---
OA_place: repository
OA_type: free access
_id: '21422'
article_processing_charge: No
author:
- first_name: Veronika
full_name: Sunko, Veronika
id: 23cb1cf6-2c7a-11ef-91a4-f72fc19f20b3
last_name: Sunko
orcid: 0000-0003-2724-3523
citation:
ama: Sunko V. Data underpinning “Magneto-optical Kerr effect in an A-type antiferromagnet.”
2026. doi:10.15479/AT-ISTA-21422
apa: Sunko, V. (2026). Data underpinning “Magneto-optical Kerr effect in an A-type
antiferromagnet.” Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-21422
chicago: Sunko, Veronika. “Data Underpinning ‘Magneto-Optical Kerr Effect in an
A-Type Antiferromagnet.’” Institute of Science and Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-21422.
ieee: V. Sunko, “Data underpinning ‘Magneto-optical Kerr effect in an A-type antiferromagnet.’”
Institute of Science and Technology Austria, 2026.
ista: Sunko V. 2026. Data underpinning ‘Magneto-optical Kerr effect in an A-type
antiferromagnet’, Institute of Science and Technology Austria, 10.15479/AT-ISTA-21422.
mla: Sunko, Veronika. Data Underpinning “Magneto-Optical Kerr Effect in an A-Type
Antiferromagnet.” Institute of Science and Technology Austria, 2026, doi:10.15479/AT-ISTA-21422.
short: V. Sunko, (2026).
corr_author: '1'
date_created: 2026-03-11T07:04:26Z
date_published: 2026-03-11T00:00:00Z
date_updated: 2026-03-11T13:01:48Z
day: '11'
department:
- _id: VeSu
doi: 10.15479/AT-ISTA-21422
file:
- access_level: open_access
checksum: 54db0b68f0cf919009317fd3da8f733b
content_type: application/zip
creator: vsunko
date_created: 2026-03-11T10:28:34Z
date_updated: 2026-03-11T10:28:34Z
file_id: '21429'
file_name: MBT_Data_Paper.zip
file_size: 85004
relation: main_file
success: 1
- access_level: open_access
checksum: df1785b7ada7cd07f76a441ee4f52266
content_type: text/plain
creator: vsunko
date_created: 2026-03-11T10:28:37Z
date_updated: 2026-03-11T10:28:37Z
file_id: '21430'
file_name: README.txt
file_size: 2593
relation: main_file
success: 1
file_date_updated: 2026-03-11T10:28:37Z
has_accepted_license: '1'
month: '03'
oa: 1
oa_version: None
publisher: Institute of Science and Technology Austria
status: public
title: Data underpinning "Magneto-optical Kerr effect in an A-type antiferromagnet"
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: research_data
user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d
year: '2026'
...
---
_id: '21442'
author:
- first_name: Alois
full_name: Schlögl, Alois
id: 45BF87EE-F248-11E8-B48F-1D18A9856A87
last_name: Schlögl
orcid: 0000-0002-5621-8100
citation:
ama: Schlögl A. CA3Simu v1.06 (vargas2026v1). 2026. doi:10.15479/AT-ISTA-21442
apa: Schlögl, A. (2026). CA3Simu v1.06 (vargas2026v1). Institute of Science and
Technology Austria. https://doi.org/10.15479/AT-ISTA-21442
chicago: Schlögl, Alois. “CA3Simu v1.06 (Vargas2026v1).” Institute of Science and
Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-21442.
ieee: A. Schlögl, “CA3Simu v1.06 (vargas2026v1).” Institute of Science and Technology
Austria, 2026.
ista: Schlögl A. 2026. CA3Simu v1.06 (vargas2026v1), Institute of Science and Technology
Austria, 10.15479/AT-ISTA-21442.
mla: Schlögl, Alois. CA3Simu v1.06 (Vargas2026v1). Institute of Science and
Technology Austria, 2026, doi:10.15479/AT-ISTA-21442.
short: A. Schlögl, (2026).
corr_author: '1'
date_created: 2026-03-12T08:20:46Z
date_published: 2026-03-12T00:00:00Z
date_updated: 2026-03-12T11:28:52Z
day: '12'
department:
- _id: ScienComp
- _id: PeJo
doi: 10.15479/AT-ISTA-21442
ec_funded: 1
file:
- access_level: open_access
checksum: 441c8827717dcda05f91c127d15cf1e9
content_type: application/gzip
creator: schloegl
date_created: 2026-03-12T08:19:14Z
date_updated: 2026-03-12T08:19:14Z
file_id: '21443'
file_name: ca3simu-vargas2026v1.tar.gz
file_size: 160410
relation: main_file
success: 1
- access_level: open_access
checksum: 3c0092076228a15c0a7ae703192d43ea
content_type: text/markdown
creator: schloegl
date_created: 2026-03-12T10:24:45Z
date_updated: 2026-03-12T10:24:45Z
file_id: '21445'
file_name: README.md
file_size: 10923
relation: main_file
success: 1
file_date_updated: 2026-03-12T10:24:45Z
has_accepted_license: '1'
keyword:
- hypocampus
- ca3 simulations
- modelling
license: https://opensource.org/licenses/GPL-3.0
month: '03'
oa: 1
project:
- _id: e62b56fe-ab3c-11f0-94c7-d181dd352b3b
grant_number: '101199096'
name: Synaptic mechanisms of engram storage and retrieval in CA3 hippocampal microcircuits
- _id: bd88be38-d553-11ed-ba76-81d5a70a6ef5
grant_number: P36232
name: Mechanisms of GABA release in hippocampal circuits
- _id: 8d9195e9-16d5-11f0-9cad-d075be887a1e
grant_number: PAT 4178023
name: Synaptic networks of human brain
- _id: 25B7EB9E-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '692692'
name: Biophysics and circuit function of a giant cortical glutamatergic synapse
publisher: Institute of Science and Technology Austria
status: public
title: CA3Simu v1.06 (vargas2026v1)
tmp:
legal_code_url: https://www.gnu.org/licenses/gpl-3.0.en.html
name: GNU General Public License 3.0
short: GPL 3.0
type: software
user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d
year: '2026'
...
---
OA_place: repository
_id: '21401'
abstract:
- lang: eng
text: "Runtime verification offers scalable solutions to improve the safety and
reliability of systems. However, systems that require verification or monitoring
by a third party to ensure compliance with a specification might contain sensitive
information, causing privacy concerns when usual runtime verification approaches
are used. Privacy is compromised if protected information about the system, or
sensitive data that is processed by the system, is revealed. In addition, revealing
the specification being monitored may undermine the essence of third-party verification.\r\n\r\nIn
this thesis, we propose a protocol for privacy-preserving runtime verification
of systems against formal sequential specifications. We develop the protocol in
two steps. In the first step, the monitor verifies whether the system satisfies
the specification without learning anything else, though both parties are aware
of the specification. In the second step, we extend the protocol to ensure that
the system remains oblivious to the monitored specification, while the monitor
learns only whether the system satisfies the specification and nothing more. Our
protocol adapts and improves existing techniques used in cryptography, and more
specifically, multi-party computation.\r\n\r\nThe sequential specification defines
the observation step of the monitor, whose granularity depends on the situation
(e.g., banks may be monitored on a daily basis). Our protocol exchanges a single
message per observation step, after an initialization phase. This design minimizes
communication overhead, enabling relatively lightweight privacy-preserving monitoring.
We implement our approach for monitoring specifications described by register
automata and evaluate it experimentally.\r\n"
acknowledgement: "This work is part of the project VAMOS, which has received funding
from the European\r\nResearch Council (ERC) under grant agreement No. 101020093,
and the Austrian Science\r\nFund (FWF) SFB project SpyCoDe F8502.\r\n"
alternative_title:
- ISTA Master’s Thesis
article_processing_charge: No
author:
- first_name: Mahyar
full_name: Karimi, Mahyar
id: 6e5417ba-5355-11ee-ae5a-94c2e510b26b
last_name: Karimi
orcid: 0009-0005-0820-1696
citation:
ama: Karimi M. Privacy-preserving runtime verification. 2026. doi:10.15479/AT-ISTA-21401
apa: Karimi, M. (2026). Privacy-preserving runtime verification. Institute
of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-21401
chicago: Karimi, Mahyar. “Privacy-Preserving Runtime Verification.” Institute of
Science and Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-21401.
ieee: M. Karimi, “Privacy-preserving runtime verification,” Institute of Science
and Technology Austria, 2026.
ista: Karimi M. 2026. Privacy-preserving runtime verification. Institute of Science
and Technology Austria.
mla: Karimi, Mahyar. Privacy-Preserving Runtime Verification. Institute of
Science and Technology Austria, 2026, doi:10.15479/AT-ISTA-21401.
short: M. Karimi, Privacy-Preserving Runtime Verification, Institute of Science
and Technology Austria, 2026.
corr_author: '1'
date_created: 2026-03-05T15:20:47Z
date_published: 2026-03-05T00:00:00Z
date_updated: 2026-03-13T13:37:20Z
day: '05'
ddc:
- '000'
degree_awarded: MS
department:
- _id: GradSch
- _id: ToHe
doi: 10.15479/AT-ISTA-21401
ec_funded: 1
file:
- access_level: open_access
checksum: 3f49f05c9d123e14d7adb73d3bc50fe2
content_type: application/pdf
creator: mkarimi
date_created: 2026-03-06T14:06:25Z
date_updated: 2026-03-10T15:20:09Z
file_id: '21404'
file_name: 2026_Karimi_Mahyar_Thesis.pdf
file_size: 766048
relation: main_file
- access_level: closed
checksum: 8fb9db4b4187e26443369a993427a5ff
content_type: application/zip
creator: mkarimi
date_created: 2026-03-06T14:06:25Z
date_updated: 2026-03-06T14:06:25Z
file_id: '21405'
file_name: 2026_Karimi_Mahyar_Thesis_src.zip
file_size: 1243394
relation: source_file
file_date_updated: 2026-03-10T15:20:09Z
has_accepted_license: '1'
keyword:
- Privacy-preserving verification
- Runtime verification
- Monitoring
- Reactive functionalities
- Cryptographic protocols
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
page: '60'
project:
- _id: 62781420-2b32-11ec-9570-8d9b63373d4d
call_identifier: H2020
grant_number: '101020093'
name: Vigilant Algorithmic Monitoring of Software
- _id: 34a4ce89-11ca-11ed-8bc3-8cc37fb6e11f
grant_number: F8512
name: Security and Privacy by Design for Complex Systems
publication_identifier:
issn:
- 2791-4585
publication_status: published
publisher: Institute of Science and Technology Austria
related_material:
record:
- id: '21020'
relation: part_of_dissertation
status: public
status: public
supervisor:
- first_name: Thomas A
full_name: Henzinger, Thomas A
id: 40876CD8-F248-11E8-B48F-1D18A9856A87
last_name: Henzinger
orcid: 0000-0002-2985-7724
title: Privacy-preserving runtime verification
type: dissertation
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
year: '2026'
...
---
OA_place: repository
OA_type: green
_id: '21438'
abstract:
- lang: eng
text: Antiferromagnets (AFMs) hold promise for applications in digital logic. However,
switching AFM domains is challenging, as magnetic fields do not couple to the
bulk antiferromagnetic order parameter. Here we show that magnetic-field-driven
switching of AFM domains can in many cases be enabled by a generic reduction of
magnetic exchange at surfaces. We use statistical mechanics and Monte Carlo simulations
to demonstrate that an inequivalence in magnetic exchange between top and bottom
surface moments, combined with the enhanced magnetic susceptibility of surface
spins, can enable deterministic selection of antiferromagnetic domains depending
on the magnetic-field ramping direction. We further show that this mechanism provides
a natural interpretation for experimental observations of hysteresis in magneto-optical
response of the van der Waals AFM $\mathrm{MnBi_2Te_4}$. Our findings highlight
the critical role of surface spins in responses of antiferromagnets to magnetic
fields. Furthermore, our results suggest that antiferromagnetic domain selection
via purely magnetic means may be a more common and experimentally accessible phenomenon
than previously assumed.
acknowledgement: SFW acknowledges funding from Chalmers University of Technology through
the department of Physics and the Areas of Advance Nano and Materials Science. VS
acknowledges funding from Institute of Science and Technology Austria. Monte Carlo
simulations were performed using computing resources from the PDC Center for High
Performance Computing. These resources were granted by the National Academic Infrastructure
for Supercomputing in Sweden (NAISS), partially funded by the Swedish Research Council
through grant agreement no. 2022-06725.
article_number: '2601.06646'
article_processing_charge: No
arxiv: 1
author:
- first_name: Sophie F.
full_name: Weber, Sophie F.
