There are two Picard recipes which can be used with ACSIS data and are of general interest:
This recipe is used to create a moments maps from a cube. It smooths the cube in frequency and spatial
extents, then uses the ClumpFind algorithm to find clumps of emission. Everything in the cube not
found in a clump is masked out, then the masked cube is collapsed to form the moments map.
Recipe options:
[1]
clumpfind
/fellwalker
/thresh
)
[clumpfind]
[25]
integ
/iwc
/itd
) [integ]
[undef]
[undef]
[0]
[3]
This recipe co-add the given files into a single map while correctly handling the exposure time FITS header and
other NDF components. The maps are combined using inverse-variance weighting and the output variance is
derived from the input variances. You can choose either wcsmosaic or a combination of wcsalign and the
Ccdpack application makemos to mosaic the images.
Recipe options:
[wcsmosaic]
median
(default), mean
or sigmas
. See ccdpack manual for advice on choosing a method.
[4]
[0]
[nearest]
There are a number of options available when running Picard recipes. The example below illustrates most of them.
params.ini
. It is called by the recpars
option. This
file has the same .ini
format used by the Orac-dr pipeline (see Section 6.2).
myfilelist.lis
in this
example).
-log
option specifies whether the log file should be written to the
screen [s
], a file [f
] or an xwindow [x
]..sdf
extension on filenames is required by Picard.
ORAC_DATA_OUT
is defined, any files created by Picard will be written in that
location. Check there if new files are expected but do not appear in your working directory.