Data Analysis and Simulations of Spectroscopic and Continuum Mapping with the ISOPHOT Interactive Analysis (PIA)

Bibcode
2000ASPC..216..619G
Gabriel, C.; Acosta-Pulido, J. A.; Hur, M.
Referencia bibliográfica

Astronomical Data Analysis Software and Systems IX, ASP Conference Proceedings, Vol. 216, edited by Nadine Manset, Christian Veillet, and Dennis Crabtree. Astronomical Society of the Pacific, ISBN 1-58381-047-1, 2000., p.619

Fecha de publicación:
0
2000
Número de autores
3
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
The ISOPHOT Interactive Analysis (PIA) is the software tool of choice for the scientific analysis of ISOPHOT data. It is used in more than 200 astronomy institutes all over the world and it has been continuously upgraded during and after the operational phase of the ISO mission. Special enhancements concerning the analysis of imaging spectrophotometry data as well as the inclusion of a raster data simulation package within the PIA capabilities are discussed here.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Design and manufacture of athermalized optomechanical mounts for GRANCAIN, the infrared imaging instrument for GTC's adaptive optics
    GRANCAIN (GRAN CAmara INfrarroja) is a first-light imaging instrument in the infrared J, H and K bands that will be integrated into the adaptive optics focus of the Gran Telescopio de Canarias. The purpose of the instrument is to capture SWIR diffraction-limited images for a field of view of 22x22 arcsec. The instrument boasts a telecentric optical
    González-Carretero, Eduardo D. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13100E..6VG
    Número de citas
    0
  • Sin árbitro
    Optical coating facilities at the Instituto de Astrofísica de Canarias
    The Instrumentation Division of the Instituto de Astrofísica de Canarias (IAC) is involved since several years in upgrading its capacities to design and manufacture optical components. To this end, we have created a new laboratory (Centre for Advanced Optical Systems, CSOA) which will be capable to design, fabricate and qualify large optical
    Insausti, M. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13100E..23I
    Número de citas
    0
  • Sin árbitro
    Measuring Rotation Periods and Stellar Oscillations in Red Giants with TESS Data
    TESS is a powerful engine for studying stellar variability. However, it has been challenging to adopt methods used for other space missions, such as Kepler, to infer rotation periods and solar-like oscillation frequencies in TESS data. The availability of multiple sectors of data for most targets, improved stability, and the release of new
    García, Rafael A. et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024tsc3.confE..32G
    Número de citas
    0