---
OA_place: publisher
OA_type: hybrid
_id: '19876'
abstract:
- lang: eng
text: "Assortative mating and sexual selection are widespread in nature and can
play an important role in speciation by facilitating the buildup and maintenance
of reproductive isolation (RI). However, their contribution to genome-wide suppression
of gene flow during RI is rarely quantified.\r\nHere, we consider a polygenic
“magic” trait that is divergently selected across two populations connected by
migration, while also serving as the basis of assortative mating, thus generating
sexual selection on one or both sexes. We obtain theoretical predictions for divergence
at\r\nindividual trait loci by assuming that the effect of all other loci on any
locus can be encapsulated via an effective migration rate, which bears a simple
relationship to measurable fitness components of migrants and various early-generation
hybrids. Our analysis clarifies how “tipping\r\npoints” (characterized by an abrupt
collapse of adaptive divergence) arise, and when assortative mating can shift
the critical level of migration beyond which divergence collapses. We quantify
the relative contributions of viability and sexual selection to genome-wide barriers
to gene\r\nflow and discuss how these depend on existing divergence levels. Our
results suggest that effective migration rates provide a useful way of understanding
genomic divergence, even in scenarios involving multiple, interacting mechanisms
of RI. "
acknowledged_ssus:
- _id: ScienComp
acknowledgement: We thank Nick Barton for useful comments on the manuscript. This
research was supported by the Scientific Service Units (SSU) of Institute of Science
and Technology Austria (ISTA) through resources provided by Scientific Computing
(SciComp).
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Parvathy
full_name: Surendranadh, Parvathy
id: 455235B8-F248-11E8-B48F-1D18A9856A87
last_name: Surendranadh
orcid: 0000-0001-6395-386X
- first_name: Himani
full_name: Sachdeva, Himani
last_name: Sachdeva
citation:
ama: Surendranadh P, Sachdeva H. Effect of assortative mating and sexual selection
on polygenic barriers to gene flow. Evolution. 2025;79(7):1185-1198. doi:10.1093/evolut/qpaf047
apa: Surendranadh, P., & Sachdeva, H. (2025). Effect of assortative mating and
sexual selection on polygenic barriers to gene flow. Evolution. Oxford
University Press. https://doi.org/10.1093/evolut/qpaf047
chicago: Surendranadh, Parvathy, and Himani Sachdeva. “Effect of Assortative Mating
and Sexual Selection on Polygenic Barriers to Gene Flow.” Evolution. Oxford
University Press, 2025. https://doi.org/10.1093/evolut/qpaf047.
ieee: P. Surendranadh and H. Sachdeva, “Effect of assortative mating and sexual
selection on polygenic barriers to gene flow,” Evolution, vol. 79, no.
7. Oxford University Press, pp. 1185–1198, 2025.
ista: Surendranadh P, Sachdeva H. 2025. Effect of assortative mating and sexual
selection on polygenic barriers to gene flow. Evolution. 79(7), 1185–1198.
mla: Surendranadh, Parvathy, and Himani Sachdeva. “Effect of Assortative Mating
and Sexual Selection on Polygenic Barriers to Gene Flow.” Evolution, vol.
79, no. 7, Oxford University Press, 2025, pp. 1185–98, doi:10.1093/evolut/qpaf047.
short: P. Surendranadh, H. Sachdeva, Evolution 79 (2025) 1185–1198.
