---
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '20934'
abstract:
- lang: eng
text: ' Supervised learning for causal discovery from observational data often achieves
competitive performance despite seemingly avoiding the explicit assumptions that
traditional methods require for identifiability. In this work, we analyze CSIvA
(Ke et al., 2023) on bivariate causal models, a transformer architecture for amortized
inference promising to train on synthetic data and transfer to real ones. First,
we bridge the gap with identifiability theory, showing that the training distribution
implicitly defines a prior on the causal model of the test observations: consistent
with classical approaches, good performance is achieved when we have a good prior
on the test data, and the underlying model is identifiable. Second, we find that
CSIvA can not generalize to classes of causal models unseen during training: to
overcome this limitation, we theoretically and empirically analyze \textit{when}
training CSIvA on datasets generated by multiple identifiable causal models with
different structural assumptions improves its generalization at test time. Overall,
we find that amortized causal discovery still adheres to identifiability theory,
violating the previous hypothesis from Lopez-Paz et al. (2015) that supervised
learning methods could overcome its restrictions.'
alternative_title:
- TMLR
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Francesco
full_name: Montagna, Francesco
id: 353afc8e-19f4-11f0-9db9-811f1723c83f
last_name: Montagna
- first_name: Maximilian T
full_name: Cairney-Leeming, Maximilian T
id: 2214a80c-31f8-11ee-a48d-cf52cc58759b
last_name: Cairney-Leeming
- first_name: Dhanya
full_name: Sridhar, Dhanya
last_name: Sridhar
- 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, Cairney-Leeming MT, Sridhar D, Locatello F. Demystifying amortized
causal discovery with transformers. Transactions on Machine Learning Research.
2025.
apa: Montagna, F., Cairney-Leeming, M. T., Sridhar, D., & Locatello, F. (2025).
Demystifying amortized causal discovery with transformers. Transactions on
Machine Learning Research. ML Research Press.
chicago: Montagna, Francesco, Maximilian T Cairney-Leeming, Dhanya Sridhar, and
Francesco Locatello. “Demystifying Amortized Causal Discovery with Transformers.”
Transactions on Machine Learning Research. ML Research Press, 2025.
ieee: F. Montagna, M. T. Cairney-Leeming, D. Sridhar, and F. Locatello, “Demystifying
amortized causal discovery with transformers,” Transactions on Machine Learning
Research. ML Research Press, 2025.
ista: Montagna F, Cairney-Leeming MT, Sridhar D, Locatello F. 2025. Demystifying
amortized causal discovery with transformers. Transactions on Machine Learning
Research.
mla: Montagna, Francesco, et al. “Demystifying Amortized Causal Discovery with Transformers.”
Transactions on Machine Learning Research, ML Research Press, 2025.
short: F. Montagna, M.T. Cairney-Leeming, D. Sridhar, F. Locatello, Transactions
on Machine Learning Research (2025).
corr_author: '1'
date_created: 2026-01-04T23:01:35Z
date_published: 2025-12-18T00:00:00Z
date_updated: 2026-01-05T09:54:59Z
day: '18'
ddc:
- '000'
department:
- _id: FrLo
external_id:
arxiv:
- '2405.16924'
file:
- access_level: open_access
checksum: 968c471bb1f682cf823b2d4cadea8a3f
content_type: application/pdf
creator: dernst
date_created: 2026-01-05T09:51:28Z
date_updated: 2026-01-05T09:51:28Z
file_id: '20939'
file_name: 2025_PMLR_Montagna.pdf
file_size: 1030280
relation: main_file
success: 1
file_date_updated: 2026-01-05T09:51:28Z
has_accepted_license: '1'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
publication: Transactions on Machine Learning Research
publication_identifier:
eissn:
- 2835-8856
publication_status: published
publisher: ML Research Press
quality_controlled: '1'
related_material:
link:
- relation: software
url: https://github.com/francescomontagna/learning-to-induce.git
scopus_import: '1'
status: public
title: Demystifying amortized causal discovery with 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: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '20935'
abstract:
- lang: eng
text: In situ cryo-electron tomography (cryo-ET) has emerged as the method of choice
to investigate the structures of biomolecules in their native context. However,
challenges remain for the efficient production and sharing of large-scale cryo-ET
datasets. Here, we combined cryogenic plasma-based focused ion beam (cryo-PFIB)
milling with recent advances in cryo-ET acquisition and processing to generate
a dataset of 1,829 annotated tomograms of the green alga Chlamydomonas reinhardtii,
which we provide as a community resource to drive method development and inspire
biological discovery. To assay data quality, we performed subtomogram averaging
of both soluble and membrane-bound complexes ranging in size from >3 MDa to ∼200
kDa, including 80S ribosomes, Rubisco, nucleosomes, microtubules, clathrin, photosystem
II, and mitochondrial ATP synthase. The majority of these density maps reached
sub-nanometer resolution, demonstrating the potential of this C. reinhardtii dataset
as well as the promise of modern cryo-ET workflows and open data sharing to empower
visual proteomics.
acknowledgement: Calculations were performed at the Max Planck Institute of Biochemistry
and the Raven Supercomputer of the Max Planck Computing and Data Facility (MPCDF)
in Garching, Germany; at the sciCORE (http://scicore.unibas.ch/) scientific computing
center at the University of Basel, Switzerland; and at Thermo Fisher Scientific,
in Eindhoven, the Netherlands. This work was supported by Thermo Fisher Scientific.
All lamella preparations and tilt-series collections used in this work were conducted
at Thermo Fisher R&D facilities in Brno and Eindhoven, utilizing Arctis and Krios
microscopes. This work was also supported by the ERC consolidator grant “cryOcean”
(fulfilled by the Swiss State Secretariat for Education, Research and Innovation,
M822.00045) as well as a Swiss Nanoscience Institute PhD school grant to B.D.E.
and P.V.d.S., an EMBO long-term postdoctoral fellowship (ALTF-383-2022) to G.T.,
an SNSF Postdoctoral Fellowship (project 210561) to F.W., a Boehringer Ingelheim
Fonds fellowship to L.L., and by the Max Planck Society to J.A.G.B. and J.M.P.
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Ron
full_name: Kelley, Ron
last_name: Kelley
- first_name: Sagar
full_name: Khavnekar, Sagar
last_name: Khavnekar
- first_name: Ricardo D.
full_name: Righetto, Ricardo D.
last_name: Righetto
- first_name: Jessica
full_name: Heebner, Jessica
last_name: Heebner
- first_name: Martin
full_name: Obr, Martin
id: 4741CA5A-F248-11E8-B48F-1D18A9856A87
last_name: Obr
orcid: 0000-0003-1756-6564
- first_name: Xianjun
full_name: Zhang, Xianjun
last_name: Zhang
- first_name: Saikat
full_name: Chakraborty, Saikat
last_name: Chakraborty
- first_name: Grigory
full_name: Tagiltsev, Grigory
last_name: Tagiltsev
- first_name: Alicia
full_name: Michael, Alicia
id: 6437c950-2a03-11ee-914d-d6476dd7b75c
last_name: Michael
orcid: 0000-0002-6080-839X
- first_name: Sofie
full_name: Van Dorst, Sofie
last_name: Van Dorst
- first_name: Florent
full_name: Waltz, Florent
last_name: Waltz
- first_name: Caitlyn L.
full_name: Mccafferty, Caitlyn L.
last_name: Mccafferty
- first_name: Lorenz
full_name: Lamm, Lorenz
last_name: Lamm
- first_name: Simon
full_name: Zufferey, Simon
last_name: Zufferey
- first_name: Philippe
full_name: Van Der Stappen, Philippe
last_name: Van Der Stappen
- first_name: Hugo
full_name: Van Den Hoek, Hugo
last_name: Van Den Hoek
- first_name: Wojciech
full_name: Wietrzynski, Wojciech
last_name: Wietrzynski
- first_name: Pavol
full_name: Harar, Pavol
id: e03d953a-6e8c-11ef-99e4-f0717d385cd5
last_name: Harar
orcid: 0000-0001-5206-1794
- first_name: William
full_name: Wan, William
last_name: Wan
- first_name: John A.G.
full_name: Briggs, John A.G.
last_name: Briggs
- first_name: Jürgen M.
full_name: Plitzko, Jürgen M.
last_name: Plitzko
- first_name: Benjamin D.
full_name: Engel, Benjamin D.
last_name: Engel
- first_name: Abhay
full_name: Kotecha, Abhay
last_name: Kotecha
citation:
ama: Kelley R, Khavnekar S, Righetto RD, et al. Toward community-driven visual proteomics
with large-scale cryo-electron tomography of Chlamydomonas reinhardtii. Molecular
Cell. doi:10.1016/j.molcel.2025.11.029
apa: Kelley, R., Khavnekar, S., Righetto, R. D., Heebner, J., Obr, M., Zhang, X.,
… Kotecha, A. (n.d.). Toward community-driven visual proteomics with large-scale
cryo-electron tomography of Chlamydomonas reinhardtii. Molecular Cell.
