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20012026
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 25.3k across the 213 of their papers we have counts for

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Showing 2004 · astro-phShow all

7 papers · 2 filters

astro-ph2004

Evolution of the infrared luminosity density and star formation history up to z~1: preliminary results from MIPS

E. Le Floc'h, C. Papovich, H. Dole +6

Using deep observations of the Chandra Deep Field South obtained with MIPS at 24mic, we present our preliminary estimates on the evolution of the infrared (IR) luminosity density o…

astro-ph2004★ 36 cited

The nature of luminous X-ray sources with mid-infrared counterparts

A. Alonso-Herrero, P. G. Perez-Gonzalez, J. Rigby +28

We investigate the luminous X-ray sources in the Lockman Hole (LH) and the Extended Groth Strip (EGS) detected at 24microns using MIPS and also with IRAC on board Spitzer. We assem…

astro-ph2004★ 59 cited

Identification of luminous infrared galaxies at 1<z<2.5

E. Le Floc'h, P. G. Perez-Gonzalez, G. H. Rieke +24

We present preliminary results on 24micron detections of luminous infrared galaxies at z>1 with the Multiband Imaging Photometer for Spitzer (MIPS). Observations were performed in…

astro-ph2004★ 77 cited

IRAC Imaging of Lockman Hole

J. -S. Huang, P. Barmby, G. G. Fazio +17

IRAC imaging of a 4'7x4'7 area in the Lockman Hole detected over 400 galaxies in the IRAC 3.6 micron and 4.5 micron bands, 120 in the 5.8 micron, and 80 in the 8 micron bandin 30 m…

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…

astro-ph2004★ 275 cited

PAHs contribution to the infrared output energy of the Universe at z~2

G. Lagache, H. Dole, J. -L. Puget +10

We present an updated phenomenological galaxy evolution model to fit the Spitzer 24, 70 and 160 microns number counts as well as all the previous mid and far infrared observations.…