---
APC_amount: 1470 EUR
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '15165'
abstract:
- lang: eng
text: Current knowledge suggests a drought Indian monsoon (perhaps a severe one)
when the El Nino Southern Oscillation and Pacific Decadal Oscillation each exhibit
positive phases (a joint positive phase). For the monsoons, which are exceptions
in this regard, we found northeast India often gets excess pre-monsoon rainfall.
Further investigation reveals that this excess pre-monsoon rainfall is produced
by the interaction of the large-scale circulation associated with the joint phase
with the mountains in northeast India. We posit that a warmer troposphere, a consequence
of excess rainfall over northeast India, drives a stronger monsoon circulation
and enhances monsoon rainfall over central India. Hence, we argue that pre-monsoon
rainfall over northeast India can be used for seasonal monsoon rainfall prediction
over central India. Most importantly, its predictive value is at its peak when
the Pacific Ocean exhibits a joint positive phase and the threat of extreme drought
monsoon looms over India.
acknowledgement: The author gratefully acknowledges ISTA for supporting this research
through funding from the European Research Council (ERC) under the European Union’s
Horizon 2020 research and innovation programme (Project CLUSTER, grant agreement
No. 805041).
article_number: e2023GL106569
article_processing_charge: Yes
article_type: original
author:
- first_name: Bidyut B
full_name: Goswami, Bidyut B
id: 3a4ac09c-6d61-11ec-bf66-884cde66b64b
last_name: Goswami
orcid: 0000-0001-8602-3083
citation:
ama: GOSWAMI BB. A pre-monsoon signal of false alarms of Indian monsoon droughts.
Geophysical Research Letters. 2024;51(5). doi:10.1029/2023GL106569
apa: GOSWAMI, B. B. (2024). A pre-monsoon signal of false alarms of Indian monsoon
droughts. Geophysical Research Letters. Wiley. https://doi.org/10.1029/2023GL106569
chicago: GOSWAMI, BIDYUT B. “A Pre-Monsoon Signal of False Alarms of Indian Monsoon
Droughts.” Geophysical Research Letters. Wiley, 2024. https://doi.org/10.1029/2023GL106569.
ieee: B. B. GOSWAMI, “A pre-monsoon signal of false alarms of Indian monsoon droughts,”
Geophysical Research Letters, vol. 51, no. 5. Wiley, 2024.
ista: GOSWAMI BB. 2024. A pre-monsoon signal of false alarms of Indian monsoon droughts.
Geophysical Research Letters. 51(5), e2023GL106569.
mla: GOSWAMI, BIDYUT B. “A Pre-Monsoon Signal of False Alarms of Indian Monsoon
Droughts.” Geophysical Research Letters, vol. 51, no. 5, e2023GL106569,
Wiley, 2024, doi:10.1029/2023GL106569.
short: B.B. GOSWAMI, Geophysical Research Letters 51 (2024).
corr_author: '1'
date_created: 2024-03-24T23:00:58Z
date_published: 2024-03-16T00:00:00Z
date_updated: 2025-09-04T13:11:41Z
day: '16'
ddc:
- '550'
department:
- _id: CaMu
doi: 10.1029/2023GL106569
ec_funded: 1
external_id:
isi:
- '001181635700001'
file:
- access_level: open_access
checksum: 243bd966aca968ec7d9e474af8639f8d
content_type: application/pdf
creator: dernst
date_created: 2024-03-25T08:36:00Z
date_updated: 2024-03-25T08:36:00Z
file_id: '15178'
file_name: 2024_GeophysResLetters_Goswami.pdf
file_size: 2887134
relation: main_file
success: 1
file_date_updated: 2024-03-25T08:36:00Z
has_accepted_license: '1'
intvolume: ' 51'
isi: 1
issue: '5'
language:
- iso: eng
month: '03'
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: Geophysical Research Letters
publication_identifier:
eissn:
- 1944-8007
issn:
- 0094-8276
publication_status: published
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: A pre-monsoon signal of false alarms of Indian monsoon droughts
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 51
year: '2024'
...
---
_id: '15166'
abstract:
- lang: eng
text: Reducing defects boosts room-temperature performance of a thermoelectric device
acknowledgement: The authors thank the Werner-Siemens-Stiftung and the Institute of
Science and Technology Austria for financial support.
article_processing_charge: No
article_type: letter_note
author:
- first_name: Navita
full_name: Navita, Navita
id: 6ebe278d-ba0b-11ee-8184-f34cdc671de4
last_name: Navita
orcid: 0000-0001-7408-8197
- first_name: Maria
full_name: Ibáñez, Maria
id: 43C61214-F248-11E8-B48F-1D18A9856A87
last_name: Ibáñez
orcid: 0000-0001-5013-2843
citation:
ama: Jakhar N, Ibáñez M. Electron highways are cooler. Science. 2024;383(6688):1184.
doi:10.1126/science.ado4077
apa: Jakhar, N., & Ibáñez, M. (2024). Electron highways are cooler. Science.
American Association for the Advancement of Science. https://doi.org/10.1126/science.ado4077
chicago: Jakhar, Navita, and Maria Ibáñez. “Electron Highways Are Cooler.” Science.
American Association for the Advancement of Science, 2024. https://doi.org/10.1126/science.ado4077.
ieee: N. Jakhar and M. Ibáñez, “Electron highways are cooler,” Science, vol.
383, no. 6688. American Association for the Advancement of Science, p. 1184, 2024.
ista: Jakhar N, Ibáñez M. 2024. Electron highways are cooler. Science. 383(6688),
1184.
mla: Jakhar, Navita, and Maria Ibáñez. “Electron Highways Are Cooler.” Science,
vol. 383, no. 6688, American Association for the Advancement of Science, 2024,
p. 1184, doi:10.1126/science.ado4077.
short: N. Jakhar, M. Ibáñez, Science 383 (2024) 1184.
corr_author: '1'
date_created: 2024-03-24T23:00:58Z
date_published: 2024-03-14T00:00:00Z
date_updated: 2025-09-04T13:12:19Z
day: '14'
department:
- _id: MaIb
doi: 10.1126/science.ado4077
external_id:
isi:
- '001273082800019'
pmid:
- '38484066'
intvolume: ' 383'
isi: 1
issue: '6688'
language:
- iso: eng
month: '03'
oa_version: None
page: '1184'
pmid: 1
project:
- _id: 9B8F7476-BA93-11EA-9121-9846C619BF3A
name: 'HighTE: The Werner Siemens Laboratory for the High Throughput Discovery of
Semiconductors for Waste Heat Recovery'
publication: Science
publication_identifier:
eissn:
- 1095-9203
issn:
- 0036-8075
publication_status: published
publisher: American Association for the Advancement of Science
quality_controlled: '1'
scopus_import: '1'
status: public
title: Electron highways are cooler
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 383
year: '2024'
...
---
_id: '15167'
abstract:
- lang: eng
text: We perform a diagrammatic analysis of the energy of a mobile impurity immersed
in a strongly interacting two-component Fermi gas to second order in the impurity-bath
interaction. These corrections demonstrate divergent behavior in the limit of
large impurity momentum. We show the fundamental processes responsible for these
logarithmically divergent terms. We study the problem in the general case without
any assumptions regarding the fermion-fermion interactions in the bath. We show
that the divergent term can be summed up to all orders in the Fermi-Fermi interaction
and that the resulting expression is equivalent to the one obtained in the few-body
calculation. Finally, we provide a perturbative calculation to the second order
in the Fermi-Fermi interaction, and we show the diagrams responsible for these
terms.
acknowledgement: We thank Félix Werner and Kris Van Houcke for interesting discussions.
article_number: '033315'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Ragheed
full_name: Al Hyder, Ragheed
id: d1c405be-ae15-11ed-8510-ccf53278162e
last_name: Al Hyder
- first_name: F.
full_name: Chevy, F.
last_name: Chevy
- first_name: X.
full_name: Leyronas, X.
last_name: Leyronas
citation:
ama: Al Hyder R, Chevy F, Leyronas X. Exploring beyond-mean-field logarithmic divergences
in Fermi-polaron energy. Physical Review A. 2024;109(3). doi:10.1103/PhysRevA.109.033315
apa: Al Hyder, R., Chevy, F., & Leyronas, X. (2024). Exploring beyond-mean-field
logarithmic divergences in Fermi-polaron energy. Physical Review A. American
Physical Society. https://doi.org/10.1103/PhysRevA.109.033315
chicago: Al Hyder, Ragheed, F. Chevy, and X. Leyronas. “Exploring Beyond-Mean-Field
Logarithmic Divergences in Fermi-Polaron Energy.” Physical Review A. American
Physical Society, 2024. https://doi.org/10.1103/PhysRevA.109.033315.
ieee: R. Al Hyder, F. Chevy, and X. Leyronas, “Exploring beyond-mean-field logarithmic
divergences in Fermi-polaron energy,” Physical Review A, vol. 109, no.
3. American Physical Society, 2024.
ista: Al Hyder R, Chevy F, Leyronas X. 2024. Exploring beyond-mean-field logarithmic
divergences in Fermi-polaron energy. Physical Review A. 109(3), 033315.
mla: Al Hyder, Ragheed, et al. “Exploring Beyond-Mean-Field Logarithmic Divergences
in Fermi-Polaron Energy.” Physical Review A, vol. 109, no. 3, 033315, American
Physical Society, 2024, doi:10.1103/PhysRevA.109.033315.
short: R. Al Hyder, F. Chevy, X. Leyronas, Physical Review A 109 (2024).
corr_author: '1'
date_created: 2024-03-24T23:00:59Z
date_published: 2024-03-19T00:00:00Z
date_updated: 2025-09-04T13:07:33Z
day: '19'
department:
- _id: MiLe
doi: 10.1103/PhysRevA.109.033315
external_id:
arxiv:
- '2311.14536'
isi:
- '001198511300017'
intvolume: ' 109'
isi: 1
issue: '3'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2311.14536
month: '03'
oa: 1
oa_version: Preprint
publication: Physical Review A
publication_identifier:
eissn:
- 2469-9934
issn:
- 2469-9926
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 109
year: '2024'
...
---
_id: '15168'
abstract:
- lang: eng
text: 'A linearly ordered (LO) k-colouring of a hypergraph is a colouring of its
vertices with colours 1, … , k such that each edge contains a unique maximal colour.
Deciding whether an input hypergraph admits LO k-colouring with a fixed number
of colours is NP-complete (and in the special case of graphs, LO colouring coincides
with the usual graph colouring). Here, we investigate the complexity of approximating
the "linearly ordered chromatic number" of a hypergraph. We prove that the following
promise problem is NP-complete: Given a 3-uniform hypergraph, distinguish between
the case that it is LO 3-colourable, and the case that it is not even LO 4-colourable.
We prove this result by a combination of algebraic, topological, and combinatorial
methods, building on and extending a topological approach for studying approximate
graph colouring introduced by Krokhin, Opršal, Wrochna, and Živný (2023).'
acknowledgement: "Marek Filakovský: This research was supported by Charles University
(project PRIMUS/\r\n21/SCI/014), the Austrian Science Fund (FWF project P31312-N35),
and MSCAfellow5_MUNI\r\n(CZ.02.01.01/00/22_010/0003229). Tamio-Vesa Nakajima: This
research was funded by UKRI EP/X024431/1 and by a Clarendon Fund Scholarship. All
data is provided in full in the results section of this paper. Jakub Opršal: 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.
Uli Wagner: This research was supported by the Austrian Science Fund (FWF project
P31312-N35)."
alternative_title:
- LIPIcs
article_number: '34'
article_processing_charge: No
arxiv: 1
author:
- first_name: Marek
full_name: Filakovský, Marek
id: 3E8AF77E-F248-11E8-B48F-1D18A9856A87
last_name: Filakovský
- first_name: Tamio Vesa
full_name: Nakajima, Tamio Vesa
last_name: Nakajima
- first_name: Jakub
full_name: Opršal, Jakub
id: ec596741-c539-11ec-b829-c79322a91242
last_name: Opršal
orcid: 0000-0003-1245-3456
- first_name: Gianluca
full_name: Tasinato, Gianluca
id: 0433290C-AF8F-11E9-A4C7-F729E6697425
last_name: Tasinato
- first_name: Uli
full_name: Wagner, Uli
id: 36690CA2-F248-11E8-B48F-1D18A9856A87
last_name: Wagner
orcid: 0000-0002-1494-0568
citation:
ama: 'Filakovský M, Nakajima TV, Opršal J, Tasinato G, Wagner U. Hardness of linearly
ordered 4-colouring of 3-colourable 3-uniform hypergraphs. In: 41st International
Symposium on Theoretical Aspects of Computer Science. Vol 289. Schloss Dagstuhl
- Leibniz-Zentrum für Informatik; 2024. doi:10.4230/LIPIcs.STACS.2024.34'
apa: 'Filakovský, M., Nakajima, T. V., Opršal, J., Tasinato, G., & Wagner, U.
(2024). Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs.
