Herschel-ATLAS : the spatial clustering of low- and high-redshift submillimetre galaxies

被引：9

作者：

Amvrosiadis, A. ^{[1
]}

Valiante, E. ^{[1
]}

Gonzalez-Nuevo, J. ^{[2
]}

Maddox, S. J. ^{[1
,3
]}

Negrello, M. ^{[1
]}

Eales, S. A. ^{[1
]}

Dunne, L. ^{[1
]}

Wang, L. ^{[4
,5
]}

van Kampen, E. ^{[6
]}

De Zotti, G. ^{[7
]}

Smith, M. W. L. ^{[1
]}

Andreani, P. ^{[6
]}

Greenslade, J. ^{[8
]}

Tai-An, C. ^{[8
]}

Michalowski, M. J. ^{[3
,9
]}

机构：

[1] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[2] Univ Oviedo, Dept Fs, C Federico Garcia Lorca 18, E-33007 Oviedo, Spain

[3] Univ Edinburgh, Royal Observ, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[4] SRON Netherlands Inst Space Res, Landleven 12, NL-9747 AD Groningen, Netherlands

[5] Univ Groningen, Kapteyn Astron Inst, Postbus 800, NL-9700 AV Groningen, Netherlands

[6] ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[7] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy

[8] Imperial Coll, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England

[9] Adam Mickiewicz Univ, Fac Phys, Astron Observ Inst, Ul Sloneczna 36, PL-60286 Poznan, Poland

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2019年 / 483卷 / 04期

基金：

英国科学技术设施理事会; 欧洲研究理事会;

关键词：

galaxies: high-redshift; galaxies: evolution; large-scale structure of Universe; submillimetre: galaxies; COSMOLOGY LEGACY SURVEY; DATA RELEASE; NUMBER COUNTS; SKY SURVEY; POPULATION; BRIGHT; MODEL; BIAS; COUNTERPARTS; EXPLORER;

D O I：

10.1093/mnras/sty3013

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present measurements of the angular correlation function of sub-millimetre (sub-mm) galaxies (SMGs) identified in four out of the five fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) - GAMA-9h, GAMA-12h, GAMA-15h, and NGP - with flux densities S-250 (mu m) > 30 mJy at 250 mu m. We show that galaxies selected at this wavelength trace the underlying matter distribution differently at low and high redshifts. We study the evolution of the clustering finding that at low redshifts sub-mm galaxies exhibit clustering strengths of r(0) similar to 2-3 h(-1) Mpc, below z < 0.3. At high redshifts, on the other hand, we find that sub-mm galaxies are more strongly clustered with correlation lengths r(0) = 8.1 +/- 0.5, 8.8 +/- 0.8, and 13.9 +/- 3.9 h(-1) Mpc at z = 1-2, 2-3. and 3-5, respectively. We show that sub-mm galaxies across the redshift range 1 < z < 5, typically reside in dark-matter halos of mass of the order of similar to 10(12.5)- 10(13.0) h(-1) M-circle dot and are consistent with being the progenitors of local massive elliptical galaxies that we see in the local Universe.

引用

页码：4649 / 4664

页数：16

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