UBVRI photometry of the optical counterparts of X-ray sources in Einstein Deep Survey Fields

Details UBVRI photometry of the optical counterparts of X-ray sources in Einstein Deep Survey Fields UBVRI photometry of the optical counterparts of X-ray sources in Einstein Deep Survey Fields

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...257l..27l&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 257, June 1, 1982, p. L27-L31

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Ubv Spectra, Visual Photometry, X Ray Sources, Electrophotometers, Heao 2, Iue, Tables (Data)

Scientific paper

We have carried out five-color photometry of the brighter optical counterparts of X-ray sources in the Einstein Deep Survey Fields in Cetus, Eridanus, and Pavo. Most of the observed objects appear to be stars showing no signs of variability; exceptions include one star that varies in brightness over a small range and at least one variable quasar with a redshift z equals 1.96.

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