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COSMOS 2□∘ Survey

Scoville, Nick (2006) COSMOS 2□∘ Survey. In: Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer-Verlag , Berlin, pp. 330-336. ISBN 978-3-540-25665-6. https://resolver.caltech.edu/CaltechAUTHORS:20191106-155935667

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Abstract

The Cosmic Evolution Survey (COSMOS) will provide complete multi-wavelength imaging and spectroscopy of a 2□∘ equatorial field aimed at sampling the full range of cosmological environments from voids to massive clusters to understand the coupled evolution of dark matter, luminous galaxies and clusters and AGN in the epoch of maximum formation activity from z = 0.5 to 3. The COSMOS survey has several major primary components: 1) HST-ACS imaging covering the entire field in I-band (8100Å); 2) ground-based broadband imaging (Subaru, NOAO and CFHT) providing photometric redshifts (typical accuracy 10%); 3) low resolution optical spectra (R = 200 with VLT-VIMOS) for 90,000 galaxies with I < 25 mag. Over 60 astronomers from Europe, North America and Japan are actively involved in COSMOS multi-λ observations and science.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/10995020_51DOIArticle
ORCID:
AuthorORCID
Scoville, Nick0000-0002-0438-3323
Additional Information:© 2005 Springer-Verlag Berlin Heidelberg. First Online: 05 January 2006.
Subject Keywords:Dark Matter; Couple Evolution; Photometric Redshift; Dark Matter Distribution; Luminous Galaxy
Series Name:ESO Astrophysics Symposia
Record Number:CaltechAUTHORS:20191106-155935667
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191106-155935667
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99714
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:07 Nov 2019 00:22
Last Modified:07 Nov 2019 00:22

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