---
_id: '15149'
abstract:
- lang: eng
  text: The genomic binding sites of the transcription factor (TF) and tumor suppressor
    p53 are unusually diverse with regard to their chromatin features, including histone
    modifications, raising the possibility that the local chromatin environment can
    contextualize p53 regulation. Here, we show that epigenetic characteristics of
    closed chromatin, such as DNA methylation, do not influence the binding of p53
    across the genome. Instead, the ability of p53 to open chromatin and activate
    its target genes is locally restricted by its cofactor Trim24. Trim24 binds to
    both p53 and unmethylated histone 3 lysine 4 (H3K4), thereby preferentially localizing
    to those p53 sites that reside in closed chromatin, whereas it is deterred from
    accessible chromatin by H3K4 methylation. The presence of Trim24 increases cell
    viability upon stress and enables p53 to affect gene expression as a function
    of the local chromatin state. These findings link H3K4 methylation to p53 function
    and illustrate how specificity in chromatin can be achieved, not by TF-intrinsic
    sensitivity to histone modifications, but by employing chromatin-sensitive cofactors
    that locally modulate TF function.
article_processing_charge: No
article_type: original
author:
- first_name: Luke
  full_name: Isbel, Luke
  last_name: Isbel
- first_name: Murat
  full_name: Iskar, Murat
  last_name: Iskar
- first_name: Sevi
  full_name: Durdu, Sevi
  last_name: Durdu
- first_name: Joscha
  full_name: Weiss, Joscha
  last_name: Weiss
- first_name: Ralph S.
  full_name: Grand, Ralph S.
  last_name: Grand
- first_name: Eric
  full_name: Hietter-Pfeiffer, Eric
  last_name: Hietter-Pfeiffer
- first_name: Zuzanna
  full_name: Kozicka, Zuzanna
  last_name: Kozicka
- first_name: Alicia
  full_name: Michael, Alicia
  id: 6437c950-2a03-11ee-914d-d6476dd7b75c
  last_name: Michael
  orcid: 0000-0002-6080-839X
- first_name: Lukas
  full_name: Burger, Lukas
  last_name: Burger
- first_name: Nicolas H.
  full_name: Thomä, Nicolas H.
  last_name: Thomä
- first_name: Dirk
  full_name: Schübeler, Dirk
  last_name: Schübeler
citation:
  ama: Isbel L, Iskar M, Durdu S, et al. Readout of histone methylation by Trim24
    locally restricts chromatin opening by p53. <i>Nature Structural &#38; Molecular
    Biology</i>. 2023;30(7):948-957. doi:<a href="https://doi.org/10.1038/s41594-023-01021-8">10.1038/s41594-023-01021-8</a>
  apa: Isbel, L., Iskar, M., Durdu, S., Weiss, J., Grand, R. S., Hietter-Pfeiffer,
    E., … Schübeler, D. (2023). Readout of histone methylation by Trim24 locally restricts
    chromatin opening by p53. <i>Nature Structural &#38; Molecular Biology</i>. Springer
    Nature. <a href="https://doi.org/10.1038/s41594-023-01021-8">https://doi.org/10.1038/s41594-023-01021-8</a>
  chicago: Isbel, Luke, Murat Iskar, Sevi Durdu, Joscha Weiss, Ralph S. Grand, Eric
    Hietter-Pfeiffer, Zuzanna Kozicka, et al. “Readout of Histone Methylation by Trim24
    Locally Restricts Chromatin Opening by P53.” <i>Nature Structural &#38; Molecular
    Biology</i>. Springer Nature, 2023. <a href="https://doi.org/10.1038/s41594-023-01021-8">https://doi.org/10.1038/s41594-023-01021-8</a>.
  ieee: L. Isbel <i>et al.</i>, “Readout of histone methylation by Trim24 locally
    restricts chromatin opening by p53,” <i>Nature Structural &#38; Molecular Biology</i>,
    vol. 30, no. 7. Springer Nature, pp. 948–957, 2023.
  ista: Isbel L, Iskar M, Durdu S, Weiss J, Grand RS, Hietter-Pfeiffer E, Kozicka
    Z, Michael AK, Burger L, Thomä NH, Schübeler D. 2023. Readout of histone methylation
    by Trim24 locally restricts chromatin opening by p53. Nature Structural &#38;
    Molecular Biology. 30(7), 948–957.
  mla: Isbel, Luke, et al. “Readout of Histone Methylation by Trim24 Locally Restricts
    Chromatin Opening by P53.” <i>Nature Structural &#38; Molecular Biology</i>, vol.
    30, no. 7, Springer Nature, 2023, pp. 948–57, doi:<a href="https://doi.org/10.1038/s41594-023-01021-8">10.1038/s41594-023-01021-8</a>.
  short: L. Isbel, M. Iskar, S. Durdu, J. Weiss, R.S. Grand, E. Hietter-Pfeiffer,
    Z. Kozicka, A.K. Michael, L. Burger, N.H. Thomä, D. Schübeler, Nature Structural
    &#38; Molecular Biology 30 (2023) 948–957.
date_created: 2024-03-21T07:53:24Z
date_published: 2023-06-29T00:00:00Z
date_updated: 2024-03-25T12:37:20Z
day: '29'
doi: 10.1038/s41594-023-01021-8
extern: '1'
external_id:
  pmid:
  - '37386214'
intvolume: '        30'
issue: '7'
keyword:
- Molecular Biology
- Structural Biology
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1038/s41594-023-01021-8
month: '06'
oa: 1
oa_version: Published Version
page: 948-957
pmid: 1
publication: Nature Structural & Molecular Biology
publication_identifier:
  eissn:
  - 1545-9985
  issn:
  - 1545-9993
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Readout of histone methylation by Trim24 locally restricts chromatin opening
  by p53
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 30
year: '2023'
...
---
_id: '15173'
abstract:
- lang: eng
  text: 'We show that the number of linear spaces on a set of n points and the number
    of rank-3 matroids on a ground set of size n are both of the form (cn+o(n))n2/6,
    where c=e3√/2−3(1+3–√)/2. This is the final piece of the puzzle for enumerating
    fixed-rank matroids at this level of accuracy: the numbers of rank-1 and rank-2
    matroids on a ground set of size n have exact representations in terms of well-known
    combinatorial functions, and it was recently proved by van der Hofstad, Pendavingh,
    and van der Pol that for constant r≥4 there are (e1−rn+o(n))nr−1/r! rank-r matroids
    on a ground set of size n. In our proof, we introduce a new approach for bounding
    the number of clique decompositions of a complete graph, using quasirandomness
    instead of the so-called entropy method that is common in this area.'
acknowledgement: "Sah and Sawhney were supported by NSF Graduate Research Fellowship
  Program DGE-1745302. Sah was supported by the PD Soros Fellowship.\r\nWe thank Michael
  Simkin for helpful comments on the manuscript. We thank Zach Hunter for\r\nseveral
  corrections."
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Matthew Alan
  full_name: Kwan, Matthew Alan
  id: 5fca0887-a1db-11eb-95d1-ca9d5e0453b3
  last_name: Kwan
  orcid: 0000-0002-4003-7567
- first_name: Ashwin
  full_name: Sah, Ashwin
  last_name: Sah
- first_name: Mehtaab
  full_name: Sawhney, Mehtaab
  last_name: Sawhney
citation:
  ama: Kwan MA, Sah A, Sawhney M. Enumerating matroids and linear spaces. <i>Comptes
    Rendus Mathematique</i>. 2023;361(G2):565-575. doi:<a href="https://doi.org/10.5802/crmath.423">10.5802/crmath.423</a>
  apa: Kwan, M. A., Sah, A., &#38; Sawhney, M. (2023). Enumerating matroids and linear
    spaces. <i>Comptes Rendus Mathematique</i>. Academie des Sciences. <a href="https://doi.org/10.5802/crmath.423">https://doi.org/10.5802/crmath.423</a>
  chicago: Kwan, Matthew Alan, Ashwin Sah, and Mehtaab Sawhney. “Enumerating Matroids
    and Linear Spaces.” <i>Comptes Rendus Mathematique</i>. Academie des Sciences,
    2023. <a href="https://doi.org/10.5802/crmath.423">https://doi.org/10.5802/crmath.423</a>.
  ieee: M. A. Kwan, A. Sah, and M. Sawhney, “Enumerating matroids and linear spaces,”
    <i>Comptes Rendus Mathematique</i>, vol. 361, no. G2. Academie des Sciences, pp.
    565–575, 2023.
  ista: Kwan MA, Sah A, Sawhney M. 2023. Enumerating matroids and linear spaces. Comptes
    Rendus Mathematique. 361(G2), 565–575.
  mla: Kwan, Matthew Alan, et al. “Enumerating Matroids and Linear Spaces.” <i>Comptes
    Rendus Mathematique</i>, vol. 361, no. G2, Academie des Sciences, 2023, pp. 565–75,
    doi:<a href="https://doi.org/10.5802/crmath.423">10.5802/crmath.423</a>.
  short: M.A. Kwan, A. Sah, M. Sawhney, Comptes Rendus Mathematique 361 (2023) 565–575.
date_created: 2024-03-24T23:01:00Z
date_published: 2023-02-01T00:00:00Z
date_updated: 2025-09-09T14:26:32Z
day: '01'
ddc:
- '510'
department:
- _id: MaKw
doi: 10.5802/crmath.423
external_id:
  arxiv:
  - '2112.03788'
  isi:
  - '001167671400009'
file:
- access_level: open_access
  checksum: d1d0e0a854a79ae95fb66d75d9117a68
  content_type: application/pdf
  creator: dernst
  date_created: 2024-03-25T07:21:52Z
  date_updated: 2024-03-25T07:21:52Z
  file_id: '15174'
  file_name: 2023_ComptesRendusMath_Kwan.pdf
  file_size: 598097
  relation: main_file
  success: 1
file_date_updated: 2024-03-25T07:21:52Z
has_accepted_license: '1'
intvolume: '       361'
isi: 1
issue: G2
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
page: 565-575
publication: Comptes Rendus Mathematique
publication_identifier:
  eissn:
  - 1778-3569
  issn:
  - 1631-073X
publication_status: published
publisher: Academie des Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: Enumerating matroids and linear spaces
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: 361
year: '2023'
...
---
_id: '15190'
abstract:
- lang: eng
  text: We report on IXPE, NICER, and XMM–Newton observations of the magnetar 1E 2259+586.
    We find that the source is significantly polarized at about or above 20  per cent
    for all phases except for the secondary peak where it is more weakly polarized.
    The polarization degree is strongest during the primary minimum which is also
    the phase where an absorption feature has been identified previously. The polarization
    angle of the photons are consistent with a rotating vector model with a mode switch
    between the primary minimum and the rest of the rotation of the neutron star.
    We propose a scenario in which the emission at the source is weakly polarized
    (as in a condensed surface) and, as the radiation passes through a plasma arch,
    resonant cyclotron scattering off of protons produces the observed polarized radiation.
    This confirms the magnetar nature of the source with a surface field greater than
    about 1015 G.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
- first_name: Roberto
  full_name: Taverna, Roberto
  last_name: Taverna
- first_name: Roberto
  full_name: Turolla, Roberto
  last_name: Turolla
- first_name: Gian Luca
  full_name: Israel, Gian Luca
  last_name: Israel
- first_name: Mason
  full_name: Ng, Mason
  last_name: Ng
- first_name: Demet
  full_name: Kırmızıbayrak, Demet
  last_name: Kırmızıbayrak
- first_name: Denis
  full_name: González-Caniulef, Denis
  last_name: González-Caniulef
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Silvia
  full_name: Zane, Silvia
  last_name: Zane
- first_name: Steven R
  full_name: Ehlert, Steven R
  last_name: Ehlert
- first_name: Michela
  full_name: Negro, Michela
  last_name: Negro
- first_name: Iván
  full_name: Agudo, Iván
  last_name: Agudo
- first_name: Lucio Angelo
  full_name: Antonelli, Lucio Angelo
  last_name: Antonelli
- first_name: Matteo
  full_name: Bachetti, Matteo
  last_name: Bachetti
- first_name: Luca
  full_name: Baldini, Luca
  last_name: Baldini
- first_name: Wayne H
  full_name: Baumgartner, Wayne H
  last_name: Baumgartner
- first_name: Ronaldo
  full_name: Bellazzini, Ronaldo
  last_name: Bellazzini
- first_name: Stefano
  full_name: Bianchi, Stefano
  last_name: Bianchi
- first_name: Stephen D
  full_name: Bongiorno, Stephen D
  last_name: Bongiorno
- first_name: Raffaella
  full_name: Bonino, Raffaella
  last_name: Bonino
- first_name: Alessandro
  full_name: Brez, Alessandro
  last_name: Brez
- first_name: Niccolò
  full_name: Bucciantini, Niccolò
  last_name: Bucciantini
- first_name: Fiamma
  full_name: Capitanio, Fiamma
  last_name: Capitanio
- first_name: Simone
  full_name: Castellano, Simone
  last_name: Castellano
- first_name: Elisabetta
  full_name: Cavazzuti, Elisabetta
  last_name: Cavazzuti
- first_name: Chien-Ting
  full_name: Chen, Chien-Ting
  last_name: Chen
- first_name: Stefano
  full_name: Ciprini, Stefano
  last_name: Ciprini
- first_name: Enrico
  full_name: Costa, Enrico
  last_name: Costa
- first_name: Alessandra
  full_name: De Rosa, Alessandra
  last_name: De Rosa
- first_name: Ettore
  full_name: Del Monte, Ettore
  last_name: Del Monte
- first_name: Laura
  full_name: Di Gesu, Laura
  last_name: Di Gesu
- first_name: Niccolò
  full_name: Di Lalla, Niccolò
  last_name: Di Lalla
- first_name: Alessandro
  full_name: Di Marco, Alessandro
  last_name: Di Marco
- first_name: Immacolata
  full_name: Donnarumma, Immacolata
  last_name: Donnarumma
- first_name: Victor
  full_name: Doroshenko, Victor
  last_name: Doroshenko
- first_name: Michal
  full_name: Dovčiak, Michal
  last_name: Dovčiak
- first_name: Teruaki
  full_name: Enoto, Teruaki
  last_name: Enoto
- first_name: Yuri
  full_name: Evangelista, Yuri
  last_name: Evangelista
- first_name: Sergio
  full_name: Fabiani, Sergio
  last_name: Fabiani
- first_name: Riccardo
  full_name: Ferrazzoli, Riccardo
  last_name: Ferrazzoli
- first_name: Javier A
  full_name: Garcia, Javier A
  last_name: Garcia
- first_name: Shuichi
  full_name: Gunji, Shuichi
  last_name: Gunji
- first_name: Kiyoshi
  full_name: Hayashida, Kiyoshi
  last_name: Hayashida
- first_name: Wataru
  full_name: Iwakiri, Wataru
  last_name: Iwakiri
- first_name: Svetlana G
  full_name: Jorstad, Svetlana G
  last_name: Jorstad
- first_name: Philip
  full_name: Kaaret, Philip
  last_name: Kaaret
- first_name: Vladimir
  full_name: Karas, Vladimir
  last_name: Karas
- first_name: Fabian
  full_name: Kislat, Fabian
  last_name: Kislat
- first_name: Takao
  full_name: Kitaguchi, Takao
  last_name: Kitaguchi
- first_name: Jeffery J
  full_name: Kolodziejczak, Jeffery J
  last_name: Kolodziejczak
- first_name: Henric
  full_name: Krawczynski, Henric
  last_name: Krawczynski
- first_name: Fabio La
  full_name: Monaca, Fabio La
  last_name: Monaca
- first_name: Luca
  full_name: Latronico, Luca
  last_name: Latronico
- first_name: Ioannis
  full_name: Liodakis, Ioannis
  last_name: Liodakis
- first_name: Simone
  full_name: Maldera, Simone
  last_name: Maldera
- first_name: Alberto
  full_name: Manfreda, Alberto
  last_name: Manfreda
- first_name: Frédéric
  full_name: Marin, Frédéric
  last_name: Marin
- first_name: Andrea
  full_name: Marinucci, Andrea
  last_name: Marinucci
- first_name: Alan P
  full_name: Marscher, Alan P
  last_name: Marscher
- first_name: Herman L
  full_name: Marshall, Herman L
  last_name: Marshall
- first_name: Francesco
  full_name: Massaro, Francesco
  last_name: Massaro
- first_name: Giorgio
  full_name: Matt, Giorgio
  last_name: Matt
- first_name: Ikuyuki
  full_name: Mitsuishi, Ikuyuki
  last_name: Mitsuishi
- first_name: Tsunefumi
  full_name: Mizuno, Tsunefumi
  last_name: Mizuno
- first_name: Fabio
  full_name: Muleri, Fabio
  last_name: Muleri
- first_name: C-Y
  full_name: Ng, C-Y
  last_name: Ng
- first_name: Stephen L
  full_name: O’Dell, Stephen L
  last_name: O’Dell
- first_name: Nicola
  full_name: Omodei, Nicola
  last_name: Omodei
- first_name: Chiara
  full_name: Oppedisano, Chiara
  last_name: Oppedisano
- first_name: Alessandro
  full_name: Papitto, Alessandro
  last_name: Papitto
- first_name: George G
  full_name: Pavlov, George G
  last_name: Pavlov
- first_name: Abel Lawrence
  full_name: Peirson, Abel Lawrence
  last_name: Peirson
- first_name: Matteo
  full_name: Perri, Matteo
  last_name: Perri
- first_name: Melissa
  full_name: Pesce-Rollins, Melissa
  last_name: Pesce-Rollins
- first_name: Pierre-Olivier
  full_name: Petrucci, Pierre-Olivier
  last_name: Petrucci
- first_name: Maura
  full_name: Pilia, Maura
  last_name: Pilia
- first_name: Andrea
  full_name: Possenti, Andrea
  last_name: Possenti
- first_name: Juri
  full_name: Poutanen, Juri
  last_name: Poutanen
- first_name: Simonetta
  full_name: Puccetti, Simonetta
  last_name: Puccetti
- first_name: Brian D
  full_name: Ramsey, Brian D
  last_name: Ramsey
- first_name: John
  full_name: Rankin, John
  last_name: Rankin
- first_name: Ajay
  full_name: Ratheesh, Ajay
  last_name: Ratheesh
- first_name: Oliver J
  full_name: Roberts, Oliver J
  last_name: Roberts
- first_name: Roger W
  full_name: Romani, Roger W
  last_name: Romani
- first_name: Carmelo
  full_name: Sgrò, Carmelo
  last_name: Sgrò
- first_name: Patrick
  full_name: Slane, Patrick
  last_name: Slane
- first_name: Paolo
  full_name: Soffitta, Paolo
  last_name: Soffitta
- first_name: Gloria
  full_name: Spandre, Gloria
  last_name: Spandre
- first_name: Douglas A
  full_name: Swartz, Douglas A
  last_name: Swartz
- first_name: Toru
  full_name: Tamagawa, Toru
  last_name: Tamagawa
- first_name: Fabrizio
  full_name: Tavecchio, Fabrizio
  last_name: Tavecchio
- first_name: Yuzuru
  full_name: Tawara, Yuzuru
  last_name: Tawara
- first_name: Allyn F
  full_name: Tennant, Allyn F
  last_name: Tennant
- first_name: Nicholas E
  full_name: Thomas, Nicholas E
  last_name: Thomas
- first_name: Francesco
  full_name: Tombesi, Francesco
  last_name: Tombesi
- first_name: Alessio
  full_name: Trois, Alessio
  last_name: Trois
- first_name: Sergey S
  full_name: Tsygankov, Sergey S
  last_name: Tsygankov
- first_name: Jacco
  full_name: Vink, Jacco
  last_name: Vink
- first_name: Martin C
  full_name: Weisskopf, Martin C
  last_name: Weisskopf
- first_name: Kinwah
  full_name: Wu, Kinwah
  last_name: Wu
- first_name: Fei
  full_name: Xie, Fei
  last_name: Xie
citation:
  ama: Heyl J, Taverna R, Turolla R, et al. The detection of polarized X-ray emission
    from the magnetar 1E 2259+586. <i>Monthly Notices of the Royal Astronomical Society</i>.
