z-logo
open-access-imgOpen Access
An Imaging and Spectroscopic Survey of Galaxies within Prominent Nearby Voids. I. The Sample and Luminosity Distribution
Author(s) -
Norman A. Grogin,
Margaret J. Geller
Publication year - 1999
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/301126
Subject(s) - astrophysics , physics , galaxy , luminosity function , redshift , astronomy , void (composites) , photometry (optics) , redshift survey , luminous infrared galaxy , galaxy group , sky , luminosity , stars , materials science , composite material
We study the optical properties of a large sample of galaxies in low-densityregions of the nearby universe. We make a 5/h Mpc-smoothed map of the galaxydensity throughout the Center for Astrophysics Redshift Survey (CfA2) toidentify galaxies within three prominent nearby ``voids'' with diameter >30/hMpc. We augment the CfA2 void galaxy sample with fainter galaxies found in thesame regions from the deeper Century and 15R Redshift Surveys. We obtain B andR CCD images and high-S/N longslit spectra for the resulting sample of 149 voidgalaxies, and also for 131 galaxies on the periphery of these voids. Here we describe the photometry for the sample, including B isophotalmagnitudes and B-R colors. For the 149 galaxies which lie in regions below themean survey density, the luminosity functions in B and R are well-fit bySchechter functions with respective parameters (alpha_B = -0.5 +/- 0.3, B_* =-18.9 +/- 0.2) and (alpha_R = -0.9 +/- 0.3, R_* = -20.4 +/- 0.3). The Bluminosity function (LF) is consistent with typical survey LFs (e.g., theSouthern Sky Redshift Survey), and the R LF is consistent with the CenturySurvey. The B and R LFs of 131 galaxies in the ``void periphery'', regionsbetween the mean density and twice the mean, have similar Schechter parameters.The CfA2 LF is inconsistent with both samples at 3.5-sigma. When we narrow our analysis to the 46 galaxies in regions below half the meandensity, the LF is steeper: alpha = -1.4 +/- 0.5. The typical survey LFs areinconsistent with this subsample at 2-sigma. The B-R color distribution ofgalaxies in the lowest-density regions is also shifted significantly (3-sigma)blue-ward of the higher density samples. The most luminous red galaxies (R <-21) are absent from the lowest density regions at 2.5-sigma.Comment: 33 pages, 16 figures; AJ in press (Dec. 1999); Version with full-resolution figures available from ftp://ftp.stsci.edu/outside-access/out.going/nagrogin/Grogin1.tar.g

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom