---
OA_place: publisher
OA_type: hybrid
_id: '19879'
abstract:
- lang: eng
  text: We consider the 4-precoloring extension problem in planar near-Eulerian- triangulations,
    i.e., plane graphs where all faces except possibly for the outer one have length
    three, all vertices not incident with the outer face have even degree, and exactly
    the vertices incident with the outer face are precolored. We give a necessary
    topological condition for the precoloring to extend, and give a complete characterization
    when the outer face has length at most five and when all vertices of the outer
    face have odd degree and are colored using only three colors.
acknowledgement: Supported by project 22-17398S (Flows and cycles in graphs on surfaces)
  of Czech Science Foundation. An extended abstract appeared in Proceedings of the
  12th European Conference on Combinatorics, Graph Theory and Applications (EUROCOMB’23)
article_number: '104138'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Zdeněk
  full_name: Dvořák, Zdeněk
  last_name: Dvořák
- first_name: Benjamin
  full_name: Moore, Benjamin
  id: 6dc1a1be-bf1c-11ed-8d2b-d044840f49d6
  last_name: Moore
- first_name: Michaela
  full_name: Seifrtová, Michaela
  last_name: Seifrtová
- first_name: Robert
  full_name: Šámal, Robert
  last_name: Šámal
citation:
  ama: Dvořák Z, Moore B, Seifrtová M, Šámal R. Precoloring extension in planar near-Eulerian-triangulations.
    <i>European Journal of Combinatorics</i>. 2025;127. doi:<a href="https://doi.org/10.1016/j.ejc.2025.104138">10.1016/j.ejc.2025.104138</a>
  apa: Dvořák, Z., Moore, B., Seifrtová, M., &#38; Šámal, R. (2025). Precoloring extension
    in planar near-Eulerian-triangulations. <i>European Journal of Combinatorics</i>.
    Elsevier. <a href="https://doi.org/10.1016/j.ejc.2025.104138">https://doi.org/10.1016/j.ejc.2025.104138</a>
  chicago: Dvořák, Zdeněk, Benjamin Moore, Michaela Seifrtová, and Robert Šámal. “Precoloring
    Extension in Planar Near-Eulerian-Triangulations.” <i>European Journal of Combinatorics</i>.
    Elsevier, 2025. <a href="https://doi.org/10.1016/j.ejc.2025.104138">https://doi.org/10.1016/j.ejc.2025.104138</a>.
  ieee: Z. Dvořák, B. Moore, M. Seifrtová, and R. Šámal, “Precoloring extension in
    planar near-Eulerian-triangulations,” <i>European Journal of Combinatorics</i>,
    vol. 127. Elsevier, 2025.
  ista: Dvořák Z, Moore B, Seifrtová M, Šámal R. 2025. Precoloring extension in planar
    near-Eulerian-triangulations. European Journal of Combinatorics. 127, 104138.
  mla: Dvořák, Zdeněk, et al. “Precoloring Extension in Planar Near-Eulerian-Triangulations.”
    <i>European Journal of Combinatorics</i>, vol. 127, 104138, Elsevier, 2025, doi:<a
    href="https://doi.org/10.1016/j.ejc.2025.104138">10.1016/j.ejc.2025.104138</a>.
  short: Z. Dvořák, B. Moore, M. Seifrtová, R. Šámal, European Journal of Combinatorics
    127 (2025).
corr_author: '1'
date_created: 2025-06-23T13:54:46Z
date_published: 2025-06-01T00:00:00Z
date_updated: 2025-09-30T13:42:59Z
day: '01'
ddc:
- '510'
department:
- _id: MaKw
doi: 10.1016/j.ejc.2025.104138
external_id:
  arxiv:
  - '2312.13061'
  isi:
  - '001443061400001'
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month: '06'
oa: 1
oa_version: Published Version
publication: European Journal of Combinatorics
publication_identifier:
  issn:
  - 0195-6698
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Precoloring extension in planar near-Eulerian-triangulations
tmp:
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type: journal_article
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year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19880'
abstract:
- lang: eng
  text: We investigate quantum transport in a two-dimensional electron system coupled
    to a chiral molecular potential, demonstrating how molecular chirality and orientation
    affect charge and spin transport properties. We propose a minimal model for realizing
    true chiral symmetry breaking on a magnetized surface, with a crucial role played
    by the tilt angle of the molecular dipole with respect to the surface. For non-zero
    tilting, we show that the Hall response exhibits clear signatures of chirality-induced
    effects, in both charge- and spin-resolved observables. Concerning the former,
    tilted enantiomers produce asymmetric Hall conductances and, even more remarkably,
    the persistence of this feature in the absence of spin–orbit coupling (SOC) signals
    how the enantiospecific charge response results from electron scattering off the
    molecular potential. Concerning spin-resolved observables where SOC plays a relevant
    role, we reveal that chiral symmetry breaking is crucial in enabling spin-flipping
    processes.
acknowledgement: We thank Artem Volosniev, Narcis Avarvari, Georgios Koutentakis,
  Sandro Wimberger, and Binghai Yan for useful discussions. R.A. received funding
  from the Austrian Academy of Science ÖWA, Grant No. PR1029OEAW03. M.L. acknowledges
  support by the European Research Council (ERC) Starting Grant No. 801770 (ANGULON).
  A.C. received funding from the European Union’s Horizon Europe research and innovation
  program under the Marie Skłodowska-Curie Grant Agreement No. 101062862-NeqMolRot.
article_number: '234106'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Ragheed
  full_name: Al Hyder, Ragheed
  id: d1c405be-ae15-11ed-8510-ccf53278162e
  last_name: Al Hyder
- first_name: Mikhail
  full_name: Lemeshko, Mikhail
  id: 37CB05FA-F248-11E8-B48F-1D18A9856A87
  last_name: Lemeshko
  orcid: 0000-0002-6990-7802
- first_name: Alberto
  full_name: Cappellaro, Alberto
  id: 9d13b3cb-30a2-11eb-80dc-f772505e8660
  last_name: Cappellaro
  orcid: 0000-0001-6110-2359
citation:
  ama: Al Hyder R, Lemeshko M, Cappellaro A. Quantum transport in the presence of
    a chiral molecular potential. <i>The Journal of Chemical Physics</i>. 2025;162(23).
    doi:<a href="https://doi.org/10.1063/5.0271155">10.1063/5.0271155</a>
  apa: Al Hyder, R., Lemeshko, M., &#38; Cappellaro, A. (2025). Quantum transport
    in the presence of a chiral molecular potential. <i>The Journal of Chemical Physics</i>.
    AIP Publishing. <a href="https://doi.org/10.1063/5.0271155">https://doi.org/10.1063/5.0271155</a>
  chicago: Al Hyder, Ragheed, Mikhail Lemeshko, and Alberto Cappellaro. “Quantum Transport
    in the Presence of a Chiral Molecular Potential.” <i>The Journal of Chemical Physics</i>.
    AIP Publishing, 2025. <a href="https://doi.org/10.1063/5.0271155">https://doi.org/10.1063/5.0271155</a>.
  ieee: R. Al Hyder, M. Lemeshko, and A. Cappellaro, “Quantum transport in the presence
    of a chiral molecular potential,” <i>The Journal of Chemical Physics</i>, vol.
    162, no. 23. AIP Publishing, 2025.
  ista: Al Hyder R, Lemeshko M, Cappellaro A. 2025. Quantum transport in the presence
    of a chiral molecular potential. The Journal of Chemical Physics. 162(23), 234106.
  mla: Al Hyder, Ragheed, et al. “Quantum Transport in the Presence of a Chiral Molecular
    Potential.” <i>The Journal of Chemical Physics</i>, vol. 162, no. 23, 234106,
    AIP Publishing, 2025, doi:<a href="https://doi.org/10.1063/5.0271155">10.1063/5.0271155</a>.
  short: R. Al Hyder, M. Lemeshko, A. Cappellaro, The Journal of Chemical Physics
    162 (2025).
corr_author: '1'
date_created: 2025-06-23T13:55:28Z
date_published: 2025-06-21T00:00:00Z
date_updated: 2025-09-30T13:40:55Z
day: '21'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1063/5.0271155
ec_funded: 1
external_id:
  arxiv:
  - '2503.14124'
  isi:
  - '001512872900010'
  pmid:
  - '40526561'
file:
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has_accepted_license: '1'
intvolume: '       162'
isi: 1
issue: '23'
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 2688CF98-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '801770'
  name: 'Angulon: physics and applications of a new quasiparticle'
- _id: bd7b5202-d553-11ed-ba76-9b1c1b258338
  grant_number: '101062862'
  name: Non-Equilibrium Field Theory of Molecular Rotations
- _id: 8fa7db46-16d5-11f0-9cad-917600954daf
  grant_number: '12078'
  name: Polarons in Lead Halide Perovskites
publication: The Journal of Chemical Physics
publication_identifier:
  eissn:
  - 1089-7690
  issn:
  - 0021-9606
publication_status: published
publisher: AIP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Quantum transport in the presence of a chiral molecular potential
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 162
year: '2025'
...
---
_id: '19885'
abstract:
- lang: eng
  text: This .zip file contains the data to reproduce the figures and supplementary
    figures of "Automated All-RF Tuning for Spin Qubit Readout and Control" by Cornelius
    Carlsson and Jaime Saez-Mollejo et al.
acknowledged_ssus:
- _id: M-Shop
- _id: NanoFab
acknowledgement: 'The authors would like to thank Barnaby van Straaten, Jonas Schuff,
  Daniel Jirovec and Hanifa Tidjani for fruitful discussions. This research was supported
  by the Scientific Service Units of ISTA through resources provided by the MIBA Machine
  Shop and the Nanofabrication Facility. G.K. acknowledges support from the NOMIS
  Foundation, the HORIZON-RIA (project no. 101069515) and the FWF Projects (DOIs:
  10.55776/F86 and 10.55776/I5060). N.A. acknowledges support from the European Research
  Council (grant agreement 948932), and the Royal Society (grant no. URF/R1/191150).
  This project received support from the US Army Research Office (ARO) under Award
  No. W911NF-24-2-0043. C.C. acknowledges support from the UKRI Doctoral Training
  Partnership related to EP/W524311/1 (project ref. 2887634).'
article_processing_charge: No
author:
- first_name: Jaime
  full_name: Saez Mollejo, Jaime
  id: e0390f72-f6e0-11ea-865d-862393336714
  last_name: Saez Mollejo
citation:
  ama: Saez Mollejo J. Automated All-RF Tuning for Spin Qubit Readout and Control.
    2025. doi:<a href="https://doi.org/10.15479/AT:ISTA:19885">10.15479/AT:ISTA:19885</a>
  apa: Saez Mollejo, J. (2025). Automated All-RF Tuning for Spin Qubit Readout and
    Control. Institute of Science and Technology Austria. <a href="https://doi.org/10.15479/AT:ISTA:19885">https://doi.org/10.15479/AT:ISTA:19885</a>
  chicago: Saez Mollejo, Jaime. “Automated All-RF Tuning for Spin Qubit Readout and
    Control.” Institute of Science and Technology Austria, 2025. <a href="https://doi.org/10.15479/AT:ISTA:19885">https://doi.org/10.15479/AT:ISTA:19885</a>.
  ieee: J. Saez Mollejo, “Automated All-RF Tuning for Spin Qubit Readout and Control.”
    Institute of Science and Technology Austria, 2025.
  ista: Saez Mollejo J. 2025. Automated All-RF Tuning for Spin Qubit Readout and Control,
    Institute of Science and Technology Austria, <a href="https://doi.org/10.15479/AT:ISTA:19885">10.15479/AT:ISTA:19885</a>.
  mla: Saez Mollejo, Jaime. <i>Automated All-RF Tuning for Spin Qubit Readout and
    Control</i>. Institute of Science and Technology Austria, 2025, doi:<a href="https://doi.org/10.15479/AT:ISTA:19885">10.15479/AT:ISTA:19885</a>.
  short: J. Saez Mollejo, (2025).
contributor:
- contributor_type: researcher
  first_name: Cornelius
  last_name: Carlsson
- contributor_type: researcher
  first_name: 'Federico '
  last_name: Fedele
- contributor_type: researcher
  first_name: Stefano
  last_name: Calcaterra
- contributor_type: researcher
  first_name: ' Daniel '
  last_name: Chrastina
- contributor_type: researcher
  first_name: 'Giovanni '
  last_name: Isella
- contributor_type: researcher
  first_name: Georgios
  id: 38DB5788-F248-11E8-B48F-1D18A9856A87
  last_name: Katsaros
  orcid: 0000-0001-8342-202X
- contributor_type: researcher
  first_name: Natalia
  last_name: Ares
corr_author: '1'
date_created: 2025-06-24T06:56:03Z
date_published: 2025-06-01T00:00:00Z
date_updated: 2025-07-01T07:19:26Z
day: '01'
ddc:
- '530'
department:
- _id: GradSch
- _id: GeKa
doi: 10.15479/AT:ISTA:19885
file:
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  date_updated: 2025-06-24T15:14:13Z
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  creator: jsaezmol
  date_created: 2025-06-25T07:11:52Z
  date_updated: 2025-06-25T07:11:52Z
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  file_size: 622
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  success: 1
file_date_updated: 2025-06-25T07:11:52Z
has_accepted_license: '1'
month: '06'
oa: 1
oa_version: Published Version
project:
- _id: 34c0acea-11ca-11ed-8bc3-8775e10fd452
  grant_number: '101069515'
  name: Integrated Germanium Quantum Technology
- _id: c0977eea-5a5b-11eb-8a69-a862db0cf4d1
  grant_number: I05060
  name: High impedance circuit quantum electrodynamics with hole spins
- _id: 34a66131-11ca-11ed-8bc3-a31681c6b03e
  grant_number: F8606
  name: 'Center for Correlated Quantum Materials and Solid State Quantum Systems:
    Conventional  and unconventional topological superconductors'
publisher: Institute of Science and Technology Austria
status: public
title: Automated All-RF Tuning for Spin Qubit Readout and Control
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
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  short: CC BY (4.0)
type: research_data
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
_id: '19915'
acknowledgement: "We thank all members of the Martin Loose lab at ISTA for helpful
  discussions and Marko Kojic for critical reading of the manuscript. This research
  was supported by the Scientific Service Units (SSU) of ISTA through resources provided
  by the Imaging & Optics Facility (IOF), the Scientific Computing (SciComp) and the
  Electron Microscopy Facility (EMF), as well as the Lab Support Facility (LSF). This
  project has received funding from the European Union’s Horizon 2020 research and
  innovation program under the Marie Skłodowska-Curie Grant Agreement No.101034413
  awarded to BLS as well as an ERC grant (ActinID, 101076260) from the European Union
  awarded to FKMS. 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.\r\n\r\nWe are grateful for Antonia Herrero (Sevilla University)
  for sharing her extensive BACTH plasmid library and other plasmids as well as cyanobacterial
  strains. Likewise, we would like to thank Tal Dagan and Fabian Nies (both Kiel University)
  for sharing cyanobacterial strains and plasmids and for valuable discussions.\r\n\r\nWe
  would further like to express our gratitude to Nicolas Sapay and Alexis Michon for
  providing the Amphipaseek code, which enabled us to perform our large-scale amphipathic
  helix screen of cyanobacterial CorR proteins. Finally, we also want to thank Jesse
  Hansen for advice in cryo-EM data processing"
article_processing_charge: No
author:
- first_name: Benjamin L
  full_name: Springstein, Benjamin L
  id: b4eb62ef-ac72-11ed-9503-ed3b4d66c083
  last_name: Springstein
  orcid: 0000-0002-3461-5391
citation:
  ama: Springstein BL. Files for “Evolutionary repurposing of a DNA segregation machinery
    into a cytoskeletal system controlling cyanobacterial cell shape.” 2025. doi:<a
    href="https://doi.org/10.15479/AT:ISTA:19915">10.15479/AT:ISTA:19915</a>
  apa: Springstein, B. L. (2025). Files for “Evolutionary repurposing of a DNA segregation
    machinery into a cytoskeletal system controlling cyanobacterial cell shape.” Institute
    of Science and Technology Austria. <a href="https://doi.org/10.15479/AT:ISTA:19915">https://doi.org/10.15479/AT:ISTA:19915</a>
  chicago: Springstein, Benjamin L. “Files for ‘Evolutionary Repurposing of a DNA
    Segregation Machinery into a Cytoskeletal System Controlling Cyanobacterial Cell
    Shape.’” Institute of Science and Technology Austria, 2025. <a href="https://doi.org/10.15479/AT:ISTA:19915">https://doi.org/10.15479/AT:ISTA:19915</a>.
  ieee: B. L. Springstein, “Files for ‘Evolutionary repurposing of a DNA segregation
    machinery into a cytoskeletal system controlling cyanobacterial cell shape.’”