last_name: Weber
- first_name: Veronika
full_name: Sunko, Veronika
id: 23cb1cf6-2c7a-11ef-91a4-f72fc19f20b3
last_name: Sunko
orcid: 0000-0003-2724-3523
citation:
ama: Weber SF, Sunko V. Deterministic domain selection of antiferromagnets via magnetic
fields. arXiv. doi:10.48550/arXiv.2601.06646
apa: Weber, S. F., & Sunko, V. (n.d.). Deterministic domain selection of antiferromagnets
via magnetic fields. arXiv. https://doi.org/10.48550/arXiv.2601.06646
chicago: Weber, Sophie F., and Veronika Sunko. “Deterministic Domain Selection of
Antiferromagnets via Magnetic Fields.” ArXiv, n.d. https://doi.org/10.48550/arXiv.2601.06646.
ieee: S. F. Weber and V. Sunko, “Deterministic domain selection of antiferromagnets
via magnetic fields,” arXiv. .
ista: Weber SF, Sunko V. Deterministic domain selection of antiferromagnets via
magnetic fields. arXiv, 2601.06646.
mla: Weber, Sophie F., and Veronika Sunko. “Deterministic Domain Selection of Antiferromagnets
via Magnetic Fields.” ArXiv, 2601.06646, doi:10.48550/arXiv.2601.06646.
short: S.F. Weber, V. Sunko, ArXiv (n.d.).
date_created: 2026-03-11T10:40:20Z
date_published: 2026-01-10T00:00:00Z
date_updated: 2026-03-16T08:57:18Z
day: '10'
department:
- _id: VeSu
doi: 10.48550/arXiv.2601.06646
external_id:
arxiv:
- '2601.06646'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2601.06646
month: '01'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
status: public
title: Deterministic domain selection of antiferromagnets via magnetic fields
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '21451'
abstract:
- lang: eng
text: The population of the little red dots (LRDs) may represent a key phase of
supermassive black hole (SMBH) growth. A cocoon of dense excited gas is emerging
as a key component to explain the most striking properties of LRDs, such as strong
Balmer breaks and Balmer absorption, as well as the weak IR emission. To dissect
the structure of LRDs, we analyzed new deep JWST/NIRSpec PRISM and G395H spectra
of FRESCO-GN-9771, one of the most luminous known LRDs at z = 5.5. These spectra
reveal a strong Balmer break, broad Balmer lines, and very narrow [O III] emission.
We revealed a forest of optical [Fe II] lines, which we argue are emerging from
a dense (nH = 109 − 10 cm−3) warm layer with electron temperature Te ≈ 7000 K.
The broad wings of Hα and Hβ have an exponential profile due to electron scattering
in this same layer. The high Hα : Hβ : Hγ flux ratio of ≈10.4 : 1 : 0.14 is an
indicator of collisional excitation and resonant scattering dominating the Balmer
line emission. A narrow Hγ component, unseen in the other two Balmer lines due
to outshining by the broad components, could trace the ISM of a normal host galaxy
with a star formation rate of ∼5 M⊙ yr−1. The warm layer is mostly opaque to Balmer
transitions, producing a characteristic P Cygni profile in the line centers suggesting
outflowing motions. This same layer is responsible for shaping the Balmer break.
The broadband spectrum can be reasonably matched by a simple photoionized slab
model that dominates the λ > 1500 Å continuum and a low-mass (∼108 M⊙) galaxy
that could explain the narrow [O III], with only a subdominant contribution to
the UV continuum. Our findings indicate that Balmer lines are not directly tracing
the gas kinematics near the SMBH and that the BH mass scale is likely much lower
than virial indicators suggest.
acknowledgement: 'We thank the scientific referee for useful and constructive comments.
We thank Ylva Götberg and Zoltan Haiman for insightful discussions about the physics
of gaseous envelopes and accretion into black holes. Funded by the European Union
(ERC, AGENTS, 101076224). Views and opinions expressed are however those of the
author(s) only and do not necessarily reflect those of the European Union or the
European Research Council. Neither the European Union nor the granting authority
can be held responsible for them. This work is based in part on observations made
with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the
Mikulski Archive for Space Telescopes at the Space Telescope Science Institute,
which is operated by the Association of Universities for Research in Astronomy,
Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated
with program #5664. This work has received funding from the Swiss State Secretariat
for Education, Research and Innovation (SERI) under contract number MB22.00072,
as well as from the Swiss National Science Foundation (SNSF) through project grant
200020_207349.'
article_number: A75
article_processing_charge: No
article_type: original
arxiv: 1
author:
- 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: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Gabriele
full_name: Pezzulli, Gabriele
last_name: Pezzulli
- first_name: Rohan P.
full_name: Naidu, Rohan P.
last_name: Naidu
- first_name: Yuzo
full_name: Ishikawa, Yuzo
last_name: Ishikawa
- first_name: Gabriel B.
full_name: Brammer, Gabriel B.
last_name: Brammer
- first_name: Seok Jun
full_name: Chang, Seok Jun
last_name: Chang
- first_name: John
full_name: Chisholm, John
last_name: Chisholm
- first_name: Anna
full_name: De Graaff, Anna
last_name: De Graaff
- first_name: Francesco
full_name: D’Eugenio, Francesco
last_name: D’Eugenio
- first_name: Claudia
full_name: Di Cesare, Claudia
id: 2d002343-372f-11ef-98ec-a164d20427cb
last_name: Di Cesare
- first_name: Anna Christina
full_name: Eilers, Anna Christina
last_name: Eilers
- first_name: Jenny E.
full_name: Greene, Jenny E.
last_name: Greene
- first_name: Max
full_name: Gronke, Max
last_name: Gronke
- first_name: Edoardo
full_name: Iani, Edoardo
id: 4053390a-6b68-11ef-9828-a3b8adef8d0a
last_name: Iani
orcid: 0000-0001-8386-3546
- first_name: Vasily
full_name: Kokorev, Vasily
last_name: Kokorev
- first_name: Gauri
full_name: Kotiwale, Gauri
id: 1438afc8-1ff6-11ee-9fa6-cd4a75d66875
last_name: Kotiwale
- first_name: Ivan
full_name: Kramarenko, Ivan
id: 9a9394cb-3200-11ee-973b-f5ba2a8b16e4
last_name: Kramarenko
orcid: 0000-0001-5346-6048
- first_name: Yilun
full_name: Ma, Yilun
last_name: Ma
- first_name: Sara
full_name: Mascia, Sara
id: edaf889c-c7cd-11ef-ab1b-bb28c431bd29
last_name: Mascia
- first_name: Benjamín
full_name: Navarrete, Benjamín
id: aa14a535-50c9-11ef-b52e-e0c373d10148
last_name: Navarrete
- first_name: Erica
full_name: Nelson, Erica
last_name: Nelson
- first_name: Pascal
full_name: Oesch, Pascal
last_name: Oesch
- first_name: Robert A.
full_name: Simcoe, Robert A.
last_name: Simcoe
- first_name: Stijn
full_name: Wuyts, Stijn
last_name: Wuyts
citation:
ama: Torralba Torregrosa A, Matthee JJ, Pezzulli G, et al. The warm outer layer
of a little red dot as the source of [Fe ii] and collisional Balmer lines with
scattering wings. Astronomy & Astrophysics. 2026;707. doi:10.1051/0004-6361/202557537
apa: Torralba Torregrosa, A., Matthee, J. J., Pezzulli, G., Naidu, R. P., Ishikawa,
Y., Brammer, G. B., … Wuyts, S. (2026). The warm outer layer of a little red dot
as the source of [Fe ii] and collisional Balmer lines with scattering wings. Astronomy
& Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202557537
chicago: Torralba Torregrosa, Alberto, Jorryt J Matthee, Gabriele Pezzulli, Rohan
P. Naidu, Yuzo Ishikawa, Gabriel B. Brammer, Seok Jun Chang, et al. “The Warm
Outer Layer of a Little Red Dot as the Source of [Fe Ii] and Collisional Balmer
Lines with Scattering Wings.” Astronomy & Astrophysics. EDP Sciences,
2026. https://doi.org/10.1051/0004-6361/202557537.
ieee: A. Torralba Torregrosa et al., “The warm outer layer of a little red
dot as the source of [Fe ii] and collisional Balmer lines with scattering wings,”
Astronomy & Astrophysics, vol. 707. EDP Sciences, 2026.
ista: Torralba Torregrosa A, Matthee JJ, Pezzulli G, Naidu RP, Ishikawa Y, Brammer
GB, Chang SJ, Chisholm J, De Graaff A, D’Eugenio F, Di Cesare C, Eilers AC, Greene
JE, Gronke M, Iani E, Kokorev V, Kotiwale G, Kramarenko I, Ma Y, Mascia S, Navarrete
B, Nelson E, Oesch P, Simcoe RA, Wuyts S. 2026. The warm outer layer of a little
red dot as the source of [Fe ii] and collisional Balmer lines with scattering
wings. Astronomy & Astrophysics. 707, A75.
mla: Torralba Torregrosa, Alberto, et al. “The Warm Outer Layer of a Little Red
Dot as the Source of [Fe Ii] and Collisional Balmer Lines with Scattering Wings.”
Astronomy & Astrophysics, vol. 707, A75, EDP Sciences, 2026, doi:10.1051/0004-6361/202557537.
short: A. Torralba Torregrosa, J.J. Matthee, G. Pezzulli, R.P. Naidu, Y. Ishikawa,
G.B. Brammer, S.J. Chang, J. Chisholm, A. De Graaff, F. D’Eugenio, C. Di Cesare,
A.C. Eilers, J.E. Greene, M. Gronke, E. Iani, V. Kokorev, G. Kotiwale, I. Kramarenko,
Y. Ma, S. Mascia, B. Navarrete, E. Nelson, P. Oesch, R.A. Simcoe, S. Wuyts, Astronomy
& Astrophysics 707 (2026).
corr_author: '1'
date_created: 2026-03-15T23:01:36Z
date_published: 2026-03-01T00:00:00Z
date_updated: 2026-03-16T10:59:16Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202557537
external_id:
arxiv:
- '2510.00103'
file:
- access_level: open_access
checksum: fcab9cb3dcf1d68612e1fdc8191643c1
content_type: application/pdf
creator: dernst
date_created: 2026-03-16T10:57:49Z
date_updated: 2026-03-16T10:57:49Z
file_id: '21460'
file_name: 2026_AstronomyAstrophysics_Torralba2.pdf
file_size: 2510157
relation: main_file
success: 1
file_date_updated: 2026-03-16T10:57:49Z
has_accepted_license: '1'
intvolume: ' 707'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
grant_number: '101076224'
name: Young galaxies as tracers and agents of cosmic reionization
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: The warm outer layer of a little red dot as the source of [Fe ii] and collisional
Balmer lines with scattering wings
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: 707
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '21452'
abstract:
- lang: eng
text: Galaxies exhibit a tight correlation between their star formation rate (SFR)
and stellar mass over a wide redshift range known as the star-forming main sequence
(SFMS). With JWST, the SFMS can now be investigated at high redshifts down to
masses of ∼106 M⊙, using sensitive star formation rate tracers such as the Hα
emission, which allow us to probe the variability in the star formation histories.
We present inferences of the SFMS based on 316 Hα-selected galaxies at z ∼ 4 − 5
with log(M★/M⊙) = 6.4 − 10.6. These galaxies were identified behind the Abell
2744 lensing cluster with NIRCam grism spectroscopy from the survey All the Little
Things (ALT). At face value, our data suggest a shallow slope in the SFMS (SFR ∝ M★α,
with α = 0.45). After we corrected this for the Hα-flux limited nature of our
survey using a Bayesian framework, the slope steepened to α = 0.59+0.10−0.09,
whereas current data on their own are inconclusive on the mass dependence of the
scatter. These slopes differ significantly from the slope of ∼1 that is expected
from the observed evolution of the galaxy stellar mass function and from simulations.