In 41st International Symposium on Theoretical Aspects of Computer Science
(Vol. 289). Clermont-Ferrand, France: Schloss Dagstuhl - Leibniz-Zentrum für Informatik.
https://doi.org/10.4230/LIPIcs.STACS.2024.34'
chicago: Filakovský, Marek, Tamio Vesa Nakajima, Jakub Opršal, Gianluca Tasinato,
and Uli Wagner. “Hardness of Linearly Ordered 4-Colouring of 3-Colourable 3-Uniform
Hypergraphs.” In 41st International Symposium on Theoretical Aspects of Computer
Science, Vol. 289. Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2024.
https://doi.org/10.4230/LIPIcs.STACS.2024.34.
ieee: M. Filakovský, T. V. Nakajima, J. Opršal, G. Tasinato, and U. Wagner, “Hardness
of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs,” in 41st
International Symposium on Theoretical Aspects of Computer Science, Clermont-Ferrand,
France, 2024, vol. 289.
ista: 'Filakovský M, Nakajima TV, Opršal J, Tasinato G, Wagner U. 2024. Hardness
of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs. 41st International
Symposium on Theoretical Aspects of Computer Science. STACS: Symposium on Theoretical
Aspects of Computer Science, LIPIcs, vol. 289, 34.'
mla: Filakovský, Marek, et al. “Hardness of Linearly Ordered 4-Colouring of 3-Colourable
3-Uniform Hypergraphs.” 41st International Symposium on Theoretical Aspects
of Computer Science, vol. 289, 34, Schloss Dagstuhl - Leibniz-Zentrum für
Informatik, 2024, doi:10.4230/LIPIcs.STACS.2024.34.
short: M. Filakovský, T.V. Nakajima, J. Opršal, G. Tasinato, U. Wagner, in:, 41st
International Symposium on Theoretical Aspects of Computer Science, Schloss Dagstuhl
- Leibniz-Zentrum für Informatik, 2024.
conference:
end_date: 2024-03-14
location: Clermont-Ferrand, France
name: 'STACS: Symposium on Theoretical Aspects of Computer Science'
start_date: 2024-03-12
corr_author: '1'
date_created: 2024-03-24T23:00:59Z
date_published: 2024-03-01T00:00:00Z
date_updated: 2026-04-07T12:36:50Z
day: '01'
ddc:
- '510'
department:
- _id: UlWa
doi: 10.4230/LIPIcs.STACS.2024.34
ec_funded: 1
external_id:
arxiv:
- '2312.12981'
isi:
- '001300393400034'
file:
- access_level: open_access
checksum: 0524d4189fd1ed08989546511343edf3
content_type: application/pdf
creator: dernst
date_created: 2024-03-25T07:44:30Z
date_updated: 2024-03-25T07:44:30Z
file_id: '15175'
file_name: 2024_LIPICs_Filakovsky.pdf
file_size: 927290
relation: main_file
success: 1
file_date_updated: 2024-03-25T07:44:30Z
has_accepted_license: '1'
intvolume: ' 289'
isi: 1
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: 26611F5C-B435-11E9-9278-68D0E5697425
call_identifier: FWF
grant_number: P31312
name: Algorithms for Embeddings and Homotopy Theory
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: 41st International Symposium on Theoretical Aspects of Computer Science
publication_identifier:
eissn:
- 1868-8969
isbn:
- '9783959773119'
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
quality_controlled: '1'
related_material:
record:
- id: '20339'
relation: dissertation_contains
status: public
scopus_import: '1'
status: public
title: Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: conference
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 289
year: '2024'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '15169'
abstract:
- lang: eng
text: Interpretation of extracellular recordings can be challenging due to the long
range of electric field. This challenge can be mitigated by estimating the current
source density (CSD). Here we introduce kCSD-python, an open Python package implementing
Kernel Current Source Density (kCSD) method and related tools to facilitate CSD
analysis of experimental data and the interpretation of results. We show how to
counter the limitations imposed by noise and assumptions in the method itself.
kCSD-python allows CSD estimation for an arbitrary distribution of electrodes
in 1D, 2D, and 3D, assuming distributions of sources in tissue, a slice, or in
a single cell, and includes a range of diagnostic aids. We demonstrate its features
in a Jupyter Notebook tutorial which illustrates a typical analytical workflow
and main functionalities useful in validating analysis results.
acknowledgement: 'The Python implementation of kCSD was started by Grzegorz Parka
during Google Summer of Code project through the International Neuroinformatics
Coordinating Facility. Jan Mąka implemented the first Python version of skCSD class.
This work was supported by the Polish National Science Centre (2013/08/W/NZ4/00691
to DKW; 2015/17/B/ST7/04123 to DKW). '
article_number: e1011941
article_processing_charge: Yes
article_type: original
author:
- first_name: Chaitanya
full_name: Chintaluri, Chaitanya
id: E4EDB536-3485-11EA-98D2-20AF3DDC885E
last_name: Chintaluri
- first_name: Marta
full_name: Bejtka, Marta
last_name: Bejtka
- first_name: Wladyslaw
full_name: Sredniawa, Wladyslaw
last_name: Sredniawa
- first_name: Michal
full_name: Czerwinski, Michal
last_name: Czerwinski
- first_name: Jakub M.
full_name: Dzik, Jakub M.
last_name: Dzik
- first_name: Joanna
full_name: Jedrzejewska-Szmek, Joanna
last_name: Jedrzejewska-Szmek
- first_name: Daniel K.
full_name: Wojciki, Daniel K.
last_name: Wojciki
citation:
ama: Chintaluri C, Bejtka M, Sredniawa W, et al. kCSD-python, reliable current source
density estimation with quality control. PLoS Computational Biology. 2024;20(3).
doi:10.1371/journal.pcbi.1011941
apa: Chintaluri, C., Bejtka, M., Sredniawa, W., Czerwinski, M., Dzik, J. M., Jedrzejewska-Szmek,
J., & Wojciki, D. K. (2024). kCSD-python, reliable current source density
estimation with quality control. PLoS Computational Biology. Public Library
of Science. https://doi.org/10.1371/journal.pcbi.1011941
chicago: Chintaluri, Chaitanya, Marta Bejtka, Wladyslaw Sredniawa, Michal Czerwinski,
Jakub M. Dzik, Joanna Jedrzejewska-Szmek, and Daniel K. Wojciki. “KCSD-Python,
Reliable Current Source Density Estimation with Quality Control.” PLoS Computational
Biology. Public Library of Science, 2024. https://doi.org/10.1371/journal.pcbi.1011941.
ieee: C. Chintaluri et al., “kCSD-python, reliable current source density
estimation with quality control,” PLoS Computational Biology, vol. 20,
no. 3. Public Library of Science, 2024.
ista: Chintaluri C, Bejtka M, Sredniawa W, Czerwinski M, Dzik JM, Jedrzejewska-Szmek
J, Wojciki DK. 2024. kCSD-python, reliable current source density estimation with
quality control. PLoS Computational Biology. 20(3), e1011941.
mla: Chintaluri, Chaitanya, et al. “KCSD-Python, Reliable Current Source Density
Estimation with Quality Control.” PLoS Computational Biology, vol. 20,
no. 3, e1011941, Public Library of Science, 2024, doi:10.1371/journal.pcbi.1011941.
short: C. Chintaluri, M. Bejtka, W. Sredniawa, M. Czerwinski, J.M. Dzik, J. Jedrzejewska-Szmek,
D.K. Wojciki, PLoS Computational Biology 20 (2024).
corr_author: '1'
date_created: 2024-03-24T23:00:59Z
date_published: 2024-03-14T00:00:00Z
date_updated: 2025-09-04T13:08:54Z
day: '14'
ddc:
- '000'
- '570'
department:
- _id: TiVo
doi: 10.1371/journal.pcbi.1011941
external_id:
isi:
- '001190689800001'
pmid:
- '38484020'
file:
- access_level: open_access
checksum: c09718d0d09614642d877d0716ce32e8
content_type: application/pdf
creator: dernst
date_created: 2025-06-25T05:47:36Z
date_updated: 2025-06-25T05:47:36Z
file_id: '19897'
file_name: 2024_PLoSCompBio_Chintaluri.pdf
file_size: 2540277
relation: main_file
success: 1
file_date_updated: 2025-06-25T05:47:36Z
has_accepted_license: '1'
intvolume: ' 20'
isi: 1
issue: '3'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
pmid: 1
publication: PLoS Computational Biology
publication_identifier:
eissn:
- 1553-7358
issn:
- 1553-734X
publication_status: published
publisher: Public Library of Science
quality_controlled: '1'
related_material:
link:
- relation: software
url: https://github.com/Neuroinflab/kCSD-python
scopus_import: '1'
status: public
title: kCSD-python, reliable current source density estimation with quality control
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 20
year: '2024'
...
---
DOAJ_listed: '1'
_id: '15170'
abstract:
- lang: eng
text: 'The James Webb Space Telescope is revealing a new population of dust-reddened
broad-line active galactic nuclei (AGN) at redshifts z ≳ 5. Here we present deep
NIRSpec/Prism spectroscopy from the Cycle 1 Treasury program Ultradeep NIRSpec
and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) of 15 AGN candidates
selected to be compact, with red continua in the rest-frame optical but with blue
slopes in the UV. From NIRCam photometry alone, they could have been dominated
by dusty star formation or an AGN. Here we show that the majority of the compact
red sources in UNCOVER are dust-reddened AGN: 60% show definitive evidence for
broad-line Hα with a FWHM > 2000 km s −1, 20% of the current data are inconclusive,
and 20% are brown dwarf stars. We propose an updated photometric criterion to
select red z > 5 AGN that excludes brown dwarfs and is expected to yield >80%
AGN. Remarkably, among all zphot > 5 galaxies with F277W – F444W > 1 in UNCOVER
at least 33% are AGN regardless of compactness, climbing to at least 80% AGN for
sources with F277W – F444W > 1.6. The confirmed AGN have black hole masses of
107–109M⊙. While their UV luminosities (−16 > MUV > −20 AB mag) are low compared
to UV-selected AGN at these epochs, consistent with percent-level scattered AGN
light or low levels of unobscured star formation, the inferred bolometric luminosities
are typical of 107–109M⊙ black holes radiating at ∼10%–40% the Eddington limit.
The number densities are surprisingly high at ∼10−5 Mpc−3 mag−1, 100 times more
common than the faintest UV-selected quasars, while accounting for ∼1% of the
UV-selected galaxies. While their UV faintness suggests they may not contribute
strongly to reionization, their ubiquity poses challenges to models of black hole
growth.'
acknowledgement: J.E.G. and A.D.G acknowledge support from NSF/AAG grant No. 1007094,
and J.E.G. also acknowledges support from NSF/AAG grant No. 1007052. A.Z. acknowledges
support by grant No. 2020750 from the United States-Israel Binational Science Foundation
(BSF) and grant No. 2109066 from the United States National Science Foundation (NSF),
and by the Ministry of Science & Technology of Israel. The Cosmic Dawn Center is
funded by the Danish National Research Foundation (DNRF) under grant No. 140. 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. P.D. acknowledges
support from the NWO grant 016.VIDI.189.162 ("ODIN") and from the European Commission's
and University of Groningen's CO-FUND Rosalind Franklin program. K.G. and T.N. acknowledge
support from Australian Research Council Laureate Fellowship FL180100060. H.A. and
I.C. acknowledge support from CNES, focused on the JWST mission, and the Programme
National Cosmology and Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, cofunded
by CEA and CNES. R.P.N. acknowledges funding from JWST programs GO-1933 and GO-2279.
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. The research of C.C.W. is supported by NOIRLab, which
is managed by the Association of Universities for Research in Astronomy (AURA) under
a cooperative agreement with the National Science Foundation. B.W. acknowledges
support from JWST-GO-02561.022-A. A.J.B. acknowledges funding support from NASA/ADAP
grant 21-ADAP21-0187. Support for this work was provided by The Brinson Foundation
through a Brinson Prize Fellowship grant. R.P.N. acknowledges support for this work
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.
C.P. thanks Marsha and Ralph Schilling for the generous support of this research.
article_number: '39'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Jenny E.
full_name: Greene, Jenny E.
last_name: Greene
- first_name: Ivo
full_name: Labbe, Ivo
last_name: Labbe
- first_name: Andy D.
full_name: Goulding, Andy D.
last_name: Goulding
- first_name: Lukas J.
full_name: Furtak, Lukas J.
last_name: Furtak
- first_name: Iryna
full_name: Chemerynska, Iryna
last_name: Chemerynska
- first_name: Vasily
full_name: Kokorev, Vasily
last_name: Kokorev
- first_name: Pratika
full_name: Dayal, Pratika
last_name: Dayal
- first_name: Marta
full_name: Volonteri, Marta
last_name: Volonteri
- first_name: Christina C.
full_name: Williams, Christina C.
last_name: Williams
- first_name: Bingjie
full_name: Wang, Bingjie
last_name: Wang
- first_name: David J.
full_name: Setton, David J.
last_name: Setton
- first_name: Adam J.
full_name: Burgasser, Adam J.
last_name: Burgasser
- first_name: Rachel
full_name: Bezanson, Rachel
last_name: Bezanson
- first_name: Hakim
full_name: Atek, Hakim
last_name: Atek
- first_name: Gabriel
full_name: Brammer, Gabriel
last_name: Brammer
- first_name: Sam E.
full_name: Cutler, Sam E.
last_name: Cutler
- first_name: Robert
full_name: Feldmann, Robert
last_name: Feldmann
- first_name: Seiji
full_name: Fujimoto, Seiji
last_name: Fujimoto
- first_name: Karl
full_name: Glazebrook, Karl
last_name: Glazebrook
- first_name: Anna
full_name: De Graaff, Anna
last_name: De Graaff
- first_name: Gourav
full_name: Khullar, Gourav
last_name: Khullar
- first_name: Joel
full_name: Leja, Joel
last_name: Leja
- first_name: Danilo
full_name: Marchesini, Danilo
last_name: Marchesini
- first_name: Michael V.
full_name: Maseda, Michael V.
last_name: Maseda
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Tim B.
full_name: Miller, Tim B.
last_name: Miller
- first_name: Rohan P.
full_name: Naidu, Rohan P.
last_name: Naidu
- first_name: Themiya
full_name: Nanayakkara, Themiya
last_name: Nanayakkara
- first_name: Pascal A.
full_name: Oesch, Pascal A.
last_name: Oesch
- first_name: Richard
full_name: Pan, Richard
last_name: Pan
- first_name: Casey
full_name: Papovich, Casey
last_name: Papovich
- first_name: Sedona H.
full_name: Price, Sedona H.
last_name: Price
- first_name: Pieter
full_name: Van Dokkum, Pieter
last_name: Van Dokkum
- first_name: John R.
full_name: Weaver, John R.
last_name: Weaver
- first_name: Katherine E.
full_name: Whitaker, Katherine E.
