---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '20546'
abstract:
- lang: eng
text: Rocky debris covers around 7.3 % of the global glacier area, influencing ice
melt rates and the surface mass balance of glaciers, making the dynamics and hydrology
of debris-covered glaciers distinct from those of clean-ice glaciers. Accurate
representation of debris in models is challenging, as measurements of the physical
properties and thickness of the supraglacial debris layer are scarce. Here, we
compile a database of measured and reported bulk physical properties and layer
thicknesses of supraglacial debris that we call the supraglacial Debris Database
(DebDaB) and that is open to community submissions. The majority of the database
(90 %) is compiled from 172 sources in the literature, and the remaining 10 %
was previously unpublished. DebDaB contains 8741 data entries for supraglacial
debris layer thickness, of which 1770 entries also include sub-debris ablation
rates, 179 thermal conductivity of debris, 160 aerodynamic surface roughness length,
79 debris albedo, 59 debris emissivity, and 37 debris porosity. The data are distributed
over 84 glaciers in 13 regions in the Global Terrestrial Network for Glaciers.
We show regional differences in the distribution of debris thickness measurements
in DebDaB and fit simplified Østrem curves to 19 glaciers with sufficient debris
thickness and ablation data. The data in DebDaB can be used for energy balance,
melt, and surface mass balance studies by incorporating site-specific debris properties
or for evaluation of remote sensing estimates of debris thickness and surface
roughness. They can also help future field campaigns on debris-covered glaciers
by identifying observation gaps. DebDaB's uneven spatial coverage points to sampling
biases in community efforts to observe debris-covered glaciers, with some regions
(e.g. central Europe and South Asia) well-sampled but others having gaps with
prevalent debris (e.g. the Andes and Alaska). Debris thickness measurements are
mostly concentrated at lower elevations, leaving higher-elevation debris-covered
areas undersampled and suggesting that our knowledge of debris properties might
not be representative of all elevations. The aims of DebDaB, as an openly available
dataset, are to evolve over time, to be updated, and to add to community submissions
as new data on supraglacial properties become available. The data described in
this paper can be accessed from Zenodo at https://doi.org/10.5281/zenodo.14224835
(Groeneveld et al., 2025).
acknowledgement: "This work was supported by SNF project RENOIR (“Resolving the thickness
of debris on Earth’s glaciers and its rate of change”; grant no. 204322). This project
received funding from the European Research Council (ERC) under the European Union’s
Horizon 2020 research and\r\ninnovation programme (grant no. 772751; RAVEN: “Rapid
mass losses of debris covered glaciers in High Mountain Asia”). The authors acknowledge
DCGWG of IACS for setting the stage and bringing together the debris-covered glacier
community to focus on broader needs transcending a specific research topic and for
starting the Zenodo community on debris-covered glaciers, where this database is
hosted. The authors thank Achim A. Beylich (topical editor), Ken\r\nMankoff (chief
editor), Morgan Jones (reviewer), and an anonymous reviewer for their constructive
feedback, comments, and discussions on the database and paper."
article_processing_charge: Yes
article_type: original
author:
- first_name: Adrià
full_name: Fontrodona-Bach, Adrià
id: f06891fd-9f42-11ee-8632-a20971c43046
last_name: Fontrodona-Bach
- first_name: Lars
full_name: Groeneveld, Lars
last_name: Groeneveld
- first_name: Evan
full_name: Miles, Evan
last_name: Miles
- first_name: Michael
full_name: McCarthy, Michael
id: 22a2674a-61ce-11ee-94b5-d18813baf16f
last_name: McCarthy
- first_name: Thomas
full_name: Shaw, Thomas
id: 3caa3f91-1f03-11ee-96ce-e0e553054d6e
last_name: Shaw
orcid: 0000-0001-7640-6152
- first_name: Juan Vicente
full_name: Melo Velasco, Juan Vicente
id: 2611dec0-b9c6-11ed-9bea-a81c2b17a549
last_name: Melo Velasco
- first_name: Francesca
full_name: Pellicciotti, Francesca
id: b28f055a-81ea-11ed-b70c-a9fe7f7b0e70
last_name: Pellicciotti
orcid: 0000-0002-5554-8087
citation:
ama: 'Fontrodona-Bach A, Groeneveld L, Miles E, et al. DebDaB: A database of supraglacial
debris thickness and physical properties. Earth System Science Data. 2025;17(8):4213-4234.
doi:10.5194/essd-17-4213-2025'
apa: 'Fontrodona-Bach, A., Groeneveld, L., Miles, E., McCarthy, M., Shaw, T., Melo
Velasco, J. V., & Pellicciotti, F. (2025). DebDaB: A database of supraglacial
debris thickness and physical properties. Earth System Science Data. Copernicus
Publications. https://doi.org/10.5194/essd-17-4213-2025'
chicago: 'Fontrodona-Bach, Adrià, Lars Groeneveld, Evan Miles, Michael McCarthy,
Thomas Shaw, Juan Vicente Melo Velasco, and Francesca Pellicciotti. “DebDaB: A
Database of Supraglacial Debris Thickness and Physical Properties.” Earth
System Science Data. Copernicus Publications, 2025. https://doi.org/10.5194/essd-17-4213-2025.'
ieee: 'A. Fontrodona-Bach et al., “DebDaB: A database of supraglacial debris
thickness and physical properties,” Earth System Science Data, vol. 17,
no. 8. Copernicus Publications, pp. 4213–4234, 2025.'
ista: 'Fontrodona-Bach A, Groeneveld L, Miles E, McCarthy M, Shaw T, Melo Velasco
JV, Pellicciotti F. 2025. DebDaB: A database of supraglacial debris thickness
and physical properties. Earth System Science Data. 17(8), 4213–4234.'
mla: 'Fontrodona-Bach, Adrià, et al. “DebDaB: A Database of Supraglacial Debris
Thickness and Physical Properties.” Earth System Science Data, vol. 17,
no. 8, Copernicus Publications, 2025, pp. 4213–34, doi:10.5194/essd-17-4213-2025.'
short: A. Fontrodona-Bach, L. Groeneveld, E. Miles, M. McCarthy, T. Shaw, J.V. Melo
Velasco, F. Pellicciotti, Earth System Science Data 17 (2025) 4213–4234.
corr_author: '1'
date_created: 2025-10-27T08:21:22Z
date_published: 2025-08-29T00:00:00Z
date_updated: 2025-12-01T15:05:58Z
day: '29'
ddc:
- '550'
department:
- _id: FrPe
doi: 10.5194/essd-17-4213-2025
external_id:
isi:
- '001560847000001'
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checksum: f77ebb9825f374134a89e0e6311fe188
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date_created: 2025-10-27T08:38:40Z
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file_size: 3842196
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intvolume: ' 17'
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month: '08'
oa: 1
oa_version: Published Version
page: 4213-4234
publication: Earth System Science Data
publication_identifier:
issn:
- 1866-3516
publication_status: published
publisher: Copernicus Publications
quality_controlled: '1'
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title: 'DebDaB: A database of supraglacial debris thickness and physical properties'
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...
---
OA_place: repository
OA_type: gold
_id: '20547'
abstract:
- lang: eng
text: "DebdaB is a database of measured and reported physical properties and thickness
of supraglacial debris that is openly available and open to community submissions.\r\n\r\nThe
majority of the database (90%) is compiled from 172 sources in the literature,
and the remaining 10% has not been published before. DebDaB contains 8,286 data
entries for supraglacial debris thickness, of which 1,852 entries also include
sub-debris ablation rates, 167 data entries of thermal conductivity of debris,
157 of aerodynamic surface roughness length, 77 of debris albedo, 56 of debris
emissivity and 37 of debris porosity. The data are distributed over 83 glaciers
in 13 regions in the Global Terrestrial Network for Glaciers. "
article_processing_charge: No
author:
- first_name: Lars
full_name: Groeneveld, Lars
last_name: Groeneveld
- first_name: Adrià
full_name: Fontrodona-Bach, Adrià
id: f06891fd-9f42-11ee-8632-a20971c43046
last_name: Fontrodona-Bach
- first_name: Evan
full_name: Miles, Evan
last_name: Miles
- first_name: Michael
full_name: McCarthy, Michael
id: 22a2674a-61ce-11ee-94b5-d18813baf16f
last_name: McCarthy
- first_name: Juan Vicente
full_name: Melo Velasco, Juan Vicente
id: 2611dec0-b9c6-11ed-9bea-a81c2b17a549
last_name: Melo Velasco
- first_name: Thomas
full_name: Shaw, Thomas
id: 3caa3f91-1f03-11ee-96ce-e0e553054d6e
last_name: Shaw
orcid: 0000-0001-7640-6152
- first_name: Francesca
full_name: Pellicciotti, Francesca
id: b28f055a-81ea-11ed-b70c-a9fe7f7b0e70
last_name: Pellicciotti
orcid: 0000-0002-5554-8087
- first_name: Andreas
full_name: Bauder, Andreas
last_name: Bauder
- first_name: Pascal
full_name: Buri, Pascal
last_name: Buri
- first_name: Marin
full_name: Kneib, Marin
last_name: Kneib
- first_name: Amit
full_name: Kumar, Amit
last_name: Kumar
- first_name: Aditya
full_name: Mishra, Aditya
last_name: Mishra
- first_name: lene
full_name: Petersen, lene
last_name: Petersen
- first_name: Roman
full_name: Renner, Roman
last_name: Renner
- first_name: Sandro
full_name: Schmid, Sandro
last_name: Schmid
citation:
ama: 'Groeneveld L, Fontrodona-Bach A, Miles E, et al. DebDaB: A database of supraglacial
debris thickness and physical properties. 2025. doi:10.5281/ZENODO.14224835'
apa: 'Groeneveld, L., Fontrodona-Bach, A., Miles, E., McCarthy, M., Melo Velasco,
J. V., Shaw, T., … Schmid, S. (2025). DebDaB: A database of supraglacial debris
thickness and physical properties. Zenodo. https://doi.org/10.5281/ZENODO.14224835'
chicago: 'Groeneveld, Lars, Adrià Fontrodona-Bach, Evan Miles, Michael McCarthy,
Juan Vicente Melo Velasco, Thomas Shaw, Francesca Pellicciotti, et al. “DebDaB:
A Database of Supraglacial Debris Thickness and Physical Properties.” Zenodo,
2025. https://doi.org/10.5281/ZENODO.14224835.'
ieee: 'L. Groeneveld et al., “DebDaB: A database of supraglacial debris thickness
and physical properties.” Zenodo, 2025.'
ista: 'Groeneveld L, Fontrodona-Bach A, Miles E, McCarthy M, Melo Velasco JV, Shaw
T, Pellicciotti F, Bauder A, Buri P, Kneib M, Kumar A, Mishra A, Petersen lene,
Renner R, Schmid S. 2025. DebDaB: A database of supraglacial debris thickness
and physical properties, Zenodo, 10.5281/ZENODO.14224835.'
mla: 'Groeneveld, Lars, et al. DebDaB: A Database of Supraglacial Debris Thickness
and Physical Properties. Zenodo, 2025, doi:10.5281/ZENODO.14224835.'
short: L. Groeneveld, A. Fontrodona-Bach, E. Miles, M. McCarthy, J.V. Melo Velasco,
T. Shaw, F. Pellicciotti, A. Bauder, P. Buri, M. Kneib, A. Kumar, A. Mishra, lene
Petersen, R. Renner, S. Schmid, (2025).
date_created: 2025-10-27T08:42:09Z
date_published: 2025-05-16T00:00:00Z
date_updated: 2025-12-01T15:05:58Z
day: '16'
ddc:
- '550'
department:
- _id: FrPe
doi: 10.5281/ZENODO.14224835
main_file_link:
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url: https://doi.org/10.5281/zenodo.15441000
month: '05'
oa: 1
oa_version: Published Version
publisher: Zenodo
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status: public
title: 'DebDaB: A database of supraglacial debris thickness and physical properties'
type: research_data_reference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_place: publisher
_id: '20551'
abstract:
- lang: eng
text: "The space of codimension-2 shapes, such as curves in 3D and surfaces in 4D,
is an infinite-dimensional manifold. This thesis explores geometric structures
and dynamics on this space, with emphasis on their implications for physics, particularly
hydrodynamics.\r\n\r\nOur investigation ranges from theoretical studies of infinite-dimensional
symplectic and prequantum geometry to numerical computation of the time evolution
of shapes. The thesis presents four main contributions.\r\n\r\nIn the first part,
we introduce implicit representations of codimension-2 shapes using a class of
complex-valued functions, and prove that the space of these implicit representations
forms a prequantum bundle over the codimension-2 shape space. This reveals a new
geometric interpretation of the canonical symplectic structure on the codimension-2
shape space.\r\n\r\nIn the second part, we use implicit representations to develop
a simulation method for the dynamics of space curves. To handle chaotic systems
such as vortex filaments in hydrodynamics, we exploit the infinite degrees of
freedom, hidden in both the configuration and dynamics of implicit representations.\r\n\r\nIn
the third part, we introduce new symplectic structures on the space of space curves,
which generalize the only previously known symplectic structure on this space,
allowing for new Hamiltonian dynamics of space curves.\r\n\r\nIn the fourth part,
we apply a symplectic viewpoint to a differential geometric problem with practical
applications. We derive a new area formula for spherical polygons via prequantization. "
acknowledged_ssus:
- _id: CampIT
acknowledgement: "Projects contained in this thesis were financially supported in
part by the\r\nEuropean Research Council with grants 1. ERC Consolidator Grant 101045083
CoDiNA,\r\nand 2. the European Union’s Horizon 2020 research and innovation programme
under grant\r\nagreement No. 638176."
alternative_title:
- ISTA Thesis
article_processing_charge: No
author:
- first_name: Sadashige
full_name: Ishida, Sadashige
id: 6F7C4B96-A8E9-11E9-A7CA-09ECE5697425
last_name: Ishida
orcid: 0000-0002-3121-3100
citation:
ama: Ishida S. Symplectic-prequantum structures and dynamics on the codimension-2
shape space. 2025. doi:10.15479/AT-ISTA-20551
apa: Ishida, S. (2025). Symplectic-prequantum structures and dynamics on the
codimension-2 shape space. Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-20551
chicago: Ishida, Sadashige. “Symplectic-Prequantum Structures and Dynamics on the
Codimension-2 Shape Space.” Institute of Science and Technology Austria, 2025.
https://doi.org/10.15479/AT-ISTA-20551.
ieee: S. Ishida, “Symplectic-prequantum structures and dynamics on the codimension-2
shape space,” Institute of Science and Technology Austria, 2025.
