Galactic Astronomy with OTELO

Bibcode
2003RMxAC..16..255A
Alfaro, E. J.; Cepa, J.; Gallego, J.; González-Serrano, J.; González, J.; Sánchez-Portal, M.
Referencia bibliográfica

Science with the GTC (Eds. José Miguel Rodríguez Espinosa, Francisco Garzón López, and Verónica Melo Martín) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 16, pp. 255-256 (2003) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
0
2003
Número de autores
6
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
OTELO (OSIRIS Tunable Emission Line Object survey) is a project aimed at studying the low end luminosity function of emission line galaxies. A broad band survey at B ≈ 24 magnitudes detection level will also be performed for a field of view of about 14 square degrees corresponding to the lowest selected redshift (z = 0.08). This huge amount of data will contain invaluable information about the stellar content of a deep portion of our own Galaxy. In this contribution we revise different Galactic projects in which these data could provide new and important insights into classical and new Galactic questions.
Tipo
Sin árbitro
Galaxias

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