simple yet effective techniques for improving post-hoc explanations'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: repository
_id: '21050'
abstract:
- lang: eng
  text: "In 1873, James C. Maxwell conjectured that the electric field generated by
    $n$ point charges in generic position has at most $(n-1)^2$ isolated zeroes. The
    first (non-optimal) upper bound was only obtained in 2007 by Gabrielov, Novikov
    and Shapiro, who also posed two additional interesting conjectures.\r\n In this
    article, we give the best upper bound known to date on the number of zeroes of
    the electric field, and construct a counterexample to a conjecture of Gabrielov,
    Novikov and Shapiro that the number of equilibria cannot exceed those of the distance
    function defined by the unit point charges.\r\n Finally, we note that it is quite
    possible that Maxwell's quadratic upper bound is not tight, so it is prudent to
    find smaller bounds. Hence, we also explore examples and construct configurations
    of charges achieving the highest ratios of the number of electric field zeroes
    by point charges found to this day."
article_processing_charge: No
arxiv: 1
author:
- first_name: Herbert
  full_name: Edelsbrunner, Herbert
  id: 3FB178DA-F248-11E8-B48F-1D18A9856A87
  last_name: Edelsbrunner
  orcid: 0000-0002-9823-6833
- first_name: Christopher D
  full_name: Fillmore, Christopher D
  id: 35638A5C-AAC7-11E9-B0BF-5503E6697425
  last_name: Fillmore
- first_name: Gonçalo
  full_name: Olivera, Gonçalo
  last_name: Olivera
citation:
  ama: Edelsbrunner H, Fillmore CD, Olivera G. Counting equilibria of the electrostatic
    potential. <i>arXiv</i>. doi:<a href="https://doi.org/10.48550/ARXIV.2501.05315">10.48550/ARXIV.2501.05315</a>
  apa: Edelsbrunner, H., Fillmore, C. D., &#38; Olivera, G. (n.d.). Counting equilibria
    of the electrostatic potential. <i>arXiv</i>. <a href="https://doi.org/10.48550/ARXIV.2501.05315">https://doi.org/10.48550/ARXIV.2501.05315</a>
  chicago: Edelsbrunner, Herbert, Christopher D Fillmore, and Gonçalo Olivera. “Counting
    Equilibria of the Electrostatic Potential.” <i>ArXiv</i>, n.d. <a href="https://doi.org/10.48550/ARXIV.2501.05315">https://doi.org/10.48550/ARXIV.2501.05315</a>.
  ieee: H. Edelsbrunner, C. D. Fillmore, and G. Olivera, “Counting equilibria of the
    electrostatic potential,” <i>arXiv</i>. .
  ista: Edelsbrunner H, Fillmore CD, Olivera G. Counting equilibria of the electrostatic
    potential. arXiv, <a href="https://doi.org/10.48550/ARXIV.2501.05315">10.48550/ARXIV.2501.05315</a>.
  mla: Edelsbrunner, Herbert, et al. “Counting Equilibria of the Electrostatic Potential.”
    <i>ArXiv</i>, doi:<a href="https://doi.org/10.48550/ARXIV.2501.05315">10.48550/ARXIV.2501.05315</a>.
  short: H. Edelsbrunner, C.D. Fillmore, G. Olivera, ArXiv (n.d.).
corr_author: '1'
date_created: 2026-01-27T14:29:27Z
date_published: 2025-03-20T00:00:00Z
date_updated: 2026-06-02T09:24:17Z
day: '20'
department:
- _id: HeEd
doi: 10.48550/ARXIV.2501.05315
external_id:
  arxiv:
  - '2501.05315'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2501.05315
month: '03'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: draft
related_material:
  record:
  - id: '21021'
    relation: dissertation_contains
    status: public
  - id: '21931'
    relation: later_version
    status: public
status: public
title: Counting equilibria of the electrostatic potential
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: preprint
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21052'
abstract:
- lang: eng
  text: "Program logics have proven a successful strategy for verification of complex
    programs. By providing local reasoning and means of abstraction and composition,
    they allow reasoning principles for individual components of a program to be combined
    to prove guarantees about a whole program. Crucially, these components and their
    proofs can be reused. However, this reuse is only available once the program logic
    has been defined. It is a frustrating fact of the status quo that whoever defines
    a new program logic must establish every part, both semantics and proof rules,
    from scratch. In spite of programming languages and program logics typically sharing
    many core features, reuse is generally not available across languages. Even inside
    one language, if the same underlying operation appears in multiple language primitives,
    reuse is typically not possible when establishing proof rules for the program
    logic.\r\nTo enable reuse across and inside languages when defining complex program
    logics (and proving them sound), we serve program logics à la carte by combining
    program logic fragments for the various effects of the language. Among other language
    features, the menu includes shared state, concurrency, and non-determinism as
    reusable, composable blocks that can be combined to define a program logic modularly.
    Our theory builds on ITrees as a framework to express language semantics and Iris
    as the underlying separation logic; the work has been mechanized in the Coq proof
    assistant."
article_processing_charge: No
article_type: original
author:
- first_name: Max
  full_name: Vistrup, Max
  last_name: Vistrup
- first_name: Michael Joachim
  full_name: Sammler, Michael Joachim
  id: 510d3901-2a03-11ee-914d-d9ae9011f0a7
  last_name: Sammler
- first_name: Ralf
  full_name: Jung, Ralf
  last_name: Jung
citation:
  ama: Vistrup M, Sammler MJ, Jung R. Program logics à la Carte. <i>Proceedings of
    the ACM on Programming Languages</i>. 2025;9(POPL):300-331. doi:<a href="https://doi.org/10.1145/3704847">10.1145/3704847</a>
  apa: Vistrup, M., Sammler, M. J., &#38; Jung, R. (2025). Program logics à la Carte.
    <i>Proceedings of the ACM on Programming Languages</i>. Association for Computing
    Machinery. <a href="https://doi.org/10.1145/3704847">https://doi.org/10.1145/3704847</a>
  chicago: Vistrup, Max, Michael Joachim Sammler, and Ralf Jung. “Program Logics à
    La Carte.” <i>Proceedings of the ACM on Programming Languages</i>. Association
    for Computing Machinery, 2025. <a href="https://doi.org/10.1145/3704847">https://doi.org/10.1145/3704847</a>.
  ieee: M. Vistrup, M. J. Sammler, and R. Jung, “Program logics à la Carte,” <i>Proceedings
    of the ACM on Programming Languages</i>, vol. 9, no. POPL. Association for Computing
    Machinery, pp. 300–331, 2025.
  ista: Vistrup M, Sammler MJ, Jung R. 2025. Program logics à la Carte. Proceedings
    of the ACM on Programming Languages. 9(POPL), 300–331.
  mla: Vistrup, Max, et al. “Program Logics à La Carte.” <i>Proceedings of the ACM
    on Programming Languages</i>, vol. 9, no. POPL, Association for Computing Machinery,
    2025, pp. 300–31, doi:<a href="https://doi.org/10.1145/3704847">10.1145/3704847</a>.
  short: M. Vistrup, M.J. Sammler, R. Jung, Proceedings of the ACM on Programming
    Languages 9 (2025) 300–331.
date_created: 2026-01-28T06:35:47Z
date_published: 2025-01-09T00:00:00Z
date_updated: 2026-02-09T06:19:36Z
day: '09'
doi: 10.1145/3704847
extern: '1'
has_accepted_license: '1'
intvolume: '         9'
issue: POPL
language:
- iso: eng
main_file_link:
- open_access: '1'
month: '01'
oa: 1
oa_version: Published Version
page: 300-331
publication: Proceedings of the ACM on Programming Languages
publication_identifier:
  issn:
  - 2475-1421
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: Program logics à la Carte
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 9
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21053'
abstract:
- lang: eng
  text: "Program verification tools are often implemented as front-end translations
    of an input program into an intermediate verification language (IVL) such as Boogie,
    GIL, Viper, or Why3. The resulting IVL program is then verified using an existing
    back-end verifier. A soundness proof for such a translational verifier needs to
    relate the input program and verification logic to the semantics of the IVL, which
    in turn needs to be connected with the verification logic implemented in the back-end
    verifiers. Performing such proofs is challenging due to the large semantic gap
    between the input and output programs and logics, especially for complex verification
    logics such as separation logic.\r\nThis paper presents a formal framework for
    reasoning about translational separation logic verifiers. At its center is a generic
    core IVL that captures the essence of different separation logics. We define its
    operational semantics and formally connect it to two different back-end verifiers,
    which use symbolic execution and verification condition generation, resp. Crucially,
    this semantics uses angelic non-determinism to enable the application of different
    proof search algorithms and heuristics in the back-end verifiers. An axiomatic
    semantics for the core IVL simplifies reasoning about the front-end translation
    by performing essential proof steps once and for all in the equivalence proof
    with the operational semantics rather than for each concrete front-end translation.\r\nWe
    illustrate the usefulness of our formal framework by instantiating our core IVL
    with elements of Viper and connecting it to two Viper back-ends as well as a front-end
    for concurrent separation logic. All our technical results have been formalized
    in Isabelle/HOL, including the core IVL and its semantics, the semantics of two
    back-ends for a subset of Viper, and all proofs."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Thibault
  full_name: Dardinier, Thibault
  last_name: Dardinier
- first_name: Michael Joachim
  full_name: Sammler, Michael Joachim
  id: 510d3901-2a03-11ee-914d-d9ae9011f0a7
  last_name: Sammler
- first_name: Gaurav
  full_name: Parthasarathy, Gaurav
  last_name: Parthasarathy
- first_name: Alexander J.
  full_name: Summers, Alexander J.
  last_name: Summers
- first_name: Peter
  full_name: Müller, Peter
  last_name: Müller
citation:
  ama: Dardinier T, Sammler MJ, Parthasarathy G, Summers AJ, Müller P. Formal foundations
    for translational separation logic verifiers. <i>Proceedings of the ACM on Programming
    Languages</i>. 2025;9(POPL):569-599. doi:<a href="https://doi.org/10.1145/3704856">10.1145/3704856</a>
  apa: Dardinier, T., Sammler, M. J., Parthasarathy, G., Summers, A. J., &#38; Müller,
    P. (2025). Formal foundations for translational separation logic verifiers. <i>Proceedings
    of the ACM on Programming Languages</i>. Association for Computing Machinery.
    <a href="https://doi.org/10.1145/3704856">https://doi.org/10.1145/3704856</a>
  chicago: Dardinier, Thibault, Michael Joachim Sammler, Gaurav Parthasarathy, Alexander
    J. Summers, and Peter Müller. “Formal Foundations for Translational Separation
    Logic Verifiers.” <i>Proceedings of the ACM on Programming Languages</i>. Association
    for Computing Machinery, 2025. <a href="https://doi.org/10.1145/3704856">https://doi.org/10.1145/3704856</a>.
  ieee: T. Dardinier, M. J. Sammler, G. Parthasarathy, A. J. Summers, and P. Müller,
    “Formal foundations for translational separation logic verifiers,” <i>Proceedings
    of the ACM on Programming Languages</i>, vol. 9, no. POPL. Association for Computing
    Machinery, pp. 569–599, 2025.
  ista: Dardinier T, Sammler MJ, Parthasarathy G, Summers AJ, Müller P. 2025. Formal
    foundations for translational separation logic verifiers. Proceedings of the ACM
    on Programming Languages. 9(POPL), 569–599.
  mla: Dardinier, Thibault, et al. “Formal Foundations for Translational Separation
    Logic Verifiers.” <i>Proceedings of the ACM on Programming Languages</i>, vol.
    9, no. POPL, Association for Computing Machinery, 2025, pp. 569–99, doi:<a href="https://doi.org/10.1145/3704856">10.1145/3704856</a>.
  short: T. Dardinier, M.J. Sammler, G. Parthasarathy, A.J. Summers, P. Müller, Proceedings
    of the ACM on Programming Languages 9 (2025) 569–599.
date_created: 2026-01-28T06:36:57Z
date_published: 2025-01-09T00:00:00Z
date_updated: 2026-02-09T06:25:01Z
day: '09'
ddc:
- '000'
doi: 10.1145/3704856
extern: '1'
external_id:
  arxiv:
  - '2407.20002'
has_accepted_license: '1'
intvolume: '         9'
issue: POPL
language:
- iso: eng
month: '01'
oa_version: Published Version
page: 569-599
publication: Proceedings of the ACM on Programming Languages
publication_identifier:
  issn:
  - 2475-1421
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
status: public
title: Formal foundations for translational separation logic verifiers
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 9
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21057'
abstract:
- lang: eng
  text: Among the most puzzling early discoveries of JWST are “little red dots” (LRDs),
    compact red sources that host broad Balmer emission lines, and in many cases exhibit
    a “V-shaped” change in slope in the rest-optical. The physical properties of LRDs
    currently have order-of-magnitude uncertainties, because models to explain the
    continuum of these sources differ immensely. Here, we leverage the complete selection
    of red sources in the RUBIES program, supplemented with public PRISM spectra,
    to study the origin of this V shape. By fitting a broken power law with a flexible
    inflection point, we find that a large fraction of red Hα emitters at 2 < z <
    6 exhibit a strong change in slope, and that all strong inflections appear associated
    with the Balmer limit (0.3645 μm). Using a simple model of a reddened active galactic
    nucleus (AGN) with an unobscured scattered-light component, we demonstrate that
    the observed V shape in LRDs is unlikely to occur at any specific wavelength if
    the entire continuum is dominated by light from a power-law AGN continuum. In
    contrast, models with an intrinsic feature at the Balmer limit, such as those
    that are dominated by an evolved stellar population, can produce the observed
    spectral shapes, provided that a reddened component picks up sufficiently redward
    of the break. While no model can comfortably explain the full LRD spectral energy
    distribution, the common inflection location suggests that a single component
    consistently dominates the rest-frame UV optical in LRDs, and that this component
    is associated with T ∼ 10^4 K hydrogen.
acknowledgement: "This work is based in part on observations made with the NASA/ESA/CSA
  James Webb Space Telescope. The data were obtained from the Mikulski Archive for
  Space Telescopes at the Space Telescope Science Institute, which is operated by
  the Association of Universities for Research in Astronomy, Inc., under NASA contract
  NAS 5-03127 for JWST. The specific observations analyzed can be accessed via DOI:
  10.17909/0esg-h949. All of the data products presented herein were retrieved from
  the Dawn JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center, which
  is funded by the Danish National Research Foundation under grant No. 140. We express
  gratitude toward the members of the GTO, GO, and DDT teams, whose public data we
  utilized in this work.\r\n\r\nSupport for this work was provided by The Brinson
  Foundation through a Brinson Prize Fellowship grant. Support for program No. 4233
  was provided by NASA through a grant from the Space Telescope Science Institute,
  which is operated by the Association of Universities for Research in Astronomy,
  Inc., under NASA contract NAS 5-03127. This research was supported by the International
  Space Science Institute (ISSI) in Bern, through ISSI International Team project
  No. 562. D.S. acknowledges helpful conversations with Xiaohui Fan and Jared Siegel
  that contributed to the quality of this work, in addition to aesthetic sign-off
  from Stephanie Permut on the colors of figures. T.B.M. was supported by a CIERA
  fellowship. The work of CCW is supported by NOIRLab, which is managed by the Association
  of Universities for Research in Astronomy (AURA) under a cooperative agreement with
  the National Science Foundation."