Elsevier. https://doi.org/10.1016/j.molcel.2025.11.029
chicago: Kelley, Ron, Sagar Khavnekar, Ricardo D. Righetto, Jessica Heebner, Martin
Obr, Xianjun Zhang, Saikat Chakraborty, et al. “Toward Community-Driven Visual
Proteomics with Large-Scale Cryo-Electron Tomography of Chlamydomonas Reinhardtii.”
Molecular Cell. Elsevier, n.d. https://doi.org/10.1016/j.molcel.2025.11.029.
ieee: R. Kelley et al., “Toward community-driven visual proteomics with large-scale
cryo-electron tomography of Chlamydomonas reinhardtii,” Molecular Cell.
Elsevier.
ista: Kelley R, Khavnekar S, Righetto RD, Heebner J, Obr M, Zhang X, Chakraborty
S, Tagiltsev G, Michael AK, Van Dorst S, Waltz F, Mccafferty CL, Lamm L, Zufferey
S, Van Der Stappen P, Van Den Hoek H, Wietrzynski W, Harar P, Wan W, Briggs JAG,
Plitzko JM, Engel BD, Kotecha A. Toward community-driven visual proteomics with
large-scale cryo-electron tomography of Chlamydomonas reinhardtii. Molecular Cell.
mla: Kelley, Ron, et al. “Toward Community-Driven Visual Proteomics with Large-Scale
Cryo-Electron Tomography of Chlamydomonas Reinhardtii.” Molecular Cell,
Elsevier, doi:10.1016/j.molcel.2025.11.029.
short: R. Kelley, S. Khavnekar, R.D. Righetto, J. Heebner, M. Obr, X. Zhang, S.
Chakraborty, G. Tagiltsev, A.K. Michael, S. Van Dorst, F. Waltz, C.L. Mccafferty,
L. Lamm, S. Zufferey, P. Van Der Stappen, H. Van Den Hoek, W. Wietrzynski, P.
Harar, W. Wan, J.A.G. Briggs, J.M. Plitzko, B.D. Engel, A. Kotecha, Molecular
Cell (n.d.).
date_created: 2026-01-04T23:01:36Z
date_published: 2025-12-19T00:00:00Z
date_updated: 2026-01-05T08:32:47Z
day: '19'
ddc:
- '570'
department:
- _id: AlMi
doi: 10.1016/j.molcel.2025.11.029
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1016/j.molcel.2025.11.029
month: '12'
oa: 1
oa_version: Published Version
publication: Molecular Cell
publication_identifier:
eissn:
- 1097-4164
issn:
- 1097-2765
publication_status: inpress
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Toward community-driven visual proteomics with large-scale cryo-electron tomography
of Chlamydomonas reinhardtii
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: repository
OA_type: gold
_id: '20936'
abstract:
- lang: eng
text: "Supplementary material for Mombarg et al. (2025, A&A). Title: \"Is a 1D perturbative
method sufficient for asteroseismic modelling of \r\n~Cephei pulsators? Implications
for measurements of rotation and internal magnetic fields\"\r\n\r\nContent:\r\n-
Non-rotating ESTER models and associated .GSM models. (Xini = 0.71, Zini = 0.014,
vertical/horizonal viscosity 10^7 cm^2/s, vertical chemical diffusion 10^4 cm^2/s
for evolution model. More details on the ESTER models can be found in the ESTER
manual.\r\n\r\n- Rotational asymmetries computed with StORM and TOP in 1/d, and
the central m=0 frequency from TOP in 1/d. (all_A*_new.pkl)\r\n\r\n- Magnetic
asymmetries in 1/d for different obliquity angles between 0 and 90 deg for ZAMS
and MAMS model, for B_0 = 75 kG. *_nu key gives unperturbed mode frequencies,
*_npg the radial order (asym_dict.pkl, asym_dict_evol.pkl)"
article_processing_charge: No
author:
- first_name: Joey
full_name: Mombarg, Joey
last_name: Mombarg
- first_name: Vincent
full_name: Vanlaer, Vincent
last_name: Vanlaer
- first_name: Srijan B
full_name: Das, Srijan B
id: 9ce7c423-dacf-11ed-8942-e09c6cb27149
last_name: Das
orcid: 0000-0003-0896-7972
- first_name: Michel
full_name: Rieutord, Michel
last_name: Rieutord
- first_name: Conny
full_name: Aerts, Conny
last_name: Aerts
- first_name: Lisa Annabelle
full_name: Bugnet, Lisa Annabelle
id: d9edb345-f866-11ec-9b37-d119b5234501
last_name: Bugnet
orcid: 0000-0003-0142-4000
- first_name: Stephane
full_name: Mathis, Stephane
last_name: Mathis
- first_name: Daniel
full_name: Reese, Daniel
last_name: Reese
- first_name: Jerome
full_name: Ballot, Jerome
last_name: Ballot
citation:
ama: Mombarg J, Vanlaer V, Das SB, et al. Is a 1D perturbative method sufficient
for asteroseismic modelling of β Cephei pulsators? 2025. doi:10.5281/ZENODO.17580178
apa: Mombarg, J., Vanlaer, V., Das, S. B., Rieutord, M., Aerts, C., Bugnet, L. A.,
… Ballot, J. (2025). Is a 1D perturbative method sufficient for asteroseismic
modelling of β Cephei pulsators? Zenodo. https://doi.org/10.5281/ZENODO.17580178
chicago: Mombarg, Joey, Vincent Vanlaer, Srijan B Das, Michel Rieutord, Conny Aerts,
Lisa Annabelle Bugnet, Stephane Mathis, Daniel Reese, and Jerome Ballot. “Is a
1D Perturbative Method Sufficient for Asteroseismic Modelling of β Cephei Pulsators?”
Zenodo, 2025. https://doi.org/10.5281/ZENODO.17580178.
ieee: J. Mombarg et al., “Is a 1D perturbative method sufficient for asteroseismic
modelling of β Cephei pulsators?” Zenodo, 2025.
ista: Mombarg J, Vanlaer V, Das SB, Rieutord M, Aerts C, Bugnet LA, Mathis S, Reese
D, Ballot J. 2025. Is a 1D perturbative method sufficient for asteroseismic modelling
of β Cephei pulsators?, Zenodo, 10.5281/ZENODO.17580178.
mla: Mombarg, Joey, et al. Is a 1D Perturbative Method Sufficient for Asteroseismic
Modelling of β Cephei Pulsators? Zenodo, 2025, doi:10.5281/ZENODO.17580178.
short: J. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S.
