---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21841'
abstract:
- lang: eng
text: The long-standing notion that genotypes map to phenotypes through simple one
gene–one trait relationships continues to shape both research in the life sciences
and public understanding, with implications for policy and funding priorities.
Yet this paradigm is increasingly recognized as inadequate for explaining continuous
phenotypic variation and the complex genetic architectures of the genotype–phenotype
map. Modern genetics emerged from the early 20th-century synthesis of Mendelian
and biometric schools of heredity, with R.A. Fisher demonstrating early on how
multiple discrete loci could collectively produce continuous variation. Despite
this fundamental insight, Mendelism—with its focus on single genes and standardized
genetic backgrounds—became the dominant framework, shaping current genetics research
and molecular biology as well as science education. The advent of large-scale
genomic data has revealed yet again the limitations of this reductionist approach.
Evidence from quantitative genetics now shows that most phenotypes arise from
complex networks of many interdependent genes and their dynamic responses to environmental
perturbations. Here we trace the historical roots of how Mendelian classical genetics
departed from the biometric school to create the current predominant paradigm
in genetics, despite fundamentally unresolved issues. Moving on from this one-sided
paradigm will require systematic development of integrative, evolutionarily grounded
experimental approaches that better capture the multigenic and context-dependent
nature of inheritance. Achieving such an extended perspective will require methodological
innovation, including advances in large-scale (e.g. automated) phenotyping. Dedicated
research programs will be necessary to advance a new era of genetic research into
the complex mechanisms underlying phenotypic variation.
acknowledgement: We thank a variety of further colleagues for the many inspiring discussions
on the nature of heredity, especially the workshops in Berlin. Special thanks also
to the Stellenbosch Institute for Advanced Studies (STIAS) to provide DT the leisure
and freedom to write up the first version of this perspective. Thanks also to three
reviewers who have helped to improve the manuscript. Two dedicated symposia on the
topic were funded by the Max-Planck Society.
article_number: iyag024
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Diethard
full_name: Tautz, Diethard
last_name: Tautz
- first_name: Luisa F
full_name: Pallares, Luisa F
last_name: Pallares
- first_name: Leif
full_name: Andersson, Leif
last_name: Andersson
- first_name: Neda
full_name: Barghi, Neda
last_name: Barghi
- first_name: Nicholas H
full_name: Barton, Nicholas H
id: 4880FE40-F248-11E8-B48F-1D18A9856A87
last_name: Barton
orcid: 0000-0002-8548-5240
- first_name: Rachael
full_name: Bay, Rachael
last_name: Bay
- first_name: Yingguang Frank
full_name: Chan, Yingguang Frank
last_name: Chan
- first_name: Angela
full_name: Hancock, Angela
last_name: Hancock
- first_name: Tobias S
full_name: Kaiser, Tobias S
last_name: Kaiser
- first_name: Daniel
full_name: Koenig, Daniel
last_name: Koenig
- first_name: Zacharias
full_name: Kontarakis, Zacharias
last_name: Kontarakis
- first_name: Miriam
full_name: Liedvogel, Miriam
last_name: Liedvogel
- first_name: Juliette
full_name: de Meaux, Juliette
last_name: de Meaux
- first_name: Magnus
full_name: Nordborg, Magnus
last_name: Nordborg
- first_name: Abraham A
full_name: Palmer, Abraham A
last_name: Palmer
- first_name: Michael
full_name: Purugganan, Michael
last_name: Purugganan
- first_name: Christian
full_name: Schlötterer, Christian
last_name: Schlötterer
- first_name: Karl
full_name: Schmid, Karl
last_name: Schmid
- first_name: Didier Y R
full_name: Stainier, Didier Y R
last_name: Stainier
- first_name: Detlef
full_name: Weigel, Detlef
last_name: Weigel
- first_name: Jochen B W
full_name: Wolf, Jochen B W
last_name: Wolf
- first_name: Dieter
full_name: Ebert, Dieter
last_name: Ebert
- first_name: Greg
full_name: Gibson, Greg
last_name: Gibson
citation:
ama: 'Tautz D, Pallares LF, Andersson L, et al. Beyond Mendel: A call to revisit
the genotype–phenotype map through new experimental paradigms. Genetics.
2026;232(4). doi:10.1093/genetics/iyag024'
apa: 'Tautz, D., Pallares, L. F., Andersson, L., Barghi, N., Barton, N. H., Bay,
R., … Gibson, G. (2026). Beyond Mendel: A call to revisit the genotype–phenotype
map through new experimental paradigms. Genetics. Oxford University Press.
https://doi.org/10.1093/genetics/iyag024'
chicago: 'Tautz, Diethard, Luisa F Pallares, Leif Andersson, Neda Barghi, Nicholas
H Barton, Rachael Bay, Yingguang Frank Chan, et al. “Beyond Mendel: A Call to
Revisit the Genotype–Phenotype Map through New Experimental Paradigms.” Genetics.
Oxford University Press, 2026. https://doi.org/10.1093/genetics/iyag024.'
ieee: 'D. Tautz et al., “Beyond Mendel: A call to revisit the genotype–phenotype
map through new experimental paradigms,” Genetics, vol. 232, no. 4. Oxford
University Press, 2026.'
ista: 'Tautz D, Pallares LF, Andersson L, Barghi N, Barton NH, Bay R, Chan YF, Hancock
A, Kaiser TS, Koenig D, Kontarakis Z, Liedvogel M, de Meaux J, Nordborg M, Palmer
AA, Purugganan M, Schlötterer C, Schmid K, Stainier DYR, Weigel D, Wolf JBW, Ebert
D, Gibson G. 2026. Beyond Mendel: A call to revisit the genotype–phenotype map
through new experimental paradigms. Genetics. 232(4), iyag024.'
mla: 'Tautz, Diethard, et al. “Beyond Mendel: A Call to Revisit the Genotype–Phenotype
Map through New Experimental Paradigms.” Genetics, vol. 232, no. 4, iyag024,
Oxford University Press, 2026, doi:10.1093/genetics/iyag024.'
short: D. Tautz, L.F. Pallares, L. Andersson, N. Barghi, N.H. Barton, R. Bay, Y.F.
Chan, A. Hancock, T.S. Kaiser, D. Koenig, Z. Kontarakis, M. Liedvogel, J. de Meaux,
M. Nordborg, A.A. Palmer, M. Purugganan, C. Schlötterer, K. Schmid, D.Y.R. Stainier,
D. Weigel, J.B.W. Wolf, D. Ebert, G. Gibson, Genetics 232 (2026).
date_created: 2026-05-07T08:53:40Z
date_published: 2026-04-01T00:00:00Z
date_updated: 2026-05-18T07:51:26Z
day: '01'
ddc:
- '570'
department:
- _id: NiBa
doi: 10.1093/genetics/iyag024
external_id:
pmid:
- '41701356'
file:
- access_level: open_access
checksum: 5a862c539f9dec4511277ad8927c549c
content_type: application/pdf
creator: dernst
date_created: 2026-05-18T07:48:45Z
date_updated: 2026-05-18T07:48:45Z
file_id: '21890'
file_name: 2026_Genetics_Tautz.pdf
file_size: 542844
relation: main_file
success: 1
file_date_updated: 2026-05-18T07:48:45Z
has_accepted_license: '1'
intvolume: ' 232'
issue: '4'
keyword:
- classic genetics
- quantitative genetics
- genotype–phenotype map
language:
- iso: eng
license: https://creativecommons.org/licenses/by/4.0/
month: '04'
oa: 1
oa_version: Published Version
pmid: 1
publication: Genetics
publication_identifier:
eissn:
- 1943-2631
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Beyond Mendel: A call to revisit the genotype–phenotype map through new experimental
paradigms'
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: 232
year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21842'
abstract:
- lang: eng
text: "AM CVn stars are ultra-compact semi-detached binaries consisting of a white
dwarf primary and a hydrogen-depleted secondary. In this\r\npaper, we present
spectroscopic and photometric results of 15 transient sources pre-classified as
AM CVn candidates. Our analysis confirms\r\n9 systems of the type AM CVn, 3 hydrogen-rich
cataclysmic variables (accreting white dwarfs with near-main-sequence stars for
donors),\r\nand 3 systems that could be evolved cataclysmic variables. Eight of
the AM CVn stars are analysed spectroscopically for the first time,\r\nwhich increases
the number of spectroscopically confirmed AM CVns by about 10%. TESS data revealed
the orbital period of the AM CVn\r\nstar ASASSN-20pv to be Porb =27.282 min, which
helps to constrain the possible values of its mass ratio. TESS also helped to
determine\r\nthe superhump periods of one AM CVn star (ASASSN-19ct, Psh =30.94
min) and two cataclysmic variables we classify as WZ Sge stars\r\n(Psh =90.77
min for ZTF18aaaasnn and Psh =91.6min for ASASSN-15na).We identified very different
abundances in the spectra of theAM\r\nCVns binaries ASASSN-15kf and ASASSN-20pv
(both Porb ∼27.5min), suggesting different type of donors. Six of the studied
AMCVns are\r\nX-ray sources, which helped to determine their mass accretion rates.
Photometry shows that the duration of all the superoutbursts detected\r\nin the
AM CVns is consistent with expectations from the disc instability model. Finally,
we provide refined criteria for the identification of\r\nnew systems using all-sky
surveys such as LSST."
acknowledgement: "We are grateful to the anonymous referee for providing\r\nus with
useful comments and suggestions that improved our manuscript.\r\nJK and LRS acknowledge
support from NASA grants NNH22ZDA001N-6152\r\nand 80NSSC24K0638. MPM is partially
supported by the Swiss National\r\nScience Foundation IZSTZ0_216537 and by UNAM
PAPIIT-IG101224. Based\r\non observations obtained at the international Gemini Observatory,
a program\r\nof NSF NOIRLab, which is managed by the Association of Universities
for\r\nResearch in Astronomy (AURA) under a cooperative agreement with the U.S.\r\nNational
Science Foundation on behalf of the Gemini Observatory partnership:\r\nthe U.S.
National Science Foundation (United States), National Research\r\nCouncil (Canada),
Agencia Nacional de Investigación y Desarrollo (Chile), Ministerio de Ciencia, Tecnología
e Innovación (Argentina), Ministério\r\nda Ciência, Tecnologia, Inovações e Comunicações
(Brazil), and Korea\r\nAstronomy and Space Science Institute (Republic of Korea).
The Gemini\r\ndata were obtained from programs GN-2023B-Q-310 and GS-2024A-Q-311\r\n(PI:
Rivera Sandoval) and processed using DRAGONS (Data Reduction for\r\nAstronomy from
Gemini Observatory North and South) The Digitized Sky\r\nSurveys were produced at
the Space Telescope Science Institute under U.S.\r\nGovernment grant NAG W-2166.
The images of these surveys are based on\r\nphotographic data obtained using the
Oschin Schmidt Telescope on Palomar\r\nMountain and the UK Schmidt Telescope. The
plates were processed into the\r\npresent compressed digital form with the permission
of these institutions.\r\nThe National Geographic Society – Palomar Observatory
Sky Atlas (POSS-I)\r\nwas made by the California Institute of Technology with grants
from the\r\nNational Geographic Society. The Second Palomar Observatory Sky Survey\r\n(POSS-II)
was made by the California Institute of Technology with funds\r\nfrom the National
Science Foundation, the National Geographic Society, the\r\nSloan Foundation, the
Samuel Oschin Foundation, and the Eastman Kodak\r\nCorporation. The Oschin Schmidt
Telescope is operated by the California\r\nInstitute of Technology and Palomar Observatory.
The UK Schmidt Telescope\r\nwas operated by the Royal Observatory Edinburgh, with
funding from the\r\nUK Science and Engineering Research Council (later the UK Particle
Physics\r\nand Astronomy Research Council), until 1988 June, and thereafter by the\r\nAnglo-Australian
Observatory. The blue plates of the southern Sky Atlas\r\nand its Equatorial Extension
(together known as the SERC-J), as well as the\r\nEquatorial Red (ER), and the Second
Epoch [red] Survey (SES) were all taken\r\nwith the UK Schmidt. Supplemental funding
for sky-survey work at the ST\r\nScI is provided by the European Southern Observatory.
Based on observations\r\nobtained with the Samuel Oschin Telescope 48-inch and the
60-inch Telescope\r\nat the Palomar Observatory as part of the Zwicky Transient
Facility project.\r\nZTF is supported by the National Science Foundation under Grants
No. AST-\r\n1440341 and AST-2034437 and a collaboration including current partners\r\nCaltech,
IPAC, the Oskar Klein Center at Stockholm University, the University\r\nof Maryland,
University of California, Berkeley, the University of Wisconsin\r\nat Milwaukee,
University of Warwick, Ruhr University, Cornell University,\r\nNorthwestern University,
and Drexel University. Operations are conducted\r\nby COO, IPAC, and UW. This work
has used data from the European\r\nSpace Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia),\r\nprocessed
by the Gaia Data Processing and Analysis Consortium (DPAC,\r\nhttps://www.cosmos.esa.int/web/gaia/dpac/consortium).
Funding for the\r\nDPAC has been provided by national institutions, in particular,
the institutions\r\nparticipating in the Gaia Multilateral Agreement. We acknowledge
with\r\nthanks the variable star observations from the AAVSO International Database\r\ncontributed
by observers worldwide and used in this research. This paper\r\nincludes data collected
by the TESS mission. Funding for the TESS mission\r\nis provided by the NASA Science
Mission Directorate. Some of the data\r\npresented in this paper were obtained from
the B. Mikulski Archive for Space\r\nTelescopes (MAST). This research has made use
of the SIMBAD database,\r\noperated at CDS, Strasbourg, France. This research has
made use of ‘Aladin\r\nsky atlas’ developed at CDS, Strasbourg Observatory, France.
This research\r\nhas made use of the VizieR catalogue access tool, CDS, Strasbourg,
France."
article_number: e052
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Jan
full_name: Kára, Jan
last_name: Kára
- first_name: Liliana
full_name: Rivera Sandoval, Liliana
last_name: Rivera Sandoval
- first_name: Wendy
full_name: Mendoza, Wendy
last_name: Mendoza
- first_name: Thomas
full_name: Maccarone, Thomas
last_name: Maccarone
- first_name: Manuel
full_name: Pichardo Marcano, Manuel
last_name: Pichardo Marcano
- first_name: Luis E.
full_name: Salazar Manzano, Luis E.
last_name: Salazar Manzano
- first_name: Ryan J.
full_name: Oelkers, Ryan J.
last_name: Oelkers
- first_name: Joannes C
full_name: van Roestel, Joannes C
id: 4d122fc8-6083-11f0-87a5-97d68b860333
last_name: van Roestel
citation:
ama: Kára J, Rivera Sandoval L, Mendoza W, et al. A study of transients from ground-based
surveys reveals new ultra-compact accreting white dwarf binaries. Publications
of the Astronomical Society of Australia. 2026;43. doi:10.1017/pasa.2026.10184
apa: Kára, J., Rivera Sandoval, L., Mendoza, W., Maccarone, T., Pichardo Marcano,
M., Salazar Manzano, L. E., … van Roestel, J. C. (2026). A study of transients
from ground-based surveys reveals new ultra-compact accreting white dwarf binaries.
