Difference between revisions of "RS Oph Analysis Yukiho 20220223"

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(First three nights (20210809, 10 and 12) combined)
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* alpha plot
 
* alpha plot
 
[[File:alpha-plot_20210809_gcut09_acut10_scut50.png|400px]]
 
[[File:alpha-plot_20210809_gcut09_acut10_scut50.png|400px]]
 +
* SED
 +
[[File:SED_202108009_erange40-1000_8bins.png|400px]]
 +
 +
== 20210810 ==
 +
* alpha plot
 +
[[File:alpha-plot_20210810_gcut09_acut10_scut50.png|400px]]
 +
* SED
 +
[[File:SED_202108009_erange40-1000_8bins.png|400px]]
 +
 +
== 20210812 ==
 +
* alpha plot
 +
[[File:alpha-plot_20210812_gcut09_acut10_scut50.png|400px]]
 
* SED
 
* SED
 
[[File:SED_202108009_erange40-1000_8bins.png|400px]]
 
[[File:SED_202108009_erange40-1000_8bins.png|400px]]

Revision as of 11:23, 23 February 2022

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

Alpha-plot AllNights gcut09.png

  • SED

SED AllRuns erange40-1000 8bins.png

  • Light curve

LightCurve erange100-1000 Nightwise.png

20210809

  • alpha plot

Alpha-plot 20210809 gcut09 acut10 scut50.png

  • SED

SED 202108009 erange40-1000 8bins.png

20210810

  • alpha plot

Alpha-plot 20210810 gcut09 acut10 scut50.png

  • SED

SED 202108009 erange40-1000 8bins.png

20210812

  • alpha plot

Alpha-plot 20210812 gcut09 acut10 scut50.png

  • SED

SED 202108009 erange40-1000 8bins.png