The bivariate K-band-submillimetre luminosity functions of the local HRS galaxy sample

被引：5
|
作者：
Andreani, P. [1 ]
Spinoglio, L. [2 ]
Boselli, A. [3 ,4 ]
Ciesla, L. [3 ,4 ]
Cortese, L. [5 ]
Vio, R. [6 ]
Baes, M. [7 ]
Bendo, G. J. [8 ]
De Looze, I. [7 ]
机构：
[1] European So Observ, D-85748 Garching, Germany
[2] Ist Astrofis & Planetol Spaziale, INAF, I-00133 Rome, Italy
[3] Univ Aix Marseille, LAM, F-13388 Marseille 13, France
[4] CNRS, UMR 7326, F-13388 Marseille, France
[5] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[6] Chip Comp Consulting Srl, I-30020 Venice, Italy
[7] Univ Ghent, Sterrenkundig Observ, B-9000 Ghent, Belgium
[8] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, UK ALMA Reg Ctr Node, Manchester M13 9PL, Lancs, England
来源：
ASTRONOMY & ASTROPHYSICS | 2014年 / 566卷
关键词：
methods: data analysis; galaxies: luminosity function; mass function; submillimeter: galaxies; galaxies: statistics; methods: statistical; HERSCHEL REFERENCE SURVEY; VIRGO CLUSTER; NEARBY GALAXIES; IRAS GALAXIES; DUST; EVOLUTION; MORPHOLOGY; CATALOG; PLANE; SPIRE;
D O I：
10.1051/0004-6361/201322747
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study the relationship between the K-band and the sub-millimetre (submm) emissions of nearby galaxies by computing the bivariate K-band-submm luminosity function (BLF) of the Herschel Reference Survey (HRS), a volume-limited sample observed in submm with Herschel/SPIRE. We derive the BLF from the K-band and submm cumulative distributions using a copula method. Using the BLF allows us to derive the relationship between the luminosities on more solid statistical ground. The analysis shows that over the whole HRS sample, no statistically meaningful conclusion can be derived for any relationship between the K-band and the submm luminosity. However, a very tight relationship between these luminosities is highlighted, by restricting our analysis to late-type galaxies. The luminosity function of late-type galaxies computed in the K-band and in the submm are dependent and the dependence is caused by the link, between the stellar mass and the cold dust mass, which has been already observed.
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页数：8
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