ista: Ishida S. 2025. Symplectic-prequantum structures and dynamics on the codimension-2
shape space. Institute of Science and Technology Austria.
mla: Ishida, Sadashige. Symplectic-Prequantum Structures and Dynamics on the
Codimension-2 Shape Space. Institute of Science and Technology Austria, 2025,
doi:10.15479/AT-ISTA-20551.
short: S. Ishida, Symplectic-Prequantum Structures and Dynamics on the Codimension-2
Shape Space, Institute of Science and Technology Austria, 2025.
corr_author: '1'
date_created: 2025-10-27T10:28:52Z
date_published: 2025-10-31T00:00:00Z
date_updated: 2026-04-07T12:02:23Z
day: '31'
ddc:
- '516'
degree_awarded: PhD
department:
- _id: GradSch
- _id: ChWo
doi: 10.15479/AT-ISTA-20551
ec_funded: 1
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language:
- iso: eng
month: '10'
oa: 1
oa_version: Published Version
page: '141'
project:
- _id: 2533E772-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '638176'
name: 'Big Splash: Efficient Simulation of Natural Phenomena at Extremely Large
Scales'
- _id: 34bc2376-11ca-11ed-8bc3-9a3b3961a088
grant_number: '101045083'
name: Computational Discovery of Numerical Algorithms for Animation and Simulation
of Natural Phenomena
publication_identifier:
isbn:
- 978-3-99078-070-1
issn:
- 2663-337X
publication_status: published
publisher: Institute of Science and Technology Austria
related_material:
record:
- id: '12846'
relation: part_of_dissertation
status: public
- id: '12431'
relation: part_of_dissertation
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- id: '17361'
relation: part_of_dissertation
status: public
- id: '20580'
relation: part_of_dissertation
status: public
status: public
supervisor:
- first_name: Christopher J
full_name: Wojtan, Christopher J
id: 3C61F1D2-F248-11E8-B48F-1D18A9856A87
last_name: Wojtan
orcid: 0000-0001-6646-5546
- first_name: Albert
full_name: Chern, Albert
last_name: Chern
title: Symplectic-prequantum structures and dynamics on the codimension-2 shape space
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type: dissertation
user_id: ba8df636-2132-11f1-aed0-ed93e2281fdd
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...
---
OA_place: publisher
_id: '20556'
abstract:
- lang: eng
text: "Verifiable Delay Functions (VDFs) introduced by Boneh et al. (CRYPTO'18)
are functions that require a prescribed number of sequential steps T to evaluate,
yet their output can be verified in time much faster than T. Since their introduction,
VDFs have gained a lot of attention due to their applications in blockchain protocols,
randomness beacons, timestamping and deniability. This thesis explores the theory
and applications of VDFs, focusing on enhancing their soundness, efficiency and
practicality.\r\n\r\nThe only practical VDFs known to date are based on repeated
squaring in hidden order groups. Consider the function VDF(x,T)=x^(2^T).\r\nThe
iterated squaring assumption states that, for a random group element x, the result
of VDF cannot be computed significantly faster than performing T sequential squarings
if the group order is unknown. To make the result verifiable a prover can compute
a proof of exponentiation (PoE) \\pi. Given \\pi, the output of VDF can be verified
in time much less than T.\r\n\r\nWe first present new constructions of statistically
sound proofs of exponentiation, which are an important building block in the construction
of SNARKs (Succinct Non-Interactive Argument of Knowledge). Statistical soundness
means that the proofs remain secure against computationally unbounded adversaries,
in particular, it remains secure even when the group order is known. We thereby
address limitations in previous PoE protocols which either required (non-standard)
hardness assumptions or a lot of parallel repetitions. Our construction significantly
reduces the proof size of statistically sound PoEs that allow for a structured
exponent, which leads to better efficiency of SNARKs and other applications.\r\n\r\nSecondly,
we introduce improved batching techniques for PoEs, which allow multiple proofs
to be aggregated and verified with minimal overhead. These protocols optimize
communication and computation complexity in large-scale blockchain environments
and enable scalable remote benchmarking of parallel computation resources.\r\n\r\nWe
then construct VDFs with enhanced properties such as zero-knowledge and watermarkability.
It was shown by Arun, Bonneau and Clark (ASIACRYPT'22) that these features enable
new cryptographic primitives called short-lived proofs and signatures. The validity
of such proofs and signatures expires after a predefined amount of time T, i.e.,
they are deniable after time T. Our constructions improve upon the constructions
by Arun, Bonneau and Clark in several dimensions (faster forging times, arguably
weaker assumptions).\r\n\r\nFinally, we apply PoEs in the realm of primality testing,
providing cryptographically sound proofs of non-primality for large Proth numbers.
This work gives a surprising application of VDFs in the area of computational
number theory.\r\n\r\nTogether, our contributions advance both the theoretical
foundations and the real-world usability of VDFs in general and in particular
of PoEs, making them more adaptable and secure for current and emerging cryptographic
applications."
alternative_title:
- ISTA Thesis
article_processing_charge: No
author:
- first_name: Charlotte
full_name: Hoffmann, Charlotte
id: 0f78d746-dc7d-11ea-9b2f-83f92091afe7
last_name: Hoffmann
orcid: 0000-0003-2027-5549
citation:
ama: Hoffmann C. Theory and applications of verifiable delay functions. 2025. doi:10.15479/AT-ISTA-20556
apa: Hoffmann, C. (2025). Theory and applications of verifiable delay functions.
Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-20556
chicago: Hoffmann, Charlotte. “Theory and Applications of Verifiable Delay Functions.”
Institute of Science and Technology Austria, 2025. https://doi.org/10.15479/AT-ISTA-20556.
ieee: C. Hoffmann, “Theory and applications of verifiable delay functions,” Institute
of Science and Technology Austria, 2025.
ista: Hoffmann C. 2025. Theory and applications of verifiable delay functions. Institute
of Science and Technology Austria.
mla: Hoffmann, Charlotte. Theory and Applications of Verifiable Delay Functions.
Institute of Science and Technology Austria, 2025, doi:10.15479/AT-ISTA-20556.
short: C. Hoffmann, Theory and Applications of Verifiable Delay Functions, Institute
of Science and Technology Austria, 2025.
corr_author: '1'
date_created: 2025-10-27T14:16:56Z
date_published: 2025-10-31T00:00:00Z
date_updated: 2026-04-16T09:11:09Z
day: '31'
ddc:
- '004'
degree_awarded: PhD
department:
- _id: GradSch
- _id: KrPi
doi: 10.15479/AT-ISTA-20556
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month: '10'
oa_version: Published Version
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publisher: Institute of Science and Technology Austria
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- id: '20701'
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status: public
- id: '20920'
relation: later_version
status: public
- id: '19778'
relation: part_of_dissertation
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status: public
supervisor:
- first_name: Krzysztof Z
full_name: Pietrzak, Krzysztof Z
id: 3E04A7AA-F248-11E8-B48F-1D18A9856A87
last_name: Pietrzak
orcid: 0000-0002-9139-1654
title: Theory and applications of verifiable delay functions
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name: Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC
BY-NC-SA 4.0)
short: CC BY-NC-SA (4.0)
type: dissertation
user_id: ba8df636-2132-11f1-aed0-ed93e2281fdd
year: '2025'
...
---
OA_place: publisher
_id: '20575'
abstract:
- lang: eng
text: "This thesis deals with eigenvalue and eigenvector universality results for
random matrix ensembles equipped with non-trivial spatial structure. We consider
both mean-field models with a general variance profile (Wigner-type matrices)
and correlation structure (correlated matrices) among the entries, as well as
non-mean-field random band matrices with bandwidth W >> N^(1/2).\r\n\r\nTo extract
the universal properties of random matrix spectra and eigenvectors, we obtain
concentration estimates for their resolvent, the local laws, which generalize
the celebrated Wigner semicircle law for a broad class of random matrices to much
finer spectral scales. The local laws hold for both a single resolvent as well
as for products of multiple resolvents, known as resolvent chains, and express
the remarkable approximately-deterministic behavior of these objects down to the
microscopic scale.\r\n\r\nOur primary tool for establishing the local laws is
the dynamical Zigzag strategy, which we develop in the setting of spatially-inhomogeneous
random matrices. Our proof method systematically addresses the challenges arising
from non-trivial spatial structures and is robust to all types of singularities
in the spectrum, as we demonstrate in the correlated setting. Furthermore, we
incorporate the analysis of the deterministic resolvent chain approximations into
the dynamical framework of the Zigzag strategy, synthesizing a unified toolkit
for establishing multi-resolvent local laws.\r\n\r\nUsing these methods, we prove
complete eigenvector delocalization, the Eigenstate Thermalization Hypothesis,
and Wigner-Dyson universality in the bulk for random band matrices down to the
optimal bandwidth W >> N^(1/2). For mean-field ensembles, we establish universality
of local eigenvalue statistics at the cups for random matrices with correlated
entries, and the Eigenstate Thermalization Hypothesis for Wigner-type matrices
in the bulk of the spectrum.\r\n\r\nFinally, this thesis also contains other applications
of the multi-resolvent local laws to spatially-inhomogeneous random matrices,
obtained prior to the development of the Zigzag strategy. In particular, we provide
a complete analysis of mesoscopic linear-eigenvalue statistics of Wigner-type
matrices in all spectral regimes, including the novel cusps, and rigorously establish
the prethermalization phenomenon for deformed Wigner matrices.\r\n\r\nThe main
body of this thesis consists of seven research papers (listed on page xi), each
presented in a separate chapter with its own introduction and all relevant context,
suitable to be read independently. We ask the reader’s indulgence for the repetitions
in the historical overviews and other minor redundancies that remain among the
chapters as a result. The overall Introduction, preceding the chapters, provides
a condensed, informal summary of the main ideas and concepts at the core of these
works.\r\n"
acknowledgement: "The work comprising this thesis was supported by the ERC Advanced
Grant \"RMTBeyond\"\r\nNo.101020331 awarded to my advisor."
alternative_title:
- ISTA Thesis
article_processing_charge: No
author:
- first_name: Volodymyr
full_name: Riabov, Volodymyr
id: 1949f904-edfb-11eb-afb5-e2dfddabb93b
last_name: Riabov
citation:
ama: Riabov V. Universality in random matrices with spatial structure. 2025. doi:10.15479/AT-ISTA-20575
apa: Riabov, V. (2025). Universality in random matrices with spatial structure.
Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-20575
chicago: Riabov, Volodymyr. “Universality in Random Matrices with Spatial Structure.”
Institute of Science and Technology Austria, 2025. https://doi.org/10.15479/AT-ISTA-20575.
ieee: V. Riabov, “Universality in random matrices with spatial structure,” Institute
of Science and Technology Austria, 2025.
ista: Riabov V. 2025. Universality in random matrices with spatial structure. Institute
of Science and Technology Austria.
mla: Riabov, Volodymyr. Universality in Random Matrices with Spatial Structure.
Institute of Science and Technology Austria, 2025, doi:10.15479/AT-ISTA-20575.
short: V. Riabov, Universality in Random Matrices with Spatial Structure, Institute
of Science and Technology Austria, 2025.
corr_author: '1'
date_created: 2025-10-29T19:12:24Z
date_published: 2025-11-03T00:00:00Z
date_updated: 2026-04-07T12:32:20Z
day: '3'
ddc:
- '515'
- '519'
degree_awarded: PhD
department:
- _id: GradSch
- _id: LaEr
doi: 10.15479/AT-ISTA-20575
ec_funded: 1
file:
- access_level: open_access
checksum: 6a0487b2b66bb35d44b394756d44b8b4
content_type: application/pdf
creator: vriabov
date_created: 2025-10-29T18:53:59Z
date_updated: 2025-10-29T18:53:59Z
file_id: '20577'
file_name: riabov_thesis-pdfa.pdf
file_size: 7536583
relation: main_file
success: 1
- access_level: closed
checksum: 224efda6bf9864d296a1e5e0124c1e8f
content_type: application/x-zip-compressed
creator: vriabov
date_created: 2025-10-29T18:54:53Z
date_updated: 2025-10-29T18:54:53Z
file_id: '20578'
file_name: manuscript.zip
file_size: 17841612
relation: source_file
file_date_updated: 2025-10-29T18:54:53Z
has_accepted_license: '1'
language:
- iso: eng
month: '11'
oa: 1
oa_version: Published Version
page: '436'
project:
- _id: 62796744-2b32-11ec-9570-940b20777f1d
call_identifier: H2020
grant_number: '101020331'
name: Random matrices beyond Wigner-Dyson-Mehta
publication_identifier:
isbn:
- 978-3-99078-064-0
issn:
- 2663-337X
publication_status: published
publisher: Institute of Science and Technology Austria
related_material:
record:
- id: '20322'
relation: part_of_dissertation
status: public
- id: '18764'
relation: part_of_dissertation
status: public
- id: '13317'
relation: part_of_dissertation
status: public
- id: '19368'
relation: part_of_dissertation
status: deleted
- id: '18554'
relation: part_of_dissertation
status: public
- id: '20576'
relation: part_of_dissertation
status: public
- id: '17174'
relation: part_of_dissertation
status: public
- id: '19547'
relation: part_of_dissertation
status: public
- id: '19598'
relation: part_of_dissertation
status: public
status: public
supervisor:
- first_name: László
full_name: Erdös, László
id: 4DBD5372-F248-11E8-B48F-1D18A9856A87
last_name: Erdös
orcid: 0000-0001-5366-9603
title: Universality in random matrices with spatial structure
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: dissertation
user_id: ba8df636-2132-11f1-aed0-ed93e2281fdd
year: '2025'
...
