9/3 2014 j_ima_iros Logic

j_ima_iros search unknown source

New	Old  Line numbers i j_ima_iros_work2.c
270315 211014
1978	1958    Loop over energies
	      for (eeuser=backproj->ee_basic; eeuser<sh->numShds; eeuser++) {

2090	2067    Loop over found sources starts.
	            for (allsrc=backproj->backmodels; allsrc<kmax; allsrc++) {
2213	2188          Search for bursts in light curves corresponding to the
        	       sources found by 'j_ima_iros'. (TslBurstChk)
            	}
2296	2264    Loop over found sources ends.

2325	2293    Loop over preset sources starts.
	            for (psrc=0; psrc<backproj->preset_src; psrc++) {
        	       Define sourceID-numbers: kmax to logger->N_SRC2
	     		(presrc = backproj->backmodels + backproj->preset_src_N_SRC2[psrc])
2605	2558          Search for bursts in light curves corresponding to the
        	       user defined sources. (TslBurstChk)
2701	2685       }
2751	2685    Loop over preset sources ends.

2768	2702    Search for bursts in detector light curve.
        	 Define special sourceID number: 0
2841	2773    Search for bursts in the 'global' light curve. (TslABurstChk)

2997	2910    Loop over edge sources start
2997	2924       for (ej=1; ej<9; ej++) {
        	       Define special sourceID-numbers: 90 - 97
3166	3083          Search for bursts in the 'edge' light curves. (TslBurstChk)
3246	3158       }

3337	3249    End of eeuser-loop (starts in 1955)

3366	3278    Call 'summary_p'.

	            Print summary of the source finding results from j_ima_iros.

	            Sort any burst detections according to their ocurrence time
        	    and their significance. For each burst period the trigger
	            with the highest significance is selected by 'summary_p' as
        	    corresponding to the most likely source.

	            Burst triggers appearing with the highest significance in a
        	    light curve from a specific source are accepted as
	            originating from that source.

	            Burst triggers appearing with the highest significance in
        	    the global (detector-) light curve or in one of the 8 'edge'
	            light curves may come from an unknown source or be the
        	    result of a Solar/magnetospheric disturbance.


	         SEARCH FOR UNKNOWN BURST SOURCES
        	 In case we find bursts in the global light curve for which there
	         is no identified source we go through the following sequence:

3433	3345    Loop over burst periods (ibu)
        	    For each burst period:
3452	3364       Loop over energies (iee)
        	       For each energy band for which a burst trigger was
             		recorded during the summary_p analysis
3505	3417          Extract a shadowgram from the burst period
        	       ['fill_burst_shd']
3626	3538          Backproject this shadowgram ['j_fitprep'] to form a sky
        	       image.
3660	3578          Find dominating source in the image
*****
	               Check new candidate against the full list of already
        	       analyzed sources 'found', 'user' and 'dominating'.
3718	3660          Add new source to this list if not seen previously.

3769	3673       End of loop over energies
3770	3674    End of loop over burst detections

3790	3694    Begin new loop over energies
3797	3701       Loop over 'dominating' sources
3835	3739          Call 'final_fit' to set up pif-map for this source
3868	3772          Call 'initPIF_LC'



4103	3997       End loop over dominating sources
4110	4004    End loop over energies

****************************************************************

4123-4139	Print full list of extra burst detections (?)

4146-4172	Print shorthand burst parameters for all bursts

4174-4250	Mini images skipped

4260-4435	Output selected burst light curves to regfile (?) (P-marked)

4441-4616	Output data to regfil (?) (Q-marked)