Mathis, D. Reese, J. Ballot, (2025).
date_created: 2026-01-05T08:39:33Z
date_published: 2025-11-11T00:00:00Z
date_updated: 2026-02-16T12:14:36Z
day: '11'
ddc:
- '520'
department:
- _id: LiBu
doi: 10.5281/ZENODO.17580178
main_file_link:
- open_access: '1'
url: https://doi.org/10.5281/zenodo.17580178
month: '11'
oa: 1
oa_version: Submitted Version
publisher: Zenodo
related_material:
record:
- id: '20931'
relation: used_in_publication
status: public
status: public
title: Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei
pulsators?
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: research_data_reference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '20940'
abstract:
- lang: eng
text: These are the raw data files that supplement our study of mode dispersion
with magnetic field of a cavity-magnonics system containing chromium trichloride
on coplanar waveguide resonator.
article_processing_charge: No
author:
- first_name: Supriya
full_name: Mandal, Supriya
last_name: Mandal
- first_name: Krishnendu
full_name: Maji, Krishnendu
id: 76bc9e9f-ba0b-11ee-8184-90edabd17a58
last_name: Maji
- first_name: Lucky
full_name: Kapoor, Lucky
id: 84b9700b-15b2-11ec-abd3-831089e67615
last_name: Kapoor
orcid: 0000-0001-8319-2148
- first_name: Souvik
full_name: Sasmal, Souvik
last_name: Sasmal
- first_name: Soham
full_name: Manni, Soham
last_name: Manni
- first_name: John
full_name: Jesudasan, John
last_name: Jesudasan
- first_name: Pratap
full_name: Raychaudhuri, Pratap
last_name: Raychaudhuri
- first_name: Arumugam
full_name: Thamizhavel, Arumugam
last_name: Thamizhavel
- first_name: Mandar M.
full_name: Deshmukh, Mandar M.
last_name: Deshmukh
citation:
ama: Mandal S, Maji K, Kapoor L, et al. Mode dispersion with magnetic field in a
cavity-magnonics system. 2025. doi:10.5281/ZENODO.15321721
apa: Mandal, S., Maji, K., Kapoor, L., Sasmal, S., Manni, S., Jesudasan, J., … Deshmukh,
M. M. (2025). Mode dispersion with magnetic field in a cavity-magnonics system.
Zenodo. https://doi.org/10.5281/ZENODO.15321721
chicago: Mandal, Supriya, Krishnendu Maji, Lucky Kapoor, Souvik Sasmal, Soham Manni,
John Jesudasan, Pratap Raychaudhuri, Arumugam Thamizhavel, and Mandar M. Deshmukh.
“Mode Dispersion with Magnetic Field in a Cavity-Magnonics System.” Zenodo, 2025.
https://doi.org/10.5281/ZENODO.15321721.
ieee: S. Mandal et al., “Mode dispersion with magnetic field in a cavity-magnonics
system.” Zenodo, 2025.
ista: Mandal S, Maji K, Kapoor L, Sasmal S, Manni S, Jesudasan J, Raychaudhuri P,
Thamizhavel A, Deshmukh MM. 2025. Mode dispersion with magnetic field in a cavity-magnonics
system, Zenodo, 10.5281/ZENODO.15321721.
mla: Mandal, Supriya, et al. Mode Dispersion with Magnetic Field in a Cavity-Magnonics
System. Zenodo, 2025, doi:10.5281/ZENODO.15321721.
short: S. Mandal, K. Maji, L. Kapoor, S. Sasmal, S. Manni, J. Jesudasan, P. Raychaudhuri,
A. Thamizhavel, M.M. Deshmukh, (2025).
date_created: 2026-01-05T10:00:06Z
date_published: 2025-05-02T00:00:00Z
date_updated: 2026-01-05T10:07:04Z
day: '02'
department:
- _id: MaIb
- _id: JoFi
doi: 10.5281/ZENODO.15321721
has_accepted_license: '1'
main_file_link:
- open_access: '1'
url: https://doi.org/10.5281/ZENODO.15321721
month: '05'
oa: 1
oa_version: Submitted Version
publisher: Zenodo
related_material:
record:
- id: '20927'
relation: used_in_publication
status: public
status: public
title: Mode dispersion with magnetic field in a cavity-magnonics system
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: research_data_reference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '20960'
abstract:
- lang: eng
text: A linker unit was designed and synthesized that can serve both as a hairpin
turn in a DNA duplex and anchor point for an aromatic helical foldamer mimicking
the shape and surface properties of B‐DNA. Methods were developed to synthesize
natural/non‐natural chimeric molecules combining foldamer and DNA segments. The
ability of the linker to position the foldamer helix and the duplex DNA so that
their rims and grooves are in register, despite their completely different chemical
nature, was demonstrated using single crystal X‐ray diffraction, circular dichroism
and molecular models. Bio‐layer interferometry confirmed that artificial hairpin
DNA duplexes keep their ability to bind to DNA binding proteins. The chimeric
molecules may pave the way to competitive inhibitors of protein‐DNA interactions
involving sequence‐selective DNA‐binding proteins.
article_number: e202505273
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Manuel
full_name: Loos, Manuel
last_name: Loos
- first_name: Felix
full_name: Xu, Felix
last_name: Xu
- first_name: Pradeep K
full_name: Mandal, Pradeep K
id: 6a3def15-d4b4-11ef-9fa9-a24c1f545ec3
last_name: Mandal
orcid: 0000-0001-5996-956X
- first_name: Tulika
full_name: Chakrabortty, Tulika
last_name: Chakrabortty
- first_name: Céline
full_name: Douat, Céline
last_name: Douat
- first_name: David B.
full_name: Konrad, David B.
last_name: Konrad
- first_name: Melis
full_name: Cabbar, Melis
last_name: Cabbar
- first_name: Johannes
full_name: Singer, Johannes
last_name: Singer
- first_name: Valentina
full_name: Corvaglia, Valentina
last_name: Corvaglia
- first_name: Thomas
full_name: Carell, Thomas
last_name: Carell
- first_name: Ivan
full_name: Huc, Ivan
last_name: Huc
citation:
ama: Loos M, Xu F, Mandal PK, et al. Interfacing B‐DNA and DNA mimic foldamers.
Angewandte Chemie International Edition. 2025;64(31). doi:10.1002/anie.202505273
apa: Loos, M., Xu, F., Mandal, P. K., Chakrabortty, T., Douat, C., Konrad, D. B.,
… Huc, I. (2025). Interfacing B‐DNA and DNA mimic foldamers. Angewandte Chemie
International Edition. Wiley. https://doi.org/10.1002/anie.202505273
chicago: Loos, Manuel, Felix Xu, Pradeep K Mandal, Tulika Chakrabortty, Céline Douat,
David B. Konrad, Melis Cabbar, et al. “Interfacing B‐DNA and DNA Mimic Foldamers.”
Angewandte Chemie International Edition. Wiley, 2025. https://doi.org/10.1002/anie.202505273.
ieee: M. Loos et al., “Interfacing B‐DNA and DNA mimic foldamers,” Angewandte
Chemie International Edition, vol. 64, no. 31. Wiley, 2025.
ista: Loos M, Xu F, Mandal PK, Chakrabortty T, Douat C, Konrad DB, Cabbar M, Singer
J, Corvaglia V, Carell T, Huc I. 2025. Interfacing B‐DNA and DNA mimic foldamers.
Angewandte Chemie International Edition. 64(31), e202505273.
mla: Loos, Manuel, et al. “Interfacing B‐DNA and DNA Mimic Foldamers.” Angewandte
Chemie International Edition, vol. 64, no. 31, e202505273, Wiley, 2025, doi:10.1002/anie.202505273.
short: M. Loos, F. Xu, P.K. Mandal, T. Chakrabortty, C. Douat, D.B. Konrad, M. Cabbar,
J. Singer, V. Corvaglia, T. Carell, I. Huc, Angewandte Chemie International Edition
64 (2025).
date_created: 2026-01-08T07:04:48Z
date_published: 2025-07-28T00:00:00Z
date_updated: 2026-01-19T11:07:53Z
day: '28'
ddc:
- '540'
doi: 10.1002/anie.202505273
extern: '1'
external_id:
pmid:
- '40346004'
has_accepted_license: '1'
intvolume: ' 64'
issue: '31'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1002/anie.202505273
month: '07'
oa: 1
oa_version: Published Version
pmid: 1
publication: Angewandte Chemie International Edition
publication_identifier:
eissn:
- 1521-3773
issn:
- 1433-7851
publication_status: published
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: Interfacing B‐DNA and DNA mimic foldamers
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: 64
year: '2025'
...