article_number: '118'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: David J.
  full_name: Setton, David J.
  last_name: Setton
- first_name: Jenny E.
  full_name: Greene, Jenny E.
  last_name: Greene
- first_name: Anna
  full_name: de Graaff, Anna
  last_name: de Graaff
- first_name: Yilun 逸伦
  full_name: Ma, Yilun 逸伦
  last_name: Ma
- first_name: Joel
  full_name: Leja, Joel
  last_name: Leja
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: Rachel
  full_name: Bezanson, Rachel
  last_name: Bezanson
- first_name: Leindert A.
  full_name: Boogaard, Leindert A.
  last_name: Boogaard
- first_name: Nikko J.
  full_name: Cleri, Nikko J.
  last_name: Cleri
- first_name: Harley
  full_name: Katz, Harley
  last_name: Katz
- first_name: Ivo
  full_name: Labbe, Ivo
  last_name: Labbe
- first_name: Michael V.
  full_name: Maseda, Michael V.
  last_name: Maseda
- first_name: Ian
  full_name: McConachie, Ian
  last_name: McConachie
- first_name: Tim B.
  full_name: Miller, Tim B.
  last_name: Miller
- first_name: Sedona H.
  full_name: Price, Sedona H.
  last_name: Price
- first_name: Katherine A.
  full_name: Suess, Katherine A.
  last_name: Suess
- first_name: Pieter
  full_name: van Dokkum, Pieter
  last_name: van Dokkum
- first_name: Bingjie 冰洁
  full_name: Wang 王, Bingjie 冰洁
  last_name: Wang 王
- first_name: Andrea
  full_name: Weibel, Andrea
  last_name: Weibel
- first_name: Katherine E.
  full_name: Whitaker, Katherine E.
  last_name: Whitaker
- first_name: Christina C.
  full_name: Williams, Christina C.
  last_name: Williams
citation:
  ama: 'Setton DJ, Greene JE, de Graaff A, et al. Little Red Dots at an inflection
    point: Ubiquitous v-shaped turnover consistently occurs at the Balmer limit. <i>The
    Astrophysical Journal</i>. 2025;995(1). doi:<a href="https://doi.org/10.3847/1538-4357/ae1500">10.3847/1538-4357/ae1500</a>'
  apa: 'Setton, D. J., Greene, J. E., de Graaff, A., Ma, Y. 逸伦, Leja, J., Matthee,
    J. J., … Williams, C. C. (2025). Little Red Dots at an inflection point: Ubiquitous
    v-shaped turnover consistently occurs at the Balmer limit. <i>The Astrophysical
    Journal</i>. IOP Publishing. <a href="https://doi.org/10.3847/1538-4357/ae1500">https://doi.org/10.3847/1538-4357/ae1500</a>'
  chicago: 'Setton, David J., Jenny E. Greene, Anna de Graaff, Yilun 逸伦 Ma, Joel Leja,
    Jorryt J Matthee, Rachel Bezanson, et al. “Little Red Dots at an Inflection Point:
    Ubiquitous v-Shaped Turnover Consistently Occurs at the Balmer Limit.” <i>The
    Astrophysical Journal</i>. IOP Publishing, 2025. <a href="https://doi.org/10.3847/1538-4357/ae1500">https://doi.org/10.3847/1538-4357/ae1500</a>.'
  ieee: 'D. J. Setton <i>et al.</i>, “Little Red Dots at an inflection point: Ubiquitous
    v-shaped turnover consistently occurs at the Balmer limit,” <i>The Astrophysical
    Journal</i>, vol. 995, no. 1. IOP Publishing, 2025.'
  ista: 'Setton DJ, Greene JE, de Graaff A, Ma Y逸伦, Leja J, Matthee JJ, Bezanson R,
    Boogaard LA, Cleri NJ, Katz H, Labbe I, Maseda MV, McConachie I, Miller TB, Price
    SH, Suess KA, van Dokkum P, Wang 王 B冰洁, Weibel A, Whitaker KE, Williams CC. 2025.
    Little Red Dots at an inflection point: Ubiquitous v-shaped turnover consistently
    occurs at the Balmer limit. The Astrophysical Journal. 995(1), 118.'
  mla: 'Setton, David J., et al. “Little Red Dots at an Inflection Point: Ubiquitous
    v-Shaped Turnover Consistently Occurs at the Balmer Limit.” <i>The Astrophysical
    Journal</i>, vol. 995, no. 1, 118, IOP Publishing, 2025, doi:<a href="https://doi.org/10.3847/1538-4357/ae1500">10.3847/1538-4357/ae1500</a>.'
  short: D.J. Setton, J.E. Greene, A. de Graaff, Y.逸伦 Ma, J. Leja, J.J. Matthee, R.
    Bezanson, L.A. Boogaard, N.J. Cleri, H. Katz, I. Labbe, M.V. Maseda, I. McConachie,
    T.B. Miller, S.H. Price, K.A. Suess, P. van Dokkum, B.冰洁 Wang 王, A. Weibel, K.E.
    Whitaker, C.C. Williams, The Astrophysical Journal 995 (2025).
date_created: 2026-01-28T15:21:47Z
date_published: 2025-12-09T00:00:00Z
date_updated: 2026-02-09T06:41:48Z
day: '09'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ae1500
external_id:
  arxiv:
  - '2411.03424'
file:
- access_level: open_access
  checksum: 2a424eb43748a6370ff058c98adb15c6
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-09T06:39:23Z
  date_updated: 2026-02-09T06:39:23Z
  file_id: '21163'
  file_name: 2025_AstrophysicalJournal_Setton.pdf
  file_size: 1989640
  relation: main_file
  success: 1
file_date_updated: 2026-02-09T06:39:23Z
has_accepted_license: '1'
intvolume: '       995'
issue: '1'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
  eissn:
  - 1538-4357
  issn:
  - 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Little Red Dots at an inflection point: Ubiquitous v-shaped turnover consistently
  occurs at the Balmer limit'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 995
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21058'
abstract:
- lang: eng
  text: Luminous broad Hα emission and red rest-optical spectral energy distributions
    (SEDs) are the hallmark of compact little red dots (LRDs), implying highly attenuated
    dusty starbursts and/or obscured active galactic nuclei (AGN). However, the lack
    of observed far-infrared (FIR) emission has proved difficult to reconcile with
    the implied attenuated luminosity in these models. Here, we utilize deep new Atacama
    Large Millimeter/submillimeter Array imaging, new and existing JWST/MIRI imaging,
    and archival Spitzer/Herschel imaging of two of the rest-optically brightest LRDs
    (z = 3.1 and z = 4.47) to place the strongest constraints on the IR luminosity
    in LRDs to date. The detections at λrest = 1–4 μm imply flat slopes in the rest-IR,
    ruling out a contribution from hot (T ≳ 500 K) dust. Similarly, FIR nondetections
    rule out any appreciable cold (T ≲ 75 K) dust component. Assuming energy balance,
    these observations are inconsistent with the typical FIR dust emission of dusty
    starbursts and quasar tori, which usually show a mixture of cold and hot dust.
    Additionally, our [C ii] nondetections rule out typical dusty starbursts. We compute
    empirical maximum IR SEDs and find that both LRDs must have log(LIR/L ) 12.2 at
    the 3σ level. These limits are in tension with the predictions of rest-optical
    spectrophotometric fits, be they galaxy-only, AGN-only, or composite. It is unlikely
    that LRDs are highly dust-reddened intrinsically blue sources with a dust temperature
    distribution that conspires to avoid current observing facilities. Rather, we
    favor an intrinsically redder LRD SED model that alleviates the need for strong
    dust attenuation.
acknowledgement: "Support for this work was provided by The Brinson Foundation through
  a Brinson Prize Fellowship grant. D.S. acknowledges Zhengrong Li for kindly sharing
  model dust SEDs, Tim Rawle for helping with accessing archival Herschel Lensing
  Survey data, and Xiaohui Fan for helpful conversations that steered the direction
  of this work. This Letter makes use of the following ALMA data: ADS/JAO.ALMA#2024.00826.S.
  ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS
  (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic
  of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory
  is operated by ESO, AUI/NRAO and NAOJ. This work is based in part on observations
  made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from
  the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute
  (DOI: 10.17909/m7ks-wg55), which is operated by the Association of Universities
  for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These
  observations are associated with program #6761.\r\n\r\nSupport for this work was
  provided by NSF/AAG #2306950. Support for this work for R.P.N. was provided by NASA
  through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space
  Telescope Science Institute, which is operated by the Association of Universities
  for Research in Astronomy, Inc., under NASA contract NAS5-26555. This work has received
  funding from the Swiss State Secretariat for Education, Research and Innovation
  (SERI) under contract number MB22.00072, as well as from the Swiss National Science
  Foundation (SNSF) through project grant 200020_207349. The Cosmic Dawn Center is
  funded by the Danish National Research Foundation under grant DNRF140. A.Z. acknowledges
  support by grant No. 2020750 from the United States–Israel Binational Science Foundation
  (BSF) and grant No. 2109066 from the United States National Science Foundation (NSF)
  and by the Israel Science Foundation grant No. 864/23. The work of C.C.W. is supported
  by NOIRLab, which is managed by the Association of Universities for Research in
  Astronomy (AURA) under a cooperative agreement with the National Science Foundation.
  S.A. acknowledges support from the JWST Mid-Infrared Instrument (MIRI) Science Team
  Lead, grant 80NSSC18K0555, from NASA Goddard Space Flight Center to the University
  of Arizona."
article_number: L10
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: David J.
  full_name: Setton, David J.
  last_name: Setton
- first_name: Jenny E.
  full_name: Greene, Jenny E.
  last_name: Greene
- first_name: Justin S.
  full_name: Spilker, Justin S.
  last_name: Spilker
- first_name: Christina C.
  full_name: Williams, Christina C.
  last_name: Williams
- first_name: Ivo
  full_name: Labbé, Ivo
  last_name: Labbé
- first_name: Yilun 逸伦
  full_name: Ma, Yilun 逸伦
  last_name: Ma
- first_name: Bingjie 冰洁
  full_name: Wang, Bingjie 冰洁
  last_name: Wang
- first_name: Katherine E.
  full_name: Whitaker, Katherine E.
  last_name: Whitaker
- first_name: Joel
  full_name: Leja, Joel
  last_name: Leja
- first_name: Anna
  full_name: de Graaff, Anna
  last_name: de Graaff
- first_name: Stacey
  full_name: Alberts, Stacey
  last_name: Alberts
- first_name: Rachel
  full_name: Bezanson, Rachel
  last_name: Bezanson
- first_name: Leindert A.
  full_name: Boogaard, Leindert A.
  last_name: Boogaard
- first_name: Gabriel
  full_name: Brammer, Gabriel
  last_name: Brammer
- first_name: Sam E.
  full_name: Cutler, Sam E.
  last_name: Cutler
- first_name: Nikko J.
  full_name: Cleri, Nikko J.
  last_name: Cleri
- first_name: Olivia R.
  full_name: Cooper, Olivia R.
  last_name: Cooper
- first_name: Pratika
  full_name: Dayal, Pratika
  last_name: Dayal
- first_name: Seiji
  full_name: Fujimoto, Seiji
  last_name: Fujimoto
- first_name: Lukas J.
  full_name: Furtak, Lukas J.
  last_name: Furtak
- first_name: Andy D.
  full_name: Goulding, Andy D.
  last_name: Goulding
- first_name: Michaela
  full_name: Hirschmann, Michaela
  last_name: Hirschmann
- first_name: Vasily
  full_name: Kokorev, Vasily
  last_name: Kokorev
- first_name: Michael V.
  full_name: Maseda, Michael V.
  last_name: Maseda
- first_name: Ian
  full_name: McConachie, Ian
  last_name: McConachie
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: Tim B.
  full_name: Miller, Tim B.
  last_name: Miller
- first_name: Rohan P.
  full_name: Naidu, Rohan P.
  last_name: Naidu
- first_name: Pascal A.
  full_name: Oesch, Pascal A.
  last_name: Oesch
- first_name: Richard
  full_name: Pan, Richard
  last_name: Pan
- first_name: Sedona H.
  full_name: Price, Sedona H.
  last_name: Price
- first_name: Katherine A.
  full_name: Suess, Katherine A.
  last_name: Suess
- first_name: John R.
  full_name: Weaver, John R.
  last_name: Weaver
- first_name: Mengyuan
  full_name: Xiao, Mengyuan
  last_name: Xiao
- first_name: Yunchong
  full_name: Zhang, Yunchong
  last_name: Zhang
- first_name: Adi
  full_name: Zitrin, Adi
  last_name: Zitrin
citation:
  ama: Setton DJ, Greene JE, Spilker JS, et al. A confirmed deficit of hot and cold
    dust emission in the most luminous Little Red Dots. <i>The Astrophysical Journal
    Letters</i>. 2025;991. doi:<a href="https://doi.org/10.3847/2041-8213/ade78b">10.3847/2041-8213/ade78b</a>
  apa: Setton, D. J., Greene, J. E., Spilker, J. S., Williams, C. C., Labbé, I., Ma,
    Y. 逸伦, … Zitrin, A. (2025). A confirmed deficit of hot and cold dust emission
    in the most luminous Little Red Dots. <i>The Astrophysical Journal Letters</i>.
    IOP Publishing. <a href="https://doi.org/10.3847/2041-8213/ade78b">https://doi.org/10.3847/2041-8213/ade78b</a>
  chicago: Setton, David J., Jenny E. Greene, Justin S. Spilker, Christina C. Williams,
    Ivo Labbé, Yilun 逸伦 Ma, Bingjie 冰洁 Wang, et al. “A Confirmed Deficit of Hot and
    Cold Dust Emission in the Most Luminous Little Red Dots.” <i>The Astrophysical
    Journal Letters</i>. IOP Publishing, 2025. <a href="https://doi.org/10.3847/2041-8213/ade78b">https://doi.org/10.3847/2041-8213/ade78b</a>.
  ieee: D. J. Setton <i>et al.</i>, “A confirmed deficit of hot and cold dust emission
    in the most luminous Little Red Dots,” <i>The Astrophysical Journal Letters</i>,
    vol. 991. IOP Publishing, 2025.
  ista: Setton DJ, Greene JE, Spilker JS, Williams CC, Labbé I, Ma Y逸伦, Wang B冰洁,
    Whitaker KE, Leja J, de Graaff A, Alberts S, Bezanson R, Boogaard LA, Brammer
    G, Cutler SE, Cleri NJ, Cooper OR, Dayal P, Fujimoto S, Furtak LJ, Goulding AD,
    Hirschmann M, Kokorev V, Maseda MV, McConachie I, Matthee JJ, Miller TB, Naidu
    RP, Oesch PA, Pan R, Price SH, Suess KA, Weaver JR, Xiao M, Zhang Y, Zitrin A.
