---
OA_type: closed access
_id: '21762'
abstract:
- lang: eng
  text: Bacteria, like eukaryotes, use conserved cytoskeletal systems for intracellular
    organization. The plasmid-encoded ParMRC system forms actin-like filaments that
    segregate low–copy number plasmids. In multicellular cyanobacteria such as Anabaena
    sp., we found that a chromosomally encoded ParMR system has evolved into a cytoskeletal
    system named CorMR with a function in cell shape control rather than DNA segregation.
    Live-cell imaging, in vitro reconstitution, and cryo–electron microscopy revealed
    that CorM formed dynamically unstable, antiparallel double-stranded filaments
    that were recruited to the membrane by CorR through an amphipathic helix conserved
    in multicellular cyanobacteria. CorMR filaments were regulated by MinC, which
    excluded them from the poles and division plane. Comparative genomics indicated
    that the repurposing of ParMR and Min systems coevolved with cyanobacterial multicellularity,
    highlighting the evolutionary plasticity of cytoskeletal systems in bacteria.
acknowledged_ssus:
- _id: Bio
- _id: ScienComp
- _id: EM-Fac
- _id: LifeSc
acknowledgement: "We thank all members of the Loose lab at ISTA for helpful discussions;
  M. Kojic for critical reading of the manuscript; A. Herrero (Sevilla University)
  for sharing her extensive BACTH plasmid library and other plasmids, as well as cyanobacterial
  strains; T. Dagan and F. Nies (both Kiel University) for sharing cyanobacterial
  strains and plasmids and for valuable discussions; N. Sapay and A. Michon for providing
  the Amphipaseek code, which enabled us to perform our large-scale amphipathic helix
  screen of cyanobacterial CorR proteins; V.-V. Hodirnau for support in cryo-ET data
  collection; and J. Hansen for advice about cryo-EM data processing.\r\nThis work
  was supported by the Scientific Service Units (SSU) of ISTA through resources provided
  by the Imaging & Optics Facility (IOF), the Scientific Computing (SciComp), the
  Electron Microscopy Facility (EMF), and the Lab Support Facility (LSF). This work
  was funded by the European Union’s Horizon 2020 research and innovation program
  (Marie Skłodowska-Curie grant 101034413 to B.L.S.); the European Research Council
  (ERC) of the European Union (grant ActinID 101076260 to F.K.M.S.); the Swiss National
  Science Foundation (starting grant TMSGI3_226208 to G.L.W.); and the Jean-Jacques
  et Letitia Lopez-Loreta Foundation (G.L.W.)."
article_number: eaea6343
article_processing_charge: No
article_type: original
author:
- first_name: Benjamin L
  full_name: Springstein, Benjamin L
  id: b4eb62ef-ac72-11ed-9503-ed3b4d66c083
  last_name: Springstein
  orcid: 0000-0002-3461-5391
- first_name: Manjunath
  full_name: Javoor, Manjunath
  id: 305ab18b-dc7d-11ea-9b2f-b58195228ea2
  last_name: Javoor
  orcid: 0000-0003-2311-2112
- first_name: Daniela
  full_name: Megrian, Daniela
  last_name: Megrian
- first_name: Roman
  full_name: Hajdu, Roman
  id: ffab949d-133f-11ed-8f02-94de21ace503
  last_name: Hajdu
- first_name: Dustin M.
  full_name: Hanke, Dustin M.
  last_name: Hanke
- first_name: Bettina
  full_name: Zens, Bettina
  id: 45FD126C-F248-11E8-B48F-1D18A9856A87
  last_name: Zens
  orcid: 0000-0002-9561-1239
- first_name: Gregor L.
  full_name: Weiss, Gregor L.
  last_name: Weiss
- first_name: Florian Km
  full_name: Schur, Florian Km
  id: 48AD8942-F248-11E8-B48F-1D18A9856A87
  last_name: Schur
  orcid: 0000-0003-4790-8078
- first_name: Martin
  full_name: Loose, Martin
  id: 462D4284-F248-11E8-B48F-1D18A9856A87
  last_name: Loose
  orcid: 0000-0001-7309-9724
citation:
  ama: Springstein BL, Javoor M, Megrian D, et al. Repurposing of a DNA segregation
    machinery into a cytoskeletal system controlling cell shape. <i>Science</i>. 2026;392(6795).
    doi:<a href="https://doi.org/10.1126/science.aea6343">10.1126/science.aea6343</a>
  apa: Springstein, B. L., Javoor, M., Megrian, D., Hajdu, R., Hanke, D. M., Zens,
    B., … Loose, M. (2026). Repurposing of a DNA segregation machinery into a cytoskeletal
    system controlling cell shape. <i>Science</i>. AAAS. <a href="https://doi.org/10.1126/science.aea6343">https://doi.org/10.1126/science.aea6343</a>
  chicago: Springstein, Benjamin L, Manjunath Javoor, Daniela Megrian, Roman Hajdu,
    Dustin M. Hanke, Bettina Zens, Gregor L. Weiss, Florian KM Schur, and Martin Loose.
    “Repurposing of a DNA Segregation Machinery into a Cytoskeletal System Controlling
    Cell Shape.” <i>Science</i>. AAAS, 2026. <a href="https://doi.org/10.1126/science.aea6343">https://doi.org/10.1126/science.aea6343</a>.
  ieee: B. L. Springstein <i>et al.</i>, “Repurposing of a DNA segregation machinery
    into a cytoskeletal system controlling cell shape,” <i>Science</i>, vol. 392,
    no. 6795. AAAS, 2026.
  ista: Springstein BL, Javoor M, Megrian D, Hajdu R, Hanke DM, Zens B, Weiss GL,
    Schur FK, Loose M. 2026. Repurposing of a DNA segregation machinery into a cytoskeletal
    system controlling cell shape. Science. 392(6795), eaea6343.
  mla: Springstein, Benjamin L., et al. “Repurposing of a DNA Segregation Machinery
    into a Cytoskeletal System Controlling Cell Shape.” <i>Science</i>, vol. 392,
    no. 6795, eaea6343, AAAS, 2026, doi:<a href="https://doi.org/10.1126/science.aea6343">10.1126/science.aea6343</a>.
  short: B.L. Springstein, M. Javoor, D. Megrian, R. Hajdu, D.M. Hanke, B. Zens, G.L.
    Weiss, F.K. Schur, M. Loose, Science 392 (2026).
corr_author: '1'
date_created: 2026-04-26T22:01:46Z
date_published: 2026-04-16T00:00:00Z
date_updated: 2026-09-03T09:36:24Z
day: '16'
department:
- _id: MaLo
- _id: FlSc
- _id: GradSch
- _id: EM-Fac
doi: 10.1126/science.aea6343
ec_funded: 1
external_id:
  pmid:
  - '41990175'
fulldoi: https://doi.org/10.1126/science.aea6343
intvolume: '       392'
issue: '6795'
language:
- iso: eng
month: '04'
oa_version: None
pmid: 1
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
  call_identifier: H2020
  grant_number: '101034413'
  name: 'IST-BRIDGE: International postdoctoral program'
- _id: bd980d18-d553-11ed-ba76-ceaa645c97eb
  grant_number: '101076260'
  name: A molecular atlas of Actin filament IDentities in the cell motility machinery
publication: Science
publication_identifier:
  eissn:
  - 1095-9203
  issn:
  - 0036-8075
publication_status: published
publisher: AAAS
quality_controlled: '1'
related_material:
  record:
  - id: '22744'
    relation: dissertation_contains
    status: public
scopus_import: '1'
status: public
title: Repurposing of a DNA segregation machinery into a cytoskeletal system controlling
  cell shape
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 392
year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '22751'
abstract:
- lang: eng
  text: 'The physical processes that led to the formation of billion-solar-mass black
    holes within the first 700 million years of cosmic time, a period known as cosmic
    dawn, remain a puzzle1. Several theoretical scenarios have been proposed to seed
    and rapidly grow black holes2,3,4, but direct observations of these mechanisms
    remain elusive. Here we present a source 660 million years after the Big Bang
    that exhibits singular properties: among the largest hydrogen Balmer breaks reported
    at any redshift, broad multi-peaked Hβ emission, and Balmer line absorption in
    several transitions. We model this source as an enshrouded black hole in which
    the Balmer break and absorption features are a result of extremely dense, turbulent
    gas forming a dust-free envelope around a supermassive black hole5,6. This source
    may provide evidence of an early black hole embedded in dense gas—a theoretical
    configuration proposed to rapidly grow black holes by super-Eddington accretion7,8.
    Radiation from the black hole seems to dominate almost all observed light, leaving
    limited room for contribution from its host galaxy. If the source merged with
    its brighter neighbour, it would resemble the recently discovered ‘little red
    dots’ with perplexing spectral energy distributions9,10,11. The redness of the
    black hole is due to gas, not dust12,13, and scattering, not kinematics, gives
    rise to the complex line shapes and luminosities—black hole masses of these sources
    may therefore be overestimated by orders of magnitude.'
acknowledgement: This work is based on observations made with the NASA/ESA/CSA James
  Webb Space Telescope. The data were obtained from the Mikulski Archive for Space
  Telescopes at the Space Telescope Science Institute, which is operated by the Association
  of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127
  for JWST. These observations are associated with programs 5224 and 3543. R.P.N.
  is a NASA Hubble Fellow. D.J.S. is a Brinson Prize Fellow. Some of the data products
  presented in this study were retrieved from the DJA. DJA is an initiative of the
  Cosmic Dawn Center (DAWN), which is funded by the Danish National Research Foundation
  under grant DNRF140. We acknowledge funding from JWST programmes GO-3516, GO-5224
  and GO-1837. Support for this work was provided by NASA through the NASA Hubble
  Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute,
  which is operated by the Association of Universities for Research in Astronomy,
  Incorporated, under NASA contract NAS5-26555. Funded by the European Union (ERC
  AGENTS, 101076224; HEAVYMETAL, 101071865; RED CARDINAL, 101076080). Views and opinions
  expressed are however those of the author(s) only and do not necessarily reflect
  those of the European Union or the European Research Council. Neither the European
  Union nor the granting authority can be held responsible for them. This work has
  received funding from the Swiss State Secretariat for Education, Research and Innovation
  (SERI) under contract number MB22.00072, as well as from the Swiss National Science
  Foundation (SNSF) through project grant 200020_207349. This work was also supported
  by JSPS KAKENHI grant no. 23H00131. The Cosmic Dawn Center is funded by the Danish
  National Research Foundation under grant DNRF140. P.N. acknowledges support from
  the Gordon and Betty Moore Foundation and the John Templeton Foundation that fund
  the Black Hole Initiative (BHI) at Harvard University, where she serves as an external
  prinicpal investigator. S. Bose acknowledges funding from a UK Research and Innovation
  (UKRI) Future Leaders Fellowship (grant no. MR/V023381/1).
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Rohan P.
  full_name: Naidu, Rohan P.
  last_name: Naidu
- 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: Harley
  full_name: Katz, Harley
  last_name: Katz
- first_name: Anna
  full_name: De Graaff, Anna
  last_name: De Graaff
- first_name: Pascal A.
  full_name: Oesch, Pascal A.
  last_name: Oesch
- first_name: Aaron
  full_name: Smith, Aaron
  last_name: Smith
- first_name: Jenny E.
  full_name: Greene, Jenny E.
  last_name: Greene
- first_name: Gabriel
  full_name: Brammer, Gabriel
  last_name: Brammer
- first_name: Andrea
  full_name: Weibel, Andrea
  last_name: Weibel
- first_name: Raphael
  full_name: Hviding, Raphael
  last_name: Hviding
- first_name: John
  full_name: Chisholm, John
  last_name: Chisholm
- first_name: Ivo
  full_name: Labbé, Ivo
  last_name: Labbé
- first_name: Robert A.
  full_name: Simcoe, Robert A.
  last_name: Simcoe
- first_name: Callum
  full_name: Witten, Callum
  last_name: Witten
- first_name: Wendy Q.
  full_name: Sun, Wendy Q.
  last_name: Sun
- first_name: Hakim
  full_name: Atek, Hakim
  last_name: Atek
- first_name: Josephine F.W.
  full_name: Baggen, Josephine F.W.
  last_name: Baggen
- first_name: Sirio
  full_name: Belli, Sirio
  last_name: Belli
- first_name: Rachel
  full_name: Bezanson, Rachel
  last_name: Bezanson
- first_name: Leindert A.
  full_name: Boogaard, Leindert A.
  last_name: Boogaard
- first_name: Sownak
  full_name: Bose, Sownak
  last_name: Bose
- first_name: Rychard J.
  full_name: Bouwens, Rychard J.
  last_name: Bouwens
- first_name: Alba
  full_name: Covelo-Paz, Alba
  last_name: Covelo-Paz
- first_name: Pratika
  full_name: Dayal, Pratika
  last_name: Dayal
- first_name: Yoshinobu
  full_name: Fudamoto, Yoshinobu
  last_name: Fudamoto
- first_name: Lukas J.
  full_name: Furtak, Lukas J.
  last_name: Furtak
- first_name: Emma
  full_name: Giovinazzo, Emma
  last_name: Giovinazzo
- first_name: Andy
  full_name: Goulding, Andy
  last_name: Goulding
- first_name: Max
  full_name: Gronke, Max
  last_name: Gronke
- first_name: Kasper E.
  full_name: Heintz, Kasper E.
  last_name: Heintz
- first_name: Michaela
  full_name: Hirschmann, Michaela
  last_name: Hirschmann
- first_name: Garth
  full_name: Illingworth, Garth
  last_name: Illingworth
- first_name: Akio K.
  full_name: Inoue, Akio K.
  last_name: Inoue
- first_name: Benjamin D.
  full_name: Johnson, Benjamin D.
  last_name: Johnson
- first_name: Joel
  full_name: Leja, Joel
  last_name: Leja
- first_name: Ecaterina
  full_name: Leonova, Ecaterina
  last_name: Leonova
- first_name: Ian
  full_name: Mcconachie, Ian
  last_name: Mcconachie
- first_name: Michael V.
  full_name: Maseda, Michael V.
  last_name: Maseda
- first_name: Priyamvada
  full_name: Natarajan, Priyamvada
  last_name: Natarajan
- first_name: Erica
  full_name: Nelson, Erica
  last_name: Nelson
- first_name: David J.
  full_name: Setton, David J.
  last_name: Setton
- first_name: Irene
  full_name: Shivaei, Irene
  last_name: Shivaei
- first_name: David
  full_name: Sobral, David
  last_name: Sobral
- first_name: Mauro
  full_name: Stefanon, Mauro
  last_name: Stefanon
- first_name: Sandro
  full_name: Tacchella, Sandro
  last_name: Tacchella
- first_name: Sune
  full_name: Toft, Sune
  last_name: Toft
- 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: Pieter
  full_name: Van Dokkum, Pieter
  last_name: Van Dokkum
- first_name: Arjen
  full_name: Van Der Wel, Arjen
  last_name: Van Der Wel
- first_name: Marta
  full_name: Volonteri, Marta
  last_name: Volonteri
- first_name: Fabian
  full_name: Walter, Fabian
  last_name: Walter
- first_name: Bingjie
  full_name: Wang, Bingjie
  last_name: Wang
- first_name: Darach
  full_name: Watson, Darach
  last_name: Watson
- first_name: Katherine
  full_name: Whitaker, Katherine
  last_name: Whitaker
citation:
  ama: Naidu RP, Matthee JJ, Katz H, et al. A gas-enshrouded and gas-reddened black
    hole at cosmic dawn. <i>Nature</i>. 2026;656(8127):329-333. doi:<a href="https://doi.org/10.1038/s41586-026-10846-4">10.1038/s41586-026-10846-4</a>
  apa: Naidu, R. P., Matthee, J. J., Katz, H., De Graaff, A., Oesch, P. A., Smith,
    A., … Whitaker, K. (2026). A gas-enshrouded and gas-reddened black hole at cosmic
    dawn. <i>Nature</i>. Springer Nature. <a href="https://doi.org/10.1038/s41586-026-10846-4">https://doi.org/10.1038/s41586-026-10846-4</a>
  chicago: Naidu, Rohan P., Jorryt J Matthee, Harley Katz, Anna De Graaff, Pascal
    A. Oesch, Aaron Smith, Jenny E. Greene, et al. “A Gas-Enshrouded and Gas-Reddened
    Black Hole at Cosmic Dawn.” <i>Nature</i>. Springer Nature, 2026. <a href="https://doi.org/10.1038/s41586-026-10846-4">https://doi.org/10.1038/s41586-026-10846-4</a>.
  ieee: R. P. Naidu <i>et al.</i>, “A gas-enshrouded and gas-reddened black hole at
    cosmic dawn,” <i>Nature</i>, vol. 656, no. 8127. Springer Nature, pp. 329–333,
    2026.
  ista: Naidu RP, Matthee JJ, Katz H, De Graaff A, Oesch PA, Smith A, Greene JE, Brammer
    G, Weibel A, Hviding R, Chisholm J, Labbé I, Simcoe RA, Witten C, Sun WQ, Atek
    H, Baggen JFW, Belli S, Bezanson R, Boogaard LA, Bose S, Bouwens RJ, Covelo-Paz
    A, Dayal P, Fudamoto Y, Furtak LJ, Giovinazzo E, Goulding A, Gronke M, Heintz
    KE, Hirschmann M, Illingworth G, Inoue AK, Johnson BD, Leja J, Leonova E, Mcconachie
    I, Maseda MV, Natarajan P, Nelson E, Setton DJ, Shivaei I, Sobral D, Stefanon
    M, Tacchella S, Toft S, Torralba Torregrosa A, Van Dokkum P, Van Der Wel A, Volonteri
    M, Walter F, Wang B, Watson D, Whitaker K. 2026. A gas-enshrouded and gas-reddened
    black hole at cosmic dawn. Nature. 656(8127), 329–333.
  mla: Naidu, Rohan P., et al. “A Gas-Enshrouded and Gas-Reddened Black Hole at Cosmic
    Dawn.” <i>Nature</i>, vol. 656, no. 8127, Springer Nature, 2026, pp. 329–33, doi:<a
    href="https://doi.org/10.1038/s41586-026-10846-4">10.1038/s41586-026-10846-4</a>.
  short: R.P. Naidu, J.J. Matthee, H. Katz, A. De Graaff, P.A. Oesch, A. Smith, J.E.