    2023;527(4):12219-12231. doi:<a href="https://doi.org/10.1093/mnras/stad3680">10.1093/mnras/stad3680</a>
  apa: Heyl, J., Taverna, R., Turolla, R., Israel, G. L., Ng, M., Kırmızıbayrak, D.,
    … Xie, F. (2023). The detection of polarized X-ray emission from the magnetar
    1E 2259+586. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford
    University Press. <a href="https://doi.org/10.1093/mnras/stad3680">https://doi.org/10.1093/mnras/stad3680</a>
  chicago: Heyl, Jeremy, Roberto Taverna, Roberto Turolla, Gian Luca Israel, Mason
    Ng, Demet Kırmızıbayrak, Denis González-Caniulef, et al. “The Detection of Polarized
    X-Ray Emission from the Magnetar 1E 2259+586.” <i>Monthly Notices of the Royal
    Astronomical Society</i>. Oxford University Press, 2023. <a href="https://doi.org/10.1093/mnras/stad3680">https://doi.org/10.1093/mnras/stad3680</a>.
  ieee: J. Heyl <i>et al.</i>, “The detection of polarized X-ray emission from the
    magnetar 1E 2259+586,” <i>Monthly Notices of the Royal Astronomical Society</i>,
    vol. 527, no. 4. Oxford University Press, pp. 12219–12231, 2023.
  ista: Heyl J et al. 2023. The detection of polarized X-ray emission from the magnetar
    1E 2259+586. Monthly Notices of the Royal Astronomical Society. 527(4), 12219–12231.
  mla: Heyl, Jeremy, et al. “The Detection of Polarized X-Ray Emission from the Magnetar
    1E 2259+586.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 527,
    no. 4, Oxford University Press, 2023, pp. 12219–31, doi:<a href="https://doi.org/10.1093/mnras/stad3680">10.1093/mnras/stad3680</a>.
  short: J. Heyl, R. Taverna, R. Turolla, G.L. Israel, M. Ng, D. Kırmızıbayrak, D.
    González-Caniulef, I. Caiazzo, S. Zane, S.R. Ehlert, M. Negro, I. Agudo, L.A.
    Antonelli, M. Bachetti, L. Baldini, W.H. Baumgartner, R. Bellazzini, S. Bianchi,
    S.D. Bongiorno, R. Bonino, A. Brez, N. Bucciantini, F. Capitanio, S. Castellano,
    E. Cavazzuti, C.-T. Chen, S. Ciprini, E. Costa, A. De Rosa, E. Del Monte, L. Di
    Gesu, N. Di Lalla, A. Di Marco, I. Donnarumma, V. Doroshenko, M. Dovčiak, T. Enoto,
    Y. Evangelista, S. Fabiani, R. Ferrazzoli, J.A. Garcia, S. Gunji, K. Hayashida,
    W. Iwakiri, S.G. Jorstad, P. Kaaret, V. Karas, F. Kislat, T. Kitaguchi, J.J. Kolodziejczak,
    H. Krawczynski, F.L. Monaca, L. Latronico, I. Liodakis, S. Maldera, A. Manfreda,
    F. Marin, A. Marinucci, A.P. Marscher, H.L. Marshall, F. Massaro, G. Matt, I.
    Mitsuishi, T. Mizuno, F. Muleri, C.-Y. Ng, S.L. O’Dell, N. Omodei, C. Oppedisano,
    A. Papitto, G.G. Pavlov, A.L. Peirson, M. Perri, M. Pesce-Rollins, P.-O. Petrucci,
    M. Pilia, A. Possenti, J. Poutanen, S. Puccetti, B.D. Ramsey, J. Rankin, A. Ratheesh,
    O.J. Roberts, R.W. Romani, C. Sgrò, P. Slane, P. Soffitta, G. Spandre, D.A. Swartz,
    T. Tamagawa, F. Tavecchio, Y. Tawara, A.F. Tennant, N.E. Thomas, F. Tombesi, A.
    Trois, S.S. Tsygankov, J. Vink, M.C. Weisskopf, K. Wu, F. Xie, Monthly Notices
    of the Royal Astronomical Society 527 (2023) 12219–12231.
date_created: 2024-03-26T09:44:24Z
date_published: 2023-12-01T00:00:00Z
date_updated: 2024-04-02T06:51:04Z
day: '01'
doi: 10.1093/mnras/stad3680
extern: '1'
external_id:
  arxiv:
  - '2311.03637'
intvolume: '       527'
issue: '4'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1093/mnras/stad3680
month: '12'
oa: 1
oa_version: Published Version
page: 12219-12231
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: The detection of polarized X-ray emission from the magnetar 1E 2259+586
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: 527
year: '2023'
...
---
_id: '15192'
abstract:
- lang: eng
  text: We searched the Gaia DR3 database for ultramassive white dwarfs with kinematics
    consistent with having escaped the nearby Hyades open cluster, identifying three
    such candidates. Two of these candidates have masses estimated from Gaia photometry
    of approximately 1.1 solar masses; their status as products of single-stellar
    evolution that have escaped the cluster was deemed too questionable for immediate
    follow-up analysis. The remaining candidate has an expected mass >1.3 solar masses,
    significantly reducing the probability of it being an interloper. Analysis of
    follow-up Gemini GMOS spectroscopy for this source reveals a nonmagnetized hydrogen
    atmosphere white dwarf with a mass and age consistent with having formed from
    a single star. Assuming a single-stellar-evolution formation channel, we estimate
    a 97.8% chance that the candidate is a true escapee from the Hyades. With a determined
    mass of 1.317 solar masses, this is potentially the most massive known single-evolution
    white dwarf and is by far the most massive with a strong association with an open
    cluster.
article_number: L41
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: David R.
  full_name: Miller, David R.
  last_name: Miller
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
- first_name: Harvey B.
  full_name: Richer, Harvey B.
  last_name: Richer
- first_name: Kareem
  full_name: El-Badry, Kareem
  last_name: El-Badry
- first_name: Antonio C.
  full_name: Rodriguez, Antonio C.
  last_name: Rodriguez
- first_name: Zachary P.
  full_name: Vanderbosch, Zachary P.
  last_name: Vanderbosch
- first_name: Jan
  full_name: van Roestel, Jan
  last_name: van Roestel
citation:
  ama: Miller DR, Caiazzo I, Heyl J, et al. An extremely massive white dwarf escaped
    from the Hyades star cluster. <i>The Astrophysical Journal Letters</i>. 2023;956(2).
    doi:<a href="https://doi.org/10.3847/2041-8213/acffc4">10.3847/2041-8213/acffc4</a>
  apa: Miller, D. R., Caiazzo, I., Heyl, J., Richer, H. B., El-Badry, K., Rodriguez,
    A. C., … van Roestel, J. (2023). An extremely massive white dwarf escaped from
    the Hyades star cluster. <i>The Astrophysical Journal Letters</i>. American Astronomical
    Society. <a href="https://doi.org/10.3847/2041-8213/acffc4">https://doi.org/10.3847/2041-8213/acffc4</a>
  chicago: Miller, David R., Ilaria Caiazzo, Jeremy Heyl, Harvey B. Richer, Kareem
    El-Badry, Antonio C. Rodriguez, Zachary P. Vanderbosch, and Jan van Roestel. “An
    Extremely Massive White Dwarf Escaped from the Hyades Star Cluster.” <i>The Astrophysical
    Journal Letters</i>. American Astronomical Society, 2023. <a href="https://doi.org/10.3847/2041-8213/acffc4">https://doi.org/10.3847/2041-8213/acffc4</a>.
  ieee: D. R. Miller <i>et al.</i>, “An extremely massive white dwarf escaped from
    the Hyades star cluster,” <i>The Astrophysical Journal Letters</i>, vol. 956,
    no. 2. American Astronomical Society, 2023.
  ista: Miller DR, Caiazzo I, Heyl J, Richer HB, El-Badry K, Rodriguez AC, Vanderbosch
    ZP, van Roestel J. 2023. An extremely massive white dwarf escaped from the Hyades
    star cluster. The Astrophysical Journal Letters. 956(2), L41.
  mla: Miller, David R., et al. “An Extremely Massive White Dwarf Escaped from the
    Hyades Star Cluster.” <i>The Astrophysical Journal Letters</i>, vol. 956, no.
    2, L41, American Astronomical Society, 2023, doi:<a href="https://doi.org/10.3847/2041-8213/acffc4">10.3847/2041-8213/acffc4</a>.
  short: D.R. Miller, I. Caiazzo, J. Heyl, H.B. Richer, K. El-Badry, A.C. Rodriguez,
    Z.P. Vanderbosch, J. van Roestel, The Astrophysical Journal Letters 956 (2023).
date_created: 2024-03-26T09:45:38Z
date_published: 2023-10-19T00:00:00Z
date_updated: 2024-04-02T06:56:01Z
day: '19'
doi: 10.3847/2041-8213/acffc4
extern: '1'
external_id:
  arxiv:
  - '2310.03204'
intvolume: '       956'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.3847/2041-8213/acffc4
month: '10'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal Letters
publication_identifier:
  eissn:
  - 2041-8213
  issn:
  - 2041-8205
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: An extremely massive white dwarf escaped from the Hyades star cluster
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: 956
year: '2023'
...
---
_id: '15193'
abstract:
- lang: eng
  text: We report on Imaging X-ray polarimetry explorer (IXPE) observations of the
    Be-transient X-ray pulsar LS V +44 17/RX J0440.9+4431 made at two luminosity levels
    during the giant outburst in January–February 2023. Considering the observed spectral
    variability and changes in the pulse profiles, the source was likely caught in
    supercritical and subcritical states with significantly different emission-region
    geometry, associated with the presence of accretion columns and hot spots, respectively.
    We focus here on the pulse-phase-resolved polarimetric analysis and find that
    the observed dependencies of the polarization degree and polarization angle (PA)
    on the pulse phase are indeed drastically different for the two observations.
    The observed differences, if interpreted within the framework of the rotating
    vector model (RVM), imply dramatic variations in the spin axis inclination, the
    position angle, and the magnetic colatitude by tens of degrees within the space
    of just a few days. We suggest that the apparent changes in the observed PA phase
    dependence are predominantly related to the presence of an unpulsed polarized
    component in addition to the polarized radiation associated with the pulsar itself.
    We then show that the observed PA phase dependence in both observations can be
    explained with a single set of RVM parameters defining the pulsar’s geometry.
    We also suggest that the additional polarized component is likely produced by
    scattering of the pulsar radiation in the equatorial disk wind.
article_number: A57
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Victor
  full_name: Doroshenko, Victor
  last_name: Doroshenko
- first_name: Juri
  full_name: Poutanen, Juri
  last_name: Poutanen
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
- first_name: Sergey S.
  full_name: Tsygankov, Sergey S.
  last_name: Tsygankov
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Roberto
  full_name: Turolla, Roberto
  last_name: Turolla
- first_name: Alexandra
  full_name: Veledina, Alexandra
  last_name: Veledina
- first_name: Martin C.
  full_name: Weisskopf, Martin C.
  last_name: Weisskopf
- first_name: Sofia V.
  full_name: Forsblom, Sofia V.
  last_name: Forsblom
- first_name: Denis
  full_name: González-Caniulef, Denis
  last_name: González-Caniulef
- first_name: Vladislav
  full_name: Loktev, Vladislav
  last_name: Loktev
- first_name: Christian
  full_name: Malacaria, Christian
  last_name: Malacaria
- first_name: Alexander A.
  full_name: Mushtukov, Alexander A.
  last_name: Mushtukov
- first_name: Valery F.
  full_name: Suleimanov, Valery F.
  last_name: Suleimanov
- first_name: Alexander A.
  full_name: Lutovinov, Alexander A.
  last_name: Lutovinov
- first_name: Ilya A.
  full_name: Mereminskiy, Ilya A.
  last_name: Mereminskiy
- first_name: Sergey V.
  full_name: Molkov, Sergey V.
  last_name: Molkov
- first_name: Alexander
  full_name: Salganik, Alexander
  last_name: Salganik
- first_name: Andrea
  full_name: Santangelo, Andrea
  last_name: Santangelo
- first_name: Andrei V.
  full_name: Berdyugin, Andrei V.
  last_name: Berdyugin
- first_name: Vadim
  full_name: Kravtsov, Vadim
  last_name: Kravtsov
- first_name: Anagha P.
  full_name: Nitindala, Anagha P.
  last_name: Nitindala
- first_name: Iván
  full_name: Agudo, Iván
  last_name: Agudo
- first_name: Lucio A.
  full_name: Antonelli, Lucio A.
  last_name: Antonelli
- first_name: Matteo
  full_name: Bachetti, Matteo
  last_name: Bachetti
- first_name: Luca
  full_name: Baldini, Luca
  last_name: Baldini
- first_name: Wayne H.
  full_name: Baumgartner, Wayne H.
  last_name: Baumgartner
- first_name: Ronaldo
  full_name: Bellazzini, Ronaldo
  last_name: Bellazzini
- first_name: Stefano
  full_name: Bianchi, Stefano
  last_name: Bianchi
- first_name: Stephen D.
  full_name: Bongiorno, Stephen D.
