CCD photometric UBVR sequences for NGC 2403 and M 81

Details CCD photometric UBVR sequences for NGC 2403 and M 81 CCD photometric UBVR sequences for NGC 2403 and M 81

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..925z&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, Aug. 1990, p. 925-931.

Astronomy and Astrophysics

Astronomy

11

Astronomical Photometry, Charge Coupled Devices, Galaxies, Ubv Spectra, Brightness, Pixels, Stellar Luminosity, Telescopes

Scientific paper

CCD UBVR Cousins photometric sequences are presented for stars in
selected fields near the galaxies NGC 2403 and M 81. The sequences reach
from about 15 to 22 mag and 17 to 21 mag in V for the fields near NGC
2403 and M 81, respectively. The limiting magnitude in U is about 20.5
mag in both cases.

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