大型天文台：全色天体物理学的过去与未来
天体物理仪器与方法
2021-04-02 v1
摘要
NASA的大型天文台从太空打开了电磁波谱，提供了对地面无法到达波长的持续观测能力。哈勃、康普顿、钱德拉和斯皮策 together 为科学界提供了一套敏捷而强大的望远镜组合，用以攻克广泛的科学问题，并应对快速变化的科学格局。随着现有大型天文台老化或退役，科学界对这些波长的获取将减少，伴随而来的是科学能力的损失。本报告由NASA宇宙起源、宇宙物理学与系外行星探测计划分析组（PAGs）委托撰写，分析了大型天文台时代来自太空的多波长观测的重要性，并给出了跨越广泛天体物理研究的实例。
引用
@article{arxiv.2104.00023,
title = {Great Observatories: The Past and Future of Panchromatic Astrophysics},
author = {L. Armus and S. T. Megeath and L. Corrales and M. Marengo and A. Kirkpatrick and J. D. Smith and M. Meyer and S. Gezari and R. P. Kraft and S. McCandliss and S. Tuttle and M. Elvis and M. Bentz and B. Binder and F. Civano and D. Dragomir and C. Espaillat and S. Finkelstein and D. B. Fox and M. Greenhouse and E. Hamden and J. Kauffmann and G. Khullar and J. Lazio and J. Lee and C. Lillie and P. Lightsey and R. Mushotzky and C. Scarlata and P. Scowen and G. R. Tremblay and Q. D. Wang and S. Wolk},
journal= {arXiv preprint arXiv:2104.00023},
year = {2021}
}
备注
A report by the Great Observatories Science Analysis Group (SAG-10), commissioned by NASA's Cosmic Origins, Physics of the Cosmos, and Exoplanet Exploration Program Analysis Groups. 87 pages, 23 figures