GALEP, Spectral Mapping of the Inner Galaxy with EMIR

Bibcode
2010hsa5.conf..411G
DOI
10.1007/978-3-642-11250-8_104
Garzón, F.; Hammersley, P. L.; González-Fernández, C.; Cabrera-Lavers, A.
Bibliographical reference

Highlights of Spanish Astrophysics V, Astrophysics and Space Science Proceedings. ISBN 978-3-642-11249-2. Springer-Verlag Berlin Heidelberg, 2010, p. 411

Advertised on:
2010
Number of authors
4
IAC number of authors
4
Citations
0
Refereed citations
0
Description
We propose to use EMIR to obtain near IR spectroscopy of many thousands Galaxy sources, mainly located in the inner regions. These will be selected from their position on IR colour-magnitude (CM) diagrams and will include disc, bar bulge and ring sources. The principal aim is to accurately classify the sources to provide a better understanding of, particularly, the redder parts of a infrared CM diagram. Without this information there will remain ambiguities in the interpretation of structures in the inner Galaxy.
Type
Non-refereed

It may interest you

  • Non-refereed
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Advertised on:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Citations
    0
  • Non-refereed
    HARMONI at ELT: HIPOTEC electronics and control system
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470nm to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The
    Menéndez Mendoza, Saúl et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..4ZM
    Citations
    0