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20032006
most citedCan the unresolved X-ray background be explained by emission from the optically-detected faint galaxies of the GOODS project?

33 citations · 64 across the 2 of their papers we have counts for

collaborators

11 papers

astro-ph200633 cited

Can the unresolved X-ray background be explained by emission from the optically-detected faint galaxies of the GOODS project?

M. A. Worsley, A. C. Fabian, F. E. Bauer +3

The emission from individual X-ray sources in the Chandra Deep Fields and XMM-Newton Lockman Hole shows that almost half of the hard X-ray background above 6 keV is unresolved and…

astro-ph200631 cited

The Properties and Redshift Evolution of Intermediate-Luminosity Off-Nuclear X-ray Sources in the Chandra Deep Fields

B. D. Lehmer, W. N. Brandt, A. E. Hornschemeier +5

We analyze a population of intermediate-redshift (z ~ 0.05-0.3), off-nuclear X-ray sources located within optically-bright galaxies in the Great Observatories Origins Deep Survey (…

astro-ph2005

The Extended Chandra Deep Field-South Survey. Chandra Point-Source Catalogs

B. D. Lehmer, W. N. Brandt, D. M. Alexander +17

We present Chandra point-source catalogs for the Extended Chandra Deep Field-South (E-CDF-S) survey. The E-CDF-S consists of four contiguous 250 ks Chandra observations covering an…

astro-ph2005

The Chandra Deep Field South/GOODS survey. Optically faint X-ray sources

V. Mainieri, P. Rosati, P. Tozzi +11

We provide important new constraints on the nature and redshift distribution of optically faint (R>25) X-ray sources in the Chandra Deep Field South Survey. We show that we can der…

astro-ph2004

The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM-Newton deep fields

M. A. Worsley, A. C. Fabian, F. E. Bauer +6

We extend our earlier work on X-ray source stacking in the deep XMM-Newton observation of the Lockman Hole, to the 2 Ms Chandra Deep Field North and the 1 Ms Chandra Deep Field Sou…

astro-ph2004

The Chandra Deep Field-North Survey: XVII. Evolution of magnetic activity in old late-type stars

E. D. Feigelson, A. E. Hornschemeier, G. Micela +11

The extremely sensitive Chandra Deep Field-North (CDF-N) pencil-beam X-ray survey is used to identify and characterize the X-ray emission from old high-latitude main sequence Galac…