last_name: Whitaker
- first_name: Adi
full_name: Zitrin, Adi
last_name: Zitrin
citation:
ama: Greene JE, Labbe I, Goulding AD, et al. UNCOVER spectroscopy confirms the surprising
ubiquity of active galactic nuclei in red sources at z > 5. Astrophysical
Journal. 2024;964. doi:10.3847/1538-4357/ad1e5f
apa: Greene, J. E., Labbe, I., Goulding, A. D., Furtak, L. J., Chemerynska, I.,
Kokorev, V., … Zitrin, A. (2024). UNCOVER spectroscopy confirms the surprising
ubiquity of active galactic nuclei in red sources at z > 5. Astrophysical
Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ad1e5f
chicago: Greene, Jenny E., Ivo Labbe, Andy D. Goulding, Lukas J. Furtak, Iryna Chemerynska,
Vasily Kokorev, Pratika Dayal, et al. “UNCOVER Spectroscopy Confirms the Surprising
Ubiquity of Active Galactic Nuclei in Red Sources at z > 5.” Astrophysical
Journal. IOP Publishing, 2024. https://doi.org/10.3847/1538-4357/ad1e5f.
ieee: J. E. Greene et al., “UNCOVER spectroscopy confirms the surprising
ubiquity of active galactic nuclei in red sources at z > 5,” Astrophysical
Journal, vol. 964. IOP Publishing, 2024.
ista: Greene JE, Labbe I, Goulding AD, Furtak LJ, Chemerynska I, Kokorev V, Dayal
P, Volonteri M, Williams CC, Wang B, Setton DJ, Burgasser AJ, Bezanson R, Atek
H, Brammer G, Cutler SE, Feldmann R, Fujimoto S, Glazebrook K, De Graaff A, Khullar
G, Leja J, Marchesini D, Maseda MV, Matthee JJ, Miller TB, Naidu RP, Nanayakkara
T, Oesch PA, Pan R, Papovich C, Price SH, Van Dokkum P, Weaver JR, Whitaker KE,
Zitrin A. 2024. UNCOVER spectroscopy confirms the surprising ubiquity of active
galactic nuclei in red sources at z > 5. Astrophysical Journal. 964, 39.
mla: Greene, Jenny E., et al. “UNCOVER Spectroscopy Confirms the Surprising Ubiquity
of Active Galactic Nuclei in Red Sources at z > 5.” Astrophysical Journal,
vol. 964, 39, IOP Publishing, 2024, doi:10.3847/1538-4357/ad1e5f.
short: J.E. Greene, I. Labbe, A.D. Goulding, L.J. Furtak, I. Chemerynska, V. Kokorev,
P. Dayal, M. Volonteri, C.C. Williams, B. Wang, D.J. Setton, A.J. Burgasser, R.
Bezanson, H. Atek, G. Brammer, S.E. Cutler, R. Feldmann, S. Fujimoto, K. Glazebrook,
A. De Graaff, G. Khullar, J. Leja, D. Marchesini, M.V. Maseda, J.J. Matthee, T.B.
Miller, R.P. Naidu, T. Nanayakkara, P.A. Oesch, R. Pan, C. Papovich, S.H. Price,
P. Van Dokkum, J.R. Weaver, K.E. Whitaker, A. Zitrin, Astrophysical Journal 964
(2024).
date_created: 2024-03-24T23:00:59Z
date_published: 2024-03-01T00:00:00Z
date_updated: 2025-09-04T13:09:41Z
day: '01'
ddc:
- '550'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ad1e5f
external_id:
arxiv:
- '2309.05714'
isi:
- '001184746500001'
file:
- access_level: open_access
checksum: 389a880e176799d5c062ea7cb82d08c9
content_type: application/pdf
creator: dernst
date_created: 2024-03-25T08:02:43Z
date_updated: 2024-03-25T08:02:43Z
file_id: '15176'
file_name: 2024_AstrophysicalJourn_Greene.pdf
file_size: 2700137
relation: main_file
success: 1
file_date_updated: 2024-03-25T08:02:43Z
has_accepted_license: '1'
intvolume: ' 964'
isi: 1
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
publication: Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: UNCOVER spectroscopy confirms the surprising ubiquity of active galactic nuclei
in red sources at z > 5
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 964
year: '2024'
...
---
OA_place: publisher
OA_type: hybrid
_id: '15171'
abstract:
- lang: eng
text: The brain’s functionality is developed and maintained through synaptic plasticity.
As synapses undergo plasticity, they also affect each other. The nature of such
‘co-dependency’ is difficult to disentangle experimentally, because multiple synapses
must be monitored simultaneously. To help understand the experimentally observed
phenomena, we introduce a framework that formalizes synaptic co-dependency between
different connection types. The resulting model explains how inhibition can gate
excitatory plasticity while neighboring excitatory–excitatory interactions determine
the strength of long-term potentiation. Furthermore, we show how the interplay
between excitatory and inhibitory synapses can account for the quick rise and
long-term stability of a variety of synaptic weight profiles, such as orientation
tuning and dendritic clustering of co-active synapses. In recurrent neuronal networks,
co-dependent plasticity produces rich and stable motor cortex-like dynamics with
high input sensitivity. Our results suggest an essential role for the neighborly
synaptic interaction during learning, connecting micro-level physiology with network-wide
phenomena.
acknowledgement: We thank C. Currin, B. Podlaski and the members of the Vogels group
for fruitful discussions. E.J.A. and T.P.V. were supported by a Research Project
Grant from the Leverhulme Trust (RPG-2016-446; TPV), a Sir Henry Dale Fellowship
from the Wellcome Trust and the Royal Society (WT100000; T.P.V.), a Wellcome Trust
Senior Research Fellowship (214316/Z/18/Z; T.P.V.) and a European Research Council
Consolidator Grant (SYNAPSEEK, 819603; T.P.V.). For the purpose of open access,
the authors have applied a CC BY public copyright license to any author accepted
manuscript version arising from this submission. Open access funding provided by
University of Basel.
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Everton J.
full_name: Agnes, Everton J.
last_name: Agnes
- first_name: Tim P
full_name: Vogels, Tim P
id: CB6FF8D2-008F-11EA-8E08-2637E6697425
last_name: Vogels
orcid: 0000-0003-3295-6181
citation:
ama: Agnes EJ, Vogels TP. Co-dependent excitatory and inhibitory plasticity accounts
for quick, stable and long-lasting memories in biological networks. Nature
Neuroscience. 2024;27:964-974. doi:10.1038/s41593-024-01597-4
apa: Agnes, E. J., & Vogels, T. P. (2024). Co-dependent excitatory and inhibitory
plasticity accounts for quick, stable and long-lasting memories in biological
networks. Nature Neuroscience. Springer Nature. https://doi.org/10.1038/s41593-024-01597-4
chicago: Agnes, Everton J., and Tim P Vogels. “Co-Dependent Excitatory and Inhibitory
Plasticity Accounts for Quick, Stable and Long-Lasting Memories in Biological
Networks.” Nature Neuroscience. Springer Nature, 2024. https://doi.org/10.1038/s41593-024-01597-4.
ieee: E. J. Agnes and T. P. Vogels, “Co-dependent excitatory and inhibitory plasticity
accounts for quick, stable and long-lasting memories in biological networks,”
Nature Neuroscience, vol. 27. Springer Nature, pp. 964–974, 2024.
ista: Agnes EJ, Vogels TP. 2024. Co-dependent excitatory and inhibitory plasticity
accounts for quick, stable and long-lasting memories in biological networks. Nature
Neuroscience. 27, 964–974.
mla: Agnes, Everton J., and Tim P. Vogels. “Co-Dependent Excitatory and Inhibitory
Plasticity Accounts for Quick, Stable and Long-Lasting Memories in Biological
Networks.” Nature Neuroscience, vol. 27, Springer Nature, 2024, pp. 964–74,
doi:10.1038/s41593-024-01597-4.
short: E.J. Agnes, T.P. Vogels, Nature Neuroscience 27 (2024) 964–974.
date_created: 2024-03-24T23:01:00Z
date_published: 2024-05-01T00:00:00Z
date_updated: 2025-09-04T13:06:06Z
day: '01'
ddc:
- '570'
department:
- _id: TiVo
doi: 10.1038/s41593-024-01597-4
ec_funded: 1
external_id:
isi:
- '001190081400001'
pmid:
- '38509348 '
file:
- access_level: open_access
checksum: dfca68a24749575b912b3a78a7de4516
content_type: application/pdf
creator: dernst
date_created: 2025-06-25T08:45:32Z
date_updated: 2025-06-25T08:45:32Z
file_id: '19902'
file_name: 2025_NatureNeuroscience_Agnes.pdf
file_size: 10508018
relation: main_file
success: 1
file_date_updated: 2025-06-25T08:45:32Z
has_accepted_license: '1'
intvolume: ' 27'
isi: 1
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
page: 964-974
pmid: 1
project:
- _id: 0aacfa84-070f-11eb-9043-d7eb2c709234
call_identifier: H2020
grant_number: '819603'
name: Learning the shape of synaptic plasticity rules for neuronal architectures
and function through machine learning.
publication: Nature Neuroscience
publication_identifier:
eissn:
- 1546-1726
issn:
- 1097-6256
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Co-dependent excitatory and inhibitory plasticity accounts for quick, stable
and long-lasting memories in biological networks
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 27
year: '2024'
...
---
_id: '15172'
abstract:
- lang: eng
text: 'We propose a novel approach to concentration for non-independent random variables.
The main idea is to “pretend” that the random variables are independent and pay
a multiplicative price measuring how far they are from actually being independent.
This price is encapsulated in the Hellinger integral between the joint and the
product of the marginals, which is then upper bounded leveraging tensorisation
properties. Our bounds represent a natural generalisation of concentration inequalities
in the presence of dependence: we recover exactly the classical bounds (McDiarmid’s
inequality) when the random variables are independent. Furthermore, in a “large
deviations” regime, we obtain the same decay in the probability as for the independent
case, even when the random variables display non-trivial dependencies. To show
this, we consider a number of applications of interest. First, we provide a bound
for Markov chains with finite state space. Then, we consider the Simple Symmetric
Random Walk, which is a non-contracting Markov chain, and a non-Markovian setting
in which the stochastic process depends on its entire past. To conclude, we propose
an application to Markov Chain Monte Carlo methods, where our approach leads to
an improved lower bound on the minimum burn-in period required to reach a certain
accuracy. In all of these settings, we provide a regime of parameters in which
our bound fares better than what the state of the art can provide.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Amedeo Roberto
full_name: Esposito, Amedeo Roberto
id: 9583e921-e1ad-11ec-9862-cef099626dc9
last_name: Esposito
- first_name: Marco
full_name: Mondelli, Marco
id: 27EB676C-8706-11E9-9510-7717E6697425
last_name: Mondelli
orcid: 0000-0002-3242-7020
citation:
ama: Esposito AR, Mondelli M. Concentration without independence via information
measures. IEEE Transactions on Information Theory. 2024;70(6):3823-3839.
doi:10.1109/TIT.2024.3367767
apa: Esposito, A. R., & Mondelli, M. (2024). Concentration without independence
via information measures. IEEE Transactions on Information Theory. IEEE.
https://doi.org/10.1109/TIT.2024.3367767
chicago: Esposito, Amedeo Roberto, and Marco Mondelli. “Concentration without Independence
via Information Measures.” IEEE Transactions on Information Theory. IEEE,
2024. https://doi.org/10.1109/TIT.2024.3367767.
ieee: A. R. Esposito and M. Mondelli, “Concentration without independence via information
measures,” IEEE Transactions on Information Theory, vol. 70, no. 6. IEEE,
pp. 3823–3839, 2024.
ista: Esposito AR, Mondelli M. 2024. Concentration without independence via information
measures. IEEE Transactions on Information Theory. 70(6), 3823–3839.
mla: Esposito, Amedeo Roberto, and Marco Mondelli. “Concentration without Independence
via Information Measures.” IEEE Transactions on Information Theory, vol.
70, no. 6, IEEE, 2024, pp. 3823–39, doi:10.1109/TIT.2024.3367767.
short: A.R. Esposito, M. Mondelli, IEEE Transactions on Information Theory 70 (2024)
3823–3839.
corr_author: '1'
date_created: 2024-03-24T23:01:00Z
date_published: 2024-06-01T00:00:00Z
date_updated: 2025-09-04T13:06:53Z
day: '01'
department:
- _id: MaMo
doi: 10.1109/TIT.2024.3367767
external_id:
arxiv:
- '2303.07245'
isi:
- '001230181100001'
intvolume: ' 70'
isi: 1
issue: '6'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2303.07245
month: '06'
oa: 1
oa_version: Preprint
page: 3823-3839
project:
- _id: 059876FA-7A3F-11EA-A408-12923DDC885E
name: Prix Lopez-Loretta 2019 - Marco Mondelli
publication: IEEE Transactions on Information Theory
publication_identifier:
eissn:
- 1557-9654
issn:
- 0018-9448
publication_status: published
publisher: IEEE
quality_controlled: '1'
related_material:
record:
- id: '14922'
relation: earlier_version
status: public
scopus_import: '1'
status: public
title: Concentration without independence via information measures
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 70
year: '2024'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '15179'
abstract:
- lang: eng
text: The fungal bioluminescence pathway can be reconstituted in other organisms
allowing luminescence imaging without exogenously supplied substrate. The pathway
starts from hispidin biosynthesis—a step catalyzed by a large fungal polyketide
synthase that requires a posttranslational modification for activity. Here, we
report identification of alternative compact hispidin synthases encoded by a phylogenetically
diverse group of plants. A hybrid bioluminescence pathway that combines plant
and fungal genes is more compact, not dependent on availability of machinery for
posttranslational modifications, and confers autonomous bioluminescence in yeast,
mammalian, and plant hosts. The compact size of plant hispidin synthases enables
additional modes of delivery of autoluminescence, such as delivery with viral
vectors.
acknowledgement: "We thank Milaboratory (milaboratory.com) for the access to computing
and storage infrastructure. We thank J. Petrasek for providing the BY-2 cell culture
line. We thank Konstantin Lukyanov laboratory and Sergey Deyev laboratory for assistance
with experiments.\r\nThis study was partially funded by Light Bio and Planta. The
Synthetic biology Group is funded by the MRC London Institute of Medical Sciences
(UKRI MC-A658-5QEA0). Cloning and luminescent assays performed in BY-2 were partially
supported by RSF, project number 22-14-00400, https://rscf.ru/project/22-14-00400/.
