Reducing Photometric Redshift Uncertainties Using Galaxy Clustering Information
In cosmology and astronomy, measuring the distances to galaxies is an important task. This is done by measuring the redshift of the spectra from these sources. Photometric redshifts are a quick way of estimating the true redshifts and are calculated using color band intensities. The errors on thes...
Main Author: | Fiedorowicz, Pier Alexander |
---|---|
Other Authors: | Rozo, Eduardo |
Language: | en_US |
Published: |
The University of Arizona.
2017
|
Online Access: | http://hdl.handle.net/10150/624981 http://arizona.openrepository.com/arizona/handle/10150/624981 |
Similar Items
-
Galaxy clustering with spectroscopic and photometric redshift surveys
by: Collister, Adrian Ashley
Published: (2006) -
Photometric redshifts and physical properties of low redshift galaxies
by: Eminian, Celine
Published: (2008) -
Measuring galaxy environment with spectroscopic and photometric redshifts
by: Chuan-Chin Lai, et al.
Published: (2013) -
Probing distant clusters : a pre-SALT photometric study of intermediate redshift galaxy cluster
by: Cluver, Michelle E
Published: (2014) -
An Analysis of Two Photometric Redshift Methods and Their Uses for Finding Void Galaxies
by: Steele, Rochelle J.
Published: (2021)