---
OA_place: repository
OA_type: green
_id: '19067'
abstract:
- lang: eng
text: Modern experimental methods enable the creation of self-assembly building
blocks with tunable interactions, but optimally exploiting this tunability for
the self-assembly of desired structures remains an important challenge. Many studies
of this inverse problem start with the so-called fully addressable limit, where
every particle in a target structure is different. This leads to clear design
principles that often result in high assembly yield, but it is not a scalable
approach—at some point, one must grapple with “reusing” building blocks, which
lowers the degree of addressability and may cause a multitude of off-target structures
to form, complicating the design process. Here, we solve a key obstacle preventing
robust inverse design in the “semiaddressable regime” by developing a highly efficient
algorithm that enumerates all structures that can be formed from a given set of
building blocks. By combining this with established partition-function-based yield
calculations, we show that it is almost always possible to find economical semiaddressable
designs where the entropic gain from reusing building blocks outweighs the presence
of off-target structures and even increases the yield of the target. Thus, not
only does our enumeration algorithm enable robust and scalable inverse design
in the semiaddressable regime, our results demonstrate that it is possible to
operate in this regime while maintaining the level of control often associated
with full addressability.
acknowledgement: We thank Daichi Hayakawa, Thomas E. Videbæk, and W. Benjamin Rogers
for important discussions and Jérémie Palacci, Anđela Šarić, and Scott Waitukaitis
for helpful comments on the manuscript. The research was supported by the Gesellschaft
für Forschungsförderung Niederösterreich under Project No. FTI23-G-011.
article_number: '058204'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Maximilian
full_name: Hübl, Maximilian
id: 5eb8629e-15b2-11ec-abd3-e6f3e5e01f32
last_name: Hübl
- first_name: Carl Peter
full_name: Goodrich, Carl Peter
id: EB352CD2-F68A-11E9-89C5-A432E6697425
last_name: Goodrich
orcid: 0000-0002-1307-5074
citation:
ama: Hübl M, Goodrich CP. Accessing semiaddressable self-assembly with efficient
structure enumeration. Physical Review Letters. 2025;134(5). doi:10.1103/PhysRevLett.134.058204
apa: Hübl, M., & Goodrich, C. P. (2025). Accessing semiaddressable self-assembly
with efficient structure enumeration. Physical Review Letters. American
Physical Society. https://doi.org/10.1103/PhysRevLett.134.058204
chicago: Hübl, Maximilian, and Carl Peter Goodrich. “Accessing Semiaddressable Self-Assembly
with Efficient Structure Enumeration.” Physical Review Letters. American
Physical Society, 2025. https://doi.org/10.1103/PhysRevLett.134.058204.
ieee: M. Hübl and C. P. Goodrich, “Accessing semiaddressable self-assembly with
efficient structure enumeration,” Physical Review Letters, vol. 134, no.
5. American Physical Society, 2025.
ista: Hübl M, Goodrich CP. 2025. Accessing semiaddressable self-assembly with efficient
structure enumeration. Physical Review Letters. 134(5), 058204.
mla: Hübl, Maximilian, and Carl Peter Goodrich. “Accessing Semiaddressable Self-Assembly
with Efficient Structure Enumeration.” Physical Review Letters, vol. 134,
no. 5, 058204, American Physical Society, 2025, doi:10.1103/PhysRevLett.134.058204.
short: M. Hübl, C.P. Goodrich, Physical Review Letters 134 (2025).
corr_author: '1'
date_created: 2025-02-23T23:01:55Z
date_published: 2025-02-07T00:00:00Z
date_updated: 2025-09-30T10:35:47Z
day: '07'
department:
- _id: CaGo
- _id: GradSch
doi: 10.1103/PhysRevLett.134.058204
external_id:
arxiv:
- '2405.13567'
isi:
- '001454696800003'
pmid:
- '39983190'
intvolume: ' 134'
isi: 1
issue: '5'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2405.13567
month: '02'
oa: 1
oa_version: Preprint
pmid: 1
project:
- _id: 8dd93da8-16d5-11f0-9cad-d2c70200d9a5
grant_number: FTI23-G-011
name: Dynamically reconfigurable self-assembly with triangular DNA-origami bricks
publication: Physical Review Letters
publication_identifier:
eissn:
- 1079-7114
issn:
- 0031-9007
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
related_material:
link:
- relation: software
url: https://github.com/mxhbl/Roly.jl
scopus_import: '1'
status: public
title: Accessing semiaddressable self-assembly with efficient structure enumeration
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 134
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19068'
abstract:
- lang: eng
text: Whether or not the neuron emits a spike in response to stimulation by an excitatory
current pulse is determined by a strength-duration curve (SDC) for the pulse parameters.
The SDC is a dependence of the minimal pulse amplitude required to elicit the
spiking response on either the pulse duration or its decay time. Excitatory neurons
affect the others through pulses of excitatory postsynaptic current. A simple
yet plausible approximation for the time course of such a pulse is the alpha function,
with linear rise at the start and exponential decay at the end. However, an exact
analytical SDC for this case is hitherto not known, even for the leaky integrate-and-fire
(LIF) neuron, the simplest spiking neuron model used in practice. We have obtained
general SDC equations for the LIF neuron. Using the Lambert W function — a widely-implemented
special function, we have found the exact analytical SDC for the spiking response
of the LIF neuron stimulated by an excitatory current pulse in the form of the
alpha function. To compare results in a unified way, we have also derived the
analytical SDCs for (i) rectangular pulse, (ii) ascending ramp pulse, and (iii)
instantly rising and exponentially decaying pulse. In the limit of no leakage,
we show that the SDC is reduced to the classical hyperbola for all considered
cases.
acknowledgement: "The author thanks T.S. Zemskova and N.D. Efimova for verifying some
of the results. This work was supported by a European Research Council Consolidator
Grant (SYNAPSEEK, 819603, to Tim P. Vogels).\r\nThe Supplementary Material for this
article contains (i) the data for graphs in Figure 1 and (ii) ready-to-use MATLAB
codes for reproducing the data. It is available online at https://doi.org/10.6084/m9.figshare.24081849."
article_number: '100548'
article_processing_charge: Yes
article_type: original
author:
- first_name: Alexander
full_name: Paraskevov, Alexander
id: d05e3c56-9262-11ed-9231-be692464e5ac
last_name: Paraskevov
citation:
ama: Paraskevov A. Analytical strength-duration curve for the spiking response of
the LIF neuron to an alpha-function-shaped excitatory current pulse. Results
in Applied Mathematics. 2025;25. doi:10.1016/j.rinam.2025.100548
apa: Paraskevov, A. (2025). Analytical strength-duration curve for the spiking response
of the LIF neuron to an alpha-function-shaped excitatory current pulse. Results
in Applied Mathematics. Elsevier. https://doi.org/10.1016/j.rinam.2025.100548
chicago: Paraskevov, Alexander. “Analytical Strength-Duration Curve for the Spiking
Response of the LIF Neuron to an Alpha-Function-Shaped Excitatory Current Pulse.”
Results in Applied Mathematics. Elsevier, 2025. https://doi.org/10.1016/j.rinam.2025.100548.
ieee: A. Paraskevov, “Analytical strength-duration curve for the spiking response
of the LIF neuron to an alpha-function-shaped excitatory current pulse,” Results
in Applied Mathematics, vol. 25. Elsevier, 2025.
ista: Paraskevov A. 2025. Analytical strength-duration curve for the spiking response
of the LIF neuron to an alpha-function-shaped excitatory current pulse. Results
in Applied Mathematics. 25, 100548.
mla: Paraskevov, Alexander. “Analytical Strength-Duration Curve for the Spiking
Response of the LIF Neuron to an Alpha-Function-Shaped Excitatory Current Pulse.”
Results in Applied Mathematics, vol. 25, 100548, Elsevier, 2025, doi:10.1016/j.rinam.2025.100548.
short: A. Paraskevov, Results in Applied Mathematics 25 (2025).
corr_author: '1'
date_created: 2025-02-23T23:01:55Z
date_published: 2025-02-01T00:00:00Z
date_updated: 2025-04-14T07:54:31Z
day: '01'
ddc:
- '570'
- '510'
department:
- _id: TiVo
doi: 10.1016/j.rinam.2025.100548
ec_funded: 1
file:
- access_level: open_access
checksum: 58fd02e951857859f39d06661a27bcc9
content_type: application/pdf
creator: dernst
date_created: 2025-02-24T13:18:47Z
date_updated: 2025-02-24T13:18:47Z
file_id: '19083'
file_name: 2025_ResultsApplMath_Paraskevov.pdf
file_size: 853322
relation: main_file
success: 1
file_date_updated: 2025-02-24T13:18:47Z
has_accepted_license: '1'
intvolume: ' 25'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
project:
- _id: 0aacfa84-070f-11eb-9043-d7eb2c709234
call_identifier: H2020
grant_number: '819603'
name: Learning the shape of synaptic plasticity rules for neuronal architectures
and function through machine learning.
publication: Results in Applied Mathematics
publication_identifier:
eissn:
- 2590-0374
publication_status: published
publisher: Elsevier
related_material:
link:
- relation: software
url: https://doi.org/10.6084/m9.figshare.24081849
scopus_import: '1'
status: public
title: Analytical strength-duration curve for the spiking response of the LIF neuron
to an alpha-function-shaped excitatory current pulse
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: 25
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19069'
abstract:
- lang: eng
text: "Context. The hydrogen Lyman-alpha (Lyα) line, the brightest rest-frame ultraviolet
line of high-redshift galaxies, exhibits a large variety of shapes, which is due
to factors at different scales, from the interstellar medium to the intergalactic
medium (IGM).\r\nAims. The aim of this work is to provide a systematic inventory
and classification of the spectral shapes of Lyα emission lines to better understand
the general population of high-redshift Lyα emitting galaxies (LAEs).\r\nMethods.
Using the unprecedentedly deep data from the MUSE eXtremely Deep Field (MXDF;
up to 140 hour exposure time), we selected 477 galaxies observed in the ∼2.8−6.6
redshift range, 15 of which have a systemic redshift from nebular lines. We developed
a method to classify Lyα emission lines in four spectral and three spatial categories
by combining a pure spectral analysis with a narrow-band image analysis. We measured
spectral properties, such as the peak separation and the blue-to-total flux ratio
for the double-peaked galaxies.\r\nResults. To ensure a robust sample for statistical
analysis, we define two unbiased subsets, inclusive and restrictive, by applying
thresholds for signal-to-noise ratio, peak separation, and Lyα luminosity, yielding
a final unbiased sample of 206 galaxies. Our analysis reveals that between 32%
and 51% of the galaxies exhibit double-peaked profiles, with peak separations
ranging from 150 km s−1 to nearly 1600 km s−1. The fraction of double-peaked galaxies
seems to evolve dependently with the Lyα luminosity, while we do not see a severe
decrease in this fraction with redshift, which is expected given the IGM attenuation
at high redshift. An artificial increase in the number of double-peaked galaxies
at the highest redshifts may cause the observation of a plateau instead of a decrease.
A notable number of these double-peaked profiles show blue-dominated spectra,
suggesting unique gas dynamics and inflow characteristics in some high-redshift
galaxies. The consequent fraction of blue-dominated spectra needs to be confirmed
by obtaining new systemic redshift measurements. Among the double-peaked galaxies,
4% are spurious detections, that is, the blue and red peaks do not come from the
same spatial location. Around 20% out of the 477 sources of the parent sample
lie in a complex environment, meaning there are other clumps or galaxies at the
same redshift within a distance of 30 kpc.\r\nConclusions. Our results suggest
that the double-peaked LAE fraction may trace the evolution of IGM attenuation,
but the faintest galaxies must be observed at high redshift. We also need more
data to confirm the trend seen at low redshift. In addition, it is crucial to
obtain secure systemic redshifts for LAEs to better constrain the nature of the
Lyα double-peaked lines. Statistical samples of double-peaked and triple-peaked
galaxies are a promising probe of the evolution of the physical properties of
galaxies across cosmic time."
acknowledgement: 'EV and AV acknowledges the support from the SNF grants PP00P2 176808
and 211023. HK acknowledges support from Japan Society for the Promotion of Science
(JSPS) Overseas Research Fellowship as well as JSPS Research Fellowships for Young
Scientists. JP acknowledges funding by the Deutsche Forschungsgemeinschaft, Grant
Wi 1369/31-1. This work is based on observations taken by VLT, which is operated
by European Southern Observatory. This research made use of ASTROPY, which is a
community-developed core Python package for Astronomy (Astropy Collaboration 2013,
2018, 2022), and other software and packages: MPDAF (Piqueras et al. 2019), PHOTUTILS
(Bradley 2023), NUMPY (van der Walt et al. 2011), SCIPY (Virtanen et al. 2020).
The plots in this paper were created using MATPLOTLIB (Hunter 2007).'
article_number: A100
article_processing_charge: No
article_type: original
author:
- first_name: Eloïse
full_name: Vitte, Eloïse
last_name: Vitte
- first_name: Anne
full_name: Verhamme, Anne
last_name: Verhamme
- first_name: Pascale
full_name: Hibon, Pascale
last_name: Hibon
- first_name: Floriane
full_name: Leclercq, Floriane
last_name: Leclercq
- first_name: Belén
full_name: Alcalde Pampliega, Belén
last_name: Alcalde Pampliega
- first_name: Josephine
full_name: Kerutt, Josephine
last_name: Kerutt
- first_name: Haruka
full_name: Kusakabe, Haruka
last_name: Kusakabe
- 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: Yucheng
full_name: Guo, Yucheng
last_name: Guo
- first_name: Roland
full_name: Bacon, Roland
last_name: Bacon
- first_name: Michael
full_name: Maseda, Michael
last_name: Maseda
- first_name: Johan
full_name: Richard, Johan
last_name: Richard
- first_name: John
full_name: Pharo, John
last_name: Pharo
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Leindert
full_name: Boogaard, Leindert
last_name: Boogaard
- first_name: Themiya
full_name: Nanayakkara, Themiya
last_name: Nanayakkara
- first_name: Thierry
full_name: Contini, Thierry
last_name: Contini
citation:
ama: 'Vitte E, Verhamme A, Hibon P, et al. The MUSE eXtremely Deep Field: Classifying
the spectral shapes of Ly α -emitting galaxies. Astronomy & Astrophysics.
