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20012024
most citedSINGS: The SIRTF Nearby Galaxies Survey

1.3k citations · 6.5k across the 34 of their papers we have counts for

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Showing 2004Show all

7 papers · 1 filter

astro-ph2004★ 133 cited

Planets and IR Excesses: Preliminary Results from a Spitzer/MIPS Survey of Solar-Type Stars

C. A. Beichman, G. Bryden, G. H. Rieke +10

As part of a large Spitzer/MIPS GTO program, we have searched for infrared excesses due to debris disks toward 26 FGK field stars known from radial velocity (RV) studies to have on…

astro-ph2004★ 290 cited

The Anatomy of Star Formation in NGC 300

G. Helou, H. Roussel, P. Appleton +19

The Spitzer Space Telescope was used to study the mid-infrared to far-infrared properties of NGC 300, and to compare dust emission to Halpha to elucidate the heating of the ISM and…

astro-ph2004★ 108 cited

Far Infrared Source Counts at 70 and 160 microns in Spitzer Deep Surveys

H. Dole, E. Le Floc'h, P. G. Perez-Gonzalez +21

We derive galaxy source counts at 70 and 160 microns using the Multiband Imaging Photometer for Spitzer (MIPS) to map the Chandra Deep Field South (CDFS) and other fields. At 70 mi…

astro-ph2004★ 113 cited

SPITZER Observations of the SCUBA/VLA Sources in the Lockman Hole: Star Formation History of Infrared-Luminous Galaxies

E. Egami, H. Dole, J. -S. Huang +24

We present Spitzer IRAC (3.6, 4.5, 5.8, 8.0 um) and MIPS (24 um) observations of the SCUBA submillimeter sources and uJy VLA radio sources in a 5'x5' area in the Lockman Hole East…

astro-ph2004★ 84 cited

Spatially Resolved Ultraviolet, H-alpha, Infrared, and Radio Star Formation in M81

K. D. Gordon, P. G. Perez-Gonzalez, K. A. Misselt +26

We present Multiband Imaging Photometer for Spitzer (MIPS) observations of M81 at 24, 70, and 160 micron. The grand design nature of M81 is clearly seen, showing two well resolved…

astro-ph2004★ 96 cited

Confusion in the infrared: Spitzer and beyond

H. Dole, G. H. Rieke, G. Lagache +23

We use the source counts measured with the Multiband Imaging Photometer for Spitzer (MIPS) at 24, 70, and 160 microns to determine the 5-sigma confusion limits due to extragalactic…