Star-forming galaxies at low-redshift in the SHARDS survey

被引：0

作者：

Lumbreras-Calle, A. ^{[1
,2
]}

Muñoz-Tuñón, C. ^{[1
,2
]}

Méndez-Abreu, J. ^{[1
,2
,3
]}

Mas-Hesse, J.M. ^{[4
]}

Pérez-González, P.G. ^{[5
]}

Alcalde Pampliega, B. ^{[5
]}

Arrabal Haro, P. ^{[1
,2
]}

Cava, A. ^{[6
]}

Domínguez Sánchez, H. ^{[7
,8
]}

Eliche-Moral, M.C. ^{[5
]}

Alonso-Herrero, A. ^{[9
]}

Borlaff, A. ^{[1
,2
]}

Gallego, J. ^{[5
]}

Hernán-Caballero, A. ^{[5
]}

Koekemoer, A.M. ^{[10
]}

Rodríguez-Muñoz, L. ^{[11
]}

机构：

[1] Instituto de Astrofísica de Canarias, Calle Vía Láctea S/n, La Laguna, Tenerife,38200, Spain

[2] Departamento de Astrofísica, Universidad de la Laguna, La Laguna, Tenerife,38205, Spain

[3] School of Physics and Astronomy, University of St. Andrews, SUPA, North Haugh, St. Andrews,KY16 9SS, United Kingdom

[4] Centro de Astrobiología, CSIC/INTA, Ctra. de Torrejn a Ajalvir, 4 km, Torrejón de Ardoz, Madrid,28850, Spain

[5] Departamento de Astrofísica y Ciencias de la Atmósfera, Facultad de CC. Físicas, Universidad Complutense de Madrid, Madrid,28040, Spain

[6] Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, Versoix,1290, Switzerland

[7] GEPI, Observatoire de Paris, CNRS, Université Paris Diderot, Place Jules Janssen, Meudon,92190, France

[8] Department of Physics and Astronomy, University of Pennsylvania, Philadelphia,PA,19104, United States

[9] Centro de Astrobiología (CAB, CSIC-INTA, ESAC Campus, Villanueva de la Cañada, Madrid,28692, Spain

[10] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore,MD,21218, United States

[11] Dipartimento di Fisica e Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, Padova,I35122, Italy

来源：

Astronomy and Astrophysics | 2019年 / 621卷

基金：

欧洲研究理事会;

关键词：

Galaxies: fundamental parameters - Galaxies: photometry - Galaxies: star formation - Galaxies: starbursts - Galaxies: stellar content;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Context. The physical processes driving the evolution of star formation (SF) in galaxies over cosmic time still present many open questions. Recent galaxy surveys allow now to study these processes in great detail at intermediate redshift (0 = z = 0:5). Aims. We build a complete sample of star-forming galaxies and analyze their properties, reaching systems with low stellar masses and low star formation rates (SFRs) at intermediate-to-low redshift. Methods. We use data from the SHARDS multiband survey in the GOODS-North field. Its depth (up to magnitude hm3si ∼ 26:5) and its spectro-photometric resolution (R ∼ 50) provides us with an ideal dataset to search for emission line galaxies (ELGs). We develop a new algorithm to identify low-redshift (z © 2019 ESO.

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