activity
20082024
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 8k across the 136 of their papers we have counts for

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Showing 2014Show all

53 papers · 1 filter

astro-ph.GA201412 cited

Star Formation in High-Redshift Cluster Ellipticals

Cory R. Wagner, Mark Brodwin, Gregory F. Snyder +11

We measure the star formation rates (SFRs) of massive () early-type galaxies (ETGs) in a sample of 11 high-redshift () galaxy clusters…

astro-ph.HE201459 cited

Coronal Properties of the Seyfert 1.9 Galaxy MCG -05-23-016 Determined from Hard X-ray Spectroscopy with NuSTAR

M. Baloković, G. Matt, F. A. Harrison +15

Measurements of the high-energy cut-off in the coronal continuum of active galactic nuclei have long been elusive for all but a small number of the brightest examples. We present a…

astro-ph.HE201464 cited

The hard X-ray spectrum of NGC 5506 as seen by NuSTAR

G. Matt, M. Balokovic, A. Marinucci +12

NuSTAR observed the bright Compton-thin, narrow line Seyfert 1 galaxy, NGC 5506, for about 56 ks. In agreement with past observations, the spectrum is well fit by a power law with…

astro-ph.GA201433 cited

A Focused, Hard X-ray Look at Arp 299 with NuSTAR

A. Ptak, A. Hornschemeier, A. Zezas +19

We report on simultaneous observations of the local starburst system Arp 299 with NuSTAR and Chandra, which provides the first resolved images of this galaxy up to energies of ~ 45…

astro-ph.HE201428 cited

The Hard X-Ray View of the Young Supernova Remnant G1.9+0.3

Andreas Zoglauer, Stephen P. Reynolds, Hongjun An +12

NuSTAR observed G1.9+0.3, the youngest known supernova remnant in the Milky Way, for 350 ks and detected emission up to 30 keV. The remnant's X-ray morphology does not change…

astro-ph.HE201435 cited

The Seyfert 2 galaxy NGC 2110: hard X-ray emission observed by NuSTAR and variability of the iron K line

A. Marinucci, G. Matt, S. Bianchi +16

We present NuSTAR observations of the bright Seyfert 2 galaxy NGC 2110 obtained in 2012, when the source was at the highest flux level ever observed, and in 2013, when the source w…