We present 2.5-11 micron spectrophotometric & imaging ISO observations of 28 Sf1, 29 Sf2
& 1 normal galaxy. The Sf1 & Sf2 MIR spectra are statistically different: Sf1 have a strong …

ESA's Infrared Space Observatory (ISO) was used to perform a deep survey with ISOCAM
through three massive gravitationally lensing clusters of galaxies. The total area surveyed …

We describe far-infrared observations of early-type galaxies selected from the Infrared
Space Observatory (ISO) archive. This rather inhomogeneous sample includes 39 giant …

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane
selected to provide information on Galactic structure, stellar populations, stellar mass-loss …

We present the results of an ISOCAM survey of the Chamaeleon I dark cloud conducted in
two broad-band filters at 6.7 and 14.3 mu m. In an area of 0.59 sq. deg. we have detected a …

Using spatial-spectral data cubes of reflection nebulae obtained by ISOCAM, we have
observed a shift in the central wavelength of the 7.7 μm band within several reflection …

Observations at near and mid-infrared wavelengths (1-18 micron) of SGR 1806-20 suggest
that it is associated with a cluster of giant massive stars which are enshrouded in a dense …

Mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are
presented together with the results of a one-year monitoring campaign of the 2.5-11.7 μm …

We present ISO photometric and spectroscopic observations of a sample of 57 bright
Asymptotic Giant Branch stars and red supergiants in the Large Magellanic Cloud, selected …

The extinction laws at 7 m and 15 m are derived for more than 120 sightlines in the inner
Galactic plane based on the ISOGAL survey data and the near-infrared data from DENIS …