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20002026
most citedSINGS: The SIRTF Nearby Galaxies Survey

1.3k citations · 18.9k across the 172 of their papers we have counts for

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33 papers · 1 filter

astro-ph2008★ 44 cited

Are red 2MASS QSOs young?

A. Georgakakis, D. L. Clements, G. Bendo +3

We use photometric data from Spitzer to explore the mid- and far-IR properties of 10 red QSOs (J-K>2, R-K>5) selected by combining the 2MASS in the NIR with the SDSS at optical wav…

astro-ph2008★ 113 cited

The JCMT Nearby Galaxies Legacy Survey I. Star Forming Molecular Gas in Virgo Cluster Spiral Galaxies

C. D. Wilson, B. E. Warren, F. P. Israel +20

We present large-area maps of the CO J=3-2 emission obtained at the James Clerk Maxwell Telescope for four spiral galaxies in the Virgo Cluster. We combine these data with publishe…

astro-ph2008★ 58 cited

Mid- to Far-IR Emission and Star Formation in Early-Type Galaxies

L M Young, G J Bendo, Danielle Lucero

Many early-type galaxies have been detected at wavelengths of 24 to 160 micron, but the emission is usually dominated by heating from an AGN or from the evolved stellar population.…

astro-ph2008★ 124 cited

The relations among 8, 24, and 160 micron dust emission within nearby spiral galaxies

G. J. Bendo, B. T. Draine, C. W. Engelbracht +9

We investigate the relations among the stellar continuum-subtracted 8 micron polycyclic aromatic hydrocarbon (PAH 8 micron) emission, 24 micron hot dust emission, and 160 micron co…

astro-ph2008★ 8 cited

LABOCA and MAMBO-2 imaging of the dust ring of the Sombrero galaxy (NGC 4594)

C. Vlahakis, M. Baes, G. Bendo +1

The Sombrero galaxy (NGC 4594) is an Sa galaxy with a symmetric dust ring. We have used the Large APEX BOlometer CAmera (LABOCA) at 870 micron and the MAx-Planck Millimeter BOlomet…

astro-ph2008★ 4 cited

A Spitzer view of star formation in early-type galaxies

L. M. Young, G. J. Bendo, D. M. Lucero

Many early-type galaxies are detected at 24 to 160 micron but the emission is usually dominated by an AGN or heating from the evolved stellar population. Here we present MIPS obser…