News on the ISOPHOT Interactive Analysis PIA

Bibcode
1998ASPC..145..165G
Gabriel, C.; Acosta-Pulido, J.; Heinrichsen, I.
Bibliographical reference

Astronomical Data Analysis Software and Systems VII, A.S.P. Conference Series, Vol. 145, 1998, R. Albrecht, R.N. Hook and H.A. Bushouse, eds.,p.165

Advertised on:
0
1998
Number of authors
3
IAC number of authors
0
Citations
14
Refereed citations
8
Description
The ISOPHOT Interactive Analysis system, a calibration and scientific analysis tool for the ISOPHOT instrument on board ESA's Infrared Space Observatory (I SO), has been further developed while ISO is in operation. In this paper we describe some of the improvements achieved in the last few months in the areas of scientific analysis capabilities, documentation and in related services to the astronomical community.
Type
Non-refereed

It may interest you

  • Non-refereed
    Unveiling galaxy protoclusters in the era of Euclid
    How large-scale structures formed in the early universe is a key cosmological question with few answers from empirical evidence. Unveiling galaxy clusters and their high-z progenitors (i.e., protoclusters) is essential to picture galaxy evolution drawn by the hierarchical formation scenario. However, unveiling these early structures at high
    Ramos Chernenko, Nataliya et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.2014R
    Citations
    0
  • Non-refereed
    Accretion and winds in neutron star low-mass X-ray binaries
    In recent decades, observations of the X-ray and radio continuum have been instrumental in studying the coupling between accretion and ejection processes in low-mass X-ray binaries (LMXBs), with emphasis on systems harbouring black hole accretors. However, we have only recently begun to systematically study the evolution of their X-ray, optical and
    Muñoz-Darias, Teo

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..138M
    Citations
    0
  • Non-refereed
    Constraining in-situ vs. ex-situ stellar mass in nearby galaxies with simulation-based inference
    Understanding the complexities of galaxy evolution and the role of mergers therein remains a fundamental challenge in astrophysics. Since galaxies can only be observed at a single point in cosmic time, tracing their merging history and its impact on a galaxy's mass assembly is heavily dependent on models or cosmological simulations. However, while
    Angeloudi, Eirini et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1948A
    Citations
    0