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.
|Original language||English (US)|
|Title of host publication||Observatory Operations|
|Subtitle of host publication||Strategies, Processes, and Systems IX|
|Editors||David S. Adler, Robert L. Seaman, Chris R. Benn|
|State||Published - 2022|
|Event||Observatory Operations: Strategies, Processes, and Systems IX 2022 - Montreal, Canada|
Duration: Jul 17 2022 → Jul 22 2022
|Name||Proceedings of SPIE - The International Society for Optical Engineering|
|Conference||Observatory Operations: Strategies, Processes, and Systems IX 2022|
|Period||7/17/22 → 7/22/22|
Bibliographical noteFunding Information:
AdUP and SA acknowledge financial support from the Côte D’Azur University through a CSI recherche grant awarded to the GRANDMA project (PI: S. Antier).
SA acknowledges the financial support of the Programme National Hautes Energies (PNHE). SA acknowledges the financial support of MITI CNRS Sciences participatives. UBAI acknowledges support from the Ministry of Innovative Development through projects FA-Atech-2018-392 and VA-FA-F-2-010. RI acknowledges Shota Rustaveli National Science Foundation (SRNSF) grant No - RF/18-1193. TAROT has been built with the support of the Institut National des Sciences de l’Univers, CNRS, France. MP, SK and MM are supported by European Structural and Investment Fund and the Czech Ministry of Education, Youth and Sports (Projects CZ.02.1.01/0.0/0.0/16 013/0001403, CZ.02.1.01/0.0/0.0/18 046/0016007 and CZ.02.1.01/0.0/0.0/15 003/0000437). NBO and DM acknowledge financial support from NASA MUREP MIRO award 80NSSC21M0001, NASA EP-SCoR award 80NSSC19M0060, and NSF EiR award 1901296. PG acknowledges financial support from NSF EiR award 1901296. DAK acknowledges support from Spanish National Research Project RTI2018-098104-JI00 (GRBPhot). XW is supported by the National Science Foundation of China (NSFC grants 12033003 and 11633002), the Scholar Program of Beijing Academy of Science and Technology (DZ:BS202002), and the Tencent Xplorer Prize. J.Mao is supported by the National Natural Science Foundation of China 11673062 and the Oversea Talent Program of Yunnan Province. The work of FN is supported by NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The GRANDMA consortium thank the amateur participants to the kilonova-catcher program. The kilonova-catcher program is supported by the IdEx Universitéde Paris, ANR-18-IDEX-0001. This research made use of the cross-match service provided by CDS, Strasbourg. MC acknowledges support from the National Science Foundation with grant numbers PHY-2010970 and OAC-2117997. MC and CA acknowledge support from a “Preparing for Astrophysics with LSST” grant with grant number KSI-2. GR acknowledges financial support from the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) through the Pro-jectruimte and VIDI grants (PI: Nissanke). Thanks to the National Astronomical Research Institute of Thailand (Public Organization), based on observations made with the Thai Robotic Telescope under program ID TRTC08D 005 and TRTC09A 002. S. Leonini thanks M. Conti, P. Rosi, and L. M. Tinjaca Ramirez. SA thanks Etienne Bertrand and le “Club des Céphéides” for their observations of ZTF21abxkven.
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- Gravitational waves
- Stars: neutron