Bibcode
Cepa, J.; Bongiovanni, A.; Ramón-Pérez, M.; Pérez García, A. M.; Alfaro, E. J.; Castaneda, H. O.; Cerviño, M.; Gallego, J.; González, J. J.; González-Serrano, J. I.; Lara-López, M. A.; Pérez-Martínez, R.; Pintos-Castro, I.; Sánchez-Portal, M.; Bland-Hawthorn, J.; Jones, D. H.
Referencia bibliográfica
Highlights on Spanish Astrophysics IX, Proceedings of the XII Scientific Meeting of the Spanish Astronomical Society held on July 18-22, 2016, in Bilbao, Spain, ISBN 978-84-606-8760-3. S. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernández-Monteagudo, A. Sánchez-Lavega, S. Pérez-Hoyos (eds.), 2017 , p. 76-87
Advertised on:
3
2017
Número de citas
0
Número de citas referidas
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Descripción
The status of OTELO and Lockman SpReSO surveys, the two large guaranteed
time programs currently under way using OSIRIS at the 10.4m GTC is
presented. The OTELO project, designed to detect the main optical
emission lines from Hα to Lyα at redshifts from 0.4 through
7, is the deepest emission line survey to date, with unprecedented
sensitivity in the detection of small equivalent widths. Lockman SpReSO
is aimed to obtaining optical spectra, up to 24.5 AB magnitudes, in the
central 24×24 square arcminutes of the Lockman Hole field, which
has been observed with ROSAT and XMM–Newton at the highest depth.
Lockman SpReSO mainly targets Far Infrared sources detected with the
Herschel Space Observatory.