3.8 Article

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

Journal

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
Volume 146, Issue 1, Pages 169-177

Publisher

E D P SCIENCES
DOI: 10.1051/aas:2000266

Keywords

methods : observational; techniques : photometric; stars : general

Ask authors/readers for more resources

A list of G81 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.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

3.8
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available