    2025. A confirmed deficit of hot and cold dust emission in the most luminous Little
    Red Dots. The Astrophysical Journal Letters. 991, L10.
  mla: Setton, David J., et al. “A Confirmed Deficit of Hot and Cold Dust Emission
    in the Most Luminous Little Red Dots.” <i>The Astrophysical Journal Letters</i>,
    vol. 991, L10, IOP Publishing, 2025, doi:<a href="https://doi.org/10.3847/2041-8213/ade78b">10.3847/2041-8213/ade78b</a>.
  short: D.J. Setton, J.E. Greene, J.S. Spilker, C.C. Williams, I. Labbé, Y.逸伦 Ma,
    B.冰洁 Wang, K.E. Whitaker, J. Leja, A. de Graaff, S. Alberts, R. Bezanson, L.A.
    Boogaard, G. Brammer, S.E. Cutler, N.J. Cleri, O.R. Cooper, P. Dayal, S. Fujimoto,
    L.J. Furtak, A.D. Goulding, M. Hirschmann, V. Kokorev, M.V. Maseda, I. McConachie,
    J.J. Matthee, T.B. Miller, R.P. Naidu, P.A. Oesch, R. Pan, S.H. Price, K.A. Suess,
    J.R. Weaver, M. Xiao, Y. Zhang, A. Zitrin, The Astrophysical Journal Letters 991
    (2025).
date_created: 2026-01-28T15:23:00Z
date_published: 2025-09-12T00:00:00Z
date_updated: 2026-02-09T07:14:08Z
day: '12'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/2041-8213/ade78b
external_id:
  arxiv:
  - '2503.02059'
file:
- access_level: open_access
  checksum: 799518db92ded4e166df4234195af998
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-09T07:10:29Z
  date_updated: 2026-02-09T07:10:29Z
  file_id: '21165'
  file_name: 2025_AstrophysicalJournalLetters_Setton.pdf
  file_size: 1394204
  relation: main_file
  success: 1
file_date_updated: 2026-02-09T07:10:29Z
has_accepted_license: '1'
intvolume: '       991'
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal Letters
publication_identifier:
  eissn:
  - 2041-8213
  issn:
  - 2041-8205
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: A confirmed deficit of hot and cold dust emission in the most luminous Little
  Red Dots
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 991
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '21060'
abstract:
- lang: eng
  text: "Compact, star-forming galaxies with high star formation rate surface densities
    (ΣSFR) are often efficient Lyman continuum (LyC) emitters at z ≤ 4.5, likely because
    intense stellar feedback creates low-density channels that allow photons to escape.
    Irregular or disturbed morphologies, such as those resulting from mergers, can
    also facilitate LyC escape by creating anisotropic gas distributions. We investigated
    the influence of galaxy morphology on LyC production and escape at redshifts 5
    ≤ z ≤ 7 using observations from various James Webb Space Telescope (JWST) surveys.
    Our sample consists of 436 sources, which are predominantly low-mass (∼10^8.15
    M\f), star-forming galaxies with ionizing photon efficiency (ξion) values consistent
    with canonical expectations. Since direct measurements of fesc are not possible
    during the Epoch of  Reionization (EoR), we predicted fesc for high-redshift galaxies
    by applying survival analysis to a subsample of LyC emitters from the Low-Redshift
    Lyman Continuum Survey (LzLCS), selected to be direct analogs of reionization-era
    galaxies. We find that these galaxies exhibit, on average, modest predicted escape
    fractions (∼0.04). In addition, we evaluated the correlation between morphological
    features and LyC emission. Our findings indicate that neither ξion nor the predicted
    fesc values show a significant correlation with the presence of merger signatures.
    This suggests that in low-mass galaxies at z ≥ 5, strong morphological disturbances
    are not the primary mechanism driving LyC emission and leakage. Instead, compactness
    and star formation activity likely play a more pivotal role in regulating LyC
    escape. "
acknowledgement: This work is based on observations made with the NASA/ESA/CSA James
  Webb Space Telescope. The data were obtained from the Mikulski Archive for Space
  Telescopes at the Space Telescope Science Institute, which is operated by the Association
  of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127
  for JWST. These observations are associated with programs GTO 1243, ERS 1345, DDT
  2750, and GTO 1180, 1181, 3215, 1210, 1286. Funded by the European Union (ERC, AGENTS,
  101076224). Views and opinions expressed are however those of the author(s) only
  and do not necessarily reflect those of the European Union or the European Research
  Council. Neither the European Union nor the granting authority can be held responsible
  for them. We acknowledge support from the INAF Large Grant 2022 “Extragalactic Surveys
  with JWST” (PI Pentericci). We acknowledge support from INAF Mini-grant “Reionization
  and Fundamental Cosmology with High-Redshift Galaxies” and from PRIN 2022 MUR project
  2022CB3PJ3 - First Light And Galaxy aSsembly (FLAGS) funded by the European Union
  – Next Generation EU. RA acknowledges support of Grant PID2023-147386NB-I00 funded
  by MICIU/AEI/10.13039/501100011033 and by ERDF/EU, and the Severo Ochoa grant CEX2021-001131-S
  funded by MCIN/AEI/10.13039/50110001103. The project that gave rise to these results
  received the support of a fellowship from the “la Caixa” Foundation (ID 100010434).
  The fellowship code is LCF/BQ/PR24/12050015. LC acknowledges support from grants
  PID2022-139567NB-I00 and PIB2021-127718NB-I00 funded by the Spanish Ministry of
  Science and Innovation/State Agency of Research MCIN/AEI/10.13039/501100011033 and
  by “ERDF A way of making Europe”.
article_number: A122
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Sara
  full_name: Mascia, Sara
  id: edaf889c-c7cd-11ef-ab1b-bb28c431bd29
  last_name: Mascia
- first_name: L.
  full_name: Pentericci, L.
  last_name: Pentericci
- first_name: M.
  full_name: Llerena, M.
  last_name: Llerena
- first_name: A.
  full_name: Calabrò, A.
  last_name: Calabrò
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: S.
  full_name: Flury, S.
  last_name: Flury
- first_name: F.
  full_name: Pacucci, F.
  last_name: Pacucci
- first_name: A.
  full_name: Jaskot, A.
  last_name: Jaskot
- first_name: R. O.
  full_name: Amorín, R. O.
  last_name: Amorín
- first_name: R.
  full_name: Bhatawdekar, R.
  last_name: Bhatawdekar
- first_name: M.
  full_name: Castellano, M.
  last_name: Castellano
- first_name: N.
  full_name: Cleri, N.
  last_name: Cleri
- first_name: L.
  full_name: Costantin, L.
  last_name: Costantin
- first_name: K.
  full_name: Davis, K.
  last_name: Davis
- first_name: Claudia
  full_name: Di Cesare, Claudia
  id: 2d002343-372f-11ef-98ec-a164d20427cb
  last_name: Di Cesare
- first_name: M.
  full_name: Dickinson, M.
  last_name: Dickinson
- first_name: A.
  full_name: Fontana, A.
  last_name: Fontana
- first_name: Y.
  full_name: Guo, Y.
  last_name: Guo
- first_name: M.
  full_name: Giavalisco, M.
  last_name: Giavalisco
- first_name: B. W.
  full_name: Holwerda, B. W.
  last_name: Holwerda
- first_name: W.
  full_name: Hu, W.
  last_name: Hu
- first_name: M.
  full_name: Huertas-Company, M.
  last_name: Huertas-Company
- first_name: Intae
  full_name: Jung, Intae
  last_name: Jung
- first_name: J.
  full_name: Kartaltepe, J.
  last_name: Kartaltepe
- first_name: D.
  full_name: Kashino, D.
  last_name: Kashino
- first_name: A. M.
  full_name: Koekemoer, A. M.
  last_name: Koekemoer
- first_name: R. A.
  full_name: Lucas, R. A.
  last_name: Lucas
- first_name: J.
  full_name: Lotz, J.
  last_name: Lotz
- first_name: L.
  full_name: Napolitano, L.
  last_name: Napolitano
- first_name: S.
  full_name: Jogee, S.
  last_name: Jogee
- first_name: S.
  full_name: Wilkins, S.
  last_name: Wilkins
citation:
  ama: Mascia S, Pentericci L, Llerena M, et al. Little impact of mergers and galaxy
    morphology on the production and escape of ionizing photons in the early Universe.
    <i>Astronomy &#38; Astrophysics</i>. 2025;701. doi:<a href="https://doi.org/10.1051/0004-6361/202553760">10.1051/0004-6361/202553760</a>
  apa: Mascia, S., Pentericci, L., Llerena, M., Calabrò, A., Matthee, J. J., Flury,
    S., … Wilkins, S. (2025). Little impact of mergers and galaxy morphology on the
    production and escape of ionizing photons in the early Universe. <i>Astronomy
    &#38; Astrophysics</i>. EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/202553760">https://doi.org/10.1051/0004-6361/202553760</a>
  chicago: Mascia, Sara, L. Pentericci, M. Llerena, A. Calabrò, Jorryt J Matthee,
    S. Flury, F. Pacucci, et al. “Little Impact of Mergers and Galaxy Morphology on
    the Production and Escape of Ionizing Photons in the Early Universe.” <i>Astronomy
    &#38; Astrophysics</i>. EDP Sciences, 2025. <a href="https://doi.org/10.1051/0004-6361/202553760">https://doi.org/10.1051/0004-6361/202553760</a>.
  ieee: S. Mascia <i>et al.</i>, “Little impact of mergers and galaxy morphology on
    the production and escape of ionizing photons in the early Universe,” <i>Astronomy
    &#38; Astrophysics</i>, vol. 701. EDP Sciences, 2025.
  ista: Mascia S, Pentericci L, Llerena M, Calabrò A, Matthee JJ, Flury S, Pacucci
    F, Jaskot A, Amorín RO, Bhatawdekar R, Castellano M, Cleri N, Costantin L, Davis
    K, Di Cesare C, Dickinson M, Fontana A, Guo Y, Giavalisco M, Holwerda BW, Hu W,
    Huertas-Company M, Jung I, Kartaltepe J, Kashino D, Koekemoer AM, Lucas RA, Lotz
    J, Napolitano L, Jogee S, Wilkins S. 2025. Little impact of mergers and galaxy
    morphology on the production and escape of ionizing photons in the early Universe.
    Astronomy &#38; Astrophysics. 701, A122.
  mla: Mascia, Sara, et al. “Little Impact of Mergers and Galaxy Morphology on the
    Production and Escape of Ionizing Photons in the Early Universe.” <i>Astronomy
    &#38; Astrophysics</i>, vol. 701, A122, EDP Sciences, 2025, doi:<a href="https://doi.org/10.1051/0004-6361/202553760">10.1051/0004-6361/202553760</a>.
  short: S. Mascia, L. Pentericci, M. Llerena, A. Calabrò, J.J. Matthee, S. Flury,
    F. Pacucci, A. Jaskot, R.O. Amorín, R. Bhatawdekar, M. Castellano, N. Cleri, L.
    Costantin, K. Davis, C. Di Cesare, M. Dickinson, A. Fontana, Y. Guo, M. Giavalisco,
    B.W. Holwerda, W. Hu, M. Huertas-Company, I. Jung, J. Kartaltepe, D. Kashino,
    A.M. Koekemoer, R.A. Lucas, J. Lotz, L. Napolitano, S. Jogee, S. Wilkins, Astronomy
    &#38; Astrophysics 701 (2025).
corr_author: '1'
date_created: 2026-01-28T15:24:24Z
date_published: 2025-09-01T00:00:00Z
date_updated: 2026-02-09T07:33:46Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202553760
external_id:
  arxiv:
  - '2501.08268'
file:
- access_level: open_access
  checksum: 990e384ca19e14b35296712d3b9e2919
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-09T07:28:08Z
  date_updated: 2026-02-09T07:28:08Z
  file_id: '21166'
  file_name: 2025_AstronomyAstrophysics_Mascia.pdf
  file_size: 9994234
  relation: main_file
  success: 1
file_date_updated: 2026-02-09T07:28:08Z
has_accepted_license: '1'
intvolume: '       701'
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
  grant_number: '101076224'
  name: Young galaxies as tracers and agents of cosmic reionization
publication: Astronomy & Astrophysics
publication_identifier:
  eissn:
  - 1432-0746
  issn:
  - 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: Little impact of mergers and galaxy morphology on the production and escape
  of ionizing photons in the early Universe
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 701
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21061'
abstract:
- lang: eng
  text: 'Detecting the first generation of stars, Population III (Pop III), has been
    a long-standing goal in astrophysics, yet they remain elusive even in the JWST
    era. Here we present a novel NIRCam-based selection method for Pop III galaxies,
    and carefully validate it through completeness and contamination simulations.
    We systematically search ≃ 500 arcmin2 across JWST legacy fields for Pop III candidates,
    including GLIMPSE, which, assisted by gravitational lensing, has produced JWST’s
    deepest NIRCam imaging thus far. We discover one promising Pop III galaxy candidate
    (GLIMPSE-16043) at z=6.50 -0.24 +0.03, a moderately lensed galaxy (µ = + 2.9 -0.2
    +0.1) with an intrinsic UV magnitude of MUV= -15.89 -0.14 +0.12. It exhibits key
    Pop III features: strong Hα emission (rest-frame EW 2810 ± 550 Å); a Balmer jump;
    no dust (UV slope β = −2.34 ± 0.36); and undetectable metal lines (e.g., [O III];
    [O III]/Hβ < 0.44), implying a gas-phase metallicity of Zgas/Z⊙ < 0.5%. These
    properties indicate the presence of a nascent, metal-deficient young stellar population
    (<5 Myr) with a stellar mass of ≃105 M⊙. Intriguingly, this source deviates significantly
    from the extrapolated UV–metallicity relation derived from recent JWST observations
    at z = 4–10, consistent with UV enhancement by a top-heavy Pop III initial mass
    function or the presence of an extremely metal-poor active galactic nucleus. We
    also  derive the first observational constraints on the Pop III UV luminosity
    function at z ≃ 6–7. The volume density of GLIMPSE-16043 (≈10^−4 cMpc−3) is in
    excellent agreement with theoretical predictions, independently reinforcing its
    plausibility. This study demonstrates the power of our novel NIRCam method to
    finally reveal distant galaxies even more pristine than the Milky Way’s most metal-poor
    satellites, thereby promising to bring us closer to the first generation of stars
    than we have ever been before.'
acknowledgement: "We are grateful to the CEERS, PRIMER, JOF, UNCOVER, and GLIMPSE
  teams for developing their NIRCam surveys, and to the various JWST and HST surveys
  acknowledged in Section 3 that enabled our search. We thank Kimihiko Nakajima and
  Kohei Inayoshi for sharing Pop III and/or AGN templates, Steven Finkelstein for
  comments on the completeness and contamination rate simulation, Aaron Yung for SEDs
  of simulated galaxies, Joel Leja, Ben Johnson, and Sandro Tacchella for advise on
  SED fitting, and Takashi Kojima and Hiroto Yanagisawa for discussions.\r\n\r\nWe
  made extensive use of the DAWN JWST Archive for various comparisons presented in
  this paper. Some of the data products presented herein were retrieved from the Dawn
  JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center (DAWN), which
  is funded by the Danish National Research Foundation under grant DNRF140. The prism
  spectra used in this paper were observed as part of the following programs, and
  we are grateful to these teams for helping build the rich spectroscopic legacy of
  JWST: 1180, 1181, 1210, 1286, 3215 (A. J. Bunker et al. 2024; F. D’Eugenio et al.