    Greene, G. Brammer, A. Weibel, R. Hviding, J. Chisholm, I. Labbé, R.A. Simcoe,
    C. Witten, W.Q. Sun, H. Atek, J.F.W. Baggen, S. Belli, R. Bezanson, L.A. Boogaard,
    S. Bose, R.J. Bouwens, A. Covelo-Paz, P. Dayal, Y. Fudamoto, L.J. Furtak, E. Giovinazzo,
    A. Goulding, M. Gronke, K.E. Heintz, M. Hirschmann, G. Illingworth, A.K. Inoue,
    B.D. Johnson, J. Leja, E. Leonova, I. Mcconachie, M.V. Maseda, P. Natarajan, E.
    Nelson, D.J. Setton, I. Shivaei, D. Sobral, M. Stefanon, S. Tacchella, S. Toft,
    A. Torralba Torregrosa, P. Van Dokkum, A. Van Der Wel, M. Volonteri, F. Walter,
    B. Wang, D. Watson, K. Whitaker, Nature 656 (2026) 329–333.
das_tickbox: '1'
dataavailabilitystatement: 'The prism spectra obtained as part of JWST-GO-5224 (MoM)
  featured in this work are available on Zenodo (https://doi.org/10.5281/zenodo.15059214).
  All processed images and spectra used in this work are publicly available via the
  DAWN JWST archive (https://dawn-cph.github.io/dja/). All results presented may be
  reproduced with the open-access reduced data described above and using the following
  publicly available software whose use is referenced in the text: msaexp, grizli,
  astropy, Cloudy, SpectRes, pysersic, COLT and numpyro.'
date_created: 2026-08-23T22:01:46Z
date_published: 2026-08-13T00:00:00Z
date_updated: 2026-09-07T12:50:34Z
day: '13'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1038/s41586-026-10846-4
external_id:
  pmid:
  - '42587117'
file:
- access_level: open_access
  checksum: 80127691cb39deb39948c337f6915f7b
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-07T12:49:32Z
  date_updated: 2026-09-07T12:49:32Z
  file_id: '22841'
  file_name: 2026_Nature_Naidu.pdf
  file_size: 15134062
  relation: main_file
  success: 1
file_date_updated: 2026-09-07T12:49:32Z
fulldoi: https://doi.org/10.1038/s41586-026-10846-4
has_accepted_license: '1'
intvolume: '       656'
issue: '8127'
language:
- iso: eng
license: https://creativecommons.org/licenses/by/4.0/
month: '08'
oa: 1
oa_version: Published Version
page: 329-333
pmid: 1
publication: Nature
publication_identifier:
  eissn:
  - 1476-4687
  issn:
  - 0028-0836
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
researchdata_availability: yes
scopus_import: '1'
status: public
supplementarymaterial: yes
title: A gas-enshrouded and gas-reddened black hole at cosmic dawn
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: 656
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '22750'
abstract:
- lang: eng
  text: 'Robust oxygenic photosynthesis requires the efficient assembly and repair
    of the multi-subunit oxygen-evolving photosystem II (PSII) complex. Previous cryogenic
    electron microscopy (cryo-EM) structures of PSII assembly/disassembly intermediates
    have relied on the analysis of deletion mutants or removal of PSII subunits in
    vitro. Here we report the cryo-EM structures of naturally occurring dimeric PSII
    intermediates from the cyanobacterium Thermosynechococcus vestitus at a resolution
    of about 2.2 Å. These intermediates contain inactive dimers lacking the oxygen-evolving
    complex (OEC) and semi-active dimers with the OEC present in one of the two monomers.
    Our structural data provide a mechanism for how assembly and disassembly of the
    Mn4CaO5 cluster is coordinated with the binding and release of the extrinsic proteins:
    restructuring of the C-terminal tail of D1 subunit during assembly or disassembly
    of the Mn cluster triggers conformational changes in D2, CP47 and CP43 to drive
    the binding/release of the extrinsic proteins. A combination of structural and
    mass spectrometry data also suggests that the inactive PSII complexes may include
    damaged complexes containing oxidized D1-His332, a monodentate ligand to one of
    the Mn ions of the OEC.'
acknowledged_ssus:
- _id: EM-Fac
- _id: LifeSc
- _id: ScienComp
acknowledgement: 'P.J.N. is grateful for the support from the Imperial College Electron
  Microscopy Center. L.A.S. acknowledges the support from the Scientific Service Units
  (SSU) of IST Austria: the Electron Microscopy Facility (EMF), the Life Science Facility
  (LSF) and the IST high-performance computing cluster. P.J.N. is grateful for the
  support of the Biotechnology & Biological Sciences Research Council (awards BB/I00937X/1,
  BB/L003260/1 and BB/P00931X/1). L.A.S. is grateful to IST Austria for providing
  the funding.'
article_number: '8433'
article_processing_charge: Yes
article_type: original
author:
- first_name: Ziyu
  full_name: Zhao, Ziyu
  id: a63fe682-9f3a-11ee-bf8c-cfdf919b9850
  last_name: Zhao
- first_name: Irene
  full_name: Vercellino, Irene
  id: 3ED6AF16-F248-11E8-B48F-1D18A9856A87
  last_name: Vercellino
  orcid: 0000-0001-5618-3449
- first_name: Julian P.
  full_name: Whitelegge, Julian P.
  last_name: Whitelegge
- first_name: Karim
  full_name: Maghlaoui, Karim
  last_name: Maghlaoui
- first_name: Wojciech
  full_name: Białek, Wojciech
  last_name: Białek
- first_name: Peter J.
  full_name: Nixon, Peter J.
  last_name: Nixon
- first_name: Leonid A
  full_name: Sazanov, Leonid A
  id: 338D39FE-F248-11E8-B48F-1D18A9856A87
  last_name: Sazanov
  orcid: 0000-0002-0977-7989
citation:
  ama: Zhao Z, Vercellino I, Whitelegge JP, et al. Cryo-EM structures of naturally
    occurring dimeric photosystem II complexes lacking the Mn4CaO5 cluster. <i>Nature
    Communications</i>. 2026;17. doi:<a href="https://doi.org/10.1038/s41467-026-75324-x">10.1038/s41467-026-75324-x</a>
  apa: Zhao, Z., Vercellino, I., Whitelegge, J. P., Maghlaoui, K., Białek, W., Nixon,
    P. J., &#38; Sazanov, L. A. (2026). Cryo-EM structures of naturally occurring
    dimeric photosystem II complexes lacking the Mn4CaO5 cluster. <i>Nature Communications</i>.
    Springer Nature. <a href="https://doi.org/10.1038/s41467-026-75324-x">https://doi.org/10.1038/s41467-026-75324-x</a>
  chicago: Zhao, Ziyu, Irene Vercellino, Julian P. Whitelegge, Karim Maghlaoui, Wojciech
    Białek, Peter J. Nixon, and Leonid A Sazanov. “Cryo-EM Structures of Naturally
    Occurring Dimeric Photosystem II Complexes Lacking the Mn4CaO5 Cluster.” <i>Nature
    Communications</i>. Springer Nature, 2026. <a href="https://doi.org/10.1038/s41467-026-75324-x">https://doi.org/10.1038/s41467-026-75324-x</a>.
  ieee: Z. Zhao <i>et al.</i>, “Cryo-EM structures of naturally occurring dimeric
    photosystem II complexes lacking the Mn4CaO5 cluster,” <i>Nature Communications</i>,
    vol. 17. Springer Nature, 2026.
  ista: Zhao Z, Vercellino I, Whitelegge JP, Maghlaoui K, Białek W, Nixon PJ, Sazanov
    LA. 2026. Cryo-EM structures of naturally occurring dimeric photosystem II complexes
    lacking the Mn4CaO5 cluster. Nature Communications. 17, 8433.
  mla: Zhao, Ziyu, et al. “Cryo-EM Structures of Naturally Occurring Dimeric Photosystem
    II Complexes Lacking the Mn4CaO5 Cluster.” <i>Nature Communications</i>, vol.
    17, 8433, Springer Nature, 2026, doi:<a href="https://doi.org/10.1038/s41467-026-75324-x">10.1038/s41467-026-75324-x</a>.
  short: Z. Zhao, I. Vercellino, J.P. Whitelegge, K. Maghlaoui, W. Białek, P.J. Nixon,
    L.A. Sazanov, Nature Communications 17 (2026).
corr_author: '1'
das_tickbox: '1'
dataavailabilitystatement: The cryo-EM maps are deposited in the Electron Microscopy
  Data Bank under accession number EMD- 51100 (inactive dimer), EMD- 51102 (active
  dimer) and EMD-51101 (semi-active dimer). The models are deposited in the Protein
  Data Bank under accession numbers 9G6F (inactive dimer), 9G6H (active dimer) and
  9G6G (semi-active dimer). Mass spectrometry data was uploaded to MassIVE with accession
  code MSV000101057. Source data are provided with this paper.
date_created: 2026-08-23T22:01:46Z
date_published: 2026-08-17T00:00:00Z
date_updated: 2026-09-07T13:17:53Z
day: '17'
ddc:
- '570'
department:
- _id: LeSa
doi: 10.1038/s41467-026-75324-x
external_id:
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language:
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month: '08'
oa: 1
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pmid: 1
publication: Nature Communications
publication_identifier:
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publication_status: published
publisher: Springer Nature
quality_controlled: '1'
researchdata_availability: yes
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Cryo-EM structures of naturally occurring dimeric photosystem II complexes
  lacking the Mn4CaO5 cluster
tmp:
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  short: CC BY-NC-ND (4.0)
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year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
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_id: '22752'
abstract:
- lang: eng
  text: "In this note we outline a new and simple approach to proving central limit
    theorems for various ‘global’ graph parameters that have robust ‘local’ approximations,
    using the Efron–Stein inequality, which relies on a combinatorial analysis of
    the stability of these approximations under resampling an edge. As an application,
    we give short proofs of a central limit theorem for the order of the giant component
    and of the \U0001D458\r\n-core for sparse random graphs."
acknowledgement: This research was funded in whole or in part by the Austrian Science
  Fund (FWF) [10.55776/P36131 (Joshua Erde), 10.55776/I6502 (Mihyun Kang), 10.55776/ESP3863424
  (Michael Anastos)] and by the Swiss National Science Foundation (SNSF) [P500-2_235474]
  (Vincent Pfenninger). For open access purposes, the authors have applied a CC BY
  public copyright license to any author accepted manuscript version arising from
  this submission. The authors thank the reviewers for helpful comments on the paper,
  and for bringing the particular form of Theorem 2.2 to our attention.
article_number: e70464
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Michael
  full_name: Anastos, Michael
  id: 0b2a4358-bb35-11ec-b7b9-e3279b593dbb
  last_name: Anastos
- first_name: Joshua
  full_name: Erde, Joshua
  last_name: Erde
- first_name: Mihyun
  full_name: Kang, Mihyun
  last_name: Kang
- first_name: Vincent
  full_name: Pfenninger, Vincent
  last_name: Pfenninger
citation:
  ama: Anastos M, Erde J, Kang M, Pfenninger V. A short proof of a central limit theorem
    for the order of the giant component and k-core. <i>Bulletin of the London Mathematical
    Society</i>. 2026;58(8). doi:<a href="https://doi.org/10.1112/blms.70464">10.1112/blms.70464</a>
  apa: Anastos, M., Erde, J., Kang, M., &#38; Pfenninger, V. (2026). A short proof
    of a central limit theorem for the order of the giant component and k-core. <i>Bulletin
    of the London Mathematical Society</i>. Wiley. <a href="https://doi.org/10.1112/blms.70464">https://doi.org/10.1112/blms.70464</a>
  chicago: Anastos, Michael, Joshua Erde, Mihyun Kang, and Vincent Pfenninger. “A
    Short Proof of a Central Limit Theorem for the Order of the Giant Component and
    K-Core.” <i>Bulletin of the London Mathematical Society</i>. Wiley, 2026. <a href="https://doi.org/10.1112/blms.70464">https://doi.org/10.1112/blms.70464</a>.
  ieee: M. Anastos, J. Erde, M. Kang, and V. Pfenninger, “A short proof of a central
    limit theorem for the order of the giant component and k-core,” <i>Bulletin of
    the London Mathematical Society</i>, vol. 58, no. 8. Wiley, 2026.
  ista: Anastos M, Erde J, Kang M, Pfenninger V. 2026. A short proof of a central
    limit theorem for the order of the giant component and k-core. Bulletin of the
    London Mathematical Society. 58(8), e70464.
  mla: Anastos, Michael, et al. “A Short Proof of a Central Limit Theorem for the
    Order of the Giant Component and K-Core.” <i>Bulletin of the London Mathematical
    Society</i>, vol. 58, no. 8, e70464, Wiley, 2026, doi:<a href="https://doi.org/10.1112/blms.70464">10.1112/blms.70464</a>.
  short: M. Anastos, J. Erde, M. Kang, V. Pfenninger, Bulletin of the London Mathematical
    Society 58 (2026).
das_tickbox: '0'
date_created: 2026-08-23T22:01:47Z
date_published: 2026-08-01T00:00:00Z
date_updated: 2026-09-07T13:56:17Z
day: '01'
ddc:
- '510'
department:
- _id: MaKw
doi: 10.1112/blms.70464
external_id:
  arxiv:
  - '2506.11651'
file:
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  date_created: 2026-09-07T13:53:26Z
  date_updated: 2026-09-07T13:53:26Z
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  file_size: 248641
  relation: main_file
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file_date_updated: 2026-09-07T13:53:26Z
fulldoi: https://doi.org/10.1112/blms.70464
has_accepted_license: '1'
intvolume: '        58'
issue: '8'
language:
- iso: eng
mathsc:
- 05C80
- 60F05
month: '08'
oa: 1
oa_version: Published Version
project:
- _id: 8f906bd2-16d5-11f0-9cad-e07be8aa9ac9
  grant_number: ESP3863424
  name: Combinatorial Optimisation Problems on Sparse Random Graphs
publication: Bulletin of the London Mathematical Society
publication_identifier:
  eissn:
  - 1469-2120
  issn:
  - 0024-6093
publication_status: published
publisher: Wiley
quality_controlled: '1'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: no
title: A short proof of a central limit theorem for the order of the giant component
  and k-core
tmp:
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  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 58
year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
_id: '22754'
abstract:
- lang: eng
  text: "Quantitative automata (QAs) extend finite-state automata on infinite words
    with weighted transitions to specify quantitative system properties. However,
    their finite weight sets rule out properties like average response time, where
    response times can be arbitrarily large. Nested quantitative automata (NQAs) overcome
    this limitation: a parent automaton spawns child automata to compute unbounded
    values over finite infixes and aggregates them into a final result. Despite this
    expressiveness, NQAs have lacked practical tool support to date.\r\n\r\nWe close
    this gap by extending the Quantitative Automata Kit (QuAK), a software tool for
    QA analysis, to support NQAs. Our core contribution is implementing a suite of
    flattening procedures that reduce NQAs to QAs, leveraging QuAK’s existing decision
    procedures. These reductions preserve the answers to threshold decision problems,
    while allowing users to specify properties in the more expressive NQA formalism.
