Advantages of NIR Multiobject Spectroscopy of z ˜ 1 Galaxies

Bibcode
2001defi.conf..153D
DOI
10.1007/10854354_32
Domínguez-Tagle, Carlos; Prada, Francisco; Manchado, A.; Mayya, Divakara
Referencia bibliográfica

Deep Fields: Proceedings of the ESO Workshop Held at Garching, Germany, 9-12 October 2000, ESO ASTROPHYSICS SYMPOSIA. ISBN 3-540-42799-6. Edited by S. Cristiani, A. Renzini, and R.E. Williams. Springer-Verlag, 2001, p. 153

Fecha de publicación:
0
2001
Número de autores
4
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
Galaxy redshift surveys from z ˜ 1 to z ˜ 4 providing thousands of identified objects are already available. Only for a small and selected sample of those galaxies, near-infrared (NIR) spectroscopy and emission line studies exist. This is mainly due to the time-consuming work of observing one object at a time. This will change with the advent of multiobject NIR spectrographs.
Tipo
Sin árbitro

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