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The Mass Function of Void Galaxies in the SDSS Data Release 2
Preprint   Open access

The Mass Function of Void Galaxies in the SDSS Data Release 2

David M Goldberg, Timothy D Jones, Fiona Hoyle, Randall R Rojas, Michael S Vogeley and Michael R Blanton
ArXiv.org
23 Jun 2004
url
https://doi.org/10.48550/arxiv.astro-ph/0406527View
Preprint (Author's original)arXiv.org - Non-exclusive license to distribute Open

Abstract

Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics
Astrophys.J. 621 (2005) 643-650 We estimate the Mass Function of void galaxies in the second public data release of the Sloan Digital Sky Survey from a sample of 1000 galaxies with local density contrasts of delta_v < -0.6. The galaxy sample is split into ellipticals and spirals using a color-Sersic index criteria. We estimate the virial masses of ellipticals using the measured spectral line-widths along with the observed size. Projection effects and uncertainties in halo properties make mass estimates of spirals more difficult. We use an inversion of the Tully-Fisher relation to estimate the isothermal rotational velocity, and introduce a scaling factor to estimate the halo extent. We then fit the measured mass function against a theoretical Press-Schechter model, and find that the distribution of galaxies in voids appears to be nearly unbiased compared to the mass.

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