دورية أكاديمية
Ready for O4 II: GRANDMA Observations of Swift GRBs during eight-weeks of Spring 2022
| العنوان: | Ready for O4 II: GRANDMA Observations of Swift GRBs during eight-weeks of Spring 2022 |
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| المؤلفون: | Tosta E Melo, I, Ducoin, J.-G, Vidadi, Z, Andrade, C, Rupchandani, V, Agayeva, S, Abdelhadi, J, Abe, L, Aguerre-Chariol, O, Aivazyan, V, Alishov, S, Antier, S, Bai, J.-M, Baransky, A, Bednarz, S, Bendjoya, Ph, Benkhaldoun, Z, Beradze, S, Bizouard, M.A, Bhardwaj, U, Blazek, M, Boër, M, Broens, E, Burkhonov, O, Christensen, N, Cooke, J, Corradi, W, Coughlin, M.W, Culino, T, Daigne, F, Dornic, D, Duverne, P.-A, Ehgamberdiev, S, Eymar, L, Fouad, A, Freeberg, M, Gendre, B, Guo, F, Gokuldass, P, Guessoum, N, Gurbanov, E, Hainich, R, Hasanov, E, Hello, P, Inasaridze, R, Iskandar, A, Ismailov, N, Janati, A, Du Laz, T. Jegou, Kann, D.A, Karpov, S, Kiendrebeogo, R.W, Klotz, A, Kneip, R, Kochiashvili, N, Kaeouach, A, Kruiswijk, K, Lamoureux, M, Leroy, N, Lin, W.L, Mao, J, Marchais, D, Mašek, M, Midavaine, T, Moller, A, Morris, D, Natsvlishvili, R, Navarete, F, Guelbenzu, A. Nicuesa, Noonan, K, Noysena, K, Oksanen, A, Orange, N.B, Pellouin, C, Peloton, J, Peng, H.W, Pilloix, M, Popowicz, A, Pradier, T, Pyshna, O, Raaijmakers, G, Rajabov, Y, Rau, A, Rinner, C, Rivet, J.-P, Ryh, A.S, Sabil, M, Sadibekova, T, Sasaki, N, Serrau, M, Simon, A, Shokry, Ahmed, Smith, K, Sokoliuk, O, Song, X, Takey, A, Thierry, P, Tillayev, Y, Turpin, D, de Ugarte Postigo, A, Vasylenko, V, Vernet, D, Wang, L, Vachier, F, Vignes, J.P, Wang, X.F, Zeng, X, Zhang, J, Zhu, Y |
| المساهمون: | Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (1965 - 2019) (UNS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UniCA)-Université Côte d'Azur (UniCA)-Centre National de la Recherche Scientifique (CNRS), Institut de RadioAstronomie Millimétrique (IRAM), Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Institut universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) |
| المصدر: | Astron.Astrophys. ; https://hal.science/hal-04274105Test ; Astron.Astrophys., 2024, 682, pp.A141. ⟨10.1051/0004-6361/202347938⟩ |
| بيانات النشر: | HAL CCSD |
| سنة النشر: | 2024 |
| مصطلحات موضوعية: | [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] |
| الوصف: | International audience ; We present a campaign designed to train the GRANDMA network and its infrastructure to follow up on transient alerts and detect their early afterglows. In preparation for O4 II campaign, we focused on GRB alerts as they are expected to be an electromagnetic counterpart of gravitational-wave events. Our goal was to improve our response to the alerts and start prompt observations as soon as possible to better prepare the GRANDMA network for the fourth observational run of LIGO-Virgo-Kagra (which started at the end of May 2023), and future missions such as SM. To receive, manage and send out observational plans to our partner telescopes we set up dedicated infrastructure and a rota of follow-up adcates were organized to guarantee round-the-clock assistance to our telescope teams. To ensure a great number of observations, we focused on Swift GRBs whose localization errors were generally smaller than the GRANDMA telescopes' field of view. This allowed us to bypass the transient identification process and focus on the reaction time and efficiency of the network. During 'Ready for O4 II', 11 Swift/INTEGRAL GRB triggers were selected, nine fields had been observed, and three afterglows were detected (GRB 220403B, GRB 220427A, GRB 220514A), with 17 GRANDMA telescopes and 17 amateur astronomers from the citizen science project Kilonova-Catcher. Here we highlight the GRB 220427A analysis where our long-term follow-up of the host galaxy allowed us to obtain a photometric redshift of $z=0.82\pm0.09$, its lightcurve elution, fit the decay slope of the afterglows, and study the properties of the host galaxy. |
| نوع الوثيقة: | article in journal/newspaper |
| اللغة: | English |
| العلاقة: | info:eu-repo/semantics/altIdentifier/arxiv/2310.17287; hal-04274105; https://hal.science/hal-04274105Test; https://hal.science/hal-04274105/documentTest; https://hal.science/hal-04274105/file/aa47938-23.pdfTest; ARXIV: 2310.17287; INSPIRE: 2714757 |
| DOI: | 10.1051/0004-6361/202347938 |
| الإتاحة: | https://doi.org/10.1051/0004-6361/202347938Test https://hal.science/hal-04274105Test https://hal.science/hal-04274105/documentTest https://hal.science/hal-04274105/file/aa47938-23.pdfTest |
| حقوق: | http://creativecommons.org/licenses/byTest/ ; info:eu-repo/semantics/OpenAccess |
| رقم الانضمام: | edsbas.FFA1DBFD |
| قاعدة البيانات: | BASE |
| DOI: | 10.1051/0004-6361/202347938 |
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