When we fixed the slope to α = 1, we found evidence for a decreasing intrinsic
scatter with stellar mass (from ∼0.5 dex at M★ = 108 M⊙ to 0.4 dex at M★ = 1010
M⊙). This difference might be explained by a (combination of) luminosity-dependent
SFR(Hα) calibration, a population of (mini)-quenched low-mass galaxies, or underestimated
dust attenuation in high-mass galaxies. Future deep observations with different
facilities can quantify these processes, which will enable us to achieve better
insights into the variability of the star formation histories.
acknowledgement: "We thank the anonymous referee for the insightful comments that
helped improving the manuscript. We thank Romain. A. Meyer for valuable discussion,
Pierluigi Rinaldi for his help with data handling and Luca Graziani and William
McClymont for providing the dustyGadget and\r\nTHESAN-ZOOM data, respectively. Funded
by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed are
however those of the author(s) only and do not necessarily reflect those of the
European Union or the European Research Council. Neither the European Union nor
the granting authority can be held responsible for them. This work is based on observations
made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from
the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute,
which is operated by the Association of Universities for Research in Astronomy,
Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated
with program # 3516. We acknowledge funding from JWST program GO-3516. Software
used in developing this work includes: matplotlib (Hunter 2007), numpy (Oliphant
2007), scipy (Virtanen et al. 2020), TOPCAT (Taylor 2005), and Astropy (Astropy
Collaboration 2013)."
article_number: A129
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Claudia
full_name: Di Cesare, Claudia
id: 2d002343-372f-11ef-98ec-a164d20427cb
last_name: Di Cesare
- 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: Alberto
full_name: Torralba, Alberto
last_name: Torralba
- first_name: Gauri
full_name: Kotiwale, Gauri
id: 1438afc8-1ff6-11ee-9fa6-cd4a75d66875
last_name: Kotiwale
- first_name: Ivan
full_name: Kramarenko, Ivan
id: 9a9394cb-3200-11ee-973b-f5ba2a8b16e4
last_name: Kramarenko
orcid: 0000-0001-5346-6048
- first_name: Jeremy
full_name: Blaizot, Jeremy
last_name: Blaizot
- first_name: Joakim
full_name: Rosdahl, Joakim
last_name: Rosdahl
- first_name: Joel
full_name: Leja, Joel
last_name: Leja
- first_name: Edoardo
full_name: Iani, Edoardo
id: 4053390a-6b68-11ef-9828-a3b8adef8d0a
last_name: Iani
orcid: 0000-0001-8386-3546
- first_name: Angela
full_name: Adamo, Angela
last_name: Adamo
- first_name: Alba
full_name: Covelo-Paz, Alba
last_name: Covelo-Paz
- first_name: Lukas J.
full_name: Furtak, Lukas J.
last_name: Furtak
- first_name: Kasper E.
full_name: Heintz, Kasper E.
last_name: Heintz
- first_name: Sara
full_name: Mascia, Sara
id: edaf889c-c7cd-11ef-ab1b-bb28c431bd29
last_name: Mascia
- first_name: Benjamín
full_name: Navarrete, Benjamín
id: aa14a535-50c9-11ef-b52e-e0c373d10148
last_name: Navarrete
- first_name: Pascal A.
full_name: Oesch, Pascal A.
last_name: Oesch
- first_name: Michael
full_name: Romano, Michael
last_name: Romano
- first_name: Irene
full_name: Shivaei, Irene
last_name: Shivaei
- first_name: Sandro
full_name: Tacchella, Sandro
last_name: Tacchella
citation:
ama: 'Di Cesare C, Matthee JJ, Naidu RP, et al. The slope and scatter of the star-forming
main sequence at z ∼ 5: Reconciling observations with simulations. Astronomy
& Astrophysics. 2026;707. doi:10.1051/0004-6361/202557790'
apa: 'Di Cesare, C., Matthee, J. J., Naidu, R. P., Torralba, A., Kotiwale, G., Kramarenko,
I., … Tacchella, S. (2026). The slope and scatter of the star-forming main sequence
at z ∼ 5: Reconciling observations with simulations. Astronomy & Astrophysics.
EDP Sciences. https://doi.org/10.1051/0004-6361/202557790'
chicago: 'Di Cesare, Claudia, Jorryt J Matthee, Rohan P. Naidu, Alberto Torralba,
Gauri Kotiwale, Ivan Kramarenko, Jeremy Blaizot, et al. “The Slope and Scatter
of the Star-Forming Main Sequence at z ∼ 5: Reconciling Observations with Simulations.”
Astronomy & Astrophysics. EDP Sciences, 2026. https://doi.org/10.1051/0004-6361/202557790.'
ieee: 'C. Di Cesare et al., “The slope and scatter of the star-forming main
sequence at z ∼ 5: Reconciling observations with simulations,” Astronomy &
Astrophysics, vol. 707. EDP Sciences, 2026.'
ista: 'Di Cesare C, Matthee JJ, Naidu RP, Torralba A, Kotiwale G, Kramarenko I,
Blaizot J, Rosdahl J, Leja J, Iani E, Adamo A, Covelo-Paz A, Furtak LJ, Heintz
KE, Mascia S, Navarrete B, Oesch PA, Romano M, Shivaei I, Tacchella S. 2026. The
slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling observations
with simulations. Astronomy & Astrophysics. 707, A129.'
mla: 'Di Cesare, Claudia, et al. “The Slope and Scatter of the Star-Forming Main
Sequence at z ∼ 5: Reconciling Observations with Simulations.” Astronomy &
Astrophysics, vol. 707, A129, EDP Sciences, 2026, doi:10.1051/0004-6361/202557790.'
short: C. Di Cesare, J.J. Matthee, R.P. Naidu, A. Torralba, G. Kotiwale, I. Kramarenko,
J. Blaizot, J. Rosdahl, J. Leja, E. Iani, A. Adamo, A. Covelo-Paz, L.J. Furtak,
K.E. Heintz, S. Mascia, B. Navarrete, P.A. Oesch, M. Romano, I. Shivaei, S. Tacchella,
Astronomy & Astrophysics 707 (2026).
corr_author: '1'
date_created: 2026-03-15T23:01:36Z
date_published: 2026-03-01T00:00:00Z
date_updated: 2026-03-16T10:52:44Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
- _id: GradSch
doi: 10.1051/0004-6361/202557790
external_id:
arxiv:
- '2510.19044'
file:
- access_level: open_access
checksum: c056b00ce7324849754521fde10fb7ca
content_type: application/pdf
creator: dernst
date_created: 2026-03-16T10:48:07Z
date_updated: 2026-03-16T10:48:07Z
file_id: '21459'
file_name: 2026_AstronomyAstrophysics_DiCesare.pdf
file_size: 1821411
relation: main_file
success: 1
file_date_updated: 2026-03-16T10:48:07Z
has_accepted_license: '1'
intvolume: ' 707'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
grant_number: '101076224'
name: Young galaxies as tracers and agents of cosmic reionization
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling
observations with simulations'
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: 707
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '21450'
abstract:
- lang: eng
text: Stellar wind mass loss of massive stars is often assumed to depend on their
metallicity Z. Therefore, evolutionary models predict that massive stars in lower-Z
environments are able to retain more of their hydrogen-rich layers and evolve
into brighter cool supergiants (cool SGs; Teff < 7 kK). Surprisingly, in galaxies
in the metallicity range 0.2 ≲ Z/Z⊙ ≲ 1.5, previous studies have not found a metallicity
dependence on the upper luminosity limit Lmax of cool SGs. Here, we add four galaxies
to the sample studied for this purpose with data from the Hubble Space Telescope
and the James Webb Space Telescope (JWST). Observations of the extremely metal-poor
dwarf galaxy I Zw 18 from JWST allow us to extend the studied metallicity range
down to Z/Z⊙ ≈ 1/40. For cool SGs in all studied galaxies, including I Zw 18,
we find a constant value of Lmax ≈ 105.6 L⊙, similar to literature results for
0.2 ≲ Z/Z⊙ ≲ 1.5. In I Zw 18 and the other studied galaxies, the presence of Wolf-Rayet
stars has been previously inferred. Although we cannot rule out that some of them
become intermediate-temperature objects, this paints a picture in which evolved
stars with L > 105.6 L⊙ burn helium as hot, helium-rich stars down to extremely
low metallicity. We argue that metallicity-independent late-phase mass loss would
be the most likely mechanism responsible for this. Regardless of the exact stripping
mechanism (winds or, for example, binary interaction), for the Early Universe
our results imply a limitation on black hole masses and a contribution of stars
born with M ≳ 30 M⊙ to its surprisingly strong nitrogen enrichment. We propose
a scenario in which single stars at low metallicity emit sufficiently hard ionizing
radiation to produce He II and C IV lines. In this scenario, late-phase metallicity-independent
mass loss produces hot, helium-rich stars. Due to the well-understood metallicity
dependence on the radiation-driven winds of hot stars, a window of opportunity
would open below 0.2 Z⊙, where self-stripped helium-rich stars can exist without
dense Wolf-Rayet winds that absorb hard ionizing radiation.
acknowledgement: "We thank our anonymous referee for carefully reading the manuscript
and providing a constructive report with helpful feedback. This work is based in
part on observations made with the NASA/ESA/CSA James Webb Space Telescope. The
data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope
Science Institute, which is operated by the Association of Universities for Research
in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations
are associated with program #1233. The specific observations analyzed can be accessed
via DOI: 10.17909/3c1d-6182. Moreover, this research is based in part on observations
made with the NASA/ESA Hubble Space Telescope obtained from the\r\nSpace Telescope
Science Institute, which is operated by the Association of Universities for Research
in Astronomy, Inc., under NASA contract NAS 5–26555. These observations are associated
with programs #13664, GO-10915, and DD-11307. This research was supported in part
by grant NSF PHY-2309135 to the Kavli Institute for Theoretical Physics (KITP).
LRP acknowledges support by grants PID2019-105552RB-C41 and PID2022-137779OB-C41
funded\r\nby MCIN/AEI/10.13039/501100011033 by “ERDF A way of making Europe”. LRP
acknowledges support from grant PID2022-140483NB-C22 funded by MCIN/AEI/10.13039/501100011033."
article_number: A116
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Abel
full_name: Schootemeijer, Abel
last_name: Schootemeijer
- first_name: Ylva Louise Linsdotter
full_name: Götberg, Ylva Louise Linsdotter
id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
last_name: Götberg
orcid: 0000-0002-6960-6911
- first_name: Norbert
full_name: Langer, Norbert
last_name: Langer
- first_name: Giacomo
full_name: Bortolini, Giacomo
last_name: Bortolini
- first_name: Alec S.
full_name: Hirschauer, Alec S.
last_name: Hirschauer
- first_name: Lee
full_name: Patrick, Lee
last_name: Patrick
citation:
ama: Schootemeijer A, Götberg YLL, Langer N, Bortolini G, Hirschauer AS, Patrick
L. A constant upper luminosity limit of cool supergiant stars down to the extremely
low metallicity of I Zw 18. Astronomy & Astrophysics. 2026;707. doi:10.1051/0004-6361/202557675
apa: Schootemeijer, A., Götberg, Y. L. L., Langer, N., Bortolini, G., Hirschauer,
A. S., & Patrick, L. (2026). A constant upper luminosity limit of cool supergiant
stars down to the extremely low metallicity of I Zw 18. Astronomy & Astrophysics.
EDP Sciences. https://doi.org/10.1051/0004-6361/202557675
chicago: Schootemeijer, Abel, Ylva Louise Linsdotter Götberg, Norbert Langer, Giacomo
Bortolini, Alec S. Hirschauer, and Lee Patrick. “A Constant Upper Luminosity Limit
of Cool Supergiant Stars down to the Extremely Low Metallicity of I Zw 18.” Astronomy
& Astrophysics. EDP Sciences, 2026. https://doi.org/10.1051/0004-6361/202557675.
ieee: A. Schootemeijer, Y. L. L. Götberg, N. Langer, G. Bortolini, A. S. Hirschauer,
and L. Patrick, “A constant upper luminosity limit of cool supergiant stars down
to the extremely low metallicity of I Zw 18,” Astronomy & Astrophysics,
vol. 707. EDP Sciences, 2026.
ista: Schootemeijer A, Götberg YLL, Langer N, Bortolini G, Hirschauer AS, Patrick
L. 2026. A constant upper luminosity limit of cool supergiant stars down to the
extremely low metallicity of I Zw 18. Astronomy & Astrophysics. 707, A116.
mla: Schootemeijer, Abel, et al. “A Constant Upper Luminosity Limit of Cool Supergiant
Stars down to the Extremely Low Metallicity of I Zw 18.” Astronomy & Astrophysics,
vol. 707, A116, EDP Sciences, 2026, doi:10.1051/0004-6361/202557675.
short: A. Schootemeijer, Y.L.L. Götberg, N. Langer, G. Bortolini, A.S. Hirschauer,
L. Patrick, Astronomy & Astrophysics 707 (2026).
date_created: 2026-03-15T23:01:35Z
date_published: 2026-03-01T00:00:00Z
date_updated: 2026-03-16T09:07:55Z
day: '01'
ddc:
- '520'
department:
- _id: YlGo
doi: 10.1051/0004-6361/202557675
external_id:
arxiv:
- '2510.12594'
file:
- access_level: open_access
checksum: 02a0cd932340207c96fdd3059490ad29
content_type: application/pdf
creator: dernst
date_created: 2026-03-16T09:05:06Z
date_updated: 2026-03-16T09:05:06Z
file_id: '21455'
file_name: 2026_AstronomyAstrophysics_Schootemeijer.pdf
file_size: 2102107
relation: main_file
success: 1
file_date_updated: 2026-03-16T09:05:06Z
has_accepted_license: '1'
intvolume: ' 707'
language:
- iso: eng
month: '03'
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: A constant upper luminosity limit of cool supergiant stars down to the extremely
low metallicity of I Zw 18
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: 707
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '20840'
abstract:
- lang: eng
text: Probing the possibility of entanglement generation through gravity offers
a path to tackle the question of whether gravitational fields possess a quantum
mechanical nature. A potential realization necessitates systems with low-frequency
dynamics at an optimal mass scale, for which the microgram-to-milligram range
is a strong contender. Here, after refining a figure-of-merit for the problem,
we present a 1-milligram torsional pendulum operating at 18 Hz. We demonstrate
laser cooling its motion from room temperature to 240 microkelvins, surpassing
by over 20-fold the coldest motions attained for oscillators ranging from micrograms
to kilograms. We quantify and contrast the utility of the current approach with
other platforms. The achieved performance and large improvement potential highlight
milligram-scale torsional pendulums as a powerful platform for precision measurements
relevant to future studies at the quantum-gravity interface.
acknowledgement: We thank Gerard Higgins, Andrei Militaru, Nikolai Kiesel, and Markus
Aspelmeyer for useful discussions on the topic of the figure-of-merit. We thank
Teodor Strömberg for helping with the additional characterizations of the optical
lever noise. We thank Johannes Fink and Scott Waitukaitis for their helpful feedback
on the manuscript. This work was supported by Institute of Science and Technology
Austria and the European Research Council under Grant No. 101087907 (ERC CoG QuHAMP).
article_number: '80'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Sofya
full_name: Agafonova, Sofya
id: 09501ff6-dca7-11ea-a8ae-b3e0b9166e80
last_name: Agafonova
orcid: 0000-0003-0582-2946
- first_name: Pere
full_name: Rosello, Pere
last_name: Rosello
- first_name: Manuel
full_name: Mekonnen, Manuel
last_name: Mekonnen
- first_name: Onur
full_name: Hosten, Onur
id: 4C02D85E-F248-11E8-B48F-1D18A9856A87
last_name: Hosten
orcid: 0000-0002-2031-204X
citation:
ama: Agafonova S, Rosello P, Mekonnen M, Hosten O. One-milligram torsional pendulum
toward experiments at the quantum-gravity interface. Communications Physics.