corr_author: '1'
date_created: 2025-06-23T13:51:00Z
date_published: 2025-07-01T00:00:00Z
date_updated: 2025-12-30T08:44:13Z
day: '01'
ddc:
- '570'
department:
- _id: NiBa
doi: 10.1093/evolut/qpaf047
external_id:
isi:
- '001490646300001'
file:
- access_level: open_access
checksum: 288ca936cef794d68a55356e70671846
content_type: application/pdf
creator: dernst
date_created: 2025-12-30T08:43:33Z
date_updated: 2025-12-30T08:43:33Z
file_id: '20898'
file_name: 2025_Evolution_Surendranadh.pdf
file_size: 2784295
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success: 1
file_date_updated: 2025-12-30T08:43:33Z
has_accepted_license: '1'
intvolume: ' 79'
isi: 1
issue: '7'
language:
- iso: eng
month: '07'
oa: 1
oa_version: Published Version
page: 1185-1198
publication: Evolution
publication_identifier:
eissn:
- 1558-5646
issn:
- 0014-3820
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
related_material:
record:
- id: '18712'
relation: research_data
status: public
scopus_import: '1'
status: public
title: Effect of assortative mating and sexual selection on polygenic barriers to
gene flow
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 79
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19877'
abstract:
- lang: eng
text: "As inference on Large Language Models (LLMs) emerges as an important workload
in machine learning applications, model weight quantization has become a standard
technique for efficient GPU deployment. Quantization not only reduces model size,
but has also been shown to yield substantial speedups for single-user inference,
due to reduced memory movement, with low accuracy impact. Yet, it remains a key
open question whether speedups are achievable also in batched settings with multiple
parallel clients, which are highly relevant for practical serving. It is unclear
whether GPU kernels can be designed to remain practically memory-bound, while
supporting the substantially increased compute requirements of batched workloads.\r\nIn
this paper, we resolve this question positively by introducing a new design for
Mixed-precision Auto-Regressive LINear kernels, called MARLIN. Concretely, given
a model whose weights are compressed via quantization to, e.g., 4 bits per element,
MARLIN shows that batchsizes up to 16-32 can be practically supported with close
to maximum (4×) quantization speedup, and larger batchsizes up to 64-128 with
gradually decreasing, but still significant, acceleration. MARLIN accomplishes
this via a combination of techniques, such as asynchronous memory access, complex
task scheduling and pipelining, and bespoke quantization support. Our experiments
show that MARLIN's near-optimal performance on individual LLM layers across different
scenarios can also lead to significant end-to-end LLM inference speedups (of up
to 2.8×) when integrated with the popular vLLM open-source serving engine. Finally,
we show that MARLIN is extensible to further compression techniques, like NVIDIA
2:4 sparsity, leading to additional speedups."
acknowledgement: The authors would like to thank the Neural Magic team, in particular
Michael Goin, Alexander Matveev, and Rob Shaw, for support with the vLLM integration.
This research was supported in part by generous grants from NVIDIA and Google.
article_processing_charge: Yes (via OA deal)
arxiv: 1
author:
- first_name: Elias
full_name: Frantar, Elias
id: 09a8f98d-ec99-11ea-ae11-c063a7b7fe5f
last_name: Frantar
- first_name: Roberto L.
full_name: Castro, Roberto L.
last_name: Castro
- first_name: Jiale
full_name: Chen, Jiale
id: 4d0a9064-1ff6-11ee-9fa6-ec046c604785
last_name: Chen
orcid: 0000-0001-5337-5875
- first_name: Torsten
full_name: Hoefler, Torsten
last_name: Hoefler
- first_name: Dan-Adrian
full_name: Alistarh, Dan-Adrian
id: 4A899BFC-F248-11E8-B48F-1D18A9856A87
last_name: Alistarh
orcid: 0000-0003-3650-940X
citation:
ama: 'Frantar E, Castro RL, Chen J, Hoefler T, Alistarh D-A. MARLIN: Mixed-precision
auto-regressive parallel inference on Large Language Models. In: Proceedings
of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel
Programming. Association for Computing Machinery; 2025:239-251. doi:10.1145/3710848.3710871'
apa: 'Frantar, E., Castro, R. L., Chen, J., Hoefler, T., & Alistarh, D.-A. (2025).
MARLIN: Mixed-precision auto-regressive parallel inference on Large Language Models.
In Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice
of Parallel Programming (pp. 239–251). Las Vegas, NV, United States: Association
for Computing Machinery. https://doi.org/10.1145/3710848.3710871'
chicago: 'Frantar, Elias, Roberto L. Castro, Jiale Chen, Torsten Hoefler, and Dan-Adrian
Alistarh. “MARLIN: Mixed-Precision Auto-Regressive Parallel Inference on Large
Language Models.” In Proceedings of the 30th ACM SIGPLAN Annual Symposium on
Principles and Practice of Parallel Programming, 239–51. Association for Computing
Machinery, 2025. https://doi.org/10.1145/3710848.3710871.'
ieee: 'E. Frantar, R. L. Castro, J. Chen, T. Hoefler, and D.-A. Alistarh, “MARLIN:
Mixed-precision auto-regressive parallel inference on Large Language Models,”
in Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice
of Parallel Programming, Las Vegas, NV, United States, 2025, pp. 239–251.'
ista: 'Frantar E, Castro RL, Chen J, Hoefler T, Alistarh D-A. 2025. MARLIN: Mixed-precision
auto-regressive parallel inference on Large Language Models. Proceedings of the
30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming.