    Institute of Science and Technology Austria, 2025.
  ista: Springstein BL. 2025. Files for ‘Evolutionary repurposing of a DNA segregation
    machinery into a cytoskeletal system controlling cyanobacterial cell shape’, Institute
    of Science and Technology Austria, <a href="https://doi.org/10.15479/AT:ISTA:19915">10.15479/AT:ISTA:19915</a>.
  mla: Springstein, Benjamin L. <i>Files for “Evolutionary Repurposing of a DNA Segregation
    Machinery into a Cytoskeletal System Controlling Cyanobacterial Cell Shape.”</i>
    Institute of Science and Technology Austria, 2025, doi:<a href="https://doi.org/10.15479/AT:ISTA:19915">10.15479/AT:ISTA:19915</a>.
  short: B.L. Springstein, (2025).
contributor:
- contributor_type: project_leader
  first_name: Benjamin L
  id: b4eb62ef-ac72-11ed-9503-ed3b4d66c083
  last_name: Springstein
  orcid: 0000-0002-3461-5391
- contributor_type: researcher
  first_name: Manjunath
  id: 305ab18b-dc7d-11ea-9b2f-b58195228ea2
  last_name: Javoor
- contributor_type: researcher
  first_name: Daniela
  last_name: Megrian
- contributor_type: researcher
  first_name: Roman
  id: ffab949d-133f-11ed-8f02-94de21ace503
  last_name: Hajdu
- contributor_type: researcher
  first_name: Dustin M
  last_name: Hanke
- contributor_type: researcher
  first_name: Florian KM
  id: 48AD8942-F248-11E8-B48F-1D18A9856A87
  last_name: Schur
  orcid: 0000-0003-4790-8078
- contributor_type: supervisor
  first_name: Martin
  id: 462D4284-F248-11E8-B48F-1D18A9856A87
  last_name: Loose
  orcid: 0000-0001-7309-9724
corr_author: '1'
date_created: 2025-06-27T07:34:52Z
date_published: 2025-06-27T00:00:00Z
date_updated: 2025-07-02T08:25:37Z
day: '27'
department:
- _id: MaLo
doi: 10.15479/AT:ISTA:19915
ec_funded: 1
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has_accepted_license: '1'
month: '06'
oa: 1
oa_version: None
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
  call_identifier: H2020
  grant_number: '101034413'
  name: 'IST-BRIDGE: International postdoctoral program'
- _id: bd980d18-d553-11ed-ba76-ceaa645c97eb
  grant_number: '101076260'
  name: A molecular atlas of Actin filament IDentities in the cell motility machinery
publisher: Institute of Science and Technology Austria
status: public
title: Files for "Evolutionary repurposing of a DNA segregation machinery into a cytoskeletal
  system controlling cyanobacterial cell shape"
tmp:
  image: /images/cc_by_nc_nd.png
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  short: CC BY-NC-ND (4.0)
type: research_data
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year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19928'
abstract:
- lang: eng
  text: 'Patho-mechanistic origins of ulcerative colitis are still poorly understood.
    The actin cross-linker filamin A (FLNA) impacts cellular responses through interaction
    with cytosolic proteins. Posttranscriptional A-to-I editing generates two forms
    of FLNA: genome-encoded FLNAQ and FLNAR. FLNA is edited in colon fibroblasts,
    smooth muscle cells, and endothelial cells. We found that the FLNA editing status
    determines colitis severity. Editing was highest in healthy colons and reduced
    during murine and human colitis. Mice that exclusively express FLNAR were highly
    resistant to DSS-induced colitis, whereas fully FLNAQ animals developed severe
    inflammation. While the genetic induction of FLNA editing influenced transcriptional
    states of structural cells and microbiome composition, we found that FLNAR exerts
    protection specifically via myeloid cells, which are physiologically unedited.
    Introducing fixed FLNAR did not hamper cell migration but reduced macrophage inflammation
    and rendered neutrophils less prone to NETosis. Thus, loss of FLNA editing correlates
    with colitis severity, and targeted editing of myeloid cells serves as a novel
    therapeutic approach in intestinal inflammation.'
acknowledgement: "Sequencing was performed by the Vienna BioCenter Core Facilities
  (Medical University of Vienna Core Facility) and the Biomedical Sequencing Facility
  at CeMM, Vienna. Cell sorting and flow cytometry were performed at the Core Facility
  Flow Cytometry and Imaging (Medical University of Vienna). We thank Jasmin Schwarz,
  Gudrun Kohl, Petra Pjevac, and Joana Seneca Silva from the Joint Microbiome Facility
  of the Medical University of Vienna and the University of Vienna for assisting with
  amplicon and metagenomic sequencing, as well as repositing of sequencing data. We
  thank Sophia Derdak and Michael Schuster for initial data analysis, Robert Vilvoi
  and Stephan Hemm for animal handling, Marcel Kertesz for mouse genotyping, and Salwan
  Roumaia for next generation sequencing sample preparation. Treatment schemes and
  graphical abstracts were created with https://BioRender.com.\r\n\r\nThis work was
  supported by the Austrian Science Fund, grant number ZK 57-B28 to C. Vesely, R.
  Gawish, and F.C. Pereira; grant number V 1025-B to R. Gawish; grant number DOC32-B28
  to R. Varada and M.F. Jantsch; and F8007 and P32678 to M.F. Jantsch. Open Access
  funding provided by Medical University of Vienna."
article_number: e20240109
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Riem
  full_name: Gawish, Riem
  last_name: Gawish
- first_name: Rajagopal
  full_name: Varada, Rajagopal
  last_name: Varada
- first_name: Florian
  full_name: Deckert, Florian
  last_name: Deckert
- first_name: Anastasiya
  full_name: Hladik, Anastasiya
  last_name: Hladik
- first_name: Linda
  full_name: Steinbichl, Linda
  last_name: Steinbichl
- first_name: Laura
  full_name: Cimatti, Laura
  last_name: Cimatti
- first_name: Katarina
  full_name: Milanovic, Katarina
  last_name: Milanovic
- first_name: Mamta
  full_name: Jain, Mamta
  last_name: Jain
- first_name: Natalya
  full_name: Torgasheva, Natalya
  last_name: Torgasheva
- first_name: Andrea
  full_name: Tanzer, Andrea
  last_name: Tanzer
- first_name: Kim
  full_name: De Paepe, Kim
  last_name: De Paepe
- first_name: Tom
  full_name: Van De Wiele, Tom
  last_name: Van De Wiele
- first_name: Bela
  full_name: Hausmann, Bela
  last_name: Hausmann
- first_name: Michaela
  full_name: Lang, Michaela
  last_name: Lang
- first_name: Martin
  full_name: Pechhacker, Martin
  last_name: Pechhacker
- first_name: Nahla
  full_name: Ibrahim, Nahla
  last_name: Ibrahim
- first_name: Ingrid
  full_name: De Vries, Ingrid
  id: 4C7D837E-F248-11E8-B48F-1D18A9856A87
  last_name: De Vries
- first_name: Christine
  full_name: Brostjan, Christine
  last_name: Brostjan
- first_name: Michael K
  full_name: Sixt, Michael K
  id: 41E9FBEA-F248-11E8-B48F-1D18A9856A87
  last_name: Sixt
  orcid: 0000-0002-6620-9179
- first_name: Christoph
  full_name: Gasche, Christoph
  last_name: Gasche
- first_name: Louis
  full_name: Boon, Louis
  last_name: Boon
- first_name: David
  full_name: Berry, David
  last_name: Berry
- first_name: Michael F.
  full_name: Jantsch, Michael F.
  last_name: Jantsch
- first_name: Fatima C.
  full_name: Pereira, Fatima C.
  last_name: Pereira
- first_name: Cornelia
  full_name: Vesely, Cornelia
  last_name: Vesely
citation:
  ama: Gawish R, Varada R, Deckert F, et al. Filamin A editing in myeloid cells reduces
    intestinal inflammation and protects from colitis. <i>Journal of Experimental
    Medicine</i>. 2025;222(9). doi:<a href="https://doi.org/10.1084/jem.20240109">10.1084/jem.20240109</a>
  apa: Gawish, R., Varada, R., Deckert, F., Hladik, A., Steinbichl, L., Cimatti, L.,
    … Vesely, C. (2025). Filamin A editing in myeloid cells reduces intestinal inflammation
    and protects from colitis. <i>Journal of Experimental Medicine</i>. Rockefeller
    University Press. <a href="https://doi.org/10.1084/jem.20240109">https://doi.org/10.1084/jem.20240109</a>
  chicago: Gawish, Riem, Rajagopal Varada, Florian Deckert, Anastasiya Hladik, Linda
    Steinbichl, Laura Cimatti, Katarina Milanovic, et al. “Filamin A Editing in Myeloid
    Cells Reduces Intestinal Inflammation and Protects from Colitis.” <i>Journal of
    Experimental Medicine</i>. Rockefeller University Press, 2025. <a href="https://doi.org/10.1084/jem.20240109">https://doi.org/10.1084/jem.20240109</a>.
  ieee: R. Gawish <i>et al.</i>, “Filamin A editing in myeloid cells reduces intestinal
    inflammation and protects from colitis,” <i>Journal of Experimental Medicine</i>,
    vol. 222, no. 9. Rockefeller University Press, 2025.
  ista: Gawish R, Varada R, Deckert F, Hladik A, Steinbichl L, Cimatti L, Milanovic
    K, Jain M, Torgasheva N, Tanzer A, De Paepe K, Van De Wiele T, Hausmann B, Lang
    M, Pechhacker M, Ibrahim N, de Vries I, Brostjan C, Sixt MK, Gasche C, Boon L,
    Berry D, Jantsch MF, Pereira FC, Vesely C. 2025. Filamin A editing in myeloid
    cells reduces intestinal inflammation and protects from colitis. Journal of Experimental
    Medicine. 222(9), e20240109.
  mla: Gawish, Riem, et al. “Filamin A Editing in Myeloid Cells Reduces Intestinal
    Inflammation and Protects from Colitis.” <i>Journal of Experimental Medicine</i>,
    vol. 222, no. 9, e20240109, Rockefeller University Press, 2025, doi:<a href="https://doi.org/10.1084/jem.20240109">10.1084/jem.20240109</a>.
  short: R. Gawish, R. Varada, F. Deckert, A. Hladik, L. Steinbichl, L. Cimatti, K.
    Milanovic, M. Jain, N. Torgasheva, A. Tanzer, K. De Paepe, T. Van De Wiele, B.
    Hausmann, M. Lang, M. Pechhacker, N. Ibrahim, I. de Vries, C. Brostjan, M.K. Sixt,
    C. Gasche, L. Boon, D. Berry, M.F. Jantsch, F.C. Pereira, C. Vesely, Journal of
    Experimental Medicine 222 (2025).
date_created: 2025-06-29T22:01:15Z
date_published: 2025-09-01T00:00:00Z
date_updated: 2025-12-30T09:00:42Z
day: '01'
ddc:
- '570'
department:
- _id: MiSi
doi: 10.1084/jem.20240109
external_id:
  isi:
  - '001502896900001'
  pmid:
  - '40471139'
file:
- access_level: open_access
  checksum: 708d61fb8cf1d83ee1e33ddcfde0857e
  content_type: application/pdf
  creator: dernst
  date_created: 2025-12-30T09:00:04Z
  date_updated: 2025-12-30T09:00:04Z
  file_id: '20899'
  file_name: 2025_JEM_Gawish.pdf
  file_size: 9349311
  relation: main_file
  success: 1
file_date_updated: 2025-12-30T09:00:04Z
has_accepted_license: '1'
intvolume: '       222'
isi: 1
issue: '9'
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
pmid: 1
publication: Journal of Experimental Medicine
publication_identifier:
  eissn:
  - 1540-9538
  issn:
  - 0022-1007
publication_status: published
publisher: Rockefeller University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Filamin A editing in myeloid cells reduces intestinal inflammation and protects
  from colitis
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: 222
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '19929'
abstract:
- lang: eng
  text: "Context. The observed Lyman-alpha (Lyα) line profile is a convolution of
    the complex Lyα radiative transfer taking place in the interstellar, circumgalactic,
    and intergalactic media (ISM, CGM, and IGM, respectively). Discerning the different
    components of the Lyα line is crucial in order to use it as a probe of galaxy
    formation or the evolution of the IGM.\r\n\r\nAims. We aim to present the second
    version of zELDA (redshift Estimator for Line profiles of Distant Lyman-Alpha
    emitters), an open-source Python module focused on modelling and fitting observed
    Lyα line profiles. This new version of zELDA focuses on disentangling the galactic
    from the IGM effects.\r\n\r\nMethods. We built realistic Lyα line profiles that
    include the ISM and IGM contributions by combining the Monte Carlo radiative-transfer
    simulations for the so-called shell model (ISM) and IGM transmission curves generated
    from TNG100. We used these mock line profiles to train different artificial neural
    networks. These use the observed spectrum as input and the outflow parameters
    of the best fitting ‘shell model’ as output along with the redshift and Lyα emission
    IGM escape fraction of the source.\r\n\r\nResults. We measured the accuracy of
    zELDA on mock Lyα line profiles. We find that zELDA is capable of reconstructing
    the ISM emerging Lyα line profile with high levels of accuracy (Kolmogórov-Smirnov<0.1)
    for 95% of the cases for HST/COS-like observations and 80% for MUSE-WIDE-like
    observations. zELDA is able to measure the IGM transmission with typical uncertainties
    below 10% for HST/COS and MUSE-WIDE data.\r\n\r\nConclusions. This work represents
    a step forward in the high-precision reconstruction of IGM-attenuated Lyα line
    profiles. zELDA allows the disentanglement of the galactic and IGM contribution
    shaping the Lyα line shape and thus allows us to use Lyα as a tool to study galaxy
    and ISM evolution."
acknowledgement: The authors acknowledge the financial support from the MICIU with
  funding from the European Union NextGenerationEU and Generalitat Valenciana in the
  call Programa de Planes Complementarios de I+D+i (PRTR 2022) Project (VAL-JPAS),
  reference ASFAE/2022/025. This work is part of the research Project PID2023-149420NB-I00
  funded by MICIU/AEI/10.13039/501100011033 and by ERDF/EU. This work is also supported
  by the project of excellence PROMETEO CIPROM/2023/21 of the Conselleria de Educación,
  Universidades y Empleo (Generalitat Valenciana). MG thanks the Max Planck Society
  for support through the Max Planck Research Group. DS acknowledges the support by
  the Tsinghua Shui Mu Scholarship, funding of the National Key R&D Program of China
  (grant no. 2023YFA1605600), the science research grants from the China Manned Space
  Project with no. CMS-CSST2021-A05, and the Tsinghua University Initiative Scientific
  Research Program (no. 20223080023). This research made use of matplotlib, a Python
  library for publication quality graphics (Hunter 2007), NumPy (Harris et al. 2020)
  and SciPy (Virtanen et al. 2020).
article_number: A139
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Siddhartha
  full_name: Gurung-López, Siddhartha
  last_name: Gurung-López
- first_name: Chris
  full_name: Byrohl, Chris
  last_name: Byrohl
- first_name: Max
  full_name: Gronke, Max
  last_name: Gronke
- first_name: Daniele
  full_name: Spinoso, Daniele
  last_name: Spinoso
- first_name: Alberto
  full_name: Torralba Torregrosa, Alberto
  id: 018f0249-0e87-11f0-b167-cbce08fbd541
  last_name: Torralba Torregrosa
  orcid: 0000-0001-5586-6950
- first_name: Alberto
  full_name: Fernández-Soto, Alberto
  last_name: Fernández-Soto
- first_name: Pablo
  full_name: Arnalte-Mur, Pablo
  last_name: Arnalte-Mur
- first_name: Vicent J.
  full_name: Martínez, Vicent J.
  last_name: Martínez
citation:
  ama: 'Gurung-López S, Byrohl C, Gronke M, et al. zELDA II: Reconstruction of galactic
    Lyman-alpha spectra attenuated by the intergalactic medium using neural networks.