2026;9. doi:10.1038/s42005-026-02514-w
apa: Agafonova, S., Rosello, P., Mekonnen, M., & Hosten, O. (2026). One-milligram
torsional pendulum toward experiments at the quantum-gravity interface. Communications
Physics. Springer Nature. https://doi.org/10.1038/s42005-026-02514-w
chicago: Agafonova, Sofia, Pere Rosello, Manuel Mekonnen, and Onur Hosten. “One-Milligram
Torsional Pendulum toward Experiments at the Quantum-Gravity Interface.” Communications
Physics. Springer Nature, 2026. https://doi.org/10.1038/s42005-026-02514-w.
ieee: S. Agafonova, P. Rosello, M. Mekonnen, and O. Hosten, “One-milligram torsional
pendulum toward experiments at the quantum-gravity interface,” Communications
Physics, vol. 9. Springer Nature, 2026.
ista: Agafonova S, Rosello P, Mekonnen M, Hosten O. 2026. One-milligram torsional
pendulum toward experiments at the quantum-gravity interface. Communications Physics.
9, 80.
mla: Agafonova, Sofia, et al. “One-Milligram Torsional Pendulum toward Experiments
at the Quantum-Gravity Interface.” Communications Physics, vol. 9, 80,
Springer Nature, 2026, doi:10.1038/s42005-026-02514-w.
short: S. Agafonova, P. Rosello, M. Mekonnen, O. Hosten, Communications Physics
9 (2026).
corr_author: '1'
date_created: 2025-12-21T11:39:04Z
date_published: 2026-03-04T00:00:00Z
date_updated: 2026-03-16T10:09:22Z
day: '04'
ddc:
- '530'
department:
- _id: GradSch
- _id: OnHo
doi: 10.1038/s42005-026-02514-w
external_id:
arxiv:
- '2408.09445'
file:
- access_level: open_access
checksum: 62e2175e7e3ad49260ae6a7b4e0860a2
content_type: application/pdf
creator: dernst
date_created: 2026-03-16T10:07:46Z
date_updated: 2026-03-16T10:07:46Z
file_id: '21457'
file_name: 2026_CommunicationsPhysics_Agafonova.pdf
file_size: 1901772
relation: main_file
success: 1
file_date_updated: 2026-03-16T10:07:46Z
has_accepted_license: '1'
intvolume: ' 9'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: bdb2a702-d553-11ed-ba76-f12e3e5a3bc6
grant_number: '101087907'
name: 'A quantum hybrid of atoms and milligram-scale pendulums: towards gravitational
quantum mechanics'
publication: Communications Physics
publication_identifier:
eissn:
- 2399-3650
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
related_material:
record:
- id: '20842'
relation: research_data
status: public
scopus_import: '1'
status: public
title: One-milligram torsional pendulum toward experiments at the quantum-gravity
interface
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: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21453'
abstract:
- lang: eng
text: "1. Collective behaviours are a fascinating study area due to the emergent
properties that can only arise in groups of interacting individuals. However,
their quantitative study is often impaired by technical difficulties, creating
either low-quality and sparse data or impractical data amounts, particularly when
capturing large groups over long periods of time. Common challenges arise from
recording group members with as little obscuring of each other as possible, as
well as in generating manageable data amounts with as high as possible information
content.\r\n2. We here provide a multicomponent system that allows to record,
analyse and simulate the long-term spatiotemporal activity patterns of insect
collectives, especially ant colonies. Our Ant Observing System, ALTAA, comprises
a flat-nest design to prevent occlusion of individuals, a recording system running
on a low-power single-board-computer, and a set of computer programmes performing
quantitative analyses to guide the formation and validation of rules underlying
the observed collective patterns. Our system is scalable in that it allows parallel,
continuous observation of a high number of colonies using low memory space, with
colony maintenance requirements (e.g. feeding, nest humidity) being achieved at
lowest possible disturbance by the experimenter.\r\n3. We showcase the potential
of the system in a study using the black garden ant, Lasius niger, where we analyse
the spatiotemporal effects of different group sizes (1, 6, 10 ants), brood (larvae)
presence or absence, as well as of different nest geometries, over a period of
1 week. We show that the ants' motion activity has a weak periodicity in the range
of 20 to 120 min promoted by larval presence, and that ants are spatially attracted
to their larvae, the water source and the walls. We also find that the presence
of nestmates lowers an individual ant's motion activity. Observed data are compared
to simulations of the temporal activity of the ants.\r\n4. ALTAA provides a powerful
toolkit to quantify and interpret spatial and temporal collective activity patterns
in (social) insects over extended periods."
acknowledgement: We thank Harikrishnan Rajendran for discussion. This project has
received funding from the European Research Council (ERC) under the European Union's
Horizon 2020 Research and Innovation Programme (grant agreement No. 771402; EPIDEMICSonCHIP
to S.C.). Open Access funding provided by Institute of Science and Technology Austria/KEMÖ.
article_processing_charge: Yes
article_type: original
author:
- first_name: Jinook
full_name: Oh, Jinook
id: 403169A4-080F-11EA-9993-BF3F3DDC885E
last_name: Oh
orcid: 0000-0001-7425-2372
- first_name: Sylvia
full_name: Cremer, Sylvia
id: 2F64EC8C-F248-11E8-B48F-1D18A9856A87
last_name: Cremer
orcid: 0000-0002-2193-3868
citation:
ama: 'Oh J, Cremer S. ALTAA: Analysis of long-term activity patterns in ant colonies.
Methods in Ecology and Evolution. 2026. doi:10.1111/2041-210x.70277'
apa: 'Oh, J., & Cremer, S. (2026). ALTAA: Analysis of long-term activity patterns
in ant colonies. Methods in Ecology and Evolution. Wiley. https://doi.org/10.1111/2041-210x.70277'
chicago: 'Oh, Jinook, and Sylvia Cremer. “ALTAA: Analysis of Long-Term Activity
Patterns in Ant Colonies.” Methods in Ecology and Evolution. Wiley, 2026.
https://doi.org/10.1111/2041-210x.70277.'
ieee: 'J. Oh and S. Cremer, “ALTAA: Analysis of long-term activity patterns in ant
colonies,” Methods in Ecology and Evolution. Wiley, 2026.'
ista: 'Oh J, Cremer S. 2026. ALTAA: Analysis of long-term activity patterns in ant
colonies. Methods in Ecology and Evolution.'
mla: 'Oh, Jinook, and Sylvia Cremer. “ALTAA: Analysis of Long-Term Activity Patterns
in Ant Colonies.” Methods in Ecology and Evolution, Wiley, 2026, doi:10.1111/2041-210x.70277.'
short: J. Oh, S. Cremer, Methods in Ecology and Evolution (2026).
corr_author: '1'
date_created: 2026-03-15T23:01:36Z
date_published: 2026-03-06T00:00:00Z
date_updated: 2026-03-16T10:31:02Z
day: '06'
ddc:
- '570'
department:
- _id: SyCr
doi: 10.1111/2041-210x.70277
ec_funded: 1
has_accepted_license: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1111/2041-210x.70277
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: 2649B4DE-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '771402'
name: Epidemics in ant societies on a chip
publication: Methods in Ecology and Evolution
publication_identifier:
eissn:
- 2041-210X
publication_status: epub_ahead
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'ALTAA: Analysis of long-term activity patterns in ant colonies'
tmp:
image: /images/cc_by.png
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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
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...
---
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OA_place: publisher
OA_type: gold
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abstract:
- lang: eng
text: This study examines the distribution, growth, and GLOF hazard of glacial lakes
across major Himalayan river basins. Basin-wise GLOF susceptibility was assessed
using glacial lake abundance, spatial distribution, and rates of lake area expansion.
The Kosi, Yarlung Zangbo, Manas, and Upper Indus basins were identified as the
most susceptible and classified as critical. The highest rates of lake size increase
were observed in the Kosi Basin, followed by Yarlung Zangbo, Manas, Karnali, Upper
Indus, and Tista, indicating their potential as future GLOF-prone regions. Moreover,
a Himalayan-scale GLOF hazard map was generated integrating population, hydropower
infrastructure, potential flood volume, roads, settlements, and railways revealing
high hazard levels in the Chenab, Jhelum, Teesta, and Beas basins in India; the
Koshi, Tama-Koshi, and Dudh-Koshi basins in Nepal; and the Kuri Chu sub-basin
of the Manas Basin in Bhutan. These findings highlight priority regions where
detailed field investigations and hydrodynamic modelling are essential before
further infrastructure development.
acknowledgement: The work is partially financed by USDMA and WIHG, Dehradun. The authors
would like to express their sincere gratitude to Dr. Ashim Sattar for his valuable
insights, constructive suggestions, and contributions toward refining and improving
the quality of this work. I want to give my special thanks to Mr. Sourav Anand and
Mr. Shivyank Negi for helping me create the database. I would also like to thank
IIT Kharagpur. For further data access, the corresponding authors can be contacted.
article_number: '2639085'
article_processing_charge: Yes
article_type: original
author:
- first_name: Litan
full_name: Mohanty, Litan
last_name: Mohanty
- first_name: Prateek
full_name: Gantayat, Prateek
id: 02734268-3e8d-11ef-80a1-cec4a088d004
last_name: Gantayat
citation:
ama: Mohanty L, GANTAYAT P. Comprehensive assessment of Himalayan glacial lakes
concerning their distribution, dynamics, and hazard potential. Geomatics Natural
Hazards and Risk. 2026;17(1). doi:10.1080/19475705.2026.2639085
apa: Mohanty, L., & GANTAYAT, P. (2026). Comprehensive assessment of Himalayan
glacial lakes concerning their distribution, dynamics, and hazard potential. Geomatics
Natural Hazards and Risk. Taylor & Francis. https://doi.org/10.1080/19475705.2026.2639085
chicago: Mohanty, Litan, and PRATEEK GANTAYAT. “Comprehensive Assessment of Himalayan
Glacial Lakes Concerning Their Distribution, Dynamics, and Hazard Potential.”
Geomatics Natural Hazards and Risk. Taylor & Francis, 2026. https://doi.org/10.1080/19475705.2026.2639085.
ieee: L. Mohanty and P. GANTAYAT, “Comprehensive assessment of Himalayan glacial
lakes concerning their distribution, dynamics, and hazard potential,” Geomatics
Natural Hazards and Risk, vol. 17, no. 1. Taylor & Francis, 2026.
ista: Mohanty L, GANTAYAT P. 2026. Comprehensive assessment of Himalayan glacial
lakes concerning their distribution, dynamics, and hazard potential. Geomatics
Natural Hazards and Risk. 17(1), 2639085.
mla: Mohanty, Litan, and PRATEEK GANTAYAT. “Comprehensive Assessment of Himalayan
Glacial Lakes Concerning Their Distribution, Dynamics, and Hazard Potential.”
