Zero-point stars in the Magellanic Clouds and M67 for CCD Stromgren photometry

Details Zero-point stars in the Magellanic Clouds and M67 for CCD Stromgren photometry Zero-point stars in the Magellanic Clouds and M67 for CCD Stromgren photometry

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...86..103r&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 86, no. 1, Nov. 1990, p. 103-106.

Astronomy and Astrophysics

Astrophysics

6

Astronomical Photometry, Charge Coupled Devices, Error Analysis, Magellanic Clouds, Stellar Color, Dwarf Stars, Giant Stars, Metallicity, Star Clusters, Stellar Luminosity

Scientific paper

The performance of CCD photometry is facilitated by having secondary
standards that can be observed together in a single exposure. Here,
Stromgren colors are presented for some stars located in the Magellanic
Clouds and M67 which can be used for photometric librations of CCD
observations. Mean errors are also given.

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