Searching for Large Scale Structure in Deep Radio Surveys

Details Searching for Large Scale Structure in Deep Radio Surveys Searching for Large Scale Structure in Deep Radio Surveys

1997-09-22

arxiv.org/abs/astro-ph/9709205v1

Mon.Not.Roy.Astron.Soc.297:545-558,1998

Astronomy and Astrophysics

Astrophysics

15 pages, 5 ps figures, Latex, Submitted to MNRAS

Scientific paper

10.1046/j.1365-8711.1998.01536.x

(Abridged Abstract) We calculate the expected amplitude of the dipole and higher spherical harmonics in the angular distribution of radio galaxies. The median redshift of radio sources in existing catalogues is z=1, which allows us to study large scale structure on scales between those accessible to present optical and infrared surveys, and that of the Cosmic Microwave Background (CMB). The dipole is due to 2 effects which turn out to be of comparable magnitude: (i) our motion with respect to the CMB, and (ii) large scale structure, parameterised here by a family of Cold Dark Matter power-spectra. We make specific predictions for the Green Bank (87GB) and Parkes-MIT-NRAO (PMN) catalogues. For these relatively sparse catalogues both the motion and large scale structure dipole effects are expected to be smaller than the Poisson shot-noise. However, we detect dipole and higher harmonics in the combined 87GB-PMN catalogue which are far larger than expected. We attribute this to a 2 % flux mismatch between the two catalogues. We also investigate the existence and extent of the Supergalactic Plane in the above catalogues. In a strip of +- 10 deg of the standard Supergalactic equator, we find a 3-sigma detection in PMN, but only 1-sigma in 87GB.

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