  2024); 1211–1215 (M. V. Maseda et al. 2024); 1345 (S. L. Finkelstein et al. 2024);
  1433 (T. Y.-Y. Hsiao et al. 2024); 1747 (G. Roberts-Borsani et al. 2025); 2028 (X.
  Wang et al. 2024); 2073 (PI: J. Hennawi); 2198 (L. Barrufet et al. 2025); 2282 (L.
  D. Bradley et al. 2023); 2561 (R. Bezanson et al. 2024; S. H. Price et al. 2024);
  2565 (T. Nanayakkara et al. 2023); 2750 (P. Arrabal Haro et al. 2023b); 2756 (PI:
  W. Chen); 2767 (C. C. Williams et al. 2023); 3073 (M. Castellano et al. 2024); 4106
  (PI: E. Nelson); 4233 (A. de Graaff et al. 2025); 4446 (B. L. Frye et al. 2024);
  4557 (PI: H. Yan); 6541 (PI: E. Egami); 6585 (PI: D. Coulter).\r\n\r\nThis work
  is based on observations made with the NASA/ESA/CSA James Webb Space Telescope.
  The data were obtained from the Mikulski Archive for Space Telescopes at the Space
  Telescope Science Institute, which is operated by the Association of Universities
  for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. The specific
  observations can be accessed via doi: 10.17909/xpxt-a441. These observations include
  data associated with program No. 03293. Support for program No. 03293 was provided
  by NASA through a grant from the Space Telescope Science Institute, which is operated
  by the Association of Universities for Research in Astronomy, Inc., under NASA contract
  NAS 5-03127.\r\n\r\nThis project has received funding from NASA through the NASA
  Hubble Fellowship grant HST-HF2-51505.001-A awarded by the Space Telescope Science
  Institute, which is operated by the Association of Universities for Research in
  Astronomy, Incorporated, under NASA contract NAS5-26555. This work has received
  funding from the Swiss State Secretariat for Education, Research and Innovation
  (SERI) under contract No. MB22.00072, as well as from the Swiss National Science
  Foundation (SNSF) through project grant 200020_207349. The Cosmic Dawn Center (DAWN)
  is funded by the Danish National Research Foundation under grant DNRF140. H.A. and
  I.C. acknowledge support from CNES, focused on the JWST mission, and the Programme
  National Cosmology and Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, co-funded
  by CEA and CNES. I.C. acknowledges funding support from the Initiative Physique
  des Infinis (IPI), a research training program of the Idex SUPER at Sorbonne Université.
  A.Z. acknowledges support by grant No. 2020750 from the United States–Israel Binational
  Science Foundation (BSF) and grant No. 2109066 from the United States National Science
  Foundation (NSF); and by the Israel Science Foundation grant No. 864/23. P.N. acknowledges
  support from the Gordon and Betty Moore Foundation and the John Templeton Foundation
  that fund the black hole Initiative (BHI) at Harvard University, where she serves
  as one of the PIs. B.L. acknowledges support from the Deutsche Forschungsgemeinschaft
  (DFG, German Research Foundation) under Germany’s Excellence Strategy EXC 2181/1—390900948
  (the Heidelberg STRUCTURES Excellence Cluster). Y.S. and G.M. have received funding
  from the European Research Council (ERC) under the European Union’s Horizon 2020
  research and innovation program (grant agreement No. 833925, project STAREX)."
article_number: '46'
article_processing_charge: Yes
article_type: original
author:
- first_name: Seiji
  full_name: Fujimoto, Seiji
  last_name: Fujimoto
- first_name: Rohan P.
  full_name: Naidu, Rohan P.
  last_name: Naidu
- first_name: John
  full_name: Chisholm, John
  last_name: Chisholm
- first_name: Hakim
  full_name: Atek, Hakim
  last_name: Atek
- first_name: Ryan
  full_name: Endsley, Ryan
  last_name: Endsley
- first_name: Vasily
  full_name: Kokorev, Vasily
  last_name: Kokorev
- first_name: Lukas J.
  full_name: Furtak, Lukas J.
  last_name: Furtak
- first_name: Richard
  full_name: Pan, Richard
  last_name: Pan
- first_name: Boyuan
  full_name: Liu, Boyuan
  last_name: Liu
- first_name: Volker
  full_name: Bromm, Volker
  last_name: Bromm
- first_name: Alessandra
  full_name: Venditti, Alessandra
  last_name: Venditti
- first_name: Eli
  full_name: Visbal, Eli
  last_name: Visbal
- first_name: Richard
  full_name: Sarmento, Richard
  last_name: Sarmento
- first_name: Andrea
  full_name: Weibel, Andrea
  last_name: Weibel
- first_name: Pascal A.
  full_name: Oesch, Pascal A.
  last_name: Oesch
- first_name: Gabriel
  full_name: Brammer, Gabriel
  last_name: Brammer
- first_name: Daniel
  full_name: Schaerer, Daniel
  last_name: Schaerer
- first_name: Angela
  full_name: Adamo, Angela
  last_name: Adamo
- first_name: Danielle A.
  full_name: Berg, Danielle A.
  last_name: Berg
- first_name: Rachel
  full_name: Bezanson, Rachel
  last_name: Bezanson
- first_name: Rychard
  full_name: Bouwens, Rychard
  last_name: Bouwens
- first_name: Iryna
  full_name: Chemerynska, Iryna
  last_name: Chemerynska
- first_name: Adélaïde
  full_name: Claeyssens, Adélaïde
  last_name: Claeyssens
- first_name: Miroslava
  full_name: Dessauges-Zavadsky, Miroslava
  last_name: Dessauges-Zavadsky
- first_name: Anna
  full_name: Frebel, Anna
  last_name: Frebel
- first_name: Damien
  full_name: Korber, Damien
  last_name: Korber
- first_name: Ivo
  full_name: Labbe, Ivo
  last_name: Labbe
- first_name: Rui
  full_name: Marques-Chaves, Rui
  last_name: Marques-Chaves
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: Kristen B. W.
  full_name: McQuinn, Kristen B. W.
  last_name: McQuinn
- first_name: Julian B.
  full_name: Muñoz, Julian B.
  last_name: Muñoz
- first_name: Priyamvada
  full_name: Natarajan, Priyamvada
  last_name: Natarajan
- first_name: Alberto
  full_name: Saldana-Lopez, Alberto
  last_name: Saldana-Lopez
- first_name: Katherine A.
  full_name: Suess, Katherine A.
  last_name: Suess
- first_name: Marta
  full_name: Volonteri, Marta
  last_name: Volonteri
- first_name: Adi
  full_name: Zitrin, Adi
  last_name: Zitrin
citation:
  ama: 'Fujimoto S, Naidu RP, Chisholm J, et al. GLIMPSE: An ultrafaint ≃10^5 M⊙ Pop
    III galaxy candidate and first constraints on the Pop III UV luminosity function
    at z ≃  6–7. <i>The Astrophysical Journal</i>. 2025;989. doi:<a href="https://doi.org/10.3847/1538-4357/ade9a1">10.3847/1538-4357/ade9a1</a>'
  apa: 'Fujimoto, S., Naidu, R. P., Chisholm, J., Atek, H., Endsley, R., Kokorev,
    V., … Zitrin, A. (2025). GLIMPSE: An ultrafaint ≃10^5 M⊙ Pop III galaxy candidate
    and first constraints on the Pop III UV luminosity function at z ≃  6–7. <i>The
    Astrophysical Journal</i>. IOP Publishing. <a href="https://doi.org/10.3847/1538-4357/ade9a1">https://doi.org/10.3847/1538-4357/ade9a1</a>'
  chicago: 'Fujimoto, Seiji, Rohan P. Naidu, John Chisholm, Hakim Atek, Ryan Endsley,
    Vasily Kokorev, Lukas J. Furtak, et al. “GLIMPSE: An Ultrafaint ≃10^5 M⊙ Pop III
    Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at
    z ≃  6–7.” <i>The Astrophysical Journal</i>. IOP Publishing, 2025. <a href="https://doi.org/10.3847/1538-4357/ade9a1">https://doi.org/10.3847/1538-4357/ade9a1</a>.'
  ieee: 'S. Fujimoto <i>et al.</i>, “GLIMPSE: An ultrafaint ≃10^5 M⊙ Pop III galaxy
    candidate and first constraints on the Pop III UV luminosity function at z ≃ 
    6–7,” <i>The Astrophysical Journal</i>, vol. 989. IOP Publishing, 2025.'
  ista: 'Fujimoto S, Naidu RP, Chisholm J, Atek H, Endsley R, Kokorev V, Furtak LJ,
    Pan R, Liu B, Bromm V, Venditti A, Visbal E, Sarmento R, Weibel A, Oesch PA, Brammer
    G, Schaerer D, Adamo A, Berg DA, Bezanson R, Bouwens R, Chemerynska I, Claeyssens
    A, Dessauges-Zavadsky M, Frebel A, Korber D, Labbe I, Marques-Chaves R, Matthee
    JJ, McQuinn KBW, Muñoz JB, Natarajan P, Saldana-Lopez A, Suess KA, Volonteri M,
    Zitrin A. 2025. GLIMPSE: An ultrafaint ≃10^5 M⊙ Pop III galaxy candidate and first
    constraints on the Pop III UV luminosity function at z ≃  6–7. The Astrophysical
    Journal. 989, 46.'
  mla: 'Fujimoto, Seiji, et al. “GLIMPSE: An Ultrafaint ≃10^5 M⊙ Pop III Galaxy Candidate
    and First Constraints on the Pop III UV Luminosity Function at z ≃  6–7.” <i>The
    Astrophysical Journal</i>, vol. 989, 46, IOP Publishing, 2025, doi:<a href="https://doi.org/10.3847/1538-4357/ade9a1">10.3847/1538-4357/ade9a1</a>.'
  short: S. Fujimoto, R.P. Naidu, J. Chisholm, H. Atek, R. Endsley, V. Kokorev, L.J.
    Furtak, R. Pan, B. Liu, V. Bromm, A. Venditti, E. Visbal, R. Sarmento, A. Weibel,
    P.A. Oesch, G. Brammer, D. Schaerer, A. Adamo, D.A. Berg, R. Bezanson, R. Bouwens,
    I. Chemerynska, A. Claeyssens, M. Dessauges-Zavadsky, A. Frebel, D. Korber, I.
    Labbe, R. Marques-Chaves, J.J. Matthee, K.B.W. McQuinn, J.B. Muñoz, P. Natarajan,
    A. Saldana-Lopez, K.A. Suess, M. Volonteri, A. Zitrin, The Astrophysical Journal
    989 (2025).
date_created: 2026-01-28T15:25:17Z
date_published: 2025-08-04T00:00:00Z
date_updated: 2026-02-09T08:11:01Z
day: '04'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ade9a1
file:
- access_level: open_access
  checksum: 9e08e77ce6d818fafd074e2b6c30bc43
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-09T07:57:01Z
  date_updated: 2026-02-09T07:57:01Z
  file_id: '21167'
  file_name: 2025_AstrophysicalJournal_Fujimoto.pdf
  file_size: 14405059
  relation: main_file
  success: 1
file_date_updated: 2026-02-09T07:57:01Z
has_accepted_license: '1'
intvolume: '       989'
language:
- iso: eng
month: '08'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
  eissn:
  - 1538-4357
  issn:
  - 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'GLIMPSE: An ultrafaint ≃10^5 M⊙ Pop III galaxy candidate and first constraints
  on the Pop III UV luminosity function at z ≃  6–7'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 989
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21062'
abstract:
- lang: eng
  text: JWST observations have unveiled faint active galactic nuclei (AGNs) at high
    redshift that provide insights into the formation of supermassive black holes
    (SMBHs). However, disentangling their stellar from AGN light is challenging. Here,
    we use an empirical approach to infer the average stellar mass of five faint broad-line
    (BL) Hα emitters at z = 4–5 with BH masses ≈6 × 10^6 M⊙, with a method independent
    of their spectral energy distribution (SED). We use the deep JWST/NIRcam grism
    survey “All the Little Things” to measure the overdensities around BL-Hα emitters
    and around a spectroscopic reference sample of ∼300 galaxies. In our reference
    sample, we find that megaparsec-scale overdensity correlates with stellar mass.
    Their large-scale environments suggest that BL-Hα emitters are hosted by galaxies
    with stellar masses ≈5 × 10^7 M⊙, ≈40 times lower than those inferred from galaxy-only
    SED fits. Adding measurements around more luminous z ≈ 6 AGNs, we find tentative
    correlations between line width, BH mass, and the overdensity, suggestive of a
    steep BH to halo mass relation. The main implications are (1) when BH masses are
    taken at face value, we confirm extremely high BH to stellar mass ratios of ≈10%,
    (2) the galaxies of low stellar mass that host growing SMBHs are in tension with
    typical hydrodynamical simulations, except those without feedback, (3) a 1% duty
    cycle implied by the host mass hints at super-Eddington accretion, (4) the masses
    are at odds with an interpretation of the line broadening in terms of high stellar
    density, (5) our results imply a luminosity-dependent diversity of galaxy masses,
    environments, and SEDs among AGN samples.
acknowledgement: 'We thank the referee for their constructive comments that helped
  to improve the paper. We thank Junyao Li for sharing model output shown in Figure
  13, Rob Crain for sharing results from the ONLYAGN EAGLE model shown in Figure 15,
  and Adi Zitrin for comments. This work is based on observations made with the NASA/ESA/CSA
  James Webb Space Telescope. The data were obtained from the Mikulski Archive for
  Space Telescopes at the Space Telescope Science Institute, which is operated by
  the Association of Universities for Research in Astronomy, Inc., under NASA contract
  NAS 5-03127 for JWST. These observations are associated with programs # 3516. Funded
  by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed are
  however those of the author(s) only and do not necessarily reflect those of the
  European Union or the European Research Council. Neither the European Union nor
  the granting authority can be held responsible for them. We acknowledge funding
  from JWST program GO-3516. Support for this work was provided by NASA through the
  NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope
  Science Institute, which is operated by the Association of Universities for Research
  in Astronomy, Incorporated, under NASA contract NAS 5-26555. A.A. acknowledges support
  by the Swedish research council Vetenskapsrådet (2021-05559).'
article_number: '246'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: Rohan P.
  full_name: Naidu, Rohan P.
  last_name: Naidu
- first_name: Gauri
  full_name: Kotiwale, Gauri
  id: 1438afc8-1ff6-11ee-9fa6-cd4a75d66875
  last_name: Kotiwale
- first_name: Lukas J.
  full_name: Furtak, Lukas J.
  last_name: Furtak
- first_name: Ivan
  full_name: Kramarenko, Ivan
  id: 9a9394cb-3200-11ee-973b-f5ba2a8b16e4
  last_name: Kramarenko
  orcid: 0000-0001-5346-6048
- first_name: Ruari
  full_name: Mackenzie, Ruari
  last_name: Mackenzie
- first_name: Jenny
  full_name: Greene, Jenny
  last_name: Greene
- first_name: Angela
  full_name: Adamo, Angela
  last_name: Adamo
- first_name: Rychard J.
  full_name: Bouwens, Rychard J.
  last_name: Bouwens
- first_name: Claudia
  full_name: Di Cesare, Claudia
  id: 2d002343-372f-11ef-98ec-a164d20427cb
  last_name: Di Cesare
- first_name: Anna-Christina
  full_name: Eilers, Anna-Christina
  last_name: Eilers
- first_name: Anna
  full_name: de Graaff, Anna
  last_name: de Graaff
- first_name: Kasper E.
