u'g'r'i'z'标准星网络

J. A. Smith; D. L. Tucker; S. Kent; M. W. Richmond; M. Fukugita; T. Ichikawa; S. -I. Ichikawa; A. M. Jorgensen; A. Uomoto; J. E. Gunn; M. Hamabe; M. Watanabe; A. Tolea; A. Henden; J. Annis; J. R. Pier; T. A. McKay; J. Brinkmann; B. Chen; J. Holtzman; K. Shimasaku; D. G. York

doi:10.1086/339311

u'g'r'i'z'标准星网络

天体物理学 2008-11-26 v2

作者: J. A. Smith , D. L. Tucker , S. Kent , M. W. Richmond , M. Fukugita , T. Ichikawa , S. -I. Ichikawa , A. M. Jorgensen , A. Uomoto , J. E. Gunn , M. Hamabe , M. Watanabe , A. Tolea , A. Henden , J. Annis , J. R. Pier , T. A. McKay , J. Brinkmann , B. Chen , J. Holtzman , K. Shimasaku , D. G. York

在 arXiv 上查看 ↗ PDF ↗ DOI ↗

摘要

我们介绍了定义u'g'r'i'z'光度计系统的158颗标准星。这些星构成了Sloan Digital Sky Survey(SDSS)光度计校准的基础。我们描述了定义仪器系统与滤光片、观测过程、reduction技术以及用于创建星体网络的软件。我们简要讨论了星体选择过程的历史、从UBVRcIc系统派生出一组转换方程的过程，以及未来工作的计划。

关键词

标准星光度计系统 SDSS校准 u'g'r'i'z' 转换方程

引用

@article{arxiv.astro-ph/0201143,
  title  = {The u'g'r'i'z' Standard Star Network},
  author = {J. A. Smith and D. L. Tucker and S. Kent and M. W. Richmond and M. Fukugita and T. Ichikawa and S. -I. Ichikawa and A. M. Jorgensen and A. Uomoto and J. E. Gunn and M. Hamabe and M. Watanabe and A. Tolea and A. Henden and J. Annis and J. R. Pier and T. A. McKay and J. Brinkmann and B. Chen and J. Holtzman and K. Shimasaku and D. G. York},
  journal= {arXiv preprint arXiv:astro-ph/0201143},
  year   = {2008}
}

备注

References to URLs in paper have been updated to reflect moved website. Accepted by AJ. 50 pages, including 20 pages of text, 9 tables, and 15 figures. Plain ASCII text versions of Tables 8 and 9 can be found at http://home.fnal.gov/~dtucker/ugriz/index.html (new URL)

u'g'r'i'z'标准星网络

摘要

关键词

引用

备注

相关论文