Spectrophotometry of bright southern stars

Details Spectrophotometry of bright southern stars Spectrophotometry of bright southern stars

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197..941t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 197, Dec. 1981, p. 941-948. Research supported by the New Zealand Unive

Astronomy and Astrophysics

Astronomy

2

Southern Sky, Stellar Magnitude, Stellar Spectra, Stellar Spectrophotometry, Calibrating, Computer Techniques, Data Reduction, Spectrum Analysis, Tables (Data)

Scientific paper

Careful intermediate resolution (10-18 nm) multicolor photometric measurements on 28 bright stars in the southern winter sky have been completed at wavelengths from 339 to 700 nm. The spectra are tied to the calibration of Alpha Lyr through secondary standards. Relative spectra are accurate to better than 0.01 mag over the entire range and it is estimated that the absolute spectra are accurate to 0.02 mag

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