---
OA_place: repository
_id: '20576'
abstract:
- lang: eng
text: We prove that a very general class of $N\times N$ Hermitian random band matrices
is in the delocalized phase when the band width $W$ exceeds the critical threshold,
$W\gg \sqrt{N}$. In this regime, we show that, in the bulk spectrum, the eigenfunctions
are fully delocalized, the eigenvalues follow the universal Wigner-Dyson statistics,
and quantum unique ergodicity holds for general diagonal observables with an optimal
convergence rate. Our results are valid for general variance profiles, arbitrary
single entry distributions, in both real-symmetric and complex-Hermitian symmetry
classes. In particular, our work substantially generalizes the recent breakthrough
result of Yau and Yin [arXiv:2501.01718], obtained for a specific complex Hermitian
Gaussian block band matrix. The main technical input is the optimal multi-resolvent
local laws -- both in the averaged and fully isotropic form. We also generalize
the $\sqrtη$-rule from [arXiv:2012.13215] to exploit the additional effect of
traceless observables. Our analysis is based on the zigzag strategy, complemented
with a new global-scale estimate derived using the static version of the master
inequalities, while the zig-step and the a priori estimates on the deterministic
approximations are proven dynamically.
acknowledgement: " Supported by the ERC\r\nAdvanced Grant ”RMTBeyond” No. 101020331."
article_processing_charge: No
author:
- first_name: László
full_name: Erdös, László
id: 4DBD5372-F248-11E8-B48F-1D18A9856A87
last_name: Erdös
orcid: 0000-0001-5366-9603
- first_name: Volodymyr
full_name: Riabov, Volodymyr
id: 1949f904-edfb-11eb-afb5-e2dfddabb93b
last_name: Riabov
citation:
ama: Erdös L, Riabov V. The zigzag strategy for random band matrices. arXiv.
doi:10.48550/ARXIV.2506.06441
apa: Erdös, L., & Riabov, V. (n.d.). The zigzag strategy for random band matrices.
arXiv. https://doi.org/10.48550/ARXIV.2506.06441
chicago: Erdös, László, and Volodymyr Riabov. “The Zigzag Strategy for Random Band
Matrices.” ArXiv, n.d. https://doi.org/10.48550/ARXIV.2506.06441.
ieee: L. Erdös and V. Riabov, “The zigzag strategy for random band matrices,” arXiv.
.
ista: Erdös L, Riabov V. The zigzag strategy for random band matrices. arXiv, 10.48550/ARXIV.2506.06441.
mla: Erdös, László, and Volodymyr Riabov. “The Zigzag Strategy for Random Band Matrices.”
ArXiv, doi:10.48550/ARXIV.2506.06441.
short: L. Erdös, V. Riabov, ArXiv (n.d.).
corr_author: '1'
date_created: 2025-10-29T19:09:03Z
date_published: 2025-06-06T00:00:00Z
date_updated: 2026-04-07T12:32:19Z
day: '06'
department:
- _id: GradSch
- _id: LaEr
doi: 10.48550/ARXIV.2506.06441
ec_funded: 1
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2506.06441
month: '06'
oa: 1
oa_version: Preprint
project:
- _id: 62796744-2b32-11ec-9570-940b20777f1d
call_identifier: H2020
grant_number: '101020331'
name: Random matrices beyond Wigner-Dyson-Mehta
publication: arXiv
publication_status: draft
related_material:
record:
- id: '20575'
relation: dissertation_contains
status: public
status: public
title: The zigzag strategy for random band matrices
type: preprint
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
year: '2025'
...
---
OA_place: repository
_id: '20580'
abstract:
- lang: eng
text: This paper explores the geometry of the space of codimension-2 submanifolds.
We implicitly represent these submanifolds by a class of complex-valued functions.
This reveals a prequantum bundle structure over the space of submanifolds, equipped
with the well-known Marsden-Weinstein symplectic structure. This bundle allows
a new physical interpretation of the Marsden-Weinstein structure as the curvature
of a connection form, which measures the average of volumes swept by the deformation
of the S^1-family of hypersurfaces, defined as the phases of a complex function
implicitly representing a submanifold.
article_processing_charge: No
arxiv: 1
author:
- first_name: Albert
full_name: Chern, Albert
last_name: Chern
- first_name: Sadashige
full_name: Ishida, Sadashige
id: 6F7C4B96-A8E9-11E9-A7CA-09ECE5697425
last_name: Ishida
orcid: 0000-0002-3121-3100
citation:
ama: Chern A, Ishida S. Implicit representations of codimension-2 submanifolds and
their prequantum structure. arXiv. doi:10.48550/ARXIV.2507.11727
apa: Chern, A., & Ishida, S. (n.d.). Implicit representations of codimension-2
submanifolds and their prequantum structure. arXiv. https://doi.org/10.48550/ARXIV.2507.11727
chicago: Chern, Albert, and Sadashige Ishida. “Implicit Representations of Codimension-2
Submanifolds and Their Prequantum Structure.” ArXiv, n.d. https://doi.org/10.48550/ARXIV.2507.11727.
ieee: A. Chern and S. Ishida, “Implicit representations of codimension-2 submanifolds
and their prequantum structure,” arXiv. .
ista: Chern A, Ishida S. Implicit representations of codimension-2 submanifolds
and their prequantum structure. arXiv, 10.48550/ARXIV.2507.11727.
mla: Chern, Albert, and Sadashige Ishida. “Implicit Representations of Codimension-2
Submanifolds and Their Prequantum Structure.” ArXiv, doi:10.48550/ARXIV.2507.11727.
short: A. Chern, S. Ishida, ArXiv (n.d.).
corr_author: '1'
date_created: 2025-10-30T18:36:56Z
date_published: 2025-07-15T00:00:00Z
date_updated: 2026-04-07T12:02:23Z
day: '15'
department:
- _id: GradSch
- _id: ChWo
doi: 10.48550/ARXIV.2507.11727
external_id:
arxiv:
- '2507.11727'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2507.11727
month: '07'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: draft
related_material:
record:
- id: '20551'
relation: dissertation_contains
status: public
status: public
title: Implicit representations of codimension-2 submanifolds and their prequantum
structure
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: preprint
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '20585'
abstract:
- lang: eng
text: Motivated by applications in medical sciences, we study finite chromatic sets
in Euclidean space from a topological perspective. Based on the persistent homology
for images, kernels and cokernels, we design provably stable homological quantifiers
that describe the geometric micro- and macro-structure of how the color classes
mingle. These can be efficiently computed using chromatic variants of Delaunay
and alpha complexes, and code that does these computations is provided.
acknowledgement: "This project has received funding from the European Research\r\nCouncil
(ERC) under the European Union’s Horizon 2020 research and innovation\r\nprogramme,
grant no. 788183, from the Wittgenstein Prize, Austrian Science Fund\r\n(FWF), grant
no. Z 342-N31, and from the DFG Collaborative Research Center TRR\r\n109, ‘Discretization
in Geometry and Dynamics’, Austrian Science Fund (FWF),\r\ngrant no. I 02979-N35."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Sebastiano
full_name: Cultrera di Montesano, Sebastiano
id: 34D2A09C-F248-11E8-B48F-1D18A9856A87
last_name: Cultrera di Montesano
orcid: 0000-0001-6249-0832
- first_name: Ondrej
full_name: Draganov, Ondrej
id: 2B23F01E-F248-11E8-B48F-1D18A9856A87
last_name: Draganov
orcid: 0000-0003-0464-3823
- first_name: Herbert
full_name: Edelsbrunner, Herbert
id: 3FB178DA-F248-11E8-B48F-1D18A9856A87
last_name: Edelsbrunner
orcid: 0000-0002-9823-6833
- first_name: Morteza
full_name: Saghafian, Morteza
id: f86f7148-b140-11ec-9577-95435b8df824
last_name: Saghafian
citation:
ama: Cultrera di Montesano S, Draganov O, Edelsbrunner H, Saghafian M. Chromatic
alpha complexes. Foundations of Data Science. 2025;8:30-62. doi:10.3934/fods.2025003
apa: Cultrera di Montesano, S., Draganov, O., Edelsbrunner, H., & Saghafian,
M. (2025). Chromatic alpha complexes. Foundations of Data Science. American
Institute of Mathematical Sciences. https://doi.org/10.3934/fods.2025003
chicago: Cultrera di Montesano, Sebastiano, Ondrej Draganov, Herbert Edelsbrunner,
and Morteza Saghafian. “Chromatic Alpha Complexes.” Foundations of Data Science.
American Institute of Mathematical Sciences, 2025. https://doi.org/10.3934/fods.2025003.
ieee: S. Cultrera di Montesano, O. Draganov, H. Edelsbrunner, and M. Saghafian,
“Chromatic alpha complexes,” Foundations of Data Science, vol. 8. American
Institute of Mathematical Sciences, pp. 30–62, 2025.
ista: Cultrera di Montesano S, Draganov O, Edelsbrunner H, Saghafian M. 2025. Chromatic
alpha complexes. Foundations of Data Science. 8, 30–62.
mla: Cultrera di Montesano, Sebastiano, et al. “Chromatic Alpha Complexes.” Foundations
of Data Science, vol. 8, American Institute of Mathematical Sciences, 2025,
pp. 30–62, doi:10.3934/fods.2025003.
short: S. Cultrera di Montesano, O. Draganov, H. Edelsbrunner, M. Saghafian, Foundations
of Data Science 8 (2025) 30–62.
corr_author: '1'
date_created: 2025-11-02T23:01:33Z
date_published: 2025-03-01T00:00:00Z
date_updated: 2025-11-04T12:25:47Z
day: '01'
department:
- _id: HeEd
doi: 10.3934/fods.2025003
ec_funded: 1
external_id:
arxiv:
- '2212.03128'
intvolume: ' 8'
language:
- iso: eng
month: '03'
oa_version: Preprint
page: 30-62
project:
- _id: 266A2E9E-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '788183'
name: Alpha Shape Theory Extended
- _id: 268116B8-B435-11E9-9278-68D0E5697425
call_identifier: FWF
grant_number: Z00342
name: Mathematics, Computer Science
- _id: 2561EBF4-B435-11E9-9278-68D0E5697425
call_identifier: FWF
grant_number: I02979-N35
name: Persistence and stability of geometric complexes
publication: Foundations of Data Science
publication_identifier:
eissn:
- 2639-8001
publication_status: epub_ahead
publisher: American Institute of Mathematical Sciences
quality_controlled: '1'
related_material:
record:
- id: '15091'
relation: earlier_version
status: public
scopus_import: '1'
status: public
title: Chromatic alpha complexes
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 8
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '20586'
abstract:
- lang: eng
text: We present the discovery of deep, irregular, periodic transits toward the
white dwarf ZTF J1944+4557 using follow-up time-series photometry and spectroscopy
from Palomar, Keck, McDonald, Perkins, and Lowell observatories. We find a predominant
period of 4.9704 hr, consistent with an orbit near the Roche limit of the white
dwarf, with individual dips over 30% deep and lasting between 15 and 40 minutes.
Similar to the first known white dwarf with transiting debris, WD 1145+017, the
transit events are well-defined with prominent out-of-transit phases where the
white dwarf appears unobscured. Spectroscopy concurrent with transit photometry
reveals that the average Ca K equivalent width remains constant in and out of
transit. The broadening observed in several absorption features cannot be reproduced
by synthetic photospheric models, suggesting the presence of circumstellar gas.
Simultaneous g + r- and g + i-band light curves from the CHIMERA instrument reveal
no color dependence to the transit depths, requiring transiting dust grains to
have sizes s ≳ 0.2 μm. The transit morphologies appear to be constantly changing
at a rate faster than the orbital period. Overall transit activity varies in the
system, with transit features completely disappearing during the seven months
between our 2023 and 2024 observing seasons and then reappearing in 2025 March,
still repeating at 4.9704 hr. Our observations of the complete cessation and resumption
of transit activity provide a novel laboratory for constraining the evolution
of disrupted debris and processes like disk exhaustion and replenishment timescales
at white dwarfs.
acknowledgement: "We first extend our gratitude to our anonymous referee, whose careful
review and recommendations enhanced this manuscript. In fruitful conversations and
correspondence with Tim Cunningham, Jay Farihi, Jim Fuller, Philip Muirhead, Saul
Rappaport, Siyi Xu (许偲艺), and Nadia Zakamska, we found guidance that improved our
interpretation of these results. We are deeply grateful for the observing support
by John Kuehne at McDonald Observatory and Colt Pauley at the Perkins Telescope
Observatory. This material is based upon work supported by the National Aeronautics
and Space Administration under grant No. 80NSSC23K1068 issued through the Science
Mission Directorate. J.A.G. is supported by the National Science Foundation Graduate
Research Fellowship Program under grant No. 2234657.\r\n\r\nThis worked is based
on observations obtained with the Samuel Oschin Telescope 48 inch and the 60 inch
Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project.
ZTF is supported by the National Science Foundation under grants No. AST-1440341
and AST-2034437 and a collaboration including current partners Caltech, IPAC, the
Oskar Klein Center at Stockholm University, the University of Maryland, University
of California, Berkeley, the University of Wisconsin at Milwaukee, University of
Warwick, Ruhr University, Cornell University, Northwestern University and Drexel
University. Operations are conducted by COO, IPAC, and UW.\r\n\r\nSome of the data
presented herein were obtained at Keck Observatory, which is a private 501(c)3 non-profit
organization operated as a scientific partnership among the California Institute
of Technology, the University of California, and the National Aeronautics and Space
Administration. The Observatory was made possible by the generous financial support
of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the
very significant cultural role and reverence that the summit of Maunakea has always
had within the Native Hawaiian community. We are most fortunate to have the opportunity
to conduct observations from this mountain.\r\n\r\nThis work has made use of data
from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia),
processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium).
Funding for the DPAC has been provided by national institutions, in particular the
institutions participating in the Gaia Multilateral Agreement.\r\n\r\nThis publication
also makes use of data products from NEOWISE, which is a project of the Jet Propulsion
Laboratory/California Institute of Technology, funded by the Planetary Science Division
of the National Aeronautics and Space Administration.\r\n\r\nThis work is based
in part on observations made with the Spitzer Space Telescope, which was operated
by the Jet Propulsion Laboratory, California Institute of Technology under a contract
with NASA.\r\n\r\nThe Pan-STARRS1 Surveys (PS1) and the PS1 public science archive
have been made possible through contributions by the Institute for Astronomy, the
University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and
its participating institutes, the Max Planck Institute for Astronomy, Heidelberg
and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins
University, Durham University, the University of Edinburgh, the Queen’s University
Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory
Global Telescope Network Incorporated, the National Central University of Taiwan,
the Space Telescope Science Institute, the National Aeronautics and Space Administration
under grant No. NNX08AR22G issued through the Planetary Science Division of the
NASA Science Mission Directorate, the National Science Foundation grant No. AST-1238877,
the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National
Laboratory, and the Gordon and Betty Moore Foundation.\r\n\r\nThis research relied
upon the SIMBAD and VizieR databases operated by CDS (Strasbourg, France) and the
bibliographic resources of The SAO Astrophysics Data System.\r\n\r\nFacilities:
PO:1.2m - Palomar Observatory's 1.2 meter Samuel Oschin Telescope (Zwicky Transient
Facility) - , Hale (CHIMERA, DBSP), Struve - McDonald Observatory's 2.1m Otto Struve
Telescope(ProEM), Perkins - Lowell Observatory's 72in Perkins Telescope (PRISM),
LDT - (LMI), Keck:I - KECK I Telescope (LRIS), Gaia - , PS1 - Panoramic Survey Telescope
and Rapid Response System Telescope #1 (Pan-STARRS), Spitzer (IRAC) - , WISE - Wide-field
Infrared Survey Explorer.\r\n\r\nSoftware: Astropy (Astropy Collaboration et al.
