OmegaCAM 辅助标准星计划
天体物理学
2007-05-23 v1
摘要
OmegaCAM 宽场成像仪将于 2007 年在位于智利 Paranal 的 ESO VLT 调查望远镜上开始运行。OmegaCAM 数据的光度校准依赖于覆盖 OmegaCAM 完全 1 平方度视场 (FoV) 的标准星测量值。一个满足这一要求的目录将被构建，用于八个 Landolt 赤道场，称为 OmegaCAM 辅助标准星目录。本文报告用于引导 OmegaCAM 辅助标准星目录构建的“初步目录”。因此，初步目录将用于评估 OmegaCAM+VST 的性能。该目录基于来自 INT 位于 La Palma 的 WFC 数据构建。
引用
@article{arxiv.astro-ph/0612469,
title = {The Secondary Standards programme for OmegaCAM at the VST},
author = {Gijs Verdoes Kleijn and Ronald Vermeij and Edwin Valentijn and Koen Kuijken},
journal= {arXiv preprint arXiv:astro-ph/0612469},
year = {2007}
}
备注
To appear in ASP conference proceedings for The Future of Photometric, Spectrophotometric, and polarimetric standardization, held in Blankenberge Belgium, may 8-11 2006. Figures available separately from manuscript and with degraded resolution. See http://www.astro-wise.org/Public/blankenberge_verdoes.ps.gz for manuscript with figures included in full resolution