Authors

S. Agayeva, Azerbaijan National Academy of Sciences
V. Aivazyan, E. Kharadze Georgian National Astrophysical Observatory
S. Alishov, Azerbaijan National Academy of Sciences
M. Almualla, American University of Sharjah
C. Andrade, College of Science and Engineering
Sarah Antier, Observatoire de la Côte d'Azur
J. M. Bai, Yunnan Observatories
A. Baransky, Taras Shevchenko National University of Kyiv
S. Basa, Laboratoire d'Astrophysique de Marseille
P. Bendjoya, Laboratoire Joseph-Louis Lagrange
Z. Benkhaldoun, Faculté des Sciences Semlalia
S. Beradze, E. Kharadze Georgian National Astrophysical Observatory
D. Berezin, National Academy of Sciences of Ukraine
U. Bhardwaj, Anton Pannekoek Instituut voor Sterrenkunde
M. Blazek, CSIC - Instituto de Astrofísica de Andalucía (IAA)
O. Burkhonov, Academy of Sciences of the Republic of Uzbekistan
E. Burns, Louisiana State University
S. Caudill, Universiteit Utrecht
N. Christensen, Observatoire de la Côte d'Azur
F. Colas, L'Observatoire de Paris
A. Coleiro, APC - AstroParticule et Cosmologie
W. Corradi, Laboratorio Nacional de Astrofisica, Itajuba
M. W. Coughlin, College of Science and Engineering
T. Culino, Observatoire de la Côte d'Azur
D. Darson, CNRS Centre National de la Recherche Scientifique
D. Datashvili, E. Kharadze Georgian National Astrophysical Observatory
G. De Wasseige, Université Catholique de Louvain
T. Dietrich, Universität Potsdam
F. Dolon, Observatoire de Haute-Provence
D. Dornic, Centre de Physique des Particules de Marseille
J. Dubouil, L'Observatoire de Paris
J. G. Ducoin, Institut d’Astrophysique de Paris
P. A. Duverne, Université Paris-Saclay

Document Type

Conference Proceeding

Publication Date

1-1-2022

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.

Publication Source (Journal or Book title)

Proceedings of SPIE the International Society for Optical Engineering

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