The OTELO survey: New evidence of downsizing from the specific star formation rates, stellar mass functions, and star formation histories of a sample of low-mass galaxies at 0.38<z <1.43
[Aims] We present an analysis of the emitters (H , H , and [O ii]) from the OTELO survey, in order to characterize the star formation properties of low-mass galaxies (<109 M stellar masses).
| Autores: | , , , , , , , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/392141 |
| Acceso en línea: | http://hdl.handle.net/10261/392141 |
| Access Level: | acceso abierto |
| Palabra clave: | Surveys Galaxies: luminosity function, mass function Galaxies: starburst Galaxies: star formation Cosmology: observations |
| Sumario: | [Aims] We present an analysis of the emitters (H , H , and [O ii]) from the OTELO survey, in order to characterize the star formation properties of low-mass galaxies (<109 M stellar masses). |
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