Publication
The OTELO Project
The OTELO Project is an extragalactic survey under way using the tunable filters of the instrument OSIRIS at the GTC. OTELO is already providing the deepest...
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PublicationThe OTELO ProjectOSIRIS is the Spanish Day One instrument for the GTC 10.4-m telescope. OSIRIS is a general purpose instrument for imaging, low-resolution long slit and multi...
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PublicationThe OTELO survey. A case study of [O III] λ4959,5007 emitters at ⟨z⟩ = 0.83Context. The OSIRIS Tunable Filter Emission Line Object (OTELO) survey is a very deep, blind exploration of a selected region of the Extended Groth Strip and is...
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PublicationThe OTELO survey. A case study of [O III] λ4959,5007 emitters at ⟨z⟩ = 0.83 (Corrigendum)
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PublicationThe OTELO survey. Faint end of the luminosity function of [O II]3727 emitters at ⟨z⟩ = 1.43Aims: In this paper, we aim to study the main properties and luminosity function (LF) of the [O II]3727 emitters detected in the OTELO survey in order to...
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PublicationThe OTELO survey. I. Description, data reduction, and multi-wavelength catalogueContext. The evolution of galaxies through cosmic time is studied observationally by means of extragalactic surveys. The usefulness of these surveys is greatly...
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PublicationThe OTELO survey. II. The faint-end of the Hα luminosity function at z ̃ 0.40Aims: We take advantage of the capability of the OTELO survey to obtain the Hα luminosity function (LF) at z ̃ 0.40. Because of the deepest coverage of OTELO...
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PublicationThe OTELO survey. III. Demography, morphology, IR luminosity and environment of AGN hostsAims: We take advantage of the capabilities of the OSIRIS Tunable Emission Line Object (OTELO) survey to select and study the AGN population in the field. In...
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PublicationThe OTELO survey. Revealing a population of low-luminosity active star-forming galaxies at z ∼ 0.9Aims: We study a sample of Hβ emission line sources at z ∼ 0.9 to identify the star-forming galaxies sample and characterise them in terms of line luminosity...