  last_name: Bongiorno
- first_name: Raffaella
  full_name: Bonino, Raffaella
  last_name: Bonino
- first_name: Alessandro
  full_name: Brez, Alessandro
  last_name: Brez
- first_name: Niccolò
  full_name: Bucciantini, Niccolò
  last_name: Bucciantini
- first_name: Fiamma
  full_name: Capitanio, Fiamma
  last_name: Capitanio
- first_name: Simone
  full_name: Castellano, Simone
  last_name: Castellano
- first_name: Elisabetta
  full_name: Cavazzuti, Elisabetta
  last_name: Cavazzuti
- first_name: Chien-Ting
  full_name: Chen, Chien-Ting
  last_name: Chen
- first_name: Stefano
  full_name: Ciprini, Stefano
  last_name: Ciprini
- first_name: Enrico
  full_name: Costa, Enrico
  last_name: Costa
- first_name: Alessandra
  full_name: De Rosa, Alessandra
  last_name: De Rosa
- first_name: Ettore
  full_name: Del Monte, Ettore
  last_name: Del Monte
- first_name: Laura
  full_name: Di Gesu, Laura
  last_name: Di Gesu
- first_name: Niccolò
  full_name: Di Lalla, Niccolò
  last_name: Di Lalla
- first_name: Alessandro
  full_name: Di Marco, Alessandro
  last_name: Di Marco
- first_name: Immacolata
  full_name: Donnarumma, Immacolata
  last_name: Donnarumma
- first_name: Michal
  full_name: Dovčiak, Michal
  last_name: Dovčiak
- first_name: Steven R.
  full_name: Ehlert, Steven R.
  last_name: Ehlert
- first_name: Teruaki
  full_name: Enoto, Teruaki
  last_name: Enoto
- first_name: Yuri
  full_name: Evangelista, Yuri
  last_name: Evangelista
- first_name: Sergio
  full_name: Fabiani, Sergio
  last_name: Fabiani
- first_name: Riccardo
  full_name: Ferrazzoli, Riccardo
  last_name: Ferrazzoli
- first_name: Javier A.
  full_name: García, Javier A.
  last_name: García
- first_name: Shuichi
  full_name: Gunji, Shuichi
  last_name: Gunji
- first_name: Kiyoshi
  full_name: Hayashida, Kiyoshi
  last_name: Hayashida
- first_name: Wataru
  full_name: Iwakiri, Wataru
  last_name: Iwakiri
- first_name: Svetlana G.
  full_name: Jorstad, Svetlana G.
  last_name: Jorstad
- first_name: Philip
  full_name: Kaaret, Philip
  last_name: Kaaret
- first_name: Vladimir
  full_name: Karas, Vladimir
  last_name: Karas
- first_name: Fabian
  full_name: Kislat, Fabian
  last_name: Kislat
- first_name: Takao
  full_name: Kitaguchi, Takao
  last_name: Kitaguchi
- first_name: Jeffery J.
  full_name: Kolodziejczak, Jeffery J.
  last_name: Kolodziejczak
- first_name: Henric
  full_name: Krawczynski, Henric
  last_name: Krawczynski
- first_name: Fabio
  full_name: La Monaca, Fabio
  last_name: La Monaca
- first_name: Luca
  full_name: Latronico, Luca
  last_name: Latronico
- first_name: Ioannis
  full_name: Liodakis, Ioannis
  last_name: Liodakis
- first_name: Simone
  full_name: Maldera, Simone
  last_name: Maldera
- first_name: Alberto
  full_name: Manfreda, Alberto
  last_name: Manfreda
- first_name: Frédéric
  full_name: Marin, Frédéric
  last_name: Marin
- first_name: Andrea
  full_name: Marinucci, Andrea
  last_name: Marinucci
- first_name: Alan P.
  full_name: Marscher, Alan P.
  last_name: Marscher
- first_name: Herman L.
  full_name: Marshall, Herman L.
  last_name: Marshall
- first_name: Francesco
  full_name: Massaro, Francesco
  last_name: Massaro
- first_name: Giorgio
  full_name: Matt, Giorgio
  last_name: Matt
- first_name: Ikuyuki
  full_name: Mitsuishi, Ikuyuki
  last_name: Mitsuishi
- first_name: Tsunefumi
  full_name: Mizuno, Tsunefumi
  last_name: Mizuno
- first_name: Fabio
  full_name: Muleri, Fabio
  last_name: Muleri
- first_name: Michela
  full_name: Negro, Michela
  last_name: Negro
- first_name: Chi-Yung
  full_name: Ng, Chi-Yung
  last_name: Ng
- first_name: Stephen L.
  full_name: O’Dell, Stephen L.
  last_name: O’Dell
- first_name: Nicola
  full_name: Omodei, Nicola
  last_name: Omodei
- first_name: Chiara
  full_name: Oppedisano, Chiara
  last_name: Oppedisano
- first_name: Alessandro
  full_name: Papitto, Alessandro
  last_name: Papitto
- first_name: George G.
  full_name: Pavlov, George G.
  last_name: Pavlov
- first_name: Abel L.
  full_name: Peirson, Abel L.
  last_name: Peirson
- first_name: Matteo
  full_name: Perri, Matteo
  last_name: Perri
- first_name: Melissa
  full_name: Pesce-Rollins, Melissa
  last_name: Pesce-Rollins
- first_name: Pierre-Olivier
  full_name: Petrucci, Pierre-Olivier
  last_name: Petrucci
- first_name: Maura
  full_name: Pilia, Maura
  last_name: Pilia
- first_name: Andrea
  full_name: Possenti, Andrea
  last_name: Possenti
- first_name: Simonetta
  full_name: Puccetti, Simonetta
  last_name: Puccetti
- first_name: Brian D.
  full_name: Ramsey, Brian D.
  last_name: Ramsey
- first_name: John
  full_name: Rankin, John
  last_name: Rankin
- first_name: Ajay
  full_name: Ratheesh, Ajay
  last_name: Ratheesh
- first_name: Oliver J.
  full_name: Roberts, Oliver J.
  last_name: Roberts
- first_name: Roger W.
  full_name: Romani, Roger W.
  last_name: Romani
- first_name: Carmelo
  full_name: Sgrò, Carmelo
  last_name: Sgrò
- first_name: Patrick
  full_name: Slane, Patrick
  last_name: Slane
- first_name: Paolo
  full_name: Soffitta, Paolo
  last_name: Soffitta
- first_name: Gloria
  full_name: Spandre, Gloria
  last_name: Spandre
- first_name: Douglas A.
  full_name: Swartz, Douglas A.
  last_name: Swartz
- first_name: Toru
  full_name: Tamagawa, Toru
  last_name: Tamagawa
- first_name: Fabrizio
  full_name: Tavecchio, Fabrizio
  last_name: Tavecchio
- first_name: Roberto
  full_name: Taverna, Roberto
  last_name: Taverna
- first_name: Yuzuru
  full_name: Tawara, Yuzuru
  last_name: Tawara
- first_name: Allyn F.
  full_name: Tennant, Allyn F.
  last_name: Tennant
- first_name: Nicholas E.
  full_name: Thomas, Nicholas E.
  last_name: Thomas
- first_name: Francesco
  full_name: Tombesi, Francesco
  last_name: Tombesi
- first_name: Alessio
  full_name: Trois, Alessio
  last_name: Trois
- first_name: Jacco
  full_name: Vink, Jacco
  last_name: Vink
- first_name: Kinwah
  full_name: Wu, Kinwah
  last_name: Wu
- first_name: Fei
  full_name: Xie, Fei
  last_name: Xie
- first_name: Silvia
  full_name: Zane, Silvia
  last_name: Zane
citation:
  ama: Doroshenko V, Poutanen J, Heyl J, et al. Complex variations in X-ray polarization
    in the X-ray pulsar LS V +44 17/RX J0440.9+4431. <i>Astronomy &#38; Astrophysics</i>.
    2023;677. doi:<a href="https://doi.org/10.1051/0004-6361/202347088">10.1051/0004-6361/202347088</a>
  apa: Doroshenko, V., Poutanen, J., Heyl, J., Tsygankov, S. S., Caiazzo, I., Turolla,
    R., … Zane, S. (2023). Complex variations in X-ray polarization in the X-ray pulsar
    LS V +44 17/RX J0440.9+4431. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences.
    <a href="https://doi.org/10.1051/0004-6361/202347088">https://doi.org/10.1051/0004-6361/202347088</a>
  chicago: Doroshenko, Victor, Juri Poutanen, Jeremy Heyl, Sergey S. Tsygankov, Ilaria
    Caiazzo, Roberto Turolla, Alexandra Veledina, et al. “Complex Variations in X-Ray
    Polarization in the X-Ray Pulsar LS V +44 17/RX J0440.9+4431.” <i>Astronomy &#38;
    Astrophysics</i>. EDP Sciences, 2023. <a href="https://doi.org/10.1051/0004-6361/202347088">https://doi.org/10.1051/0004-6361/202347088</a>.
  ieee: V. Doroshenko <i>et al.</i>, “Complex variations in X-ray polarization in
    the X-ray pulsar LS V +44 17/RX J0440.9+4431,” <i>Astronomy &#38; Astrophysics</i>,
    vol. 677. EDP Sciences, 2023.
  ista: Doroshenko V et al. 2023. Complex variations in X-ray polarization in the
    X-ray pulsar LS V +44 17/RX J0440.9+4431. Astronomy &#38; Astrophysics. 677, A57.
  mla: Doroshenko, Victor, et al. “Complex Variations in X-Ray Polarization in the
    X-Ray Pulsar LS V +44 17/RX J0440.9+4431.” <i>Astronomy &#38; Astrophysics</i>,
    vol. 677, A57, EDP Sciences, 2023, doi:<a href="https://doi.org/10.1051/0004-6361/202347088">10.1051/0004-6361/202347088</a>.
  short: V. Doroshenko, J. Poutanen, J. Heyl, S.S. Tsygankov, I. Caiazzo, R. Turolla,
    A. Veledina, M.C. Weisskopf, S.V. Forsblom, D. González-Caniulef, V. Loktev, C.
    Malacaria, A.A. Mushtukov, V.F. Suleimanov, A.A. Lutovinov, I.A. Mereminskiy,
    S.V. Molkov, A. Salganik, A. Santangelo, A.V. Berdyugin, V. Kravtsov, A.P. Nitindala,
    I. Agudo, L.A. Antonelli, M. Bachetti, L. Baldini, W.H. Baumgartner, R. Bellazzini,
    S. Bianchi, S.D. Bongiorno, R. Bonino, A. Brez, N. Bucciantini, F. Capitanio,
    S. Castellano, E. Cavazzuti, C.-T. Chen, S. Ciprini, E. Costa, A. De Rosa, E.
    Del Monte, L. Di Gesu, N. Di Lalla, A. Di Marco, I. Donnarumma, M. Dovčiak, S.R.
    Ehlert, T. Enoto, Y. Evangelista, S. Fabiani, R. Ferrazzoli, J.A. García, S. Gunji,
    K. Hayashida, W. Iwakiri, S.G. Jorstad, P. Kaaret, V. Karas, F. Kislat, T. Kitaguchi,
    J.J. Kolodziejczak, H. Krawczynski, F. La Monaca, L. Latronico, I. Liodakis, S.
    Maldera, A. Manfreda, F. Marin, A. Marinucci, A.P. Marscher, H.L. Marshall, F.
    Massaro, G. Matt, I. Mitsuishi, T. Mizuno, F. Muleri, M. Negro, C.-Y. Ng, S.L.
    O’Dell, N. Omodei, C. Oppedisano, A. Papitto, G.G. Pavlov, A.L. Peirson, M. Perri,
    M. Pesce-Rollins, P.-O. Petrucci, M. Pilia, A. Possenti, S. Puccetti, B.D. Ramsey,
    J. Rankin, A. Ratheesh, O.J. Roberts, R.W. Romani, C. Sgrò, P. Slane, P. Soffitta,
    G. Spandre, D.A. Swartz, T. Tamagawa, F. Tavecchio, R. Taverna, Y. Tawara, A.F.
    Tennant, N.E. Thomas, F. Tombesi, A. Trois, J. Vink, K. Wu, F. Xie, S. Zane, Astronomy
    &#38; Astrophysics 677 (2023).
date_created: 2024-03-26T09:46:01Z
date_published: 2023-09-04T00:00:00Z
date_updated: 2024-04-02T06:57:11Z
day: '04'
doi: 10.1051/0004-6361/202347088
extern: '1'
external_id:
  arxiv:
  - '2306.02116'
intvolume: '       677'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1051/0004-6361/202347088
month: '09'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
  eissn:
  - 1432-0746
  issn:
  - 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: Complex variations in X-ray polarization in the X-ray pulsar LS V +44 17/RX
  J0440.9+4431
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: 677
year: '2023'
...
---
_id: '15194'
abstract:
- lang: eng
  text: "AM Canum Venaticorum (AM CVn) systems are ultracompact binaries where a white
    dwarf accretes from a helium-rich degenerate or semidegenerate donor. Some AM
    CVn systems will be among the loudest sources of gravitational waves for the upcoming
    Laser Interferometer Space Antenna; yet the formation channel of AM CVns remains
    uncertain. We report the study and characterization of a new eclipsing AM CVn,
    SRGeJ045359.9+622444 (hereafter, SRGeJ0453), discovered from a joint Spektrum-Roentgen-Gamma
    (SRG) Extended Roentgen Survey with an Imaging Telescope Array (eROSITA) mission
    and Zwicky Transient Facility program to identify cataclysmic variables (CVs).
    We obtained optical photometry to confirm the eclipse of SRGeJ0453 and determine
    the orbital period to be \r\n. We constrain the binary parameters by modeling
    the high-speed photometry and radial-velocity curves and find Mdonor = 0.044 ±
    0.024M⊙ and Rdonor = 0.078 ± 0.012R⊙. The X-ray spectrum is approximated by a
    power-law model with an unusually flat photon index of Γ ∼ 1 previously seen in
    magnetic CVs with SRG/eROSITA, but verifying that the magnetic nature of SRGeJ0453
    requires further investigation. Optical spectroscopy suggests that the donor star
    of SRGeJ0453 could have initially been a He star or a He white dwarf. SRGeJ0453
    is the ninth eclipsing AM CVn system published to date, and its lack of optical
    outbursts have made it elusive in previous surveys. The discovery of SRGeJ0453
    using joint X-ray and optical surveys highlights the potential for discovering
    similar systems in the near future."
article_number: '63'
article_processing_charge: No
article_type: original
author:
- first_name: Antonio C.
  full_name: Rodriguez, Antonio C.
  last_name: Rodriguez
- first_name: Ilkham
  full_name: Galiullin, Ilkham
  last_name: Galiullin
- first_name: Marat
  full_name: Gilfanov, Marat
  last_name: Gilfanov
- first_name: Shrinivas R.
  full_name: Kulkarni, Shrinivas R.
  last_name: Kulkarni
- first_name: Irek
  full_name: Khamitov, Irek
  last_name: Khamitov
- first_name: Ilfan
  full_name: Bikmaev, Ilfan
  last_name: Bikmaev
- first_name: Jan
  full_name: van Roestel, Jan
  last_name: van Roestel
- first_name: Lev
  full_name: Yungelson, Lev
  last_name: Yungelson
- first_name: Kareem
  full_name: El-Badry, Kareem
  last_name: El-Badry
- first_name: Rashid
  full_name: Sunayev, Rashid
  last_name: Sunayev
- 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: Andrew
  full_name: Drake, Andrew
  last_name: Drake
- 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: Frank J.
  full_name: Masci, Frank J.
  last_name: Masci
- first_name: Pavel
  full_name: Medvedev, Pavel
  last_name: Medvedev
- first_name: Josiah
  full_name: Purdum, Josiah
  last_name: Purdum
- first_name: Nail
  full_name: Sakhibullin, Nail
  last_name: Sakhibullin
- first_name: Alexander
  full_name: Sklyanov, Alexander
  last_name: Sklyanov
- first_name: Roger
  full_name: Smith, Roger
  last_name: Smith
- first_name: Paula
  full_name: Szkody, Paula
  last_name: Szkody
- first_name: Zachary P.
  full_name: Vanderbosch, Zachary P.
  last_name: Vanderbosch
citation:
  ama: 'Rodriguez AC, Galiullin I, Gilfanov M, et al. SRGeJ045359.9+622444: A 55 minute
    period eclipsing AM Canum Venaticorum star discovered from a joint SRG/eROSITA
    + ZTF search. <i>The Astrophysical Journal</i>. 2023;954(1). doi:<a href="https://doi.org/10.3847/1538-4357/ace698">10.3847/1538-4357/ace698</a>'
  apa: 'Rodriguez, A. C., Galiullin, I., Gilfanov, M., Kulkarni, S. R., Khamitov,
    I., Bikmaev, I., … Vanderbosch, Z. P. (2023). SRGeJ045359.9+622444: A 55 minute
    period eclipsing AM Canum Venaticorum star discovered from a joint SRG/eROSITA
    + ZTF search. <i>The Astrophysical Journal</i>. American Astronomical Society.
    <a href="https://doi.org/10.3847/1538-4357/ace698">https://doi.org/10.3847/1538-4357/ace698</a>'
  chicago: 'Rodriguez, Antonio C., Ilkham Galiullin, Marat Gilfanov, Shrinivas R.
