The EUCLID-NIS Mission

Bibcode
2010hsa5.conf..469B
DOI
10.1007/978-3-642-11250-8_131
Balcells, M.
Referencia bibliográfica

Highlights of Spanish Astrophysics V, Astrophysics and Space Science Proceedings. ISBN 978-3-642-11249-2. Springer-Verlag Berlin Heidelberg, 2010, p. 469

Fecha de publicación:
0
2010
Número de autores
1
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
Obtaining a measure of the baryonic acoustic oscillations (BAO) is among the top goals of cosmology in the beginning of the twenty-first century. Detection of BAOs offers the possibility to test the standard cosmological model, by providing strong constraints on the equation of state of dark energy. The EUCLID-NIS mission proposes to measure BAOs by mapping the 3D distribution of baryons at intermediate redshift, 1 < z < 3. Such map will be derived from spectroscopic redshifts in the J and H bands, for the order of 108 galaxies, from space. In the current design, the instrument utilizes digital micromirror devices (DMD) from Texas Instruments.
Tipo
Sin árbitro

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