    <i>Astronomy &#38; Astrophysics</i>. 2025;698. doi:<a href="https://doi.org/10.1051/0004-6361/202453547">10.1051/0004-6361/202453547</a>'
  apa: 'Gurung-López, S., Byrohl, C., Gronke, M., Spinoso, D., Torralba Torregrosa,
    A., Fernández-Soto, A., … Martínez, V. J. (2025). zELDA II: Reconstruction of
    galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural
    networks. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/202453547">https://doi.org/10.1051/0004-6361/202453547</a>'
  chicago: 'Gurung-López, Siddhartha, Chris Byrohl, Max Gronke, Daniele Spinoso, Alberto
    Torralba Torregrosa, Alberto Fernández-Soto, Pablo Arnalte-Mur, and Vicent J.
    Martínez. “ZELDA II: Reconstruction of Galactic Lyman-Alpha Spectra Attenuated
    by the Intergalactic Medium Using Neural Networks.” <i>Astronomy &#38; Astrophysics</i>.
    EDP Sciences, 2025. <a href="https://doi.org/10.1051/0004-6361/202453547">https://doi.org/10.1051/0004-6361/202453547</a>.'
  ieee: 'S. Gurung-López <i>et al.</i>, “zELDA II: Reconstruction of galactic Lyman-alpha
    spectra attenuated by the intergalactic medium using neural networks,” <i>Astronomy
    &#38; Astrophysics</i>, vol. 698. EDP Sciences, 2025.'
  ista: 'Gurung-López S, Byrohl C, Gronke M, Spinoso D, Torralba Torregrosa A, Fernández-Soto
    A, Arnalte-Mur P, Martínez VJ. 2025. zELDA II: Reconstruction of galactic Lyman-alpha
    spectra attenuated by the intergalactic medium using neural networks. Astronomy
    &#38; Astrophysics. 698, A139.'
  mla: 'Gurung-López, Siddhartha, et al. “ZELDA II: Reconstruction of Galactic Lyman-Alpha
    Spectra Attenuated by the Intergalactic Medium Using Neural Networks.” <i>Astronomy
    &#38; Astrophysics</i>, vol. 698, A139, EDP Sciences, 2025, doi:<a href="https://doi.org/10.1051/0004-6361/202453547">10.1051/0004-6361/202453547</a>.'
  short: S. Gurung-López, C. Byrohl, M. Gronke, D. Spinoso, A. Torralba Torregrosa,
    A. Fernández-Soto, P. Arnalte-Mur, V.J. Martínez, Astronomy &#38; Astrophysics
    698 (2025).
date_created: 2025-06-29T22:01:15Z
date_published: 2025-06-01T00:00:00Z
date_updated: 2026-02-16T12:11:56Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202453547
external_id:
  arxiv:
  - '2501.04077'
  isi:
  - '001507317300003'
file:
- access_level: open_access
  checksum: a50a817b72f03534c6a867035b51e433
  content_type: application/pdf
  creator: dernst
  date_created: 2025-06-30T08:28:40Z
  date_updated: 2025-06-30T08:28:40Z
  file_id: '19933'
  file_name: 2025_AstronomyAstrophysics_GurungLopez.pdf
  file_size: 5758102
  relation: main_file
  success: 1
file_date_updated: 2025-06-30T08:28:40Z
has_accepted_license: '1'
intvolume: '       698'
isi: 1
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
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: 'zELDA II: Reconstruction of galactic Lyman-alpha spectra attenuated by the
  intergalactic medium using neural networks'
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: 698
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '19930'
abstract:
- lang: eng
  text: We present an analysis of the UV continuum slope, β, using a sample of 726
    galaxies with z > 4, selected from a mixture of JWST ERS, GTO, and GO observational
    programs. We considered only spectroscopic data obtained with the low-resolution
    (R ∼ 30 − 300) PRISM/CLEAR NIRSpec configuration. Studying the correlation between
    β and MUV, we find an overall decreasing trend, described by β = ( − 0.055 ± 0.017)MUV + ( − 2.98 ± 0.34).
    This is consistent with previous studies, where brighter galaxies show redder
    β values. However, when analyzing the trend in separate redshift bins, we find
    that at high redshift the relation becomes much flatter and is consistent with
    a flat slope within 1σ. Furthermore, we find that β tends to decrease with redshift,
    following β = ( − 0.075 ± 0.010)z + ( − 1.496 ± 0.056). This is consistent with
    most recent results showing a steepening of the spectra at higher z. We selected
    a sample of galaxies with extremely blue slopes (i.e., β < −2.6). Such slopes
    are steeper than predicted by stellar evolution models – even for dust-free, young,
    metal-poor populations – when the contribution of nebular emission is included.
    We selected 44 extremely blue galaxies (XBGs) and investigated the possible physical
    origin of their steep slopes by comparing them to a subsample of redder galaxies
    (matched in Δz = ±0.5 and ΔMUV = ±0.2). We find that XBGs have younger stellar
    populations, stronger ionization fields, lower dust attenuation, and lower but
    not pristine metallicity (∼10% Z⊙) compared to red galaxies. However, these properties
    alone cannot explain the extreme β values. Using indirect inference of Lyman continuum
    escape with the most recent models, we estimated the escape fraction fesc > 10%
    in at least 25% of the XBGs, whereas all the red sources exhibit much lower fesc
    values. A reduced nebular continuum contribution – resulting from either a high
    escape fraction or a bursty star formation history – is likely the origin of the
    extremely blue slopes.
acknowledgement: We acknowledges support from the INAF Large Grant for Extragalactic
  Surveys with JWST and from the PRIN 2022 MUR project 2022CB3PJ3 – First Light And
  Galaxy aSsembly (FLAGS) funded by the European Union – Next Generation EU. PS acknowledges
  INAF Mini Grant 2022 “The evolution of passive galaxies through cosmic time”. Part
  of the research activities described in this paper were carried out with the contribution
  of the Next Generation EU funds within the National Recovery and Resilience Plan
  (PNRR), Mission 4 – Education and Research, Component 2 – From Research to Business
  (M4C2), Investment Line 3.1 – Strengthening and creation of Research Infrastructures,
  Project IR0000034 – “STILES – Strengthening the Italian Leadership in ELT and SKA”.
  RA acknowledges support of Grant project 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.
article_number: A234
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: D.
  full_name: Dottorini, D.
  last_name: Dottorini
- first_name: A.
  full_name: Calabrò, A.
  last_name: Calabrò
- first_name: L.
  full_name: Pentericci, L.
  last_name: Pentericci
- first_name: Sara
  full_name: Mascia, Sara
  id: edaf889c-c7cd-11ef-ab1b-bb28c431bd29
  last_name: Mascia
- first_name: M.
  full_name: Llerena, M.
  last_name: Llerena
- first_name: L.
  full_name: Napolitano, L.
  last_name: Napolitano
- first_name: P.
  full_name: Santini, P.
  last_name: Santini
- first_name: G.
  full_name: Roberts-Borsani, G.
  last_name: Roberts-Borsani
- first_name: M.
  full_name: Castellano, M.
  last_name: Castellano
- first_name: R.
  full_name: Amorin, R.
  last_name: Amorin
- first_name: M.
  full_name: Dickinson, M.
  last_name: Dickinson
- first_name: A.
  full_name: Fontana, A.
  last_name: Fontana
- first_name: N.
  full_name: Hathi, N.
  last_name: Hathi
- first_name: M.
  full_name: Hirschmann, M.
  last_name: Hirschmann
- 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: E.
  full_name: Merlin, E.
  last_name: Merlin
- first_name: A.
  full_name: Morales, A.
  last_name: Morales
- first_name: F.
  full_name: Pacucci, F.
  last_name: Pacucci
- first_name: S.
  full_name: Wilkins, S.
  last_name: Wilkins
- first_name: P.
  full_name: Arrabal Haro, P.
  last_name: Arrabal Haro
- first_name: M.
  full_name: Bagley, M.
  last_name: Bagley
- first_name: S. L.
  full_name: Finkelstein, S. L.
  last_name: Finkelstein
- first_name: J.
  full_name: Kartaltepe, J.
  last_name: Kartaltepe
- first_name: C.
  full_name: Papovich, C.
  last_name: Papovich
- first_name: N.
  full_name: Pirzkal, N.
  last_name: Pirzkal
citation:
  ama: 'Dottorini D, Calabrò A, Pentericci L, et al. Evolution of the UV slope of
    galaxies at cosmic morning (z &#62; 4): The properties of extremely blue galaxies.
    <i>Astronomy &#38; Astrophysics</i>. 2025;698. doi:<a href="https://doi.org/10.1051/0004-6361/202453267">10.1051/0004-6361/202453267</a>'
  apa: 'Dottorini, D., Calabrò, A., Pentericci, L., Mascia, S., Llerena, M., Napolitano,
    L., … Pirzkal, N. (2025). Evolution of the UV slope of galaxies at cosmic morning
    (z &#62; 4): The properties of extremely blue galaxies. <i>Astronomy &#38; Astrophysics</i>.
    EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/202453267">https://doi.org/10.1051/0004-6361/202453267</a>'
  chicago: 'Dottorini, D., A. Calabrò, L. Pentericci, Sara Mascia, M. Llerena, L.
    Napolitano, P. Santini, et al. “Evolution of the UV Slope of Galaxies at Cosmic
    Morning (z &#62; 4): The Properties of Extremely Blue Galaxies.” <i>Astronomy
    &#38; Astrophysics</i>. EDP Sciences, 2025. <a href="https://doi.org/10.1051/0004-6361/202453267">https://doi.org/10.1051/0004-6361/202453267</a>.'
  ieee: 'D. Dottorini <i>et al.</i>, “Evolution of the UV slope of galaxies at cosmic
    morning (z &#62; 4): The properties of extremely blue galaxies,” <i>Astronomy
    &#38; Astrophysics</i>, vol. 698. EDP Sciences, 2025.'
  ista: 'Dottorini D, Calabrò A, Pentericci L, Mascia S, Llerena M, Napolitano L,
    Santini P, Roberts-Borsani G, Castellano M, Amorin R, Dickinson M, Fontana A,
    Hathi N, Hirschmann M, Koekemoer AM, Lucas RA, Merlin E, Morales A, Pacucci F,
    Wilkins S, Arrabal Haro P, Bagley M, Finkelstein SL, Kartaltepe J, Papovich C,
    Pirzkal N. 2025. Evolution of the UV slope of galaxies at cosmic morning (z &#62;
    4): The properties of extremely blue galaxies. Astronomy &#38; Astrophysics. 698,
    A234.'
  mla: 'Dottorini, D., et al. “Evolution of the UV Slope of Galaxies at Cosmic Morning
    (z &#62; 4): The Properties of Extremely Blue Galaxies.” <i>Astronomy &#38; Astrophysics</i>,
    vol. 698, A234, EDP Sciences, 2025, doi:<a href="https://doi.org/10.1051/0004-6361/202453267">10.1051/0004-6361/202453267</a>.'
  short: D. Dottorini, A. Calabrò, L. Pentericci, S. Mascia, M. Llerena, L. Napolitano,
    P. Santini, G. Roberts-Borsani, M. Castellano, R. Amorin, M. Dickinson, A. Fontana,
    N. Hathi, M. Hirschmann, A.M. Koekemoer, R.A. Lucas, E. Merlin, A. Morales, F.
    Pacucci, S. Wilkins, P. Arrabal Haro, M. Bagley, S.L. Finkelstein, J. Kartaltepe,
    C. Papovich, N. Pirzkal, Astronomy &#38; Astrophysics 698 (2025).
date_created: 2025-06-29T22:01:15Z
date_published: 2025-06-01T00:00:00Z
date_updated: 2026-02-16T12:11:39Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202453267
external_id:
  arxiv:
  - '2412.01623'
  isi:
  - '001510826300019'
file:
- access_level: open_access
  checksum: 100f897d468de9d0113277c870035b62
  content_type: application/pdf
  creator: dernst
  date_created: 2025-06-30T08:22:08Z
  date_updated: 2025-06-30T08:22:08Z
  file_id: '19932'
  file_name: 2025_AstronomyAstrophysics_Dottorini.pdf
  file_size: 2442076
  relation: main_file
  success: 1
file_date_updated: 2025-06-30T08:22:08Z
has_accepted_license: '1'
intvolume: '       698'
isi: 1
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
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: 'Evolution of the UV slope of galaxies at cosmic morning (z > 4): The properties
  of extremely blue galaxies'
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: 698
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '19931'
abstract:
- lang: eng
  text: JWST observations have uncovered a new population of red, compact objects
    at high redshifts dubbed “little red dots” (LRDs), which typically show broad
    emission lines and are thought to be dusty active galactic nuclei (AGNs). Some
    of their other features, however, challenge the AGN explanation, such as prominent
    Balmer breaks and extremely faint or even missing metal high-ionization lines,
    X-ray, or radio emission, including in deep stacks. Time variability is another
    robust test of AGN activity. Here, we exploit the z = 7.045 multiply imaged LRD
    A2744-QSO1, which offers a particularly unique test of variability due to lensing-induced
    time delays between the three images spanning 22 yr (2.7 yr in the rest-frame),
    to investigate its photometric and spectroscopic variability. We find the equivalent
    widths (EWs) of the broad Hα and Hβ lines, which are independent of magnification
    and other systematics, to exhibit significant variations, of up to 18 ± 3% for
    Hα and up to 22 ± 8% in Hβ, on a timescale of 875 d (2.4 yr) in the rest-frame.
    This suggests that A2744-QSO1 is indeed an AGN. We find no significant photometric
    variability beyond the limiting systematic uncertainties, so it currently cannot
    be determined whether the EW variations are due to line-flux or continuum variability.