    Kulkarni, Irek Khamitov, Ilfan Bikmaev, Jan van Roestel, et al. “SRGeJ045359.9+622444:
    A 55 Minute Period Eclipsing AM Canum Venaticorum Star Discovered from a Joint
    SRG/EROSITA + ZTF Search.” <i>The Astrophysical Journal</i>. American Astronomical
    Society, 2023. <a href="https://doi.org/10.3847/1538-4357/ace698">https://doi.org/10.3847/1538-4357/ace698</a>.'
  ieee: 'A. C. Rodriguez <i>et al.</i>, “SRGeJ045359.9+622444: A 55 minute period
    eclipsing AM Canum Venaticorum star discovered from a joint SRG/eROSITA + ZTF
    search,” <i>The Astrophysical Journal</i>, vol. 954, no. 1. American Astronomical
    Society, 2023.'
  ista: 'Rodriguez AC, Galiullin I, Gilfanov M, Kulkarni SR, Khamitov I, Bikmaev I,
    van Roestel J, Yungelson L, El-Badry K, Sunayev R, Prince TA, Buntov M, Caiazzo
    I, Drake A, Gorbachev M, Graham MJ, Gumerov R, Irtuganov E, Laher RR, Masci FJ,
    Medvedev P, Purdum J, Sakhibullin N, Sklyanov A, Smith R, Szkody P, Vanderbosch
    ZP. 2023. SRGeJ045359.9+622444: A 55 minute period eclipsing AM Canum Venaticorum
    star discovered from a joint SRG/eROSITA + ZTF search. The Astrophysical Journal.
    954(1), 63.'
  mla: 'Rodriguez, Antonio C., et al. “SRGeJ045359.9+622444: A 55 Minute Period Eclipsing
    AM Canum Venaticorum Star Discovered from a Joint SRG/EROSITA + ZTF Search.” <i>The
    Astrophysical Journal</i>, vol. 954, no. 1, 63, American Astronomical Society,
    2023, doi:<a href="https://doi.org/10.3847/1538-4357/ace698">10.3847/1538-4357/ace698</a>.'
  short: A.C. Rodriguez, I. Galiullin, M. Gilfanov, S.R. Kulkarni, I. Khamitov, I.
    Bikmaev, J. van Roestel, L. Yungelson, K. El-Badry, R. Sunayev, T.A. Prince, M.
    Buntov, I. Caiazzo, A. Drake, M. Gorbachev, M.J. Graham, R. Gumerov, E. Irtuganov,
    R.R. Laher, F.J. Masci, P. Medvedev, J. Purdum, N. Sakhibullin, A. Sklyanov, R.
    Smith, P. Szkody, Z.P. Vanderbosch, The Astrophysical Journal 954 (2023).
date_created: 2024-03-26T09:46:30Z
date_published: 2023-08-23T00:00:00Z
date_updated: 2024-04-02T06:58:03Z
day: '23'
doi: 10.3847/1538-4357/ace698
extern: '1'
intvolume: '       954'
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/ace698
month: '08'
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: 'SRGeJ045359.9+622444: A 55 minute period eclipsing AM Canum Venaticorum star
  discovered from a joint SRG/eROSITA + ZTF search'
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: 954
year: '2023'
...
---
_id: '15195'
abstract:
- lang: eng
  text: 'White dwarfs, the extremely dense remnants left behind by most stars after
    their death, are characterized by a mass comparable to that of the Sun compressed
    into the size of an Earth-like planet. In the resulting strong gravity, heavy
    elements sink towards the centre and the upper layer of the atmosphere contains
    only the lightest element present, usually hydrogen or helium1,2. Several mechanisms
    compete with gravitational settling to change a white dwarf’s surface composition
    as it cools3, and the fraction of white dwarfs with helium atmospheres is known
    to increase by a factor of about 2.5 below a temperature of about 30,000 kelvin4,5,6,7,8;
    therefore, some white dwarfs that appear to have hydrogen-dominated atmospheres
    above 30,000 kelvin are bound to transition to be helium-dominated as they cool
    below it. Here we report observations of ZTF J203349.8+322901.1, a transitioning
    white dwarf with two faces: one side of its atmosphere is dominated by hydrogen
    and the other one by helium. This peculiar nature is probably caused by the presence
    of a small magnetic field, which creates an inhomogeneity in temperature, pressure
    or mixing strength over the surface9,10,11. ZTF J203349.8+322901.1 might be the
    most extreme member of a class of magnetic, transitioning white dwarfs—together
    with GD 323 (ref. 12), a white dwarf that shows similar but much more subtle variations.
    This class of white dwarfs could help shed light on the physical mechanisms behind
    the spectral evolution of white dwarfs.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Kevin B.
  full_name: Burdge, Kevin B.
  last_name: Burdge
- first_name: Pier-Emmanuel
  full_name: Tremblay, Pier-Emmanuel
  last_name: Tremblay
- first_name: James
  full_name: Fuller, James
  last_name: Fuller
- first_name: Lilia
  full_name: Ferrario, Lilia
  last_name: Ferrario
- first_name: Boris T.
  full_name: Gänsicke, Boris T.
  last_name: Gänsicke
- first_name: J. J.
  full_name: Hermes, J. J.
  last_name: Hermes
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
- first_name: Adela
  full_name: Kawka, Adela
  last_name: Kawka
- first_name: S. R.
  full_name: Kulkarni, S. R.
  last_name: Kulkarni
- first_name: Thomas R.
  full_name: Marsh, Thomas R.
  last_name: Marsh
- first_name: Przemek
  full_name: Mróz, Przemek
  last_name: Mróz
- first_name: Thomas A.
  full_name: Prince, Thomas A.
  last_name: Prince
- first_name: Harvey B.
  full_name: Richer, Harvey B.
  last_name: Richer
- first_name: Antonio C.
  full_name: Rodriguez, Antonio C.
  last_name: Rodriguez
- first_name: Jan
  full_name: van Roestel, Jan
  last_name: van Roestel
- first_name: Zachary P.
  full_name: Vanderbosch, Zachary P.
  last_name: Vanderbosch
- first_name: Stéphane
  full_name: Vennes, Stéphane
  last_name: Vennes
- first_name: Dayal
  full_name: Wickramasinghe, Dayal
  last_name: Wickramasinghe
- first_name: Vikram S.
  full_name: Dhillon, Vikram S.
  last_name: Dhillon
- first_name: Stuart P.
  full_name: Littlefair, Stuart P.
  last_name: Littlefair
- first_name: James
  full_name: Munday, James
  last_name: Munday
- first_name: Ingrid
  full_name: Pelisoli, Ingrid
  last_name: Pelisoli
- first_name: Daniel
  full_name: Perley, Daniel
  last_name: Perley
- first_name: Eric C.
  full_name: Bellm, Eric C.
  last_name: Bellm
- first_name: Elmé
  full_name: Breedt, Elmé
  last_name: Breedt
- first_name: Alex J.
  full_name: Brown, Alex J.
  last_name: Brown
- first_name: Richard
  full_name: Dekany, Richard
  last_name: Dekany
- first_name: Andrew
  full_name: Drake, Andrew
  last_name: Drake
- first_name: Martin J.
  full_name: Dyer, Martin J.
  last_name: Dyer
- first_name: Matthew J.
  full_name: Graham, Matthew J.
  last_name: Graham
- first_name: Matthew J.
  full_name: Green, Matthew J.
  last_name: Green
- first_name: Russ R.
  full_name: Laher, Russ R.
  last_name: Laher
- first_name: Paul
  full_name: Kerry, Paul
  last_name: Kerry
- first_name: Steven G.
  full_name: Parsons, Steven G.
  last_name: Parsons
- first_name: Reed L.
  full_name: Riddle, Reed L.
  last_name: Riddle
- first_name: Ben
  full_name: Rusholme, Ben
  last_name: Rusholme
- first_name: Dave I.
  full_name: Sahman, Dave I.
  last_name: Sahman
citation:
  ama: Caiazzo I, Burdge KB, Tremblay P-E, et al. A rotating white dwarf shows different
    compositions on its opposite faces. <i>Nature</i>. 2023;620(7972):61-66. doi:<a
    href="https://doi.org/10.1038/s41586-023-06171-9">10.1038/s41586-023-06171-9</a>
  apa: Caiazzo, I., Burdge, K. B., Tremblay, P.-E., Fuller, J., Ferrario, L., Gänsicke,
    B. T., … Sahman, D. I. (2023). A rotating white dwarf shows different compositions
    on its opposite faces. <i>Nature</i>. Springer Nature. <a href="https://doi.org/10.1038/s41586-023-06171-9">https://doi.org/10.1038/s41586-023-06171-9</a>
  chicago: Caiazzo, Ilaria, Kevin B. Burdge, Pier-Emmanuel Tremblay, James Fuller,
    Lilia Ferrario, Boris T. Gänsicke, J. J. Hermes, et al. “A Rotating White Dwarf
    Shows Different Compositions on Its Opposite Faces.” <i>Nature</i>. Springer Nature,
    2023. <a href="https://doi.org/10.1038/s41586-023-06171-9">https://doi.org/10.1038/s41586-023-06171-9</a>.
  ieee: I. Caiazzo <i>et al.</i>, “A rotating white dwarf shows different compositions
    on its opposite faces,” <i>Nature</i>, vol. 620, no. 7972. Springer Nature, pp.
    61–66, 2023.
  ista: Caiazzo I, Burdge KB, Tremblay P-E, Fuller J, Ferrario L, Gänsicke BT, Hermes
    JJ, Heyl J, Kawka A, Kulkarni SR, Marsh TR, Mróz P, Prince TA, Richer HB, Rodriguez
    AC, van Roestel J, Vanderbosch ZP, Vennes S, Wickramasinghe D, Dhillon VS, Littlefair
    SP, Munday J, Pelisoli I, Perley D, Bellm EC, Breedt E, Brown AJ, Dekany R, Drake
    A, Dyer MJ, Graham MJ, Green MJ, Laher RR, Kerry P, Parsons SG, Riddle RL, Rusholme
    B, Sahman DI. 2023. A rotating white dwarf shows different compositions on its
    opposite faces. Nature. 620(7972), 61–66.
  mla: Caiazzo, Ilaria, et al. “A Rotating White Dwarf Shows Different Compositions
    on Its Opposite Faces.” <i>Nature</i>, vol. 620, no. 7972, Springer Nature, 2023,
    pp. 61–66, doi:<a href="https://doi.org/10.1038/s41586-023-06171-9">10.1038/s41586-023-06171-9</a>.
  short: I. Caiazzo, K.B. Burdge, P.-E. Tremblay, J. Fuller, L. Ferrario, B.T. Gänsicke,
    J.J. Hermes, J. Heyl, A. Kawka, S.R. Kulkarni, T.R. Marsh, P. Mróz, T.A. Prince,
    H.B. Richer, A.C. Rodriguez, J. van Roestel, Z.P. Vanderbosch, S. Vennes, D. Wickramasinghe,
    V.S. Dhillon, S.P. Littlefair, J. Munday, I. Pelisoli, D. Perley, E.C. Bellm,
    E. Breedt, A.J. Brown, R. Dekany, A. Drake, M.J. Dyer, M.J. Graham, M.J. Green,
    R.R. Laher, P. Kerry, S.G. Parsons, R.L. Riddle, B. Rusholme, D.I. Sahman, Nature
    620 (2023) 61–66.
date_created: 2024-03-26T09:46:57Z
date_published: 2023-07-19T00:00:00Z
date_updated: 2024-10-14T12:32:28Z
day: '19'
doi: 10.1038/s41586-023-06171-9
extern: '1'
external_id:
  arxiv:
  - '2308.07430'
intvolume: '       620'
issue: '7972'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2308.07430
month: '07'
oa: 1
oa_version: Preprint
page: 61-66
publication: Nature
publication_identifier:
  eissn:
  - 1476-4687
  issn:
  - 0028-0836
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: A rotating white dwarf shows different compositions on its opposite faces
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 620
year: '2023'
...
---
_id: '15196'
abstract:
- lang: eng
  text: We report the discovery of ZTF J0127+5258, a compact mass-transferring binary
    with an orbital period of 13.7 minutes. The system contains a white dwarf accretor,
    which likely originated as a post–common envelope carbon–oxygen (CO) white dwarf,
    and a warm donor (Teff,donor = 16,400 ± 1000 K). The donor probably formed during
    a common envelope phase between the CO white dwarf and an evolving giant that
    left behind a helium star or white dwarf in a close orbit with the CO white dwarf.
    We measure gravitational wave–driven orbital inspiral with ∼51σ significance,
    which yields a joint constraint on the component masses and mass transfer rate.
    While the accretion disk in the system is dominated by ionized helium emission,
    the donor exhibits a mixture of hydrogen and helium absorption lines. Phase-resolved
    spectroscopy yields a donor radial velocity semiamplitude of 771 ± 27 km s−1,
    and high-speed photometry reveals that the system is eclipsing. We detect a Chandra
    X-ray counterpart with LX ∼ 3 × 1031 erg s−1. Depending on the mass transfer rate,
    the system will likely either evolve into a stably mass-transferring helium cataclysmic
    variable, merge to become an R CrB star, or explode as a Type Ia supernova in
    the next million years. We predict that the Laser Space Interferometer Antenna
    (LISA) will detect the source with a signal-to-noise ratio of 24 ± 6 after 4 yr
    of observations. The system is the first LISA-loud mass-transferring binary with
    an intrinsically luminous donor, a class of sources that provide the opportunity
    to leverage the synergy between optical and infrared time domain surveys, X-ray
    facilities, and gravitational-wave observatories to probe general relativity,
    accretion physics, and binary evolution.
article_number: L1
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Kevin B.
  full_name: Burdge, Kevin B.
  last_name: Burdge
- first_name: Kareem
  full_name: El-Badry, Kareem
  last_name: El-Badry
- first_name: Saul
  full_name: Rappaport, Saul
  last_name: Rappaport
- first_name: Tin Long
  full_name: Sunny Wong, Tin Long
  last_name: Sunny Wong
- first_name: Evan B.
  full_name: Bauer, Evan B.
  last_name: Bauer
- first_name: Lars
  full_name: Bildsten, Lars
  last_name: Bildsten
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Deepto
  full_name: Chakrabarty, Deepto
  last_name: Chakrabarty
- first_name: Emma
  full_name: Chickles, Emma
  last_name: Chickles
- first_name: Matthew J.
  full_name: Graham, Matthew J.
  last_name: Graham
- first_name: Erin
  full_name: Kara, Erin
  last_name: Kara
- first_name: S. R.
  full_name: Kulkarni, S. R.
  last_name: Kulkarni
- first_name: Thomas R.
  full_name: Marsh, Thomas R.
  last_name: Marsh
- first_name: Melania
  full_name: Nynka, Melania
  last_name: Nynka
- first_name: Thomas A.
  full_name: Prince, Thomas A.
  last_name: Prince
- first_name: Robert A.
  full_name: Simcoe, Robert A.
  last_name: Simcoe
- first_name: Jan
  full_name: van Roestel, Jan
  last_name: van Roestel
- first_name: Zach
  full_name: Vanderbosch, Zach
  last_name: Vanderbosch
- first_name: Eric C.
  full_name: Bellm, Eric C.
  last_name: Bellm
- first_name: Richard G.
  full_name: Dekany, Richard G.
  last_name: Dekany
- first_name: Andrew J.
  full_name: Drake, Andrew J.
  last_name: Drake
- first_name: George
  full_name: Helou, George
  last_name: Helou
- first_name: Frank J.
  full_name: Masci, Frank J.
  last_name: Masci
- first_name: Jennifer
  full_name: Milburn, Jennifer
  last_name: Milburn
- first_name: Reed
  full_name: Riddle, Reed
  last_name: Riddle
- first_name: Ben
  full_name: Rusholme, Ben
  last_name: Rusholme
- first_name: Roger
  full_name: Smith, Roger
  last_name: Smith
citation:
  ama: Burdge KB, El-Badry K, Rappaport S, et al. Orbital decay in an accreting and
    eclipsing 13.7 minute orbital period binary with a luminous donor. <i>The Astrophysical
    Journal Letters</i>. 2023;953(1). doi:<a href="https://doi.org/10.3847/2041-8213/ace7cf">10.3847/2041-8213/ace7cf</a>
  apa: Burdge, K. B., El-Badry, K., Rappaport, S., Sunny Wong, T. L., Bauer, E. B.,
    Bildsten, L., … Smith, R. (2023). Orbital decay in an accreting and eclipsing
    13.7 minute orbital period binary with a luminous donor. <i>The Astrophysical
    Journal Letters</i>. American Astronomical Society. <a href="https://doi.org/10.3847/2041-8213/ace7cf">https://doi.org/10.3847/2041-8213/ace7cf</a>
  chicago: Burdge, Kevin B., Kareem El-Badry, Saul Rappaport, Tin Long Sunny Wong,
    Evan B. Bauer, Lars Bildsten, Ilaria Caiazzo, et al. “Orbital Decay in an Accreting
    and Eclipsing 13.7 Minute Orbital Period Binary with a Luminous Donor.” <i>The
    Astrophysical Journal Letters</i>. American Astronomical Society, 2023. <a href="https://doi.org/10.3847/2041-8213/ace7cf">https://doi.org/10.3847/2041-8213/ace7cf</a>.
