Difference between revisions of "RS Oph Analysis Yukiho 20220223"
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*Source-dependent analysis using lstchain v0.7.3 for R0-DL1a and v0.7.5 above DL1a. | *Source-dependent analysis using lstchain v0.7.3 for R0-DL1a and v0.7.5 above DL1a. | ||
*Cleaning method: tailcut84 + pedestal cleaning + dynamic cleaning. | *Cleaning method: tailcut84 + pedestal cleaning + dynamic cleaning. | ||
| − | *Observations: 20210809(Run5580-5584), 20210810(Run5630-5639) | + | *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 | + | * For the the data after the moon break, only analysis with v0.7.3 (namely without dynamic cleaning and MC tuning) is performed. |
== Monte Carlo information == | == Monte Carlo information == | ||
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* Zenith 40deg, Azimuth 180 deg | * Zenith 40deg, Azimuth 180 deg | ||
* NSB is tuned to the RS Oph observations. PSF is tuned as well. | * 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 == | == First three nights (20210809, 10 and 12) combined == | ||
| Line 39: | Line 45: | ||
* 20210829, alpha plot | * 20210829, alpha plot | ||
[[File:alpha-plot_20210829_gcut09_acut10_scut50.png|400px]] | [[File:alpha-plot_20210829_gcut09_acut10_scut50.png|400px]] | ||
| + | |||
| + | * 20210830, alpha plot | ||
| + | [[File:alpha-plot_20210830_gcut09_acut10_scut50.png|400px]] | ||
| + | |||
| + | * 20210901, alpha plot | ||
| + | [[File:alpha-plot_20210901_gcut09_acut10_scut50.png|400px]] | ||
| + | |||
| + | * 20210902, alpha plot | ||
| + | [[File:alpha-plot_20210902_gcut09_acut10_scut50.png|400px]] | ||
Latest revision as of 11:42, 23 February 2022
Contents
Overview[edit]
- 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 the data after the moon break, only analysis with v0.7.3 (namely without dynamic cleaning and MC tuning) is performed.
Monte Carlo information[edit]
- 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[edit]
- intensity > 50
- gammaness > 0.9
- alpha < 10 deg
- leakage < 0.2
First three nights (20210809, 10 and 12) combined[edit]
- alpha plot
- SED
- Light curve
20210809[edit]
- alpha plot
- SED
20210810[edit]
- alpha plot
- SED
20210812[edit]
- alpha plot
- SED
After the moon break (20210829/30, 20210901/02)[edit]
- 20210829, alpha plot
- 20210830, alpha plot
- 20210901, alpha plot
- 20210902, alpha plot
