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20062026
most citedThe Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance

8k citations · 12.7k across the 69 of their papers we have counts for

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Showing 2017 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2017★ 66 cited

Heavy X-ray obscuration in the most-luminous galaxies discovered by WISE

F. Vito, W. N. Brandt, D. Stern +11

Hot Dust-Obscured Galaxies (Hot DOGs) are hyperluminous () infrared galaxies with extremely high (up to hundreds of K) dust tempe…

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★ 26 cited

Overdensities of SMGs around WISE-selected, ultra-luminous, high-redshift AGN

Suzy F. Jones, Andrew W. Blain, Roberto J. Assef +9

We investigate extremely luminous dusty galaxies in the environments around WISE-selected hot dust obscured galaxies (Hot DOGs) and WISE/radio-selected active galactic nuclei (AGNs…

astro-ph.GA2017★ 63 cited

Eddington-Limited Accretion in z~2 WISE-selected Hot, Dust-Obscured Galaxies

Jingwen Wu, Hyunsung D. Jun, Roberto J. Assef +12

Hot, Dust-Obscured Galaxies, or "Hot DOGs", are a rare, dusty, hyperluminous galaxy population discovered by the WISE mission. Predominantly at redshifts 2-3, they include the most…

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…