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.
Cite
@article{arxiv.1502.01673,
title = {Present and future of the OTELO project},
author = {M. Ramón-Pérez and A. Bongiovanni and J. Cepa and A. M Pérez-García and E. J. Alfaro and H. Castañeda and A. Ederoclite and J. I. González-Serrano and J. J. González and J. Gallego and M. Sánchez-Portal},
journal= {arXiv preprint arXiv:1502.01673},
year = {2015}
}
Comments
Oral contribution presented in the XI Scientific Meeting of the Spanish Astronomical Society held on September 8-12, in Teruel, Spain (7 pages, 2 figures, 1 table). To appear in Highlights of Spanish Astrophysics VIII, Proceedings of the XI Scientific Meeting of the Spanish Astronomical Society. Eds. A. J. Cenarro, F. Figueras, C. Hern\'andez-Monteagudo, J. Trujillo, L. Valdivielso