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20102026
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 3.5k across the 68 of their papers we have counts for

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Showing 2014Show all

6 papers · 1 filter

astro-ph.HE2014★ 154 cited

NuSTAR Spectroscopy of Multi-Component X-ray Reflection from NGC 1068

Franz E. Bauer, Patricia Arevalo, Dominic J. Walton +26

We report on observations of NGC1068 with NuSTAR, which provide the best constraints to date on its ~keV spectral shape. We find no strong variability over the past two decade…

astro-ph.HE2014★ 767 cited

An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

M. Bachetti, F. A. Harrison, D. J. Walton +21

Ultraluminous X-ray sources (ULX) are off-nuclear point sources in nearby galaxies whose X-ray luminosity exceeds the theoretical maximum for spherical infall (the Eddington limit)…

astro-ph.HE2014★ 118 cited

No Time for Dead Time: Timing analysis of bright black hole binaries with NuSTAR

Matteo Bachetti, Fiona A. Harrison, Rick Cook +20

Timing of high-count rate sources with the NuSTAR Small Explorer Mission requires specialized analysis techniques. NuSTAR was primarily designed for spectroscopic observations of s…

astro-ph.HE2014★ 137 cited

The 2-79 keV X-ray Spectrum of the Circinus Galaxy with NuSTAR, XMM-Newton and Chandra: a Fully Compton-Thick AGN

P. Arévalo, F. E. Bauer, S. Puccetti +24

The Circinus galaxy is one of the nearest obscured AGN, making it an ideal target for detailed study. Combining archival Chandra and XMM-Newton data with new NuSTAR observations, w…

astro-ph.HE2014★ 87 cited

The Broad-band X-ray Spectrum of IC 4329A from a Joint NuSTAR/Suzaku Observation

Laura Brenneman, G. Madejski, F. Fuerst +16

We have obtained a deep, simultaneous observation of the bright, nearby Seyfert galaxy IC 4329A with Suzaku and NuSTAR. Through a detailed spectral analysis, we are able to robustl…

astro-ph.HE2014★ 52 cited

Reflection From the Strong Gravity Regime in a z=0.658 Gravitationally Lensed-Quasar

Rubens C. Reis, Mark T. Reynolds, Jon M. Miller +1

The co-evolution of a supermassive black hole with its host galaxy through cosmic time is encoded in its spin. At , supermassive black holes are thought to grow mostly by merg…