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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: | アンドロメダ座 |
| 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 |
Catalogs and designations:
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INHABITED SKY
