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Discovery of low-redshift X-ray selected quasars: New clues to the QSO phenomenon

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/183288· OSTI ID:7054747
Using the CTIO 4 m and 1.5 m telescopes to identify serendipitous X-ray sources discovered by the Einstein Observatory, we have identified as quasars all six sources in four high-latitude IPC fields (approx.4 deg/sup 2/). These X-ray selected QSOs have low redshifts (zapprox.0.08--0.23 for five objects and z=0.73 for the sixth) and relatively faint optical magnitudes (approx. =18) and are radio quiet. Our sample selected with intermediate (approx.10/sup 4/ s) X-ray exposures appears similar in space density, colors, and magnitude versus redshift relation to a complete optically selected sample at the same mean magnitude. Spectrophotometry of the six objects and comparisons with other X-ray QSOs and Seyfert 1 galaxies reveals a strong correlation between X-ray luminosity and both continuum and broad-line (e.g., H..beta..) emission luminosities for these radio quiet quasars and Seyfert 1 galaxies. The ratio of H..beta../(O III) emission line fluxes is found to correlate well with L/sub x/ and may be used as a luminosity indicator. No such emission line versus L/sub x/ correlations are found for radio-bright QSOs, however. The five low z objects have very similar values of L/sub x//L/sub opt/approx.0.4, although L/sub x/ varies by a factor of approx.10. We conclude that photoionization by a continuum extending to X-ray energies is the dominant excitation in radio-quiet QSOs and that X-ray selected QSO samples will enable new studies of QSO evolution and the diffuse X-ray background.
Research Organization:
Harvard-Smithsonian Center for Astrophysics
OSTI ID:
7054747
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 239:2; ISSN AJLEA
Country of Publication:
United States
Language:
English