    These results are consistent with a typical damped random walk variability model
    for an AGN such as A2744-QSO1 (MBH = 4 × 107 M⊙) given the sparse sampling of
    the light curve with the available data. Our results therefore support the AGN
    interpretation of this LRD, and highlight the need for further photometric and
    spectroscopic monitoring in order to build a detailed and reliable light curve.
acknowledgement: 'We would like to thank Xihan Ji, Hannah Übler, and Roberto Maiolino,
  for cordial and useful discussions. The BGU lensing group 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.D. warmly thanks the European
  Commission’s and University of Groningen’s CO-FUND Rosalind Franklin program. This
  work is based on observations obtained with the NASA/ESA/CSA JWST, namely programs
  GO-2756, -2561, -2883, -3538, -4111, and -3516, retrieved from the Mikulski Archive
  for Space Telescopes (MAST) at the Space Telescope Science Institute (STScI). STScI
  is operated by the Association of Universities for Research in Astronomy, Inc. under
  NASA contract NAS 5-26555. The spectroscopy products presented herein, from JWST
  program GO-2561, 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 data used in this work may be retrieved from
  the MAST archive at: http://dx.doi.org/10.17909/p7t7-te67. This work also makes
  use of the Center for Computational Astrophysics at the Flatiron Institute which
  is supported by the Simons Foundation. Support for JWST programs GO-2561, -4111,
  and -3516 was provided by NASA through grants from STScI. This research made use
  of Astropy, (http://www.astropy.org) a community-developed core Python package for
  Astronomy (Astropy Collaboration 2013, 2018) and Photutils, an Astropy package for
  detection and photometry of astronomical sources (Bradley et al. 2024), as well
  as the packages NumPy (van der Walt et al. 2011), SciPy (Virtanen et al. 2020),
  Matplotlib (Hunter 2007), and the MAAT Astronomy and Astrophysics tools for MATLAB
  (Ofek 2014).'
article_number: A227
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Lukas J.
  full_name: Furtak, Lukas J.
  last_name: Furtak
- first_name: Amy R.
  full_name: Secunda, Amy R.
  last_name: Secunda
- first_name: Jenny E.
  full_name: Greene, Jenny E.
  last_name: Greene
- first_name: Adi
  full_name: Zitrin, Adi
  last_name: Zitrin
- first_name: Ivo
  full_name: Labbé, Ivo
  last_name: Labbé
- first_name: Miriam
  full_name: Golubchik, Miriam
  last_name: Golubchik
- first_name: Rachel
  full_name: Bezanson, Rachel
  last_name: Bezanson
- first_name: Vasily
  full_name: Kokorev, Vasily
  last_name: Kokorev
- first_name: Hakim
  full_name: Atek, Hakim
  last_name: Atek
- first_name: Gabriel B.
  full_name: Brammer, Gabriel B.
  last_name: Brammer
- first_name: Iryna
  full_name: Chemerynska, Iryna
  last_name: Chemerynska
- first_name: Sam E.
  full_name: Cutler, Sam E.
  last_name: Cutler
- first_name: Pratika
  full_name: Dayal, Pratika
  last_name: Dayal
- first_name: Robert
  full_name: Feldmann, Robert
  last_name: Feldmann
- first_name: Seiji
  full_name: Fujimoto, Seiji
  last_name: Fujimoto
- first_name: Karl
  full_name: Glazebrook, Karl
  last_name: Glazebrook
- first_name: Joel
  full_name: Leja, Joel
  last_name: Leja
- first_name: Yilun
  full_name: Ma, Yilun
  last_name: Ma
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: Rohan P.
  full_name: Naidu, Rohan P.
  last_name: Naidu
- first_name: Erica J.
  full_name: Nelson, Erica J.
  last_name: Nelson
- 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: Bingjie
  full_name: Wang, Bingjie
  last_name: Wang
- first_name: John R.
  full_name: Weaver, John R.
  last_name: Weaver
- first_name: Katherine E.
  full_name: Whitaker, Katherine E.
  last_name: Whitaker
citation:
  ama: Furtak LJ, Secunda AR, Greene JE, et al. Investigating photometric and spectroscopic
    variability in the multiply imaged little red dot A2744-QSO1. <i>Astronomy &#38;
    Astrophysics</i>. 2025;698. doi:<a href="https://doi.org/10.1051/0004-6361/202554110">10.1051/0004-6361/202554110</a>
  apa: Furtak, L. J., Secunda, A. R., Greene, J. E., Zitrin, A., Labbé, I., Golubchik,
    M., … Whitaker, K. E. (2025). Investigating photometric and spectroscopic variability
    in the multiply imaged little red dot A2744-QSO1. <i>Astronomy &#38; Astrophysics</i>.
    EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/202554110">https://doi.org/10.1051/0004-6361/202554110</a>
  chicago: Furtak, Lukas J., Amy R. Secunda, Jenny E. Greene, Adi Zitrin, Ivo Labbé,
    Miriam Golubchik, Rachel Bezanson, et al. “Investigating Photometric and Spectroscopic
    Variability in the Multiply Imaged Little Red Dot A2744-QSO1.” <i>Astronomy &#38;
    Astrophysics</i>. EDP Sciences, 2025. <a href="https://doi.org/10.1051/0004-6361/202554110">https://doi.org/10.1051/0004-6361/202554110</a>.
  ieee: L. J. Furtak <i>et al.</i>, “Investigating photometric and spectroscopic variability
    in the multiply imaged little red dot A2744-QSO1,” <i>Astronomy &#38; Astrophysics</i>,
    vol. 698. EDP Sciences, 2025.
  ista: Furtak LJ, Secunda AR, Greene JE, Zitrin A, Labbé I, Golubchik M, Bezanson
    R, Kokorev V, Atek H, Brammer GB, Chemerynska I, Cutler SE, Dayal P, Feldmann
    R, Fujimoto S, Glazebrook K, Leja J, Ma Y, Matthee JJ, Naidu RP, Nelson EJ, Oesch
    PA, Pan R, Price SH, Suess KA, Wang B, Weaver JR, Whitaker KE. 2025. Investigating
    photometric and spectroscopic variability in the multiply imaged little red dot
    A2744-QSO1. Astronomy &#38; Astrophysics. 698, A227.
  mla: Furtak, Lukas J., et al. “Investigating Photometric and Spectroscopic Variability
    in the Multiply Imaged Little Red Dot A2744-QSO1.” <i>Astronomy &#38; Astrophysics</i>,
    vol. 698, A227, EDP Sciences, 2025, doi:<a href="https://doi.org/10.1051/0004-6361/202554110">10.1051/0004-6361/202554110</a>.
  short: L.J. Furtak, A.R. Secunda, J.E. Greene, A. Zitrin, I. Labbé, M. Golubchik,
    R. Bezanson, V. Kokorev, H. Atek, G.B. Brammer, I. Chemerynska, S.E. Cutler, P.
    Dayal, R. Feldmann, S. Fujimoto, K. Glazebrook, J. Leja, Y. Ma, J.J. Matthee,
    R.P. Naidu, E.J. Nelson, P.A. Oesch, R. Pan, S.H. Price, K.A. Suess, B. Wang,
    J.R. Weaver, K.E. Whitaker, Astronomy &#38; Astrophysics 698 (2025).
date_created: 2025-06-29T22:01:16Z
date_published: 2025-06-01T00:00:00Z
date_updated: 2026-02-16T12:11:22Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202554110
external_id:
  arxiv:
  - '2502.07875'
  isi:
  - '001510826300017'
file:
- access_level: open_access
  checksum: 567fa02a9791d489355ec75d02bb1cb9
  content_type: application/pdf
  creator: dernst
  date_created: 2025-06-30T08:44:24Z
  date_updated: 2025-06-30T08:44:24Z
  file_id: '19934'
  file_name: 2025_AstronomyAstrophysics_Furtak.pdf
  file_size: 1835865
  relation: main_file
  success: 1
file_date_updated: 2025-06-30T08:44:24Z
has_accepted_license: '1'
intvolume: '       698'
isi: 1
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
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: Investigating photometric and spectroscopic variability in the multiply imaged
  little red dot A2744-QSO1
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: 698
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19935'
abstract:
- lang: eng
  text: "The separation logic framework Iris has been built on the premise that all
    assertions are stable, meaning they unconditionally enjoy the famous frame rule.
    This gives Iris—and the numerous program logics that build on it—very modular
    reasoning principles. But stability also comes at a cost. It excludes a core feature
    of the Viper verifier family, heap-dependent expression assertions, which lift
    program expressions to the assertion level in order to reduce redundancy between
    code and specifications and better facilitate SMT-based automation.\r\nIn this
    paper, we bring heap-dependent expression assertions to Iris with Daenerys. To
    do so, we must first revisit the very core of Iris, extending it with a new form
    of unstable resources (and adapting the frame rule accordingly). On top, we then
    build a program logic with heap-dependent expression assertions and lay the foundations
    for connecting Iris to SMT solvers. We apply Daenerys to several case studies,
    including some that go beyond what Viper and Iris can do individually and others
    that benefit from the connection to SMT."
acknowledgement: "We would like to thank the anonymous reviewers for their helpful
  feedback and Alex Summers\r\nfor insightful discussions. This work was funded in
  part by a Google PhD Fellowship for the first\r\nauthor."
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Simon
  full_name: Spies, Simon
  last_name: Spies
- first_name: Niklas
  full_name: Mück, Niklas
  last_name: Mück
- first_name: Haoyi
  full_name: Zeng, Haoyi
  last_name: Zeng
- first_name: Michael Joachim
  full_name: Sammler, Michael Joachim
  id: 510d3901-2a03-11ee-914d-d9ae9011f0a7
  last_name: Sammler
- first_name: Andrea
  full_name: Lattuada, Andrea
  last_name: Lattuada
- first_name: Peter
  full_name: Müller, Peter
  last_name: Müller
- first_name: Derek
  full_name: Dreyer, Derek
  last_name: Dreyer
citation:
  ama: Spies S, Mück N, Zeng H, et al. Destabilizing Iris. <i>Proceedings of the ACM
    on Programming Languages</i>. 2025;9(PLDI):848-873. doi:<a href="https://doi.org/10.1145/3729284">10.1145/3729284</a>
  apa: Spies, S., Mück, N., Zeng, H., Sammler, M. J., Lattuada, A., Müller, P., &#38;
    Dreyer, D. (2025). Destabilizing Iris. <i>Proceedings of the ACM on Programming
    Languages</i>. Association for Computing Machinery. <a href="https://doi.org/10.1145/3729284">https://doi.org/10.1145/3729284</a>
  chicago: Spies, Simon, Niklas Mück, Haoyi Zeng, Michael Joachim Sammler, Andrea
    Lattuada, Peter Müller, and Derek Dreyer. “Destabilizing Iris.” <i>Proceedings
    of the ACM on Programming Languages</i>. Association for Computing Machinery,
    2025. <a href="https://doi.org/10.1145/3729284">https://doi.org/10.1145/3729284</a>.
  ieee: S. Spies <i>et al.</i>, “Destabilizing Iris,” <i>Proceedings of the ACM on
    Programming Languages</i>, vol. 9, no. PLDI. Association for Computing Machinery,
    pp. 848–873, 2025.
  ista: Spies S, Mück N, Zeng H, Sammler MJ, Lattuada A, Müller P, Dreyer D. 2025.
    Destabilizing Iris. Proceedings of the ACM on Programming Languages. 9(PLDI),
    848–873.
  mla: Spies, Simon, et al. “Destabilizing Iris.” <i>Proceedings of the ACM on Programming
    Languages</i>, vol. 9, no. PLDI, Association for Computing Machinery, 2025, pp.
    848–73, doi:<a href="https://doi.org/10.1145/3729284">10.1145/3729284</a>.
  short: S. Spies, N. Mück, H. Zeng, M.J. Sammler, A. Lattuada, P. Müller, D. Dreyer,
    Proceedings of the ACM on Programming Languages 9 (2025) 848–873.
corr_author: '1'
date_created: 2025-06-30T08:47:31Z
date_published: 2025-06-01T00:00:00Z
date_updated: 2025-06-30T09:10:11Z
day: '01'
ddc:
- '000'
department:
- _id: MiSa
doi: 10.1145/3729284
file:
- access_level: open_access
  checksum: 6b72d84c10a10ba7cd1646e2c36dc1ff
  content_type: application/pdf
  creator: dernst
  date_created: 2025-06-30T09:01:08Z
  date_updated: 2025-06-30T09:01:08Z
  file_id: '19938'
  file_name: 2025_ProcACMProg_Spies.pdf
  file_size: 843343
  relation: main_file
  success: 1
file_date_updated: 2025-06-30T09:01:08Z
has_accepted_license: '1'
intvolume: '         9'
issue: PLDI
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
page: 848-873
publication: Proceedings of the ACM on Programming Languages
publication_identifier:
  eissn:
  - 2475-1421
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: Destabilizing Iris
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
_id: '19936'
abstract:
- lang: eng
  text: 'There has been a recent upsurge of interest in formal, machine-checked verification
    of timing guarantees for C implementations of real-time system schedulers. However,
    prior work has only considered tick-based schedulers, which enjoy a clearly defined
    notion of time: the time "quantum". In this work, we present a new approach to
    real-time systems verification for interrupt-free schedulers, which are commonly
    used in deeply embedded and resource-constrained systems but which do not enjoy
    a natural notion of periodic time. Our approach builds on and connects two recently
    developed Rocq-based systems—RefinedC (for foundational C verification) and Prosa
    (for verified response-time analysis)—adapting the former to reason about timed
    traces and the latter to reason about overheads. We apply the resulting system,
    which we call RefinedProsa, to verify Rössl, a simple yet representative, fixed-priority,
    non-preemptive, interrupt-free scheduler implemented in C.'
acknowledgement: "We would like to thank the anonymous reviewers for their helpful
  feedback.\r\nThis project has received funding from the European Research Council
  (ERC) under the European\r\nUnion’s Horizon 2020 research and innovation programme
  (grant agreement No 803111)."
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Kimaya
  full_name: Bedarkar, Kimaya
  last_name: Bedarkar
- first_name: Laila
  full_name: Elbeheiry, Laila
  last_name: Elbeheiry
- first_name: Michael Joachim
  full_name: Sammler, Michael Joachim
  id: 510d3901-2a03-11ee-914d-d9ae9011f0a7
  last_name: Sammler
- first_name: Lennard
  full_name: Gäher, Lennard
  last_name: Gäher
- first_name: Björn
  full_name: Brandenburg, Björn
  last_name: Brandenburg
- first_name: Derek
  full_name: Dreyer, Derek
  last_name: Dreyer
- first_name: Deepak
  full_name: Garg, Deepak
  last_name: Garg
citation:
  ama: 'Bedarkar K, Elbeheiry L, Sammler MJ, et al. RefinedProsa: Connecting response-time
    analysis with C verification for interrupt-free schedulers. <i>Proceedings of
    the ACM on Programming Languages</i>. 2025;9(PLDI):73-97. doi:<a href="https://doi.org/10.1145/3729249">10.1145/3729249</a>'
  apa: 'Bedarkar, K., Elbeheiry, L., Sammler, M. J., Gäher, L., Brandenburg, B., Dreyer,
    D., &#38; Garg, D. (2025). RefinedProsa: Connecting response-time analysis with
    C verification for interrupt-free schedulers. <i>Proceedings of the ACM on Programming
    Languages</i>. Association for Computing Machinery. <a href="https://doi.org/10.1145/3729249">https://doi.org/10.1145/3729249</a>'
  chicago: 'Bedarkar, Kimaya, Laila Elbeheiry, Michael Joachim Sammler, Lennard Gäher,
    Björn Brandenburg, Derek Dreyer, and Deepak Garg. “RefinedProsa: Connecting Response-Time
    Analysis with C Verification for Interrupt-Free Schedulers.” <i>Proceedings of
    the ACM on Programming Languages</i>. Association for Computing Machinery, 2025.
