OSIRIS Large Guaranteed Time Programs

Bibcode
2017hsa9.conf...76C
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

Fecha de publicación:
3
2017
Número de autores
16
Número de autores del IAC
4
Número de citas
0
Número de citas referidas
0
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.
Tipo
Sin árbitro

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