LST+MAGIC

Proposed quality (multiple possible per date if needed): good , medium , bad

TBC : to be confirmed

Date	Runs LST	Runs MAGIC	Telescopes	Quality	Comments
2022-10-19	9740, 9741, 9742, 9743, 9744, 9745	2005868-2005873	L1M2	medium (moon)+?	moon + TBC
2022-10-20	9786, 9787, 9788, 9789	2005912-2005915	L1M2	good/medium +?	mix dark/moon + TBC
2022-10-21	9817, 9818, 9819, 9820, 9821, 9822, 9823	2005952-2005958	L1M2	good+?	TBC
2022-10-24	9874, 9875, 9876, 9877	2006022-2006025	L1M2	good+?	TBC
2022-10-28	9976, 9977, 9978	2006159-2006162	L1M2	good+?	TBC
2022-11-16	10624, 10625, 10626, 10627, 10628, 10629	2006571-2006575	L1M12	medium (moon)+?	moon + TBC
2022-11-20	10905, 10906, 10907	2006706-2006710	L1M2	good+?	TBC
2022-11-25	11044, 11045, 11046, 11047	2006927-2006930	L1M2	good+?	TBC
2023-03-25	12462, 12463, 12464	5106992-5106994	L1M12	bad	e.g. Calima (dust = xxµg/m³)
2023-03-26	12485, 12486, 12487, 12488, 12489	5107035-5107038	L1M12	bad	TBC
2023-03-29	12566	5107128	L1M12	bad	TBC
2023-03-30	12590, 12591, 12592, 12593, 12594	5107139-5107143	L1M12	bad	TBC
2023-04-19	missing	in	spreadsheet
2023-04-20	12801, 12802, 12803, 12804, 12805, 12806	5107463-5107467	L1M12	good+?	TBC

Preliminary performance benchmark

Using MC data from /fefs/aswg/LST1MAGIC/mc/special/20230425/DL1Stereo/ST0316A/NSB2.124/ (semi-automatic processing of LST+MAGIC mc by Julian).

Keep one file per node (as already merged) of diffuse gammas and protons for cut optimisation and sensitivity curves and retrain RFs using the standard settings and the remaining data.

-> event distributions may not be fairly distributed along pointings.

Cut optimisation :

- Re-normalise MC from the simulated E^-2 power law to:

 - For point source gamma : Crab (CRAB_HEGRA in pyirf.spectral) or G106 tail spectrum (rescaled times 100 to avoid numerical issues) -- should be a secondary for the flux sensitivity
 - For protons : IRFDOC_PROTON_SPECTRUM or PDG_ALL_PARTICLE (from pyirf.spectral)
 - For electrons : use gamma diffuse since no dedicated simu available, normalise to IRFDOC_ELECTRON_SPECTRUM in pyirf.spectral

- Find angular and gammaness cut for optimal sensitivity

 - Using all proton with offset to the center of the fov of less than 1 degree -> increase available statistic and should be valid as long as the proton acceptance is roughly uniform in this region
 - exploring te cut grid : 
     THETA_CUT_MIN = 0.0125
     THETA_CUT_MAX = 0.3
     THETA_CUT_STEP = 0.0125
     GH_CUT_MIN = 0.4
     GH_CUT_MAX = 1
     GH_CUT_STEP = 0.005