PPoPP: Symposium on Principles and Practice of Parallel Programming, 239–251.'
mla: 'Frantar, Elias, et al. “MARLIN: Mixed-Precision Auto-Regressive Parallel Inference
on Large Language Models.” Proceedings of the 30th ACM SIGPLAN Annual Symposium
on Principles and Practice of Parallel Programming, Association for Computing
Machinery, 2025, pp. 239–51, doi:10.1145/3710848.3710871.'
short: E. Frantar, R.L. Castro, J. Chen, T. Hoefler, D.-A. Alistarh, in:, Proceedings
of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel
Programming, Association for Computing Machinery, 2025, pp. 239–251.
conference:
end_date: 2025-03-05
location: Las Vegas, NV, United States
name: 'PPoPP: Symposium on Principles and Practice of Parallel Programming'
start_date: 2025-03-01
corr_author: '1'
date_created: 2025-06-23T13:51:58Z
date_published: 2025-02-28T00:00:00Z
date_updated: 2025-09-30T13:41:57Z
day: '28'
ddc:
- '000'
department:
- _id: DaAl
doi: 10.1145/3710848.3710871
external_id:
arxiv:
- '2408.11743'
isi:
- '001437826500019'
file:
- access_level: open_access
checksum: a0566ea3c168e8273501a5eb7d767cf8
content_type: application/pdf
creator: dernst
date_created: 2025-06-24T06:04:17Z
date_updated: 2025-06-24T06:04:17Z
file_id: '19883'
file_name: 2025_PPoPP_Frantar.pdf
file_size: 1330044
relation: main_file
success: 1
file_date_updated: 2025-06-24T06:04:17Z
has_accepted_license: '1'
isi: 1
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
page: 239-251
publication: Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and
Practice of Parallel Programming
publication_identifier:
isbn:
- '9798400714436'
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
related_material:
record:
- id: '19884'
relation: software
status: public
scopus_import: '1'
status: public
title: 'MARLIN: Mixed-precision auto-regressive parallel inference on Large Language
Models'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: conference
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19878'
abstract:
- lang: eng
text: Rock debris partially covers glaciers worldwide, with varying extents and
distributions, and controls sub‐debris melt rates by modifying energy transfer
from the atmosphere to the ice. Two key physical properties controlling this energy
exchange are thermal conductivity (k) and aerodynamic roughness length (z0). Accurate
representation of these properties in energy‐balance models is critical for understanding
climate‐glacier interactions and predicting the behavior of debris‐covered glaciers.
However, k and z0 have been derived at very few sites from limited local measurements,
using different approaches, and most model applications rely on values reported
from these few sites and studies. We derive k and z0 using established and modified
approaches from data at three locations on Pirámide Glacier in the central Chilean
Andes. By comparing methods and evaluating melt simulated with an energy‐balance
model, we reveal substantial differences between approaches. These lead to discrepancies
between ice melt from energy‐balance simulations and observed data, and highlight
the impact of method choice on calculated ice melt. Optimizing k against measured
melt appears a viable approach to constrain melt simulations. Determining z0 seems
less critical, as it has a smaller impact on total melt. Profile aerodynamic method
measurements for estimating z0, despite higher costs, are independent of ice melt
calculations. The large, unexpected differences between methods indicate a substantial
knowledge gap. The fact that field‐derived k and z0 fail to work well in energy‐balance
models, suggests that model values represent bulk properties distinct from theoretical
field measurements. Addressing this gap is essential for improving glacier melt
predictions.
acknowledgement: This project received funding from the Swiss National Science Foundation
(Grant 204322, project “REsolving the thickNess Of debris on Earth's glacIers and
its Rate of change,” RENOIR). We thank Lars Groeneveld, Diego Hernández, Alonso
Mejías, Gabriela Reyes and Gabriela Tala for their support during fieldwork. Open
access funding provided by Institute of Science and Technology Austria/KEMÖ.
article_number: e2025JF008360
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Juan Vicente
full_name: Melo Velasco, Juan Vicente
id: 2611dec0-b9c6-11ed-9bea-a81c2b17a549
last_name: Melo Velasco
- first_name: Evan
full_name: Miles, Evan
last_name: Miles
- first_name: Michael
full_name: McCarthy, Michael
id: 22a2674a-61ce-11ee-94b5-d18813baf16f
last_name: McCarthy
- first_name: Thomas
full_name: Shaw, Thomas
id: 3caa3f91-1f03-11ee-96ce-e0e553054d6e
last_name: Shaw
orcid: 0000-0001-7640-6152
- first_name: Catriona Louise
full_name: Fyffe, Catriona Louise
id: 001b0422-8d15-11ed-bc51-cab6c037a228
last_name: Fyffe
- first_name: Adrià
full_name: Fontrodona-Bach, Adrià
id: f06891fd-9f42-11ee-8632-a20971c43046
last_name: Fontrodona-Bach
- first_name: Francesca
full_name: Pellicciotti, Francesca
id: b28f055a-81ea-11ed-b70c-a9fe7f7b0e70
last_name: Pellicciotti
orcid: 0000-0002-5554-8087
citation:
ama: 'Melo Velasco JV, Miles E, McCarthy M, et al. Method dependence in thermal
conductivity and aerodynamic roughness length estimates on a debris‐covered glacier.
