Quantitative Morphological Analysis of Galaxies at Intermediate Red Shift: Clues to Galaxy Evolution

Bibcode
2003RMxAC..16..315T
Trujillo, I.; Gutiérrez, Carlos M.; Alfonso, J.; Aguerri, J. A. L.; Cepa, Jordi
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. 315-316 (2003) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
0
2003
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We have developed morphological analysis software for studying galaxies from low to high redshifts. This code is designed to extract quantitative information about the morphology of the different components of galaxies (bulges and disks) imaged with both HST and ground-based observations. We present here some of its possible applications to the GTC in order to follow galaxy morphological evolution up to z ˜ 0.5.
Tipo
Sin árbitro
Galaxias
Fotometría

Te puede interesar

  • Sin árbitro
    NIRPS near-infrared spectrograph: AITV phase at ESO3.6m/La Silla
    NIRPS is a fiber-fed AO nIR spectrograph working simultaneously with HARPS at the La Silla-ESO 3.6m telescope. The cryogenic spectrograph operating at 75K employs a cross-dispersed echelle grating (R4), covering a wavelength range of 0.98-1.80 microns in a single image using a Teledyne Hawaii-4RG infrared detector. In early 2022, the NIRPS
    Malo, Lison et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..46M
    Número de citas
    0
  • Sin árbitro
    Transport, handling, and integration of the adaptive optics system for GTC: from the laboratory to the telescope
    The Gran Telescopio de Canarias Adaptive Optics System (GTCAO) is currently in its commissioning phase at Roque de Los Muchachos Observatory (ORM). The GTCAO is a single-conjugated post-focal system equipped with a Shack- Hartmann Wavefront Sensor (WFS) and a Deformable Mirror (DM) conjugated to the pupil, achieving a Strehl Ratio of 65% in the K
    González Carretero, Eduardo D. et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..96G
    Número de citas
    0
  • Sin árbitro
    Euclid commissioning results: the near infrared spectrometer and photometer (NISP) signal detection chain
    Euclid, the M2 mission of the ESA's Cosmic Vision 2015-2025 program, aims to explore the Dark Universe by conducting a survey of approximately 14 000 deg 2 and creating a 3D map of the observable Universe of around 1.5 billion galaxies up to redshift z ∼ 2. This mission uses two main cosmological probes: weak gravitational lensing and galaxy
    Cogato, F. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13092E..3GC
    Número de citas
    0