    <a href="https://doi.org/10.1145/3729249">https://doi.org/10.1145/3729249</a>.'
  ieee: 'K. Bedarkar <i>et al.</i>, “RefinedProsa: Connecting response-time analysis
    with C verification for interrupt-free schedulers,” <i>Proceedings of the ACM
    on Programming Languages</i>, vol. 9, no. PLDI. Association for Computing Machinery,
    pp. 73–97, 2025.'
  ista: 'Bedarkar K, Elbeheiry L, Sammler MJ, Gäher L, Brandenburg B, Dreyer D, Garg
    D. 2025. RefinedProsa: Connecting response-time analysis with C verification for
    interrupt-free schedulers. Proceedings of the ACM on Programming Languages. 9(PLDI),
    73–97.'
  mla: 'Bedarkar, Kimaya, et al. “RefinedProsa: Connecting Response-Time Analysis
    with C Verification for Interrupt-Free Schedulers.” <i>Proceedings of the ACM
    on Programming Languages</i>, vol. 9, no. PLDI, Association for Computing Machinery,
    2025, pp. 73–97, doi:<a href="https://doi.org/10.1145/3729249">10.1145/3729249</a>.'
  short: K. Bedarkar, L. Elbeheiry, M.J. Sammler, L. Gäher, B. Brandenburg, D. Dreyer,
    D. Garg, Proceedings of the ACM on Programming Languages 9 (2025) 73–97.
corr_author: '1'
date_created: 2025-06-30T08:47:58Z
date_published: 2025-06-13T00:00:00Z
date_updated: 2025-06-30T09:09:55Z
day: '13'
ddc:
- '000'
department:
- _id: MiSa
doi: 10.1145/3729249
file:
- access_level: open_access
  checksum: 8c18d777feb342a7265c54b16205ec4c
  content_type: application/pdf
  creator: dernst
  date_created: 2025-06-30T09:08:05Z
  date_updated: 2025-06-30T09:08:05Z
  file_id: '19939'
  file_name: 2025_ProcACMProg_Bedarkar.pdf
  file_size: 1043790
  relation: main_file
  success: 1
file_date_updated: 2025-06-30T09:08:05Z
has_accepted_license: '1'
intvolume: '         9'
issue: PLDI
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
page: 73-97
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: 'RefinedProsa: Connecting response-time analysis with C verification for interrupt-free
  schedulers'
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_type: closed access
_id: '19937'
abstract:
- lang: eng
  text: Simplets are elementary units within simplicial complexes and are fundamental
    for analyzing the structure of simplicial complexes. Previous efforts have mainly
    focused on accurately counting or approximating the number of simplets rather
    than studying their frequencies. However, analyzing simplet frequencies is more
    practical for large-scale simplicial complexes. This paper introduces the Simplet
    Frequency Distribution (SFD) vector, which enables the analysis of simplet frequencies
    in simplicial complexes. Additionally, we provide a bound on the sample complexity
    required to approximate the SFD vector using any uniform sampling-based algorithm
    accurately. We extend the definition of simplet frequency distribution to encompass
    simplices, allowing for the analysis of simplet frequencies within simplices of
    simplicial complexes. This paper introduces the Simplet Degree Vector (SDV) and
    the Simplet Degree Centrality (SDC), facilitating this analysis for each simplex.
    Furthermore, we present a bound on the sample complexity required for accurately
    approximating the SDV and SDC for a set of simplices using any uniform sampling-based
    algorithm. We also introduce algorithms for approximating SFD, geometric SFD,
    SDV, and SDC. We also validate the theoretical bounds with experiments on random
    simplicial complexes and demonstrate the practical application through a case
    study.
acknowledgement: "The authors would like to thank the anonymous reviewers for their
  valuable comments and suggestions, which improved this paper.\r\nWork by the first
  and fourth authors is partially supported by the European Research Council (ERC),
  grant no. 788183, by the Wittgenstein Prize, Austrian Science Fund (FWF), grant
  no. Z 342-N31, and by the DFG Collaborative Research Center TRR 109, Austrian Science
  Fund (FWF), grant no. I 02979-N35."
article_number: '122425'
article_processing_charge: No
article_type: original
author:
- first_name: Mohammad
  full_name: Mahini, Mohammad
  last_name: Mahini
- first_name: Hamid
  full_name: Beigy, Hamid
  last_name: Beigy
- first_name: Salman
  full_name: Qadami, Salman
  last_name: Qadami
- first_name: Morteza
  full_name: Saghafian, Morteza
  id: f86f7148-b140-11ec-9577-95435b8df824
  last_name: Saghafian
citation:
  ama: 'Mahini M, Beigy H, Qadami S, Saghafian M. Simplet-based signatures and approximation
    in simplicial complexes: Frequency, degree, and centrality. <i>Information Sciences</i>.
    2025;719(11). doi:<a href="https://doi.org/10.1016/j.ins.2025.122425">10.1016/j.ins.2025.122425</a>'
  apa: 'Mahini, M., Beigy, H., Qadami, S., &#38; Saghafian, M. (2025). Simplet-based
    signatures and approximation in simplicial complexes: Frequency, degree, and centrality.
    <i>Information Sciences</i>. Elsevier. <a href="https://doi.org/10.1016/j.ins.2025.122425">https://doi.org/10.1016/j.ins.2025.122425</a>'
  chicago: 'Mahini, Mohammad, Hamid Beigy, Salman Qadami, and Morteza Saghafian. “Simplet-Based
    Signatures and Approximation in Simplicial Complexes: Frequency, Degree, and Centrality.”
    <i>Information Sciences</i>. Elsevier, 2025. <a href="https://doi.org/10.1016/j.ins.2025.122425">https://doi.org/10.1016/j.ins.2025.122425</a>.'
  ieee: 'M. Mahini, H. Beigy, S. Qadami, and M. Saghafian, “Simplet-based signatures
    and approximation in simplicial complexes: Frequency, degree, and centrality,”
    <i>Information Sciences</i>, vol. 719, no. 11. Elsevier, 2025.'
  ista: 'Mahini M, Beigy H, Qadami S, Saghafian M. 2025. Simplet-based signatures
    and approximation in simplicial complexes: Frequency, degree, and centrality.
    Information Sciences. 719(11), 122425.'
  mla: 'Mahini, Mohammad, et al. “Simplet-Based Signatures and Approximation in Simplicial
    Complexes: Frequency, Degree, and Centrality.” <i>Information Sciences</i>, vol.
    719, no. 11, 122425, Elsevier, 2025, doi:<a href="https://doi.org/10.1016/j.ins.2025.122425">10.1016/j.ins.2025.122425</a>.'
  short: M. Mahini, H. Beigy, S. Qadami, M. Saghafian, Information Sciences 719 (2025).
corr_author: '1'
date_created: 2025-06-30T08:48:48Z
date_published: 2025-11-01T00:00:00Z
date_updated: 2025-12-30T09:05:32Z
day: '01'
department:
- _id: HeEd
doi: 10.1016/j.ins.2025.122425
ec_funded: 1
external_id:
  isi:
  - '001516170500002'
intvolume: '       719'
isi: 1
issue: '11'
language:
- iso: eng
month: '11'
oa_version: None
project:
- _id: 266A2E9E-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '788183'
  name: Alpha Shape Theory Extended
- _id: 268116B8-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: Z00342
  name: Mathematics, Computer Science
- _id: 2561EBF4-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: I02979-N35
  name: Persistence and stability of geometric complexes
publication: Information Sciences
publication_identifier:
  issn:
  - 0020-0255
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Simplet-based signatures and approximation in simplicial complexes: Frequency,
  degree, and centrality'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 719
year: '2025'
...
---
_id: '19956'
abstract:
- lang: eng
  text: The specific introduction of 1H-13C or 1H-15N moieties into otherwise deuterated
    proteins holds great potential for high-resolution solution and magic-angle spinning
    (MAS) NMR studies of protein structure and dynamics. Arginine residues play key
    roles for example at active sites of enzymes. Taking advantage of a chemically
    synthesized Arg with a 13C-1H2 group in an otherwise deuterated backbone, we demonstrate
    here the usefulness of proton-detected arginine MAS NMR approaches to probe arginine
    dynamics. In experiments on crystalline ubiquitin and the 134 kDa tetrameric enzyme
    malate dehydrogenase we detected a wide range of motions, from sites that are
    rigid on time scales of at least tens of milliseconds to residues undergoing predominantly
    nanosecond motions. Spin-relaxation and dipolar-coupling measurements enabled
    quantitative determination of these dynamics. We observed microsecond dynamics
    of residue Arg54 in crystalline ubiquitin, whose backbone is known to sample different
    β-turn conformations on this time scale. The labeling scheme and experiments presented
    here expand the toolkit for high-resolution proton-detected MAS NMR
acknowledged_ssus:
- _id: NMR
- _id: LifeSc
article_processing_charge: No
author:
- first_name: Paul
  full_name: Schanda, Paul
  id: 7B541462-FAF6-11E9-A490-E8DFE5697425
  last_name: Schanda
  orcid: 0000-0002-9350-7606
citation:
  ama: Schanda P. Arginine Dynamics Probed by Magic-Angle Spinning NMR with a Specific
    Isotope-Labeling Scheme. 2025. doi:<a href="https://doi.org/10.15479/AT-ISTA-19956">10.15479/AT-ISTA-19956</a>
  apa: Schanda, P. (2025). Arginine Dynamics Probed by Magic-Angle Spinning NMR with
    a Specific Isotope-Labeling Scheme. Institute of Science and Technology Austria.
    <a href="https://doi.org/10.15479/AT-ISTA-19956">https://doi.org/10.15479/AT-ISTA-19956</a>
  chicago: Schanda, Paul. “Arginine Dynamics Probed by Magic-Angle Spinning NMR with
    a Specific Isotope-Labeling Scheme.” Institute of Science and Technology Austria,
    2025. <a href="https://doi.org/10.15479/AT-ISTA-19956">https://doi.org/10.15479/AT-ISTA-19956</a>.
  ieee: P. Schanda, “Arginine Dynamics Probed by Magic-Angle Spinning NMR with a Specific
    Isotope-Labeling Scheme.” Institute of Science and Technology Austria, 2025.
  ista: Schanda P. 2025. Arginine Dynamics Probed by Magic-Angle Spinning NMR with
    a Specific Isotope-Labeling Scheme, Institute of Science and Technology Austria,
    <a href="https://doi.org/10.15479/AT-ISTA-19956">10.15479/AT-ISTA-19956</a>.
  mla: Schanda, Paul. <i>Arginine Dynamics Probed by Magic-Angle Spinning NMR with
    a Specific Isotope-Labeling Scheme</i>. Institute of Science and Technology Austria,
    2025, doi:<a href="https://doi.org/10.15479/AT-ISTA-19956">10.15479/AT-ISTA-19956</a>.
  short: P. Schanda, (2025).
contributor:
- contributor_type: researcher
  first_name: Darja
  last_name: Rohden
- contributor_type: researcher
  first_name: Federico
  last_name: Napoli
- contributor_type: researcher
  first_name: Ben
  last_name: Tatman
- contributor_type: researcher
  first_name: Paul
  last_name: Schanda
corr_author: '1'
date_created: 2025-07-03T04:21:37Z
date_published: 2025-07-03T00:00:00Z
date_updated: 2025-12-29T14:52:16Z
day: '03'
ddc:
- '572'
department:
- _id: PaSc
doi: 10.15479/AT-ISTA-19956
file:
- access_level: open_access
  checksum: a2ef61aa9fb5313c7d426913eb0482c0
  content_type: application/octet-stream
  creator: pschanda
  date_created: 2025-07-03T10:30:14Z
  date_updated: 2025-07-03T10:30:14Z
  file_id: '19960'
  file_name: README
  file_size: 1160
  relation: main_file
  success: 1
- access_level: open_access
  checksum: 8fb77b96d0fcc95c9903005652207a8c
  content_type: application/zip
  creator: pschanda
  date_created: 2025-07-03T10:30:55Z
  date_updated: 2025-07-03T10:30:55Z
  file_id: '19961'
  file_name: data_Arg_MASNMR_Rohden.zip
  file_size: 128597184
  relation: main_file
  success: 1
- access_level: open_access
  checksum: a60cc16d20b089c4bef94040a99cfba5
  content_type: application/x-xz
  creator: pschanda
  date_created: 2025-08-14T07:06:58Z
  date_updated: 2025-08-14T07:06:58Z
  file_id: '20172'
  file_name: 20240903_ubi_DN_Argd1C13_2D_spectra.tar.xz
  file_size: 4766564
  relation: main_file
  success: 1
file_date_updated: 2025-08-14T07:06:58Z
has_accepted_license: '1'
month: '07'
oa: 1
oa_version: None
project:
- _id: eb9c82eb-77a9-11ec-83b8-aadd536561cf
  grant_number: I05812
  name: AlloSpace. The emergence and mechanisms of allostery
publisher: Institute of Science and Technology Austria
related_material:
  record:
  - id: '20258'
    relation: used_in_publication
    status: public
status: public
title: Arginine Dynamics Probed by Magic-Angle Spinning NMR with a Specific Isotope-Labeling
  Scheme
tmp:
  image: /images/cc_by_nc.png
  legal_code_url: https://creativecommons.org/licenses/by-nc/4.0/legalcode
  name: Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)
  short: CC BY-NC (4.0)
type: research_data
user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '19963'
abstract:
- lang: eng
  text: The acquisition of cellular identity requires large-scale alterations in cellular
    state. The noncanonical proteasome activator PSME3 is known to regulate diverse
    cellular processes, but its importance for differentiation remains unclear. Here,
    we demonstrate that PSME3 binds dynamically to highly active promoters over the
    course of differentiation. However, loss of PSME3 does not globally affect mRNA
    transcription. We find instead that PSME3 influences the levels of several adhesion-related
    proteins and acts upstream of the HSP90 co-chaperone NUDC to regulate cell motility
    and myoblast differentiation in a proteasome-independent manner. Our findings
    reveal several new facets of PSME3 functionality and highlight its importance
    for the differentiation of myogenic cells.
acknowledged_ssus:
- _id: LifeSc
- _id: Bio
acknowledgement: 'All proteomics analysis was done by the ISTA LSF Mass Spectrometry
  Service: Ewelina Dutkiewicz-Kopczynska processed the samples (digest and cleanup);
  Bella Bruszel optimized the acquisition methods, acquired the data, and performed
  all searches; and Armel Nicolas provided pre- and post-project consulting and post-processed
  the search results using a development version of their data analysis package, proteoCraft
  (publication pending). The authors would like to thank Saki for their clarity of
  thought and insight, as well as Dr. Lorenzo Puri and the members of his laboratory
  for invaluable discussions relating to the project. This research was further supported
  by the Lab Support Facility and the Imaging and Optics Facility of ISTA.'
article_number: e202503208
article_processing_charge: Yes
article_type: original
author:
- first_name: Kenneth D
  full_name: Kuhn, Kenneth D
  id: 7deed7e0-0133-11f0-8590-c4600b08d0f4
  last_name: Kuhn
- first_name: Ukrae H.
  full_name: Cho, Ukrae H.
  last_name: Cho
- first_name: Martin W
  full_name: Hetzer, Martin W
  id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
  last_name: Hetzer
  orcid: 0000-0002-2111-992X
citation:
  ama: Kuhn KD, Cho UH, Hetzer M. PSME3 regulates migration and differentiation of
    myoblasts. <i>Life Science Alliance</i>. 2025;8(9). doi:<a href="https://doi.org/10.26508/lsa.202503208">10.26508/lsa.202503208</a>
  apa: Kuhn, K. D., Cho, U. H., &#38; Hetzer, M. (2025). PSME3 regulates migration
    and differentiation of myoblasts. <i>Life Science Alliance</i>. Embo Press. <a
    href="https://doi.org/10.26508/lsa.202503208">https://doi.org/10.26508/lsa.202503208</a>
  chicago: Kuhn, Kenneth D, Ukrae H. Cho, and Martin Hetzer. “PSME3 Regulates Migration
    and Differentiation of Myoblasts.” <i>Life Science Alliance</i>. Embo Press, 2025.
