Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

被引：147

作者：

Driver, Simon P. ^{[1
]}

Bellstedt, Sabine ^{[1
]}

Robotham, Aaron S. G. ^{[1
]}

Baldry, Ivan K. ^{[2
]}

Davies, Luke J. ^{[1
]}

Liske, Jochen ^{[3
]}

Obreschkow, Danail ^{[1
]}

Taylor, Edward N. ^{[4
]}

Wright, Angus H. ^{[5
]}

Alpaslan, Mehmet ^{[6
]}

Bamford, Steven P. ^{[7
]}

Bauer, Amanda E. ^{[8
]}

Bland-Hawthorn, Joss ^{[9
]}

Bilicki, Maciej ^{[10
]}

Bravo, Matias ^{[1
]}

Brough, Sarah ^{[11
]}

Casura, Sarah ^{[3
]}

Cluver, Michelle E. ^{[4
,12
]}

Colless, Matthew ^{[13
]}

Conselice, Christopher J. ^{[14
]}

Croom, Scott M. ^{[9
]}

de Jong, Jelte ^{[15
,16
]}

D'Eugenio, Franceso ^{[17
,18
,19
]}

De Propris, Roberto ^{[20
]}

Dogruel, Burak ^{[4
]}

Drinkwater, Michael J. ^{[21
]}

Dvornik, Andrej ^{[5
]}

Farrow, Daniel J. ^{[22
]}

Frenk, Carlos S. ^{[23
]}

Giblin, Benjamin ^{[24
]}

Graham, Alister W. ^{[4
]}

Grootes, Meiert W. ^{[25
]}

Gunawardhana, Madusha L. P. ^{[15
]}

Hashemizadeh, Abdolhosein ^{[1
]}

Haeussler, Boris ^{[26
]}

Heymans, Catherine ^{[5
,24
]}

Hildebrandt, Hendrik ^{[5
]}

Holwerda, Benne W. ^{[27
]}

Hopkins, Andrew M. ^{[28
]}

Jarrett, Tom H. ^{[29
]}

Jones, D. Heath ^{[30
]}

Kelvin, Lee S. ^{[31
]}

Koushan, Soheil ^{[1
]}

Kuijken, Konrad ^{[15
]}

Lara-Lopez, Maritza A. ^{[32
]}

Lange, Rebecca ^{[33
]}

Lopez-Sanchez, Angel R. ^{[28
]}

Loveday, Jon ^{[34
]}

Mahajan, Smriti ^{[35
]}

Meyer, Martin ^{[1
]}

机构：

[1] Univ Western Australia, Int Ctr Radio Astron Res ICRAR, Crawley, WA 6009, Australia

[2] Liverpool John Moores Univ, Astrophys Res Inst, 146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England

[3] Univ Hamburg, Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany

[4] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

[5] Ruhr Univ Bochum, Fac Phys & Astron, Astron Inst AIRUB, D-44780 Bochum, Germany

[6] Imagen Technol, 151 W 26th St, New York, NY 10001 USA

[7] Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England

[8] Vera C Rubin Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA

[9] Univ Sydney, Sch Phys, Sydney Astrophoton Instrumentat Labs, Sydney, NSW 2006, Australia

[10] Polish Acad Sci, Ctr Theoret Phys, Al Lotnikow 32-46, PL-02668 Warsaw, Poland

[11] Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia

[12] Univ Western Cape, Dept Phys & Astron, Robert Sobukwe Rd, ZA-7535 Bellville, South Africa

[13] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia

[14] Univ Manchester, Jodrell Bank, Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England

[15] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands

[16] Univ Groningen, Kapetyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands

[17] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HA, England

[18] Univ Cambridge, Kavli Inst Cosmol, Cambridge CB3 0HA, England

[19] Univ Ghent, Sterrenkundig Observ, Krijgslaan 281 S9, B-9000 Ghent, Belgium

[20] Univ Turku, FINCA, Vesilinnantie 5, F-20014 Turku, Finland

[21] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072, Australia

[22] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany

[23] Univ Durham, Inst Computat Cosmol, Phys Dept, Durham DH1 3LE, England

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

[25] Netherlands eSci Ctr, Sci Pk 140, NL-1098 XG Amsterdam, Netherlands

[26] European Southern Observ, Alonso de Cordova 3107,Casilla 19001, Santiago, Chile

