Interpreting the Statistical Properties of High-z Extragalactic Sources Detected by the South Pole Telescope Survey

被引：3
|
作者：
Cai, Zhen-Yi [1 ,2 ]
Negrello, Mattia [3 ]
De Zotti, Gianfranco [4 ]
机构：
[1] Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China
[2] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China
[3] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales
[4] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy
来源：
ASTROPHYSICAL JOURNAL | 2022年 / 932卷 / 01期
基金：
美国国家科学基金会; 美国国家航空航天局;
关键词：
STAR-FORMING GALAXIES; COSMOLOGY LEGACY SURVEY; NUMBER COUNTS; SUBMILLIMETER GALAXIES; REDSHIFT DISTRIBUTION; DEEP FIELD; MILKY-WAY; HERSCHEL; EVOLUTION; CATALOG;
D O I：
10.3847/1538-4357/ac6c83
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The results of the recently published spectroscopically complete survey of dusty star-forming galaxies detected by the South Pole Telescope over 2500 deg(2) proved to be challenging for galaxy formation models that generally underpredict the observed abundance of high-z galaxies. In this paper we interpret these results in the light of a physically grounded model for the evolution of spheroidal galaxies. The model accurately reproduces the measured redshift distribution of galaxies without any adjustment of the parameters. The data do not support the indications of an excess of z > 4 dusty galaxies reported by some analyses of Herschel surveys.
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页数：8
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