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19992025
most citedChandra Detects Relativistic Broad Absorption Lines from APM 08279+5255

288 citations · 1.1k across the 12 of their papers we have counts for

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astro-ph2005★ 33 cited

Variation in the Scattering Shroud Surrounding Markarian 231

S. C. Gallagher, Gary D. Schmidt, Paul S. Smith +5

We present a detailed study of the nuclear structure of the highly polarized broad absorption line quasar, Mrk 231, through a multiwavelength campaign of Chandra observations, opti…

astro-ph2003★ 209 cited

XMM-NEWTON Reveals the Quasar Outflow in PG 1115+080

G. Chartas, W. N. Brandt, S. C. Gallagher

We report on an observation of the Broad Absorption Line (BAL) quasar PG 1115+080 performed with the XMM-Newton observatory. Spectral analysis reveals the second case of a relativi…

astro-ph2002★ 185 cited

The Chandra Deep Field-North Survey. XIV. X-ray detected Obscured AGNs and Starburst Galaxies in the Bright Submm Source Population

D. M. Alexander, F. E. Bauer, W. N. Brandt +6

We provide X-ray constraints and perform the first X-ray spectral analyses for bright (f_850>=5mJy; S/N>=4) SCUBA sources in an 8.4'x8.4' area of the 2 Ms Chandra Deep Field-North…

astro-ph2002★ 288 cited

Chandra Detects Relativistic Broad Absorption Lines from APM 08279+5255

G. Chartas, W. N. Brandt, S. C. Gallagher +1

We report the discovery of X-ray broad absorption lines (BALs) from the BALQSO APM 08279+5255 originating from material moving at relativistic velocities with respect to the centra…

astro-ph2001

X-ray Spectroscopy of BAL and Mini-BAL QSOs

S. C. Gallagher, W. N. Brandt, G. Chartas +1

BAL QSOs are notoriously faint X-ray sources, presumably due to extreme intrinsic absorption. However, several objects have begun to appear through the obscuration with recent X-ra…

astro-ph2000★ 43 cited

Observational Similarities and Potential Connections Between Luminous Ultrasoft NLS1s and BALQSOs

W. N. Brandt, S. C. Gallagher

Luminous ultrasoft NLS1s and low-ionization BALQSOs share many properties, and they both represent important extremes of the active galaxy phenomenon. We briefly discuss their obse…