MIDAS models interstellar/intergalactic absorption lines.

Details MIDAS models interstellar/intergalactic absorption lines. MIDAS models interstellar/intergalactic absorption lines.

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988msngr..54...61p&link_type=abstract

The Messenger, vol. 54, p. 61-63

Astronomy and Astrophysics

Astronomy

Absorption Lines:Numerical Simulations, Supernova 1986G In Ngc 5128

Scientific paper

Most of the current tools available in MIDAS, as weil as in other image processing systems for Astronomy, are dedicated to the first step of data reduc- . tion which is to eliminate the instrumental signatures from the observations. This is clearly the main priority for such a system and continuous development is going on to support all the instruments available at La Silla. Very little effort has been dedicated to the complementary problem, the development of analysis tools to bring physical interpretation closer to the observed data. This article describes a new MIDAS context CLOUD - that allows such an analysis, namely, to model the absorption of interstellar or intergalactic clouds as observed in spectroscopic data.

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