Geomatics Natural Hazards and Risk, vol. 17, no. 1, 2639085, Taylor &
Francis, 2026, doi:10.1080/19475705.2026.2639085.
short: L. Mohanty, P. GANTAYAT, Geomatics Natural Hazards and Risk 17 (2026).
date_created: 2026-03-15T23:01:36Z
date_published: 2026-03-04T00:00:00Z
date_updated: 2026-03-16T10:21:38Z
day: '04'
ddc:
- '550'
department:
- _id: FrPe
doi: 10.1080/19475705.2026.2639085
file:
- access_level: open_access
checksum: 78f7a3020bf5966e820340a711ea3a6b
content_type: application/pdf
creator: dernst
date_created: 2026-03-16T10:18:26Z
date_updated: 2026-03-16T10:18:26Z
file_id: '21458'
file_name: 2026_Geomatics_Mohanty.pdf
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language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
publication: Geomatics Natural Hazards and Risk
publication_identifier:
eissn:
- 1947-5713
issn:
- 1947-5705
publication_status: published
publisher: Taylor & Francis
quality_controlled: '1'
scopus_import: '1'
status: public
title: Comprehensive assessment of Himalayan glacial lakes concerning their distribution,
dynamics, and hazard potential
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 17
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---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21009'
abstract:
- lang: eng
text: We demonstrate that periodically driven quantum rotors provide a promising
and broadly applicable platform to implement multigap topological phases, where
groups of bands can acquire topological invariants due to non-Abelian braiding
of band degeneracies. By adiabatically varying the periodic kicks to the rotor
we find nodal-line braiding, which causes sign flips of topological charges of
band nodes and can prevent them from annihilating, indicated by nonzero values
of the patch Euler class. In particular, we report on the emergence of an anomalous
Dirac string phase arising in the strongly driven regime, a truly out-of-equilibrium
phase of the quantum rotor. This phase emanates from braiding processes involving
all (quasienergy) gaps and manifests itself with edge states at zero angular momentum.
Our results reveal direct applications in state-of-the-art experiments of quantum
rotors, such as linear molecules driven by periodic far-off-resonant laser pulses
or artificial quantum rotors in optical lattices, whose extensive versatility
offers precise modification and observation of novel non-Abelian topological properties.
acknowledgement: We thank G. M. Koutentakis, S. Wimberger, J. G. E. Harris, T. Enss,
and A. Ghazaryan for fruitful discussions. M.L. acknowledges support by the European
Research Council (ERC) Starting Grant No. 801770 (ANGULON). R.-J.S. acknowledges
funding from a EPSRC ERC underwrite (Grant No. EP/X025829/1), a EPSRC New Investigator
Award (Grant No. EP/W00187X/1), and Trinity College, Cambridge. F.N.Ü. acknowledges
support from the Marie Skłodowska-Curie Programme of the European Commission (Grant
No. 893915), a Simons Investigator Award (Grant No. 511029), Trinity College Cambridge,
and the Royal Society (Grant No. URF/R1/241667).
article_number: '012216'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Volker
full_name: Karle, Volker
id: D7C012AE-D7ED-11E9-95E8-1EC5E5697425
last_name: Karle
orcid: 0000-0002-6963-0129
- first_name: Mikhail
full_name: Lemeshko, Mikhail
id: 37CB05FA-F248-11E8-B48F-1D18A9856A87
last_name: Lemeshko
orcid: 0000-0002-6990-7802
- first_name: Adrien
full_name: Bouhon, Adrien
last_name: Bouhon
- first_name: Robert-Jan
full_name: Slager, Robert-Jan
last_name: Slager
- first_name: F. Nur
full_name: Ünal, F. Nur
last_name: Ünal
citation:
ama: Karle V, Lemeshko M, Bouhon A, Slager R-J, Ünal FN. Anomalous multigap topological
phases in periodically driven quantum rotors. Physical Review A. 2026;113(1).
doi:10.1103/db9d-9bns
apa: Karle, V., Lemeshko, M., Bouhon, A., Slager, R.-J., & Ünal, F. N. (2026).
Anomalous multigap topological phases in periodically driven quantum rotors. Physical
Review A. American Physical Society. https://doi.org/10.1103/db9d-9bns
chicago: Karle, Volker, Mikhail Lemeshko, Adrien Bouhon, Robert-Jan Slager, and
F. Nur Ünal. “Anomalous Multigap Topological Phases in Periodically Driven Quantum
Rotors.” Physical Review A. American Physical Society, 2026. https://doi.org/10.1103/db9d-9bns.
ieee: V. Karle, M. Lemeshko, A. Bouhon, R.-J. Slager, and F. N. Ünal, “Anomalous
multigap topological phases in periodically driven quantum rotors,” Physical
Review A, vol. 113, no. 1. American Physical Society, 2026.
ista: Karle V, Lemeshko M, Bouhon A, Slager R-J, Ünal FN. 2026. Anomalous multigap
topological phases in periodically driven quantum rotors. Physical Review A. 113(1),
012216.
mla: Karle, Volker, et al. “Anomalous Multigap Topological Phases in Periodically
Driven Quantum Rotors.” Physical Review A, vol. 113, no. 1, 012216, American
Physical Society, 2026, doi:10.1103/db9d-9bns.
short: V. Karle, M. Lemeshko, A. Bouhon, R.-J. Slager, F.N. Ünal, Physical Review
A 113 (2026).
corr_author: '1'
date_created: 2026-01-20T10:06:07Z
date_published: 2026-01-12T00:00:00Z
date_updated: 2026-03-16T12:21:55Z
day: '12'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1103/db9d-9bns
ec_funded: 1
external_id:
arxiv:
- '2408.16848'
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checksum: ca62a5050a234c0554e2583b1c126057
content_type: application/pdf
creator: dernst
date_created: 2026-01-21T09:04:48Z
date_updated: 2026-01-21T09:04:48Z
file_id: '21029'
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month: '01'
oa: 1
oa_version: Published Version
project:
- _id: 2688CF98-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '801770'
name: 'Angulon: physics and applications of a new quasiparticle'
publication: Physical Review A
publication_identifier:
eissn:
- 2469-9934
issn:
- 2469-9926
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
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title: Anomalous multigap topological phases in periodically driven quantum rotors
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...
---
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acknowledgement: "Finally, I gratefully acknowledge funding from the DOC Fellowship
of the Austrian Academy\r\nof Sciences (OeAW): grant agreement 26360."
alternative_title:
- ISTA Thesis
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ama: Dunajova Z. Geometry-driven self-organization of migrating cells and chiral
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apa: Dunajova, Z. (2026). Geometry-driven self-organization of migrating cells
and chiral filaments. Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-21423
chicago: Dunajova, Zuzana. “Geometry-Driven Self-Organization of Migrating Cells
and Chiral Filaments.” Institute of Science and Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-21423.
ieee: Z. Dunajova, “Geometry-driven self-organization of migrating cells and chiral
filaments,” Institute of Science and Technology Austria, 2026.
ista: Dunajova Z. 2026. Geometry-driven self-organization of migrating cells and
chiral filaments. Institute of Science and Technology Austria.
mla: Dunajova, Zuzana. Geometry-Driven Self-Organization of Migrating Cells and
Chiral Filaments. Institute of Science and Technology Austria, 2026, doi:10.15479/AT-ISTA-21423.
short: Z. Dunajova, Geometry-Driven Self-Organization of Migrating Cells and Chiral
Filaments, Institute of Science and Technology Austria, 2026.
corr_author: '1'
date_created: 2026-03-11T08:30:49Z
date_published: 2026-03-11T00:00:00Z
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ddc:
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name: Motile active matter models of migrating cells and chiral filaments
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isbn:
- 978-3-99078-076-3
issn:
- 2663-337X
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publisher: Institute of Science and Technology Austria
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full_name: Hannezo, Edouard B
id: 3A9DB764-F248-11E8-B48F-1D18A9856A87
last_name: Hannezo
orcid: 0000-0001-6005-1561
title: Geometry-driven self-organization of migrating cells and chiral filaments
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image: /images/cc_by_nc_sa.png
legal_code_url: https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode
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abstract:
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text: These files contain supplementary movies accompanying the PhD thesis “Geometry-driven
self-organization of migrating cells and chiral filaments” by Zuzana Dunajova
(2026). The videos provide additional visual material supporting the experiments
and results described in the thesis.
acknowledged_ssus:
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- _id: ScienComp
article_processing_charge: No
author:
- first_name: Zuzana
full_name: Dunajova, Zuzana
id: 4B39F286-F248-11E8-B48F-1D18A9856A87
last_name: Dunajova
citation:
ama: Dunajova Z. Supplementary movies to PhD thesis “Geometry-driven self-organization
of migrating cells and chiral filaments.” 2026. doi:10.15479/AT-ISTA-21439
apa: Dunajova, Z. (2026). Supplementary movies to PhD thesis “Geometry-driven self-organization
of migrating cells and chiral filaments.” Institute of Science and Technology
Austria. https://doi.org/10.15479/AT-ISTA-21439
chicago: Dunajova, Zuzana. “Supplementary Movies to PhD Thesis ‘Geometry-Driven
Self-Organization of Migrating Cells and Chiral Filaments.’” Institute of Science
and Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-21439.
ieee: Z. Dunajova, “Supplementary movies to PhD thesis ‘Geometry-driven self-organization
of migrating cells and chiral filaments.’” Institute of Science and Technology
Austria, 2026.
ista: Dunajova Z. 2026. Supplementary movies to PhD thesis “Geometry-driven self-organization
of migrating cells and chiral filaments”, Institute of Science and Technology
Austria, 10.15479/AT-ISTA-21439.
mla: Dunajova, Zuzana. Supplementary Movies to PhD Thesis “Geometry-Driven Self-Organization
of Migrating Cells and Chiral Filaments.” Institute of Science and Technology
Austria, 2026, doi:10.15479/AT-ISTA-21439.
short: Z. Dunajova, (2026).
contributor:
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first_name: Saren
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last_name: Tasciyan
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first_name: Philipp
id: 40136C2A-F248-11E8-B48F-1D18A9856A87
last_name: Radler
orcid: '0000-0001-9198-2182 '
corr_author: '1'
date_created: 2026-03-11T21:05:20Z
date_published: 2026-03-12T00:00:00Z
date_updated: 2026-03-18T14:11:36Z
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grant_number: '26360'
name: Motile active matter models of migrating cells and chiral filaments
publisher: Institute of Science and Technology Austria
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OA_type: gold
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_id: '21370'
abstract:
- lang: eng
text: Through digital imaging, microscopy has evolved from primarily being a means
for visual observation of life at the micro- and nano-scale, to a quantitative
tool with ever-increasing resolution and throughput. Artificial intelligence,
deep neural networks, and machine learning (ML) are all niche terms describing
computational methods that have gained a pivotal role in microscopy-based research
over the past decade. This Roadmap encompasses key aspects of how ML is applied
to microscopy image data, with the aim of gaining scientific knowledge by improved
image quality, automated detection, segmentation, classification and tracking
of objects, and efficient merging of information from multiple imaging modalities.
We aim to give the reader an overview of the key developments and an understanding
of possibilities and limitations of ML for microscopy. It will be of interest
to a wide cross-disciplinary audience in the physical sciences and life sciences.
article_number: '012501'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Giovanni
full_name: Volpe, Giovanni
last_name: Volpe
- first_name: Carolina
full_name: Wählby, Carolina
last_name: Wählby
- first_name: Lei
full_name: Tian, Lei
last_name: Tian
- first_name: Michael
full_name: Hecht, Michael
last_name: Hecht
- first_name: Artur
full_name: Yakimovich, Artur
last_name: Yakimovich
- first_name: Kristina
full_name: Monakhova, Kristina
last_name: Monakhova
- first_name: Laura
full_name: Waller, Laura
last_name: Waller
- first_name: Ivo F.
full_name: Sbalzarini, Ivo F.
last_name: Sbalzarini
- first_name: Christopher A.
full_name: Metzler, Christopher A.
last_name: Metzler
- first_name: Mingyang
full_name: Xie, Mingyang
last_name: Xie
- first_name: Kevin
full_name: Zhang, Kevin
last_name: Zhang
- first_name: Isaac C
full_name: Lenton, Isaac C
id: a550210f-223c-11ec-8182-e2d45e817efb
last_name: Lenton
orcid: 0000-0002-5010-6984
- first_name: Halina
full_name: Rubinsztein-Dunlop, Halina
last_name: Rubinsztein-Dunlop
- first_name: Daniel
full_name: Brunner, Daniel
last_name: Brunner
- first_name: Bijie
full_name: Bai, Bijie
last_name: Bai
- first_name: Aydogan
full_name: Ozcan, Aydogan
last_name: Ozcan
- first_name: Daniel
full_name: Midtvedt, Daniel
last_name: Midtvedt
- first_name: Hao
full_name: Wang, Hao
last_name: Wang
- first_name: Tongyu
full_name: Li, Tongyu
last_name: Li
- first_name: Nataša
full_name: Sladoje, Nataša
last_name: Sladoje
- first_name: Joakim
full_name: Lindblad, Joakim
last_name: Lindblad
- first_name: Jason T.
full_name: Smith, Jason T.
last_name: Smith
- first_name: Marien
full_name: Ochoa, Marien
last_name: Ochoa
- first_name: Margarida
full_name: Barroso, Margarida
last_name: Barroso
- first_name: Xavier
full_name: Intes, Xavier
last_name: Intes
- first_name: Tong
full_name: Qiu, Tong
last_name: Qiu
- first_name: Li Yu
full_name: Yu, Li Yu
last_name: Yu
- first_name: Sixian
full_name: You, Sixian
last_name: You
- first_name: Yongtao
full_name: Liu, Yongtao
last_name: Liu
- first_name: Maxim A.
full_name: Ziatdinov, Maxim A.
last_name: Ziatdinov
- first_name: Sergei V.