    The tool handles all combinations of parent aggregators (including limits and
    averages) and child functions (extrema and monotonic or bounded summations) for
    which emptiness and universality are known to be decidable. Experiments on response-time
    and resource-consumption benchmarks demonstrate QuAK’s effectiveness."
acknowledgement: This work was supported by the European Research Council (ERC) Grants
  VAMOS (No. 101020093) and HYPER (No. 101055412).
alternative_title:
- LNCS
article_processing_charge: No
arxiv: 1
author:
- first_name: Thomas A
  full_name: Henzinger, Thomas A
  id: 40876CD8-F248-11E8-B48F-1D18A9856A87
  last_name: Henzinger
  orcid: 0000-0002-2985-7724
- first_name: Nicolas Adrien
  full_name: Mazzocchi, Nicolas Adrien
  id: b26baa86-3308-11ec-87b0-8990f34baa85
  last_name: Mazzocchi
- first_name: Naci E
  full_name: Sarac, Naci E
  id: 8C6B42F8-C8E6-11E9-A03A-F2DCE5697425
  last_name: Sarac
- first_name: Harun
  full_name: Yılmaz, Harun
  last_name: Yılmaz
citation:
  ama: 'Henzinger TA, Mazzocchi NA, Sarac NE, Yılmaz H. Extending QuAK with nested
    quantitative automata. In: <i>38th International Conference on Computer Aided
    Verification</i>. Vol 16683. Springer Nature; 2026:418-432. doi:<a href="https://doi.org/10.1007/978-3-032-32526-6_20">10.1007/978-3-032-32526-6_20</a>'
  apa: 'Henzinger, T. A., Mazzocchi, N. A., Sarac, N. E., &#38; Yılmaz, H. (2026).
    Extending QuAK with nested quantitative automata. In <i>38th International Conference
    on Computer Aided Verification</i> (Vol. 16683, pp. 418–432). Lisbon, Portugal:
    Springer Nature. <a href="https://doi.org/10.1007/978-3-032-32526-6_20">https://doi.org/10.1007/978-3-032-32526-6_20</a>'
  chicago: Henzinger, Thomas A, Nicolas Adrien Mazzocchi, Naci E Sarac, and Harun
    Yılmaz. “Extending QuAK with Nested Quantitative Automata.” In <i>38th International
    Conference on Computer Aided Verification</i>, 16683:418–32. Springer Nature,
    2026. <a href="https://doi.org/10.1007/978-3-032-32526-6_20">https://doi.org/10.1007/978-3-032-32526-6_20</a>.
  ieee: T. A. Henzinger, N. A. Mazzocchi, N. E. Sarac, and H. Yılmaz, “Extending QuAK
    with nested quantitative automata,” in <i>38th International Conference on Computer
    Aided Verification</i>, Lisbon, Portugal, 2026, vol. 16683, pp. 418–432.
  ista: 'Henzinger TA, Mazzocchi NA, Sarac NE, Yılmaz H. 2026. Extending QuAK with nested
    quantitative automata. 38th International Conference on Computer Aided Verification.
    CAV: Computer Aided Verification, LNCS, vol. 16683, 418–432.'
  mla: Henzinger, Thomas A., et al. “Extending QuAK with Nested Quantitative Automata.”
    <i>38th International Conference on Computer Aided Verification</i>, vol. 16683,
    Springer Nature, 2026, pp. 418–32, doi:<a href="https://doi.org/10.1007/978-3-032-32526-6_20">10.1007/978-3-032-32526-6_20</a>.
  short: T.A. Henzinger, N.A. Mazzocchi, N.E. Sarac, H. Yılmaz, in:, 38th International
    Conference on Computer Aided Verification, Springer Nature, 2026, pp. 418–432.
conference:
  end_date: 2026-07-29
  location: Lisbon, Portugal
  name: 'CAV: Computer Aided Verification'
  start_date: 2026-07-26
das_tickbox: '1'
dataavailabilitystatement: 'The artifact supporting the experimental results in this
  paper is available in the QuAK repository at https://github.com/ista-vamos/nested-quak.
  It contains the extended QuAK implementation, benchmark generators, example inputs,
  and scripts/logs for reproducing the reported tables. The artifact is intended to
  reproduce the experiments under the setup described in Sect. 4; runtimes may vary
  across machines, and the reported timeout and memory-exhaustion results depend on
  the stated hardware limits. No sensitive or restricted data are used. An archived
  version is available on Zenodo at DOI: http://doi.org/10.5281/zenodo.19844606.'
date_created: 2026-08-23T22:01:47Z
date_published: 2026-01-01T00:00:00Z
date_updated: 2026-09-09T06:37:41Z
day: '01'
ddc:
- '000'
department:
- _id: ToHe
doi: 10.1007/978-3-032-32526-6_20
ec_funded: 1
external_id:
  arxiv:
  - '2605.12418'
file:
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language:
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month: '01'
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oa_version: Published Version
page: 418-432
project:
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  call_identifier: H2020
  grant_number: '101020093'
  name: Vigilant Algorithmic Monitoring of Software
publication: 38th International Conference on Computer Aided Verification
publication_identifier:
  eissn:
  - 1611-3349
  isbn:
  - '9783032325259'
  issn:
  - 0302-9743
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
researchdata_availability: yes
scopus_import: '1'
status: public
supplementarymaterial: no
title: Extending QuAK with nested quantitative automata
tmp:
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  short: CC BY (4.0)
type: conference
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DOAJ_listed: '1'
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abstract:
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  text: The eigenstate thermalization hypothesis (ETH) posits how isolated quantum
    many-body systems thermalize, assuming that individual eigenstates at the same
    energy density have identical expectation values of local observables in the limit
    of large systems. While the ETH apparently holds across a wide range of interacting
    quantum systems, in this work, we show that it may require generalization in the
    presence of thermal first-order phase transitions. We introduce a class of all-to-all
    spin models, featuring first-order thermal phase transitions that stem from two
    distinct local maxima of entropy (two mean-field solutions that we dub “branches”)
    that exchange dominance in the many-body density of states as the energy is varied.
    We argue that, for energies in the vicinity of the thermal phase transition, eigenstate
    expectation values do not need to converge to the same thermal value. The system
    has a regime with coexistence of two classes of eigenstates corresponding to the
    two branches with distinct expectation values at the same energy density and another
    regime with Schrödinger-cat-like eigenstates that are interbranch superpositions;
    these two regimes are separated by an eigenstate phase transition. We propose
    a more general form of the ETH , support our results by semiclassical calculations
    and an exact diagonalization study of a microscopic spin model, and argue that
    the structure of eigenstates in the vicinity of thermal first-order phase transitions
    can be experimentally probed via nonequilibrium dynamics.
acknowledgement: A. A. acknowledges discussions and prior collaboration on related
  topics with Anatoly Dymarsky. M. S. acknowledges Ashwin Vishwanath for introducing
  him to the idea of thermal first-order phase transitions in quantum systems. This
  research was supported in part by Grant No. NSF PHY-2309135 to the Kavli Institute
  for Theoretical Physics (KITP) and by the Erwin Schrödinger International Institute
  for Mathematics and Physics (ESI). O. K. D. acknowledges support from the NSF through
  a grant for ITAMP at Harvard University. D. A. H. was supported in part by NSF QLCI
  Grant No. OMA-2120757.
article_number: '031042'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Maksym
  full_name: Serbyn, Maksym
  id: 47809E7E-F248-11E8-B48F-1D18A9856A87
  last_name: Serbyn
  orcid: 0000-0002-2399-5827
- first_name: Alexander
  full_name: Avdoshkin, Alexander
  last_name: Avdoshkin
- first_name: Oriana K.
  full_name: Diessel, Oriana K.
  last_name: Diessel
- first_name: David A.
  full_name: Huse, David A.
  last_name: Huse
citation:
  ama: Serbyn M, Avdoshkin A, Diessel OK, Huse DA. Eigenstate thermalization in thermal
    first-order phase transitions. <i>Physical Review X</i>. 2026;16(3). doi:<a href="https://doi.org/10.1103/4zs8-7kf4">10.1103/4zs8-7kf4</a>
  apa: Serbyn, M., Avdoshkin, A., Diessel, O. K., &#38; Huse, D. A. (2026). Eigenstate
    thermalization in thermal first-order phase transitions. <i>Physical Review X</i>.
    American Physical Society. <a href="https://doi.org/10.1103/4zs8-7kf4">https://doi.org/10.1103/4zs8-7kf4</a>
  chicago: Serbyn, Maksym, Alexander Avdoshkin, Oriana K. Diessel, and David A. Huse.
    “Eigenstate Thermalization in Thermal First-Order Phase Transitions.” <i>Physical
    Review X</i>. American Physical Society, 2026. <a href="https://doi.org/10.1103/4zs8-7kf4">https://doi.org/10.1103/4zs8-7kf4</a>.
  ieee: M. Serbyn, A. Avdoshkin, O. K. Diessel, and D. A. Huse, “Eigenstate thermalization
    in thermal first-order phase transitions,” <i>Physical Review X</i>, vol. 16,
    no. 3. American Physical Society, 2026.
  ista: Serbyn M, Avdoshkin A, Diessel OK, Huse DA. 2026. Eigenstate thermalization
    in thermal first-order phase transitions. Physical Review X. 16(3), 031042.
  mla: Serbyn, Maksym, et al. “Eigenstate Thermalization in Thermal First-Order Phase
    Transitions.” <i>Physical Review X</i>, vol. 16, no. 3, 031042, American Physical
    Society, 2026, doi:<a href="https://doi.org/10.1103/4zs8-7kf4">10.1103/4zs8-7kf4</a>.
  short: M. Serbyn, A. Avdoshkin, O.K. Diessel, D.A. Huse, Physical Review X 16 (2026).
corr_author: '1'
das_tickbox: '1'
dataavailabilitystatement: There are no publicly available research data or software
  supporting this manuscript. Requests for further information or data should be sent
  to the authors.
date_created: 2026-08-24T06:57:25Z
date_published: 2026-08-18T00:00:00Z
date_updated: 2026-09-09T07:01:47Z
day: '18'
ddc:
- '530'
department:
- _id: MaSe
doi: 10.1103/4zs8-7kf4
external_id:
  arxiv:
  - '2601.08347'
file:
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  checksum: 8bf0d88f17783dc1e6bf4c754534d734
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  creator: dernst
  date_created: 2026-09-09T07:00:24Z
  date_updated: 2026-09-09T07:00:24Z
  file_id: '22862'
  file_name: 2026_PhysicalReviewX_Serbyn.pdf
  file_size: 2537492
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T07:00:24Z
fulldoi: https://doi.org/10.1103/4zs8-7kf4
has_accepted_license: '1'
intvolume: '        16'
issue: '3'
language:
- iso: eng
month: '08'
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'
researchdata_availability: upon request
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Eigenstate thermalization in thermal first-order phase transitions
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'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '22753'
abstract:
- lang: eng
  text: Radial glial progenitors (RGPs) produce all excitatory neurons in the developing
    cerebral cortex. Mosaic analysis with double markers (MADM)-based lineage tracing
    in vivo has revealed a quantitative framework of RGP lineage progression1. Here
    we established MADM technology2,3 in mouse embryonic stem cells to probe RGP lineage
    progression in a self-organizing cortical organoid system. We found that RGPs
    exhibit a high level of plasticity in proliferative potential in organoids rather
    than strict temporally stereotyped lineage progression as observed in vivo. RGPs
    in organoids showed increased lineage restriction, diminishing cell-type diversity
    in clones of cortical projection neurons, despite uniform single-cell transcriptional
    signatures of RGPs and a unitary lineage trajectory. Thus, critical non-cell-autonomous
    cues that are absent in self-organizing systems and/or the genuine stem cell niche
    are essential for faithful temporal control of RGP lineage progression and the
    generation of clonal cortical cell-type diversity.
acknowledged_ssus:
- _id: Bio
- _id: LifeSc
- _id: PreCl
acknowledgement: We thank M. L. de Guevara, S. Jayaram and A. Heger for technical
  assistance with mESC derivation; M. Goudarzi for assistance with organoid imaging;
  M. Leeb and F. Freeman for advice in culturing mESCs and organoids; S. Gobeil and
  L. Sweeney for reagents and advice for organoid clearing; A. Heger for mouse colony
  management; J. Hauser for technical assistance; the Stanford Brain Organogenesis
  Workshop; and all members of the Hippenmeyer laboratory for discussion and/or comments
  on the manuscript. This study was supported by the Scientific Service Units (SSU)
  of the Institute of Science and Technology, Austria through resources provided by
  the Imaging and Optics Facility (IOF), Laboratory Support Facility (LSF) and Preclinical
  Facility (PCF). M.S. received funding from the European Commission (IST plus postdoctoral
  fellowship). This work was supported by ISTA institutional funds to S.H., FWF SFB
  F78 Neuro Stem Modulation to S.H., and by the European Research Council (ERC) under
  the European Union’s Horizon 2020 Research And Innovation Program (grant agreement
  725780 LinPro) to S.H. Open access funding provided by Institute of Science and
  Technology (IST Austria).
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Melissa A
  full_name: Stouffer, Melissa A
  id: 4C9372C4-F248-11E8-B48F-1D18A9856A87
  last_name: Stouffer
- first_name: Osvaldo
  full_name: Miranda, Osvaldo
  id: 862A3C56-A8BF-11E9-B4FA-D9E3E5697425
  last_name: Miranda
  orcid: 0000-0001-6618-6889
- first_name: Florian
  full_name: Pauler, Florian
  id: 48EA0138-F248-11E8-B48F-1D18A9856A87
  last_name: Pauler
  orcid: 0000-0002-7462-0048
- first_name: Fabrizia
  full_name: Pipicelli, Fabrizia
  id: 649134fd-d012-11ed-8f82-db1e5050f9ba
  last_name: Pipicelli
- first_name: Carmen
  full_name: Streicher, Carmen
  id: 36BCB99C-F248-11E8-B48F-1D18A9856A87
  last_name: Streicher
- first_name: Giselle T
  full_name: Cheung, Giselle T
  id: 471195F6-F248-11E8-B48F-1D18A9856A87
  last_name: Cheung
  orcid: 0000-0001-8457-2572
- first_name: Simon
  full_name: Hippenmeyer, Simon
  id: 37B36620-F248-11E8-B48F-1D18A9856A87
  last_name: Hippenmeyer
  orcid: 0000-0003-2279-1061
citation:
  ama: Stouffer MA, Miranda O, Pauler F, et al. Temporal uncoupling of radial glia
    lineage progression in cortical organoids. <i>Nature</i>. 2026. doi:<a href="https://doi.org/10.1038/s41586-026-10916-7">10.1038/s41586-026-10916-7</a>
  apa: Stouffer, M. A., Miranda, O., Pauler, F., Pipicelli, F., Streicher, C., Cheung,
    G. T., &#38; Hippenmeyer, S. (2026). Temporal uncoupling of radial glia lineage
    progression in cortical organoids. <i>Nature</i>. Springer Nature. <a href="https://doi.org/10.1038/s41586-026-10916-7">https://doi.org/10.1038/s41586-026-10916-7</a>
  chicago: Stouffer, Melissa A, Osvaldo Miranda, Florian Pauler, Fabrizia Pipicelli,
    Carmen Streicher, Giselle T Cheung, and Simon Hippenmeyer. “Temporal Uncoupling
    of Radial Glia Lineage Progression in Cortical Organoids.” <i>Nature</i>. Springer
    Nature, 2026. <a href="https://doi.org/10.1038/s41586-026-10916-7">https://doi.org/10.1038/s41586-026-10916-7</a>.
  ieee: M. A. Stouffer <i>et al.</i>, “Temporal uncoupling of radial glia lineage
    progression in cortical organoids,” <i>Nature</i>. Springer Nature, 2026.
  ista: Stouffer MA, Miranda O, Pauler F, Pipicelli F, Streicher C, Cheung GT, Hippenmeyer
    S. 2026. Temporal uncoupling of radial glia lineage progression in cortical organoids.
    Nature.
  mla: Stouffer, Melissa A., et al. “Temporal Uncoupling of Radial Glia Lineage Progression
    in Cortical Organoids.” <i>Nature</i>, Springer Nature, 2026, doi:<a href="https://doi.org/10.1038/s41586-026-10916-7">10.1038/s41586-026-10916-7</a>.
  short: M.A. Stouffer, O. Miranda, F. Pauler, F. Pipicelli, C. Streicher, G.T. Cheung,
    S. Hippenmeyer, Nature (2026).
corr_author: '1'
das_tickbox: '1'
dataavailabilitystatement: All data generated and analysed in this study are included
  in the paper, source data and/or Supplementary Tables 2 and 3. Raw sequencing data
  have been deposited with Gene Expression Omnibus (GEO) accession number GSE327470.