  ieee: K. B. Burdge <i>et al.</i>, “Orbital decay in an accreting and eclipsing 13.7
    minute orbital period binary with a luminous donor,” <i>The Astrophysical Journal
    Letters</i>, vol. 953, no. 1. American Astronomical Society, 2023.
  ista: Burdge KB, El-Badry K, Rappaport S, Sunny Wong TL, Bauer EB, Bildsten L, Caiazzo
    I, Chakrabarty D, Chickles E, Graham MJ, Kara E, Kulkarni SR, Marsh TR, Nynka
    M, Prince TA, Simcoe RA, van Roestel J, Vanderbosch Z, Bellm EC, Dekany RG, Drake
    AJ, Helou G, Masci FJ, Milburn J, Riddle R, Rusholme B, Smith R. 2023. Orbital
    decay in an accreting and eclipsing 13.7 minute orbital period binary with a luminous
    donor. The Astrophysical Journal Letters. 953(1), L1.
  mla: Burdge, Kevin B., et al. “Orbital Decay in an Accreting and Eclipsing 13.7
    Minute Orbital Period Binary with a Luminous Donor.” <i>The Astrophysical Journal
    Letters</i>, vol. 953, no. 1, L1, American Astronomical Society, 2023, doi:<a
    href="https://doi.org/10.3847/2041-8213/ace7cf">10.3847/2041-8213/ace7cf</a>.
  short: K.B. Burdge, K. El-Badry, S. Rappaport, T.L. Sunny Wong, E.B. Bauer, L. Bildsten,
    I. Caiazzo, D. Chakrabarty, E. Chickles, M.J. Graham, E. Kara, S.R. Kulkarni,
    T.R. Marsh, M. Nynka, T.A. Prince, R.A. Simcoe, J. van Roestel, Z. Vanderbosch,
    E.C. Bellm, R.G. Dekany, A.J. Drake, G. Helou, F.J. Masci, J. Milburn, R. Riddle,
    B. Rusholme, R. Smith, The Astrophysical Journal Letters 953 (2023).
date_created: 2024-03-26T09:47:22Z
date_published: 2023-08-08T00:00:00Z
date_updated: 2024-04-02T07:01:46Z
day: '08'
doi: 10.3847/2041-8213/ace7cf
extern: '1'
external_id:
  arxiv:
  - '2303.13573'
intvolume: '       953'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.3847/2041-8213/ace7cf
month: '08'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal Letters
publication_identifier:
  eissn:
  - 2041-8213
  issn:
  - 2041-8205
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Orbital decay in an accreting and eclipsing 13.7 minute orbital period binary
  with a luminous donor
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: 953
year: '2023'
...
---
_id: '15197'
abstract:
- lang: eng
  text: Recently, the inner main belt asteroid (152830) Dinkinesh was identified as
    an additional fly- by target for the Lucy mission. The heliocentric orbit and
    approximate absolute magnitude of Dinkinesh are known, but little additional information
    was available prior to its selection as a target. In particular, the lack of color
    spectrophotometry or spectra made it impossible to assign a spectral type to Dinkinesh
    from which its albedo could be estimated. We set out to remedy this knowledge
    gap by obtaining visible wavelength spectra with the Keck telescope on 2022 November
    23 and with Gemini-South on 2022 December 27. The spectra measured with the Keck
    I/Low Resolution Imaging Spectrometer (LRIS) and the Gemini South/Gemini Multi-Object
    Spectrograph South (GMOS-S) are most similar to the average spectrum of S- and
    Sq-type asteroids. The most diagnostic feature is the ≈15 ± 1% silicate absorption
    feature at ≈0.9–1.0 μm. Small S- and Sq-type asteroids have moderately high albedos
    ranging from 0.17 to 0.35. Using this albedo range for Dinkinesh in combination
    with measured absolute magnitude, it is possible to derive an effective diameter
    and surface brightness for this body. The albedo, size and surface brightness
    are important inputs required for planning a successful encounter by the Lucy
    spacecraft.
article_number: '115562'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: B.T.
  full_name: Bolin, B.T.
  last_name: Bolin
- first_name: K.S.
  full_name: Noll, K.S.
  last_name: Noll
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: C.
  full_name: Fremling, C.
  last_name: Fremling
- first_name: R.P.
  full_name: Binzel, R.P.
  last_name: Binzel
citation:
  ama: Bolin BT, Noll KS, Caiazzo I, Fremling C, Binzel RP. Keck and Gemini spectral
    characterization of Lucy mission fly-by target (152830) Dinkinesh. <i>Icarus</i>.
    2023;400. doi:<a href="https://doi.org/10.1016/j.icarus.2023.115562">10.1016/j.icarus.2023.115562</a>
  apa: Bolin, B. T., Noll, K. S., Caiazzo, I., Fremling, C., &#38; Binzel, R. P. (2023).
    Keck and Gemini spectral characterization of Lucy mission fly-by target (152830)
    Dinkinesh. <i>Icarus</i>. Elsevier. <a href="https://doi.org/10.1016/j.icarus.2023.115562">https://doi.org/10.1016/j.icarus.2023.115562</a>
  chicago: Bolin, B.T., K.S. Noll, Ilaria Caiazzo, C. Fremling, and R.P. Binzel. “Keck
    and Gemini Spectral Characterization of Lucy Mission Fly-by Target (152830) Dinkinesh.”
    <i>Icarus</i>. Elsevier, 2023. <a href="https://doi.org/10.1016/j.icarus.2023.115562">https://doi.org/10.1016/j.icarus.2023.115562</a>.
  ieee: B. T. Bolin, K. S. Noll, I. Caiazzo, C. Fremling, and R. P. Binzel, “Keck
    and Gemini spectral characterization of Lucy mission fly-by target (152830) Dinkinesh,”
    <i>Icarus</i>, vol. 400. Elsevier, 2023.
  ista: Bolin BT, Noll KS, Caiazzo I, Fremling C, Binzel RP. 2023. Keck and Gemini
    spectral characterization of Lucy mission fly-by target (152830) Dinkinesh. Icarus.
    400, 115562.
  mla: Bolin, B. T., et al. “Keck and Gemini Spectral Characterization of Lucy Mission
    Fly-by Target (152830) Dinkinesh.” <i>Icarus</i>, vol. 400, 115562, Elsevier,
    2023, doi:<a href="https://doi.org/10.1016/j.icarus.2023.115562">10.1016/j.icarus.2023.115562</a>.
  short: B.T. Bolin, K.S. Noll, I. Caiazzo, C. Fremling, R.P. Binzel, Icarus 400 (2023).
date_created: 2024-03-26T09:47:44Z
date_published: 2023-04-07T00:00:00Z
date_updated: 2024-04-02T07:02:28Z
day: '07'
doi: 10.1016/j.icarus.2023.115562
extern: '1'
external_id:
  arxiv:
  - '2303.08130'
intvolume: '       400'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2303.08130
month: '04'
oa: 1
oa_version: Preprint
publication: Icarus
publication_identifier:
  issn:
  - 0019-1035
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Keck and Gemini spectral characterization of Lucy mission fly-by target (152830)
  Dinkinesh
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 400
year: '2023'
...
---
_id: '15198'
abstract:
- lang: eng
  text: The axion-nucleon coupling enables the production of axions through the decay
    of excited 57Fe nuclei, and axions produced in the Sun through this process are
    often a target of helioscope searches. We show for the first time that hot, highly
    magnetic white dwarfs such as ZTF J1901+1458 are a viable target to search for
    the x-ray signature of axions that were produced by the 57Fe transition in the
    core and then converted to photons in the magnetosphere. We calculate that a 100
    ks observation of ZTF J1901+1458 with NuSTAR would constrain the coupling of axions
    to nucleons and photons at a level below the bounds of both current and future
    planned helioscopes.
article_number: L101303
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Leesa
  full_name: Fleury, Leesa
  last_name: Fleury
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
citation:
  ama: Fleury L, Caiazzo I, Heyl J. Constraining axions with ZTF J1901+1458. <i>Physical
    Review D</i>. 2023;107(10). doi:<a href="https://doi.org/10.1103/physrevd.107.l101303">10.1103/physrevd.107.l101303</a>
  apa: Fleury, L., Caiazzo, I., &#38; Heyl, J. (2023). Constraining axions with ZTF
    J1901+1458. <i>Physical Review D</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevd.107.l101303">https://doi.org/10.1103/physrevd.107.l101303</a>
  chicago: Fleury, Leesa, Ilaria Caiazzo, and Jeremy Heyl. “Constraining Axions with
    ZTF J1901+1458.” <i>Physical Review D</i>. American Physical Society, 2023. <a
    href="https://doi.org/10.1103/physrevd.107.l101303">https://doi.org/10.1103/physrevd.107.l101303</a>.
  ieee: L. Fleury, I. Caiazzo, and J. Heyl, “Constraining axions with ZTF J1901+1458,”
    <i>Physical Review D</i>, vol. 107, no. 10. American Physical Society, 2023.
  ista: Fleury L, Caiazzo I, Heyl J. 2023. Constraining axions with ZTF J1901+1458.
    Physical Review D. 107(10), L101303.
  mla: Fleury, Leesa, et al. “Constraining Axions with ZTF J1901+1458.” <i>Physical
    Review D</i>, vol. 107, no. 10, L101303, American Physical Society, 2023, doi:<a
    href="https://doi.org/10.1103/physrevd.107.l101303">10.1103/physrevd.107.l101303</a>.
  short: L. Fleury, I. Caiazzo, J. Heyl, Physical Review D 107 (2023).
date_created: 2024-03-26T09:48:05Z
date_published: 2023-05-17T00:00:00Z
date_updated: 2024-04-02T07:11:34Z
day: '17'
doi: 10.1103/physrevd.107.l101303
extern: '1'
external_id:
  arxiv:
  - '2208.00405'
intvolume: '       107'
issue: '10'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2208.00405
month: '05'
oa: 1
oa_version: Preprint
publication: Physical Review D
publication_identifier:
  eissn:
  - 2470-0029
  issn:
  - 2470-0010
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Constraining axions with ZTF J1901+1458
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 107
year: '2023'
...
---
_id: '15199'
abstract:
- lang: eng
  text: Gaia Data Release 2 revealed a population of ultramassive white dwarfs on
    the Q branch that are moving anomalously fast for a local disc population with
    their young photometric ages. As the velocity dispersion of stars in the local
    disc increases with age, a proposed explanation of these white dwarfs is that
    they experience a cooling delay that causes current cooling models to infer photometric
    ages much younger than their true ages. To explore this explanation, we investigate
    the kinematics of ultramassive white dwarfs within 200 pc of the Sun using the
    improved Gaia Early Data Release 3 observations. We analyse the transverse motions
    of 0.95–1.25 M⊙ white dwarfs, subdivided by mass and age, and determine the distributions
    of the three-dimensional components of the transverse velocities. The results
    are compared to expectations based on observed kinematics of local main-sequence
    stars. We find a population of photometrically young (∼0.5–1.5 Gyr) ultramassive
    (∼1.15–1.25 M⊙) white dwarfs for which the transverse velocity component in the
    direction of Galactic rotation is more dispersed than for local disc stars of
    any age; thus, it is too dispersed to be explained by any cooling delay in white
    dwarfs originating from the local disc. Furthermore, the dispersion ratio of the
    velocity components in the Galactic plane for this population is also inconsistent
    with a local disc origin. We discuss some possible explanations of this kinematically
    anomalous population, such as a halo origin or production through dynamical effects
    of stellar triple systems.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Leesa
  full_name: Fleury, Leesa
  last_name: Fleury
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
citation:
  ama: 'Fleury L, Caiazzo I, Heyl J. The origin of ultramassive white dwarfs: hints
    from <i>Gaia</i> EDR3. <i>Monthly Notices of the Royal Astronomical Society</i>.
    2023;520(1):364-374. doi:<a href="https://doi.org/10.1093/mnras/stad068">10.1093/mnras/stad068</a>'
  apa: 'Fleury, L., Caiazzo, I., &#38; Heyl, J. (2023). The origin of ultramassive
    white dwarfs: hints from <i>Gaia</i> EDR3. <i>Monthly Notices of the Royal Astronomical
    Society</i>. Oxford University Press. <a href="https://doi.org/10.1093/mnras/stad068">https://doi.org/10.1093/mnras/stad068</a>'
  chicago: 'Fleury, Leesa, Ilaria Caiazzo, and Jeremy Heyl. “The Origin of Ultramassive
    White Dwarfs: Hints from <i>Gaia</i> EDR3.” <i>Monthly Notices of the Royal Astronomical
    Society</i>. Oxford University Press, 2023. <a href="https://doi.org/10.1093/mnras/stad068">https://doi.org/10.1093/mnras/stad068</a>.'
  ieee: 'L. Fleury, I. Caiazzo, and J. Heyl, “The origin of ultramassive white dwarfs:
    hints from <i>Gaia</i> EDR3,” <i>Monthly Notices of the Royal Astronomical Society</i>,
    vol. 520, no. 1. Oxford University Press, pp. 364–374, 2023.'
  ista: 'Fleury L, Caiazzo I, Heyl J. 2023. The origin of ultramassive white dwarfs:
    hints from <i>Gaia</i> EDR3. Monthly Notices of the Royal Astronomical Society.
    520(1), 364–374.'
  mla: 'Fleury, Leesa, et al. “The Origin of Ultramassive White Dwarfs: Hints from
    <i>Gaia</i> EDR3.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol.
    520, no. 1, Oxford University Press, 2023, pp. 364–74, doi:<a href="https://doi.org/10.1093/mnras/stad068">10.1093/mnras/stad068</a>.'
  short: L. Fleury, I. Caiazzo, J. Heyl, Monthly Notices of the Royal Astronomical
    Society 520 (2023) 364–374.
date_created: 2024-03-26T09:48:27Z
date_published: 2023-01-12T00:00:00Z
date_updated: 2024-04-02T07:13:10Z
day: '12'
doi: 10.1093/mnras/stad068
extern: '1'
external_id:
  arxiv:
  - '2205.01015'
intvolume: '       520'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2205.01015
month: '01'
oa: 1
oa_version: Preprint
page: 364-374
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: 'The origin of ultramassive white dwarfs: hints from <i>Gaia</i> EDR3'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 520
year: '2023'
...
---
_id: '15200'
abstract:
- lang: eng
  text: Magnetic cataclysmic variables (CVs) are luminous Galactic X-ray sources,
    which have been difficult to find in purely optical surveys due to their lack
    of outburst behavior. The eROSITA telescope on board the Spektr-RG mission is
    conducting an all-sky X-ray survey and recently released the public eROSITA Final
    Equatorial Depth Survey (eFEDS) catalog. We crossmatched the eFEDS catalog with
    photometry from the Zwicky Transient Facility and discovered two new magnetic
    CVs. We obtained high-cadence optical photometry and phase-resolved spectroscopy
    for each magnetic CV candidate and found them both to be polars. Among the newly
    discovered magnetic CVs is eFEDS J085037.2+044359/ZTFJ0850+0443, an eclipsing
    polar with orbital period Porb = 1.72 hr and WD mass MWD = 0.81 ± 0.08M⊙. We suggest
    that eFEDS J085037.2+044359/ZTFJ0850+0443 is a low magnetic field strength polar,
    with BWD ≲ 10 MG. We also discovered a non-eclipsing polar, eFEDS J092614.1+010558/ZTFJ0926+0105,
    with orbital period Porb = 1.47 hr and magnetic field strength BWD = 36–42 MG.
article_number: '141'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- 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: Thomas A.
  full_name: Prince, Thomas A.
  last_name: Prince
- first_name: Paula
  full_name: Szkody, Paula
  last_name: Szkody
- first_name: Kevin B.
  full_name: Burdge, Kevin B.
  last_name: Burdge
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Jan
  full_name: van Roestel, Jan
  last_name: van Roestel
- first_name: Zachary P.
  full_name: Vanderbosch, Zachary P.
  last_name: Vanderbosch
- first_name: Kareem
  full_name: El-Badry, Kareem
  last_name: El-Badry
- first_name: Eric C.
  full_name: Bellm, Eric C.
  last_name: Bellm
- first_name: Boris T.
  full_name: Gänsicke, Boris T.
  last_name: Gänsicke
- first_name: Matthew J.
  full_name: Graham, Matthew J.
  last_name: Graham
- first_name: Ashish A.
  full_name: Mahabal, Ashish A.
  last_name: Mahabal
- first_name: Frank J.
  full_name: Masci, Frank J.
  last_name: Masci
- first_name: Przemek
  full_name: Mróz, Przemek
  last_name: Mróz
- first_name: Reed
  full_name: Riddle, Reed
  last_name: Riddle
- first_name: Ben
  full_name: Rusholme, Ben
  last_name: Rusholme
citation:
  ama: Rodriguez AC, Kulkarni SR, Prince TA, et al. Discovery of two polars from a
    crossmatch of ZTF and the SRG/eFEDS x-ray catalog. <i>The Astrophysical Journal</i>.
