The IRIS data is a reprocessing of the IRAS data set
and has the same geometry as the IRAS Sky Survey Atlas (ISSA,
labeled as IRAS nnn micron in <i>SkyView</i>) surveys.
This new generation of IRAS images, called IRIS,
benefits from a better zodiacal light subtraction,
from a calibration and zero level compatible with DIRBE,
and from a better destriping.
At 100 micron the IRIS product is also a significant improvement
from the Schlegel et al. (1998) maps.
IRIS keeps the full ISSA resolution,
it includes well calibrated point sources and the
diffuse emission calibration at scales smaller
than 1 degree was corrected for the variation of
the IRAS detector responsivity with scale and brightness.
The uncertainty on the IRIS calibration and zero level
are dominated by the uncertainty on the DIRBE calibration
and on the accuracy of the zodiacal light model.
<p>
More information about the IRIS dataset is available at
<a href="https://www.cita.utoronto.ca/~mamd/IRIS"> the IRIS website</a>
whence most of the preceding description came. Provenance: Original IRAS data: NASA/JPL IPAC, <br>
IRIS Reprocessing: Canadian Institute for Theoretical Astrophysics/Institut
d'Astrophysique Spatiale<br>
See the
<a href="https://www.cita.utoronto.ca/~mamd/IRIS"> IRIS website</a>.. This is a service of NASA HEASARC.