This is a "sollicited" proposal to use ISOCAM's CVF filters as a follow up of
several observations already performed using only ISOCAM discrete filters.
The main justification for using the CVF to repeat a number of already existing
filter observations is to facilitate the understanding of the photometry
obtained with ISOCAM's discrete filters by being able to assess the relative
contribution of PAHs, H2, and continuum emission within the bandpass of the
filters.
A small consortium led by Diego Cesarsky was organized, including some ten
astronomers from France, Germany, Italy, Holland and the USA to define the
relevant supplementary observations and to carry out the data reduction; the
list is presented below as participating Co-Is. Each Co-I may invite a student
or colleague of his/her to join the ISOCAM CVF consortium. When applicable, the
PI of the proposal that led to these observations will be invited to join
the consortium.
The ISO products will be made available to the general community ONE month
after their reception by the consortium PI. The data will be made available in
the ftp area to be created and advertised in the Orsay ISO Centre web page (URL
http://iscam1.station.fr)