关于即将进行的 PLANCK 任务中太阳系天体凌星：数据标记与同时多频观测
地球与行星天体物理
2015-05-13 v2 宇宙学与河外天体物理
天体物理仪器与方法
摘要
在当前和未来主要致力于精确绘制宇宙微波背景（CMB）图的微波巡天背景下，太阳系的毫米和亚毫米发射将构成潜在的污染源，同时也为新的太阳系研究提供了机会。特别是，即将进行的欧空局 Planck 任务将能够观测行星和一些大型小行星的点状热发射以及弥散的黄道光发射（ZLE）。在简要介绍该领域后，我们重点讨论了 Planck 时间有序数据中太阳系离散天体的识别。
引用
@article{arxiv.0902.0468,
title = {On the Transits of Solar System Objects in the Forthcoming PLANCK Mission: Data Flagging and Coeval Multifrequency Observations},
author = {Michele Maris and Carlo Burigana},
journal= {arXiv preprint arXiv:0902.0468},
year = {2015}
}
备注
10 pages, 1 figure. Talk held at the Workshop "Future Ground based Solar System Research: Synergies with Space Probes and Space Telescope". 7 pages, 1 figure, 1 table, latex, svjour3.sty, graphicx.sty. Accepted for the pubblication in "Earth Moon and Planets" June 30th, 2009. With respect to V1: improved english style, improved references, corrected typos, a table added