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Narrowband selected high-redshift galaxy candidates contaminated by lower redshift [OIII] ultra-strong emitter line galaxies
| Indexado |
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| DOI | 10.1051/0004-6361/201425183 | ||||
| Año | 2015 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. From this work and the literature we remark that the [OIII] line appears to be a common source of contamination in high-redshift LBG and LAE samples and we suggest that efforts be made to characterize with high accuracy the [OIII] luminosity function out to redshift similar to 3 or higher.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Penin, Aurelie | Mujer |
Aix Marseille Univ - Francia
Univ KwaZulu Natal - República de Sudáfrica Laboratoire d'Astrophysique de Marseille - Francia University of KwaZulu-Natal - República de Sudáfrica |
| 2 | Cuby, J. G. | Hombre |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| 3 | Clement, Benjamin | Hombre |
UNIV ARIZONA - Estados Unidos
UNIV LYON 1 - Francia The University of Arizona - Estados Unidos Université Claude Bernard Lyon 1 - Francia |
| 4 | Hibon, Pascale | Mujer |
Observatorio Gemini - Chile
Gemini ObservatorySouthern Operations Center - Chile |
| 5 | Kneib, Jean-Paul | Hombre |
Aix Marseille Univ - Francia
Ecole Polytech Fed Lausanne - Suiza Laboratoire d'Astrophysique de Marseille - Francia Swiss Federal Institute of Technology EPFL, Lausanne - Suiza Ecole Polytechnique Fédérale de Lausanne - Suiza |
| 6 | Cassata, P. | Hombre |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| 7 | Ilbert, O. | Hombre |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| Fuente |
|---|
| CNRS |
| European Research Council |
| Agence Nationale de la Recherche |
| Centre National de la Recherche Scientifique |
| ERC advanced LIDA |
| Agradecimiento |
|---|
| The authors would like to thank the referee whose comments improved this manuscript. We thank Hakim Atek, Brian Lemaux, Danka Paraficz, Johan Richard, and Tayyaba Zafar for valuable discussions. We thank Len Cowie for providing the USEL templates. This work received support from the Agence Nationale de la Recherche bearing the reference ANR-09-BLAN-0234. J.P.K. acknowledges support from ERC advanced LIDA and from CNRS. |
| The authors would like to thank the referee whose comments improved this manuscript. We thank Hakim Atek, Brian Lemaux, Danka Paraficz, Johan Richard, and Tayyaba Zafar for valuable discussions. We thank Len Cowie for providing the USEL templates. This work received support from the Agence Nationale de la Recherche bearing the reference ANR-09-BLAN-0234. J.P.K. acknowledges support from ERC advanced LIDA and from CNRS. |