Plant transformations were funded by RFBR and MOST, project number 21-54-52004.
Plant imaging experiments were funded by RSF, project number 22-74-00124, https://rscf.ru/project/22-74-00124/.
Viral delivery experiments were funded by the grant PID2019-108203RB-I00 Plan Nacional
I + D from the Ministerio de Ciencia e Innovación (Spain) through the Agencia Estatal
de Investigación (cofinanced by the European Regional Development Fund)."
article_number: adk1992
article_processing_charge: Yes
article_type: original
author:
- first_name: Kseniia A.
full_name: Palkina, Kseniia A.
last_name: Palkina
- first_name: Tatiana A.
full_name: Karataeva, Tatiana A.
last_name: Karataeva
- first_name: Maxim M.
full_name: Perfilov, Maxim M.
last_name: Perfilov
- first_name: Liliia I.
full_name: Fakhranurova, Liliia I.
last_name: Fakhranurova
- first_name: Nadezhda M.
full_name: Markina, Nadezhda M.
last_name: Markina
- first_name: Louisa
full_name: Gonzalez Somermeyer, Louisa
id: 4720D23C-F248-11E8-B48F-1D18A9856A87
last_name: Gonzalez Somermeyer
orcid: 0000-0001-9139-5383
- first_name: Elena
full_name: Garcia-Perez, Elena
last_name: Garcia-Perez
- first_name: Marta
full_name: Vazquez-Vilar, Marta
last_name: Vazquez-Vilar
- first_name: Marta
full_name: Rodriguez-Rodriguez, Marta
last_name: Rodriguez-Rodriguez
- first_name: Victor
full_name: Vazquez-Vilriales, Victor
last_name: Vazquez-Vilriales
- first_name: Ekaterina S.
full_name: Shakhova, Ekaterina S.
last_name: Shakhova
- first_name: Tatiana
full_name: Mitiouchkina, Tatiana
last_name: Mitiouchkina
- first_name: Olga A.
full_name: Belozerova, Olga A.
last_name: Belozerova
- first_name: Sergey I.
full_name: Kovalchuk, Sergey I.
last_name: Kovalchuk
- first_name: Anna
full_name: Alekberova, Anna
last_name: Alekberova
- first_name: Alena K.
full_name: Malyshevskaia, Alena K.
last_name: Malyshevskaia
- first_name: Evgenia N.
full_name: Bugaeva, Evgenia N.
last_name: Bugaeva
- first_name: Elena B.
full_name: Guglya, Elena B.
last_name: Guglya
- first_name: Anastasia
full_name: Balakireva, Anastasia
last_name: Balakireva
- first_name: Nikita
full_name: Sytov, Nikita
last_name: Sytov
- first_name: Anastasia
full_name: Bezlikhotnova, Anastasia
last_name: Bezlikhotnova
- first_name: Daria I.
full_name: Boldyreva, Daria I.
last_name: Boldyreva
- first_name: Vladislav V.
full_name: Babenko, Vladislav V.
last_name: Babenko
- first_name: Fyodor
full_name: Kondrashov, Fyodor
id: 44FDEF62-F248-11E8-B48F-1D18A9856A87
last_name: Kondrashov
orcid: 0000-0001-8243-4694
- first_name: Vladimir V.
full_name: Choob, Vladimir V.
last_name: Choob
- first_name: Diego
full_name: Orzaez, Diego
last_name: Orzaez
- first_name: Ilia V.
full_name: Yampolsky, Ilia V.
last_name: Yampolsky
- first_name: Alexander S.
full_name: Mishin, Alexander S.
last_name: Mishin
- first_name: Karen S.
full_name: Sarkisyan, Karen S.
last_name: Sarkisyan
citation:
ama: Palkina KA, Karataeva TA, Perfilov MM, et al. A hybrid pathway for self-sustained
luminescence. Science Advances. 2024;10(10). doi:10.1126/sciadv.adk1992
apa: Palkina, K. A., Karataeva, T. A., Perfilov, M. M., Fakhranurova, L. I., Markina,
N. M., Gonzalez Somermeyer, L., … Sarkisyan, K. S. (2024). A hybrid pathway for
self-sustained luminescence. Science Advances. American Association for
the Advancement of Science. https://doi.org/10.1126/sciadv.adk1992
chicago: Palkina, Kseniia A., Tatiana A. Karataeva, Maxim M. Perfilov, Liliia I.
Fakhranurova, Nadezhda M. Markina, Louisa Gonzalez Somermeyer, Elena Garcia-Perez,
et al. “A Hybrid Pathway for Self-Sustained Luminescence.” Science Advances.
American Association for the Advancement of Science, 2024. https://doi.org/10.1126/sciadv.adk1992.
ieee: K. A. Palkina et al., “A hybrid pathway for self-sustained luminescence,”
Science Advances, vol. 10, no. 10. American Association for the Advancement
of Science, 2024.
ista: Palkina KA, Karataeva TA, Perfilov MM, Fakhranurova LI, Markina NM, Gonzalez
Somermeyer L, Garcia-Perez E, Vazquez-Vilar M, Rodriguez-Rodriguez M, Vazquez-Vilriales
V, Shakhova ES, Mitiouchkina T, Belozerova OA, Kovalchuk SI, Alekberova A, Malyshevskaia
AK, Bugaeva EN, Guglya EB, Balakireva A, Sytov N, Bezlikhotnova A, Boldyreva DI,
Babenko VV, Kondrashov F, Choob VV, Orzaez D, Yampolsky IV, Mishin AS, Sarkisyan
KS. 2024. A hybrid pathway for self-sustained luminescence. Science Advances.
10(10), adk1992.
mla: Palkina, Kseniia A., et al. “A Hybrid Pathway for Self-Sustained Luminescence.”
Science Advances, vol. 10, no. 10, adk1992, American Association for the
Advancement of Science, 2024, doi:10.1126/sciadv.adk1992.
short: K.A. Palkina, T.A. Karataeva, M.M. Perfilov, L.I. Fakhranurova, N.M. Markina,
L. Gonzalez Somermeyer, E. Garcia-Perez, M. Vazquez-Vilar, M. Rodriguez-Rodriguez,
V. Vazquez-Vilriales, E.S. Shakhova, T. Mitiouchkina, O.A. Belozerova, S.I. Kovalchuk,
A. Alekberova, A.K. Malyshevskaia, E.N. Bugaeva, E.B. Guglya, A. Balakireva, N.
Sytov, A. Bezlikhotnova, D.I. Boldyreva, V.V. Babenko, F. Kondrashov, V.V. Choob,
D. Orzaez, I.V. Yampolsky, A.S. Mishin, K.S. Sarkisyan, Science Advances 10 (2024).
date_created: 2024-03-25T08:54:33Z
date_published: 2024-03-01T00:00:00Z
date_updated: 2025-09-04T13:16:05Z
day: '01'
ddc:
- '580'
department:
- _id: FyKo
doi: 10.1126/sciadv.adk1992
external_id:
isi:
- '001187580500013'
pmid:
- '38457503'
file:
- access_level: open_access
checksum: a19c43b260ea0bbaf895a29712e3153c
content_type: application/pdf
creator: dernst
date_created: 2024-03-25T09:42:10Z
date_updated: 2024-03-25T09:42:10Z
file_id: '15185'
file_name: 2024_ScienceAdv_Palkina.pdf
file_size: 1499302
relation: main_file
success: 1
file_date_updated: 2024-03-25T09:42:10Z
has_accepted_license: '1'
intvolume: ' 10'
isi: 1
issue: '10'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
pmid: 1
publication: Science Advances
publication_identifier:
eissn:
- 2375-2548
publication_status: published
publisher: American Association for the Advancement of Science
quality_controlled: '1'
scopus_import: '1'
status: public
title: A hybrid pathway for self-sustained luminescence
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 10
year: '2024'
...
---
APC_amount: 5666,27 EUR
OA_place: publisher
OA_type: gold
_id: '15180'
abstract:
- lang: eng
text: Characterizing the prevalence and properties of faint active galactic nuclei
(AGNs) in the early Universe is key for understanding the formation of supermassive
black holes (SMBHs) and determining their role in cosmic reionization. We perform
a spectroscopic search for broad Hα emitters at z ≈ 4–6 using deep JWST/NIRCam
imaging and wide field slitless spectroscopy from the EIGER and FRESCO surveys.
We identify 20 Hα lines at z = 4.2–5.5 that have broad components with line widths
from ∼1200–3700 km s−1, contributing ∼30%–90% of the total line flux. We interpret
these broad components as being powered by accretion onto SMBHs with implied masses
∼107–8M⊙. In the UV luminosity range MUV,AGN+host = −21 to −18, we measure number
densities of ≈10−5 cMpc−3. This is an order of magnitude higher than expected
from extrapolating quasar UV luminosity functions (LFs). Yet, such AGN are found
in only <1% of star-forming galaxies at z ∼ 5. The number density discrepancy
is much lower when compared to the broad Hα LF. The SMBH mass function agrees
with large cosmological simulations. In two objects, we detect complex Hα profiles
that we tentatively interpret as caused by absorption signatures from dense gas
fueling SMBH growth and outflows. We may be witnessing early AGN feedback that
will clear dust-free pathways through which more massive blue quasars are seen.
We uncover a strong correlation between reddening and the fraction of total galaxy
luminosity arising from faint AGN. This implies that early SMBH growth is highly
obscured and that faint AGN are only minor contributors to cosmic reionization.
acknowledgement: "We thank the anonymous referee for constructive comments that helped
improve the manuscript. This work is based on observations made with the NASA/ESA/CSA
James Webb Space Telescope. The data were obtained from the Mikulski Archive for
Space Telescopes at the Space Telescope Science Institute, which is operated by
the Association of Universities for Research in Astronomy, Inc., under NASA contract
NAS 5-03127 for JWST. These observations are associated with program Nos. 1243 and
1895. The specific observations analyzed can be accessed via doi:10.17909/4xx0-zj76.
Funded by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed
are however those of the author(s) only and do not necessarily reflect those of
the European Union or the European Research Council. Neither the European Union
nor the granting authority can be held responsible for them. R.P.N. acknowledges
funding from JWST programs GO-1933 and GO-2279. Support for this work for R.P.N.
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.
Support for this work for G.I. was provided by NASA through grant JWST-GO-01895
awarded by the Space Telescope Science Institute, which is operated by the Association
of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.
This work has received funding from the Swiss State Secretariat for Education, Research
and Innovation (SERI) under contract No. MB22.00072, as well as from the Swiss National
Science Foundation (SNSF) through project grant 200020_207349. The Cosmic Dawn Center
(DAWN) is funded by the Danish National Research Foundation under grant No. 140.\r\nFacility:
JWST - James Webb Space Telescope, HST - Hubble Space Telescope satellite\r\nSoftware:
Python, matplotlib (Hunter 2007), numpy (Harris et al. 2020), scipy (Virtanen et
al. 2020), Astropy (Astropy Collaboration et al. 2013, 2018), Imfit (Erwin 2015)."
article_number: '129'
article_processing_charge: Yes
article_type: original
author:
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Rohan P.
full_name: Naidu, Rohan P.
last_name: Naidu
- first_name: Gabriel
full_name: Brammer, Gabriel
last_name: Brammer
- first_name: John
full_name: Chisholm, John
last_name: Chisholm
- first_name: Anna-Christina
full_name: Eilers, Anna-Christina
last_name: Eilers
- first_name: Andy
full_name: Goulding, Andy
last_name: Goulding
- first_name: Jenny
full_name: Greene, Jenny
last_name: Greene
- first_name: Daichi
full_name: Kashino, Daichi
last_name: Kashino
- first_name: Ivo
full_name: Labbe, Ivo
last_name: Labbe
- first_name: Simon J.
full_name: Lilly, Simon J.
last_name: Lilly
- first_name: Ruari
full_name: Mackenzie, Ruari
last_name: Mackenzie
- first_name: Pascal A.
full_name: Oesch, Pascal A.
last_name: Oesch
- first_name: Andrea
full_name: Weibel, Andrea
last_name: Weibel
- first_name: Stijn
full_name: Wuyts, Stijn
last_name: Wuyts
- first_name: Mengyuan
full_name: Xiao, Mengyuan
last_name: Xiao
- first_name: Rongmon
full_name: Bordoloi, Rongmon
last_name: Bordoloi
- first_name: Rychard
full_name: Bouwens, Rychard
last_name: Bouwens
- first_name: Pieter
full_name: van Dokkum, Pieter
last_name: van Dokkum
- first_name: Garth
full_name: Illingworth, Garth
last_name: Illingworth
- first_name: Ivan
full_name: Kramarenko, Ivan
last_name: Kramarenko
- first_name: Michael V.
full_name: Maseda, Michael V.
last_name: Maseda
- first_name: Charlotte
full_name: Mason, Charlotte
last_name: Mason
- first_name: Romain A.
full_name: Meyer, Romain A.
last_name: Meyer
- first_name: Erica J.
full_name: Nelson, Erica J.
last_name: Nelson
- first_name: Naveen A.
full_name: Reddy, Naveen A.
last_name: Reddy
- first_name: Irene
full_name: Shivaei, Irene
last_name: Shivaei
- first_name: Robert A.
full_name: Simcoe, Robert A.
last_name: Simcoe
- first_name: Minghao
full_name: Yue, Minghao
last_name: Yue
citation:
ama: 'Matthee JJ, Naidu RP, Brammer G, et al. Little Red Dots: An abundant population
of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST
surveys. The Astrophysical Journal. 2024;963(2). doi:10.3847/1538-4357/ad2345'
apa: 'Matthee, J. J., Naidu, R. P., Brammer, G., Chisholm, J., Eilers, A.-C., Goulding,
A., … Yue, M. (2024). Little Red Dots: An abundant population of faint active
galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys. The
Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ad2345'
chicago: 'Matthee, Jorryt J, Rohan P. Naidu, Gabriel Brammer, John Chisholm, Anna-Christina
Eilers, Andy Goulding, Jenny Greene, et al. “Little Red Dots: An Abundant Population
of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST
Surveys.” The Astrophysical Journal. American Astronomical Society, 2024.
https://doi.org/10.3847/1538-4357/ad2345.'
ieee: 'J. J. Matthee et al., “Little Red Dots: An abundant population of
faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys,”
The Astrophysical Journal, vol. 963, no. 2. American Astronomical Society,
2024.'
ista: 'Matthee JJ, Naidu RP, Brammer G, Chisholm J, Eilers A-C, Goulding A, Greene
J, Kashino D, Labbe I, Lilly SJ, Mackenzie R, Oesch PA, Weibel A, Wuyts S, Xiao
M, Bordoloi R, Bouwens R, van Dokkum P, Illingworth G, Kramarenko I, Maseda MV,
Mason C, Meyer RA, Nelson EJ, Reddy NA, Shivaei I, Simcoe RA, Yue M. 2024. Little
Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed
by the EIGER and FRESCO JWST surveys. The Astrophysical Journal. 963(2), 129.'
mla: 'Matthee, Jorryt J., et al. “Little Red Dots: An Abundant Population of Faint
Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys.”
