Evolution of the most massive galaxies to z= 0.6 - I. A new method for physical parameter estimation-Reference-Cited by-同舟云学术

Evolution of the most massive galaxies to z= 0.6 - I. A new method for physical parameter estimation

Published:2012-01 Issue: Volume: Page:no-no
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Chen Yan-Mei,Kauffmann Guinevere,Tremonti Christy A.,White Simon,Heckman Timothy M.,Kovač Katarina,Bundy Kevin,Chisholm John,Maraston Claudia,Schneider Donald P.,Bolton Adam S.,Weaver Benjamin A.,Brinkmann Jon

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/421/1/314/3132359/mnras0421-0314.pdf

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1. The Third Data Release of the Sloan Digital Sky Survey

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3. THE EIGHTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST DATA FROM SDSS-III

4. The history of star-forming galaxies in the Sloan Digital Sky Survey

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