Journal of Geophysical Research: Earth Surface. 2025;130(6). doi:10.1029/2025jf008360'
apa: 'Melo Velasco, J. V., Miles, E., McCarthy, M., Shaw, T., Fyffe, C. L., Fontrodona-Bach,
A., & Pellicciotti, F. (2025). Method dependence in thermal conductivity and
aerodynamic roughness length estimates on a debris‐covered glacier. Journal
of Geophysical Research: Earth Surface. Wiley. https://doi.org/10.1029/2025jf008360'
chicago: 'Melo Velasco, Juan Vicente, Evan Miles, Michael McCarthy, Thomas Shaw,
Catriona Louise Fyffe, Adrià Fontrodona-Bach, and Francesca Pellicciotti. “Method
Dependence in Thermal Conductivity and Aerodynamic Roughness Length Estimates
on a Debris‐covered Glacier.” Journal of Geophysical Research: Earth Surface.
Wiley, 2025. https://doi.org/10.1029/2025jf008360.'
ieee: 'J. V. Melo Velasco et al., “Method dependence in thermal conductivity
and aerodynamic roughness length estimates on a debris‐covered glacier,” Journal
of Geophysical Research: Earth Surface, vol. 130, no. 6. Wiley, 2025.'
ista: 'Melo Velasco JV, Miles E, McCarthy M, Shaw T, Fyffe CL, Fontrodona-Bach A,
Pellicciotti F. 2025. Method dependence in thermal conductivity and aerodynamic
roughness length estimates on a debris‐covered glacier. Journal of Geophysical
Research: Earth Surface. 130(6), e2025JF008360.'
mla: 'Melo Velasco, Juan Vicente, et al. “Method Dependence in Thermal Conductivity
and Aerodynamic Roughness Length Estimates on a Debris‐covered Glacier.” Journal
of Geophysical Research: Earth Surface, vol. 130, no. 6, e2025JF008360, Wiley,
2025, doi:10.1029/2025jf008360.'
short: 'J.V. Melo Velasco, E. Miles, M. McCarthy, T. Shaw, C.L. Fyffe, A. Fontrodona-Bach,
F. Pellicciotti, Journal of Geophysical Research: Earth Surface 130 (2025).'
corr_author: '1'
date_created: 2025-06-23T13:54:01Z
date_published: 2025-06-15T00:00:00Z
date_updated: 2025-09-30T13:42:28Z
day: '15'
ddc:
- '550'
department:
- _id: FrPe
doi: 10.1029/2025jf008360
external_id:
isi:
- '001508794200001'
file:
- access_level: open_access
checksum: ca91541516c71d240321630ca42b4dc4
content_type: application/pdf
creator: dernst
date_created: 2025-06-24T06:27:34Z
date_updated: 2025-06-24T06:27:34Z
file_id: '19886'
file_name: 2025_JGREarthSurface_MeloVelasco.pdf
file_size: 3949928
relation: main_file
success: 1
file_date_updated: 2025-06-24T06:27:34Z
has_accepted_license: '1'
intvolume: ' 130'
isi: 1
issue: '6'
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
publication: 'Journal of Geophysical Research: Earth Surface'
publication_identifier:
eissn:
- 2169-9011
issn:
- 2169-9003
publication_status: published
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: Method dependence in thermal conductivity and aerodynamic roughness length
estimates on a debris‐covered glacier
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: 130
year: '2025'
...
---
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.
European Journal of Combinatorics. 2025;127. doi:10.1016/j.ejc.2025.104138
apa: Dvořák, Z., Moore, B., Seifrtová, M., & Šámal, R. (2025). Precoloring extension
in planar near-Eulerian-triangulations. European Journal of Combinatorics.
Elsevier. https://doi.org/10.1016/j.ejc.2025.104138
chicago: Dvořák, Zdeněk, Benjamin Moore, Michaela Seifrtová, and Robert Šámal. “Precoloring
Extension in Planar Near-Eulerian-Triangulations.” European Journal of Combinatorics.
Elsevier, 2025. https://doi.org/10.1016/j.ejc.2025.104138.
ieee: Z. Dvořák, B. Moore, M. Seifrtová, and R. Šámal, “Precoloring extension in
planar near-Eulerian-triangulations,” European Journal of Combinatorics,
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.”
European Journal of Combinatorics, vol. 127, 104138, Elsevier, 2025, doi:10.1016/j.ejc.2025.104138.
