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Summary Statement — Carnegie-Spitzer-IMACS Redshift Survey

Only in current section. The Carnegie-Spitzer-IMACS Redshift Survey. The Carnegie-Spitzer-IMACS (CSI) survey, currently underway at the Magellan-Baade 6.5m telescope in Chile, has been specifically designed to characterize normal galaxies and their environments to z=1.5. The survey selection is done using 3.6μm observations of Spitzer Legacy fields, providing as close a selection by stellar mass as possible. 1 z)=1% for galaxies brighter than i'=23 mag and σ. Principal Investigator: Daniel D. Kelson.

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Summary Statement — Carnegie-Spitzer-IMACS Redshift Survey | csi.obs.carnegiescience.edu Reviews

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Only in current section. The Carnegie-Spitzer-IMACS Redshift Survey. The Carnegie-Spitzer-IMACS (CSI) survey, currently underway at the Magellan-Baade 6.5m telescope in Chile, has been specifically designed to characterize normal galaxies and their environments to z=1.5. The survey selection is done using 3.6μm observations of Spitzer Legacy fields, providing as close a selection by stellar mass as possible. 1 z)=1% for galaxies brighter than i'=23 mag and σ. Principal Investigator: Daniel D. Kelson.

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Summary Statement — Carnegie-Spitzer-IMACS Redshift Survey | csi.obs.carnegiescience.edu Reviews

https://csi.obs.carnegiescience.edu

Only in current section. The Carnegie-Spitzer-IMACS Redshift Survey. The Carnegie-Spitzer-IMACS (CSI) survey, currently underway at the Magellan-Baade 6.5m telescope in Chile, has been specifically designed to characterize normal galaxies and their environments to z=1.5. The survey selection is done using 3.6μm observations of Spitzer Legacy fields, providing as close a selection by stellar mass as possible. 1 z)=1% for galaxies brighter than i'=23 mag and σ. Principal Investigator: Daniel D. Kelson.

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Summary Statement — Carnegie-Spitzer-IMACS Redshift Survey

http://csi.obs.carnegiescience.edu/Summary/sendto_form

Send this page to somebody. Fill in the email address of your friend to send an email with the address. The e-mail address to send this link to. A comment about this link. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California, 91101 USA. Powered by Plone CMS, the Open Source Content Management System. This site conforms to the following standards:. Usable in any browser.

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Example Spectral Energy Distributions — Carnegie-Spitzer-IMACS Redshift Survey

http://csi.obs.carnegiescience.edu/Examples

Example Spectral Energy Distributions. Example Spectral Energy Distributions. Band images of the galaxies. In particular, we note the top-left and bottom-left, two galaxies for which broadband photometry alone would be insufficient to provide redshift estimates. Low dispersion spectroscopy is key to isolating Balmer breaks and emission lines in blue galaxies, leading to redshift uncertainties with very little dependence on spectral type. Powered by Plone CMS, the Open Source Content Management System.

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Carnegie-Spitzer-IMACS Redshift Survey — Carnegie-Spitzer-IMACS Redshift Survey

http://csi.obs.carnegiescience.edu/sitemap

An overview of the available content on this site. Keep the pointer still over an item for a few seconds to get its description. The Carnegie-Spitzer-IMACS Redshift Survey of Galaxy Evolution since z=1.5: I. Description and Methodology. A Direct Measurement of Hierarchical Growth in Galaxy Groups since z 1. The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5 z 1 in the CDFS with CSI. Example Spectral Energy Distributions. Powered by Plone CMS, the Open Source Content Management System.

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Papers — Carnegie-Spitzer-IMACS Redshift Survey

http://csi.obs.carnegiescience.edu/Papers

The Carnegie-Spitzer-IMACS Redshift Survey of Galaxy Evolution since z=1.5: I. Description and Methodology. A Direct Measurement of Hierarchical Growth in Galaxy Groups since z 1. The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5 z 1 in the CDFS with CSI. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California, 91101 USA. Powered by Plone CMS, the Open Source Content Management System. This site conforms to the following standards:. Usable in any browser.

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Animations — Carnegie-Spitzer-IMACS Redshift Survey

http://csi.obs.carnegiescience.edu/Movies

These are simple renderings of preprogrammed paths through some of the CSI data. In three-dimensional comoving coordinates we show 30,000 galaxies from the CSI redshift catalog down to logM=10.3 dex. Blue spheres are those selected to be star-forming by their (U-V) and (V-J) colors, and yellow spheres are those selected to be quiescent by the same method (see,e.g., Williams et al 2009, Kelson et al 2014). Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California, 91101 USA.

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Summary Statement — Carnegie-Spitzer-IMACS Redshift Survey

Only in current section. The Carnegie-Spitzer-IMACS Redshift Survey. The Carnegie-Spitzer-IMACS (CSI) survey, currently underway at the Magellan-Baade 6.5m telescope in Chile, has been specifically designed to characterize normal galaxies and their environments to z=1.5. The survey selection is done using 3.6μm observations of Spitzer Legacy fields, providing as close a selection by stellar mass as possible. 1 z)=1% for galaxies brighter than i'=23 mag and σ. Principal Investigator: Daniel D. Kelson.

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