A new system of faint near-infrared standard stars

被引：718

作者：

Persson, SE

Murphy, DC

Krzeminski, W

Roth, M

Rieke, MJ

机构：

[1] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA

[2] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

来源：

ASTRONOMICAL JOURNAL | 1998年 / 116卷 / 05期

关键词：

infrared radiation; stars : general; techniques : photometric;

D O I：

10.1086/300607

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A new grid of 65 faint near-infrared standard stars is presented. They are spread around the sky, lie between 10th and 12th magnitude at K, and are measured in most cases to precisions better than 0.001 mag in the J, H, K, and K, bands; the latter is a medium-band modified K. A secondary list of red stars suitable for determining color transformations between photometric systems is also presented.

引用

收藏

页码：2475 / 2488

页数：14

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