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'
file:
- access_level: open_access
checksum: 8b3585df45b25091fba9bee9854b7d01
content_type: application/pdf
creator: dernst
date_created: 2025-06-24T06:33:30Z
date_updated: 2025-06-24T06:33:30Z
file_id: '19887'
file_name: 2025_EuropJournCombinatorics_Dvorak.pdf
file_size: 564203
relation: main_file
success: 1
file_date_updated: 2025-06-24T06:33:30Z
has_accepted_license: '1'
intvolume: ' 127'
isi: 1
language:
- iso: eng
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:
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: 127
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. The Journal of Chemical Physics. 2025;162(23).
doi:10.1063/5.0271155
apa: Al Hyder, R., Lemeshko, M., & Cappellaro, A. (2025). Quantum transport
in the presence of a chiral molecular potential. The Journal of Chemical Physics.
AIP Publishing. https://doi.org/10.1063/5.0271155
chicago: Al Hyder, Ragheed, Mikhail Lemeshko, and Alberto Cappellaro. “Quantum Transport
in the Presence of a Chiral Molecular Potential.” The Journal of Chemical Physics.
AIP Publishing, 2025. https://doi.org/10.1063/5.0271155.
ieee: R. Al Hyder, M. Lemeshko, and A. Cappellaro, “Quantum transport in the presence
of a chiral molecular potential,” The Journal of Chemical Physics, 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.” The Journal of Chemical Physics, vol. 162, no. 23, 234106,
AIP Publishing, 2025, doi:10.1063/5.0271155.
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:
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doi: 10.1063/5.0271155
ec_funded: 1
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arxiv:
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publication: The Journal of Chemical Physics
publication_identifier:
eissn:
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issn:
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publication_status: published
publisher: AIP Publishing
quality_controlled: '1'
scopus_import: '1'
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title: Quantum transport in the presence of a chiral molecular potential
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type: journal_article
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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:10.15479/AT:ISTA:19885
apa: Saez Mollejo, J. (2025). Automated All-RF Tuning for Spin Qubit Readout and
Control. Institute of Science and Technology Austria. https://doi.org/10.15479/AT:ISTA:19885
chicago: Saez Mollejo, Jaime. “Automated All-RF Tuning for Spin Qubit Readout and
Control.” Institute of Science and Technology Austria, 2025. https://doi.org/10.15479/AT:ISTA:19885.
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, 10.15479/AT:ISTA:19885.
mla: Saez Mollejo, Jaime. Automated All-RF Tuning for Spin Qubit Readout and
Control. Institute of Science and Technology Austria, 2025, doi:10.15479/AT:ISTA:19885.
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:
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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
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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:
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short: CC BY (4.0)
type: research_data
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: publisher
_id: '19903'
abstract:
- lang: eng
text: "Cooperation, that is, one person paying a cost for another's benefit, is
a fundamental principle without which no form of society could exist. The extent
to which humans cooperate with each other is also an essential feature that differentiates
them from other animals. Cooperation occurs even in the absence of altruistic
motivations, when it is selfishly incentivised by the expectation of a future
reward. For example, many economic interactions are well described that way. This
kind of cooperation requires that people exhibit reciprocal behaviour that acts
as a mechanism that rewards cooperation.\r\nWith game-theoretic models, it is
possible to formally study potential such mechanisms and under what conditions
they can exist. This thesis contributes to this effort by analysing recently introduced
models of cooperation that advance on previous work by taking into account the
potential for pre-existing inequality among cooperating individuals as well as
the different forms that reciprocity can take.\r\nIndividuals may differ both
intrinsically, in their abilities, as well as extrinsically, in the amount of
resources they have available. Allowing for such differences in a model of cooperation
helps to understand how inequality affects the potential for, and outcomes of,
cooperation among unequals. In this thesis, it is shown that in the presence of
intrinsic inequality, a similar unequal distribution of resources can increase
the potential for cooperation. This effect is stronger the smaller the group is
in which cooperation takes place. It is also shown that under particular assumptions,
if the unequal members of a group vary the size of their contributions to a cooperative
effort over time, they can thereby increase their efficiency and improve the collective
outcome.\r\nCooperative behaviour in a two-person interaction can be rewarded
either by direct reciprocation whenever the same two people interact again, or
indirectly by a third party who observed the interaction. In the latter case of
indirect reciprocity, individuals are proximally rewarded by a good reputation,
which ultimately translates to being rewarded with cooperative behaviour by others.
This mechanism can enable selfishly motivated cooperation even in circumstances
where individuals are unlikely to meet again, akin to how money facilitates trade.
