Reconstructed Density and Velocity Fields from the 2MASS Redshift Survey

Details Reconstructed Density and Velocity Fields from the 2MASS Redshift Survey Reconstructed Density and Velocity Fields from the 2MASS Redshift Survey

2006-09-29

arxiv.org/abs/astro-ph/0610005v1

Mon.Not.Roy.Astron.Soc.373:45-64,2006

Astronomy and Astrophysics

Astrophysics

21 pages. 22 figures, accepted for publication in MNRAS. The figures are coarsely resolved, a version of this paper with high

Scientific paper

10.1111/j.1365-2966.2006.11049.x

We present the reconstructed real-space density and the predicted velocity fields from the Two Mass Redshift Survey (2MRS). The 2MRS is the densest all-sky redshift survey to date and includes about 23,200 galaxies with extinction corrected magnitudes brighter than K = 11.25. Our method is based on the expansion of these fields in Fourier-Bessel functions. Within this framework, the linear redshift distortions only affect the density field in the radial direction and can easily be deconvolved using a distortion matrix. Moreover, in this coordinate system, the velocity field is related to the density field by a simple linear transformation. The shot noise errors in the reconstructions are suppressed by means of a Wiener filter which yields a minimum variance estimate of the density and velocity fields. Using the reconstructed real-space density fields, we identify all major superclusters and voids. At 50 Mpc/h, our reconstructed velocity field indicates a back-side infall to the Great Attractor region of vi = (491 +/- 200)(beta/0.5) km/sec in the Local Group frame and v = (64 +/- 205)(beta/0.5) km/sec in the cosmic microwave background (CMB) frame and beta is the redshift distortion parameter. The direction of the reconstructed dipole agrees well with the dipole derived by Erdogdu et al. (2006). The misalignment between the reconstructed 2MRS and the CMB dipoles drops to 13 degrees at around 5000 km/sec but then increases at larger distances. A version of this paper with high resolution figures can be obtained from http://www.nottingham.ac.uk/~ppzzpe

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