Difference between revisions of "RS Oph Analysis v0.9.x AllSky"

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(Created page with "= Overview = *Source-dependent/independent analysis using LSTCHAIN v0.9.10 and v.9.14dev with last commit e5835d5ab7792cbb528118de9cebe4a60f7802a8 for the DL2 to DL3 stage (ir...")
 
 
Line 1: Line 1:
 
= Overview =
 
= Overview =
−
*Source-dependent/independent analysis using LSTCHAIN v0.9.10 and v.9.14dev with last commit e5835d5ab7792cbb528118de9cebe4a60f7802a8 for the DL2 to DL3 stage (irf interpolation). The MC production processed with LSTOSA v0.8.2 using LSTCHAIN v0.9.6
+
*Source-independent analysis using LSTCHAIN v0.9.10 (DL1->DL2) and LSTCHAIN v0.9.14.dev79+g6a03d48.d20230508 (DL2 to DL3 stage (irf interpolation)). The MC production processed with lstMCpipe v0.9.0 using LSTCHAIN v0.9.9.
 +
 
 +
*Source-dependent analysis using LSTCHAIN v0.9.14.dev139+g90d0450 (DL1->DL2) and LSTCHAIN v0.9.14.dev79+g6a03d48.d20230508 (DL2 to DL3 stage (irf interpolation)). The MC production processed with lstMCpipe v0.9.1.dev14+gfb9c7c using LSTCHAIN v0.9.14.dev139+g90d0450.
 +
 
  
 
*Cleaning method tail cut 84 and dynamic cleaning. Also, the MC files are tuned to match the NSB in the FoV.
 
*Cleaning method tail cut 84 and dynamic cleaning. Also, the MC files are tuned to match the NSB in the FoV.
−
*Observations used in the analysis:
+
*Observations used in the analysis: 5580->5584, 5630->5639, 5696->5704, 5890->5893, 5912->5917, 5942->5945, 5970->5973.
 +
 
  
 
== Monte Carlo information ==
 
== Monte Carlo information ==
 
* AllSky MC prodution.
 
* AllSky MC prodution.
−
* Link to MC files used: /fefs/aswg/data/mc/DL1/AllSky/20221108_galsource_min_413_tuned_nsb/...  
+
* Link to MC files used (srcind): /fefs/aswg/data/mc/DL1/AllSky/20221108_galsource_min_413_tuned_nsb/...  
 
:- Particle types: gamma diffuse and protons
 
:- Particle types: gamma diffuse and protons
 
:- MC prod (deg): 20221108_galsource_min_413_tuned_nsb
 
:- MC prod (deg): 20221108_galsource_min_413_tuned_nsb
Line 13: Line 17:
 
:- Other information: MC production through PR in lstMCpipe Github webpage (https://github.com/cta-observatory/lstmcpipe/tree/master/production_configs/20221108_galsource_min_413_tuned_nsb)
 
:- Other information: MC production through PR in lstMCpipe Github webpage (https://github.com/cta-observatory/lstmcpipe/tree/master/production_configs/20221108_galsource_min_413_tuned_nsb)
 
:- MC files are tuned to match the NSB in the FoV.
 
:- MC files are tuned to match the NSB in the FoV.
 +
 +
* Link to MC files used (srcdep): /fefs/aswg/workspace/MC_data_simlink/DL1/AllSky/20230301_srcdep_galsource_min_413_tuned_nsb/...
 +
:- Particle types: gamma diffuse and protons
 +
:- MC prod (deg): 20230301_srcdep_galsource_min_413_tuned_nsb
 +
:- Dec band (deg): dec_min_431
 +
:- Other information: MC processed by Arnau (config files in path: /fefs/aswg/workspace/arnau.aguasca/scripts/lstMCpipe/v0.10.X/20230301_srcdep_galsource_min_413_tuned_nsb/)
 +
:- MC files are tuned to match the NSB in the FoV.
 +
  
 
== DL1 data ==  
 
== DL1 data ==  
−
* Processed with LSTOSA using LSTCHAIN v0.9.6.
+
* Processed with LSTOSA using LSTCHAIN v0.9.2.
 
:- Dynamic cleaning and tail cut cleaning with pedestal threshold applied by the the standard parameters using pipeline LSTOSA.
 
:- Dynamic cleaning and tail cut cleaning with pedestal threshold applied by the the standard parameters using pipeline LSTOSA.
  