While these two forms of reciprocity have mostly been studied in isolation, this
thesis analyses both direct and indirect reciprocity in a general model in order
to compare their relative effectiveness under different circumstances. The contribution
of this thesis is an extension of previous work regarding a specific kind of interaction,
whose parameters allow for convenient mathematical analysis, to the most general
set of possible interactions."
acknowledgement: "The research for this thesis was supported by the European Research
Council\r\n(grant agreements No. 863818 and No. 850529), the European Union’s Horizon
2020 research and innovation programme (Marie Skłodowska-Curie grant agreement No.
754411),\r\nthe Austrian Science Fund (grant DOI 10.55776/COE12), the French Agence
Nationale\r\nde la Recherche under the Programme d’investissements d’avenir (project
reference 17-\r\nEURE-0010) and the Australian Government through the Australian
Research Council\r\n(grant No. SR200100005, “Securing Antarctica’s Environmental
Future”)."
alternative_title:
- ISTA Thesis
article_processing_charge: No
author:
- first_name: Valentin
full_name: Hübner, Valentin
id: 2c8aa207-dc7d-11ea-9b2f-f22972ecd910
last_name: Hübner
orcid: 0009-0001-5009-4987
citation:
ama: Hübner V. Reciprocity and inequality in social dilemmas. 2025. doi:10.15479/AT-ISTA-19903
apa: Hübner, V. (2025). Reciprocity and inequality in social dilemmas. Institute
of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-19903
chicago: Hübner, Valentin. “Reciprocity and Inequality in Social Dilemmas.” Institute
of Science and Technology Austria, 2025. https://doi.org/10.15479/AT-ISTA-19903.
ieee: V. Hübner, “Reciprocity and inequality in social dilemmas,” Institute of Science
and Technology Austria, 2025.
ista: Hübner V. 2025. Reciprocity and inequality in social dilemmas. Institute of
Science and Technology Austria.
mla: Hübner, Valentin. Reciprocity and Inequality in Social Dilemmas. Institute
of Science and Technology Austria, 2025, doi:10.15479/AT-ISTA-19903.
short: V. Hübner, Reciprocity and Inequality in Social Dilemmas, Institute of Science
and Technology Austria, 2025.
corr_author: '1'
date_created: 2025-06-25T13:50:10Z
date_published: 2025-06-25T00:00:00Z
date_updated: 2026-04-07T12:30:57Z
day: '25'
ddc:
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degree_awarded: PhD
department:
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- _id: KrCh
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page: '157'
project:
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call_identifier: H2020
grant_number: '863818'
name: 'Formal Methods for Stochastic Models: Algorithms and Applications'
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grant_number: '754411'
name: ISTplus - Postdoctoral Fellowships
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issn:
- 2663-337X
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publisher: Institute of Science and Technology Austria
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status: public
supervisor:
- first_name: Krishnendu
full_name: Chatterjee, Krishnendu
id: 2E5DCA20-F248-11E8-B48F-1D18A9856A87
last_name: Chatterjee
orcid: 0000-0002-4561-241X
title: Reciprocity and inequality in social dilemmas
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type: dissertation
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---
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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:10.15479/AT:ISTA:19915
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. https://doi.org/10.15479/AT:ISTA:19915
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. https://doi.org/10.15479/AT:ISTA:19915.
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, 10.15479/AT:ISTA:19915.
mla: 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, doi:10.15479/AT:ISTA:19915.
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: 2026-06-10T08:05:45Z
day: '27'
department:
- _id: MaLo
doi: 10.15479/AT:ISTA:19915
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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'
- _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
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: research_data
user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d
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. Journal of Experimental
Medicine. 2025;222(9). doi:10.1084/jem.20240109
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. Journal of Experimental Medicine. Rockefeller
University Press. https://doi.org/10.1084/jem.20240109
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.” Journal of
Experimental Medicine. Rockefeller University Press, 2025. https://doi.org/10.1084/jem.20240109.
ieee: R. Gawish et al., “Filamin A editing in myeloid cells reduces intestinal
inflammation and protects from colitis,” Journal of Experimental Medicine,
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.” Journal of Experimental Medicine,
vol. 222, no. 9, e20240109, Rockefeller University Press, 2025, doi:10.1084/jem.20240109.
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:
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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
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file_date_updated: 2025-12-30T09:00:04Z
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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.
Astronomy & Astrophysics. 2025;698. doi:10.1051/0004-6361/202453547'
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. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202453547'
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.” Astronomy & Astrophysics.
EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202453547.'
ieee: 'S. Gurung-López et al., “zELDA II: Reconstruction of galactic Lyman-alpha
spectra attenuated by the intergalactic medium using neural networks,” Astronomy
& Astrophysics, 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
& 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.” Astronomy
& Astrophysics, vol. 698, A139, EDP Sciences, 2025, doi:10.1051/0004-6361/202453547.'
short: S. Gurung-López, C. Byrohl, M. Gronke, D. Spinoso, A. Torralba Torregrosa,
A. Fernández-Soto, P. Arnalte-Mur, V.J. Martínez, Astronomy & 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 > 4): The properties of extremely blue galaxies.
Astronomy & Astrophysics. 2025;698. doi:10.1051/0004-6361/202453267'
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 > 4): The properties of extremely blue galaxies. Astronomy & Astrophysics.
EDP Sciences. https://doi.org/10.1051/0004-6361/202453267'
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 > 4): The Properties of Extremely Blue Galaxies.” Astronomy
& Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202453267.'
ieee: 'D. Dottorini et al., “Evolution of the UV slope of galaxies at cosmic
morning (z > 4): The properties of extremely blue galaxies,” Astronomy
& Astrophysics, 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 >
4): The properties of extremely blue galaxies. Astronomy & Astrophysics. 698,
A234.'
mla: 'Dottorini, D., et al. “Evolution of the UV Slope of Galaxies at Cosmic Morning
(z > 4): The Properties of Extremely Blue Galaxies.” Astronomy & Astrophysics,
vol. 698, A234, EDP Sciences, 2025, doi:10.1051/0004-6361/202453267.'
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 & 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. Astronomy &
Astrophysics. 2025;698. doi:10.1051/0004-6361/202554110
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. Astronomy & Astrophysics.
EDP Sciences. https://doi.org/10.1051/0004-6361/202554110
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.” Astronomy &
Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202554110.
ieee: L. J. Furtak et al., “Investigating photometric and spectroscopic variability
in the multiply imaged little red dot A2744-QSO1,” Astronomy & Astrophysics,
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 & Astrophysics. 698, A227.
mla: Furtak, Lukas J., et al. “Investigating Photometric and Spectroscopic Variability
in the Multiply Imaged Little Red Dot A2744-QSO1.” Astronomy & Astrophysics,
vol. 698, A227, EDP Sciences, 2025, doi:10.1051/0004-6361/202554110.
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 & 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. Proceedings of the ACM
on Programming Languages. 2025;9(PLDI):848-873. doi:10.1145/3729284
apa: Spies, S., Mück, N., Zeng, H., Sammler, M. J., Lattuada, A., Müller, P., &
Dreyer, D. (2025). Destabilizing Iris. Proceedings of the ACM on Programming
Languages. Association for Computing Machinery. https://doi.org/10.1145/3729284
chicago: Spies, Simon, Niklas Mück, Haoyi Zeng, Michael Joachim Sammler, Andrea
Lattuada, Peter Müller, and Derek Dreyer. “Destabilizing Iris.” Proceedings
of the ACM on Programming Languages. Association for Computing Machinery,
2025. https://doi.org/10.1145/3729284.
ieee: S. Spies et al., “Destabilizing Iris,” Proceedings of the ACM on
Programming Languages, 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.” Proceedings of the ACM on Programming
Languages, vol. 9, no. PLDI, Association for Computing Machinery, 2025, pp.
848–73, doi:10.1145/3729284.
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. Proceedings of
the ACM on Programming Languages. 2025;9(PLDI):73-97. doi:10.1145/3729249'
apa: 'Bedarkar, K., Elbeheiry, L., Sammler, M. J., 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. Association for Computing Machinery. https://doi.org/10.1145/3729249'
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.” Proceedings of
the ACM on Programming Languages. Association for Computing Machinery, 2025.
https://doi.org/10.1145/3729249.'
ieee: 'K. Bedarkar et al., “RefinedProsa: Connecting response-time analysis
with C verification for interrupt-free schedulers,” Proceedings of the ACM
on Programming Languages, 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.” Proceedings of the ACM
on Programming Languages, vol. 9, no. PLDI, Association for Computing Machinery,
2025, pp. 73–97, doi:10.1145/3729249.'
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. Information Sciences.
2025;719(11). doi:10.1016/j.ins.2025.122425'
apa: 'Mahini, M., Beigy, H., Qadami, S., & Saghafian, M. (2025). Simplet-based
signatures and approximation in simplicial complexes: Frequency, degree, and centrality.
Information Sciences. Elsevier. https://doi.org/10.1016/j.ins.2025.122425'
chicago: 'Mahini, Mohammad, Hamid Beigy, Salman Qadami, and Morteza Saghafian. “Simplet-Based
Signatures and Approximation in Simplicial Complexes: Frequency, Degree, and Centrality.”