Publications of the Astronomical Society of Australia. Cambridge University
Press. https://doi.org/10.1017/pasa.2026.10184
chicago: Kára, Jan, Liliana Rivera Sandoval, Wendy Mendoza, Thomas Maccarone, Manuel
Pichardo Marcano, Luis E. Salazar Manzano, Ryan J. Oelkers, and Joannes C van
Roestel. “A Study of Transients from Ground-Based Surveys Reveals New Ultra-Compact
Accreting White Dwarf Binaries.” Publications of the Astronomical Society of
Australia. Cambridge University Press, 2026. https://doi.org/10.1017/pasa.2026.10184.
ieee: J. Kára et al., “A study of transients from ground-based surveys reveals
new ultra-compact accreting white dwarf binaries,” Publications of the Astronomical
Society of Australia, vol. 43. Cambridge University Press, 2026.
ista: Kára J, Rivera Sandoval L, Mendoza W, Maccarone T, Pichardo Marcano M, Salazar
Manzano LE, Oelkers RJ, van Roestel JC. 2026. A study of transients from ground-based
surveys reveals new ultra-compact accreting white dwarf binaries. Publications
of the Astronomical Society of Australia. 43, e052.
mla: Kára, Jan, et al. “A Study of Transients from Ground-Based Surveys Reveals
New Ultra-Compact Accreting White Dwarf Binaries.” Publications of the Astronomical
Society of Australia, vol. 43, e052, Cambridge University Press, 2026, doi:10.1017/pasa.2026.10184.
short: J. Kára, L. Rivera Sandoval, W. Mendoza, T. Maccarone, M. Pichardo Marcano,
L.E. Salazar Manzano, R.J. Oelkers, J.C. van Roestel, Publications of the Astronomical
Society of Australia 43 (2026).
date_created: 2026-05-07T08:55:00Z
date_published: 2026-03-27T00:00:00Z
date_updated: 2026-05-12T06:57:40Z
day: '27'
ddc:
- '520'
department:
- _id: IlCa
doi: 10.1017/pasa.2026.10184
file:
- access_level: open_access
checksum: f8f3cd3765948e8b276176c71c9d4e02
content_type: application/pdf
creator: dernst
date_created: 2026-05-12T06:54:10Z
date_updated: 2026-05-12T06:54:10Z
file_id: '21862'
file_name: 2026_PublAstronomicalSocAustralia_Kara.pdf
file_size: 3681016
relation: main_file
success: 1
file_date_updated: 2026-05-12T06:54:10Z
has_accepted_license: '1'
intvolume: ' 43'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
publication: Publications of the Astronomical Society of Australia
publication_identifier:
eissn:
- 1448-6083
issn:
- 1323-3580
publication_status: published
publisher: Cambridge University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: A study of transients from ground-based surveys reveals new ultra-compact accreting
white dwarf binaries
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: 43
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21844'
abstract:
- lang: eng
text: Little red dots (LRDs) are a newly identified class of broad-line active galactic
nuclei (AGNs) with a distinctive V-shaped spectrum characterized by red optical
and blue UV continuum emission. Their high abundance at redshifts of z ∼ 6–8 and
decline at lower redshifts suggest a transient origin. We propose that the spectral
shape of LRDs originates from compact binary black hole systems, in which each
black hole is surrounded by a mini-disk and embedded within a larger circumbinary
disk. With a binary separation of ≲103 Schwarzschild radii, the Wien tail of a
T ≃ 5000 K blackbody spectrum at the inner edge of the circumbinary disk produces
the red optical emission, while the mini-disks power the UV continuum. Binary
torques carve out a gap between the circumbinary disk and the mini-disks, setting
the turnover wavelength of the V-shaped spectrum around the Balmer limit. This
scenario naturally reproduces LRD spectra requiring only modest dust attenuation
(AV ≲ 1 mag), resolving overestimated luminosities for LRDs in previous studies
and alleviating a tension with the so-called Sołtan argument. This model predicts
distinct spectral evolution as the binary orbit decays through binary disk interactions
and gravitational-wave (GW) emission, linking early-stage “proto-LRD” binaries
to the broader AGN population and late-stage “LRD descendants” to coalescing binaries
detectable in GW experiments.
acknowledgement: We greatly thank Kenta Hotokezaka and Hanpu Liu for constructive
discussions. K.I., J.S., X.C., and L.C.H. acknowledge support from National Natural
Science Foundation of China (grant Nos. 12573015, 1251101148, 12233001, and 12473037),
the Beijing Natural Science Foundation (grant No. IS25003), and the China Manned
Space Program (grant No. CMS-CSST-2025-A09). J.S. is also supported by “The Fundamental
Research Funds for the Central Universities, Peking University” (grant No. 7100604896).
Z.H. acknowledges support by US NSF grant AST-2006176 and by NASA grant Nos. 80NSSC24K0440
and 80NSSC22K0822.
article_number: '25'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Kohei
full_name: Inayoshi, Kohei
last_name: Inayoshi
- first_name: Jinyi
full_name: Shangguan, Jinyi
last_name: Shangguan
- first_name: Xian
full_name: Chen, Xian
last_name: Chen
- first_name: Luis C.
full_name: Ho, Luis C.
last_name: Ho
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
orcid: 0000-0003-3633-5403
citation:
ama: Inayoshi K, Shangguan J, Chen X, Ho LC, Haiman Z. The emergence of Little Red
Dots from binary massive black holes. The Astrophysical Journal. 2026;1002(1).
doi:10.3847/1538-4357/ae548d
apa: Inayoshi, K., Shangguan, J., Chen, X., Ho, L. C., & Haiman, Z. (2026).
The emergence of Little Red Dots from binary massive black holes. The Astrophysical
Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae548d
chicago: Inayoshi, Kohei, Jinyi Shangguan, Xian Chen, Luis C. Ho, and Zoltán Haiman.
“The Emergence of Little Red Dots from Binary Massive Black Holes.” The Astrophysical
Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae548d.
ieee: K. Inayoshi, J. Shangguan, X. Chen, L. C. Ho, and Z. Haiman, “The emergence
of Little Red Dots from binary massive black holes,” The Astrophysical Journal,
vol. 1002, no. 1. IOP Publishing, 2026.
ista: Inayoshi K, Shangguan J, Chen X, Ho LC, Haiman Z. 2026. The emergence of Little
Red Dots from binary massive black holes. The Astrophysical Journal. 1002(1),
25.
mla: Inayoshi, Kohei, et al. “The Emergence of Little Red Dots from Binary Massive
Black Holes.” The Astrophysical Journal, vol. 1002, no. 1, 25, IOP Publishing,
2026, doi:10.3847/1538-4357/ae548d.
short: K. Inayoshi, J. Shangguan, X. Chen, L.C. Ho, Z. Haiman, The Astrophysical
Journal 1002 (2026).
date_created: 2026-05-10T22:02:14Z
date_published: 2026-05-01T00:00:00Z
date_updated: 2026-05-11T07:09:12Z
day: '01'
ddc:
- '520'
department:
- _id: ZoHa
doi: 10.3847/1538-4357/ae548d
external_id:
arxiv:
- '2505.05322'
file:
- access_level: open_access
checksum: b4506dfef3dd6da335775071d8f2a0a6
content_type: application/pdf
creator: dernst
date_created: 2026-05-11T07:07:22Z
date_updated: 2026-05-11T07:07:22Z
file_id: '21853'
file_name: 2026_AstrophysicalJour_Inayoshi.pdf
file_size: 3041897
relation: main_file
success: 1
file_date_updated: 2026-05-11T07:07:22Z
has_accepted_license: '1'
intvolume: ' 1002'
issue: '1'
language:
- iso: eng
month: '05'
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: The emergence of Little Red Dots from binary massive black holes
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: 1002
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21845'
abstract:
- lang: eng
text: UTe2 exhibits the remarkable phenomenon of re-entrant superconductivity, whereby
the zero-resistance state reappears above 40 tesla after being suppressed with
a field of around 10 tesla. One potential pairing mechanism, invoked in the related
re-entrant superconductors UCoGe and URhGe, involves transverse fluctuations of
a ferromagnetic order parameter. However, the requisite ferromagnetic order—present
in both UCoGe and URhGe—is absent in UTe2, and neutron scattering shows instead
that the magnetic susceptibility is peaked at an antiferromagnetic wavevector.
Here, we measure the magnetotropic susceptibility of UTe2 across two field-angle
planes. This quantity is sensitive to the magnetic susceptibility in a direction
transverse to the applied magnetic field—a quantity that is not accessed in conventional
magnetization measurements. We observe a very large decrease in the magnetotropic
susceptibility over a broad range of field orientations, indicating a large increase
in the transverse magnetic susceptibility. Because our technique probes the magnetic
susceptibility in the long wavelength (q = 0) limit, this suggests that the strong
transverse susceptibility arises from ferromagnetic spin fluctuations. These ferromagnetic
fluctuations are likely important for understanding the pairing mechanism in UTe2,
as all three superconducting phases of UTe2 surround this region of enhanced susceptibility
in the field-angle phase diagram.
acknowledged_ssus:
- _id: NanoFab
acknowledgement: We appreciate technical support from Salvatore Bagiante, Evgeniia
Volobueva, Lubuna Shafeek, Ali Bangura, and Zoltán Köllö, and scientific discussions
with Daniel Agterberg, Johnpierre Paglione, Qimiao Si, Josephine Yu and Yue Yu.
V.Z., A.N., M.N., and K.A.M. acknowledge funding received from the European Research
Council (ERC) under the European Union’s Horizon 2020 research and innovation programme
(TROPIC-101078696). V.Z., A.N., M.N., and K.A.M. thank the ISTA Nanofabrication
Facility for technical support. B.J.R. acknowledges funding from the Office of Basic
Energy Sciences of the United States Department of Energy under award number DE-SC0020143
for data analysis and writing. The National High Magnetic Field Laboratory is supported
by the National Science Foundation through NSF/DMR-2128556*, the State of Florida,
and the U.S. Department of Energy. A.S. acknowledges support from the DOE/BES “Science
of 100 T” grant. A.S. thanks Downtown Subscription in Santa Fe, NM, for their patience
in hosting him. Sample preparation and characterization were supported by the NSF
through DMR-2105191.
article_number: '3742'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Valeska
full_name: Zambra, Valeska
id: 467ed36b-dc96-11ea-b7c8-b043a380b282
last_name: Zambra
orcid: 0000-0002-8806-5719
- first_name: Amit
full_name: Nathwani, Amit
id: 1a362536-4d02-11f1-8543-8351136efc50
last_name: Nathwani
- first_name: Muhammad
full_name: Nauman, Muhammad
id: 32c21954-2022-11eb-9d5f-af9f93c24e71
last_name: Nauman
orcid: 0000-0002-2111-4846
- first_name: Sylvia K.
full_name: Lewin, Sylvia K.
last_name: Lewin
- first_name: Corey E.
full_name: Frank, Corey E.
last_name: Frank
- first_name: Nicholas P.
full_name: Butch, Nicholas P.
last_name: Butch
- first_name: Arkady
full_name: Shekhter, Arkady
last_name: Shekhter
- first_name: B. J.
full_name: Ramshaw, B. J.
last_name: Ramshaw
- first_name: Kimberly A
full_name: Modic, Kimberly A
id: 13C26AC0-EB69-11E9-87C6-5F3BE6697425
last_name: Modic
orcid: 0000-0001-9760-3147
citation:
ama: Zambra V, Nathwani A, Nauman M, et al. Giant transverse magnetic fluctuations
at the edge of re-entrant superconductivity in UTe2. Nature Communications.
2026;17. doi:10.1038/s41467-026-71899-7
apa: Zambra, V., Nathwani, A., Nauman, M., Lewin, S. K., Frank, C. E., Butch, N.
P., … Modic, K. A. (2026). Giant transverse magnetic fluctuations at the edge
of re-entrant superconductivity in UTe2. Nature Communications. Springer
Nature. https://doi.org/10.1038/s41467-026-71899-7
chicago: Zambra, Valeska, Amit Nathwani, Muhammad Nauman, Sylvia K. Lewin, Corey
E. Frank, Nicholas P. Butch, Arkady Shekhter, B. J. Ramshaw, and Kimberly A Modic.
“Giant Transverse Magnetic Fluctuations at the Edge of Re-Entrant Superconductivity
in UTe2.” Nature Communications. Springer Nature, 2026. https://doi.org/10.1038/s41467-026-71899-7.
ieee: V. Zambra et al., “Giant transverse magnetic fluctuations at the edge
of re-entrant superconductivity in UTe2,” Nature Communications, vol. 17.
Springer Nature, 2026.
ista: Zambra V, Nathwani A, Nauman M, Lewin SK, Frank CE, Butch NP, Shekhter A,
Ramshaw BJ, Modic KA. 2026. Giant transverse magnetic fluctuations at the edge
of re-entrant superconductivity in UTe2. Nature Communications. 17, 3742.
mla: Zambra, Valeska, et al. “Giant Transverse Magnetic Fluctuations at the Edge
of Re-Entrant Superconductivity in UTe2.” Nature Communications, vol. 17,
3742, Springer Nature, 2026, doi:10.1038/s41467-026-71899-7.
short: V. Zambra, A. Nathwani, M. Nauman, S.K. Lewin, C.E. Frank, N.P. Butch, A.
Shekhter, B.J. Ramshaw, K.A. Modic, Nature Communications 17 (2026).
corr_author: '1'
date_created: 2026-05-10T22:02:15Z
date_published: 2026-04-29T00:00:00Z
date_updated: 2026-05-11T06:36:00Z
day: '29'
ddc:
- '530'
department:
- _id: KiMo
- _id: GradSch
doi: 10.1038/s41467-026-71899-7
external_id:
arxiv:
- '2506.08984'
file:
- access_level: open_access
checksum: 8cb95b033ad2a1a7a8181f6f078c05b5
content_type: application/pdf
creator: dernst
date_created: 2026-05-11T06:32:12Z
date_updated: 2026-05-11T06:32:12Z
file_id: '21850'
file_name: 2026_NatureComm_Zambra.pdf
file_size: 1784917
relation: main_file
success: 1
file_date_updated: 2026-05-11T06:32:12Z
has_accepted_license: '1'
intvolume: ' 17'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
project:
- _id: bd968c70-d553-11ed-ba76-cde40b0aba64
grant_number: '101078696'
name: Gaining leverage with spin liquids and superconductors
publication: Nature Communications
publication_identifier:
eissn:
- 2041-1723
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
related_material:
record:
- id: '21174'
relation: research_data
status: public
scopus_import: '1'
status: public
title: Giant transverse magnetic fluctuations at the edge of re-entrant superconductivity
in UTe2
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 17
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21846'
abstract:
- lang: eng
text: 'We compile a sample of 83 little red dots (LRDs) with JWST imaging and find
that a substantial fraction (∼43%, rising to ≳80% for the most luminous LRDs)
host one or more spatially offset, UV-bright companions at projected separations
of 0.5 kpc ≲ d ≲ 5 kpc, with median 〈d〉 = 1.0 kpc. This fraction is even higher
when smaller spatial scales are probed at high signal-to-noise ratio: the two
most strongly lensed LRDs, A383-LRD1 and the newly discovered A68-LRD1, both have
UV-bright companions at separations of only d ∼ 0.3 kpc, below the resolution
limit of most unlensed JWST samples. We explore whether these ubiquitous red/blue
configurations may be physically linked to the formation of LRDs, in analogy with
the “synchronized pair” scenario originally proposed for direct-collapse black
hole formation. In this picture, UV radiation from the companions, with typically
modest stellar masses (M∗ ∼ 108−109 M⊙), suppresses molecular hydrogen cooling
in nearby gas, allowing nearly isothermal collapse and the formation of extremely
compact objects, such as massive black holes, supermassive stars, or quasi-stars.
Using component-resolved photometry and spectral energy distribution modeling,
we infer Lyman–Werner radiation fields of J21,LW ∼ 102.5–105 at the locations
of the red components, comparable to those required in direct-collapse models,
suggesting that the necessary photodissociation conditions are realized in many
LRD systems. This framework provides a simple and self-consistent explanation
for the extreme compactness and distinctive spectral properties of LRDs and links
long-standing theoretical models for early compact object formation directly to
a population now observed with JWST in the early Universe.'
acknowledgement: 'We thank Earl Bellinger, Fabio Pacucci, Andrea Ferrara, and Dale
Kocevski for useful discussions. This work is based on observations made with the
NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski
Archive for Space Telescopes at the Space Telescope Science Institute, which is
operated by the Association of Universities for Research in Astronomy, Inc., under
NASA contract NAS 5-03127 for JWST. These imaging observations are associated with
programs 1345, 1180, 1181, 1243, 6882, 2561, 1324, 4111, and 1895. The compiled
dataset can be accessed at doi:10.17909/1m8f-9c47. The Cosmic Dawn Center (DAWN)
is funded by the Danish National Research Foundation under grant DNRF140. J.M. and
A.T. acknowledge funding by the European Union (ERC, AGENTS, 101076224). This work
was performed in part at Aspen Center for Physics, which is supported by National
Science Foundation grant PHY-2210452. This work used the following Python packages:
Matplotlib (J. D. Hunter 2007), SciPy (P. Virtanen et al. 2020), NumPy (S. van der
Walt et al. 2011), AstroPy (Astropy Collaboration et al. 2022), colossus (B. Diemer
2018), and photutils (L. Bradley et al. 2025).'
article_number: L4
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Josephine F.W.
full_name: Baggen, Josephine F.W.
last_name: Baggen
- first_name: Matthew T.
full_name: Scoggins, Matthew T.
last_name: Scoggins
- first_name: Pieter
full_name: Van Dokkum, Pieter
last_name: Van Dokkum
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
orcid: 0000-0003-3633-5403
- first_name: Alberto
full_name: Torralba Torregrosa, Alberto
id: 018f0249-0e87-11f0-b167-cbce08fbd541
last_name: Torralba Torregrosa
orcid: 0000-0001-5586-6950
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
citation:
ama: 'Baggen JFW, Scoggins MT, Van Dokkum P, Haiman Z, Torralba Torregrosa A, Matthee
JJ. Connecting the dots: UV-bright companions of Little Red Dots as Lyman–Werner
sources enabling direct-collapse Black Hole formation. The Astrophysical Journal
Letters. 2026;1002(1). doi:10.3847/2041-8213/ae58a5'
apa: 'Baggen, J. F. W., Scoggins, M. T., Van Dokkum, P., Haiman, Z., Torralba Torregrosa,
A., & Matthee, J. J. (2026). Connecting the dots: UV-bright companions of
Little Red Dots as Lyman–Werner sources enabling direct-collapse Black Hole formation.