full_name: Kalinin, Sergei V.
last_name: Kalinin
- first_name: Arlo
full_name: Sheridan, Arlo
last_name: Sheridan
- first_name: Uri
full_name: Manor, Uri
last_name: Manor
- first_name: Elias
full_name: Nehme, Elias
last_name: Nehme
- first_name: Ofri
full_name: Goldenberg, Ofri
last_name: Goldenberg
- first_name: Yoav
full_name: Shechtman, Yoav
last_name: Shechtman
- first_name: Henrik K.
full_name: Moberg, Henrik K.
last_name: Moberg
- first_name: Christoph
full_name: Langhammer, Christoph
last_name: Langhammer
- first_name: Barbora
full_name: Špačková, Barbora
last_name: Špačková
- first_name: Saga
full_name: Helgadottir, Saga
last_name: Helgadottir
- first_name: Benjamin
full_name: Midtvedt, Benjamin
last_name: Midtvedt
- first_name: Aykut
full_name: Argun, Aykut
last_name: Argun
- first_name: Tobias
full_name: Thalheim, Tobias
last_name: Thalheim
- first_name: Frank
full_name: Cichos, Frank
last_name: Cichos
- first_name: Stefano
full_name: Bo, Stefano
last_name: Bo
- first_name: Lars
full_name: Hubatsch, Lars
last_name: Hubatsch
- first_name: Jesus
full_name: Pineda, Jesus
last_name: Pineda
- first_name: Carlo
full_name: Manzo, Carlo
last_name: Manzo
- first_name: Harshith
full_name: Bachimanchi, Harshith
last_name: Bachimanchi
- first_name: Erik
full_name: Selander, Erik
last_name: Selander
- first_name: Antoni
full_name: Homs-Corbera, Antoni
last_name: Homs-Corbera
- first_name: Martin
full_name: Fränzl, Martin
last_name: Fränzl
- first_name: Kevin
full_name: De Haan, Kevin
last_name: De Haan
- first_name: Yair
full_name: Rivenson, Yair
last_name: Rivenson
- first_name: Zofia
full_name: Korczak, Zofia
last_name: Korczak
- first_name: Caroline Beck
full_name: Adiels, Caroline Beck
last_name: Adiels
- first_name: Mite
full_name: Mijalkov, Mite
last_name: Mijalkov
- first_name: Dániel
full_name: Veréb, Dániel
last_name: Veréb
- first_name: Yu Wei
full_name: Chang, Yu Wei
last_name: Chang
- first_name: Joana B.
full_name: Pereira, Joana B.
last_name: Pereira
- first_name: Damian
full_name: Matuszewski, Damian
last_name: Matuszewski
- first_name: Gustaf
full_name: Kylberg, Gustaf
last_name: Kylberg
- first_name: Ida Maria
full_name: Sintorn, Ida Maria
last_name: Sintorn
- first_name: Juan C.
full_name: Caicedo, Juan C.
last_name: Caicedo
- first_name: Beth A.
full_name: Cimini, Beth A.
last_name: Cimini
- first_name: Muyinatu A.
full_name: Lediju Bell, Muyinatu A.
last_name: Lediju Bell
- first_name: Bruno M.
full_name: Saraiva, Bruno M.
last_name: Saraiva
- first_name: Guillaume
full_name: Jacquemet, Guillaume
last_name: Jacquemet
- first_name: Ricardo
full_name: Henriques, Ricardo
last_name: Henriques
- first_name: Wei
full_name: Ouyang, Wei
last_name: Ouyang
- first_name: Trang
full_name: Le, Trang
last_name: Le
- first_name: Estibaliz
full_name: Gómez-De-Mariscal, Estibaliz
last_name: Gómez-De-Mariscal
- first_name: Daniel
full_name: Sage, Daniel
last_name: Sage
- first_name: Arrate
full_name: Muñoz-Barrutia, Arrate
last_name: Muñoz-Barrutia
- first_name: Ebba Josefson
full_name: Lindqvist, Ebba Josefson
last_name: Lindqvist
- first_name: Johanna
full_name: Bergman, Johanna
last_name: Bergman
citation:
ama: 'Volpe G, Wählby C, Tian L, et al. Roadmap on deep learning for microscopy.
Journal of Physics: Photonics. 2026;8(1). doi:10.1088/2515-7647/ae0fd1'
apa: 'Volpe, G., Wählby, C., Tian, L., Hecht, M., Yakimovich, A., Monakhova, K.,
… Bergman, J. (2026). Roadmap on deep learning for microscopy. Journal of Physics:
Photonics. IOP Publishing. https://doi.org/10.1088/2515-7647/ae0fd1'
chicago: 'Volpe, Giovanni, Carolina Wählby, Lei Tian, Michael Hecht, Artur Yakimovich,
Kristina Monakhova, Laura Waller, et al. “Roadmap on Deep Learning for Microscopy.”
Journal of Physics: Photonics. IOP Publishing, 2026. https://doi.org/10.1088/2515-7647/ae0fd1.'
ieee: 'G. Volpe et al., “Roadmap on deep learning for microscopy,” Journal
of Physics: Photonics, vol. 8, no. 1. IOP Publishing, 2026.'
ista: 'Volpe G, Wählby C, Tian L, Hecht M, Yakimovich A, Monakhova K, Waller L,
Sbalzarini IF, Metzler CA, Xie M, Zhang K, Lenton IC, Rubinsztein-Dunlop H, Brunner
D, Bai B, Ozcan A, Midtvedt D, Wang H, Li T, Sladoje N, Lindblad J, Smith JT,
Ochoa M, Barroso M, Intes X, Qiu T, Yu LY, You S, Liu Y, Ziatdinov MA, Kalinin
SV, Sheridan A, Manor U, Nehme E, Goldenberg O, Shechtman Y, Moberg HK, Langhammer
C, Špačková B, Helgadottir S, Midtvedt B, Argun A, Thalheim T, Cichos F, Bo S,
Hubatsch L, Pineda J, Manzo C, Bachimanchi H, Selander E, Homs-Corbera A, Fränzl
M, De Haan K, Rivenson Y, Korczak Z, Adiels CB, Mijalkov M, Veréb D, Chang YW,
Pereira JB, Matuszewski D, Kylberg G, Sintorn IM, Caicedo JC, Cimini BA, Lediju
Bell MA, Saraiva BM, Jacquemet G, Henriques R, Ouyang W, Le T, Gómez-De-Mariscal
E, Sage D, Muñoz-Barrutia A, Lindqvist EJ, Bergman J. 2026. Roadmap on deep learning
for microscopy. Journal of Physics: Photonics. 8(1), 012501.'
mla: 'Volpe, Giovanni, et al. “Roadmap on Deep Learning for Microscopy.” Journal
of Physics: Photonics, vol. 8, no. 1, 012501, IOP Publishing, 2026, doi:10.1088/2515-7647/ae0fd1.'
short: 'G. Volpe, C. Wählby, L. Tian, M. Hecht, A. Yakimovich, K. Monakhova, L.
Waller, I.F. Sbalzarini, C.A. Metzler, M. Xie, K. Zhang, I.C. Lenton, H. Rubinsztein-Dunlop,
D. Brunner, B. Bai, A. Ozcan, D. Midtvedt, H. Wang, T. Li, N. Sladoje, J. Lindblad,
J.T. Smith, M. Ochoa, M. Barroso, X. Intes, T. Qiu, L.Y. Yu, S. You, Y. Liu, M.A.
Ziatdinov, S.V. Kalinin, A. Sheridan, U. Manor, E. Nehme, O. Goldenberg, Y. Shechtman,
H.K. Moberg, C. Langhammer, B. Špačková, S. Helgadottir, B. Midtvedt, A. Argun,
T. Thalheim, F. Cichos, S. Bo, L. Hubatsch, J. Pineda, C. Manzo, H. Bachimanchi,
E. Selander, A. Homs-Corbera, M. Fränzl, K. De Haan, Y. Rivenson, Z. Korczak,
C.B. Adiels, M. Mijalkov, D. Veréb, Y.W. Chang, J.B. Pereira, D. Matuszewski,
G. Kylberg, I.M. Sintorn, J.C. Caicedo, B.A. Cimini, M.A. Lediju Bell, B.M. Saraiva,
G. Jacquemet, R. Henriques, W. Ouyang, T. Le, E. Gómez-De-Mariscal, D. Sage, A.
Muñoz-Barrutia, E.J. Lindqvist, J. Bergman, Journal of Physics: Photonics 8 (2026).'
date_created: 2026-03-01T23:01:39Z
date_published: 2026-03-01T00:00:00Z
date_updated: 2026-03-23T13:18:11Z
day: '01'
ddc:
- '530'
department:
- _id: ScWa
doi: 10.1088/2515-7647/ae0fd1
external_id:
arxiv:
- '2303.03793'
file:
- access_level: open_access
checksum: 172720f1f0c5c9d06a282e52023a0030
content_type: application/pdf
creator: dernst
date_created: 2026-03-02T09:05:53Z
date_updated: 2026-03-02T09:05:53Z
file_id: '21375'
file_name: 2026_JPhysPhotonics_Volpe.pdf
file_size: 16789781
relation: main_file
success: 1
file_date_updated: 2026-03-02T09:05:53Z
has_accepted_license: '1'
intvolume: ' 8'
issue: '1'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
publication: 'Journal of Physics: Photonics'
publication_identifier:
eissn:
- 2515-7647
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Roadmap on deep learning for microscopy
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: '2026'
...
---
OA_place: publisher
OA_type: hybrid
_id: '21470'
abstract:
- lang: eng
text: Despite its pivotal role in optical manipulation, high capacity communications,
and quantum information, a general measure of orbital angular momentum (OAM) in
structured light remains elusive. In optical fields, where multiple vortices coexist,
the local nature of vortex OAM and the absence of a common rotation axis make
the total OAM of the field difficult to quantify. Here, we introduce the R index—a
metric that captures the intrinsic OAM content of any structured optical field,
from pure Laguerre–Gaussian modes to arbitrary multi vortex superpositions. Not
only does this metric quantify the total OAM, it also assesses field purity, providing
insight into the fidelity and robustness of the OAM generation. By unifying OAM
characterization into a single figure of merit, the R index enables direct comparison
across diverse beam profiles and facilitates the identification of optimal configurations
for both foundational studies and applied technologies.
acknowledgement: This research was funded in whole or in part by the Austrian Science
Fund (FWF) [10.55776/F1004]. For open access purposes, the author has applied a
CC BY public copyright license to any author accepted manuscript version arising
from this submission.
article_number: '015071'
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Monika
full_name: Bahl, Monika
last_name: Bahl
- first_name: Georgios
full_name: Koutentakis, Georgios
id: d7b23d3a-9e21-11ec-b482-f76739596b95
last_name: Koutentakis
- first_name: Mikhail
full_name: Maslov, Mikhail
id: 2E65BB0E-F248-11E8-B48F-1D18A9856A87
last_name: Maslov
orcid: 0000-0003-4074-2570
- first_name: Tom
full_name: Jungnickel, Tom
last_name: Jungnickel
- first_name: Timo
full_name: Gaßen, Timo
last_name: Gaßen
- first_name: Mikhail
full_name: Lemeshko, Mikhail
id: 37CB05FA-F248-11E8-B48F-1D18A9856A87
last_name: Lemeshko
orcid: 0000-0002-6990-7802
- first_name: Oliver H.
full_name: Heckl, Oliver H.
last_name: Heckl
citation:
ama: 'Bahl M, Koutentakis G, Maslov M, et al. The R-index: A universal metric for
evaluating OAM content and mode purity in optical fields. Journal of Physics:
Photonics. 2026;8(1). doi:10.1088/2515-7647/ae3506'
apa: 'Bahl, M., Koutentakis, G., Maslov, M., Jungnickel, T., Gaßen, T., Lemeshko,
M., & Heckl, O. H. (2026). The R-index: A universal metric for evaluating
OAM content and mode purity in optical fields. Journal of Physics: Photonics.
IOP Publishing. https://doi.org/10.1088/2515-7647/ae3506'
chicago: 'Bahl, Monika, Georgios Koutentakis, Mikhail Maslov, Tom Jungnickel, Timo
Gaßen, Mikhail Lemeshko, and Oliver H. Heckl. “The R-Index: A Universal Metric
for Evaluating OAM Content and Mode Purity in Optical Fields.” Journal of Physics:
Photonics. IOP Publishing, 2026. https://doi.org/10.1088/2515-7647/ae3506.'
ieee: 'M. Bahl et al., “The R-index: A universal metric for evaluating OAM
content and mode purity in optical fields,” Journal of Physics: Photonics,
vol. 8, no. 1. IOP Publishing, 2026.'
ista: 'Bahl M, Koutentakis G, Maslov M, Jungnickel T, Gaßen T, Lemeshko M, Heckl
OH. 2026. The R-index: A universal metric for evaluating OAM content and mode
purity in optical fields. Journal of Physics: Photonics. 8(1), 015071.'
mla: 'Bahl, Monika, et al. “The R-Index: A Universal Metric for Evaluating OAM Content
and Mode Purity in Optical Fields.” Journal of Physics: Photonics, vol.