---
OA_type: closed access
_id: '20973'
abstract:
- lang: eng
text: CuAgSe-based materials are attractive for low-temperature thermoelectric (TE)
applications but are limited by bipolar conduction and relatively high thermal
conductivity. Herein, we report a ligand-free aqueous synthesis of Te-doped CuAgSe
(CuAgSe1-xTex), where structural and electronic modulation improve carrier transport
and suppress phonon propagation. Ex-situ time-resolved X-ray diffraction reveals
a spontaneous growth mechanism, while density functional theory calculations show
that Te-5s and 5p orbitals hybridization generates localized states and an asymmetric
density of states, thereby enhancing the Seebeck coefficient. Electron microscopy
and strain analyses confirm that Te-doping introduces a high density of lattice
dislocations and grain boundaries, leading to a reduced lattice thermal conductivity
of 0.11 W m−1K−1 at 443 K. These synergistic effects translate into device-level
performance—the first integrated CuAgSe thermoelectric modules, exhibit a maximum
cooling temperature difference of 27.3 K, and power density of 0.34 W cm−2 with
a conversion efficiency of 3.6% at a modest temperature gradient of 136 K. These
results demonstrate that CuAgSe1-xTex enables efficient energy harvesting and
localized cooling under small temperature gradient, underscoring the importance
of structural and electronic design beyond conventional zT benchmarks.
acknowledgement: K.H.L. acknowledges financial support from the National Natural Science
Foundation of China (NSFC) (Grant Number 22208293) and the National Foreign Expert
Project (Y20240175). Y.L. acknowledges funding from the NSFC (Grant Number 22209034),
the Innovation and Entrepreneurship Project of Overseas Returnees in Anhui Province
(Grant Number 2022LCX002), and the Fundamental Research Funds for the Central Universities
(JZ2024HGTB0239). Y.Z. acknowledges funding from the NSFC (Grant Number 52502313)
and Wenzhou Basic Scientific Research Project (Grant Number G20240034). Q. W. acknowledges
financial support from the NSFC (Grant Number 22208292), the High-Level Overseas-Educated
Talents Return Program, and the “Pioneer” and “Leading Goose” R&D Program of Zhejiang
[2025C04021]. K.H.L., Q. W., and X. Y. also acknowledge the Research Funds of the
Institute of Zhejiang University-Quzhou (Grants No. IZQ2022RCZX101, IZQ2021RCZX003,
IZQ2021RCZX002, and IZQ2024KJ0004). M.H. acknowledges the funding from the Australian
Research Council and the iLAuNCH Trailblazer, Department of Education, Australia.
M.H. acknowledges the computational support from the National Computational Infrastructure
(NCI), Australia, and Pawsey Supercomputing Centre, Australia.
article_number: e13035
article_processing_charge: No
article_type: original
author:
- first_name: Weite
full_name: Meng, Weite
last_name: Meng
- first_name: Mingquan
full_name: Li, Mingquan
last_name: Li
- first_name: Qingyue
full_name: Wang, Qingyue
last_name: Wang
- first_name: Pingan
full_name: Song, Pingan
last_name: Song
- first_name: Xuan
full_name: Yang, Xuan
last_name: Yang
- first_name: Wen Jun
full_name: Wang, Wen Jun
last_name: Wang
- first_name: Min
full_name: Hong, Min
last_name: Hong
- first_name: Maria
full_name: Ibáñez, Maria
id: 43C61214-F248-11E8-B48F-1D18A9856A87
last_name: Ibáñez
orcid: 0000-0001-5013-2843
- first_name: Andreu
full_name: Cabot, Andreu
last_name: Cabot
- first_name: Yu
full_name: Zhang, Yu
last_name: Zhang
- first_name: Yu
full_name: Liu, Yu
last_name: Liu
- first_name: Khak Ho
full_name: Lim, Khak Ho
last_name: Lim
citation:
ama: Meng W, Li M, Wang Q, et al. Efficient near room temperature thermoelectric
cooling and power generation with CuAgSe. Small. 2025. doi:10.1002/smll.202513035
apa: Meng, W., Li, M., Wang, Q., Song, P., Yang, X., Wang, W. J., … Lim, K. H. (2025).
Efficient near room temperature thermoelectric cooling and power generation with
CuAgSe. Small. Wiley. https://doi.org/10.1002/smll.202513035
chicago: Meng, Weite, Mingquan Li, Qingyue Wang, Pingan Song, Xuan Yang, Wen Jun
Wang, Min Hong, et al. “Efficient near Room Temperature Thermoelectric Cooling
and Power Generation with CuAgSe.” Small. Wiley, 2025. https://doi.org/10.1002/smll.202513035.
ieee: W. Meng et al., “Efficient near room temperature thermoelectric cooling
and power generation with CuAgSe,” Small. Wiley, 2025.
ista: Meng W, Li M, Wang Q, Song P, Yang X, Wang WJ, Hong M, Ibáñez M, Cabot A,
Zhang Y, Liu Y, Lim KH. 2025. Efficient near room temperature thermoelectric cooling
and power generation with CuAgSe. Small., e13035.
mla: Meng, Weite, et al. “Efficient near Room Temperature Thermoelectric Cooling
and Power Generation with CuAgSe.” Small, e13035, Wiley, 2025, doi:10.1002/smll.202513035.
short: W. Meng, M. Li, Q. Wang, P. Song, X. Yang, W.J. Wang, M. Hong, M. Ibáñez,
A. Cabot, Y. Zhang, Y. Liu, K.H. Lim, Small (2025).
date_created: 2026-01-11T23:01:34Z
date_published: 2025-12-30T00:00:00Z
date_updated: 2026-01-12T09:37:19Z
day: '30'
department:
- _id: MaIb
doi: 10.1002/smll.202513035
external_id:
pmid:
- '41470065'
language:
- iso: eng
month: '12'
oa_version: None
pmid: 1
publication: Small
publication_identifier:
eissn:
- 1613-6829
issn:
- 1613-6810
publication_status: epub_ahead
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: Efficient near room temperature thermoelectric cooling and power generation
with CuAgSe
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '20976'
abstract:
- lang: eng
text: We present an experimental demonstration of an impedance-engineered Josephson
parametric amplifier (IEJPA) fabricated in a single-step lithography process.
Impedance-engineering is implemented using a lumped-element series LC circuit.
We use a simpler lithography process where the entire device—impedance transformer
and Josephson parametric amplifier (JPA)—is patterned in a single electron beam
lithography step, followed by a double-angle Dolan-bridge technique for Al–AlOx–Al
deposition. We observe amplification with 18 dB gain over a wide 400 MHz bandwidth
centered around 5.3 GHz with added noise approaching the quantum limit, and a
saturation power of −114 dBm. To accurately explain our experimental results,
we extend existing theories for IEJPAs to incorporate the full sine nonlinearity
of both the JPA and the transformer. Our work provides a route to simpler realization
of broadband JPAs and a theoretical foundation for a regime of JPA operation that
has been less explored in literature.
acknowledgement: The authors acknowledge receiving support from the Space Technology
Cell at IISc and ISRO through the project STC-0444(2022) and the Ministry of Electronics
and Information Technology of the Government of India, under the centre of Excellence
of Quantum Technology at the Indian Institute of Science, as well as the office
of Principle Scientific Advisor, Government of India. S.H. and A.P. acknowledge
the support of the Kishore Vaigyanik Protsahan Yojana (KVPY). A.S. acknowledges
the support of a New Faculty Initiation Grant (NFIG) from IIT Madras.
article_number: '254001'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Lipi
full_name: Patel, Lipi
last_name: Patel
- first_name: Samarth
full_name: Hawaldar, Samarth
id: 221708e1-1ff6-11ee-9fa6-85146607433e
last_name: Hawaldar
orcid: 0000-0002-1965-4309
- first_name: Aditya
full_name: Panikkar, Aditya
last_name: Panikkar
- first_name: Athreya
full_name: Shankar, Athreya
last_name: Shankar
- first_name: Baladitya
full_name: Suri, Baladitya
last_name: Suri
citation:
ama: Patel L, Hawaldar S, Panikkar A, Shankar A, Suri B. Impedance-engineered Josephson
parametric amplifier with single-step lithography. Applied Physics Letters.