The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ae58a5'
chicago: 'Baggen, Josephine F.W., Matthew T. Scoggins, Pieter Van Dokkum, Zoltán
Haiman, Alberto Torralba Torregrosa, and Jorryt J Matthee. “Connecting the Dots:
UV-Bright Companions of Little Red Dots as Lyman–Werner Sources Enabling Direct-Collapse
Black Hole Formation.” The Astrophysical Journal Letters. IOP Publishing,
2026. https://doi.org/10.3847/2041-8213/ae58a5.'
ieee: 'J. F. W. Baggen, M. T. Scoggins, P. Van Dokkum, Z. Haiman, A. Torralba Torregrosa,
and J. J. Matthee, “Connecting the dots: UV-bright companions of Little Red Dots
as Lyman–Werner sources enabling direct-collapse Black Hole formation,” The
Astrophysical Journal Letters, vol. 1002, no. 1. IOP Publishing, 2026.'
ista: 'Baggen JFW, Scoggins MT, Van Dokkum P, Haiman Z, Torralba Torregrosa A, Matthee
JJ. 2026. Connecting the dots: UV-bright companions of Little Red Dots as Lyman–Werner
sources enabling direct-collapse Black Hole formation. The Astrophysical Journal
Letters. 1002(1), L4.'
mla: 'Baggen, Josephine F. W., et al. “Connecting the Dots: UV-Bright Companions
of Little Red Dots as Lyman–Werner Sources Enabling Direct-Collapse Black Hole
Formation.” The Astrophysical Journal Letters, vol. 1002, no. 1, L4, IOP
Publishing, 2026, doi:10.3847/2041-8213/ae58a5.'
short: J.F.W. Baggen, M.T. Scoggins, P. Van Dokkum, Z. Haiman, A. Torralba Torregrosa,
J.J. Matthee, The Astrophysical Journal Letters 1002 (2026).
date_created: 2026-05-10T22:02:15Z
date_published: 2026-04-10T00:00:00Z
date_updated: 2026-05-11T06:48:33Z
day: '10'
ddc:
- '520'
department:
- _id: ZoHa
- _id: JoMa
doi: 10.3847/2041-8213/ae58a5
external_id:
arxiv:
- '2602.02702'
file:
- access_level: open_access
checksum: 8c31d8603cd6ad39c772a72d136dc3f8
content_type: application/pdf
creator: dernst
date_created: 2026-05-11T06:44:37Z
date_updated: 2026-05-11T06:44:37Z
file_id: '21851'
file_name: 2026_AstrophysicalJourLetters_Baggen.pdf
file_size: 13359642
relation: main_file
success: 1
file_date_updated: 2026-05-11T06:44:37Z
has_accepted_license: '1'
intvolume: ' 1002'
issue: '1'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
grant_number: '101076224'
name: Young galaxies as tracers and agents of cosmic reionization
publication: The Astrophysical Journal Letters
publication_identifier:
eissn:
- 2041-8213
issn:
- 2041-8205
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Connecting the dots: UV-bright companions of Little Red Dots as Lyman–Werner
sources enabling direct-collapse Black Hole formation'
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: 1002
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21847'
abstract:
- lang: eng
text: Analog quantum simulators provide access to many-body dynamics beyond the
reach of classical computation. However, extracting physical insights from experimental
data is often hindered by measurement noise, limited observables, and incomplete
knowledge of the underlying microscopic model. Here, we develop a machine learning
approach based on a variational autoencoder (VAE) to analyze interference measurements
of tunnel-coupled one-dimensional Bose gases, which realize the sine-Gordon quantum
field theory. Trained in an unsupervised manner, the VAE learns a minimal latent
representation that strongly correlates with the equilibrium control parameter
of the system. Applied to nonequilibrium protocols, the latent space uncovers
signatures of frozen-in solitons following rapid cooling, and reveals anomalous
postquench dynamics not captured by conventional correlation-based methods. These
results demonstrate that generative models can extract physically interpretable
variables directly from noisy and sparse experimental data, providing complementary
probes of equilibrium and nonequilibrium physics in quantum simulators. More broadly,
our work highlights how machine learning can supplement established field-theoretical
techniques, paving the way for scalable, data-driven discovery in quantum many-body
systems.
acknowledgement: "We thank Sebastian Erne and Igor Mazets for helpful discussions
and sharing codes for the transfer matrix sampling. This research was funded in
part by the European Research Council: ERC Advanced Grant “Emergence in Quantum
Physics” (EmQ) under Grant Agreement No. 101097858 and ERC Advanced Grant “Artificial
agency and learning in quantum environments” (QuantAI) under Grant Agreement No.
101055129. This work was also supported by the Austrian Science Fund (FWF) (SFB
BeyondC F7102, 10.55776/F71). G.F.-F. acknowledges the European Research Council
AdG NOQIA; MCIN/AEI [PGC2018-0910.13039/501100011033, CEX2019-000910-S/10.13039/501100011033,
Plan National FIDEUA PID2019-106901GB-I00, Plan National STAMEENA PID2022-139099NB,
I00, project funded by MCIN/AEI/10.13039/501100011033 and by the “European Union
NextGenerationEU/PRTR” (PRTR-C17.I1), FPI]; QUANTERA DYNAMITE PCI2022-132919 under
Grant Agreement No. 101017733; Ministry for Digital Transformation and of Civil
Service of the Spanish Government through the QUANTUM ENIA project call—Quantum
Spain project, and by the European Union through the Recovery, Transformation and
Resilience Plan—NextGenerationEU within the framework of the Digital Spain 2026
Agenda; Fundació Cellex; Fundació Mir-Puig; Generalitat de Catalunya (European Social
Fund FEDER and CERCA program); Barcelona Supercomputing Center MareNostrum (FI-2023-3-0024);
(HORIZON-CL4-2022-QUANTUM-02-SGA PASQuanS2.1, 101113690, EU Horizon 2020 FET-OPEN
OPTOlogic, Grant No. 899794, QU-ATTO, 101168628), EU Horizon Europe Program (This
project has received funding from the European Union's Horizon Europe research and
innovation program under Grant Agreement No. 101080086 NeQST); ICFO Internal “QuantumGaudi”
project. This research was funded in whole or in part by the Austrian Science Fund
(FWF) [10.55776/COE1] through the Cluster of Excellence quantA (Quantum Science
Austria).\r\n\r\nThe views and opinions expressed in this article 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."
article_number: '023094'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Frederik Skovbo
full_name: Moller, Frederik Skovbo
id: 43cbcc83-0564-11f0-a935-e37325525859
last_name: Moller
- first_name: Gabriel
full_name: Fernández-Fernández, Gabriel
last_name: Fernández-Fernández
- first_name: Thomas
full_name: Schweigler, Thomas
last_name: Schweigler
- first_name: Paulin
full_name: De Schoulepnikoff, Paulin
last_name: De Schoulepnikoff
- first_name: Jörg
full_name: Schmiedmayer, Jörg
last_name: Schmiedmayer
- first_name: Gorka
full_name: Muñoz-Gil, Gorka
last_name: Muñoz-Gil
citation:
ama: Moller FS, Fernández-Fernández G, Schweigler T, De Schoulepnikoff P, Schmiedmayer
J, Muñoz-Gil G. Learning minimal representations of many-body physics from snapshots
of a quantum simulator. Physical Review Research. 2026;8(2). doi:10.1103/r7pj-gl7r
apa: Moller, F. S., Fernández-Fernández, G., Schweigler, T., De Schoulepnikoff,
P., Schmiedmayer, J., & Muñoz-Gil, G. (2026). Learning minimal representations
of many-body physics from snapshots of a quantum simulator. Physical Review
Research. American Physical Society. https://doi.org/10.1103/r7pj-gl7r
chicago: Moller, Frederik Skovbo, Gabriel Fernández-Fernández, Thomas Schweigler,
Paulin De Schoulepnikoff, Jörg Schmiedmayer, and Gorka Muñoz-Gil. “Learning Minimal
Representations of Many-Body Physics from Snapshots of a Quantum Simulator.” Physical
Review Research. American Physical Society, 2026. https://doi.org/10.1103/r7pj-gl7r.
ieee: F. S. Moller, G. Fernández-Fernández, T. Schweigler, P. De Schoulepnikoff,
J. Schmiedmayer, and G. Muñoz-Gil, “Learning minimal representations of many-body
physics from snapshots of a quantum simulator,” Physical Review Research,
vol. 8, no. 2. American Physical Society, 2026.
ista: Moller FS, Fernández-Fernández G, Schweigler T, De Schoulepnikoff P, Schmiedmayer
J, Muñoz-Gil G. 2026. Learning minimal representations of many-body physics from
snapshots of a quantum simulator. Physical Review Research. 8(2), 023094.
mla: Moller, Frederik Skovbo, et al. “Learning Minimal Representations of Many-Body
Physics from Snapshots of a Quantum Simulator.” Physical Review Research,
vol. 8, no. 2, 023094, American Physical Society, 2026, doi:10.1103/r7pj-gl7r.
short: F.S. Moller, G. Fernández-Fernández, T. Schweigler, P. De Schoulepnikoff,
J. Schmiedmayer, G. Muñoz-Gil, Physical Review Research 8 (2026).
date_created: 2026-05-10T22:02:15Z
date_published: 2026-04-29T00:00:00Z
date_updated: 2026-05-11T06:58:56Z
day: '29'
ddc:
- '530'
department:
- _id: EdHa
doi: 10.1103/r7pj-gl7r
external_id:
arxiv:
- '2509.13821'
file:
- access_level: open_access
checksum: dbfc58e1e176f7b63e0d274eb0d1bffa
content_type: application/pdf
creator: dernst
date_created: 2026-05-11T06:56:58Z
date_updated: 2026-05-11T06:56:58Z
file_id: '21852'
file_name: 2026_PhysicalReviewResearch_Moller.pdf
file_size: 1829628
relation: main_file
success: 1
file_date_updated: 2026-05-11T06:56:58Z
has_accepted_license: '1'
intvolume: ' 8'
issue: '2'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
publication: Physical Review Research
publication_identifier:
eissn:
- 2643-1564
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Learning minimal representations of many-body physics from snapshots of a quantum
simulator
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 8
year: '2026'
...
---
OA_place: publisher
_id: '21863'
abstract:
- lang: eng
text: "Atoms and photons, two things so different but yet so alike. The former,
the building block of matter, something we learn about in school and imagine it
as some tiny marbles encircled by other tinier marbles. The latter, an electromagnetic
wave, a light particle or an excitation of the electromagnetic field. Quantum
mechanics tells us about the properties of these two entities. And even if it
sounds, looks and writes counter-intuitive, it has proven right for over a century
now.\r\n\r\nIn this work, I elaborate on how we tested the laws of quantum mechanics
and how we used them learn more about the tiny building blocks of nature and the
fields they use to talk to each other. The atoms we use, are artificial. Superconducting
qubits, small electrical circuits with quantized energy levels behave like electrons
that transition between different orbitals in an atom. One of the qubits' advantages,
is also a big disadvantage. We design the circuits' energy levels and fabricate
them in a cleanroom. This allows for arbitrary spaced energy levels but in contrast
to real atoms, prevents two superconducting qubits from being alike. Still, this
qubit platform is one of the frontrunners for future quantum computing technology
and testing fundamental physics due to their scalability.\r\n\r\nWe interface
superconducting qubits, which operate in the GHz regime, with microwave photons.
We use 3D aluminum cavities as mediators between qubits and photons. The cavities
allow for non-destructive readout of the qubit state, they shield the qubits from
noise at the qubit frequency and they give us an easy way to frequency-tune these
joint systems.\r\n\r\nWe need to operate superconducting qubits and their cavities
at millikelvin temperatures in dilution refrigerators. At higher temperatures,
superconductivity suffers and even worse, the environment is filled with thermal
noise photons. This poses a fundamental limitation on the scalability of superconducting
qubit devices. Also connecting multiple devices in different fridges does not
work over room temperature links because the microwave photons used for this purpose
will be covered in noise and the quantum information they carry, will be unusable.\r\n\r\nInfrared
photons do not suffer from this noise problem since there are close to zero thermal
noise photons at their frequencies at room temperature. We cannot simply interface
superconducting devices with optical photons due their frequency mismatch and
the destructive effect of optical photons on superconductors. Therefore, we use
microwave-to-optics transducers that allow to convert microwave photons into optical
ones and vice-versa. The transducers that we use are macroscopic electro-optic
transducers using the Pockels effect in a disk-shaped Lithium Niobate whispering
gallery mode resonator. By using a strong optical pump, photons from the two frequency
domains experience a beam-splitter interaction and get converted from one to the
other.\r\n\r\nWe measure the generated optical photons using elaborate optical
setups, optical heterodyning and single photon detectors to gain knowledge about
the qubit state or the converted microwave photons. Bridging the microwave and
the optical world allows us to take advantage of both of their strengths but it
also requires deep knowledge about both of their working principles.\r\n\r\nIn
this work, we describe two experiments that our group conducted to showcase the
opportunities that arise from interfacing superconducting qubits with optical
photons but also the pitfalls, one may encounter on the way.\r\n\r\nIn the first
experiment, we managed to all-optically read out a superconducting qubit. We show
that the assignment fidelity, the probability that a measurement of the qubit
state matches the prepared state, is close to equal for all-optical, microwave-to-optics
and conventional microwave readout. We show T1 and T2 measurements for all three
readout types and give an analysis of the noise caused by the optics. Finally,
we show that the infrared light does not affect the qubit performance in a negative
way but that the heating it causes does. This is an important insight that we
used in the next experiment.\r\n\r\nThe second experiment is the upconversion
of itinerant single microwave photons to the optical domain. We show that we can
generate single microwave photons from a qubit-cavity system. We upconvert these
single photons, measure them with a single photon detector and reconstruct their
shape. By conducting a single photon Rabi measurement, we show correlations between
the microwave and the optical domain. And by thorough signal-to-noise measurements
and noise analysis, we find that we can generate single infrared photons with
high signal-to-noise ratio 5.1 and low transducer added noise (<0.012 quanta).
We show that this measurement creates a path towards entanglement of a superconducting
qubit and an optical photon and what parameters need to be improved to achieve
it. Additionally, this experiment is a proof of principle for an on-demand infrared
single photon source. More generally, it allows to link microwave quantum technology
in general to the optical domain."
acknowledged_ssus:
- _id: M-Shop
- _id: NanoFab
- _id: LifeSc
- _id: SSU
acknowledgement: "The author of this work was supported by the European Research Council
under grant no.\r\n101089099 (ERC CoG cQEO) and the European Union’s Horizon 2020
research and innovation\r\nprogram under grant no. 899354 (FETopen SuperQuLAN).\r\nThis
work was also supported by the European Research Council under grant nos. 758053\r\n(ERC
StG QUNNECT), 101248662 (ERC POC CoupledEOT), and the European Innovation\r\nCouncil
no. 101187231 (PathfinderOpen CIELO). This research was funded in whole or in part\r\nby
the Austrian Science Fund (FWF) [10.55776/F71]. For open access purposes, the author\r\nhas
applied a CC BY public copyright license to any author accepted manuscript version
arising\r\nfrom this submission.\r\niii\r\nMy co-authors in the works mentioned
later acknowledge generous support from the ISTFELLOW program, the NOMIS-ISTA fellowship,
the Horizon Europe Program HORIZONCL4-2022-QUANTUM-01-SGA via Project No. 101113946
OpenSuperQPlus100 and a DOC fellowship of the Austrian Academy of Sciences at IST
Austria.\r\n"
alternative_title:
- ISTA Thesis
article_processing_charge: No
author:
- first_name: Thomas
full_name: Werner, Thomas
id: 1fcd8497-dba3-11ea-a45e-c6fbd715f7c7
last_name: Werner
orcid: 0009-0001-2346-5236
citation:
ama: Werner T. Interfacing superconducting qubits with optical photons. 2026. doi:10.15479/AT-ISTA-21863
apa: Werner, T. (2026). Interfacing superconducting qubits with optical photons.
Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-21863
chicago: Werner, Thomas. “Interfacing Superconducting Qubits with Optical Photons.”
Institute of Science and Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-21863.
ieee: T. Werner, “Interfacing superconducting qubits with optical photons,” Institute
of Science and Technology Austria, 2026.
ista: Werner T. 2026. Interfacing superconducting qubits with optical photons. Institute
of Science and Technology Austria.
mla: Werner, Thomas. Interfacing Superconducting Qubits with Optical Photons.
Institute of Science and Technology Austria, 2026, doi:10.15479/AT-ISTA-21863.
short: T. Werner, Interfacing Superconducting Qubits with Optical Photons, Institute
of Science and Technology Austria, 2026.
corr_author: '1'
date_created: 2026-05-12T09:04:02Z
date_published: 2026-05-12T00:00:00Z
date_updated: 2026-05-20T13:35:43Z
day: '12'
ddc:
- '530'
- '537'
- '539'
degree_awarded: PhD
department:
- _id: GradSch
- _id: JoFi
doi: 10.15479/AT-ISTA-21863
ec_funded: 1
file:
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checksum: a5b4d8dba83f96e955a3625c0eebee98
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creator: twerner
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relation: source_file
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has_accepted_license: '1'
keyword:
- Superconducting qubits
- Quantum optics
- Single photons and quantum effects
- Nonlinear optics
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
page: '97'
project:
- _id: bdadfa0d-d553-11ed-ba76-fb85edbd456a
grant_number: '101089099'
name: 'Cavity Quantum Electro Optics: Microwave photonics with nonclassical states'
- _id: 9B868D20-BA93-11EA-9121-9846C619BF3A
call_identifier: H2020
grant_number: '899354'
name: Quantum Local Area Networks with Superconducting Qubits
- _id: 26336814-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '758053'
name: A Fiber Optic Transceiver for Superconducting Qubits
- _id: 5b807754-ab3d-11f0-914f-ff8c34502cc9
grant_number: '101248662'
name: Integrated optical coupling for low loss electro-optic interconnects
- _id: 91aaf765-16d5-11f0-9cad-a8e7e44cccb7
grant_number: '101187231'
name: 'Cavity-Integrated Electro-Optics: Measuring, Converting and Manipulating
Microwaves with Light'
- _id: bdb108fd-d553-11ed-ba76-83dc74a9864f
grant_number: F07105
name: QUANTUM INFORMATION SYSTEMS BEYOND CLASSICAL CAPABILITIES / P5- Integration
of Superconducting Quantum Circuits
- _id: bdb7cfc1-d553-11ed-ba76-d2eaab167738
grant_number: '101080139'
name: Open Superconducting Quantum Computers (OpenSuperQPlus)
- _id: 9B861AAC-BA93-11EA-9121-9846C619BF3A
name: NOMIS Fellowship Program
publication_identifier:
issn:
- 2663-337X
publication_status: published
publisher: Institute of Science and Technology Austria
related_material:
record:
- id: '19073'
relation: part_of_dissertation
status: public
- id: '21870'
relation: part_of_dissertation
status: public
status: public
supervisor:
- first_name: Johannes M
full_name: Fink, Johannes M
id: 4B591CBA-F248-11E8-B48F-1D18A9856A87
last_name: Fink
orcid: 0000-0001-8112-028X
title: Interfacing superconducting qubits with optical photons
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)
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type: dissertation
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
year: '2026'
...