  Source data are provided with this paper. All scripts used to prepare data and figures
  for this manuscript are accessible on GitHub at https://github.com/fpauler/Temporal-Uncoupling-of-Radial-Glia-Lineage-Progression-in-Cortical-Organoid.
date_created: 2026-08-23T22:01:47Z
date_published: 2026-08-12T00:00:00Z
date_updated: 2026-09-09T07:11:02Z
day: '12'
ddc:
- '570'
department:
- _id: SiHi
doi: 10.1038/s41586-026-10916-7
ec_funded: 1
external_id:
  pmid:
  - '42587153'
file:
- access_level: open_access
  checksum: 11383e28fc430b28d2666f73833e8b56
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-07T13:24:10Z
  date_updated: 2026-09-07T13:24:10Z
  file_id: '22844'
  file_name: 2026_Nature_Stouffer.pdf
  file_size: 48513068
  relation: main_file
  success: 1
file_date_updated: 2026-09-07T13:24:10Z
fulldoi: https://doi.org/10.1038/s41586-026-10916-7
has_accepted_license: '1'
language:
- iso: eng
month: '08'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 059F6AB4-7A3F-11EA-A408-12923DDC885E
  grant_number: F7805
  name: Stem Cell Modulation in Neural Development and Regeneration/ P05-Molecular
    Mechanisms of Neural Stem Cell Lineage Progression
- _id: 260018B0-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '725780'
  name: Principles of Neural Stem Cell Lineage Progression in Cerebral Cortex Development
publication: Nature
publication_identifier:
  eissn:
  - 1476-4687
  issn:
  - 0028-0836
publication_status: epub_ahead
publisher: Springer Nature
quality_controlled: '1'
researchdata_availability: yes
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Temporal uncoupling of radial glia lineage progression in cortical organoids
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '22771'
abstract:
- lang: eng
  text: Elucidating reaction mechanisms requires efficient generation of transition
    states (TSs) and products. Existing diffusion and sequence-based models accelerate
    parts of this process over traditional string-based methods, but typically still
    require manual enumeration of either TSs or products, and stochastic diffusion
    dynamics can be inefficient and hard to control. We introduce MolGEN, a conditional
    flow-matching framework that uses deterministic optimal transport to map Gaussian
    priors to chemical distributions. For TS generation, MolGEN improves TS geometry
    and barrier-height prediction over diffusion models while enabling sub-second
    sampling. For reaction product generation, it achieves competitive top-k accuracy
    while preserving mass and electron balance. Using the same backbone for TS and
    product sampling, MolGEN enables template-free generative exploration of reaction
    networks without the repeated quantum-chemistry searches required by prior methods.
    For the γ-ketohydroperoxide decomposition network, it produces more valid TSs
    than string-based methods using only 12 quantum-chemistry evaluations instead
    of 1156, and identifies a lower-barrier pathway.
acknowledgement: P.T. thanks valued discussions with Dr. Peichen Zhong, Dr. Hao Tang,
  and Dr. Chengbin Zhao. P.T. thanks Dr. Dingshun Lv, Dr. Zechang Sun, and Dr. Chenxi
  Hu for identifying an important bug in an early version of the code package. The
  authors acknowledge the resources of the National Energy Research Scientific Computing
  Center (NERSC), a Department of Energy Office of Science User Facility using NERSC
  award DOEERCAP0031751 ‘GenAI@NERSC’. P.T. acknowledges funding from the BIDMaP Postdoctoral
  Fellowship.
article_number: '8769'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Ping
  full_name: Tuo, Ping
  id: 6e5644c0-c180-11ed-a2da-facc4c9f4f09
  last_name: Tuo
- first_name: Jiale
  full_name: Chen, Jiale
  id: 4d0a9064-1ff6-11ee-9fa6-ec046c604785
  last_name: Chen
  orcid: 0000-0001-5337-5875
- first_name: Ju
  full_name: Li, Ju
  last_name: Li
citation:
  ama: Tuo P, Chen J, Li J. Flow matching for reaction pathway generation. <i>Nature
    Communications</i>. 2026;17. doi:<a href="https://doi.org/10.1038/s41467-026-75654-w">10.1038/s41467-026-75654-w</a>
  apa: Tuo, P., Chen, J., &#38; Li, J. (2026). Flow matching for reaction pathway
    generation. <i>Nature Communications</i>. Springer Nature. <a href="https://doi.org/10.1038/s41467-026-75654-w">https://doi.org/10.1038/s41467-026-75654-w</a>
  chicago: Tuo, Ping, Jiale Chen, and Ju Li. “Flow Matching for Reaction Pathway Generation.”
    <i>Nature Communications</i>. Springer Nature, 2026. <a href="https://doi.org/10.1038/s41467-026-75654-w">https://doi.org/10.1038/s41467-026-75654-w</a>.
  ieee: P. Tuo, J. Chen, and J. Li, “Flow matching for reaction pathway generation,”
    <i>Nature Communications</i>, vol. 17. Springer Nature, 2026.
  ista: Tuo P, Chen J, Li J. 2026. Flow matching for reaction pathway generation.
    Nature Communications. 17, 8769.
  mla: Tuo, Ping, et al. “Flow Matching for Reaction Pathway Generation.” <i>Nature
    Communications</i>, vol. 17, 8769, Springer Nature, 2026, doi:<a href="https://doi.org/10.1038/s41467-026-75654-w">10.1038/s41467-026-75654-w</a>.
  short: P. Tuo, J. Chen, J. Li, Nature Communications 17 (2026).
das_tickbox: '1'
dataavailabilitystatement: Structures generated in this study are provided in the
  Source Data file, and deposited in the GitHub repository https://github.com/tuoping/MolGEN
  and the figshare database under accession code https://doi.org/10.6084/m9.figshare.30576365.
  Source data are provided in this paper. The MolGEN codebase is available as an open-source
  repository for continuous development at https://github.com/tuoping/MolGEN. A release
  of the code used in this work has been archived on Zenodo47.
date_created: 2026-08-30T22:01:43Z
date_published: 2026-08-21T00:00:00Z
date_updated: 2026-09-09T07:28:15Z
day: '21'
ddc:
- '000'
department:
- _id: DaAl
- _id: GradSch
doi: 10.1038/s41467-026-75654-w
external_id:
  arxiv:
  - '2507.10530'
  pmid:
  - '42469237'
file:
- access_level: open_access
  checksum: 3cfb714304eec29b97dcaf7fb86dd6e3
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-09T07:25:19Z
  date_updated: 2026-09-09T07:25:19Z
  file_id: '22864'
  file_name: 2026_NatureComm_Tuo.pdf
  file_size: 1526298
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T07:25:19Z
fulldoi: https://doi.org/10.1038/s41467-026-75654-w
has_accepted_license: '1'
intvolume: '        17'
language:
- iso: eng
month: '08'
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'
researchdata_availability: yes
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Flow matching for reaction pathway generation
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'
...
---
OA_place: repository
_id: '22852'
abstract:
- lang: eng
  text: "This Research Data contains supplemental videos for Chapter 4 \"Designing
    bistable nanostructures for target behavior\" of my PhD Thesis \"Biological functionality
    without biochemistry: designing nanomachines for target behavior\".\r\nSupplemental
    video 1: Video showing the transition pathway of a bistable nanostructure with
    sphere-based arms, corresponding to the Machine in Scenario 4.\r\nSupplemental
    video 2: Video showing the transition pathway of the Source in Scenario 1. The
    arm tips change sides during the transition, demonstrating that the arms pass
    through each other.\r\nSupplemental video 3: Video showing the transition pathway
    of a fully polyhedral hinge structure with unconstrained arms. Note that we only
    show the ends of the arms.\r\nSupplemental video 4: Video showing the transition
    pathway of the coupled energy-delivery reaction of a Machine (gray) and a Source
    (blue) nanostructure for the optimized parameters in Scenario 3. Note that we
    only show the ends of the arms."
acknowledged_ssus:
- _id: ScienComp
article_processing_charge: No
author:
- first_name: Andreas
  full_name: Ehrmann, Andreas
  id: eaa689ed-f6e0-11ea-865d-bd98cbcf83c2
  last_name: Ehrmann
  orcid: 0000-0002-0997-5678
citation:
  ama: Ehrmann A. Supplemental videos for Designing bistable nanostructures for target
    behavior. 2026. doi:<a href="https://doi.org/10.15479/AT-ISTA-22852">10.15479/AT-ISTA-22852</a>
  apa: Ehrmann, A. (2026). Supplemental videos for Designing bistable nanostructures
    for target behavior. Institute of Science and Technology Austria. <a href="https://doi.org/10.15479/AT-ISTA-22852">https://doi.org/10.15479/AT-ISTA-22852</a>
  chicago: Ehrmann, Andreas. “Supplemental Videos for Designing Bistable Nanostructures
    for Target Behavior.” Institute of Science and Technology Austria, 2026. <a href="https://doi.org/10.15479/AT-ISTA-22852">https://doi.org/10.15479/AT-ISTA-22852</a>.
  ieee: A. Ehrmann, “Supplemental videos for Designing bistable nanostructures for
    target behavior.” Institute of Science and Technology Austria, 2026.
  ista: Ehrmann A. 2026. Supplemental videos for Designing bistable nanostructures
    for target behavior, Institute of Science and Technology Austria, <a href="https://doi.org/10.15479/AT-ISTA-22852">10.15479/AT-ISTA-22852</a>.
  mla: Ehrmann, Andreas. <i>Supplemental Videos for Designing Bistable Nanostructures
    for Target Behavior</i>. Institute of Science and Technology Austria, 2026, doi:<a
    href="https://doi.org/10.15479/AT-ISTA-22852">10.15479/AT-ISTA-22852</a>.
  short: A. Ehrmann, (2026).
contributor:
- contributor_type: data_collector
  first_name: Andreas
  id: eaa689ed-f6e0-11ea-865d-bd98cbcf83c2
  last_name: Ehrmann
  orcid: 0000-0002-0997-5678
corr_author: '1'
date_created: 2026-09-08T11:32:53Z
date_published: 2026-09-09T00:00:00Z
date_updated: 2026-09-09T07:24:10Z
day: '09'
department:
- _id: GradSch
- _id: CaGo
- _id: EdHa
doi: 10.15479/AT-ISTA-22852
doi_confirm: '1'
file:
- access_level: open_access
  checksum: 966417b3eab49523068bb0dfba4ecc07
  content_type: video/mp4
  creator: aehrmann
  date_created: 2026-09-08T11:31:32Z
  date_updated: 2026-09-08T11:31:32Z
  file_id: '22853'
  file_name: Supplemental video 1.mp4
  file_size: 1513964
  relation: main_file
  success: 1
- access_level: open_access
  checksum: deddcae30875bff8e59d5dc9ee3c196f
  content_type: video/mp4
  creator: aehrmann
  date_created: 2026-09-08T11:31:37Z
  date_updated: 2026-09-08T11:31:37Z
  file_id: '22854'
  file_name: Supplemental video 2.mp4
  file_size: 2634179
  relation: main_file
  success: 1
- access_level: open_access
  checksum: 721446b7595edc670d877185637cf15c
  content_type: video/mp4
  creator: aehrmann
  date_created: 2026-09-08T11:31:42Z
  date_updated: 2026-09-08T11:31:42Z
  file_id: '22855'
  file_name: Supplemental video 3.mp4
  file_size: 2080684
  relation: main_file
  success: 1
- access_level: open_access
  checksum: da44153821aa4f8f3cbc2860ef6d1bad
  content_type: video/mp4
  creator: aehrmann
  date_created: 2026-09-08T11:31:48Z
  date_updated: 2026-09-08T11:31:48Z
  file_id: '22856'
  file_name: Supplemental video 4.mp4
  file_size: 4047831
  relation: main_file
  success: 1
- access_level: open_access
  checksum: 1e94cd067809e1a93e21676181b4c102
  content_type: text/plain
  creator: aehrmann
  date_created: 2026-09-08T18:36:14Z
  date_updated: 2026-09-08T18:36:14Z
  file_id: '22860'
  file_name: README.txt
  file_size: 1122
  relation: main_file
  success: 1
file_date_updated: 2026-09-08T18:36:14Z
fulldoi: https://doi.org/10.15479/AT-ISTA-22852
has_accepted_license: '1'
keyword:
- functional nanostructures
- bistability
- target behavior
- transition pathway
license: https://creativecommons.org/licenses/by-nc-sa/4.0/
month: '09'
oa: 1
oa_version: None
project:
- _id: 90a98bb5-16d5-11f0-9cad-9675f3f8015d
  grant_number: PAT 8537123
  name: Functional bio-inspired nanomachines from sticky colloids
publisher: Institute of Science and Technology Austria
status: public
title: Supplemental videos for Designing bistable nanostructures for target behavior
tmp:
  image: /images/cc_by_nc_sa.png
  legal_code_url: https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode
  name: Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC
    BY-NC-SA 4.0)
  short: CC BY-NC-SA (4.0)
type: research_data
user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d
year: '2026'
...
---
OA_type: closed access
_id: '22769'
abstract:
- lang: eng
  text: Using transition metals efficiently in aqueous batteries requires transferring
    multiple electrons per metal, which leads to difficult-to-manage conversion reactions.
    It is now shown how vanadium can be changed from one-electron insertion to four-electron
    conversion.
article_processing_charge: No
article_type: comment
author:
- first_name: Stefan Alexander
  full_name: Freunberger, Stefan Alexander
  id: A8CA28E6-CE23-11E9-AD2D-EC27E6697425
  last_name: Freunberger
  orcid: 0000-0003-2902-5319
citation:
  ama: Freunberger SA. Triggering conversion in vanadium electrodes. <i>Nature Materials</i>.
    2026;25(9):1482-1483. doi:<a href="https://doi.org/10.1038/s41563-026-02714-3">10.1038/s41563-026-02714-3</a>
  apa: Freunberger, S. A. (2026). Triggering conversion in vanadium electrodes. <i>Nature
    Materials</i>. Springer Nature. <a href="https://doi.org/10.1038/s41563-026-02714-3">https://doi.org/10.1038/s41563-026-02714-3</a>
  chicago: Freunberger, Stefan Alexander. “Triggering Conversion in Vanadium Electrodes.”
    <i>Nature Materials</i>. Springer Nature, 2026. <a href="https://doi.org/10.1038/s41563-026-02714-3">https://doi.org/10.1038/s41563-026-02714-3</a>.
  ieee: S. A. Freunberger, “Triggering conversion in vanadium electrodes,” <i>Nature
    Materials</i>, vol. 25, no. 9. Springer Nature, pp. 1482–1483, 2026.
  ista: Freunberger SA. 2026. Triggering conversion in vanadium electrodes. Nature
    Materials. 25(9), 1482–1483.
  mla: Freunberger, Stefan Alexander. “Triggering Conversion in Vanadium Electrodes.”
    <i>Nature Materials</i>, vol. 25, no. 9, Springer Nature, 2026, pp. 1482–83, doi:<a
    href="https://doi.org/10.1038/s41563-026-02714-3">10.1038/s41563-026-02714-3</a>.
  short: S.A. Freunberger, Nature Materials 25 (2026) 1482–1483.
corr_author: '1'
das_tickbox: '0'
date_created: 2026-08-26T18:48:33Z
date_published: 2026-09-01T00:00:00Z
date_updated: 2026-09-09T07:17:13Z
day: '01'
department:
- _id: StFr
doi: 10.1038/s41563-026-02714-3
external_id:
  pmid:
  - '42649374'
fulldoi: https://doi.org/10.1038/s41563-026-02714-3
intvolume: '        25'
issue: '9'
language:
- iso: eng
month: '09'
oa_version: None
page: 1482-1483
pmid: 1
publication: Nature Materials
publication_identifier:
  eissn:
  - 1476-4660
  issn:
  - 1476-1122
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
researchdata_availability: not applicable
scopus_import: '1'
status: public
supplementarymaterial: not applicable
title: Triggering conversion in vanadium electrodes
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 25
year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '22773'
abstract:
- lang: eng
  text: An important quantity in liquid state theory is the radial distribution function
    g(r). It can be calculated within the framework of classical density functional
    theory in two very distinct ways. In the test-particle route, one fixes a single
    fluid particle, turning it into an external potential in which the inhomogeneous
    structure of the fluid is calculated by minimizing the functional. The second
    route to g(r) in density functional theory employs the Ornstein–Zernike equation
    and the pair direct correlation function, that can be obtained from the second
    functional derivatives of the excess (over the ideal gas) free energy functional.
