Extrapolation of Galactic Dust Emission at 100 Microns to CMBR Frequencies Using FIRAS

Abstract

We present predicted full-sky maps of submillimeter and microwave emission from the diffuse interstellar dust in the Galaxy. These maps are extrapolated from the 100 micron emission and 100/240 micron flux ratio maps that Schlegel, Finkbeiner, & Davis (1998; SFD98) generated from IRAS and COBE/DIRBE data. Results are presented for a number of physically plausible emissivity models. We find that no power law emissivity function fits the FIRAS data from 200 - 2100 GHz. In this paper we provide a formalism for a multi-component model for the dust emission. A two-component model with a mixture of silicate and carbon-dominated grains (motivated by Pollack et al., 1994}) provides a fit to an accuracy of about 15% to all the FIRAS data over the entire high-latitude sky. Small systematic differences are found between the atomic and molecular phases of the ISM. Our predictions for the thermal (vibrational) emission from Galactic dust at ν< 3000 GHz are available for general use. These full-sky predictions can be made at the DIRBE resolution of 40' or at the higher resolution of 6.1 arcmin from the SFD98 DIRBE-corrected IRAS maps.

48 pages, AAS LaTeX, 6 figures, ApJ (accepted). Data described in the text, as well as 4 additional figures, are available at http://astro.berkeley.edu/dust

References in corpus (1)

• Extrapolation of Galactic Dust Emission at 100 Microns to CMBR Frequencies Using FIRAS

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• The Distortion of the Cosmic Microwave Background Spectrum Due to Intergalactic Dust
• Using peak distribution of the cosmic microwave background for MAP and Planck data analysis: formalism and simulations
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• Cross-Correlation analysis of WMAP and EGRET in Wavelet Space
• Cross-correlation analysis of CMB with foregrounds for residuals
• Biparametric Adaptive Filter: detection of compact sources in complex microwave backgrounds
• CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
• Error estimation for the MAP experiment
• AKARI far-infrared maps of the zodiacal dust bands
• A Spatially Resolved Radio Spectral Index Study of the Dwarf Irregular Galaxy NGC\,1569
• Model of the polarized foreground diffuse Galactic emissions from 33 to 353 GHz
• Bayesian foreground analysis with CMB data
• First Results from the Arcminute Cosmology Bolometer Array Receiver
• The Dust Temperature of the "Dusty" Radio Galaxy MG 1019+0535: Evidence for an Outflow
• Towards understanding the Planck thermal dust models
• Separation of CMB $\mu$ spectral distortions from foregrounds with poorly defined spectral shapes
• Cosmic ray backgrounds for dark matter indirect detection
• Spinning Dust Emission from Wobbling Grains: Important Physical Effects and Implications
• Polarization power spectra and dust cloud morphology
• Radio Variability and Broad-Band Spectra of Infrared Galaxies with and without OH Megamaser Emission
• Evaluation of the single-component thermal dust emission model in CMB experiments
• The long wavelength view of GG Tau A: Rocks in the Ring World
• The Detector System for the Stratospheric Kinetic Inductance Polarimeter (SKIP)
• Half-wave Plates for the Spider Cosmic Microwave Background Polarimeter
• Evidence for anomalous dust-correlated emission at 8 GHz
• Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz
• HP2 Survey V. Ophiuchus: Filament formation in a dispersing cloud complex
• Constraints on the SZ Power Spectrum on Degree Angular Scales in WMAP Data
• Mitigating Bias in CMB B-modes from Foreground Cleaning Using a Moment Expansion
• The Superhorizon Test of Future B-mode Experiments
• Observing the Epoch of Reionization with the Cosmic Microwave Background
• The effect of cosmic variance on the characteristics of dust polarization power spectra
• CO Component Estimation Based on the Independent Component Analysis
• Identifying frequency decorrelated dust residuals in B-mode maps by exploiting the spectral capability of bolometric interferometry
• On the wavelet analysis of CMB time ordered data: application to Archeops
• Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
• The contribution of CHONS particles to the diffuse high Galactic latitude IR emission
• Model Independent Foreground Power Spectrum Estimation using WMAP 5-year Data
• Experiences with Airborne and Ground-Based Polarimetry
• Thermal and non-thermal Sunyaev-Zel'dovich effect in the cavities of the galaxy cluster MS 0735.6+7421: the role of the thermal density in the cavity
• Simulation of Cosmic Microwave Background Polarization Fields for AMiBA Experiment
• Assessment of Models of Galactic Thermal Dust Emission Using COBE/FIRAS and COBE/DIRBE Observations
• Sparse estimation of model-based diffuse thermal dust emission
• Design and Performance of 30/40 GHz Diplexed Focal Plane for BICEP Array
• Interstellar radiation as a Maxwell field: improved numerical scheme and application to the spectral energy density
• Resolving high-z Galaxy Cluster properties through joint X-ray and Millimeter analysis: a case study of SPT-CLJ0615-5746
• Spectral energy density in an axisymmetric galaxy as predicted by an analytical model for the Maxwell field
• Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements
• Cosmic rays, gas and dust in the Central Molecular Zone I -- $X_{CO}$ factors, cosmic-ray densities and dust opacities
• Spectrum of the Anomalous Microwave Emission in the North Celestial Pole with WMAP 7-Year data
• Testing the CMB Data for Systematic Effects
• A characterization of the diffuse Galactic emissions in the anti-center of the Galaxy
• Fermi-bubble bulk and edge analysis reveals dust, cooling breaks, and cosmic-ray diffusion, facilitating a self-consistent model
• Perturbed nonlinear models from Noncommutativity
• Molecular phonons and their absorption/emission spectra from the far IR to microwaves
• A Foreground Model Independent Bayesian CMB Temperature and Polarization Signal Reconstruction and Cosmological Parameter Estimation over Large Angular Scales
• Comparison of 13CO Line and Far-Infrared Continuum Emission as a Diagnostic of Dust and Molecular Gas Physical Conditions: III. Systematic Effects and Scientific Implications
• "Ashfall" Induced by Molecular Outflow in Protostar Evolution. II. Analytical Study on the Maximum Size of Dust Grains Lifted by Outflows
• Correlation Analysis between Tibet AS-$\gamma$ TeV Cosmic Ray and WMAP Nine-year Data
• Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach
• Do We Have Sufficient Knowledge of the Galactic Foreground Emission in Cosmic Microwave Background Science?
• Detection of polarized Fermi-bubble synchrotron and dust emission
• Intrinsic advantages of the w component and spherical imaging for wide-field radio interferometry
• Why don't clumps of cirrus dust gravitationally collapse?
• Multi-frequency point source detection with fully convolutional networks: Performance in realistic microwave sky simulations