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abstract:
- lang: eng
text: Superconducting qubits are a leading candidate for utility-scale quantum computing
due to their fast gate speeds and steadily decreasing error rates. The requirement
for millikelvin operating temperatures, however, creates a significant scaling
bottleneck. Modular architectures using optical fiber links could bridge separate
cryogenic nodes, but superconducting circuits do not have coherent optical transitions
and microwave-to-optical conversion has not been shown for any non-classical photon
state. In this work, we demonstrate the on-demand generation and tomographic reconstruction
of itinerant single microwave photons at 8.9 GHz from a superconducting qubit.
We upconvert this non-Gaussian state with a transducer added noise below 0.012
quanta and count the converted telecom photons at 193.4 THz with a signal-to-noise
ratio of up to 5.1$\pm$1.1. We characterize the trade-offs between throughput
and noise, and establish a viable path toward heralded entanglement distribution
and gate teleportation. Looking ahead, these results empower existing superconducting
devices to take a key role in distributed quantum technologies and heterogeneous
quantum systems.
acknowledgement: "We thank Fritz Diorico and Onur Hosten who suggested the filter
cavity design, and gave important insights about the assembly and the testing of
the FabryPerot filter cavities. Ekatrina Fedotova and Diego A.\r\nLancheros Naranjo
worked on the filter cavity setup in\r\nthe early stages of this work. Gustavo Wiederhecker
and\r\nYiewen Chu provided insights as to the origins of the\r\nobserved optical
noise and Nicola Carlon Zambon suggested using telecom filters to mitigate it further.
This\r\nwork was supported by the European Research Council under grant agreement
no. 101089099 (ERC CoG\r\ncQEO), and 101248662 (ERC POC CoupledEOT), the\r\nEuropean
Unions Horizon 2020 research and innovation\r\nprogram under grant agreement no.
899354 (FETopen\r\nSuperQuLAN), the European Innovation Council no.\r\n101187231
(PathfinderOpen CIELO), and the Austrian\r\nScience Fund (FWF) no. F7105 (SFB BeyondC).
J.F.\r\nand L.K. acknowledge support from the Horizon Europe\r\nProgram HORIZON-CL4-2022-QUANTUM-01-SGA
via\r\nProject No. 101113946 OpenSuperQPlus100. A.M. acknowledges support from the
NOMIS-ISTA fellowship."
article_processing_charge: No
arxiv: 1
author:
- first_name: Thomas
full_name: Werner, Thomas
id: 1fcd8497-dba3-11ea-a45e-c6fbd715f7c7
last_name: Werner
orcid: 0009-0001-2346-5236
- first_name: Erfan
full_name: Riyazi, Erfan
id: 53322f94-5355-11ee-ae5a-ff6f81c87d51
last_name: Riyazi
- first_name: Samarth
full_name: Hawaldar, Samarth
id: 221708e1-1ff6-11ee-9fa6-85146607433e
last_name: Hawaldar
orcid: 0000-0002-1965-4309
- first_name: Rishabh
full_name: Sahu, Rishabh
id: 47D26E34-F248-11E8-B48F-1D18A9856A87
last_name: Sahu
orcid: 0000-0001-6264-2162
- first_name: Georg M
full_name: Arnold, Georg M
id: 3770C838-F248-11E8-B48F-1D18A9856A87
last_name: Arnold
orcid: 0000-0003-1397-7876
- first_name: Paul Falthansl-Scheinecker
full_name: Paul Falthansl-Scheinecker, Paul Falthansl-Scheinecker
last_name: Paul Falthansl-Scheinecker
- first_name: Jennifer A. Sánchez
full_name: Naranjo, Jennifer A. Sánchez
last_name: Naranjo
- first_name: Dante
full_name: Loi, Dante
last_name: Loi
- first_name: Lucky N.
full_name: Kapoor, Lucky N.
last_name: Kapoor
- first_name: Martin
full_name: Zemlicka, Martin
id: 2DCF8DE6-F248-11E8-B48F-1D18A9856A87
last_name: Zemlicka
orcid: 0009-0005-0878-3032
- first_name: Liu
full_name: Qiu, Liu
id: 45e99c0d-1eb1-11eb-9b96-ed8ab2983cac
last_name: Qiu
orcid: 0000-0003-4345-4267
- first_name: Andrei
full_name: Militaru, Andrei
id: d67706f8-8eb1-11ee-ad1b-9c30dfa19e0b
last_name: Militaru
- first_name: Johannes M
full_name: Fink, Johannes M
id: 4B591CBA-F248-11E8-B48F-1D18A9856A87
last_name: Fink
orcid: 0000-0001-8112-028X
citation:
ama: Werner T, Riyazi E, Hawaldar S, et al. Electro-optic conversion of itinerant
Fock states. arXiv. doi:10.48550/arXiv.2602.00928
apa: Werner, T., Riyazi, E., Hawaldar, S., Sahu, R., Arnold, G. M., Paul Falthansl-Scheinecker,
P. F.-S., … Fink, J. M. (n.d.). Electro-optic conversion of itinerant Fock states.
arXiv. https://doi.org/10.48550/arXiv.2602.00928
chicago: Werner, Thomas, Erfan Riyazi, Samarth Hawaldar, Rishabh Sahu, Georg M Arnold,
Paul Falthansl-Scheinecker Paul Falthansl-Scheinecker, Jennifer A. Sánchez Naranjo,
et al. “Electro-Optic Conversion of Itinerant Fock States.” ArXiv, n.d.
https://doi.org/10.48550/arXiv.2602.00928.
ieee: T. Werner et al., “Electro-optic conversion of itinerant Fock states,”
arXiv. .
ista: Werner T, Riyazi E, Hawaldar S, Sahu R, Arnold GM, Paul Falthansl-Scheinecker
PF-S, Naranjo JAS, Loi D, Kapoor LN, Zemlicka M, Qiu L, Militaru A, Fink JM. Electro-optic
conversion of itinerant Fock states. arXiv, 10.48550/arXiv.2602.00928.
mla: Werner, Thomas, et al. “Electro-Optic Conversion of Itinerant Fock States.”
ArXiv, doi:10.48550/arXiv.2602.00928.
short: T. Werner, E. Riyazi, S. Hawaldar, R. Sahu, G.M. Arnold, P.F.-S. Paul Falthansl-Scheinecker,
J.A.S. Naranjo, D. Loi, L.N. Kapoor, M. Zemlicka, L. Qiu, A. Militaru, J.M. Fink,
ArXiv (n.d.).
corr_author: '1'
date_created: 2026-05-12T13:58:18Z
date_published: 2026-01-31T00:00:00Z
date_updated: 2026-05-20T13:35:42Z
day: '31'
department:
- _id: JoFi
- _id: GradSch
doi: 10.48550/arXiv.2602.00928
ec_funded: 1
external_id:
arxiv:
- '2602.00928'
language:
- iso: eng
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grant_number: '101089099'
name: 'Cavity Quantum Electro Optics: Microwave photonics with nonclassical states'
- _id: 5b807754-ab3d-11f0-914f-ff8c34502cc9
grant_number: '101248662'
name: Integrated optical coupling for low loss electro-optic interconnects
- _id: 9B868D20-BA93-11EA-9121-9846C619BF3A
call_identifier: H2020
grant_number: '899354'
name: Quantum Local Area Networks with Superconducting Qubits
- _id: 91aaf765-16d5-11f0-9cad-a8e7e44cccb7
grant_number: '101187231'
name: 'Cavity-Integrated Electro-Optics: Measuring, Converting and Manipulating
Microwaves with Light'
- _id: 26927A52-B435-11E9-9278-68D0E5697425
call_identifier: FWF
grant_number: F07105
name: Integrating superconducting quantum circuits
- _id: 9B861AAC-BA93-11EA-9121-9846C619BF3A
name: NOMIS Fellowship Program
publication: arXiv
publication_status: draft
related_material:
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relation: dissertation_contains
status: public
scopus_import: '1'
status: public
title: Electro-optic conversion of itinerant Fock states
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: '2026'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21881'
abstract:
- lang: eng
text: "I review recent contributions on nonlinear Dirichlet forms. Then, I specialise
to the case of 2-\r\nhomogeneous and local forms. Inspired by the theory of Finsler
manifolds and metric measure spaces, I establish new properties of such nonlinear
Dirichlet forms, which are reminiscent of differential calculus formulae."
acknowledgement: I am thankful to G. Savaré, for introducing me to the study of nonlinear
Dirichlet forms and metric measure spaces, and to D. Manini for stimulating discussions.
Open access funding provided by Institute of Science and Technology (IST Austria).
The author has been funded by the European Union’s Horizon 2020 research and innovation
program under the Marie Skłodowska-Curie grant agreement No 754362. Partial support
has been obtained from the EFI ANR-17-CE40-0030 Project of the French National Research
Agency.
article_number: '33'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Giovanni
full_name: Brigati, Giovanni
id: 63ff57e8-1fbb-11ee-88f2-f558ffc59cf1
last_name: Brigati
citation:
ama: Brigati G. Nonlinear Dirichlet forms, energy spaces, and calculus rules. La
Matematica. 2026;5(2). doi:10.1007/s44007-026-00217-w
apa: Brigati, G. (2026). Nonlinear Dirichlet forms, energy spaces, and calculus
rules. La Matematica. Springer Nature. https://doi.org/10.1007/s44007-026-00217-w
chicago: Brigati, Giovanni. “Nonlinear Dirichlet Forms, Energy Spaces, and Calculus
Rules.” La Matematica. Springer Nature, 2026. https://doi.org/10.1007/s44007-026-00217-w.
ieee: G. Brigati, “Nonlinear Dirichlet forms, energy spaces, and calculus rules,”
La Matematica, vol. 5, no. 2. Springer Nature, 2026.
ista: Brigati G. 2026. Nonlinear Dirichlet forms, energy spaces, and calculus rules.
La Matematica. 5(2), 33.
mla: Brigati, Giovanni. “Nonlinear Dirichlet Forms, Energy Spaces, and Calculus
Rules.” La Matematica, vol. 5, no. 2, 33, Springer Nature, 2026, doi:10.1007/s44007-026-00217-w.
short: G. Brigati, La Matematica 5 (2026).
corr_author: '1'
date_created: 2026-05-17T22:02:10Z
date_published: 2026-04-29T00:00:00Z
date_updated: 2026-05-18T08:27:08Z
day: '29'
ddc:
- '510'
department:
- _id: JaMa
doi: 10.1007/s44007-026-00217-w
external_id:
arxiv:
- '2309.00377'
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file_size: 394082
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issue: '2'
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month: '04'
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publication: La Matematica
publication_identifier:
eissn:
- 2730-9657
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publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Nonlinear Dirichlet forms, energy spaces, and calculus rules
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: 5
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...
---
DOAJ_listed: '1'
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_id: '21882'
abstract:
- lang: eng
text: The nature of little red dots (LRDs) has largely been investigated through
their continuum emission, with lines assumed to arise from a broad-line region.
In this paper, we instead use recombination lines to infer the intrinsic properties
of the central engine. Our analysis first reveals a tension between the ionizing
properties implied from Hα and He ii λ4686. The high Hα EWs require copious H-ionizing
photons, more than the bluest active galactic nucleus (AGN) ionizing spectra can
provide. In contrast, He ii emission is marginally detected, and its low EW is,
at most, consistent with the softest AGN spectra. The low He ii/Hβ (∼10−2, <20× local
AGN median) further points to an unusually soft ionizing spectrum. We extend our
analysis to dense gas envelopes (quasi-star/black-hole star) and find that hydrogen
recombination lines become optically thick and lose diagnostic power, but He ii
remains optically thin and a robust tracer. Photoionization modeling with Cloudy
rules out standard AGN accretion disk spectra. Alternative explanations include
exotic AGN with red rest-optical emission, high average optical depth (>10) from
gas/dust, and soft ionizing spectra with abundant H-ionizing photons, consistent
with, e.g., a cold accretion disk or a composite of AGN and stars. The latter
is an intriguing scenario since high hydrogen densities are highly conducive for
star formation, and nuclear star clusters are found in the vicinity of local massive
black holes. While previous studies have mostly focused on features dominated
by the absorbing hydrogen cloud, the He ii-based diagnostic proposed here represents
a crucial step toward understanding the central engine of LRDs.
acknowledgement: "B.W. thanks Michael Eracleous for valuable discussions. B.W. and
J.L. acknowledge support from JWST-GO-04233.009. B.W. also acknowledges support
provided by NASA through Hubble Fellowship grant HST-HF2-51592.001 awarded by the
Space Telescope Science Institute, which is operated by the Association of Universities
for Research in Astronomy, Inc., for NASA, under the contract NAS 5-26555. K.I.
acknowledges support from the National Natural Science Foundation of China (12573015,
W2532003), the Beijing Natural Science Foundation (IS25003), and the China Manned
Space Program (CMS-CSST-2025-A09). R.E.H. acknowledges support by the German Aerospace
Center (DLR) and the Federal Ministry for Economic Affairs and Energy (BMWi) through
program 50OR2403 “RUBIES.”\r\n\r\nThis work is based on observations made with the
NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski
Archive for Space Telescopes at the Space Telescope Science Institute, which is
operated by the Association of Universities for Research in Astronomy, Inc., under
NASA contract NAS 5-03127 for JWST. These observations are associated with program
# 1433, 2561, 4106, 4233, 5224, 6585. The specific observations analyzed can be
accessed via DOI: 10.17909/9hpc-nc45. Computations for this research were performed
on the Pennsylvania State University’s Institute for Computational and Data Sciences’
Roar supercomputer; and on computational resources managed and supported by Princeton
Research Computing, a consortium of groups including the Princeton Institute for
Computational Science and Engineering (PICSciE) and Research Computing at Princeton
University. Some of the stellar spectra are retrieved from the POLLUX database (pollux.oreme.org)
operated at LUPM (Université de Montpellier—CNRS, France) with the support of the
PNPS and INSU. This publication made use of the NASA Astrophysical Data System for
bibliographic information."
article_number: '10'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Bingjie
full_name: Wang, Bingjie
last_name: Wang
- first_name: Joel
full_name: Leja, Joel
last_name: Leja
- first_name: Harley
full_name: Katz, Harley
last_name: Katz
- first_name: Kohei
full_name: Inayoshi, Kohei
last_name: Inayoshi
- first_name: Nikko J.
full_name: Cleri, Nikko J.
last_name: Cleri
- first_name: Anna
full_name: De Graaff, Anna
last_name: De Graaff
- first_name: Raphael E.
full_name: Hviding, Raphael E.
last_name: Hviding
- first_name: Pieter
full_name: Van Dokkum, Pieter
last_name: Van Dokkum
- first_name: Jenny E.
full_name: Greene, Jenny E.
last_name: Greene
- first_name: Ivo
full_name: Labbé, Ivo
last_name: Labbé
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Ian
full_name: Mcconachie, Ian
last_name: Mcconachie
- first_name: Rohan P.
full_name: Naidu, Rohan P.
last_name: Naidu
- first_name: Erica J.
full_name: Nelson, Erica J.
last_name: Nelson
citation:
ama: 'Wang B, Leja J, Katz H, et al. The missing hard photons of Little Red Dots:
Their incident ionizing spectra resemble massive stars. The Astrophysical Journal.
2026;1003(1). doi:10.3847/1538-4357/ae5bab'
apa: 'Wang, B., Leja, J., Katz, H., Inayoshi, K., Cleri, N. J., De Graaff, A., …
Nelson, E. J. (2026). The missing hard photons of Little Red Dots: Their incident
ionizing spectra resemble massive stars. The Astrophysical Journal. IOP
Publishing. https://doi.org/10.3847/1538-4357/ae5bab'
chicago: 'Wang, Bingjie, Joel Leja, Harley Katz, Kohei Inayoshi, Nikko J. Cleri,
Anna De Graaff, Raphael E. Hviding, et al. “The Missing Hard Photons of Little
Red Dots: Their Incident Ionizing Spectra Resemble Massive Stars.” The Astrophysical
Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae5bab.'
ieee: 'B. Wang et al., “The missing hard photons of Little Red Dots: Their
incident ionizing spectra resemble massive stars,” The Astrophysical Journal,
vol. 1003, no. 1. IOP Publishing, 2026.'
ista: 'Wang B, Leja J, Katz H, Inayoshi K, Cleri NJ, De Graaff A, Hviding RE, Van
Dokkum P, Greene JE, Labbé I, Matthee JJ, Mcconachie I, Naidu RP, Nelson EJ. 2026.