    <a href="https://doi.org/10.26508/lsa.202503208">https://doi.org/10.26508/lsa.202503208</a>.
  ieee: K. D. Kuhn, U. H. Cho, and M. Hetzer, “PSME3 regulates migration and differentiation
    of myoblasts,” <i>Life Science Alliance</i>, vol. 8, no. 9. Embo Press, 2025.
  ista: Kuhn KD, Cho UH, Hetzer M. 2025. PSME3 regulates migration and differentiation
    of myoblasts. Life Science Alliance. 8(9), e202503208.
  mla: Kuhn, Kenneth D., et al. “PSME3 Regulates Migration and Differentiation of
    Myoblasts.” <i>Life Science Alliance</i>, vol. 8, no. 9, e202503208, Embo Press,
    2025, doi:<a href="https://doi.org/10.26508/lsa.202503208">10.26508/lsa.202503208</a>.
  short: K.D. Kuhn, U.H. Cho, M. Hetzer, Life Science Alliance 8 (2025).
corr_author: '1'
date_created: 2025-07-06T22:01:22Z
date_published: 2025-09-01T00:00:00Z
date_updated: 2025-12-30T09:17:55Z
day: '01'
ddc:
- '570'
department:
- _id: MaHe
doi: 10.26508/lsa.202503208
external_id:
  isi:
  - '001511452100001'
  pmid:
  - '40537284'
file:
- access_level: open_access
  checksum: 591d47aa39fc969986c7d3b966890f5f
  content_type: application/pdf
  creator: dernst
  date_created: 2025-12-30T09:17:09Z
  date_updated: 2025-12-30T09:17:09Z
  file_id: '20904'
  file_name: 2025_LifeScienceAlliance_Kuhn.pdf
  file_size: 5471288
  relation: main_file
  success: 1
file_date_updated: 2025-12-30T09:17:09Z
has_accepted_license: '1'
intvolume: '         8'
isi: 1
issue: '9'
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
pmid: 1
publication: Life Science Alliance
publication_identifier:
  eissn:
  - 2575-1077
publication_status: published
publisher: Embo Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: PSME3 regulates migration and differentiation of myoblasts
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: 8
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19964'
abstract:
- lang: eng
  text: It has been suggested that giant planet occurrence peaks for stars with M*
    ≈ 3 M⊙ at a value a factor of 4 higher than observed for solar-mass stars. This
    population of giant planets predicted to frequently orbit main-sequence B stars
    at a ≈ 10 au is difficult to characterize during the few hundred million years
    while fusion persists in their host stars. By the time those stars become massive,
    young white dwarfs, any giant planets present would still be luminous as a consequence
    of their recent formation. From an initial sample of 2195 Gaia-identified massive,
    young white dwarfs, we use homogeneous Spitzer Infrared Array Camera (IRAC) photometry
    to search for evidence of unresolved giant planets. For 30 systems, these IRAC
    data provide sensitivity to objects with M ≲ 10 MJup, and we identify one candidate
    with M ≈ 4 MJup orbiting the white dwarf GALEX J071816.4+373139. Correcting for
    the possibility that some of the white dwarfs in our sample result from mergers,
    we find a giant planet occurrence  n GP = 0.11+0.13-0.07 for stars with initial
    masses M* ≳ 3 M⊙. Our occurrence inference is consistent with both the Doppler-inferred
    occurrence of giant planets orbiting M* ≈ 2 M⊙ giant stars and the theoretically
    predicted factor of 4 enhancement in the occurrence of giant planets orbiting
    M* ≈ 3 M⊙ stars relative to solar-mass stars. Future James Webb Space Telescope
    NIRCam observations of our sample would provide sensitivity to Saturn-mass planets
    and thereby a definitive estimate of the occurrence of giant planets orbiting
    stars with M* ≳ 3 M⊙.
acknowledgement: "We thank Jay Farihi, Guangwei Fu, J. J. Hermes, Mary Anne Limbach,
  and Daniel Thorngren for useful discussions. S.C. thanks Siyu Yao for her constant
  inspiration and encouragement. S.C. acknowledges the support of the Martin A. and
  Helen Chooljian Member Fund, funding from the Zurich Insurance Company, and the
  Fund for Natural Sciences at the Institute for Advanced Study. This work has made
  use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia),
  processed by the Gaia Data Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/consortium).
  Funding for the DPAC has been provided by national institutions, in particular the
  institutions participating in the Gaia Multilateral Agreement. This work is based
  in part on observations made with the Spitzer Space Telescope, which is operated
  by the Jet Propulsion Laboratory, California Institute of Technology under a contract
  with NASA. This publication makes use of data products from the Wide-field Infrared
  Survey Explorer, which is a joint project of the University of California, Los Angeles,
  and the Jet Propulsion Laboratory/California Institute of Technology, funded by
  the National Aeronautics and Space Administration. This research has made use of
  the NASA Exoplanet Archive, which is operated by the California Institute of Technology,
  under contract with the National Aeronautics and Space Administration under the
  Exoplanet Exploration Program. This research has made use of NASA’s Astrophysics
  Data System.\r\nFacilities: ADS - , ESO:VISTA - European Southern Observatory's
  4.1 meter Visible and Infrared Survey Telescope for Astronomy, Exoplanet Archive
  - , Gaia - , IRSA - , NEOWISE - , Spitzer - Spitzer Space Telescope satellite, UKIRT
  - United Kingdom Infrared Telescope, WISE - Wide-field Infrared Survey Explorer.\r\nSoftware:
  astropy (Astropy Collaboration et al. 2013, 2018, 2022), numpy (C. R. Harris et
  al. 2020), matplotlib (J. D. Hunter 2007), R (R Core Team 2024), SciPy (P. Virtanen
  et al. 2020)."
article_number: '47'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Sihao
  full_name: Cheng, Sihao
  last_name: Cheng
- first_name: Kevin C.
  full_name: Schlaufman, Kevin C.
  last_name: Schlaufman
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
citation:
  ama: Cheng S, Schlaufman KC, Caiazzo I. A candidate giant planet companion to the
    massive, young White Dwarf GALEX J071816.4+373139 informs the occurrence of giant
    planets orbiting B stars. <i>The Astronomical Journal</i>. 2025;170(1). doi:<a
    href="https://doi.org/10.3847/1538-3881/addd21">10.3847/1538-3881/addd21</a>
  apa: Cheng, S., Schlaufman, K. C., &#38; Caiazzo, I. (2025). A candidate giant planet
    companion to the massive, young White Dwarf GALEX J071816.4+373139 informs the
    occurrence of giant planets orbiting B stars. <i>The Astronomical Journal</i>.
    IOP Publishing. <a href="https://doi.org/10.3847/1538-3881/addd21">https://doi.org/10.3847/1538-3881/addd21</a>
  chicago: Cheng, Sihao, Kevin C. Schlaufman, and Ilaria Caiazzo. “A Candidate Giant
    Planet Companion to the Massive, Young White Dwarf GALEX J071816.4+373139 Informs
    the Occurrence of Giant Planets Orbiting B Stars.” <i>The Astronomical Journal</i>.
    IOP Publishing, 2025. <a href="https://doi.org/10.3847/1538-3881/addd21">https://doi.org/10.3847/1538-3881/addd21</a>.
  ieee: S. Cheng, K. C. Schlaufman, and I. Caiazzo, “A candidate giant planet companion
    to the massive, young White Dwarf GALEX J071816.4+373139 informs the occurrence
    of giant planets orbiting B stars,” <i>The Astronomical Journal</i>, vol. 170,
    no. 1. IOP Publishing, 2025.
  ista: Cheng S, Schlaufman KC, Caiazzo I. 2025. A candidate giant planet companion
    to the massive, young White Dwarf GALEX J071816.4+373139 informs the occurrence
    of giant planets orbiting B stars. The Astronomical Journal. 170(1), 47.
  mla: Cheng, Sihao, et al. “A Candidate Giant Planet Companion to the Massive, Young
    White Dwarf GALEX J071816.4+373139 Informs the Occurrence of Giant Planets Orbiting
    B Stars.” <i>The Astronomical Journal</i>, vol. 170, no. 1, 47, IOP Publishing,
    2025, doi:<a href="https://doi.org/10.3847/1538-3881/addd21">10.3847/1538-3881/addd21</a>.
  short: S. Cheng, K.C. Schlaufman, I. Caiazzo, The Astronomical Journal 170 (2025).
date_created: 2025-07-06T22:01:22Z
date_published: 2025-07-01T00:00:00Z
date_updated: 2026-02-19T09:31:41Z
day: '01'
ddc:
- '520'
department:
- _id: IlCa
doi: 10.3847/1538-3881/addd21
external_id:
  arxiv:
  - '2408.03985'
  isi:
  - '001514518100001'
file:
- access_level: open_access
  checksum: 144b0e46aa3dff0cdf8c6ee7d4fe2fe4
  content_type: application/pdf
  creator: dernst
  date_created: 2025-07-08T06:40:54Z
  date_updated: 2025-07-08T06:40:54Z
  file_id: '19975'
  file_name: 2025_AstronomicalJour_Cheng.pdf
  file_size: 931173
  relation: main_file
  success: 1
file_date_updated: 2025-07-08T06:40:54Z
has_accepted_license: '1'
intvolume: '       170'
isi: 1
issue: '1'
language:
- iso: eng
month: '07'
oa: 1
oa_version: Published Version
publication: The Astronomical Journal
publication_identifier:
  eissn:
  - 1538-3881
  issn:
  - 0004-6256
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: A candidate giant planet companion to the massive, young White Dwarf GALEX
  J071816.4+373139 informs the occurrence of giant planets orbiting B stars
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: 170
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19965'
abstract:
- lang: eng
  text: Multiagent learning is challenging when agents face mixed-motivation interactions,
    where conflicts of interest arise as agents independently try to optimize their
    respective outcomes. Recent advancements in evolutionary game theory have identified
    a class of “zero-determinant” strategies, which confer an agent with significant
    unilateral control over outcomes in repeated games. Building on these insights,
    we present a comprehensive generalization of zero-determinant strategies to stochastic
    games, encompassing dynamic environments. We propose an algorithm that allows
    an agent to discover strategies enforcing predetermined linear (or approximately
    linear) payoff relationships. Of particular interest is the relationship in which
    both payoffs are equal, which serves as a proxy for fairness in symmetric games.
    We demonstrate that an agent can discover strategies enforcing such relationships
    through experience alone, without coordinating with an opponent. In finding and
    using such a strategy, an agent (“enforcer”) can incentivize optimal and equitable
    outcomes, circumventing potential exploitation. In particular, from the opponent’s
    viewpoint, the enforcer transforms a mixed-motivation problem into a cooperative
    problem, paving the way for more collaboration and fairness in multiagent systems.
acknowledgement: 'We gratefully acknowledge the support from the European Research
  Council (Starting Grant 850529: E-DIRECT) and the Max Planck Society (C.H.), the
  European Research Council (Consolidator Grant 863818: ForM-SMArt) (K.C.), the Shanghai
  Pujiang Program (No. 23PJ1405500) (Q.S.), the Army Research Office (Grant No. W911NF-18-1-0325)
  (N.E.L.), and the John Templeton Foundation (Grant No. 62281) (J.B.P.).'
article_number: e2319927121
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Alex
  full_name: Mcavoy, Alex
  last_name: Mcavoy
- first_name: Udari Madhushani
  full_name: Sehwag, Udari Madhushani
  last_name: Sehwag
- first_name: Christian
  full_name: Hilbe, Christian
  id: 2FDF8F3C-F248-11E8-B48F-1D18A9856A87
  last_name: Hilbe
  orcid: 0000-0001-5116-955X
- first_name: Krishnendu
  full_name: Chatterjee, Krishnendu
  id: 2E5DCA20-F248-11E8-B48F-1D18A9856A87
  last_name: Chatterjee
  orcid: 0000-0002-4561-241X
- first_name: Wolfram
  full_name: Barfuss, Wolfram
  last_name: Barfuss
- first_name: Qi
  full_name: Su, Qi
  last_name: Su
- first_name: Naomi Ehrich
  full_name: Leonard, Naomi Ehrich
  last_name: Leonard
- first_name: Joshua B.
  full_name: Plotkin, Joshua B.
  last_name: Plotkin
citation:
  ama: Mcavoy A, Sehwag UM, Hilbe C, et al. Unilateral incentive alignment in two-agent
    stochastic games. <i>Proceedings of the National Academy of Sciences</i>. 2025;122(25).
    doi:<a href="https://doi.org/10.1073/pnas.2319927121">10.1073/pnas.2319927121</a>
  apa: Mcavoy, A., Sehwag, U. M., Hilbe, C., Chatterjee, K., Barfuss, W., Su, Q.,
    … Plotkin, J. B. (2025). Unilateral incentive alignment in two-agent stochastic
    games. <i>Proceedings of the National Academy of Sciences</i>. National Academy
    of Sciences. <a href="https://doi.org/10.1073/pnas.2319927121">https://doi.org/10.1073/pnas.2319927121</a>
  chicago: Mcavoy, Alex, Udari Madhushani Sehwag, Christian Hilbe, Krishnendu Chatterjee,
    Wolfram Barfuss, Qi Su, Naomi Ehrich Leonard, and Joshua B. Plotkin. “Unilateral
    Incentive Alignment in Two-Agent Stochastic Games.” <i>Proceedings of the National
    Academy of Sciences</i>. National Academy of Sciences, 2025. <a href="https://doi.org/10.1073/pnas.2319927121">https://doi.org/10.1073/pnas.2319927121</a>.
  ieee: A. Mcavoy <i>et al.</i>, “Unilateral incentive alignment in two-agent stochastic
    games,” <i>Proceedings of the National Academy of Sciences</i>, vol. 122, no.
    25. National Academy of Sciences, 2025.
  ista: Mcavoy A, Sehwag UM, Hilbe C, Chatterjee K, Barfuss W, Su Q, Leonard NE, Plotkin
    JB. 2025. Unilateral incentive alignment in two-agent stochastic games. Proceedings
    of the National Academy of Sciences. 122(25), e2319927121.
  mla: Mcavoy, Alex, et al. “Unilateral Incentive Alignment in Two-Agent Stochastic
    Games.” <i>Proceedings of the National Academy of Sciences</i>, vol. 122, no.
    25, e2319927121, National Academy of Sciences, 2025, doi:<a href="https://doi.org/10.1073/pnas.2319927121">10.1073/pnas.2319927121</a>.
  short: A. Mcavoy, U.M. Sehwag, C. Hilbe, K. Chatterjee, W. Barfuss, Q. Su, N.E.
    Leonard, J.B. Plotkin, Proceedings of the National Academy of Sciences 122 (2025).
date_created: 2025-07-06T22:01:23Z
date_published: 2025-06-24T00:00:00Z
date_updated: 2025-09-30T13:47:14Z
day: '24'
ddc:
- '000'
department:
- _id: KrCh
doi: 10.1073/pnas.2319927121
ec_funded: 1
external_id:
  isi:
  - '001522351900001'
  pmid:
  - '40523172'
file:
- access_level: open_access
  checksum: 3b35befd959a3e37aa9080a64a6afaf3
  content_type: application/pdf
  creator: dernst
  date_created: 2025-07-08T05:52:26Z
  date_updated: 2025-07-08T05:52:26Z
  file_id: '19972'
  file_name: 2025_PNAS_McAvoy.pdf
  file_size: 29525932
  relation: main_file
  success: 1
file_date_updated: 2025-07-08T05:52:26Z
has_accepted_license: '1'
intvolume: '       122'
isi: 1
issue: '25'
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 0599E47C-7A3F-11EA-A408-12923DDC885E
  call_identifier: H2020
  grant_number: '863818'
  name: 'Formal Methods for Stochastic Models: Algorithms and Applications'
publication: Proceedings of the National Academy of Sciences
publication_identifier:
  eissn:
  - 1091-6490
  issn:
  - 0027-8424
publication_status: published
publisher: National Academy of Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: Unilateral incentive alignment in two-agent stochastic games
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: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 122
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19966'
abstract:
- lang: eng
  text: Recently discovered nanofluidic memristors, have raised promises for the development
    of iontronics and neuromorphic computing with ions. Ionic memory effects are related
    to ion dynamics inside nanochannels, with timescales associated with the manifold
    physicochemical phenomena occurring at confined interfaces. Here, we explore experimentally
    the frequency-dependent current–voltage response of model nanochannels—namely
    glass nanopipettes—to investigate memory effects in ion transport. This characterisation,
    which we refer to as mem-spectrometry, highlights two characteristic frequencies,
    associated with short and long timescales of the order of 50 ms and 50 s in the
    present system. Whereas the former can be associated with ionic diffusion, very
    long timescales are difficult to explain with conventional transport phenomena.
