Measurements of the Cross Spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz

Abstract

We present measurements of the power spectra of cosmic infrared background (CIB) and cosmic microwave background (CMB) fluctuations in six frequency bands. Maps at the lower three frequency bands, 95, 150, and 220 GHz (3330, 2000, 1360 $\mu$m) are from the South Pole Telescope, while the upper three frequency bands, 600, 857, and 1200 GHz (500, 350, 250 $\mu$m) are observed with Herschel/SPIRE. From these data, we produce 21 angular power spectra (six auto- and fifteen cross-frequency) spanning the multipole range $600\le \ell \le 11,000$. Our measurements are the first to cross-correlate measurements near the peak of the CIB spectrum with maps at 95 GHz, complementing and extending the measurements from Planck Collaboration et al. (2014) at 218, 550, and 857 GHz. The observed fluctuations originate largely from clustered, infrared-emitting, dusty star-forming galaxies, the CMB, and to a lesser extent radio galaxies, active galactic nuclei, and the Sunyaev-Zel'dovich effect.

arXiv comment21 pages, 3 figures; Accepted by ApJS (updated to accepted version)

References in corpus (75)

• Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy
• Interstellar Dust Grains
• The Herschel-SPIRE instrument and its in-flight performance
• Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
• A Deep Sub-millimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• The Evolution of the Stellar Mass Functions of Star-Forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey
• Dusty Star-Forming Galaxies at High Redshift
• The Cosmic Infrared Background: Measurements and Implications
• MASTER of the CMB Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex CMB Data Sets
• Dusty star forming galaxies at high redshift
• The 10 Meter South Pole Telescope
• The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
• IRIS: A new generation of IRAS maps
• The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra
• GASS: The Parkes Galactic All-Sky Survey. I. Survey Description, Goals, and Initial Data Release
• A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey
• Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
• Modelling the infrared galaxy evolution using a phenomenological approach
• Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
• HerMES: The SPIRE confusion limit
• Dusty Infrared Galaxies: Sources of the Cosmic Infrared Background
• A measurement of secondary cosmic microwave background anisotropies with two years of South Pole Telescope observations
• Galaxy growth in a massive halo in the first billion years of cosmic history
• A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies
• Planck Early Results XVIII: The power spectrum of cosmic infrared background anisotropies
• A measurement of secondary cosmic microwave background anisotropies from the 2500-square-degree SPT-SZ survey
• The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters
• On the Cluster Physics of Sunyaev-Zel'dovich Surveys II: Deconstructing the Thermal SZ Power Spectrum
• Impact of Cluster Physics on the Sunyaev-Zel'dovich Power Spectrum
• Simulations of the Sunyaev-Zel'dovich Power Spectrum with AGN Feedback
• GASS: The Parkes Galactic All-Sky Survey. II. Stray-Radiation Correction and Second Data Release
• Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
• BLAST: Resolving the Cosmic Submillimeter Background
• HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-Forming Galaxies
• Cosmic microwave background constraints on the duration and timing of reionization from the South Pole Telescope
• Xspect, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars
• Angular Power Spectra of the Millimeter Wavelength Background Light from Dusty Star-forming Galaxies with the South Pole Telescope
• The Herschel Stripe 82 Survey (HerS): Maps and Early Catalog
• HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift
• Flux calibration of the Herschel-SPIRE photometer
• BLAST: Correlations in the Cosmic Far-Infrared Background at 250, 350, and 500 microns Reveal Clustering of Star-Forming Galaxies
• The Atacama Cosmology Telescope: A Measurement of the 600< ell <8000 Cosmic Microwave Background Power Spectrum at 148 GHz
• Sub-millimetre galaxies reside in dark matter halos with masses greater than 3x10^11 solar masses
• Templates for the Sunyaev-Zel'dovich Angular Power Spectrum
• The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared
• The first release of data from the Herschel ATLAS: the SPIRE images
• Probing Early Structure Formation with Far-Infrared Background Correlations
• The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study
• Correlated Anisotropies in the Cosmic Far-Infrared Background Detected by MIPS/Spitzer: Constraint on the Bias
• Improved Models for Cosmic Infrared Background Anisotropies: New Constraints on the IR Galaxy Population
• Statistical properties of dust far-infrared emission
• A CMB lensing mass map and its correlation with the cosmic infrared background
• Flux Calibration of Broadband Far Infrared and Submillimetre Photometric Instruments: Theory and Application to Herschel-SPIRE
• Sunyaev-Zeldovich effect from hydrodynamical simulations: maps and low order statistics
• Unbiased Estimation of an Angular Power Spectrum
• Accurate Galactic 21-cm H I measurements with the NRAO Green Bank Telescope
• Modelling the correlation between the thermal Sunyaev Zel'dovich effect and the cosmic infrared background
• HerMES: SPIRE Science Demonstration Phase Maps
• H-ATLAS: The cosmic abundance of dust from the far-infrared background power spectrum
• Observational limits to source confusion in the millimetre/submillimetre waveband
• Measurement of CIB power spectra over large sky areas from Planck HFI maps
• Correlations in the Far Infrared Background
• Asymmetric Beams in Cosmic Microwave Background Anisotropy Experiments
• An accurate measurement of the anisotropies and mean level of the Cosmic Infrared Background at 100 and 160 um
• Herschel-ATLAS: Statistical Properties of Galactic Cirrus in the GAMA-9 Hour Science Demonstration Phase Field
• Direct Estimate of Cirrus Noise in Herschel Hi-GAL Images
• A Simple Empirically Motivated Template for the Unresolved Thermal Sunyaev-Zeldovich Effect
• Correlations in the (Sub)millimeter background from ACTxBLAST
• Measuring star formation in high-z massive galaxies: A mid-infrared to submillimeter study of the GOODS NICMOS Survey sample
• BLAST05: Power Spectra of Bright Galactic Cirrus at Submillimeter Wavelengths
• Power Spectrum Analysis of Far-IR Background Fluctuations in 160 Micron Maps From the Multiband Imaging Photometer for Spitzer
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• Observational Limits on Patchy Reionization: Implications for B-modes
• Operations and Performance of the PACS Instrument 3He Sorption Cooler on board of the Herschel Space Observatory

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• The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect
• CMB/kSZ and Compton-$y$ Maps from 2500 square degrees of SPT-SZ and Planck Survey Data
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• Constraining Cluster Virialization Mechanism and Cosmology using Thermal-SZ-selected clusters from Future CMB Surveys
• First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations
• Constraining the Star Formation Rate using Joint CIB Continuum and [CII] Intensity Mapping
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Forecasting ground-based sensitivity to the Rayleigh scattering of the CMB in the presence of astrophysical foregrounds
• Challenges of standard halo models in constraining galaxy properties from CIB anisotropies