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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: | Andromède |
Right ascension: | 00h08m16.95s |
Declination: | +34°29'42.9" |
Apparent magnitude: | 8.766 |
Distance: | 266.667 parsecs |
Proper motion RA: | 5.3 |
Proper motion Dec: | -4.5 |
B-T magnitude: | 9.152 |
V-T magnitude: | 8.798 |
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