The Astrophysical Journal, vol. 963, no. 2, 129, American Astronomical
Society, 2024, doi:10.3847/1538-4357/ad2345.'
short: J.J. Matthee, R.P. Naidu, G. Brammer, J. Chisholm, A.-C. Eilers, A. Goulding,
J. Greene, D. Kashino, I. Labbe, S.J. Lilly, R. Mackenzie, P.A. Oesch, A. Weibel,
S. Wuyts, M. Xiao, R. Bordoloi, R. Bouwens, P. van Dokkum, G. Illingworth, I.
Kramarenko, M.V. Maseda, C. Mason, R.A. Meyer, E.J. Nelson, N.A. Reddy, I. Shivaei,
R.A. Simcoe, M. Yue, The Astrophysical Journal 963 (2024).
corr_author: '1'
date_created: 2024-03-25T08:54:47Z
date_published: 2024-03-07T00:00:00Z
date_updated: 2025-09-04T13:15:26Z
day: '07'
ddc:
- '550'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ad2345
external_id:
isi:
- '001184703600001'
file:
- access_level: open_access
checksum: dc7af4694f9f94a551417ab49fa43edf
content_type: application/pdf
creator: dernst
date_created: 2024-03-25T09:31:58Z
date_updated: 2024-03-25T09:31:58Z
file_id: '15184'
file_name: 2024_AstrophysicalJourn_Matthee.pdf
file_size: 6047536
relation: main_file
success: 1
file_date_updated: 2024-03-25T09:31:58Z
has_accepted_license: '1'
intvolume: ' 963'
isi: 1
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
grant_number: '101076224'
name: Young galaxies as tracers and agents of cosmic reionization
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
related_material:
link:
- description: News on ISTA website
relation: press_release
url: https://ista.ac.at/en/news/baby-quasars-growing-supermassive-black-holes/
scopus_import: '1'
status: public
title: 'Little Red Dots: An abundant population of faint active galactic nuclei at
z ∼ 5 revealed by the EIGER and FRESCO JWST surveys'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 963
year: '2024'
...
---
DOAJ_listed: '1'
_id: '15181'
abstract:
- lang: eng
text: We demonstrate the failure of the adiabatic Born-Oppenheimer approximation
to describe the ground state of a quantum impurity within an ultracold Fermi gas
despite substantial mass differences between the bath and impurity species. Increasing
repulsion leads to the appearance of nonadiabatic couplings between the fast bath
and slow impurity degrees of freedom, which reduce the parity symmetry of the
latter according to the pseudo Jahn-Teller effect. The presence of this mechanism
is associated to a conical intersection involving the impurity position and the
inverse of the interaction strength, which acts as a synthetic dimension. We elucidate
the presence of these effects via a detailed ground-state analysis involving the
comparison of ab initio fully correlated simulations with effective models. Our
study suggests ultracold atomic ensembles as potent emulators of complex molecular
phenomena.
acknowledgement: "This work has been funded by the Cluster of Excellence “Advanced
Imaging of Matter” of the Deutsche Forschungsgemeinschaft (DFG) - EXC 2056 - Project
ID 390715994.\r\nG.M.K. gratefully acknowledges funding from the European Union’s
Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie
Grant Agreement No. 101034413."
article_number: '013257'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: A.
full_name: Becker, A.
last_name: Becker
- first_name: Georgios
full_name: Koutentakis, Georgios
id: d7b23d3a-9e21-11ec-b482-f76739596b95
last_name: Koutentakis
- first_name: P.
full_name: Schmelcher, P.
last_name: Schmelcher
citation:
ama: Becker A, Koutentakis G, Schmelcher P. Synthetic dimension-induced pseudo Jahn-Teller
effect in one-dimensional confined fermions. Physical Review Research.
2024;6(1). doi:10.1103/physrevresearch.6.013257
apa: Becker, A., Koutentakis, G., & Schmelcher, P. (2024). Synthetic dimension-induced
pseudo Jahn-Teller effect in one-dimensional confined fermions. Physical Review
Research. American Physical Society. https://doi.org/10.1103/physrevresearch.6.013257
chicago: Becker, A., Georgios Koutentakis, and P. Schmelcher. “Synthetic Dimension-Induced
Pseudo Jahn-Teller Effect in One-Dimensional Confined Fermions.” Physical Review
Research. American Physical Society, 2024. https://doi.org/10.1103/physrevresearch.6.013257.
ieee: A. Becker, G. Koutentakis, and P. Schmelcher, “Synthetic dimension-induced
pseudo Jahn-Teller effect in one-dimensional confined fermions,” Physical Review
Research, vol. 6, no. 1. American Physical Society, 2024.
ista: Becker A, Koutentakis G, Schmelcher P. 2024. Synthetic dimension-induced pseudo
Jahn-Teller effect in one-dimensional confined fermions. Physical Review Research.
6(1), 013257.
mla: Becker, A., et al. “Synthetic Dimension-Induced Pseudo Jahn-Teller Effect in
One-Dimensional Confined Fermions.” Physical Review Research, vol. 6, no.
1, 013257, American Physical Society, 2024, doi:10.1103/physrevresearch.6.013257.
short: A. Becker, G. Koutentakis, P. Schmelcher, Physical Review Research 6 (2024).
date_created: 2024-03-25T08:57:07Z
date_published: 2024-03-01T00:00:00Z
date_updated: 2025-05-14T09:32:03Z
day: '01'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1103/physrevresearch.6.013257
ec_funded: 1
external_id:
arxiv:
- '2310.17995'
file:
- access_level: open_access
checksum: 4e0e58d1f58386fb016284c84db2a300
content_type: application/pdf
creator: dernst
date_created: 2024-03-25T09:24:55Z
date_updated: 2024-03-25T09:24:55Z
file_id: '15183'
file_name: 2024_PhysicalReviewResearch_Becker.pdf
file_size: 2207067
relation: main_file
success: 1
file_date_updated: 2024-03-25T09:24:55Z
has_accepted_license: '1'
intvolume: ' 6'
issue: '1'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Physical Review Research
publication_identifier:
eissn:
- 2643-1564
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined
fermions
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: 6
year: '2024'
...
---
APC_amount: 2940 EUR
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '15186'
abstract:
- lang: eng
text: The elimination of rain evaporation in the planetary boundary layer (PBL)
has been found to lead to convective self‐aggregation (CSA) even without radiative
feedback, but the precise mechanisms underlying this phenomenon remain unclear.
We conducted cloud‐resolving simulations with two domain sizes and progressively
reduced rain evaporation in the PBL. Surprisingly, CSA only occurred when rain
evaporation was almost completely removed. The additional convective heating resulting
from the reduction of evaporative cooling in the moist patch was found to be the
trigger, thereafter a dry subsidence intrusion into the PBL in the dry patch takes
over and sets CSA in motion. Temperature and moisture anomalies oppose each other
in their buoyancy effects, hence explaining the need for almost total rain evaporation
removal. We also found radiative cooling and not cold pools to be the leading
cause for the comparative ease of CSA to take place in the larger domain.
acknowledgement: "YLH is supported by funding from the European Union's Horizon 2020
research and innovation programme under the Marie Skłodowska-Curie Grant 101034413.
CM gratefully acknowledges funding from the European Research Council (ERC) under
the European Union's Horizon 2020 research and innovation program (Project CLUSTER,
Grant 805041). The authors warmly thank Steven Sherwood, Jiawei Bao, Bidyut Goswami,
and Martin Janssens for stimulating and helpful discussions. They also thank Christopher
Holloway and an anonymous reviewer for providing helpful feedback that greatly improved
this manuscript.\r\n"
article_number: ' e2023GL106523'
article_processing_charge: Yes
article_type: original
author:
- first_name: Yi-Ling
full_name: Hwong, Yi-Ling
id: 1217aa61-4dd1-11ec-9ac3-f2ba3f17ee22
last_name: Hwong
orcid: 0000-0001-9281-3479
- first_name: Caroline J
full_name: Muller, Caroline J
id: f978ccb0-3f7f-11eb-b193-b0e2bd13182b
last_name: Muller
orcid: 0000-0001-5836-5350
citation:
ama: Hwong Y-L, Muller CJ. The unreasonable efficiency of total rain evaporation
removal in triggering convective self‐aggregation. Geophysical Research Letters.
2024;51(6). doi:10.1029/2023gl106523
apa: Hwong, Y.-L., & Muller, C. J. (2024). The unreasonable efficiency of total
rain evaporation removal in triggering convective self‐aggregation. Geophysical
Research Letters. Wiley. https://doi.org/10.1029/2023gl106523
chicago: Hwong, Yi-Ling, and Caroline J Muller. “The Unreasonable Efficiency of
Total Rain Evaporation Removal in Triggering Convective Self‐aggregation.” Geophysical
Research Letters. Wiley, 2024. https://doi.org/10.1029/2023gl106523.
ieee: Y.-L. Hwong and C. J. Muller, “The unreasonable efficiency of total rain evaporation
removal in triggering convective self‐aggregation,” Geophysical Research Letters,
vol. 51, no. 6. Wiley, 2024.
ista: Hwong Y-L, Muller CJ. 2024. The unreasonable efficiency of total rain evaporation
removal in triggering convective self‐aggregation. Geophysical Research Letters.
51(6), e2023GL106523.
mla: Hwong, Yi-Ling, and Caroline J. Muller. “The Unreasonable Efficiency of Total
Rain Evaporation Removal in Triggering Convective Self‐aggregation.” Geophysical
Research Letters, vol. 51, no. 6, e2023GL106523, Wiley, 2024, doi:10.1029/2023gl106523.
short: Y.-L. Hwong, C.J. Muller, Geophysical Research Letters 51 (2024).
corr_author: '1'
date_created: 2024-03-25T10:27:30Z
date_published: 2024-03-19T00:00:00Z
date_updated: 2025-09-04T13:16:39Z
day: '19'
ddc:
- '550'
department:
- _id: CaMu
doi: 10.1029/2023gl106523
ec_funded: 1
external_id:
isi:
- '001187002300001'
file:
- access_level: open_access
checksum: eacb011091a503b9e7b748fef639ba4c
content_type: application/pdf
creator: dernst
date_created: 2024-03-25T11:28:25Z
date_updated: 2024-03-25T11:28:25Z
file_id: '15187'
file_name: 2024_GeophysResLetters_Hwong.pdf
file_size: 1280108
relation: main_file
success: 1
file_date_updated: 2024-03-25T11:28:25Z
has_accepted_license: '1'
intvolume: ' 51'
isi: 1
issue: '6'
keyword:
- General Earth and Planetary Sciences
- Geophysics
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
- _id: 629205d8-2b32-11ec-9570-e1356ff73576
call_identifier: H2020
grant_number: '805041'
name: Organization of CLoUdS, and implications of Tropical cyclones and for the
Energetics of the tropics, in current and waRming climate
publication: Geophysical Research Letters
publication_identifier:
eissn:
- 1944-8007
issn:
- 0094-8276
publication_status: published
publisher: Wiley
quality_controlled: '1'
related_material:
record:
- id: '19307'
relation: research_data
status: public
scopus_import: '1'
status: public
title: The unreasonable efficiency of total rain evaporation removal in triggering
convective self‐aggregation
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 51
year: '2024'
...
---
_id: '15189'
abstract:
- lang: eng
text: Cataclysmic variables (CVs) that have evolved past the period minimum during
their lifetimes are predicted to be systems with a brown dwarf donor. While population
synthesis models predict that around 40–70 per cent of the Galactic CVs are post-period
minimum systems referred to as ‘period bouncers’, only a few dozen confirmed systems
are known. We report the study and characterization of a new eclipsing CV, SRGeJ041130.3+685350
(SRGeJ0411), discovered from a joint SRG/eROSITA and ZTF programme. The optical
spectrum of SRGeJ0411 shows prominent hydrogen and helium emission lines, typical
for CVs. We obtained optical high-speed photometry to confirm the eclipse of SRGeJ0411
and determine the orbital period to be Porb ≈ 97.530 min. The spectral energy
distribution suggests that the donor has an effective temperature of ≲ 1800 K.
