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  • Time: MJD
  • Frequency: Hz
  • Energy: eV or multiples (keV, MeV, GeV)
  • Fluxes (nuFnu): erg/cm2/s (or Jy*Hz, if easier)
  • Fluxes should be already corrected and dereddened (ground based observatories should correct also for the extinction due to the airmass). Use as reference AV=0.277 and the extinction laws of Cardelli et al. (1989).
  • Include also the observed magnitudes (for NIR/optical/UV data).
  • Inclued also some short text explaining the data analysis performed.
  • Include also the list of people (and their affiliations) to be included in the authors list.

Deadline to send data: 31 July 2009