  full_name: Heintz, Kasper E.
  last_name: Heintz
- first_name: Daichi
  full_name: Kashino, Daichi
  last_name: Kashino
- first_name: Michael V.
  full_name: Maseda, Michael V.
  last_name: Maseda
- first_name: Sandro
  full_name: Tacchella, Sandro
  last_name: Tacchella
- first_name: Alberto
  full_name: Torralba Torregrosa, Alberto
  id: 018f0249-0e87-11f0-b167-cbce08fbd541
  last_name: Torralba Torregrosa
  orcid: 0000-0001-5586-6950
citation:
  ama: Matthee JJ, Naidu RP, Kotiwale G, et al. Environmental evidence for overly
    massive Black Holes in low-mass galaxies and a Black Hole–Halo mass relation at
    z ∼ 5. <i>The Astrophysical Journal</i>. 2025;988(2). doi:<a href="https://doi.org/10.3847/1538-4357/ade886">10.3847/1538-4357/ade886</a>
  apa: Matthee, J. J., Naidu, R. P., Kotiwale, G., Furtak, L. J., Kramarenko, I.,
    Mackenzie, R., … Torralba Torregrosa, A. (2025). Environmental evidence for overly
    massive Black Holes in low-mass galaxies and a Black Hole–Halo mass relation at
    z ∼ 5. <i>The Astrophysical Journal</i>. IOP Publishing. <a href="https://doi.org/10.3847/1538-4357/ade886">https://doi.org/10.3847/1538-4357/ade886</a>
  chicago: Matthee, Jorryt J, Rohan P. Naidu, Gauri Kotiwale, Lukas J. Furtak, Ivan
    Kramarenko, Ruari Mackenzie, Jenny Greene, et al. “Environmental Evidence for
    Overly Massive Black Holes in Low-Mass Galaxies and a Black Hole–Halo Mass Relation
    at z ∼ 5.” <i>The Astrophysical Journal</i>. IOP Publishing, 2025. <a href="https://doi.org/10.3847/1538-4357/ade886">https://doi.org/10.3847/1538-4357/ade886</a>.
  ieee: J. J. Matthee <i>et al.</i>, “Environmental evidence for overly massive Black
    Holes in low-mass galaxies and a Black Hole–Halo mass relation at z ∼ 5,” <i>The
    Astrophysical Journal</i>, vol. 988, no. 2. IOP Publishing, 2025.
  ista: Matthee JJ, Naidu RP, Kotiwale G, Furtak LJ, Kramarenko I, Mackenzie R, Greene
    J, Adamo A, Bouwens RJ, Di Cesare C, Eilers A-C, de Graaff A, Heintz KE, Kashino
    D, Maseda MV, Tacchella S, Torralba Torregrosa A. 2025. Environmental evidence
    for overly massive Black Holes in low-mass galaxies and a Black Hole–Halo mass
    relation at z ∼ 5. The Astrophysical Journal. 988(2), 246.
  mla: Matthee, Jorryt J., et al. “Environmental Evidence for Overly Massive Black
    Holes in Low-Mass Galaxies and a Black Hole–Halo Mass Relation at z ∼ 5.” <i>The
    Astrophysical Journal</i>, vol. 988, no. 2, 246, IOP Publishing, 2025, doi:<a
    href="https://doi.org/10.3847/1538-4357/ade886">10.3847/1538-4357/ade886</a>.
  short: J.J. Matthee, R.P. Naidu, G. Kotiwale, L.J. Furtak, I. Kramarenko, R. Mackenzie,
    J. Greene, A. Adamo, R.J. Bouwens, C. Di Cesare, A.-C. Eilers, A. de Graaff, K.E.
    Heintz, D. Kashino, M.V. Maseda, S. Tacchella, A. Torralba Torregrosa, The Astrophysical
    Journal 988 (2025).
corr_author: '1'
date_created: 2026-01-28T15:25:42Z
date_published: 2025-07-29T00:00:00Z
date_updated: 2026-02-09T08:22:01Z
day: '29'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ade886
external_id:
  arxiv:
  - '2412.02846'
file:
- access_level: open_access
  checksum: a49fbed72f2ff9c0b13129acb6f44f9d
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-09T08:20:14Z
  date_updated: 2026-02-09T08:20:14Z
  file_id: '21168'
  file_name: 2025_AstrophysicalJournal_Matthee.pdf
  file_size: 6237415
  relation: main_file
  success: 1
file_date_updated: 2026-02-09T08:20:14Z
has_accepted_license: '1'
intvolume: '       988'
issue: '2'
language:
- iso: eng
month: '07'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
  grant_number: '101076224'
  name: Young galaxies as tracers and agents of cosmic reionization
publication: The Astrophysical Journal
publication_identifier:
  eissn:
  - 1538-4357
  issn:
  - 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Environmental evidence for overly massive Black Holes in low-mass galaxies
  and a Black Hole–Halo mass relation at z ∼ 5
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 988
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21063'
abstract:
- lang: eng
  text: "We report the detection of a 13σ Hα emission line from HDF850.1 at z = 5.188
    ± 0.001 using the FRESCO (First Reionization Era SpectroscopicallyComplete Observations)
    NIRCam F444W grism observations. Detection of Hα in HDF850.1 is noteworthy, given
    its high far-infrared (IR) luminosity, substantial dust obscuration, and the historical
    challenges in deriving its redshift.\r\nHDF850.1 shows a clear detection in the
    F444W imaging data, distributed between a northern and southern component, mirroring
    that seen in [C II] from the Plateau de Bure Interferometer. Modelling the spectral
    energy distribution of each component separately, we find that the northern component
    has a higher mass, star formation rate (SFR), and dust extinction than the southern
    component. The observed Hα emission appears to arise entirely from the less-obscured
    southern component and shows a similar \x04v∼ + 130 km s −1 velocity offset to
    that seen for [C II] relative to the source systemic redshift. Leveraging Hα-derived
    redshiftsfrom FRESCO observations, we find that HDF850.1 isforming in one of the
    richest environments identified to date at z > 5, with 100 z = 5.17–5.20 galaxies
    distributed across 13 smaller structures and a ∼(15 cMpc)3 volume. Based on the
    evolution of analogous structures in cosmological simulations, the z = 5.17–5.20
    structures seem likely to collapse into\r\na single > 1014M cluster by z ∼ 0.
    Comparing galaxy properties forming within this overdensity with those outside,
    we find the masses, SFRs, and UV luminosities inside the overdensity to be clearly
    higher. The prominence of Hα line emission from HDF850.1 and other known highly
    obscured z > 5 galaxies illustrates the potential of NIRCam-grism programs to
    map both\r\nthe early build-up of IR-luminous galaxies and overdense structures."
acknowledgement: "We are grateful to Roberto Neri and collaborators for providing
  us with spatially resolved information on both the dust-continuum and [C ii] line
  emission from their high spatial resolution PdBI observations. This project was
  made possible in part by the Leiden University Fund/Bouwens Astrophysics Fund. RJB
  acknowledges support from NWO grants 600.065.140.11N211 (vrij competitie) and TOP
  grant TOP1.16.057. The Cosmic Dawn Center (DAWN) is funded by the Danish National
  Research Foundation under grant no. 140. Cloud-based data processing and file storage
  for this work is provided by the AWS Cloud Credits for Research program. Support
  for this work was provided by NASA through grant JWST-GO-01895 awarded by the Space
  Telescope Science Institute, which is operated by the Association of Universities
  for Research in Astronomy, Inc., under NASA contract NAS 5–26555. RPN acknowledges
  funding from JWST programs GO-1933 and GO-2279. Support for this work was provided
  by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by
  the Space Telescope Science Institute, which is operated by the Association of Universities
  for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. MS acknowledges
  support from the CIDEGENT/2021/059 grant, from project PID2019-109592GB-I00/AEI/10.13039/501100011033
  from the Spanish Ministerio de Ciencia e Innovación – Agencia Estatal de Investigación.
  This study forms part of the Astrophysics and High Energy Physics programme and
  was supported by MCIN with funding from European Union NextGenerationEU (PRTR-C17.I1)
  and by Generalitat Valenciana under the project n. ASFAE/2022/025. RAM acknowledges
  support from the ERC Advanced Grant 740246 (Cosmic_Gas) and the Swiss National Science
  Foundation through project grant 200020_207349.\r\n\r\nThis work is based on observations
  made with the NASA/ESA/CSA JWST. The data were obtained from the Mikulski Archive
  for Space Telescopes at the Space Telescope Science Institute, which is operated
  by the Association of Universities for Research in Astronomy, Inc., under NASA contract
  NAS 5–03127 for JWST. These observations are associated with program no. 1895.\r\n\r\nThis
  paper made use of several publicly available software packages. We are indebted
  to the respective authors for their work: ipython (Pérez & Granger 2007), matplotlib
  (Hunter 2007), numpy (Oliphant 2006), scipy (Virtanen et al. 2020), jupyter (Kluyver
  et al. 2016), astropy (Astropy Collaboration 2013, 2018), grizli (v1.7.11; Brammer
  2018; Brammer et al. 2022), eazy (Brammer, van Dokkum & Coppi 2008), and SExtractor
  (Bertin & Arnouts 1996)."
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Thomas
  full_name: Herard-Demanche, Thomas
  last_name: Herard-Demanche
- first_name: Rychard J
  full_name: Bouwens, Rychard J
  last_name: Bouwens
- first_name: Pascal A
  full_name: Oesch, Pascal A
  last_name: Oesch
- first_name: Rohan P
  full_name: Naidu, Rohan P
  last_name: Naidu
- first_name: Roberto
  full_name: Decarli, Roberto
  last_name: Decarli
- first_name: Erica J
  full_name: Nelson, Erica J
  last_name: Nelson
- first_name: Gabriel
  full_name: Brammer, Gabriel
  last_name: Brammer
- first_name: Andrea
  full_name: Weibel, Andrea
  last_name: Weibel
- first_name: Mengyuan
  full_name: Xiao, Mengyuan
  last_name: Xiao
- first_name: Mauro
  full_name: Stefanon, Mauro
  last_name: Stefanon
- first_name: Fabian
  full_name: Walter, Fabian
  last_name: Walter
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: Romain A
  full_name: Meyer, Romain A
  last_name: Meyer
- first_name: Stijn
  full_name: Wuyts, Stijn
  last_name: Wuyts
- first_name: Naveen
  full_name: Reddy, Naveen
  last_name: Reddy
- first_name: Lucie
  full_name: Rowland, Lucie
  last_name: Rowland
- first_name: Ivana
  full_name: van Leeuwen, Ivana
  last_name: van Leeuwen
- first_name: Pablo Arrabal
  full_name: Haro, Pablo Arrabal
  last_name: Haro
- first_name: Helmut
  full_name: Dannerbauer, Helmut
  last_name: Dannerbauer
- first_name: Alice E
  full_name: Shapley, Alice E
  last_name: Shapley
- first_name: John
  full_name: Chisholm, John
  last_name: Chisholm
- first_name: Pieter
  full_name: van Dokkum, Pieter
  last_name: van Dokkum
- first_name: Ivo
  full_name: Labbe, Ivo
  last_name: Labbe
- first_name: Garth
  full_name: Illingworth, Garth
  last_name: Illingworth
- first_name: Daniel
  full_name: Schaerer, Daniel
  last_name: Schaerer
- first_name: Irene
  full_name: Shivaei, Irene
  last_name: Shivaei
citation:
  ama: 'Herard-Demanche T, Bouwens RJ, Oesch PA, et al. Mapping dusty galaxy growth
    at z &#62; 5 with FRESCO: Detection of Hα in submm galaxy HDF850.1 and the surrounding
    overdense structures. <i>Monthly Notices of the Royal Astronomical Society</i>.
    2025;537(2):788-808. doi:<a href="https://doi.org/10.1093/mnras/staf030">10.1093/mnras/staf030</a>'
  apa: 'Herard-Demanche, T., Bouwens, R. J., Oesch, P. A., Naidu, R. P., Decarli,
    R., Nelson, E. J., … Shivaei, I. (2025). Mapping dusty galaxy growth at z &#62;
    5 with FRESCO: Detection of Hα in submm galaxy HDF850.1 and the surrounding overdense
    structures. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University
    Press. <a href="https://doi.org/10.1093/mnras/staf030">https://doi.org/10.1093/mnras/staf030</a>'
  chicago: 'Herard-Demanche, Thomas, Rychard J Bouwens, Pascal A Oesch, Rohan P Naidu,
    Roberto Decarli, Erica J Nelson, Gabriel Brammer, et al. “Mapping Dusty Galaxy
    Growth at z &#62; 5 with FRESCO: Detection of Hα in Submm Galaxy HDF850.1 and
    the Surrounding Overdense Structures.” <i>Monthly Notices of the Royal Astronomical
    Society</i>. Oxford University Press, 2025. <a href="https://doi.org/10.1093/mnras/staf030">https://doi.org/10.1093/mnras/staf030</a>.'
  ieee: 'T. Herard-Demanche <i>et al.</i>, “Mapping dusty galaxy growth at z &#62;
    5 with FRESCO: Detection of Hα in submm galaxy HDF850.1 and the surrounding overdense
    structures,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 537,
    no. 2. Oxford University Press, pp. 788–808, 2025.'
  ista: 'Herard-Demanche T, Bouwens RJ, Oesch PA, Naidu RP, Decarli R, Nelson EJ,
    Brammer G, Weibel A, Xiao M, Stefanon M, Walter F, Matthee JJ, Meyer RA, Wuyts
    S, Reddy N, Rowland L, van Leeuwen I, Haro PA, Dannerbauer H, Shapley AE, Chisholm
    J, van Dokkum P, Labbe I, Illingworth G, Schaerer D, Shivaei I. 2025. Mapping
    dusty galaxy growth at z &#62; 5 with FRESCO: Detection of Hα in submm galaxy
    HDF850.1 and the surrounding overdense structures. Monthly Notices of the Royal
    Astronomical Society. 537(2), 788–808.'
  mla: 'Herard-Demanche, Thomas, et al. “Mapping Dusty Galaxy Growth at z &#62; 5
    with FRESCO: Detection of Hα in Submm Galaxy HDF850.1 and the Surrounding Overdense
    Structures.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 537,
    no. 2, Oxford University Press, 2025, pp. 788–808, doi:<a href="https://doi.org/10.1093/mnras/staf030">10.1093/mnras/staf030</a>.'
  short: T. Herard-Demanche, R.J. Bouwens, P.A. Oesch, R.P. Naidu, R. Decarli, E.J.
