<--- Back to Details
First PageDocument Content
Astronomy / Physical cosmology / Observational astronomy / Astronomical surveys / UKIRT Infrared Deep Sky Survey / Large-scale structure of the cosmos / Redshift survey / 2dF Galaxy Redshift Survey / Weak gravitational lensing / Quasar / Photometric redshift / Redshift
Date: 2009-04-01 07:04:11
Astronomy
Physical cosmology
Observational astronomy
Astronomical surveys
UKIRT Infrared Deep Sky Survey
Large-scale structure of the cosmos
Redshift survey
2dF Galaxy Redshift Survey
Weak gravitational lensing
Quasar
Photometric redshift
Redshift

Add to Reading List

Source URL: star-www.dur.ac.uk

Download Document from Source Website

File Size: 289,00 KB

Share Document on Facebook

Similar Documents

Physical cosmology / Astronomy / Observational astronomy / Large-scale structure of the cosmos / Astronomical spectroscopy / Redshift / Photometry / Galaxy / Cosmic distance ladder / Photometric redshift / Spiral galaxy / Elliptical galaxy

Photometric Z Discovery of Distant Galaxies Travis A. Rector and Andy Puckett University of Alaska Anchorage 3211 Providence Dr., Anchorage, AK USA email:

DocID: 1qDV6 - View Document

A unified approach to photometric redshift evaluation for galaxies and QSOs O. Laurino1, R. D’Abrusco2, G. Riccio1, M. Brescia3, S.G. Djorgovski4, G. Longo1 1-Dept. Physical Sciences, Univ. Napoli 2-Dept. Astronomy, Un

DocID: 1nKVU - View Document

A The Astrophysical Journal, 652:97Y106, 2006 November 20 # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. COMPARING DYNAMICAL AND PHOTOMETRIC MASS ESTIMATES OF LOW- AND HIGH-REDSHIFT

DocID: 1nCvJ - View Document

FINAL WORKSHOP OF GRID PROJECTS, ”PON RICERCA, AVVISO 1575” 1 A Web Application for Photometric Redshift Estimation

DocID: 1n2Xh - View Document

A The Astrophysical Journal, 652:97Y106, 2006 November 20 # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. COMPARING DYNAMICAL AND PHOTOMETRIC MASS ESTIMATES OF LOW- AND HIGH-REDSHIFT

DocID: 1mMO4 - View Document