    Since typically an approximate excess free energy functional is employed, the
    test-particle route, which requires only one functional derivative, is more accurate
    than the Ornstein–Zernike route. Here we study a two-dimensional core-shoulder
    particle system and find that in some circumstances the results from the Ornstein–Zernike
    route can be comparable in accuracy to the test-particle results for r > σ, the
    core diameter. We also examine in detail the asymptotic r → ∞ decay of g(r), finding
    a variety of possible decay wavelengths at different state points and state points
    where there is a crossover from one wavelength to a very different one. This behavior
    is a signature pointing to the rich phase behavior of the incipient solid phases.
acknowledgement: We are grateful to Florian Sanmüller and Matthias Schmidt for valuable
  comments on the manuscript and helpful discussions. The simulation results presented
  here were enabled via a generous allocation of CPU time by the Austrian Scientific
  Computing (ASC) under Project No. 71263. The authors thank Katrin Muck for her guidance
  related to the use of HPC. A.J.A. gratefully acknowledges support from the EPSRC
  under Grant No. EP/P015689/1. This research was funded in part by the Austrian Science
  Fund (FWF) under project no. PIN8759524 with Grant-DOI 10.55776/PIN8759524, gratefully
  acknowledged by GK.
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Michael
  full_name: Wassermair, Michael
  id: 23d132c4-4e98-11ef-b275-9e8d4cd8c917
  last_name: Wassermair
  orcid: 0009-0003-6339-4051
- first_name: Gerhard
  full_name: Kahl, Gerhard
  last_name: Kahl
- first_name: Andrew J.
  full_name: Archer, Andrew J.
  last_name: Archer
- first_name: Roland
  full_name: Roth, Roland
  last_name: Roth
citation:
  ama: Wassermair M, Kahl G, Archer AJ, Roth R. Radial distribution function in a
    two-dimensional core-shoulder particle system. <i>Journal of Physical Chemistry
    B</i>. 2026;130(33):8514-8526. doi:<a href="https://doi.org/10.1021/acs.jpcb.6c00653">10.1021/acs.jpcb.6c00653</a>
  apa: Wassermair, M., Kahl, G., Archer, A. J., &#38; Roth, R. (2026). Radial distribution
    function in a two-dimensional core-shoulder particle system. <i>Journal of Physical
    Chemistry B</i>. American Chemical Society. <a href="https://doi.org/10.1021/acs.jpcb.6c00653">https://doi.org/10.1021/acs.jpcb.6c00653</a>
  chicago: Wassermair, Michael, Gerhard Kahl, Andrew J. Archer, and Roland Roth. “Radial
    Distribution Function in a Two-Dimensional Core-Shoulder Particle System.” <i>Journal
    of Physical Chemistry B</i>. American Chemical Society, 2026. <a href="https://doi.org/10.1021/acs.jpcb.6c00653">https://doi.org/10.1021/acs.jpcb.6c00653</a>.
  ieee: M. Wassermair, G. Kahl, A. J. Archer, and R. Roth, “Radial distribution function
    in a two-dimensional core-shoulder particle system,” <i>Journal of Physical Chemistry
    B</i>, vol. 130, no. 33. American Chemical Society, pp. 8514–8526, 2026.
  ista: Wassermair M, Kahl G, Archer AJ, Roth R. 2026. Radial distribution function
    in a two-dimensional core-shoulder particle system. Journal of Physical Chemistry
    B. 130(33), 8514–8526.
  mla: Wassermair, Michael, et al. “Radial Distribution Function in a Two-Dimensional
    Core-Shoulder Particle System.” <i>Journal of Physical Chemistry B</i>, vol. 130,
    no. 33, American Chemical Society, 2026, pp. 8514–26, doi:<a href="https://doi.org/10.1021/acs.jpcb.6c00653">10.1021/acs.jpcb.6c00653</a>.
  short: M. Wassermair, G. Kahl, A.J. Archer, R. Roth, Journal of Physical Chemistry
    B 130 (2026) 8514–8526.
corr_author: '1'
das_tickbox: '0'
date_created: 2026-08-30T22:01:44Z
date_published: 2026-08-20T00:00:00Z
date_updated: 2026-09-09T11:11:12Z
day: '20'
ddc:
- '530'
- '540'
department:
- _id: AnSa
doi: 10.1021/acs.jpcb.6c00653
external_id:
  arxiv:
  - '2603.24537'
  pmid:
  - '42622279'
file:
- access_level: open_access
  checksum: 67313d68ab13b553a38e8b4bf99983d2
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-09T11:05:02Z
  date_updated: 2026-09-09T11:05:02Z
  file_id: '22871'
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  file_size: 7472078
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T11:05:02Z
fulldoi: https://doi.org/10.1021/acs.jpcb.6c00653
has_accepted_license: '1'
intvolume: '       130'
issue: '33'
language:
- iso: eng
month: '08'
oa: 1
oa_version: Published Version
page: 8514-8526
pmid: 1
publication: Journal of Physical Chemistry B
publication_identifier:
  eissn:
  - 1520-5207
  issn:
  - 1520-6106
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Radial distribution function in a two-dimensional core-shoulder particle system
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: 130
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '22815'
abstract:
- lang: eng
  text: The mass assembly and chemical enrichment of the first galaxies provide key
    insights into their star formation histories and the earliest stellar populations
    at cosmic dawn. Here we compile and utilise new, high-quality spectroscopic JWST/NIRSpec
    Prism observations from the JWST archive. In particular, we extend the wavelength
    coverage beyond the standard pipeline cut-off (5.3 μm) up to 5.5 μm, which enables
    for the first time a detailed examination of the rest-frame optical emission-line
    properties for galaxies at z ≈ 10. Crucially, the improved calibration allows
    us to detect Hβ and the [O III] λλ4959, 5007 doublet and resolve the auroral [O III]
    λ4363 line for the 11 galaxies in our sample (z = 9.3 − 10.0) to obtain direct
    Te-based metallicity measurements. We find that the interstellar medium (ISM)
    of all galaxies shows high ionisation fields and electron temperatures, with derived
    metallicities in the range 12 + log(O/H) = 7.1 − 8.3 (3–50% solar), consistent
    with previous strong-line diagnostics based on JWST data at high redshifts. We
    derive an empirical relation for MUV and 12 + log(O/H) at z ≈ 10, useful for future
    higher-redshift studies, and show that the sample galaxies are ‘typical’ star-forming
    galaxies though with relatively high specific star formation rates (median sSFR
    = SFRHβ/M★ = 38 Gyr−1) and with evidence of bursty star formation on 10 Myr versus
    100 Myr timescales (log10(SFR10/SFR100)≈0.7). Combining the rest-frame optical
    line analysis and detailed UV to optical spectro-photometric modelling, we determine
    the mass-metallicity relation (MZR) and the fundamental metallicity relation (FMR)
    of the sample, pushing the previous redshift frontier of these measurements to
    z = 10. These results, together with literature measurements, point to a gradually
    decreasing MZR at higher redshifts, with a break in the FMR at z ≈ 3, decreasing
    to metallicities ≈3× lower at z = 10 than observed in galaxies during the majority
    of cosmic time at z = 0 − 3, likely caused by massive pristine gas inflows diluting
    the observed metal abundances during early galaxy assembly at cosmic dawn.
acknowledgement: We would like to thank the referee for providing a comprehensive
  and constructive report, greatly improving the results presented in this work. We
  further express our greatest gratitude to the investigators on the major JWST observing
  programs, such as RUBIES, CAPERS, UNCOVER, and JADES. The work presented here would
  not have been possible without their major efforts in designing and obtaining the
  observational data included in our work here. The Cosmic Dawn Center (DAWN) is funded
  by the Danish National Research Foundation under grant DNRF140. The data products
  presented herein were retrieved from the DAWN JWST Archive (DJA). DJA is an initiative
  of the Cosmic Dawn Center, which is funded by the Danish National Research Foundation
  under grant DNRF140. This work has received funding from the Swiss State Secretariat
  for Education, Research and Innovation (SERI) under contract number MB22.00072,
  as well as from the Swiss National Science Foundation (SNSF) through project grant
  200020_207349. This work is based in part on observations made with the NASA/ESA/CSA
  James Webb Space Telescope. The data were obtained from the Mikulski Archive for
  Space Telescopes (MAST) at the Space Telescope Science Institute, which is operated
  by the Association of Universities for Research in Astronomy, Inc., under NASA contract
  NAS 5-03127 for JWST. Software used in this work includes MATPLOTLIB (Hunter 2007),
  NUMPY (Harris et al. 2020), SCIPY (Virtanen et al. 2020), and ASTROPY (Astropy Collaboration
  2013).
article_number: A203
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Clara L.
  full_name: Pollock, Clara L.
  last_name: Pollock
- first_name: Rashmi
  full_name: Gottumukkala, Rashmi
  last_name: Gottumukkala
- first_name: Kasper E.
  full_name: Heintz, Kasper E.
  last_name: Heintz
- first_name: Gabriel B.
  full_name: Brammer, Gabriel B.
  last_name: Brammer
- 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: Joris
  full_name: Witstok, Joris
  last_name: Witstok
- first_name: Karla Z.
  full_name: Arellano-Córdova, Karla Z.
  last_name: Arellano-Córdova
- first_name: Fergus
  full_name: Cullen, Fergus
  last_name: Cullen
- first_name: Dirk
  full_name: Scholte, Dirk
  last_name: Scholte
- first_name: Chamilla
  full_name: Terp, Chamilla
  last_name: Terp
- first_name: Lucie
  full_name: Rowland, Lucie
  last_name: Rowland
- first_name: Albert
  full_name: Sneppen, Albert
  last_name: Sneppen
- first_name: Kei
  full_name: Ito, Kei
  last_name: Ito
- first_name: Francesco
  full_name: Valentino, Francesco
  last_name: Valentino
- 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: Darach
  full_name: Watson, Darach
  last_name: Watson
- first_name: Sune
  full_name: Toft, Sune
  last_name: Toft
citation:
  ama: Pollock CL, Gottumukkala R, Heintz KE, et al. Novel z ∼ 10 auroral line measurements
    extend the gradual offset of the fundamental metallicity relation deep into the
    first gigayear of cosmic time. <i>Astronomy &#38; Astrophysics</i>. 2026;708.
    doi:<a href="https://doi.org/10.1051/0004-6361/202556032">10.1051/0004-6361/202556032</a>
  apa: Pollock, C. L., Gottumukkala, R., Heintz, K. E., Brammer, G. B., Roberts-Borsani,
    G., Oesch, P. A., … Toft, S. (2026). Novel z ∼ 10 auroral line measurements extend
    the gradual offset of the fundamental metallicity relation deep into the first
    gigayear of cosmic time. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a
    href="https://doi.org/10.1051/0004-6361/202556032">https://doi.org/10.1051/0004-6361/202556032</a>
  chicago: Pollock, Clara L., Rashmi Gottumukkala, Kasper E. Heintz, Gabriel B. Brammer,
    Guido Roberts-Borsani, Pascal A. Oesch, Joris Witstok, et al. “Novel z ∼ 10 Auroral
    Line Measurements Extend the Gradual Offset of the Fundamental Metallicity Relation
    Deep into the First Gigayear of Cosmic Time.” <i>Astronomy &#38; Astrophysics</i>.
    EDP Sciences, 2026. <a href="https://doi.org/10.1051/0004-6361/202556032">https://doi.org/10.1051/0004-6361/202556032</a>.
  ieee: C. L. Pollock <i>et al.</i>, “Novel z ∼ 10 auroral line measurements extend
    the gradual offset of the fundamental metallicity relation deep into the first
    gigayear of cosmic time,” <i>Astronomy &#38; Astrophysics</i>, vol. 708. EDP Sciences,
    2026.
  ista: Pollock CL, Gottumukkala R, Heintz KE, Brammer GB, Roberts-Borsani G, Oesch
    PA, Witstok J, Arellano-Córdova KZ, Cullen F, Scholte D, Terp C, Rowland L, Sneppen
    A, Ito K, Valentino F, Matthee JJ, Watson D, Toft S. 2026. Novel z ∼ 10 auroral
    line measurements extend the gradual offset of the fundamental metallicity relation
    deep into the first gigayear of cosmic time. Astronomy &#38; Astrophysics. 708,
    A203.
  mla: Pollock, Clara L., et al. “Novel z ∼ 10 Auroral Line Measurements Extend the
    Gradual Offset of the Fundamental Metallicity Relation Deep into the First Gigayear
    of Cosmic Time.” <i>Astronomy &#38; Astrophysics</i>, vol. 708, A203, EDP Sciences,
    2026, doi:<a href="https://doi.org/10.1051/0004-6361/202556032">10.1051/0004-6361/202556032</a>.
  short: C.L. Pollock, R. Gottumukkala, K.E. Heintz, G.B. Brammer, G. Roberts-Borsani,
    P.A. Oesch, J. Witstok, K.Z. Arellano-Córdova, F. Cullen, D. Scholte, C. Terp,
    L. Rowland, A. Sneppen, K. Ito, F. Valentino, J.J. Matthee, D. Watson, S. Toft,
    Astronomy &#38; Astrophysics 708 (2026).
das_tickbox: '0'
date_created: 2026-09-06T22:01:56Z
date_published: 2026-04-01T00:00:00Z
date_updated: 2026-09-09T12:07:45Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202556032
external_id:
  arxiv:
  - '2506.15779'
file:
- access_level: open_access
  checksum: 4ab5af6fac257723afe2b7cf9fcbfa4c
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-09T12:03:50Z
  date_updated: 2026-09-09T12:03:50Z
  file_id: '22874'
  file_name: 2026_AstronomyAstrophysics_Pollock.pdf
  file_size: 1854789
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T12:03:50Z
fulldoi: https://doi.org/10.1051/0004-6361/202556032
has_accepted_license: '1'
intvolume: '       708'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
  eissn:
  - 1432-0746
  issn:
  - 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: no
title: Novel z ∼ 10 auroral line measurements extend the gradual offset of the fundamental
  metallicity relation deep into the first gigayear of cosmic time
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: 708
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '22772'
abstract:
- lang: eng
  text: The cytoplasmic antiviral sensor MDA5 is activated by double-stranded RNAs.
    Endogenous double-stranded RNAs are modified by the A-to-I RNA-editing ADAR family
    to prevent activation of MDA5. In vivo, cytoplasmic ADAR1p150 is critically required
    to suppress MDA5 activation, yet the editing signature of all ADAR isoforms is
    strongly overlapping in mice. Further, it is not clear how A-to-I modifications
    in dsRNA prevent MDA5 activation. Here we show that 3′ UTRs harboring inverted
    repeats activate MDA5 in vitro and in cells. In vitro editing by either ADAR isoform
    leads to editing at overlapping hotspot regions and prevents MDA5 activation in
    vitro and in cells. Remarkably, only inosines introduced by RNA editing are capable
    of suppressing MDA5 activation, while replacing guanosines with inosines during
    in vitro transcription has no impact on MDA5 activation. A comparison of inosines
    introduced by ADAR1p150 in vitro, in cells, and in vivo suggests that a small
    number of A-to-I conversions may be critically required to suppress MDA5 activation.
    As those critical editing events are predominantly altering A:U basepairs into
    I:U wobble basepairs, we suggest that the helical distortion introduced by those
    wobble pairs may prevent MDA5 polymerization and thus downstream activation of
    the type I interferon response.
acknowledgement: This work was supported by Austrian Science Fund project F80-07 to
  M.F.J., F80-03 to C.B., and ZK57-B28 to C.V.; National Health and Medical Research
  Council Australia (NHMRC; GNT2018098 to C.R.W.). The work was supported in part
  by the Victorian State Government Operational Infrastructure Support Scheme to St
  Vincent’s Institute and Hudson Institute of Medical Research. R.V. and A.L. were
  supported by Doc Fund/DOC32 of the Austrian Science Fund. Funding to pay the Open
  Access publication charges for this article was provided by Austrian Science Fund.