    We develop a minimal model accounting for these mem-spectrometry results, pointing
    to surface charge regulation and ionic adsorption-desorption as possible origins
    for the long-term memory. Our work demonstrates the relevance of mem-spectrometry
    to highlight subtle ion transport properties in nanochannels, giving hereby new
    insights on the mechanisms governing ion transport and current rectification in
    charged conical nanopores.
acknowledgement: The authors acknowledge ERC n-AQUA for funding. S J acknowledges
  CNRS for funding. The authors thank Hummink for pipette supply and characterization.
  P R acknowledges funding from the European Union Horizon 2020 research and innovation
  program under the Marie Skodowska-Curie Grant Agreement No. 101034413.
article_number: '065001'
article_processing_charge: Yes
article_type: original
author:
- first_name: Simon
  full_name: Jouveshomme, Simon
  last_name: Jouveshomme
- first_name: Mathieu
  full_name: Lizée, Mathieu
  last_name: Lizée
- first_name: Paul
  full_name: Robin, Paul
  id: 48c58128-57b0-11ee-9095-dc28fd97fc1d
  last_name: Robin
  orcid: 0000-0002-5728-9189
- first_name: Lydéric
  full_name: Bocquet, Lydéric
  last_name: Bocquet
citation:
  ama: Jouveshomme S, Lizée M, Robin P, Bocquet L. Multiple ionic memories in asymmetric
    nanochannels revealed by mem-spectrometry. <i>New Journal of Physics</i>. 2025;27(6).
    doi:<a href="https://doi.org/10.1088/1367-2630/ade61b">10.1088/1367-2630/ade61b</a>
  apa: Jouveshomme, S., Lizée, M., Robin, P., &#38; Bocquet, L. (2025). Multiple ionic
    memories in asymmetric nanochannels revealed by mem-spectrometry. <i>New Journal
    of Physics</i>. IOP Publishing. <a href="https://doi.org/10.1088/1367-2630/ade61b">https://doi.org/10.1088/1367-2630/ade61b</a>
  chicago: Jouveshomme, Simon, Mathieu Lizée, Paul Robin, and Lydéric Bocquet. “Multiple
    Ionic Memories in Asymmetric Nanochannels Revealed by Mem-Spectrometry.” <i>New
    Journal of Physics</i>. IOP Publishing, 2025. <a href="https://doi.org/10.1088/1367-2630/ade61b">https://doi.org/10.1088/1367-2630/ade61b</a>.
  ieee: S. Jouveshomme, M. Lizée, P. Robin, and L. Bocquet, “Multiple ionic memories
    in asymmetric nanochannels revealed by mem-spectrometry,” <i>New Journal of Physics</i>,
    vol. 27, no. 6. IOP Publishing, 2025.
  ista: Jouveshomme S, Lizée M, Robin P, Bocquet L. 2025. Multiple ionic memories
    in asymmetric nanochannels revealed by mem-spectrometry. New Journal of Physics.
    27(6), 065001.
  mla: Jouveshomme, Simon, et al. “Multiple Ionic Memories in Asymmetric Nanochannels
    Revealed by Mem-Spectrometry.” <i>New Journal of Physics</i>, vol. 27, no. 6,
    065001, IOP Publishing, 2025, doi:<a href="https://doi.org/10.1088/1367-2630/ade61b">10.1088/1367-2630/ade61b</a>.
  short: S. Jouveshomme, M. Lizée, P. Robin, L. Bocquet, New Journal of Physics 27
    (2025).
date_created: 2025-07-06T22:01:23Z
date_published: 2025-06-01T00:00:00Z
date_updated: 2025-09-30T13:47:45Z
day: '01'
ddc:
- '530'
department:
- _id: EdHa
doi: 10.1088/1367-2630/ade61b
ec_funded: 1
external_id:
  isi:
  - '001517731700001'
file:
- access_level: open_access
  checksum: e0e11aa01c54b20ee6cdd1f6b999571f
  content_type: application/pdf
  creator: dernst
  date_created: 2025-07-08T06:11:59Z
  date_updated: 2025-07-08T06:11:59Z
  file_id: '19973'
  file_name: 2025_NewJourPhysics_Jouveshomme.pdf
  file_size: 1296141
  relation: main_file
  success: 1
file_date_updated: 2025-07-08T06:11:59Z
has_accepted_license: '1'
intvolume: '        27'
isi: 1
issue: '6'
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
  call_identifier: H2020
  grant_number: '101034413'
  name: 'IST-BRIDGE: International postdoctoral program'
publication: New Journal of Physics
publication_identifier:
  eissn:
  - 1367-2630
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Multiple ionic memories in asymmetric nanochannels revealed by mem-spectrometry
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: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 27
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '19967'
abstract:
- lang: eng
  text: "Context. Investigating the ionizing emission of star-forming galaxies and
    the escape fraction of ionizing photons is critical to understanding their contribution
    to reionization and their impact on the surrounding environment. The number of
    ionizing photons available to reionize the intergalactic medium (IGM) depends
    on not only the abundance of galaxies but also their efficiency in producing ionizing
    photons (ξion). This quantity is thus fundamental to quantify the role of faint
    versus bright sources in driving this process, as we must assess their relative
    contribution to the total ionizing emissivity.\r\n\r\nAims. Our goal is to estimate
    the ξion using Balmer lines (Hα or Hβ) in a sample of 761 galaxies at 4 ≤ z ≤ 10
    selected from different JWST spectroscopic surveys. We aim to determine the redshift
    evolution of ξion and the relation of ξion with the physical properties of the
    galaxies.\r\n\r\nMethods. We used the available HST and JWST photometry to perform
    a spectral energy distribution (SED) fitting in the sample to determine their
    physical properties and relate them with ξion. We used the BAGPIPES code for the
    SED fitting and assumed a delayed exponential model for the star formation history.
    We used the NIRSpec spectra from prism or grating configurations to estimate Balmer
    luminosities, and then constrained ξion values after dust correction.\r\n\r\nResults.
    We find a mean value of 1025.22 Hz erg−1 for ξion in the sample with an observed
    scatter of 0.42 dex. We find an increase in the median values of ξion with redshift
    from 1025.09 Hz erg−1 at z ∼ 4.18 to 1025.28 Hz erg−1 at z ∼ 7.14, confirming
    the redshift evolution of ξion found in other studies. Regarding the relation
    between ξion and physical properties, we find a decrease in ξion with increasing
    stellar mass, indicating that low-mass galaxies are efficient producers of ionizing
    photons. We also find an increase in ξion with increasing specific star formation
    rate (sSFR) and increasing UV absolute magnitude. This indicates that faint galaxies
    and galaxies with high sSFR are also efficient producers. We also investigated
    the relation of ξion with the rest-frame equivalent width (EW) of [OIII]λ5007
    and find that galaxies with the higher EW([OIII]λ5007) are more efficient producers
    of ionizing photons, with the best fit leading to the relation log(ξion)  =  0.43 × log(EW[OIII])+23.99.
    Similarly, we find that galaxies with higher O32 = [OIII]λ5007/[OII]λλ3727,3729
    and lower gas-phase metallicities (based on the R23 = ([OIII]λλ4959,5007+[OII]λλ3727,3729)/Hβ
    calibration) show higher ξion values."
acknowledgement: We thank the anonymous referee for the detailed review and useful
  suggestions that helped to improve this paper. We wish to thank all our colleagues
  in the CEERS collaboration for their hard work and valuable contributions to this
  project. We thank Pietro Bergamini for providing us with the magnification factors
  for the lensed sources. MLl acknowledges support from the INAF Large Grant 2022
  “Extragalactic Surveys with JWST” (PI L. Pentericci), the PRIN 2022 MUR project
  2022CB3PJ3 – First Light And Galaxy aSsembly (FLAGS) funded by the European Union
  – Next Generation EU, and INAF Mini-grant “Galaxies in the epoch of Reionization
  and their analogs at lower redshift” (PI M. Llerena). 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 This work is based on observations made
  with the NASA/ESA/CSA James Webb Space Telescope (JWST). The JWST data presented
  in this article were obtained from the Mikulski Archive for Space Telescopes (MAST)
  at the Space Telescope Science Institute. The specific observations analyzed are
  associated with program JWST-GO-3073 and can be accessed via DOI. We acknowledge
  support from INAF Mini-grant “Reionization and Fundamental Cosmology with High-Redshift
  Galaxies”. This work has made extensive use of Python packages astropy (Astropy
  Collaboration 2018), numpy (Harris et al. 2020), Matplotlib (Hunter 2007) and LiMe
  (Fernández et al. 2024).
article_number: A302
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: M.
  full_name: Llerena, M.
  last_name: Llerena
- first_name: L.
  full_name: Pentericci, L.
  last_name: Pentericci
- first_name: L.
  full_name: Napolitano, L.
  last_name: Napolitano
- first_name: Sara
  full_name: Mascia, Sara
  id: edaf889c-c7cd-11ef-ab1b-bb28c431bd29
  last_name: Mascia
- first_name: R.
  full_name: Amorín, R.
  last_name: Amorín
- first_name: A.
  full_name: Calabrò, A.
  last_name: Calabrò
- first_name: M.
  full_name: Castellano, M.
  last_name: Castellano
- first_name: N. J.
  full_name: Cleri, N. J.
  last_name: Cleri
- first_name: M.
  full_name: Giavalisco, M.
  last_name: Giavalisco
- first_name: N. A.
  full_name: Grogin, N. A.
  last_name: Grogin
- first_name: N. P.
  full_name: Hathi, N. P.
  last_name: Hathi
- first_name: M.
  full_name: Hirschmann, M.
  last_name: Hirschmann
- first_name: A. M.
  full_name: Koekemoer, A. M.
  last_name: Koekemoer
- first_name: T.
  full_name: Nanayakkara, T.
  last_name: Nanayakkara
- first_name: F.
  full_name: Pacucci, F.
  last_name: Pacucci
- first_name: L.
  full_name: Shen, L.
  last_name: Shen
- first_name: S. M.
  full_name: Wilkins, S. M.
  last_name: Wilkins
- first_name: I.
  full_name: Yoon, I.
  last_name: Yoon
- first_name: L. Y.A.
  full_name: Yung, L. Y.A.
  last_name: Yung
- first_name: R.
  full_name: Bhatawdekar, R.
  last_name: Bhatawdekar
- first_name: R. A.
  full_name: Lucas, R. A.
  last_name: Lucas
- first_name: X.
  full_name: Wang, X.
  last_name: Wang
- first_name: P.
  full_name: Arrabal Haro, P.
  last_name: Arrabal Haro
- first_name: M. B.
  full_name: Bagley, M. B.
  last_name: Bagley
- first_name: S. L.
  full_name: Finkelstein, S. L.
  last_name: Finkelstein
- first_name: J. S.
  full_name: Kartaltepe, J. S.
  last_name: Kartaltepe
- first_name: E.
  full_name: Merlin, E.
  last_name: Merlin
- first_name: C.
  full_name: Papovich, C.
  last_name: Papovich
- first_name: N.
  full_name: Pirzkal, N.
  last_name: Pirzkal
- first_name: P.
  full_name: Santini, P.
  last_name: Santini
citation:
  ama: Llerena M, Pentericci L, Napolitano L, et al. The ionizing photon production
    efficiency of star-forming galaxies at z ∼ 4–10. <i>Astronomy &#38; Astrophysics</i>.
    2025;698. doi:<a href="https://doi.org/10.1051/0004-6361/202453251">10.1051/0004-6361/202453251</a>
  apa: Llerena, M., Pentericci, L., Napolitano, L., Mascia, S., Amorín, R., Calabrò,
    A., … Santini, P. (2025). The ionizing photon production efficiency of star-forming
    galaxies at z ∼ 4–10. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/202453251">https://doi.org/10.1051/0004-6361/202453251</a>
  chicago: Llerena, M., L. Pentericci, L. Napolitano, Sara Mascia, R. Amorín, A. Calabrò,
    M. Castellano, et al. “The Ionizing Photon Production Efficiency of Star-Forming
    Galaxies at z ∼ 4–10.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2025.
    <a href="https://doi.org/10.1051/0004-6361/202453251">https://doi.org/10.1051/0004-6361/202453251</a>.
  ieee: M. Llerena <i>et al.</i>, “The ionizing photon production efficiency of star-forming
    galaxies at z ∼ 4–10,” <i>Astronomy &#38; Astrophysics</i>, vol. 698. EDP Sciences,
    2025.
  ista: Llerena M, Pentericci L, Napolitano L, Mascia S, Amorín R, Calabrò A, Castellano
    M, Cleri NJ, Giavalisco M, Grogin NA, Hathi NP, Hirschmann M, Koekemoer AM, Nanayakkara
    T, Pacucci F, Shen L, Wilkins SM, Yoon I, Yung LYA, Bhatawdekar R, Lucas RA, Wang
    X, Arrabal Haro P, Bagley MB, Finkelstein SL, Kartaltepe JS, Merlin E, Papovich
    C, Pirzkal N, Santini P. 2025. The ionizing photon production efficiency of star-forming
    galaxies at z ∼ 4–10. Astronomy &#38; Astrophysics. 698, A302.
  mla: Llerena, M., et al. “The Ionizing Photon Production Efficiency of Star-Forming
    Galaxies at z ∼ 4–10.” <i>Astronomy &#38; Astrophysics</i>, vol. 698, A302, EDP
    Sciences, 2025, doi:<a href="https://doi.org/10.1051/0004-6361/202453251">10.1051/0004-6361/202453251</a>.
  short: M. Llerena, L. Pentericci, L. Napolitano, S. Mascia, R. Amorín, A. Calabrò,
    M. Castellano, N.J. Cleri, M. Giavalisco, N.A. Grogin, N.P. Hathi, M. Hirschmann,
    A.M. Koekemoer, T. Nanayakkara, F. Pacucci, L. Shen, S.M. Wilkins, I. Yoon, L.Y.A.
    Yung, R. Bhatawdekar, R.A. Lucas, X. Wang, P. Arrabal Haro, M.B. Bagley, S.L.
    Finkelstein, J.S. Kartaltepe, E. Merlin, C. Papovich, N. Pirzkal, P. Santini,
    Astronomy &#38; Astrophysics 698 (2025).
date_created: 2025-07-06T22:01:23Z
date_published: 2025-06-20T00:00:00Z
date_updated: 2026-02-16T12:12:15Z
day: '20'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202453251
external_id:
  arxiv:
  - '2412.01358'
  isi:
  - '001512479700026'
file:
- access_level: open_access
  checksum: 92745034d9448d38b6b0394407ae39a0
  content_type: application/pdf
  creator: dernst
  date_created: 2025-07-08T06:17:02Z
  date_updated: 2025-07-08T06:17:02Z
  file_id: '19974'
  file_name: 2025_AstronomyAstrophysics_Llerena.pdf
  file_size: 7557993
  relation: main_file
  success: 1
file_date_updated: 2025-07-08T06:17:02Z
has_accepted_license: '1'
intvolume: '       698'
isi: 1
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
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: The ionizing photon production efficiency of star-forming galaxies at z ∼ 4–10
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: 698
year: '2025'
...
---
OA_type: closed access
_id: '19968'
abstract:
- lang: eng
  text: In the dynamic arena of innovation, the relations between academia and industry
    are a keystone for breakthroughs and practical applications. Yet, the groundwork
    of these pivotal University-Industry (U-I) partnerships remains covered in complexity.