2025;694. doi:10.1051/0004-6361/202450426'
apa: 'Vitte, E., Verhamme, A., Hibon, P., Leclercq, F., Alcalde Pampliega, B., Kerutt,
J., … Contini, T. (2025). The MUSE eXtremely Deep Field: Classifying the spectral
shapes of Ly α -emitting galaxies. Astronomy & Astrophysics. EDP Sciences.
https://doi.org/10.1051/0004-6361/202450426'
chicago: 'Vitte, Eloïse, Anne Verhamme, Pascale Hibon, Floriane Leclercq, Belén
Alcalde Pampliega, Josephine Kerutt, Haruka Kusakabe, et al. “The MUSE EXtremely
Deep Field: Classifying the Spectral Shapes of Ly α -Emitting Galaxies.” Astronomy
& Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202450426.'
ieee: 'E. Vitte et al., “The MUSE eXtremely Deep Field: Classifying the spectral
shapes of Ly α -emitting galaxies,” Astronomy & Astrophysics, vol.
694. EDP Sciences, 2025.'
ista: 'Vitte E, Verhamme A, Hibon P, Leclercq F, Alcalde Pampliega B, Kerutt J,
Kusakabe H, Matthee JJ, Guo Y, Bacon R, Maseda M, Richard J, Pharo J, Schaye J,
Boogaard L, Nanayakkara T, Contini T. 2025. The MUSE eXtremely Deep Field: Classifying
the spectral shapes of Ly α -emitting galaxies. Astronomy & Astrophysics.
694, A100.'
mla: 'Vitte, Eloïse, et al. “The MUSE EXtremely Deep Field: Classifying the Spectral
Shapes of Ly α -Emitting Galaxies.” Astronomy & Astrophysics, vol.
694, A100, EDP Sciences, 2025, doi:10.1051/0004-6361/202450426.'
short: E. Vitte, A. Verhamme, P. Hibon, F. Leclercq, B. Alcalde Pampliega, J. Kerutt,
H. Kusakabe, J.J. Matthee, Y. Guo, R. Bacon, M. Maseda, J. Richard, J. Pharo,
J. Schaye, L. Boogaard, T. Nanayakkara, T. Contini, Astronomy & Astrophysics
694 (2025).
date_created: 2025-02-23T23:01:56Z
date_published: 2025-02-01T00:00:00Z
date_updated: 2026-02-16T12:08:40Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202450426
external_id:
isi:
- '001417357000009'
file:
- access_level: open_access
checksum: ed2a5bba313e54ed250be348bd8c1d95
content_type: application/pdf
creator: dernst
date_created: 2025-02-25T07:19:34Z
date_updated: 2025-02-25T07:19:34Z
file_id: '19087'
file_name: 2025_AstronomyAstrophysics_Vitte.pdf
file_size: 3444203
relation: main_file
success: 1
file_date_updated: 2025-02-25T07:19:34Z
has_accepted_license: '1'
intvolume: ' 694'
isi: 1
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
issnl:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The MUSE eXtremely Deep Field: Classifying the spectral shapes of Ly α -emitting
galaxies'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 694
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '19070'
abstract:
- lang: eng
text: "Context. Recent observations suggest a significant and rapid buildup of dust
in galaxies at high redshift (z > 4); this presents new challenges to our understanding
of galaxy formation in the early Universe. Although our understanding of the physics
of dust production and destruction in a galaxy’s interstellar medium (ISM) is
improving, investigating the baryonic processes in the early universe remains
a complex task owing to the inherent degeneracies in cosmological simulations
and chemical evolution models.\r\nAims. In this work we characterized the evolution
of 98 z ∼ 5 star-forming galaxies observed as part of the ALMA Large Program ALPINE
by constraining the physical processes underpinning the gas and dust production,
consumption, and destruction in their ISM.\r\nMethods. We made use of chemical
evolution models to simultaneously reproduce the observed dust and gas content
of our galaxies, obtained respectively from spectral energy distribution (SED)
fitting and ionized carbon measurements. For each galaxy we constrained the initial
gas mass, gas inflows and outflows, and efficiencies of dust growth and destruction.
We tested these models with both the canonical Chabrier and a top-heavy initial
mass function (IMF); the latter allowed rapid dust production on shorter timescales.\r\nResults.
We successfully reproduced the gas and dust content in most of the older galaxies
(≳600 Myr) regardless of the assumed IMF, predicting dust production primarily
through Type II supernovae (SNe) and no dust growth in the ISM, as well as moderate
inflow of primordial gas. In the case of intermediate-age galaxies (300−600 Myr),
we reproduced the gas and dust content through Type II SNe and dust growth in
ISM, though we observed an overprediction of dust mass in older galaxies, potentially
indicating an unaccounted dust destruction mechanism and/or an overestimation
of the observed dust masses. The number of young galaxies (≲300 Myr) reproduced,
increases for models assuming top-heavy IMF but with maximal prescriptions of
dust production. Galactic outflows are required (up to a mass-loading factor of
2) to reproduce the observed gas and dust mass, and to recover the decreasing
trend of gas and dust over stellar mass with age. Assuming the Chabrier IMF, models
are able to reproduce ∼65% of the total sample, while with top-heavy IMF the fraction
increases to ∼93%, alleviating the tension between the observations and the models.
Observations from the James Webb Space Telescope (JWST) will allow us to remove
degeneracies in the diverse intrinsic properties of these galaxies (e.g., star
formation histories and metallicity), thereby refining our models."
acknowledgement: 'We warmly thank the referee for her/his useful comments and suggestions
that greatly improved the quality of our paper. P.S., A.N., and M.R. acknowledge
support from the Narodowe Centrum Nauki (UMO2020/38/E/ST9/00077). M.R. acknowledges
support from the Foundation for Polish Science (FNP) under the program START 063.2023.
D.D. acknowledges support from the National Science Center (NCN) grant SONATA (UMO2020/39/D/ST9/00720).
J. and K.M. are grateful for the support from the Polish National Science Centre
via grant UMO-018/30/E/ST9/00082. J. acknowledges support from the European Union
(MSCA EDUCADO, GA 101119830 and WIDERA ExGal-Twin, GA 101158446). M.B. gratefully
acknowledges support from the ANID BASAL project FB210003 and from the FONDECYT
regular grant 1211000. This work was supported by the French government through
the France 2030 investment plan managed by the National Research Agency (ANR), as
part of the Initiative of Excellence of Université Côte d’Azur under reference number
ANR-15-IDEX-01. M.H. acknowledges support from the Polish National Science Center
(UMO-2022/45/N/ST9/01336). E.I. acknowledges funding by ANID FONDECYT Regular 1221846.
G.E.M. acknowledges the Villum Fonden research grant 13160 “Gas to stars, stars
to dust: tracing star formation across cosmic time”, grant 37440, “The Hidden Cosmos”,
and the Cosmic Dawn Center of Excellence funded by the Danish National Research
Foundation under the grant No. 140.'
article_number: A82
article_processing_charge: Yes
article_type: original
author:
- first_name: P.
full_name: Sawant, P.
last_name: Sawant
- first_name: A.
full_name: Nanni, A.
last_name: Nanni
- first_name: M.
full_name: Romano, M.
last_name: Romano
- first_name: D.
full_name: Donevski, D.
last_name: Donevski
- first_name: G.
full_name: Bruzual, G.
last_name: Bruzual
- first_name: N.
full_name: Ysard, N.
last_name: Ysard
- first_name: B. C.
full_name: Lemaux, B. C.
last_name: Lemaux
- first_name: H.
full_name: Inami, H.
last_name: Inami
- first_name: F.
full_name: Calura, F.
last_name: Calura
- first_name: F.
full_name: Pozzi, F.
last_name: Pozzi
- first_name: K.
full_name: Małek, K.
last_name: Małek
- first_name: J.
full_name: Junais, J.
last_name: Junais
- first_name: M.
full_name: Boquien, M.
last_name: Boquien
- first_name: A. L.
full_name: Faisst, A. L.
last_name: Faisst
- first_name: M.
full_name: Hamed, M.
last_name: Hamed
- first_name: M.
full_name: Ginolfi, M.
last_name: Ginolfi
- first_name: G.
full_name: Zamorani, G.
last_name: Zamorani
- first_name: G.
full_name: Lorenzon, G.
last_name: Lorenzon
- first_name: J.
full_name: Molina, J.
last_name: Molina
- first_name: S.
full_name: Bardelli, S.
last_name: Bardelli
- first_name: E.
full_name: Ibar, E.
last_name: Ibar
- first_name: D.
full_name: Vergani, D.
last_name: Vergani
- first_name: Claudia
full_name: Di Cesare, Claudia
id: 2d002343-372f-11ef-98ec-a164d20427cb
last_name: Di Cesare
- first_name: M.
full_name: Béthermin, M.
last_name: Béthermin
- first_name: D.
full_name: Burgarella, D.
last_name: Burgarella
- first_name: P.
full_name: Cassata, P.
last_name: Cassata
- first_name: M.
full_name: Dessauges-Zavadsky, M.
last_name: Dessauges-Zavadsky
- first_name: E.
full_name: D'Onghia, E.
last_name: D'Onghia
- first_name: Y.
full_name: Dubois, Y.
last_name: Dubois
- first_name: G. E.
full_name: Magdis, G. E.
last_name: Magdis
- first_name: H.
full_name: Mendez-Hernandez, H.
last_name: Mendez-Hernandez
citation:
ama: 'Sawant P, Nanni A, Romano M, et al. The ALPINE-ALMA [CII] survey: Unveiling
the baryon evolution in the interstellar medium of z ∼ 5 star-forming galaxies.
Astronomy & Astrophysics. 2025;694. doi:10.1051/0004-6361/202451542'
apa: 'Sawant, P., Nanni, A., Romano, M., Donevski, D., Bruzual, G., Ysard, N., …
Mendez-Hernandez, H. (2025). The ALPINE-ALMA [CII] survey: Unveiling the baryon
evolution in the interstellar medium of z ∼ 5 star-forming galaxies. Astronomy
& Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202451542'
chicago: 'Sawant, P., A. Nanni, M. Romano, D. Donevski, G. Bruzual, N. Ysard, B.
C. Lemaux, et al. “The ALPINE-ALMA [CII] Survey: Unveiling the Baryon Evolution
in the Interstellar Medium of z ∼ 5 Star-Forming Galaxies.” Astronomy &
Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202451542.'
ieee: 'P. Sawant et al., “The ALPINE-ALMA [CII] survey: Unveiling the baryon
evolution in the interstellar medium of z ∼ 5 star-forming galaxies,” Astronomy
& Astrophysics, vol. 694. EDP Sciences, 2025.'
ista: 'Sawant P, Nanni A, Romano M, Donevski D, Bruzual G, Ysard N, Lemaux BC, Inami
H, Calura F, Pozzi F, Małek K, Junais J, Boquien M, Faisst AL, Hamed M, Ginolfi
M, Zamorani G, Lorenzon G, Molina J, Bardelli S, Ibar E, Vergani D, Di Cesare
C, Béthermin M, Burgarella D, Cassata P, Dessauges-Zavadsky M, D’Onghia E, Dubois
Y, Magdis GE, Mendez-Hernandez H. 2025. The ALPINE-ALMA [CII] survey: Unveiling
the baryon evolution in the interstellar medium of z ∼ 5 star-forming galaxies.
Astronomy & Astrophysics. 694, A82.'
mla: 'Sawant, P., et al. “The ALPINE-ALMA [CII] Survey: Unveiling the Baryon Evolution
in the Interstellar Medium of z ∼ 5 Star-Forming Galaxies.” Astronomy &
Astrophysics, vol. 694, A82, EDP Sciences, 2025, doi:10.1051/0004-6361/202451542.'
short: P. Sawant, A. Nanni, M. Romano, D. Donevski, G. Bruzual, N. Ysard, B.C. Lemaux,
H. Inami, F. Calura, F. Pozzi, K. Małek, J. Junais, M. Boquien, A.L. Faisst, M.
Hamed, M. Ginolfi, G. Zamorani, G. Lorenzon, J. Molina, S. Bardelli, E. Ibar,
D. Vergani, C. Di Cesare, M. Béthermin, D. Burgarella, P. Cassata, M. Dessauges-Zavadsky,
E. D’Onghia, Y. Dubois, G.E. Magdis, H. Mendez-Hernandez, Astronomy & Astrophysics
694 (2025).
date_created: 2025-02-23T23:01:56Z
date_published: 2025-02-01T00:00:00Z
date_updated: 2026-02-16T12:08:24Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202451542
external_id:
isi:
- '001414753300028'
file:
- access_level: open_access
checksum: 792cbcda14148c352dc8c5a26058827d
content_type: application/pdf
creator: dernst
date_created: 2025-02-25T07:05:19Z
date_updated: 2025-02-25T07:05:19Z
file_id: '19086'
file_name: 2025_AstronomyAstrophysics_Sawant.pdf
file_size: 7624067
relation: main_file
success: 1
file_date_updated: 2025-02-25T07:05:19Z
has_accepted_license: '1'
intvolume: ' 694'
isi: 1
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The ALPINE-ALMA [CII] survey: Unveiling the baryon evolution in the interstellar
medium of z ∼ 5 star-forming galaxies'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 694
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19071'
abstract:
- lang: eng
text: "An action of a complex reductive group G on a smooth projective variety X
is regular when all regular unipotent elements in G act with finitely many fixed
points. Then the complex G\r\n-equivariant cohomology ring of X is isomorphic
to the coordinate ring of a certain regular fixed point scheme. Examples include
partial flag varieties, smooth Schubert varieties and Bott-Samelson varieties.
