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A two-parameter model for the infrared/submillimeter/radio spectral energy distributions of galaxies and active galactic nuclei
ABSTRACT A two-parameter semi-empirical model is presented for the spectral energy
distributions of galaxies with contributions to their infrared–submillimeter–radio emission …
distributions of galaxies with contributions to their infrared–submillimeter–radio emission …
The herschel atlas
The Herschel ATLAS is the largest open-time key project that will be carried out on the
Herschel Space Observatory. It will survey 570 deg 2 of the extragalactic sky, 4 times larger …
Herschel Space Observatory. It will survey 570 deg 2 of the extragalactic sky, 4 times larger …
S-COSMOS: The Spitzer legacy survey of the Hubble Space Telescope ACS 2 deg2 COSMOS field I: survey strategy and first analysis
Abstract The COSMOS Spitzer survey (S-COSMOS) is a Legacy program (Cycles 2+ 3)
designed to carry out a uniform deep survey of the full 2 deg 2 COSMOS field in all seven …
designed to carry out a uniform deep survey of the full 2 deg 2 COSMOS field in all seven …
The cosmic infrared background resolved by Spitzer-Contributions of mid-infrared galaxies to the far-infrared background
H Dole, G Lagache, JL Puget, KI Caputi… - Astronomy & …, 2006 - aanda.org
Aims. We quantify the contributions of 24 μm galaxies to the Far-Infrared (FIR) Background
at 70 and 160 μm. We provide new estimates of the Cosmic Infrared Background (CIB), and …
at 70 and 160 μm. We provide new estimates of the Cosmic Infrared Background (CIB), and …
Evolution of the dusty infrared luminosity function from z= 0 to z= 2.3 using observations from Spitzer
Aims. We derive the evolution of the infrared luminosity function (LF) over the last 4/5ths of
cosmic time using deep 24 and 70 μm imaging of the GOODS North and South fields …
cosmic time using deep 24 and 70 μm imaging of the GOODS North and South fields …
Dust obscuration and metallicity at high redshift: new inferences from UV, Hα, and 8 μm observations of z∼ 2 star-forming galaxies
We use a sample of 90 spectroscopically confirmed Lyman break galaxies with Hα
measurements and Spitzer MIPS 24 μm observations to constrain the relationship between …
measurements and Spitzer MIPS 24 μm observations to constrain the relationship between …
The 0.4 z 1.3 star formation history of the Universe as viewed in the far-infrared
Aims. We use the deepest existing mid-and far-infrared observations (reaching~ 3 mJy at 70
μm) obtained with Spitzer in the Great Observatories Origins Deep Survey (GOODS) and Far …
μm) obtained with Spitzer in the Great Observatories Origins Deep Survey (GOODS) and Far …
Deep Spitzer 24 μm COSMOS imaging. I. The evolution of luminous dusty galaxies—confronting the models
E Le Floc'h, H Aussel, O Ilbert, L Riguccini… - The Astrophysical …, 2009 - iopscience.iop.org
We present the first results obtained from the identification of∼ 30,000 sources in the
Spitzer/24 μm observations of the COSMOS field at S 24 μm≳ 80 μJy. Using accurate …
Spitzer/24 μm observations of the COSMOS field at S 24 μm≳ 80 μJy. Using accurate …
A lower-limit flux for the extragalactic background light
TM Kneiske, H Dole - Astronomy & Astrophysics, 2010 - aanda.org
Context. The extragalactic background light (EBL) contains information about the evolution
of galaxies from very early times up to the present. The spectral energy distribution is not …
of galaxies from very early times up to the present. The spectral energy distribution is not …
A hybrid model for the evolution of galaxies and Active Galactic Nuclei in the infrared
We present a comprehensive investigation of the cosmological evolution of the luminosity
function of galaxies and active galactic nuclei (AGNs) in the infrared (IR). Based on the …
function of galaxies and active galactic nuclei (AGNs) in the infrared (IR). Based on the …