Search found 3 matches
- Mon May 22, 2023 8:42 am
- Forum: Data analysis
- Topic: How to derive flux upper limit
- Replies: 1
- Views: 27894
Re: How to derive flux upper limit
With the task apetool, one could create a flux limit map corresponding to a likelihood threshold (e.g., probability < 4e-6) with a given background map. Note that the apetool result is given in terms of minimum photon counts required by the threshold. It can be converted to flux adopting an ECF. The...
- Thu Dec 01, 2022 2:17 pm
- Forum: evatt
- Topic: How to apply the astrometric corrections to the event files ?
- Replies: 3
- Views: 29296
Re: How to apply the astrometric corrections to the event files ?
Yes, the first step is to correct the attitude table. Please see an example below: ftcopy "300007/fm00_300007_120_EventList_001_c001.fits[2][col TIME,RA=RA-0.001389444,DEC=DEC+0.001171111,ROLL]" cor_fm00_300007_120_EventList_001_c001.fits clobber=yes evatt EVENTFILE=cor_fm00_300007_120_Eve...
- Tue Feb 22, 2022 1:12 pm
- Forum: evtool
- Topic: How to remove the bad events ?
- Replies: 2
- Views: 27518
Re: How to remove the bad events ?
Such events do not exist in the calibrated event files. The corresponding exposure time sections are excluded from the good time intervals. So no additional treatment about them is needed. If you plot the image and the exposure map, you can see in such regions the image is relatively darker and the ...