We also show that a more general version of the fixed point scheme allows a generalisation
to GKM spaces, such as toric varieties."
acknowledgement: 'The first author was supported by an FWF grant “Geometry of the
top of the nilpotent cone” number P 35847. The second author was supported by an
Austrian Academy of Sciences DOC Fellowship “Topology of open smooth varieties with
a torus action”. '
article_number: '1'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Tamás
full_name: Hausel, Tamás
id: 4A0666D8-F248-11E8-B48F-1D18A9856A87
last_name: Hausel
orcid: 0000-0002-9582-2634
- first_name: Kamil P
full_name: Rychlewicz, Kamil P
id: 85A07246-A8BF-11E9-B4FA-D9E3E5697425
last_name: Rychlewicz
citation:
ama: Hausel T, Rychlewicz KP. Spectrum of equivariant cohomology as a fixed point
scheme. Epijournal de Geometrie Algebrique. 2025;9. doi:10.46298/epiga.2025.12591
apa: Hausel, T., & Rychlewicz, K. P. (2025). Spectrum of equivariant cohomology
as a fixed point scheme. Epijournal de Geometrie Algebrique. EPI Sciences.
https://doi.org/10.46298/epiga.2025.12591
chicago: Hausel, Tamás, and Kamil P Rychlewicz. “Spectrum of Equivariant Cohomology
as a Fixed Point Scheme.” Epijournal de Geometrie Algebrique. EPI Sciences,
2025. https://doi.org/10.46298/epiga.2025.12591.
ieee: T. Hausel and K. P. Rychlewicz, “Spectrum of equivariant cohomology as a fixed
point scheme,” Epijournal de Geometrie Algebrique, vol. 9. EPI Sciences,
2025.
ista: Hausel T, Rychlewicz KP. 2025. Spectrum of equivariant cohomology as a fixed
point scheme. Epijournal de Geometrie Algebrique. 9, 1.
mla: Hausel, Tamás, and Kamil P. Rychlewicz. “Spectrum of Equivariant Cohomology
as a Fixed Point Scheme.” Epijournal de Geometrie Algebrique, vol. 9, 1,
EPI Sciences, 2025, doi:10.46298/epiga.2025.12591.
short: T. Hausel, K.P. Rychlewicz, Epijournal de Geometrie Algebrique 9 (2025).
corr_author: '1'
date_created: 2025-02-23T23:01:56Z
date_published: 2025-02-03T00:00:00Z
date_updated: 2025-04-15T06:31:58Z
day: '03'
ddc:
- '510'
department:
- _id: TaHa
doi: 10.46298/epiga.2025.12591
external_id:
arxiv:
- '2212.11836'
file:
- access_level: open_access
checksum: 3915c6f117461502f7103878460428df
content_type: application/pdf
creator: dernst
date_created: 2025-02-25T06:53:27Z
date_updated: 2025-02-25T06:53:27Z
file_id: '19085'
file_name: 2025_Epiga_Hausel.pdf
file_size: 3276395
relation: main_file
success: 1
file_date_updated: 2025-02-25T06:53:27Z
has_accepted_license: '1'
intvolume: ' 9'
language:
- iso: eng
license: https://creativecommons.org/licenses/by-sa/4.0/
month: '02'
oa: 1
oa_version: Published Version
project:
- _id: 34b2c9cb-11ca-11ed-8bc3-a50ba74ca4a3
grant_number: P35847
name: Geometry of the tip of the global nilpotent cone
- _id: 34cd0f74-11ca-11ed-8bc3-bf0492a14a24
grant_number: '26525'
name: Topology of open smooth varieties with a torus action
publication: Epijournal de Geometrie Algebrique
publication_identifier:
eissn:
- 2491-6765
publication_status: published
publisher: EPI Sciences
quality_controlled: '1'
related_material:
record:
- id: '17157'
relation: earlier_version
status: public
scopus_import: '1'
status: public
title: Spectrum of equivariant cohomology as a fixed point scheme
tmp:
image: /images/cc_by_sa.png
legal_code_url: https://creativecommons.org/licenses/by-sa/4.0/legalcode
name: Creative Commons Attribution-ShareAlike 4.0 International Public License (CC
BY-SA 4.0)
short: CC BY-SA (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 9
year: '2025'
...
---
OA_type: closed access
_id: '19072'
abstract:
- lang: eng
text: Pathogenic fungal and bacterial cells are enveloped within a cell wall, a
molecular barrier at their cell surface, and a critical architecture that constantly
evolves during pathogenesis. Understanding the molecular composition, structural
organization, and mobility of polysaccharides constituting this cell envelope
is crucial to correlate cell wall organization with its role in pathogenicity
and to identify potential antifungal targets. For the fungal pathogen Cryptococcus
neoformans, the characterization of the cell envelope has been complexified by
the presence of an additional external polysaccharide capsular shell. Here, we
investigate how magic-angle spinning (MAS) solid-state NMR techniques increase
the analytical capabilities to characterize the structure and dynamics of this
encapsulated pathogen. The versatility of proton detection experiments, dynamic-based
filters, and relaxation measurements facilitate the discrimination of the highly
mobile external capsular structure from the internal rigid cell wall of C. neoformans.
In addition, we report the in situ detection of triglyceride molecules from lipid
droplets based on NMR dynamic filters. Together, we demonstrate a nondestructive
technique to study the cell wall architecture of encapsulated microbes using C.
neoformans as a model, an airborne opportunistic fungal pathogen that infects
mainly immunocompromised but also competent hosts.
acknowledgement: We thank the ANR (ANR-16-CE11-0020-02 to A. Loquet, and V.A. and
ANR-21-CE17-0032-01 grant FUNPOLYVAC to V.A.) as well as the Swiss National Science
Foundation for early postdoc mobility project P2EZP2_184258 to A. Lends. This work
has benefited from the Biophysical and Structural Chemistry Platform at Institut
Européen de Chimie et Biologie IECB, Centre National de la Recherche Scientifique
CNRS Unité d’Appui et de Recherche UAR 3033, INSERM US001, and CNRS (IR-RMN FR3050
and Infranalytics FR2054).
article_processing_charge: No
article_type: original
author:
- first_name: Alons
full_name: Lends, Alons
last_name: Lends
- first_name: Gaelle
full_name: Lamon, Gaelle
last_name: Lamon
- first_name: Loic
full_name: Delcourte, Loic
last_name: Delcourte
- first_name: Aude
full_name: Sturny-Leclere, Aude
last_name: Sturny-Leclere
- first_name: Axelle
full_name: Grélard, Axelle
last_name: Grélard
- first_name: Estelle
full_name: Morvan, Estelle
last_name: Morvan
- first_name: Muhammed Bilal
full_name: Abdul-Shukkoor, Muhammed Bilal
last_name: Abdul-Shukkoor
- first_name: Mélanie
full_name: Berbon, Mélanie
last_name: Berbon
- first_name: Alicia
full_name: Vallet, Alicia
last_name: Vallet
- first_name: Birgit
full_name: Habenstein, Birgit
last_name: Habenstein
- first_name: Erick J.
full_name: Dufourc, Erick J.
last_name: Dufourc
- first_name: Paul
full_name: Schanda, Paul
id: 7B541462-FAF6-11E9-A490-E8DFE5697425
last_name: Schanda
orcid: 0000-0002-9350-7606
- first_name: Vishukumar
full_name: Aimanianda, Vishukumar
last_name: Aimanianda
- first_name: Antoine
full_name: Loquet, Antoine
last_name: Loquet
citation:
ama: Lends A, Lamon G, Delcourte L, et al. Molecular distinction of cell wall and
capsular polysaccharides in encapsulated pathogens by in situ magic-angle spinning
NMR techniques. Journal of the American Chemical Society. 2025;147(8):6813-6824.
doi:10.1021/jacs.4c16975
apa: Lends, A., Lamon, G., Delcourte, L., Sturny-Leclere, A., Grélard, A., Morvan,
E., … Loquet, A. (2025). Molecular distinction of cell wall and capsular polysaccharides
in encapsulated pathogens by in situ magic-angle spinning NMR techniques. Journal
of the American Chemical Society. American Chemical Society. https://doi.org/10.1021/jacs.4c16975
chicago: Lends, Alons, Gaelle Lamon, Loic Delcourte, Aude Sturny-Leclere, Axelle
Grélard, Estelle Morvan, Muhammed Bilal Abdul-Shukkoor, et al. “Molecular Distinction
of Cell Wall and Capsular Polysaccharides in Encapsulated Pathogens by in Situ
Magic-Angle Spinning NMR Techniques.” Journal of the American Chemical Society.
American Chemical Society, 2025. https://doi.org/10.1021/jacs.4c16975.
ieee: A. Lends et al., “Molecular distinction of cell wall and capsular polysaccharides
in encapsulated pathogens by in situ magic-angle spinning NMR techniques,” Journal
of the American Chemical Society, vol. 147, no. 8. American Chemical Society,
pp. 6813–6824, 2025.
ista: Lends A, Lamon G, Delcourte L, Sturny-Leclere A, Grélard A, Morvan E, Abdul-Shukkoor
MB, Berbon M, Vallet A, Habenstein B, Dufourc EJ, Schanda P, Aimanianda V, Loquet
A. 2025. Molecular distinction of cell wall and capsular polysaccharides in encapsulated
pathogens by in situ magic-angle spinning NMR techniques. Journal of the American
Chemical Society. 147(8), 6813–6824.
mla: Lends, Alons, et al. “Molecular Distinction of Cell Wall and Capsular Polysaccharides
in Encapsulated Pathogens by in Situ Magic-Angle Spinning NMR Techniques.” Journal
of the American Chemical Society, vol. 147, no. 8, American Chemical Society,
2025, pp. 6813–24, doi:10.1021/jacs.4c16975.
short: A. Lends, G. Lamon, L. Delcourte, A. Sturny-Leclere, A. Grélard, E. Morvan,
M.B. Abdul-Shukkoor, M. Berbon, A. Vallet, B. Habenstein, E.J. Dufourc, P. Schanda,
V. Aimanianda, A. Loquet, Journal of the American Chemical Society 147 (2025)
6813–6824.
date_created: 2025-02-23T23:01:56Z
date_published: 2025-02-16T00:00:00Z
date_updated: 2025-09-30T10:36:53Z
day: '16'
department:
- _id: PaSc
doi: 10.1021/jacs.4c16975
external_id:
isi:
- '001423628600001'
pmid:
- '39955787'
intvolume: ' 147'
isi: 1
issue: '8'
language:
- iso: eng
month: '02'
oa_version: None
page: 6813-6824
pmid: 1
publication: Journal of the American Chemical Society
publication_identifier:
eissn:
- 1520-5126
issn:
- 0002-7863
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Molecular distinction of cell wall and capsular polysaccharides in encapsulated
pathogens by in situ magic-angle spinning NMR techniques
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 147
year: '2025'
...
---
OA_type: closed access
_id: '19075'
abstract:
- lang: eng
text: Thermoelectric (TE) materials can convert the heat produced during biochemical
reactions into electrical signals, enabling the self-powered detection of biomarkers.
In this work, we design and fabricate a simple Ag2Se nanofilm-based TE biosensor
to precisely quantify hydrogen peroxide (H2O2) levels in liquid samples. A chemical
reaction involving horseradish peroxidase, ABTS and H2O2 in the specimens produces
a photothermal agent—ABTS (2,2′-azino-bis(3-ethylbenzothiazoline-6-sulfonic acid))
free radical, which triggers the heat fluctuations at the TE sensor through the
photo-thermal effect, eventually enabling the sensing of H2O2. Consequently, the
constructed sensor can achieve a detection limit of 0.26 μM by a three-leg TE
device design. Further investigations suggest that the application of our TE sensor
can be extended in testing H2O2 in beverages (including milk, soda water, and
lemonade) and evaluating the load of bacterial pathogens relevant to dental diseases
and infections including Streptococcus sanguinis and Methicillin-resistant Staphylococcus
aureus with high analytical accuracy. This strategy utilizes the combination of
high thermoelectric performance with chemical reactions to realize a straightforward
and accurate biomarker detection method, making it suitable for applications in
medical diagnostics, personalized health monitoring, and the food industry.
acknowledgement: This work was supported by the Sichuan Science and Technology Program
(Grant No. 2023YFG0220, 2023ZYD0064, and 2024YFHZ0309) and the Fundamental Research
Funds for the Central Universities and Research Funding from West China School/Hospital
of Stomatology Sichuan University, No. QDJF2022-2.
article_processing_charge: No
article_type: original
author:
- first_name: Huangshui
full_name: Ma, Huangshui
last_name: Ma
- first_name: Shiyu
full_name: Pu, Shiyu
last_name: Pu
- first_name: Shiyu
full_name: Jia, Shiyu
last_name: Jia
- first_name: Shengduo
full_name: Xu, Shengduo
id: 12ab8624-4c8a-11ec-9e11-e1ac2438f22f
last_name: Xu
- first_name: Qiwei
full_name: Yu, Qiwei
last_name: Yu
- first_name: Lei
full_name: Yang, Lei
last_name: Yang
- first_name: Hao
full_name: Wu, Hao
last_name: Wu
- first_name: Qiang
full_name: Sun, Qiang
last_name: Sun
citation:
ama: Ma H, Pu S, Jia S, et al. Laser-assisted thermoelectric-enhanced hydrogen peroxide
biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens.
Nanoscale. 2025;17(10):5858-5868. doi:10.1039/d4nr04860a
apa: Ma, H., Pu, S., Jia, S., Xu, S., Yu, Q., Yang, L., … Sun, Q. (2025). Laser-assisted
thermoelectric-enhanced hydrogen peroxide biosensors based on Ag2Se nanofilms
for sensitive detection of bacterial pathogens. Nanoscale. Royal Society
of Chemistry. https://doi.org/10.1039/d4nr04860a
chicago: Ma, Huangshui, Shiyu Pu, Shiyu Jia, Shengduo Xu, Qiwei Yu, Lei Yang, Hao
Wu, and Qiang Sun. “Laser-Assisted Thermoelectric-Enhanced Hydrogen Peroxide Biosensors
Based on Ag2Se Nanofilms for Sensitive Detection of Bacterial Pathogens.” Nanoscale.
Royal Society of Chemistry, 2025. https://doi.org/10.1039/d4nr04860a.
ieee: H. Ma et al., “Laser-assisted thermoelectric-enhanced hydrogen peroxide
biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens,”
Nanoscale, vol. 17, no. 10. Royal Society of Chemistry, pp. 5858–5868,
2025.
ista: Ma H, Pu S, Jia S, Xu S, Yu Q, Yang L, Wu H, Sun Q. 2025. Laser-assisted thermoelectric-enhanced
hydrogen peroxide biosensors based on Ag2Se nanofilms for sensitive detection
of bacterial pathogens. Nanoscale. 17(10), 5858–5868.
mla: Ma, Huangshui, et al. “Laser-Assisted Thermoelectric-Enhanced Hydrogen Peroxide
Biosensors Based on Ag2Se Nanofilms for Sensitive Detection of Bacterial Pathogens.”
