--- _id: '15204' abstract: - lang: eng text: Using observations of X-ray pulsar Hercules X-1 by the Imaging X-ray Polarimetry Explorer we report a highly significant (>17σ) detection of the polarization signal from an accreting neutron star. The observed degree of linear polarization of ~10% is far below theoretical expectations for this object, and stays low throughout the spin cycle of the pulsar. Both the degree and angle of polarization exhibit variability with the pulse phase, allowing us to measure the pulsar spin position angle 57(2) deg and the magnetic obliquity 12(4) deg, which is an essential step towards detailed modelling of the intrinsic emission of X-ray pulsars. Combining our results with the optical polarimetric data, we find that the spin axis of the neutron star and the angular momentum of the binary orbit are misaligned by at least ~20 deg, which is a strong argument in support of the models explaining the stability of the observed superorbital variability with the precession of the neutron star. 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: Sergey S. full_name: Tsygankov, Sergey S. last_name: Tsygankov - first_name: Valery F. full_name: Suleimanov, Valery F. last_name: Suleimanov - first_name: Matteo full_name: Bachetti, Matteo last_name: Bachetti - first_name: Ilaria full_name: Caiazzo, Ilaria id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d last_name: Caiazzo orcid: 0000-0002-4770-5388 - first_name: Enrico full_name: Costa, Enrico last_name: Costa - first_name: Alessandro full_name: Di Marco, Alessandro last_name: Di Marco - first_name: Jeremy full_name: Heyl, Jeremy last_name: Heyl - first_name: Fabio full_name: La Monaca, Fabio last_name: La Monaca - first_name: Fabio full_name: Muleri, Fabio last_name: Muleri - first_name: Alexander A. full_name: Mushtukov, Alexander A. last_name: Mushtukov - first_name: George G. full_name: Pavlov, George G. last_name: Pavlov - first_name: Brian D. full_name: Ramsey, Brian D. last_name: Ramsey - first_name: John full_name: Rankin, John last_name: Rankin - first_name: Andrea full_name: Santangelo, Andrea last_name: Santangelo - first_name: Paolo full_name: Soffitta, Paolo last_name: Soffitta - first_name: Rüdiger full_name: Staubert, Rüdiger last_name: Staubert - first_name: Martin C. full_name: Weisskopf, Martin C. last_name: Weisskopf - first_name: Silvia full_name: Zane, Silvia last_name: Zane - first_name: Iván full_name: Agudo, Iván last_name: Agudo - first_name: Lucio A. full_name: Antonelli, Lucio A. last_name: Antonelli - 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: Stefano full_name: Ciprini, Stefano last_name: Ciprini - 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: 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: 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: Vladimir full_name: Karas, Vladimir last_name: Karas - 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: 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: 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: 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: 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: 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: Ajay full_name: Ratheesh, Ajay last_name: Ratheesh - 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: Gloria full_name: Spandre, Gloria last_name: Spandre - first_name: Rashid A. full_name: Sunyaev, Rashid A. last_name: Sunyaev - 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: Nicolas E. full_name: Thomas, Nicolas 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: Roberto full_name: Turolla, Roberto last_name: Turolla - 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 citation: ama: Doroshenko V, Poutanen J, Tsygankov SS, et al. Determination of X-ray pulsar geometry with IXPE polarimetry. Nature Astronomy. 2022;6(12):1433-1443. doi:10.1038/s41550-022-01799-5 apa: Doroshenko, V., Poutanen, J., Tsygankov, S. S., Suleimanov, V. F., Bachetti, M., Caiazzo, I., … Xie, F. (2022). Determination of X-ray pulsar geometry with IXPE polarimetry. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-022-01799-5 chicago: Doroshenko, Victor, Juri Poutanen, Sergey S. Tsygankov, Valery F. Suleimanov, Matteo Bachetti, Ilaria Caiazzo, Enrico Costa, et al. “Determination of X-Ray Pulsar Geometry with IXPE Polarimetry.” Nature Astronomy. Springer Nature, 2022. https://doi.org/10.1038/s41550-022-01799-5. ieee: V. Doroshenko et al., “Determination of X-ray pulsar geometry with IXPE polarimetry,” Nature Astronomy, vol. 6, no. 12. Springer Nature, pp. 1433–1443, 2022. ista: Doroshenko V, Poutanen J, Tsygankov SS, Suleimanov VF, Bachetti M, Caiazzo I, Costa E, Di Marco A, Heyl J, La Monaca F, Muleri F, Mushtukov AA, Pavlov GG, Ramsey BD, Rankin J, Santangelo A, Soffitta P, Staubert R, Weisskopf MC, Zane S, Agudo I, Antonelli LA, Baldini L, Baumgartner WH, Bellazzini R, Bianchi S, Bongiorno SD, Bonino R, Brez A, Bucciantini N, Capitanio F, Castellano S, Cavazzuti E, Ciprini S, De Rosa A, Del Monte E, Di Gesu L, Di Lalla N, Donnarumma I, Dovčiak M, Ehlert SR, Enoto T, Evangelista Y, Fabiani S, Ferrazzoli R, Garcia JA, Gunji S, Hayashida K, Iwakiri W, Jorstad SG, Karas V, Kitaguchi T, Kolodziejczak JJ, Krawczynski H, Latronico L, Liodakis I, Maldera S, Manfreda A, Marin F, Marinucci A, Marscher AP, Marshall HL, Matt G, Mitsuishi I, Mizuno T, Ng C-Y, O’Dell SL, Omodei N, Oppedisano C, Papitto A, Peirson AL, Perri M, Pesce-Rollins M, Pilia M, Possenti A, Puccetti S, Ratheesh A, Romani RW, Sgrò C, Slane P, Spandre G, Sunyaev RA, Tamagawa T, Tavecchio F, Taverna R, Tawara Y, Tennant AF, Thomas NE, Tombesi F, Trois A, Turolla R, Vink J, Wu K, Xie F. 2022. Determination of X-ray pulsar geometry with IXPE polarimetry. Nature Astronomy. 6(12), 1433–1443. mla: Doroshenko, Victor, et al. “Determination of X-Ray Pulsar Geometry with IXPE Polarimetry.” Nature Astronomy, vol. 6, no. 12, Springer Nature, 2022, pp. 1433–43, doi:10.1038/s41550-022-01799-5. short: V. Doroshenko, J. Poutanen, S.S. Tsygankov, V.F. Suleimanov, M. Bachetti, I. Caiazzo, E. Costa, A. Di Marco, J. Heyl, F. La Monaca, F. Muleri, A.A. Mushtukov, G.G. Pavlov, B.D. Ramsey, J. Rankin, A. Santangelo, P. Soffitta, R. Staubert, M.C. Weisskopf, S. Zane, I. Agudo, L.A. Antonelli, L. Baldini, W.H. Baumgartner, R. Bellazzini, S. Bianchi, S.D. Bongiorno, R. Bonino, A. Brez, N. Bucciantini, F. Capitanio, S. Castellano, E. Cavazzuti, S. Ciprini, A. De Rosa, E. Del Monte, L. Di Gesu, N. Di Lalla, I. Donnarumma, 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, V. Karas, T. Kitaguchi, J.J. Kolodziejczak, H. Krawczynski, L. Latronico, I. Liodakis, S. Maldera, A. Manfreda, F. Marin, A. Marinucci, A.P. Marscher, H.L. Marshall, G. Matt, I. Mitsuishi, T. Mizuno, C.-Y. Ng, S.L. O’Dell, N. Omodei, C. Oppedisano, A. Papitto, A.L. Peirson, M. Perri, M. Pesce-Rollins, M. Pilia, A. Possenti, S. Puccetti, A. Ratheesh, R.W. Romani, C. Sgrò, P. Slane, G. Spandre, R.A. Sunyaev, T. Tamagawa, F. Tavecchio, R. Taverna, Y. Tawara, A.F. Tennant, N.E. Thomas, F. Tombesi, A. Trois, R. Turolla, J. Vink, K. Wu, F. Xie, Nature Astronomy 6 (2022) 1433–1443. date_created: 2024-03-26T09:51:04Z date_published: 2022-10-22T00:00:00Z date_updated: 2024-04-02T07:16:54Z day: '22' doi: 10.1038/s41550-022-01799-5 extern: '1' external_id: arxiv: - '2206.07138' fulldoi: https://doi.org/10.1038/s41550-022-01799-5 intvolume: ' 6' issue: '12' keyword: - Astronomy and Astrophysics language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2206.07138 month: '10' oa: 1 oa_version: Preprint page: 1433-1443 publication: Nature Astronomy publication_identifier: issn: - 2397-3366 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Determination of X-ray pulsar geometry with IXPE polarimetry type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 6 year: '2022' ... --- _id: '15205' abstract: - lang: eng text: 'Magnetars are neutron stars with ultrastrong magnetic fields, which can be observed in x-rays. Polarization measurements could provide information on their magnetic fields and surface properties. We observed polarized x-rays from the magnetar 4U 0142+61 using the Imaging X-ray Polarimetry Explorer and found a linear polarization degree of 13.5 ± 0.8% averaged over the 2– to 8–kilo–electron volt band. The polarization changes with energy: The degree is 15.0 ± 1.0% at 2 to 4 kilo–electron volts, drops below the instrumental sensitivity ~4 to 5 kilo–electron volts, and rises to 35.2 ± 7.1% at 5.5 to 8 kilo–electron volts. The polarization angle also changes by 90° at ~4 to 5 kilo–electron volts. These results are consistent with a model in which thermal radiation from the magnetar surface is reprocessed by scattering off charged particles in the magnetosphere.' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Roberto full_name: Taverna, Roberto last_name: Taverna - first_name: Roberto full_name: Turolla, Roberto last_name: Turolla - first_name: Fabio full_name: Muleri, Fabio last_name: Muleri - first_name: Jeremy full_name: Heyl, Jeremy last_name: Heyl - first_name: Silvia full_name: Zane, Silvia last_name: Zane - first_name: Luca full_name: Baldini, Luca last_name: Baldini - first_name: Denis full_name: González-Caniulef, Denis last_name: González-Caniulef - first_name: Matteo full_name: Bachetti, Matteo last_name: Bachetti - first_name: John full_name: Rankin, John last_name: Rankin - 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: Victor full_name: Doroshenko, Victor last_name: Doroshenko - first_name: Manel full_name: Errando, Manel last_name: Errando - first_name: Ephraim full_name: Gau, Ephraim last_name: Gau - first_name: Demet full_name: Kırmızıbayrak, Demet last_name: Kırmızıbayrak - first_name: Henric full_name: Krawczynski, Henric last_name: Krawczynski - first_name: Michela full_name: Negro, Michela last_name: Negro - first_name: Mason full_name: Ng, Mason last_name: Ng - first_name: Nicola full_name: Omodei, Nicola last_name: Omodei - first_name: Andrea full_name: Possenti, Andrea last_name: Possenti - first_name: Toru full_name: Tamagawa, Toru last_name: Tamagawa - first_name: Keisuke full_name: Uchiyama, Keisuke last_name: Uchiyama - first_name: Martin C. full_name: Weisskopf, Martin C. last_name: Weisskopf - first_name: Ivan full_name: Agudo, Ivan 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: 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: 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: 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: Vladimir full_name: Karas, Vladimir last_name: Karas - first_name: Takao full_name: Kitaguchi, Takao last_name: Kitaguchi - first_name: Jeffery J. full_name: Kolodziejczak, Jeffery J. last_name: Kolodziejczak - 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: 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: Stephen C.-Y. full_name: Ng, Stephen 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: 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: Maura full_name: Pilia, Maura last_name: Pilia - 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: 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: 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: Kinwah full_name: Wu, Kinwah last_name: Wu - first_name: Fei full_name: Xie, Fei last_name: Xie citation: ama: Taverna R, Turolla R, Muleri F, et al. Polarized x-rays from a magnetar. Science. 