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Photometry of stars in the uvgr system Photoelectric photometry is presented for over 400 stars using the uvgrsystem of Thuan and Gunn. Stars were selected to cover a wide range ofspectral type, luminosity class, and metallicity. A mean main sequenceis derived along with reddening curves and approximate transformationsto the UBVR system. The calibration of the standard-star sequence issignificantly improved.
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Observation and Astrometry data
Constellation: | うお座 |
Right ascension: | 00h56m53.78s |
Declination: | +07°24'41.9" |
Apparent magnitude: | 9.286 |
Proper motion RA: | 4.5 |
Proper motion Dec: | 6.9 |
B-T magnitude: | 10.637 |
V-T magnitude: | 9.398 |
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