The missing hard photons of Little Red Dots: Their incident ionizing spectra resemble
massive stars. The Astrophysical Journal. 1003(1), 10.'
mla: 'Wang, Bingjie, et al. “The Missing Hard Photons of Little Red Dots: Their
Incident Ionizing Spectra Resemble Massive Stars.” The Astrophysical Journal,
vol. 1003, no. 1, 10, IOP Publishing, 2026, doi:10.3847/1538-4357/ae5bab.'
short: B. Wang, J. Leja, H. Katz, K. Inayoshi, N.J. Cleri, A. De Graaff, R.E. Hviding,
P. Van Dokkum, J.E. Greene, I. Labbé, J.J. Matthee, I. Mcconachie, R.P. Naidu,
E.J. Nelson, The Astrophysical Journal 1003 (2026).
date_created: 2026-05-17T22:02:10Z
date_published: 2026-05-01T00:00:00Z
date_updated: 2026-05-18T08:18:39Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ae5bab
external_id:
arxiv:
- '2508.18358'
file:
- access_level: open_access
checksum: ee9ebc8ae2304fec04f24b82ebaac8bc
content_type: application/pdf
creator: dernst
date_created: 2026-05-18T08:17:26Z
date_updated: 2026-05-18T08:17:26Z
file_id: '21891'
file_name: 2026_AstrophysicalJourn_Wang.pdf
file_size: 2584417
relation: main_file
success: 1
file_date_updated: 2026-05-18T08:17:26Z
has_accepted_license: '1'
intvolume: ' 1003'
issue: '1'
language:
- iso: eng
month: '05'
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: 'The missing hard photons of Little Red Dots: Their incident ionizing spectra
resemble massive stars'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 1003
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '21884'
abstract:
- lang: eng
text: "We show that a randomly perturbed digraph, where we start with a dense digraph
Dα and add a small number of random edges to it, will typically contain a fixed
orientation of a bounded-degree spanning tree. This answers a question posed by
Araujo, Balogh, Krueger, Piga and Treglown and generalizes the corresponding result
for randomly perturbed graphs by Krivelevich, Kwan and Sudakov. More specifically,
we prove that there exists a constant c=c(α,Δ) such that if \r\nT is an oriented
tree with maximum degree Δ and Dα is an n-vertex digraph with minimum semidegree
αn, then the graph obtained by adding cn uniformly random edges to Dα will contain
T with high probability."
acknowledgement: "We thank the anonymous referees for many helpful comments on an
earlier version of this\r\narticle. Kalina Petrova was supported by grant no. CRSII5
173721 of the Swiss National\r\nScience Foundation, and by the European Union’s
Horizon 2020 research and innovation\r\nprogramme under the Marie Sk lodowska-Curie
grant agreement No. 101034413"
article_number: P2.24
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Patryk
full_name: Morawski, Patryk
last_name: Morawski
- first_name: Kalina H
full_name: Petrova, Kalina H
id: 554ff4e4-f325-11ee-b0c4-a10dbd523381
last_name: Petrova
citation:
ama: Morawski P, Petrova KH. Randomly perturbed digraphs also have bounded-degree
spanning trees. Electronic Journal of Combinatorics. 2026;33(2). doi:10.37236/13316
apa: Morawski, P., & Petrova, K. H. (2026). Randomly perturbed digraphs also
have bounded-degree spanning trees. Electronic Journal of Combinatorics.
Electronic Journal of Combinatorics. https://doi.org/10.37236/13316
chicago: Morawski, Patryk, and Kalina H Petrova. “Randomly Perturbed Digraphs Also
Have Bounded-Degree Spanning Trees.” Electronic Journal of Combinatorics.
Electronic Journal of Combinatorics, 2026. https://doi.org/10.37236/13316.
ieee: P. Morawski and K. H. Petrova, “Randomly perturbed digraphs also have bounded-degree
spanning trees,” Electronic Journal of Combinatorics, vol. 33, no. 2. Electronic
Journal of Combinatorics, 2026.
ista: Morawski P, Petrova KH. 2026. Randomly perturbed digraphs also have bounded-degree
spanning trees. Electronic Journal of Combinatorics. 33(2), P2.24.
mla: Morawski, Patryk, and Kalina H. Petrova. “Randomly Perturbed Digraphs Also
Have Bounded-Degree Spanning Trees.” Electronic Journal of Combinatorics,
vol. 33, no. 2, P2.24, Electronic Journal of Combinatorics, 2026, doi:10.37236/13316.
short: P. Morawski, K.H. Petrova, Electronic Journal of Combinatorics 33 (2026).
corr_author: '1'
date_created: 2026-05-17T22:02:11Z
date_published: 2026-05-08T00:00:00Z
date_updated: 2026-05-18T08:50:18Z
day: '08'
ddc:
- '510'
department:
- _id: MaKw
doi: 10.37236/13316
ec_funded: 1
external_id:
arxiv:
- '2306.14648'
file:
- access_level: open_access
checksum: 9e8402cb2e8870ba7ded9ae7b308201a
content_type: application/pdf
creator: dernst
date_created: 2026-05-18T08:46:26Z
date_updated: 2026-05-18T08:46:26Z
file_id: '21893'
file_name: 2026_ElectrJournCombinatorics_Morawski.pdf
file_size: 399969
relation: main_file
success: 1
file_date_updated: 2026-05-18T08:46:26Z
has_accepted_license: '1'
intvolume: ' 33'
issue: '2'
language:
- iso: eng
license: https://creativecommons.org/licenses/by-nd/4.0/
month: '05'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Electronic Journal of Combinatorics
publication_identifier:
eissn:
- 1077-8926
publication_status: published
publisher: Electronic Journal of Combinatorics
quality_controlled: '1'
scopus_import: '1'
status: public
title: Randomly perturbed digraphs also have bounded-degree spanning trees
tmp:
image: /image/cc_by_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nd/4.0/legalcode
name: Creative Commons Attribution-NoDerivatives 4.0 International (CC BY-ND 4.0)
short: CC BY-ND (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 33
year: '2026'
...
---
APC_amount: 1352,08 EUR
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21894'
abstract:
- lang: eng
text: "The Dean–Kawasaki equation—one of the most fundamental SPDEs of\r\nfluctuating
hydrodynamics—has been proposed as a model for density fluctuations in weakly
interacting particle systems. In its original form, it is highly\r\nsingular and
fails to be renormalizable, even by approaches such as regularity structures and
paracontrolled distributions, hindering mathematical approaches to its rigorous
justification. It has been understood recently that it is\r\nnatural to introduce
a suitable regularization, for example, by applying a formal spatial discretization
or by truncating high-frequency noise: This yields\r\nwell-posed equations that
should still precisely approximate the law of the\r\nparticle density fluctuations.\r\nIn
the present work, we prove that a regularization in the form of a formal\r\ndiscretization
of the Dean–Kawasaki equation indeed accurately describes\r\ndensity fluctuations
in systems of weakly interacting diffusing particles: We\r\nshow that, in suitable
weak metrics, the law of fluctuations as predicted by\r\nthe discretized Dean–Kawasaki
SPDE approximates the law of fluctuations\r\nof the original particle system,
up to an error that is of arbitrarily high order in\r\nthe inverse particle number
and a discretization error. In particular, the Dean–\r\nKawasaki equation provides
a means for efficient and accurate simulations of\r\ndensity fluctuations in weakly
interacting particle systems."
acknowledgement: All authors gratefully acknowledge funding from the Austrian Science
Fund (FWF) through the project F65. CR gratefully acknowledges support from the
Austrian Science Fund (FWF), grants P30000, P33010, W1245. FC gratefully acknowledges
funding from the European Union’s Horizon 2020 research and innovation programme
under the Marie Skłodowska-Curie grant agreement No. 754411.
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Federico
full_name: Cornalba, Federico
last_name: Cornalba
- first_name: Julian L
full_name: Fischer, Julian L
id: 2C12A0B0-F248-11E8-B48F-1D18A9856A87
last_name: Fischer
orcid: 0000-0002-0479-558X
- first_name: Jonas
full_name: Ingmanns, Jonas
id: 71523d30-15b2-11ec-abd3-f80aa909d6b0
last_name: Ingmanns
orcid: 0009-0008-1310-7946
- first_name: Claudia
full_name: Raithel, Claudia
last_name: Raithel
citation:
ama: Cornalba F, Fischer JL, Ingmanns J, Raithel C. Density fluctuations in weakly
interacting particle systems via the Dean–Kawasaki equation. The Annals of
Probability. 2026;54(1):155-215. doi:10.1214/25-aop1763
apa: Cornalba, F., Fischer, J. L., Ingmanns, J., & Raithel, C. (2026). Density
fluctuations in weakly interacting particle systems via the Dean–Kawasaki equation.
The Annals of Probability. Institute of Mathematical Statistics. https://doi.org/10.1214/25-aop1763
chicago: Cornalba, Federico, Julian L Fischer, Jonas Ingmanns, and Claudia Raithel.
“Density Fluctuations in Weakly Interacting Particle Systems via the Dean–Kawasaki
Equation.” The Annals of Probability. Institute of Mathematical Statistics,
2026. https://doi.org/10.1214/25-aop1763.
ieee: F. Cornalba, J. L. Fischer, J. Ingmanns, and C. Raithel, “Density fluctuations
in weakly interacting particle systems via the Dean–Kawasaki equation,” The
Annals of Probability, vol. 54, no. 1. Institute of Mathematical Statistics,
pp. 155–215, 2026.
ista: Cornalba F, Fischer JL, Ingmanns J, Raithel C. 2026. Density fluctuations
in weakly interacting particle systems via the Dean–Kawasaki equation. The Annals
of Probability. 54(1), 155–215.
mla: Cornalba, Federico, et al. “Density Fluctuations in Weakly Interacting Particle
Systems via the Dean–Kawasaki Equation.” The Annals of Probability, vol.
54, no. 1, Institute of Mathematical Statistics, 2026, pp. 155–215, doi:10.1214/25-aop1763.
short: F. Cornalba, J.L. Fischer, J. Ingmanns, C. Raithel, The Annals of Probability
54 (2026) 155–215.
corr_author: '1'
date_created: 2026-05-20T08:25:25Z
date_published: 2026-01-01T00:00:00Z
date_updated: 2026-05-21T07:21:25Z
day: '01'
ddc:
- '510'
department:
- _id: JuFi
doi: 10.1214/25-aop1763
ec_funded: 1
external_id:
arxiv:
- '2303.00429'
file:
- access_level: open_access
checksum: 3e60c0e25a1c96342029a7d2b031505f
content_type: application/pdf
creator: dernst
date_created: 2026-05-21T07:11:27Z
date_updated: 2026-05-21T07:11:27Z
file_id: '21906'
file_name: 2026_AnnalsProbability_Cornalba.pdf
file_size: 865745
relation: main_file
success: 1
file_date_updated: 2026-05-21T07:11:27Z
has_accepted_license: '1'
intvolume: ' 54'
issue: '1'
keyword:
- Weakly interacting particle systems
- fluctuating hydrodynamics
- Dean-Kawasaki equation
- stochastic PDEs
- numerical approximation
language:
- iso: eng
month: '01'
oa: 1
oa_version: Published Version
page: 155-215
project:
- _id: 260C2330-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '754411'
name: ISTplus - Postdoctoral Fellowships
- _id: fc31cba2-9c52-11eb-aca3-ff467d239cd2
grant_number: F6504
name: Taming Complexity in Partial Differential Systems
publication: The Annals of Probability
publication_identifier:
eissn:
- 2168-894X
issn:
- 0091-1798
publication_status: published
publisher: Institute of Mathematical Statistics
quality_controlled: '1'
scopus_import: '1'
status: public
title: Density fluctuations in weakly interacting particle systems via the Dean–Kawasaki
equation
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: 54
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21895'
abstract:
- lang: eng
text: The mammalian brain organises knowledge about entities in the world and relationships
between them using cognitive maps. When forming a cognitive map, there is a necessary
trade-off between extending the map to make novel inferences, and storing a veridical
copy of past experience. However, the neural mechanisms that control this trade-off
remain unknown. Using a cross-scale approach that combines a pharmacological intervention
in humans with neural network modelling, we show that the neuromodulator noradrenaline
elicits a significant ‘spread of association’ across hippocampal cognitive maps.
This neural spread of association can be explained by changes in synaptic plasticity
that predict overgeneralisation in behaviour. Thus, elevated noradrenaline during
learning increases the ‘smoothing kernel’ for plasticity across the cognitive
map, allowing disparate memories to become linked and distorted.
acknowledgement: 'We would like to thank Chamith Halahakoon, Phil Cowen, Angharad
De Cates, Beata Godlewska, Riccardo De Giorgi, Katherine Smith and Edoardo Ostinelli
for enabling this study by providing medical cover. We would like to thank Douglas
F. Tomé and Everton J. Agnes for their guidance and advice with earlier versions
of the neural network model. We would like to thank Rob Froemke for helpful discussion
when preparing the experiments. We thank Leonie Glitz and Valentina Mancini for
comments on an earlier version of the manuscript. R.S.K. was supported by an EPSRC/MRC-funded
studentship (EP/L016052/1). P.P. was supported by the Cambridge Trust, Trinity Henry
Barlow Scholarship and Trinity Hall Brockhouse Scholarship. L.C. is supported by
the Foundation for Science and Technology (FCT) (Portuguese State Budget: UID/PSI/01662/2020;
Research fellowship: 2021.00415.CEECIND). W.T.C. is funded by the Wellcome Trust
[225924/Z/22/Z]. H.C.B. is supported by a UKRI Future Leaders Fellowship (MR/W008939/1)
and the Wellcome Institutional Strategic Support Fund. H.C.B. and J.X.O. are supported
by the Medical Research Council (MR/W01971X/1). The study was supported by the NIHR
Oxford Health Biomedical Research Centre (NIHR203316). The views expressed are those
of the author(s) and not necessarily those of the NIHR or the Department of Health
and Social Care. The Wellcome Centre for Integrative Neuroimaging is supported by
core funding from the Wellcome Trust (203139/Z/16/Z and 203139/A/16/Z). This research
was funded in part by the Wellcome Trust. For the purpose of open access, the author(s)
have applied a CC BY public copyright license to any Author Accepted Manuscript
version arising from this submission.'
article_number: '3961'
article_processing_charge: Yes
article_type: original
author:
- first_name: Renée S.
full_name: Koolschijn, Renée S.
last_name: Koolschijn
- first_name: Prakriti
full_name: Parthasarathy, Prakriti
last_name: Parthasarathy
- first_name: Michael
full_name: Browning, Michael
last_name: Browning
- first_name: Xenia
full_name: Przygodda, Xenia
last_name: Przygodda
- first_name: Liliana P.
full_name: Capitão, Liliana P.
last_name: Capitão
- first_name: William T.
full_name: Clarke, William T.
last_name: Clarke
- first_name: Tim P
full_name: Vogels, Tim P
id: CB6FF8D2-008F-11EA-8E08-2637E6697425
last_name: Vogels
orcid: 0000-0003-3295-6181
- first_name: Jill X.
full_name: O’Reilly, Jill X.
last_name: O’Reilly
- first_name: Helen C.
full_name: Barron, Helen C.
last_name: Barron
citation:
ama: Koolschijn RS, Parthasarathy P, Browning M, et al. Noradrenaline causes a spread
of association in the hippocampal cognitive map. Nature Communications.
