Infrared Imaging of Perpendicular Nested Bars in Spiral Galaxies with the Infrared Camera at the Carlos Sánchez Telescope

Bibcode
2001Ap&SS.276..675K
DOI
10.1023/A:1017576924822
Kemp, S. N.; Chan, S. J.; Beckman, J. E.; Hammersley, P. L.
Referencia bibliográfica

Astrophysics and Space Science, v. 276, Issue 2/4, p. 675-682 (2001).

Fecha de publicación:
3
2001
Revista
Astrophysics and Space Science
Número de autores
4
Número de autores del IAC
3
Número de citas
0
Número de citas referidas
0
Descripción
Images are presented of some of the galaxies in the sample of the BARS `International Time Project' in the near-infrared JHK_s bands, obtained with the Infra-Red Camera at the 1.5 m Carlos Sánchez Telescope, Teide Observatory, between 1996 and 1998. We discuss the scientific importance of imaging galaxies in the near-infrared bands and recent and future developments concerning the Infra-Red Camera.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    3D scaling laws and projection effects in The300-NIKA2 Sunyaev-Zeldovich Large Program Twin Samples
    The abundance of galaxy clusters with mass and redshift is a wellknown cosmological probe. The cluster mass is a key parameter for studies that aim to constrain cosmological parameters using galaxy clusters, making it critical to understand and properly account for the errors in its estimates. Subsequently, it becomes important to correctly
    Paliwal, A. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300037P
    Número de citas
    0
  • Sin árbitro
    Generating galaxy clusters mass density maps from mock multiview images via deep learning
    Galaxy clusters are composed of dark matter, gas and stars. Their dark matter component, which amounts to around 80% of the total mass, cannot be directly observed but traced by the distribution of diffused gas and galaxy members. In this work, we aim to infer the cluster's projected total mass distribution from mock observational data, i.e. stars
    de Andres, Daniel et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300013D
    Número de citas
    0
  • Sin árbitro
    The European Low Frequency Survey. Observing the radio sky to understand the beginning of the Universe
    In this paper we present the European Low Frequency Survey (ELFS), a project that will enable the detection of primordial B-mode polarization by measuring the Galactic and extra-Galactic foregrounds in the 5- 120 GHz frequency window. Indeed, the main difficulty in measuring the Bmode polarization comes not just from its sheer faintness, but from
    Mennella, A. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300031M
    Número de citas
    0