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Offline 70um filtering of photometry observations with IDL
For photometry observations of a single source, we suggest using the
following two procedures for cleaning up artifacts at 70 um. The IDL tools
assume access to the IDL astrolib.
(1) bcd_column_fiter.pro
- Calculates the median value for each column.
- Subtracts value for each column for each BCD.
- Updates the bcds in input list.
(2) bcd_time_filter.pro
- Calculates median for each pixel for the data set to derive
pixel-to-pixel additive correction (ignoring source and bad pixels).
The procedure derives a one correction for the entire input data set
(only one time correction). If used for a large data set, you may
want to divide the data up into multiple sets in time order.
- Subtracts value from each pixel for each BCD.
- Updates the bcds in input list.
Download the software
tgz package of README plus two procedures
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