Information Sciences. Elsevier, 2025. https://doi.org/10.1016/j.ins.2025.122425.'
ieee: 'M. Mahini, H. Beigy, S. Qadami, and M. Saghafian, “Simplet-based signatures
and approximation in simplicial complexes: Frequency, degree, and centrality,”
Information Sciences, 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.” Information Sciences, vol.
719, no. 11, 122425, Elsevier, 2025, doi:10.1016/j.ins.2025.122425.'
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'
...
---
APC_amount: 4215,38 EUR
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. Life Science Alliance. 2025;8(9). doi:10.26508/lsa.202503208
apa: Kuhn, K. D., Cho, U. H., & Hetzer, M. (2025). PSME3 regulates migration
and differentiation of myoblasts. Life Science Alliance. Embo Press. https://doi.org/10.26508/lsa.202503208
chicago: Kuhn, Kenneth D, Ukrae H. Cho, and Martin Hetzer. “PSME3 Regulates Migration
and Differentiation of Myoblasts.” Life Science Alliance. Embo Press, 2025.
https://doi.org/10.26508/lsa.202503208.
ieee: K. D. Kuhn, U. H. Cho, and M. Hetzer, “PSME3 regulates migration and differentiation
of myoblasts,” Life Science Alliance, 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.” Life Science Alliance, vol. 8, no. 9, e202503208, Embo Press,
2025, doi:10.26508/lsa.202503208.
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: 2026-05-20T08:38:04Z
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
project:
- _id: B67AFEDC-15C9-11EA-A837-991A96BB2854
name: IST Austria Open Access Fund
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. The Astronomical Journal. 2025;170(1). doi:10.3847/1538-3881/addd21
apa: Cheng, S., Schlaufman, K. C., & 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.
IOP Publishing. https://doi.org/10.3847/1538-3881/addd21
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.” The Astronomical Journal.
IOP Publishing, 2025. https://doi.org/10.3847/1538-3881/addd21.
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,” The Astronomical Journal, 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.” The Astronomical Journal, vol. 170, no. 1, 47, IOP Publishing,
2025, doi:10.3847/1538-3881/addd21.
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. Proceedings of the National Academy of Sciences. 2025;122(25).
doi:10.1073/pnas.2319927121
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. Proceedings of the National Academy of Sciences. National Academy
of Sciences. https://doi.org/10.1073/pnas.2319927121
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.” Proceedings of the National
Academy of Sciences. National Academy of Sciences, 2025. https://doi.org/10.1073/pnas.2319927121.
ieee: A. Mcavoy et al., “Unilateral incentive alignment in two-agent stochastic
games,” Proceedings of the National Academy of Sciences, 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.” Proceedings of the National Academy of Sciences, vol. 122, no.
25, e2319927121, National Academy of Sciences, 2025, doi:10.1073/pnas.2319927121.
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. New Journal of Physics. 2025;27(6).
doi:10.1088/1367-2630/ade61b
apa: Jouveshomme, S., Lizée, M., Robin, P., & Bocquet, L. (2025). Multiple ionic
memories in asymmetric nanochannels revealed by mem-spectrometry. New Journal
of Physics. IOP Publishing. https://doi.org/10.1088/1367-2630/ade61b
chicago: Jouveshomme, Simon, Mathieu Lizée, Paul Robin, and Lydéric Bocquet. “Multiple
Ionic Memories in Asymmetric Nanochannels Revealed by Mem-Spectrometry.” New
Journal of Physics. IOP Publishing, 2025. https://doi.org/10.1088/1367-2630/ade61b.
ieee: S. Jouveshomme, M. Lizée, P. Robin, and L. Bocquet, “Multiple ionic memories
in asymmetric nanochannels revealed by mem-spectrometry,” New Journal of Physics,
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.” New Journal of Physics, vol. 27, no. 6,
065001, IOP Publishing, 2025, doi:10.1088/1367-2630/ade61b.
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. Astronomy & Astrophysics.
2025;698. doi:10.1051/0004-6361/202453251
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. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202453251
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.” Astronomy & Astrophysics. EDP Sciences, 2025.
https://doi.org/10.1051/0004-6361/202453251.
ieee: M. Llerena et al., “The ionizing photon production efficiency of star-forming
galaxies at z ∼ 4–10,” Astronomy & Astrophysics, 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 & Astrophysics. 698, A302.
mla: Llerena, M., et al. “The Ionizing Photon Production Efficiency of Star-Forming
Galaxies at z ∼ 4–10.” Astronomy & Astrophysics, vol. 698, A302, EDP
Sciences, 2025, doi:10.1051/0004-6361/202453251.
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 & 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'
...