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Finding galaxy clusters with spectro-photometric density in SDSS

Published online by Cambridge University Press:  01 July 2007

Joo H. Yoon ,
Kevin Schawinski ,
Yun-Kyeong Sheen ,
Chang H. Ree  and
Sukyoung K. Yi
Joo H. Yoon
Affiliation:
Department of Astronomy, Yonsei University, Seoul 120-749, Korea Center for Space Astrophysics, Yonsei University, Seoul 120-749, Korea
Kevin Schawinski
Affiliation:
Department of Physics, University of Oxford, Oxford OX1 3RH, UK email: jhyoon@galaxy.yonsei.ac.kr
Yun-Kyeong Sheen
Affiliation:
Department of Astronomy, Yonsei University, Seoul 120-749, Korea Center for Space Astrophysics, Yonsei University, Seoul 120-749, Korea
Chang H. Ree
Affiliation:
Center for Space Astrophysics, Yonsei University, Seoul 120-749, Korea
Sukyoung K. Yi
Affiliation:
Department of Astronomy, Yonsei University, Seoul 120-749, Korea Center for Space Astrophysics, Yonsei University, Seoul 120-749, Korea
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Abstract

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We have attempted to overcome the incompleteness of spectroscopic survey and found galaxy clusters by measuring the spectro-photometric density of galaxies.

Keywords

cataloguessurveysgalaxies: clustersgalaxies: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 421 - 426
Copyright
Copyright © International Astronomical Union 2008

References

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