2022;378(6620):646-650. doi:10.1126/science.add0080 apa: Taverna, R., Turolla, R., Muleri, F., Heyl, J., Zane, S., Baldini, L., … Xie, F. (2022). Polarized x-rays from a magnetar. Science. American Association for the Advancement of Science. https://doi.org/10.1126/science.add0080 chicago: Taverna, Roberto, Roberto Turolla, Fabio Muleri, Jeremy Heyl, Silvia Zane, Luca Baldini, Denis González-Caniulef, et al. “Polarized X-Rays from a Magnetar.” Science. American Association for the Advancement of Science, 2022. https://doi.org/10.1126/science.add0080. ieee: R. Taverna et al., “Polarized x-rays from a magnetar,” Science, vol. 378, no. 6620. American Association for the Advancement of Science, pp. 646–650, 2022. ista: Taverna R, Turolla R, Muleri F, Heyl J, Zane S, Baldini L, González-Caniulef D, Bachetti M, Rankin J, Caiazzo I, Di Lalla N, Doroshenko V, Errando M, Gau E, Kırmızıbayrak D, Krawczynski H, Negro M, Ng M, Omodei N, Possenti A, Tamagawa T, Uchiyama K, Weisskopf MC, Agudo I, Antonelli LA, Baumgartner WH, Bellazzini R, Bianchi S, Bongiorno SD, Bonino R, Brez A, Bucciantini N, Capitanio F, Castellano S, Cavazzuti E, Ciprini S, Costa E, De Rosa A, Del Monte E, Di Gesu L, Di Marco A, Donnarumma I, Dovčiak M, Ehlert SR, Enoto T, Evangelista Y, Fabiani S, Ferrazzoli R, Garcia JA, Gunji S, Hayashida K, Iwakiri W, Jorstad SG, Karas V, Kitaguchi T, Kolodziejczak JJ, La Monaca F, Latronico L, Liodakis I, Maldera S, Manfreda A, Marin F, Marinucci A, Marscher AP, Marshall HL, Matt G, Mitsuishi I, Mizuno T, Ng SC-Y, O’Dell SL, Oppedisano C, Papitto A, Pavlov GG, Peirson AL, Perri M, Pesce-Rollins M, Pilia M, Poutanen J, Puccetti S, Ramsey BD, Ratheesh A, Romani RW, Sgrò C, Slane P, Soffitta P, Spandre G, Tavecchio F, Tawara Y, Tennant AF, Thomas NE, Tombesi F, Trois A, Tsygankov SS, Vink J, Wu K, Xie F. 2022. Polarized x-rays from a magnetar. Science. 378(6620), 646–650. mla: Taverna, Roberto, et al. “Polarized X-Rays from a Magnetar.” Science, vol. 378, no. 6620, American Association for the Advancement of Science, 2022, pp. 646–50, doi:10.1126/science.add0080. short: R. Taverna, R. Turolla, F. Muleri, J. Heyl, S. Zane, L. Baldini, D. González-Caniulef, M. Bachetti, J. Rankin, I. Caiazzo, N. Di Lalla, V. Doroshenko, M. Errando, E. Gau, D. Kırmızıbayrak, H. Krawczynski, M. Negro, M. Ng, N. Omodei, A. Possenti, T. Tamagawa, K. Uchiyama, M.C. Weisskopf, 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, S. Ciprini, E. Costa, A. De Rosa, E. Del Monte, L. Di Gesu, A. Di Marco, I. Donnarumma, 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, V. Karas, T. Kitaguchi, J.J. Kolodziejczak, F. La Monaca, L. Latronico, I. Liodakis, S. Maldera, A. Manfreda, F. Marin, A. Marinucci, A.P. Marscher, H.L. Marshall, G. Matt, I. Mitsuishi, T. Mizuno, S.C.-Y. Ng, S.L. O’Dell, C. Oppedisano, A. Papitto, G.G. Pavlov, A.L. Peirson, M. Perri, M. Pesce-Rollins, M. Pilia, J. Poutanen, S. Puccetti, B.D. Ramsey, A. Ratheesh, R.W. Romani, C. Sgrò, P. Slane, P. Soffitta, G. Spandre, F. Tavecchio, Y. Tawara, A.F. Tennant, N.E. Thomas, F. Tombesi, A. Trois, S.S. Tsygankov, J. Vink, K. Wu, F. Xie, Science 378 (2022) 646–650. date_created: 2024-03-26T09:51:30Z date_published: 2022-11-03T00:00:00Z date_updated: 2024-04-02T07:17:25Z day: '03' doi: 10.1126/science.add0080 extern: '1' external_id: arxiv: - '2205.08898' fulldoi: https://doi.org/10.1126/science.add0080 intvolume: ' 378' issue: '6620' keyword: - Multidisciplinary language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2205.08898 month: '11' oa: 1 oa_version: Preprint page: 646-650 publication: Science publication_identifier: eissn: - 1095-9203 issn: - 0036-8075 publication_status: published publisher: American Association for the Advancement of Science quality_controlled: '1' scopus_import: '1' status: public title: Polarized x-rays from a magnetar type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 378 year: '2022' ... --- _id: '15206' abstract: - lang: eng text: We use the Relativistic Precession Model (RPM) and quasi-periodic oscillation (QPO) observations from the Rossi X-ray Timing Explorer to derive constraints on the properties of the black holes that power these sources and to test general relativity (GR) in the strong field regime. We build upon past techniques by using pairs of simultaneously measured QPOs, rather than triplets, and by including characteristic frequencies from the broad noise components of the power spectra in our fits. We find the inclusion of these broad noise components causes an overestimate in masses and underestimate in spins compared to values derived independently from optical spectra. We extend the underlying space-time metric to constrain potential deviations from the predictions of GR for astrophysical black holes. To do this, we modify the RPM model to a Kerr–Newman–deSitter space-time and model changes in the radial, ecliptic, and vertical frequencies. We compare our models with X-ray data of XTE J1550-564 and GRO J1655-40 using robust statistical techniques to constrain the parameters of the black holes and the deviations from GR. For both sources, using QPO and characteristic frequency data, we constrain particular deviations from GR to be less than one part per thousand. article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Katherine full_name: Rink, Katherine last_name: Rink - 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: 'Rink K, Caiazzo I, Heyl J. Testing general relativity using quasi-periodic oscillations from X-ray black holes: XTE J1550-564 and GRO J1655-40. Monthly Notices of the Royal Astronomical Society. 2022;517(1):1389-1397. doi:10.1093/mnras/stac2740' apa: 'Rink, K., Caiazzo, I., & Heyl, J. (2022). Testing general relativity using quasi-periodic oscillations from X-ray black holes: XTE J1550-564 and GRO J1655-40. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stac2740' chicago: 'Rink, Katherine, Ilaria Caiazzo, and Jeremy Heyl. “Testing General Relativity Using Quasi-Periodic Oscillations from X-Ray Black Holes: XTE J1550-564 and GRO J1655-40.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2022. https://doi.org/10.1093/mnras/stac2740.' ieee: 'K. Rink, I. Caiazzo, and J. Heyl, “Testing general relativity using quasi-periodic oscillations from X-ray black holes: XTE J1550-564 and GRO J1655-40,” Monthly Notices of the Royal Astronomical Society, vol. 517, no. 1. Oxford University Press, pp. 1389–1397, 2022.' ista: 'Rink K, Caiazzo I, Heyl J. 2022. Testing general relativity using quasi-periodic oscillations from X-ray black holes: XTE J1550-564 and GRO J1655-40. Monthly Notices of the Royal Astronomical Society. 517(1), 1389–1397.' mla: 'Rink, Katherine, et al. “Testing General Relativity Using Quasi-Periodic Oscillations from X-Ray Black Holes: XTE J1550-564 and GRO J1655-40.” Monthly Notices of the Royal Astronomical Society, vol. 517, no. 1, Oxford University Press, 2022, pp. 1389–97, doi:10.1093/mnras/stac2740.' short: K. Rink, I. Caiazzo, J. Heyl, Monthly Notices of the Royal Astronomical Society 517 (2022) 1389–1397. date_created: 2024-03-26T09:51:55Z date_published: 2022-09-28T00:00:00Z date_updated: 2024-04-02T07:18:07Z day: '28' doi: 10.1093/mnras/stac2740 extern: '1' external_id: arxiv: - '2107.06828' fulldoi: https://doi.org/10.1093/mnras/stac2740 intvolume: ' 517' issue: '1' keyword: - Space and Planetary Science - Astronomy and Astrophysics language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2107.06828 month: '09' oa: 1 oa_version: Preprint page: 1389-1397 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: 'Testing general relativity using quasi-periodic oscillations from X-ray black holes: XTE J1550-564 and GRO J1655-40' type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 517 year: '2022' ... --- _id: '15207' abstract: - lang: eng text: Of more than a thousand known cataclysmic variables (CVs), where a white dwarf is accreting from a hydrogen-rich star, only a dozen have orbital periods below 75 minutes1,2,3,4,5,6,7,8,9. One way to achieve these short periods requires the donor star to have undergone substantial nuclear evolution before interacting with the white dwarf10,11,12,13,14, and it is expected that these objects will transition to helium accretion. These transitional CVs have been proposed as progenitors of helium CVs13,14,15,16,17,18. However, no known transitional CV is expected to reach an orbital period short enough to account for most of the helium CV population, leaving the role of this evolutionary pathway unclear. Here we report observations of ZTF J1813+4251, a 51-minute-orbital-period, fully eclipsing binary system consisting of a star with a temperature comparable to that of the Sun but a density 100 times greater owing to its helium-rich composition, accreting onto a white dwarf. Phase-resolved spectra, multi-band light curves and the broadband spectral energy distribution allow us to obtain precise and robust constraints on the masses, radii and temperatures of both components. Evolutionary modelling shows that ZTF J1813+4251 is destined to become a helium CV binary, reaching an orbital period under 20 minutes, rendering ZTF J1813+4251 a previously missing link between helium CV binaries and hydrogen-rich CVs. 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: Thomas R. full_name: Marsh, Thomas R. last_name: Marsh - first_name: Saul full_name: Rappaport, Saul last_name: Rappaport - first_name: Warren R. full_name: Brown, Warren R. last_name: Brown - 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: V. S. full_name: Dhillon, V. S. last_name: Dhillon - first_name: Jim full_name: Fuller, Jim last_name: Fuller - 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: Erin full_name: Kara, Erin last_name: Kara - first_name: S. R. full_name: Kulkarni, S. R. last_name: Kulkarni - first_name: S. P. full_name: Littlefair, S. P. last_name: Littlefair - first_name: Przemek full_name: Mróz, Przemek last_name: Mróz - first_name: Pablo full_name: Rodríguez-Gil, Pablo last_name: Rodríguez-Gil - first_name: Jan van full_name: Roestel, Jan van last_name: Roestel - first_name: Robert A. full_name: Simcoe, Robert A. last_name: Simcoe - first_name: Eric C. full_name: Bellm, Eric C. last_name: Bellm - first_name: Andrew J. full_name: Drake, Andrew J. last_name: Drake - first_name: Richard G. full_name: Dekany, Richard G. last_name: Dekany - first_name: Steven L. full_name: Groom, Steven L. last_name: Groom - 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: Reed full_name: Riddle, Reed last_name: Riddle - first_name: Roger M. full_name: Smith, Roger M. last_name: Smith - first_name: Thomas A. full_name: Prince, Thomas A. last_name: Prince citation: ama: Burdge KB, El-Badry K, Marsh TR, et al. A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary. Nature. 2022;610(7932):467-471. doi:10.1038/s41586-022-05195-x apa: Burdge, K. B., El-Badry, K., Marsh, T. R., Rappaport, S., Brown, W. R., Caiazzo, I., … Prince, T. A. (2022). A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary. Nature. Springer Nature. https://doi.org/10.1038/s41586-022-05195-x chicago: Burdge, Kevin B., Kareem El-Badry, Thomas R. Marsh, Saul Rappaport, Warren R. Brown, Ilaria Caiazzo, Deepto Chakrabarty, et al. “A Dense 0.1-Solar-Mass Star in a 51-Minute-Orbital-Period Eclipsing Binary.” Nature. Springer Nature, 2022. https://doi.org/10.1038/s41586-022-05195-x. ieee: K. B. Burdge et al., “A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary,” Nature, vol. 610, no. 7932. Springer Nature, pp. 467–471, 2022. ista: Burdge KB, El-Badry K, Marsh TR, Rappaport S, Brown WR, Caiazzo I, Chakrabarty D, Dhillon VS, Fuller J, Gänsicke BT, Graham MJ, Kara E, Kulkarni SR, Littlefair SP, Mróz P, Rodríguez-Gil P, Roestel J van, Simcoe RA, Bellm EC, Drake AJ, Dekany RG, Groom SL, Laher RR, Masci FJ, Riddle R, Smith RM, Prince TA. 2022. A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary. Nature. 610(7932), 467–471. mla: Burdge, Kevin B., et al. “A Dense 0.1-Solar-Mass Star in a 51-Minute-Orbital-Period Eclipsing Binary.” Nature, vol. 610, no. 7932, Springer Nature, 2022, pp. 467–71, doi:10.1038/s41586-022-05195-x. short: K.B. Burdge, K. El-Badry, T.R. Marsh, S. Rappaport, W.R. Brown, I. Caiazzo, D. Chakrabarty, V.S. Dhillon, J. Fuller, B.T. Gänsicke, M.J. Graham, E. Kara, S.R. Kulkarni, S.P. Littlefair, P. Mróz, P. Rodríguez-Gil, J. van Roestel, R.A. Simcoe, E.C. Bellm, A.J. Drake, R.G. Dekany, S.L. Groom, R.R. Laher, F.J. Masci, R. Riddle, R.M. Smith, T.A. Prince, Nature 610 (2022) 467–471. date_created: 2024-03-26T09:52:17Z date_published: 2022-10-05T00:00:00Z date_updated: 2024-04-02T07:18:43Z day: '05' doi: 10.1038/s41586-022-05195-x extern: '1' external_id: arxiv: - '2210.01809' pmid: - '36198793' fulldoi: https://doi.org/10.1038/s41586-022-05195-x intvolume: ' 610' issue: '7932' language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2210.01809 month: '10' oa: 1 oa_version: Preprint page: 467-471 pmid: 1 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 dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 610 year: '2022' ... --- _id: '15208' abstract: - lang: eng text: This year, a new era of observations of compact objects in X-ray polarization is commencing. Among the key targets for the Imaging X-ray Polarimetry Explorer mission are the magnetars 4U 0142+61 and 1RXS J170849.0-400910. Here, we present detailed predictions of the expected polarization from these sources that incorporate realistic models of emission physics at the surface (gaseous or condensed), the temperature distribution on the surface, general relativity, quantum electrodynamics, and scattering in the magnetosphere, accounting for the broad-band spectral energy distribution from below 1 keV to nearly 100 keV. We find that either atmospheres or condensed surfaces can account for the emission at a few keV. In both cases, either a small hot polar cap or scattering is required to account for the emission at 5–10 keV and, above 10 keV, scattering by a hard population of electrons can account for the rising power in the hard X-rays observed in many magnetars in quiescence. Although these different scenarios result in very similar spectral energy distributions, they generate dramatically different polarization signatures from 2 to 8 keV, which is the range of sensitivity of the Imaging X-ray Polarimetry Explorer. Observations of these sources in X-ray polarization will therefore probe the emission from magnetars in an essentially new way. 