    2023;945(2). doi:<a href="https://doi.org/10.3847/1538-4357/acbb6f">10.3847/1538-4357/acbb6f</a>
  apa: Rodriguez, A. C., Kulkarni, S. R., Prince, T. A., Szkody, P., Burdge, K. B.,
    Caiazzo, I., … Rusholme, B. (2023). Discovery of two polars from a crossmatch
    of ZTF and the SRG/eFEDS x-ray catalog. <i>The Astrophysical Journal</i>. American
    Astronomical Society. <a href="https://doi.org/10.3847/1538-4357/acbb6f">https://doi.org/10.3847/1538-4357/acbb6f</a>
  chicago: Rodriguez, Antonio C., Shrinivas R. Kulkarni, Thomas A. Prince, Paula Szkody,
    Kevin B. Burdge, Ilaria Caiazzo, Jan van Roestel, et al. “Discovery of Two Polars
    from a Crossmatch of ZTF and the SRG/EFEDS x-Ray Catalog.” <i>The Astrophysical
    Journal</i>. American Astronomical Society, 2023. <a href="https://doi.org/10.3847/1538-4357/acbb6f">https://doi.org/10.3847/1538-4357/acbb6f</a>.
  ieee: A. C. Rodriguez <i>et al.</i>, “Discovery of two polars from a crossmatch
    of ZTF and the SRG/eFEDS x-ray catalog,” <i>The Astrophysical Journal</i>, vol.
    945, no. 2. American Astronomical Society, 2023.
  ista: Rodriguez AC, Kulkarni SR, Prince TA, Szkody P, Burdge KB, Caiazzo I, van
    Roestel J, Vanderbosch ZP, El-Badry K, Bellm EC, Gänsicke BT, Graham MJ, Mahabal
    AA, Masci FJ, Mróz P, Riddle R, Rusholme B. 2023. Discovery of two polars from
    a crossmatch of ZTF and the SRG/eFEDS x-ray catalog. The Astrophysical Journal.
    945(2), 141.
  mla: Rodriguez, Antonio C., et al. “Discovery of Two Polars from a Crossmatch of
    ZTF and the SRG/EFEDS x-Ray Catalog.” <i>The Astrophysical Journal</i>, vol. 945,
    no. 2, 141, American Astronomical Society, 2023, doi:<a href="https://doi.org/10.3847/1538-4357/acbb6f">10.3847/1538-4357/acbb6f</a>.
  short: A.C. Rodriguez, S.R. Kulkarni, T.A. Prince, P. Szkody, K.B. Burdge, I. Caiazzo,
    J. van Roestel, Z.P. Vanderbosch, K. El-Badry, E.C. Bellm, B.T. Gänsicke, M.J.
    Graham, A.A. Mahabal, F.J. Masci, P. Mróz, R. Riddle, B. Rusholme, The Astrophysical
    Journal 945 (2023).
date_created: 2024-03-26T09:48:51Z
date_published: 2023-03-15T00:00:00Z
date_updated: 2024-04-02T07:13:55Z
day: '15'
doi: 10.3847/1538-4357/acbb6f
extern: '1'
external_id:
  arxiv:
  - '2206.04714'
intvolume: '       945'
issue: '2'
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/acbb6f
month: '03'
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: Discovery of two polars from a crossmatch of ZTF and the SRG/eFEDS x-ray catalog
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: 945
year: '2023'
...
---
_id: '15201'
abstract:
- lang: eng
  text: "We present a systematic study of the unbinned, photon-by-photon likelihood
    technique which can be used as an alternative method to analyse phase-dependent,
    X-ray spectro-polarimetric observations obtained with IXPE and other photoelectric
    polarimeters. We apply the unbinned technique to models of the luminous X-ray
    pulsar Hercules X-1, for which we produce simulated observations using the IXPEOBSSIM
    package. We consider minimal knowledge about the actual physical process responsible
    for the polarized emission from the accreting pulsar and assume that the observed
    phase-dependent polarization angle can be described by the rotating vector model.
    Using the unbinned technique, the detector’s modulation factor, and the polarization
    information alone, we found that both the rotating vector model and the underlying
    spectro-polarimetry model can reconstruct equally well the geometric configuration
    angles of the accreting pulsar. However, the measured polarization fraction becomes
    biased with respect to the underlying model unless the energy dispersion and effective
    area of the detector are also taken into account. To this end, we present an energy-dispersed
    likelihood estimator that is proved to be unbiased. For different analyses, we
    obtain posterior distributions from multiple IXPEOBSSIM realizations and show
    that the unbinned technique yields \r\n smaller error bars than the binned technique.
    We also discuss alternative sources, such as magnetars, in which the unbinned
    technique and the rotating vector model might be applied."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Denis
  full_name: González-Caniulef, Denis
  last_name: González-Caniulef
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
citation:
  ama: González-Caniulef D, Caiazzo I, Heyl J. Unbinned likelihood analysis for X-ray
    polarization. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;519(4):5902-5912.
    doi:<a href="https://doi.org/10.1093/mnras/stad033">10.1093/mnras/stad033</a>
  apa: González-Caniulef, D., Caiazzo, I., &#38; Heyl, J. (2023). Unbinned likelihood
    analysis for X-ray polarization. <i>Monthly Notices of the Royal Astronomical
    Society</i>. Oxford University Press. <a href="https://doi.org/10.1093/mnras/stad033">https://doi.org/10.1093/mnras/stad033</a>
  chicago: González-Caniulef, Denis, Ilaria Caiazzo, and Jeremy Heyl. “Unbinned Likelihood
    Analysis for X-Ray Polarization.” <i>Monthly Notices of the Royal Astronomical
    Society</i>. Oxford University Press, 2023. <a href="https://doi.org/10.1093/mnras/stad033">https://doi.org/10.1093/mnras/stad033</a>.
  ieee: D. González-Caniulef, I. Caiazzo, and J. Heyl, “Unbinned likelihood analysis
    for X-ray polarization,” <i>Monthly Notices of the Royal Astronomical Society</i>,
    vol. 519, no. 4. Oxford University Press, pp. 5902–5912, 2023.
  ista: González-Caniulef D, Caiazzo I, Heyl J. 2023. Unbinned likelihood analysis
    for X-ray polarization. Monthly Notices of the Royal Astronomical Society. 519(4),
    5902–5912.
  mla: González-Caniulef, Denis, et al. “Unbinned Likelihood Analysis for X-Ray Polarization.”
    <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 519, no. 4, Oxford
    University Press, 2023, pp. 5902–12, doi:<a href="https://doi.org/10.1093/mnras/stad033">10.1093/mnras/stad033</a>.
  short: D. González-Caniulef, I. Caiazzo, J. Heyl, Monthly Notices of the Royal Astronomical
    Society 519 (2023) 5902–5912.
date_created: 2024-03-26T09:49:52Z
date_published: 2023-01-16T00:00:00Z
date_updated: 2024-04-02T07:14:49Z
day: '16'
doi: 10.1093/mnras/stad033
extern: '1'
external_id:
  arxiv:
  - '2204.00140'
intvolume: '       519'
issue: '4'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2204.00140
month: '01'
oa: 1
oa_version: Preprint
page: 5902-5912
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: Unbinned likelihood analysis for X-ray polarization
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 519
year: '2023'
...
---
_id: '15202'
abstract:
- lang: eng
  text: Magnetars are the most strongly magnetized neutron stars, and one of the most
    promising targets for X-ray polarimetric measurements. We present here the first
    Imaging X-ray Polarimetry Explorer observation of the magnetar 1RXS J170849.0-400910,
    jointly analyzed with a new Swift observation and archival NICER data. The total
    (energy- and phase-integrated) emission in the 2–8 keV energy range is linerarly
    polarized, at a ∼35% level. The phase-averaged polarization signal shows a marked
    increase with energy, ranging from ∼20% at 2–3 keV up to ∼80% at 6–8 keV, while
    the polarization angle remains constant. This indicates that radiation is mostly
    polarized in a single direction. The spectrum is well reproduced by a combination
    of either two thermal (blackbody) components or a blackbody and a power law. Both
    the polarization degree and angle also show a variation with the spin phase, and
    the former is almost anticorrelated with the source counts in the 2–8 and 2–4
    keV bands. We discuss the possible implications and interpretations, based on
    a joint analysis of the spectral, polarization, and pulsation properties of the
    source. A scenario in which the surface temperature is not homogeneous, with a
    hotter cap covered by a gaseous atmosphere and a warmer region in a condensed
    state, provides a satisfactory description of both the phase- and energy-dependent
    spectro-polarimetric data. The (comparatively) small size of the two emitting
    regions, required to explain the observed pulsations, does not allow to reach
    a robust conclusion about the presence of vacuum birefringence effects.
article_number: L27
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Silvia
  full_name: Zane, Silvia
  last_name: Zane
- first_name: Roberto
  full_name: Taverna, Roberto
  last_name: Taverna
- first_name: Denis
  full_name: González–Caniulef, Denis
  last_name: González–Caniulef
- first_name: Fabio
  full_name: Muleri, Fabio
  last_name: Muleri
- first_name: Roberto
  full_name: Turolla, Roberto
  last_name: Turolla
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
- first_name: Keisuke
  full_name: Uchiyama, Keisuke
  last_name: Uchiyama
- first_name: Mason
  full_name: Ng, Mason
  last_name: Ng
- first_name: Toru
  full_name: Tamagawa, Toru
  last_name: Tamagawa
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Niccolò
  full_name: Di Lalla, Niccolò
  last_name: Di Lalla
- first_name: Herman L.
  full_name: Marshall, Herman L.
  last_name: Marshall
- first_name: Matteo
  full_name: Bachetti, Matteo
  last_name: Bachetti
- first_name: Fabio
  full_name: La Monaca, Fabio
  last_name: La Monaca
- first_name: Ephraim
  full_name: Gau, Ephraim
  last_name: Gau
- first_name: Alessandro
  full_name: Di Marco, Alessandro
  last_name: Di Marco
- first_name: Luca
  full_name: Baldini, Luca
  last_name: Baldini
- first_name: Michela
  full_name: Negro, Michela
  last_name: Negro
- first_name: Nicola
  full_name: Omodei, Nicola
  last_name: Omodei
- first_name: John
  full_name: Rankin, John
  last_name: Rankin
- first_name: Giorgio
  full_name: Matt, Giorgio
  last_name: Matt
- first_name: George G.
  full_name: Pavlov, George G.
  last_name: Pavlov
- first_name: Takao
  full_name: Kitaguchi, Takao
  last_name: Kitaguchi
- first_name: Henric
  full_name: Krawczynski, Henric
  last_name: Krawczynski
- first_name: Fabian
  full_name: Kislat, Fabian
  last_name: Kislat
- first_name: Ruth
  full_name: Kelly, Ruth
  last_name: Kelly
- first_name: Iván
  full_name: Agudo, Iván
  last_name: Agudo
- first_name: Lucio A.
  full_name: Antonelli, Lucio A.
  last_name: Antonelli
- first_name: Wayne H.
  full_name: Baumgartner, Wayne H.
  last_name: Baumgartner
- first_name: Ronaldo
  full_name: Bellazzini, Ronaldo
  last_name: Bellazzini
- first_name: Stefano
  full_name: Bianchi, Stefano
  last_name: Bianchi
- first_name: Stephen D.
  full_name: Bongiorno, Stephen D.
  last_name: Bongiorno
- first_name: Raffaella
  full_name: Bonino, Raffaella
  last_name: Bonino
- first_name: Alessandro
  full_name: Brez, Alessandro
  last_name: Brez
- first_name: Niccolò
  full_name: Bucciantini, Niccolò
  last_name: Bucciantini
- first_name: Fiamma
  full_name: Capitanio, Fiamma
  last_name: Capitanio
- first_name: Simone
  full_name: Castellano, Simone
  last_name: Castellano
- first_name: Elisabetta
  full_name: Cavazzuti, Elisabetta
  last_name: Cavazzuti
- first_name: Chieng-Ting
  full_name: Chen, Chieng-Ting
  last_name: Chen
- first_name: Stefano
  full_name: Ciprini, Stefano
  last_name: Ciprini
- first_name: Enrico
  full_name: Costa, Enrico
  last_name: Costa
- first_name: Alessandra
  full_name: De Rosa, Alessandra
  last_name: De Rosa
- first_name: Ettore
  full_name: Del Monte, Ettore
  last_name: Del Monte
- first_name: Laura
  full_name: Di Gesu, Laura
  last_name: Di Gesu
- first_name: Immacolata
  full_name: Donnarumma, Immacolata
  last_name: Donnarumma
- first_name: Victor
  full_name: Doroshenko, Victor
  last_name: Doroshenko
- first_name: Michal
  full_name: Dovčiak, Michal
  last_name: Dovčiak
- first_name: Steven R.
  full_name: Ehlert, Steven R.
  last_name: Ehlert
- first_name: Teruaki
  full_name: Enoto, Teruaki
  last_name: Enoto
- first_name: Yuri
  full_name: Evangelista, Yuri
  last_name: Evangelista
- first_name: Sergio
  full_name: Fabiani, Sergio
  last_name: Fabiani
- first_name: Riccardo
  full_name: Ferrazzoli, Riccardo
  last_name: Ferrazzoli
- first_name: Javier A.
  full_name: Garcia, Javier A.
  last_name: Garcia
- first_name: Shuichi
  full_name: Gunji, Shuichi
  last_name: Gunji
- first_name: Kiyoshi
  full_name: Hayashida, Kiyoshi
  last_name: Hayashida
- first_name: Wataru
  full_name: Iwakiri, Wataru
  last_name: Iwakiri
- first_name: Svetlana G.
  full_name: Jorstad, Svetlana G.
  last_name: Jorstad
- first_name: Philip
  full_name: Kaaret, Philip
  last_name: Kaaret
- first_name: Vladimir
  full_name: Karas, Vladimir
  last_name: Karas
- first_name: Jeffery J.
  full_name: Kolodziejczak, Jeffery J.
  last_name: Kolodziejczak
- first_name: Luca
  full_name: Latronico, Luca
  last_name: Latronico
- first_name: Ioannis
  full_name: Liodakis, Ioannis
  last_name: Liodakis
- first_name: Simone
  full_name: Maldera, Simone
  last_name: Maldera
- first_name: Alberto
  full_name: Manfreda, Alberto
  last_name: Manfreda
- first_name: Frédéric
  full_name: Marin, Frédéric
  last_name: Marin
- first_name: Andrea
  full_name: Marinucci, Andrea
  last_name: Marinucci
- first_name: Alan P.
  full_name: Marscher, Alan P.
  last_name: Marscher
- first_name: Francesco
  full_name: Massaro, Francesco
  last_name: Massaro
- first_name: Ikuyuki
  full_name: Mitsuishi, Ikuyuki
  last_name: Mitsuishi
- first_name: Tsunefumi
  full_name: Mizuno, Tsunefumi
  last_name: Mizuno
- first_name: C.-Y.
  full_name: Ng, C.-Y.
  last_name: Ng
- first_name: Stephen L.
  full_name: O’Dell, Stephen L.
  last_name: O’Dell
- first_name: Chiara
  full_name: Oppedisano, Chiara
  last_name: Oppedisano
- first_name: Alessandro
  full_name: Papitto, Alessandro
  last_name: Papitto
- first_name: Abel L.
  full_name: Peirson, Abel L.
  last_name: Peirson
- first_name: Matteo
  full_name: Perri, Matteo
  last_name: Perri
- first_name: Melissa
  full_name: Pesce-Rollins, Melissa
  last_name: Pesce-Rollins
- first_name: Pierre-Olivier
  full_name: Petrucci, Pierre-Olivier
  last_name: Petrucci
- first_name: Maura
  full_name: Pilia, Maura
  last_name: Pilia
- first_name: Andrea
  full_name: Possenti, Andrea
  last_name: Possenti
- first_name: Juri
  full_name: Poutanen, Juri
  last_name: Poutanen
- first_name: Simonetta
  full_name: Puccetti, Simonetta
  last_name: Puccetti
- first_name: Brian D.
  full_name: Ramsey, Brian D.
  last_name: Ramsey
- first_name: Ajay
  full_name: Ratheesh, Ajay
  last_name: Ratheesh
- first_name: Oliver J.
  full_name: Roberts, Oliver J.
  last_name: Roberts
- first_name: Roger W.
  full_name: Romani, Roger W.
  last_name: Romani
- first_name: Carmelo
  full_name: Sgró, Carmelo
  last_name: Sgró
- first_name: Patrick
  full_name: Slane, Patrick
  last_name: Slane
- first_name: Paolo
  full_name: Soffitta, Paolo
  last_name: Soffitta
- first_name: Gloria
  full_name: Spandre, Gloria
  last_name: Spandre
- first_name: Douglas A.
  full_name: Swartz, Douglas A.
  last_name: Swartz
- first_name: Fabrizio
  full_name: Tavecchio, Fabrizio
  last_name: Tavecchio
- first_name: Yuzuru
  full_name: Tawara, Yuzuru
  last_name: Tawara
- first_name: Allyn F.
  full_name: Tennant, Allyn F.
  last_name: Tennant
- first_name: Nicholas E.
  full_name: Thomas, Nicholas E.
  last_name: Thomas
- first_name: Francesco
  full_name: Tombesi, Francesco
  last_name: Tombesi
- first_name: Alessio
  full_name: Trois, Alessio
  last_name: Trois
- first_name: Sergey S.
  full_name: Tsygankov, Sergey S.
  last_name: Tsygankov
- first_name: Jacco
  full_name: Vink, Jacco
  last_name: Vink
- first_name: Martin C.
  full_name: Weisskopf, Martin C.
  last_name: Weisskopf
- first_name: Kinwah
  full_name: Wu, Kinwah
  last_name: Wu
- first_name: Fei
  full_name: Xie, Fei
  last_name: Xie
citation:
  ama: Zane S, Taverna R, González–Caniulef D, et al. A strong x-ray polarization
    signal from the magnetar 1RXS J170849.0-400910. <i>The Astrophysical Journal Letters</i>.