2026;17. doi:10.1038/s41467-026-70659-x
apa: Koolschijn, R. S., Parthasarathy, P., Browning, M., Przygodda, X., Capitão,
L. P., Clarke, W. T., … Barron, H. C. (2026). Noradrenaline causes a spread of
association in the hippocampal cognitive map. Nature Communications. Springer
Nature. https://doi.org/10.1038/s41467-026-70659-x
chicago: Koolschijn, Renée S., Prakriti Parthasarathy, Michael Browning, Xenia Przygodda,
Liliana P. Capitão, William T. Clarke, Tim P Vogels, Jill X. O’Reilly, and Helen
C. Barron. “Noradrenaline Causes a Spread of Association in the Hippocampal Cognitive
Map.” Nature Communications. Springer Nature, 2026. https://doi.org/10.1038/s41467-026-70659-x.
ieee: R. S. Koolschijn et al., “Noradrenaline causes a spread of association
in the hippocampal cognitive map,” Nature Communications, vol. 17. Springer
Nature, 2026.
ista: Koolschijn RS, Parthasarathy P, Browning M, Przygodda X, Capitão LP, Clarke
WT, Vogels TP, O’Reilly JX, Barron HC. 2026. Noradrenaline causes a spread of
association in the hippocampal cognitive map. Nature Communications. 17, 3961.
mla: Koolschijn, Renée S., et al. “Noradrenaline Causes a Spread of Association
in the Hippocampal Cognitive Map.” Nature Communications, vol. 17, 3961,
Springer Nature, 2026, doi:10.1038/s41467-026-70659-x.
short: R.S. Koolschijn, P. Parthasarathy, M. Browning, X. Przygodda, L.P. Capitão,
W.T. Clarke, T.P. Vogels, J.X. O’Reilly, H.C. Barron, Nature Communications 17
(2026).
date_created: 2026-05-20T14:30:37Z
date_published: 2026-05-01T00:00:00Z
date_updated: 2026-05-21T07:05:01Z
day: '01'
ddc:
- '570'
department:
- _id: TiVo
doi: 10.1038/s41467-026-70659-x
external_id:
pmid:
- '41832186'
file:
- access_level: open_access
checksum: 1b529e06b1c5d6e085d60743317fd4f9
content_type: application/pdf
creator: dernst
date_created: 2026-05-21T07:01:35Z
date_updated: 2026-05-21T07:01:35Z
file_id: '21905'
file_name: 2026_NatureComm_Koolschijn.pdf
file_size: 2059139
relation: main_file
success: 1
file_date_updated: 2026-05-21T07:01:35Z
has_accepted_license: '1'
intvolume: ' 17'
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
pmid: 1
publication: Nature Communications
publication_identifier:
eissn:
- 2041-1723
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Noradrenaline causes a spread of association in the hippocampal cognitive map
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 17
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21897'
abstract:
- lang: eng
text: Ultracompact binary systems, consisting of two compact objects in an orbit
$\lesssim 0.5 {\rm R}_\odot$, should exhibit measurable rates of orbital period
change ($\dot{P} \ne 0$) due to the emission of gravitational waves (GWs). Measurements
of $\dot{P}$ have so far been limited to the shortest-period ultracompact binaries
($\lesssim 20$ min). Among the AM CVn-type subclass, several works have proposed
the presence of extra angular momentum loss beyond GW emission, with magnetic
braking being a widely discussed mechanism. If present, this magnetic braking
would dominate the angular momentum loss of AM CVn-type binaries with orbital
periods $\gtrsim 30$ min. In this work, we present a long-term eclipse timing
study of two AM CVn-type binaries, YZ LMi and Gaia14aae, with respective orbital
periods of 28.3 min and 49.7 min and continuous observations since 2006 and 2015.
Both systems show $\dot{P}$ consistent with zero within $2\sigma$. Their $3\sigma$
upper limits are $1.1 \times 10^{-13}\, {\rm s \, s}^{-1}$ and $9.7 \times 10^{-14}\,
{\rm s \, s}^{-1}$, respectively. These non-detections are most simply explained
by a scenario in which secular angular momentum loss is not substantially stronger
than GW emission at all orbital periods, but is combined with deviations from
the secular $\dot{P}$ whose time-scales span decades but whose amplitude is $\lesssim
10^{-13}\, {\rm s \, s}^{-1}$. Our non-detections of $\dot{P}$ represent a limit
on the strength of any enhanced angular momentum loss beyond pure GW emission.
acknowledgement: "We are grateful to the anonymousreferee fortheirinsightful comments.
MJG thanks Mitch Begelman and the JILA department at the University of Colorado,
Boulder, for providing office space at which much of this paper was written. This
work is supported in part by the United States National Aeronautics and Space Administration
(NASA) under grants\r\n80NSSC24K0436, 80NSSC22K0479, and 80NSSC24K0380, and the
United States National Science Foundation (NSF) under grant AST-2508429. VSD and
HiPERCAM are funded by the Science and Technology Facilities Council (grant ST/Z000033/1).
IP acknowledges support from the Royal Society through a University Research Fellowship
(URF\\R1\\231496). This project has received funding from the European Research
Council under the European Union’s Horizon 2020 research and innovation programme
(grant agreement numbers 101002408 – MOS100PC). CMC receives funding from United
Kingdom Research and Innovation grant numbers ST/X005933/1 and ST/W001934/1. This
article is based in part on observations made in the Observatorios de Canarias del
Instituto de Astrofísica de Canarias (IAC) with the the William Herschel Telescope
(WHT) operated on the island of La Palma by the Isaac Newton Group (ING) in the
Observatorio del Roque de los Muchachos. It is also based in part on observations
made with the Gran Telescopio Canarias (GTC) under proposal ID GTC18-24A, installed
at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica
de Canarias, in the island of La Palma. Further data were obtained using the 2.4
m Thai National Telescope (TNT) operated by the National Astronomy Research Institute
of Thailand\r\n(NARIT), and the 200-inch Hale Telescope at Palomar Observatory operated
by the California Institute of Technology. Software packages used in this work include
the ultracam and hipercam reduction pipelines, lcurve (C. M. Copperwheat et al.
2010), numpy, astropy, matplotlib, and emcee (D. Foreman-Mackey et al. 2013)."
article_number: stag673
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Matthew J
full_name: Green, Matthew J
last_name: Green
- first_name: Thomas R
full_name: Marsh, Thomas R
last_name: Marsh
- first_name: Joannes C
full_name: van Roestel, Joannes C
id: 4d122fc8-6083-11f0-87a5-97d68b860333
last_name: van Roestel
- first_name: Tin Long Sunny
full_name: Wong, Tin Long Sunny
last_name: Wong
- first_name: Diogo
full_name: Belloni, Diogo
last_name: Belloni
- first_name: Mukremin
full_name: Kilic, Mukremin
last_name: Kilic
- first_name: Elmé
full_name: Breedt, Elmé
last_name: Breedt
- first_name: Alex
full_name: Brown, Alex
last_name: Brown
- first_name: Chris M
full_name: Copperwheat, Chris M
last_name: Copperwheat
- first_name: Anurak
full_name: Chakpor, Anurak
last_name: Chakpor
- first_name: V S
full_name: Dhillon, V S
last_name: Dhillon
- first_name: Noel Castro
full_name: Segura, Noel Castro
last_name: Segura
- first_name: Martin J
full_name: Dyer, Martin J
last_name: Dyer
- first_name: James
full_name: Garbutt, James
last_name: Garbutt
- first_name: Dan
full_name: Jarvis, Dan
last_name: Jarvis
- first_name: Vasu
full_name: Kengkriangkrai, Vasu
last_name: Kengkriangkrai
- first_name: Mark R
full_name: Kennedy, Mark R
last_name: Kennedy
- first_name: Paul
full_name: Kerry, Paul
last_name: Kerry
- first_name: Thomas
full_name: Kupfer, Thomas
last_name: Kupfer
- first_name: S P
full_name: Littlefair, S P
last_name: Littlefair
- first_name: James
full_name: McCormac, James
last_name: McCormac
- first_name: James
full_name: Munday, James
last_name: Munday
- first_name: Steven G
full_name: Parsons, Steven G
last_name: Parsons
- first_name: Eleanor
full_name: Pike, Eleanor
last_name: Pike
- first_name: Ingrid
full_name: Pelisoli, Ingrid
last_name: Pelisoli
- first_name: Pablo
full_name: Rodríguez-Gil, Pablo
last_name: Rodríguez-Gil
- first_name: David I
full_name: Sahman, David I
last_name: Sahman
- first_name: Amalie
full_name: Yates, Amalie
last_name: Yates
citation:
ama: Green MJ, Marsh TR, van Roestel JC, et al. No period change in two long-period
AM CVn binaries. Monthly Notices of the Royal Astronomical Society. 2026;548(3).
doi:10.1093/mnras/stag673
apa: Green, M. J., Marsh, T. R., van Roestel, J. C., Wong, T. L. S., Belloni, D.,
Kilic, M., … Yates, A. (2026). No period change in two long-period AM CVn binaries.
Monthly Notices of the Royal Astronomical Society. Oxford University Press.
https://doi.org/10.1093/mnras/stag673
chicago: Green, Matthew J, Thomas R Marsh, Joannes C van Roestel, Tin Long Sunny
Wong, Diogo Belloni, Mukremin Kilic, Elmé Breedt, et al. “No Period Change in
Two Long-Period AM CVn Binaries.” Monthly Notices of the Royal Astronomical
Society. Oxford University Press, 2026. https://doi.org/10.1093/mnras/stag673.
ieee: M. J. Green et al., “No period change in two long-period AM CVn binaries,”
Monthly Notices of the Royal Astronomical Society, vol. 548, no. 3. Oxford
University Press, 2026.
ista: Green MJ, Marsh TR, van Roestel JC, Wong TLS, Belloni D, Kilic M, Breedt E,
Brown A, Copperwheat CM, Chakpor A, Dhillon VS, Segura NC, Dyer MJ, Garbutt J,
Jarvis D, Kengkriangkrai V, Kennedy MR, Kerry P, Kupfer T, Littlefair SP, McCormac
J, Munday J, Parsons SG, Pike E, Pelisoli I, Rodríguez-Gil P, Sahman DI, Yates
A. 2026. No period change in two long-period AM CVn binaries. Monthly Notices
of the Royal Astronomical Society. 548(3), stag673.
mla: Green, Matthew J., et al. “No Period Change in Two Long-Period AM CVn Binaries.”
Monthly Notices of the Royal Astronomical Society, vol. 548, no. 3, stag673,
Oxford University Press, 2026, doi:10.1093/mnras/stag673.
short: M.J. Green, T.R. Marsh, J.C. van Roestel, T.L.S. Wong, D. Belloni, M. Kilic,
E. Breedt, A. Brown, C.M. Copperwheat, A. Chakpor, V.S. Dhillon, N.C. Segura,
M.J. Dyer, J. Garbutt, D. Jarvis, V. Kengkriangkrai, M.R. Kennedy, P. Kerry, T.
Kupfer, S.P. Littlefair, J. McCormac, J. Munday, S.G. Parsons, E. Pike, I. Pelisoli,
P. Rodríguez-Gil, D.I. Sahman, A. Yates, Monthly Notices of the Royal Astronomical
Society 548 (2026).
date_created: 2026-05-20T14:34:03Z
date_published: 2026-04-09T00:00:00Z
date_updated: 2026-05-21T06:41:41Z
day: '09'
ddc:
- '520'
department:
- _id: IlCa
doi: 10.1093/mnras/stag673
external_id:
arxiv:
- '2604.06460'
file:
- access_level: open_access
checksum: 2c4463926c5cb84ce555ef2005b52ddd
content_type: application/pdf
creator: dernst
date_created: 2026-05-21T06:37:42Z
date_updated: 2026-05-21T06:37:42Z
file_id: '21903'
file_name: 2026_MNRAS_Green.pdf
file_size: 3960296
relation: main_file
success: 1
file_date_updated: 2026-05-21T06:37:42Z
has_accepted_license: '1'
intvolume: ' 548'
issue: '3'
keyword:
- 'binaries: close – stars'
- dwarf novae – novae
- cataclysmic variables – white dwarfs
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: No period change in two long-period AM CVn binaries
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: 548
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21898'
abstract:
- lang: eng
text: We investigate the nature and spectroscopic diversity of early galaxies from
a sample of 41 sources at $z\geqslant 10$ with James Webb Space Telescope (JWST)/NIRSpec
prism observations. We compare the properties of strong ultraviolet (UV) line
emitters, traced by intense C iv emission, with those of more ‘typical’ sources
with weak or undetected C iv. The more typical (or ‘C iv-weak’) sources reveal
significant scatter in their C iii] line strengths, UV continuum slopes, and physical
sizes, spanning C iii] equivalent widths (EWs) of $\sim$1–51 Å, UV slopes of $\beta
\sim -1.6$ to $-2.6$, and half-light radii of $\sim$50–1000 pc. In contrast, C iv-strong
sources occupy the tail of these distributions, with C iii] EWs of 16–51 Å, UV
slopes $\beta \lesssim -2.5$, compact morphologies ($r_{\rm 50} \lesssim 100$ pc),
and elevated star formation surface densities ($\Sigma _{\rm SFR} \gtrsim 100\,
M_\odot \, \mathrm{yr}^{-1}\, \mathrm{kpc}^{-2}$). These properties suggest concentrated
starbursts that temporarily outshine the host galaxy. Comparing average properties
from composite spectra, we find the diversity of the sample is primarily driven
by bursty star formation on very short time-scales ($\le$3 Myr), with strong C iv
emitters observed at the apex of the bursts and sources devoid of emission lines
during relative inactivity. An apparent association between strong C iv and enhanced
nitrogen abundance suggests both may be modulated by the same duty cycle, reflecting
a generic mode of star formation. We show that active galactic nuclei are unlikely
to contribute significantly to this duty cycle based on UV line diagnostics and
photoionization models. Our results support a picture whereby brief bursts and
lulls can explain the spectral diversity and early growth of bright galaxies in
the first 500 Myr.
acknowledgement: "We thank the anonymous referee for useful and constructive\r\nfeedback
that improved the manuscript. GRB is grateful to Vasily\r\nBelokurov and Sarah Kane
for providing the relevant abundances\r\nforthe Aurora data in Fig. 11, as well
asto Tiger Yu-Yang Hsiao for\r\nhelpful discussions regarding the MACS 0647-JD source.
We are\r\nalso grateful to Gabe Brammerfor useful discussions and his continuous
efforts in maintaining and improving the msaexp code,\r\nfrom which the high-z community
continues to benefit greatly.\r\nLastly, we also thank the numerous teams of the
observational\r\nprograms used in this study, for developing these valuable data\r\nsets.
The data used in this study are derived from the following\r\nprograms: 1181 (PI
Eisenstein; D. J. Eisenstein et al. 2023a), 1210\r\n(PI Luetzgendorf; D. J. Eisenstein
et al. 2023a), 1211 (PI Isaak;\r\nM. V. Maseda et al. 2024), 1286 (PI Luetzgendorf;
D. J. Eisenstein\r\net al. 2023a), 1287 (PI Isaak; D. J. Eisenstein et al. 2023a),
1345\r\n(PI Finkelstein; S. L. Finkelstein et al. 2025), 1433 (PI Coe; T. Y.-\r\nY.
Hsiao et al. 2024a), 2561 (PI Labbé; R. Bezanson et al. 2022),\r\n2750 (PI Arrabal
Haro; P. Arrabal Haro et al. 2023b), 3073 (PI\r\nCastellano; M. Castellano et al.
2024), 3215 (PIs Eisenstein &\r\nMaiolino; D. J. Eisenstein et al. 2023b), 5224
(PIs Oesch & Naidu;\r\nOesch et al. in preparation), 6368 (PI Dickinson; V. Kokorev
et al.\r\n2025). The authors acknowledge the aforementioned teams and\r\nPIs where
development of their observing program(s) was done\r\nwith a zero-exclusive-access
period.\r\nThis work is based on observations made with the\r\nNASA/ESA/CSA JWST.
The data were obtained from the\r\nMikulski Archive for Space Telescopes at the
Space Telescope\r\nScience Institute, which is operated by the Association of\r\nUniversities
for Research in Astronomy, Inc., under NASA\r\ncontract NAS 5-03127 for JWST. The
specific observations\r\nanalysed can be accessed via DOI 10.17909/jqj3-ws37. Some\r\nof
the data products presented herein were retrieved from the\r\nDawn JWST Archive
(DJA). DJA is an initiative of the Cosmic\r\nDawn Center (DAWN), which is funded
by the Danish National\r\nResearch Foundation under grant DNRF140.\r\nRSE acknowledges
generous financial support from the Peter\r\nand Patricia Gruber Foundation. YF
acknowledgessupportsfrom\r\nJSPS KAKENHI Grant Numbers JP22K21349 and JP23K13149.\r\nThis
work has received funding from the Swiss State Secretariat\r\nfor Education, Research
and Innovation (SERI) under contract\r\nnumber MB22.00072, as well as from the Swiss
National Science\r\nFoundation (SNSF) through project grant 200020_207349."
article_number: stag701
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Guido
full_name: Roberts-Borsani, Guido
last_name: Roberts-Borsani
- first_name: Pascal A
full_name: Oesch, Pascal A
last_name: Oesch
- first_name: Richard
full_name: Ellis, Richard
last_name: Ellis
- first_name: Andrea
full_name: Weibel, Andrea
last_name: Weibel
- first_name: Emma
full_name: Giovinazzo, Emma
last_name: Giovinazzo
- first_name: Rychard
full_name: Bouwens, Rychard
last_name: Bouwens
- first_name: Pratika
full_name: Dayal, Pratika
last_name: Dayal
- first_name: Adriano
full_name: Fontana, Adriano
last_name: Fontana
- first_name: Kasper E
full_name: Heintz, Kasper E
last_name: Heintz
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Romain A
full_name: Meyer, Romain A
last_name: Meyer
- first_name: Laura
full_name: Pentericci, Laura
last_name: Pentericci
- first_name: Alice
full_name: Shapley, Alice
last_name: Shapley
- first_name: Sandro
full_name: Tacchella, Sandro
last_name: Tacchella
- first_name: Tommaso
full_name: Treu, Tommaso
last_name: Treu
- first_name: Fabian
full_name: Walter, Fabian
last_name: Walter
- first_name: Hakim
full_name: Atek, Hakim
last_name: Atek
- first_name: Sownak
full_name: Bose, Sownak
last_name: Bose
- first_name: Marco
full_name: Castellano, Marco
last_name: Castellano
- first_name: Yoshinobu
full_name: Fudamoto, Yoshinobu
last_name: Fudamoto
- first_name: Takahiro
full_name: Morishita, Takahiro
last_name: Morishita
- first_name: Rohan P
full_name: Naidu, Rohan P
last_name: Naidu
- first_name: Ryan L
full_name: Sanders, Ryan L
last_name: Sanders
- first_name: Arjen
full_name: van der Wel, Arjen
last_name: van der Wel
citation:
ama: 'Roberts-Borsani G, Oesch PA, Ellis R, et al. JWST spectroscopic insights into
the diversity of galaxies in the first 500 Myr: Short-lived snapshots along a
common evolutionary pathway. Monthly Notices of the Royal Astronomical Society.
