First Results of the CMASF CCD Observations in Argentina

Details First Results of the CMASF CCD Observations in Argentina First Results of the CMASF CCD Observations in Argentina

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..25...47m&link_type=abstract

Third International Meeting of Dynamic Astronomy in Latin America (Eds. Carlos Abad, Ángel Bongiovanni, & Yaneth Guillén) Revist

Astronomy and Astrophysics

Astronomy

Astrometry, Stars: Catalogues, Surveys

Scientific paper

The CCD meridian circle of San Fernando (CMASF) is installed in the Carlos U. Cesco observatory in San Juan (Argentina) at 69° W, 31° S and 2300 m of altitude. It is operated jointly by the Real Instituto y Observatorio de la Armada (ROA) and the Observatorio Astronómico Félix Aguilar (OAFA). In December 1999, a CCD camera was installed in the instrument. Since then, the sky band with declinations between +3° and -55° 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° to -15° are shown.

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