2025;127(25). doi:10.1063/5.0290636
apa: Patel, L., Hawaldar, S., Panikkar, A., Shankar, A., & Suri, B. (2025).
Impedance-engineered Josephson parametric amplifier with single-step lithography.
Applied Physics Letters. AIP Publishing. https://doi.org/10.1063/5.0290636
chicago: Patel, Lipi, Samarth Hawaldar, Aditya Panikkar, Athreya Shankar, and Baladitya
Suri. “Impedance-Engineered Josephson Parametric Amplifier with Single-Step Lithography.”
Applied Physics Letters. AIP Publishing, 2025. https://doi.org/10.1063/5.0290636.
ieee: L. Patel, S. Hawaldar, A. Panikkar, A. Shankar, and B. Suri, “Impedance-engineered
Josephson parametric amplifier with single-step lithography,” Applied Physics
Letters, vol. 127, no. 25. AIP Publishing, 2025.
ista: Patel L, Hawaldar S, Panikkar A, Shankar A, Suri B. 2025. Impedance-engineered
Josephson parametric amplifier with single-step lithography. Applied Physics Letters.
127(25), 254001.
mla: Patel, Lipi, et al. “Impedance-Engineered Josephson Parametric Amplifier with
Single-Step Lithography.” Applied Physics Letters, vol. 127, no. 25, 254001,
AIP Publishing, 2025, doi:10.1063/5.0290636.
short: L. Patel, S. Hawaldar, A. Panikkar, A. Shankar, B. Suri, Applied Physics
Letters 127 (2025).
date_created: 2026-01-11T23:01:34Z
date_published: 2025-12-22T00:00:00Z
date_updated: 2026-01-12T09:57:53Z
day: '22'
department:
- _id: JoFi
doi: 10.1063/5.0290636
external_id:
arxiv:
- '2507.09298'
intvolume: ' 127'
issue: '25'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2507.09298
month: '12'
oa: 1
oa_version: Preprint
publication: Applied Physics Letters
publication_identifier:
eissn:
- 1077-3118
issn:
- 0003-6951
publication_status: published
publisher: AIP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Impedance-engineered Josephson parametric amplifier with single-step lithography
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 127
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '20977'
abstract:
- lang: eng
text: Hippocampal sharp-wave ripples (SPW-Rs) are high-frequency oscillations critical
for memory consolidation. Despite extensive characterization in rodents, their
detection in humans is limited by coarse spatial sampling, interictal epileptiform
discharges (IEDs), and a lack of consensus on human ripple localization and morphology.
Here, we demonstrate that mouse and human hippocampal ripples share spatial, spectral
and temporal features, which are clearly distinct from IEDs. In recordings from
male APP/PS1 mice, SPW-Rs were distinguishable from IEDs by multiple criteria.
Hippocampal ripples recorded during NREM sleep in female and male surgical epilepsy
patients exhibited similar narrowband frequency peaks and multiple ripple cycles
in the CA1 and subiculum regions. Conversely, IEDs showed a broad spatial extent
and wide-band frequency power. We developed a semi-automated, ripple curation
toolbox (ripmap) to separate event waveforms by low-dimensional embedding to reduce
false-positive rate in selected ripple channels. Our approach improves ripple
detection and provides a firm foundation for future human memory research.
acknowledgement: We thank Karl Rössler and Sebastian Brandner for the human SEEG implantations;
Katja Kobow for providing the histopathological findings of the patients; Jay Jeschke
for help with human electrode localization; Esha Brahmbhatt and Deren Aykan for
help with animal habituation; Mursel Karadas for the rodent treadmill design; Nicholas
Paleologos, Noam Nitzan, Michael D Hadler and Samuel McKenzie for rating events
in a human ripple survey included in a previous version of the manuscript; Nicholas
Paleologos for sharing NYU iEEG data for validating UMAP parameters; Julio Esparza
for help on the topological analysis through discussions; Thomas Hainmüller, Yiyao
Zhang and Mursel Karadas for feedback on the manuscript. We would like to acknowledge
Corticale SRL (Genoa, Italy) for providing the SiNAPS probes, and NeuroNexus (Ann
Arbor, MI) for their contribution of the data acquisition system and Radiens software.
We further acknowledge both Corticale and NeuroNexus for training and support making
this research possible. This work was supported by the German Research Foundation
(DFG; Walter Benjamin Fellowship MA 10301/1-1, A.M.), NYU Langone Health Finding
a Cure for Epilepsy and Seizures (FACES, A.M.), the NOMIS Fellowship (A.N.-O.),
the National Institutes of Health (R01NS127954, K23NS104252, A.L.; MH122391, U19NS107616,
R01MH139216 G.B.,), and the NYU Department of Neurology (A.L.).
article_number: '11636'
article_processing_charge: Yes
article_type: original
author:
- first_name: Anna
full_name: Maslarova, Anna
last_name: Maslarova
- first_name: Jiyun N.
full_name: Shin, Jiyun N.
last_name: Shin
- first_name: Andrea C
full_name: Navas Olivé, Andrea C
id: 739d26c9-52e8-11ee-8d72-f14d3893b4ce
last_name: Navas Olivé
orcid: 0000-0002-9280-8597
- first_name: Mihály
full_name: Vöröslakos, Mihály
last_name: Vöröslakos
- first_name: Hajo
full_name: Hamer, Hajo
last_name: Hamer
- first_name: Arnd
full_name: Doerfler, Arnd
last_name: Doerfler
- first_name: Simon
full_name: Henin, Simon
last_name: Henin
- first_name: György
full_name: Buzsáki, György
last_name: Buzsáki
- first_name: Anli
full_name: Liu, Anli
last_name: Liu
citation:
ama: Maslarova A, Shin JN, Navas Olivé AC, et al. Spatiotemporal patterns differentiate
hippocampal sharp-wave ripples from interictal epileptiform discharges in mice
and humans. Nature Communications. 2025;16. doi:10.1038/s41467-025-66562-6
apa: Maslarova, A., Shin, J. N., Navas Olivé, A. C., Vöröslakos, M., Hamer, H.,
Doerfler, A., … Liu, A. (2025). Spatiotemporal patterns differentiate hippocampal
sharp-wave ripples from interictal epileptiform discharges in mice and humans.
Nature Communications. Springer Nature. https://doi.org/10.1038/s41467-025-66562-6
chicago: Maslarova, Anna, Jiyun N. Shin, Andrea C Navas Olivé, Mihály Vöröslakos,
Hajo Hamer, Arnd Doerfler, Simon Henin, György Buzsáki, and Anli Liu. “Spatiotemporal
Patterns Differentiate Hippocampal Sharp-Wave Ripples from Interictal Epileptiform
Discharges in Mice and Humans.” Nature Communications. Springer Nature,
2025. https://doi.org/10.1038/s41467-025-66562-6.
ieee: A. Maslarova et al., “Spatiotemporal patterns differentiate hippocampal
sharp-wave ripples from interictal epileptiform discharges in mice and humans,”
Nature Communications, vol. 16. Springer Nature, 2025.
ista: Maslarova A, Shin JN, Navas Olivé AC, Vöröslakos M, Hamer H, Doerfler A, Henin
S, Buzsáki G, Liu A. 2025. Spatiotemporal patterns differentiate hippocampal sharp-wave
ripples from interictal epileptiform discharges in mice and humans. Nature Communications.
