Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59...65g&link_type=abstract
(Astronomicheskii Zhurnal, vol. 59, Jan.-Feb. 1982, p. 65-72.) Soviet Astronomy, vol. 26, Jan.-Feb. 1982, p. 40-44. Translation
Astronomy and Astrophysics
Astronomy
3
Astronomical Catalogs, Astronomical Photometry, Stellar Spectrophotometry, Ubv Spectra, Color Photography, Data Acquisition, Light Amplifiers, Radiant Flux Density, Stellar Magnitude
Scientific paper
Spectrophotometric data obtained at the Shternberg Astronomical Institute are compared with photometry in the V band of the U, B, V system and with the 13-color photometry of Johnson and Mitchell both for the Shternberg catalog as a whole and separately for groups of stars measured with different amplifying equipment. Stars with V greater than 4.5 m observed with the Cactus amplifier give an energy flux systematically (3-4.5)% lower than bright (V less than 2.5 m) stars as well as all stars observed with a more advanced electromagnetic amplifier. For the catalog as a whole, effects associated with magnitude and spectral type amount to no more than (1-1.5)%.
Glushneva I. N.
Ovchinnikov S. L.
No associations
LandOfFree
The Shternberg stellar spectrophotometry - Detailed comparison with V-band and Johnson-Mitchell 13-color photometry does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Shternberg stellar spectrophotometry - Detailed comparison with V-band and Johnson-Mitchell 13-color photometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Shternberg stellar spectrophotometry - Detailed comparison with V-band and Johnson-Mitchell 13-color photometry will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1647114