activity
19952005
most citedAn X-ray Galaxy Cluster Survey for Investigations of Dark Energy

4 citations · 4 across the 3 of their papers we have counts for

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Showing 2005Show all

6 papers · 1 filter

astro-ph2005

XMM-Newton Archival Study of the ULX Population in Nearby Galaxies

L. M. Winter, R. F. Mushotzky, C. S. Reynolds

We present the results of an archival XMM-Newton study of the bright X-ray point sources (L_X > 10^38 erg/s) in 32 nearby galaxies. From our list of approximately 100 point sources…

astro-ph2005

Oxygen and Iron Abundances in Nearby Galaxies Using Ultraluminous X-ray Sources

Lisa M. Winter, Richard F. Mushotzky, Christopher S. Reynolds

We determined oxygen and iron abundances of the interstellar medium (ISM) using K-shell (O) and L-shell (Fe) X-ray photo-ionization edges towards Ultra luminous X-ray sources (ULXs…

astro-ph2005

Evidence for Gravitational Infall of Matter onto the Super-Massive Black Hole in the quasar PG 1211+143?

J. N. Reeves, K. Pounds, P. Uttley +5

We report the detection of redshifted iron K-alpha absorption lines in the Chandra LETG spectrum of the narrow-line quasar, PG 1211+143. The absorption lines are observed at 4.22 k…

astro-ph2005

Simultaneous Ultraviolet and X-ray Observations of the Seyfert Galaxy NGC 4151. I. Physical Conditions in the X-ray Absorbers

S. B. Kraemer, I. M. George, D. M. Crenshaw +9

We present a detailed analysis of the intrinsic X-ray absorption in the Seyfert 1 galaxy NGC 4151 using Chandra/HETGS data obtained 2002 May, as part of a program which included si…

astro-ph20054 cited

An X-ray Galaxy Cluster Survey for Investigations of Dark Energy

Z. Haiman, S. Allen, N. Bahcall +34

The amount and nature of dark energy (DE) can be tightly constrained by measuring the spatial correlation features and evolution of a sample of ~ 100,000 galaxy clusters over the r…

astro-ph2005

Radio Emission Associated with the ULX in Holmberg II

Neal A. Miller, Richard Mushotzky, Susan Neff

We report the detection of radio emission coincident with the ultraluminous X-ray source (ULX) in Holmberg II. The radio emission is diffuse and resolved, covering an area ~60 by 4…