gogreensurvey.ca

GOGREEN – Gemini Observations of Galaxies in Rich Early ENvironments

Gemini Observatory / AURA]. Survey will take advantage of upgraded detectors, which make Gemini’s GMOS spectrographs the best in the world for studying distant galaxy clusters. With up to 15 hours of total integration time on the faintest galaxies, the spectra will allow us to measure the dynamics of different galaxy populations, their stellar populations, and to obtain a robust measurement of the abundance of low-mass, quiescent galaxies. By combining GOGREEN. Related Surveys & Collaborations.

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GOGREEN – Gemini Observations of Galaxies in Rich Early ENvironments | gogreensurvey.ca Reviews

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Gemini Observatory / AURA]. Survey will take advantage of upgraded detectors, which make Gemini’s GMOS spectrographs the best in the world for studying distant galaxy clusters. With up to 15 hours of total integration time on the faintest galaxies, the spectra will allow us to measure the dynamics of different galaxy populations, their stellar populations, and to obtain a robust measurement of the abundance of low-mass, quiescent galaxies. By combining GOGREEN. Related Surveys & Collaborations.

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GOGREEN – Gemini Observations of Galaxies in Rich Early ENvironments | gogreensurvey.ca Reviews

https://gogreensurvey.ca

Gemini Observatory / AURA]. Survey will take advantage of upgraded detectors, which make Gemini’s GMOS spectrographs the best in the world for studying distant galaxy clusters. With up to 15 hours of total integration time on the faintest galaxies, the spectra will allow us to measure the dynamics of different galaxy populations, their stellar populations, and to obtain a robust measurement of the abundance of low-mass, quiescent galaxies. By combining GOGREEN. Related Surveys & Collaborations.

INTERNAL PAGES

gogreensurvey.ca

1

Nod & Shuffle – GOGREEN

http://gogreensurvey.ca/nod-shuffle

Nod & Shuffle. Capability applies techniques adopted for infrared-to-optical spectroscopy, whereby the sky is sampled with the same pixels used to observe the science target. The N. Observation mode was not designed or developed as one of Gemini’s original capabilities. The concept was first invented, and implemented on the AAT, by Glazebrook and Bland-Hawthorn (. Soon after it was implemented on. By the GMOS Nod and Shuffle Commissioning Team. The principal advantages of observing with N&S include:.

2

Publications – GOGREEN

http://gogreensurvey.ca/data-releases/publicationspress

1 The GEEC2 spectroscopic survey of Galaxy groups at 0.8 z 1. ML Balogh et al., 2014, MNRAS, 443, 2679. 2 Star formation and environmental quenching of GEEC2 group galaxies at z 1. A Mok et al., 2014, MNRAS, 438, 3070. 3 Efficient satellite quenching at z 1 from the GEEC2 spectroscopic survey of galaxy groups. A Mok et al., 2013, MNRAS, 431, 1090. 4 Direct observational evidence for a large transient galaxy population in groups at 0.85 z 1. ML Balogh et al., 2011, MNRAS, 412, 2303. X000B7; Contact Us.

3

Releases – GOGREEN

http://gogreensurvey.ca/data-releases

Related Surveys & Collaborations. X000B7; Contact Us.

4

Data Packages – GOGREEN

http://gogreensurvey.ca/data-releases/data-packages

Advanced data products will be released no later than 1 year. The end of the survey. For more information about the survey progress, click here. Related Surveys & Collaborations. X000B7; Contact Us.

5

About this Website – GOGREEN

http://gogreensurvey.ca/webmaster

This webpage was developed, customized and maintained by:. E-mail : fm2river@uwaterloo.ca. The site was created using the free open-source CMS software of WordPress. And uses the latest version of the blank theme GeneratePress. Created by Thomas Usborne. Last updated – Thursday March 26, 2015 @ 12:00 PM. Related Surveys & Collaborations. X000B7; Contact Us.

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localgroup.ps.uci.edu

Michael C. Cooper

http://localgroup.ps.uci.edu/cooper

Michael C. Cooper. University of California Irvine. Michael C. Cooper. Department of Physics and Astronomy. University of California Irvine. Office: 2123 Reines Hall. Cooper -at- uci.edu. Center for Galaxy Evolution. DEEP2 Data Release 1. DEEP2 Data Release 2. DEEP2 Data Release 3. DEEP2 Data Release 4. DEEP3 Preliminary Data Release. Arizona CDFS Environment Survey. IMACS Spectroscopy of UDS/COSMOS. DEEP2 DEIMOS Data Pipeline.

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GOGREEN – Gemini Observations of Galaxies in Rich Early ENvironments

Gemini Observatory / AURA]. Survey will take advantage of upgraded detectors, which make Gemini’s GMOS spectrographs the best in the world for studying distant galaxy clusters. With up to 15 hours of total integration time on the faintest galaxies, the spectra will allow us to measure the dynamics of different galaxy populations, their stellar populations, and to obtain a robust measurement of the abundance of low-mass, quiescent galaxies. By combining GOGREEN. Related Surveys & Collaborations.

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