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: Denis full_name: González-Caniulef, Denis last_name: González-Caniulef - first_name: Jeremy full_name: Heyl, Jeremy last_name: Heyl - first_name: Rodrigo full_name: Fernández, Rodrigo last_name: Fernández citation: ama: Caiazzo I, González-Caniulef D, Heyl J, Fernández R. Probing magnetar emission mechanisms with X-ray spectropolarimetry. Monthly Notices of the Royal Astronomical Society. 2022;514(4):5024-5034. doi:10.1093/mnras/stac1571 apa: Caiazzo, I., González-Caniulef, D., Heyl, J., & Fernández, R. (2022). Probing magnetar emission mechanisms with X-ray spectropolarimetry. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stac1571 chicago: Caiazzo, Ilaria, Denis González-Caniulef, Jeremy Heyl, and Rodrigo Fernández. “Probing Magnetar Emission Mechanisms with X-Ray Spectropolarimetry.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2022. https://doi.org/10.1093/mnras/stac1571. ieee: I. Caiazzo, D. González-Caniulef, J. Heyl, and R. Fernández, “Probing magnetar emission mechanisms with X-ray spectropolarimetry,” Monthly Notices of the Royal Astronomical Society, vol. 514, no. 4. Oxford University Press, pp. 5024–5034, 2022. ista: Caiazzo I, González-Caniulef D, Heyl J, Fernández R. 2022. Probing magnetar emission mechanisms with X-ray spectropolarimetry. Monthly Notices of the Royal Astronomical Society. 514(4), 5024–5034. mla: Caiazzo, Ilaria, et al. “Probing Magnetar Emission Mechanisms with X-Ray Spectropolarimetry.” Monthly Notices of the Royal Astronomical Society, vol. 514, no. 4, Oxford University Press, 2022, pp. 5024–34, doi:10.1093/mnras/stac1571. short: I. Caiazzo, D. González-Caniulef, J. Heyl, R. Fernández, Monthly Notices of the Royal Astronomical Society 514 (2022) 5024–5034. date_created: 2024-03-26T09:52:41Z date_published: 2022-06-09T00:00:00Z date_updated: 2024-10-14T12:32:39Z day: '09' doi: 10.1093/mnras/stac1571 extern: '1' external_id: arxiv: - '2112.03401' fulldoi: https://doi.org/10.1093/mnras/stac1571 intvolume: ' 514' issue: '4' keyword: - Space and Planetary Science - Astronomy and Astrophysics language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2112.03401 month: '06' oa: 1 oa_version: Preprint page: 5024-5034 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: Probing magnetar emission mechanisms with X-ray spectropolarimetry type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 514 year: '2022' ... --- _id: '15209' abstract: - lang: eng text: It has been recently suggested that white dwarfs generate magnetic fields in a process analogous to the Earth. The crystallization of the core creates a compositional inversion that drives convection, and combined with rotation, this can sustain a magnetic dynamo. We reanalyse the dynamo mechanism, arising from the slow crystallization of the core, and find convective turnover times tconv of weeks to months – longer by orders of magnitude than previously thought. With white dwarf spin periods P ≪ tconv, crystallization-driven dynamos are almost always in the fast-rotating regime, where the magnetic field B is at least in equipartition with the convective motion and is possibly further enhanced by a factor of B ∝ (tconv/P)1/2, depending on the assumed dynamo scaling law. We track the growth of the crystallized core using MESA and compute the magnetic field B(Teff) as a function of the white dwarf’s effective temperature Teff. We compare this prediction with observations and show that crystallization-driven dynamos can explain some – but not all – of the ∼MG magnetic fields measured for single white dwarfs, as well as the stronger fields measured for white dwarfs in cataclysmic variables, which were spun up by mass accretion to short P. Our B(Teff) curves might also explain the clustering of white dwarfs with Balmer emission lines around Teff ≈ 7500 K. article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Sivan full_name: Ginzburg, Sivan last_name: Ginzburg - first_name: Jim full_name: Fuller, Jim last_name: Fuller - first_name: Adela full_name: Kawka, Adela last_name: Kawka - first_name: Ilaria full_name: Caiazzo, Ilaria id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d last_name: Caiazzo orcid: 0000-0002-4770-5388 citation: ama: Ginzburg S, Fuller J, Kawka A, Caiazzo I. Slow convection and fast rotation in crystallization-driven white dwarf dynamos. Monthly Notices of the Royal Astronomical Society. 2022;514(3):4111-4119. doi:10.1093/mnras/stac1363 apa: Ginzburg, S., Fuller, J., Kawka, A., & Caiazzo, I. (2022). Slow convection and fast rotation in crystallization-driven white dwarf dynamos. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stac1363 chicago: Ginzburg, Sivan, Jim Fuller, Adela Kawka, and Ilaria Caiazzo. “Slow Convection and Fast Rotation in Crystallization-Driven White Dwarf Dynamos.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2022. https://doi.org/10.1093/mnras/stac1363. ieee: S. Ginzburg, J. Fuller, A. Kawka, and I. Caiazzo, “Slow convection and fast rotation in crystallization-driven white dwarf dynamos,” Monthly Notices of the Royal Astronomical Society, vol. 514, no. 3. Oxford University Press, pp. 4111–4119, 2022. ista: Ginzburg S, Fuller J, Kawka A, Caiazzo I. 2022. Slow convection and fast rotation in crystallization-driven white dwarf dynamos. Monthly Notices of the Royal Astronomical Society. 514(3), 4111–4119. mla: Ginzburg, Sivan, et al. “Slow Convection and Fast Rotation in Crystallization-Driven White Dwarf Dynamos.” Monthly Notices of the Royal Astronomical Society, vol. 514, no. 3, Oxford University Press, 2022, pp. 4111–19, doi:10.1093/mnras/stac1363. short: S. Ginzburg, J. Fuller, A. Kawka, I. Caiazzo, Monthly Notices of the Royal Astronomical Society 514 (2022) 4111–4119. date_created: 2024-03-26T09:53:04Z date_published: 2022-05-16T00:00:00Z date_updated: 2024-04-02T07:24:15Z day: '16' doi: 10.1093/mnras/stac1363 extern: '1' external_id: arxiv: - '2202.12902' fulldoi: https://doi.org/10.1093/mnras/stac1363 intvolume: ' 514' issue: '3' keyword: - Space and Planetary Science - Astronomy and Astrophysics language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2202.12902 month: '05' oa: 1 oa_version: Preprint page: 4111-4119 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: Slow convection and fast rotation in crystallization-driven white dwarf dynamos type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 514 year: '2022' ... --- _id: '15210' abstract: - lang: eng text: The maximum mass of a star that can produce a white dwarf (WD) is an important astrophysical quantity. One of the best approaches to establishing this limit is to search for WDs in young star clusters in which only massive stars have had time to evolve and where the mass of the progenitor can be established from the cooling time of the WD together with the age of the cluster. Searches in young Milky Way clusters have not thus far yielded WD members more massive than about 1.1 M⊙, well below the Chandrasekhar mass of 1.38 M⊙, nor progenitors with masses in excess of about 6 M⊙. However, the hunt for potentially massive WDs that escaped their cluster environs is yielding interesting candidates. To expand the cluster sample further, we used HST to survey four young and massive star clusters in the Magellanic Clouds for bright WDs that could have evolved from stars as massive as 10 M⊙. We located five potential WD candidates in the oldest of the four clusters examined, the first extragalactic single WDs thus far discovered. As these hot WDs are very faint at optical wavelengths, final confirmation will likely have to await spectroscopy with 30 m class telescopes. article_number: L20 article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Harvey B. full_name: Richer, Harvey B. last_name: Richer - first_name: Roger E. full_name: Cohen, Roger E. last_name: Cohen - first_name: Jeremy full_name: Heyl, Jeremy last_name: Heyl - first_name: Jason full_name: Kalirai, Jason last_name: Kalirai - first_name: Ilaria full_name: Caiazzo, Ilaria id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d last_name: Caiazzo orcid: 0000-0002-4770-5388 - first_name: Matteo full_name: Correnti, Matteo last_name: Correnti - first_name: Jeffrey full_name: Cummings, Jeffrey last_name: Cummings - first_name: Paul full_name: Goudfrooij, Paul last_name: Goudfrooij - first_name: Bradley M. S. full_name: Hansen, Bradley M. S. last_name: Hansen - first_name: Molly full_name: Peeples, Molly last_name: Peeples - first_name: Elena full_name: Sabbi, Elena last_name: Sabbi - first_name: Pier-Emmanuel full_name: Tremblay, Pier-Emmanuel last_name: Tremblay - first_name: Benjamin full_name: Williams, Benjamin last_name: Williams citation: ama: Richer HB, Cohen RE, Heyl J, et al. When do stars go boom? The Astrophysical Journal Letters. 2022;931(2). doi:10.3847/2041-8213/ac6585 apa: Richer, H. B., Cohen, R. E., Heyl, J., Kalirai, J., Caiazzo, I., Correnti, M., … Williams, B. (2022). When do stars go boom? The Astrophysical Journal Letters. American Astronomical Society. https://doi.org/10.3847/2041-8213/ac6585 chicago: Richer, Harvey B., Roger E. Cohen, Jeremy Heyl, Jason Kalirai, Ilaria Caiazzo, Matteo Correnti, Jeffrey Cummings, et al. “When Do Stars Go Boom?” The Astrophysical Journal Letters. American Astronomical Society, 2022. https://doi.org/10.3847/2041-8213/ac6585. ieee: H. B. Richer et al., “When do stars go boom?,” The Astrophysical Journal Letters, vol. 931, no. 2. American Astronomical Society, 2022. ista: Richer HB, Cohen RE, Heyl J, Kalirai J, Caiazzo I, Correnti M, Cummings J, Goudfrooij P, Hansen BMS, Peeples M, Sabbi E, Tremblay P-E, Williams B. 2022. When do stars go boom? The Astrophysical Journal Letters. 931(2), L20. mla: Richer, Harvey B., et al. “When Do Stars Go Boom?” The Astrophysical Journal Letters, vol. 931, no. 2, L20, American Astronomical Society, 2022, doi:10.3847/2041-8213/ac6585. short: H.B. Richer, R.E. Cohen, J. Heyl, J. Kalirai, I. Caiazzo, M. Correnti, J. Cummings, P. Goudfrooij, B.M.S. Hansen, M. Peeples, E. Sabbi, P.-E. Tremblay, B. Williams, The Astrophysical Journal Letters 931 (2022). date_created: 2024-03-26T10:28:48Z date_published: 2022-05-30T00:00:00Z date_updated: 2024-04-02T07:25:50Z day: '30' doi: 10.3847/2041-8213/ac6585 extern: '1' external_id: arxiv: - '2203.11264' fulldoi: https://doi.org/10.3847/2041-8213/ac6585 intvolume: ' 931' issue: '2' keyword: - Space and Planetary Science - Astronomy and Astrophysics language: - iso: eng license: https://creativecommons.org/licenses/by/4.0/ main_file_link: - open_access: '1' url: https://doi.org/10.3847/2041-8213/ac6585 month: '05' 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: When do stars go boom? 