2013, 2018, 2022), astroquery (A. Ginsburg et al. 2019), ccdproc (M. Craig et al.
2017), cuvarbase (J. Hoffman 2022), extinction (K. Barbary 2016), hipercam (V. S.
Dhillon et al. 2021), lmfit (M. Newville et al. 2014), matplotlib (J. D. Hunter
2007), numpy (C. R. Harris et al. 2020), pandas (The pandas Development Team 2025),
phot2lc (Z. Vanderbosch 2023), photutils (L. Bradley et al. 2024), Pyriod (K. Bell
2022), scipy (P. Virtanen et al. 2020)."
article_number: '167'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Joseph A.
full_name: Guidry, Joseph A.
last_name: Guidry
- first_name: Zachary P.
full_name: Vanderbosch, Zachary P.
last_name: Vanderbosch
- first_name: J. J.
full_name: Hermes, J. J.
last_name: Hermes
- first_name: Dimitri
full_name: Veras, Dimitri
last_name: Veras
- first_name: Mark A.
full_name: Hollands, Mark A.
last_name: Hollands
- first_name: Soumyadeep
full_name: Bhattacharjee, Soumyadeep
last_name: Bhattacharjee
- first_name: Ilaria
full_name: Caiazzo, Ilaria
id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
last_name: Caiazzo
orcid: 0000-0002-4770-5388
- first_name: Kareem
full_name: El-Badry, Kareem
last_name: El-Badry
- first_name: Malia L.
full_name: Kao, Malia L.
last_name: Kao
- first_name: Lou Baya
full_name: Ould Rouis, Lou Baya
last_name: Ould Rouis
- first_name: Antonio C.
full_name: Rodriguez, Antonio C.
last_name: Rodriguez
- first_name: Jan
full_name: Van Roestel, Jan
last_name: Van Roestel
citation:
ama: Guidry JA, Vanderbosch ZP, Hermes JJ, et al. Transiting planetary debris near
the Roche limit of a white dwarf on a 4.97 hr orbit—and its vanishing. The
Astrophysical Journal. 2025;992(2). doi:10.3847/1538-4357/adfecb
apa: Guidry, J. A., Vanderbosch, Z. P., Hermes, J. J., Veras, D., Hollands, M. A.,
Bhattacharjee, S., … Van Roestel, J. (2025). Transiting planetary debris near
the Roche limit of a white dwarf on a 4.97 hr orbit—and its vanishing. The
Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/adfecb
chicago: Guidry, Joseph A., Zachary P. Vanderbosch, J. J. Hermes, Dimitri Veras,
Mark A. Hollands, Soumyadeep Bhattacharjee, Ilaria Caiazzo, et al. “Transiting
Planetary Debris near the Roche Limit of a White Dwarf on a 4.97 Hr Orbit—and
Its Vanishing.” The Astrophysical Journal. IOP Publishing, 2025. https://doi.org/10.3847/1538-4357/adfecb.
ieee: J. A. Guidry et al., “Transiting planetary debris near the Roche limit
of a white dwarf on a 4.97 hr orbit—and its vanishing,” The Astrophysical Journal,
vol. 992, no. 2. IOP Publishing, 2025.
ista: Guidry JA, Vanderbosch ZP, Hermes JJ, Veras D, Hollands MA, Bhattacharjee
S, Caiazzo I, El-Badry K, Kao ML, Ould Rouis LB, Rodriguez AC, Van Roestel J.
2025. Transiting planetary debris near the Roche limit of a white dwarf on a 4.97
hr orbit—and its vanishing. The Astrophysical Journal. 992(2), 167.
mla: Guidry, Joseph A., et al. “Transiting Planetary Debris near the Roche Limit
of a White Dwarf on a 4.97 Hr Orbit—and Its Vanishing.” The Astrophysical Journal,
vol. 992, no. 2, 167, IOP Publishing, 2025, doi:10.3847/1538-4357/adfecb.
short: J.A. Guidry, Z.P. Vanderbosch, J.J. Hermes, D. Veras, M.A. Hollands, S. Bhattacharjee,
I. Caiazzo, K. El-Badry, M.L. Kao, L.B. Ould Rouis, A.C. Rodriguez, J. Van Roestel,
The Astrophysical Journal 992 (2025).
date_created: 2025-11-02T23:01:33Z
date_published: 2025-10-20T00:00:00Z
date_updated: 2026-02-16T12:43:29Z
day: '20'
ddc:
- '520'
department:
- _id: IlCa
doi: 10.3847/1538-4357/adfecb
external_id:
arxiv:
- '2508.18348'
isi:
- '001592080300001'
file:
- access_level: open_access
checksum: 24892d1b5bfa1867eb0a353f10c31b82
content_type: application/pdf
creator: dernst
date_created: 2025-11-04T12:33:51Z
date_updated: 2025-11-04T12:33:51Z
file_id: '20601'
file_name: 2025_AstrophysicalJour_Guidry.pdf
file_size: 5323398
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file_date_updated: 2025-11-04T12:33:51Z
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issue: '2'
language:
- iso: eng
month: '10'
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: Transiting planetary debris near the Roche limit of a white dwarf on a 4.97
hr orbit—and its vanishing
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: 992
year: '2025'
...
---
OA_place: publisher
OA_type: gold
_id: '20587'
abstract:
- lang: eng
text: "The blocks in the Bitcoin blockchain \"record\" the amount of work W that
went into creating them through proofs of work. When honest parties control a
majority of the work, consensus is achieved by picking the chain with the highest
recorded weight. Resources other than work have been considered to secure such
longest-chain blockchains. In Chia, blocks record the amount of disk-space S (via
a proof of space) and sequential computational steps V (through a VDF).\r\nIn
this paper, we ask what weight functions Γ(S,V,W) (that assign a weight to a block
as a function of the recorded space, speed, and work) are secure in the sense
that whenever the weight of the resources controlled by honest parties is larger
than the weight of adversarial parties, the blockchain is secure against private
double-spending attacks.\r\nWe completely classify such functions in an idealized
\"continuous\" model: Γ(S,V,W) is secure against private double-spending attacks
if and only if it is homogeneous of degree one in the \"timed\" resources V and
W, i.e., αΓ(S,V,W) = Γ(S,α V, α W). This includes the Bitcoin rule Γ(S,V,W) =
W and the Chia rule Γ(S,V,W) = S ⋅ V. In a more realistic model where blocks are
created at discrete time-points, one additionally needs some mild assumptions
on the dependency on S (basically, the weight should not grow too much if S is
slightly increased, say linear as in Chia).\r\nOur classification is more general
and allows various instantiations of the same resource. It provides a powerful
tool for designing new longest-chain blockchains. E.g., consider combining different
PoWs to counter centralization, say the Bitcoin PoW W₁ and a memory-hard PoW W₂.
Previous work suggested to use W₁+W₂ as weight. Our results show that using e.g.,
√{W₁}⋅ √{W₂} or min{W₁,W₂} are also secure, and we argue that in practice these
are much better choices."
acknowledgement: "This research was funded in whole or in part by the Austrian Science
Fund (FWF)\r\n10.55776/F85. For open access purposes, the author has applied a CC
BY public copyright license\r\nto any author-accepted manuscript version arising
from this submission."
alternative_title:
- LIPIcs
article_number: '16'
article_processing_charge: Yes
arxiv: 1
author:
- first_name: Mirza Ahad
full_name: Baig, Mirza Ahad
id: 3EDE6DE4-AA5A-11E9-986D-341CE6697425
last_name: Baig
- first_name: Christoph Ullrich
full_name: Günther, Christoph Ullrich
id: ec98511c-eb8e-11eb-b029-edd25d7271a1
last_name: Günther
- first_name: Krzysztof Z
full_name: Pietrzak, Krzysztof Z
id: 3E04A7AA-F248-11E8-B48F-1D18A9856A87
last_name: Pietrzak
orcid: 0000-0002-9139-1654
citation:
ama: 'Baig MA, Günther CU, Pietrzak KZ. Nakamoto consensus from multiple resources.
In: 7th Conference on Advances in Financial Technologies. Vol 354. Schloss
Dagstuhl - Leibniz-Zentrum für Informatik; 2025. doi:10.4230/LIPIcs.AFT.2025.16'
apa: 'Baig, M. A., Günther, C. U., & Pietrzak, K. Z. (2025). Nakamoto consensus
from multiple resources. In 7th Conference on Advances in Financial Technologies
(Vol. 354). Pittsburgh, PA, United States: Schloss Dagstuhl - Leibniz-Zentrum
für Informatik. https://doi.org/10.4230/LIPIcs.AFT.2025.16'
chicago: Baig, Mirza Ahad, Christoph Ullrich Günther, and Krzysztof Z Pietrzak.
“Nakamoto Consensus from Multiple Resources.” In 7th Conference on Advances
in Financial Technologies, Vol. 354. Schloss Dagstuhl - Leibniz-Zentrum für
Informatik, 2025. https://doi.org/10.4230/LIPIcs.AFT.2025.16.
ieee: M. A. Baig, C. U. Günther, and K. Z. Pietrzak, “Nakamoto consensus from multiple
resources,” in 7th Conference on Advances in Financial Technologies, Pittsburgh,
PA, United States, 2025, vol. 354.
ista: 'Baig MA, Günther CU, Pietrzak KZ. 2025. Nakamoto consensus from multiple
resources. 7th Conference on Advances in Financial Technologies. AFT: Conference
on Advances in Financial Technologies, LIPIcs, vol. 354, 16.'
mla: Baig, Mirza Ahad, et al. “Nakamoto Consensus from Multiple Resources.” 7th
Conference on Advances in Financial Technologies, vol. 354, 16, Schloss Dagstuhl
- Leibniz-Zentrum für Informatik, 2025, doi:10.4230/LIPIcs.AFT.2025.16.
short: M.A. Baig, C.U. Günther, K.Z. Pietrzak, in:, 7th Conference on Advances in
Financial Technologies, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2025.
conference:
end_date: 2025-10-10
location: Pittsburgh, PA, United States
name: 'AFT: Conference on Advances in Financial Technologies'
start_date: 2025-10-08
corr_author: '1'
date_created: 2025-11-02T23:01:34Z
date_published: 2025-10-06T00:00:00Z
date_updated: 2026-04-15T08:45:18Z
day: '06'
ddc:
- '000'
department:
- _id: KrPi
doi: 10.4230/LIPIcs.AFT.2025.16
external_id:
arxiv:
- '2508.01448'
file:
- access_level: open_access
checksum: b638adcd4fbffa77116c35393e165eb7
content_type: application/pdf
creator: dernst
date_created: 2025-11-04T08:19:02Z
date_updated: 2025-11-04T08:19:02Z
file_id: '20598'
file_name: 2025_LIPIcsAFT_Baig.pdf
file_size: 1061847
relation: main_file
success: 1
file_date_updated: 2025-11-04T08:19:02Z
has_accepted_license: '1'
intvolume: ' 354'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://eprint.iacr.org/2025/1410
month: '10'
oa: 1
oa_version: Published Version
project:
- _id: 34a4ce89-11ca-11ed-8bc3-8cc37fb6e11f
grant_number: F8512
name: Security and Privacy by Design for Complex Systems
- _id: 34a34d57-11ca-11ed-8bc3-a2688a8724e1
grant_number: F8509
name: Security and Privacy by Design for Complex Systems
publication: 7th Conference on Advances in Financial Technologies
publication_identifier:
isbn:
- '9783959774000'
issn:
- 1868-8969
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
quality_controlled: '1'
related_material:
record:
- id: '21651'
relation: dissertation_contains
status: public
scopus_import: '1'
status: public
title: Nakamoto consensus from multiple resources
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 354
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '20588'
abstract:
- lang: eng
text: 'In this second paper on our variability survey of central stars of planetary
nebulae (CSPNe) using the Zwicky Transient Facility (ZTF), we report 11 long-timescale
variables with variability timescales ranging from months to years. We also present
preliminary analyses based on spectroscopic and/or photometric follow-up observations
for six of them. Among them is NGC 6833, which shows a 980 days periodic variability
with strange characteristics: “triangle-shaped” brightening in r, i, and WISE
bands but almost coincidental shallow dips in the g-band. The most plausible explanation
is a wide binary with the photometric period being the orbital period. Long-period
near-sinusoidal variability was detected in two other systems, NGC 6905 and Kn
26, with periods of 700 days and 230 days, respectively, making them additional
wide-binary candidates. The latter also shows a short period at 1.18 hr. We then
present CTSS 2 and K 3-5, which show brightening and significant reddening over
the whole ZTF baseline. A stellar model fit to the optical spectrum of CTSS 2
reveals it to be one of the youngest post-AGB CSPNe known. Both show high-density
emission-line cores. We propose these to be late-thermal-pulse candidates, currently
evolving towards the AGB phase. We then present recent HST/COS ultraviolet spectroscopy
of the known wide-binary candidate LoTr 1, showing that the hot star is a spectroscopic
twin of the extremely hot white dwarf in UCAC2 46706450. Similar to this object,
LoTr 1 also has a fast rotating wide subgiant companion. We suggest that the long
photometric period of 11 yr is the binary orbital period. Finally, we briefly
discuss the ZTF light curves of the remaining variables, namely Tan 2, K 3-20,
WHTZ 3, Kn J1857+3931, and IPHAS J1927+0814. With these examples, we present the
effectiveness of the von Neumann statistics and Pearson Skew-based metric space
in searching for long-timescale variables.'
acknowledgement: "This work is based on observations obtained with the Samuel Oschin
Telescope 48 inch and the 60 inch Telescope at the Palomar Observatory as part of
the Zwicky Transient Facility project. ZTF is supported by the National Science
Foundation under grant Nos. AST-1440341 and AST-2034437 and a collaboration including
current partners Caltech, IPAC, the Oskar Klein Center at Stockholm University,
the University of Maryland, University of California, Berkeley, the University of
Wisconsin at Milwaukee, University of Warwick, Ruhr University Bochum, Cornell University,
Northwestern University, and Drexel University. Operations are conducted by COO,
IPAC, and UW.\r\n\r\nThis work has made use of data from the European Space Agency
(ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data
Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/consortium).
