The clustering of merging star-forming haloes: dust emission as high frequency arcminute CMB foreground

Details The clustering of merging star-forming haloes: dust emission as high frequency arcminute CMB foreground The clustering of merging star-forming haloes: dust emission as high frequency arcminute CMB foreground

2007-07-02

arxiv.org/abs/0707.0288v2

Nuovo Cim.B122:1463-1466,2007

Astronomy and Astrophysics

Astrophysics

18 pages, 16 figures. Accepted by Astronomy & Astrophysics

Scientific paper

10.1393/ncb/i2008-10490-1

Future observations of CMB anisotropies will be able to probe high multipole regions of the angular power spectrum, corresponding to a resolution of a few arcminutes. Dust emission from merging haloes is one of the foregrounds that will affect such very small scales. We estimate the contribution to CMB angular fluctuations from objects that are bright in the sub-millimeter band due to intense star formation bursts following merging episodes. We base our approach on the Lacey-Cole merger model and on the Kennicutt relation which connects the star formation rate in galaxies with their infrared luminosity. We set the free parameters of the model in order to not exceed the SCUBA source counts, the Madau plot of star formation rate in the universe and COBE/FIRAS data on the intensity of the sub-millimeter cosmic background radiation. We show that the angular power spectrum arising from the distribution of such star-forming haloes will be one of the most significant foregrounds in the high frequency channels of future CMB experiments, such as PLANCK, ACT and SPT. The correlation term, due to the clustering of multiple haloes at redshift z~2-6, is dominant in the broad range of angular scales 200

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