    Nelson, G. Brammer, A. Weibel, M. Xiao, M. Stefanon, F. Walter, J.J. Matthee,
    R.A. Meyer, S. Wuyts, N. Reddy, L. Rowland, I. van Leeuwen, P.A. Haro, H. Dannerbauer,
    A.E. Shapley, J. Chisholm, P. van Dokkum, I. Labbe, G. Illingworth, D. Schaerer,
    I. Shivaei, Monthly Notices of the Royal Astronomical Society 537 (2025) 788–808.
date_created: 2026-01-28T15:25:53Z
date_published: 2025-02-01T00:00:00Z
date_updated: 2026-02-09T08:50:55Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1093/mnras/staf030
external_id:
  arxiv:
  - '2309.04525'
file:
- access_level: open_access
  checksum: 4cbade43244eaa8b60bb05a90ae613da
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-09T08:39:19Z
  date_updated: 2026-02-09T08:39:19Z
  file_id: '21169'
  file_name: 2025_MonthlyNoticesRAS_HerardDemanche.pdf
  file_size: 2787493
  relation: main_file
  success: 1
file_date_updated: 2026-02-09T08:39:19Z
has_accepted_license: '1'
intvolume: '       537'
issue: '2'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
page: 788-808
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
  eissn:
  - 1365-2966
  issn:
  - 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
status: public
title: 'Mapping dusty galaxy growth at z > 5 with FRESCO: Detection of Hα in submm
  galaxy HDF850.1 and the surrounding overdense structures'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 537
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '21066'
abstract:
- lang: eng
  text: "Causal discovery from observational data holds great promise, but existing
    methods rely on strong assumptions about the underlying causal structure, often
    requiring full observability of all relevant variables. We tackle these challenges
    by leveraging the score function ∇logp(X)\r\n of observed variables for causal
    discovery and propose the following contributions. First, we generalize the existing
    results of identifiability with the score to additive noise models with minimal
    requirements on the causal mechanisms. Second, we establish conditions for inferring
    causal relations from the score even in the presence of hidden variables; this
    result is two-faced: we demonstrate the score’s potential as an alternative to
    conditional independence tests to infer the equivalence class of causal graphs
    with hidden variables, and we provide the necessary conditions for identifying
    direct causes in latent variable models. Building on these insights, we propose
    a flexible algorithm for causal discovery across linear, nonlinear, and latent
    variable models, which we empirically validate."
acknowledgement: "Philipp M. Faller was supported by a doctoral scholarship of the
  Studienstiftung des deutschen\r\nVolkes (German Academic Scholarship Foundation).
  This work has been supported by AFOSR,\r\ngrant n. FA8655-20-1-7035. FM is supported
  by Programma Operativo Nazionale ricerca e innovazione 2014-2020. We thank Atalanti
  A. Mastakouri, Kun Zhang and Haoyue Dai for the insightful discussions."
alternative_title:
- PMLR
article_processing_charge: No
arxiv: 1
author:
- first_name: Francesco
  full_name: Montagna, Francesco
  last_name: Montagna
- first_name: Philipp
  full_name: Faller, Philipp
  last_name: Faller
- first_name: Patrik
  full_name: Blöbaum, Patrik
  last_name: Blöbaum
- first_name: Elke
  full_name: Kirschbaum, Elke
  last_name: Kirschbaum
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
citation:
  ama: 'Montagna F, Faller P, Blöbaum P, Kirschbaum E, Locatello F. Score matching
    through the roof: Linear, nonlinear, and latent variables causal discovery. In:
    <i>Proceedings of the Fourth Conference on Causal Learning and Reasoning</i>.
    Vol 275. ML Research Press; 2025:552-605.'
  apa: 'Montagna, F., Faller, P., Blöbaum, P., Kirschbaum, E., &#38; Locatello, F.
    (2025). Score matching through the roof: Linear, nonlinear, and latent variables
    causal discovery. In <i>Proceedings of the Fourth Conference on Causal Learning
    and Reasoning</i> (Vol. 275, pp. 552–605). Lausanne, Switzerland: ML Research
    Press.'
  chicago: 'Montagna, Francesco, Philipp Faller, Patrik Blöbaum, Elke Kirschbaum,
    and Francesco Locatello. “Score Matching through the Roof: Linear, Nonlinear,
    and Latent Variables Causal Discovery.” In <i>Proceedings of the Fourth Conference
    on Causal Learning and Reasoning</i>, 275:552–605. ML Research Press, 2025.'
  ieee: 'F. Montagna, P. Faller, P. Blöbaum, E. Kirschbaum, and F. Locatello, “Score
    matching through the roof: Linear, nonlinear, and latent variables causal discovery,”
    in <i>Proceedings of the Fourth Conference on Causal Learning and Reasoning</i>,
    Lausanne, Switzerland, 2025, vol. 275, pp. 552–605.'
  ista: 'Montagna F, Faller P, Blöbaum P, Kirschbaum E, Locatello F. 2025. Score matching
    through the roof: Linear, nonlinear, and latent variables causal discovery. Proceedings
    of the Fourth Conference on Causal Learning and Reasoning. CLeaR: Conference on
    Causal Learning and Reasoning, PMLR, vol. 275, 552–605.'
  mla: 'Montagna, Francesco, et al. “Score Matching through the Roof: Linear, Nonlinear,
    and Latent Variables Causal Discovery.” <i>Proceedings of the Fourth Conference
    on Causal Learning and Reasoning</i>, vol. 275, ML Research Press, 2025, pp. 552–605.'
  short: F. Montagna, P. Faller, P. Blöbaum, E. Kirschbaum, F. Locatello, in:, Proceedings
    of the Fourth Conference on Causal Learning and Reasoning, ML Research Press,
    2025, pp. 552–605.
conference:
  end_date: 2025-05-09
  location: Lausanne, Switzerland
  name: 'CLeaR: Conference on Causal Learning and Reasoning'
  start_date: 2025-05-07
corr_author: '1'
date_created: 2026-01-29T14:19:09Z
date_published: 2025-05-01T00:00:00Z
date_updated: 2026-02-10T11:54:02Z
day: '01'
ddc:
- '000'
department:
- _id: FrLo
external_id:
  arxiv:
  - '2407.18755'
file:
- access_level: open_access
  checksum: f2bc44b2320667d4049b3518b1f2fe5d
  content_type: application/pdf
  creator: flocatel
  date_created: 2026-01-29T14:17:48Z
  date_updated: 2026-01-29T14:17:48Z
  file_id: '21067'
  file_name: montagna25a.pdf
  file_size: 1739334
  relation: main_file
  success: 1
file_date_updated: 2026-01-29T14:17:48Z
has_accepted_license: '1'
intvolume: '       275'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://proceedings.mlr.press/v275/montagna25a.html
month: '05'
oa: 1
oa_version: Published Version
page: 552-605
publication: Proceedings of the Fourth Conference on Causal Learning and Reasoning
publication_identifier:
  eissn:
  - 2640-3498
publication_status: published
publisher: ML Research Press
quality_controlled: '1'
status: public
title: 'Score matching through the roof: Linear, nonlinear, and latent variables causal
  discovery'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 275
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '21068'
abstract:
- lang: eng
  text: "Causal reasoning and discovery, two fundamental tasks of causal analysis,\r\noften
    face challenges in applications due to the complexity, noisiness, and highdimensionality
    of real-world data. Despite recent progress in identifying latent\r\ncausal structures
    using causal representation learning (CRL), what makes learned\r\nrepresentations
    useful for causal downstream tasks and how to evaluate them are\r\nstill not well
    understood. In this paper, we reinterpret CRL using a measurement\r\nmodel framework,
    where the learned representations are viewed as proxy measurements of the latent
    causal variables. Our approach clarifies the conditions under\r\nwhich learned
    representations support downstream causal reasoning and provides\r\na principled
    basis for quantitatively assessing the quality of representations using\r\na new
    Test-based Measurement EXclusivity (T-MEX) score. We validate T-MEX\r\nacross
    diverse causal inference scenarios, including numerical simulations and\r\nreal-world
    ecological video analysis, demonstrating that the proposed framework\r\nand corresponding
    score effectively assess the identification of learned representations and their
    usefulness for causal downstream tasks. Reproducible code can\r\nbe found at https://github.com/shimenghuang/a-measurement-perspective-of-crl."
acknowledgement: "This research was funded in whole or in part by the Austrian Science
  Fund (FWF) 10.55776/COE12. For open access purposes, the author has applied a CC
  BY public copyright license to any accepted manuscript version arising from this
  submission.\r\n"
alternative_title:
- Advances in Neural Information Processing Systems
article_processing_charge: No
arxiv: 1
author:
- first_name: Dingling
  full_name: Yao, Dingling
  id: d3e02e50-48a8-11ee-8f62-c108061797fa
  last_name: Yao
- first_name: Shimeng
  full_name: Huang, Shimeng
  id: 989c2a06-fb4e-11ef-a992-ab766442255b
  last_name: Huang
  orcid: 0000-0001-6919-821X
- first_name: Riccardo
  full_name: Cadei, Riccardo
  id: 0fa8b76f-72f0-11ef-b75a-a5da96e5ad6b
  last_name: Cadei
- first_name: Kun
  full_name: Zhang, Kun
  last_name: Zhang
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
citation:
  ama: 'Yao D, Huang S, Cadei R, Zhang K, Locatello F. The third pillar of causal
    analysis? A measurement perspective on causal representations. In: <i>39th Annual
    Conference on Neural Information Processing Systems</i>. Vol 38. Neural Information
    Processing Systems Foundation; 2025.'
  apa: 'Yao, D., Huang, S., Cadei, R., Zhang, K., &#38; Locatello, F. (2025). The
    third pillar of causal analysis? A measurement perspective on causal representations.
    In <i>39th Annual Conference on Neural Information Processing Systems</i> (Vol.
    38). San Diego, CA, United States: Neural Information Processing Systems Foundation.'
  chicago: Yao, Dingling, Shimeng Huang, Riccardo Cadei, Kun Zhang, and Francesco
    Locatello. “The Third Pillar of Causal Analysis? A Measurement Perspective on
    Causal Representations.” In <i>39th Annual Conference on Neural Information Processing
    Systems</i>, Vol. 38. Neural Information Processing Systems Foundation, 2025.
  ieee: D. Yao, S. Huang, R. Cadei, K. Zhang, and F. Locatello, “The third pillar
    of causal analysis? A measurement perspective on causal representations,” in <i>39th
    Annual Conference on Neural Information Processing Systems</i>, San Diego, CA,
    United States, 2025, vol. 38.
  ista: 'Yao D, Huang S, Cadei R, Zhang K, Locatello F. 2025. The third pillar of
    causal analysis? A measurement perspective on causal representations. 39th Annual
    Conference on Neural Information Processing Systems. NeurIPS: Neural Information
    Processing Systems, Advances in Neural Information Processing Systems, vol. 38.'
  mla: Yao, Dingling, et al. “The Third Pillar of Causal Analysis? A Measurement Perspective
    on Causal Representations.” <i>39th Annual Conference on Neural Information Processing
    Systems</i>, vol. 38, Neural Information Processing Systems Foundation, 2025.
  short: D. Yao, S. Huang, R. Cadei, K. Zhang, F. Locatello, in:, 39th Annual Conference
    on Neural Information Processing Systems, Neural Information Processing Systems
    Foundation, 2025.
conference:
  end_date: 2025-12-07
  location: San Diego, CA, United States
  name: 'NeurIPS: Neural Information Processing Systems'
  start_date: 2025-12-02
corr_author: '1'
date_created: 2026-01-29T14:24:56Z
date_published: 2025-12-15T00:00:00Z
date_updated: 2026-02-10T12:08:52Z
day: '15'
ddc:
- '000'
department:
- _id: FrLo
external_id:
  arxiv:
  - '2505.17708'
has_accepted_license: '1'
intvolume: '        38'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2505.17708
month: '12'
oa: 1
oa_version: Preprint
publication: 39th Annual Conference on Neural Information Processing Systems
publication_identifier:
  issn:
  - 1049-5258
publication_status: epub_ahead
publisher: Neural Information Processing Systems Foundation
quality_controlled: '1'
related_material:
  link:
  - relation: software
    url: https://github.com/shimenghuang/a-measurement-perspective-of-crl
status: public
title: The third pillar of causal analysis? A measurement perspective on causal representations
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 38
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '21070'
abstract:
- lang: eng
  text: 'Deep learning systems deployed in real-world applications often encounter
    data that is different from their in-distribution (ID). A reliable model should
    ideally abstain from making decisions in this out-of-distribution (OOD) setting.
    Existing state-of-the-art methods primarily focus on feature distances, such as
    k-th nearest neighbors and distances to decision boundaries, either overlooking
    or ineffectively using in-distribution statistics. In this work, we propose a
    novel angle-based metric for OOD detection that is computed relative to the in-distribution
    structure. We demonstrate that the angles between feature representations and
    decision boundaries, viewed from the mean of in-distribution features, serve as
    an effective discriminative factor between ID and OOD data. We evaluate our method
    on nine ImageNet-pretrained models. Our approach achieves the lowest FPR in 5
    out of 9 ImageNet models, obtains the best average FPR overall, and consistently
    ranking among the top 3 across all evaluated models. Furthermore, we highlight
    the benefits of contrastive representations by showing strong performance with
    ResNet SCL and CLIP architectures. Finally, we demonstrate that the scale-invariant
    nature of our score enables an ensemble strategy via simple score summation. '
acknowledgement: "This research was funded in whole or in part by the Austrian Science
  Fund (FWF) 10.55776/COE12. For open access purposes, the author has applied a CC
  BY public copyright license to any accepted manuscript version arising from this
  submission.\r\n"
alternative_title:
- Advances in Neural Information Processing Systems
article_processing_charge: No
arxiv: 1
author:
- first_name: Berker
  full_name: Demirel, Berker
  id: 8b4bc47f-3200-11ee-973b-8f0e7be21a9f
  last_name: Demirel
- first_name: 'Marco '
  full_name: 'Fumero, Marco '
  last_name: Fumero
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
citation:
  ama: 'Demirel B, Fumero M, Locatello F. Out-of-Distribution detection with relative
    angles. In: <i>39th Annual Conference on Neural Information Processing Systems</i>.
    Vol 38. Neural Information Processing Systems Foundation; 2025.'
  apa: 'Demirel, B., Fumero, M., &#38; Locatello, F. (2025). Out-of-Distribution detection
    with relative angles. In <i>39th Annual Conference on Neural Information Processing
    Systems</i> (Vol. 38). San Diego, CA, United States: Neural Information Processing
    Systems Foundation.'
  chicago: Demirel, Berker, Marco  Fumero, and Francesco Locatello. “Out-of-Distribution
    Detection with Relative Angles.” In <i>39th Annual Conference on Neural Information
    Processing Systems</i>, Vol. 38. Neural Information Processing Systems Foundation,
    2025.
  ieee: B. Demirel, M. Fumero, and F. Locatello, “Out-of-Distribution detection with
    relative angles,” in <i>39th Annual Conference on Neural Information Processing
    Systems</i>, San Diego, CA, United States, 2025, vol. 38.
  ista: 'Demirel B, Fumero M, Locatello F. 2025. Out-of-Distribution detection with
    relative angles. 39th Annual Conference on Neural Information Processing Systems.
    NeurIPS: Neural Information Processing Systems, Advances in Neural Information
    Processing Systems, vol. 38.'
  mla: Demirel, Berker, et al. “Out-of-Distribution Detection with Relative Angles.”
