SWIMS Imaging Data Reduction Pipeline, written in Python, processes SWSB*/SWSR* FITS data to produce a final stacked (and mosaicked) image in a standard procedure.
File | Contents |
swsred_20210131.tgz | Python core scripts (swsred/*py) and configuration/utility files |
&ref(): File not found: "swsred_calib_bpm_20210131.tgz" at page "Data_Reduction/Imaging_Data_Reduction/material"; | Bad pixel mask files |
&ref(): File not found: "swsred_calib_mosaic_20210131.tgz" at page "Data_Reduction/Imaging_Data_Reduction/material"; | Mosaic parameter files |
&ref(): File not found: "swsred_calib_flat_s18a_20210131.tgz" at page "Data_Reduction/Imaging_Data_Reduction/material"; | Flat files for S18A data |
&ref(): File not found: "swsred_calib_flat_s18b_20210131.tgz" at page "Data_Reduction/Imaging_Data_Reduction/material"; | Flat files for S18B data |
&ref(): File not found: "swsred_calib_flat_s20b_20210131.tgz" at page "Data_Reduction/Imaging_Data_Reduction/material"; | Flat files for S20B data |
Package | Tested version | |
Python | 2.7.17 | 3.7.7 |
astropy | 2.0.9 | 4.0 |
numpy | 1.16.6 | 1.18.1 |
scipy | 1.2.1 | 1.4.1 |
matplotlib | 2.2.3 | 3.1.3 |
sextractor | 2.19.5 | 2.19.5 |
scamp | 2.7.8 | 2.7.8 |
swarp | 2.38.0 | 2.38.0 |
Also, Internet connection is required during reducing data to access Pan-STARRS/2MASS catalogs.
% cd SWSRED_DIRECTORY % tar xvf swsred_20200501.tgz % tar xvf swsred_calib_20200501.tgz
% export PYTHONPATH="SWSRED_DIRECTORY:${PYTHONPATH}
Please send your bug reports or questions to konishi__at__ioa.s.u-tokyo.ac.jp.