Autor: |
Xu, Hai, Dai, Y. Sophia, Huang, Jia-Sheng, Wang, Zhaoyu, Cheng, Cheng, Shao, Xu, Wu, Shumei, Yang, Xiaohu, Jing, Yipeng, Sawicki, Marcin, Liu, Feng-Yuan |
Rok vydání: |
2020 |
Předmět: |
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Druh dokumentu: |
Working Paper |
DOI: |
10.3847/1538-4357/abbeff |
Popis: |
In this paper we present a simple color-magnitude selection and obtain a large sample of 33,893 massive quiescent galaxies at intermediate redshifts (110.5, with a median of log(M*/M_sun)=11.0. A small fraction of our galaxies is also covered by the HST CANDELS. Morphological analysis in the observed H band shows that the majority of this subsample are early-type galaxies. As massive early-type galaxies trace the high density regions in the large scale structure in the universe, our study provides a quick and simple way to obtain a statistical significant sample of massive galaxies in a relative narrow redshift range. Our sample is 7-20 times larger at the massive end (log(M*/M_sun)>10.5) than any existing samples obtained in previous surveys. This is a pioneer study, and the technique introduced here can be applied to future wide-field survey to study large scale structure, and to identify high density region and clusters. Comment: 16 pages, 16 figures, accepted for publication in ApJ |
Databáze: |
arXiv |
Externí odkaz: |
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