We constrain the donor mass with the period–density relationship for Roche lobe-filling
stars and find that Mdonor ≲ 0.04 M⊙. The binary parameters are consistent with
evolutionary models for post-period minimum CVs, suggesting that SRGeJ0411 is
a new period bouncer. The optical emission lines of SRGeJ0411 are single-peaked
despite the system being eclipsing, which is typically only seen due to stream-fed
accretion in polars. X-ray spectroscopy hints that the white dwarf in SRGeJ0411
could be magnetic, but verifying the magnetic nature of SRGeJ0411 requires further
investigation. The lack of optical outbursts has made SRGeJ0411 elusive in previous
surveys, and joint X-ray and optical surveys highlight the potential for discovering
similar systems in the near future.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Ilkham
full_name: Galiullin, Ilkham
last_name: Galiullin
- first_name: Antonio C
full_name: Rodriguez, Antonio C
last_name: Rodriguez
- first_name: Shrinivas R
full_name: Kulkarni, Shrinivas R
last_name: Kulkarni
- first_name: Rashid
full_name: Sunyaev, Rashid
last_name: Sunyaev
- first_name: Marat
full_name: Gilfanov, Marat
last_name: Gilfanov
- first_name: Ilfan
full_name: Bikmaev, Ilfan
last_name: Bikmaev
- first_name: Lev
full_name: Yungelson, Lev
last_name: Yungelson
- first_name: Jan
full_name: van Roestel, Jan
last_name: van Roestel
- first_name: Boris T
full_name: Gänsicke, Boris T
last_name: Gänsicke
- first_name: Irek
full_name: Khamitov, Irek
last_name: Khamitov
- first_name: Paula
full_name: Szkody, Paula
last_name: Szkody
- first_name: Kareem
full_name: El-Badry, Kareem
last_name: El-Badry
- first_name: Mikhail
full_name: Suslikov, Mikhail
last_name: Suslikov
- first_name: Thomas A
full_name: Prince, Thomas A
last_name: Prince
- first_name: Mikhail
full_name: Buntov, Mikhail
last_name: Buntov
- first_name: Ilaria
full_name: Caiazzo, Ilaria
id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
last_name: Caiazzo
orcid: 0000-0002-4770-5388
- first_name: Mark
full_name: Gorbachev, Mark
last_name: Gorbachev
- first_name: Matthew J
full_name: Graham, Matthew J
last_name: Graham
- first_name: Rustam
full_name: Gumerov, Rustam
last_name: Gumerov
- first_name: Eldar
full_name: Irtuganov, Eldar
last_name: Irtuganov
- first_name: Russ R
full_name: Laher, Russ R
last_name: Laher
- first_name: Pavel
full_name: Medvedev, Pavel
last_name: Medvedev
- first_name: Reed
full_name: Riddle, Reed
last_name: Riddle
- first_name: Ben
full_name: Rusholme, Ben
last_name: Rusholme
- first_name: Nail
full_name: Sakhibullin, Nail
last_name: Sakhibullin
- first_name: Alexander
full_name: Sklyanov, Alexander
last_name: Sklyanov
- first_name: Zachary P
full_name: Vanderbosch, Zachary P
last_name: Vanderbosch
citation:
ama: 'Galiullin I, Rodriguez AC, Kulkarni SR, et al. A joint SRG/eROSITA + ZTF search:
Discovery of a 97-min period eclipsing cataclysmic variable with evidence of a
brown dwarf secondary. Monthly Notices of the Royal Astronomical Society.
2024;528(1):676-692. doi:10.1093/mnras/stae012'
apa: 'Galiullin, I., Rodriguez, A. C., Kulkarni, S. R., Sunyaev, R., Gilfanov, M.,
Bikmaev, I., … Vanderbosch, Z. P. (2024). A joint SRG/eROSITA + ZTF search: Discovery
of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf
secondary. Monthly Notices of the Royal Astronomical Society. Oxford University
Press. https://doi.org/10.1093/mnras/stae012'
chicago: 'Galiullin, Ilkham, Antonio C Rodriguez, Shrinivas R Kulkarni, Rashid Sunyaev,
Marat Gilfanov, Ilfan Bikmaev, Lev Yungelson, et al. “A Joint SRG/EROSITA + ZTF
Search: Discovery of a 97-Min Period Eclipsing Cataclysmic Variable with Evidence
of a Brown Dwarf Secondary.” Monthly Notices of the Royal Astronomical Society.
Oxford University Press, 2024. https://doi.org/10.1093/mnras/stae012.'
ieee: 'I. Galiullin et al., “A joint SRG/eROSITA + ZTF search: Discovery
of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf
secondary,” Monthly Notices of the Royal Astronomical Society, vol. 528,
no. 1. Oxford University Press, pp. 676–692, 2024.'
ista: 'Galiullin I, Rodriguez AC, Kulkarni SR, Sunyaev R, Gilfanov M, Bikmaev I,
Yungelson L, van Roestel J, Gänsicke BT, Khamitov I, Szkody P, El-Badry K, Suslikov
M, Prince TA, Buntov M, Caiazzo I, Gorbachev M, Graham MJ, Gumerov R, Irtuganov
E, Laher RR, Medvedev P, Riddle R, Rusholme B, Sakhibullin N, Sklyanov A, Vanderbosch
ZP. 2024. A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing
cataclysmic variable with evidence of a brown dwarf secondary. Monthly Notices
of the Royal Astronomical Society. 528(1), 676–692.'
mla: 'Galiullin, Ilkham, et al. “A Joint SRG/EROSITA + ZTF Search: Discovery of
a 97-Min Period Eclipsing Cataclysmic Variable with Evidence of a Brown Dwarf
Secondary.” Monthly Notices of the Royal Astronomical Society, vol. 528,
no. 1, Oxford University Press, 2024, pp. 676–92, doi:10.1093/mnras/stae012.'
short: I. Galiullin, A.C. Rodriguez, S.R. Kulkarni, R. Sunyaev, M. Gilfanov, I.
Bikmaev, L. Yungelson, J. van Roestel, B.T. Gänsicke, I. Khamitov, P. Szkody,
K. El-Badry, M. Suslikov, T.A. Prince, M. Buntov, I. Caiazzo, M. Gorbachev, M.J.
Graham, R. Gumerov, E. Irtuganov, R.R. Laher, P. Medvedev, R. Riddle, B. Rusholme,
N. Sakhibullin, A. Sklyanov, Z.P. Vanderbosch, Monthly Notices of the Royal Astronomical
Society 528 (2024) 676–692.
date_created: 2024-03-26T09:43:55Z
date_published: 2024-01-04T00:00:00Z
date_updated: 2024-04-02T06:50:01Z
day: '04'
doi: 10.1093/mnras/stae012
extern: '1'
external_id:
arxiv:
- '2401.04178'
intvolume: ' 528'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stae012
month: '01'
oa: 1
oa_version: Published Version
page: 676-692
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing cataclysmic
variable with evidence of a brown dwarf secondary'
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: 528
year: '2024'
...
---
_id: '15191'
abstract:
- lang: eng
text: Despite their shared origin, members of globular clusters display star-to-star
variations in composition. The observed pattern of element abundances is unique
to these stellar environments and cannot be fully explained by any proposed mechanism.
It remains unclear whether stars form with chemical heterogeneity or inherit it
from interactions with other members. These scenarios may be differentiated by
the dependence of chemical spread on stellar mass; however, obtaining a sufficiently
large mass baseline requires abundance measurements on the lower main sequence,
which is too faint for spectroscopy even in the nearest globular clusters. We
developed a stellar modeling method to obtain precise chemical abundances for
stars near the end of the main sequence from multiband photometry, and we applied
it to the globular cluster 47 Tucanae. The computational efficiency is attained
by matching chemical elements to the model components that are most sensitive
to their abundance. We determined [O/Fe] for ∼5000 members below the main-sequence
knee at the level of accuracy, comparable to the spectroscopic measurements of
evolved members in the literature. The inferred distribution disfavors stellar
interactions as the origin of chemical spread; however, an accurate theory of
accretion is required to draw a more definitive conclusion. We anticipate that
future observations of 47 Tucanae with the James Webb Space Telescope will extend
the mass baseline of our analysis into the substellar regime. Therefore, we present
predicted color–magnitude diagrams and mass–magnitude relations for the brown
dwarf members of 47 Tucanae.
article_number: '139'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Roman
full_name: Gerasimov, Roman
last_name: Gerasimov
- first_name: Adam J.
full_name: Burgasser, Adam J.
last_name: Burgasser
- first_name: Ilaria
full_name: Caiazzo, Ilaria
id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
last_name: Caiazzo
orcid: 0000-0002-4770-5388
- first_name: Derek
full_name: Homeier, Derek
last_name: Homeier
- first_name: Harvey B.
full_name: Richer, Harvey B.
last_name: Richer
- first_name: Matteo
full_name: Correnti, Matteo
last_name: Correnti
- first_name: Jeremy
full_name: Heyl, Jeremy
last_name: Heyl
citation:
ama: Gerasimov R, Burgasser AJ, Caiazzo I, et al. Exploring the chemistry and mass
function of the globular cluster 47 Tucanae with new theoretical color–magnitude
diagrams. The Astrophysical Journal. 2024;961(1). doi:10.3847/1538-4357/ad08bf
apa: Gerasimov, R., Burgasser, A. J., Caiazzo, I., Homeier, D., Richer, H. B., Correnti,
M., & Heyl, J. (2024). Exploring the chemistry and mass function of the globular
cluster 47 Tucanae with new theoretical color–magnitude diagrams. The Astrophysical
Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ad08bf
chicago: Gerasimov, Roman, Adam J. Burgasser, Ilaria Caiazzo, Derek Homeier, Harvey
B. Richer, Matteo Correnti, and Jeremy Heyl. “Exploring the Chemistry and Mass
Function of the Globular Cluster 47 Tucanae with New Theoretical Color–Magnitude
Diagrams.” The Astrophysical Journal. American Astronomical Society, 2024.
https://doi.org/10.3847/1538-4357/ad08bf.
ieee: R. Gerasimov et al., “Exploring the chemistry and mass function of
the globular cluster 47 Tucanae with new theoretical color–magnitude diagrams,”
The Astrophysical Journal, vol. 961, no. 1. American Astronomical Society,
2024.
ista: Gerasimov R, Burgasser AJ, Caiazzo I, Homeier D, Richer HB, Correnti M, Heyl
J. 2024. Exploring the chemistry and mass function of the globular cluster 47
Tucanae with new theoretical color–magnitude diagrams. The Astrophysical Journal.
961(1), 139.
mla: Gerasimov, Roman, et al. “Exploring the Chemistry and Mass Function of the
Globular Cluster 47 Tucanae with New Theoretical Color–Magnitude Diagrams.” The
Astrophysical Journal, vol. 961, no. 1, 139, American Astronomical Society,
2024, doi:10.3847/1538-4357/ad08bf.
short: R. Gerasimov, A.J. Burgasser, I. Caiazzo, D. Homeier, H.B. Richer, M. Correnti,
J. Heyl, The Astrophysical Journal 961 (2024).
date_created: 2024-03-26T09:44:50Z
date_published: 2024-01-22T00:00:00Z
date_updated: 2024-04-02T06:52:43Z
day: '22'
doi: 10.3847/1538-4357/ad08bf
extern: '1'
external_id:
arxiv:
- '2310.11800'
intvolume: ' 961'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.3847/1538-4357/ad08bf
month: '01'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Exploring the chemistry and mass function of the globular cluster 47 Tucanae
with new theoretical color–magnitude diagrams
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: 961
year: '2024'
...
---
OA_place: publisher
OA_type: hybrid
_id: '15247'
abstract:
- lang: eng
text: Extending the notion of sunflowers, we call a family of at least two sets
an odd-sunflower if every element of the underlying set is contained in an odd
number of sets or in none of them. It follows from the Erdős–Szemerédi conjecture,
recently proved by Naslund and Sawin, that there is a constant <2 such that every
family of subsets of an n-element set that contains no odd-sunflower consists
of at most n sets. We construct such families of size at least 1.5021n. We also
characterize minimal odd-sunflowers of triples.
acknowledgement: We are grateful to Balázs Keszegh, and to the members of the Miklós
Schweitzer Competition committee of 2022 for valuable discussions, and Shira Zerbib
for pointing out several important mathematical typos.
article_number: '105889'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Peter
full_name: Frankl, Peter
last_name: Frankl
- first_name: János
full_name: Pach, János
id: E62E3130-B088-11EA-B919-BF823C25FEA4
last_name: Pach
- first_name: Dömötör
full_name: Pálvölgyi, Dömötör
last_name: Pálvölgyi
citation:
ama: Frankl P, Pach J, Pálvölgyi D. Odd-sunflowers. Journal of Combinatorial
Theory, Series A. 2024;206(8). doi:10.1016/j.jcta.2024.105889
apa: Frankl, P., Pach, J., & Pálvölgyi, D. (2024). Odd-sunflowers. Journal
of Combinatorial Theory, Series A. Elsevier. https://doi.org/10.1016/j.jcta.2024.105889
chicago: Frankl, Peter, János Pach, and Dömötör Pálvölgyi. “Odd-Sunflowers.” Journal
of Combinatorial Theory, Series A. Elsevier, 2024. https://doi.org/10.1016/j.jcta.2024.105889.
ieee: P. Frankl, J. Pach, and D. Pálvölgyi, “Odd-sunflowers,” Journal of Combinatorial
Theory, Series A, vol. 206, no. 8. Elsevier, 2024.
ista: Frankl P, Pach J, Pálvölgyi D. 2024. Odd-sunflowers. Journal of Combinatorial
Theory, Series A. 206(8), 105889.
mla: Frankl, Peter, et al. “Odd-Sunflowers.” Journal of Combinatorial Theory,
Series A, vol. 206, no. 8, 105889, Elsevier, 2024, doi:10.1016/j.jcta.2024.105889.
short: P. Frankl, J. Pach, D. Pálvölgyi, Journal of Combinatorial Theory, Series
A 206 (2024).
corr_author: '1'
date_created: 2024-03-31T22:01:11Z
date_published: 2024-08-01T00:00:00Z
date_updated: 2025-09-04T13:20:39Z
day: '01'
ddc:
- '510'
department:
- _id: HeEd
doi: 10.1016/j.jcta.2024.105889
external_id:
arxiv:
- '2310.16701'
isi:
- '001217739200001'
file:
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checksum: ffc29d65e712849f0d31009271e06a63
content_type: application/pdf
creator: dernst
date_created: 2025-01-09T08:37:20Z
date_updated: 2025-01-09T08:37:20Z
file_id: '18791'
file_name: 2024_JourCombiTheoryA_Frankl.pdf
file_size: 366029
relation: main_file
success: 1
file_date_updated: 2025-01-09T08:37:20Z
has_accepted_license: '1'
intvolume: ' 206'
isi: 1
issue: '8'
language:
- iso: eng
license: https://creativecommons.org/licenses/by-nc/4.0/
month: '08'
oa: 1
oa_version: Published Version
publication: Journal of Combinatorial Theory, Series A
publication_identifier:
eissn:
- 1096-0899
issn:
- 0097-3165
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Odd-sunflowers
tmp:
image: /images/cc_by_nc.png
legal_code_url: https://creativecommons.org/licenses/by-nc/4.0/legalcode
name: Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)
short: CC BY-NC (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 206
year: '2024'
...