  For open access purposes, the author has applied a CC BY public copyright license
  to any author accepted manuscript version arising from this submission.
article_number: gkag845
article_processing_charge: Yes
article_type: original
author:
- first_name: Rajagopal
  full_name: Varada, Rajagopal
  last_name: Varada
- first_name: Alina F.
  full_name: Leuchtenberger, Alina F.
  last_name: Leuchtenberger
- first_name: Cornelia
  full_name: Vesely, Cornelia
  last_name: Vesely
- first_name: Beata M
  full_name: Kaczmarek, Beata M
  id: 36FA4AFA-F248-11E8-B48F-1D18A9856A87
  last_name: Kaczmarek
- first_name: Hamid
  full_name: Mansouri Khosravi, Hamid
  last_name: Mansouri Khosravi
- first_name: Therese C.
  full_name: Mandl, Therese C.
  last_name: Mandl
- first_name: Katarina
  full_name: Milanovic, Katarina
  last_name: Milanovic
- first_name: Kasra
  full_name: Honarmand Tamizkar, Kasra
  last_name: Honarmand Tamizkar
- first_name: Vinod
  full_name: Rajendra, Vinod
  last_name: Rajendra
- first_name: Hannes
  full_name: Senoner, Hannes
  last_name: Senoner
- first_name: Linda
  full_name: Steinbichl, Linda
  last_name: Steinbichl
- first_name: Marija
  full_name: Borojevic, Marija
  last_name: Borojevic
- first_name: Andy
  full_name: Sombke, Andy
  last_name: Sombke
- first_name: Katy
  full_name: Schmidt, Katy
  last_name: Schmidt
- first_name: Margret
  full_name: Eckhard, Margret
  last_name: Eckhard
- first_name: Ivo L.
  full_name: Hofacker, Ivo L.
  last_name: Hofacker
- first_name: Carl
  full_name: Walkley, Carl
  last_name: Walkley
- first_name: Jacki E.
  full_name: Heraud-Farlow, Jacki E.
  last_name: Heraud-Farlow
- first_name: Ernesto
  full_name: Picardi, Ernesto
  last_name: Picardi
- first_name: Carrie A
  full_name: Bernecky, Carrie A
  id: 2CB9DFE2-F248-11E8-B48F-1D18A9856A87
  last_name: Bernecky
  orcid: 0000-0003-0893-7036
- first_name: Michael F.
  full_name: Jantsch, Michael F.
  last_name: Jantsch
citation:
  ama: Varada R, Leuchtenberger AF, Vesely C, et al. Distinguishing self from non-self
    RNA by editing-specific inosine patterns. <i>Nucleic Acids Research</i>. 2026;54(16).
    doi:<a href="https://doi.org/10.1093/nar/gkag845">10.1093/nar/gkag845</a>
  apa: Varada, R., Leuchtenberger, A. F., Vesely, C., Kaczmarek, B. M., Mansouri Khosravi,
    H., Mandl, T. C., … Jantsch, M. F. (2026). Distinguishing self from non-self RNA
    by editing-specific inosine patterns. <i>Nucleic Acids Research</i>. Oxford University
    Press. <a href="https://doi.org/10.1093/nar/gkag845">https://doi.org/10.1093/nar/gkag845</a>
  chicago: Varada, Rajagopal, Alina F. Leuchtenberger, Cornelia Vesely, Beata M Kaczmarek,
    Hamid Mansouri Khosravi, Therese C. Mandl, Katarina Milanovic, et al. “Distinguishing
    Self from Non-Self RNA by Editing-Specific Inosine Patterns.” <i>Nucleic Acids
    Research</i>. Oxford University Press, 2026. <a href="https://doi.org/10.1093/nar/gkag845">https://doi.org/10.1093/nar/gkag845</a>.
  ieee: R. Varada <i>et al.</i>, “Distinguishing self from non-self RNA by editing-specific
    inosine patterns,” <i>Nucleic Acids Research</i>, vol. 54, no. 16. Oxford University
    Press, 2026.
  ista: Varada R, Leuchtenberger AF, Vesely C, Kaczmarek BM, Mansouri Khosravi H,
    Mandl TC, Milanovic K, Honarmand Tamizkar K, Rajendra V, Senoner H, Steinbichl
    L, Borojevic M, Sombke A, Schmidt K, Eckhard M, Hofacker IL, Walkley C, Heraud-Farlow
    JE, Picardi E, Bernecky C, Jantsch MF. 2026. Distinguishing self from non-self
    RNA by editing-specific inosine patterns. Nucleic Acids Research. 54(16), gkag845.
  mla: Varada, Rajagopal, et al. “Distinguishing Self from Non-Self RNA by Editing-Specific
    Inosine Patterns.” <i>Nucleic Acids Research</i>, vol. 54, no. 16, gkag845, Oxford
    University Press, 2026, doi:<a href="https://doi.org/10.1093/nar/gkag845">10.1093/nar/gkag845</a>.
  short: R. Varada, A.F. Leuchtenberger, C. Vesely, B.M. Kaczmarek, H. Mansouri Khosravi,
    T.C. Mandl, K. Milanovic, K. Honarmand Tamizkar, V. Rajendra, H. Senoner, L. Steinbichl,
    M. Borojevic, A. Sombke, K. Schmidt, M. Eckhard, I.L. Hofacker, C. Walkley, J.E.
    Heraud-Farlow, E. Picardi, C. Bernecky, M.F. Jantsch, Nucleic Acids Research 54
    (2026).
das_tickbox: '1'
dataavailabilitystatement: "Sequencing data has been deposited at GEO and is available
  under accession number GSE293616.\r\nEditing analysis of protected dsRNA is available
  in GitHub, https://github.com/BioinfoUNIBA/Mouse-dsRNA-mda5, and Zenodo, https://doi.org/10.5281/zenodo.17876716."
date_created: 2026-08-30T22:01:44Z
date_published: 2026-09-09T00:00:00Z
date_updated: 2026-09-09T11:31:04Z
day: '09'
ddc:
- '570'
department:
- _id: CaBe
- _id: GradSch
doi: 10.1093/nar/gkag845
external_id:
  pmid:
  - '42635125'
file:
- access_level: open_access
  checksum: 319904a237f73dcc55daa4a56baa98fa
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-09T11:29:49Z
  date_updated: 2026-09-09T11:29:49Z
  file_id: '22872'
  file_name: 2026_NucleicAcidsResearch_Varada.pdf
  file_size: 6016116
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T11:29:49Z
fulldoi: https://doi.org/10.1093/nar/gkag845
has_accepted_license: '1'
intvolume: '        54'
issue: '16'
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 8dc144d4-16d5-11f0-9cad-9d9e86aea1f7
  grant_number: F8003
  name: 'RNAdeco: decorating RNA for a purpose/ P03- Roles of A-to-I editing in dsRNA
    recognition'
publication: Nucleic Acids Research
publication_identifier:
  eissn:
  - 1362-4962
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
researchdata_availability: yes
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Distinguishing self from non-self RNA by editing-specific inosine patterns
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
_id: '22814'
abstract:
- lang: eng
  text: "We present a study of a pseudo little red dot with no metal lines (Pseudo-LRD-NOM),
    a highly magnified lowmass galaxy behind the lensing cluster A370 at z = 5.96.
    We classify this object as a pseudo-LRD because its red\r\nrest-frame optical
    color is contaminated by a prominent Hα line (with EW0 ≳ 800 Å) present in its
    JWST\r\nNIRSpec spectrum. Hα is dominated by a narrow component and also has a
    minor broad component indicative of\r\nan active black hole with MBH ≈ 5.6 × 10^6
    M⊙. A narrow Hβ emission line is also detected (where the signal-tonoise ratio,
    S/N, is 8), producing a Balmer decrement (narrow) Hα/Hβ = 11. The rest-frame UV
    spectral slope is ßspec/uv = - 1.20 ± 0.28. All these features can be ascribed
    to high dust attenuation. However, no [O III]λ5007 or\r\nany other metal lines
    are detected in the spectrum, so [O III]5007/Hβ < 0.25, at odds with a simple
    dust attenuation explanation. Accounting for all the spectral properties requires
    the model of a starburst with moderate\r\ncolor excess E(B − V )≈0.2–0.5, high
    gas density (nH ≳ 10^6 cm^−3\r\n), and low- to extremely-low gas/stellar\r\nmetallicities
    (Z = 0.01–0.1 Z⊙). The demagnified stellar mass is\r\n× 2.25+\r\n0\r\n1\r\n.\r\n.\r\n8\r\n3\r\n3\r\n0
    10^7 M , and the stellar-mass surface\r\ndensity is = +\r\n* 418 M pc 310\r\n725
    2, similar to that of massive/nuclear star clusters. Pseudo-LRD-NOM provides\r\nevidence
    of massive black-hole growth occurring in a high-density, dusty starburst that
    is at the early stages of its\r\nchemical enrichment, and is likely a precursor
    to a real LRD."
acknowledgement: "We are grateful to Daniela Calzetti, Andrea Ferrara, Kohei Inayoshi,
  Roberto Maiolino, Gabriele Pezzulli, Fengwu Sun, and Z. Yan for useful discussions;
  José M. Diego for providing us the most updated magnification value for our source;
  Raphael Hviding for making his Python package unite public and instructing us regarding
  its use; and Elka Rusta and Stefania Salvadori for providing us their galaxy SED
  models with hybrid Pop III stellar populations. We also thank the anonymous referee
  for a useful and constructive report.\r\n\r\nThis work is based on observations
  made with the NASA/ESA/CSA JWST. 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 the JWST GTO program
  PID 1208. The specific observations analyzed here can be accessed via doi:10.17909/pyr9-5r43.
  Some of the analyzed data products were retrieved from the Dawn JWST Archive (DJA).
  DJA is an initiative of the Cosmic Dawn Center (DAWN), which is funded by the Danish
  National Research Foundation under grant DNRF140. This work is also based on observations
  made with the NASA/ESA Hubble Space Telescope obtained from the Space Telescope
  Science Institute, which is operated by the Association of Universities for Research
  in Astronomy, Inc., under NASA contract NAS 526555.\r\n\r\nK.I.C. and R.N.C. acknowledge
  funding from the Dutch Research Council (NWO) through the award of the Vici grant
  VI.C.212.036."
article_number: '203'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Karina I.
  full_name: Caputi, Karina I.
  last_name: Caputi
- first_name: Ryan A.
  full_name: Cooper, Ryan A.
  last_name: Cooper
- first_name: Pierluigi
  full_name: Rinaldi, Pierluigi
  last_name: Rinaldi
- first_name: Rafael
  full_name: Navarro-Carrera, Rafael
  last_name: Navarro-Carrera
- first_name: Edoardo
  full_name: Iani, Edoardo
  id: 4053390a-6b68-11ef-9828-a3b8adef8d0a
  last_name: Iani
  orcid: 0000-0001-8386-3546
- first_name: Abigail A.
  full_name: Tumborang, Abigail A.
  last_name: Tumborang
citation:
  ama: 'Caputi KI, Cooper RA, Rinaldi P, Navarro-Carrera R, Iani E, Tumborang AA.
    Pseudo Little Red Dot: An active black hole embedded in a dense and dusty, metal-poor
    starburst galaxy at z = 5.96. <i>The Astrophysical Journal</i>. 2026;1007(2).
    doi:<a href="https://doi.org/10.3847/1538-4357/ae80b9">10.3847/1538-4357/ae80b9</a>'
  apa: 'Caputi, K. I., Cooper, R. A., Rinaldi, P., Navarro-Carrera, R., Iani, E.,
    &#38; Tumborang, A. A. (2026). Pseudo Little Red Dot: An active black hole embedded
    in a dense and dusty, metal-poor starburst galaxy at z = 5.96. <i>The Astrophysical
    Journal</i>. IOP Publishing. <a href="https://doi.org/10.3847/1538-4357/ae80b9">https://doi.org/10.3847/1538-4357/ae80b9</a>'
  chicago: 'Caputi, Karina I., Ryan A. Cooper, Pierluigi Rinaldi, Rafael Navarro-Carrera,
    Edoardo Iani, and Abigail A. Tumborang. “Pseudo Little Red Dot: An Active Black
    Hole Embedded in a Dense and Dusty, Metal-Poor Starburst Galaxy at z = 5.96.”
    <i>The Astrophysical Journal</i>. IOP Publishing, 2026. <a href="https://doi.org/10.3847/1538-4357/ae80b9">https://doi.org/10.3847/1538-4357/ae80b9</a>.'
  ieee: 'K. I. Caputi, R. A. Cooper, P. Rinaldi, R. Navarro-Carrera, E. Iani, and
    A. A. Tumborang, “Pseudo Little Red Dot: An active black hole embedded in a dense
    and dusty, metal-poor starburst galaxy at z = 5.96,” <i>The Astrophysical Journal</i>,
    vol. 1007, no. 2. IOP Publishing, 2026.'
  ista: 'Caputi KI, Cooper RA, Rinaldi P, Navarro-Carrera R, Iani E, Tumborang AA.
    2026. Pseudo Little Red Dot: An active black hole embedded in a dense and dusty,
    metal-poor starburst galaxy at z = 5.96. The Astrophysical Journal. 1007(2), 203.'
  mla: 'Caputi, Karina I., et al. “Pseudo Little Red Dot: An Active Black Hole Embedded
    in a Dense and Dusty, Metal-Poor Starburst Galaxy at z = 5.96.” <i>The Astrophysical
    Journal</i>, vol. 1007, no. 2, 203, IOP Publishing, 2026, doi:<a href="https://doi.org/10.3847/1538-4357/ae80b9">10.3847/1538-4357/ae80b9</a>.'
  short: K.I. Caputi, R.A. Cooper, P. Rinaldi, R. Navarro-Carrera, E. Iani, A.A. Tumborang,
    The Astrophysical Journal 1007 (2026).
das_tickbox: '0'
date_created: 2026-09-06T22:01:56Z
date_published: 2026-08-20T00:00:00Z
date_updated: 2026-09-09T12:19:54Z
day: '20'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ae80b9
external_id:
  arxiv:
  - '2601.11466'
file:
- access_level: open_access
  checksum: cf878372382ac61b22f679b558bb4e4e
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-09T12:19:36Z
  date_updated: 2026-09-09T12:19:36Z
  file_id: '22887'
  file_name: 2026_AstrophysicalJour_Caputi.pdf
  file_size: 2636477
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T12:19:36Z
fulldoi: https://doi.org/10.3847/1538-4357/ae80b9
has_accepted_license: '1'
intvolume: '      1007'
issue: '2'
language:
- iso: eng
month: '08'
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'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: no
title: 'Pseudo Little Red Dot: An active black hole embedded in a dense and dusty,
  metal-poor starburst galaxy at z = 5.96'
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: 1007
year: '2026'
...
---
OA_type: closed access
_id: '22812'
abstract:
- lang: eng
  text: Efficient data structures for computing the cutset of a set of nodes in a
    graph undergoing dynamic edge insertions/deletions are well-studied in undirected
    graphs. We study this problem in directed graphs and show a reduction from the
    Online Boolean Matrix-Vector Multiplication Conjecture (OMv) introduced by Henzinger
    et al. [STOC’15]. We prove conditional on OMv that a dynamic data structure computing
    the directed cutset of a set of nodes cannot have an amortized time of both O(n2−ε)
    for a query operation and O(n1−ε) for an update operation, for any constant ε > 0,
    even when an adversary’s operations are restricted to the incremental or decremental
    settings. We further give algorithms to match these lower bounds.
acknowledgement: This project has received funding from the European Union’s Horizon
  2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement
  No. 101034413 and from the European Research Council (ERC) under the European Union’s
  Horizon 2020 research and innovation programme (MoDynStruct, No. 101019564) Image
  1 dummy alt text. Zofia Stefankovic was partially supported by the ISTernship program
  of the Institute of Science and Technology Austria and OEAD.
article_number: '106663'
article_processing_charge: No
article_type: original
author:
- first_name: Niklas
  full_name: Hahn, Niklas
  id: 0a01c7b2-b823-11ed-9928-cc3f874f9ffd
  last_name: Hahn
- first_name: Monika H
  full_name: Henzinger, Monika H
  id: 540c9bbd-f2de-11ec-812d-d04a5be85630
  last_name: Henzinger
  orcid: 0000-0002-5008-6530
- first_name: Zofia
  full_name: Stefankovic, Zofia
  last_name: Stefankovic
citation:
  ama: Hahn N, Henzinger M, Stefankovic Z. Tight bounds on the performance of dynamic
    directed cutset data structures based on OMv. <i>Information Processing Letters</i>.
