HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift

Abstract

We quantify the fraction of the cosmic infrared background (CIB) that originates from galaxies identified in the UV/optical/near-infrared by stacking 81,250 (~35.7 arcmin^2) K-selected sources (K_AB < 24.0), split according to their rest-frame U - V vs. V - J colors into 72,216 star-forming and 9,034 quiescent galaxies, on maps from Spitzer/MIPS (24um), Herschel/SPIRE (250, 350, 500um), Herschel/PACS (100, 160um), and AzTEC (1100um). The fraction of the CIB resolved by our catalog is (69 $\pm$ 15)% at 24um, (78 $\pm$ 17)% at 70um, (58 $\pm$ 13)% at 100um, (78 $\pm$ 18)% at 160um, (80 $\pm$ 17)% at 250um, (69 $\pm$ 14)% at 350um, (65 $\pm$ 12)% at 500um, and (45 $\pm$ 8)% at 1100um. Of that total, about 95% originates from star-forming galaxies, while the remaining 5% is from apparently quiescent galaxies. The CIB at $\lambda$ < 200um is sourced predominantly from galaxies at z < 1, while at $\lambda$ > 200um the bulk originates from 1 < z < 2. Galaxies with stellar masses log(M/ M_sun)=9.5-11 are responsible for the majority of the CIB, with those in the log(M/ M_sun)=9.5-10 contributing mostly at $\lambda$ < 250um, and those in the log(M/ M_sun)=10.5-11 bin dominating at $\lambda$ > 350um. The contribution from galaxies in the log(M/ M_sun)=9.0-9.5 and log(M/ M_sun)=11.0-12.0 stellar mass bins contribute the least, both of order 5%, although the highest stellar-mass bin is a significant contributor to the luminosity density at z > 2. The luminosities of the galaxies responsible for the CIB shifts from a combination of "normal" and luminous infrared galaxies (LIRGs) at $\lambda$ < 160um, to LIRGs at 160um < $\lambda$ < 500um, to finally LIRGs and ultra-luminous infrared galaxies (ULIRGs) at $\lambda$ > 500um. Stacking analyses were performed with SIMSTACK (available at http://www.astro.caltech.edu/~viero/viero_homepage/toolbox.html) which accounts for possible biases due to clustering.

arXiv comment24 pages, 12 Figures, and 8 Tables. Accepted for publication in The Astrophysical Journal. Tabulated data and Software available at http://www.astro.caltech.edu/~viero/viero_homepage/toolbox.html