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: 931 year: '2022' ... --- _id: '15211' abstract: - lang: eng text: Over a dozen millisecond pulsars are ablating low-mass companions in close binary systems. In the original ‘black widow’, the eight-hour orbital period eclipsing pulsar PSR J1959+2048 (PSR B1957+20)1, high-energy emission originating from the pulsar2 is irradiating and may eventually destroy3 a low-mass companion. These systems are not only physical laboratories that reveal the interesting results of exposing a close companion star to the relativistic energy output of a pulsar, but are also believed to harbour some of the most massive neutron stars4, allowing for robust tests of the neutron star equation of state. Here we report observations of ZTF J1406+1222, a wide hierarchical triple hosting a 62-minute orbital period black widow candidate, the optical flux of which varies by a factor of more than ten. ZTF J1406+1222 pushes the boundaries of evolutionary models5, falling below the 80-minute minimum orbital period of hydrogen-rich systems. The wide tertiary companion is a rare low-metallicity cool subdwarf star, and the system has a Galactic halo orbit consistent with passing near the Galactic Centre, making it a probe of formation channels, neutron star kick physics6 and binary evolution. article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Kevin B. full_name: Burdge, Kevin B. last_name: Burdge - first_name: Thomas R. full_name: Marsh, Thomas R. last_name: Marsh - first_name: Jim full_name: Fuller, Jim last_name: Fuller - first_name: Eric C. full_name: Bellm, Eric C. last_name: Bellm - 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: Michael W. full_name: Coughlin, Michael W. last_name: Coughlin - first_name: Kishalay full_name: De, Kishalay last_name: De - first_name: V. S. full_name: Dhillon, V. S. last_name: Dhillon - first_name: Matthew J. full_name: Graham, Matthew J. last_name: Graham - first_name: Pablo full_name: Rodríguez-Gil, Pablo last_name: Rodríguez-Gil - first_name: Amruta D. full_name: Jaodand, Amruta D. last_name: Jaodand - first_name: David L. full_name: Kaplan, David L. last_name: Kaplan - first_name: Erin full_name: Kara, Erin last_name: Kara - first_name: Albert K. H. full_name: Kong, Albert K. H. last_name: Kong - first_name: S. R. full_name: Kulkarni, S. R. last_name: Kulkarni - first_name: Kwan-Lok full_name: Li, Kwan-Lok last_name: Li - first_name: S. P. full_name: Littlefair, S. P. last_name: Littlefair - first_name: Walid A. full_name: Majid, Walid A. last_name: Majid - first_name: Przemek full_name: Mróz, Przemek last_name: Mróz - first_name: Aaron B. full_name: Pearlman, Aaron B. last_name: Pearlman - first_name: E. S. full_name: Phinney, E. S. last_name: Phinney - first_name: Jan van full_name: Roestel, Jan van last_name: Roestel - first_name: Robert A. full_name: Simcoe, Robert A. last_name: Simcoe - first_name: Igor full_name: Andreoni, Igor last_name: Andreoni - first_name: Andrew J. full_name: Drake, Andrew J. last_name: Drake - first_name: Richard G. full_name: Dekany, Richard G. last_name: Dekany - first_name: Dmitry A. full_name: Duev, Dmitry A. last_name: Duev - first_name: Erik C. full_name: Kool, Erik C. last_name: Kool - first_name: Ashish A. full_name: Mahabal, Ashish A. last_name: Mahabal - first_name: Michael S. full_name: Medford, Michael S. last_name: Medford - first_name: Reed full_name: Riddle, Reed last_name: Riddle - first_name: Thomas A. full_name: Prince, Thomas A. last_name: Prince citation: ama: Burdge KB, Marsh TR, Fuller J, et al. A 62-minute orbital period black widow binary in a wide hierarchical triple. Nature. 2022;605(7908):41-45. doi:10.1038/s41586-022-04551-1 apa: Burdge, K. B., Marsh, T. R., Fuller, J., Bellm, E. C., Caiazzo, I., Chakrabarty, D., … Prince, T. A. (2022). A 62-minute orbital period black widow binary in a wide hierarchical triple. Nature. Springer Nature. https://doi.org/10.1038/s41586-022-04551-1 chicago: Burdge, Kevin B., Thomas R. Marsh, Jim Fuller, Eric C. Bellm, Ilaria Caiazzo, Deepto Chakrabarty, Michael W. Coughlin, et al. “A 62-Minute Orbital Period Black Widow Binary in a Wide Hierarchical Triple.” Nature. Springer Nature, 2022. https://doi.org/10.1038/s41586-022-04551-1. ieee: K. B. Burdge et al., “A 62-minute orbital period black widow binary in a wide hierarchical triple,” Nature, vol. 605, no. 7908. Springer Nature, pp. 41–45, 2022. ista: Burdge KB, Marsh TR, Fuller J, Bellm EC, Caiazzo I, Chakrabarty D, Coughlin MW, De K, Dhillon VS, Graham MJ, Rodríguez-Gil P, Jaodand AD, Kaplan DL, Kara E, Kong AKH, Kulkarni SR, Li K-L, Littlefair SP, Majid WA, Mróz P, Pearlman AB, Phinney ES, Roestel J van, Simcoe RA, Andreoni I, Drake AJ, Dekany RG, Duev DA, Kool EC, Mahabal AA, Medford MS, Riddle R, Prince TA. 2022. A 62-minute orbital period black widow binary in a wide hierarchical triple. Nature. 605(7908), 41–45. mla: Burdge, Kevin B., et al. “A 62-Minute Orbital Period Black Widow Binary in a Wide Hierarchical Triple.” Nature, vol. 605, no. 7908, Springer Nature, 2022, pp. 41–45, doi:10.1038/s41586-022-04551-1. short: K.B. Burdge, T.R. Marsh, J. Fuller, E.C. Bellm, I. Caiazzo, D. Chakrabarty, M.W. Coughlin, K. De, V.S. Dhillon, M.J. Graham, P. Rodríguez-Gil, A.D. Jaodand, D.L. Kaplan, E. Kara, A.K.H. Kong, S.R. Kulkarni, K.-L. Li, S.P. Littlefair, W.A. Majid, P. Mróz, A.B. Pearlman, E.S. Phinney, J. van Roestel, R.A. Simcoe, I. Andreoni, A.J. Drake, R.G. Dekany, D.A. Duev, E.C. Kool, A.A. Mahabal, M.S. Medford, R. Riddle, T.A. Prince, Nature 605 (2022) 41–45. date_created: 2024-03-26T10:29:26Z date_published: 2022-05-04T00:00:00Z date_updated: 2024-04-02T07:26:19Z day: '04' doi: 10.1038/s41586-022-04551-1 extern: '1' external_id: arxiv: - '2205.02278' pmid: - '35508781' fulldoi: https://doi.org/10.1038/s41586-022-04551-1 intvolume: ' 605' issue: '7908' keyword: - Multidisciplinary language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2205.02278 month: '05' oa: 1 oa_version: Preprint page: 41-45 pmid: 1 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 62-minute orbital period black widow binary in a wide hierarchical triple type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 605 year: '2022' ... --- _id: '15212' abstract: - lang: eng text: We determine the distribution of cooling ages of massive Gaia EDR3 white dwarfs identified with over 90 per cent probability within 200 pc and with mass in the range 0.95–1.25 M⊙. Using three sets of publicly available models, we consider sub-samples of these white dwarfs sorted into three equally spaced mass bins. Under the assumption of a constant white dwarf formation rate, we find an excess of white dwarfs, both along the Q branch and below it, corresponding respectively to stars that are in the process of freezing and those that are completely frozen. We compare the cooling age distributions for each of these bins to the recently determined time-varying star formation rate of Gaia DR2 main sequence stars. For white dwarfs in the two lightest mass bins, spanning the mass range 0.95–1.15 M⊙, we find that the cumulative cooling age distribution is statistically consistent with the expectation from the star formation rate. For white dwarfs in the heaviest mass bin, 1.15–1.25 M⊙, we find that their cumulative distribution is inconsistent with the star formation rate for all of the models considered; instead, we find that their cooling age distribution is well fitted by a linear combination of the distribution expected for single stellar evolution products and the distribution expected for double white dwarf merger products when approximately 40–50 per cent of the 1.15–1.25 M⊙ white dwarfs that formed over the past 4 Gyr are produced through double white dwarf mergers. 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 cooling of massive white dwarfs from Gaia EDR3. Monthly Notices of the Royal Astronomical Society. 2022;511(4):5984-5993. doi:10.1093/mnras/stac458 apa: Fleury, L., Caiazzo, I., & Heyl, J. (2022). The cooling of massive white dwarfs from Gaia EDR3. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stac458 chicago: Fleury, Leesa, Ilaria Caiazzo, and Jeremy Heyl. “The Cooling of Massive White Dwarfs from Gaia EDR3.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2022. https://doi.org/10.1093/mnras/stac458. ieee: L. Fleury, I. Caiazzo, and J. Heyl, “The cooling of massive white dwarfs from Gaia EDR3,” Monthly Notices of the Royal Astronomical Society, vol. 511, no. 4. Oxford University Press, pp. 5984–5993, 2022. ista: Fleury L, Caiazzo I, Heyl J. 2022. The cooling of massive white dwarfs from Gaia EDR3. Monthly Notices of the Royal Astronomical Society. 511(4), 5984–5993. mla: Fleury, Leesa, et al. “The Cooling of Massive White Dwarfs from Gaia EDR3.” Monthly Notices of the Royal Astronomical Society, vol. 511, no. 4, Oxford University Press, 2022, pp. 5984–93, doi:10.1093/mnras/stac458. short: L. Fleury, I. Caiazzo, J. Heyl, Monthly Notices of the Royal Astronomical Society 511 (2022) 5984–5993. date_created: 2024-03-26T10:31:05Z date_published: 2022-02-21T00:00:00Z date_updated: 2024-04-02T07:26:50Z day: '21' doi: 10.1093/mnras/stac458 extern: '1' external_id: arxiv: - '2110.00598' fulldoi: https://doi.org/10.1093/mnras/stac458 intvolume: ' 511' issue: '4' keyword: - Space and Planetary Science - Astronomy and Astrophysics language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2110.00598 month: '02' oa: 1 oa_version: Preprint page: 5984-5993 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 cooling of massive white dwarfs from Gaia EDR3 type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 511 year: '2022' ... --- _id: '15213' abstract: - lang: eng text: We searched through the entire Gaia EDR3 candidate white dwarf catalog for stars with proper motions and positions that are consistent with them having escaped from the Alpha Persei cluster within the past 81 Myr, the age of the cluster. In this search we found five candidate white dwarf escapees from Alpha Persei and obtained spectra for all of them. We confirm that three are massive white dwarfs sufficiently young to have originated in the cluster. All these are more massive than any white dwarf previously associated with a cluster using Gaia astrometry, and possess some of the most massive progenitors. In particular, the white dwarf Gaia EDR3 4395978097863572, which lies within 25 pc of the cluster center, has a mass of about 1.20 solar masses and evolved from an 8.5 solar-mass star, pushing the upper limit for white dwarf formation from a single massive star, while still leaving a substantial gap between the resulting white dwarf mass and the Chandrasekhar mass. article_number: L24 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: Pier-Emmanuel full_name: Tremblay, Pier-Emmanuel last_name: Tremblay citation: ama: Miller DR, Caiazzo I, Heyl J, Richer HB, Tremblay P-E. The ultramassive white dwarfs of the Alpha Persei cluster. The Astrophysical Journal Letters. 2022;926(2). doi:10.3847/2041-8213/ac50a5 apa: Miller, D. R., Caiazzo, I., Heyl, J., Richer, H. B., & Tremblay, P.-E. (2022). The ultramassive white dwarfs of the Alpha Persei cluster. The Astrophysical Journal Letters. American Astronomical Society. https://doi.org/10.3847/2041-8213/ac50a5 chicago: Miller, David R., Ilaria Caiazzo, Jeremy Heyl, Harvey B. Richer, and Pier-Emmanuel Tremblay. “The Ultramassive White Dwarfs of the Alpha Persei Cluster.” The Astrophysical Journal Letters. American Astronomical Society, 2022. https://doi.org/10.3847/2041-8213/ac50a5. ieee: D. R. Miller, I. Caiazzo, J. Heyl, H. B. Richer, and P.-E. Tremblay, “The ultramassive white dwarfs of the Alpha Persei cluster,” The Astrophysical Journal Letters, vol. 926, no. 2. American Astronomical Society, 2022. ista: Miller DR, Caiazzo I, Heyl J, Richer HB, Tremblay P-E. 2022. The ultramassive white dwarfs of the Alpha Persei cluster. The Astrophysical Journal Letters. 926(2), L24. mla: Miller, David R., et al. “The Ultramassive White Dwarfs of the Alpha Persei Cluster.” The Astrophysical Journal Letters, vol. 926, no. 2, L24, American Astronomical Society, 2022, doi:10.3847/2041-8213/ac50a5. short: D.R. Miller, I. Caiazzo, J. Heyl, H.B. Richer, P.