Pan-STARRS测光与天体测量定标
天体物理仪器与方法
2020-11-18 v3
摘要
我们给出 Pan-STARRS1 巡天的测光与天体测量定标的细节。测光目标是减少相机和探测器引入的系统效应，并将所有观测置于一个在整个巡天区域（赤纬 = -30 度以北约 30,000 平方度）具有一致零点的测光系统上。天体测量定标补偿类似的系统效应，使得位置、自行和视差同样可靠。Pan-STARRS 数据发布 2 (DR2) 的天体测量与 Gaia DR1 发布相绑定。
引用
@article{arxiv.1612.05242,
title = {Pan-STARRS Photometric and Astrometric Calibration},
author = {Eugene. A. Magnier and Edward. F. Schlafly and Douglas P. Finkbeiner and J. L. Tonry and B. Goldman and S. Röser and E. Schilbach and K. C. Chambers and H. A. Flewelling and M. E. Huber and P. A. Price and W. E. Sweeney and C. Z. Waters and L. Denneau and P. Draper and K. W. Hodapp and R. Jedicke and R. -P. Kudritzki and N. Metcalfe and C. W. Stubbs and R. J. Wainscoast},
journal= {arXiv preprint arXiv:1612.05242},
year = {2020}
}
备注
Pan-STARRS Public Data Release 2 : Paper V