8, no. 1, 015071, IOP Publishing, 2026, doi:10.1088/2515-7647/ae3506.'
short: 'M. Bahl, G. Koutentakis, M. Maslov, T. Jungnickel, T. Gaßen, M. Lemeshko,
O.H. Heckl, Journal of Physics: Photonics 8 (2026).'
corr_author: '1'
date_created: 2026-03-22T23:04:32Z
date_published: 2026-03-10T00:00:00Z
date_updated: 2026-03-23T13:26:26Z
day: '10'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1088/2515-7647/ae3506
external_id:
arxiv:
- '2508.12973'
file:
- access_level: open_access
checksum: 0ec8a2d3f9efa704203a41f068344974
content_type: application/pdf
creator: dernst
date_created: 2026-03-23T13:24:01Z
date_updated: 2026-03-23T13:24:01Z
file_id: '21476'
file_name: 2026_JPhysPhotonics_Bahl.pdf
file_size: 1150404
relation: main_file
success: 1
file_date_updated: 2026-03-23T13:24:01Z
has_accepted_license: '1'
intvolume: ' 8'
issue: '1'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: 7c040762-9f16-11ee-852c-dd79eeee4ab3
grant_number: F100403
name: Coherent Optical Metrology Beyond Electric-Dipole-Allowed Transitions
publication: 'Journal of Physics: Photonics'
publication_identifier:
eissn:
- 2515-7647
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The R-index: A universal metric for evaluating OAM content and mode purity
in optical fields'
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: '2026'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21469'
abstract:
- lang: eng
text: "Terahertz (THz) spectroscopy is a powerful probe of low-energy excitations
in complex materials. Extending it into the nonlinear regime broadens its scope
and can provide valuable insight into interactions among these modes. However,
interpreting nonlinear spectra is challenging because resonant features in this
case do not always reflect intrinsic material dynamics. Here, we study nonlinear
THz-induced Kerr effect in a generic material LaAlO3. After detailed analysis
of temporal oscillations of the Kerr signal, we identify an \U0001D438\U0001D454
Raman mode at 1.1 THz excited through a two-photon process, while two additional
peaks (0.86 and 0.36 THz) arise from phase matching of the near-infrared probe
beam with co- and counterpropagating THz pump fields, mediated by off-resonant
electronic hyperpolarizability. These results demonstrate the crucial role of
kinematic effects in shaping THz-induced Kerr response and establish a framework
for interpreting nonlinear spectroscopies in complex materials."
acknowledgement: Z. A. acknowledges support from the collaborative research project
SFB Q-M&S funded by the Austrian Science Fund (FWF, Grant No. PR1050F8602). S. F. M.
acknowledges support and funding from the Deutsche Forschungsgemeinschaft (DFG,
Grant No. 469405347).
article_number: '106901'
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Chao
full_name: Shen, Chao
id: f84c083e-dc8d-11ea-abe3-aaf3d822a8bb
last_name: Shen
- first_name: Maximilian
full_name: Frenzel, Maximilian
last_name: Frenzel
- first_name: Sebastian F.
full_name: Maehrlein, Sebastian F.
last_name: Maehrlein
- first_name: Zhanybek
full_name: Alpichshev, Zhanybek
id: 45E67A2A-F248-11E8-B48F-1D18A9856A87
last_name: Alpichshev
orcid: 0000-0002-7183-5203
citation:
ama: Shen C, Frenzel M, Maehrlein SF, Alpichshev Z. Disentangling electronic and
ionic nonlinear polarization effects in bulk THz Kerr response. Physical Review
Letters. 2026;136(10). doi:10.1103/1c5k-9z82
apa: Shen, C., Frenzel, M., Maehrlein, S. F., & Alpichshev, Z. (2026). Disentangling
electronic and ionic nonlinear polarization effects in bulk THz Kerr response.
Physical Review Letters. American Physical Society. https://doi.org/10.1103/1c5k-9z82
chicago: Shen, Chao, Maximilian Frenzel, Sebastian F. Maehrlein, and Zhanybek Alpichshev.
“Disentangling Electronic and Ionic Nonlinear Polarization Effects in Bulk THz
Kerr Response.” Physical Review Letters. American Physical Society, 2026.
https://doi.org/10.1103/1c5k-9z82.
ieee: C. Shen, M. Frenzel, S. F. Maehrlein, and Z. Alpichshev, “Disentangling electronic
and ionic nonlinear polarization effects in bulk THz Kerr response,” Physical
Review Letters, vol. 136, no. 10. American Physical Society, 2026.
ista: Shen C, Frenzel M, Maehrlein SF, Alpichshev Z. 2026. Disentangling electronic
and ionic nonlinear polarization effects in bulk THz Kerr response. Physical Review
Letters. 136(10), 106901.
mla: Shen, Chao, et al. “Disentangling Electronic and Ionic Nonlinear Polarization
Effects in Bulk THz Kerr Response.” Physical Review Letters, vol. 136,
no. 10, 106901, American Physical Society, 2026, doi:10.1103/1c5k-9z82.
short: C. Shen, M. Frenzel, S.F. Maehrlein, Z. Alpichshev, Physical Review Letters
136 (2026).
corr_author: '1'
date_created: 2026-03-22T23:04:31Z
date_published: 2026-03-13T00:00:00Z
date_updated: 2026-03-23T13:11:09Z
day: '13'
ddc:
- '530'
department:
- _id: ZhAl
- _id: GradSch
doi: 10.1103/1c5k-9z82
file:
- access_level: open_access
checksum: 712b05b4b0e0fbe9fd426a8c9d41ce20
content_type: application/pdf
creator: dernst
date_created: 2026-03-23T13:08:06Z
date_updated: 2026-03-23T13:08:06Z
file_id: '21475'
file_name: 2026_PhysicalReviewLetters_Shen.pdf
file_size: 1375532
relation: main_file
success: 1
file_date_updated: 2026-03-23T13:08:06Z
has_accepted_license: '1'
intvolume: ' 136'
issue: '10'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: 34a97cc6-11ca-11ed-8bc3-9acbba792f33
grant_number: F8602
name: 'Center for Correlated Quantum Materials and Solid State Quantum Systems:
Nonlinear THz spectroscopy of quantum critical materials'
publication: Physical Review Letters
publication_identifier:
eissn:
- 1079-7114
issn:
- 0031-9007
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Disentangling electronic and ionic nonlinear polarization effects in bulk THz
Kerr response
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 136
year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
_id: '21472'
abstract:
- lang: eng
text: We study the ground state energy of a gas of spin 1/2 fermions with repulsive
short-range interactions. We derive an upper bound that agrees, at low density
e, with the Huang–Yang conjecture. The latter captures the first three terms in
an asymptotic low-density expansion, and in particular the Huang–Yang correction
term of order e^7/3. Our trial state is constructed using an adaptation of the
bosonic Bogoliubov theory to the Fermi system, where the correlation structure
of fermionic particles is incorporated by quasi-bosonic Bogoliubov transformations.
In the latter, it is important to consider a modified zero-energy scattering equation
that takes into account the presence of the Fermi sea, in the spirit of the Bethe–Goldstone
equation.
acknowledgement: "We thank the referees for valuable remarks. This work was partially
funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)
via the TRR 352 – Project-ID 470903074. PTN was partially supported by the European
Research Council via the ERC Consolidator Grant RAMBAS – Project-Nr. 10104424.\r\nOpen
access publishing facilitated by Università degli Studi di Milano, as part of the
Wiley - CRUI-CARE agreement."
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Emanuela L.
full_name: Giacomelli, Emanuela L.
last_name: Giacomelli
- first_name: Christian
full_name: Hainzl, Christian
last_name: Hainzl
- first_name: Phan Thành
full_name: Nam, Phan Thành
last_name: Nam
- first_name: Robert
full_name: Seiringer, Robert
id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
last_name: Seiringer
orcid: 0000-0002-6781-0521
citation:
ama: 'Giacomelli EL, Hainzl C, Nam PT, Seiringer R. The Huang–Yang formula for the
low-density Fermi gas: Upper bound. Communications on Pure and Applied Mathematics.
2026. doi:10.1002/cpa.70040'
apa: 'Giacomelli, E. L., Hainzl, C., Nam, P. T., & Seiringer, R. (2026). The
Huang–Yang formula for the low-density Fermi gas: Upper bound. Communications
on Pure and Applied Mathematics. Wiley. https://doi.org/10.1002/cpa.70040'
chicago: 'Giacomelli, Emanuela L., Christian Hainzl, Phan Thành Nam, and Robert
Seiringer. “The Huang–Yang Formula for the Low-Density Fermi Gas: Upper Bound.”
Communications on Pure and Applied Mathematics. Wiley, 2026. https://doi.org/10.1002/cpa.70040.'
ieee: 'E. L. Giacomelli, C. Hainzl, P. T. Nam, and R. Seiringer, “The Huang–Yang
formula for the low-density Fermi gas: Upper bound,” Communications on Pure
and Applied Mathematics. Wiley, 2026.'
ista: 'Giacomelli EL, Hainzl C, Nam PT, Seiringer R. 2026. The Huang–Yang formula
for the low-density Fermi gas: Upper bound. Communications on Pure and Applied
Mathematics.'
mla: 'Giacomelli, Emanuela L., et al. “The Huang–Yang Formula for the Low-Density
Fermi Gas: Upper Bound.” Communications on Pure and Applied Mathematics,
Wiley, 2026, doi:10.1002/cpa.70040.'
short: E.L. Giacomelli, C. Hainzl, P.T. Nam, R. Seiringer, Communications on Pure
and Applied Mathematics (2026).
date_created: 2026-03-22T23:04:33Z
date_published: 2026-03-13T00:00:00Z
date_updated: 2026-03-23T13:32:14Z
day: '13'
department:
- _id: RoSe
doi: 10.1002/cpa.70040
external_id:
arxiv:
- '2409.17914'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1002/cpa.70040
month: '03'
oa: 1
oa_version: Published Version
publication: Communications on Pure and Applied Mathematics
publication_identifier:
eissn:
- 1097-0312
issn:
- 0010-3640
publication_status: epub_ahead
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The Huang–Yang formula for the low-density Fermi gas: Upper bound'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21473'
abstract:
- lang: eng
text: Physical exercise acutely improves hippocampus-dependent memory. Whereas animal
studies have offered cellular- and synaptic-level accounts of these effects, human
neuroimaging studies show that exercise improves hippocampal-cortical connectivity
at the macroscale level. However, the neurophysiological basis of exercise-induced
effects on hippocampal-cortical circuits remains unknown. Experimental evidence
supports the idea that hippocampal sharp wave-ripples (SWR) play a critical role
in learning and memory. Coupling between SWRs in the hippocampus and neocortex
may reflect modulations in inter-regional connectivity required by mnemonic processes.
Here, we examine the hypothesis that exercise modulates hippocampal-cortical ripple
dynamics in the human brain. We performed intracranial recordings in epilepsy
patients undergoing pre-surgical evaluation, during awake resting state, before
and after an exercise session. Exercise increased ripple rate in the hippocampus.
Exercise also enhanced the coupling and phase-synchrony between cortical ripples
in the limbic and the default mode (DM) cortical networks and hippocampal SWRs.
Further, a higher heart rate during exercise, reflecting exercise intensity, was
related to a subsequent increase in resting state ripples across specific cortical
networks, including the DM network. These results offer the first direct evidence
that a single exercise session elicits changes in ripple events, a well-established
neurophysiological marker of mnemonic processing. The characterisation and anatomical
distribution of the described modulation points to hippocampal ripples as a potential
mechanism by which exercise elicits its reported short-term effects in cognition.
acknowledgement: We acknowledge the generosity of the patients, who contributed time
and effort to take part in this study.
article_number: fcag041
article_processing_charge: Yes
article_type: original
author:
- first_name: Araceli R.
full_name: Cardenas, Araceli R.
last_name: Cardenas
- first_name: Juan F
full_name: Ramirez Villegas, Juan F
id: 44B06F76-F248-11E8-B48F-1D18A9856A87
last_name: Ramirez Villegas
- first_name: Christopher K.
full_name: Kovach, Christopher K.
last_name: Kovach
- first_name: Phillip E.
full_name: Gander, Phillip E.
last_name: Gander
- first_name: Rachel C.
full_name: Cole, Rachel C.
last_name: Cole
- first_name: Andrew J.
full_name: Grossbach, Andrew J.
last_name: Grossbach
- first_name: Hiroto
full_name: Kawasaki, Hiroto
last_name: Kawasaki
- first_name: Jeremy D.W.
full_name: Greenlee, Jeremy D.W.
last_name: Greenlee
- first_name: Matthew A.
full_name: Howard, Matthew A.
last_name: Howard
- first_name: Kirill V.
full_name: Nourski, Kirill V.
last_name: Nourski
- first_name: Matthew I.
full_name: Banks, Matthew I.
last_name: Banks
- first_name: Michelle W.
full_name: Voss, Michelle W.
last_name: Voss
citation:
ama: Cardenas AR, Ramirez Villegas JF, Kovach CK, et al. Exercise enhances hippocampal-cortical
ripple interactions in the human brain. Brain Communications. 2026;8(2).
doi:10.1093/braincomms/fcag041
apa: Cardenas, A. R., Ramirez Villegas, J. F., Kovach, C. K., Gander, P. E., Cole,
R. C., Grossbach, A. J., … Voss, M. W. (2026). Exercise enhances hippocampal-cortical
ripple interactions in the human brain. Brain Communications. Oxford University
Press. https://doi.org/10.1093/braincomms/fcag041
chicago: Cardenas, Araceli R., Juan F Ramirez Villegas, Christopher K. Kovach, Phillip
E. Gander, Rachel C. Cole, Andrew J. Grossbach, Hiroto Kawasaki, et al. “Exercise
Enhances Hippocampal-Cortical Ripple Interactions in the Human Brain.” Brain
Communications. Oxford University Press, 2026. https://doi.org/10.1093/braincomms/fcag041.
ieee: A. R. Cardenas et al., “Exercise enhances hippocampal-cortical ripple
interactions in the human brain,” Brain Communications, vol. 8, no. 2.
