B3 Vertaisarvioimaton artikkeli konferenssijulkaisussa
Variability studies of active galactic nuclei from the long-term monitoring program with the Cherenkov Telescope Array
Tekijät: Grolleron, G.; Becerra Gonzalez, J.; Biteau, J.; Cerruti, M.; Grau, R.; Gréaux, L.; Hovatta, T.; Lenain, J.-P.; Lindfors, E.; Max-Moerbeck, W.; Miceli, D.; Moralejo, A.; Nilsson, K.; Pueschel, E.; Sarkar, A.; Suutarinen, S. for the Cherenkov Telescope Array Consortium
Toimittaja: Saito, Takayuki; Okumura, Kimihiro
Konferenssin vakiintunut nimi: International Cosmic Ray Conference
Kustantaja: Sissa Medialab Srl
Julkaisuvuosi: 2024
Journal: POS Proceedings of Science
Kokoomateoksen nimi: 38th International Cosmic Ray Conference
Tietokannassa oleva lehden nimi: Proceedings of Science
Artikkelin numero: 856
Vuosikerta: 444
eISSN: 1824-8039
DOI: https://doi.org/10.22323/1.444.0856
Verkko-osoite: https://doi.org/10.22323/1.444.0856
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/478211073
Blazars are active galactic nuclei (AGN) with a relativistic jet oriented toward the observer. This jet is composed of accelerated particles which can display emission over the entire electromagnetic spectrum. Spectral variability has been observed on short- and long-time scales in AGN, with a power spectral density (PSD) that can show a break at frequencies below the well-known red-noise process. This break frequency in the PSD has been observed in X-rays to scale with the accretion regime and the mass of the central black hole. It is expected that a break could also be seen in the very-high-energy gamma rays, but constraining the shape of the PSD in these wavelengths has not been possible with the current instruments. The Cherenkov Telescope Array (CTA) will be more sensitive by a factor of five to ten depending on energy than the current generation of imaging atmospheric Cherenkov telescopes, therefore it will be possible with CTA to reconstruct the PSD with a high accuracy, bringing new information about AGN variability. In this work, we focus on the AGN long-term monitoring program planned with CTA. The program is proposed to begin with early-start observing campaigns with CTA precursors. This would allow us to probe longer time scales on the AGN PSD.
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Julkaisussa olevat rahoitustiedot:
This work was conducted in the context of the CTA Consortium. We gratefully acknowledge financial support from the agencies and organizations listed here: https://www.cta-observatory.org/consortium_acknowledgments/.
