REDUCE_SCAN_FAINT_POINT_SOURCES

Process SCAN data from faint compact sources

Description:

This is the recipe for processing SCAN data for faint compact sources. The makemap configuration file is tuned to best deal with such data, though the user may specify their own.

Raw data are passed to the map maker which are processed using the blank_field config file to produce an image, which is calibrated in mJy/beam, displayed and tagged as a reduced product. The noise is estimated and the NEFD is calculated. Once all the individual observations have been processed, a coadd is created and displayed. This image is processed with a matched filter to enhance the signal-to-noise ratio of point sources. This image is tagged as a reduced product. The noise properties and NEFD for the new Group image are calculated and written to log files. A signal-to-noise ratio image is created from the matched-filtered image.

Finally, the CUPID task findclumps is run using the fellwalker algorithm to create a source catalogue.

Notes:

Available Parameters :

The following parameters can be set via the -recpars option:
FINDCLUMPS_CFG
Name of a config file for use with the CUPID findclumps task. The file must exist in the current working directory, $FINDCLUMPS_CONFIG_DIR or $ORAC_DATA_OUT.
MAKEMAP_CONFIG
Name of a config file for use with the SMURF makemap task. The file must exist in the current working directory, $MAKEMAP_CONFIG_DIR, $ORAC_DATA_OUT, $ORAC_DATA_CAL or $STARLINK_DIR/share/smurf.
MAKEMAP_PIXSIZE
Size of the pixels in the output map. If not specified, the recipe uses the appropriate default value. Note that the timeseries will be downsampled to match this scale during the map-making process.
MAKEMAP_REF
Name of a reference image (NDF format) to use to define the output pixel grid. The NDF can be either 2D or 3D and the spatial WCS frame will be extracted.

Display

The Frame image is displayed in Gaia window 1. The Group image is displayed in Gaia window 2; its variance is displayed in window 3.