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20042013
most citedThe 24 Micron Source Counts in Deep Spitzer Surveys

335 citations · 1.3k across the 20 of their papers we have counts for

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astro-ph2008★ 70 cited

The IR Luminosity Functions of Rich Clusters

Lei Bai, George H. Rieke, Marcia J. Rieke +2

We present MIPS observations of the cluster A3266. About 100 spectroscopic cluster members have been detected at 24 micron. The IR luminosity function in A3266 is very similar to t…

astro-ph2008★ 50 cited

The Late Stellar Assembly of Massive Cluster Galaxies Via Major Merging

Kim-Vy H. Tran, John Moustakas, Anthony H. Gonzalez +3

We present multi-wavelength observations of the brightest galaxies in four X-ray luminous groups at z~0.37 that will merge to form a cluster comparable in mass to Coma. Ordered by…

astro-ph2008★ 36 cited

Spitzer 24 micron detections of starburst galaxies in Abell 851

A. Dressler, J. Rigby, A. Oemler +4

Spitzer-MIPS 24 micron and ground-based observations of the rich galaxy cluster Abell 851 at z=0.41 are used to derive star formation rates from the mid-IR 24 micron and from [O II…

astro-ph2008★ 7 cited

The Flux Auto- and Cross-Correlation of the Lyman-alpha Forest. I. Spectroscopy of QSO Pairs with Arcminute Separations and Similar Redshifts

Andrew R. Marble, Kristoffer A. Eriksen, Chris D. Impey +2

The Lyman-alpha forest has opened a new redshift regime for cosmological investigation. At z > 2 it provides a unique probe of cosmic geometry and an independent constraint on dark…

astro-ph2007★ 27 cited

Search for IR Emission from Intracluster Dust in A2029

Lei Bai, George H. Rieke, Marcia J. Rieke

We have searched for IR emission from the intracluster dust (ICD) in the galaxy cluster A2029. Weak signals of enhanced extended emission in the cluster are detected at both 24 and…

astro-ph2007★ 84 cited

IR observations of MS 1054-03: Star Formation and its Evolution in Rich Galaxy Clusters

Lei Bai, Delphine Marcillac, George H. Rieke +6

We study the infrared (IR) properties of galaxies in the cluster MS 1054-03 at z=0.83 by combining MIPS 24 micron data with spectra of more than 400 galaxies and a very deep K-band…