Line 38: Line 50:
 
   }
 
   }
  
−
* Original DL1a files (processed up to DL1 by LSTOSA using LSTCHAIN v0.9.2)
+
* Original DL1a files (processed up to DL1 by LSTOSA using LSTCHAIN v0.9.2).
 
  /fefs/aswg/data/real/DL1/{}/v0.9/tailcut84/dl1_LST-1.RunXXXXX.XXXX.h5
 
  /fefs/aswg/data/real/DL1/{}/v0.9/tailcut84/dl1_LST-1.RunXXXXX.XXXX.h5
  
Line 46: Line 58:
  
 
     "increase_nsb": true,
 
     "increase_nsb": true,
−
     "extra_noise_in_dim_pixels": 0.937,
+
     "extra_noise_in_dim_pixels": 0.84,
−
     "extra_bias_in_dim_pixels": 0.323,
+
     "extra_bias_in_dim_pixels": 0.326,
 
     "transition_charge": 8,
 
     "transition_charge": 8,
−
     "extra_noise_in_bright_pixels": 1.041,
+
     "extra_noise_in_bright_pixels": 1.064,
  
  
−
* Original DL1a files
+
* Original DL1a files (srcind)
 
  /fefs/aswg/data/mc/DL1/AllSky/20221108_galsource_min_413_tuned_nsb/{TrainingDataset,TestingDataset}/dec_min_413/{particle}/node...
 
  /fefs/aswg/data/mc/DL1/AllSky/20221108_galsource_min_413_tuned_nsb/{TrainingDataset,TestingDataset}/dec_min_413/{particle}/node...
 +
* Original DL1a files (srcdep)
 +
/fefs/aswg/workspace/MC_data_simlink/DL1/AllSky/20230301_srcdep_galsource_min_413_tuned_nsb/{TrainingDataset,TestingDataset}/dec_min_413/{particle}/node...
 +
  
 
== Random forest ==
 
== Random forest ==
  
 
* Disp_norm parameterisation
 
* Disp_norm parameterisation
 +
 +
*; Source-independent
 +
:- Processed with lstMCpipe using LSTCHAIN v0.9.9.
 +
:- Path:
 +
/fefs/aswg/data/mc/models/AllSky/20221108_galsource_min_413_tuned_nsb/dec_min_413/
  
 
*; Source-dependent  
 
*; Source-dependent  
−
:- LSTCHAIN v0.9.10
+
:- LSTCHAIN v0.9.14.dev139+g90d0450
 
:- Config file:
 
:- Config file:
−
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/lstchain_src_dep_tailcut84_config_dispnorm_v0.9.4.json
+
  /fefs/aswg/workspace/arnau.aguasca/scripts/lstMCpipe/v0.10.X/20230301_srcdep_galsource_min_413_tuned_nsb/lstchain_config_2023-03-01.json
 
:- path:
 
:- path:
−
  /fefs/aswg/workspace/MC_data_simlink/models/AllSky/galsource_min_413_tuned_nsb_NOpsf_srcdep/dec_min_413/
+
  /fefs/aswg/workspace/MC_data_simlink/models/AllSky/20230301_srcdep_galsource_min_413_tuned_nsb/dec_min_413/
  
−
*; Source-independent
 
−
:- Processed with lstMCpipe using LSTCHAIN v0.9.9.
 
−
:- Path:
 
−
/fefs/aswg/data/mc/models/AllSky/20221108_galsource_min_413_tuned_nsb/dec_min_413/
 
  
 
== DL1 to DL2 data ==
 
== DL1 to DL2 data ==
  
 
=== Real data ===
 
=== Real data ===
−
*; Source-dependent
+
 
 +
*; Source-independent
 
:- LSTCHAIN v0.9.10
 
:- LSTCHAIN v0.9.10
 
:- Config file:
 
:- Config file:
−
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.6/lstchain_config_srcdep_lstmcpipe_tailcut84_dispnorm_v0.9.6.json
+
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/standard_real_config_lstchain_belong_v0.10.0.json
  
−
*; Source-independent
+
*; Source-dependent
−
:- LSTCHAIN v0.9.10
+
:- LSTCHAIN v0.9.14.dev139+g90d0450
 
:- Config file:
 
:- Config file:
−
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.6/lstchain_config_lstmcpipe_tailcut84_dispnorm_v0.9.6.json
+
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.13/standard_real_srcdep_config_lstchain_belong_extra_srcdep_params.json
 +
 
  
 
=== MC data ===
 
=== MC data ===
 +
 +
*; Source-independent
 +
:- Processed with lstMCpipe using LSTCHAIN v0.9.9.
 +
:- Config file:
 +
https://github.com/cta-observatory/lstmcpipe/blob/master/production_configs/20221108_galsource_min_413_tuned_nsb/lstchain_config_2022-11-08.json
  
 
*; Source-dependent  
 
*; Source-dependent  
−
:- Processed with lstMCpipe using LSTCHAIN v0.9.6.
+
:- LSTCHAIN v0.9.14.dev139+g90d0450
 
:- Config file:
 
:- Config file:
−
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.4/lstchain_config_srcdep_lstmcpipe_tailcut84_dispnorm_v0.9.6.json
+
  /fefs/aswg/workspace/arnau.aguasca/scripts/lstMCpipe/v0.10.X/20230301_srcdep_galsource_min_413_tuned_nsb/lstchain_config_2023-03-01.json
  
−
*; Source-independent
+
== Quality cuts optimization for detection (srcind) ==
−
:- Processed with lstMCpipe using LSTCHAIN v0.9.6.
+
 
−
:- Config file:
+
Since the AllSky MC is a tailored production than the Fixed MC production, we cannot use high-zenith Crab observations to find the best cuts for detection. To do so, I found the best cuts (gammaness and theta) that minimise the sensitivity of MC gammas re-weightening the slope the the spectrum reported by MAGIC (Gamma = -3.7) and using OFF data from real OFF data (3 reflected OFF regions from runs 5890,5891,5892,5893, 5912,5913,5914,5915,5916,5917, 5942, 5943, 5944, 5945, 5970, 5971, 5972, 5973). I used a grid of gammaness and theta2 values. The best cuts are gammaness = 0.9 and theta2 = 0.01 deg2.
−
/fefs/aswg/data/models/AllSky/galsource_min_413_tuned_nsb/dec_min_413/lstchain_config_2022-05-23.json
+
 
 +
== Theta2 plot ==
  
−
== Quality cuts optimization ==
+
* Right after the outburst (run id <= 5704)
−
Since the AllSky MC is a tailored production than the Fixed MC production, we cannot use high-zenith Crab observations to find the best cuts.
+
[[File:Theta2 plot RSOph.pdf|400px]]
  
 +
* After moon break (run id >= 5890)
 +
[[File:Theta2 plot RSOph afterMoonBreak.pdf|400px]]
  
 
== DL3 data selection ==
 
== DL3 data selection ==
Line 115: Line 141:
 
   },
 
   },
 
   "DL3FixedCuts": {
 
   "DL3FixedCuts": {
−
    "fixed_gh_cut": 0.6,
+
     "gh_efficiency": 0.7,
−
     "gh_efficiency": 0.9,
+
     "theta_containment": 0.7,
−
    "fixed_theta_cut": 0.2,
+
     "alpha_containment": 0.7,
−
     "theta_containment": 0.68,
 
−
     "alpha_containment": 0.68,
 
 
     "allowed_tels": [1]
 
     "allowed_tels": [1]
 
   }
 
   }
  
 
== High-level analysis ==
 
== High-level analysis ==
 +
 +
*; Source-independent
 +
*:- IRF: point-like, single-offset, node interpolation.
 +
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/DL3IRF-generated-configs/config_thetaChange_int50_leak0.2_gh0.9_geff0.7_th0.2_tc0.7_a15_ac0.68.json
 +
::- Produced DL3 files
 +
/fefs/aswg/workspace/arnau.aguasca/Analysis/results/LST/real/DL3/RSOph/srcind/v0.9.14.dev79+g6a03d48.d20230508/tailcut84_dynclg_tNSBtoRSOph/AllSky_20221108_galsource_min_413_tuned_nsb_dec_min_413/int_50_lk_0.2_gh_dyn_0.7_th_dyn_0.7/interp_node/
 +
 
*; Source-dependent  
 
*; Source-dependent  
−
*:- IRF: point-like, single-offset
+
*:- IRF: point-like, single-offset, nearest node.
−
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/DL3IRF-generated-configs/config_int50_leak0.2_gh0.7_geff0.9_th0.2_tc0.68_a15_ac0.68.json
+
  /fefs/aswg/workspace/arnau.aguasca/scripts/_configs/DL3IRF-generated-configs/config_thetaChange_int50_leak0.2_gh0.9_geff0.5_th0.2_tc0.7_a15_ac0.7.json
 
::- Produced DL3 files
 
::- Produced DL3 files
 +
/fefs/aswg/workspace/arnau.aguasca/Analysis/results/LST/real/DL3/RSOph/nearest_node/srcdep/v0.9.14.dev79+g6a03d48.d20230508/tailcut84_dynclg_tNSBtoRSOph/AllSky_20230301_srcdep_galsource_min_413_tuned_nsb_dec_min_413/int50_lk0.2_geff0.5_aeff0.7/
  
−
/fefs/aswg/workspace/arnau.aguasca/Analysis/results/real/DL3/RSOph/nearest_node/...
 