    2026;195. doi:<a href="https://doi.org/10.1016/j.ipl.2026.106663">10.1016/j.ipl.2026.106663</a>
  apa: Hahn, N., Henzinger, M., &#38; Stefankovic, Z. (2026). Tight bounds on the
    performance of dynamic directed cutset data structures based on OMv. <i>Information
    Processing Letters</i>. Elsevier. <a href="https://doi.org/10.1016/j.ipl.2026.106663">https://doi.org/10.1016/j.ipl.2026.106663</a>
  chicago: Hahn, Niklas, Monika Henzinger, and Zofia Stefankovic. “Tight Bounds on
    the Performance of Dynamic Directed Cutset Data Structures Based on OMv.” <i>Information
    Processing Letters</i>. Elsevier, 2026. <a href="https://doi.org/10.1016/j.ipl.2026.106663">https://doi.org/10.1016/j.ipl.2026.106663</a>.
  ieee: N. Hahn, M. Henzinger, and Z. Stefankovic, “Tight bounds on the performance
    of dynamic directed cutset data structures based on OMv,” <i>Information Processing
    Letters</i>, vol. 195. Elsevier, 2026.
  ista: Hahn N, Henzinger M, Stefankovic Z. 2026. Tight bounds on the performance
    of dynamic directed cutset data structures based on OMv. Information Processing
    Letters. 195, 106663.
  mla: Hahn, Niklas, et al. “Tight Bounds on the Performance of Dynamic Directed Cutset
    Data Structures Based on OMv.” <i>Information Processing Letters</i>, vol. 195,
    106663, Elsevier, 2026, doi:<a href="https://doi.org/10.1016/j.ipl.2026.106663">10.1016/j.ipl.2026.106663</a>.
  short: N. Hahn, M. Henzinger, Z. Stefankovic, Information Processing Letters 195
    (2026).
das_tickbox: '1'
dataavailabilitystatement: No data was used for the research described in the article.
date_created: 2026-09-06T22:01:55Z
date_published: 2026-08-30T00:00:00Z
date_updated: 2026-09-09T11:55:47Z
day: '30'
department:
- _id: MoHe
doi: 10.1016/j.ipl.2026.106663
ec_funded: 1
fulldoi: https://doi.org/10.1016/j.ipl.2026.106663
intvolume: '       195'
keyword:
- Dynamic algorithms
- Graph algorithms
- Directed graphs
- Lower bounds
- Upper bounds
language:
- iso: eng
month: '08'
oa_version: None
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
  call_identifier: H2020
  grant_number: '101034413'
  name: 'IST-BRIDGE: International postdoctoral program'
- _id: bd9ca328-d553-11ed-ba76-dc4f890cfe62
  call_identifier: H2020
  grant_number: '101019564'
  name: The design and evaluation of modern fully dynamic data structures
publication: Information Processing Letters
publication_identifier:
  issn:
  - 0020-0190
publication_status: epub_ahead
publisher: Elsevier
quality_controlled: '1'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: no
title: Tight bounds on the performance of dynamic directed cutset data structures
  based on OMv
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 195
year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '22813'
abstract:
- lang: eng
  text: "Consider a bipartite quantum system, where Alice and Bob jointly possess\r\na
    pure state |ψ\x02. Using local quantum operations on their respective subsystems,
    and\r\nunlimited classical communication, Alice and Bob may be able to transform
    |ψ\x02 into\r\nanother state |φ\x02. Famously, Nielsen’s theorem [28] provides
    a necessary and sufficient\r\nalgebraic criterion for such a transformation to
    be possible (namely, the entanglement\r\nspectrum of |φ\x02 should majorise the
    entanglement spectrum of |ψ\x02). In the paper where\r\nNielsen proved this theorem,
    he conjectured that in the limit of large dimensionality, for\r\nalmost all pairs
    of states |ψ\x02, |φ\x02 (according to the natural unitary invariant measure)
    such\r\na transformation is not possible. That is to say, typical pairs of quantum
    states |ψ\x02, |φ\x02\r\nare entangled in fundamentally different ways, that cannot
    be converted to each other via\r\nlocal operations and classical communication.ViaNielsen’s
    theorem, this conjecture can\r\nbe equivalently stated as a conjecture about majorisation
    of spectra of random matrices\r\nfrom the so-called trace-normalised complex Wishart–Laguerre
    ensemble. Concretely,\r\nlet X and Y be independent n × m random matrices whose
    entries are i.i.d. standard\r\ncomplex Gaussians; then Nielsen’s conjecture says
    that the probability that the spectrum\r\nof XX†/ tr(XX†) majorises the spectrum
    of YY†/ tr(YY†) tends to zero as both n and\r\nm grow large. We prove this conjecture,
    and we also confirm some related predictions\r\nof Cunden et al. [12]."
acknowledgement: Open access funding provided by Institute of Science and Technology
  (IST Austria). Vishesh Jain was partially supported by NSF CAREER award DMS-2237646.
  Matthew Kwan was supported by ERC Starting Grant “RANDSTRUCT” No. 101076777. Marcus
  Michelen was supported in part by NSF grants DMS-2137623 and DMS-2246624.
article_number: '214'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Vishesh
  full_name: Jain, Vishesh
  last_name: Jain
- first_name: Matthew Alan
  full_name: Kwan, Matthew Alan
  id: 5fca0887-a1db-11eb-95d1-ca9d5e0453b3
  last_name: Kwan
  orcid: 0000-0002-4003-7567
- first_name: Marcus
  full_name: Michelen, Marcus
  last_name: Michelen
citation:
  ama: Jain V, Kwan MA, Michelen M. Entangled states are typically incomparable. <i>Communications
    in Mathematical Physics</i>. 2026;407(10). doi:<a href="https://doi.org/10.1007/s00220-026-05711-4">10.1007/s00220-026-05711-4</a>
  apa: Jain, V., Kwan, M. A., &#38; Michelen, M. (2026). Entangled states are typically
    incomparable. <i>Communications in Mathematical Physics</i>. Springer. <a href="https://doi.org/10.1007/s00220-026-05711-4">https://doi.org/10.1007/s00220-026-05711-4</a>
  chicago: Jain, Vishesh, Matthew Alan Kwan, and Marcus Michelen. “Entangled States
    Are Typically Incomparable.” <i>Communications in Mathematical Physics</i>. Springer,
    2026. <a href="https://doi.org/10.1007/s00220-026-05711-4">https://doi.org/10.1007/s00220-026-05711-4</a>.
  ieee: V. Jain, M. A. Kwan, and M. Michelen, “Entangled states are typically incomparable,”
    <i>Communications in Mathematical Physics</i>, vol. 407, no. 10. Springer, 2026.
  ista: Jain V, Kwan MA, Michelen M. 2026. Entangled states are typically incomparable.
    Communications in Mathematical Physics. 407(10), 214.
  mla: Jain, Vishesh, et al. “Entangled States Are Typically Incomparable.” <i>Communications
    in Mathematical Physics</i>, vol. 407, no. 10, 214, Springer, 2026, doi:<a href="https://doi.org/10.1007/s00220-026-05711-4">10.1007/s00220-026-05711-4</a>.
  short: V. Jain, M.A. Kwan, M. Michelen, Communications in Mathematical Physics 407
    (2026).
corr_author: '1'
das_tickbox: '1'
dataavailabilitystatement: No datasets were used in this research.
date_created: 2026-09-06T22:01:56Z
date_published: 2026-08-28T00:00:00Z
date_updated: 2026-09-09T12:35:24Z
day: '28'
ddc:
- '500'
department:
- _id: MaKw
doi: 10.1007/s00220-026-05711-4
external_id:
  arxiv:
  - '2406.03335'
  pmid:
  - '42668663'
file:
- access_level: open_access
  checksum: 61c226b6314a88db25e864e4218d5de3
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-09T12:32:53Z
  date_updated: 2026-09-09T12:32:53Z
  file_id: '22888'
  file_name: 2026_CommMathPhysics_Jain.pdf
  file_size: 463477
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T12:32:53Z
fulldoi: https://doi.org/10.1007/s00220-026-05711-4
has_accepted_license: '1'
intvolume: '       407'
issue: '10'
language:
- iso: eng
month: '08'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: bd95085b-d553-11ed-ba76-e55d3349be45
  grant_number: '101076777'
  name: Randomness and structure in combinatorics
publication: Communications in Mathematical Physics
publication_identifier:
  eissn:
  - 1432-0916
  issn:
  - 0010-3616
publication_status: published
publisher: Springer
quality_controlled: '1'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: no
title: Entangled states are typically incomparable
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: 407
year: '2026'
...
---
OA_place: publisher
OA_type: hybrid
_id: '22818'
abstract:
- lang: eng
  text: 'Physical processes at play in the genesis and evolution of tropical cyclones
    are conducive to the formation of warm cores at their centres. When the warm anomaly
    is particularly large in the upper troposphere, it is referred to as a high-level
    warm core. Previous works documented the generation of high-level warm cores as
    a consequence of stratospheric air intrusion into the troposphere induced by the
    upper-level dynamics of a tropical cyclone. However, little attention has been
    given to their effects on the storm''s subsequent evolution. It has been suggested
    that the presence of a high-level warm core can have opposite effects on tropical
    cyclone intensity: both strengthening and weakening have been described as possible
    consequences of its formation. In this study, we examine the role of high-level
    warm cores in the intensification and dissipation processes of tropical cyclones,
    as reproduced in numerical models of different complexities, namely the model
    “System for Atmospheric Modeling” (SAM) run under idealized conditions and the
    model Nonhydrostatic ICosahedral Atmospheric Model run under realistic conditions
    following the DYnamics of the Atmospheric general circulation Modeled On Non-hydrostatic
    Domains summer protocol. Our results confirm the hypothesis of a stratospheric
    origin behind the formation of high-level warm cores. Their initial role is shown
    to be an enhancement of storm intensity, by a lowering of the hydrostatic sea-level
    pressure (HSLP) associated with the presence of warm air aloft. However, as the
    warm anomaly intensifies and extends to lower levels, it also increases static
    stability in the air column, with the consequence of inhibiting convection and
    ultimately contributing to cyclone dissipation. These findings suggest that high-level
    warm cores play a dual role in the tropical cyclone life cycle, providing a stabilizing
    mechanism that can limit cyclone strength and longevity.'
acknowledgement: "The authors thank Tom Beucler, Hamish Ramsay, and two anonymous
  reviewers for insightful comments and constructive feedback on earlier versions
  of this work.\r\n\r\nThis work is partially funded by the National Recovery and
  Resilience Plan project TeRABIT (Terabit network for Research and Academic Big data
  in Italy—IR0000022—PNRRMissione4—Componente2—Investim ento3.1—CUPI53C21000370006)
  in the frame of the European Union—NextGenerationEU funding. C. Muller gratefully
  acknowledges funding from the European Research Council (ERC) under the European
  Union's Horizon 2020 research and innovation program (Project CLUSTER, Grant 805041).
  This work is an outcome of the project MIUR—Dipartimenti di Eccellenza 2023–2027.\r\n\r\nThis
  work used resources of the Deutsches Klimarechenzentrum (DKRZ) granted by its Scientific
  Steering Committee (WLA) under project bb1153. Open access publishing facilitated
  by Universita degli Studi di Milano-Bicocca, as part of the Wiley - CRUI-CARE agreement."
article_number: e70280
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Andrea
  full_name: Davin, Andrea
  last_name: Davin
- first_name: Giousef Alexandros
  full_name: Charinti, Giousef Alexandros
  id: 7f7cc04c-074c-11ed-af92-eb16afd85c75
  last_name: Charinti
- first_name: Caroline J
  full_name: Muller, Caroline J
  id: f978ccb0-3f7f-11eb-b193-b0e2bd13182b
  last_name: Muller
  orcid: 0000-0001-5836-5350
- first_name: Andrea
  full_name: Polesello, Andrea
  id: 74c777f4-32da-11ee-b498-874db0835561
  last_name: Polesello
- first_name: Claudia
  full_name: Pasquero, Claudia
  last_name: Pasquero
citation:
  ama: Davin A, Charinti GA, Muller CJ, Polesello A, Pasquero C. Stratospheric influence
    on tropical cyclone evolution. <i>Quarterly Journal of the Royal Meteorological
    Society</i>. 2026. doi:<a href="https://doi.org/10.1002/qj.70280">10.1002/qj.70280</a>
  apa: Davin, A., Charinti, G. A., Muller, C. J., Polesello, A., &#38; Pasquero, C.
    (2026). Stratospheric influence on tropical cyclone evolution. <i>Quarterly Journal
    of the Royal Meteorological Society</i>. Wiley. <a href="https://doi.org/10.1002/qj.70280">https://doi.org/10.1002/qj.70280</a>
  chicago: Davin, Andrea, Giousef Alexandros Charinti, Caroline J Muller, Andrea Polesello,
    and Claudia Pasquero. “Stratospheric Influence on Tropical Cyclone Evolution.”
    <i>Quarterly Journal of the Royal Meteorological Society</i>. Wiley, 2026. <a
    href="https://doi.org/10.1002/qj.70280">https://doi.org/10.1002/qj.70280</a>.
  ieee: A. Davin, G. A. Charinti, C. J. Muller, A. Polesello, and C. Pasquero, “Stratospheric
    influence on tropical cyclone evolution,” <i>Quarterly Journal of the Royal Meteorological
    Society</i>. Wiley, 2026.
  ista: Davin A, Charinti GA, Muller CJ, Polesello A, Pasquero C. 2026. Stratospheric
    influence on tropical cyclone evolution. Quarterly Journal of the Royal Meteorological
    Society., e70280.
  mla: Davin, Andrea, et al. “Stratospheric Influence on Tropical Cyclone Evolution.”
    <i>Quarterly Journal of the Royal Meteorological Society</i>, e70280, Wiley, 2026,
    doi:<a href="https://doi.org/10.1002/qj.70280">10.1002/qj.70280</a>.
  short: A. Davin, G.A. Charinti, C.J. Muller, A. Polesello, C. Pasquero, Quarterly
    Journal of the Royal Meteorological Society (2026).
das_tickbox: '1'
dataavailabilitystatement: The data that support the findings of this study are available
  from the corresponding author upon reasonable request.
date_created: 2026-09-06T22:01:57Z
date_published: 2026-08-26T00:00:00Z
date_updated: 2026-09-09T12:43:30Z
day: '26'
ddc:
- '550'
department:
- _id: CaMu
- _id: GradSch
doi: 10.1002/qj.70280
ec_funded: 1
fulldoi: https://doi.org/10.1002/qj.70280
has_accepted_license: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1002/qj.70280
month: '08'
oa: 1
oa_version: Published Version
project:
- _id: 629205d8-2b32-11ec-9570-e1356ff73576
  call_identifier: H2020
  grant_number: '805041'
  name: Organization of CLoUdS, and implications of Tropical  cyclones and for the
    Energetics of the tropics, in current and waRming climate
publication: Quarterly Journal of the Royal Meteorological Society
publication_identifier:
  eissn:
  - 1477-870X
  issn:
  - 0035-9009
publication_status: epub_ahead
publisher: Wiley
quality_controlled: '1'
researchdata_availability: upon request
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Stratospheric influence on tropical cyclone evolution
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '22817'
abstract:
- lang: eng
  text: Using deep, medium-resolution, JWST rest-optical spectra of a sample of typical
    star-forming galaxies (Lyman-break galaxies and Lyman-α emitters) from the LyC22
    survey at z ∼ 3, we determined the nebular abundances of N, O, and Ne relative
    to H for a subsample of 25 objects with a direct method based on auroral [O III]
    λ4363 line detections. Our measurements increased the number of accurate N/O determinations
    at z ∼ 2 − 4 using a homogeneous approach. We found a mean value of log(N/O) =
    −+0.25−0.21 over a metallicity range of 12 + log(O/H) = 7.56 to 8.44. The observed
    N/O ratio and scatter are indistinguishable from that observed in low-z galaxies
    and H II regions over the same metallicity range, thus showing no redshift evolution
    of N/O for typical galaxies over a significant fraction of cosmic time. We also
    show that typical z ∼ 3 galaxies have a similar offset in the BPT diagram to galaxies
    from the low-z Lyman Continuum Survey (LzLCS) when compared to the average of
    SDSS galaxies, and we demonstrate that this offset is not due to enhanced nitrogen
    abundances. Our results establish a basis for future studies of the evolution
    of N and O at higher redshifts.
acknowledgement: "Y.I., N.G., R.M.-C., and D.S. acknowledge support from\r\nproject
  No. 224866 carried out in the framework of the Joint Call “UkrainianSwiss Joint
  Research Projects: Call for Proposals 2023”. This work is based in\r\npart on observations
  made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from
  the Mikulski Archive for Space Telescopes\r\nat the Space Telescope Science Institute,
  which is operated by the Association\r\nof Universities for Research in Astronomy,
  Inc., under NASA contract NAS 5-\r\n03127 for JWST. These observations are associated
  with program # 1869. Support for program # 1869 was provided by NASA through a grant
  from the Space\r\nTelescope Science Institute, which is operated by the Association
  of Universities\r\nfor Research in Astronomy, Inc., under NASA contract NAS 5-03127"
article_number: A242
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: D.
  full_name: Schaerer, D.
  last_name: Schaerer
- first_name: Y. I.
  full_name: Izotov, Y. I.
  last_name: Izotov
- first_name: R.
  full_name: Marques-Chaves, R.
  last_name: Marques-Chaves
- first_name: C. C.
  full_name: Steidel, C. C.
  last_name: Steidel
- first_name: N.
  full_name: Reddy, N.
  last_name: Reddy
- first_name: A. E.
  full_name: Shapley, A. E.
  last_name: Shapley
- first_name: Sara
  full_name: Mascia, Sara
  id: edaf889c-c7cd-11ef-ab1b-bb28c431bd29
  last_name: Mascia
- first_name: J.
  full_name: Chisholm, J.
  last_name: Chisholm
- first_name: S. R.
  full_name: Flury, S. R.
  last_name: Flury
- first_name: N.
  full_name: Guseva, N.
  last_name: Guseva
- first_name: T.
  full_name: Heckman, T.
  last_name: Heckman
- first_name: A.
  full_name: Henry, A.
  last_name: Henry
- first_name: A. K.
  full_name: Inoue, A. K.
  last_name: Inoue
- first_name: I.
  full_name: Jung, I.
  last_name: Jung
- first_name: H.
  full_name: Kusakabe, H.
  last_name: Kusakabe
- first_name: K.
  full_name: Mawatari, K.
  last_name: Mawatari
- first_name: P.
  full_name: Oesch, P.
  last_name: Oesch
- first_name: G.
  full_name: Östlin, G.
  last_name: Östlin
- first_name: L.
  full_name: Pentericci, L.
  last_name: Pentericci
- first_name: N.
  full_name: Roy, N.
  last_name: Roy
- first_name: A.
  full_name: Saldana-Lopez, A.
  last_name: Saldana-Lopez
- first_name: R.
  full_name: Sato, R.
  last_name: Sato
- first_name: E.
  full_name: Vanzella, E.
  last_name: Vanzella
- first_name: A.
  full_name: Verhamme, A.
  last_name: Verhamme
- first_name: B.
  full_name: Wang, B.
  last_name: Wang
citation:
  ama: Schaerer D, Izotov YI, Marques-Chaves R, et al. Nitrogen abundances in star-forming
    galaxies 2.2 Gyr after the Big Bang are not elevated. <i>Astronomy &#38; Astrophysics</i>.
