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20112025
most citedMid-Infrared Selection of AGN with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-Selected AGN in COSMOS

827 citations · 2.1k across the 18 of their papers we have counts for

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10 papers · 1 filter

astro-ph.GA2025

The Host Galaxy of FRB 20190520B and Its Unique Ionized Gas Distribution

Xiang-Lei Chen, Chao-Wei Tsai, Daniel Stern +13

The properties of host galaxies associated with Fast Radio Bursts (FRBs) provide critical information for inferring the progenitors and radiation mechanisms of these bursts. We rep…

astro-ph.GA2023★ 10 cited

Discovery of a Low-Redshift Hot Dust-Obscured Galaxy

Guodong Li, Chao-Wei Tsai, Daniel Stern +10

We report the discovery of the hyperluminous, highly obscured AGN WISE J190445.04+485308.9 (W1904+4853 hereafter, ) at z=0.415. Its well-s…

astro-ph.GA2021★ 36 cited

Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA

Tanio Diaz-Santos, Roberto J. Assef, Peter R. M. Eisenhardt +9

Hot, dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous obscured quasars identified by WISE. We present ALMA observations of the [CII] fine-structure line and und…

astro-ph.GA2019★ 2 cited

The Contribution of Galaxies to the Cosmic Infrared Background as Measured Using WISE

Sean E. Lake, Edward L. Wright, Roberto J. Assef +4

The study of the extragalactic background light (EBL) in the optical and near infrared has received a lot of attention in the last decade, especially near a wavelength of $λ\approx…

astro-ph.GA2017★ 34 cited

The role of the most luminous, obscured AGN in galaxy assembly at z~2

Duncan Farrah, Sara Petty, Brian Connolly +14

We present HST WFC3 F160W imaging and infrared spectral energy distributions for twelve extremely luminous, obscured AGN at , selected via "Hot, Dust Obscured" mid-infra…

astro-ph.GA2017★ 4 cited

The 2.4 m Galaxy Luminosity Function as Measured Using WISE. III. Measurement Results

S. E. Lake, E. L. Wright, R. J. Assef +5

The WISE satellite surveyed the entire sky multiple times in four infrared wavelengths (3.4, 4.6, 12, and m; Wright et al. 2010). The unprecedented combination of coverage a…

astro-ph.GA2017★ 1 cited

The 2.4 m Galaxy Luminosity Function as Measured Using WISE. II. Sample Selection

S. E. Lake, E. L. Wright, R. J. Assef +5

The WISE satellite surveyed the entire sky multiple times in four infrared (IR) wavelengths ( and m, Wright et al. 2010). This all-sky IR photometric surve…

astro-ph.GA2016★ 4 cited

-corrections: an Examination of their Contribution to the Uncertainty of Luminosity Measurements

Sean E. Lake, E. L. Wright

In this paper we provide formulae that can be used to determine the uncertainty contributed to a measurement by a -correction and, thus, valuable information about which flux me…

astro-ph.GA2014★ 125 cited

NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-Selected Quasars at z ~ 2

D. Stern, G. B. Lansbury, R. J. Assef +30

We report on a NuSTAR and XMM-Newton program that has observed a sample of three extremely luminous, heavily obscured WISE-selected AGN at z~2 in a broad X-ray band (0.1 - 79 keV).…

astro-ph.GA2011★ 29 cited

Optical Spectroscopic Survey of High Latitude WISE Selected Sources

Sean E. Lake, Edward L. Wright, Sara Petty +5

We report on the results of an optical spectroscopic survey at high Galactic latitude (b\geq30°) of a sample of WISE-selected targets, grouped by WISE W1 (λ_eff = 3.4 \mum) flux, w…