RS Oph Analysis Yukiho 20220223
Contents
Overview
- Source-dependent analysis using lstchain v0.7.3 for R0-DL1a and v0.7.5 above DL1a.
- Cleaning method: tailcut84 + pedestal cleaning + dynamic cleaning.
- Observations: 20210809(Run5580-5584), 20210810(Run5630-5639), 20210812(Run 5696-5704), 20210829(Run5890-5893), 20210830(Run5912-5917), 20210901(Run5942-5945) and 20210902(Run5970-5973)
- For the late observations after 20210829, only analysis with v0.7.3 (namely without dynamic cleaning and MC tuning) is performed.
Monte Carlo information
- Particle types: point gamma, proton
- Zenith 40deg, Azimuth 180 deg
- NSB is tuned to the RS Oph observations. PSF is tuned as well.
Event selection
- intensity > 50
- gammaness > 0.9
- alpha < 10 deg
- leakage < 0.2
First three nights (20210809, 10 and 12) combined
- alpha plot
- SED
- Light curve
20210809
- alpha plot
- SED
20210810
- alpha plot
- SED
20210812
- alpha plot
- SED
After the moon break (20210829/30, 20210901/02)
- 20210829, alpha plot
- 20210830, alpha plot
- 20210901, alpha plot
- 20210902, alpha plot