References in corpus (164)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Star Formation in Galaxies Along the Hubble Sequence
• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory
• The Herschel-SPIRE instrument and its in-flight performance
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• EAZY: A Fast, Public Photometric Redshift Code
• On the normalisation of the cosmic star formation history
• An analytic model for the spatial clustering of dark matter haloes
• Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
• Spectral Energy Distributions and Multiwavelength Selection of Type 1 Quasars
• Constraints on the relationship between stellar mass and halo mass at low and high redshift
• A Deep Sub-millimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution
• GOODS-Herschel: an infrared main sequence for star-forming galaxies
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
• Halo occupation numbers and galaxy bias
• A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4
• The Evolution of the Stellar Mass Functions of Star-Forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• The Infrared Spectral Energy Distribution of Normal Star-Forming Galaxies: Calibration at Far-Infrared and Submillimeter Wavelengths
• Mid-Infrared Selection of AGN with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-Selected AGN in COSMOS
• Infrared luminosity functions from the Chandra Deep Field South : the Spitzer view on the history of dusty star formation at 0<z<1
• The Herschel Multi-tiered Extragalactic Survey: HerMES
• The Cosmic Infrared Background: Measurements and Implications
• The Spectrum of the Extragalactic Far Infrared Background from the COBE Firas Observations
• Dusty star forming galaxies at high redshift
• SWIRE: The SIRTF Wide-area InfraRed Extragalactic Survey
• Ram Pressure Stripping of Spiral Galaxies in Clusters
• Obscured and unobscured active galactic nuclei in the Spitzer Space Telescope First Look Survey
• The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
• The SCUBA Local Universe Galaxy Survey I: First Measurements of the Submillimetre Luminosity and Dust Mass Functions
• The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
• PACS Evolutionary Probe (PEP) - A Herschel Key Program
• The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations
• The nature of faint submm-selected galaxies
• A Public Ks-selected Catalog in the COSMOS/UltraVISTA Field: Photometry, Photometric Redshifts and Stellar Population Parameters
• Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies
• The Mid-IR Properties of Starburst Galaxies from Spitzer-IRS Spectroscopy
• Far-infrared Spectral Energy Distribution Fitting for Galaxies Near and Far
• Mid-Infrared Spectral Diagnosis of Submillimeter Galaxies
• Ram pressure stripping the hot gaseous halos of galaxies in groups and clusters
• The LABOCA Survey of the Extended Chandra Deep Field South
• The Many Manifestations of Downsizing: Hierarchical Galaxy Formation Models confront Observations
• IRAC Mid-Infrared Imaging of the Hubble Deep Field South: Star Formation Histories and Stellar Masses of Red Galaxies at z>2
• What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
• The SCUBA Local Universe Galaxy Survey II. 450 micron data - evidence for cold dust in bright IRAS Galaxies
• Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges
• The 24 Micron Source Counts in Deep Spitzer Surveys
• The infrared luminosity function of galaxies at redshifts z=1 and z~2 in the GOODS fields
• The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs
• Low Resolution Spectral Templates For AGNs and Galaxies From 0.03 -- 30 microns
• Absolute Calibration and Characterization of the Multiband Imaging Photometer for Spitzer. I. The Stellar Calibrator Sample and the 24 micron Calibration
• Clustering of Submillimeter-Selected Galaxies
• HerMES: The SPIRE confusion limit
• Dusty Infrared Galaxies: Sources of the Cosmic Infrared Background
• A Herschel view of the far-infrared properties of submillimetre galaxies
• Mass downsizing and "top-down" assembly of early-type galaxies
• High resolution mid-infrared spectroscopy of ultraluminous infrared galaxies
• The first Herschel view of the mass-SFR link in high-z galaxies
• On the Lack of Evolution in Galaxy Star Formation Efficiency
• Herschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years
• HerMES: SPIRE galaxy number counts at 250, 350 and 500 microns
• A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies
• In-flight calibration of the Herschel-SPIRE instrument
• Planck Early Results XVIII: The power spectrum of cosmic infrared background anisotropies
• The Canada-UK Deep Submillimetre Survey: The Survey of the 14-hour field
• HerMES: deep number counts at 250, 350, and 500 microns in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
• The UKIRT Infrared Deep Sky Survey First Data Release
• Rapid Growth of Black Holes in Massive Star-Forming Galaxies
• Absolute Calibration and Characterization of the Multiband Imaging Photometer for Spitzer. II. 70 micron Imaging
• Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
• Submillimetre and far-infrared spectral energy distributions of galaxies: the luminosity-temperature relation and consequences for photometric redshifts
• Chandra and Spitzer unveil heavily obscured quasars in the SWIRE/Chandra Survey
• Herschel unveils a puzzling uniformity of distant dusty galaxies
• On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density
• Over half of the far-infrared background light comes from galaxies at z >= 1.2
• The Herschel Multi-Tiered Extragalactic Survey: Source Extraction and Cross-Identifications in Confusion-Dominated SPIRE Images
• Building the cosmic infrared background brick by brick with Herschel/PEP
• BLAST: Resolving the Cosmic Submillimeter Background
• Mid-Infrared Spectroscopy of Submillimeter Galaxies: Extended Star Formation in Massive High Redshift Galaxies
• GOODS-Herschel: Impact of Active Galactic Nuclei and Star Formation Activity on Infrared Spectral Energy Distributions at High Redshift
• A Redshift Survey of Herschel Far-Infrared Selected Starbursts and Implications for Obscured Star Formation
• The Emission by Dust and Stars of Nearby Galaxies in the Herschel KINGFISH Survey
• HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-Forming Galaxies
• Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel
• Spitzer IRAC confirmation of z_850-dropout galaxies in the Hubble Ultra Deep Field: stellar masses and ages at z~7
• Modeling the evolution of infrared galaxies: A Parametric backwards evolution model
• The AzTEC mm-Wavelength Camera
