Present and future of the OTELO project

Bibcode
2015hsa8.conf..304R
Ramón-Pérez, M.; Bongiovanni, A.; Cepa, J.; Pérez García, A.; Alfaro, E. J.; Castañeda, H.; Ederoclite, A.; González-Serrano, J. I.; González, J. J.; Gallego, J.; Sánchez-Portal, M.
Bibliographical reference

Highlights of Spanish Astrophysics VIII, Proceedings of the XI Scientific Meeting of the Spanish Astronomical Society held on September 8-12, 2014, in Teruel, Spain, ISBN 978-84-606-8760-3. A. J. Cenarro, F. Figueras, C. Hernández-Monteagudo, J. Trujillo Bueno, and L. Valdivielso (eds.), p. 304-309

Advertised on:
5
2015
Number of authors
11
IAC number of authors
4
Citations
0
Refereed citations
0
Description
OTELO 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.
Type
Non-refereed

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