16, 11636.
mla: Maslarova, Anna, et al. “Spatiotemporal Patterns Differentiate Hippocampal
Sharp-Wave Ripples from Interictal Epileptiform Discharges in Mice and Humans.”
Nature Communications, vol. 16, 11636, Springer Nature, 2025, doi:10.1038/s41467-025-66562-6.
short: A. Maslarova, J.N. Shin, A.C. Navas Olivé, M. Vöröslakos, H. Hamer, A. Doerfler,
S. Henin, G. Buzsáki, A. Liu, Nature Communications 16 (2025).
date_created: 2026-01-11T23:01:35Z
date_published: 2025-12-30T00:00:00Z
date_updated: 2026-01-12T09:31:56Z
day: '30'
ddc:
- '570'
department:
- _id: PeJo
doi: 10.1038/s41467-025-66562-6
external_id:
pmid:
- '39975118'
file:
- access_level: open_access
checksum: a8a1670e197484382e087be60f643945
content_type: application/pdf
creator: dernst
date_created: 2026-01-12T09:30:15Z
date_updated: 2026-01-12T09:30:15Z
file_id: '20978'
file_name: 2025_NatureComm_Maslarova.pdf
file_size: 7629997
relation: main_file
success: 1
file_date_updated: 2026-01-12T09:30:15Z
has_accepted_license: '1'
intvolume: ' 16'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 9B861AAC-BA93-11EA-9121-9846C619BF3A
name: NOMIS Fellowship Program
publication: Nature Communications
publication_identifier:
eissn:
- 2041-1723
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Spatiotemporal patterns differentiate hippocampal sharp-wave ripples from interictal
epileptiform discharges in mice and humans
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 16
year: '2025'
...
---
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '20990'
abstract:
- lang: eng
text: Modeling the response of material and chemical systems to electric fields
remains a longstanding challenge. Machine learning interatomic potentials (MLIPs)
offer an efficient and scalable alternative to quantum mechanical methods, but
do not by themselves incorporate electrical response. Here, we show that polarization
and Born effective charge (BEC) tensors can be directly extracted from long-range
MLIPs within the Latent Ewald Summation (LES) framework, solely by learning from
energy and force data. Using this approach, we predict the infrared spectra of
bulk water under zero or finite external electric fields, ionic conductivities
of high-pressure superionic ice, and the phase transition and hysteresis in ferroelectric
PbTiO3 perovskite. This work thus extends the capability of MLIPs to predict electrical
response –without training on charges or polarization or BECs– and enables accurate
modeling of electric-field-driven processes in diverse systems at scale.
acknowledgement: The authors thank for valuable discussions with Pinchen Xie, David
Limmer, Jeff Neaton, and Greg Voth. The authors thank Sebastien Hamel for providing
the DFT MD trajectories for superionic water, and help clarifying questions related
to the pseudopotentials. The authors thank Federico Grasselli and Stefano Baroni
for providing data and notebooks for computing the conductivity of a molten salt.
This research used the Savio computational cluster resource provided by the Berkeley
Research Computing program at the University of California, Berkeley (supported
by the UC Berkeley Chancellor, Vice Chancellor for Research, and Chief Information
Officer). D.S.K. and P.Z. acknowledge funding from the BIDMaP Postdoctoral Fellowship.
article_number: '384'
article_processing_charge: Yes
article_type: original
author:
- first_name: Peichen
full_name: Zhong, Peichen
last_name: Zhong
- first_name: Dongjin
full_name: Kim, Dongjin
last_name: Kim
- first_name: Daniel S.
full_name: King, Daniel S.
last_name: King
- first_name: Bingqing
full_name: Cheng, Bingqing
id: cbe3cda4-d82c-11eb-8dc7-8ff94289fcc9
last_name: Cheng
orcid: 0000-0002-3584-9632
citation:
ama: Zhong P, Kim D, King DS, Cheng B. Machine learning interatomic potential can
infer electrical response. npj Computational Materials. 2025;11. doi:10.1038/s41524-025-01911-z
apa: Zhong, P., Kim, D., King, D. S., & Cheng, B. (2025). Machine learning interatomic
potential can infer electrical response. Npj Computational Materials. Springer
Nature. https://doi.org/10.1038/s41524-025-01911-z
chicago: Zhong, Peichen, Dongjin Kim, Daniel S. King, and Bingqing Cheng. “Machine
Learning Interatomic Potential Can Infer Electrical Response.” Npj Computational
Materials. Springer Nature, 2025. https://doi.org/10.1038/s41524-025-01911-z.
ieee: P. Zhong, D. Kim, D. S. King, and B. Cheng, “Machine learning interatomic
potential can infer electrical response,” npj Computational Materials,
vol. 11. Springer Nature, 2025.
ista: Zhong P, Kim D, King DS, Cheng B. 2025. Machine learning interatomic potential
can infer electrical response. npj Computational Materials. 11, 384.
mla: Zhong, Peichen, et al. “Machine Learning Interatomic Potential Can Infer Electrical
Response.” Npj Computational Materials, vol. 11, 384, Springer Nature,
2025, doi:10.1038/s41524-025-01911-z.
short: P. Zhong, D. Kim, D.S. King, B. Cheng, Npj Computational Materials 11 (2025).
corr_author: '1'
date_created: 2026-01-15T12:17:07Z
date_published: 2025-12-29T00:00:00Z
date_updated: 2026-01-20T07:23:34Z
day: '29'
ddc:
- '540'
department:
- _id: BiCh
doi: 10.1038/s41524-025-01911-z
file:
- access_level: open_access
checksum: cc999804ba3bfed809ae46c73869e4e3
content_type: application/pdf
creator: dernst
date_created: 2026-01-20T07:22:04Z
date_updated: 2026-01-20T07:22:04Z
file_id: '21005'
file_name: 2025_npj_Zhong.pdf
file_size: 2686255
relation: main_file
success: 1
file_date_updated: 2026-01-20T07:22:04Z
has_accepted_license: '1'
intvolume: ' 11'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
publication: npj Computational Materials
publication_identifier:
eissn:
- 2057-3960
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Machine learning interatomic potential can infer electrical response
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: 11
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '21003'
abstract:
- lang: eng
text: We extend work of Heath-Brown and Salberger, based on the determinant method,
to provide a uniform upper bound for the number of integral points of bounded
height on an affine surface, which are subject to a polynomial congruence condition.
