Deep multicolor NIR survey of the Galactic plane

Bibcode
2004ASPC..317..275C
Cabrera-Lavers, A.; Garzon, F.; Vicente, B.; Hammersley, P.
Referencia bibliográfica

Milky Way Surveys: The Structure and Evolution of our Galaxy, Proceedings of ASP Conference #317. The 5th Boston University Astrophysics Conference held 15-17 June, 2003 at Boston University, Boston, MA, USA. Edited by Dan Clemens, Ronak Shah, and Teresa Brainerd. San Francisco: Astronomical Society of the Pacific, 2004., p.275

Fecha de publicación:
12
2004
Número de autores
4
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
We present a deep multicolor NIR survey that we are currently undertaking at the Instituto de Astrofísica de Canarias (Spain). The aim of the survey is obtain deep star counts in selected areas distributed along the Galactic plane to analyze the large scale structure of the Milky Way and the galactic components, in particular the Galactic bar. We are at least one magnitude deeper than in 2MASS and DENIS Galactic surveys, and even more in the inner Galaxy, as we are less limited by source confusion. This provides a better analysis of those regions where the extinction is higher.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    NEOMIR: ESA's space-based infrared mission for NEO detection and early warning
    The Near-Earth Object Mission in the Infra-Red (NEOMIR) is the first ESA's space-based mission fully dedicated to discovering near-Earth objects (NEOs), with a focus to detect and raise early warning for the smaller objects that are coming from the Sun direction, thus nearly impossible to be detected by ground-based optical survey. NEOMIR is
    Conversi, L. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13092E..2HC
    Número de citas
    0
  • Sin árbitro
    Upgrading the polarisation modulation unit of the Gregor Infrared Spectrograph
    The Gregor Infrared Spectrograph (GRIS) is installed at the Gregor telescope at Observatorio del Teide, Spain. The instrument started observations in 2012 and underwent several upgrades in the following years. Currently, it is experiencing the most significant upgrade so far, which includes, among other things, adding two optical channels to
    Quintero Noda, C. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..2EQ
    Número de citas
    0
  • Sin árbitro
    Small-ELF Telescope opto-mechanical system: progress on design, manufacturing, and tensegrity prototyping
    Small-ELF (SELF) is a 3.5-meter telescope currently entering the manufacturing phase and will serve as a technology precursor for the much larger telescope named ELF (Exo-Life Finder). The primary objective of the proposed design approach is to to radically improve the system's capabilities for the detection of biomarkers and life in the
    Zhou, Ye et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..3RZ
    Número de citas
    0