RS Oph Analysis Mab Bernardos v09X
Revision as of 15:15, 28 March 2022 by Misabelber (talk | contribs)
Contents
Overview
- Source independent analysis using lstchain v0.9.4
- Cleaning method: tailcut84 + pedestal cleaning + dynamic cleaning.
- Observations: 20210809(Run5580-5584), 20210810(Run5630-5639), 20210812(Run 5696-5704)
Monte Carlo information
- Particle types: point gamma, proton
- Zenith 40deg, Azimuth 180 deg
- Path to MC DL1 data:
"/fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/[gamma, gamma-diffuse, proton, electron]/zenith_40deg/south_pointing/0220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1"
- Path to trained models:
"/fefs/aswg/data/models/20200629_prod5_trans_80/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1"
- Path to IRFs:
"/fefs/aswg/data/mc/IRF/20200629_prod5_trans_80/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1/off0.4deg"
- Path to config file:
"/fefs/aswg/data/mc/IRF/20200629_prod5_trans_80/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1/off0.4deg/lstchain_config_NSBtuning.json"
- NSB is tuned to RS Oph observations:
- Tuned NSB
"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,
- Tuned PSF
"increase_psf": true, "smeared_light_fraction": 0.175
Event selection
Standard lstchain cuts were used:
"intensity": [100, Infinity], "width": [0, Infinity], "length": [0, Infinity], "r": [0, 1], "wl": [0.1, 1], "leakage_intensity_width_2": [0, 0.2], "event_type": [32, 32]
"global_gh_cut": 0.7, "gh_efficiency": 0.9, "global_alpha_cut": 10, "global_theta_cut": 0.2, "theta_containment": 0.68, "allowed_tels": [1]
First three nights (20210809, 20210810, 20210812) combined
- Theta2 plots
- Full energy range
- Per energy bin
- SED
- Best fit spectral parameters:
- Lightcurve