Clash: Extreme emission-line galaxies and their implication on selection of high-redshift galaxies

We utilize the Cluster Lensing And Supernova survey with Hubble observations of 25 clusters to search for extreme emission-line galaxies (EELGs). The selections are carried out in two central bands: F105W (Y105) and F125W (J125), as the flux of the central bands could be enhanced by the presence of...

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Detalles Bibliográficos
Autores: Huang, Xingxing, Zheng, Wei, Wang, Junxian, Ford, Holland, Lemze, Doron, Moustakas, John, Shu, Xinwen, Van der Wel, Arjen, Zitrin, Adi, Frye, Brenda L., Postman, Marc, Bartelmann, Matthias, Benítez, Narciso, Bradley, Larry, Broadhurst, Tom, Coe, Dan, Donahue, Megan, Infante, Leopoldo, Kelson, Daniel, Koekemoer, Anton, Lahav, Ofer, Medezinski, Elinor, Moustakas, Leonidas, Rosati, Piero, Seitz, Stella, Umetsu, Keiichi
Tipo de recurso: artículo
Estado:Versión aceptada para publicación
Fecha de publicación:2015
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/397495
Acceso en línea:http://hdl.handle.net/10261/397495
Access Level:acceso abierto
Palabra clave:Galaxies: high-redshift
Galaxies: formation
Galaxies: photometry
Descripción
Sumario:We utilize the Cluster Lensing And Supernova survey with Hubble observations of 25 clusters to search for extreme emission-line galaxies (EELGs). The selections are carried out in two central bands: F105W (Y105) and F125W (J125), as the flux of the central bands could be enhanced by the presence of [O iii] λλ4959, 5007 at redshifts of ∼0.93–1.14 and 1.57–1.79, respectively. The multiband observations help to constrain the equivalent widths (EWs) of emission lines. Thanks to cluster lensing, we are able to identify 52 candidates down to an intrinsic limiting magnitude of 28.5 and to a rest-frame [O iii] λλ4959, 5007 EW of ≃ 3700 Å. Our samples include a number of EELGs at lower luminosities that are missed in other surveys, and the extremely high EW can only be found in such faint galaxies. These EELGs can mimic a dropout feature similar to that of high-redshift galaxies and contaminate the color–color selection of high-redshift galaxies when the signal-to-noise ratio is limited or the band coverage is incomplete. © 2015. The American Astronomical Society. All rights reserved.

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