通过光学光谱揭示 INTEGRAL 目标的本质
天体物理学
2009-11-11 v1
摘要
自 2002 年10月发射后，INTEGRAL 卫星正以前所未有的灵敏度和位置精度对硬 X 射线天空进行深层勘测。这使得通过在较长波段的目录进行位置交叉相关，确定仍不明确性质的硬 X 射线源的可能光学/近红外候选对象。本文将描述这项工作以及旨在通过光学光谱确定未知 INTEGRAL 目标性质的观测活动，以及该搜索的主要结果。还将阐述这一识别计划的未来前景。
引用
@article{arxiv.astro-ph/0604481,
title = {Unveiling the nature of INTEGRAL sources through optical spectroscopy},
author = {Nicola Masetti},
journal= {arXiv preprint arXiv:astro-ph/0604481},
year = {2009}
}
备注
6 pages (including discussion), 1 figure. To appear on the Procs. of Frascati Workshop 2005 on Multifrequency Behaviour of High Energy Cosmic Sources (held in Vulcano, Italy, 23-28 May 2005; ed. F. Giovannelli & L. Sabau-Graziati, to be published on ChJAA Suppl.). This contribution depicts the situation on the subject at the time of the conference (May 2005)