activity
19962026
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 17k across the 230 of their papers we have counts for

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Showing 2019Show all

19 papers · 1 filter

astro-ph.GA2019★ 11 cited

The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223

R. Carvajal, F. E. Bauer, R. J. Bouwens +15

The Hubble Frontier Fields offer an exceptionally deep window into the high-redshift universe, covering a substantially larger area than the Hubble Ultra-Deep field at low magnific…

astro-ph.GA2019★ 33 cited

Spectral Classification and Ionized Gas Outflows in WISE-Selected Hot Dust-Obscured Galaxies

Hyunsung D. Jun, Roberto J. Assef, Franz E. Bauer +7

We present VLT/XSHOOTER rest-frame UV-optical spectra of 10 Hot Dust-Obscured Galaxies (Hot DOGs) at to investigate AGN diagnostics and to assess the presence and effect o…

astro-ph.GA2019★ 49 cited

An ALMA CO(2-1) Survey of Nearby Palomar-Green Quasars

Jinyi Shangguan, Luis C. Ho, Franz E. Bauer +2

The properties of the molecular gas can shed light on the physical conditions of quasar host galaxies and the effect of feedback from accreting supermassive black holes. We present…

astro-ph.GA2019★ 43 cited

BAT AGN Spectroscopic Survey -- XIX: Type 1 versus Type 2 AGN dichotomy from the point of view of ionized outflows

A. F. Rojas, E. Sani, I. Gavignaud +18

We present a detailed study of ionized outflows in a large sample of ~650 hard X-ray detected AGN. Using optical spectroscopy from the BAT AGN Spectroscopic Survey (BASS) we are ab…

astro-ph.GA2019★ 13 cited

How to Fuel an AGN: Mapping Circumnuclear Gas in NGC 6240 with ALMA

Anne M. Medling, George C. Privon, Loreto Barcos-Muñoz +15

Dynamical black hole mass measurements in some gas-rich galaxy mergers indicate that they are overmassive relative to their host galaxy properties. Overmassive black holes in these…

astro-ph.GA2019★ 102 cited

The X-ray properties of quasars: no evident evolution of accretion physics in the first Gyr of the Universe

Fabio Vito, William Nielsen Brandt, Franz Erik Bauer +10

X-ray emission from QSOs has been used to assess SMBH accretion properties up to ~6. However, at only ~15 QSOs are covered by sensitive X-ray observations, preventing a st…