Difference between revisions of "RS Oph Analysis Yukiho 20220223"
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* SED | * SED | ||
[[File:SED_20210812_erange40-1000_8bins.png|400px]] | [[File:SED_20210812_erange40-1000_8bins.png|400px]] | ||
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| + | == After the moon break (20210829/30, 20210901/02) == | ||
| + | * 20210829, alpha plot | ||
| + | [[File:alpha-plot_20210829_gcut09_acut10_scut50.png|400px]] | ||
Revision as of 11:33, 23 February 2022
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) and 20210812(Run 5696-5704).
- 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.
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
