The GRANDMA network in preparation for the fourth gravitational-wave observing run
S. Agayeva, V. Aivazyan, S. Alishov, M. Almualla, C. Andrade, S., Antier, J.-M. Bai, A. Baransky, S. Basa, P. Bendjoya, Z. Benkhaldoun, S., Beradze, D. Berezin, U. Bhardwaj, M. Blazek, O. Burkhonov, E. Burns, S., Caudill, N. Christensen, F. Colas, A. Coleiro, W. Corradi

TL;DR
GRANDMA is a global telescope network designed to detect and study electromagnetic counterparts of gravitational-wave sources, preparing for the upcoming LIGO/VIRGO O4 run and expanding its transient astronomy capabilities.
Contribution
This paper provides an overview of GRANDMA's development, coordination, and readiness for the fourth gravitational-wave observing run, including its diverse telescope network and citizen science program.
Findings
GRANDMA has coordinated 30 telescopes worldwide.
The network is prepared for the LIGO/VIRGO O4 observational campaign.
GRANDMA can discover and follow up various astronomical transients.
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,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
