activity
20022023
most citedThe 70 Month Swift-BAT All-Sky Hard X-Ray Survey

619 citations · 4.5k across the 68 of their papers we have counts for

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Showing 2013Show all

7 papers · 1 filter

astro-ph.HE2013★ 112 cited

Long-term variability of AGN at hard X-rays

S. Soldi, V. Beckmann, W. H. Baumgartner +6

Variability at all observed wavelengths is a distinctive property of AGN. Hard X-rays provide us with a view of the innermost regions of AGN, mostly unbiased by absorption along th…

astro-ph.CO2013★ 17 cited

Reflection-dominated nuclear X-ray emission in the early-type galaxy ESO 565--G019

P. Gandhi, Y. Terashima, S. Yamada +8

We present the discovery of a reflection-dominated active galactic nucleus (AGN) in the early-type radio-quiet galaxy ESO 565--G019 with Suzaku and Swift/BAT. The source X-ray spec…

astro-ph.HE2013★ 6 cited

White Paper for Blazar Observations with a GEMS-like X-ray Polarimetry Mission

Henric Krawczynski, Lorella Angelini, Matthew Baring +27

In this document, we describe the scientific potential of blazar observations with a X-ray polarimetry mission like GEMS (Gravity and Extreme Magnetism SMEX). We describe five blaz…

astro-ph.HE2013★ 66 cited

Kepler observations of rapid optical variability in the BL Lac object W2R1926+42

R. Edelson, R. Mushotzky, S. Vaughan +4

We present the first Kepler monitoring of a strongly variable BL Lac, W2R1926+42. The light curve covers 181 days with ~0.2% errors, 30 minute sampling and >90% duty cycle, showing…

astro-ph.HE2013★ 6 cited

White Paper on GEMS Study of Polarized X-rays from Neutron Stars

Pranab Ghosh, Lorella Angelini, Matthew Baring +27

We examine the expected X-ray polarization properties of neutron-star X-ray sources of various types, e.g., accretion and rotation powered pulsars, magnetars, and low-mass X-ray bi…

astro-ph.HE2013★ 47 cited

Studying Faint Ultra Hard X-ray Emission from AGN in GOALS LIRGs with Swift BAT

Michael Koss, Richard Mushotzky, Wayne Baumgartner +4

We present the first analysis of the all-sky Swift BAT ultra hard X-ray (14-195 keV) data for a targeted list of objects. We find the BAT data can be studied at 3x fainter limits t…