Exploratory Chandra Observations of Large Bright Quasar Survey BAL QSOs

Details Exploratory Chandra Observations of Large Bright Quasar Survey BAL QSOs Exploratory Chandra Observations of Large Bright Quasar Survey BAL QSOs

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprd11006g&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

Broad Absorption Line QSOs are notoriously faint X-ray sources. To elucidate the X-ray properties of the population as a whole, we are conducting a survey of a well-defined sample of 18 BAL QSOs from the Large Bright Quasar Survey with the Chandra ACIS-S3 instrument. The low background and excellent spatial resolution of Chandra permit sensitive observations in a relatively short time. With the ACIS data and optical spectroscopic follow-up with the Hobby-Eberly Telescope, we compare the X-ray properties of the BAL QSOs with their ultraviolet absorption and emission-line characteristics.

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