星形成星系 X 射线数量计数
天体物理学
2017-08-23 v2
摘要
研究正常星系在微弱 (-18 < Log F < -15 cgs) X 射线（0.5-2.0 keV 能段）下的数量计数行为。联合利用射电、远红外和 X 射线观测信息，可在整个flux范围内确定星系的 LogN-LogS，且精度在因数3以内。
引用
@article{arxiv.astro-ph/0404087,
title = {X-ray number counts of star forming galaxies},
author = {Piero Ranalli and Andrea Comastri and Giancarlo Setti},
journal= {arXiv preprint arXiv:astro-ph/0404087},
year = {2017}
}
备注
LaTeX (includes ws-procs9x6.cls), 2 pages, 2 figures; proc. conf. "Multiwavelength AGN Surveys", Cozumel, Mexico 2003. Revised version (one typo corrected)