This is applied to get a new uniform bound for points on diagonal quadric surfaces,
and to a problem about the representation of integers as a sum of four unlike
powers.
acknowledgement: "Supported by FWF grant (DOI 10.55776/P36278), Supported by European
Union’s Horizon 2020 research and innovation program under the Marie Skłodowska-Curie
Grant\r\nAgreement No. 101034413."
article_number: '12'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Timothy D
full_name: Browning, Timothy D
id: 35827D50-F248-11E8-B48F-1D18A9856A87
last_name: Browning
orcid: 0000-0002-8314-0177
- first_name: Matteo
full_name: Verzobio, Matteo
id: 7aa8f170-131e-11ed-88e1-a9efd01027cb
last_name: Verzobio
orcid: 0000-0002-0854-0306
citation:
ama: Browning TD, Verzobio M. Counting integer points on affine surfaces with a
side condition. Discrete Analysis. 2025;2025. doi:10.19086/da.143787
apa: 'Browning, T. D., & Verzobio, M. (2025). Counting integer points on affine
surfaces with a side condition. Discrete Analysis. Cambridge: Alliance
of Diamond Open Access Journals. https://doi.org/10.19086/da.143787'
chicago: 'Browning, Timothy D, and Matteo Verzobio. “Counting Integer Points on
Affine Surfaces with a Side Condition.” Discrete Analysis. Cambridge: Alliance
of Diamond Open Access Journals, 2025. https://doi.org/10.19086/da.143787.'
ieee: 'T. D. Browning and M. Verzobio, “Counting integer points on affine surfaces
with a side condition,” Discrete Analysis, vol. 2025. Cambridge: Alliance
of Diamond Open Access Journals, 2025.'
ista: Browning TD, Verzobio M. 2025. Counting integer points on affine surfaces
with a side condition. Discrete Analysis. 2025, 12.
mla: 'Browning, Timothy D., and Matteo Verzobio. “Counting Integer Points on Affine
Surfaces with a Side Condition.” Discrete Analysis, vol. 2025, 12, Cambridge:
Alliance of Diamond Open Access Journals, 2025, doi:10.19086/da.143787.'
short: T.D. Browning, M. Verzobio, Discrete Analysis 2025 (2025).
corr_author: '1'
date_created: 2026-01-18T23:02:44Z
date_published: 2025-09-01T00:00:00Z
date_updated: 2026-02-12T08:03:12Z
day: '01'
ddc:
- '510'
department:
- _id: TiBr
doi: 10.19086/da.143787
ec_funded: 1
external_id:
arxiv:
- '2408.11453'
file:
- access_level: open_access
checksum: 3d38e850b40f3e1abbfd30073bd4388a
content_type: application/pdf
creator: dernst
date_created: 2026-02-12T07:50:47Z
date_updated: 2026-02-12T07:50:47Z
file_id: '21214'
file_name: 2025_DiscreteAnalysis_Browning.pdf
file_size: 393625
relation: main_file
success: 1
file_date_updated: 2026-02-12T07:50:47Z
has_accepted_license: '1'
intvolume: ' 2025'
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
project:
- _id: bd8a4fdc-d553-11ed-ba76-80a0167441a3
grant_number: P36278
name: Rational curves via function field analytic number theory
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Discrete Analysis
publication_identifier:
eissn:
- 2397-3129
publication_status: published
publisher: 'Cambridge: Alliance of Diamond Open Access Journals'
scopus_import: '1'
status: public
title: Counting integer points on affine surfaces with a side condition
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: 2025
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21007'
abstract:
- lang: eng
text: 'Currently, the best known tradeoff between approximation ratio and complexity
for the Sparsest Cut problem is achieved by the algorithm in [Sherman, FOCS 2009]:
it computes O(√(log n)/ε)-approximation using O(nε logO(1) n) maxflows for any
ε∈[Θ(1/log n),Θ(1)]. It works by solving the SDP relaxation of [Arora-Rao-Vazirani,
STOC 2004] using the Multiplicative Weights Update algorithm (MW) of [Arora-Kale,
JACM 2016]. To implement one MW step, Sherman approximately solves a multicommodity
flow problem using another application of MW. Nested MW steps are solved via a
certain "chaining" algorithm that combines results of multiple calls to the maxflow
algorithm. We present an alternative approach that avoids solving the multicommodity
flow problem and instead computes "violating paths". This simplifies Sherman''s
algorithm by removing a need for a nested application of MW, and also allows parallelization:
we show how to compute O(√(log n)/ε)-approximation via O(logO(1) n) maxflows using
O(nε) processors. We also revisit Sherman''s chaining algorithm, and present a
simpler version together with a new analysis.'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Vladimir
full_name: Kolmogorov, Vladimir
id: 3D50B0BA-F248-11E8-B48F-1D18A9856A87
last_name: Kolmogorov
citation:
ama: Kolmogorov V. A simpler and parallelizable O(√log n)-approximation algorithm
for SPARSEST CUT. ACM Transactions on Algorithms. 2025;21(4):1-22. doi:10.1145/3748723
apa: Kolmogorov, V. (2025). A simpler and parallelizable O(√log n)-approximation
algorithm for SPARSEST CUT. ACM Transactions on Algorithms. Association
for Computing Machinery. https://doi.org/10.1145/3748723
chicago: Kolmogorov, Vladimir. “A Simpler and Parallelizable O(√log n)-Approximation
Algorithm for SPARSEST CUT.” ACM Transactions on Algorithms. Association
for Computing Machinery, 2025. https://doi.org/10.1145/3748723.
ieee: V. Kolmogorov, “A simpler and parallelizable O(√log n)-approximation algorithm
for SPARSEST CUT,” ACM Transactions on Algorithms, vol. 21, no. 4. Association
for Computing Machinery, pp. 1–22, 2025.
ista: Kolmogorov V. 2025. A simpler and parallelizable O(√log n)-approximation algorithm
for SPARSEST CUT. ACM Transactions on Algorithms. 21(4), 1–22.
mla: Kolmogorov, Vladimir. “A Simpler and Parallelizable O(√log n)-Approximation
Algorithm for SPARSEST CUT.” ACM Transactions on Algorithms, vol. 21, no.
4, Association for Computing Machinery, 2025, pp. 1–22, doi:10.1145/3748723.
short: V. Kolmogorov, ACM Transactions on Algorithms 21 (2025) 1–22.
corr_author: '1'
date_created: 2026-01-20T10:04:02Z
date_published: 2025-10-01T00:00:00Z
date_updated: 2026-01-21T09:46:26Z
day: '01'
ddc:
- '510'
department:
- _id: VlKo
doi: 10.1145/3748723
external_id:
arxiv:
- '2307.00115'
file:
- access_level: open_access
checksum: 4a80fdb1e3711b9a2768d2bb8f6d3b4e
content_type: application/pdf
creator: dernst
date_created: 2026-01-21T09:38:09Z
date_updated: 2026-01-21T09:38:09Z
file_id: '21031'
file_name: 2025_ACMToA_Kolmogorov.pdf
file_size: 2208302
relation: main_file
success: 1
file_date_updated: 2026-01-21T09:38:09Z
has_accepted_license: '1'
intvolume: ' 21'
issue: '4'
language:
- iso: eng
month: '10'
oa: 1
oa_version: Published Version
page: 1-22
publication: ACM Transactions on Algorithms
publication_identifier:
eissn:
- 1549-6333
issn:
- 1549-6325
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
related_material:
record:
- id: '17236'
relation: shorter_version
status: public
scopus_import: '1'
status: public
title: A simpler and parallelizable O(√log n)-approximation algorithm for SPARSEST
CUT
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: 21
year: '2025'
...
---
OA_place: repository
_id: '21016'
abstract:
- lang: eng
text: Motivated by applications in chemistry, we give a homlogical definition of
tunnels, or more generally cobordisms, connecting disjoint parts of a cell complex.
For a filtered complex, this defines a persistence module. We give a method for
identifying birth and death times using kernel persistence and a matrix reduction
algorithm for pairing birth and death times.
acknowledgement: "Y. B. B. and L. F. were funded by the Independent Research Fund
Denmark, grant\r\nnumber 1026-00037. T. H. was partially supported by the European
Research Council\r\n(ERC) Horizon 2020, grant number 788183."
article_number: '2505.17858'
article_processing_charge: No
arxiv: 1
author:
- first_name: Yossi
full_name: Bleile, Yossi
id: 920a7385-7995-11ef-9bfd-8c434cd8f3c2
last_name: Bleile
orcid: 0000-0002-4861-9174
- first_name: Lisbeth
full_name: Fajstrup, Lisbeth
last_name: Fajstrup
- first_name: Teresa
full_name: Heiss, Teresa
id: 4879BB4E-F248-11E8-B48F-1D18A9856A87
last_name: Heiss
orcid: 0000-0002-1780-2689
- first_name: Anne Marie
full_name: Svane, Anne Marie
last_name: Svane
- first_name: Søren Strandskov
full_name: Sørensen, Søren Strandskov
last_name: Sørensen
citation:
ama: Bleile Y, Fajstrup L, Heiss T, Svane AM, Sørensen SS. Identifying cobordisms
using kernel persistence. arXiv. doi:10.48550/arXiv.2505.17858
apa: Bleile, Y., Fajstrup, L., Heiss, T., Svane, A. M., & Sørensen, S. S. (n.d.).
