Photometric Properties of Void Galaxies in the Sloan Digital Sky Survey
نویسندگان
چکیده
Using a nearest neighbor analysis, we construct a sample of void galaxies from the Sloan Digital Sky Survey (SDSS) and compare the photometric properties of these galaxies to the population of non-void (wall) galaxies. We trace the density field of galaxies using a volume-limited sample with zmax = 0.089. Galaxies from the flux-limited SDSS with z ≤ zmax and fewer than three volume-limited neighbors within 7hMpc are classified as void galaxies. This criterion implies a density contrast δρ/ρ < −0.6 around void galaxies. From 155,000 galaxies, we obtain a sub-sample of 13,742 galaxies with z ≤ zmax, from which we identify 1,010 galaxies as void galaxies. To identify an additional 194 faint void galaxies from the SDSS in the nearby universe, r ∼< 72h Mpc, we employ volume-limited samples extracted from the Updated Zwicky Catalog and the Southern Sky Redshift Survey with zmax = 0.025 to trace the galaxy distribution. Our void galaxies span a range of absolute magnitude from Mr = −13.5 to Mr = −22.5. Using SDSS photometry, we compare the colors, concentration indices, and Sersic indices of the void and wall samples. Void galaxies are significantly bluer than galaxies lying at higher density. The population of void galaxies with Mr ∼< M ∗ + 1 and brighter is on average bluer and more concentrated (later type) than galaxies outside of voids. The latter behavior is only partly explained by the paucity of luminous red galaxies in voids. These results generally agree with the predictions of semi-analytic models for galaxy formation in cold dark matter models, which indicate that void galaxies should be relatively bluer, more disklike, and have higher specific star formation rates. Subject headings: cosmology: observations — large-scale structure of universe — methods: statistical — galaxies: photometry — galaxies: structure Department of Physics, Drexel University, 3141 Chestnut Street, Philadelphia, PA 19104 Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349-0059
منابع مشابه
Spectroscopic Properties of Void Galaxies in the Sloan Digital Sky Survey
We study the spectroscopic properties of a sample of 10 void galaxies identified in the Sloan Digital Sky Survey (SDSS) and compare these with the properties of galaxies in higher density regions (wall galaxies). This sample of void galaxies covers the range of absolute magnitude from Mr 1⁄4 13:5 to Mr 1⁄4 22:5 in regions with density contrast / < 0:6. We compare the equivalent widths of H , [O...
متن کاملA Galaxy Photometric Redshift Catalog for the Sloan Digital Sky Survey Data
We present and describe a catalog of galaxy photometric redshifts (photo-z’s) for the Sloan Digital Sky Survey (SDSS) Data Release 6 (DR6). We use the Artificial Neural Network (ANN) technique to calculate photo-z’s and the Nearest Neighbor Error (NNE) method to estimate photo-z errors for ∼ 77 million objects classified as galaxies in DR6 with r < 22. The photo-z and photo-z error estimators a...
متن کاملA Galaxy Photometric Redshift Catalog for the Sloan Digital Sky Survey Data Release 6
We present and describe a catalog of galaxy photometric redshifts (photo-z’s) for the Sloan Digital Sky Survey (SDSS) Data Release 6 (DR6). We use the Artificial Neural Network (ANN) technique to calculate photo-z’s and the Nearest Neighbor Error (NNE) method to estimate photo-z errors for ∼ 77 million objects classified as galaxies in DR6 with r < 22. The photo-z and photo-z error estimators a...
متن کاملar X iv : a st ro - p h / 98 05 31 4 v 1 2 5 M ay 1 99 8 The Sloan Digital Sky Survey
The Sloan Digital Sky Survey is an ambitious, multi-institutional project to create a huge digital imaging and spectroscopic data bank of 25% of the celestial sphere, approximately 10,000 deg2 centred on the north galactic polar cap. The photometric atlas will be in 5 specially-chosen colours, covering the π ster of the Survey area to a limiting magnitude of r∼23.1, on 0 . 4 pixels, resulting i...
متن کاملar X iv : a st ro - p h / 98 05 31 4 v 2 1 9 A ug 1 99 8 The Sloan Digital Sky Survey
The Sloan Digital Sky Survey is an ambitious, multi-institutional project to create a huge digital imaging and spectroscopic data bank of 25% of the celestial sphere, approximately 10,000 deg2 centred on the north galactic polar cap. The photometric atlas will be in 5 specially-chosen colours, covering the π ster of the Survey area to a limiting magnitude of r∼23.1, on 0 . 4 pixels, resulting i...
متن کامل