-E. Tremblay, The Astrophysical Journal Letters 926 (2022). date_created: 2024-03-26T10:31:25Z date_published: 2022-02-21T00:00:00Z date_updated: 2024-04-02T07:27:20Z day: '21' doi: 10.3847/2041-8213/ac50a5 extern: '1' external_id: arxiv: - '2110.09668' fulldoi: https://doi.org/10.3847/2041-8213/ac50a5 intvolume: ' 926' 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/ac50a5 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: The ultramassive white dwarfs of the Alpha Persei 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: 926 year: '2022' ... --- _id: '15214' abstract: - lang: eng text: We search through an eight million cubic parsec volume surrounding the Pleiades star cluster and the Sun to identify both the current and past members of the Pleiades cluster within the Gaia EDR3 data set. We find nearly 1300 current cluster members and 289 former cluster candidates. Many of these candidates lie well in front of or behind the cluster from our point of view, so formerly they were considered cluster members, but their parallaxes put them more than 10 pc from the center of the cluster today. Over the past 100 Myr we estimate that the cluster has lost twenty percent of its mass including two massive white dwarf stars and the α2 Canum Venaticorum type variable star, 41 Tau. All three white dwarfs associated with the cluster are massive (1.01–1.06 M⊙) and have progenitors with main-sequence masses of about six solar masses. Although we did not associate any giant stars with the cluster, the cooling time of the oldest white dwarf of 60 Myr gives a firm lower limit on the age of the cluster. article_number: '132' 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: Harvey B. full_name: Richer, Harvey B. last_name: Richer citation: ama: Heyl J, Caiazzo I, Richer HB. Reconstructing the Pleiades with Gaia EDR3. The Astrophysical Journal. 2022;926(2). doi:10.3847/1538-4357/ac45fc apa: Heyl, J., Caiazzo, I., & Richer, H. B. (2022). Reconstructing the Pleiades with Gaia EDR3. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ac45fc chicago: Heyl, Jeremy, Ilaria Caiazzo, and Harvey B. Richer. “Reconstructing the Pleiades with Gaia EDR3.” The Astrophysical Journal. American Astronomical Society, 2022. https://doi.org/10.3847/1538-4357/ac45fc. ieee: J. Heyl, I. Caiazzo, and H. B. Richer, “Reconstructing the Pleiades with Gaia EDR3,” The Astrophysical Journal, vol. 926, no. 2. American Astronomical Society, 2022. ista: Heyl J, Caiazzo I, Richer HB. 2022. Reconstructing the Pleiades with Gaia EDR3. The Astrophysical Journal. 926(2), 132. mla: Heyl, Jeremy, et al. “Reconstructing the Pleiades with Gaia EDR3.” The Astrophysical Journal, vol. 926, no. 2, 132, American Astronomical Society, 2022, doi:10.3847/1538-4357/ac45fc. short: J. Heyl, I. Caiazzo, H.B. Richer, The Astrophysical Journal 926 (2022). date_created: 2024-03-26T10:31:44Z date_published: 2022-02-18T00:00:00Z date_updated: 2024-04-02T07:27:52Z day: '18' doi: 10.3847/1538-4357/ac45fc extern: '1' external_id: arxiv: - '2110.03837' fulldoi: https://doi.org/10.3847/1538-4357/ac45fc intvolume: ' 926' 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/ac45fc month: '02' 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: Reconstructing the Pleiades with Gaia EDR3 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: 926 year: '2022' ... --- _id: '15268' abstract: - lang: eng text: Apolipoprotein A‐I (apoA‐I) has a key function in the reverse cholesterol transport. However, aggregation of apoA‐I single point mutants can lead to hereditary amyloid pathology. Although several studies have tackled the biophysical and structural consequences introduced by these mutations, there is little information addressing the relationship between the evolutionary and structural features that contribute to the amyloid behavior of apoA‐I. We combined evolutionary studies, in silico mutagenesis and molecular dynamics (MD) simulations to provide a comprehensive analysis of the conservation and pathogenic role of the aggregation‐prone regions (APRs) present in apoA‐I. Sequence analysis demonstrated that among the four amyloidogenic regions described for human apoA‐I, only two (APR1 and APR4) are evolutionary conserved across different species of Sarcopterygii. Moreover, stability analysis carried out with the FoldX engine showed that APR1 contributes to the marginal stability of apoA‐I. Structural properties of full‐length apoA‐I models suggest that aggregation is avoided by placing APRs into highly packed and rigid portions of its native fold. Compared to silent variants extracted from the gnomAD database, the thermodynamic and pathogenic impact of amyloid mutations showed evidence of a higher destabilizing effect. MD simulations of the amyloid variant G26R evidenced the partial unfolding of the alpha‐helix bundle with the concomitant exposure of APR1 to the solvent, suggesting an insight into the early steps involved in its aggregation. Our findings highlight APR1 as a relevant component for apoA‐I structural integrity and emphasize a destabilizing effect of amyloid variants that leads to the exposure of this region. article_processing_charge: No article_type: original author: - first_name: Romina A. full_name: Gisonno, Romina A. last_name: Gisonno - first_name: Tomas full_name: Masson, Tomas id: 93ac43e8-8599-11eb-9b86-f6efb0a4c207 last_name: Masson orcid: 0000-0002-2634-6283 - first_name: Nahuel A. full_name: Ramella, Nahuel A. last_name: Ramella - first_name: Exequiel E. full_name: Barrera, Exequiel E. last_name: Barrera - first_name: Víctor full_name: Romanowski, Víctor last_name: Romanowski - first_name: M. Alejandra full_name: Tricerri, M. Alejandra last_name: Tricerri citation: ama: 'Gisonno RA, Masson T, Ramella NA, Barrera EE, Romanowski V, Tricerri MA. Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior. Proteins: Structure, Function, and Bioinformatics. 2022;90(1):258-269. doi:10.1002/prot.26217' apa: 'Gisonno, R. A., Masson, T., Ramella, N. A., Barrera, E. E., Romanowski, V., & Tricerri, M. A. (2022). Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior. Proteins: Structure, Function, and Bioinformatics. Wiley. https://doi.org/10.1002/prot.26217' chicago: 'Gisonno, Romina A., Tomas Masson, Nahuel A. Ramella, Exequiel E. Barrera, Víctor Romanowski, and M. Alejandra Tricerri. “Evolutionary and Structural Constraints Influencing Apolipoprotein A‐I Amyloid Behavior.” Proteins: Structure, Function, and Bioinformatics. Wiley, 2022. https://doi.org/10.1002/prot.26217.' ieee: 'R. A. Gisonno, T. Masson, N. A. Ramella, E. E. Barrera, V. Romanowski, and M. A. Tricerri, “Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior,” Proteins: Structure, Function, and Bioinformatics, vol. 90, no. 1. Wiley, pp. 258–269, 2022.' ista: 'Gisonno RA, Masson T, Ramella NA, Barrera EE, Romanowski V, Tricerri MA. 2022. Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior. Proteins: Structure, Function, and Bioinformatics. 90(1), 258–269.' mla: 'Gisonno, Romina A., et al. “Evolutionary and Structural Constraints Influencing Apolipoprotein A‐I Amyloid Behavior.” Proteins: Structure, Function, and Bioinformatics, vol. 90, no. 1, Wiley, 2022, pp. 258–69, doi:10.1002/prot.26217.' short: 'R.A. Gisonno, T. Masson, N.A. Ramella, E.E. Barrera, V. Romanowski, M.A. Tricerri, Proteins: Structure, Function, and Bioinformatics 90 (2022) 258–269.' corr_author: '1' date_created: 2024-04-03T07:49:53Z date_published: 2022-01-01T00:00:00Z date_updated: 2024-10-09T21:08:44Z day: '01' department: - _id: MaJö doi: 10.1002/prot.26217 external_id: pmid: - '34414600' fulldoi: https://doi.org/10.1002/prot.26217 intvolume: ' 90' issue: '1' keyword: - Molecular Biology - Biochemistry - Structural Biology language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1101/2020.09.18.304337 month: '01' oa: 1 oa_version: Preprint page: 258-269 pmid: 1 publication: 'Proteins: Structure, Function, and Bioinformatics' publication_identifier: eissn: - 1097-0134 issn: - 0887-3585 publication_status: published publisher: Wiley quality_controlled: '1' status: public title: Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 90 year: '2022' ... --- _id: '17057' abstract: - lang: eng text: Martin Loose studied chemistry at the University of Heidelberg, Germany. He then joined Petra Schwille's group at the Max Planck Institute of Molecular Cell Biology and Genetics in Dresden, where he obtained his PhD degree in 2010 for work on self-organization and pattern formation in the bacterial Min protein system. He then moved to Tim Mitchison's lab at Harvard Medical School, Boston, USA for his postdoc, funded by Human Frontier Science Program (HSFP) and European Molecular Biology Organization (EMBO) long-term fellowships; there, he discovered that the bacterial cell division proteins FtsA and FtsZ self-organize into dynamic cytoskeletal patterns. Martin established his independent research group at the Institute of Science and Technology (IST) Austria in 2015, supported by an European Research Council (ERC) starting grant and HFSP Young Investigator Grant. His lab studies the self-organization of bacterial cell division and small GTPase networks. article_number: jcs259715 article_processing_charge: No author: - first_name: Martin full_name: Loose, Martin id: 462D4284-F248-11E8-B48F-1D18A9856A87 last_name: Loose orcid: 0000-0001-7309-9724 citation: ama: Loose M. Cell Scientist to Watch – Martin Loose. Vol 135. The Company of Biologists; 2022. doi:10.1242/jcs.259715 apa: Loose, M. (2022). Cell scientist to watch – Martin Loose. Journal of Cell Science (Vol. 135). The Company of Biologists. https://doi.org/10.1242/jcs.259715 chicago: Loose, Martin. Cell Scientist to Watch – Martin Loose. Journal of Cell Science. Vol. 135. The Company of Biologists, 2022. https://doi.org/10.1242/jcs.259715. ieee: M. Loose, Cell scientist to watch – Martin Loose, vol. 135, no. 2. The Company of Biologists, 2022. ista: Loose M. 2022. Cell scientist to watch – Martin Loose, The Company of Biologists,p. mla: Loose, Martin. “Cell Scientist to Watch – Martin Loose.” Journal of Cell Science, vol. 135, no. 2, jcs259715, The Company of Biologists, 2022, doi:10.1242/jcs.259715. short: M. Loose, Cell Scientist to Watch – Martin Loose, The Company of Biologists, 2022. date_created: 2024-05-28T13:28:30Z date_published: 2022-01-19T00:00:00Z date_updated: 2026-06-18T17:51:26Z day: '19' ddc: - '570' department: - _id: MaLo doi: 10.1242/jcs.259715 external_id: isi: - '000762665200015' fulldoi: https://doi.org/10.1242/jcs.259715 intvolume: ' 135' isi: 1 issue: '2' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1242/jcs.259715 month: '01' oa: 1 oa_version: Published Version publication: Journal of Cell Science publication_identifier: eissn: - 1477-9137 issn: - 0021-9533 publication_status: published publisher: The Company of Biologists quality_controlled: '1' status: public title: Cell scientist to watch – Martin Loose type: other_academic_publication user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 135 year: '2022' ... --- _id: '17059' abstract: - lang: eng text: The recent focus on the efficiency of deep neural networks (DNNs) has led to significant work on model compression approaches, of which weight pruning is one of the most popular. At the same time, there is rapidly-growing computational support for efficiently executing the unstructured-sparse models obtained via pruning. Yet, most existing pruning methods minimize just the number of remaining weights, i.e. the size of the model, rather than optimizing for inference time. We address this gap by introducing SPDY, a new compression method which automatically determines layer-wise sparsity targets achieving a desired inference speedup on a given system, while minimizing accuracy loss. SPDY is the composition of two new techniques. The first is an efficient and general dynamic programming algorithm for solving constrained layer-wise compression problems, given a set of layer-wise error scores. The second technique is a local search procedure for automatically determining such scores in an accurate and robust manner. Experiments across popular vision and language models show that SPDY guarantees speedups while recovering higher accuracy relative to existing strategies, both for one-shot and gradual pruning scenarios, and is compatible with most existing pruning approaches. We also extend our approach to the recently-proposed task of pruning with very little data, where we achieve the best known accuracy recovery when pruning to the GPU-supported 2:4 sparsity pattern. acknowledgement: "We gratefully acknowledge funding from the European Research Council (ERC) under the European Union’s Horizon 2020 programme (grant agreement No 805223 ScaleML),\r\nas well as computational support from AWS EC2. We thank Eldar Kurtic for code and hyper-parameters for BERT pruning, and the Neural Magic Team, notably Michael Goin and\r\nMark Kurtz, for support with their software." alternative_title: - PMLR article_processing_charge: Yes author: - first_name: Elias full_name: Frantar, Elias id: 09a8f98d-ec99-11ea-ae11-c063a7b7fe5f last_name: Frantar - first_name: Dan-Adrian full_name: Alistarh, Dan-Adrian id: 4A899BFC-F248-11E8-B48F-1D18A9856A87 last_name: Alistarh orcid: 0000-0003-3650-940X citation: ama: 'Frantar E, Alistarh D-A. SPDY: Accurate pruning with speedup guarantees. In: 39th International Conference on Machine Learning. Vol 162. ML Research Press; 2022:6726-6743.' apa: 'Frantar, E., & Alistarh, D.