Assessing the Photometric Calibration of the ASAS Survey

被引：0

作者：

Berdnikov, L. N. ^{[1
]}

Dambis, A. K. ^{[1
]}

机构：

[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Univ Skii Pr 13, Moscow 119991, Russia

来源：

CALIBRATION AND STANDARDIZATION OF MISSIONS AND LARGE SURVEYS IN ASTRONOMY AND ASTROPHYSICS | 2016年 / 503卷

关键词：

SKY AUTOMATED SURVEY; CATALOG;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We compare bona fide calibrated mean VIC magnitudes of several hundred stars found in the CCD frames taken in 2012 during our photometric observations of 109 Cepheids and RR Lyrae type stars made at the South African Astronomical Observatory to the corresponding mean VIC magnitudes measured in the course of the ASAS survey to assess the quality of ASAS photometry and derive the appropriate transformation equations. We conclude that as far as the only serious caveat due to photometric errors, which range from similar to 0.05(m) for relatively bright stars to about similar to 0.15(m) for similar to 14(m) stars and translates into extra fractional distance error of 0.025 - 0.07

引用

页码：261 / 264

页数：4

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