• HerMES: Far-infrared properties of known AGN in the HerMES fields
• Spitzer Deep and Wide Legacy Mid- and Far-Infrared Number Counts and Lower Limits of Cosmic Infrared Background
• Observations of a z=1.44 Dusty, Ultraluminous Galaxy and Implications for Deep Sub-mm Surveys
• The Herschel census of infrared SEDs through cosmic time
• Rapid dust production in submillimeter galaxies at z>4?
• A population of hot, dusty ultra-luminous galaxies at z~2
• Angular Power Spectra of the Millimeter Wavelength Background Light from Dusty Star-forming Galaxies with the South Pole Telescope
• The Balloon-borne Large Aperture Submillimeter Telescope: BLAST
• Tracing the Star Formation-Density Relation to z~2
• Mid-IR Luminosities and UV/Optical Star Formation Rates at z<1.4
• The data reduction pipeline for the Hi-GAL survey
• Reliable Identification of Compton-thick Quasars at z~2: Spitzer Mid-IR spectroscopy of HDF-oMD49
• Obscuration in extremely luminous quasars
• BLAST: Correlations in the Cosmic Far-Infrared Background at 250, 350, and 500 microns Reveal Clustering of Star-Forming Galaxies
• A large population of mid-infrared selected, obscured active galaxies in the Bootes field
• An Accounting of the Dust-Obscured Star Formation and Accretion Histories Over the Last ~11~Billion Years
• The Most Massive Galaxies at 3.0<z<4.0 in the NEWFIRM Medium-Band Survey: Properties and Improved Constraints on the Stellar Mass Function
• AzTEC Half Square Degree Survey of the SHADES Fields -- I. Maps, Catalogues, and Source Counts
• Absolute Calibration and Characterization of the Multiband Imaging Photometer for Spitzer. III. An Asteroid-based Calibration of MIPS at 160 microns
• How to distinguish starbursts and quiescently star-forming galaxies: The `bimodal' submillimetre galaxy population as a case study
• Hubble Space Telescope images of submillimeter sources: large, irregular galaxies at high redshift
• Sub-millimetre galaxies reside in dark matter halos with masses greater than 3x10^11 solar masses
• Widespread and Hidden Active Galactic Nuclei in Star-Forming Galaxies at Redshift > 0.3
• Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours
• The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts
• The bi-variate luminosity-color distribution of IRAS galaxies, and implications for the high redshift Universe
• Dust grain growth in the interstellar medium of 5<z<6.5 quasars
• Specific star-formation and the relation to stellar mass from 0<z<2 as seen in the far-infrared at 70 and 160mu
• An AzTEC 1.1 mm survey of the GOODS-N field -- II. Multi-wavelength identifications and redshift distribution
• The dust content of high-z submillimeter galaxies revealed by Herschel
• Correlated Anisotropies in the Cosmic Far-Infrared Background Detected by MIPS/Spitzer: Constraint on the Bias
• A backward evolution model for infrared surveys: the role of AGN- and Color-L_TIR distributions
• Improved Models for Cosmic Infrared Background Anisotropies: New Constraints on the IR Galaxy Population
• HerMES: Unveiling obscured star formation - the far infrared luminosity function of ultraviolet-selected galaxies at z~1.5
• Connecting stellar mass and star-formation rate to dark matter halo mass out to z ~ 2
• A CMB lensing mass map and its correlation with the cosmic infrared background
• A New Population of High Redshift, Dusty Lyman-Alpha Emitters and Blobs Discovered by WISE
• The Hubble Space Telescope GOODS NICMOS Survey: Overview and the Evolution of Massive Galaxies at 1.5 < z < 3
• Power spectrum of the cosmic infrared background at 60 and 100 microns with IRAS
• Herschel-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths
• Evolution of the Far-Infrared-Radio Correlation and Infrared SEDs of Massive Galaxies over z = 0 - 2
• The Modelling of Intermediate Age Stellar Populations. II. Average spectra for upper AGB stars, and their use
• Far-infrared properties of submillimeter and optically faint radio galaxies
• Confirming a Population of Hot-Dust Dominated, Star Forming Ultraluminous Galaxies at High-Redshift
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Exploring the evolutionary paths of the most massive galaxies since z~2
• BLAST: A Far-Infrared Measurement of the History of Star Formation
• Herschel reveals a T_dust-unbiased selection of z~2 ULIRGs
• Shells of dust around AGB stars: effects on the integrated spectrum of Single Stellar Populations
• Far-Infrared Properties of Spitzer-selected Luminous Starbursts
• GOODS-Herschel: Separating High Redshift active galactic Nuclei and star forming galaxies Using Infrared Color Diagnostics
• HerMES: SPIRE Science Demonstration Phase Maps
• Quantifying Photometric Redshift Errors in the Absence of Spectroscopic Redshifts
• The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 4 sq. deg Galactic Plane Survey in Vulpecula (l=59)
• Radio and mid-infrared identification of BLAST source counterparts in the Chandra Deep Field South
• The roles of star formation and AGN activity of IRS sources in the HerMES fields
• The Cosmic Far-Infrared Background Buildup Since Redshift 2 at 70 and 160 microns in the COSMOS and GOODS fields
• A Simultaneous Stacking and Deblending Algorithm for Astronomical Images
• Where stars form and live at high redshift: clues from the infrared
• Power-Law Template for IR Point Source Clustering
• Origins of the extragalactic background at 1mm from a combined analysis of the AzTEC and MAMBO data in GOODS-N
• A Population of Dust-Rich Quasars at z ~ 1.5
• Herschel ATLAS: The cosmic star formation history of quasar host galaxies
• Temperature Profiles and the Effect of AGN on Submillimeter Emission from BLAST Observations of Resolved Galaxies
• Interferometric CO Observations of submillimeter-faint, radio-selected starburst galaxies at z~2
• Sub-millimeter detections of Spitzer Space Telescope galaxy populations
• A Conditional Luminosity Function Model of the Cosmic Far-Infrared Background Anisotropy Power Spectrum
• Measuring star formation in high-z massive galaxies: A mid-infrared to submillimeter study of the GOODS NICMOS Survey sample
• A Far-IR Characterization of 24 micron Selected Galaxies at 0<z<2.5 using Stacking at 70 microns and 160 microns in the COSMOS Field
• Discovery of "Warm Dust" Galaxies in Clusters at z~0.3: Evidence for Stripping of Cool Dust in the Dense Environment?
• Herschel observations of a z~2 stellar mass selected galaxy sample drawn from the GOODS NICMOS Survey
• A panchromatic study of BLAST counterparts: total star-formation rate, morphology, AGN fraction and stellar mass

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