2026;548(3). doi:10.1093/mnras/stag701'
apa: 'Roberts-Borsani, G., Oesch, P. A., Ellis, R., Weibel, A., Giovinazzo, E.,
Bouwens, R., … van der Wel, A. (2026). JWST spectroscopic insights into the diversity
of galaxies in the first 500 Myr: Short-lived snapshots along a common evolutionary
pathway. Monthly Notices of the Royal Astronomical Society. Oxford University
Press. https://doi.org/10.1093/mnras/stag701'
chicago: 'Roberts-Borsani, Guido, Pascal A Oesch, Richard Ellis, Andrea Weibel,
Emma Giovinazzo, Rychard Bouwens, Pratika Dayal, et al. “JWST Spectroscopic Insights
into the Diversity of Galaxies in the First 500 Myr: Short-Lived Snapshots along
a Common Evolutionary Pathway.” Monthly Notices of the Royal Astronomical Society.
Oxford University Press, 2026. https://doi.org/10.1093/mnras/stag701.'
ieee: 'G. Roberts-Borsani et al., “JWST spectroscopic insights into the diversity
of galaxies in the first 500 Myr: Short-lived snapshots along a common evolutionary
pathway,” Monthly Notices of the Royal Astronomical Society, vol. 548,
no. 3. Oxford University Press, 2026.'
ista: 'Roberts-Borsani G, Oesch PA, Ellis R, Weibel A, Giovinazzo E, Bouwens R,
Dayal P, Fontana A, Heintz KE, Matthee JJ, Meyer RA, Pentericci L, Shapley A,
Tacchella S, Treu T, Walter F, Atek H, Bose S, Castellano M, Fudamoto Y, Morishita
T, Naidu RP, Sanders RL, van der Wel A. 2026. JWST spectroscopic insights into
the diversity of galaxies in the first 500 Myr: Short-lived snapshots along a
common evolutionary pathway. Monthly Notices of the Royal Astronomical Society.
548(3), stag701.'
mla: 'Roberts-Borsani, Guido, et al. “JWST Spectroscopic Insights into the Diversity
of Galaxies in the First 500 Myr: Short-Lived Snapshots along a Common Evolutionary
Pathway.” Monthly Notices of the Royal Astronomical Society, vol. 548,
no. 3, stag701, Oxford University Press, 2026, doi:10.1093/mnras/stag701.'
short: G. Roberts-Borsani, P.A. Oesch, R. Ellis, A. Weibel, E. Giovinazzo, R. Bouwens,
P. Dayal, A. Fontana, K.E. Heintz, J.J. Matthee, R.A. Meyer, L. Pentericci, A.
Shapley, S. Tacchella, T. Treu, F. Walter, H. Atek, S. Bose, M. Castellano, Y.
Fudamoto, T. Morishita, R.P. Naidu, R.L. Sanders, A. van der Wel, Monthly Notices
of the Royal Astronomical Society 548 (2026).
date_created: 2026-05-20T14:34:29Z
date_published: 2026-05-01T00:00:00Z
date_updated: 2026-05-21T06:16:04Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1093/mnras/stag701
external_id:
arxiv:
- '2508.21708'
file:
- access_level: open_access
checksum: b8f52c6fc5e06b3a505310e7d5898ecf
content_type: application/pdf
creator: dernst
date_created: 2026-05-21T06:14:23Z
date_updated: 2026-05-21T06:14:23Z
file_id: '21902'
file_name: 2026_MNRAS_RobertsBorsani.pdf
file_size: 3539140
relation: main_file
success: 1
file_date_updated: 2026-05-21T06:14:23Z
has_accepted_license: '1'
intvolume: ' 548'
issue: '3'
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'JWST spectroscopic insights into the diversity of galaxies in the first 500
Myr: Short-lived snapshots along a common evolutionary pathway'
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: 548
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '21899'
abstract:
- lang: eng
text: Cell extrusion is an essential mechanism for controlling cell density in epithelial
tissues. Another essential element of epithelia is curvature, which is required
to achieve complex shapes, like in the lung or intestine. Here, we introduce a
three-dimensional bubbly vertex model to study the interplay between extrusion
and curvature. We find a generic cellular bulging instability at topological defects,
which is much stronger than for standard vertex models. Analyzing cell shapes
in three-dimensional imaging data of spherical mouse colon organoids, we infer
that pentagonal cells have an increased basal interfacial tension, suggesting
that cells at topological defects react to the different force conditions. Using
the bubbly vertex model, we show that such basal tensions stabilize against the
predicted instability and result in better cell shape control than tissue-scale
mechanisms such as lumen pressure and spontaneous curvature. Our theory suggests
that epithelial curvature naturally leads to bulged and extrusionlike cell shapes
because the interfacial curvature of individual cells at the defects strongly
amplifies buckling effected by tissue-scale topological defects in elastic sheets.
Our results highlight the complex interplay of forces across scales in three-dimensional
tissue organization.
acknowledgement: O. M. D., M. B., and U.S. S. acknowledge support from the Max Planck
School Matter to Life, with funding by the German Federal Ministry of Education
and Research (BMBF), the Dieter Schwarz Foundation, and the Max Planck Society.
M. B. and U.S. S. acknowledge support from the cluster of excellence 3DMM2O (EXC
2082/1-390761711 and EXC 2082/2-390761711) funded by the Deutsche Forschungsgemeinschaft
(DFG, German Research Foundation). The authors acknowledge the data storage service
SDS@hd supported by the Ministry of Science, Research and the Arts Baden-Württemberg
(MWK) and the DFG through Grant No. INST 35/1503-1 FUGG. For the publication fee
we acknowledge financial support by Heidelberg University. O. M. D. thanks Edouard
Hannezo for valuable discussions. U.S. S. is a member of the Interdisciplinary Center
for Scientific Computing (IWR) at Heidelberg.
article_number: '021023'
article_processing_charge: Yes
article_type: original
author:
- first_name: Oliver M
full_name: Drozdowski, Oliver M
id: cd4ed792-b872-11ef-bb90-b7b3a3f62f75
last_name: Drozdowski
- first_name: Büşra
full_name: "Kocameşe-Tamgac\U0001D6A4, Büşra"
last_name: "Kocameşe-Tamgac\U0001D6A4"
- first_name: Kim E.
full_name: Boonekamp, Kim E.
last_name: Boonekamp
- first_name: Michael
full_name: Boutros, Michael
last_name: Boutros
- first_name: Ulrich S.
full_name: Schwarz, Ulrich S.
last_name: Schwarz
citation:
ama: "Drozdowski OM, Kocameşe-Tamgac\U0001D6A4 B, Boonekamp KE, Boutros M, Schwarz
US. Cell bulging and extrusion in a three-dimensional bubbly vertex model for
curved epithelial sheets. Physical Review X. 2026;16(2). doi:10.1103/x82g-cq7n"
apa: "Drozdowski, O. M., Kocameşe-Tamgac\U0001D6A4, B., Boonekamp, K. E., Boutros,
M., & Schwarz, U. S. (2026). Cell bulging and extrusion in a three-dimensional
bubbly vertex model for curved epithelial sheets. Physical Review X. American
Physical Society. https://doi.org/10.1103/x82g-cq7n"
chicago: "Drozdowski, Oliver M, Büşra Kocameşe-Tamgac\U0001D6A4, Kim E. Boonekamp,
Michael Boutros, and Ulrich S. Schwarz. “Cell Bulging and Extrusion in a Three-Dimensional
Bubbly Vertex Model for Curved Epithelial Sheets.” Physical Review X. American
Physical Society, 2026. https://doi.org/10.1103/x82g-cq7n."
ieee: "O. M. Drozdowski, B. Kocameşe-Tamgac\U0001D6A4, K. E. Boonekamp, M. Boutros,
and U. S. Schwarz, “Cell bulging and extrusion in a three-dimensional bubbly vertex
model for curved epithelial sheets,” Physical Review X, vol. 16, no. 2.
American Physical Society, 2026."
ista: "Drozdowski OM, Kocameşe-Tamgac\U0001D6A4 B, Boonekamp KE, Boutros M, Schwarz
US. 2026. Cell bulging and extrusion in a three-dimensional bubbly vertex model
for curved epithelial sheets. Physical Review X. 16(2), 021023."
mla: Drozdowski, Oliver M., et al. “Cell Bulging and Extrusion in a Three-Dimensional
Bubbly Vertex Model for Curved Epithelial Sheets.” Physical Review X, vol.
16, no. 2, 021023, American Physical Society, 2026, doi:10.1103/x82g-cq7n.
short: "O.M. Drozdowski, B. Kocameşe-Tamgac\U0001D6A4, K.E. Boonekamp, M. Boutros,
U.S. Schwarz, Physical Review X 16 (2026)."
date_created: 2026-05-20T14:35:57Z
date_published: 2026-04-30T00:00:00Z
date_updated: 2026-05-21T06:08:11Z
day: '30'
ddc:
- '530'
department:
- _id: EdHa
doi: 10.1103/x82g-cq7n
file:
- access_level: open_access
checksum: a90e905968648ac4425c256de901e9c3
content_type: application/pdf
creator: dernst
date_created: 2026-05-21T06:05:49Z
date_updated: 2026-05-21T06:05:49Z
file_id: '21901'
file_name: 2026_PhysicalReviewX_Drozdowski.pdf
file_size: 5603164
relation: main_file
success: 1
file_date_updated: 2026-05-21T06:05:49Z
has_accepted_license: '1'
intvolume: ' 16'
issue: '2'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
publication: Physical Review X
publication_identifier:
issn:
- 2160-3308
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Cell bulging and extrusion in a three-dimensional bubbly vertex model for curved
epithelial sheets
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: 16
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21914'
abstract:
- lang: eng
text: 'Cyclic adenosine monophosphate (cAMP) is a fundamental second messenger involved
in diverse signaling pathways across both animals and plants. While the role of
3′,5′-cAMP has been extensively characterized, the biological significance of
its structural isomer, 2′,3′-cAMP, remains largely unexplored, particularly in
plants. Here, we show that 2′,3′-cAMP and 3′,5′-cAMP represent parallel signaling
systems in Arabidopsis thaliana, with different enzymatic origins and largely
distinct downstream effects. In vitro enzymatic assays show that plant adenylate
cyclases (ACs), including AFB5 and HpAC1, produce specifically 3′,5′-cAMP from
ATP, whereas the TIR domain of protein L7 also catalyzes the formation of 2′,3′-cAMP
from RNA. Comprehensive multiomics analyses reveal that two isomers elicit distinct
yet partially overlapping metabolic, proteomic, and transcriptional response:
2′,3′-cAMP activates broad, stress-adaptive gene expression reprogramming, while
3′,5′-cAMP fine-tunes responses related to nutrient status and cellular homeostasis.
Our findings establish the existence of dual cAMP signaling systems in plants,
each with specialized functions and provide insights into the complex regulatory
networks governing plant physiology.'
acknowledged_ssus:
- _id: MassSpec
- _id: LifeSc
acknowledgement: " We thank J. Chai and D. Yu for providing the MBP-fused L7TIR plasmid
and K. Jaworski (Nicolaus Copernicus University) for the GST-HpAC1 plasmid. We
also thank M. Randuch and L. Fiedler for providing vectors for recombinant AFB5
and ADCY. We are also grateful to E. Dutkiewicz, L. Trübestein, N. Krasnici and
A. Michaelis for excellent technical\r\nassistance. We acknowledge the support of
the LSF Mass Spectrometry Service and the Lab\r\nSupport Facility at the Institute
of Science and Technology Austria for their contributions,\r\nincluding consultation
on size exclusion chromatography, LC/MS experimental design,\r\nmetabolomics sample
preparation, LC/MS method optimization, data acquisition, raw data\r\nanalysis,
and absolute quantification. This project is supported by the European\r\nResearch
Council (ERC) under the European Union’s Horizon 2020 research and innovation\r\nprogram
(101142681 CYNIPS) and Austrian Science Fund (FWF; P 37051-B), both to J.Friml.\r\nWe
acknowledge the generous support of the Taif University Researchers Supporting\r\nProject:
TURSP-HC2022/02 and Max-Planck-Society to A.S. "
article_number: aea7828
article_processing_charge: Yes
article_type: original
author:
- first_name: Mingyue
full_name: Li, Mingyue
id: 01f96916-0235-11eb-9379-a323192643b7
last_name: Li
- first_name: Monika
full_name: Chodasiewicz, Monika
last_name: Chodasiewicz
- first_name: Malavika
full_name: Muraleedharan, Malavika
last_name: Muraleedharan
- first_name: Israel M.
full_name: Lopez, Israel M.
last_name: Lopez
- first_name: Michal
full_name: Gorka, Michal
last_name: Gorka
- first_name: Olga
full_name: Kerber, Olga
last_name: Kerber
- first_name: Saqer S.
full_name: Alotaibi, Saqer S.
last_name: Alotaibi
- first_name: Andrew D.L.
full_name: Nelson, Andrew D.L.
last_name: Nelson
- first_name: Rene
full_name: Lenobel, Rene
last_name: Lenobel
- first_name: Jaroslava
full_name: Friedecká, Jaroslava
last_name: Friedecká
- first_name: Aleksandra
full_name: Skirycz, Aleksandra
last_name: Skirycz
- first_name: Jiří
full_name: Friml, Jiří
id: 4159519E-F248-11E8-B48F-1D18A9856A87
last_name: Friml
orcid: 0000-0002-8302-7596
citation:
ama: Li M, Chodasiewicz M, Muraleedharan M, et al. Biogenesis and downstream effects
of 3’,5’ and 2’,3’ cAMP isomers in plants. Science Advances. 2026;12(19).
doi:10.1126/sciadv.aea7828
apa: Li, M., Chodasiewicz, M., Muraleedharan, M., Lopez, I. M., Gorka, M., Kerber,
O., … Friml, J. (2026). Biogenesis and downstream effects of 3’,5’ and 2’,3’ cAMP
isomers in plants. Science Advances. AAAS. https://doi.org/10.1126/sciadv.aea7828
chicago: Li, Mingyue, Monika Chodasiewicz, Malavika Muraleedharan, Israel M. Lopez,
Michal Gorka, Olga Kerber, Saqer S. Alotaibi, et al. “Biogenesis and Downstream
Effects of 3’,5’ and 2’,3’ CAMP Isomers in Plants.” Science Advances. AAAS,
2026. https://doi.org/10.1126/sciadv.aea7828.
ieee: M. Li et al., “Biogenesis and downstream effects of 3’,5’ and 2’,3’
cAMP isomers in plants,” Science Advances, vol. 12, no. 19. AAAS, 2026.
ista: Li M, Chodasiewicz M, Muraleedharan M, Lopez IM, Gorka M, Kerber O, Alotaibi
SS, Nelson ADL, Lenobel R, Friedecká J, Skirycz A, Friml J. 2026. Biogenesis and
downstream effects of 3’,5’ and 2’,3’ cAMP isomers in plants. Science Advances.
12(19), aea7828.
mla: Li, Mingyue, et al. “Biogenesis and Downstream Effects of 3’,5’ and 2’,3’ CAMP
Isomers in Plants.” Science Advances, vol. 12, no. 19, aea7828, AAAS, 2026,
doi:10.1126/sciadv.aea7828.
short: M. Li, M. Chodasiewicz, M. Muraleedharan, I.M. Lopez, M. Gorka, O. Kerber,
S.S. Alotaibi, A.D.L. Nelson, R. Lenobel, J. Friedecká, A. Skirycz, J. Friml,
Science Advances 12 (2026).
corr_author: '1'
date_created: 2026-05-24T22:01:31Z
date_published: 2026-05-08T00:00:00Z
date_updated: 2026-06-02T14:36:41Z
day: '08'
ddc:
- '580'
department:
- _id: JiFr
doi: 10.1126/sciadv.aea7828
external_id:
pmid:
- '42102187'
file:
- access_level: open_access
checksum: 75b8ef2db078652c750e34e9cd98a808
content_type: application/pdf
creator: dernst
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date_updated: 2026-06-02T14:33:55Z
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file_size: 2014452
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has_accepted_license: '1'
intvolume: ' 12'
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oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 8f347782-16d5-11f0-9cad-8c19706ee739
grant_number: '101142681'
name: Cyclic nucleotides as second messengers in plants
- _id: 7bcece63-9f16-11ee-852c-ae94e099eeb6
grant_number: P37051
name: Guanylate cyclase activity of TIR1/AFBs auxin receptors
publication: Science Advances
publication_identifier:
eissn:
- 2375-2548
publication_status: published
publisher: AAAS
quality_controlled: '1'
scopus_import: '1'
status: public
title: Biogenesis and downstream effects of 3',5' and 2',3' cAMP isomers in plants
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: 12
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21915'
abstract:
- lang: eng
text: Hydrological models commonly use very simple snow accumulation and melt models
based on air temperature information, namely, a temperature threshold for snow
accumulation as well as for snowmelt, and a melt factor. This utility emerges
due to the simplicity, efficiency, and generally good performance of such models
if sufficient calibration information is available. At scales beyond single gauged
catchments, the estimation and evaluation of the temperature thresholds and the
melt factor has been difficult due to a lack of observations on snow accumulation
and melt. Using a recently published Northern Hemisphere snow water equivalent
dataset (NH-SWE) and co-located climate station observations of temperature and
precipitation (4736 stations across the Northern Hemisphere), this work estimates
melt factors and temperature thresholds for snow modelling based on station observations
and provides the first large-scale and long-term (1950–2023) evaluation of a simple
temperature-index snow model and its parameters across a diverse range of snow
climates. Our study reveals that the 0 °C as precipitation-phase threshold captures
most snowfall days (89 %) and the 0 °C as snowmelt initiation threshold captures
most snowmelt days (76 %). Adjusting large-scale uniform threshold values does
not consistently improve performance across all snow accumulation and melt metrics.