Identifying cobordisms using kernel persistence. arXiv. https://doi.org/10.48550/arXiv.2505.17858
chicago: Bleile, Yossi, Lisbeth Fajstrup, Teresa Heiss, Anne Marie Svane, and Søren
Strandskov Sørensen. “Identifying Cobordisms Using Kernel Persistence.” ArXiv,
n.d. https://doi.org/10.48550/arXiv.2505.17858.
ieee: Y. Bleile, L. Fajstrup, T. Heiss, A. M. Svane, and S. S. Sørensen, “Identifying
cobordisms using kernel persistence,” arXiv. .
ista: Bleile Y, Fajstrup L, Heiss T, Svane AM, Sørensen SS. Identifying cobordisms
using kernel persistence. arXiv, 2505.17858.
mla: Bleile, Yossi, et al. “Identifying Cobordisms Using Kernel Persistence.” ArXiv,
2505.17858, doi:10.48550/arXiv.2505.17858.
short: Y. Bleile, L. Fajstrup, T. Heiss, A.M. Svane, S.S. Sørensen, ArXiv (n.d.).
date_created: 2026-01-20T10:12:21Z
date_published: 2025-05-23T00:00:00Z
date_updated: 2026-01-21T10:34:57Z
day: '23'
department:
- _id: HeEd
doi: 10.48550/arXiv.2505.17858
ec_funded: 1
external_id:
arxiv:
- '2505.17858'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2505.17858
month: '05'
oa: 1
oa_version: Preprint
project:
- _id: 266A2E9E-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '788183'
name: Alpha Shape Theory Extended
publication: arXiv
publication_status: submitted
status: public
title: Identifying cobordisms using kernel persistence
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
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. ACM Transactions on Computer Systems. 2025.
doi:10.1145/3769423'
apa: 'Neiheiser, R., Matos, M., & Rodrigues, L. (2025). Kauri: BFT consensus
with pipelined tree-based dissemination and aggregation. ACM Transactions on
Computer Systems. Association for Computing Machinery. https://doi.org/10.1145/3769423'
chicago: 'Neiheiser, Ray, Miguel Matos, and Luis Rodrigues. “Kauri: BFT Consensus
with Pipelined Tree-Based Dissemination and Aggregation.” ACM Transactions
on Computer Systems. Association for Computing Machinery, 2025. https://doi.org/10.1145/3769423.'
ieee: 'R. Neiheiser, M. Matos, and L. Rodrigues, “Kauri: BFT consensus with pipelined
tree-based dissemination and aggregation,” ACM Transactions on Computer Systems.
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.” ACM Transactions on Computer Systems, 3769423, Association
for Computing Machinery, 2025, doi:10.1145/3769423.'
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: 2026-01-21T08:11:23Z
day: '05'
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: 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: 13th International Conference
on Learning Representations. ICLR; 2025.'
apa: 'Gairola, S., Böhle, M., Locatello, F., & Schiele, B. (2025). How to probe:
Simple yet effective techniques for improving post-hoc explanations. In 13th
International Conference on Learning Representations. 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 13th International Conference on Learning Representations. 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 13th International
Conference on Learning Representations, 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.” 13th International Conference on Learning
Representations, 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: 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. Proceedings of
the ACM on Programming Languages. 2025;9(POPL):300-331. doi:10.1145/3704847
apa: Vistrup, M., Sammler, M. J., & Jung, R. (2025). Program logics à la Carte.
Proceedings of the ACM on Programming Languages. Association for Computing
Machinery. https://doi.org/10.1145/3704847
chicago: Vistrup, Max, Michael Joachim Sammler, and Ralf Jung. “Program Logics à
La Carte.” Proceedings of the ACM on Programming Languages. Association
for Computing Machinery, 2025. https://doi.org/10.1145/3704847.
ieee: M. Vistrup, M. J. Sammler, and R. Jung, “Program logics à la Carte,” Proceedings
of the ACM on Programming Languages, 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.” Proceedings of the ACM
on Programming Languages, vol. 9, no. POPL, Association for Computing Machinery,
2025, pp. 300–31, doi:10.1145/3704847.
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. Proceedings of the ACM on Programming
Languages. 2025;9(POPL):569-599. doi:10.1145/3704856
apa: Dardinier, T., Sammler, M. J., Parthasarathy, G., Summers, A. J., & Müller,
P. (2025). Formal foundations for translational separation logic verifiers. Proceedings
of the ACM on Programming Languages. Association for Computing Machinery.
https://doi.org/10.1145/3704856
chicago: Dardinier, Thibault, Michael Joachim Sammler, Gaurav Parthasarathy, Alexander
J. Summers, and Peter Müller. “Formal Foundations for Translational Separation
Logic Verifiers.” Proceedings of the ACM on Programming Languages. Association
for Computing Machinery, 2025. https://doi.org/10.1145/3704856.
ieee: T. Dardinier, M. J. Sammler, G. Parthasarathy, A. J. Summers, and P. Müller,
“Formal foundations for translational separation logic verifiers,” Proceedings
of the ACM on Programming Languages, 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.” Proceedings of the ACM on Programming Languages, vol.
9, no. POPL, Association for Computing Machinery, 2025, pp. 569–99, doi:10.1145/3704856.
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. The
Astrophysical Journal. 2025;995(1). doi:10.3847/1538-4357/ae1500'
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. The Astrophysical
Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae1500'
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.” The
Astrophysical Journal. IOP Publishing, 2025. https://doi.org/10.3847/1538-4357/ae1500.'
ieee: 'D. J. Setton et al., “Little Red Dots at an inflection point: Ubiquitous
v-shaped turnover consistently occurs at the Balmer limit,” The Astrophysical
Journal, 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.” The Astrophysical
Journal, vol. 995, no. 1, 118, IOP Publishing, 2025, doi:10.3847/1538-4357/ae1500.'
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. The Astrophysical Journal
Letters. 2025;991. doi:10.3847/2041-8213/ade78b
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. The Astrophysical Journal Letters.
IOP Publishing. https://doi.org/10.3847/2041-8213/ade78b
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.” The Astrophysical
Journal Letters. IOP Publishing, 2025. https://doi.org/10.3847/2041-8213/ade78b.
ieee: D. J. Setton et al., “A confirmed deficit of hot and cold dust emission
in the most luminous Little Red Dots,” The Astrophysical Journal Letters,
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.” The Astrophysical Journal Letters,
vol. 991, L10, IOP Publishing, 2025, doi:10.3847/2041-8213/ade78b.
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.
Astronomy & Astrophysics. 2025;701. doi:10.1051/0004-6361/202553760
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. Astronomy
& Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202553760
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.” Astronomy
& Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202553760.
ieee: S. Mascia et al., “Little impact of mergers and galaxy morphology on
the production and escape of ionizing photons in the early Universe,” Astronomy
& Astrophysics, 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 & 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.” Astronomy
& Astrophysics, vol. 701, A122, EDP Sciences, 2025, doi:10.1051/0004-6361/202553760.
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
& 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. The Astrophysical Journal. 2025;989. doi:10.3847/1538-4357/ade9a1'
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. The
Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ade9a1'
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.” The Astrophysical Journal. IOP Publishing, 2025. https://doi.org/10.3847/1538-4357/ade9a1.'
ieee: 'S. Fujimoto 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,” The Astrophysical Journal, 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.” The
Astrophysical Journal, vol. 989, 46, IOP Publishing, 2025, doi:10.3847/1538-4357/ade9a1.'
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'
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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'
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