Redshift survey in 15 quasar fields (Morris+, 2006)

Details Redshift survey in 15 quasar fields (Morris+, 2006) Redshift survey in 15 quasar fields (Morris+, 2006)

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..73671261m&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/367/1261. Originally published in: 2006MNRAS.367.1261M

Physics

Qsos, Galaxies: Photometry, Redshifts

Scientific paper

We investigate the relative distribution of the gaseous contents of the Universe (as traced by a sample of Ly{alpha} absorbers), and the luminous baryonic matter (as traced by a redshift survey of galaxies in the same volume searched for Ly{alpha} absorbers), along 16 lines of sight (LOS) between redshifts 0 and 1. Our galaxy redshift survey was made with the multi-object spectrograph on the Canada-France-Hawaii Telescope and, when combined with galaxies from the literature in the same LOS, gives us a galaxy sample of 636 objects. By combining this with an absorption-line sample of 406 absorbing systems drawn from published works, we are able to study the relationship between gas and galaxies over the latter half of the age of the Universe.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

Redshift survey in 15 quasar fields (Morris+, 2006) 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 Redshift survey in 15 quasar fields (Morris+, 2006), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Redshift survey in 15 quasar fields (Morris+, 2006) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1100439