python photo_plot.py Drout_list_ZOMG.fits -pdf BB_M31_Drout.pdf --gal M31 python photo_plot.py Drout_list_ZOMG.fits -pdf BB_M33_Drout.pdf --gal M33
ran Drout_list.py on Drout_list_init.tsv ->Drout_list_FINAL.fits/tsv ran final_check.py on Drout_list_FINAL.fits to see if any remaining matches in Mould/McQuinn IRAS photometry matches to 2MASS things
wrote mag2flux.py
uses: http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec4_4c.html#wappco for aperture correction
run final_check.py -> GENERATES Drout_list_ZOMG.tsv/fits
python photo_plot.py photometry_ZOMG.tsv -pdf allSED.pdf python photo_plot.py photometry_ZOMG.tsv -pdf M31A_SED.pdf --idlist M31A_IDs.list python photo_plot.py photometry_ZOMG.tsv -pdf M31B_SED.pdf --idlist M31B_IDs.list
#in tables/ table_converter.py
python LBV_db.py tables/*.fits --master tables/MasseyXL.fit python LBV_query.py catalog.json python LBV_photo.py catalog.json -2MASS dMASStables -WISE dWISEtables #python LBV_photo_corr.py
python LBV_SEDplot.py photometry.fits #python LBV_html.py photometry.fits -o LBV_M31_photo.html
python LBV_specmatch.py -> generates .list files of IDs
##M31 see readme in m312013 python LBV_SEDspec.py photometry_corr_FINAL.tsv M31A_FINAL.list -pdf BB_spec_M31A.pdf python LBV_SEDspec.py photometry_corr_FINAL.tsv M31B_FINAL.list -pdf BB_spec_M31B.pdf
---> stitch_spec.py --list M31A_FINAL.list --outdir M312013/M31A/ stitch_spec.py --list M31B_FINAL.list --outdir M312013/M31B/