The OTELO project

J. Cepa*, E. J. Alfaro, J. Bland-Hawthorn, H. O. Castañeda, J. Gallego, J. I. González-Serrano, J. J. González, D. Heath Jones, A. M. Pérez-García, M. Sánchez-Portal

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contributionpeer-review

6 Citations (Scopus)

Abstract

OTELO, (OSIRIS Tunable Emission Line Object Survey), will survey emission line objects using OSIRIS tunable filters in selected atmospheric windows relatively free of sky emission lines. Different high latitude and low extinction sky regions with enough angular separations will be observed yielding a total area of 1{2 square degrees. A 5 depth of 8×10 -18 erg/cm2/s will allow detecting objects of EW-6, making OTELO the deepest emission line survey to date. OTELO is a deep space probe that will provide a representative sample of the Universe from z =0.24 through 6.7. Given the observing procedure, OTELO will allow studying clearly de fined volumes of Universe at a known ux limit. In this contribution, a review of the project status is presented,together with some of the most significant evolutionary studies that will be tackled.

Original languageEnglish
Title of host publicationII International GTC Workshop
Subtitle of host publicationscience with GTC 1st-light instruments and the LMT
EditorsAna María Hidalgo-Gámez
Place of PublicationMexico City
PublisherUniversidad Nacional Autonoma de Mexico
Pages82-87
Number of pages6
ISBN (Print)970322802X, 9789703228027
Publication statusPublished - 2005
Externally publishedYes
EventInternational GTC Workshop: Science with GTC 1st-light Instruments and the LMT - México, D.F., Mexico
Duration: 16 Feb 200418 Feb 2004

Publication series

NameRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
Volume24
ISSN (Print)1405-2059

Conference

ConferenceInternational GTC Workshop
CountryMexico
City México, D.F.
Period16/02/0418/02/04

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