Nanoscale, vol. 17, no. 10, Royal Society of Chemistry, 2025, pp. 5858–68,
doi:10.1039/d4nr04860a.
short: H. Ma, S. Pu, S. Jia, S. Xu, Q. Yu, L. Yang, H. Wu, Q. Sun, Nanoscale 17
(2025) 5858–5868.
date_created: 2025-02-23T23:01:57Z
date_published: 2025-03-14T00:00:00Z
date_updated: 2025-09-30T10:38:50Z
day: '14'
department:
- _id: MaIb
doi: 10.1039/d4nr04860a
external_id:
isi:
- '001416656400001'
pmid:
- '39927897'
intvolume: ' 17'
isi: 1
issue: '10'
language:
- iso: eng
month: '03'
oa_version: None
page: 5858-5868
pmid: 1
publication: Nanoscale
publication_identifier:
eissn:
- 2040-3372
issn:
- 2040-3364
publication_status: published
publisher: Royal Society of Chemistry
quality_controlled: '1'
scopus_import: '1'
status: public
title: Laser-assisted thermoelectric-enhanced hydrogen peroxide biosensors based on
Ag2Se nanofilms for sensitive detection of bacterial pathogens
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 17
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19076'
abstract:
- lang: eng
text: For accurate perception and motor control, an animal must distinguish between
sensory experiences elicited by external stimuli and those elicited by its own
actions. The diversity of behaviors and their complex influences on the senses
make this distinction challenging. Here, we uncover an action–cue hub that coordinates
motor commands with visual processing in the brain’s first visual relay. We show
that the ventral lateral geniculate nucleus (vLGN) acts as a corollary discharge
center, integrating visual translational optic flow signals with motor copies
from saccades, locomotion and pupil dynamics. The vLGN relays these signals to
correct action-specific visual distortions and to refine perception, as shown
for the superior colliculus and in a depth-estimation task. Simultaneously, brain-wide
vLGN projections drive corrective actions necessary for accurate visuomotor control.
Our results reveal an extended corollary discharge architecture that refines early
visual transformations and coordinates actions via a distributed hub-and-spoke
network to enable visual perception during action.
acknowledged_ssus:
- _id: ScienComp
- _id: PreCl
- _id: LifeSc
- _id: Bio
acknowledgement: We thank Y. Ben-Simon for generously making viral vectors for retrograde
tracing available, as well as J. Watson and F. Marr for reagents. We also thank
R. Shigemoto, W. Młynarski and members of the Neuroethology group for their comments
on the manuscript and L. Burnett for her schematic drawings. This research was supported
by the Scientific Service Units of ISTA through resources provided by Scientific
Computing, the Preclinical Facility, the Lab Support Facility and the Imaging and
Optics Facility, in particular F. Lange, M. Schunn and T. Asenov. This work was
supported by European Research Council Starting Grant no. 756502 (M.J.) and European
Research Council Consolidator Grant no. 101086580 (M.J.); and EMBO ALTF grant no.
1098-2017 (A.S.) and Human Frontiers Science Program grant no. LT000256/2018-L (A.S.).
Open access funding provided by Institute of Science and Technology (IST Austria).
article_number: '7278'
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Tomas A
full_name: Vega Zuniga, Tomas A
id: 2E7C4E78-F248-11E8-B48F-1D18A9856A87
last_name: Vega Zuniga
- first_name: Anton L
full_name: Sumser, Anton L
id: 3320A096-F248-11E8-B48F-1D18A9856A87
last_name: Sumser
orcid: 0000-0002-4792-1881
- first_name: Olga
full_name: Symonova, Olga
id: 3C0C7BC6-F248-11E8-B48F-1D18A9856A87
last_name: Symonova
orcid: 0000-0003-2012-9947
- first_name: Peter
full_name: Koppensteiner, Peter
id: 3B8B25A8-F248-11E8-B48F-1D18A9856A87
last_name: Koppensteiner
orcid: 0000-0002-3509-1948
- first_name: Florian
full_name: Schmidt, Florian
id: A2EF226A-AF19-11E9-924C-0525E6697425
last_name: Schmidt
- first_name: Maximilian A
full_name: Jösch, Maximilian A
id: 2BD278E6-F248-11E8-B48F-1D18A9856A87
last_name: Jösch
orcid: 0000-0002-3937-1330
citation:
ama: Vega Zuniga TA, Sumser AL, Symonova O, Koppensteiner P, Schmidt F, Jösch MA.
A thalamic hub-and-spoke network enables visual perception during action by coordinating
visuomotor dynamics. Nature Neuroscience. 2025;28. doi:10.1038/s41593-025-01874-w
apa: Vega Zuniga, T. A., Sumser, A. L., Symonova, O., Koppensteiner, P., Schmidt,
F., & Jösch, M. A. (2025). A thalamic hub-and-spoke network enables visual
perception during action by coordinating visuomotor dynamics. Nature Neuroscience.
Springer Nature. https://doi.org/10.1038/s41593-025-01874-w
chicago: Vega Zuniga, Tomas A, Anton L Sumser, Olga Symonova, Peter Koppensteiner,
Florian Schmidt, and Maximilian A Jösch. “A Thalamic Hub-and-Spoke Network Enables
Visual Perception during Action by Coordinating Visuomotor Dynamics.” Nature
Neuroscience. Springer Nature, 2025. https://doi.org/10.1038/s41593-025-01874-w.
ieee: T. A. Vega Zuniga, A. L. Sumser, O. Symonova, P. Koppensteiner, F. Schmidt,
and M. A. Jösch, “A thalamic hub-and-spoke network enables visual perception during
action by coordinating visuomotor dynamics,” Nature Neuroscience, vol.
28. Springer Nature, 2025.
ista: Vega Zuniga TA, Sumser AL, Symonova O, Koppensteiner P, Schmidt F, Jösch MA.
2025. A thalamic hub-and-spoke network enables visual perception during action
by coordinating visuomotor dynamics. Nature Neuroscience. 28, 7278.
mla: Vega Zuniga, Tomas A., et al. “A Thalamic Hub-and-Spoke Network Enables Visual
Perception during Action by Coordinating Visuomotor Dynamics.” Nature Neuroscience,
vol. 28, 7278, Springer Nature, 2025, doi:10.1038/s41593-025-01874-w.
short: T.A. Vega Zuniga, A.L. Sumser, O. Symonova, P. Koppensteiner, F. Schmidt,
M.A. Jösch, Nature Neuroscience 28 (2025).
corr_author: '1'
date_created: 2025-02-23T23:01:58Z
date_published: 2025-03-01T00:00:00Z
date_updated: 2025-09-30T10:40:49Z
day: '01'
department:
- _id: MaJö
- _id: PreCl
doi: 10.1038/s41593-025-01874-w
ec_funded: 1
external_id:
isi:
- '001416866800001'
pmid:
- '39930095'
has_accepted_license: '1'
intvolume: ' 28'
isi: 1
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1038/s41593-025-01874-w
month: '03'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 2634E9D2-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '756502'
name: Circuits of Visual Attention
- _id: bdaf81a8-d553-11ed-ba76-c95961984540
grant_number: '101086580'
name: 'Action Selection in the Midbrain: Neuromodulation of Visuomotor Senses'
- _id: 264FEA02-B435-11E9-9278-68D0E5697425
grant_number: ALTF 1098-2017
name: Connecting sensory with motor processing in the superior colliculus
- _id: 266D407A-B435-11E9-9278-68D0E5697425
grant_number: LT000256
name: Neuronal networks of salience and spatial detection in the murine superior
colliculus
publication: Nature Neuroscience
publication_identifier:
eissn:
- 1546-1726
issn:
- 1097-6256
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
related_material:
link:
- description: News on ISTA Website
relation: press_release
url: https://ista.ac.at/en/news/high-tech-video-optimization-in-our-brain/
record:
- id: '18579'
relation: research_data
status: public
scopus_import: '1'
status: public
title: A thalamic hub-and-spoke network enables visual perception during action by
coordinating visuomotor dynamics
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 28
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19080'
abstract:
- lang: eng
text: We examine mesoscale convective organisation in the tropical western Pacific
using a multivariate analysis of column humidity, precipitation and sea surface
temperature (SST) observations. We demonstrate that in boreal summer and autumn,
convection remains spatially random despite radiative-feedbacks acting to aggregate
convection, which we attribute to the high density of convective moisture sources
and the role of wind shear. Instead, in winter and spring, a weak meridional SST
gradient exists and convection is usually clustered over the regions of warmer
SSTs, with significant meridional humidity gradients. However, this is sporadically
interrupted by episodes of convection migration to the coldest SSTs and limited
spatial humidity variance. These episodes are the result of westward propagating
equatorial waves, which remove meridional humidity gradients. It appears that
the drivers of mesoscale convective clustering and humidity variability in the
Pacific warm pool are the SST gradients, shear, and equatorial wave dynamics.
acknowledgement: This paper is based on A.C. Ph.D. thesis, chapter 4. A.C. was supported
by an ICTP Ph.D scholarship and subsequently by funding from the European Union’s
Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie
grant agreement No 101034413. MVDV was supported by an ICTP diploma programme scholarship
while carrying out analysis for this publication. The funders played no role in
study design, data collection, analysis and interpretation of data, or the writing
of this manuscript. We would like to thank Maria Gehne of NOAA for providing the
code for the wave activity calculation and advice on its use, and Fred Kucharski,
Erika Coppola, Hernández-Deckers, Caroline Muller and Paolina Cerlini for their
insightful comments and advice
article_number: '69'
article_processing_charge: Yes
article_type: original
author:
- first_name: Adrian Mike
full_name: Tompkins, Adrian Mike
last_name: Tompkins
- first_name: Alejandro
full_name: Casallas Garcia, Alejandro
id: 92081129-2d75-11ef-a48d-b04dd7a2385a
last_name: Casallas Garcia
orcid: 0000-0002-1988-5035
- first_name: Michie Vianca
full_name: De Vera, Michie Vianca
last_name: De Vera
citation:
ama: Tompkins AM, Casallas Garcia A, De Vera MV. Drivers of mesoscale convective
aggregation and spatial humidity variability in the tropical western Pacific.
npj Climate and Atmospheric Science. 2025;8. doi:10.1038/s41612-024-00848-2
apa: Tompkins, A. M., Casallas Garcia, A., & De Vera, M. V. (2025). Drivers
of mesoscale convective aggregation and spatial humidity variability in the tropical
western Pacific. Npj Climate and Atmospheric Science. Springer Nature.
https://doi.org/10.1038/s41612-024-00848-2
chicago: Tompkins, Adrian Mike, Alejandro Casallas Garcia, and Michie Vianca De
Vera. “Drivers of Mesoscale Convective Aggregation and Spatial Humidity Variability
in the Tropical Western Pacific.” Npj Climate and Atmospheric Science.
Springer Nature, 2025. https://doi.org/10.1038/s41612-024-00848-2.
ieee: A. M. Tompkins, A. Casallas Garcia, and M. V. De Vera, “Drivers of mesoscale
convective aggregation and spatial humidity variability in the tropical western
Pacific,” npj Climate and Atmospheric Science, vol. 8. Springer Nature,
2025.
ista: Tompkins AM, Casallas Garcia A, De Vera MV. 2025. Drivers of mesoscale convective
aggregation and spatial humidity variability in the tropical western Pacific.
npj Climate and Atmospheric Science. 8, 69.
mla: Tompkins, Adrian Mike, et al. “Drivers of Mesoscale Convective Aggregation
and Spatial Humidity Variability in the Tropical Western Pacific.” Npj Climate
and Atmospheric Science, vol. 8, 69, Springer Nature, 2025, doi:10.1038/s41612-024-00848-2.
short: A.M. Tompkins, A. Casallas Garcia, M.V. De Vera, Npj Climate and Atmospheric
Science 8 (2025).
corr_author: '1'
date_created: 2025-02-24T10:18:50Z
date_published: 2025-02-24T00:00:00Z
date_updated: 2025-09-30T10:41:20Z
day: '24'
ddc:
- '550'
department:
- _id: CaMu
doi: 10.1038/s41612-024-00848-2
ec_funded: 1
external_id:
isi:
- '001432282900002'
file:
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content_type: application/pdf
creator: acasalla
date_created: 2025-02-24T10:18:47Z
date_updated: 2025-02-24T10:18:47Z
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file_size: 5807997
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creator: acasalla
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intvolume: ' 8'
isi: 1
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: npj Climate and Atmospheric Science
publication_identifier:
eissn:
- 2397-3722
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Drivers of mesoscale convective aggregation and spatial humidity variability
in the tropical western Pacific
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 8
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '19276'
abstract:
- lang: eng
text: Impurity motion in a many-body environment has been a central issue in the
field of low-temperature physics for decades. In bosonic quantum fluids, the onset
of a drag force experienced by point-like objects is due to collective environment
excitations, driven by the exchange of linear momentum between the impurity and
the many-body bath. In this work we consider a rotating impurity, with the aim
of exploring how angular momentum is exchanged with the surrounding bosonic environment.
In order to elucidate these issues, we employ a quasiparticle approach based on
the angulon theory, which allows us to effectively deal with the non-trivial algebra
of quantized angular momentum in the presence of a many-body environment. We uncover
how impurity dressing by environmental excitations can establish an exchange channel,
whose effectiveness crucially depends on the initial state of the impurity. Remarkably,
we find that there is a critical value of initial angular momentum, above which
this channel effectively freezes.
acknowledgement: We acknowledge Henrik Stapelfeldt for enlightening discussions. M.L.
acknowledges support by the European Research Council (ERC) Starting Grant No. 801770
(ANGULON). A.C. received funding from the European Union’s Horizon Europe research
and innovation program under the Marie Skłodowska-Curie Grant Agreement No. 101062862—NeqMolRot.
article_number: '074104'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Alberto
full_name: Cappellaro, Alberto
id: 9d13b3cb-30a2-11eb-80dc-f772505e8660
last_name: Cappellaro
orcid: 0000-0001-6110-2359
- first_name: Giacomo
full_name: Bighin, Giacomo
id: 4CA96FD4-F248-11E8-B48F-1D18A9856A87
last_name: Bighin
orcid: 0000-0001-8823-9777
- first_name: Igor
full_name: Cherepanov, Igor
id: 339C7E5A-F248-11E8-B48F-1D18A9856A87
last_name: Cherepanov
- first_name: Mikhail
full_name: Lemeshko, Mikhail
id: 37CB05FA-F248-11E8-B48F-1D18A9856A87
last_name: Lemeshko
orcid: 0000-0002-6990-7802
citation:
ama: Cappellaro A, Bighin G, Cherepanov I, Lemeshko M. Environment-limited transfer
of angular momentum in Bose liquids. Journal of Chemical Physics. 2025;162(7).
doi:10.1063/5.0253451
apa: Cappellaro, A., Bighin, G., Cherepanov, I., & Lemeshko, M. (2025). Environment-limited
transfer of angular momentum in Bose liquids. Journal of Chemical Physics.
