The angular two-point correlation function of galaxies down to BJ less than or approximately = 26 magnitudes on less than or approximately = 10 arcmins scales

Details The angular two-point correlation function of galaxies down to BJ less than or approximately = 26 magnitudes on less than or approximately = 10 arcmins scales The angular two-point correlation function of galaxies down to BJ less than or approximately = 26 magnitudes on less than or approximately = 10 arcmins scales

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...439...14n&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 439, no. 1, p. 14-28

Computer Science

Numerical Analysis

28

Angular Correlation, Cosmology, Faint Objects, Galactic Clusters, Galactic Evolution, Red Shift, Stellar Magnitude, Brightness Distribution, Numerical Analysis

Scientific paper

We place constaints on the evolution of galaxy clustering from deep CCD frames in Gunn gri from two widely separated, intermediate Galactic latitude fields (b greater than or approximately = 30 deg), each roughly square in shape and approximately = 0.5 deg in extent. More than 90% of the galaxies brighter than gri approximately 24.5 mag are detected. For each field in each passband, a total of greater than or approximately = 23,000 objects are found. Neuschaefer, Windhorst, & Dressler (1991) (the first paper in the series) and Neuschaefer & Windhorst (1994) (the second paper in the series) discuss the details of the photometric and astrometric calibrations, object classification and galaxy counts. The current paper, the third in the series, presents the faint galaxy angular two-point correlation function (as a function of median redshift and apparent magnitude) and assesses the relative importance of effects due to sample completeness, galaxy surface brightness, evolution in galaxy spectra, evolution in clustering, as well as the overall matter density in the universe. Galaxies undergo a moderate bluing trend with increasing sample depth, consistent with previous work.

Affiliated with

Also associated with

No associations

Rating

The angular two-point correlation function of galaxies down to BJ less than or approximately = 26 magnitudes on less than or approximately = 10 arcmins scales does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The angular two-point correlation function of galaxies down to BJ less than or approximately = 26 magnitudes on less than or approximately = 10 arcmins scales, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The angular two-point correlation function of galaxies down to BJ less than or approximately = 26 magnitudes on less than or approximately = 10 arcmins scales will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1819285