activity
20052026
most citedThe Chandra COSMOS Legacy survey: overview and point source catalog

511 citations · 5.3k across the 96 of their papers we have counts for

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Showing astro-ph.HEShow all

30 papers · 1 filter

astro-ph.HE2024

Stripe 82X Data Release 3: Multiwavelength Catalog with New Spectroscopic Redshifts and Black Hole Masses

Stephanie M. LaMassa, Alessandro Peca, C. Megan Urry +10

We present the third catalog release of the wide-area (31.3 deg) Stripe 82 X-ray survey. This catalog combines previously published X-ray source properties with multiwavelength…

astro-ph.HE2023★ 3 cited

The High Energy X-ray Probe (HEX-P): Bringing the Cosmic X-ray Background into Focus

Francesca Civano, Xiurui Zhao, Peter Boorman +29

Since the discovery of the cosmic X-ray background (CXB), astronomers have strived to understand the accreting supermassive black holes (SMBHs) contributing to its peak in the 10-4…

astro-ph.HE2023★ 3 cited

The High Energy X-ray Probe (HEX-P): The Circum-nuclear Environment of Growing Supermassive Black Holes

P. G. Boorman, N. Torres-Albà, A. Annuar +32

Ever since the discovery of the first Active Galactic Nuclei (AGN), substantial observational and theoretical effort has been invested into understanding how massive black holes ha…

astro-ph.HE2023

NGC 4388: A Test Case for Relativistic Disk Reflection and Fe K Fluorescence Features

Tahir Yaqoob, P. Tzanavaris, S. LaMassa

We present a new analysis of the Suzaku X-ray spectrum of the Compton-thin Seyfert 2 galaxy NGC 4388. The spectrum above 2 keV can be described by a remarkably simple and rat…

astro-ph.HE2023★ 5 cited

The Complex X-ray Obscuration Environment in the Radio Loud Type 2 Quasar 3C 223

Stephanie M. LaMassa, Tahir Yaqoob, Panayiotis Tzanavaris +4

3C 223 is a radio loud, Type 2 quasar at with an intriguing XMM-Newton spectrum that implicated it as a rare, Compton-thick ( cm$^…

astro-ph.HE2021★ 6 cited

Are Compton-thin AGNs Globally Compton Thin?

P. Tzanavaris, T. Yaqoob, S. LaMassa +2

We select eight nearby AGNs which, based on previous work, appear to be Compton-thin in the line of sight. We model with MYTORUS their broadband X-ray spectra from 20 individual ob…