Microwave and radio emission of dusty star-forming galaxies: Implication for the cosmic radio background

Abstract

We use the most up-to-date cosmological evolution models of star-forming (SF) galaxies and radio sources to compute the extragalactic number counts and the cosmic background from 408MHz to 12THz. The model of SF galaxies reproduces the constraints obtained by Spitzer, Herschel, and ground-based submm/mm experiments: number counts, redshift distribution of galaxies, cosmic background intensity and anisotropies. The template SEDs of this model are extrapolated to the radio adding synchrotron, free-free, and spinning dust emissions. To fix the synchrotron intensity, we use the IR/radio flux ratio, q70, and a spectral index beta=-3. For a constant q70, our model added to the AGN contribution provides a good fit to the number counts from 12THz to 408MHz and to the CIB. Spinning dust accounts for up to 20% of the cosmic microwave background produced by SF galaxies, but for less than 10% of the total background when AGN are included. The SF galaxies account for 77.5% of the number counts at 1.4GHz for a flux of 1e-4Jy. However, the model does not explain the CRB measured with the ARCADE2 experiment. Considering the case when q70 decreases strongly with redshift, this still does not explain the ARCADE2 results. It also yields to an overestimate of the low-flux number counts in the radio. Thus, we rule out a steep variation of q70 with redshift at least for z<3.5. Adding a population of faint SF galaxies at high redshift (Lir<1e11Lsun and 4<z<6), which would reproduce the ARCADE2 results, leads to predictions of the CIB much higher than what is observed, ruling out this as the explanation for the ARCADE2 results. Considering our findings and previous studies, we conclude that if the radio emission measured by ARCADE2 is astrophysical in origin, it has to originate in the Galaxy or in a new kind of radio sources (with no mid- to far-IR counterparts) or emission mechanism still to be discovered.

accepted for publication by A&A, modification of one citation

References in corpus (14)

• 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
• Separation of anomalous and synchrotron emissions using WMAP polarization data
• Spitzer Deep and Wide Legacy Mid- and Far-Infrared Number Counts and Lower Limits of Cosmic Infrared Background
• Exploring the infrared/radio correlation at high redshift
• High-resolution radio continuum survey of M33 II. Thermal and nonthermal emission
• The Atacama Cosmology Telescope: Extragalactic Sources at 148 GHz in the 2008 Survey
• A multi-resolution analysis of the radio-FIR correlation in the Large Magellanic Cloud
• Centimeter-wave continuum radiation from the rho Ophiuchi molecular cloud
• The contribution of the Unresolved Extragalactic Radio Sources to the Brightness Temperature of the sky
• TRIS II: search for CMB spectral distortions at 0.60, 0.82 and 2.5 GHz
• An evolution of the IR-Radio correlation at very low flux densities?
• Modelling the spinning dust emission from dense interstellar clouds
• TRIS III: the diffuse galactic radio emission at $\delta =+42^{\circ }$
• Are Active Galactic Nuclei the Solution to the Excess Cosmic Radio Background at 1.4 GHz?

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