  
−
*; Source-independent
+
== Analysis results src ind ==
 +
 
 +
* The srcind high-level results will be used in the paper publication.
 +
 
 +
* High-level analysis performed with gammapy-v1.0. Fitting process using the joint method in gammapy for the srcind results.
 +
 
 +
* Spectral Energy distribution
 +
 
 +
:* 20210809
 +
:[[File:LST-1MAGICHESS_SED_RSOph_20210809_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
 +
:* 20210810
 +
:[[File:LST-1MAGICHESS_SED_RSOph_20210810_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
 +
:* 20210812
 +
:[[File:LST-1MAGICHESS_SED_RSOph_20210812_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
 +
:* All data from Aug 9, 10 and 12
 +
:[[File:LST-1MAGIC_SED_RSOph_09to12_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
 +
 
 +
* Light curve
 +
 
 +
:* Above E>100 GeV (MAGIC comparison)
 +
:[[File:LST-1MAGIC_lightcurve_RSOph_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
 +
 
 +
:* Above E>250 GeV (HESS comparison)
 +
:[[File:LST-1HESS_lightcurve_RSOph_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
 +
 
 +
 
 +
== Analysis results src dep ==
 +
 
 +
* Comparison with srcind and srcdep
 +
 
 +
::* 20210809
 +
::[[File:plot_LST-1MAGICHESS_SED_RSOph_final_srcind&srcdep_comparison_20210809.pdf|400px]]
 +
::* 20210810
 +
::[[File:plot_LST-1MAGICHESS_SED_RSOph_final_srcind&srcdep_comparison_20210810.pdf|400px]]
 +
::* 20210812
 +
::[[File:plot_LST-1MAGICHESS_SED_RSOph_final_srcind&srcdep_comparison_20210812.pdf|400px]]
 +
::* All data from Aug 9, 10 and 12
 +
::[[File:plot_LST-1MAGICHESS_SED_RSOph_final_srcind&srcdep_comparison_09to12.pdf|400px]]
 +
 
 +
:* Light curve
  
−
== Analysis results ==
+
::* Above E>100 GeV (MAGIC comparison)
−
* High level analysis performed with gammapy-v0.20.1
+
::[[File:LST-1MAGIC_lightcurve_RSOph_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
  
−
=== Alpha plot ===
+
::* Above E>250 GeV (HESS comparison)
−
* Filters in EventSelector applied:
+
::[[File:LST-1HESS_lightcurve_RSOph_interp_node_srcind_v0.9.14dev_AllSkyMC.pdf|400px]]
−
  "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]
 
−
    }
 
−
  }
 

Latest revision as of 18:23, 10 August 2023

Overview[edit]

  • Source-independent analysis using LSTCHAIN v0.9.10 (DL1->DL2) and LSTCHAIN v0.9.14.dev79+g6a03d48.d20230508 (DL2 to DL3 stage (irf interpolation)). The MC production processed with lstMCpipe v0.9.0 using LSTCHAIN v0.9.9.
  • Source-dependent analysis using LSTCHAIN v0.9.14.dev139+g90d0450 (DL1->DL2) and LSTCHAIN v0.9.14.dev79+g6a03d48.d20230508 (DL2 to DL3 stage (irf interpolation)). The MC production processed with lstMCpipe v0.9.1.dev14+gfb9c7c using LSTCHAIN v0.9.14.dev139+g90d0450.


  • Cleaning method tail cut 84 and dynamic cleaning. Also, the MC files are tuned to match the NSB in the FoV.
  • Observations used in the analysis: 5580->5584, 5630->5639, 5696->5704, 5890->5893, 5912->5917, 5942->5945, 5970->5973.


