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http://hdl.handle.net/1843/59878
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DC Field | Value | Language |
---|---|---|
dc.creator | S. Agayeva | pt_BR |
dc.creator | Philippe Bendjoya | pt_BR |
dc.creator | Z. Vidadi | pt_BR |
dc.creator | J. Zhu | pt_BR |
dc.creator | Y. Zhu | pt_BR |
dc.creator | Zouhair Benkhaldoun | pt_BR |
dc.creator | S. Beradze | pt_BR |
dc.creator | D. Berezin | pt_BR |
dc.creator | U. Bhardwaj | pt_BR |
dc.creator | M. Blazek | pt_BR |
dc.creator | O. Burkhonov | pt_BR |
dc.creator | E. Burns | pt_BR |
dc.creator | S. Caudill | pt_BR |
dc.creator | N. Christensen | pt_BR |
dc.creator | V. Aivazyan | pt_BR |
dc.creator | F. Colas | pt_BR |
dc.creator | A. Coleiro | pt_BR |
dc.creator | Wagner José Corradi Barbosa | pt_BR |
dc.creator | M. W. Coughlin | pt_BR |
dc.creator | T. Culino | pt_BR |
dc.creator | D. Darson | pt_BR |
dc.creator | D. Datashvili | pt_BR |
dc.creator | G. de Wasseige | pt_BR |
dc.creator | T. Dietrich | pt_BR |
dc.creator | F. Dolon | pt_BR |
dc.creator | Sabahaddin Alishov | pt_BR |
dc.creator | D. Dornic | pt_BR |
dc.creator | J. Dubouil | pt_BR |
dc.creator | J.-G. Ducoin | pt_BR |
dc.creator | P.-A. Duverne | pt_BR |
dc.creator | A. Esamdin | pt_BR |
dc.creator | A. Fouad | pt_BR |
dc.creator | F. Guo | pt_BR |
dc.creator | V. Godunova | pt_BR |
dc.creator | P. Gokuldass | pt_BR |
dc.creator | N. Guessoum | pt_BR |
dc.creator | M. Almualla | pt_BR |
dc.creator | E. Gurbanov | pt_BR |
dc.creator | R. Hainich | pt_BR |
dc.creator | E. Hasanov | pt_BR |
dc.creator | P. Hello | pt_BR |
dc.creator | T. Hussenot-desenonges | pt_BR |
dc.creator | R. Inasaridze | pt_BR |
dc.creator | A. Iskandar | pt_BR |
dc.creator | E. E. O. Ishida | pt_BR |
dc.creator | Nariman Ismailov | pt_BR |
dc.creator | T. Jegou du Laz | pt_BR |
dc.creator | C. Andrade | pt_BR |
dc.creator | D. A. Kann | pt_BR |
dc.creator | G. Kapanadze | pt_BR |
dc.creator | Sergey Karpov | pt_BR |
dc.creator | R. W. Kiendrebeogo | pt_BR |
dc.creator | A. Klotz | pt_BR |
dc.creator | Nino Kochiashvili | pt_BR |
dc.creator | A. Kaeouach | pt_BR |
dc.creator | J.-P. Kneib | pt_BR |
dc.creator | W. Kou | pt_BR |
dc.creator | K. Kruiswijk | pt_BR |
dc.creator | Sarah Antier | pt_BR |
dc.creator | S. Lombardo | pt_BR |
dc.creator | M. Lamoureux | pt_BR |
dc.creator | N. Leroy | pt_BR |
dc.creator | A. Le Van Su | pt_BR |
dc.creator | J. Mao | pt_BR |
dc.creator | M. Masek | pt_BR |
dc.creator | T. Midavaine | pt_BR |
dc.creator | Anais Möller | pt_BR |
dc.creator | D. Morris | pt_BR |
dc.creator | R. Natsvlishvili | pt_BR |
dc.creator | J.-M. Bai | pt_BR |
dc.creator | F. Navarete | pt_BR |
dc.creator | S. Nissanke | pt_BR |
dc.creator | K. Noonan | pt_BR |
dc.creator | K. Noysena | pt_BR |
dc.creator | N. B. Orange | pt_BR |
dc.creator | J. Peloton | pt_BR |
dc.creator | M. Pilloix | pt_BR |
dc.creator | T. Pradier | pt_BR |
dc.creator | M. Prouza | pt_BR |
dc.creator | G. Raaijmakers | pt_BR |
dc.creator | A. Baransky | pt_BR |
dc.creator | Y. Rajabov | pt_BR |
dc.creator | J.-P. Rivet | pt_BR |
dc.creator | Y. Romanyuk | pt_BR |
dc.creator | L. Rousselot | pt_BR |
dc.creator | F. Rünger | pt_BR |
dc.creator | V. Rupchandani | pt_BR |
dc.creator | T. Sadibekova | pt_BR |
dc.creator | N. Sasaki | pt_BR |
dc.creator | A. Simon | pt_BR |
dc.creator | K. Smith | pt_BR |
dc.creator | S. Basa | pt_BR |
dc.creator | O. Sokoliuk | pt_BR |
dc.creator | X. Song | pt_BR |
dc.creator | A. Takey | pt_BR |
dc.creator | Y. Tillayev | pt_BR |
dc.creator | I. Tosta e Melo | pt_BR |
dc.creator | D. Turpin | pt_BR |
dc.creator | Antonio de Ugarte Postigo | pt_BR |
dc.creator | M. Vardosanidze | pt_BR |
dc.creator | X. F. Wang | pt_BR |
dc.creator | D. Vernet | pt_BR |
dc.date.accessioned | 2023-10-23T21:21:33Z | - |
dc.date.available | 2023-10-23T21:21:33Z | - |
dc.date.issued | 2022 | - |
dc.citation.issue | 9 | pt_BR |
dc.citation.spage | 52 | pt_BR |
dc.identifier.doi | https://doi.org/10.48550/arXiv.2207.10178 | pt_BR |
dc.identifier.uri | http://hdl.handle.net/1843/59878 | - |