-A. (2022). SPDY: Accurate pruning with speedup guarantees. In 39th International Conference on Machine Learning (Vol. 162, pp. 6726–6743). Baltimore, MD, United States: ML Research Press.' chicago: 'Frantar, Elias, and Dan-Adrian Alistarh. “SPDY: Accurate Pruning with Speedup Guarantees.” In 39th International Conference on Machine Learning, 162:6726–43. ML Research Press, 2022.' ieee: 'E. Frantar and D.-A. Alistarh, “SPDY: Accurate pruning with speedup guarantees,” in 39th International Conference on Machine Learning, Baltimore, MD, United States, 2022, vol. 162, pp. 6726–6743.' ista: 'Frantar E, Alistarh D-A. 2022. SPDY: Accurate pruning with speedup guarantees. 39th International Conference on Machine Learning. ICML: International Conference on Machine Learning, PMLR, vol. 162, 6726–6743.' mla: 'Frantar, Elias, and Dan-Adrian Alistarh. “SPDY: Accurate Pruning with Speedup Guarantees.” 39th International Conference on Machine Learning, vol. 162, ML Research Press, 2022, pp. 6726–43.' short: E. Frantar, D.-A. Alistarh, in:, 39th International Conference on Machine Learning, ML Research Press, 2022, pp. 6726–6743. conference: end_date: 2022-07-23 location: Baltimore, MD, United States name: 'ICML: International Conference on Machine Learning' start_date: 2022-07-17 corr_author: '1' date_created: 2024-05-28T13:45:20Z date_published: 2022-07-20T00:00:00Z date_updated: 2025-04-14T07:49:14Z day: '20' ddc: - '000' department: - _id: DaAl ec_funded: 1 external_id: isi: - '000922378801029' file: - access_level: open_access checksum: 5179a1e4dfc0fbfab6674907299e414a content_type: application/pdf creator: dernst date_created: 2024-08-19T06:54:41Z date_updated: 2024-08-19T06:54:41Z file_id: '17440' file_name: 2022_PMLR_Frantar.pdf file_size: 615916 relation: main_file success: 1 file_date_updated: 2024-08-19T06:54:41Z has_accepted_license: '1' intvolume: ' 162' isi: 1 language: - iso: eng month: '07' oa: 1 oa_version: Published Version page: 6726-6743 project: - _id: 268A44D6-B435-11E9-9278-68D0E5697425 call_identifier: H2020 grant_number: '805223' name: Elastic Coordination for Scalable Machine Learning publication: 39th International Conference on Machine Learning publication_status: published publisher: ML Research Press quality_controlled: '1' scopus_import: '1' status: public title: 'SPDY: Accurate pruning with speedup guarantees' tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 162 year: '2022' ... --- _id: '17060' abstract: - lang: eng text: "Payment channel networks (PCNs) are one of the most prominent solutions to the limited transaction throughput of blockchains. Nevertheless, PCNs suffer themselves from a throughput limitation due to the capital constraints of their channels. A similar dependence on high capital is also found in inter-bank payment settlements, where the so-called netting technique is used to mitigate liquidity demands.\r\nIn this work, we alleviate this limitation by introducing the notion of transaction aggregation: instead of executing transactions sequentially through a PCN, we enable senders to aggregate multiple transactions and execute them simultaneously to benefit from several amounts that may \"cancel out\". Two direct advantages of our proposal is the decrease in intermediary fees paid by senders as well as the obfuscation of the transaction data from the intermediaries.\r\nWe formulate the transaction aggregation as a computational problem, a generalization of the Bank Clearing Problem. We present a generic framework for the transaction aggregation execution, and thereafter we propose Wiser as an implementation of this framework in a specific hub-based setting. To overcome the NP-hardness of the transaction aggregation problem, in Wiser we propose a fixed-parameter linear algorithm for a special case of transaction aggregation as well as the Bank Clearing Problem. Wiser can also be seen as a modern variant of the Hawala money transfer system, as well as a decentralized implementation of the overseas remittance service of Wise." acknowledgement: "This work was supported partially by ERC Starting Grant QIP–805241, by the Vienna business agency (Wirtschaftsagentur) through the Vienna Cybersecurity and Privacy Research Center\r\n(ViSP) and by the Austrian Science Fund (FWF) project I 4800-N (ADVISE).\r\nThe first author would like to thank Daniel Dadush for suggesting the use of discrepancy techniques to solve the transaction aggregation problem." article_processing_charge: Yes (in subscription journal) arxiv: 1 author: - first_name: Samarth full_name: Tiwari, Samarth last_name: Tiwari - first_name: Michelle X full_name: Yeo, Michelle X id: 2D82B818-F248-11E8-B48F-1D18A9856A87 last_name: Yeo orcid: 0009-0001-3676-4809 - first_name: Zeta full_name: Avarikioti, Zeta last_name: Avarikioti - first_name: Iosif full_name: Salem, Iosif last_name: Salem - first_name: Krzysztof Z full_name: Pietrzak, Krzysztof Z id: 3E04A7AA-F248-11E8-B48F-1D18A9856A87 last_name: Pietrzak orcid: 0000-0002-9139-1654 - first_name: Stefan full_name: Schmid, Stefan last_name: Schmid citation: ama: 'Tiwari S, Yeo MX, Avarikioti Z, Salem I, Pietrzak KZ, Schmid S. Wiser: Increasing throughput in payment channel networks with transaction aggregation. In: Proceedings of the 4th ACM Conference on Advances in Financial Technologies. Association for Computing Machinery; 2022:217-231. doi:10.1145/3558535.3559775' apa: 'Tiwari, S., Yeo, M. X., Avarikioti, Z., Salem, I., Pietrzak, K. Z., & Schmid, S. (2022). Wiser: Increasing throughput in payment channel networks with transaction aggregation. In Proceedings of the 4th ACM Conference on Advances in Financial Technologies (pp. 217–231). Cambridge, MA, United States: Association for Computing Machinery. https://doi.org/10.1145/3558535.3559775' chicago: 'Tiwari, Samarth, Michelle X Yeo, Zeta Avarikioti, Iosif Salem, Krzysztof Z Pietrzak, and Stefan Schmid. “Wiser: Increasing Throughput in Payment Channel Networks with Transaction Aggregation.” In Proceedings of the 4th ACM Conference on Advances in Financial Technologies, 217–31. Association for Computing Machinery, 2022. https://doi.org/10.1145/3558535.3559775.' ieee: 'S. Tiwari, M. X. Yeo, Z. Avarikioti, I. Salem, K. Z. Pietrzak, and S. Schmid, “Wiser: Increasing throughput in payment channel networks with transaction aggregation,” in Proceedings of the 4th ACM Conference on Advances in Financial Technologies, Cambridge, MA, United States, 2022, pp. 217–231.' ista: 'Tiwari S, Yeo MX, Avarikioti Z, Salem I, Pietrzak KZ, Schmid S. 2022. Wiser: Increasing throughput in payment channel networks with transaction aggregation. Proceedings of the 4th ACM Conference on Advances in Financial Technologies. AFT: Conference on Advances in Financial Technologies, 217–231.' mla: 'Tiwari, Samarth, et al. “Wiser: Increasing Throughput in Payment Channel Networks with Transaction Aggregation.” Proceedings of the 4th ACM Conference on Advances in Financial Technologies, Association for Computing Machinery, 2022, pp. 217–31, doi:10.1145/3558535.3559775.' short: S. Tiwari, M.X. Yeo, Z. Avarikioti, I. Salem, K.Z. Pietrzak, S. Schmid, in:, Proceedings of the 4th ACM Conference on Advances in Financial Technologies, Association for Computing Machinery, 2022, pp. 217–231. conference: end_date: 2022-09-21 location: Cambridge, MA, United States name: 'AFT: Conference on Advances in Financial Technologies' start_date: 2022-09-19 date_created: 2024-05-28T13:58:35Z date_published: 2022-09-19T00:00:00Z date_updated: 2025-09-10T09:57:48Z day: '19' ddc: - '000' department: - _id: KrPi doi: 10.1145/3558535.3559775 external_id: arxiv: - '2205.11597' isi: - '001041852800015' file: - access_level: open_access checksum: 54a7d405f8e57dba24728599ca63818c content_type: application/pdf creator: dernst date_created: 2024-08-19T06:45:21Z date_updated: 2024-08-19T06:45:21Z file_id: '17439' file_name: 2022_AFT_Tiwari.pdf file_size: 574728 relation: main_file success: 1 file_date_updated: 2024-08-19T06:45:21Z fulldoi: https://doi.org/10.1145/3558535.3559775 has_accepted_license: '1' isi: 1 language: - iso: eng month: '09' oa: 1 oa_version: Published Version page: 217-231 publication: Proceedings of the 4th ACM Conference on Advances in Financial Technologies publication_identifier: isbn: - '9781450398619' publication_status: published publisher: Association for Computing Machinery quality_controlled: '1' scopus_import: '1' status: public title: 'Wiser: Increasing throughput in payment channel networks with transaction aggregation' tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: conference user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 year: '2022' ... --- _id: '17061' abstract: - lang: eng text: Across many domains of interaction, both natural and artificial, individuals use past experience to shape future behaviors. The results of such learning processes depend on what individuals wish to maximize. A natural objective is one’s own success. However, when two such “selfish” learners interact with each other, the outcome can be detrimental to both, especially when there are conflicts of interest. Here, we explore how a learner can align incentives with a selfish opponent. Moreover, we consider the dynamics that arise when learning rules themselves are subject to evolutionary pressure. By combining extensive simulations and analytical techniques, we demonstrate that selfish learning is unstable in most classical two-player repeated games. If evolution operates on the level of long-run payoffs, selection instead favors learning rules that incorporate social (other-regarding) preferences. To further corroborate these results, we analyze data from a repeated prisoner’s dilemma experiment. We find that selfish learning is insufficient to explain human behavior when there is a trade-off between payoff maximization and fairness. acknowledgement: The authors are grateful to Jörg Oechssler for many helpful comments. A.M. was supported by a Simons Postdoctoral Fellowship (Math+X) at the University of Pennsylvania; K.C. was supported by the European Research Council Consolidator Grant 863818 (ForM-SMArt); and C.H. was supported by the European Research Council Starting Grant 850529 (E-DIRECT). article_number: pgac141 article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Alex full_name: McAvoy, Alex last_name: McAvoy - first_name: Julian full_name: Kates-Harbeck, Julian last_name: Kates-Harbeck - first_name: Krishnendu full_name: Chatterjee, Krishnendu id: 2E5DCA20-F248-11E8-B48F-1D18A9856A87 last_name: Chatterjee orcid: 0000-0002-4561-241X - first_name: Christian full_name: Hilbe, Christian id: 2FDF8F3C-F248-11E8-B48F-1D18A9856A87 last_name: Hilbe orcid: 0000-0001-5116-955X citation: ama: McAvoy A, Kates-Harbeck J, Chatterjee K, Hilbe C. Evolutionary instability of selfish learning in repeated games. PNAS Nexus. 2022;1(4). doi:10.1093/pnasnexus/pgac141 apa: McAvoy, A., Kates-Harbeck, J., Chatterjee, K., & Hilbe, C. (2022). Evolutionary instability of selfish learning in repeated games. PNAS Nexus. Oxford University Press. https://doi.org/10.1093/pnasnexus/pgac141 chicago: McAvoy, Alex, Julian Kates-Harbeck, Krishnendu Chatterjee, and Christian Hilbe. “Evolutionary Instability of Selfish Learning in Repeated Games.” PNAS Nexus. Oxford University Press, 2022. https://doi.org/10.1093/pnasnexus/pgac141. ieee: A. McAvoy, J. Kates-Harbeck, K. Chatterjee, and C. Hilbe, “Evolutionary instability of selfish learning in repeated games,” PNAS Nexus, vol. 1, no. 4. Oxford University Press, 2022. ista: McAvoy A, Kates-Harbeck J, Chatterjee K, Hilbe C. 2022. Evolutionary instability of selfish learning in repeated games. PNAS Nexus. 