Supernova Observations and Data Reduction

Winter School 2005
Asiago (Italy) - February 7-11, 2005




General guidelines for the Lectures


  • Each lecture should last about 1.5 hours, divided in two parts, 45 minutes each, separated by a 10-15 minutes break.
  • We do not want to give introductions to astronomy basics and we will assume they are well known by the attendands. We will try to concentrate only on the aspects related to Supernovae.
  • Given the quite wide range of expertise level in the audience, the lectures should be pretty didactical, with a style closer to a university lecture than to a conference seminar. Nevertheless, the tone should be kept rather friendly and not too academical.
  • The general idea is to provide the attendants with all the knowledge required to write a proposal and properly reduce the data. For this reason, real and practical cases should be shown and described.
  • The length of the lectures should allow us to give a detailed overview of the topics covered.
  • Given the length of the lecture, we should try as much as possible to keep the thing interesting and stimulating.
  • The lectures should give to everybody the opportunity of asking questions and to have personal discussion with the lecturers. For this, the nights at the telescope can also be used.
  • Some practical exercises could also be proposed. For this purpose, we will distribute a set of data to be reduced by everybody and then collect the results (even after the school) and compare them. Lecturers can also provide their own data set for the participants who want to verify their understanding of the problems.

    School Topics

    For each of the topics to be covered by the lectures, here follows a tentative list of items that we would like to be discussed:

    1. B. Schmidt: Observations: methods, calibrations, problems and precautions

    2. S. Benetti: Data reduction for Optical Imaging and Spectroscopy

    3. C. Gerardy: Data reduction for IR Imaging and Spectroscopy

    4. P. Antilogus: Integral Field Spectroscopy

    5. F. Patat: Polarimetry and Spectropolarimetry




    Sponsored by The Physics of Type Ia Supernovae - a European Research and Training Network


    Last modified: Thu Jan 13 12:38:49 CET 2005

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