---
OA_place: publisher
OA_type: hybrid
_id: '15248'
abstract:
- lang: eng
text: Applying the technique of p-adic integration, we prove the topological mirror
symmetry conjecture of Hausel-Thaddeus for the moduli spaces of (strongly) parabolic
Higgs bundles for the structure groups SLn and PGLn, building on previous work
of Groechenig-Wyss-Ziegler on the non-parabolic case. We also prove the E-polynomial
of the smooth moduli space of parabolic GLn-Higgs bundles is independent of the
degree of the underlying vector bundles.
acknowledgement: Shiyu Shen has received funding from the European Union's Horizon
2020 research and innovation program under the Marie Skłodowska-Curie grant agreement
No. 101034413.
article_number: '109616'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Shiyu
full_name: Shen, Shiyu
id: 544cccd3-9005-11ec-87bc-94aef1c5b814
last_name: Shen
orcid: 0000-0002-4444-8718
citation:
ama: Shen S. Mirror symmetry for parabolic Higgs bundles via p-adic integration.
Advances in Mathematics. 2024;443(5). doi:10.1016/j.aim.2024.109616
apa: Shen, S. (2024). Mirror symmetry for parabolic Higgs bundles via p-adic integration.
Advances in Mathematics. Elsevier. https://doi.org/10.1016/j.aim.2024.109616
chicago: Shen, Shiyu. “Mirror Symmetry for Parabolic Higgs Bundles via P-Adic Integration.”
Advances in Mathematics. Elsevier, 2024. https://doi.org/10.1016/j.aim.2024.109616.
ieee: S. Shen, “Mirror symmetry for parabolic Higgs bundles via p-adic integration,”
Advances in Mathematics, vol. 443, no. 5. Elsevier, 2024.
ista: Shen S. 2024. Mirror symmetry for parabolic Higgs bundles via p-adic integration.
Advances in Mathematics. 443(5), 109616.
mla: Shen, Shiyu. “Mirror Symmetry for Parabolic Higgs Bundles via P-Adic Integration.”
Advances in Mathematics, vol. 443, no. 5, 109616, Elsevier, 2024, doi:10.1016/j.aim.2024.109616.
short: S. Shen, Advances in Mathematics 443 (2024).
corr_author: '1'
date_created: 2024-03-31T22:01:11Z
date_published: 2024-05-01T00:00:00Z
date_updated: 2025-09-04T13:21:18Z
day: '01'
ddc:
- '510'
department:
- _id: TaHa
doi: 10.1016/j.aim.2024.109616
ec_funded: 1
external_id:
arxiv:
- '2302.02817'
isi:
- '001216128200001'
file:
- access_level: open_access
checksum: 68f2f08136ccf547891a16a2c0621e97
content_type: application/pdf
creator: dernst
date_created: 2024-07-22T12:10:03Z
date_updated: 2024-07-22T12:10:03Z
file_id: '17315'
file_name: 2024_AdvancesMath_Shen.pdf
file_size: 702889
relation: main_file
success: 1
file_date_updated: 2024-07-22T12:10:03Z
has_accepted_license: '1'
intvolume: ' 443'
isi: 1
issue: '5'
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Advances in Mathematics
publication_identifier:
eissn:
- 1090-2082
issn:
- 0001-8708
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Mirror symmetry for parabolic Higgs bundles via p-adic integration
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 443
year: '2024'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '15249'
abstract:
- lang: eng
text: Observationally mapping the relation between galaxies and the intergalactic
medium (IGM) is of key interest for studies of cosmic reionization. Diffuse hydrogen
gas has typically been observed in H I Lyman-α (Lyα) absorption in the spectra
of bright background quasars. However, it is important to extend these measurements
to background galaxies as quasars become increasingly rare at high redshift and
rarely probe closely separated sight lines. Here, we use deep integral field spectroscopy
in the MUSE eXtremely Deep Field to demonstrate the measurement of the Lyα transmission
at z ≈ 4 in absorption to a background galaxy at z = 4.77. The H I transmission
is consistent with independent quasar sight lines at similar redshifts. Exploiting
the high number of spectroscopic redshifts of faint galaxies (500 between z =
4.0–4.7 within a radius of 8 arcmin) that are tracers of the density field, we
show that Lyα transmission is inversely correlated with galaxy density, i.e. transparent
regions in the Lyα forest mark underdense regions at z ≈ 4. Due to large-scale
clustering, galaxies are surrounded by excess H I absorption over the cosmic mean
out to 4 cMpc/h70. We also find that redshifts from the peak of the Lyα line are
typically offset from the systemic redshift by +170 km s−1. This work extends
results from z ≈ 2–3 to higher redshifts and demonstrates the power of deep integral
field spectroscopy to simultaneously measure the ionization structure of the IGM
and the large-scale density field in the early Universe.
acknowledgement: We thank the referee for constructive comments that helped improving
the paper. Based on observations collected at the European Southern Observatory
under ESO programme 1101.A-0127. Funded by the European Union (ERC, AGENTS, 101076224).
Views and opinions expressed are however those of the author(s) only and do not
necessarily reflect those of the European Union or the European Research Council.
Neither the European Union nor the granting authority can be held responsible for
them. GP acknowledges support from the Netherlands Research School for Astronomy
(Nederlandse Onderzoekschool Voor Astronomie, NOVA). JB acknowledges financial support
from the Fundação para a Ciência e a Tecnologia (FCT) through national funds PTDC/FIS-AST/4862/2020,
work contract 2020.03379.CEECIND, and research grants UIDB/04434/2020 and UIDP/04434/2020.
TU and LW acknowledge funding by the European Research Council through ERC-AdG SPECMAP-CGM,
GA 101020943. TG is supported by the ERC Starting grant 757258 ‘TRIPLE’.
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- 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: Christopher
full_name: Golling, Christopher
last_name: Golling
- first_name: Ruari
full_name: Mackenzie, Ruari
last_name: Mackenzie
- first_name: Gabriele
full_name: Pezzulli, Gabriele
last_name: Pezzulli
- first_name: Simon
full_name: Lilly, Simon
last_name: Lilly
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Roland
full_name: Bacon, Roland
last_name: Bacon
- first_name: Haruka
full_name: Kusakabe, Haruka
last_name: Kusakabe
- first_name: Tanya
full_name: Urrutia, Tanya
last_name: Urrutia
- first_name: Leindert
full_name: Boogaard, Leindert
last_name: Boogaard
- first_name: Jarle
full_name: Brinchmann, Jarle
last_name: Brinchmann
- first_name: Michael V.
full_name: Maseda, Michael V.
last_name: Maseda
- first_name: Thibault
full_name: Garel, Thibault
last_name: Garel
- first_name: Nicolas F.
full_name: Bouché, Nicolas F.
last_name: Bouché
- first_name: Lutz
full_name: Wisotzki, Lutz
last_name: Wisotzki
citation:
ama: Matthee JJ, Golling C, Mackenzie R, et al. Large-scale excess H I absorption
around z ≈ 4 galaxies detected in a background galaxy spectrum in the MUSE eXtremely
deep field. Monthly Notices of the Royal Astronomical Society. 2024;529(3):2794-2806.
doi:10.1093/mnras/stae673
apa: Matthee, J. J., Golling, C., Mackenzie, R., Pezzulli, G., Lilly, S., Schaye,
J., … Wisotzki, L. (2024). Large-scale excess H I absorption around z ≈ 4 galaxies
detected in a background galaxy spectrum in the MUSE eXtremely deep field. Monthly
Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stae673
chicago: Matthee, Jorryt J, Christopher Golling, Ruari Mackenzie, Gabriele Pezzulli,
Simon Lilly, Joop Schaye, Roland Bacon, et al. “Large-Scale Excess H I Absorption
around z ≈ 4 Galaxies Detected in a Background Galaxy Spectrum in the MUSE EXtremely
Deep Field.” Monthly Notices of the Royal Astronomical Society. Oxford
University Press, 2024. https://doi.org/10.1093/mnras/stae673.
ieee: J. J. Matthee et al., “Large-scale excess H I absorption around z ≈
4 galaxies detected in a background galaxy spectrum in the MUSE eXtremely deep
field,” Monthly Notices of the Royal Astronomical Society, vol. 529, no.
3. Oxford University Press, pp. 2794–2806, 2024.
ista: Matthee JJ, Golling C, Mackenzie R, Pezzulli G, Lilly S, Schaye J, Bacon R,
Kusakabe H, Urrutia T, Boogaard L, Brinchmann J, Maseda MV, Garel T, Bouché NF,
Wisotzki L. 2024. Large-scale excess H I absorption around z ≈ 4 galaxies detected
in a background galaxy spectrum in the MUSE eXtremely deep field. Monthly Notices
of the Royal Astronomical Society. 529(3), 2794–2806.
mla: Matthee, Jorryt J., et al. “Large-Scale Excess H I Absorption around z ≈ 4
Galaxies Detected in a Background Galaxy Spectrum in the MUSE EXtremely Deep Field.”
Monthly Notices of the Royal Astronomical Society, vol. 529, no. 3, Oxford
University Press, 2024, pp. 2794–806, doi:10.1093/mnras/stae673.
short: J.J. Matthee, C. Golling, R. Mackenzie, G. Pezzulli, S. Lilly, J. Schaye,
R. Bacon, H. Kusakabe, T. Urrutia, L. Boogaard, J. Brinchmann, M.V. Maseda, T.
Garel, N.F. Bouché, L. Wisotzki, Monthly Notices of the Royal Astronomical Society
529 (2024) 2794–2806.
corr_author: '1'
date_created: 2024-03-31T22:01:12Z
date_published: 2024-04-01T00:00:00Z
date_updated: 2025-09-04T13:18:02Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1093/mnras/stae673
external_id:
arxiv:
- '2305.15346'
isi:
- '001188770300019'
file:
- access_level: open_access
checksum: 1e65c40a71e565eebdc4c5ff11822ba2
content_type: application/pdf
creator: dernst
date_created: 2024-04-02T08:42:17Z
date_updated: 2024-04-02T08:42:17Z
file_id: '15255'
file_name: 2024_MonthlyNRoyalAstronSoc_Matthee.pdf
file_size: 2626735
relation: main_file
success: 1
file_date_updated: 2024-04-02T08:42:17Z
has_accepted_license: '1'
intvolume: ' 529'
isi: 1
issue: '3'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
page: 2794-2806
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
grant_number: '101076224'
name: Young galaxies as tracers and agents of cosmic reionization
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Large-scale excess H I absorption around z ≈ 4 galaxies detected in a background
galaxy spectrum in the MUSE eXtremely deep field
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 529
year: '2024'
...
---
_id: '15250'
abstract:
- lang: eng
text: Orphan solute carrier (SLC) represents a group of membrane transporters whose
exact functions and substrate specificities are not known. Elucidating the function
and regulation of orphan SLC transporters is not only crucial for advancing our
knowledge of cellular and molecular biology but can potentially lead to the development
of new therapeutic strategies. Here, we provide evidence for the biological function
of a ubiquitous orphan lysosomal SLC, the Major Facilitator Superfamily Domain-containing
Protein 1 (MFSD1), which has remained phylogenetically unassigned. Targeted metabolomics
revealed that dipeptides containing either lysine or arginine residues accumulate
in lysosomes of cells lacking MFSD1. Whole-cell patch-clamp electrophysiological
recordings of HEK293-cells expressing MFSD1 on the cell surface displayed transport
affinities for positively charged dipeptides in the lower mM range, while dipeptides
that carry a negative net charge were not transported. This was also true for
single amino acids and tripeptides, which MFSD1 failed to transport. Our results
identify MFSD1 as a highly selective lysosomal lysine/arginine/histidine-containing
dipeptide exporter, which functions as a uniporter.
acknowledged_ssus:
- _id: Bio
acknowledgement: We thank the Metabolomics Facility at Vienna BioCenter Core Facilities,
which is a member of the Vienna BioCenter and funded by the City of Vienna through
the Vienna Business Agency (shared research facility), for the LC–MS/MS analysis;
and the BioImaging Facility at IST Austria for technical support and assistance.
