The Hα nature of the Universe at z ˜ 0.83

Bibcode
2007RMxAC..29..178V
Villar, V.; Gallego, J.; Pascual, S.; Zamorano, J.; Noeske, K.; Koo, D. C.
Referencia bibliográfica

First Light Science with the GTC (Eds. R. Guzmán, C. Packham, J. M. Rodríguez-Espinosa, & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 29, pp. 178-178 (2007) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
6
2007
Número de autores
6
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We present here the results of a survey searching for current-star forming galaxies at at z ˜ 0.83. Objects are selected by their emission in the Hα line through the narrow band filter technique.
Tipo
Sin árbitro
Galaxias
Función de luminosidad
Galaxias

Te puede interesar

  • Sin árbitro
    Application of Bayesian Inference to disentangle CMB foregrounds
    Both Galactic dust emission and Cosmic infrared background anisotropies (CIB) act as a dominant foreground contaminant for the measurements of the CMB anisotropies (intensity and polarization) at the frequency range above 217 GHz. The Galactic dust and CIB share a similar form of spectral energy distribution, which makes it harder to disentangle
    Adak, Debabrata et al.

    Fecha de publicación:

    1
    2024
    Bibcode
    2024asi..confP..71A
    Número de citas
    0
  • Sin árbitro
    Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems
    The evolution of stars and their hosting binary systems is a highly interactive process and cannot be investigated in a segregated manner. Due to the constraints drawn by stellar binarity, oscillating red-giant stars in binary systems represent a unique opportunity to study the details of the structure and evolution of stars in the advanced phases
    Beck, P. G. et al.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024aecc.conf...24B
    Número de citas
    0
  • Sin árbitro
    Triple-Double Radio Galaxies: Clues for understanding recurrent AGN activity
    Using LOFAR Two-metre Sky Survey (LoTSS), we discovered three cycles of episodic jet activity (J1225+4011, Chavan et al. 2023, MNRAS) in a giant radio galaxy, which is an extremely rare class of restarted Active Galactic Nuclei (AGN), making it only fourth of its kind. It is also called 'Triple-Double Radio Galaxy' (TDRG). J1225+4011 extends up to
    Chavan, Kshitij et al.

    Fecha de publicación:

    1
    2024
    Bibcode
    2024asi..confP..64C
    Número de citas
    0