Secondary UBVRI-CCD standard stars in the neighbourhood of Landolt standard stars

Details Secondary UBVRI-CCD standard stars in the neighbourhood of Landolt standard stars Secondary UBVRI-CCD standard stars in the neighbourhood of Landolt standard stars

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26as..146..169g&link_type=abstract

Astronomy and Astrophysics Supplement, v.146, p.169-177

Astronomy and Astrophysics

Astrophysics

29

Methods: Observational, Techniques: Photometric, Stars: General

Scientific paper

A list of 681 UBVRI secondary standard stars for CCD photometry is presented. Visual magnitude ranges from 9.7 to 19.4, and the B-V colour index varies from 1.15 to 1.97. The stars are grouped into 11 different fields, each of them is generally observable in a single CCD frame. The stars are located near Landolt UBVRI equatorial standards, accessible to telescopes in both hemispheres, and mainly within the 5 - 8 hours range of right ascension. Photometry, equatorial coordinates and finding charts are provided. Based on observations made at the Centro Astronómico Hispano-Alemán and the Observatorio Astronómico Nacional in Calar Alto, Almería, Spain. Full version of Table 4 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

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