[27] Univ Louisville, Dept Phys & Astron, 102 Nat Sci Bldg, Louisville, KY 40292 USA

[28] Macquarie Univ, Australian Astron Opt, 105 Delhi Rd, N Ryde, NSW 2113, Australia

[29] Univ Cape Town, Dept Astron, ZA-7700 Cape Town, South Africa

[30] Univ Newcastle, Pathways & Acad Learning Support Ctr, Callaghan, NSW 2308, Australia

[31] Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA

[32] Armagh Observ & Planetarium, Coll Hill, Armagh BT61 DG, North Ireland

[33] Curtin Univ, Curtin Inst Computat, POB U 1987, Perth, WA 6845, Australia

[34] Univ Sussex, Astron Ctr, Brighton BN1 9QH, E Sussex, England

[35] Indian Inst Sci Educ & Res Mohali IISERM, Manauli 140306, Punjab, India

[36] Univ North Georgia, Dept Phys & Astron, 3820 Mundy Mill Rd, Oakwood, GA 30566 USA

[37] Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai Campus, Guangzhou 519082, Peoples R China

[38] Macquarie Univ, Dept Phys & Astron, N Ryde, NSW 2109, Australia

[39] Macquarie Univ, Astron Astrophys & Astrophoton Res Ctr, Sydney, NSW 2109, Australia

[40] INAF Osservatorio Astron Padova, Via Osservatorio 5, I-35122 Padua, Italy

[41] Univ Bristol, Sch Phys, Astrophys Grp, Tyndall Ave, Bristol BS8 1TL, Avon, England

[42] Univ Hull, EA Milne Ctr Astrophys, Cottingham Rd, Kingston Upon Hull HU6 7RX, Yorks, England

[43] Univ Cent Lancashire, Sch Nat Sci, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England

[44] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA

[45] Queen Mary Univ London, Sch Phys & Astron, Mile End Rd, London E1 4NS, England

[46] Mas Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany

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

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2022年 / 513卷 / 01期

基金：

欧洲研究理事会; 英国科学技术设施理事会; 欧盟地平线“2020”; 澳大利亚研究理事会;

关键词：

catalogues; surveys; galaxies: distances and redshift; galaxies: fundamental parameters; galaxies: luminosity function; mass function; cosmological parameters; DIGITAL SKY SURVEY; LARGE-SCALE STRUCTURE; STAR-FORMATION HISTORY; REDSHIFT SURVEY; LUMINOSITY FUNCTION; MILKY-WAY; PHOTOMETRIC REDSHIFTS; VELOCITY DISPERSIONS; METALLICITY RELATION; FORMING GALAXIES;

D O I：

10.1093/mnras/stac472

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248 682 galaxy spectra, and, in combination with earlier surveys, results in 330 542 redshifts across five sky regions covering similar to 250 deg(2). The redshift density, is the highest available over such a sustained area, has exceptionally high completeness (95 per cent to r(KiDS) = 19.65 mag), and is well-suited for the study of galaxy mergers, galaxy groups, and the low redshift (z < 0.25) galaxy population. DR4 includes 32 value-added tables or Data Management Units (DMUs) that provide a number of measured and derived data products including GALEX, ESO KiDS, ESO VIKING, WISE, and HerschelSpace Observatory imaging. Within this release, we provide visual morphologies for 15 330 galaxies to z < 0.08, photometric redshift estimates for all 18 million objects to r(KiDS) similar to 25 mag, and stellar velocity dispersions for 111 830 galaxies. We conclude by deriving the total galaxy stellar mass function (GSMF) and its sub-division by morphological class (elliptical, compact-bulge and disc, diffuse-bulge and disc, and disc only). This extends our previous measurement of the total GSMF down to 10(6.75) M-circle dot h(70)(-2) and we find a total stellar mass density of rho(*) = (2.97 +/- 0.04) x 10(8) M-circle dot h(70) Mpc(-3) or Omega(*)=(2.17 +/- 0.03) x 10(-3) h(70)(-1). We conclude that at z < 0.1, the Universe has converted 4.9 +/- 0.1 per cent of the baryonic mass implied by big bang Nucleosynthesis into stars that are gravitationally bound within the galaxy population.

引用

页码：439 / 467

页数：29

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Galaxy And Mass Assembly (GAMA): Data Release 4 and the z &lt; 0.1 total and z &lt; 0.08 morphological galaxy stellar mass functions

Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions