From Espresso to Codex

Bibcode
2009svlt.conf..243L
DOI
10.1007/978-1-4020-9190-2_41
Liske, J.; Pasquini, L.; Bonifacio, P.; Bouchy, F.; Carswell, R. F.; Cristiani, S.; Dessauges, M.; D'Odorico, S.; D'Odorico, V.; Grazian, A.; Garcia-Lopez, R.; Haehnelt, M.; Israelian, G.; Lovis, C.; Martin, E.; Mayor, M.; Molaro, P.; Murphy, M. T.; Pepe, F.; Queloz, D.; Rebolo, R.; Udry, S.; Vanzella, E.; Viel, M.; Wiklind, T.; Zapatero, M.; Zucker, S.
Referencia bibliográfica

Science with the VLT in the ELT Era, Astrophysics and Space Science Proceedings. ISBN 978-1-4020-9189-6. Springer Netherlands, 2009, p. 243

Fecha de publicación:
0
2009
Número de autores
27
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
CODEX and ESPRESSO are concepts for ultra-stable, high-resolution spectrographs at the E-ELT and VLT, respectively. Both instruments are well motivated by distinct sets of science drivers. However, ESPRESSO will also be a stepping stone towards CODEX both in a scientific as well as in a technical sense. Here we discuss this role of ESPRESSO with respect to one of the most exciting CODEX science cases, i.e. the dynamical determination of the cosmic expansion history.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Fecha de publicación:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Número de citas
    0
  • Sin árbitro
    Co-phasing the distributed aperture of a Fizeau interferometer via photonic lanterns and machine learning
    The advantage of large optical telescopes from the ground for high-contrast direct imaging relies on achieving exquisite control of the incident optical wavefront. Since the exoplanet problem almost always has a bright star within a small field of view there are usually ample photons for measuring the atmospheric and telescopedistorted wavefront. A
    Padrón-Brito, Auxiliadora et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..25P
    Número de citas
    0
  • Sin árbitro
    Unveiling Chiron, an odd ice ball, with Webb: Ice and Gas Phases Revealed
    We present unprecedented findings on (2060) Chiron using James Webb Space Telescope (JWST) NIRSpec imaging and spectroscopy from cycle 1 GTO program 1273. Our study (Pinilla-Alonso et al. 2024 A&A Letter) marks the first detection of carbon dioxide (CO 2) and methane (CH 4) active outgassing and coma emission at heliocentric distances of ~18 au
    Pinilla-Alonso, Noemí et al.

    Fecha de publicación:

    10
    2024
    Bibcode
    2024DPS....5640508P
    Número de citas
    0