Oxford University Press, 2026.
ista: Cardenas AR, Ramirez Villegas JF, Kovach CK, Gander PE, Cole RC, Grossbach
AJ, Kawasaki H, Greenlee JDW, Howard MA, Nourski KV, Banks MI, Voss MW. 2026.
Exercise enhances hippocampal-cortical ripple interactions in the human brain.
Brain Communications. 8(2), fcag041.
mla: Cardenas, Araceli R., et al. “Exercise Enhances Hippocampal-Cortical Ripple
Interactions in the Human Brain.” Brain Communications, vol. 8, no. 2,
fcag041, Oxford University Press, 2026, doi:10.1093/braincomms/fcag041.
short: A.R. Cardenas, J.F. Ramirez Villegas, C.K. Kovach, P.E. Gander, R.C. Cole,
A.J. Grossbach, H. Kawasaki, J.D.W. Greenlee, M.A. Howard, K.V. Nourski, M.I.
Banks, M.W. Voss, Brain Communications 8 (2026).
corr_author: '1'
date_created: 2026-03-22T23:04:34Z
date_published: 2026-03-09T00:00:00Z
date_updated: 2026-03-23T14:30:47Z
day: '09'
ddc:
- '570'
department:
- _id: JoCs
doi: 10.1093/braincomms/fcag041
file:
- access_level: open_access
checksum: b5b45c16defeaf88056fc3b939bd0350
content_type: application/pdf
creator: dernst
date_created: 2026-03-23T14:27:39Z
date_updated: 2026-03-23T14:27:39Z
file_id: '21478'
file_name: 2026_BrainCommunications_Cardenas.pdf
file_size: 33974419
relation: main_file
success: 1
file_date_updated: 2026-03-23T14:27:39Z
has_accepted_license: '1'
intvolume: ' 8'
issue: '2'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
publication: Brain Communications
publication_identifier:
eissn:
- 2632-1297
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Exercise enhances hippocampal-cortical ripple interactions in the human brain
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: '2026'
...
---
OA_place: publisher
OA_type: hybrid
_id: '21471'
acknowledgement: We thank the Barton group at the Institute of Scienceand Technology
Austria for many fruitful conversationsthat triggered the germination of the ideas
and questions discussed here. N. H. Barton, P. Surendranadh, A. Pal,Z. Mérai, and
two anonymous reviewers provided useful comments on the manuscript.
article_number: e70175
article_processing_charge: No
article_type: letter_note
author:
- first_name: Sofia Maria
full_name: Backlund, Sofia Maria
id: a19ed178-1337-11ed-9389-c30ab879a82a
last_name: Backlund
- first_name: Sean
full_name: Stankowski, Sean
id: 43161670-5719-11EA-8025-FABC3DDC885E
last_name: Stankowski
- first_name: Rosina Matilde
full_name: Soler Schaller, Rosina Matilde
id: 9e668447-8c32-11ed-b0c7-8dc2d7b80803
last_name: Soler Schaller
citation:
ama: 'Backlund SM, Stankowski S, Soler Schaller RM. Seeds as space-time travelers:
How does evolution balance the joint benefits and trade-offs of dormancy and dispersal?
American Journal of Botany. 2026;113(3). doi:10.1002/ajb2.70175'
apa: 'Backlund, S. M., Stankowski, S., & Soler Schaller, R. M. (2026). Seeds
as space-time travelers: How does evolution balance the joint benefits and trade-offs
of dormancy and dispersal? American Journal of Botany. Wiley. https://doi.org/10.1002/ajb2.70175'
chicago: 'Backlund, Sofia Maria, Sean Stankowski, and Rosina Matilde Soler Schaller.
“Seeds as Space-Time Travelers: How Does Evolution Balance the Joint Benefits
and Trade-Offs of Dormancy and Dispersal?” American Journal of Botany.
Wiley, 2026. https://doi.org/10.1002/ajb2.70175.'
ieee: 'S. M. Backlund, S. Stankowski, and R. M. Soler Schaller, “Seeds as space-time
travelers: How does evolution balance the joint benefits and trade-offs of dormancy
and dispersal?,” American Journal of Botany, vol. 113, no. 3. Wiley, 2026.'
ista: 'Backlund SM, Stankowski S, Soler Schaller RM. 2026. Seeds as space-time travelers:
How does evolution balance the joint benefits and trade-offs of dormancy and dispersal?
American Journal of Botany. 113(3), e70175.'
mla: 'Backlund, Sofia Maria, et al. “Seeds as Space-Time Travelers: How Does Evolution
Balance the Joint Benefits and Trade-Offs of Dormancy and Dispersal?” American
Journal of Botany, vol. 113, no. 3, e70175, Wiley, 2026, doi:10.1002/ajb2.70175.'
short: S.M. Backlund, S. Stankowski, R.M. Soler Schaller, American Journal of Botany
113 (2026).
corr_author: '1'
date_created: 2026-03-22T23:04:33Z
date_published: 2026-03-11T00:00:00Z
date_updated: 2026-03-23T14:47:52Z
day: '11'
ddc:
- '580'
- '570'
department:
- _id: NiBa
- _id: GradSch
doi: 10.1002/ajb2.70175
external_id:
pmid:
- '41814642'
file:
- access_level: open_access
checksum: 6116108a12c4a5cc91fc653d67885309
content_type: application/pdf
creator: dernst
date_created: 2026-03-23T14:01:44Z
date_updated: 2026-03-23T14:01:44Z
file_id: '21477'
file_name: 2026_AmericanJourBotany_Backlund.pdf
file_size: 495080
relation: main_file
success: 1
file_date_updated: 2026-03-23T14:01:44Z
has_accepted_license: '1'
intvolume: ' 113'
issue: '3'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
pmid: 1
publication: American Journal of Botany
publication_identifier:
eissn:
- 1537-2197
issn:
- 0002-9122
publication_status: published
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Seeds as space-time travelers: How does evolution balance the joint benefits
and trade-offs of dormancy and dispersal?'
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: 113
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '21481'
abstract:
- lang: eng
text: 'The Hα emission line in galaxies is a powerful tracer of their recent star
formation activity. With the advent of JWST, we are now able to routinely observe
Hα in galaxies at high redshift (z ≳ 3) and thus measure their star formation
rates (SFRs). However, using classical SFR(Hα) calibrations to derive the SFRs
leads to biased results because high-redshift galaxies are commonly characterized
by low metallicities and bursty star formation histories, affecting the conversion
factor between the Hα luminosity (LHα) and the SFR. We developed a set of new
SFR(Hα) calibrations that allowed us to predict the SFRs of Hα-emitters at z ≳ 3
with very little error. We used the SPHINX cosmological simulations to select
a sample of star-forming galaxies representative of the Hα-emitter population
observed with JWST. We then derived linear corrections to the classical SFR(Hα)
calibrations that took variations in the physical properties (e.g., stellar metallicities)
among individual galaxies into account. We obtained two new SFR(Hα) calibrations
that compared to the classical calibrations reduce the root mean squared error
(RMSE) in the predicted SFRs by ΔRMSE ≈ 0.04 dex and ΔRMSE ≈ 0.06 dex, respectively.
Using the recent JWST NIRCam/grism observations of Hα-emitters at z ∼ 6, we show
that the new calibrations affect the high-redshift galaxy population statistics:
(i) the estimated cosmic SFR density decreases by ΔρSFR ≈ 12%, and (ii) the observed
slope of the star formation main sequence increases by Δ∂logSFR/∂logM★ = 0.08 ± 0.02.'
acknowledgement: "We thank the anonymous referee for the insightful comments that
helped improve the manuscript. We also thank Thibault Garel, Pascal Oesch, Irene
Shivaei, Charlotte Simmonds, Andrew Hopkins, Daniel Schaerer, and Rashmi Gottumukkala
for useful comments and productive discussions. We gratefully acknowledge support
from the CBPsmn (PSMN, Pôle Scientifique de Modélisation Numérique) of the ENS de
Lyon for the computing resources.\r\nFunded by the European Union (ERC, AGENTS,
101076224). Views and opinions expressed are however those of the author(s) only
and do not necessarily reflect those of the European Union or the European Research
Council. Neither the European Union nor the granting authority can be held responsible
for them. This work made extensive use of several open-source software packages,
and we gratefully acknowledge the efforts of their authors: numpy (Harris et al.
2020), astropy (Astropy Collaboration 2022), matplotlib (Hunter 2007), ipython (Perez
& Granger 2007), and scikit-learn (Pedregosa et al. 2011)."
article_number: A184
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Ivan
full_name: Kramarenko, Ivan
id: 9a9394cb-3200-11ee-973b-f5ba2a8b16e4
last_name: Kramarenko
orcid: 0000-0001-5346-6048
- first_name: J.
full_name: Rosdahl, J.
last_name: Rosdahl
- first_name: J.
full_name: Blaizot, J.
last_name: Blaizot
- 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: H.
full_name: Katz, H.
last_name: Katz
- first_name: Claudia
full_name: Di Cesare, Claudia
id: 2d002343-372f-11ef-98ec-a164d20427cb
last_name: Di Cesare
citation:
ama: Kramarenko I, Rosdahl J, Blaizot J, Matthee JJ, Katz H, Di Cesare C. H α as
a tracer of star formation in the SPHINX cosmological simulations. Astronomy
& Astrophysics. 2026;707. doi:10.1051/0004-6361/202557114
apa: Kramarenko, I., Rosdahl, J., Blaizot, J., Matthee, J. J., Katz, H., & Di
Cesare, C. (2026). H α as a tracer of star formation in the SPHINX cosmological
simulations. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202557114
chicago: Kramarenko, Ivan, J. Rosdahl, J. Blaizot, Jorryt J Matthee, H. Katz, and
Claudia Di Cesare. “H α as a Tracer of Star Formation in the SPHINX Cosmological
Simulations.” Astronomy & Astrophysics. EDP Sciences, 2026. https://doi.org/10.1051/0004-6361/202557114.
ieee: I. Kramarenko, J. Rosdahl, J. Blaizot, J. J. Matthee, H. Katz, and C. Di Cesare,
“H α as a tracer of star formation in the SPHINX cosmological simulations,” Astronomy
& Astrophysics, vol. 707. EDP Sciences, 2026.
ista: Kramarenko I, Rosdahl J, Blaizot J, Matthee JJ, Katz H, Di Cesare C. 2026.
H α as a tracer of star formation in the SPHINX cosmological simulations. Astronomy
& Astrophysics. 707, A184.
mla: Kramarenko, Ivan, et al. “H α as a Tracer of Star Formation in the SPHINX Cosmological
Simulations.” Astronomy & Astrophysics, vol. 707, A184, EDP Sciences,
2026, doi:10.1051/0004-6361/202557114.
short: I. Kramarenko, J. Rosdahl, J. Blaizot, J.J. Matthee, H. Katz, C. Di Cesare,
Astronomy & Astrophysics 707 (2026).
corr_author: '1'
date_created: 2026-03-23T14:58:03Z
date_published: 2026-03-05T00:00:00Z
date_updated: 2026-03-23T15:46:31Z
day: '05'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202557114
external_id:
arxiv:
- '2509.05403'
file:
- access_level: open_access
checksum: 7429076b381dd498084f40ffd199e714
content_type: application/pdf
creator: dernst
date_created: 2026-03-23T15:44:09Z
date_updated: 2026-03-23T15:44:09Z
file_id: '21492'
file_name: 2026_AstronomyAstrophysics_Kramarenko.pdf
file_size: 904565
relation: main_file
success: 1
file_date_updated: 2026-03-23T15:44:09Z
has_accepted_license: '1'
intvolume: ' 707'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
grant_number: '101076224'
name: Young galaxies as tracers and agents of cosmic reionization
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
status: public
title: H α as a tracer of star formation in the SPHINX cosmological simulations
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: 707
year: '2026'
...