Galaxy evolution studies observing Emission Line Galaxies with the GTC

Bibcode
2003RMxAC..16..221G
Gallego, J.
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. 221-224 (2003) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
0
2003
Número de autores
1
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Emission line galaxies are the most easily detected and studied objects in the high redshift Universe. They are being used to trace the evolution of the critical observables of the Universe such as star formation rate densities, starburst properties, and abundances. The GTC will be a very powerful tool for studying the evolution of emission line galaxy populations at different redshifts. Large surveys, such as OTELO, carried out with OSIRIS and extended by follow-up spectroscopic studies in the near infrared using EMIR will enable the GTC to make a major impact in extragalactic astronomy.
Tipo
Sin árbitro
Galaxias

Te puede interesar

  • Sin árbitro
    New Robotic Telescope system progress towards critical design review
    The 4m class New Robotic Telescope (NRT) is an optical facility designed to revolutionize the rapid follow-up and classification of variable and transient objects. The project is at the stage where key systems are progressing through their detailed design phases, which presents a major engineering challenge for all project partners to manage design
    Copley, David et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..3WC
    Número de citas
    0
  • Sin árbitro
    Phase diversity application on the EST MCAO testbench
    Phase Diversity (PD) is a technique widely used to measure and compensate for Non-Common Path Aberrations (NCPA) in optical systems. Beyond its traditional applications, PD has found further uses in solar astrophysics, where it enhances image quality by processing multiple images to correct residual aberrations. In this work, we introduce a
    Rodriguez-Linares, Nicolas et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13097E..5OR
    Número de citas
    0
  • Sin árbitro
    First light of the upgraded Gregor Infrared Spectrograph
    For more than ten years, the Gregor Infrared Spectrograph (GRIS) has been the infrared spectropolarimeter on the Gregor telescope since its inauguration in 2012. The instrument mainly performs polarimetric observations of the wavelength regions at 1083 and 1565nm, which have high scientific potential. There, observers can find spectral lines that
    Quintero Noda, C. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..42Q
    Número de citas
    0