1(4), pgac141. mla: McAvoy, Alex, et al. “Evolutionary Instability of Selfish Learning in Repeated Games.” PNAS Nexus, vol. 1, no. 4, pgac141, Oxford University Press, 2022, doi:10.1093/pnasnexus/pgac141. short: A. McAvoy, J. Kates-Harbeck, K. Chatterjee, C. Hilbe, PNAS Nexus 1 (2022). date_created: 2024-05-28T14:23:12Z date_published: 2022-09-01T00:00:00Z date_updated: 2025-06-11T13:54:20Z day: '01' ddc: - '000' department: - _id: KrCh doi: 10.1093/pnasnexus/pgac141 ec_funded: 1 external_id: arxiv: - '2105.06199' pmid: - '36714856' file: - access_level: open_access checksum: 79a8e3e4be7e8a2b407b4efddd65f3f3 content_type: application/pdf creator: dernst date_created: 2024-08-06T07:33:30Z date_updated: 2024-08-06T07:33:30Z file_id: '17400' file_name: 2022_PNASNexus_McAvoy.pdf file_size: 2410962 relation: main_file success: 1 file_date_updated: 2024-08-06T07:33:30Z fulldoi: https://doi.org/10.1093/pnasnexus/pgac141 has_accepted_license: '1' intvolume: ' 1' issue: '4' language: - iso: eng month: '09' oa: 1 oa_version: Published Version pmid: 1 project: - _id: 0599E47C-7A3F-11EA-A408-12923DDC885E call_identifier: H2020 grant_number: '863818' name: 'Formal Methods for Stochastic Models: Algorithms and Applications' publication: PNAS Nexus publication_identifier: issn: - 2752-6542 publication_status: published publisher: Oxford University Press quality_controlled: '1' related_material: link: - relation: software url: https://github.com/alexmcavoy/fmtl/ scopus_import: '1' status: public title: Evolutionary instability of selfish learning in repeated games 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: 1 year: '2022' ... --- _id: '17065' abstract: - lang: eng text: Past work on optimizing fabrication plans given a carpentry design can provide Pareto-optimal plans trading off between material waste, fabrication time, precision, and other considerations. However, when developing fabrication plans, experts rarely restrict to a single design, instead considering families of design variations, sometimes adjusting designs to simplify fabrication. Jointly exploring the design and fabrication plan spaces for each design is intractable using current techniques. We present a new approach to jointly optimize design and fabrication plans for carpentered objects. To make this bi-level optimization tractable, we adapt recent work from program synthesis based on equality graphs (e-graphs), which encode sets of equivalent programs. Our insight is that subproblems within our bi-level problem share significant substructures. By representing both designs and fabrication plans in a new bag of parts (BOP) e-graph, we amortize the cost of optimizing design components shared among multiple candidates. Even using BOP e-graphs, the optimization space grows quickly in practice. Hence, we also show how a feedback-guided search strategy dubbed Iterative Contraction and Expansion on E-graphs (ICEE) can keep the size of the e-graph manageable and direct the search towards promising candidates. We illustrate the advantages of our pipeline through examples from the carpentry domain. acknowledgement: The authors would like to thank anonymous reviewers for their helpful feedback; Haomiao Wu for her contribution to the algorithm development in the early stage of the project; Elias Baldwin, David Tsay, Alexander Lefort, and Qiyang Tan for helping the experiments. article_number: '32' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Haisen full_name: Zhao, Haisen id: fb7f793a-80d1-11eb-8869-d56e5b2a8ff4 last_name: Zhao orcid: 0000-0002-6389-1045 - first_name: Max full_name: Willsey, Max last_name: Willsey - first_name: Amy full_name: Zhu, Amy last_name: Zhu - first_name: Chandrakana full_name: Nandi, Chandrakana last_name: Nandi - first_name: Zachary full_name: Tatlock, Zachary last_name: Tatlock - first_name: Justin full_name: Solomon, Justin last_name: Solomon - first_name: Adriana full_name: Schulz, Adriana last_name: Schulz citation: ama: Zhao H, Willsey M, Zhu A, et al. Co-optimization of design and fabrication plans for carpentry. ACM Transactions on Graphics. 2022;41(3). doi:10.1145/3508499 apa: Zhao, H., Willsey, M., Zhu, A., Nandi, C., Tatlock, Z., Solomon, J., & Schulz, A. (2022). Co-optimization of design and fabrication plans for carpentry. ACM Transactions on Graphics. Association for Computing Machinery. https://doi.org/10.1145/3508499 chicago: Zhao, Haisen, Max Willsey, Amy Zhu, Chandrakana Nandi, Zachary Tatlock, Justin Solomon, and Adriana Schulz. “Co-Optimization of Design and Fabrication Plans for Carpentry.” ACM Transactions on Graphics. Association for Computing Machinery, 2022. https://doi.org/10.1145/3508499. ieee: H. Zhao et al., “Co-optimization of design and fabrication plans for carpentry,” ACM Transactions on Graphics, vol. 41, no. 3. Association for Computing Machinery, 2022. ista: Zhao H, Willsey M, Zhu A, Nandi C, Tatlock Z, Solomon J, Schulz A. 2022. Co-optimization of design and fabrication plans for carpentry. ACM Transactions on Graphics. 41(3), 32. mla: Zhao, Haisen, et al. “Co-Optimization of Design and Fabrication Plans for Carpentry.” ACM Transactions on Graphics, vol. 41, no. 3, 32, Association for Computing Machinery, 2022, doi:10.1145/3508499. short: H. Zhao, M. Willsey, A. Zhu, C. Nandi, Z. Tatlock, J. Solomon, A. Schulz, ACM Transactions on Graphics 41 (2022). date_created: 2024-05-29T06:09:23Z date_published: 2022-03-09T00:00:00Z date_updated: 2024-08-06T07:03:14Z day: '09' department: - _id: BeBi doi: 10.1145/3508499 external_id: arxiv: - '2107.12265' fulldoi: https://doi.org/10.1145/3508499 intvolume: ' 41' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.2107.12265 month: '03' oa: 1 oa_version: Preprint publication: ACM Transactions on Graphics publication_identifier: eissn: - 1557-7368 issn: - 0730-0301 publication_status: published publisher: Association for Computing Machinery quality_controlled: '1' scopus_import: '1' status: public title: Co-optimization of design and fabrication plans for carpentry type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 41 year: '2022' ... --- _id: '17066' abstract: - lang: eng text: A cell’s size affects the likelihood that it will die. But how is cell size controlled in this context and how does cell size impact commitment to the cell death fate? We present evidence that the caspase CED-3 interacts with the RhoGEF ECT-2 in Caenorhabditis elegans neuroblasts that generate “unwanted” cells. We propose that this interaction promotes polar actomyosin contractility, which leads to unequal neuroblast division and the generation of a daughter cell that is below the critical “lethal” size threshold. Furthermore, we find that hyperactivation of ECT-2 RhoGEF reduces the sizes of unwanted cells. Importantly, this suppresses the “cell death abnormal” phenotype caused by the partial loss of ced-3 caspase and therefore increases the likelihood that unwanted cells die. A putative null mutation of ced-3 caspase, however, is not suppressed, which indicates that cell size affects CED-3 caspase activation and/or activity. Therefore, we have uncovered novel sequential and reciprocal interactions between the apoptosis pathway and cell size that impact a cell’s commitment to the cell death fate. acknowledgement: "We thank members of the Conradt, Lambie, and Hajnal labs for discussions and comments on the manuscript. We thank M. Bauer, L. Jocham, N. Lebedeva, and L. McGuinness for excellent technical support; A. Hajnal and T. Kohlbrenner (University of Zurich, Switzerland) for allele zh135; and H.R. Horvitz (Massachusetts of Technology, USA) for plasmid pET-CED-3.\r\nSome strains were provided by the Caenorhabditis Genetics Center (CGC), which is funded by NIH Office of Research Infrastructure Programs (https://orip.nih.gov/) (P40 OD010440). This work was supported by UCL (Capital Equipment Fund, CEF2), a predoctoral fellowship from the China Scholarship Council (https://www.csc.edu.cn/) to HW, a predoctoral fellowship from the Studienstiftung des Deutschen Volkes (https://www.studienstiftung.de/) to NM, a Wolfson Fellowship from the Royal Society (https://royalsociety.org/) to BC (RSWF\\R1\\180008), the Deutsche Forschungsgemeinschaft (https://www.dfg.de/en/index.jsp) (ZA619/3-1 and ZA619/3-2 to EZ; C0204/10-1 and EXC114 to BC), and the Biotechnology and Biological Sciences Research Council (https://bbsrc.ukri.org/) (BB/V007572/1 to BC). " article_number: e3001786 article_processing_charge: Yes article_type: original author: - first_name: Aditya full_name: Sethi, Aditya last_name: Sethi - first_name: Hai full_name: Wei, Hai last_name: Wei - first_name: Nikhil full_name: Mishra, Nikhil id: C4D70E82-1081-11EA-B3ED-9A4C3DDC885E last_name: Mishra orcid: 0000-0002-6425-5788 - first_name: Ioannis full_name: Segos, Ioannis last_name: Segos - first_name: Eric J. full_name: Lambie, Eric J. last_name: Lambie - first_name: Esther full_name: Zanin, Esther last_name: Zanin - first_name: Barbara full_name: Conradt, Barbara last_name: Conradt citation: ama: Sethi A, Wei H, Mishra N, et al. A caspase–RhoGEF axis contributes to the cell size threshold for apoptotic death in developing Caenorhabditis elegans. PLOS Biology. 2022;20(10). doi:10.1371/journal.pbio.3001786 apa: Sethi, A., Wei, H., Mishra, N., Segos, I., Lambie, E. J., Zanin, E., & Conradt, B. (2022). A caspase–RhoGEF axis contributes to the cell size threshold for apoptotic death in developing Caenorhabditis elegans. PLOS Biology. Public Library of Science. https://doi.org/10.1371/journal.pbio.3001786 chicago: Sethi, Aditya, Hai Wei, Nikhil Mishra, Ioannis Segos, Eric J. Lambie, Esther Zanin, and Barbara Conradt. “A Caspase–RhoGEF Axis Contributes to the Cell Size Threshold for Apoptotic Death in Developing Caenorhabditis Elegans.” PLOS Biology. Public Library of Science, 2022. https://doi.org/10.1371/journal.pbio.3001786. ieee: A. Sethi et al., “A caspase–RhoGEF axis contributes to the cell size threshold for apoptotic death in developing Caenorhabditis elegans,” PLOS Biology, vol. 20, no. 10. Public Library of Science, 2022. ista: Sethi A, Wei H, Mishra N, Segos I, Lambie EJ, Zanin E, Conradt B. 2022. A caspase–RhoGEF axis contributes to the cell size threshold for apoptotic death in developing Caenorhabditis elegans. PLOS Biology. 