Estimated melt factors based on observations converge towards 3–5 mm (°C d)−1
for deeper snowpack climates (peak snow water equivalent >300 mm), but their estimation
may be more challenging for colder climates with shallower snowpacks (<300 mm),
conditions where the derived melt factors cover a wider range (1 to 12 mm (°C d)−1)
and a much higher interannual and spatial variability. The temperature-index snow
model performs consistently well, on average, across the available Northern Hemisphere
data set for estimating long-term mean values of seasonal snow cover onset, snowmelt
season onset, mean snow accumulation and snowmelt rates, but challenges may arise
due to biases in temperature records or solid precipitation undercatch. Peak snow
water equivalent is likely underestimated for deep or alpine snowpacks, while
it is likely overestimated for shallow snowpacks in the coldest and continental
climates. The best median performance of the temperature-index approach lies on
relatively shallow snowpacks in temperate climates. This study provides valuable
insights into temperature-threshold snowfall modelling and temperature-index melt
modelling for applications across diverse climates and environments, and the results
should help refine regional modelling approaches to enhance our understanding
of snowpack responses to global warming.
acknowledgement: 'AFB acknowledges funding from the UK''s Natural Environment Research
Council (NERC) CENTA2 doctoral training program, grant number NE/S007350/1. AFB
acknowledges support from the School of Geography, Earth and Environmental Science
research fund. The computations described in this paper were performed using the
University of Birmingham''s BlueBEAR HPC service, which provides a High Performance
Computing service to the University''s research community. See http://www.birmingham.ac.uk/bear
(last access: 15 December 2025) for more details. This research has been supported
by the Natural Environment Research Council (grant no. CENTA2 NE/S007350/1).'
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: Bettina
full_name: Schaefli, Bettina
last_name: Schaefli
- first_name: Ross
full_name: Woods, Ross
last_name: Woods
- first_name: Joshua R.
full_name: Larsen, Joshua R.
last_name: Larsen
citation:
ama: Fontrodona-Bach A, Schaefli B, Woods R, Larsen JR. Estimating robust melt factors
and temperature thresholds for snow modelling across the Northern Hemisphere.
Hydrology and Earth System Sciences. 2026;30(9):2613-2636. doi:10.5194/hess-30-2613-2026
apa: Fontrodona-Bach, A., Schaefli, B., Woods, R., & Larsen, J. R. (2026). Estimating
robust melt factors and temperature thresholds for snow modelling across the Northern
Hemisphere. Hydrology and Earth System Sciences. Copernicus Publications.
https://doi.org/10.5194/hess-30-2613-2026
chicago: Fontrodona-Bach, Adrià, Bettina Schaefli, Ross Woods, and Joshua R. Larsen.
“Estimating Robust Melt Factors and Temperature Thresholds for Snow Modelling
across the Northern Hemisphere.” Hydrology and Earth System Sciences. Copernicus
Publications, 2026. https://doi.org/10.5194/hess-30-2613-2026.
ieee: A. Fontrodona-Bach, B. Schaefli, R. Woods, and J. R. Larsen, “Estimating robust
melt factors and temperature thresholds for snow modelling across the Northern
Hemisphere,” Hydrology and Earth System Sciences, vol. 30, no. 9. Copernicus
Publications, pp. 2613–2636, 2026.
ista: Fontrodona-Bach A, Schaefli B, Woods R, Larsen JR. 2026. Estimating robust
melt factors and temperature thresholds for snow modelling across the Northern
Hemisphere. Hydrology and Earth System Sciences. 30(9), 2613–2636.
mla: Fontrodona-Bach, Adrià, et al. “Estimating Robust Melt Factors and Temperature
Thresholds for Snow Modelling across the Northern Hemisphere.” Hydrology and
Earth System Sciences, vol. 30, no. 9, Copernicus Publications, 2026, pp.
2613–36, doi:10.5194/hess-30-2613-2026.
short: A. Fontrodona-Bach, B. Schaefli, R. Woods, J.R. Larsen, Hydrology and Earth
System Sciences 30 (2026) 2613–2636.
corr_author: '1'
date_created: 2026-05-24T22:01:32Z
date_published: 2026-05-04T00:00:00Z
date_updated: 2026-06-02T09:24:00Z
day: '04'
ddc:
- '550'
department:
- _id: FrPe
doi: 10.5194/hess-30-2613-2026
file:
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checksum: 8bde4775545f9e049ea3806144b0d5f1
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creator: dernst
date_created: 2026-06-02T09:22:26Z
date_updated: 2026-06-02T09:22:26Z
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file_name: 2026_HydrologyEarthSystemSciences_FontrodonaBach.pdf
file_size: 11250378
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success: 1
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intvolume: ' 30'
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language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
page: 2613-2636
publication: Hydrology and Earth System Sciences
publication_identifier:
eissn:
- 1607-7938
issn:
- 1027-5606
publication_status: published
publisher: Copernicus Publications
quality_controlled: '1'
scopus_import: '1'
status: public
title: Estimating robust melt factors and temperature thresholds for snow modelling
across the Northern Hemisphere
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: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21917'
abstract:
- lang: eng
text: A defining feature of quantum many-body systems is the exponential scaling
of the Hilbert space with the number of degrees of freedom. This exponential complexity
naïvely renders a complete state characterization, for instance via the complete
set of bipartite Renyi entropies for all disjoint regions, a challenging task.
Recently, a compact way of storing subregions' purities by encoding them as amplitudes
of a fictitious quantum wave function, known as entanglement feature, was proposed.
Notably, the entanglement feature can be a simple object even for highly entangled
quantum states. However the complexity and practical usage of the entanglement
feature for general quantum states has not been explored. In this work, we demonstrate
that the entanglement feature can be efficiently learned using only a polynomial
amount of samples in the number of degrees of freedom through the so-called tensor
cross interpolation (TCI) algorithm, assuming it is expressible as a finite bond
dimension MPS. We benchmark this learning process on Haar and random MPS states,
confirming analytic expectations. Applying the TCI algorithm to quantum eigenstates
of various one dimensional quantum systems, we identify cases where eigenstates
have entanglement feature learnable with TCI. We conclude with possible applications
of the learned entanglement feature, such as quantifying the distance between
different entanglement patterns and finding the optimal one-dimensional ordering
of physical indices in a given state, highlighting the potential utility of the
proposed purity interpolation method.
acknowledgement: "We acknowledge useful discussions with Richard Küng\r\non the interpolation
methods and error spreading, Ilia\r\nA. Luchnikov, Margarita Davydova, and, in particular,
Hiroshi Shinaoka, Marc Ritter, Yuriel Nuñez\r\nfor useful discussions about TCI
and the various\r\nworkarounds within the TensorCrossInterpolation.jl\r\nlibrary.
We also acknowledge the comments of anonymous Referee B, that encouraged us to expand
the\r\nmanuscript with discussion of additional applications\r\nof entanglement
feature in Section 4.3. M.S. acknowledges discussions with D. V. Savostyanov at
the 2nd\r\nInternational Quantum Tensor Networks (IQTN) plenary meeting at Flatiron
Institute’s Center for Computational Quantum Physics (CCQ) for introduction\r\nto
the TCI approach. D.K and M.S. acknowledge support by the European Research Council
(ERC) under We acknowledge useful discussions with Richard Küng\r\non the interpolation
methods and error spreading, Ilia\r\nA. Luchnikov, Margarita Davydova, and, in particular,
Hiroshi Shinaoka, Marc Ritter, Yuriel Nuñez\r\nfor useful discussions about TCI
and the various\r\nworkarounds within the TensorCrossInterpolation.jl\r\nlibrary.
We also acknowledge the comments of anonymous Referee B, that encouraged us to expand
the\r\nmanuscript with discussion of additional applications\r\nof entanglement
feature in Section 4.3. M.S. acknowledges discussions with D. V. Savostyanov at
the 2nd\r\nInternational Quantum Tensor Networks (IQTN) plenary meeting at Flatiron
Institute’s Center for Computational Quantum Physics (CCQ) for introduction\r\nto
the TCI approach. D.K and M.S. acknowledge support by the European Research Council
(ERC) under We acknowledge useful discussions with Richard Küng\r\non the interpolation
methods and error spreading, Ilia\r\nA. Luchnikov, Margarita Davydova, and, in particular,
Hiroshi Shinaoka, Marc Ritter, Yuriel Nuñez\r\nfor useful discussions about TCI
and the various\r\nworkarounds within the TensorCrossInterpolation.jl\r\nlibrary.
We also acknowledge the comments of anonymous Referee B, that encouraged us to expand
the\r\nmanuscript with discussion of additional applications\r\nof entanglement
feature in Section 4.3. M.S. acknowledges discussions with D. V. Savostyanov at
the 2nd\r\nInternational Quantum Tensor Networks (IQTN) plenary meeting at Flatiron
Institute’s Center for Computational Quantum Physics (CCQ) for introduction\r\nto
the TCI approach. D.K and M.S. acknowledge support by the European Research Council
(ERC) under the European Union’s Horizon 2020 research and innovation program (Grant
Agreement No. 850899).\r\nR.V. acknowledges partial support from the US Department
of Energy, Office of Science, Basic Energy\r\nSciences, under award No. DE-SC0023999,
and the\r\nSwiss National Science Foundation (grant 10008234).\r\nThis research
was supported in part by grant NSF\r\nPHY-2309135 to the Kavli Institute for Theoretical\r\nPhysics
(KITP)"
article_number: '2114'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Dmytro
full_name: Kolisnyk, Dmytro
id: 530a7320-5355-11ee-ae5a-82a46997aaa7
last_name: Kolisnyk
orcid: 0000-0002-8612-8202
- first_name: Raimel A
full_name: Medina Ramos, Raimel A
id: CE680B90-D85A-11E9-B684-C920E6697425
last_name: Medina Ramos
orcid: 0000-0002-5383-2869
- first_name: Romain
full_name: Vasseur, Romain
last_name: Vasseur
- first_name: Maksym
full_name: Serbyn, Maksym
id: 47809E7E-F248-11E8-B48F-1D18A9856A87
last_name: Serbyn
orcid: 0000-0002-2399-5827
citation:
ama: Kolisnyk D, Medina Ramos RA, Vasseur R, Serbyn M. Tensor cross interpolation
of purities in quantum many-body systems. Quantum. 2026;10. doi:10.22331/q-2026-05-22-2114
apa: Kolisnyk, D., Medina Ramos, R. A., Vasseur, R., & Serbyn, M. (2026). Tensor
cross interpolation of purities in quantum many-body systems. Quantum.
Verein zur Förderung des Open Access Publizierens in den Quantenwissenschaften.
https://doi.org/10.22331/q-2026-05-22-2114
chicago: Kolisnyk, Dmytro, Raimel A Medina Ramos, Romain Vasseur, and Maksym Serbyn.
“Tensor Cross Interpolation of Purities in Quantum Many-Body Systems.” Quantum.
Verein zur Förderung des Open Access Publizierens in den Quantenwissenschaften,
2026. https://doi.org/10.22331/q-2026-05-22-2114.
ieee: D. Kolisnyk, R. A. Medina Ramos, R. Vasseur, and M. Serbyn, “Tensor cross
interpolation of purities in quantum many-body systems,” Quantum, vol.
10. Verein zur Förderung des Open Access Publizierens in den Quantenwissenschaften,
2026.
ista: Kolisnyk D, Medina Ramos RA, Vasseur R, Serbyn M. 2026. Tensor cross interpolation
of purities in quantum many-body systems. Quantum. 10, 2114.
mla: Kolisnyk, Dmytro, et al. “Tensor Cross Interpolation of Purities in Quantum
Many-Body Systems.” Quantum, vol. 10, 2114, Verein zur Förderung des Open
Access Publizierens in den Quantenwissenschaften, 2026, doi:10.22331/q-2026-05-22-2114.
short: D. Kolisnyk, R.A. Medina Ramos, R. Vasseur, M. Serbyn, Quantum 10 (2026).
corr_author: '1'
date_created: 2026-05-26T19:39:12Z
date_published: 2026-05-22T00:00:00Z
date_updated: 2026-06-02T09:15:13Z
day: '22'
ddc:
- '530'
department:
- _id: MaSe
- _id: GradSch
doi: 10.22331/q-2026-05-22-2114
ec_funded: 1
external_id:
arxiv:
- '2503.17230'
file:
- access_level: open_access
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oa: 1
oa_version: Published Version
project:
- _id: 23841C26-32DE-11EA-91FC-C7463DDC885E
call_identifier: H2020
grant_number: '850899'
name: 'Non-Ergodic Quantum Matter: Universality, Dynamics and Control'
publication: Quantum
publication_identifier:
eissn:
- 2521-327X
publication_status: published
publisher: Verein zur Förderung des Open Access Publizierens in den Quantenwissenschaften
quality_controlled: '1'
status: public
title: Tensor cross interpolation of purities in quantum many-body systems
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: '2026'
...
---
OA_place: publisher
_id: '21918'
acknowledged_ssus:
- _id: ScienComp
acknowledgement: "At different stages of my PhD, my work was supported by several
grants: the\r\nDOC fellowship of the Austrian Academy of Sciences (26293, awarded
to me),\r\nthe FWF-SFB grant (PT1032F06504 n. F65, awarded to Jan Maas), and the
ERC\r\ngrant (PR1032ERC01 n. 716117, awarded to Jan Maas). I also appreciate the
help\r\nfrom the Scientific Computing unit for their advice on the cluster usage."
alternative_title:
- ISTA Thesis
article_processing_charge: No
author:
- first_name: Kseniia
full_name: Khudiakova, Kseniia
id: 4E6DC800-AE37-11E9-AC72-31CAE5697425
last_name: Khudiakova
orcid: 0000-0002-6246-1465
citation:
ama: Khudiakova K. How epistasis and purifying selection shape genetic diversity.
2026. doi:10.15479/AT-ISTA-21918
apa: Khudiakova, K. (2026). How epistasis and purifying selection shape genetic
diversity. Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-21918
chicago: Khudiakova, Kseniia. “How Epistasis and Purifying Selection Shape Genetic
Diversity.” Institute of Science and Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-21918.
ieee: K. Khudiakova, “How epistasis and purifying selection shape genetic diversity,”
Institute of Science and Technology Austria, 2026.
ista: Khudiakova K. 2026. How epistasis and purifying selection shape genetic diversity.
Institute of Science and Technology Austria.
mla: Khudiakova, Kseniia. How Epistasis and Purifying Selection Shape Genetic
Diversity. Institute of Science and Technology Austria, 2026, doi:10.15479/AT-ISTA-21918.
short: K. Khudiakova, How Epistasis and Purifying Selection Shape Genetic Diversity,
Institute of Science and Technology Austria, 2026.
corr_author: '1'
date_created: 2026-05-27T06:26:08Z
date_published: 2026-06-07T00:00:00Z
date_updated: 2026-06-12T12:43:35Z
day: '07'
ddc:
- '576'
degree_awarded: PhD
department:
- _id: GradSch
- _id: NiBa
- _id: JaMa
doi: 10.15479/AT-ISTA-21918
ec_funded: 1
file:
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language:
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license: https://creativecommons.org/licenses/by-nc-nd/4.0/
month: '06'
oa_version: Published Version
page: '89'
project:
- _id: 256E75B8-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '716117'
name: Optimal Transport and Stochastic Dynamics
- _id: 34d33d68-11ca-11ed-8bc3-ec13763c0ca8
grant_number: '26293'
name: The impact of deleterious mutations on small populations
- _id: fc31cba2-9c52-11eb-aca3-ff467d239cd2
grant_number: F6504
name: Taming Complexity in Partial Differential Systems
publication_identifier:
issn:
- 2663-337X
publication_status: published
publisher: Institute of Science and Technology Austria
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status: public
- id: '12513'
relation: part_of_dissertation
status: deleted
- id: '21967'
relation: part_of_dissertation
status: public
- id: '21968'
relation: part_of_dissertation
status: public
status: public
supervisor:
- first_name: Nicholas H
full_name: Barton, Nicholas H
id: 4880FE40-F248-11E8-B48F-1D18A9856A87
last_name: Barton
orcid: 0000-0002-8548-5240
- first_name: Jan
full_name: Maas, Jan
id: 4C5696CE-F248-11E8-B48F-1D18A9856A87
last_name: Maas
orcid: 0000-0002-0845-1338
title: How epistasis and purifying selection shape genetic diversity
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: dissertation
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
year: '2026'
...