AIP Publishing. https://doi.org/10.1063/5.0253451
chicago: Cappellaro, Alberto, Giacomo Bighin, Igor Cherepanov, and Mikhail Lemeshko.
“Environment-Limited Transfer of Angular Momentum in Bose Liquids.” Journal
of Chemical Physics. AIP Publishing, 2025. https://doi.org/10.1063/5.0253451.
ieee: A. Cappellaro, G. Bighin, I. Cherepanov, and M. Lemeshko, “Environment-limited
transfer of angular momentum in Bose liquids,” Journal of Chemical Physics,
vol. 162, no. 7. AIP Publishing, 2025.
ista: Cappellaro A, Bighin G, Cherepanov I, Lemeshko M. 2025. Environment-limited
transfer of angular momentum in Bose liquids. Journal of Chemical Physics. 162(7),
074104.
mla: Cappellaro, Alberto, et al. “Environment-Limited Transfer of Angular Momentum
in Bose Liquids.” Journal of Chemical Physics, vol. 162, no. 7, 074104,
AIP Publishing, 2025, doi:10.1063/5.0253451.
short: A. Cappellaro, G. Bighin, I. Cherepanov, M. Lemeshko, Journal of Chemical
Physics 162 (2025).
corr_author: '1'
date_created: 2025-03-02T23:01:51Z
date_published: 2025-02-21T00:00:00Z
date_updated: 2026-01-20T10:11:27Z
day: '21'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1063/5.0253451
ec_funded: 1
external_id:
arxiv:
- '2501.16066'
isi:
- '001427233100008'
pmid:
- '39964008'
file:
- access_level: open_access
checksum: c67c37788a949af9f0f45b22a27f8087
content_type: application/pdf
creator: dernst
date_created: 2025-03-04T10:48:03Z
date_updated: 2025-03-04T10:48:03Z
file_id: '19292'
file_name: 2025_JourChemicalPhysics_Cappellaro.pdf
file_size: 6455134
relation: main_file
success: 1
file_date_updated: 2025-03-04T10:48:03Z
has_accepted_license: '1'
intvolume: ' 162'
isi: 1
issue: '7'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 2688CF98-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '801770'
name: 'Angulon: physics and applications of a new quasiparticle'
- _id: bd7b5202-d553-11ed-ba76-9b1c1b258338
grant_number: '101062862'
name: Non-Equilibrium Field Theory of Molecular Rotations
publication: Journal of Chemical Physics
publication_identifier:
eissn:
- 1089-7690
issn:
- 0021-9606
publication_status: published
publisher: AIP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Environment-limited transfer of angular momentum in Bose liquids
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: 162
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19277'
abstract:
- lang: eng
text: Light-driven molecular rotary motors perform chirality-controlled unidirectional
rotations fueled by light and heat. This unique function renders them appealing
for the construction of dynamic molecular systems, actuating materials, and molecular
machines. Achieving a combination of high photoefficiency, visible-light responsiveness,
synthetic accessibility, and easy tuning of dynamic properties within a single
scaffold is critical for these applications but remains a longstanding challenge.
Herein, a series of highly photoefficient visible-light–responsive molecular motors
(MMs), featuring various rotary speeds, was obtained by a convenient one-step
formylation of their parent motors. This strategy greatly improves all aspects
of the performance of MMs—red-shifted wavelengths of excitation, high photoisomerization
quantum yields, and high photostationary state distributions of isomers—beyond
the state-of-the-art light-responsive MM systems. The development of this late-stage
functionalization strategy of MMs opens avenues for the construction of high-performance
molecular machines and devices for applications in materials science and biological
systems, representing a major advance in the synthetic toolbox of molecular machines.
acknowledgement: 'R. Sneep is acknowledged for mass spectral analysis and SFC training.
We thank A. S. Lubbe from University of Groningen for help with this manuscript
and for fruitful discussions. We thank P. Cieciórski from University of Warsaw for
help with the figure preparation. This work was supported from the following sources:
China Scholarship Council, CSC PhD Fellowship no. 201808330459 to J.S.; the Netherlands
Organization for Scientific Research (NWO-CW) (B.L.F); the Dutch Ministry of Education,
Culture, and Science (Gravitation program no. 024.001.035) (B.L.F.); Polish National
Agency for Academic Exchange (reg. no.: BPN/PPO/2023/1/00014); and National Science
Center Poland (reg. no.: 2024/03/1/ST5/00003) (W.D.).'
article_number: eadr9326
article_processing_charge: Yes
article_type: original
author:
- first_name: Jinyu
full_name: Sheng, Jinyu
id: 639f0526-27c9-11ee-95a6-966cd7f102d8
last_name: Sheng
- first_name: Carlijn L.F.
full_name: Van Beek, Carlijn L.F.
last_name: Van Beek
- first_name: Charlotte N.
full_name: Stindt, Charlotte N.
last_name: Stindt
- first_name: Wojciech
full_name: Danowski, Wojciech
last_name: Danowski
- first_name: Joanna
full_name: Jankowska, Joanna
last_name: Jankowska
- first_name: Stefano
full_name: Crespi, Stefano
last_name: Crespi
- first_name: Daisy R.S.
full_name: Pooler, Daisy R.S.
last_name: Pooler
- first_name: Michiel F.
full_name: Hilbers, Michiel F.
last_name: Hilbers
- first_name: Wybren Jan
full_name: Buma, Wybren Jan
last_name: Buma
- first_name: Ben L.
full_name: Feringa, Ben L.
last_name: Feringa
citation:
ama: Sheng J, Van Beek CLF, Stindt CN, et al. General strategy for boosting the
performance of speed-tunable rotary molecular motors with visible light. Science
Advances. 2025;11(8). doi:10.1126/sciadv.adr9326
apa: Sheng, J., Van Beek, C. L. F., Stindt, C. N., Danowski, W., Jankowska, J.,
Crespi, S., … Feringa, B. L. (2025). General strategy for boosting the performance
of speed-tunable rotary molecular motors with visible light. Science Advances.
AAAS. https://doi.org/10.1126/sciadv.adr9326
chicago: Sheng, Jinyu, Carlijn L.F. Van Beek, Charlotte N. Stindt, Wojciech Danowski,
Joanna Jankowska, Stefano Crespi, Daisy R.S. Pooler, Michiel F. Hilbers, Wybren
Jan Buma, and Ben L. Feringa. “General Strategy for Boosting the Performance of
Speed-Tunable Rotary Molecular Motors with Visible Light.” Science Advances.
AAAS, 2025. https://doi.org/10.1126/sciadv.adr9326.
ieee: J. Sheng et al., “General strategy for boosting the performance of
speed-tunable rotary molecular motors with visible light,” Science Advances,
vol. 11, no. 8. AAAS, 2025.
ista: Sheng J, Van Beek CLF, Stindt CN, Danowski W, Jankowska J, Crespi S, Pooler
DRS, Hilbers MF, Buma WJ, Feringa BL. 2025. General strategy for boosting the
performance of speed-tunable rotary molecular motors with visible light. Science
Advances. 11(8), eadr9326.
mla: Sheng, Jinyu, et al. “General Strategy for Boosting the Performance of Speed-Tunable
Rotary Molecular Motors with Visible Light.” Science Advances, vol. 11,
no. 8, eadr9326, AAAS, 2025, doi:10.1126/sciadv.adr9326.
short: J. Sheng, C.L.F. Van Beek, C.N. Stindt, W. Danowski, J. Jankowska, S. Crespi,
D.R.S. Pooler, M.F. Hilbers, W.J. Buma, B.L. Feringa, Science Advances 11 (2025).
date_created: 2025-03-02T23:01:51Z
date_published: 2025-02-21T00:00:00Z
date_updated: 2025-09-30T10:46:23Z
day: '21'
ddc:
- '540'
department:
- _id: RaKl
doi: 10.1126/sciadv.adr9326
external_id:
isi:
- '001425511500020'
pmid:
- '39970219'
file:
- access_level: open_access
checksum: 34ad18a07cb87fdde7bdb626fdeef832
content_type: application/pdf
creator: dernst
date_created: 2025-03-04T10:57:39Z
date_updated: 2025-03-04T10:57:39Z
file_id: '19293'
file_name: 2025_ScienceAdvance_Sheng.pdf
file_size: 584613
relation: main_file
success: 1
file_date_updated: 2025-03-04T10:57:39Z
has_accepted_license: '1'
intvolume: ' 11'
isi: 1
issue: '8'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
pmid: 1
publication: Science Advances
publication_identifier:
eissn:
- 2375-2548
publication_status: published
publisher: AAAS
quality_controlled: '1'
scopus_import: '1'
status: public
title: General strategy for boosting the performance of speed-tunable rotary molecular
motors with visible light
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 11
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '19279'
abstract:
- lang: eng
text: Recent experimental advances in nanofluidics have allowed to explore ion transport
across molecular-scale pores, in particular, for iontronic applications. Two-dimensional
nanochannels—in which a single molecular layer of electrolyte is confined between
solid walls—constitute a unique platform to investigate fluid and ion transport
in extreme confinement, highlighting unconventional transport properties. In this
work, we study ionic association in 2D nanochannels, and its consequences on non-linear
ionic transport, using both molecular dynamics simulations and analytical theory.
We show that under sufficient confinement, ions assemble into pairs or larger
clusters in a process analogous to a Kosterlitz–Thouless transition, here modified
by the dielectric confinement. We further show that the breaking of pairs results
in an electric-field dependent conduction, a mechanism usually known as the second
Wien effect. However the 2D nature of the system results in non-universal, temperature-dependent,
scaling of the conductivity with electric field, leading to ionic coulomb blockade
in some regimes. A 2D generalization of the Onsager theory fully accounts for
the non-linear transport. These results suggest ways to exploit electrostatic
interactions between ions to build new nanofluidic devices.
acknowledgement: The authors thank B. Coquinot and G. Monet for fruitful discussions.
L.B. acknowledges support from ERC-Synergy Grant Agreement No. 101071937, n-AQUA.
P.R. acknowledges support from the European Union’s Horizon 2020 research and innovation
program under Marie Sklodowska-Curie Grant Agreement No. 101034413.
article_number: '064703'
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Damien
full_name: Toquer, Damien
last_name: Toquer
- first_name: Lydéric
full_name: Bocquet, Lydéric
last_name: Bocquet
- first_name: Paul
full_name: Robin, Paul
id: 48c58128-57b0-11ee-9095-dc28fd97fc1d
last_name: Robin
orcid: 0000-0002-5728-9189
citation:
ama: Toquer D, Bocquet L, Robin P. Ionic association and Wien effect in 2D confined
electrolytes. Journal of Chemical Physics. 2025;162(6). doi:10.1063/5.0241949
apa: Toquer, D., Bocquet, L., & Robin, P. (2025). Ionic association and Wien
effect in 2D confined electrolytes. Journal of Chemical Physics. AIP Publishing.
https://doi.org/10.1063/5.0241949
chicago: Toquer, Damien, Lydéric Bocquet, and Paul Robin. “Ionic Association and
Wien Effect in 2D Confined Electrolytes.” Journal of Chemical Physics.
AIP Publishing, 2025. https://doi.org/10.1063/5.0241949.
ieee: D. Toquer, L. Bocquet, and P. Robin, “Ionic association and Wien effect in
2D confined electrolytes,” Journal of Chemical Physics, vol. 162, no. 6.
AIP Publishing, 2025.
ista: Toquer D, Bocquet L, Robin P. 2025. Ionic association and Wien effect in 2D
confined electrolytes. Journal of Chemical Physics. 162(6), 064703.
mla: Toquer, Damien, et al. “Ionic Association and Wien Effect in 2D Confined Electrolytes.”
Journal of Chemical Physics, vol. 162, no. 6, 064703, AIP Publishing, 2025,
doi:10.1063/5.0241949.
short: D. Toquer, L. Bocquet, P. Robin, Journal of Chemical Physics 162 (2025).
corr_author: '1'
date_created: 2025-03-02T23:01:52Z
date_published: 2025-02-14T00:00:00Z
date_updated: 2025-09-30T10:44:48Z
day: '14'
ddc:
- '540'
department:
- _id: EdHa
doi: 10.1063/5.0241949
ec_funded: 1
external_id:
arxiv:
- '2410.03316'
isi:
- '001421300300001'
pmid:
- '39932241'
file:
- access_level: open_access
checksum: c9008c2c50c917673aa588f75acbcb40
content_type: application/pdf
creator: dernst
date_created: 2025-03-04T10:29:36Z
date_updated: 2025-03-04T10:29:36Z
file_id: '19290'
file_name: 2025_JourChemicalPhysics_Toquer.pdf
file_size: 5807062
relation: main_file
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file_date_updated: 2025-03-04T10:29:36Z
has_accepted_license: '1'
intvolume: ' 162'
isi: 1
issue: '6'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Journal of Chemical Physics
publication_identifier:
eissn:
- 1089-7690
issn:
- 0021-9606
publication_status: published
publisher: AIP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Ionic association and Wien effect in 2D confined electrolytes
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 162
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '19281'
abstract:
- lang: eng
text: "In this work, we consider the list-decodability and list-recoverability of
codes in the zero-rate regime. Briefly, a code \U0001D49E ⊆ [q]ⁿ is (p,\U0001D4C1,L)-list-recoverable
if for all tuples of input lists (Y₁,… ,Y_n) with each Y_i ⊆ [q] and |Y_i| = \U0001D4C1,
the number of codewords c ∈ \U0001D49E such that c_i ∉ Y_i for at most pn choices
of i ∈ [n] is less than L; list-decoding is the special case of \U0001D4C1 = 1.
