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20002026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 16.5k across the 104 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 8 cited

The Molecular Hydrogen Explorer H2EX

F. Boulanger, J. P. Maillard, P. Appleton +12

The Molecular Hydrogen Explorer, H2EX, was proposed in response to the ESA 2015 - 2025 Cosmic Vision Call as a medium class space mission with NASA and CSA participations. The miss…

astro-ph2006★ 35 cited

The role of the LIRG and ULIRG phases in the evolution of Ks-selected galaxies

K. I. Caputi, H. Dole, G. Lagache +5

We investigate the role of the luminous infrared galaxy (LIRG) and ultra-luminous infrared galaxy (ULIRG) phases in the evolution of Ks-selected galaxies and, in particular, Extrem…

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★ 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-ph2003★ 69 cited

The large-scale anomalous microwave emission revisited by WMAP

G. Lagache

We present a new study of the high latitude galactic contributions to the millimeter sky, based on an analysis of the WMAP data combined with several templates of dust emission (DI…