20(10), e3001786. mla: Sethi, Aditya, et al. “A Caspase–RhoGEF Axis Contributes to the Cell Size Threshold for Apoptotic Death in Developing Caenorhabditis Elegans.” PLOS Biology, vol. 20, no. 10, e3001786, Public Library of Science, 2022, doi:10.1371/journal.pbio.3001786. short: A. Sethi, H. Wei, N. Mishra, I. Segos, E.J. Lambie, E. Zanin, B. Conradt, PLOS Biology 20 (2022). date_created: 2024-05-29T06:09:34Z date_published: 2022-10-06T00:00:00Z date_updated: 2024-08-06T07:08:54Z day: '06' ddc: - '570' department: - _id: CaHe doi: 10.1371/journal.pbio.3001786 external_id: pmid: - '36201522' file: - access_level: open_access checksum: a7b46460b7819c196028481cc18a7c85 content_type: application/pdf creator: dernst date_created: 2024-08-06T07:07:52Z date_updated: 2024-08-06T07:07:52Z file_id: '17399' file_name: 2022_PlosBio_Sethi.pdf file_size: 2515388 relation: main_file success: 1 file_date_updated: 2024-08-06T07:07:52Z fulldoi: https://doi.org/10.1371/journal.pbio.3001786 has_accepted_license: '1' intvolume: ' 20' issue: '10' language: - iso: eng month: '10' oa: 1 oa_version: Published Version pmid: 1 publication: PLOS Biology publication_identifier: issn: - 1545-7885 publication_status: published publisher: Public Library of Science quality_controlled: '1' scopus_import: '1' status: public title: A caspase–RhoGEF axis contributes to the cell size threshold for apoptotic death in developing Caenorhabditis elegans 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: 20 year: '2022' ... --- _id: '17067' abstract: - lang: eng text: 'Human doublecortin (DCX) mutations are associated with severe brain malformations leading to aberrant neuron positioning (heterotopia), intellectual disability and epilepsy. DCX is a microtubule-associated protein which plays a key role during neurodevelopment in neuronal migration and differentiation. Dcx knockout (KO) mice show disorganized hippocampal pyramidal neurons. The CA2/CA3 pyramidal cell layer is present as two abnormal layers and disorganized CA3 KO pyramidal neurons are also more excitable than wild-type (WT) cells. To further identify abnormalities, we characterized Dcx KO hippocampal neurons at subcellular, molecular and ultrastructural levels. Severe defects were observed in mitochondria, affecting number and distribution. Also, the Golgi apparatus was visibly abnormal, increased in volume and abnormally organized. Transcriptome analyses from laser microdissected hippocampal tissue at postnatal day 60 (P60) highlighted organelle abnormalities. Ultrastructural studies of CA3 cells performed in P60 (young adult) and > 9 months (mature) tissue showed that organelle defects are persistent throughout life. Locomotor activity and fear memory of young and mature adults were also abnormal: Dcx KO mice consistently performed less well than WT littermates, with defects becoming more severe with age. Thus, we show that disruption of a neurodevelopmentally-regulated gene can lead to permanent organelle anomalies contributing to abnormal adult behavior.' acknowledgement: "We thank Sylvie Dumont for initial aid with laser microdissection and G. Martinez-Lorenzana for experimental help with electron microscopy. We thank the animal experimentation facility and cellular and tissue imaging platforms at the Institut du Fer à Moulin, supported also by the Région Ile de France and the FRC Rotary. The Francis lab was associated with the BioPsy Labex project and the Ecole des Neurosciences de Paris Ile-de-France (ENP) network. Our salaries and lab were supported by Inserm, the Centre national de la recherche scientifique (CNRS) and Sorbonne University. The Francis group obtained the following funding contributing to this project: the European Union (EU- HEALTH-2013, DESIRE, N° 60253), the JTC 2015 Neurodevelopmental Disorders affiliated with the French Agence National de la Recherche (for \r\nNEURON8-Full- 815-006 STEM-MCD, to FF), E-Rare-3, the ERA-Net for Research on Rare Diseases affiliated with the French ANR (ERARE18-049), the European Cooperation on Science and Technology (COST Action CA16118)." article_number: '105702' article_processing_charge: Yes article_type: original author: - first_name: Melissa A full_name: Stouffer, Melissa A id: 4C9372C4-F248-11E8-B48F-1D18A9856A87 last_name: Stouffer - first_name: R. full_name: Khalaf-Nazzal, R. last_name: Khalaf-Nazzal - first_name: C. full_name: Cifuentes-Diaz, C. last_name: Cifuentes-Diaz - first_name: G. full_name: Albertini, G. last_name: Albertini - first_name: E. full_name: Bandet, E. last_name: Bandet - first_name: G. full_name: Grannec, G. last_name: Grannec - first_name: V. full_name: Lavilla, V. last_name: Lavilla - first_name: J.-F. full_name: Deleuze, J.-F. last_name: Deleuze - first_name: R. full_name: Olaso, R. last_name: Olaso - first_name: M. full_name: Nosten-Bertrand, M. last_name: Nosten-Bertrand - first_name: F. full_name: Francis, F. last_name: Francis citation: ama: Stouffer MA, Khalaf-Nazzal R, Cifuentes-Diaz C, et al. Doublecortin mutation leads to persistent defects in the Golgi apparatus and mitochondria in adult hippocampal pyramidal cells. Neurobiology of Disease. 2022;168. doi:10.1016/j.nbd.2022.105702 apa: Stouffer, M. A., Khalaf-Nazzal, R., Cifuentes-Diaz, C., Albertini, G., Bandet, E., Grannec, G., … Francis, F. (2022). Doublecortin mutation leads to persistent defects in the Golgi apparatus and mitochondria in adult hippocampal pyramidal cells. Neurobiology of Disease. Elsevier. https://doi.org/10.1016/j.nbd.2022.105702 chicago: Stouffer, Melissa A, R. Khalaf-Nazzal, C. Cifuentes-Diaz, G. Albertini, E. Bandet, G. Grannec, V. Lavilla, et al. “Doublecortin Mutation Leads to Persistent Defects in the Golgi Apparatus and Mitochondria in Adult Hippocampal Pyramidal Cells.” Neurobiology of Disease. Elsevier, 2022. https://doi.org/10.1016/j.nbd.2022.105702. ieee: M. A. Stouffer et al., “Doublecortin mutation leads to persistent defects in the Golgi apparatus and mitochondria in adult hippocampal pyramidal cells,” Neurobiology of Disease, vol. 168. Elsevier, 2022. ista: Stouffer MA, Khalaf-Nazzal R, Cifuentes-Diaz C, Albertini G, Bandet E, Grannec G, Lavilla V, Deleuze J-F, Olaso R, Nosten-Bertrand M, Francis F. 2022. Doublecortin mutation leads to persistent defects in the Golgi apparatus and mitochondria in adult hippocampal pyramidal cells. Neurobiology of Disease. 168, 105702. mla: Stouffer, Melissa A., et al. “Doublecortin Mutation Leads to Persistent Defects in the Golgi Apparatus and Mitochondria in Adult Hippocampal Pyramidal Cells.” Neurobiology of Disease, vol. 168, 105702, Elsevier, 2022, doi:10.1016/j.nbd.2022.105702. short: M.A. Stouffer, R. Khalaf-Nazzal, C. Cifuentes-Diaz, G. Albertini, E. Bandet, G. Grannec, V. Lavilla, J.-F. Deleuze, R. Olaso, M. Nosten-Bertrand, F. Francis, Neurobiology of Disease 168 (2022). date_created: 2024-05-29T06:10:05Z date_published: 2022-06-15T00:00:00Z date_updated: 2024-08-06T06:57:39Z day: '15' ddc: - '570' department: - _id: SiHi doi: 10.1016/j.nbd.2022.105702 external_id: pmid: - '35339680' file: - access_level: open_access checksum: b705d3d23d0b424ba29920be7ab64c23 content_type: application/pdf creator: dernst date_created: 2024-08-06T06:54:24Z date_updated: 2024-08-06T06:54:24Z file_id: '17398' file_name: 2022_NeurobioDisease_Stouffer.pdf file_size: 8890818 relation: main_file success: 1 file_date_updated: 2024-08-06T06:54:24Z fulldoi: https://doi.org/10.1016/j.nbd.2022.105702 has_accepted_license: '1' intvolume: ' 168' language: - iso: eng license: https://creativecommons.org/licenses/by-nc-nd/4.0/ month: '06' oa: 1 oa_version: Published Version pmid: 1 publication: Neurobiology of Disease publication_identifier: issn: - 0969-9961 publication_status: published publisher: Elsevier quality_controlled: '1' scopus_import: '1' status: public title: Doublecortin mutation leads to persistent defects in the Golgi apparatus and mitochondria in adult hippocampal pyramidal cells 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: 168 year: '2022' ... --- _id: '17068' abstract: - lang: eng text: In plants, the antagonism between growth and defense is hardwired by hormonal signaling. The perception of pathogen-associated molecular patterns (PAMPs) from invading microorganisms inhibits auxin signaling and plant growth. Conversely, pathogens manipulate auxin signaling to promote disease, but how this hormone inhibits immunity is not fully understood. Ustilago maydis is a maize pathogen that induces auxin signaling in its host. We characterized a U. maydis effector protein, Naked1 (Nkd1), that is translocated into the host nucleus. Through its native ethylene-responsive element binding factor-associated amphiphilic repression (EAR) motif, Nkd1 binds to the transcriptional co-repressors TOPLESS/TOPLESS-related (TPL/TPRs) and prevents the recruitment of a transcriptional repressor involved in hormonal signaling, leading to the de-repression of auxin and jasmonate signaling and thereby promoting susceptibility to (hemi)biotrophic pathogens. A moderate upregulation of auxin signaling inhibits the PAMP-triggered reactive oxygen species (ROS) burst, an early defense response. Thus, our findings establish a clear mechanism for auxin-induced pathogen susceptibility. Engineered Nkd1 variants with increased expression or increased EAR-mediated TPL/TPR binding trigger typical salicylic-acid-mediated defense reactions, leading to pathogen resistance. This implies that moderate binding of Nkd1 to TPL is a result of a balancing evolutionary selection process to enable TPL manipulation while avoiding host recognition. acknowledgement: "The research leading to these results received funding from the European Research Council under the European Union Seventh Framework Programme ERC-2013-STG grant agreement \r\n335691; the Austrian Science Fund (FWF) P27818-B22,I 3033-B22; the Austrian Academy of Sciences (OEAW); and the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy - EXC 2070-390732324.\r\nWe would like to thank the GMI/IMBA/IMP core facilities for excellent technical support, especially the BioOptics and Molecular Biology Services. We thank the Plant Sciences and Next Generation Sequencing Facilities at the Vienna BioCenter Core Facilities GmbH (VBCF). We are grateful to the Jirí Friml and Jürgen Kleine-Vehn laboratories for providing useful A. thaliana lines. We thank Mathias Madalinski for peptide synthesis and Dr. J. Matthew Watson for proofreading and valuable feedback on the manuscript. The authors declare no competing interests." article_number: '100269' article_processing_charge: Yes article_type: original author: - first_name: Fernando full_name: Navarrete, Fernando last_name: Navarrete - first_name: Michelle C full_name: Gallei, Michelle C id: 35A03822-F248-11E8-B48F-1D18A9856A87 last_name: Gallei orcid: 0000-0003-1286-7368 - first_name: Aleksandra E. full_name: Kornienko, Aleksandra E. last_name: Kornienko - first_name: Indira full_name: Saado, Indira last_name: Saado - first_name: Mamoona full_name: Khan, Mamoona last_name: Khan - first_name: Khong-Sam full_name: Chia, Khong-Sam last_name: Chia - first_name: Martin A. full_name: Darino, Martin A. last_name: Darino - first_name: Janos full_name: Bindics, Janos last_name: Bindics - first_name: Armin full_name: Djamei, Armin last_name: Djamei citation: ama: Navarrete F, Gallei MC, Kornienko AE, et al. TOPLESS promotes plant immunity by repressing auxin signaling and is targeted by the fungal effector Naked1. Plant Communications. 2022;3(2). doi:10.1016/j.xplc.2021.100269 apa: Navarrete, F., Gallei, M. C., Kornienko, A. E., Saado, I., Khan, M., Chia, K.-S., … Djamei, A. (2022). TOPLESS promotes plant immunity by repressing auxin signaling and is targeted by the fungal effector Naked1. Plant Communications. Elsevier. https://doi.org/10.1016/j.xplc.2021.100269 chicago: Navarrete, Fernando, Michelle C Gallei, Aleksandra E. Kornienko, Indira Saado, Mamoona Khan, Khong-Sam Chia, Martin A. Darino, Janos Bindics, and Armin Djamei. “TOPLESS Promotes Plant Immunity by Repressing Auxin Signaling and Is Targeted by the Fungal Effector Naked1.” Plant Communications. Elsevier, 2022. https://doi.org/10.1016/j.xplc.2021.100269. ieee: F. Navarrete et al., “TOPLESS promotes plant immunity by repressing auxin signaling and is targeted by the fungal effector Naked1,” Plant Communications, vol. 3, no. 2. Elsevier, 2022. ista: Navarrete F, Gallei MC, Kornienko AE, Saado I, Khan M, Chia K-S, Darino MA, Bindics J, Djamei A. 2022. TOPLESS promotes plant immunity by repressing auxin signaling and is targeted by the fungal effector Naked1. Plant Communications. 3(2), 100269. mla: Navarrete, Fernando, et al. “TOPLESS Promotes Plant Immunity by Repressing Auxin Signaling and Is Targeted by the Fungal Effector Naked1.” Plant Communications, vol. 3, no. 2, 100269, Elsevier, 2022, doi:10.1016/j.xplc.2021.100269. short: F. Navarrete, M.C. Gallei, A.E. Kornienko, I. Saado, M. Khan, K.-S. Chia, M.A. Darino, J. Bindics, A. Djamei, Plant Communications 3 (2022). date_created: 2024-05-29T06:10:22Z date_published: 2022-03-14T00:00:00Z date_updated: 2024-08-05T10:27:03Z day: '14' ddc: - '580' department: - _id: JiFr doi: 10.1016/j.xplc.2021.100269 external_id: pmid: - '35529945' file: - access_level: open_access checksum: 1eeb6ee65419e4aa34627fea6857f343 content_type: application/pdf creator: dernst date_created: 2024-08-05T10:26:29Z date_updated: 2024-08-05T10:26:29Z file_id: '17393' file_name: 2022_PlantComm_Navarrete.pdf file_size: 3216686 relation: main_file success: 1 file_date_updated: 2024-08-05T10:26:29Z fulldoi: https://doi.org/10.1016/j.xplc.2021.100269 has_accepted_license: '1' intvolume: ' 3' issue: '2' language: - iso: eng month: '03' oa: 1 oa_version: Published Version pmid: 1 publication: Plant Communications publication_identifier: issn: - 2590-3462 publication_status: published publisher: Elsevier quality_controlled: '1' scopus_import: '1' status: public title: TOPLESS promotes plant immunity by repressing auxin signaling and is targeted by the fungal effector Naked1 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: 3 year: '2022' ...