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CCD survey with the CMASF from the Southern Hemisphere

Published online by Cambridge University Press:  01 October 2007

M. Vallejo
Affiliation:
Real Instituto y Observatorio de la Armada, San Fernando, Spain. email: ppmu@roa.es
J. L. Muiños
Affiliation:
Real Instituto y Observatorio de la Armada, San Fernando, Spain. email: ppmu@roa.es
F. Belizón
Affiliation:
Real Instituto y Observatorio de la Armada, San Fernando, Spain. email: ppmu@roa.es
F. J. Montojo
Affiliation:
Real Instituto y Observatorio de la Armada, San Fernando, Spain. email: ppmu@roa.es
C. C. Mallamaci
Affiliation:
Observatorio Astronómico Félix Aguilar, San Juan, Argentina. email: ccmalla@gmail.com
J. A. Pérez
Affiliation:
Observatorio Astronómico Félix Aguilar, San Juan, Argentina. email: ccmalla@gmail.com
L. F. Marmolejo
Affiliation:
Observatorio Astronómico Félix Aguilar, San Juan, Argentina. email: ccmalla@gmail.com
J. L. Navarro
Affiliation:
Observatorio Astronómico Félix Aguilar, San Juan, Argentina. email: ccmalla@gmail.com
J. Sedeño
Affiliation:
Observatorio Astronómico Félix Aguilar, San Juan, Argentina. email: ccmalla@gmail.com
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Abstract

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A subcatalogue with positions and magnitudes of stars brighter than V = 16 and declinations between −30° and 0° is presented. The observations have been carried out with the Círculo Meridiano Automático de San Fernando at the Carlos Ulrrico Cesco Observatory in San Juan (Argentina) in the framework of an agreement between the ROA and the OAFA. The final goal of this collaboration is to publish a survey of positions and magnitudes of stars brighter than V = 16 and with declinations between −55° and +30°.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Carlsberg Meridian Catalogue, La Palma 2005, No. 14, Copenhagen University Observatory, Institute of Astronomy of Cambridge, Real Instituto y Observatorio de la Armada en San FernandoGoogle Scholar
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