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

Autor: H. Domínguez Sánchez, Lucia Rodríguez-Muñoz, P. Arrabal Haro, M. C. Eliche-Moral, Anton M. Koekemoer, Antonio Hernán-Caballero, B. Alcalde Pampliega, A. Lumbreras-Calle, J. M. Mas-Hesse, Jairo Méndez-Abreu, Pablo G. Pérez-González, Casiana Muñoz-Tuñón, Almudena Alonso-Herrero, Alejandro Borlaff, Antonio Cava, Jesús Gallego
Přispěvatelé: Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
Jazyk: angličtina
Rok vydání: 2019
Předmět:
Zdroj: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A52. ⟨10.1051/0004-6361/201731670⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
ISSN: 0004-6361
DOI: 10.1051/0004-6361/201731670⟩
Popis: 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. In this work, 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. We use data from the SHARDS multiband survey in the GOODS-North field. Its depth (up to magnitude $\langle m_{3\sigma}\rangle\sim26.5$) and its spectro-photometric resolution ($R\sim50$) provides us with an ideal dataset to search for emission line galaxies (ELGs). We develop a new algorithm to identify low-redshift ($z$
Comment: Accepted for publication in Astronomy & Astrophysics. 17 pages, 17 figures
Databáze: OpenAIRE