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20042009
most citedDust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

1.1k citations · 1.6k across the 6 of their papers we have counts for

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astro-ph200878 cited

Spitzer Observations of the z=2.73 Lensed Lyman Break Galaxy, MS1512-cB58

Brian Siana, Harry I. Teplitz, Ranga-Ram Chary +2

We present Spitzer infrared (IR) photometry and spectroscopy of the lensed Lyman break galaxy (LBG), MS1512-cB58 at z=2.73. The large (factor ~30) magnification allows for the most…

astro-ph200820 cited

A Lyman Break Galaxy Candidate at z~9

Alaina L. Henry, Matthew A. Malkan, James W. Colbert +3

We report the discovery of a z~9 Lyman Break Galaxy (LBG) candidate, selected from the NICMOS Parallel Imaging Survey as a J-dropout with J110 - H160 = 1.7. Spitzer/IRAC photometry…

astro-ph2007379 cited

Mid-Infrared Spectral Diagnosis of Submillimeter Galaxies

Alexandra Pope, Ranga-Ram Chary, David M. Alexander +6

We present deep mid-infrared spectroscopy with the Spitzer Space Telescope of 13 submillimeter galaxies (SMGs) in the Great Observatories Origins Deep Survey North (GOODS-N) field.…

astro-ph200795 cited

A Detailed Study of Gas and Star Formation in a Highly Magnified Lyman Break Galaxy at z=3.07

K. E. K. Coppin, A. M. Swinbank, R. Neri +10

We report the detection of CO(3-2) emission from a bright, gravitationally lensed Lyman Break Galaxy, LBGJ213512.73-010143 (the 'Cosmic Eye'), at z=3.07 using the Plateau de Bure I…

astro-ph200725 cited

HUDF-JD2: Mid-infrared Evidence for a z~2 Luminous Infrared Galaxy

Ranga-Ram Chary, Harry I. Teplitz, Mark E. Dickinson +5

The Hubble Ultra Deep Field source JD2 presented in Mobasher et al. (2005) is an unusual galaxy that is very faint at all wavelengths shortward of 1.1 micron. Photometric redshift…

astro-ph20071.1k cited

Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

B. T. Draine, D. A. Dale, G. Bendo +17

Physical dust models are presented for 65 galaxies in the SINGS survey that are strongly detected in the four IRAC bands and three MIPS bands. For each galaxy we estimate (1) the t…