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19952026
most citedThe Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance

8k citations · 17.2k across the 40 of their papers we have counts for

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16 papers · 1 filter

astro-ph2008★ 104 cited

A catalog of mid-infrared sources in the Extended Groth Strip

P. Barmby, J. -S. Huang, M. L. N. Ashby +3

The Extended Groth Strip (EGS) is one of the premier fields for extragalactic deep surveys. Deep observations of the EGS with the Infrared Array Camera (IRAC) on the Spitzer Space…

astro-ph2007★ 63 cited

The rest-frame -band luminosity function of galaxies in clusters to

R. De Propris, S. A. Stanford, P. R. Eisenhardt +2

We derive the rest-frame -band luminosity function for galaxies in 32 clusters at using deep m and m imaging from the Spitzer Space Telescope InfraRe…

astro-ph2006★ 71 cited

Multiaperture Photometry of Galaxies in the Coma Cluster

P. R. Eisenhardt, R. De Propris, A. Gonzalez +3

We present a set of photometry for 745 band selected objects in a region centered on the core of the Coma cluster. This includes 516 galaxi…

astro-ph2006★ 595 cited

The All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets

M. Davis, P. Guhathakurta, N. Konidaris +53

In this the first of a series of Letters, we present a description of the panchromatic data sets that have been acquired in the Extended Groth Strip region of the sky. Our survey,…

astro-ph2005★ 628 cited

The Mass Assembly History of Field Galaxies: Detection of an Evolving Mass Limit for Star Forming Galaxies

Kevin Bundy, Richard S. Ellis, Christopher J. Conselice +7

We characterize the mass-dependent evolution in a large sample of more than 8,000 galaxies using spectroscopic redshifts drawn from the DEEP2 Galaxy Redshift Survey in the range 0.…

astro-ph2005★ 31 cited

Preliminary Design of The Wide-Field Infrared Survey Explorer (WISE)

A. K. Mainzer, P. Eisenhardt, E. L. Wright +5

The Wide-field Infrared Survey Explorer (WISE), a NASA MIDEX mission, will survey the entire sky in four bands from 3.3 to 23 microns with a sensitivity 1000 times greater than the…