The authors want to thank N. Kastner for help with the live cell imaging and A. Korošec for help with flow cytometry. This work was supported
by the Austrian Science Fund (FWF), grant P 36621- B (to M.R.), grant P 36667 (to
W.S.), and core funding from IST Austria (to D.S.).
article_number: e2319686121
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Danila
full_name: Boytsov, Danila
last_name: Boytsov
- first_name: Gregor M.
full_name: Madej, Gregor M.
last_name: Madej
- first_name: Georg
full_name: Horn, Georg
last_name: Horn
- first_name: Nadine
full_name: Blaha, Nadine
last_name: Blaha
- first_name: Thomas
full_name: Köcher, Thomas
last_name: Köcher
- first_name: Harald H.
full_name: Sitte, Harald H.
last_name: Sitte
- first_name: Daria E
full_name: Siekhaus, Daria E
id: 3D224B9E-F248-11E8-B48F-1D18A9856A87
last_name: Siekhaus
orcid: 0000-0001-8323-8353
- first_name: Christine
full_name: Ziegler, Christine
last_name: Ziegler
- first_name: Walter
full_name: Sandtner, Walter
last_name: Sandtner
- first_name: Marko
full_name: Roblek, Marko
id: 3047D808-F248-11E8-B48F-1D18A9856A87
last_name: Roblek
orcid: 0000-0001-9588-1389
citation:
ama: Boytsov D, Madej GM, Horn G, et al. Orphan lysosomal solute carrier MFSD1 facilitates
highly selective dipeptide transport. Proceedings of the National Academy of
Sciences of the United States of America. 2024;121(13). doi:10.1073/pnas.2319686121
apa: Boytsov, D., Madej, G. M., Horn, G., Blaha, N., Köcher, T., Sitte, H. H., …
Roblek, M. (2024). Orphan lysosomal solute carrier MFSD1 facilitates highly selective
dipeptide transport. Proceedings of the National Academy of Sciences of the
United States of America. National Academy of Sciences. https://doi.org/10.1073/pnas.2319686121
chicago: Boytsov, Danila, Gregor M. Madej, Georg Horn, Nadine Blaha, Thomas Köcher,
Harald H. Sitte, Daria E Siekhaus, Christine Ziegler, Walter Sandtner, and Marko
Roblek. “Orphan Lysosomal Solute Carrier MFSD1 Facilitates Highly Selective Dipeptide
Transport.” Proceedings of the National Academy of Sciences of the United States
of America. National Academy of Sciences, 2024. https://doi.org/10.1073/pnas.2319686121.
ieee: D. Boytsov et al., “Orphan lysosomal solute carrier MFSD1 facilitates
highly selective dipeptide transport,” Proceedings of the National Academy
of Sciences of the United States of America, vol. 121, no. 13. National Academy
of Sciences, 2024.
ista: Boytsov D, Madej GM, Horn G, Blaha N, Köcher T, Sitte HH, Siekhaus DE, Ziegler
C, Sandtner W, Roblek M. 2024. Orphan lysosomal solute carrier MFSD1 facilitates
highly selective dipeptide transport. Proceedings of the National Academy of Sciences
of the United States of America. 121(13), e2319686121.
mla: Boytsov, Danila, et al. “Orphan Lysosomal Solute Carrier MFSD1 Facilitates
Highly Selective Dipeptide Transport.” Proceedings of the National Academy
of Sciences of the United States of America, vol. 121, no. 13, e2319686121,
National Academy of Sciences, 2024, doi:10.1073/pnas.2319686121.
short: D. Boytsov, G.M. Madej, G. Horn, N. Blaha, T. Köcher, H.H. Sitte, D.E. Siekhaus,
C. Ziegler, W. Sandtner, M. Roblek, Proceedings of the National Academy of Sciences
of the United States of America 121 (2024).
corr_author: '1'
date_created: 2024-03-31T22:01:12Z
date_published: 2024-03-26T00:00:00Z
date_updated: 2025-09-04T13:19:02Z
day: '26'
ddc:
- '570'
department:
- _id: DaSi
doi: 10.1073/pnas.2319686121
external_id:
isi:
- '001206419000003'
pmid:
- '38507452'
file:
- access_level: open_access
checksum: 06f9e60b1146a685d58bf33999422fa8
content_type: application/pdf
creator: dernst
date_created: 2024-04-02T08:54:28Z
date_updated: 2024-04-02T08:54:28Z
file_id: '15256'
file_name: 2024_PNAS_Boytsov.pdf
file_size: 2483787
relation: main_file
success: 1
file_date_updated: 2024-04-02T08:54:28Z
has_accepted_license: '1'
intvolume: ' 121'
isi: 1
issue: '13'
language:
- iso: eng
month: '03'
oa: 1
oa_version: Published Version
pmid: 1
publication: Proceedings of the National Academy of Sciences of the United States
of America
publication_identifier:
eissn:
- 1091-6490
publication_status: published
publisher: National Academy of Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: Orphan lysosomal solute carrier MFSD1 facilitates highly selective dipeptide
transport
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 121
year: '2024'
...
---
OA_place: repository
OA_type: green
_id: '15251'
abstract:
- lang: eng
text: Brassinosteroids are steroidal phytohormones that regulate plant development
and physiology, including adaptation to environmental stresses. Brassinosteroids
are synthesized in the cell interior but bind receptors at the cell surface, necessitating
a yet to be identified export mechanism. Here, we show that a member of the ATP-binding
cassette (ABC) transporter superfamily, ABCB19, functions as a brassinosteroid
exporter. We present its structure in both the substrate-unbound and the brassinosteroid-bound
states. Bioactive brassinosteroids are potent activators of ABCB19 ATP hydrolysis
activity, and transport assays showed that ABCB19 transports brassinosteroids.
In Arabidopsis thaliana, ABCB19 and its close homolog, ABCB1, positively regulate
brassinosteroid responses. Our results uncover an elusive export mechanism for
bioactive brassinosteroids that is tightly coordinated with brassinosteroid signaling.
acknowledgement: "We thank the Cryo-EM Center of the University of Science and Technology
of China for the EM facility support, Y. Yin (Iowa State University, Ames, IA, USA)
for providing the anti-BES1 antibody, Y. Gao and all other staff members for their
technical support on cryo-EM data collection, S. Vanneste (VIB, Ghent University,
Ghent, Belgium) for useful discussions, and M. De Cock for help in preparing the
manuscript.\r\nThis work was supported by the National Natural Science Foundation
of China (grants 31870732 and 32322041 to L.S., grant 31900885 to X.L., and grant
32321001 to L.S.); the Strategic Priority Research Program of the Chinese Academy
of Sciences (grant XDB37020103 to L.S.); the Natural Science Foundation of Anhui
Province (grant 2008085MC90 to X.L. and grant 2008085J15 to L.S.); Fundamental Research
Funds for the Central Universities (grant WK9100000031 to L.S.); USTC Research Funds
of the Double First-Class Initiative (grant YD9100002004 to L.S. and grant YD9100002020
to X.L.); Research Foundation-Flanders (grant G002121N to E.R. and postdoctoral
fellowships 12R7822N and 12R7819N to N.V.); and Chinese Scholarship Council predoctoral
fellowships (Y.W. and H.Z.). L.S. is supported by an Outstanding Young Scholar Award
from the Qiu Shi Science and Technologies Foundation and a Young Scholar Award from
the Cyrus Tang Foundation."
article_processing_charge: No
article_type: original
author:
- first_name: Wei
full_name: Ying, Wei
last_name: Ying
- first_name: Yaowei
full_name: Wang, Yaowei
last_name: Wang
- first_name: Hong
full_name: Wei, Hong
last_name: Wei
- first_name: Yongming
full_name: Luo, Yongming
last_name: Luo
- first_name: Qian
full_name: Ma, Qian
last_name: Ma
- first_name: Heyuan
full_name: Zhu, Heyuan
last_name: Zhu
- first_name: Hilde
full_name: Janssens, Hilde
last_name: Janssens
- first_name: Nemanja
full_name: Vukašinović, Nemanja
last_name: Vukašinović
- first_name: Miroslav
full_name: Kvasnica, Miroslav
last_name: Kvasnica
- first_name: Johan M.
full_name: Winne, Johan M.
last_name: Winne
- first_name: Yongxiang
full_name: Gao, Yongxiang
last_name: Gao
- first_name: Shutang
full_name: Tan, Shutang
id: 2DE75584-F248-11E8-B48F-1D18A9856A87
last_name: Tan
orcid: 0000-0002-0471-8285
- first_name: Jiří
full_name: Friml, Jiří
id: 4159519E-F248-11E8-B48F-1D18A9856A87
last_name: Friml
orcid: 0000-0002-8302-7596
- first_name: Xin
full_name: Liu, Xin
last_name: Liu
- first_name: Eugenia
full_name: Russinova, Eugenia
last_name: Russinova
- first_name: Linfeng
full_name: Sun, Linfeng
last_name: Sun
citation:
ama: Ying W, Wang Y, Wei H, et al. Structure and function of the Arabidopsis ABC
transporter ABCB19 in brassinosteroid export. Science. 2024;383(6689):eadj4591.
doi:10.1126/science.adj4591
apa: Ying, W., Wang, Y., Wei, H., Luo, Y., Ma, Q., Zhu, H., … Sun, L. (2024). Structure
and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid export.
Science. American Association for the Advancement of Science. https://doi.org/10.1126/science.adj4591
chicago: Ying, Wei, Yaowei Wang, Hong Wei, Yongming Luo, Qian Ma, Heyuan Zhu, Hilde
Janssens, et al. “Structure and Function of the Arabidopsis ABC Transporter ABCB19
in Brassinosteroid Export.” Science. American Association for the Advancement
of Science, 2024. https://doi.org/10.1126/science.adj4591.
ieee: W. Ying et al., “Structure and function of the Arabidopsis ABC transporter
ABCB19 in brassinosteroid export,” Science, vol. 383, no. 6689. American
Association for the Advancement of Science, p. eadj4591, 2024.
ista: Ying W, Wang Y, Wei H, Luo Y, Ma Q, Zhu H, Janssens H, Vukašinović N, Kvasnica
M, Winne JM, Gao Y, Tan S, Friml J, Liu X, Russinova E, Sun L. 2024. Structure
and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid export.
Science. 383(6689), eadj4591.
mla: Ying, Wei, et al. “Structure and Function of the Arabidopsis ABC Transporter
ABCB19 in Brassinosteroid Export.” Science, vol. 383, no. 6689, American
Association for the Advancement of Science, 2024, p. eadj4591, doi:10.1126/science.adj4591.
short: W. Ying, Y. Wang, H. Wei, Y. Luo, Q. Ma, H. Zhu, H. Janssens, N. Vukašinović,
M. Kvasnica, J.M. Winne, Y. Gao, S. Tan, J. Friml, X. Liu, E. Russinova, L. Sun,
Science 383 (2024) eadj4591.
date_created: 2024-03-31T22:01:12Z
date_published: 2024-03-22T00:00:00Z
date_updated: 2025-09-04T13:19:48Z
day: '22'
department:
- _id: JiFr
doi: 10.1126/science.adj4591
external_id:
isi:
- '001252955200028'
pmid:
- '38513023'
intvolume: ' 383'
isi: 1
issue: '6689'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: http://hdl.handle.net/1854/LU-01HTMBK3P3PPNB73YFCMFXP3ZZ
month: '03'
oa: 1
oa_version: Submitted Version
page: eadj4591
pmid: 1
publication: Science
publication_identifier:
eissn:
- 1095-9203
publication_status: published
publisher: American Association for the Advancement of Science
quality_controlled: '1'
scopus_import: '1'
status: public
title: Structure and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid
export
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 383
year: '2024'
...
---
_id: '15252'
abstract:
- lang: eng
text: A measurable map between measure spaces is shown to have bounded compression
if and only if its image via the measure-algebra functor is Lipschitz-continuous
w.r.t. the measure-algebra distances. This provides a natural interpretation of
maps of bounded compression/deformation by means of the measure-algebra functor
and corrobo-rates the assertion that maps of bounded deformation are a natural
class of morphisms for the category of complete and separable metric measure spaces.
acknowledgement: "The author gratefully acknowledges funding of his current position
by the Austrian Science\r\nFund (FWF), grant ESPRIT208. He is grateful to Enrico
Pasqualetto for pointing out some\r\nreferences on maps of bounded compression."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Lorenzo
full_name: Dello Schiavo, Lorenzo
id: ECEBF480-9E4F-11EA-B557-B0823DDC885E
last_name: Dello Schiavo
orcid: 0000-0002-9881-6870
citation:
ama: Dello Schiavo L. A characterization of maps of bounded compression. Mathematical
Communications. 2024;29(1):137-142.
apa: Dello Schiavo, L. (2024). A characterization of maps of bounded compression.
Mathematical Communications. Udruga Matematicara Osijek.
chicago: Dello Schiavo, Lorenzo. “A Characterization of Maps of Bounded Compression.”
Mathematical Communications. Udruga Matematicara Osijek, 2024.
ieee: L. Dello Schiavo, “A characterization of maps of bounded compression,” Mathematical
Communications, vol. 29, no. 1. Udruga Matematicara Osijek, pp. 137–142, 2024.
ista: Dello Schiavo L. 2024. A characterization of maps of bounded compression.
Mathematical Communications. 29(1), 137–142.
mla: Dello Schiavo, Lorenzo. “A Characterization of Maps of Bounded Compression.”
Mathematical Communications, vol. 29, no. 1, Udruga Matematicara Osijek,
2024, pp. 137–42.
short: L. Dello Schiavo, Mathematical Communications 29 (2024) 137–142.
corr_author: '1'
date_created: 2024-03-31T22:01:12Z
date_published: 2024-01-01T00:00:00Z
date_updated: 2025-04-14T12:59:08Z
day: '01'
department:
- _id: JaMa
external_id:
arxiv:
- '2304.11348'
intvolume: ' 29'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.2304.11348
month: '01'
oa: 1
oa_version: Preprint
page: 137-142
project:
- _id: 34dbf174-11ca-11ed-8bc3-afe9d43d4b9c
grant_number: E208
name: Configuration Spaces over Non-Smooth Spaces
publication: Mathematical Communications
publication_identifier:
eissn:
- 1848-8013
issn:
- 1331-0623
publication_status: published
publisher: Udruga Matematicara Osijek
quality_controlled: '1'
scopus_import: '1'
status: public
title: A characterization of maps of bounded compression
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 29
year: '2024'
...