在特德天文台使用ASTRI迷你阵列的银河系观测站科学
高能天体物理现象
2022-08-08 v1 天体物理仪器与方法
摘要
ASTRI（意大利复制技术镜面天体物理，Astrofisica con Specchi a Tecnologia Replicante Italiana）迷你阵列将由位于特德天文台（Observatorio del Teide）址的九台成像大气切伦科夫望远镜组成。该阵列最适合于0.3-200 TeV范围内的天体物理观测，角分辨率为数角分，能量分辨率为10-15%。前四年的核心科学计划将致力于有限数量的关键目标，以解决甚高能领域最重要的开放科学问题。同时，得益于约10度的宽视场，ASTRI迷你阵列将观测许多额外的视场源，这些源将构成长期观测站计划的基础，最终覆盖所有可观测天空。在本文中，我们回顾了不同的天体物理银河系环境，例如脉冲星风云、超新星遗迹和伽马射线双星，并展示了针对其中部分视场源的一组ASTRI迷你阵列模拟结果，以凸显该阵列的预期性能（即使在大的偏离角下）以及将补充核心科学计划的重要额外观测站科学。
引用
@article{arxiv.2208.03181,
title = {Galactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide},
author = {A. D'Aì and E. Amato and A. Burtovoi and A. A. Compagnino and M. Fiori and A. Giuliani and N. La Palombara and A. Paizis and G. Piano and F. G. Saturni and A. Tutone and A. Belfiore and M. Cardillo and S. Crestan and G. Cusumano and M. Della Valle and M. Del Santo and A. La Barbera and V. La Parola and S. Lombardi and S. Mereghetti and G. Morlino and F. Pintore and P. Romano and S. Vercellone and A. Antonelli and C. Arcaro and C. Bigongiari and M. Böettcher and P. Bruno and A. Bulgarelli and V. Conforti and A. Costa and E. de Gouveia Dal Pino and V. Fioretti and S. Germani and A. Ghedina and F. Gianotti and V. Giordano and F. Incardona and G. Leto and F. Longo and A. López Oramas and F. Lucarelli and B. Olmi and A. Pagliaro and N. Parmiggiani and G. Romeo and A. Stamerra and V. Testa and G. Tosti and G. Umana and L. Zampieri and P. Caraveo and G. Pareschi},
journal= {arXiv preprint arXiv:2208.03181},
year = {2022}
}
备注
Accepted for publication in Journal of High-Energy Astrophysics