Data Reduction Pipeline for EMIR; a near-IR multiobject spectrograph for the Spanish 10m telescope

Bibcode
2002SPIE.4847..402G
DOI
10.1117/12.460344
Gallego, Jesus; Cardiel, Nicolas; Serrano, Angel; Gorgas, Javier; Zamorano, Jaime; Garzon, Francisco; Garcia-Dabo, Cesar-Enrique; Gil de Paz, Armando
Bibliographical reference

Astronomical Data Analysis II. Edited by Starck, Jean-Luc; Murtagh, Fionn D. Proceedings of the SPIE, Volume 4847, pp. 402-409 (2002).

Advertised on:
12
2002
Number of authors
8
IAC number of authors
1
Citations
1
Refereed citations
0
Description
EMIR (Espectrografo Multiobjeto Infrarrojo) is a near-infrared wide-field camera and multi-object spectrograph to be built for the 10.4m Spanish telescope (Gran Telescopio Canarias, GTC) at La Palma. The Data Reduction Pipeline (DRP), which is being designed and built by the EMIR Universidad Complutense de Madrid group, will be optimized for handling and reducing near-infrared data acquired with EMIR. Both reduced data and associated error frames will be delivered to the end-users as a final product.
Type
Non-refereed

It may interest you

  • Non-refereed
    Magnetohydrodynamic Processes in Solar Plasmas
    Magnetohydrodynamic Processes in Solar Plasmas provides a comprehensive theory and practice of basic plasma processes in the Sun and heliosphere. It deals with the basic dynamics of the Sun from its interior up to its outer atmosphere in the framework of Magnetohydrodynamics. Topics covered include essential phenomena in the solar interior such as
    Srivastava, Abhishek Kumar et al.

    Advertised on:

    5
    2024
    Bibcode
    2024mpsp.book.....S
    Citations
    0
  • Non-refereed
    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.

    Advertised on:

    1
    2024
    Bibcode
    2024asi..confP..71A
    Citations
    0
  • Non-refereed
    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.

    Advertised on:

    3
    2024
    Bibcode
    2024aecc.conf...24B
    Citations
    0