    <i>39th Annual Conference on Neural Information Processing Systems</i>, vol. 38,
    Neural Information Processing Systems Foundation, 2025.
  short: B. Demirel, M. Fumero, F. Locatello, in:, 39th Annual Conference on Neural
    Information Processing Systems, Neural Information Processing Systems Foundation,
    2025.
conference:
  end_date: 2025-12-07
  location: San Diego, CA, United States
  name: 'NeurIPS: Neural Information Processing Systems'
  start_date: 2025-12-02
corr_author: '1'
date_created: 2026-01-29T14:26:47Z
date_published: 2025-12-01T00:00:00Z
date_updated: 2026-02-16T11:38:25Z
day: '01'
ddc:
- '000'
department:
- _id: FrLo
external_id:
  arxiv:
  - '2410.04525'
has_accepted_license: '1'
intvolume: '        38'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2410.04525
month: '12'
oa: 1
oa_version: Preprint
publication: 39th Annual Conference on Neural Information Processing Systems
publication_identifier:
  issn:
  - 1049-5258
publication_status: epub_ahead
publisher: Neural Information Processing Systems Foundation
quality_controlled: '1'
related_material:
  link:
  - relation: software
    url: https://github.com/berkerdemirel/ORA-OOD-Detection-with-Relative-Angles
status: public
title: Out-of-Distribution detection with relative angles
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 38
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '21072'
abstract:
- lang: eng
  text: Language and vision-language models have shown impressive performance across
    a wide range of tasks, but their internal mechanisms remain only partly understood.
    In this work, we study how individual attention heads in text-generative models
    specialize in specific semantic or visual attributes. Building on an established
    interpretability method, we reinterpret the practice of probing intermediate activations
    with the final decoding layer through the lens of signal processing. This lets
    us analyze multiple samples in a principled way and rank attention heads based
    on their relevance to target concepts. Our results show consistent patterns of
    specialization at the head level across both unimodal and multimodal transformers.
    Remarkably, we find that editing as few as 1% of the heads, selected using our
    method, can reliably suppress or enhance targeted concepts in the model output.
    We validate our approach on language tasks such as question answering and toxicity
    mitigation, as well as vision-language tasks including image classification and
    captioning. Our findings highlight an interpretable and controllable structure
    within attention layers, offering simple tools for understanding and editing large-scale
    generative models.
acknowledgement: 'The authors acknowledge the Area Science Park supercomputing platform
  ORFEO made available for conducting the research reported in this paper, and the
  technical support of the Laboratory of Data Engineering staff. LB, DD and AC were
  supported by the project “Supporto alla diagnosi di malattie rare tramite l’intelligenza
  artificiale" CUP: F53C22001770002 and “Valutazione automatica delle immagini diagnostiche
  tramite l’intelligenza artificiale", CUP: F53C22001780002. LB was supported by the
  European Union – NextGenerationEU within the project PNRR “Finanziamento di progetti
  presentati da giovani ricercatori" - Mission 4 Component 2 Investment 1.2, CUP:
  J93C25000440001. AC was supported by the European Union – NextGenerationEU within
  the project PNRR “PRP@CERIC" IR0000028 - Mission 4 Component 2 Investment 3.1 Action
  3.1.1. '
article_processing_charge: No
arxiv: 1
author:
- first_name: Lorenzo
  full_name: Basile, Lorenzo
  last_name: Basile
- first_name: Valentino
  full_name: Maiorca, Valentino
  last_name: Maiorca
- first_name: Diego
  full_name: Doimo, Diego
  last_name: Doimo
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
- first_name: Alberto
  full_name: Cazzaniga, Alberto
  last_name: Cazzaniga
citation:
  ama: 'Basile L, Maiorca V, Doimo D, Locatello F, Cazzaniga A. Head pursuit: Probing
    attention specialization in multimodal transformers. In: <i>39th Annual Conference
    on Neural Information Processing Systems</i>. Vol 38. Neural Information Processing
    Systems Foundation; 2025.'
  apa: 'Basile, L., Maiorca, V., Doimo, D., Locatello, F., &#38; Cazzaniga, A. (2025).
    Head pursuit: Probing attention specialization in multimodal transformers. In
    <i>39th Annual Conference on Neural Information Processing Systems</i> (Vol. 38).
    San Diego, CA, United States: Neural Information Processing Systems Foundation.'
  chicago: 'Basile, Lorenzo, Valentino Maiorca, Diego Doimo, Francesco Locatello,
    and Alberto Cazzaniga. “Head Pursuit: Probing Attention Specialization in Multimodal
    Transformers.” In <i>39th Annual Conference on Neural Information Processing Systems</i>,
    Vol. 38. Neural Information Processing Systems Foundation, 2025.'
  ieee: 'L. Basile, V. Maiorca, D. Doimo, F. Locatello, and A. Cazzaniga, “Head pursuit:
    Probing attention specialization in multimodal transformers,” in <i>39th Annual
    Conference on Neural Information Processing Systems</i>, San Diego, CA, United
    States, 2025, vol. 38.'
  ista: 'Basile L, Maiorca V, Doimo D, Locatello F, Cazzaniga A. 2025. Head pursuit:
    Probing attention specialization in multimodal transformers. 39th Annual Conference
    on Neural Information Processing Systems. NeurIPS: Neural Information Processing
    Systems vol. 38.'
  mla: 'Basile, Lorenzo, et al. “Head Pursuit: Probing Attention Specialization in
    Multimodal Transformers.” <i>39th Annual Conference on Neural Information Processing
    Systems</i>, vol. 38, Neural Information Processing Systems Foundation, 2025.'
  short: L. Basile, V. Maiorca, D. Doimo, F. Locatello, A. Cazzaniga, in:, 39th Annual
    Conference on Neural Information Processing Systems, Neural Information Processing
    Systems Foundation, 2025.
conference:
  end_date: 2025-12-07
  location: San Diego, CA, United States
  name: 'NeurIPS: Neural Information Processing Systems'
  start_date: 2025-12-02
date_created: 2026-01-29T14:29:23Z
date_published: 2025-12-15T00:00:00Z
date_updated: 2026-02-11T08:55:36Z
day: '15'
ddc:
- '000'
department:
- _id: FrLo
external_id:
  arxiv:
  - '2510.21518'
file:
- access_level: open_access
  checksum: 85be3f98663e2595cf37001852b477cb
  content_type: application/pdf
  creator: flocatel
  date_created: 2026-01-29T14:29:14Z
  date_updated: 2026-01-29T14:29:14Z
  file_id: '21073'
  file_name: 2510.21518v2.pdf
  file_size: 4271547
  relation: main_file
  success: 1
file_date_updated: 2026-01-29T14:29:14Z
has_accepted_license: '1'
intvolume: '        38'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2510.21518
month: '12'
oa: 1
oa_version: Preprint
publication: 39th Annual Conference on Neural Information Processing Systems
publication_identifier:
  issn:
  - 1049-5258
publication_status: epub_ahead
publisher: Neural Information Processing Systems Foundation
quality_controlled: '1'
status: public
title: 'Head pursuit: Probing attention specialization in multimodal transformers'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 38
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '21074'
abstract:
- lang: eng
  text: Neural models learn representations of high-dimensional data on low-dimensional
    manifolds. Multiple factors, including stochasticities in the training process,
    model architectures, and additional inductive biases, may induce different representations,
    even when learning the same task on the same data. However, it has recently been
    shown that when a latent structure is shared between distinct latent spaces, relative
    distances between representations can be preserved, up to distortions. Building
    on this idea, we demonstrate that exploiting the differential-geometric structure
    of latent spaces of neural models, it is possible to capture precisely the transformations
    between representational spaces trained on similar data distributions. Specifically,
    we assume that distinct neural models parametrize approximately the same underlying
    manifold, and introduce a representation based on the pullback metric that captures
    the intrinsic structure of the latent space, while scaling efficiently to large
    models. We validate experimentally our method on model stitching and retrieval
    tasks, covering autoencoders and vision foundation discriminative models, across
    diverse architectures, datasets, pretraining schemes and modalities. Code is available
    at the following link.
acknowledgement: 'We thank Gregor Krzmanc, German Magai, Vital Fernandez for insightful
  discussions in the early stages of the project. HY was supported by the Research
  Council of Finland Flagship programme: Finnish Center for Artificial Intelligence
  FCAI. HY wishes to acknowledge CSC - IT Center for Science, Finland, for computational
  resources. GA was supported by the DFF Sapere Aude Starting Grant “GADL”. SH was
  supported by a research grant (42062) from VILLUM FONDEN and partly funded by the
  Novo Nordisk Foundation through the Center for Basic Research in Life Science (NNF20OC0062606).
  SH received funding from the European Research Council (ERC) under the European
  Union’s Horizon Programme (grant agreement 101125003). MF is supported by the MSCA
  IST-Bridge fellowship which has received funding from the European Union’s Horizon
  2020 research and innovation program under the Marie Skłodowska-Curie grant agreement
  No 101034413.'
alternative_title:
- Advances in Neural Information Processing Systems
article_processing_charge: No
arxiv: 1
author:
- first_name: Hanlin
  full_name: Yu, Hanlin
  last_name: Yu
- first_name: Befrin
  full_name: Inal, Befrin
  last_name: Inal
- first_name: Georgios
  full_name: Arvanitidis, Georgios
  last_name: Arvanitidis
- first_name: Soren
  full_name: Hauberg, Soren
  last_name: Hauberg
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
- first_name: Marco
  full_name: Fumero, Marco
  id: 1c1593eb-393f-11ef-bb8e-ab4f1e979650
  last_name: Fumero
citation:
  ama: 'Yu H, Inal B, Arvanitidis G, Hauberg S, Locatello F, Fumero M. Connecting
    neural models latent geometries with relative geodesic representations. In: <i>39th
    Annual Conference on Neural Information Processing Systems</i>. Vol 38. Neural
    Information Processing Systems Foundation; 2025.'
  apa: 'Yu, H., Inal, B., Arvanitidis, G., Hauberg, S., Locatello, F., &#38; Fumero,
    M. (2025). Connecting neural models latent geometries with relative geodesic representations.
    In <i>39th Annual Conference on Neural Information Processing Systems</i> (Vol.
    38). San Diego, CA, United States: Neural Information Processing Systems Foundation.'
  chicago: Yu, Hanlin, Befrin Inal, Georgios Arvanitidis, Soren Hauberg, Francesco
    Locatello, and Marco Fumero. “Connecting Neural Models Latent Geometries with
    Relative Geodesic Representations.” In <i>39th Annual Conference on Neural Information
    Processing Systems</i>, Vol. 38. Neural Information Processing Systems Foundation,
    2025.
  ieee: H. Yu, B. Inal, G. Arvanitidis, S. Hauberg, F. Locatello, and M. Fumero, “Connecting
    neural models latent geometries with relative geodesic representations,” in <i>39th
    Annual Conference on Neural Information Processing Systems</i>, San Diego, CA,
    United States, 2025, vol. 38.
  ista: 'Yu H, Inal B, Arvanitidis G, Hauberg S, Locatello F, Fumero M. 2025. Connecting
    neural models latent geometries with relative geodesic representations. 39th Annual
    Conference on Neural Information Processing Systems. NeurIPS: Neural Information
    Processing Systems, Advances in Neural Information Processing Systems, vol. 38.'
  mla: Yu, Hanlin, et al. “Connecting Neural Models Latent Geometries with Relative
    Geodesic Representations.” <i>39th Annual Conference on Neural Information Processing
    Systems</i>, vol. 38, Neural Information Processing Systems Foundation, 2025.
  short: H. Yu, B. Inal, G. Arvanitidis, S. Hauberg, F. Locatello, M. Fumero, in:,
    39th Annual Conference on Neural Information Processing Systems, Neural Information
    Processing Systems Foundation, 2025.
conference:
  end_date: 2025-12-07
  location: San Diego, CA, United States
  name: 'NeurIPS: Neural Information Processing Systems'
  start_date: 2025-12-02
corr_author: '1'
date_created: 2026-01-29T14:31:52Z
date_published: 2025-12-15T00:00:00Z
date_updated: 2026-02-11T09:03:37Z
day: '15'
ddc:
- '000'
department:
- _id: FrLo
ec_funded: 1
external_id:
  arxiv:
  - '2506.01599'
file:
- access_level: open_access
  checksum: b1a645418025f46394764cd16d0cb089
  content_type: application/pdf
  creator: flocatel
  date_created: 2026-01-29T14:31:42Z
  date_updated: 2026-01-29T14:31:42Z
  file_id: '21075'
  file_name: 2506.01599v2.pdf
  file_size: 7749349
  relation: main_file
  success: 1
file_date_updated: 2026-01-29T14:31:42Z
has_accepted_license: '1'
intvolume: '        38'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
  call_identifier: H2020
  grant_number: '101034413'
  name: 'IST-BRIDGE: International postdoctoral program'
publication: 39th Annual Conference on Neural Information Processing Systems
publication_identifier:
  issn:
  - 1049-5258
publication_status: epub_ahead
publisher: Neural Information Processing Systems Foundation
quality_controlled: '1'
status: public
title: Connecting neural models latent geometries with relative geodesic representations
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 38
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '21076'
abstract:
- lang: eng
  text: In many scientific experiments, the data annotating cost constraints the pace
    for testing novel hypotheses. Yet, modern machine learning pipelines offer a promising
    solution—provided their predictions yield correct conclusions. We focus on Prediction-Powered
    Causal Inferences (PPCI), i.e., estimating the treatment effect in an unlabeled
    target experiment, relying on training data with the same outcome annotated but
    potentially different treatment or effect modifiers. We first show that conditional
    calibration guarantees valid PPCI at population level. Then, we introduce a sufficient
    representation constraint transferring validity across experiments, which we propose
    to enforce in practice in Deconfounded Empirical Risk Minimization, our new model-agnostic
    training objective. We validate our method on synthetic and real-world scientific
    data, solving impossible problem instances for Empirical Risk Minimization even
    with standard invariance constraints. In particular, for the first time, we achieve
    valid causal inference on a scientific experiment with complex recording and no
    human annotations, fine-tuning a foundational model on our similar annotated experiment.
acknowledgement: We thank the Causal Learning and Artificial Intelligence group at
  ISTA for the continuous feedback on the project and valuable discussions. We thank
  the Social Immunity group at ISTA, particularly Jinook Oh, for the annotation program
  and Michaela Hoenigsberger for supporting our ecological experiment. Riccardo Cadei
  is supported by a Google Research Scholar Award and a Google Initiated Gift to Francesco
  Locatello. This research was funded in part by the Austrian Science Fund (FWF) 10.55776/COE12).
  It was further partially supported by the ISTA Interdisciplinary Project Committee
  for the collaborative project “ALED” between Francesco Locatello and Sylvia Cremer.
  For open access purposes, the author has applied a CC BY public copyright license
  to any author accepted manuscript version arising from this submission.
alternative_title:
- Advances in Neural Information Processing Systems
article_processing_charge: No
author:
- first_name: Riccardo
  full_name: Cadei, Riccardo
  id: 0fa8b76f-72f0-11ef-b75a-a5da96e5ad6b
  last_name: Cadei
- first_name: Ilker
  full_name: Demirel, Ilker
  last_name: Demirel
- first_name: Piersilvio
  full_name: De Bartolomeis, Piersilvio
  last_name: De Bartolomeis
- first_name: Lukas
  full_name: Lindorfer, Lukas
  id: 85f0e6d3-06b3-11ec-8982-8c5049fa4455
  last_name: Lindorfer
- first_name: Sylvia
  full_name: Cremer, Sylvia
  id: 2F64EC8C-F248-11E8-B48F-1D18A9856A87
  last_name: Cremer
  orcid: 0000-0002-2193-3868
- first_name: Cordelia
  full_name: Schmid, Cordelia
  last_name: Schmid
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
citation:
  ama: 'Cadei R, Demirel I, De Bartolomeis P, et al. Prediction-powered causal inferences.