    2023;944(2). doi:<a href="https://doi.org/10.3847/2041-8213/acb703">10.3847/2041-8213/acb703</a>
  apa: Zane, S., Taverna, R., González–Caniulef, D., Muleri, F., Turolla, R., Heyl,
    J., … Xie, F. (2023). A strong x-ray polarization signal from the magnetar 1RXS
    J170849.0-400910. <i>The Astrophysical Journal Letters</i>. American Astronomical
    Society. <a href="https://doi.org/10.3847/2041-8213/acb703">https://doi.org/10.3847/2041-8213/acb703</a>
  chicago: Zane, Silvia, Roberto Taverna, Denis González–Caniulef, Fabio Muleri, Roberto
    Turolla, Jeremy Heyl, Keisuke Uchiyama, et al. “A Strong X-Ray Polarization Signal
    from the Magnetar 1RXS J170849.0-400910.” <i>The Astrophysical Journal Letters</i>.
    American Astronomical Society, 2023. <a href="https://doi.org/10.3847/2041-8213/acb703">https://doi.org/10.3847/2041-8213/acb703</a>.
  ieee: S. Zane <i>et al.</i>, “A strong x-ray polarization signal from the magnetar
    1RXS J170849.0-400910,” <i>The Astrophysical Journal Letters</i>, vol. 944, no.
    2. American Astronomical Society, 2023.
  ista: Zane S et al. 2023. A strong x-ray polarization signal from the magnetar 1RXS
    J170849.0-400910. The Astrophysical Journal Letters. 944(2), L27.
  mla: Zane, Silvia, et al. “A Strong X-Ray Polarization Signal from the Magnetar
    1RXS J170849.0-400910.” <i>The Astrophysical Journal Letters</i>, vol. 944, no.
    2, L27, American Astronomical Society, 2023, doi:<a href="https://doi.org/10.3847/2041-8213/acb703">10.3847/2041-8213/acb703</a>.
  short: S. Zane, R. Taverna, D. González–Caniulef, F. Muleri, R. Turolla, J. Heyl,
    K. Uchiyama, M. Ng, T. Tamagawa, I. Caiazzo, N. Di Lalla, H.L. Marshall, M. Bachetti,
    F. La Monaca, E. Gau, A. Di Marco, L. Baldini, M. Negro, N. Omodei, J. Rankin,
    G. Matt, G.G. Pavlov, T. Kitaguchi, H. Krawczynski, F. Kislat, R. Kelly, I. Agudo,
    L.A. Antonelli, W.H. Baumgartner, R. Bellazzini, S. Bianchi, S.D. Bongiorno, R.
    Bonino, A. Brez, N. Bucciantini, F. Capitanio, S. Castellano, E. Cavazzuti, C.-T.
    Chen, S. Ciprini, E. Costa, A. De Rosa, E. Del Monte, L. Di Gesu, I. Donnarumma,
    V. Doroshenko, M. Dovčiak, S.R. Ehlert, T. Enoto, Y. Evangelista, S. Fabiani,
    R. Ferrazzoli, J.A. Garcia, S. Gunji, K. Hayashida, W. Iwakiri, S.G. Jorstad,
    P. Kaaret, V. Karas, J.J. Kolodziejczak, L. Latronico, I. Liodakis, S. Maldera,
    A. Manfreda, F. Marin, A. Marinucci, A.P. Marscher, F. Massaro, I. Mitsuishi,
    T. Mizuno, C.-Y. Ng, S.L. O’Dell, C. Oppedisano, A. Papitto, A.L. Peirson, M.
    Perri, M. Pesce-Rollins, P.-O. Petrucci, M. Pilia, A. Possenti, J. Poutanen, S.
    Puccetti, B.D. Ramsey, A. Ratheesh, O.J. Roberts, R.W. Romani, C. Sgró, P. Slane,
    P. Soffitta, G. Spandre, D.A. Swartz, F. Tavecchio, Y. Tawara, A.F. Tennant, N.E.
    Thomas, F. Tombesi, A. Trois, S.S. Tsygankov, J. Vink, M.C. Weisskopf, K. Wu,
    F. Xie, The Astrophysical Journal Letters 944 (2023).
date_created: 2024-03-26T09:50:12Z
date_published: 2023-02-15T00:00:00Z
date_updated: 2024-04-02T07:15:41Z
day: '15'
doi: 10.3847/2041-8213/acb703
extern: '1'
external_id:
  arxiv:
  - '2301.12919'
intvolume: '       944'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.3847/2041-8213/acb703
month: '02'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal Letters
publication_identifier:
  eissn:
  - 2041-8213
  issn:
  - 2041-8205
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: A strong x-ray polarization signal from the magnetar 1RXS J170849.0-400910
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: 944
year: '2023'
...
---
_id: '15225'
abstract:
- lang: eng
  text: We argue that measurements of X-ray polarization using the recently launched
    Imaging X-ray Polarimetry Explorer will answer many open questions about magnetars
    in particular the physical state of their surfaces, whether vacuum birefringence
    exists, and the nature of the hard X-ray emission from these objects. We outline
    the capabilities of the instrument, specific models and the results of simulations
    for the magnetar 4U 0142+61.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Denis
  full_name: González-Caniulef, Denis
  last_name: González-Caniulef
citation:
  ama: Heyl J, Caiazzo I, González-Caniulef D. X-ray polarization at the crossroads.
    <i>Proceedings of the International Astronomical Union</i>. 2023;16(S363):80-91.
    doi:<a href="https://doi.org/10.1017/s1743921322000916">10.1017/s1743921322000916</a>
  apa: Heyl, J., Caiazzo, I., &#38; González-Caniulef, D. (2023). X-ray polarization
    at the crossroads. <i>Proceedings of the International Astronomical Union</i>.
    Cambridge University Press. <a href="https://doi.org/10.1017/s1743921322000916">https://doi.org/10.1017/s1743921322000916</a>
  chicago: Heyl, Jeremy, Ilaria Caiazzo, and Denis González-Caniulef. “X-Ray Polarization
    at the Crossroads.” <i>Proceedings of the International Astronomical Union</i>.
    Cambridge University Press, 2023. <a href="https://doi.org/10.1017/s1743921322000916">https://doi.org/10.1017/s1743921322000916</a>.
  ieee: J. Heyl, I. Caiazzo, and D. González-Caniulef, “X-ray polarization at the
    crossroads,” <i>Proceedings of the International Astronomical Union</i>, vol.
    16, no. S363. Cambridge University Press, pp. 80–91, 2023.
  ista: Heyl J, Caiazzo I, González-Caniulef D. 2023. X-ray polarization at the crossroads.
    Proceedings of the International Astronomical Union. 16(S363), 80–91.
  mla: Heyl, Jeremy, et al. “X-Ray Polarization at the Crossroads.” <i>Proceedings
    of the International Astronomical Union</i>, vol. 16, no. S363, Cambridge University
    Press, 2023, pp. 80–91, doi:<a href="https://doi.org/10.1017/s1743921322000916">10.1017/s1743921322000916</a>.
  short: J. Heyl, I. Caiazzo, D. González-Caniulef, Proceedings of the International
    Astronomical Union 16 (2023) 80–91.
date_created: 2024-03-26T10:35:20Z
date_published: 2023-02-27T00:00:00Z
date_updated: 2024-04-04T09:46:17Z
day: '27'
doi: 10.1017/s1743921322000916
extern: '1'
external_id:
  arxiv:
  - '2203.09066'
intvolume: '        16'
issue: S363
keyword:
- Astronomy and Astrophysics
- Space and Planetary Science
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1017/S1743921322000916
month: '02'
oa: 1
oa_version: Published Version
page: 80-91
publication: Proceedings of the International Astronomical Union
publication_identifier:
  eissn:
  - 1743-9221
  issn:
  - 1743-9213
publication_status: published
publisher: Cambridge University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: X-ray polarization at the crossroads
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: 8b945eb4-e2f2-11eb-945a-df72226e66a9
volume: 16
year: '2023'
...
---
_id: '15226'
abstract:
- lang: eng
  text: "Due to the rich phenomenology and extreme magnetic conditions, magnetars
    will be targets of great interest for the upcoming polarimetry space missions.
    In particular, the Imaging X-ray Polarimetry Explorer (IXPE), recently launched
    in December 2021, will operate in the 2–8 keV range. This will open a new window
    to study the polarized, persistent X-ray emission from magnetars. In this talk,
    I will present simulations of IXPE observations of magnetars using the IXPEObsSim
    package. I will discuss future prospect to discriminate between different magnetar’s
    emission mechanisms, as well as a potential detection of the signal of vacuum
    birefringence using IXPE.\r\n\r\n"
article_processing_charge: No
article_type: original
author:
- first_name: Denis
  full_name: González-Caniulef, Denis
  last_name: González-Caniulef
- first_name: Ilaria
  full_name: Caiazzo, Ilaria
  id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d
  last_name: Caiazzo
  orcid: 0000-0002-4770-5388
- first_name: Jeremy
  full_name: Heyl, Jeremy
  last_name: Heyl
citation:
  ama: González-Caniulef D, Caiazzo I, Heyl J. IXPE simulations for magnetars. <i>Proceedings
    of the International Astronomical Union</i>. 2023;16(S363):314-317. doi:<a href="https://doi.org/10.1017/s1743921322000679">10.1017/s1743921322000679</a>
  apa: González-Caniulef, D., Caiazzo, I., &#38; Heyl, J. (2023). IXPE simulations
    for magnetars. <i>Proceedings of the International Astronomical Union</i>. Cambridge
    University Press. <a href="https://doi.org/10.1017/s1743921322000679">https://doi.org/10.1017/s1743921322000679</a>
  chicago: González-Caniulef, Denis, Ilaria Caiazzo, and Jeremy Heyl. “IXPE Simulations
    for Magnetars.” <i>Proceedings of the International Astronomical Union</i>. Cambridge
    University Press, 2023. <a href="https://doi.org/10.1017/s1743921322000679">https://doi.org/10.1017/s1743921322000679</a>.
  ieee: D. González-Caniulef, I. Caiazzo, and J. Heyl, “IXPE simulations for magnetars,”
    <i>Proceedings of the International Astronomical Union</i>, vol. 16, no. S363.
    Cambridge University Press, pp. 314–317, 2023.
  ista: González-Caniulef D, Caiazzo I, Heyl J. 2023. IXPE simulations for magnetars.
    Proceedings of the International Astronomical Union. 16(S363), 314–317.
  mla: González-Caniulef, Denis, et al. “IXPE Simulations for Magnetars.” <i>Proceedings
    of the International Astronomical Union</i>, vol. 16, no. S363, Cambridge University
    Press, 2023, pp. 314–17, doi:<a href="https://doi.org/10.1017/s1743921322000679">10.1017/s1743921322000679</a>.
  short: D. González-Caniulef, I. Caiazzo, J. Heyl, Proceedings of the International
    Astronomical Union 16 (2023) 314–317.
date_created: 2024-03-26T10:35:43Z
date_published: 2023-02-27T00:00:00Z
date_updated: 2024-04-04T12:54:59Z
day: '27'
doi: 10.1017/s1743921322000679
extern: '1'
intvolume: '        16'
issue: S363
keyword:
- Astronomy and Astrophysics
- Space and Planetary Science
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1017/S1743921322000679
month: '02'
oa: 1
oa_version: Published Version
page: 314-317
publication: Proceedings of the International Astronomical Union
publication_identifier:
  eissn:
  - 1743-9221
  issn:
  - 1743-9213
publication_status: published
publisher: Cambridge University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: IXPE simulations for magnetars
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: 8b945eb4-e2f2-11eb-945a-df72226e66a9
volume: 16
year: '2023'
...
---
_id: '15292'
abstract:
- lang: eng
  text: We present a rigid body animation technique which prevents solids from interpenetrating,
    dissipates energy through friction, and propagates shocks through contacts. We
    employ the Alternating Direction Method of Multipliers (ADMM) to couple non-smooth
    Coulomb friction with impact propagation, allowing efficient and accurate non-smooth
    dynamics along with a correct transmission of impacts through assemblies of rigid
    bodies. We further extend our method to model adhesion, dynamic friction and lubricated
    contact.
acknowledgement: We thank the anonymous reviewers and the members of the Visual Computing
  Group at ISTA for their helpful comments. This research was supported by the Scientific
  Service Units (SSU) of ISTA through resources provided by Scientific Computing,
  and was funded in part by the European Union (ERC-2021-COG 101045083 CoDiNA)
article_processing_charge: No
author:
- first_name: Yi-Lu
  full_name: Chen, Yi-Lu
  id: 0b467602-dbcd-11ea-9d1d-ed480aa46b70
  last_name: Chen
- first_name: Mickaël
  full_name: Ly, Mickaël
  id: 6340d7f0-b48d-11eb-b10d-b7487e71d9f1
  last_name: Ly
- first_name: Christopher J
  full_name: Wojtan, Christopher J
  id: 3C61F1D2-F248-11E8-B48F-1D18A9856A87
  last_name: Wojtan
  orcid: 0000-0001-6646-5546
citation:
  ama: Chen Y-L, Ly M, Wojtan C. <i>Unified Treatment of Contact, Friction and Shock-Propagation
    in Rigid Body Animation</i>. ACM; 2023. doi:<a href="https://doi.org/10.1145/3606037.3606836">10.1145/3606037.3606836</a>
  apa: 'Chen, Y.-L., Ly, M., &#38; Wojtan, C. (2023). <i>Unified treatment of contact,
    friction and shock-propagation in rigid body animation</i>. <i>Proceedings of
    the ACM SIGGRAPH/Eurographics Symposium on Computer Animation</i>. Los Angeles,
    CA, United States: ACM. <a href="https://doi.org/10.1145/3606037.3606836">https://doi.org/10.1145/3606037.3606836</a>'
  chicago: Chen, Yi-Lu, Mickaël Ly, and Chris Wojtan. <i>Unified Treatment of Contact,
    Friction and Shock-Propagation in Rigid Body Animation</i>. <i>Proceedings of
    the ACM SIGGRAPH/Eurographics Symposium on Computer Animation</i>. ACM, 2023.
    <a href="https://doi.org/10.1145/3606037.3606836">https://doi.org/10.1145/3606037.3606836</a>.
  ieee: Y.-L. Chen, M. Ly, and C. Wojtan, <i>Unified treatment of contact, friction
    and shock-propagation in rigid body animation</i>. ACM, 2023.
  ista: Chen Y-L, Ly M, Wojtan C. 2023. Unified treatment of contact, friction and
    shock-propagation in rigid body animation, ACM,p.
  mla: Chen, Yi-Lu, et al. “Unified Treatment of Contact, Friction and Shock-Propagation
    in Rigid Body Animation.” <i>Proceedings of the ACM SIGGRAPH/Eurographics Symposium
    on Computer Animation</i>, ACM, 2023, doi:<a href="https://doi.org/10.1145/3606037.3606836">10.1145/3606037.3606836</a>.
  short: Y.-L. Chen, M. Ly, C. Wojtan, Unified Treatment of Contact, Friction and
    Shock-Propagation in Rigid Body Animation, ACM, 2023.
conference:
  end_date: 2023-08-06
  location: Los Angeles, CA, United States
  name: 'SCA: Symposium on Computer Animation'
  start_date: 2023-08-04
corr_author: '1'
date_created: 2024-04-03T14:57:23Z
date_published: 2023-08-01T00:00:00Z
date_updated: 2025-04-14T12:58:27Z
day: '01'
ddc:
- '005'
- '531'
department:
- _id: GradSch
- _id: ChWo
doi: 10.1145/3606037.3606836
file:
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  date_created: 2024-04-03T14:58:23Z
  date_updated: 2024-04-03T14:58:23Z
  file_id: '15294'
  file_name: frictionPoster_clean.pdf
  file_size: 3951968
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file_date_updated: 2024-04-03T14:58:24Z
has_accepted_license: '1'
language:
- iso: eng
month: '08'
oa: 1
oa_version: None
project:
- _id: 34bc2376-11ca-11ed-8bc3-9a3b3961a088
  grant_number: '101045083'
  name: Computational Discovery of Numerical Algorithms for Animation and Simulation
    of Natural Phenomena
publication: Proceedings of the ACM SIGGRAPH/Eurographics Symposium on Computer Animation
publication_status: published
publisher: ACM
related_material:
  record:
  - id: '14748'
    relation: other
    status: public
status: public
title: Unified treatment of contact, friction and shock-propagation in rigid body
  animation
type: conference_poster
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2023'
...
