RS Oph Analysis Yukiho v09X

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Overview

• Source-dependent approach using lstchain v0.9.4
• Cleaning method: tailcut84 + pedestal cleaning + dynamic cleaning.

Monte Carlo information

• Zenith 40deg, Azimuth 180 deg
• NSB and PSF tuned for RS Oph observations:

   "increase_nsb": true,
   "extra_noise_in_dim_pixels": 0.6,
   "extra_bias_in_dim_pixels": 0.269,
   "transition_charge": 8,
   "extra_noise_in_bright_pixels": 0.566,
   "increase_psf": true,
   "smeared_light_fraction": 0.175

• Path to MC DL1 data:

   "/fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/gamma/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1/off0.4deg/"
   "/fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/proton/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1"

Analysis settings

Event selection

     "intensity": [50, Infinity],
     "width": [0, Infinity],
     "length": [0, Infinity],
     "wl": [0.01, 1],
     "r": [0, 1],
     "leakage_intensity_width_2": [0, 0.2]

Cuts

• arbitrarily chosen to keep S/N ~ 5% for RS Oph observations

   "fixed_gh_cut": 0.9,
   "fixed_alpha_cut": 10

Analysis results

Three nights (9, 10 and 12 of August 2021) combined

• SED

File:SED RSOph v09 AllNights Yukiho.pdf SED