Funding for the DPAC has been provided by national institutions, in particular,
the institutions participating in the Gaia Multilateral Agreement.\r\n\r\nWe are
grateful to the staffs of Palomar Observatory and the Hobby-Eberly Telescope for
assistance with the observations and data management. The Liverpool Telescope is
operated on the island of La Palma by Liverpool John Moores University in the Spanish
Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias
with financial support from the UK Science and Technology Facilities Council.\r\n\r\nThe
Low-Resolution Spectrograph 2 (LRS2) on HET was developed and funded by the University
of Texas at Austin McDonald Observatory and Department of Astronomy, and by Pennsylvania
State University. We thank the Leibniz-Institut für Astrophysik Potsdam (AIP) and
the Institut für Astrophysik Göttingen (IAG) for their contributions to the construction
of the integral field units. We acknowledge the Texas Advanced Computing Center
(TACC) at The University of Texas at Austin for providing high performance computing,
visualization, and storage resources that have contributed to the results reported
within this paper.\r\n\r\nThe Isaac Newton Telescope is operated on the island of
La Palma by the Isaac Newton Group of Telescopes in the Spanish Observatorio del
Roque de los Muchachos of the Instituto de Astrofísica de Canarias\r\n\r\nS.B. thanks
Frank J. Masci and Zachary P. Vanderbosch for useful discussions and suggestions
regarding solving the issues with ZTF forced photometry on extended sources. S.B.
also thanks Jim Fuller, Charles C. Steidel, Lynne Hillenbrand, and Adolfo Carvalho
for useful discussions on methods and science. S.B. acknowledges financial support
from the Wallace L. W. Sargent Graduate Fellowship during the first year of his
graduate studies at Caltech. N.C. was supported through the Cancer Research UK grant
A24042.\r\n\r\nN.R. is supported by the Deutsche Forschungsgemeinschaft (DFG) through
grant RE3915/2-1.\r\n\r\nD.J. acknowledges support from the Agencia Estatal de Investigación
del Ministerio de Ciencia, Innovación y Universidades (MICIU/AEI) under grant “Nebulosas
planetarias como clave para comprender la evolución de estrellas binarias” and the
European Regional Development Fund (ERDF) with reference PID-2022-136653NA-I00 (DOI:10.13039/501100011033).
D.J. also acknowledges support from the Agencia Estatal de Investigación del Ministerio
de Ciencia, Innovación y Universidades (MICIU/AEI) under grant “Revolucionando el
conocimiento de la evolución de estrellas poco masivas” and the the European Union
NextGenerationEU/PRTR with reference CNS2023-143910 (DOI:10.13039/501100011033).\r\n\r\nWe
have used Python packages Numpy (Harris et al. 2020), SciPy (Virtanen et al. 2020),
Matplotlib (Hunter 2007), Pandas (pandas development team 2020), Astropy (Astropy
Collaboration et al. 2013, 2018), and Astroquery (Ginsburg et al. 2019) at various
stages of this research."
article_number: '104206'
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Soumyadeep
full_name: Bhattacharjee, Soumyadeep
last_name: Bhattacharjee
- first_name: Nicole
full_name: Reindl, Nicole
last_name: Reindl
- first_name: Howard E.
full_name: Bond, Howard E.
last_name: Bond
- first_name: Klaus
full_name: Werner, Klaus
last_name: Werner
- first_name: Gregory R.
full_name: Zeimann, Gregory R.
last_name: Zeimann
- first_name: David
full_name: Jones, David
last_name: Jones
- first_name: Kareem
full_name: El-Badry, Kareem
last_name: El-Badry
- first_name: Nina
full_name: Mackensen, Nina
last_name: Mackensen
- first_name: Nicholas
full_name: Chornay, Nicholas
last_name: Chornay
- first_name: S. R.
full_name: Kulkarni, S. R.
last_name: Kulkarni
- first_name: Ilaria
full_name: Caiazzo, Ilaria
id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
last_name: Caiazzo
orcid: 0000-0002-4770-5388
- first_name: Jan
full_name: Van Roestel, Jan
last_name: Van Roestel
- first_name: Antonio C.
full_name: Rodriguez, Antonio C.
last_name: Rodriguez
- first_name: Thomas A.
full_name: Prince, Thomas A.
last_name: Prince
- first_name: Ben
full_name: Rusholme, Ben
last_name: Rusholme
- first_name: Russ R.
full_name: Laher, Russ R.
last_name: Laher
- first_name: Roger
full_name: Smith, Roger
last_name: Smith
citation:
ama: Bhattacharjee S, Reindl N, Bond HE, et al. Variability of central stars of
planetary nebulae with the Zwicky Transient Facility. II. Long-timescale variables
including wide binary and late thermal pulse candidates. Publications of the
Astronomical Society of the Pacific. 2025;137(10). doi:10.1088/1538-3873/ae051e
apa: Bhattacharjee, S., Reindl, N., Bond, H. E., Werner, K., Zeimann, G. R., Jones,
D., … Smith, R. (2025). Variability of central stars of planetary nebulae with
the Zwicky Transient Facility. II. Long-timescale variables including wide binary
and late thermal pulse candidates. Publications of the Astronomical Society
of the Pacific. IOP Publishing. https://doi.org/10.1088/1538-3873/ae051e
chicago: Bhattacharjee, Soumyadeep, Nicole Reindl, Howard E. Bond, Klaus Werner,
Gregory R. Zeimann, David Jones, Kareem El-Badry, et al. “Variability of Central
Stars of Planetary Nebulae with the Zwicky Transient Facility. II. Long-Timescale
Variables Including Wide Binary and Late Thermal Pulse Candidates.” Publications
of the Astronomical Society of the Pacific. IOP Publishing, 2025. https://doi.org/10.1088/1538-3873/ae051e.
ieee: S. Bhattacharjee et al., “Variability of central stars of planetary
nebulae with the Zwicky Transient Facility. II. Long-timescale variables including
wide binary and late thermal pulse candidates,” Publications of the Astronomical
Society of the Pacific, vol. 137, no. 10. IOP Publishing, 2025.
ista: Bhattacharjee S, Reindl N, Bond HE, Werner K, Zeimann GR, Jones D, El-Badry
K, Mackensen N, Chornay N, Kulkarni SR, Caiazzo I, Van Roestel J, Rodriguez AC,
Prince TA, Rusholme B, Laher RR, Smith R. 2025. Variability of central stars of
planetary nebulae with the Zwicky Transient Facility. II. Long-timescale variables
including wide binary and late thermal pulse candidates. Publications of the Astronomical
Society of the Pacific. 137(10), 104206.
mla: Bhattacharjee, Soumyadeep, et al. “Variability of Central Stars of Planetary
Nebulae with the Zwicky Transient Facility. II. Long-Timescale Variables Including
Wide Binary and Late Thermal Pulse Candidates.” Publications of the Astronomical
Society of the Pacific, vol. 137, no. 10, 104206, IOP Publishing, 2025, doi:10.1088/1538-3873/ae051e.
short: S. Bhattacharjee, N. Reindl, H.E. Bond, K. Werner, G.R. Zeimann, D. Jones,
K. El-Badry, N. Mackensen, N. Chornay, S.R. Kulkarni, I. Caiazzo, J. Van Roestel,
A.C. Rodriguez, T.A. Prince, B. Rusholme, R.R. Laher, R. Smith, Publications of
the Astronomical Society of the Pacific 137 (2025).
date_created: 2025-11-02T23:01:34Z
date_published: 2025-10-01T00:00:00Z
date_updated: 2025-12-01T15:13:50Z
day: '01'
ddc:
- '520'
department:
- _id: IlCa
doi: 10.1088/1538-3873/ae051e
external_id:
arxiv:
- '2502.18651'
isi:
- '001595690000001'
file:
- access_level: open_access
checksum: cc7d00c349d48458accb0d3df67e4879
content_type: application/pdf
creator: dernst
date_created: 2025-11-04T08:26:39Z
date_updated: 2025-11-04T08:26:39Z
file_id: '20599'
file_name: 2025_PASP_BhattacharjeeS.pdf
file_size: 12677603
relation: main_file
success: 1
file_date_updated: 2025-11-04T08:26:39Z
has_accepted_license: '1'
intvolume: ' 137'
isi: 1
issue: '10'
language:
- iso: eng
month: '10'
oa: 1
oa_version: Published Version
publication: Publications of the Astronomical Society of the Pacific
publication_identifier:
issn:
- 1538-3873
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Variability of central stars of planetary nebulae with the Zwicky Transient
Facility. II. Long-timescale variables including wide binary and late thermal pulse
candidates
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: 137
year: '2025'
...
---
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '20589'
abstract:
- lang: eng
text: "Context. This paper investigates the star formation histories (SFHs) of a
sample of massive galaxies (M⋆ ≥ 1010 M⊙) in the redshift range 1 < z < 4.5.\r\nMethods.
We analyzed spectro-photometric data, combining broadband photometry from HST
and JWST with low-resolution grism spectroscopy from JWST/NIRISS, obtained as
part of the MIRI Deep Imaging Survey program. SFHs were derived through spectral
energy distribution fitting using two independent codes, BAGPIPES and synthesizer,
under various SFH assumptions. This approach enables a comprehensive assessment
of the biases introduced by different modeling choices.\r\nResults. The inclusion
of NIRISS spectroscopy, even with its low resolution, significantly improves constraints
on key physical parameters, such as the mass-weighted stellar age (tM) and formation
redshift (zform), by narrowing their posterior distributions. The massive galaxies
in our sample exhibit rapid stellar mass assembly, forming 50% of their mass between
3 ≤ z ≤ 9. The highest inferred formation redshifts are compatible with elevated
star formation efficiencies (ϵ) at early epochs. Nonparametric SFHs generally
imply an earlier and slower mass assembly compared to parametric forms, highlighting
the sensitivity of inferred formation timescales to the chosen SFH model–particularly
for galaxies at z < 2. We find that quiescent galaxies are, on average, older
(tM ∼ 1.1 Gyr) and assembled more rapidly at earlier times than their star-forming
counterparts. These findings support the “downsizing” scenario, in which more
massive and passive systems form earlier and more efficiently."
acknowledgement: MA acknowledges financial support from Comunidad de Madrid under
Atracción de Talento grant 2020-T2/TIC-19971. This work has made use of the Rainbow
Cosmological Surveys Database, which is operated by the Centro de Astrobiología
(CAB/INTA), partnered with the University of California Observatories at Santa Cruz
(UCO/Lick,UCSC). The project that gave rise to these results received the support
of a fellowship from the “la Caixa” Foundation (ID 100010434). The fellowship code
is LCF/BQ/PR24/12050015. LC acknowledges support from grants PID2022-139567NB-I00
and PIB2021-127718NB-I00 funded by the Spanish Ministry of Science and Innovation/State
Agency of Research MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”.
This work is based on observations made with the NASA/ ESA/CSA JWST. The data were
obtained from the Mikulski Archive for Space Telescopes (MAST) 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.
article_number: A224
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: M.
full_name: Annunziatella, M.
last_name: Annunziatella
- first_name: P. G.
full_name: P’Erez-Gonz’Alez, P. G.
last_name: P’Erez-Gonz’Alez
- first_name: J.
full_name: Álvarez-Márquez, J.
last_name: Álvarez-Márquez
- first_name: L.
full_name: Costantin, L.
last_name: Costantin
- first_name: Edoardo
full_name: Iani, Edoardo
id: 4053390a-6b68-11ef-9828-a3b8adef8d0a
last_name: Iani
orcid: 0000-0001-8386-3546
- first_name: Unknown
full_name: Labiano, Unknown
last_name: Labiano
- first_name: P.
full_name: Rinaldi, P.
last_name: Rinaldi
- first_name: L.
full_name: Boogaard, L.
last_name: Boogaard
- first_name: R. A.
full_name: Meyer, R. A.
last_name: Meyer
- first_name: G.
full_name: Östlin, G.
last_name: Östlin
- first_name: L.
full_name: Colina, L.
last_name: Colina
- first_name: J.
full_name: Melinder, J.
last_name: Melinder
- first_name: I.
full_name: Jermann, I.
last_name: Jermann
- first_name: S.
full_name: Gillman, S.
last_name: Gillman
- first_name: D.
full_name: Langeroodi, D.
last_name: Langeroodi
- first_name: J.
full_name: Hjorth, J.
last_name: Hjorth
- first_name: A.
full_name: Alonso-Herrero, A.
last_name: Alonso-Herrero
- first_name: A.
full_name: Eckart, A.
last_name: Eckart
- first_name: F.
full_name: Walter, F.
last_name: Walter
- first_name: P. P.
full_name: Van Der Werf, P. P.
last_name: Van Der Werf
- first_name: A.
full_name: Bik, A.
last_name: Bik
- first_name: F.
full_name: Peißker, F.
last_name: Peißker
- first_name: K. I.
full_name: Caputi, K. I.
last_name: Caputi
- first_name: M.
full_name: García-Marín, M.
last_name: García-Marín
- first_name: G.
full_name: Wright, G.
last_name: Wright
- first_name: T. R.
full_name: Greve, T. R.
last_name: Greve
citation:
ama: 'Annunziatella M, P’Erez-Gonz’Alez PG, Álvarez-Márquez J, et al. MIDIS: Unveiling
the star formation history in massive galaxies at 1 < z < 4.5 with spectro-photometric
analysis. Astronomy & Astrophysics. 2025;702. doi:10.1051/0004-6361/202453298'
apa: 'Annunziatella, M., P’Erez-Gonz’Alez, P. G., Álvarez-Márquez, J., Costantin,
L., Iani, E., Labiano, U., … Greve, T. R. (2025). MIDIS: Unveiling the star formation
history in massive galaxies at 1 < z < 4.5 with spectro-photometric analysis.
Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202453298'
chicago: 'Annunziatella, M., P. G. P’Erez-Gonz’Alez, J. Álvarez-Márquez, L. Costantin,
Edoardo Iani, Unknown Labiano, P. Rinaldi, et al. “MIDIS: Unveiling the Star Formation
History in Massive Galaxies at 1 < z < 4.5 with Spectro-Photometric Analysis.”
Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202453298.'
ieee: 'M. Annunziatella et al., “MIDIS: Unveiling the star formation history
in massive galaxies at 1 < z < 4.5 with spectro-photometric analysis,”
Astronomy & Astrophysics, vol. 702. EDP Sciences, 2025.'
ista: 'Annunziatella M, P’Erez-Gonz’Alez PG, Álvarez-Márquez J, Costantin L, Iani
E, Labiano U, Rinaldi P, Boogaard L, Meyer RA, Östlin G, Colina L, Melinder J,
Jermann I, Gillman S, Langeroodi D, Hjorth J, Alonso-Herrero A, Eckart A, Walter
F, Van Der Werf PP, Bik A, Peißker F, Caputi KI, García-Marín M, Wright G, Greve
TR. 2025. MIDIS: Unveiling the star formation history in massive galaxies at 1 < z <
4.5 with spectro-photometric analysis. Astronomy & Astrophysics. 702, A224.'
mla: 'Annunziatella, M., et al. “MIDIS: Unveiling the Star Formation History in
Massive Galaxies at 1 < z < 4.5 with Spectro-Photometric Analysis.” Astronomy
& Astrophysics, vol. 702, A224, EDP Sciences, 2025, doi:10.1051/0004-6361/202453298.'
short: M. Annunziatella, P.G. P’Erez-Gonz’Alez, J. Álvarez-Márquez, L. Costantin,
E. Iani, U. Labiano, P. Rinaldi, L. Boogaard, R.A. Meyer, G. Östlin, L. Colina,
J. Melinder, I. Jermann, S. Gillman, D. Langeroodi, J. Hjorth, A. Alonso-Herrero,
A. Eckart, F. Walter, P.P. Van Der Werf, A. Bik, F. Peißker, K.I. Caputi, M. García-Marín,
G. Wright, T.R. Greve, Astronomy & Astrophysics 702 (2025).
date_created: 2025-11-02T23:01:34Z
date_published: 2025-10-24T00:00:00Z
date_updated: 2026-02-16T12:14:12Z
day: '24'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202453298
external_id:
arxiv:
- '2508.16951'
isi:
- '001600932400021'
file:
- access_level: open_access
checksum: 0cd0c3fc75b7f6589088a2b7bd60c0ed
content_type: application/pdf
creator: dernst
date_created: 2025-11-04T09:36:30Z
date_updated: 2025-11-04T09:36:30Z
file_id: '20600'
file_name: 2025_AstronomyAstrophysics_Annunziatella.pdf
file_size: 5107702
relation: main_file
success: 1
file_date_updated: 2025-11-04T09:36:30Z
has_accepted_license: '1'
intvolume: ' 702'
isi: 1
language:
- iso: eng
month: '10'
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: 'MIDIS: Unveiling the star formation history in massive galaxies at 1 < z <
4.5 with spectro-photometric analysis'
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: 702
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '20590'
abstract:
- lang: eng
text: 'Moist convection is a fundamental process occurring in the Earth''s atmosphere.
It plays a central role in the weather and climate of the Tropics, where, to first
order, the heating of the atmosphere by convection is in balance with the cooling
of the atmosphere by the emission of radiation to outer space. In this study,
we use a cloud-resolving model in radiative–convective equilibrium with an imposed
constant rate of radiative cooling and study the response of moist convection
to varying this rate of radiative cooling. In particular, we study two types of
simulation: varying air temperature (VAT) simulations, where the air temperature
is allowed to adjust to the imposed radiative cooling, and constant air temperature
(CAT) simulations, where the surface temperature is tuned to ensure that the atmospheric
temperature profile in the domain is constant. We recover the previously known
result that, in response to increasing radiative cooling, the area of convection
expands rapidly, while the intensity of convection does not change. We find that
this response is explained by the increased boundary-layer variability in simulations
with greater radiative cooling, which compensates for the decreasing temperature
by adding a larger initial velocity close to the cloud base. We also propose a
fundamental scaling of the non-dimensional cumulus mass flux in moist convection,
which is robust across models of different complexity. We aim to bridge the gap
between highly idealised prototypes of moist convection, such as the “Rainy–Bénard
convection” introduced by Vallis et al., and comprehensive cloud-resolving models.'
acknowledged_ssus:
- _id: ScienComp
acknowledgement: "The authors gratefully acknowledge discussions with Professor Robert
Plant (University of Reading, UK), Professor Steve Sherwood (University of New South
Wales, Australia), Professor Steve Tobias, Professor Douglas Parker, and Gregory
Dritschel (University of Leeds, UK). Discussions with colleagues at the Institute
of Science and Technology Austria played a large role in shaping this study. The
authors are particularly grateful for inputs and discussions from Dr. Jiawei Bao,
Dr. Alejandro Casallas, and Alzbeta Pechacova.\r\nThis project has received funding
from the European Union's Horizon 2020 research and innovation programme under the
Marie Sklodowska–Curie grant agreement No. 101034413. C. Muller gratefully acknowledges
funding from the European Research Council (ERC) under the European Union's Horizon
2020 research and innovation program (Project CLUSTER, Grant Agreement No. 805041).
This research was supported by the Scientific Service Units (SSU) of IST Austria
through resources provided by Scientific Computing (SciComp). Open Access funding
provided by Institute of Science and Technology Austria/KEMÖ."
article_number: e70044
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Lokahith N
full_name: Agasthya, Lokahith N
id: cd100965-0804-11ed-9c55-f4878ff4e877
last_name: Agasthya
- first_name: Caroline J
full_name: Muller, Caroline J
id: f978ccb0-3f7f-11eb-b193-b0e2bd13182b
last_name: Muller
orcid: 0000-0001-5836-5350
citation:
ama: 'Agasthya LN, Muller CJ. Moist convection and radiative cooling: Dynamical
response and scaling. Quarterly Journal of the Royal Meteorological Society.
2025. doi:10.1002/qj.70044'
apa: 'Agasthya, L. N., & Muller, C. J. (2025). Moist convection and radiative
cooling: Dynamical response and scaling. Quarterly Journal of the Royal Meteorological
Society. Wiley. https://doi.org/10.1002/qj.70044'
chicago: 'Agasthya, Lokahith N, and Caroline J Muller. “Moist Convection and Radiative
Cooling: Dynamical Response and Scaling.” Quarterly Journal of the Royal Meteorological
Society. Wiley, 2025. https://doi.org/10.1002/qj.70044.'
ieee: 'L. N. Agasthya and C. J. Muller, “Moist convection and radiative cooling:
Dynamical response and scaling,” Quarterly Journal of the Royal Meteorological
Society. Wiley, 2025.'
ista: 'Agasthya LN, Muller CJ. 2025. Moist convection and radiative cooling: Dynamical
response and scaling. Quarterly Journal of the Royal Meteorological Society.,
e70044.'
mla: 'Agasthya, Lokahith N., and Caroline J. Muller. “Moist Convection and Radiative
Cooling: Dynamical Response and Scaling.” Quarterly Journal of the Royal Meteorological
Society, e70044, Wiley, 2025, doi:10.1002/qj.70044.'
short: L.N. Agasthya, C.J. Muller, Quarterly Journal of the Royal Meteorological
Society (2025).
corr_author: '1'
date_created: 2025-11-02T23:01:34Z
date_published: 2025-10-18T00:00:00Z
date_updated: 2025-12-01T15:15:18Z
day: '18'
ddc:
- '550'
department:
- _id: CaMu
doi: 10.1002/qj.70044
ec_funded: 1
external_id:
isi:
- '001595821400001'
has_accepted_license: '1'
isi: 1
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1002/qj.70044
month: '10'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
- _id: 629205d8-2b32-11ec-9570-e1356ff73576
call_identifier: H2020
grant_number: '805041'
name: Organization of CLoUdS, and implications of Tropical cyclones and for the
Energetics of the tropics, in current and waRming climate
publication: Quarterly Journal of the Royal Meteorological Society
publication_identifier:
eissn:
- 1477-870X
issn:
- 0035-9009
publication_status: epub_ahead
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Moist convection and radiative cooling: Dynamical response and scaling'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '20591'
abstract:
- lang: eng
text: In this paper we derive estimates for the Hessian of the logarithm (log-Hessian)
for solutions to the heat equation. For initial data in the form of log-Lipschitz
perturbation of strongly log-concave measures, the log-Hessian admits an explicit,
uniform (in space) lower bound. This yields a new estimate for the Lipschitz constant
of a transport map pushing forward the standard Gaussian to a measure in this
class. On the other hand, we show that assuming only fast decay of the tails of
the initial datum does not suffice to guarantee uniform log-Hessian upper bounds.
acknowledgement: This research was funded in part by the Austrian Science Fund (FWF)
project 10.55776/F65 and by the European Union’s Horizon 2020 research and innovation
programme under the Marie Sklodowska-Curie grant agreement No 101034413. The authors
thank Professors Jean Dolbeault, Jan Maas, and Nikita Simonov for many useful comments,
and Professors Kazuhiro Ishige, Asuka Takatsu, and Yair Shenfeld for inspiring interactions.
article_number: '71'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Giovanni
full_name: Brigati, Giovanni
id: 63ff57e8-1fbb-11ee-88f2-f558ffc59cf1
last_name: Brigati
- first_name: Francesco
full_name: Pedrotti, Francesco
id: d3ac8ac6-dc8d-11ea-abe3-e2a9628c4c3c
last_name: Pedrotti
citation:
ama: Brigati G, Pedrotti F. Heat flow, log-concavity, and Lipschitz transport maps.
Electronic Communications in Probability. 2025;30. doi:10.1214/25-ECP717
apa: Brigati, G., & Pedrotti, F. (2025). Heat flow, log-concavity, and Lipschitz
transport maps. Electronic Communications in Probability. Institute of
Mathematical Statistics. https://doi.org/10.1214/25-ECP717
chicago: Brigati, Giovanni, and Francesco Pedrotti. “Heat Flow, Log-Concavity, and
Lipschitz Transport Maps.” Electronic Communications in Probability. Institute
of Mathematical Statistics, 2025. https://doi.org/10.1214/25-ECP717.
ieee: G. Brigati and F. Pedrotti, “Heat flow, log-concavity, and Lipschitz transport
maps,” Electronic Communications in Probability, vol. 30. Institute of
Mathematical Statistics, 2025.
ista: Brigati G, Pedrotti F. 2025. Heat flow, log-concavity, and Lipschitz transport
maps. Electronic Communications in Probability. 30, 71.
mla: Brigati, Giovanni, and Francesco Pedrotti. “Heat Flow, Log-Concavity, and Lipschitz
Transport Maps.” Electronic Communications in Probability, vol. 30, 71,
Institute of Mathematical Statistics, 2025, doi:10.1214/25-ECP717.
short: G. Brigati, F. Pedrotti, Electronic Communications in Probability 30 (2025).
corr_author: '1'
date_created: 2025-11-02T23:01:35Z
date_published: 2025-09-25T00:00:00Z
date_updated: 2025-12-01T15:08:54Z
day: '25'
ddc:
- '500'
department:
- _id: JaMa
doi: 10.1214/25-ECP717
ec_funded: 1
external_id:
arxiv:
- '2404.15205'
isi:
- '001611557000018'
file:
- access_level: open_access
checksum: 67858edbd74658fe38955fa1216f2f18
content_type: application/pdf
creator: dernst
date_created: 2025-11-04T07:34:05Z
date_updated: 2025-11-04T07:34:05Z
file_id: '20596'
file_name: 2025_ElectronJourProbab_Brigati.pdf
file_size: 278078
relation: main_file
success: 1
file_date_updated: 2025-11-04T07:34:05Z
has_accepted_license: '1'
intvolume: ' 30'
isi: 1
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
project:
- _id: fc31cba2-9c52-11eb-aca3-ff467d239cd2
grant_number: F6504
name: Taming Complexity in Partial Differential Systems
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Electronic Communications in Probability
publication_identifier:
eissn:
- 1083-589X
publication_status: published
publisher: Institute of Mathematical Statistics
quality_controlled: '1'
related_material:
record:
- id: '17353'
relation: earlier_version
status: public
scopus_import: '1'
status: public
title: Heat flow, log-concavity, and Lipschitz transport maps
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: 30
year: '2025'
...
---
OA_place: repository
OA_type: green
_id: '20592'
abstract:
- lang: eng
text: "Filtering-based probabilistic numerical solvers for ordinary differential
equations (ODEs), also known as ODE filters, have been established as efficient
methods for quantifying numerical uncertainty in the solution of ODEs. In practical
applications, however, the underlying dynamical system often contains uncertain
parameters, requiring the propagation of this model uncertainty to the ODE solution.
In this paper, we demonstrate that ODE filters, despite their probabilistic nature,
do not automatically solve this uncertainty propagation problem. To address this
limitation, we present a novel approach that combines ODE filters with numerical
quadrature to properly marginalize over uncertain parameters, while accounting
for both parameter uncertainty and numerical solver uncertainty. Experiments across
multiple dynamical systems demonstrate that the resulting uncertainty estimates
closely match reference solutions. Notably, we show\r\nhow the numerical uncertainty
from the ODE solver can help prevent overconfidence in the propagated uncertainty
estimates, especially when using larger step sizes. Our results illustrate that
probabilistic numerical methods can effectively quantify both numerical and parametric
uncertainty in dynamical systems. "
acknowledgement: "NB gratefully acknowledge co-funding by the European Union (ERC,
ANUBIS, 101123955. Views and opinions expressed are however those of the author(s)
only and do not necessarily reflect those of the European Union or the European
Research Council. Neither the European Union nor the granting authority can be held
responsible for them). NB thanks the International\r\nMax Planck Research School
for Intelligent Systems (IMPRS-IS) for their support."
alternative_title:
- PMLR
article_processing_charge: No
arxiv: 1
author:
- first_name: Dingling
full_name: Yao, Dingling
id: d3e02e50-48a8-11ee-8f62-c108061797fa
last_name: Yao
- first_name: Filip
full_name: Tronarp, Filip
last_name: Tronarp
- first_name: Nathanael
full_name: Bosch, Nathanael
last_name: Bosch
citation:
ama: 'Yao D, Tronarp F, Bosch N. Propagating model uncertainty through filtering-based
probabilistic numerical ODE solvers. In: Proceedings of the 1st International
Conference on Probabilistic Numerics. Vol 271. ML Research Press; 2025.'
apa: 'Yao, D., Tronarp, F., & Bosch, N. (2025). Propagating model uncertainty
through filtering-based probabilistic numerical ODE solvers. In Proceedings
of the 1st International Conference on Probabilistic Numerics (Vol. 271).
Sophia Antipolis, France: ML Research Press.'
chicago: Yao, Dingling, Filip Tronarp, and Nathanael Bosch. “Propagating Model Uncertainty
through Filtering-Based Probabilistic Numerical ODE Solvers.” In Proceedings
of the 1st International Conference on Probabilistic Numerics, Vol. 271. ML
Research Press, 2025.
ieee: D. Yao, F. Tronarp, and N. Bosch, “Propagating model uncertainty through filtering-based
probabilistic numerical ODE solvers,” in Proceedings of the 1st International
Conference on Probabilistic Numerics, Sophia Antipolis, France, 2025, vol.
