First results of the CMASF CCD observations in Argentina

被引：0

作者：

Muinos, J. L. ^{[1
,2
]}

Belizon, F. ^{[1
,2
]}

Vallejo, M. ^{[1
,2
]}

Montojo, F. J. ^{[1
,2
]}

Mallamaci, C. C. ^{[3
]}

Perez, J. A. ^{[3
]}

机构：

[1] Real Inst, San Fernando De Henares, Spain

[2] Observ Armada, San Fernando De Henares, Spain

[3] Observ Astron Felix Aguilar, San Juan, Argentina

来源：

THIRD INTERNATIONAL MEETING OF DYNAMIC ASTRONOMY IN LATIN AMERICA (ADELA-2004) | 2006年 / 25卷

关键词：

astrometry; stars : catalogues; surveys;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The CCD meridian circle of San Fernando (CMASF) is installed in the Carlos U. Cesco observatory in San Juan (Argentina) at 69 degrees W, 31 degrees S and 2300 in of altitude. It is operated jointly by the Real Instituto y Observatorio de la Armada (ROA) and the Observatorio Astronomico Felix Aguilar (OAFA). In December 1999, a CCD camera was installed in the instrument. Since then, the sky band with declinations between +3 degrees and -55 degrees\ has been observed in order to publish a catalogue of positions and magnitudes of the stars brighter than V=16. In this paper, the first results of a preliminar catalogue with the stars in the band +3 degrees to -15 degrees are shown.

引用

页码：47 / +

页数：2