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dc.contributor.authorRamón-Pérez, M.
dc.contributor.authorBongiovanni, A.
dc.contributor.authorCepa, J.
dc.contributor.authorPérez-García, A. M.
dc.contributor.authorAlfaro, E. J.
dc.contributor.authorCastañeda, H.
dc.contributor.authorEderoclite, A.
dc.contributor.authorGonzález Serrano, José Ignacio 
dc.contributor.authorGonzález, J. J.
dc.contributor.authorGallego, J.
dc.contributor.authorSánchez-Portal, M.
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2022-07-01T13:19:09Z
dc.date.available2022-07-01T13:19:09Z
dc.date.issued2014
dc.identifier.isbn978-84-606-8760-3
dc.identifier.otherAYA2011-29517-C03-01es_ES
dc.identifier.urihttp://hdl.handle.net/10902/25244
dc.description.abstractOTELO is an emission-line object survey carried out with the red tunable filter of the instrument OSIRIS at the GTC, whose aim is to become the deepest emission-line object survey to date. With 100% of the data of the first pointing finally obtained in June 2014, we present here some aspects of the processing of the data and the very first results of the OTELO survey. We also explain the next steps to be followed in the near future.es_ES
dc.description.sponsorshipThis work was supported by the Spanish Ministry of Economy and Competitiveness (MINECO) under the grant AYA2011-29517-C03-01. Based on observations made with the Gran Telescopio de Canarias (GTC), installed in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias, in the island of La Palma.es_ES
dc.format.extent6 p.es_ES
dc.language.isoenges_ES
dc.sourceHighlights of Astronomy and Astrophysics VIII: Proceedings of the XI Scientific Meeting of the Spanish Astronomical Society (SEA) held in Teruel, September 8-12, 2014, [Barcelona], Sociedad Española de Astronomía, 2014es_ES
dc.titlePresent and future of the OTELO projectes_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.rights.accessRightsopenAccesses_ES
dc.type.versionpublishedVersiones_ES


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