271.
ista: 'Yao D, Tronarp F, Bosch N. 2025. Propagating model uncertainty through filtering-based
probabilistic numerical ODE solvers. Proceedings of the 1st International Conference
on Probabilistic Numerics. ProbNum: Conference on Probabilistic Numerics, PMLR,
vol. 271.'
mla: Yao, Dingling, et al. “Propagating Model Uncertainty through Filtering-Based
Probabilistic Numerical ODE Solvers.” Proceedings of the 1st International
Conference on Probabilistic Numerics, vol. 271, ML Research Press, 2025.
short: D. Yao, F. Tronarp, N. Bosch, in:, Proceedings of the 1st International Conference
on Probabilistic Numerics, ML Research Press, 2025.
conference:
end_date: 2025-09-03
location: Sophia Antipolis, France
name: 'ProbNum: Conference on Probabilistic Numerics'
start_date: 2025-09-01
date_created: 2025-11-02T23:01:35Z
date_published: 2025-01-01T00:00:00Z
date_updated: 2025-11-10T08:33:11Z
day: '01'
ddc:
- '000'
department:
- _id: FrLo
external_id:
arxiv:
- '2503.04684'
has_accepted_license: '1'
intvolume: ' 271'
language:
- iso: eng
license: https://creativecommons.org/licenses/by-sa/4.0/
main_file_link:
- open_access: '1'
url: https://openreview.net/forum?id=sgPCP9jOlS
month: '01'
oa: 1
oa_version: Preprint
publication: Proceedings of the 1st International Conference on Probabilistic Numerics
publication_identifier:
eissn:
- 2640-3498
publication_status: published
publisher: ML Research Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Propagating model uncertainty through filtering-based probabilistic numerical
ODE solvers
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: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 271
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '20593'
abstract:
- lang: eng
text: “Quasi-solid-state” conversion mechanisms using sparingly solvating electrolytes
(SPSEs) bridge the gap between traditional solid–liquid–solid and solid-state
sulfur conversion in lithium–sulfur (Li–S) batteries. Although these terms are
commonly used, their precise distinctions and impacts on key performance metrics,
such as rate capability, energy density, and capacity fading, remain poorly understood.
In this work, we employ operando small- and wide-angle X-ray scattering alongside
cryogenic transmission electron microscopy (cryo-TEM) to compare Li–S batteries
in sparingly solvating and solvating ether-based electrolytes. We find that, unlike
solvating electrolytes, SPSEs lead to an extended presence of lithium sulfide
during cycling, coexisting with sulfur at a 50% state of charge and beyond. In
the charged state, solid sulfur is present in its amorphous form inside the carbon
black nanopores. These findings indicate that the limited solubility confines
polysulfides in regions near the carbon surface, where these polysulfides enable
conversion between the coexisting solid discharge and charge product.
acknowledgement: This work was funded by the European Union (ERC-2022-STG, SOLIDCON,
101078271). Views and opinions expressed are, however, those of the authors only
and do not necessarily reflect those of the European Union or the European Research
Council Executive Agency. Neither the European Union nor the granting authority
can be held responsible for them. TEM measurements were carried out on a JEOL JEM
F200 TEM equipped with an energy filter funded by the FFG (grant number 37120633).
The authors thank Klara Neumayr, Ayca Senol Güngör, and Lorenz Gruber for valuable
discussions and support with lab work. N.K. thanks Oskar Paris from Montanuniversität
Leoben for providing access to the gas sorption analyzer.
article_processing_charge: Yes (in subscription journal)
article_type: letter_note
author:
- first_name: Pronoy
full_name: Dutta, Pronoy
last_name: Dutta
- first_name: Jean Marc
full_name: Von Mentlen, Jean Marc
last_name: Von Mentlen
- first_name: Soumyadip
full_name: Mondal, Soumyadip
id: d25d21ef-dc8d-11ea-abe3-ec4576307f48
last_name: Mondal
- first_name: Nikolaos
full_name: Kostoglou, Nikolaos
last_name: Kostoglou
- first_name: Bodo D.
full_name: Wilts, Bodo D.
last_name: Wilts
- first_name: Stefan Alexander
full_name: Freunberger, Stefan Alexander
id: A8CA28E6-CE23-11E9-AD2D-EC27E6697425
last_name: Freunberger
orcid: 0000-0003-2902-5319
- first_name: Gregor A.
full_name: Zickler, Gregor A.
last_name: Zickler
- first_name: Christian
full_name: Prehal, Christian
last_name: Prehal
citation:
ama: 'Dutta P, Von Mentlen JM, Mondal S, et al. Bridging solution and solid-state
mechanism: Confined quasi-solid-state conversion in Li–S batteries. ACS Energy
Letters. 2025;10:5722-5732. doi:10.1021/acsenergylett.5c02093'
apa: 'Dutta, P., Von Mentlen, J. M., Mondal, S., Kostoglou, N., Wilts, B. D., Freunberger,
S. A., … Prehal, C. (2025). Bridging solution and solid-state mechanism: Confined
quasi-solid-state conversion in Li–S batteries. ACS Energy Letters. American
Chemical Society. https://doi.org/10.1021/acsenergylett.5c02093'
chicago: 'Dutta, Pronoy, Jean Marc Von Mentlen, Soumyadip Mondal, Nikolaos Kostoglou,
Bodo D. Wilts, Stefan Alexander Freunberger, Gregor A. Zickler, and Christian
Prehal. “Bridging Solution and Solid-State Mechanism: Confined Quasi-Solid-State
Conversion in Li–S Batteries.” ACS Energy Letters. American Chemical Society,
2025. https://doi.org/10.1021/acsenergylett.5c02093.'
ieee: 'P. Dutta et al., “Bridging solution and solid-state mechanism: Confined
quasi-solid-state conversion in Li–S batteries,” ACS Energy Letters, vol.
10. American Chemical Society, pp. 5722–5732, 2025.'
ista: 'Dutta P, Von Mentlen JM, Mondal S, Kostoglou N, Wilts BD, Freunberger SA,
Zickler GA, Prehal C. 2025. Bridging solution and solid-state mechanism: Confined
quasi-solid-state conversion in Li–S batteries. ACS Energy Letters. 10, 5722–5732.'
mla: 'Dutta, Pronoy, et al. “Bridging Solution and Solid-State Mechanism: Confined
Quasi-Solid-State Conversion in Li–S Batteries.” ACS Energy Letters, vol.
10, American Chemical Society, 2025, pp. 5722–32, doi:10.1021/acsenergylett.5c02093.'
short: P. Dutta, J.M. Von Mentlen, S. Mondal, N. Kostoglou, B.D. Wilts, S.A. Freunberger,
G.A. Zickler, C. Prehal, ACS Energy Letters 10 (2025) 5722–5732.
date_created: 2025-11-02T23:01:35Z
date_published: 2025-10-25T00:00:00Z
date_updated: 2025-12-01T15:11:44Z
day: '25'
ddc:
- '540'
department:
- _id: StFr
doi: 10.1021/acsenergylett.5c02093
external_id:
isi:
- '001600396000001'
file:
- access_level: open_access
checksum: 368eb041c395a5155218f858947df419
content_type: application/pdf
creator: dernst
date_created: 2025-11-04T07:56:19Z
date_updated: 2025-11-04T07:56:19Z
file_id: '20597'
file_name: 2025_ACSEnergyLetters_Dutta.pdf
file_size: 9307654
relation: main_file
success: 1
file_date_updated: 2025-11-04T07:56:19Z
has_accepted_license: '1'
intvolume: ' 10'
isi: 1
language:
- iso: eng
month: '10'
oa: 1
oa_version: Published Version
page: 5722-5732
publication: ACS Energy Letters
publication_identifier:
eissn:
- 2380-8195
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
related_material:
link:
- relation: software
url: ' https://doi.org/10.5281/zenodo.17144229'
scopus_import: '1'
status: public
title: 'Bridging solution and solid-state mechanism: Confined quasi-solid-state conversion
in Li–S batteries'
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: 10
year: '2025'
...
---
OA_place: publisher
OA_type: hybrid
_id: '20594'
abstract:
- lang: eng
text: (Scanning) transmission electron microscopy ((S)TEM) has significantly advanced
materials science but faces challenges in correlating precise atomic structure
information with the functional properties of devices due to its time-intensive
nature. To address this, an analytical workflow is introduced for the holistic
characterization, modelling, and simulation of device heterostructures. This workflow
automates the experimental (S)TEM data analysis, providing an in-depth characterization
of crystallographic information, 3D orientation, elemental composition, and strain
distribution. It reduces a process that typically takes days for a trained human
into an automatic routine solved in minutes. Utilizing a physics-guided artificial
intelligence model, it generates representative descriptions of materials and
samples. The workflow culminates in creating digital twins of systems limited
with at least one axis of translational invariance –3D finite element and atomic
models of millions of atoms–enabling simulations that provide crucial insights
into device behavior in practical applications. Demonstrated with SiGe planar
heterostructures for scalable spin qubits, the workflow links digital twins to
theoretical properties, revealing how atomic structure impacts materials and functional
properties such as spatially-resolved phononic or electronic characteristics,
or (inverse) spin orbit lengths. The versatility of the workflow is demonstrated
through its application to a wide array of materials systems, device configurations,
and sample morphologies.
acknowledgement: 'ICN2 acknowledged funding from Generalitat de Catalunya 2021SGR00457,
2021SGR00997 and 2021SGR01519. The authors thank support from the project AMaDE
(PID2023-149158OB-C43), funded by MCIN/ AEI/10.13039/501100011033/. This study was
part of the Advanced Materials programme and was supported by MCIN with funding
from European Union NextGenerationEU (PRTR-C17.I1) and by Generalitat de Catalunya
(In-CAEM Project). The authors acknowledged support from CSIC Interdisciplinary
Thematic Platform (PTI+) on Quantum Technologies (PTI-QTEP+). This research work
had been funded by the European Commission – NextGenerationEU (Regulation EU 2020/2094),
through CSIC''s Quantum Technologies Platform (QTEP). ICN2 was supported by the
Severo Ochoa program from Spanish MCIN / AEI (Grant No.: CEX2021-001214-S) and was
funded by the CERCA Programme / Generalitat de Catalunya. Part of the present work
had been performed in the framework of Universitat Autònoma de Barcelona Materials
Science PhD program. I.P.H. acknowledged funding from AGAUR-FI scholarship (2023FI-00268)
Joan Oró of the Secretariat of Universities of the Generalitat of Catalonia and
the European SocialPlus Fund. M.B. acknowledged support from SUR Generalitat de
Catalunya and the EU Social Fund; project ref. 2020 FI 00103. This study was supported
by EU HORIZON INFRA TECH 2022 project IMPRESS (Ref.: 101094299). Authors acknowledged
the use of instrumentation as well as the technical advice provided by the Joint
Electron Microscopy Center at ALBA (JEMCA). ICN2 acknowledged funding from Grant
IU16-014206 (METCAM-FIB) funded by the European Union through the European Regional
Development Fund (ERDF), with the support of the Ministry of Research and Universities,
Generalitat de Catalunya. ICN2 was a founding member of e-DREAM.[135] S.R. was also
supported by MICIN with European funds NextGenerationEU (PRTRC17.I1) funded by Generalitat
de Catalunya. P.O. acknowledged support from the EU MaX CoE (Grant No. 101093374),
Grants No. PCI2022-134972-2 and No. PID2022-139776NB-C62 funded by the Spanish MCIN/AEI/10.13039/501100011033
and by the ERDF, A way of making Europe.The authors thank the Catalan Quantum Academy
for support. The authors acknowledged Dámaso Torres for his support in designing
the graphical material.'
article_number: e06785
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Marc
full_name: Botifoll, Marc
last_name: Botifoll
- first_name: Ivan
full_name: Pinto-Huguet, Ivan
last_name: Pinto-Huguet
- first_name: Enzo
full_name: Rotunno, Enzo
last_name: Rotunno
- first_name: Thomas
full_name: Galvani, Thomas
last_name: Galvani
- first_name: Catalina
full_name: Coll, Catalina
last_name: Coll
- first_name: Payam Habibzadeh
full_name: Kavkani, Payam Habibzadeh
last_name: Kavkani
- first_name: Maria Chiara
full_name: Spadaro, Maria Chiara
last_name: Spadaro
- first_name: Yann Michel
full_name: Niquet, Yann Michel
last_name: Niquet
- first_name: Martin Børstad
full_name: Eriksen, Martin Børstad
last_name: Eriksen
- first_name: Sara
full_name: Martí-Sánchez, Sara
last_name: Martí-Sánchez
- first_name: Georgios
full_name: Katsaros, Georgios
id: 38DB5788-F248-11E8-B48F-1D18A9856A87
last_name: Katsaros
orcid: 0000-0001-8342-202X
- first_name: Giordano
full_name: Scappucci, Giordano
last_name: Scappucci
- first_name: Peter
full_name: Krogstrup, Peter
last_name: Krogstrup
- first_name: Giovanni
full_name: Isella, Giovanni
last_name: Isella
- first_name: Andreu
full_name: Cabot, Andreu
last_name: Cabot
- first_name: Gonzalo
full_name: Merino, Gonzalo
last_name: Merino
- first_name: Pablo
full_name: Ordejón, Pablo
last_name: Ordejón
- first_name: Stephan
full_name: Roche, Stephan
last_name: Roche
- first_name: Vincenzo
full_name: Grillo, Vincenzo
last_name: Grillo
- first_name: Jordi
full_name: Arbiol, Jordi
last_name: Arbiol
citation:
ama: 'Botifoll M, Pinto-Huguet I, Rotunno E, et al. Artificial intelligence-assisted
workflow for transmission electron microscopy: From data analysis automation to
materials knowledge unveiling. Advanced Materials. 2025. doi:10.1002/adma.202506785'
apa: 'Botifoll, M., Pinto-Huguet, I., Rotunno, E., Galvani, T., Coll, C., Kavkani,
P. H., … Arbiol, J. (2025). Artificial intelligence-assisted workflow for transmission
electron microscopy: From data analysis automation to materials knowledge unveiling.
Advanced Materials. Wiley. https://doi.org/10.1002/adma.202506785'
chicago: 'Botifoll, Marc, Ivan Pinto-Huguet, Enzo Rotunno, Thomas Galvani, Catalina
Coll, Payam Habibzadeh Kavkani, Maria Chiara Spadaro, et al. “Artificial Intelligence-Assisted
Workflow for Transmission Electron Microscopy: From Data Analysis Automation to
Materials Knowledge Unveiling.” Advanced Materials. Wiley, 2025. https://doi.org/10.1002/adma.202506785.'
ieee: 'M. Botifoll et al., “Artificial intelligence-assisted workflow for
transmission electron microscopy: From data analysis automation to materials knowledge
unveiling,” Advanced Materials. Wiley, 2025.'
ista: 'Botifoll M, Pinto-Huguet I, Rotunno E, Galvani T, Coll C, Kavkani PH, Spadaro
MC, Niquet YM, Eriksen MB, Martí-Sánchez S, Katsaros G, Scappucci G, Krogstrup
P, Isella G, Cabot A, Merino G, Ordejón P, Roche S, Grillo V, Arbiol J. 2025.
