Transient Observations with LST-1: Key Results and Future Prospects

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Hauptverfasser: Seglar-Arroyo, Monica, Berti, Alessio, Carosi, Alessandro, Cicciari, Gloria Maria, Donini, Alice, Fiasson, Armand, Aguasca-Cabot, Arnau, de Bony, Mathieu, Bordas, Pol, Ribó, Marc, Ruiz-Velasco, Edna, Schüssler, Fabian
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Veröffentlicht: 2025
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author Seglar-Arroyo, Monica
Berti, Alessio
Carosi, Alessandro
Cicciari, Gloria Maria
Donini, Alice
Fiasson, Armand
Aguasca-Cabot, Arnau
de Bony, Mathieu
Bordas, Pol
Ribó, Marc
Ruiz-Velasco, Edna
Schüssler, Fabian
author_facet Seglar-Arroyo, Monica
Berti, Alessio
Carosi, Alessandro
Cicciari, Gloria Maria
Donini, Alice
Fiasson, Armand
Aguasca-Cabot, Arnau
de Bony, Mathieu
Bordas, Pol
Ribó, Marc
Ruiz-Velasco, Edna
Schüssler, Fabian
contents The recent detections of the afterglow phase of long gamma-ray bursts (lGRBs) at very high energies (VHE, >100 GeV) mark a significant advance in astrophysics of transient phenomena, offering deeper insights into the acceleration mechanisms, jet structure, and physical processes driving GRB emission. In the multi-messenger landscape, both high-energy neutrino and gravitational wave detections are providing new insights into the physics of extreme cosmic accelerators and highlighting the need for rapid and broadband follow-up observations. The Large-Sized Telescope (LST-1), the first telescope of the LST array, part of the Cherenkov Telescope Array Observatory (CTAO) North site, is particularly well-suited for real-time, rapid follow-up of transients. In this contribution, we present the latest achievements of the transient observational program with LST-1, which is now in advanced commissioning on La Palma, Canary Islands. We outline the observational strategies in place and describe the dynamic handling of events by the transient handler of LST-1 (e.g., its ability to handle poorly localised events, including gravitational waves, GRBs and neutrinos). We present the key results from transient observation campaigns conducted so far, discuss the lessons learned, and outline the promising prospects for the future LST-1+MAGIC combined transient program with fast response, via a Transient Handler.
format Preprint
id arxiv_https___arxiv_org_abs_2509_06668
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Transient Observations with LST-1: Key Results and Future Prospects
Seglar-Arroyo, Monica
Berti, Alessio
Carosi, Alessandro
Cicciari, Gloria Maria
Donini, Alice
Fiasson, Armand
Aguasca-Cabot, Arnau
de Bony, Mathieu
Bordas, Pol
Ribó, Marc
Ruiz-Velasco, Edna
Schüssler, Fabian
High Energy Astrophysical Phenomena
The recent detections of the afterglow phase of long gamma-ray bursts (lGRBs) at very high energies (VHE, >100 GeV) mark a significant advance in astrophysics of transient phenomena, offering deeper insights into the acceleration mechanisms, jet structure, and physical processes driving GRB emission. In the multi-messenger landscape, both high-energy neutrino and gravitational wave detections are providing new insights into the physics of extreme cosmic accelerators and highlighting the need for rapid and broadband follow-up observations. The Large-Sized Telescope (LST-1), the first telescope of the LST array, part of the Cherenkov Telescope Array Observatory (CTAO) North site, is particularly well-suited for real-time, rapid follow-up of transients. In this contribution, we present the latest achievements of the transient observational program with LST-1, which is now in advanced commissioning on La Palma, Canary Islands. We outline the observational strategies in place and describe the dynamic handling of events by the transient handler of LST-1 (e.g., its ability to handle poorly localised events, including gravitational waves, GRBs and neutrinos). We present the key results from transient observation campaigns conducted so far, discuss the lessons learned, and outline the promising prospects for the future LST-1+MAGIC combined transient program with fast response, via a Transient Handler.
title Transient Observations with LST-1: Key Results and Future Prospects
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2509.06668