    In: <i>39th Annual Conference on Neural Information Processing Systems</i>. Vol
    38. Neural Information Processing Systems Foundation; 2025.'
  apa: 'Cadei, R., Demirel, I., De Bartolomeis, P., Lindorfer, L., Cremer, S., Schmid,
    C., &#38; Locatello, F. (2025). Prediction-powered causal inferences. In <i>39th
    Annual Conference on Neural Information Processing Systems</i> (Vol. 38). San
    Diego, CA, United States: Neural Information Processing Systems Foundation.'
  chicago: Cadei, Riccardo, Ilker Demirel, Piersilvio De Bartolomeis, Lukas Lindorfer,
    Sylvia Cremer, Cordelia Schmid, and Francesco Locatello. “Prediction-Powered Causal
    Inferences.” In <i>39th Annual Conference on Neural Information Processing Systems</i>,
    Vol. 38. Neural Information Processing Systems Foundation, 2025.
  ieee: R. Cadei <i>et al.</i>, “Prediction-powered causal inferences,” in <i>39th
    Annual Conference on Neural Information Processing Systems</i>, San Diego, CA,
    United States, 2025, vol. 38.
  ista: 'Cadei R, Demirel I, De Bartolomeis P, Lindorfer L, Cremer S, Schmid C, Locatello
    F. 2025. Prediction-powered causal inferences. 39th Annual Conference on Neural
    Information Processing Systems. NeurIPS: Neural Information Processing Systems,
    Advances in Neural Information Processing Systems, vol. 38.'
  mla: Cadei, Riccardo, et al. “Prediction-Powered Causal Inferences.” <i>39th Annual
    Conference on Neural Information Processing Systems</i>, vol. 38, Neural Information
    Processing Systems Foundation, 2025.
  short: R. Cadei, I. Demirel, P. De Bartolomeis, L. Lindorfer, S. Cremer, C. Schmid,
    F. Locatello, in:, 39th Annual Conference on Neural Information Processing Systems,
    Neural Information Processing Systems Foundation, 2025.
conference:
  end_date: 2025-12-07
  location: San Diego, CA, United States
  name: 'NeurIPS: Neural Information Processing Systems'
  start_date: 2025-12-02
date_created: 2026-01-29T14:35:11Z
date_published: 2025-12-15T00:00:00Z
date_updated: 2026-02-16T11:39:33Z
day: '15'
ddc:
- '000'
department:
- _id: FrLo
- _id: SyCr
file:
- access_level: open_access
  checksum: 92467fa566cd36671a6a3b9e71ae0f71
  content_type: application/pdf
  creator: flocatel
  date_created: 2026-01-29T14:35:02Z
  date_updated: 2026-01-29T14:35:02Z
  file_id: '21077'
  file_name: 17546_Prediction_Powered_Causa.pdf
  file_size: 8489023
  relation: main_file
  success: 1
file_date_updated: 2026-01-29T14:35:02Z
has_accepted_license: '1'
intvolume: '        38'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
publication: 39th Annual Conference on Neural Information Processing Systems
publication_identifier:
  issn:
  - 1049-5258
publication_status: epub_ahead
publisher: Neural Information Processing Systems Foundation
quality_controlled: '1'
status: public
title: Prediction-powered causal inferences
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 38
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '21089'
abstract:
- lang: eng
  text: 'Hypertrace logic is a sorted first-order logic with separate sorts for time
    and execution traces. Its formulas specify hyperproperties, which are properties
    relating multiple traces. In this work, we extend hypertrace logic by introducing
    trace quantifiers that range over the set of all possible traces. In this extended
    logic, formulas can quantify over two kinds of trace variables: constrained trace
    variables, which range over a fixed set of traces defined by the model, and unconstrained
    trace variables, which can be assigned to any trace. In comparison, hyperlogics
    such as HyperLTL have only constrained trace quantifiers. We use hypertrace logic
    to study how different quantifier patterns affect the decidability of the satisfiability
    problem. We prove that hypertrace logic without constrained trace quantifiers
    is equivalent to monadic second-order logic of one successor (S1S), and therefore
    satisfiable, and that the trace-prefixed fragment (all trace quantifiers precede
    all time quantifiers) is equivalent to HyperQPTL. Moreover, we show that all hypertrace
    formulas where the only alternation between constrained trace quantifiers is from
    an existential to a universal quantifier are equisatisfiable to formulas without
    constraints on their trace variables and, therefore, decidable as well. Our framework
    allows us to study also time-prefixed hyperlogics, for which we provide new decidability
    and undecidability results.'
acknowledgement: This work was supported in part by the Austrian Science Fund (FWF)
  SFB project SpyCoDe 10.55776/F85 and by the ERC Advanced Grant VAMOS 101020093.
alternative_title:
- LIPIcs
article_processing_charge: No
arxiv: 1
author:
- first_name: Marek
  full_name: Chalupa, Marek
  id: 87e34708-d6c6-11ec-9f5b-9391e7be2463
  last_name: Chalupa
- first_name: Thomas A
  full_name: Henzinger, Thomas A
  id: 40876CD8-F248-11E8-B48F-1D18A9856A87
  last_name: Henzinger
  orcid: 0000-0002-2985-7724
- first_name: Ana A
  full_name: Oliveira da Costa, Ana A
  id: 8b282559-50b0-11ef-861e-d6ace0d92e9b
  last_name: Oliveira da Costa
citation:
  ama: 'Chalupa M, Henzinger TA, Oliveira da Costa AA. Flavors of quantifiers in hyperlogics.
    In: <i>45th Annual Conference on Foundations of Software Technology and Theoretical
    Computer Science</i>. Vol 360. Schloss Dagstuhl - Leibniz-Zentrum für Informatik;
    2025:20:1-20:18. doi:<a href="https://doi.org/10.4230/LIPICS.FSTTCS.2025.20">10.4230/LIPICS.FSTTCS.2025.20</a>'
  apa: 'Chalupa, M., Henzinger, T. A., &#38; Oliveira da Costa, A. A. (2025). Flavors
    of quantifiers in hyperlogics. In <i>45th Annual Conference on Foundations of
    Software Technology and Theoretical Computer Science</i> (Vol. 360, p. 20:1-20:18).
    Pilani, India: Schloss Dagstuhl - Leibniz-Zentrum für Informatik. <a href="https://doi.org/10.4230/LIPICS.FSTTCS.2025.20">https://doi.org/10.4230/LIPICS.FSTTCS.2025.20</a>'
  chicago: Chalupa, Marek, Thomas A Henzinger, and Ana A Oliveira da Costa. “Flavors
    of Quantifiers in Hyperlogics.” In <i>45th Annual Conference on Foundations of
    Software Technology and Theoretical Computer Science</i>, 360:20:1-20:18. Schloss
    Dagstuhl - Leibniz-Zentrum für Informatik, 2025. <a href="https://doi.org/10.4230/LIPICS.FSTTCS.2025.20">https://doi.org/10.4230/LIPICS.FSTTCS.2025.20</a>.
  ieee: M. Chalupa, T. A. Henzinger, and A. A. Oliveira da Costa, “Flavors of quantifiers
    in hyperlogics,” in <i>45th Annual Conference on Foundations of Software Technology
    and Theoretical Computer Science</i>, Pilani, India, 2025, vol. 360, p. 20:1-20:18.
  ista: 'Chalupa M, Henzinger TA, Oliveira da Costa AA. 2025. Flavors of quantifiers
    in hyperlogics. 45th Annual Conference on Foundations of Software Technology and
    Theoretical Computer Science. FSTTCS: Conference on Foundations of Software Technology
    and Theoretical Computer Science, LIPIcs, vol. 360, 20:1-20:18.'
  mla: Chalupa, Marek, et al. “Flavors of Quantifiers in Hyperlogics.” <i>45th Annual
    Conference on Foundations of Software Technology and Theoretical Computer Science</i>,
    vol. 360, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2025, p. 20:1-20:18,
    doi:<a href="https://doi.org/10.4230/LIPICS.FSTTCS.2025.20">10.4230/LIPICS.FSTTCS.2025.20</a>.
  short: M. Chalupa, T.A. Henzinger, A.A. Oliveira da Costa, in:, 45th Annual Conference
    on Foundations of Software Technology and Theoretical Computer Science, Schloss
    Dagstuhl - Leibniz-Zentrum für Informatik, 2025, p. 20:1-20:18.
conference:
  end_date: 2025-12-19
  location: Pilani, India
  name: 'FSTTCS: Conference on Foundations of Software Technology and Theoretical
    Computer Science'
  start_date: 2025-12-17
corr_author: '1'
date_created: 2026-01-29T15:39:15Z
date_published: 2025-12-09T00:00:00Z
date_updated: 2026-02-11T09:35:04Z
day: '09'
ddc:
- '000'
department:
- _id: ToHe
doi: 10.4230/LIPICS.FSTTCS.2025.20
ec_funded: 1
external_id:
  arxiv:
  - '2510.12298'
file:
- access_level: open_access
  checksum: 8188ee5c7b14193d48eeb655e9bbdc47
  content_type: application/pdf
  creator: dernst
  date_created: 2026-02-11T09:33:20Z
  date_updated: 2026-02-11T09:33:20Z
  file_id: '21213'
  file_name: 2025_LIPIcS_Chalupa.pdf
  file_size: 933970
  relation: main_file
  success: 1
file_date_updated: 2026-02-11T09:33:20Z
has_accepted_license: '1'
intvolume: '       360'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
page: 20:1-20:18
project:
- _id: 34a1b658-11ca-11ed-8bc3-c75229f0241e
  grant_number: F8502
  name: Interface Theory for Security and Privacy
- _id: 62781420-2b32-11ec-9570-8d9b63373d4d
  call_identifier: H2020
  grant_number: '101020093'
  name: Vigilant Algorithmic Monitoring of Software
publication: 45th Annual Conference on Foundations of Software Technology and Theoretical
  Computer Science
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
quality_controlled: '1'
scopus_import: '1'
status: public
title: Flavors of quantifiers in hyperlogics
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 360
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '21090'
abstract:
- lang: eng
  text: Fairness in AI is traditionally studied as a static property evaluated once,
    over a fixed dataset. However, real-world AI systems operate sequentially, with
    outcomes and environments evolving over time. This paper proposes a framework
    for analysing fairness as a runtime property. Using a minimal yet expressive model
    based on sequences of coin tosses with possibly evolving biases, we study the
    problems of monitoring and enforcing fairness expressed in either toss outcomes
    or coin biases. Since there is no one-size-fits-all solution for either problem,
    we provide a summary of monitoring and enforcement strategies, parametrised by
    environment dynamics, prediction horizon, and confidence thresholds. For both
    problems, we present general results under simple or minimal assumptions. We survey
    existing solutions for the monitoring problem for Markovian and additive dynamics,
    and existing solutions for the enforcement problem in static settings with known
    dynamics.
acknowledgement: 'This work is supported by the European Research Council under Grant
  No.: ERC-2020-AdG 101020093.'
alternative_title:
- LNCS
article_processing_charge: No
arxiv: 1
author:
- first_name: Filip
  full_name: Cano Cordoba, Filip
  id: 708cad98-e86a-11ef-8098-bdae2d7c6af1
  last_name: Cano Cordoba
  orcid: 0000-0002-0783-904X
- first_name: Thomas A
  full_name: Henzinger, Thomas A
  id: 40876CD8-F248-11E8-B48F-1D18A9856A87
  last_name: Henzinger
  orcid: 0000-0002-2985-7724
- first_name: Konstantin
  full_name: Kueffner, Konstantin
  id: 8121a2d0-dc85-11ea-9058-af578f3b4515
  last_name: Kueffner
  orcid: 0000-0001-8974-2542
citation:
  ama: 'Cano Cordoba F, Henzinger TA, Kueffner K. Algorithmic fairness: A runtime
    perspective. In: <i>25th International Conference on Runtime Verification</i>.
    Vol 16087. Springer Nature; 2025:1-21. doi:<a href="https://doi.org/10.1007/978-3-032-05435-7_1">10.1007/978-3-032-05435-7_1</a>'
  apa: 'Cano Cordoba, F., Henzinger, T. A., &#38; Kueffner, K. (2025). Algorithmic
    fairness: A runtime perspective. In <i>25th International Conference on Runtime
    Verification</i> (Vol. 16087, pp. 1–21). Graz, Austria: Springer Nature. <a href="https://doi.org/10.1007/978-3-032-05435-7_1">https://doi.org/10.1007/978-3-032-05435-7_1</a>'
  chicago: 'Cano Cordoba, Filip, Thomas A Henzinger, and Konstantin Kueffner. “Algorithmic
    Fairness: A Runtime Perspective.” In <i>25th International Conference on Runtime
    Verification</i>, 16087:1–21. Springer Nature, 2025. <a href="https://doi.org/10.1007/978-3-032-05435-7_1">https://doi.org/10.1007/978-3-032-05435-7_1</a>.'
  ieee: 'F. Cano Cordoba, T. A. Henzinger, and K. Kueffner, “Algorithmic fairness:
    A runtime perspective,” in <i>25th International Conference on Runtime Verification</i>,
    Graz, Austria, 2025, vol. 16087, pp. 1–21.'
  ista: 'Cano Cordoba F, Henzinger TA, Kueffner K. 2025. Algorithmic fairness: A runtime
    perspective. 25th International Conference on Runtime Verification. RV: Runtime
    Verification, LNCS, vol. 16087, 1–21.'
  mla: 'Cano Cordoba, Filip, et al. “Algorithmic Fairness: A Runtime Perspective.”
    <i>25th International Conference on Runtime Verification</i>, vol. 16087, Springer
    Nature, 2025, pp. 1–21, doi:<a href="https://doi.org/10.1007/978-3-032-05435-7_1">10.1007/978-3-032-05435-7_1</a>.'
  short: F. Cano Cordoba, T.A. Henzinger, K. Kueffner, in:, 25th International Conference
    on Runtime Verification, Springer Nature, 2025, pp. 1–21.
conference:
  end_date: 2025-09-19
  location: Graz, Austria
  name: 'RV: Runtime Verification'
  start_date: 2025-09-15
corr_author: '1'
date_created: 2026-01-29T16:01:41Z
date_published: 2025-09-13T00:00:00Z
date_updated: 2026-02-16T11:57:00Z
day: '13'
department:
- _id: ToHe
doi: 10.1007/978-3-032-05435-7_1
ec_funded: 1
external_id:
  arxiv:
  - '2507.20711'
intvolume: '     16087'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2507.20711
month: '09'
oa: 1
oa_version: Preprint
page: 1-21
project:
- _id: 62781420-2b32-11ec-9570-8d9b63373d4d
  call_identifier: H2020
  grant_number: '101020093'
  name: Vigilant Algorithmic Monitoring of Software
publication: 25th International Conference on Runtime Verification
publication_identifier:
  eisbn:
  - '9783032054357'
  eissn:
  - 1611-3349
  issn:
  - 0302-9743
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
status: public
title: 'Algorithmic fairness: A runtime perspective'
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 16087
year: '2025'
...