    This paper delves into these intricate relations, unraveling the factors that
    help successful collaborations. Grounded in the Resource-Based Theory, our study
    transcends traditional analytical boundaries, leveraging a neural network model
    to understand a comprehensive dataset from the UK’s Higher Education Statistics
    Agency, SCIMAGO Rankings, and Clarivate Publications. This novel approach helps
    to make clear the interplay of academic load, administrative support, scientific
    output, and university rank in sculpting U-I collaboration dynamics. Our findings
    suggest that reduced academic load and robust administrative support significantly
    bolster U-I collaborations. However, the influence of scientific output and university
    ranking is more nuanced, challenging the common belief. High scientific output,
    while indicative of expertise, doesn't always align with industry goals. Similarly,
    while higher-ranked universities could attract more collaborations, the benefits
    are not universal. This paper not only contributes to a deeper understanding of
    U-I collaborations, but also provides actionable insights for university administrators,
    policymakers, and industry leaders. In a world where innovation is key, understanding
    these collaborative dynamics is crucial for fostering partnerships that push the
    boundaries of research and practical application.
article_processing_charge: No
author:
- first_name: Carlos
  full_name: Plata, Carlos
  last_name: Plata
- first_name: Alejandro
  full_name: Casallas Garcia, Alejandro
  id: 92081129-2d75-11ef-a48d-b04dd7a2385a
  last_name: Casallas Garcia
  orcid: 0000-0002-1988-5035
citation:
  ama: 'Plata C, Casallas Garcia A. Machine learning analysis of the factors influencing
    university-industry collaborations. In: <i>85th Annual Meeting of the Academy
    of Management</i>. Vol 2025. Academy of Management; 2025. doi:<a href="https://doi.org/10.5465/AMPROC.2025.54bp">10.5465/AMPROC.2025.54bp</a>'
  apa: 'Plata, C., &#38; Casallas Garcia, A. (2025). Machine learning analysis of
    the factors influencing university-industry collaborations. In <i>85th Annual
    Meeting of the Academy of Management</i> (Vol. 2025). Copenhagen, Denmark: Academy
    of Management. <a href="https://doi.org/10.5465/AMPROC.2025.54bp">https://doi.org/10.5465/AMPROC.2025.54bp</a>'
  chicago: Plata, Carlos, and Alejandro Casallas Garcia. “Machine Learning Analysis
    of the Factors Influencing University-Industry Collaborations.” In <i>85th Annual
    Meeting of the Academy of Management</i>, Vol. 2025. Academy of Management, 2025.
    <a href="https://doi.org/10.5465/AMPROC.2025.54bp">https://doi.org/10.5465/AMPROC.2025.54bp</a>.
  ieee: C. Plata and A. Casallas Garcia, “Machine learning analysis of the factors
    influencing university-industry collaborations,” in <i>85th Annual Meeting of
    the Academy of Management</i>, Copenhagen, Denmark, 2025, vol. 2025, no. 1.
  ista: 'Plata C, Casallas Garcia A. 2025. Machine learning analysis of the factors
    influencing university-industry collaborations. 85th Annual Meeting of the Academy
    of Management. AOM: Annual Meeting of the Academy of Management vol. 2025.'
  mla: Plata, Carlos, and Alejandro Casallas Garcia. “Machine Learning Analysis of
    the Factors Influencing University-Industry Collaborations.” <i>85th Annual Meeting
    of the Academy of Management</i>, vol. 2025, no. 1, Academy of Management, 2025,
    doi:<a href="https://doi.org/10.5465/AMPROC.2025.54bp">10.5465/AMPROC.2025.54bp</a>.
  short: C. Plata, A. Casallas Garcia, in:, 85th Annual Meeting of the Academy of
    Management, Academy of Management, 2025.
conference:
  end_date: 2025-07-29
  location: Copenhagen, Denmark
  name: 'AOM: Annual Meeting of the Academy of Management'
  start_date: 2025-07-25
date_created: 2025-07-06T22:01:23Z
date_published: 2025-06-17T00:00:00Z
date_updated: 2025-09-09T08:39:03Z
day: '17'
department:
- _id: CaMu
doi: 10.5465/AMPROC.2025.54bp
intvolume: '      2025'
issue: '1'
language:
- iso: eng
month: '06'
oa_version: None
publication: 85th Annual Meeting of the Academy of Management
publication_identifier:
  eissn:
  - 2151-6561
  issn:
  - 0065-0668
publication_status: published
publisher: Academy of Management
quality_controlled: '1'
scopus_import: '1'
status: public
title: Machine learning analysis of the factors influencing university-industry collaborations
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 2025
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '19969'
abstract:
- lang: eng
  text: "In the stochastic population protocol model, we are given a connected graph
    with n nodes, and in every time step, a scheduler samples an edge of the graph
    uniformly at random and the nodes connected by this edge interact. A fundamental
    task in this model is stable leader election, in which all nodes start in an identical
    state and the aim is to reach a configuration in which (1)\r\nexactly one node
    is elected as leader and (2) this node remains as the unique leader no matter
    what sequence of interactions follows. On cliques, the complexity of this problem
    has recently been settled: time-optimal protocols stabilize in (n log n) expected
    steps using (log log n) states, whereas protocols that use O(1) states require
    (n2) expected steps. In this work, we investigate the complexity of stable leader
    election on graphs. We provide the first non-trivial time lower bounds on general
    graphs, showing that, when moving beyond cliques, the complexity of stable leader
    election can range from O(1) to (n3) expected steps. We describe a protocol that
    is time-optimal on many graph families, but uses polynomially-many states. In
    contrast, we give a near-time-optimal protocol that uses only O(log2 n) states
    that is at most a factor O(log n) slower. Finally, we observe that for many graphs
    the constant-state protocol of Beauquier et al. [OPODIS 2013] is at most a factor
    O(n log n) slower than the fast polynomial-state protocol, and among constant-state
    protocols, this protocol has near-optimal average case complexity on dense random
    graphs."
acknowledgement: We thank all anonymous reviewers for their helpful comments. We would
  also like to thank Jakob Solnerzik and Olivier Stietel for catching some errors
  in the proofs. Open Access funding enabled and organized by Projekt DEAL. We gratefully
  acknowledge funding from the European Research Council (ERC) under the European
  Union’s Horizon 2020 research and innovation programme (grant agreement No 805223
  ScaleML).
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Dan-Adrian
  full_name: Alistarh, Dan-Adrian
  id: 4A899BFC-F248-11E8-B48F-1D18A9856A87
  last_name: Alistarh
  orcid: 0000-0003-3650-940X
- first_name: Joel
  full_name: Rybicki, Joel
  id: 334EFD2E-F248-11E8-B48F-1D18A9856A87
  last_name: Rybicki
  orcid: 0000-0002-6432-6646
- first_name: Sasha
  full_name: Voitovych, Sasha
  last_name: Voitovych
citation:
  ama: Alistarh D-A, Rybicki J, Voitovych S. Near-optimal leader election in population
    protocols on graphs. <i>Distributed Computing</i>. 2025;38:207-245. doi:<a href="https://doi.org/10.1007/s00446-025-00487-7">10.1007/s00446-025-00487-7</a>
  apa: Alistarh, D.-A., Rybicki, J., &#38; Voitovych, S. (2025). Near-optimal leader
    election in population protocols on graphs. <i>Distributed Computing</i>. Springer
    Nature. <a href="https://doi.org/10.1007/s00446-025-00487-7">https://doi.org/10.1007/s00446-025-00487-7</a>
  chicago: Alistarh, Dan-Adrian, Joel Rybicki, and Sasha Voitovych. “Near-Optimal
    Leader Election in Population Protocols on Graphs.” <i>Distributed Computing</i>.
    Springer Nature, 2025. <a href="https://doi.org/10.1007/s00446-025-00487-7">https://doi.org/10.1007/s00446-025-00487-7</a>.
  ieee: D.-A. Alistarh, J. Rybicki, and S. Voitovych, “Near-optimal leader election
    in population protocols on graphs,” <i>Distributed Computing</i>, vol. 38. Springer
    Nature, pp. 207–245, 2025.
  ista: Alistarh D-A, Rybicki J, Voitovych S. 2025. Near-optimal leader election in
    population protocols on graphs. Distributed Computing. 38, 207–245.
  mla: Alistarh, Dan-Adrian, et al. “Near-Optimal Leader Election in Population Protocols
    on Graphs.” <i>Distributed Computing</i>, vol. 38, Springer Nature, 2025, pp.
    207–45, doi:<a href="https://doi.org/10.1007/s00446-025-00487-7">10.1007/s00446-025-00487-7</a>.
  short: D.-A. Alistarh, J. Rybicki, S. Voitovych, Distributed Computing 38 (2025)
    207–245.
corr_author: '1'
date_created: 2025-07-06T22:01:24Z
date_published: 2025-09-01T00:00:00Z
date_updated: 2025-12-30T09:04:18Z
day: '01'
ddc:
- '510'
department:
- _id: DaAl
doi: 10.1007/s00446-025-00487-7
ec_funded: 1
external_id:
  arxiv:
  - '2205.12597'
  isi:
  - '001518300400001'
file:
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  checksum: 2789c0fdfb58f64930f05f6ac2b3ca61
  content_type: application/pdf
  creator: dernst
  date_created: 2025-12-30T09:03:55Z
  date_updated: 2025-12-30T09:03:55Z
  file_id: '20900'
  file_name: 2025_DistributedComp_Alistarh.pdf
  file_size: 770705
  relation: main_file
  success: 1
file_date_updated: 2025-12-30T09:03:55Z
has_accepted_license: '1'
intvolume: '        38'
isi: 1
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
page: 207-245
project:
- _id: 268A44D6-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '805223'
  name: Elastic Coordination for Scalable Machine Learning
publication: Distributed Computing
publication_identifier:
  eissn:
  - 1432-0452
  issn:
  - 0178-2770
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
related_material:
  record:
  - id: '11844'
    relation: earlier_version
    status: public
scopus_import: '1'
status: public
title: Near-optimal leader election in population protocols on graphs
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: 38
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '19982'
abstract:
- lang: eng
  text: "Dynamically maintaining the minimum cut in a graph G under edge insertions
    and deletion is a fundamental problem in dynamic graph algorithms for which no
    conditional lower bound on the time per operation exists. In an n-node graph the
    best known (1 + o (1))-approximate algorithm takes  update time [14]. If the minimum
    cut is guaranteed to be (log n )o (1), a deterministic exact algorithm with n
    o (1) update time exists [8].\r\nWe present the first fully dynamic algorithm
    for (1 + o (1))-approximate minimum cut with n o(1) update time. Our main technical
    contribution is to show that it suffices to consider small-volume cuts in suitably
    contracted graphs."
acknowledgement: This project has received funding from the European Research Council
  (ERC) under the European Union’sHorizon 2020 research and innovation programme (MoDynStruct,
  No. 101019564) and the Austrian Science Fund(FWF) grant DOI 10.55776/Z422, grant
  DOI 10.55776/I5982, and grant DOI 10.55776/P33775 with additional funding from the
  netidee SCIENCE Stiftung, 2020–2024.
article_processing_charge: No
arxiv: 1
author:
- first_name: Antoine
  full_name: El-Hayek, Antoine
  id: 888a098e-fcac-11ee-aff7-d347be57b725
  last_name: El-Hayek
  orcid: 0000-0003-4268-7368
- first_name: Monika H
  full_name: Henzinger, Monika H
  id: 540c9bbd-f2de-11ec-812d-d04a5be85630
  last_name: Henzinger
  orcid: 0000-0002-5008-6530
- first_name: Jason
  full_name: Li, Jason
  last_name: Li
citation:
  ama: 'El-Hayek A, Henzinger M, Li J. Fully dynamic approximate minimum cut in subpolynomial
    time per operation. In: <i>Proceedings of the 2025 Annual ACM-SIAM Symposium on
    Discrete Algorithms</i>. Society for Industrial and Applied Mathematics; 2025:750-784.
    doi:<a href="https://doi.org/10.1137/1.9781611978322.22">10.1137/1.9781611978322.22</a>'
  apa: 'El-Hayek, A., Henzinger, M., &#38; Li, J. (2025). Fully dynamic approximate
    minimum cut in subpolynomial time per operation. In <i>Proceedings of the 2025
    Annual ACM-SIAM Symposium on Discrete Algorithms</i> (pp. 750–784). New Orleans,
    LA, United States: Society for Industrial and Applied Mathematics. <a href="https://doi.org/10.1137/1.9781611978322.22">https://doi.org/10.1137/1.9781611978322.22</a>'
  chicago: El-Hayek, Antoine, Monika Henzinger, and Jason Li. “Fully Dynamic Approximate
    Minimum Cut in Subpolynomial Time per Operation.” In <i>Proceedings of the 2025
    Annual ACM-SIAM Symposium on Discrete Algorithms</i>, 750–84. Society for Industrial
    and Applied Mathematics, 2025. <a href="https://doi.org/10.1137/1.9781611978322.22">https://doi.org/10.1137/1.9781611978322.22</a>.
  ieee: A. El-Hayek, M. Henzinger, and J. Li, “Fully dynamic approximate minimum cut
    in subpolynomial time per operation,” in <i>Proceedings of the 2025 Annual ACM-SIAM
    Symposium on Discrete Algorithms</i>, New Orleans, LA, United States, 2025, pp.
    750–784.
  ista: 'El-Hayek A, Henzinger M, Li J. 2025. Fully dynamic approximate minimum cut
    in subpolynomial time per operation. Proceedings of the 2025 Annual ACM-SIAM Symposium
    on Discrete Algorithms. SODA: Symposium on Discrete Algorithms, 750–784.'
  mla: El-Hayek, Antoine, et al. “Fully Dynamic Approximate Minimum Cut in Subpolynomial
    Time per Operation.” <i>Proceedings of the 2025 Annual ACM-SIAM Symposium on Discrete
    Algorithms</i>, Society for Industrial and Applied Mathematics, 2025, pp. 750–84,
    doi:<a href="https://doi.org/10.1137/1.9781611978322.22">10.1137/1.9781611978322.22</a>.
  short: A. El-Hayek, M. Henzinger, J. Li, in:, Proceedings of the 2025 Annual ACM-SIAM
    Symposium on Discrete Algorithms, Society for Industrial and Applied Mathematics,
    2025, pp. 750–784.
conference:
  end_date: 2025-01-15
  location: New Orleans, LA, United States
  name: 'SODA: Symposium on Discrete Algorithms'
  start_date: 2025-01-12
corr_author: '1'
date_created: 2025-07-10T13:08:57Z
date_published: 2025-01-07T00:00:00Z
date_updated: 2025-12-29T12:30:04Z
day: '07'
department:
- _id: MoHe
doi: 10.1137/1.9781611978322.22
ec_funded: 1
external_id:
  arxiv:
  - '2412.15069'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2412.15069
month: '01'
oa: 1
oa_version: Preprint
page: 750-784
project:
- _id: bd9ca328-d553-11ed-ba76-dc4f890cfe62
  call_identifier: H2020
  grant_number: '101019564'
  name: The design and evaluation of modern fully dynamic data structures
- _id: 34def286-11ca-11ed-8bc3-da5948e1613c
  grant_number: Z00422
  name: Efficient algorithms
- _id: bda196b2-d553-11ed-ba76-8e8ee6c21103
  grant_number: I05982
  name: Static and Dynamic Hierarchical Graph Decompositions
- _id: bd9e3a2e-d553-11ed-ba76-8aa684ce17fe
  grant_number: P33775
  name: Fast Algorithms for a Reactive Network Layer
publication: Proceedings of the 2025 Annual ACM-SIAM Symposium on Discrete Algorithms
publication_identifier:
  eisbn:
  - '9781611978322'
publication_status: published
publisher: Society for Industrial and Applied Mathematics
quality_controlled: '1'
status: public
title: Fully dynamic approximate minimum cut in subpolynomial time per operation
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
