activity
19952009
most citedMultiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges

346 citations · 1.9k across the 36 of their papers we have counts for

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Showing 2003Show all

15 papers · 1 filter

astro-ph2003

IZw1 observed with XMM-Newton: Low-energy spectral complexity, iron lines, and hard X-ray flares

L. C. Gallo, Th. Boller, W. N. Brandt +2

We present a 20 ks XMM-Newton observation of the prototypical Narrow-Line Seyfert 1 galaxy IZw1. The best-fit model to the data is a double blackbody plus a dominant power-law, on…

astro-ph2003

Dramatic X-ray Spectral Variability of the Broad Absorption Line Quasar PG2112+059

S. C. Gallagher, W. N. Brandt, Beverley J. Wills +3

With a 1999 ASCA observation, PG2112+059 became notable as the first Broad Absorption Line (BAL) quasar found to exhibit a typical radio-quiet quasar X-ray continuum underlying a l…

astro-ph2003

Arakelian 564: An XMM-Newton view

C. Vignali, W. N. Brandt, Th. Boller +2

We report on two XMM-Newton observations of the bright narrow-line Seyfert 1 galaxy Ark 564 taken one year apart (2000 June and 2001 June). The 0.6-10 keV continuum is well describ…

astro-ph2003

The X-ray variability of the Narrow-Line Seyfert 1 galaxy IRAS 13224-3809 from an XMM-Newton observation

L. C. Gallo, Th. Boller, Y. Tanaka +5

We report on the XMM-Newton timing properties of the most X-ray variable, radio-quiet, NLS1 IRAS 13224-3809. IRAS 13224-3809 continues to display the extremely variable behavior th…

astro-ph2003

The Space Density of High-Redshift QSOs in the GOODS Survey

S. Cristiani, D. M. Alexander, F. Bauer +14

We present a sample of 17 high-redshift (3.5<z<5.2) QSO candidates in the 320 sq.arcmin area of the Great Observatories Origins Deep Survey, selected in the magnitude range 22.45<z…

astro-ph2003

The X-ray Properties of the Nearby Star-Forming Galaxy IC 342: The XMM-Newton View

F. E. Bauer, W. N. Brandt, B. Lehmer

We present the X-ray properties of IC342 using XMM-Newton. Thirty-five sources are detected coincident with the disk of IC342 (more than tripling the number known), of which ~31 ar…