# uvot_fluxes_wget.pl vrs. 2012-06-15 fem at 131030d21h55m18s890182usUT
# /Home/eud/uvot_tdrss/perl/uvot_fluxes_wget.pl -seq=00020313001 -use_uvot -rebin -plot_mag -sens_corr -search_src_reg -wrk_dir=/local/home/khamseen/khamseen10/uvot_tdrss/uvot_lc -web -useprev -zp_2011 -search_src_reg -gamma=1.0 -use_filter_wtd=white v b u
# Current directory: /local/home/khamseen/khamseen10/uvot_tdrss/uvot_lc
# ========= unknown GRB ===================
Used archived BAT position of 200.53200 48.00600
Reference: GCN_FOM_Notice_Wed_30_Oct_13_10:31:41_UT
The position is (13:22:07.68, +48:00:21.6)
Using source region:
# Region file format: DS9 version 3.0
# uvot_fluxes.pl bat
global font="helvetica 12 bold" select=1 edit=1 move=1 delete=1 include=1 fixed=0 source=1
fk5;circle(200.532,+48.006,3") # color=red dash=0
Region file centered at (200.532,+48.006), which is (13:22:07.68, +48:00:21.6)
Made source region file with 5" aper with name uvot_flux_src5.reg
Coincidence losses are calculated using a 5" aperture.
Exposure times (t_exp) have NOT been corrected for coinc. loss, but rates and mags have been.
The no. of background pixels has been corrected by the ratio of coincidence loss corrections in the source and background regions.
The errors have been adjusted to account for the binomial distribution of counts at large rates.
A table entry starting with # is an exposure with no aspect solution.
A table entry starting with ! has no pixels in either source or background region.
A table entry starting with % is unreliable because it is not well inside the image.
Upper limits in tables give the 0.9987 confidence limit using Bayesian analysis for detection taking the observed counts into account.
Upper limits in plots give the 0.9772 confidence limit using Bayesian analysis.
Weighted rates in tables (wtd_rate) combine rates from different exposures weighted by the expected source rate divided by the background rate
The source is assumed to produce the same magnitude in all filters.
The source is assumed to decay as t**(-1.0), and the rate is normalized so that the white filter produces 1 cps at 1000 sec.
The Rebinned Data for All_files combine rates from different exposures weighted by the expected rate divided by the observed sigma squared.
A plot of these data is stored in uvot_fluxes_wtd_date.ps and .gif.
A zero point of 20.29 is adopted for weighting rates.
*** Since no accurate position is available, set rates to 0. and compute ULs based on expected background in source aperture.
Because there are many possible positions for a source, the confidence levels should be increased for upper limits.
Using the ratio of the BAT region and the aperture of 3600.0,
3 sigma should become about 5.1 sigma and 2 sigma should become about 4.5 sigma.
Accordingly confidence limits in the tables have been adjusted from 0.9987 to 0.99999964.
No adjustment has been made for the confidence limits for the rebinned data or the plots.
Subtract UTCF of -11.1961 from trigger time of 404782248.58 in BAT summary file
# ============ Reading file sw00020313001uuu_sk.img ================
Long-term sensitivity correction is 0.090 at 404821924
The processing date in extension 0 is: 2013-10-30T21:37:18
The trigger time is: 404782259.7761. The reference is BAT GRB summary file
Using zero point of 18.430 for filter U
Use aperture correction of 1.100 based on aperture of 3.00
Using background region based on sources found in extension 3:
# Region file format: DS9 version 3.0
global color=red font="helvetica 10 normal" select=1 edit=1 move=1 delete=1 include=1 fixed=0 source
fk5;circle(200.532,+48.006,25")
fk5;-circle(200.532,+48.006,12.5")
Ext Exposure t-trig coinc t_exp src pix bkg pix net_rate +/- mag UL sum_rate +/- mag UL sumexp wtd_rate +/- mag wt/t
1 uu404821923I 39663.8 0.99 301.3 170.9 112 8763 5832 0.000 0.048 99.00 20.0 0.0000 0.0483 99.00 20.0 301 0.000 10.656 99.00 0.008
2 uu404828785I 46525.4 0.98 37.2 46.4 112 2583 5852 0.000 0.215 99.00 18.3 0.0000 0.0489 99.00 19.9 338 0.000 10.465 99.00 0.007
3 uu404833039I 50779.8 0.99 319.3 180.6 116 8322 5868 0.000 0.045 99.00 20.0 0.0000 0.0333 99.00 20.4 658 0.000 8.078 99.00 0.007
4 uu404844100I 61840.6 0.99 277.4 108.5 112 5775 5832 0.000 0.042 99.00 20.1 0.0000 0.0266 99.00 20.6 935 0.000 7.066 99.00 0.007
Sum (T+ 39664 to 62122): 493.1 493.1 (est. in src region) SNR_unwtd_sum: 0.00 0.999999638888889 signif. UL: 20.60
0 935 404832717 50457.2 11665.2 -10793.4 0.0000 0.0266 99.000 99.000 -99.000
Total wtd_rate (for all exposures so far): 0.000 +/- 6.999 snr: 0.0 mag: 99.00 UL: 14.55
Rebinned Data for sw00020313001uuu_sk.img using a zero point of 18.430:
No Exposure t-avg + / - net_rate +/- mag +/- t-avg sum_rate +/- mag +/- UL3
0 927 50469.6 11652.8 -10805.7 0.0000 0.0266 99.00 99.00 50469.6 0.0000 0.0266 99.00 99.00 21.10
The data range from T+39663.8 s (0.46 d) to T+62122.4 s (0.72 d)
Wrote uvot_fluxes_131030d21h55m18s890182usUT.qdp
Wrote uvot_fluxes_131030d21h55m18s890182usUT.gif
Wrote uvot_fluxes_131030d21h55m18s890182usUT.ps
Wrote uvot_fluxes_131030d21h55m18s890182usUT_vis.qdp
Wrote uvot_fluxes_131030d21h55m18s890182usUT_uv.qdp
Wrote uvot_fluxes_131030d21h55m18s890182usUT_vis.gif
Wrote uvot_fluxes_131030d21h55m18s890182usUT_vis.ps
# ================ Make Light Curve for Weighted Filters ==========
Use the following filters with indicated color corrections (mags):
u (0) , white (0) , b (0) , v (0) ,
Rebinned Data for All_files using a zero point of 20.290:
No Exposure t-avg + / - net_rate +/- mag +/- t-avg sum_rate +/- mag +/- UL3
0 0.00361 48570.4 13552.0 -8906.6 0.0000 0.1455 99.00 99.00 48570.4 0.0000 0.1455 99.00 99.00 21.11
The data range from T+39663.8 s (0.46 d) to T+62122.4 s (0.72 d)
Wrote uvot_fluxes_wtd_131030d21h55m18s890182usUT.qdp
Wrote uvot_fluxes_wtd_131030d21h55m18s890182usUT.gif
Wrote uvot_fluxes_wtd_131030d21h55m18s890182usUT.ps
Normal end of uvot_fluxes_wget.pl vrs. 2012-06-15 fem