Difference between revisions of "Analysis A. Aguasca-Cabot lstchain v0.8.X"

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=== Alpha plot ===
 
=== Alpha plot ===
* Filters in EventSelector applied:
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* Filters in EventSelector applied: None
 
[[File:Alpha RSOph v0.8.4.png|600px]]
 
[[File:Alpha RSOph v0.8.4.png|600px]]
  
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=== Light curve results ===
 
=== Light curve results ===
 
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<div><ul>
 +
<li style="display: inline-block;"> [[File:Daywise-LS-RSOph-v0.8.X.png|thumb|none|800px|Day-wise light curve]] </li>
 +
<li style="display: inline-block;"> [[File:Runwise-LC-RSOph-v0.8.X.png|thumb|none|800px|Day- and run-wise light curve]] </li>
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</ul></div>
  
 
= Crab Check =
 
= Crab Check =
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== Spectral results ==
 
== Spectral results ==
[[File:SED Crab v0.8.X.png]]
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[[File:SED Crab v0.8.X.png|600px]]

Latest revision as of 18:03, 28 February 2022

Overview[edit]

  • Source-dependent analysis using LSTCHAIN v0.8.4 and LSTCHAIN v0.8.2 for stage DL0 to DL1 using lstMCpipe
  • Cleaning method tail cut 84 and dynamic cleaning. Also, tuned NSB and PSF.
  • Observations used in the analysis: 5580-5584, 5630-5639 and 5696-5704.

Monte Carlo information[edit]

  • Link to MC files used:
- Particle types: gamma off0.4deg, proton
- ZD (deg): 40
- AZ (deg): 180
- Other information: DL1 MC files are produced with lstMCpipe v0.5.1, but using LSTCHAIN v0.8.2. Link to DL0 MC files used:
/fefs/aswg/data/mc/DL0/20200629_prod5_trans_80/{particle}/zenith_40deg/south_pointing

DL1 data[edit]

  • LSTCHAIN v0.8.4
- Source-dependent parameters added using script `lstchain_add_source_dependent_parameters.py`.
- Dynamic cleaning applied using srcipt `lstchain_dl1ab.py`.
 "dynamic_cleaning": {
   "apply": true,
   "threshold": 267,
   "fraction_cleaning_intensity": 0.03
 }

Real data[edit]

  • Original DL1a files
/fefs/aswg/data/real/DL1/{20210809,20210810,20210812}/v0.7.3/tailcut84/dl1_LST-1.Run0XXXX.XXXX.h5

MC data[edit]

  • Tuned NSB
- MC: gamma_40deg_180deg_run1000___cta-prod5-lapalma_4LSTs_MAGIC_desert-2158m_mono_off0.4.simtel.gz
- DL1a run: /fefs/aswg/data/real/DL1/20210809/v0.7.3/tailcut84/dl1_LST-1.Run05584.0000.h5
   "increase_nsb": true,
   "extra_noise_in_dim_pixels": 0.599,
   "extra_bias_in_dim_pixels": 0.225,
   "transition_charge": 8,
   "extra_noise_in_bright_pixels": 0.112,
  • Tunned PSF
   "increase_psf": true,
   "smeared_light_fraction": 0.175

  • Original DL1a files
/fefs/aswg/workspace/arnau.aguasca/Analysis/results/MC/lstMCpipe/DL1/20200629_prod5_trans_80/{particle}/{zenith}/{azimuth}/
/{if gamma: off_0.4deg}/20220131_v0.8.2_prod5_trans_80_zen40deg_dynamic_cleaning

Random forest[edit]

  • LSTCHAIN v0.8.4
  • Source-dependent, dispnorm
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/XXXXXXXXX

DL1 to DL2 data[edit]

  • LSTCHAIN v0.8.4
  • Config file
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/XXXXXXXXX

DL3 data selection[edit]

  • Quality cuts
 "EventSelector": {
   "filters": {
     "intensity": [50, Infinity],
     "width": [0, Infinity],
     "length": [0, Infinity],
     "r": [0, 1],
     "wl": [0.1, 1],
     "leakage_intensity_width_2": [0, 0.2]
   }
 },
 "DL3FixedCuts": {
   "fixed_gh_cut": 0.7,
   "fixed_alpha_cut": 15,
   "allowed_tels": [1]
 }

High-level analysis[edit]

DL2 to DL3 stage and IRF production performed using Seiya's fork of LSTCHAIN. Repository used: https://github.com/aaguasca/cta-lstchain

  • IRF: point-like, single-offset
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/XXXX
  • Produced DL3 files
/fefs/aswg/workspace/arnau.aguasca/XXXX

Analysis results[edit]

  • High level analysis performed with gammapy-v0.18.2

Alpha plot[edit]

  • Filters in EventSelector applied: None

Alpha RSOph v0.8.4.png

Spectral results[edit]

SED RSOph 1643846999.521488.png

Light curve results[edit]

  • Day-wise light curve
  • Day- and run-wise light curve

Crab Check[edit]

Data reduction Specifications[edit]

  • DL1 to DL3 specifications
  • High-level specifications

Spectral results[edit]

SED Crab v0.8.X.png