CCD standards for U and I in the open cluster NGC 7790

Details CCD standards for U and I in the open cluster NGC 7790 CCD standards for U and I in the open cluster NGC 7790

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...376..745p&link_type=abstract

Astronomy and Astrophysics, v.376, p.745-750 (2001)

Astronomy and Astrophysics

Astrophysics

6

Techniques: Photometric, Astronomical Data Bases: Miscellaneous, Open Clusters: Individual: Ngc 7790

Scientific paper

Photometric U and I standard sequences in the field of the open cluster NGC 7790 are presented. The intention is to achieve wide ranges in magnitude and colour, making these sequences suitable for calibrating deep CCD photometry. The 84 standard stars extend the BVR sequences of Odewahn et al. (\cite{Odewahn92}) to the near UV and IR, respectively. Based on observations collected at the National Astronomical Observatory Rozhen, Bulgaria. This work is part of a common project between the Universitätssternwarte Bonn, Germany, and the Institute of Astronomy of the Bulgarian Academy of Sciences to study binary open star clusters and clusters in the direction of the Galactic anticentre. Full 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/cgi-bin/qcat?J/A+A/376/745

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