dc.description.abstract | GRANDMA is a world-wide collaboration with the primary scientific goal of studying gravitational-wave sources, discovering their electromagnetic counterparts and characterizing their emission. GRANDMA involves astronomers, astrophysicists, gravitational-wave physicists, and theorists. GRANDMA is now a truly global network of telescopes, with (so far) 30 telescopes in both hemispheres. It incorporates a citizen science programme (Kilonova-Catcher) which constitutes an opportunity to spread the interest in time-domain astronomy. The telescope network is an heterogeneous set of already-existing observing facilities that operate coordinated as a single observatory. Within the network there are wide-field imagers that can observe large areas of the sky to search for optical counterparts, narrow-field instruments that do targeted searches within a predefined list of host-galaxy candidates, and larger telescopes that are devoted to characterization and follow-up of the identified counterparts. Here we present an overview of GRANDMA after the third observing run of the LIGO/VIRGO gravitational-wave observatories in 2019 − 2020 and its ongoing preparation for the forthcoming fourth observational campaign (O4). Additionally, we review the potential of GRANDMA for the discovery and follow-up of other types of astronomical transients. | pt_BR |
dc.description.resumo | GRANDMA is a world-wide collaboration with the primary scientific goal of studying gravitational-wave sources, discovering their electromagnetic counterparts and characterizing their emission. GRANDMA involves astronomers, astrophysicists, gravitational-wave physicists, and theorists. GRANDMA is now a truly global network of telescopes, with (so far) 30 telescopes in both hemispheres. It incorporates a citizen science programme (Kilonova-Catcher) which constitutes an opportunity to spread the interest in time-domain astronomy. The telescope network is an heterogeneous set of already-existing observing facilities that operate coordinated as a single observatory. Within the network there are wide-field imagers that can observe large areas of the sky to search for optical counterparts, narrow-field instruments that do targeted searches within a predefined list of host-galaxy candidates, and larger telescopes that are devoted to characterization and follow-up of the identified counterparts. Here we present an overview of GRANDMA after the third observing run of the LIGO/VIRGO gravitational-wave observatories in 2019 − 2020 and its ongoing preparation for the forthcoming fourth observational campaign (O4). Additionally, we review the potential of GRANDMA for the discovery and follow-up of other types of astronomical transients. | pt_BR |
dc.format.mimetype | pt_BR | |
dc.language | por | pt_BR |
dc.publisher | Universidade Federal de Minas Gerais | pt_BR |
dc.publisher.country | Brasil | pt_BR |
dc.publisher.department | ICX - DEPARTAMENTO DE FÍSICA | pt_BR |
dc.publisher.initials | UFMG | pt_BR |
dc.relation.ispartof | Society of Photo-Optical Instrumentation Engineers, Astronomical Telescopes + Instrumentation | pt_BR |
dc.rights | Acesso Aberto | pt_BR |
dc.subject | Stars: neutron | pt_BR |
dc.subject | Gravitational waves | pt_BR |
dc.subject.other | Estrelas | pt_BR |
dc.subject.other | Neutrons | pt_BR |
dc.subject.other | Ondas gravitacionais | pt_BR |
dc.title | The GRANDMA network in preparation for the fourth gravitational-wave observing run | pt_BR |
dc.type | Artigo de Evento | pt_BR |
dc.url.externa | https://www.spiedigitallibrary.org/conference-proceedings-of-spie/12186/2630240/The-GRANDMA-network-in-preparation-for-the-fourth-gravitational-wave/10.1117/12.2630240.full?SSO=1 | pt_BR |
dc.identifier.orcid | https://orcid.org/0000-0002-5150-5282 | pt_BR |
Appears in Collections: | Artigo de Evento |
Files in This Item:
File | Description | Size | Format | |
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The grandma network in preparation for the fourth gravitational-wave observing run.pdf | 1.38 MB | Adobe PDF | View/Open |
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