---
_id: '17074'
abstract:
- lang: eng
  text: We verify Bogoliubov's approximation for translation invariant Bose gases
    in the mean field regime, i.e. we prove that the ground state energy EN is given
    by EN=NeH+infσ(H)+oN→∞(1), where N is the number of particles, eH is the minimal
    Hartree energy and H is the Bogoliubov Hamiltonian. As an intermediate result
    we show the existence of approximate ground states ΨN, i.e. states satisfying
    ⟨HN⟩ΨN=EN+oN→∞(1), exhibiting complete Bose--Einstein condensation with respect
    to one of the Hartree minimizers.
acknowledgement: "We are grateful to Rupert Frank for helpful discussions at an early
  stage of this project.\r\nFunding from the European Union’s Horizon 2020 research
  and innovation programme\r\nunder the ERC grant agreement No 694227 is acknowledged."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Morris
  full_name: Brooks, Morris
  id: B7ECF9FC-AA38-11E9-AC9A-0930E6697425
  last_name: Brooks
  orcid: 0000-0002-6249-0928
- first_name: Robert
  full_name: Seiringer, Robert
  id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
  last_name: Seiringer
  orcid: 0000-0002-6781-0521
citation:
  ama: Brooks M, Seiringer R. Validity of Bogoliubov’s approximation fortranslation-invariant
    Bose gases. <i>Probability and Mathematical Physics</i>. 2023;3(4):939-1000. doi:<a
    href="https://doi.org/10.2140/pmp.2022.3.939">10.2140/pmp.2022.3.939</a>
  apa: Brooks, M., &#38; Seiringer, R. (2023). Validity of Bogoliubov’s approximation
    fortranslation-invariant Bose gases. <i>Probability and Mathematical Physics</i>.
    Mathematical Sciences Publishers. <a href="https://doi.org/10.2140/pmp.2022.3.939">https://doi.org/10.2140/pmp.2022.3.939</a>
  chicago: Brooks, Morris, and Robert Seiringer. “Validity of Bogoliubov’s Approximation
    Fortranslation-Invariant Bose Gases.” <i>Probability and Mathematical Physics</i>.
    Mathematical Sciences Publishers, 2023. <a href="https://doi.org/10.2140/pmp.2022.3.939">https://doi.org/10.2140/pmp.2022.3.939</a>.
  ieee: M. Brooks and R. Seiringer, “Validity of Bogoliubov’s approximation fortranslation-invariant
    Bose gases,” <i>Probability and Mathematical Physics</i>, vol. 3, no. 4. Mathematical
    Sciences Publishers, pp. 939–1000, 2023.
  ista: Brooks M, Seiringer R. 2023. Validity of Bogoliubov’s approximation fortranslation-invariant
    Bose gases. Probability and Mathematical Physics. 3(4), 939–1000.
  mla: Brooks, Morris, and Robert Seiringer. “Validity of Bogoliubov’s Approximation
    Fortranslation-Invariant Bose Gases.” <i>Probability and Mathematical Physics</i>,
    vol. 3, no. 4, Mathematical Sciences Publishers, 2023, pp. 939–1000, doi:<a href="https://doi.org/10.2140/pmp.2022.3.939">10.2140/pmp.2022.3.939</a>.
  short: M. Brooks, R. Seiringer, Probability and Mathematical Physics 3 (2023) 939–1000.
corr_author: '1'
date_created: 2024-05-29T06:12:54Z
date_published: 2023-02-21T00:00:00Z
date_updated: 2025-04-14T07:26:59Z
day: '21'
department:
- _id: RoSe
doi: 10.2140/pmp.2022.3.939
ec_funded: 1
external_id:
  arxiv:
  - '2111.13864'
intvolume: '         3'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2111.13864
month: '02'
oa: 1
oa_version: Preprint
page: 939-1000
project:
- _id: 25C6DC12-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '694227'
  name: Analysis of quantum many-body systems
publication: Probability and Mathematical Physics
publication_identifier:
  eissn:
  - 2690-1005
  issn:
  - 2690-0998
publication_status: published
publisher: Mathematical Sciences Publishers
quality_controlled: '1'
scopus_import: '1'
status: public
title: Validity of Bogoliubov’s approximation fortranslation-invariant Bose gases
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 3
year: '2023'
...
---
_id: '17078'
abstract:
- lang: eng
  text: For the emergence of life, the abiotic synthesis of RNA from its monomers
    is a central step. We found that in alkaline, drying conditions in bulk and at
    heated air‐water interfaces, 2′,3′‐cyclic nucleotides oligomerised without additional
    catalyst, forming up to 10‐mers within a day. The oligomerisation proceeded at
    a pH range of 7–12, at temperatures between 40–80 °C and was marginally enhanced
    by K<jats:sup>+</jats:sup> ions. Among the canonical ribonucleotides, cGMP oligomerised
    most efficiently. Quantification was performed using HPLC coupled to ESI‐TOF by
    fitting the isotope distribution to the mass spectra. Our study suggests a oligomerisation
    mechanism where cGMP aids the incorporation of the relatively unreactive nucleotides
    C, A and U. The 2′,3′‐cyclic ribonucleotides are byproducts of prebiotic phosphorylation,
    nucleotide syntheses and RNA hydrolysis, indicating direct recycling pathways.
    The simple reaction condition offers a plausible entry point for RNA to the evolution
    of life on early Earth.
acknowledgement: We would like to thank Ulrich Gerland, Tobias Göppel, Joachim Rosenberger
  and Bernhard Altaner for their helpful remarks and discussions; Thomas Matreux,
  Alexandra Kühnlein, Noël Yeh Martin and Maximilian Weingart for comments on the
  manuscript. The authors thank J. Kussmann (LMU Munich) for providing a development
  version of the FermiONs++ program package. Financial support was provided by the
  European Research Council (ERC Evotrap, grant no. 787356, the Simons Foundation
  (grant no. 327125), the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)
  – Project-ID 364653263 – TRR 235 (CRC 235), the Deutsche Forschungsgemeinschaft
  (DFG, German Research Foundation) under Germany's Excellence Strategy – EXC-2094
  – 390783311, and the Center for NanoScience. Open Access funding enabled and organized
  by Projekt DEAL.
article_number: e202200026
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Avinash Vicholous
  full_name: Dass, Avinash Vicholous
  last_name: Dass
- first_name: Sreekar
  full_name: Wunnava, Sreekar
  last_name: Wunnava
- first_name: Juliette
  full_name: Langlais, Juliette
  last_name: Langlais
- first_name: Beatriz
  full_name: von der Esch, Beatriz
  last_name: von der Esch
- first_name: Maik
  full_name: Krusche, Maik
  last_name: Krusche
- first_name: Lennard
  full_name: Ufer, Lennard
  last_name: Ufer
- first_name: Nico
  full_name: Chrisam, Nico
  last_name: Chrisam
- first_name: Romeo C. A.
  full_name: Dubini, Romeo C. A.
  last_name: Dubini
- first_name: Florian
  full_name: Gartner, Florian
  last_name: Gartner
- first_name: Severin
  full_name: Angerpointner, Severin
  last_name: Angerpointner
- first_name: Christina F.
  full_name: Dirscherl, Christina F.
  last_name: Dirscherl
- first_name: Petra
  full_name: Rovo, Petra
  id: c316e53f-b965-11eb-b128-bb26acc59c00
  last_name: Rovo
  orcid: 0000-0001-8729-7326
- first_name: Christof B.
  full_name: Mast, Christof B.
  last_name: Mast
- first_name: Judit E.
  full_name: Šponer, Judit E.
  last_name: Šponer
- first_name: Christian
  full_name: Ochsenfeld, Christian
  last_name: Ochsenfeld
- first_name: Erwin
  full_name: Frey, Erwin
  last_name: Frey
- first_name: Dieter
  full_name: Braun, Dieter
  last_name: Braun
citation:
  ama: Dass AV, Wunnava S, Langlais J, et al. RNA oligomerisation without added catalyst
    from 2′,3′‐cyclic nucleotides by drying at air-water interfaces. <i>ChemSystemsChem</i>.
    2023;5(1). doi:<a href="https://doi.org/10.1002/syst.202200026">10.1002/syst.202200026</a>
  apa: Dass, A. V., Wunnava, S., Langlais, J., von der Esch, B., Krusche, M., Ufer,
    L., … Braun, D. (2023). RNA oligomerisation without added catalyst from 2′,3′‐cyclic
    nucleotides by drying at air-water interfaces. <i>ChemSystemsChem</i>. Wiley.
    <a href="https://doi.org/10.1002/syst.202200026">https://doi.org/10.1002/syst.202200026</a>
  chicago: Dass, Avinash Vicholous, Sreekar Wunnava, Juliette Langlais, Beatriz von
    der Esch, Maik Krusche, Lennard Ufer, Nico Chrisam, et al. “RNA Oligomerisation
    without Added Catalyst from 2′,3′‐cyclic Nucleotides by Drying at Air-Water Interfaces.”
    <i>ChemSystemsChem</i>. Wiley, 2023. <a href="https://doi.org/10.1002/syst.202200026">https://doi.org/10.1002/syst.202200026</a>.
  ieee: A. V. Dass <i>et al.</i>, “RNA oligomerisation without added catalyst from
    2′,3′‐cyclic nucleotides by drying at air-water interfaces,” <i>ChemSystemsChem</i>,
    vol. 5, no. 1. Wiley, 2023.
  ista: Dass AV, Wunnava S, Langlais J, von der Esch B, Krusche M, Ufer L, Chrisam
    N, Dubini RCA, Gartner F, Angerpointner S, Dirscherl CF, Rovo P, Mast CB, Šponer
    JE, Ochsenfeld C, Frey E, Braun D. 2023. RNA oligomerisation without added catalyst
    from 2′,3′‐cyclic nucleotides by drying at air-water interfaces. ChemSystemsChem.
    5(1), e202200026.
  mla: Dass, Avinash Vicholous, et al. “RNA Oligomerisation without Added Catalyst
    from 2′,3′‐cyclic Nucleotides by Drying at Air-Water Interfaces.” <i>ChemSystemsChem</i>,
    vol. 5, no. 1, e202200026, Wiley, 2023, doi:<a href="https://doi.org/10.1002/syst.202200026">10.1002/syst.202200026</a>.
  short: A.V. Dass, S. Wunnava, J. Langlais, B. von der Esch, M. Krusche, L. Ufer,
    N. Chrisam, R.C.A. Dubini, F. Gartner, S. Angerpointner, C.F. Dirscherl, P. Rovo,
    C.B. Mast, J.E. Šponer, C. Ochsenfeld, E. Frey, D. Braun, ChemSystemsChem 5 (2023).
date_created: 2024-05-29T06:13:48Z
date_published: 2023-01-01T00:00:00Z
date_updated: 2025-07-10T11:51:15Z
day: '01'
ddc:
- '530'
department:
- _id: NMR
doi: 10.1002/syst.202200026
file:
- access_level: open_access
  checksum: b1e78c60e371f87bdf43970f17d1cb0b
  content_type: application/pdf
  creator: dernst
  date_created: 2024-07-31T11:20:58Z
  date_updated: 2024-07-31T11:20:58Z
  file_id: '17355'
  file_name: 2023_ChemSystemsChem_Dass.pdf
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file_date_updated: 2024-07-31T11:20:58Z
has_accepted_license: '1'
intvolume: '         5'
issue: '1'
language:
- iso: eng
month: '01'
oa: 1
oa_version: Published Version
publication: ChemSystemsChem
publication_identifier:
  issn:
  - 2570-4206
publication_status: published
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: RNA oligomerisation without added catalyst from 2′,3′‐cyclic nucleotides by
  drying at air-water interfaces
tmp:
  image: /images/cc_by_nc_nd.png
  legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
  name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
    (CC BY-NC-ND 4.0)
  short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 5
year: '2023'
...
---
_id: '17079'
abstract:
- lang: eng
  text: We study moments of characteristic polynomials of truncated Haar distributed
    matrices from the three classical compact groups O(N), U(N) and Sp(2N). For finite
    matrix size we calculate the moments in terms of hypergeometric functions of matrix
    argument and give explicit integral representations highlighting the duality between
    the moment and the matrix size as well as the duality between the orthogonal and
    symplectic cases. Asymptotic expansions in strong and weak non-unitarity regimes
    are obtained. Using the connection to matrix hypergeometric functions, we establish
    limit theorems for the log-modulus of the characteristic polynomial evaluated
    on the unit circle.
acknowledgement: N.S. gratefully acknowledges financial support of the Royal Society,
  grant URF/R1/180707. We would like to thank Emma Bailey, Yan Fyodorov and Jordan
  Stoyanov for helpful comments an an earlier version of this paper. We are grateful
  for the comments of an anonymous referee.
article_number: '2250049'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Alexander
  full_name: Serebryakov, Alexander
  last_name: Serebryakov
- first_name: Nick
  full_name: Simm, Nick
  last_name: Simm
- first_name: Guillaume
  full_name: Dubach, Guillaume
  id: D5C6A458-10C4-11EA-ABF4-A4B43DDC885E
  last_name: Dubach
  orcid: 0000-0001-6892-8137
citation:
  ama: 'Serebryakov A, Simm N, Dubach G. Characteristic polynomials of random truncations:
    Moments, duality and asymptotics. <i>Random Matrices: Theory and Applications</i>.
    2023;12(01). doi:<a href="https://doi.org/10.1142/s2010326322500496">10.1142/s2010326322500496</a>'
  apa: 'Serebryakov, A., Simm, N., &#38; Dubach, G. (2023). Characteristic polynomials
    of random truncations: Moments, duality and asymptotics. <i>Random Matrices: Theory
    and Applications</i>. World Scientific Publishing. <a href="https://doi.org/10.1142/s2010326322500496">https://doi.org/10.1142/s2010326322500496</a>'
  chicago: 'Serebryakov, Alexander, Nick Simm, and Guillaume Dubach. “Characteristic
    Polynomials of Random Truncations: Moments, Duality and Asymptotics.” <i>Random
    Matrices: Theory and Applications</i>. World Scientific Publishing, 2023. <a href="https://doi.org/10.1142/s2010326322500496">https://doi.org/10.1142/s2010326322500496</a>.'
  ieee: 'A. Serebryakov, N. Simm, and G. Dubach, “Characteristic polynomials of random
    truncations: Moments, duality and asymptotics,” <i>Random Matrices: Theory and
    Applications</i>, vol. 12, no. 01. World Scientific Publishing, 2023.'
  ista: 'Serebryakov A, Simm N, Dubach G. 2023. Characteristic polynomials of random
    truncations: Moments, duality and asymptotics. Random Matrices: Theory and Applications.
    12(01), 2250049.'
  mla: 'Serebryakov, Alexander, et al. “Characteristic Polynomials of Random Truncations:
    Moments, Duality and Asymptotics.” <i>Random Matrices: Theory and Applications</i>,
    vol. 12, no. 01, 2250049, World Scientific Publishing, 2023, doi:<a href="https://doi.org/10.1142/s2010326322500496">10.1142/s2010326322500496</a>.'
  short: 'A. Serebryakov, N. Simm, G. Dubach, Random Matrices: Theory and Applications
    12 (2023).'
date_created: 2024-05-29T06:14:26Z
date_published: 2023-01-01T00:00:00Z
date_updated: 2025-09-09T14:27:10Z
day: '01'
department:
- _id: LaEr
doi: 10.1142/s2010326322500496
external_id:
  arxiv:
  - '2109.10331'
  isi:
  - '000848874400001'
intvolume: '        12'
isi: 1
issue: '01'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2109.10331
month: '01'
oa: 1
oa_version: Preprint
publication: 'Random Matrices: Theory and Applications'
publication_identifier:
  eissn:
  - 2010-3271
  issn:
  - 2010-3263
publication_status: published
publisher: World Scientific Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Characteristic polynomials of random truncations: Moments, duality and asymptotics'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 12
year: '2023'
...