    2026;708. doi:<a href="https://doi.org/10.1051/0004-6361/202556832">10.1051/0004-6361/202556832</a>
  apa: Schaerer, D., Izotov, Y. I., Marques-Chaves, R., Steidel, C. C., Reddy, N.,
    Shapley, A. E., … Wang, B. (2026). Nitrogen abundances in star-forming galaxies
    2.2 Gyr after the Big Bang are not elevated. <i>Astronomy &#38; Astrophysics</i>.
    EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/202556832">https://doi.org/10.1051/0004-6361/202556832</a>
  chicago: Schaerer, D., Y. I. Izotov, R. Marques-Chaves, C. C. Steidel, N. Reddy,
    A. E. Shapley, Sara Mascia, et al. “Nitrogen Abundances in Star-Forming Galaxies
    2.2 Gyr after the Big Bang Are Not Elevated.” <i>Astronomy &#38; Astrophysics</i>.
    EDP Sciences, 2026. <a href="https://doi.org/10.1051/0004-6361/202556832">https://doi.org/10.1051/0004-6361/202556832</a>.
  ieee: D. Schaerer <i>et al.</i>, “Nitrogen abundances in star-forming galaxies 2.2
    Gyr after the Big Bang are not elevated,” <i>Astronomy &#38; Astrophysics</i>,
    vol. 708. EDP Sciences, 2026.
  ista: Schaerer D, Izotov YI, Marques-Chaves R, Steidel CC, Reddy N, Shapley AE,
    Mascia S, Chisholm J, Flury SR, Guseva N, Heckman T, Henry A, Inoue AK, Jung I,
    Kusakabe H, Mawatari K, Oesch P, Östlin G, Pentericci L, Roy N, Saldana-Lopez
    A, Sato R, Vanzella E, Verhamme A, Wang B. 2026. Nitrogen abundances in star-forming
    galaxies 2.2 Gyr after the Big Bang are not elevated. Astronomy &#38; Astrophysics.
    708, A242.
  mla: Schaerer, D., et al. “Nitrogen Abundances in Star-Forming Galaxies 2.2 Gyr
    after the Big Bang Are Not Elevated.” <i>Astronomy &#38; Astrophysics</i>, vol.
    708, A242, EDP Sciences, 2026, doi:<a href="https://doi.org/10.1051/0004-6361/202556832">10.1051/0004-6361/202556832</a>.
  short: D. Schaerer, Y.I. Izotov, R. Marques-Chaves, C.C. Steidel, N. Reddy, A.E.
    Shapley, S. Mascia, J. Chisholm, S.R. Flury, N. Guseva, T. Heckman, A. Henry,
    A.K. Inoue, I. Jung, H. Kusakabe, K. Mawatari, P. Oesch, G. Östlin, L. Pentericci,
    N. Roy, A. Saldana-Lopez, R. Sato, E. Vanzella, A. Verhamme, B. Wang, Astronomy
    &#38; Astrophysics 708 (2026).
das_tickbox: '1'
dataavailabilitystatement: "The data used are publicly available at the Mikulski Archive
  for Space Telescope (MAST),\r\nand can be accessed at https://dx.doi.org/10.17909/x6d5-vd44."
date_created: 2026-09-06T22:01:57Z
date_published: 2026-04-01T00:00:00Z
date_updated: 2026-09-09T12:59:51Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202556832
external_id:
  arxiv:
  - '2601.06968'
file:
- access_level: open_access
  checksum: 94cc1327f363d69995984b06e18e2645
  content_type: application/pdf
  creator: dernst
  date_created: 2026-09-09T12:55:37Z
  date_updated: 2026-09-09T12:55:37Z
  file_id: '22890'
  file_name: 2026_AstronomyAstrophysics_Schaerer.pdf
  file_size: 591297
  relation: main_file
  success: 1
file_date_updated: 2026-09-09T12:55:37Z
fulldoi: https://doi.org/10.1051/0004-6361/202556832
has_accepted_license: '1'
intvolume: '       708'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
  eissn:
  - 1432-0746
  issn:
  - 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
researchdata_availability: yes
scopus_import: '1'
status: public
supplementarymaterial: no
title: Nitrogen abundances in star-forming galaxies 2.2 Gyr after the Big Bang are
  not elevated
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: 708
year: '2026'
...
---
OA_type: closed access
_id: '22819'
abstract:
- lang: eng
  text: Bio-inspired photonic synapses integrate optical sensing, memory, and processing
    in a single platform, overcoming the bottlenecks of traditional CMOS-based vision
    sensors. Most existing neuromorphic vision systems either rely on electrical inputs
    for bidirectional conductance modulation, limiting their operating speed and bandwidth,
    or lack nonvolatility, leading to nonlinear weight updates and poor efficiency
    in image recognition tasks. Here, we report a two-terminal, fully light-controlled
    synaptic memristor based on CsPbBr3/ZnO nanorod heterojunction that demonstrates
    4-bit memory storage and optical logic operations within a single architecture.
    The device emulates essential functions of both excitatory and inhibitory synapses,
    utilizing positive photoconductivity under UV illumination (λ = 375 nm) and anomalous
    negative photoconductivity under visible light (λ = 450 nm). By controlling defect
    concentrations at the CsPbBr3/ZnO nanorod interface, the device exhibits nonvolatile
    multibit memory with near-linear, symmetric conductance modulation, achieving
    92.4% image recognition accuracy with a convolutional neural network. The bidirectional
    photoresponse enables reconfigurable optical logic operations, demonstrating integrated
    logic-in-memory. Additionally, when integrated on a flexible platform, the device
    demonstrates stable synaptic performance under repeated mechanical bending. These
    results highlight the potential of CsPbBr3/ZnO nanorod heterojunction-based all-photonic
    synapses as building blocks for multibit storage, optical information processing,
    and wearable neuromorphic vision systems.
acknowledgement: SS sincerely acknowledges the fellowship received from the Ministryof
  Education, Government of India, to carry out this research. SKRacknowledges the
  financial support from DST Nano-mission (Projectno. DST/NM/TUE/QM8 2019G 5). The
  authors also thank the CentralResearch Facility (CRF) at IIT Kharagpur for providing
  the characteriza-tion tools.
article_number: e75437
article_processing_charge: No
author:
- first_name: Subham
  full_name: Saha, Subham
  last_name: Saha
- first_name: Shreyasi
  full_name: Das, Shreyasi
  id: c102f9d5-4f26-11ef-94d5-9047d2a9105b
  last_name: Das
- first_name: Baidyanath
  full_name: Roy, Baidyanath
  last_name: Roy
- first_name: Santu Kumar
  full_name: Ghosh, Santu Kumar
  last_name: Ghosh
- first_name: Rohit
  full_name: Satpathy, Rohit
  last_name: Satpathy
- first_name: James
  full_name: Bullock, James
  last_name: Bullock
- first_name: Ranjith R.
  full_name: Unnithan, Ranjith R.
  last_name: Unnithan
- first_name: Samit K.
  full_name: Ray, Samit K.
  last_name: Ray
citation:
  ama: Saha S, Das S, Roy B, et al. Interface engineered perovskite-oxide heterojunction
    all-photonic synapses for multibit memory, optical logic, and wearable neuromorphic
    vision. <i>Small</i>. 2026. doi:<a href="https://doi.org/10.1002/smll.75437">10.1002/smll.75437</a>
  apa: Saha, S., Das, S., Roy, B., Ghosh, S. K., Satpathy, R., Bullock, J., … Ray,
    S. K. (2026). Interface engineered perovskite-oxide heterojunction all-photonic
    synapses for multibit memory, optical logic, and wearable neuromorphic vision.
    <i>Small</i>. Wiley. <a href="https://doi.org/10.1002/smll.75437">https://doi.org/10.1002/smll.75437</a>
  chicago: Saha, Subham, Shreyasi Das, Baidyanath Roy, Santu Kumar Ghosh, Rohit Satpathy,
    James Bullock, Ranjith R. Unnithan, and Samit K. Ray. “Interface Engineered Perovskite-Oxide
    Heterojunction All-Photonic Synapses for Multibit Memory, Optical Logic, and Wearable
    Neuromorphic Vision.” <i>Small</i>. Wiley, 2026. <a href="https://doi.org/10.1002/smll.75437">https://doi.org/10.1002/smll.75437</a>.
  ieee: S. Saha <i>et al.</i>, “Interface engineered perovskite-oxide heterojunction
    all-photonic synapses for multibit memory, optical logic, and wearable neuromorphic
    vision,” <i>Small</i>. Wiley, 2026.
  ista: Saha S, Das S, Roy B, Ghosh SK, Satpathy R, Bullock J, Unnithan RR, Ray SK.
    2026. Interface engineered perovskite-oxide heterojunction all-photonic synapses
    for multibit memory, optical logic, and wearable neuromorphic vision. Small.,
    e75437.
  mla: Saha, Subham, et al. “Interface Engineered Perovskite-Oxide Heterojunction
    All-Photonic Synapses for Multibit Memory, Optical Logic, and Wearable Neuromorphic
    Vision.” <i>Small</i>, e75437, Wiley, 2026, doi:<a href="https://doi.org/10.1002/smll.75437">10.1002/smll.75437</a>.
  short: S. Saha, S. Das, B. Roy, S.K. Ghosh, R. Satpathy, J. Bullock, R.R. Unnithan,
    S.K. Ray, Small (2026).
das_tickbox: '1'
dataavailabilitystatement: The data that support the findings of this study are available
  in theSupporting Information of this article.
date_created: 2026-09-06T22:01:58Z
date_published: 2026-08-25T00:00:00Z
date_updated: 2026-09-09T13:40:30Z
day: '25'
department:
- _id: HrPo
doi: 10.1002/smll.75437
external_id:
  pmid:
  - '42643004'
fulldoi: https://doi.org/10.1002/smll.75437
keyword:
- all-optical synapse
- bidirectional photoresponse
- defect engineering
- flexible neuromorphic vision
- multibit nonvolatile memory
- negativephotoconductivity
- optical logic gate
language:
- iso: eng
month: '08'
oa_version: None
pmid: 1
publication: Small
publication_identifier:
  eissn:
  - 1613-6829
  issn:
  - 1613-6810
publication_status: epub_ahead
publisher: Wiley
quality_controlled: '1'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: yes
title: Interface engineered perovskite-oxide heterojunction all-photonic synapses
  for multibit memory, optical logic, and wearable neuromorphic vision
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
OA_place: repository
OA_type: green
_id: '22821'
abstract:
- lang: eng
  text: "With probability 1, we assess the average behaviour of various arithmetic
    functions at the values of degree \U0001D451 polynomials \U0001D453∈ℤ⁢[\U0001D461]
    that are ordered by height. This allows us to establish averaged versions of the
    Bateman–Horn conjecture, the polynomial Chowla conjecture and to address a basic
    question about the integral Hasse principle for norm form equations. Moreover,
    we are able to quantify the error term in the asymptotics and the size of the
    exceptional set of \U0001D453, both with arbitrary logarithmic power savings."
acknowledgement: Tim Browning was supported by an FWF grant (DOI 10.55776/P32428),
  Efthymios Sofos was supported by EPSRC New Horizons grant EP/V048236/1, and Joni
  Teräväinen was supported by Academy of Finland grant no. 340098, a von Neumann Fellowship
  (NSF grant DMS-1926686), and funding from European Union’s Horizon Europe research
  and innovation programme under Marie Skłodowska-Curie grant agreement no. 101058904.
  This material is based upon work supported by a grant from the Institute for Advanced
  Study School of Mathematics. The authors are extremely grateful to the anonymous
  referee and to Yijie Diao for useful comments.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Timothy D
  full_name: Browning, Timothy D
  id: 35827D50-F248-11E8-B48F-1D18A9856A87
  last_name: Browning
  orcid: 0000-0002-8314-0177
- first_name: Efthymios
  full_name: Sofos, Efthymios
  last_name: Sofos
- first_name: Joni
  full_name: Teräväinen, Joni
  last_name: Teräväinen
citation:
  ama: Browning TD, Sofos E, Teräväinen J. Bateman-Horn, polynomial Chowla and the
    Hasse principle with probability. <i>Journal für die reine und angewandte Mathematik</i>.
    2026. doi:<a href="https://doi.org/10.1515/crelle-2026-0062">10.1515/crelle-2026-0062</a>
  apa: Browning, T. D., Sofos, E., &#38; Teräväinen, J. (2026). Bateman-Horn, polynomial
    Chowla and the Hasse principle with probability. <i>Journal Für Die Reine Und
    Angewandte Mathematik</i>. De Gruyter. <a href="https://doi.org/10.1515/crelle-2026-0062">https://doi.org/10.1515/crelle-2026-0062</a>
  chicago: Browning, Timothy D, Efthymios Sofos, and Joni Teräväinen. “Bateman-Horn,
    Polynomial Chowla and the Hasse Principle with Probability.” <i>Journal Für Die
    Reine Und Angewandte Mathematik</i>. De Gruyter, 2026. <a href="https://doi.org/10.1515/crelle-2026-0062">https://doi.org/10.1515/crelle-2026-0062</a>.
  ieee: T. D. Browning, E. Sofos, and J. Teräväinen, “Bateman-Horn, polynomial Chowla
    and the Hasse principle with probability,” <i>Journal für die reine und angewandte
    Mathematik</i>. De Gruyter, 2026.
  ista: Browning TD, Sofos E, Teräväinen J. 2026. Bateman-Horn, polynomial Chowla
    and the Hasse principle with probability. Journal für die reine und angewandte
    Mathematik.
  mla: Browning, Timothy D., et al. “Bateman-Horn, Polynomial Chowla and the Hasse
    Principle with Probability.” <i>Journal Für Die Reine Und Angewandte Mathematik</i>,
    De Gruyter, 2026, doi:<a href="https://doi.org/10.1515/crelle-2026-0062">10.1515/crelle-2026-0062</a>.
  short: T.D. Browning, E. Sofos, J. Teräväinen, Journal Für Die Reine Und Angewandte
    Mathematik (2026).
corr_author: '1'
date_created: 2026-09-06T22:01:58Z
date_published: 2026-08-25T00:00:00Z
date_updated: 2026-09-09T13:28:45Z
day: '25'
department:
- _id: TiBr
doi: 10.1515/crelle-2026-0062
external_id:
  arxiv:
  - '2212.10373'
fulldoi: https://doi.org/10.1515/crelle-2026-0062
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2212.10373
month: '08'
oa: 1
oa_version: Preprint
project:
- _id: 26AEDAB2-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: P32428
  name: New frontiers of the Manin conjecture
publication: Journal für die reine und angewandte Mathematik
publication_identifier:
  eissn:
  - 1435-5345
  issn:
  - 0075-4102
publication_status: epub_ahead
publisher: De Gruyter
quality_controlled: '1'
scopus_import: '1'
status: public
title: Bateman-Horn, polynomial Chowla and the Hasse principle with probability
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