In recent work by Resch, Yuan and Zhang (ICALP 2023) the zero-rate threshold for
list-recovery was determined for all parameters: that is, the work explicitly
computes p_*: = p_*(q,\U0001D4C1,L) with the property that for all ε > 0 (a) there
exist positive-rate (p_*-ε,\U0001D4C1,L)-list-recoverable codes, and (b) any (p_*+ε,\U0001D4C1,L)-list-recoverable
code has rate 0. In fact, in the latter case the code has constant size, independent
on n. However, the constant size in their work is quite large in 1/ε, at least
|\U0001D49E| ≥ (1/(ε))^O(q^L).\r\nOur contribution in this work is to show that
for all choices of q,\U0001D4C1 and L with q ≥ 3, any (p_*+ε,\U0001D4C1,L)-list-recoverable
code must have size O_{q,\U0001D4C1,L}(1/ε), and furthermore this upper bound
is complemented by a matching lower bound Ω_{q,\U0001D4C1,L}(1/ε). This greatly
generalizes work by Alon, Bukh and Polyanskiy (IEEE Trans. Inf. Theory 2018) which
focused only on the case of binary alphabet (and thus necessarily only list-decoding).
We remark that we can in fact recover the same result for q = 2 and even L, as
obtained by Alon, Bukh and Polyanskiy: we thus strictly generalize their work.
\r\nOur main technical contribution is to (a) properly define a linear programming
relaxation of the list-recovery condition over large alphabets; and (b) to demonstrate
that a certain function defined on a q-ary probability simplex is maximized by
the uniform distribution. This represents the core challenge in generalizing to
larger q (as a binary simplex can be naturally identified with a one-dimensional
interval). We can subsequently re-utilize certain Schur convexity and convexity
properties established for a related function by Resch, Yuan and Zhang along with
ideas of Alon, Bukh and Polyanskiy."
acknowledgement: "The research of C. Yuan was support in part by the National Key
R&D Program of China\r\nunder Grant 2023YFE0123900 and Natural Science Foundation
of Shanghai under the 2024 Shanghai Action Plan for Science, Technology and Innovation
Grant 24BC3200700. The research of N. Resch is supported in part by an NWO (Dutch
Research Council) grant with number C.2324.0590, and this work was done in part
while he was visiting the Simons Institute for the Theory of Computing, supported
by DOE grant #DE-SC0024124."
alternative_title:
- LIPIcs
article_number: '82'
article_processing_charge: Yes
arxiv: 1
author:
- first_name: Nicolas
full_name: Resch, Nicolas
last_name: Resch
- first_name: Chen
full_name: Yuan, Chen
last_name: Yuan
- first_name: Yihan
full_name: Zhang, Yihan
id: 2ce5da42-b2ea-11eb-bba5-9f264e9d002c
last_name: Zhang
orcid: 0000-0002-6465-6258
citation:
ama: 'Resch N, Yuan C, Zhang Y. Tight bounds on list-decodable and list-recoverable
zero-rate codes. In: 16th Innovations in Theoretical Computer Science Conference.
Vol 325. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2025. doi:10.4230/LIPIcs.ITCS.2025.82'
apa: 'Resch, N., Yuan, C., & Zhang, Y. (2025). Tight bounds on list-decodable
and list-recoverable zero-rate codes. In 16th Innovations in Theoretical Computer
Science Conference (Vol. 325). New York, NY, United States: Schloss Dagstuhl
- Leibniz-Zentrum für Informatik. https://doi.org/10.4230/LIPIcs.ITCS.2025.82'
chicago: Resch, Nicolas, Chen Yuan, and Yihan Zhang. “Tight Bounds on List-Decodable
and List-Recoverable Zero-Rate Codes.” In 16th Innovations in Theoretical Computer
Science Conference, Vol. 325. Schloss Dagstuhl - Leibniz-Zentrum für Informatik,
2025. https://doi.org/10.4230/LIPIcs.ITCS.2025.82.
ieee: N. Resch, C. Yuan, and Y. Zhang, “Tight bounds on list-decodable and list-recoverable
zero-rate codes,” in 16th Innovations in Theoretical Computer Science Conference,
New York, NY, United States, 2025, vol. 325.
ista: 'Resch N, Yuan C, Zhang Y. 2025. Tight bounds on list-decodable and list-recoverable
zero-rate codes. 16th Innovations in Theoretical Computer Science Conference.
ITCS: Innovations in Theoretical Computer Science, LIPIcs, vol. 325, 82.'
mla: Resch, Nicolas, et al. “Tight Bounds on List-Decodable and List-Recoverable
Zero-Rate Codes.” 16th Innovations in Theoretical Computer Science Conference,
vol. 325, 82, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2025, doi:10.4230/LIPIcs.ITCS.2025.82.
short: N. Resch, C. Yuan, Y. Zhang, in:, 16th Innovations in Theoretical Computer
Science Conference, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2025.
conference:
end_date: 2025-01-10
location: New York, NY, United States
name: 'ITCS: Innovations in Theoretical Computer Science'
start_date: 2025-01-07
corr_author: '1'
date_created: 2025-03-02T23:01:53Z
date_published: 2025-02-11T00:00:00Z
date_updated: 2025-09-30T10:42:35Z
day: '11'
ddc:
- '510'
- '000'
department:
- _id: MaMo
doi: 10.4230/LIPIcs.ITCS.2025.82
external_id:
arxiv:
- '2309.01800'
isi:
- '001532717300082'
file:
- access_level: open_access
checksum: df3921ddf1b360b07f43d427fea51242
content_type: application/pdf
creator: dernst
date_created: 2025-03-04T09:35:57Z
date_updated: 2025-03-04T09:35:57Z
file_id: '19286'
file_name: 2025_LIPIcs_Resch.pdf
file_size: 898601
relation: main_file
success: 1
file_date_updated: 2025-03-04T09:35:57Z
has_accepted_license: '1'
intvolume: ' 325'
isi: 1
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
publication: 16th Innovations in Theoretical Computer Science Conference
publication_identifier:
isbn:
- '9783959773614'
issn:
- 1868-8969
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
quality_controlled: '1'
scopus_import: '1'
status: public
title: Tight bounds on list-decodable and list-recoverable zero-rate codes
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: conference
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 325
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19282'
abstract:
- lang: eng
text: Osmium complexes with osmium in different oxidation states (II, III, IV, and
VI) have been reported to exhibit antiproliferative activity in cancer cell lines.
Herein, we demonstrate unexplored opportunities offered by 187Os nuclear forward
scattering (NFS) and nuclear inelastic scattering (NIS) of synchrotron radiation
for characterization of hyperfine interactions and lattice dynamics in a benchmark
Os(VI) complex, K2[OsO2(OH)4]. We determined the isomer shift [δ = 3.3(1) millimeters
per second] relative to [OsIVCl6]2− and quadrupole splitting [ΔEQ = 12.0(2) millimeters
per second] with NFS. We estimated the Lamb-Mössbauer factor [0.80(4)], extracted
the density of phonon states, and carried out a thermodynamics characterization
using the NIS data combined with first-principles calculations. Overall, we provide
evidence that 187Os nuclear resonance scattering is a reliable technique for the
investigation of hyperfine interactions and Os-specific vibrations in osmium(VI)
species and is thus applicable for such measurements in osmium complexes of other
oxidation states, including those with anticancer activity such as Os(III) and
Os(IV).
acknowledgement: "The European Synchrotron Radiation Facility is acknowledged for
providing synchrotron radiation beamtime at the Nuclear Resonance beamlines ID18
and ID14. The technical assistance of J.-P. Celse is acknowledged during the beamtime
at the ESRF. V.B.A. and G.E.B. are thankful to Karl Mayer Stiftung (Triesen, Liechtenstein)
and Valüna Stiftung (Vaduz, Liechtenstein) for financial support in purchasing the
187Os metal. We are also thankful to A. Dobrov for help in the synthesis of 187OsO4
from 187Os. Ab initio calculations were done on the ASPIRE-2A cluster (www.nscc.sg)
under computational projects 11001278, 11003762, 51000267, and 11003763. This work
used computational resources of the supercomputer Fugaku provided by RIKEN/NSCC
through the HPCI System Research Project (project ID: hp240202). The computational
resources of the HPC-NUS are gratefully acknowledged.\r\nThis work was supported
by the Austrian Science Fund (FWF) grant I4729 (V.B.A.), King Saud University Researchers
Supporting Project no. RSP2025R266 (L.F.C. and A.A.A.-K.), and National University
of Singapore research projects A-8000709-00-00, A-8000017-00-00, and A-8001894-00-00
(Z.H. and L.U.)."
article_number: eads3406
article_processing_charge: Yes
article_type: original
author:
- first_name: Iryna
full_name: Stepanenko, Iryna
id: 2a1f3914-89ea-11ee-b4f9-b6c903344e34
last_name: Stepanenko
- first_name: Zhishuo
full_name: Huang, Zhishuo
last_name: Huang
- first_name: Liviu
full_name: Ungur, Liviu
last_name: Ungur
- first_name: Dimitrios
full_name: Bessas, Dimitrios
last_name: Bessas
- first_name: Aleksandr
full_name: Chumakov, Aleksandr
last_name: Chumakov
- first_name: Ilya
full_name: Sergueev, Ilya
last_name: Sergueev
- first_name: Gabriel E.
full_name: Büchel, Gabriel E.
last_name: Büchel
- first_name: Abdullah A.
full_name: Al-Kahtani, Abdullah A.
last_name: Al-Kahtani
- first_name: Liviu F.
full_name: Chibotaru, Liviu F.
last_name: Chibotaru
- first_name: Joshua
full_name: Telser, Joshua
last_name: Telser
- first_name: Vladimir B.
full_name: Arion, Vladimir B.
last_name: Arion
citation:
ama: Stepanenko I, Huang Z, Ungur L, et al. 187Os nuclear resonance scattering to
explore hyperfine interactions and lattice dynamics for biological applications.
Science Advances. 2025;11(6). doi:10.1126/sciadv.ads3406
apa: Stepanenko, I., Huang, Z., Ungur, L., Bessas, D., Chumakov, A., Sergueev, I.,
… Arion, V. B. (2025). 187Os nuclear resonance scattering to explore hyperfine
interactions and lattice dynamics for biological applications. Science Advances.
AAAS. https://doi.org/10.1126/sciadv.ads3406
chicago: Stepanenko, Iryna, Zhishuo Huang, Liviu Ungur, Dimitrios Bessas, Aleksandr
Chumakov, Ilya Sergueev, Gabriel E. Büchel, et al. “187Os Nuclear Resonance Scattering
to Explore Hyperfine Interactions and Lattice Dynamics for Biological Applications.”
Science Advances. AAAS, 2025. https://doi.org/10.1126/sciadv.ads3406.
ieee: I. Stepanenko et al., “187Os nuclear resonance scattering to explore
hyperfine interactions and lattice dynamics for biological applications,” Science
Advances, vol. 11, no. 6. AAAS, 2025.
ista: Stepanenko I, Huang Z, Ungur L, Bessas D, Chumakov A, Sergueev I, Büchel GE,
Al-Kahtani AA, Chibotaru LF, Telser J, Arion VB. 2025. 187Os nuclear resonance
scattering to explore hyperfine interactions and lattice dynamics for biological
applications. Science Advances. 11(6), eads3406.
mla: Stepanenko, Iryna, et al. “187Os Nuclear Resonance Scattering to Explore Hyperfine
Interactions and Lattice Dynamics for Biological Applications.” Science Advances,
vol. 11, no. 6, eads3406, AAAS, 2025, doi:10.1126/sciadv.ads3406.
short: I. Stepanenko, Z. Huang, L. Ungur, D. Bessas, A. Chumakov, I. Sergueev, G.E.
Büchel, A.A. Al-Kahtani, L.F. Chibotaru, J. Telser, V.B. Arion, Science Advances
11 (2025).
date_created: 2025-03-02T23:01:53Z
date_published: 2025-02-07T00:00:00Z
date_updated: 2026-02-23T08:05:58Z
day: '07'
ddc:
- '530'
department:
- _id: StFr
doi: 10.1126/sciadv.ads3406
external_id:
isi:
- '001416079000003'
pmid:
- '39919179'
file:
- access_level: open_access
checksum: ae8f7e9914e4d2549ed9578e58a10c3c
content_type: application/pdf
creator: dernst
date_created: 2025-03-04T09:52:02Z
date_updated: 2025-03-04T09:52:02Z
file_id: '19287'
file_name: 2025_ScienceAdvance_Stepanenko.pdf
file_size: 1385761
relation: main_file
success: 1
file_date_updated: 2025-03-04T09:52:02Z
has_accepted_license: '1'
intvolume: ' 11'
isi: 1
issue: '6'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
pmid: 1
publication: Science Advances
publication_identifier:
eissn:
- 2375-2548
publication_status: published
publisher: AAAS
quality_controlled: '1'
scopus_import: '1'
status: public
title: 187Os nuclear resonance scattering to explore hyperfine interactions and lattice
dynamics for biological applications
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 11
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '19283'
abstract:
- lang: eng
text: "Context. The presence of dips in the gravity mode period spacing versus period
diagram of γ Doradus stars is now well established thanks to recent asteroseismic
studies. Such Lorentzian-shaped inertial dips arise from the interaction of gravito-inertial
modes in the radiative envelope of intermediate-mass main sequence stars with
pure inertial modes in their convective core, and allow us to study stellar internal
properties. This window onto stellar internal dynamics is extremely valuable in
the context of the understanding of angular-momentum transport inside stars, as
it allows us to probe rotation in their core.\r\n\r\nAims. We investigate the
signature and the detectability of a differential rotation between the convective
core and the near-core region inside γ Doradus stars from the properties of inertial
dips.\r\n\r\nMethods. We studied the coupling between gravito-inertial modes in
the radiative zone and pure inertial modes in the convective core in the sub-inertial
regime, allowing for a two-zone differential rotation from the two sides of the
core-to-envelope boundary. We solved the coupling equation numerically and matched
the result to an analytical derivation of the Lorentzian dip properties. We then
used typical values of measured near-core rotation and buoyancy travel time to
infer ranges of parameters for which differential core to near-core rotation would
be detectable in current Kepler data.\r\n\r\nResults. We show that increasing
the convective core rotation with respect to the near-core rotation leads to a
shift of the period of the observed dip to lower periods. In addition, the dip
gets deeper and thinner as the convective core rotation increases. We demonstrate
that such a signature is detectable in Kepler data, given appropriate dip-parameter
ranges and near-core structural properties.\r\n\r\nConclusions. Studying the dip
properties in asteroseismic data thus allows us to access core to near-core radial
differential rotation and to better understand the transport of angular momentum
at convective–radiative interfaces in intermediate-mass main sequence stars."
acknowledgement: 'We thank the referee for very constructive and detailed comments
that led to an improvement of the quality of our study. L.B. and L.B. gratefully
acknowledge support from the European Research Council (ERC) under the Horizon Europe
programme (Calcifer; Starting Grant agreement N°101165631). S. Mathis acknowledges
support from the PLATO CNES grant at CEA/DAp and from the European Research Council
through HORIZON ERC SyG Grant 4D-STAR 101071505. While partially funded by the European
Union, views and opinions expressed are however those of the author 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. L. Barrault thanks the members of the asteroseismology group of the Institute
of Astronomy (IvS) of KU Leuven, in particular T. Van Reeth, M. Vanrespaille, Z.
Guo and C. Aerts, for their warm welcome during a work visit in Spring 2024, and
very insightful input on the present study. The authors thank also the members of
the Asteroseismology and Stellar Dynamics group of the Institute of Science and
Technology Austria (ISTA) for very useful discussion: K. M. Smith, L. Einramhof,
S. Torres and A. Cristea.'
article_number: A225
article_processing_charge: Yes
article_type: original
author:
- first_name: Lucas
full_name: Barrault, Lucas
id: 4471a8fd-32c1-11ee-a9a4-fb670d398f64
last_name: Barrault
- first_name: S.
full_name: Mathis, S.
last_name: Mathis
- first_name: Lisa Annabelle
full_name: Bugnet, Lisa Annabelle
id: d9edb345-f866-11ec-9b37-d119b5234501
last_name: Bugnet
orcid: 0000-0003-0142-4000
citation:
ama: Barrault L, Mathis S, Bugnet LA. Constraining differential rotation in γ Doradus
stars from the properties of inertial dips. Astronomy & Astrophysics.
2025;694. doi:10.1051/0004-6361/202451541
apa: Barrault, L., Mathis, S., & Bugnet, L. A. (2025). Constraining differential
rotation in γ Doradus stars from the properties of inertial dips. Astronomy
& Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202451541
chicago: Barrault, Lucas, S. Mathis, and Lisa Annabelle Bugnet. “Constraining Differential
Rotation in γ Doradus Stars from the Properties of Inertial Dips.” Astronomy
& Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202451541.
ieee: L. Barrault, S. Mathis, and L. A. Bugnet, “Constraining differential rotation
in γ Doradus stars from the properties of inertial dips,” Astronomy & Astrophysics,
vol. 694. EDP Sciences, 2025.
ista: Barrault L, Mathis S, Bugnet LA. 2025. Constraining differential rotation
in γ Doradus stars from the properties of inertial dips. Astronomy & Astrophysics.
694, A225.
mla: Barrault, Lucas, et al. “Constraining Differential Rotation in γ Doradus Stars
from the Properties of Inertial Dips.” Astronomy & Astrophysics, vol.
694, A225, EDP Sciences, 2025, doi:10.1051/0004-6361/202451541.
short: L. Barrault, S. Mathis, L.A. Bugnet, Astronomy & Astrophysics 694 (2025).
corr_author: '1'
date_created: 2025-03-02T23:01:53Z
date_published: 2025-02-01T00:00:00Z
date_updated: 2026-02-16T12:09:14Z
day: '01'
ddc:
- '520'
department:
- _id: LiBu
doi: 10.1051/0004-6361/202451541
external_id:
isi:
- '001424452400025'
file:
- access_level: open_access
checksum: 568a5e5951f20483663df145a780fc3d
content_type: application/pdf
creator: dernst
date_created: 2025-03-04T09:57:03Z
date_updated: 2025-03-04T09:57:03Z
file_id: '19288'
file_name: 2025_AstronomyAstrophysics_Barrault.pdf
file_size: 7438476
relation: main_file
success: 1
file_date_updated: 2025-03-04T09:57:03Z
has_accepted_license: '1'
intvolume: ' 694'
isi: 1
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
project:
- _id: 914d8549-16d5-11f0-9cad-bbe6324c93a9
grant_number: '101165631'
name: 'Unveiling the mysteries of stellar dynamics: a pioneering journey in magnetoasteroseismology'
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: Constraining differential rotation in γ Doradus stars from the properties of
inertial dips
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: 694
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
_id: '19284'
abstract:
- lang: eng
text: The Hα nebular emission line is an optimal tracer for recent star formation
in galaxies. With the advent of JWST, this line has recently become observable
at z > 3 for the first time. We present a catalog of 1050 Hα emitters at 3.7 < z < 6.7
in the GOODS fields obtained from a blind search in JWST NIRCam/grism data. We
made use of the FRESCO survey’s 124 arcmin2 of observations in GOODS-North and
GOODS-South with the F444W filter, probing Hα at 4.9 < z < 6.7, and the CONGRESS
survey’s 62 arcmin2 of observations in GOODS-North with F356W, probing Hα at 3.8 < z < 5.1.
We found an overdensity with 98 sources at z ∼ 4.4 in GOODS-N, and confirmed previously
reported overdensities at z ∼ 5.2 in GOODS-N and at z ∼ 5.4 and z ∼ 5.9 in GOODS-S.
We computed the observed Hα luminosity functions (LFs) in three bins centered
at z ∼ 4.45, 5.30, and 6.15, which are the first such measurements at z > 3 obtained
based purely on spectroscopic data, robustly tracing galaxy star formation rates
(SFRs) beyond the peak of the cosmic star formation history. We compared our results
with theoretical predictions from three different simulations and found good agreement
at z ∼ 4 − 6. The UV LFs of this spectroscopically confirmed sample are in good
agreement with pre-JWST measurements obtained with photometrically selected objects.
Finally, we derived SFR functions and integrated them to compute the evolution
of the cosmic SFR densities across z ∼ 4 − 6, finding values in good agreement
with recent UV estimates from Lyman-break galaxies, which imply a continuous decrease
in SFR density by a factor of three over z ∼ 4 to z ∼ 6. Our work shows the power
of NIRCam grism observations to efficiently provide new tests for early galaxy
formation models based on emission line statistics.
acknowledgement: 'This work is based on observations made with the NASA/ESA/CSA James
Webb Space Telescope. The data were obtained from the Mikulski Archive for Space
Telescopes at the Space Telescope Science Institute, which is operated by the Association
of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127
for JWST. These observations are associated with program Nos. 1895 and 3577. The
authors sincerely thank the CONGRESS team (PIs: Egami & Sun) for developing their
observing program with a zero-exclusive-access period. We thank Aswin Vijayan and
Harley Katz for their help in analyzing the simulation data from FLARES and SPHINX.
This work has received funding from the Swiss State Secretariat for Education, Research,
and Innovation (SERI) under contract number MB22.00072, as well as from the Swiss
National Science Foundation (SNSF) through project grant 200020_207349. The Cosmic
Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant
DNRF140. Support for program #1895 was provided by NASA through a grant from the
Space Telescope Science Institute, which is operated by the Association of Universities
for Research in Astronomy, Inc., under NASA contract NAS 5-03127. Support for this
work for RPN was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A
awarded by the Space Telescope Science Institute, which is operated by the Association
of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555.
MS acknowledges support from the European Research Commission Consolidator Grant
101088789 (SFEER), from the CIDEGENT/2021/059 grant by Generalitat Valenciana, and
from project PID2023-149420NB-I00 funded by MICIU/AEI/10.13039/501100011033 and
by ERDF/EU.'
article_number: A178
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Alba
full_name: Covelo-Paz, Alba
last_name: Covelo-Paz
- first_name: Emma
full_name: Giovinazzo, Emma
last_name: Giovinazzo
- first_name: Pascal A.
full_name: Oesch, Pascal A.
last_name: Oesch
- first_name: Romain A.
full_name: Meyer, Romain A.
last_name: Meyer
- first_name: Andrea
full_name: Weibel, Andrea
last_name: Weibel
- first_name: Gabriel
full_name: Brammer, Gabriel
last_name: Brammer
- first_name: Yoshinobu
full_name: Fudamoto, Yoshinobu
last_name: Fudamoto
- first_name: Josephine
full_name: Kerutt, Josephine
last_name: Kerutt
- first_name: Jamie
full_name: Lin, Jamie
last_name: Lin
- first_name: Jasleen
full_name: Matharu, Jasleen
last_name: Matharu
- first_name: Rohan P.
full_name: Naidu, Rohan P.
last_name: Naidu
- first_name: Anna
full_name: Velichko, Anna
last_name: Velichko
- first_name: Victoria
full_name: Bollo, Victoria
last_name: Bollo
- first_name: Rychard
full_name: Bouwens, Rychard
last_name: Bouwens
- first_name: John
full_name: Chisholm, John
last_name: Chisholm
- first_name: Garth D.
full_name: Illingworth, Garth D.
last_name: Illingworth
- first_name: Ivan
full_name: Kramarenko, Ivan
id: 9a9394cb-3200-11ee-973b-f5ba2a8b16e4
last_name: Kramarenko
orcid: 0000-0001-5346-6048
- first_name: Daniel
full_name: Magee, Daniel
last_name: Magee
- first_name: Michael
full_name: Maseda, Michael
last_name: Maseda
- 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: Erica
full_name: Nelson, Erica
last_name: Nelson
- first_name: Naveen
full_name: Reddy, Naveen
last_name: Reddy
- first_name: Daniel
full_name: Schaerer, Daniel
last_name: Schaerer
- first_name: Mauro
full_name: Stefanon, Mauro
last_name: Stefanon
- first_name: Mengyuan
full_name: Xiao, Mengyuan
last_name: Xiao
citation:
ama: 'Covelo-Paz A, Giovinazzo E, Oesch PA, et al. An Hα view of galaxy buildup
in the first 2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy.
Astronomy & Astrophysics. 2025;694. doi:10.1051/0004-6361/202452363'
apa: 'Covelo-Paz, A., Giovinazzo, E., Oesch, P. A., Meyer, R. A., Weibel, A., Brammer,
G., … Xiao, M. (2025). An Hα view of galaxy buildup in the first 2 Gyr: Luminosity
functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy. Astronomy & Astrophysics.
EDP Sciences. https://doi.org/10.1051/0004-6361/202452363'
chicago: 'Covelo-Paz, Alba, Emma Giovinazzo, Pascal A. Oesch, Romain A. Meyer, Andrea
Weibel, Gabriel Brammer, Yoshinobu Fudamoto, et al. “An Hα View of Galaxy Buildup
in the First 2 Gyr: Luminosity Functions at z ∼ 4−6.5 from NIRCam/Grism Spectroscopy.”
Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202452363.'
ieee: 'A. Covelo-Paz et al., “An Hα view of galaxy buildup in the first 2
Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy,” Astronomy
& Astrophysics, vol. 694. EDP Sciences, 2025.'
ista: 'Covelo-Paz A, Giovinazzo E, Oesch PA, Meyer RA, Weibel A, Brammer G, Fudamoto
Y, Kerutt J, Lin J, Matharu J, Naidu RP, Velichko A, Bollo V, Bouwens R, Chisholm
J, Illingworth GD, Kramarenko I, Magee D, Maseda M, Matthee JJ, Nelson E, Reddy
N, Schaerer D, Stefanon M, Xiao M. 2025. An Hα view of galaxy buildup in the first
2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy. Astronomy
& Astrophysics. 694, A178.'
mla: 'Covelo-Paz, Alba, et al. “An Hα View of Galaxy Buildup in the First 2 Gyr:
Luminosity Functions at z ∼ 4−6.5 from NIRCam/Grism Spectroscopy.” Astronomy
& Astrophysics, vol. 694, A178, EDP Sciences, 2025, doi:10.1051/0004-6361/202452363.'
short: A. Covelo-Paz, E. Giovinazzo, P.A. Oesch, R.A. Meyer, A. Weibel, G. Brammer,
Y. Fudamoto, J. Kerutt, J. Lin, J. Matharu, R.P. Naidu, A. Velichko, V. Bollo,
R. Bouwens, J. Chisholm, G.D. Illingworth, I. Kramarenko, D. Magee, M. Maseda,
J.J. Matthee, E. Nelson, N. Reddy, D. Schaerer, M. Stefanon, M. Xiao, Astronomy
& Astrophysics 694 (2025).
date_created: 2025-03-02T23:01:54Z
date_published: 2025-02-12T00:00:00Z
date_updated: 2026-02-16T12:08:59Z
day: '12'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202452363
external_id:
arxiv:
- '2409.17241'
isi:
- '001420194600001'
file:
- access_level: open_access
checksum: b1e74644a0cd37550e9a553f8675c93f
content_type: application/pdf
creator: dernst
date_created: 2025-03-04T09:29:01Z
date_updated: 2025-03-04T09:29:01Z
file_id: '19285'
file_name: 2025_AstronomyAstrophysics_CoveloPaz.pdf
file_size: 1865856
relation: main_file
success: 1
file_date_updated: 2025-03-04T09:29:01Z
has_accepted_license: '1'
intvolume: ' 694'
isi: 1
language:
- iso: eng
month: '02'
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'
related_material:
link:
- relation: software
url: ' https://github.com/astroalba/fresco'
scopus_import: '1'
status: public
title: 'An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z
∼ 4−6.5 from NIRCam/grism spectroscopy'
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: 694
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '19363'
abstract:
- lang: eng
text: For a general family of non-negative functions matching upper and lower bounds
are established for their average over the values of any equidistributed sequence.
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Yik Tung
full_name: Chan, Yik Tung
id: c4c0afc8-9262-11ed-9231-d8b0bc743af1
last_name: Chan
orcid: 0000-0001-8467-4106
- first_name: Peter
full_name: Koymans, Peter
last_name: Koymans
- first_name: Carlo
full_name: Pagano, Carlo
last_name: Pagano
- first_name: Efthymios
full_name: Sofos, Efthymios
last_name: Sofos
citation:
ama: Chan S, Koymans P, Pagano C, Sofos E. Averages of multiplicative functions
along equidistributed sequences. Journal of Number Theory. 2025;273:1-36.
doi:10.1016/j.jnt.2025.01.005
apa: Chan, S., Koymans, P., Pagano, C., & Sofos, E. (2025). Averages of multiplicative
functions along equidistributed sequences. Journal of Number Theory. Elsevier.
https://doi.org/10.1016/j.jnt.2025.01.005
chicago: Chan, Stephanie, Peter Koymans, Carlo Pagano, and Efthymios Sofos. “Averages
of Multiplicative Functions along Equidistributed Sequences.” Journal of Number
Theory. Elsevier, 2025. https://doi.org/10.1016/j.jnt.2025.01.005.
ieee: S. Chan, P. Koymans, C. Pagano, and E. Sofos, “Averages of multiplicative
functions along equidistributed sequences,” Journal of Number Theory, vol.
