Near-IR spectra of inner red giants (Gonzalez-Fernandez+, 2008)

Bibcode
2008yCat..34790131G
Gonzalez-Fernandez, C.; Cabrera-Lavers, A.; Hammersley, P. L.; Garzon, F.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/479/131. Originally published in: 2008A&A...479..131G

Advertised on:
2
2008
Number of authors
4
IAC number of authors
0
Citations
0
Refereed citations
0
Description
From the equivalent widths of the main features of the K band spectra (the NaI, CaI and CO bandheads) we have derived the metallicities of the sources by means of the empirical scale obtained by Ramirez et al. (2000AJ....120..833R) and Frogel et al. (2001AJ....122.1896F) for luminous red giants. (2 data files).
Related projects
Project Image
Morphology and dynamics of the Milky Way
This project consists of two parts, each differentiated but both complementary: morphology and dynamics. Detailed study of the morphology of the Milky Way pretends to provide a data base for the stellar distribution in the most remote and heavily obscured regions of our Galaxy, through the development of semiempirical models based on the
Martín
López Corredoira
In progress
Type
Non-refereed
The Milky Way and the Local Group (MWLG)

It may interest you

  • Non-refereed
    Conceptual design of the infrared integral field spectropolarimeter for the European Solar Telescope
    The European Solar Telescope (EST) will be Europe's most ambitious ground-based infrastructure in solar physics. It will have a primary mirror with a diameter of 4.2m, which will make it the largest in Europe, and of identical aperture as the largest solar telescope available worldwide, namely the Daniel K. Inouye Telescope (DKIST) installed at the
    Quintero Noda, C. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..2CQ
    Citations
    0
  • Non-refereed
    Detector upgrade in EMIR@GTC: on-sky performances
    EMIR was shipped to the GTC on May 2016 and had its first light on June 2016. Since the beginning, the EMIR performances have been severely hampered by the many instabilities in the infrared detector, a 2048x2048 Hawaii2, built with the old original technology of the Teledyne Hawaii series. Despite of this, the instrument has proven to be powerful
    Garzón, Francisco et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..27G
    Citations
    0
  • Non-refereed
    The Large Interferometer For Exoplanets (LIFE): a space mission for mid-infrared nulling interferometry
    The Large Interferometer For Exoplanets (LIFE) is a proposed space mission that enables the spectral characterization of the thermal emission of exoplanets in the solar neighborhood. The mission is designed to search for global atmospheric biosignatures on dozens of temperate terrestrial exoplanets and it will naturally investigate the diversity of
    Glauser, Adrian M. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13095E..1DG
    Citations
    0