Euclid: the selection of quiescent and star-forming galaxies using observed colours

被引：13

作者：

Bisigello, L. ^{[1
,2
]}

Kuchner, U. ^{[1
]}

Conselice, C. J. ^{[1
]}

Andreon, S. ^{[3
]}

Bolzonella, M. ^{[2
]}

Duc, P-A ^{[4
]}

Garilli, B. ^{[5
]}

Humphrey, A. ^{[6
]}

Maraston, C. ^{[7
]}

Moresco, M. ^{[2
,8
]}

Pozzetti, L. ^{[2
]}

Tortora, C. ^{[9
]}

Zamorani, G. ^{[2
]}

Auricchio, N. ^{[2
]}

Brinchmann, J. ^{[6
]}

Capobianco, V ^{[10
]}

Carretero, J. ^{[11
]}

Castander, F. J. ^{[12
,13
]}

Castellano, M. ^{[14
]}

Cavuoti, S. ^{[15
,16
,17
]}

Cimatti, A. ^{[8
,9
]}

Cledassou, R. ^{[18
]}

Congedo, G. ^{[19
]}

Conversi, L. ^{[20
]}

Corcione, L. ^{[10
]}

Cropper, M. S. ^{[21
]}

Dusini, S. ^{[22
]}

Frailis, M. ^{[23
]}

Franceschi, E. ^{[2
]}

Franzetti, P. ^{[5
]}

Fumana, M. ^{[5
]}

Hormuth, F. ^{[24
]}

Israel, H. ^{[25
]}

Jahnke, K. ^{[26
]}

Kermiche, S. ^{[27
]}

Kitching, T. ^{[21
]}

Kohley, R. ^{[20
]}

Kubik, B. ^{[28
]}

Kunz, M. ^{[29
,30
]}

Le Fevre, O. ^{[31
]}

Ligori, S. ^{[10
]}

Lilje, P. B. ^{[32
]}

Lloro, I ^{[12
,13
]}

Maiorano, E. ^{[2
]}

Marggraf, O. ^{[33
]}

Massey, R. ^{[34
]}

Masters, D. C. ^{[35
]}

Mei, S. ^{[36
,37
]}

Mellier, Y. ^{[38
,39
]}

Meylan, G. ^{[40
]}

机构：

[1] Univ Nottingham, Univ Pk, Nottingham NG7 2RD, England

[2] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy

[3] INAF Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy

[4] Univ Strasbourg, Observ Astron Strasbourg ObAS, CNRS, UMR 7550, F-67000 Strasbourg, France

[5] INAF IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy

[6] Univ Porto, CAUP, Inst Astrofis & Ciencias Espaco, Rua Estrelas, P-4150762 Porto, Portugal

[7] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[8] Univ Bologna, Dipartimento Fis & Astron, Via Gobetti 93-2, I-40129 Bologna, Italy

[9] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

[10] INAF Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy

[11] Inst Fis Altes Energies IFAE, E-08193 Barcelona, Spain

[12] CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain

[13] Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain

[14] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

[15] Univ Federico II, Dept Phys E Pancini, Via Cinthia 6, I-80126 Naples, Italy

[16] INFN, Sect Naples, Via Cinthia 6, I-80126 Naples, Italy

[17] INAF Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy

[18] Ctr Natl Etud Spatiales, F-31401 Toulouse, France

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

[20] ESAC ESA, Camino Bajo Castillo S-N, E-28692 Madrid, Spain

[21] Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England

[22] INFN Padova, Via Marzolo 8, I-35131 Padua, Italy

[23] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34131 Trieste, Italy

[24] von Hoerner & Sulger GmbH, Schlosspl 8, D-68723 Schwetzingen, Germany

[25] Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany

[26] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[27] Aix Marseille Univ, CPPM, CNRS, IN2P3, F-13284 Marseille, France

[28] Inst Phys Nucl, 4 Rue Enrico Fermi, F-69622 Villeurbanne, France

[29] Univ Geneva, Dept Phys Theor, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland

[30] Univ Geneva, Ctr Astroparticle Phys, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland

[31] Aix Marseille Univ, CNRS, CNES, LAM, F-13284 Marseille, France

[32] Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway

[33] Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany

[34] Univ Durham, Ctr Extragalact Astron, Dept Phys, South Rd, Durham DH1 3LE, England

[35] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[36] Univ Paris Denis Diderot, Univ Paris Sorbonne Cite PSC, F-75205 Paris 13, France

[37] Sorbonne Univ, Observ Paris, Univ PSL, CNRS,LERMA, F-75014 Paris, France

[38] Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France

[39] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France

[40] Ecole Polytech Fed Lausanne, Observ Sauverny, CH-1290 Versoix, Switzerland

[41] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[42] Univ Paris Saclay, Univ Paris Diderot, Sorbonne Paris Cite, AIM,CEA,CNRS, F-91191 Gif Sur Yvette, France

[43] Italian Space Agcy, Space Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy

[44] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany

[45] Inst Space Sci IEEC CSIC, C Can Magrans S-N, E-08193 Barcelona, Spain

[46] Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1349018 Lisbon, Portugal

[47] Univ Lisbon, Fac Ciencias, Dept Fis, Edificio C8, P-1749016 Lisbon, Portugal

[48] Univ Politecn Cartagena, Dept Elect & Tecnol Comp, E-30202 Cartagena, Spain

[49] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy

[50] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2020年 / 494卷 / 02期

基金：

美国国家航空航天局; 芬兰科学院;

关键词：

galaxies: evolution; galaxies: general; galaxies: photometry; CHALLENGE LIGHTCONE SIMULATION; EVOLUTION SURVEY COSMOS; ENVIRONMENTAL DEPENDENCE; MAGNITUDE DISTRIBUTION; PHOTOMETRIC REDSHIFTS; LUMINOSITY FUNCTION; FORMATION RATES; LEGACY SURVEY; STELLAR MASS; RED SEQUENCE;

D O I：

10.1093/mnras/staa885

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Euclid mission will observe well over a billion galaxies out to z similar to 6 and beyond. This will offer an unrivalled opportunity to investigate several key questions for understanding galaxy formation and evolution. The first step for many of these studies will be the selection of a sample of quiescent and star-forming galaxies, as is often done in the literature by using well-known colour techniques such as the UV/diagram. However, given the limited number of filters available for the Euclid telescope, the recovery of such rest-frame colours will be challenging. We therefore investigate the use of observed Euclid colours, on their own and together with ground-based u-band observations, for selecting quiescent and star-forming galaxies. The most efficient colour combination, among the ones tested in this work, consists of the (u - VIS) and (VIS - J) colours. We find that this combination allows users to select a sample of quiescent galaxies complete to above similar to 70 per cent and with less than 15 per cent contamination at redshifts in the range 0.75 < z < 1. For galaxies at high-z or without the u-band complementary observations, the (VIS - Y) and (J - H) colours represent a valid alternative, with > 65 per cent completeness level and contamination below 20 per cent at 1 < z < 2 for finding quiescent galaxies. In comparison, the sample of quiescent galaxies selected with the traditional UVJ technique is only similar to 20 per cent complete at z < 3, when recovering the rest-frame colours using mock Euclid observations. This shows that our new methodology is the most suitable one when only Euclid bands, along with u-band imaging, are available.

引用

页码：2337 / 2354

页数：18

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