273. Elsevier, pp. 1–36, 2025.
ista: Chan S, Koymans P, Pagano C, Sofos E. 2025. Averages of multiplicative functions
along equidistributed sequences. Journal of Number Theory. 273, 1–36.
mla: Chan, Stephanie, et al. “Averages of Multiplicative Functions along Equidistributed
Sequences.” Journal of Number Theory, vol. 273, Elsevier, 2025, pp. 1–36,
doi:10.1016/j.jnt.2025.01.005.
short: S. Chan, P. Koymans, C. Pagano, E. Sofos, Journal of Number Theory 273 (2025)
1–36.
corr_author: '1'
date_created: 2025-03-09T23:01:26Z
date_published: 2025-08-01T00:00:00Z
date_updated: 2025-12-30T08:06:16Z
day: '01'
ddc:
- '510'
department:
- _id: TiBr
doi: 10.1016/j.jnt.2025.01.005
external_id:
isi:
- '001444208500001'
file:
- access_level: open_access
checksum: 752c407eb186d391380b10a7505f66cf
content_type: application/pdf
creator: dernst
date_created: 2025-12-30T08:05:42Z
date_updated: 2025-12-30T08:05:42Z
file_id: '20889'
file_name: 2025_JourNumberTheory_Chan.pdf
file_size: 685204
relation: main_file
success: 1
file_date_updated: 2025-12-30T08:05:42Z
has_accepted_license: '1'
intvolume: ' 273'
isi: 1
language:
- iso: eng
month: '08'
oa: 1
oa_version: Published Version
page: 1-36
publication: Journal of Number Theory
publication_identifier:
issn:
- 0022-314X
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Averages of multiplicative functions along equidistributed sequences
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: 273
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19365'
abstract:
- lang: eng
text: We present a comprehensive analysis of H i absorption around 96 Lyα emitters
(LAEs) at z ≈ 3.3 (median Lyα luminosity ≈1042 erg s−1). These LAEs were identified
within eight MUSE fields, each (math. formular) on the sky and centered on a bright
background quasar, as part of the MUSEQuBES survey. Using Voigt profile fitting
for all H i absorbers detected within ±500 km s−1 of these LAEs, we compiled
a catalog of 800 H i absorption components. Our analysis shows that H i absorption
is enhanced near the LAEs compared to the intergalactic medium. However, no trend
is found between the column densities of H i absorbers and their impact parameters
from the LAEs (spanning ≈54–260 pkpc). Additionally, all galaxies associated
with Lyman-limit systems have impact parameters >50 pkpc from the quasar sightlines,
suggesting that true absorber hosts may be too faint to detect. The LAEs show
an overall H i covering fraction (fc(H i)) of ≈88% for a threshold (math. formular)
(H i) = 15. Notably, at the same threshold, the LAEs in pairs/groups exhibit a
100% H i covering fraction out to ≈250 pkpc. In contrast, isolated LAEs consistently
show a lower fc(H i) of ≈80%. This environmental influence on fc(H i) is also
evident up to ≈300 km s−1 in differential bins of line-of-sight velocity. We find
an anticorrelation between fc(H i) and the equivalent width of rest-frame Lyα
emission (EW0). Based on the Lyα shell model, this could imply that gas-rich galaxies
tend to reside in gas-rich environments or that the LAEs with higher EW0 are more
efficient at ionizing their surrounding medium.
acknowledgement: "We would like to thank the anonymous referee for useful comments.
We thank Marijke Segers, Lorrie Straka, and Monica Turner for their early contributions
to the MUSEQuBES project. We thank Raghunathan Srianand for useful suggestions.
E.B. thanks Labanya Kumar Guha and Yucheng Guo for helpful discussions. S.C. gratefully
acknowledges the fund support from the European Research Council (ERC).\r\n\r\nSoftware:
NumPy (C. R. Harris et al. 2020), SciPy (P. Virtanen et al. 2020), Matplotlib (J.
D. Hunter 2007), and AstroPy (Astropy Collaboration et al. 2013, 2018)."
article_number: '171'
article_processing_charge: Yes
article_type: original
author:
- first_name: Eshita
full_name: Banerjee, Eshita
last_name: Banerjee
- first_name: Sowgat
full_name: Muzahid, Sowgat
last_name: Muzahid
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Jérémy
full_name: Blaizot, Jérémy
last_name: Blaizot
- first_name: Nicolas
full_name: Bouché, Nicolas
last_name: Bouché
- first_name: Sebastiano
full_name: Cantalupo, Sebastiano
last_name: Cantalupo
- first_name: Sean D.
full_name: Johnson, Sean D.
last_name: Johnson
- 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: Anne
full_name: Verhamme, Anne
last_name: Verhamme
citation:
ama: 'Banerjee E, Muzahid S, Schaye J, et al. MUSEQuBES: Connecting H i Absorption
with Lyα emitters at z ≈ 3.3. The Astrophysical Journal. 2025;980(2). doi:10.3847/1538-4357/ada7e9'
apa: 'Banerjee, E., Muzahid, S., Schaye, J., Blaizot, J., Bouché, N., Cantalupo,
S., … Verhamme, A. (2025). MUSEQuBES: Connecting H i Absorption with Lyα emitters
at z ≈ 3.3. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ada7e9'
chicago: 'Banerjee, Eshita, Sowgat Muzahid, Joop Schaye, Jérémy Blaizot, Nicolas
Bouché, Sebastiano Cantalupo, Sean D. Johnson, Jorryt J Matthee, and Anne Verhamme.
“MUSEQuBES: Connecting H i Absorption with Lyα Emitters at z ≈ 3.3.” The Astrophysical
Journal. IOP Publishing, 2025. https://doi.org/10.3847/1538-4357/ada7e9.'
ieee: 'E. Banerjee et al., “MUSEQuBES: Connecting H i Absorption with Lyα
emitters at z ≈ 3.3,” The Astrophysical Journal, vol. 980, no. 2. IOP Publishing,
2025.'
ista: 'Banerjee E, Muzahid S, Schaye J, Blaizot J, Bouché N, Cantalupo S, Johnson
SD, Matthee JJ, Verhamme A. 2025. MUSEQuBES: Connecting H i Absorption with Lyα
emitters at z ≈ 3.3. The Astrophysical Journal. 980(2), 171.'
mla: 'Banerjee, Eshita, et al. “MUSEQuBES: Connecting H i Absorption with Lyα Emitters
at z ≈ 3.3.” The Astrophysical Journal, vol. 980, no. 2, 171, IOP Publishing,
2025, doi:10.3847/1538-4357/ada7e9.'
short: E. Banerjee, S. Muzahid, J. Schaye, J. Blaizot, N. Bouché, S. Cantalupo,
S.D. Johnson, J.J. Matthee, A. Verhamme, The Astrophysical Journal 980 (2025).
date_created: 2025-03-09T23:01:26Z
date_published: 2025-02-20T00:00:00Z
date_updated: 2026-02-16T12:42:00Z
day: '20'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ada7e9
external_id:
isi:
- '001421001500001'
file:
- access_level: open_access
checksum: 1d33a8eb59f42a0c7a943c8859e9b883
content_type: application/pdf
creator: dernst
date_created: 2025-03-10T11:54:52Z
date_updated: 2025-03-10T11:54:52Z
file_id: '19379'
file_name: 2025_AstrophysicalJour_Banerjee.pdf
file_size: 1194131
relation: main_file
success: 1
file_date_updated: 2025-03-10T11:54:52Z
has_accepted_license: '1'
intvolume: ' 980'
isi: 1
issue: '2'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'MUSEQuBES: Connecting H i Absorption with Lyα emitters at z ≈ 3.3'
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: 980
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '19366'
abstract:
- lang: eng
text: Staphylococcus aureus (S. aureus) is one of the most common causative agents
of mammary gland infection and mastitis, but the specific role of S. aureus-derived
extracellular vesicles (SaEVs) in mastitis has been poorly studied to date. Here,
we aimed to investigate the response of bovine monocyte-derived macrophages (boMdM)
to SaEVs of the genotype B (GTB) mastitis-related strain M5512B. Specifically,
we evaluated the effects on the actin cytoskeleton, gene expression, and the SaEV
proteomic cargo. Furthermore, we assessed to what extent the cellular and molecular
response of boMdM to SaEVs differed from peripheral mononuclear blood cells (PBMCs)
used for in vitro derivation of the former. We observed that SaEVs induced morphological
changes in boMdM, leading to a pro-inflammatory and pyroptosis-related increased
gene expression. Additionally, our study revealed that boMdM and PBMCs exhibited
stimulus-specific differing responses. The proteomic analysis of SaEVs identified
clusters of proteins related to virulence and antibiotic resistance, supporting
the theory that S. aureus might use EVs to evade host defences and colonize the
mammary gland. Our results bring new insights into how SaEVs might impact the
host during an S. aureus infection, which can be useful for future S. aureus vaccine
development.
acknowledgement: "The authors thank Michele Guastalla for his contributions to the
boMdM analyses and Stephan Handschin from the Scientific Center for Optical and
Electron Microscopy (ScopeM) of ETH Zurich for the TEM imaging. We gratefully acknowledge
the Functional Genomics Center Zurich (FGCZ) for performing the mass spectrometry
analysis for this study.\r\nOpen access funding provided by Swiss Federal Institute
of Technology Zurich. This work was supported by basic funding from ETH Zurich."
article_processing_charge: Yes
article_type: original
author:
- first_name: Mara D.
full_name: Saenz-De-Juano, Mara D.
last_name: Saenz-De-Juano
- first_name: Giulia
full_name: Silvestrelli, Giulia
id: 12632ae8-799e-11ef-94a2-e5a3b5ef49e9
last_name: Silvestrelli
- first_name: Samuel
full_name: Buri, Samuel
last_name: Buri
- first_name: Léa V.
full_name: Zinsli, Léa V.
last_name: Zinsli
- first_name: Mathias
full_name: Schmelcher, Mathias
last_name: Schmelcher
- first_name: Susanne E.
full_name: Ulbrich, Susanne E.
last_name: Ulbrich
citation:
ama: Saenz-De-Juano MD, Silvestrelli G, Buri S, Zinsli LV, Schmelcher M, Ulbrich
SE. Mastitis-related Staphylococcus aureus-derived extracellular vesicles induce
a pro-inflammatory response in bovine monocyte-derived macrophages. Scientific
Reports. 2025;15:6059. doi:10.1038/s41598-025-90466-6
apa: Saenz-De-Juano, M. D., Silvestrelli, G., Buri, S., Zinsli, L. V., Schmelcher,
M., & Ulbrich, S. E. (2025). Mastitis-related Staphylococcus aureus-derived
extracellular vesicles induce a pro-inflammatory response in bovine monocyte-derived
macrophages. Scientific Reports. Springer Nature. https://doi.org/10.1038/s41598-025-90466-6
chicago: Saenz-De-Juano, Mara D., Giulia Silvestrelli, Samuel Buri, Léa V. Zinsli,
Mathias Schmelcher, and Susanne E. Ulbrich. “Mastitis-Related Staphylococcus Aureus-Derived
Extracellular Vesicles Induce a pro-Inflammatory Response in Bovine Monocyte-Derived
Macrophages.” Scientific Reports. Springer Nature, 2025. https://doi.org/10.1038/s41598-025-90466-6.
ieee: M. D. Saenz-De-Juano, G. Silvestrelli, S. Buri, L. V. Zinsli, M. Schmelcher,
and S. E. Ulbrich, “Mastitis-related Staphylococcus aureus-derived extracellular
vesicles induce a pro-inflammatory response in bovine monocyte-derived macrophages,”
Scientific Reports, vol. 15. Springer Nature, p. 6059, 2025.
ista: Saenz-De-Juano MD, Silvestrelli G, Buri S, Zinsli LV, Schmelcher M, Ulbrich
SE. 2025. Mastitis-related Staphylococcus aureus-derived extracellular vesicles
induce a pro-inflammatory response in bovine monocyte-derived macrophages. Scientific
Reports. 15, 6059.
mla: Saenz-De-Juano, Mara D., et al. “Mastitis-Related Staphylococcus Aureus-Derived
Extracellular Vesicles Induce a pro-Inflammatory Response in Bovine Monocyte-Derived
Macrophages.” Scientific Reports, vol. 15, Springer Nature, 2025, p. 6059,
doi:10.1038/s41598-025-90466-6.
short: M.D. Saenz-De-Juano, G. Silvestrelli, S. Buri, L.V. Zinsli, M. Schmelcher,
S.E. Ulbrich, Scientific Reports 15 (2025) 6059.
date_created: 2025-03-09T23:01:26Z
date_published: 2025-02-19T00:00:00Z
date_updated: 2025-09-30T10:58:59Z
day: '19'
ddc:
- '570'
department:
- _id: LoSw
doi: 10.1038/s41598-025-90466-6
external_id:
isi:
- '001426697000031'
pmid:
- '39972051'
file:
- access_level: open_access
checksum: 51b55ae299de1fa126016a11024b499a
content_type: application/pdf
creator: dernst
date_created: 2025-03-10T12:00:34Z
date_updated: 2025-03-10T12:00:34Z
file_id: '19380'
file_name: 2025_ScientificReports_SaenzdeJuano.pdf
file_size: 2780316
relation: main_file
success: 1
file_date_updated: 2025-03-10T12:00:34Z
has_accepted_license: '1'
intvolume: ' 15'
isi: 1
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
page: '6059'
pmid: 1
publication: Scientific Reports
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ama: De Jaeger-Braet JG. Arabidopsis accessions and their difference in heat tolerance
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apa: De Jaeger-Braet, J. G. (2025). Arabidopsis accessions and their difference
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https://doi.org/10.1093/plphys/kiaf055
chicago: De Jaeger-Braet, Joke G. “Arabidopsis Accessions and Their Difference in
Heat Tolerance during Meiosis.” Plant Physiology. Oxford University Press,
2025. https://doi.org/10.1093/plphys/kiaf055.
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tolerance during meiosis,” Plant Physiology, vol. 197, no. 2. Oxford University
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Tolerance during Meiosis.” Plant Physiology, vol. 197, no. 2, kiaf055,
Oxford University Press, 2025, doi:10.1093/plphys/kiaf055.
short: J.G. De Jaeger-Braet, Plant Physiology 197 (2025).
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title: Arabidopsis accessions and their difference in heat tolerance during meiosis
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