Artificial intelligence-assisted workflow for transmission electron microscopy:
From data analysis automation to materials knowledge unveiling. Advanced Materials.,
e06785.'
mla: 'Botifoll, Marc, et al. “Artificial Intelligence-Assisted Workflow for Transmission
Electron Microscopy: From Data Analysis Automation to Materials Knowledge Unveiling.”
Advanced Materials, e06785, Wiley, 2025, doi:10.1002/adma.202506785.'
short: M. Botifoll, I. Pinto-Huguet, E. Rotunno, T. Galvani, C. Coll, P.H. Kavkani,
M.C. Spadaro, Y.M. Niquet, M.B. Eriksen, S. Martí-Sánchez, G. Katsaros, G. Scappucci,
P. Krogstrup, G. Isella, A. Cabot, G. Merino, P. Ordejón, S. Roche, V. Grillo,
J. Arbiol, Advanced Materials (2025).
date_created: 2025-11-02T23:01:35Z
date_published: 2025-10-22T00:00:00Z
date_updated: 2025-12-01T15:12:53Z
day: '22'
ddc:
- '530'
department:
- _id: GeKa
doi: 10.1002/adma.202506785
external_id:
arxiv:
- '2411.01024'
isi:
- '001597428400001'
has_accepted_license: '1'
isi: 1
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1002/adma.202506785
month: '10'
oa: 1
oa_version: Published Version
publication: Advanced Materials
publication_identifier:
eissn:
- 1521-4095
issn:
- 0935-9648
publication_status: epub_ahead
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Artificial intelligence-assisted workflow for transmission electron microscopy:
From data analysis automation to materials knowledge unveiling'
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2025'
...
---
OA_type: closed access
_id: '20603'
abstract:
- lang: eng
text: "We study the growth of sumsets A+B⊂S⊂G, where S does not contain an arithmetic
progression of length 2k+1, and where G is a commutative group, in which every
nonzero element has an order of at least 2k+1. More specifically, we show the
following: if A,B⊂G are sets such that A+B does not contain an arithmetic progression
of length 2k+1, then\r\n|A+B|≥|A|2k−13k−2|B|k3k−2.\r\nAs an application we derive
upper bounds on the cardinality of the summands in sumsets A+B+C contained in
the set of t-th powers, where t≥2 is an integer. In particular, we show that min(|A|,|B|,|C|)≪(logN)4/5
for t=2, and min(|A|,|B|,|C|)≪t(logN)1/2 for t≥3."
acknowledgement: "The authors would like to thank the referee and Ilya Shkredov for
comments on the manuscript.\r\nC. E. is supported by a joint FWF-ANR project ArithRand,
grant numbers FWF I 4945-N and ANR-20-CE91-0006.\r\n"
article_processing_charge: No
article_type: original
author:
- first_name: Christian
full_name: Elsholtz, Christian
last_name: Elsholtz
- first_name: Imre Z.
full_name: Ruzsa, Imre Z.
last_name: Ruzsa
- first_name: Lena
full_name: Wurzinger, Lena
id: 50c57d72-32a8-11ee-aeea-d652094d2ccd
last_name: Wurzinger
orcid: 0009-0004-5360-0074
citation:
ama: Elsholtz C, Ruzsa IZ, Wurzinger L. Sumset growth in progression-free sets.
Acta Arithmetica. 2025;220:289-303. doi:10.4064/aa250115-14-7
apa: Elsholtz, C., Ruzsa, I. Z., & Wurzinger, L. (2025). Sumset growth in progression-free
sets. Acta Arithmetica. Institute of Mathematics. https://doi.org/10.4064/aa250115-14-7
chicago: Elsholtz, Christian, Imre Z. Ruzsa, and Lena Wurzinger. “Sumset Growth
in Progression-Free Sets.” Acta Arithmetica. Institute of Mathematics,
2025. https://doi.org/10.4064/aa250115-14-7.
ieee: C. Elsholtz, I. Z. Ruzsa, and L. Wurzinger, “Sumset growth in progression-free
sets,” Acta Arithmetica, vol. 220. Institute of Mathematics, pp. 289–303,
2025.
ista: Elsholtz C, Ruzsa IZ, Wurzinger L. 2025. Sumset growth in progression-free
sets. Acta Arithmetica. 220, 289–303.
mla: Elsholtz, Christian, et al. “Sumset Growth in Progression-Free Sets.” Acta
Arithmetica, vol. 220, Institute of Mathematics, 2025, pp. 289–303, doi:10.4064/aa250115-14-7.
short: C. Elsholtz, I.Z. Ruzsa, L. Wurzinger, Acta Arithmetica 220 (2025) 289–303.
corr_author: '1'
date_created: 2025-11-04T14:33:16Z
date_published: 2025-09-12T00:00:00Z
date_updated: 2025-12-01T15:18:09Z
day: '12'
department:
- _id: TiBr
doi: 10.4064/aa250115-14-7
external_id:
isi:
- '001570716800001'
intvolume: ' 220'
isi: 1
language:
- iso: eng
month: '09'
oa_version: None
page: 289-303
publication: Acta Arithmetica
publication_identifier:
eissn:
- 1730-6264
issn:
- 0065-1036
publication_status: published
publisher: Institute of Mathematics
quality_controlled: '1'
scopus_import: '1'
status: public
title: Sumset growth in progression-free sets
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 220
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '20604'
abstract:
- lang: eng
text: Entry into and exit from cellular quiescence require dynamic adjustments in
nutrient acquisition, yet the mechanisms by which quiescent cells downregulate
amino acid (AA) transport remain poorly understood. Here we show that cells entering
quiescence selectively target plasma membrane-resident amino acid transporters
for endocytosis and lysosomal degradation. This process matches amino acid uptake
with reduced translational demand and promotes survival during extended periods
of quiescence. Mechanistically, we identify the α-arrestin TXNIP as a key regulator
of this metabolic adaptation, since it mediates the endocytosis of the SLC7A5-SLC3A2
(LAT1-4F2hc) AA transporter complex in response to reduced AKT signaling. To promote
transporter ubiquitination, TXNIP interacts with NEDD4L and other HECT-type ubiquitin
ligases. Loss of TXNIP disrupts this regulation, resulting in dysregulated amino
acid uptake, sustained mTORC1 signaling, and ultimately cell death under prolonged
quiescence. The characterization of a novel TXNIP loss-of-function variant in
a patient with a severe metabolic disease further supports its role in nutrient
homeostasis and human health. Together, these findings highlight TXNIP’s central
role in controlling nutrient acquisition and metabolic plasticity with implications
for quiescence biology and diseases.
acknowledgement: We thank the patient and his family. We are grateful to Hemmo Meyer
and Simona Polo for providing the YFP-tagged HECT-type ubiquitin ligases and to
our protein core facility for excellent support. This research was funded in part
by the Austrian Science Fund (FWF) (10.55776/P35874, 10.55776/P34907 to DT, 10.55776/P35832,
10.55776/P36600 to HF, 10.55776/P36925 to VR, 10.55776/P30196 to SH, 10.55776/FG20
to HF, BS, DT, LAH, KT and MA, 10.55776/DOC82 to DT, SK, LAH). JK is a recipient
of a DOC Fellowship of the Austrian Academy of Sciences. KT acknowledges support
from the DFG (German Research Foundation, project No TH 1358/3-2), the MESI-STRAT
project (grant agreement No 754688) which has received funding from the European
Union’s Horizon 2020 research and innovation programme, and from the European Union
European Research Council (ERC AdG BEYOND STRESS, grant agreement No 101054429)
which has received funding from the European Union’s Horizon Europe research and
innovation programme. Views & opinions are those of the authors. For open access
purposes, the author has applied a CC BY public copyright license to any author
accepted manuscript version arising from this submission.
article_processing_charge: Yes
article_type: original
author:
- first_name: Jennifer
full_name: Kahlhofer, Jennifer
last_name: Kahlhofer
- first_name: Nikolas
full_name: Marchet, Nikolas
last_name: Marchet
- first_name: Kristian
full_name: Zubak, Kristian
last_name: Zubak
- first_name: Brigitta
full_name: Seifert, Brigitta
last_name: Seifert
- first_name: Madlen
full_name: Hotze, Madlen
last_name: Hotze
- first_name: Anna-Sophia
full_name: Egger-Hörschinger, Anna-Sophia
last_name: Egger-Hörschinger
- first_name: Lucija
full_name: Kucej, Lucija
last_name: Kucej
- first_name: Claudia
full_name: Manzl, Claudia
last_name: Manzl
- first_name: Yannick
full_name: Weyer, Yannick
last_name: Weyer
- first_name: Sabine
full_name: Weys, Sabine
id: caffa136-9669-11ed-9092-ceac12ac9c05
last_name: Weys
- first_name: Martin
full_name: Offterdinger, Martin
last_name: Offterdinger
- first_name: Sebastian
full_name: Herzog, Sebastian
last_name: Herzog
- first_name: Veronika
full_name: Reiterer, Veronika
last_name: Reiterer
- first_name: Chiara
full_name: Volani, Chiara
last_name: Volani
- first_name: Marcel
full_name: Kwiatkowski, Marcel
last_name: Kwiatkowski
- first_name: Saskia B
full_name: Wortmann, Saskia B
last_name: Wortmann
- first_name: Siamak
full_name: Nemati, Siamak
last_name: Nemati
- first_name: Johannes A
full_name: Mayr, Johannes A
last_name: Mayr
- first_name: Johannes
full_name: Zschocke, Johannes
last_name: Zschocke
- first_name: Bernhard
full_name: Radlinger, Bernhard
last_name: Radlinger
- first_name: Kathrin
full_name: Thedieck, Kathrin
last_name: Thedieck
- first_name: Leopold
full_name: Kremser, Leopold
last_name: Kremser
- first_name: Bettina
full_name: Sarg, Bettina
last_name: Sarg
- first_name: Lukas A
full_name: Huber, Lukas A
last_name: Huber
- first_name: Hesso
full_name: Farhan, Hesso
last_name: Farhan
- first_name: Mariana E G
full_name: de Araujo, Mariana E G
last_name: de Araujo
- first_name: Susanne
full_name: Kaser, Susanne
last_name: Kaser
- first_name: Sabine
full_name: Scholl-Bürgi, Sabine
last_name: Scholl-Bürgi
- first_name: Daniela
full_name: Karall, Daniela
last_name: Karall
- first_name: David
full_name: Teis, David
last_name: Teis
citation:
ama: Kahlhofer J, Marchet N, Zubak K, et al. TXNIP mediates LAT1/SLC7A5 endocytosis
to limit amino acid uptake in cells entering quiescence. The EMBO Journal.
2025;44:7119-7153. doi:10.1038/s44318-025-00608-9
apa: Kahlhofer, J., Marchet, N., Zubak, K., Seifert, B., Hotze, M., Egger-Hörschinger,
A.-S., … Teis, D. (2025). TXNIP mediates LAT1/SLC7A5 endocytosis to limit amino
acid uptake in cells entering quiescence. The EMBO Journal. Embo Press.
https://doi.org/10.1038/s44318-025-00608-9
chicago: Kahlhofer, Jennifer, Nikolas Marchet, Kristian Zubak, Brigitta Seifert,
Madlen Hotze, Anna-Sophia Egger-Hörschinger, Lucija Kucej, et al. “TXNIP Mediates
LAT1/SLC7A5 Endocytosis to Limit Amino Acid Uptake in Cells Entering Quiescence.”
The EMBO Journal. Embo Press, 2025. https://doi.org/10.1038/s44318-025-00608-9.
ieee: J. Kahlhofer et al., “TXNIP mediates LAT1/SLC7A5 endocytosis to limit
amino acid uptake in cells entering quiescence,” The EMBO Journal, vol.
44. Embo Press, pp. 7119–7153, 2025.
ista: Kahlhofer J, Marchet N, Zubak K, Seifert B, Hotze M, Egger-Hörschinger A-S,
Kucej L, Manzl C, Weyer Y, Weys S, Offterdinger M, Herzog S, Reiterer V, Volani
C, Kwiatkowski M, Wortmann SB, Nemati S, Mayr JA, Zschocke J, Radlinger B, Thedieck
K, Kremser L, Sarg B, Huber LA, Farhan H, de Araujo MEG, Kaser S, Scholl-Bürgi
S, Karall D, Teis D. 2025. TXNIP mediates LAT1/SLC7A5 endocytosis to limit amino
acid uptake in cells entering quiescence. The EMBO Journal. 44, 7119–7153.
mla: Kahlhofer, Jennifer, et al. “TXNIP Mediates LAT1/SLC7A5 Endocytosis to Limit
Amino Acid Uptake in Cells Entering Quiescence.” The EMBO Journal, vol.
44, Embo Press, 2025, pp. 7119–53, doi:10.1038/s44318-025-00608-9.
short: J. Kahlhofer, N. Marchet, K. Zubak, B. Seifert, M. Hotze, A.-S. Egger-Hörschinger,
L. Kucej, C. Manzl, Y. Weyer, S. Weys, M. Offterdinger, S. Herzog, V. Reiterer,
C. Volani, M. Kwiatkowski, S.B. Wortmann, S. Nemati, J.A. Mayr, J. Zschocke, B.
Radlinger, K. Thedieck, L. Kremser, B. Sarg, L.A. Huber, H. Farhan, M.E.G. de
Araujo, S. Kaser, S. Scholl-Bürgi, D. Karall, D. Teis, The EMBO Journal 44 (2025)
7119–7153.
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title: TXNIP mediates LAT1/SLC7A5 endocytosis to limit amino acid uptake in cells
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the Imaging & Optics Facility, the Lab\r\nSupport Facility, and the Miba Machine
Shop. I would like to thank two staff scientists in particular:\r\nRobert Hauschild
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Institute of Science and Technology Austria.'
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Equilibria. Institute of Science and Technology Austria, 2025, doi:10.15479/AT-ISTA-20607.'
short: 'S. Mondal, Oxygen and Sulfur Redox : Conversion Kinetics and Phase Equilibria,
Institute of Science and Technology Austria, 2025.'
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