Prospects and latest optical intensity interferometry results with the {MAGIC} and {CTAO}-North {LST} telescopes
Along with their gamma-ray observations at very high energies ({VHE};20 {GeV} – 100 {TeV}), the two 17-m {MAGIC} telescopes (at Roque de los Muchachos Observatory, La Palma) have also been utilized as an optical stellar intensity interferometer ({SII}) for the last six years. The calibration and validation of the setup, alongside the first measurement of the stellar angular diameter of 13 massive stars, were published in a performance paper in early 2024. Around the same time, the technical advancements developed for {MAGIC} were applied to the first Large-Sized Telescope of the northern hemisphere array of the Cherenkov Telescope Array Observatory ({CTAO}-North {LST}-1), a 23-m diameter telescope located near {MAGIC}. Three more {LSTs} should be completed beginning of 2026 and they may be equipped in the same manner as {LST}-1. We will focus on our first measurements with the {MAGIC}+{LST}-1 {SII} and our prospects for this and the {MAGIC}+{LST}1-4 {SII} for the study of several objects that are also known to emit in gamma rays: novae, such as the upcoming T {CrB}; winds from massive stars, particularly colliding-wind binaries; and Be stars which are typical companions in {VHE} gamma-ray binaries.
- Veröffentlicht in:
39th International Cosmic Ray Conference ({ICRC}2025) - Gravitational Wave, Multi-Messenger & Synergies - Typ:
Inproceedings - Autoren:
- Jahr:
2025 - Source:
https://infoscience.epfl.ch/handle/20.500.14299/259447
Informationen zur Zitierung
: Prospects and latest optical intensity interferometry results with the {MAGIC} and {CTAO}-North {LST} telescopes, 39th International Cosmic Ray Conference ({ICRC}2025) - Gravitational Wave, Multi-Messenger & Synergies, 2025, December, https://infoscience.epfl.ch/handle/20.500.14299/259447, Martinez.etal.2025a,
@Inproceedings{Martinez.etal.2025a,
author={Martínez, Irene Jiménez; Santos, Alejo Cifuentes; Hassan, T.; Acciari, Victor; Burelli, Irene; Cortina, Juan; della Volpe, Domenico; Díaz Ginzo, Carlos; García-Lago, Fernando Frías; Jorge, Iñigo; Martínez, Gustavo; Mirzoyan, Razmik; Polo, Miguel; Raiola, Aramis; Rodríguez-Vázquez, Juan José; Saha, Prasenjit; Schweizer, Thomas; Stanic, Lucijana; Abe, K.; Abe, S.; Abhir, J.; Abhishek, A.; Acciari, V. A.; Aguasca-Cabot, A.; Agudo, I.; Aniello, T.; Ansoldi, S.; Antonelli, L. A.; Arbet Engels, A.; Arcaro, C.; Arnesen, T. T. H.; Babić, A.; Bakshi, C.; Barres de Almeida, U.; Barrio, J. A.; Barrios Jiménez, L.; Batković, I.; Baxter, J.; Becerra González, J.; Bednarek, W.; Bernardini, E.; Bernete, J.; Berti, A.; Besenrieder, J.; Bigongiari, C.; Biland, A.; Blanch, O.; Bonnoli, G.; Bošnjak, None; Bronzini, E.; Burelli, I.; Campoy-Ordaz, A.; Carosi, A.; Carosi, R.; Carretero-Castrillo, M.; Zhang, W.; Cerasole, D.; Ceribella, G.; Cerviño, A.; Chai, Y.; Chilingarian, A.; Cifuentes, A.; Colombo, E.; Contreras, J. L.; Cortina, J.; Covino, S.; D’Amico, G.; Da Vela, P.; Dazzi, F.; De Angelis, A.; De Lotto, B.; de Menezes, R.; Delfino, M.; Delgado, J.; Delgado Mendez, C.; Di Pierro, F.; Di Tria, R.; Di Venere, L.; Dinesh, A.; Dominis Prester, D.; Donini, A.; Dorner, D.; Doro, M.; Eisenberger, L.; Elsaesser, D.; Yoshikoshi, T.; Fariña, L.; Foffano, L.; Font, L.; Fröse, S.; Fukazawa, Y.; García López, R. J.; Garcia Soto, S.; Garczarczyk, M.; Gasparyan, S.; Gaug, M.; Giesbrecht Paiva, J.; Giglietto, N.; Giordano, F.; Yoshida, T.; Al, Et},
title={Prospects and latest optical intensity interferometry results with the {MAGIC} and {CTAO}-North {LST} telescopes},
booktitle={39th International Cosmic Ray Conference ({ICRC}2025) - Gravitational Wave, Multi-Messenger & Synergies},
month={December},
url={https://infoscience.epfl.ch/handle/20.500.14299/259447},
year={2025},
abstract={Along with their gamma-ray observations at very high energies ({VHE};20 {GeV} – 100 {TeV}), the two 17-m {MAGIC} telescopes (at Roque de los Muchachos Observatory, La Palma) have also been utilized as an optical stellar intensity interferometer ({SII}) for the last six years. The calibration and validation of the setup, alongside the first measurement of the stellar angular diameter of 13...}}