Monte Carlo information[edit]

  • AllSky MC prodution.
  • Link to MC files used (srcind): /fefs/aswg/data/mc/DL1/AllSky/20221108_galsource_min_413_tuned_nsb/...
- Particle types: gamma diffuse and protons
- MC prod (deg): 20221108_galsource_min_413_tuned_nsb
- Dec band (deg): dec_min_431
- Other information: MC production through PR in lstMCpipe Github webpage (https://github.com/cta-observatory/lstmcpipe/tree/master/production_configs/20221108_galsource_min_413_tuned_nsb)
- MC files are tuned to match the NSB in the FoV.
  • Link to MC files used (srcdep): /fefs/aswg/workspace/MC_data_simlink/DL1/AllSky/20230301_srcdep_galsource_min_413_tuned_nsb/...
- Particle types: gamma diffuse and protons
- MC prod (deg): 20230301_srcdep_galsource_min_413_tuned_nsb
- Dec band (deg): dec_min_431
- Other information: MC processed by Arnau (config files in path: /fefs/aswg/workspace/arnau.aguasca/scripts/lstMCpipe/v0.10.X/20230301_srcdep_galsource_min_413_tuned_nsb/)
- MC files are tuned to match the NSB in the FoV.


DL1 data[edit]

  • Processed with LSTOSA using LSTCHAIN v0.9.2.
- Dynamic cleaning and tail cut cleaning with pedestal threshold applied by the the standard parameters using pipeline LSTOSA.
 "dynamic_cleaning": {
   "apply": true,
   "threshold": 267,
   "fraction_cleaning_intensity": 0.03
 }

Real data[edit]

  • Parameters for the tail cut cleaning with pedestal threshold
 "tailcuts_clean_with_pedestal_threshold": {
   "picture_thresh":8,
   "boundary_thresh":4,
   "sigma":2.5,
   "keep_isolated_pixels":false,
   "min_number_picture_neighbors":2,
   "use_only_main_island":false,
   "delta_time": 2
 }
  • Original DL1a files (processed up to DL1 by LSTOSA using LSTCHAIN v0.9.2).
/fefs/aswg/data/real/DL1/{}/v0.9/tailcut84/dl1_LST-1.RunXXXXX.XXXX.h5

MC data[edit]

  • Tuned NSB
   "increase_nsb": true,
   "extra_noise_in_dim_pixels": 0.84,
   "extra_bias_in_dim_pixels": 0.326,
   "transition_charge": 8,
   "extra_noise_in_bright_pixels": 1.064,


  • Original DL1a files (srcind)
/fefs/aswg/data/mc/DL1/AllSky/20221108_galsource_min_413_tuned_nsb/{TrainingDataset,TestingDataset}/dec_min_413/{particle}/node...
  • Original DL1a files (srcdep)
/fefs/aswg/workspace/MC_data_simlink/DL1/AllSky/20230301_srcdep_galsource_min_413_tuned_nsb/{TrainingDataset,TestingDataset}/dec_min_413/{particle}/node...


Random forest[edit]

  • Disp_norm parameterisation
  • Source-independent
- Processed with lstMCpipe using LSTCHAIN v0.9.9.
- Path:
/fefs/aswg/data/mc/models/AllSky/20221108_galsource_min_413_tuned_nsb/dec_min_413/
  • Source-dependent
- LSTCHAIN v0.9.14.dev139+g90d0450
- Config file:
/fefs/aswg/workspace/arnau.aguasca/scripts/lstMCpipe/v0.10.X/20230301_srcdep_galsource_min_413_tuned_nsb/lstchain_config_2023-03-01.json
- path:
/fefs/aswg/workspace/MC_data_simlink/models/AllSky/20230301_srcdep_galsource_min_413_tuned_nsb/dec_min_413/


DL1 to DL2 data[edit]

Real data[edit]

  • Source-independent
- LSTCHAIN v0.9.10
- Config file:
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/standard_real_config_lstchain_belong_v0.10.0.json
  • Source-dependent
- LSTCHAIN v0.9.14.dev139+g90d0450
- Config file:
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.13/standard_real_srcdep_config_lstchain_belong_extra_srcdep_params.json


MC data[edit]

  • Source-independent
- Processed with lstMCpipe using LSTCHAIN v0.9.9.
- Config file:
https://github.com/cta-observatory/lstmcpipe/blob/master/production_configs/20221108_galsource_min_413_tuned_nsb/lstchain_config_2022-11-08.json
  • Source-dependent
- LSTCHAIN v0.9.14.dev139+g90d0450
- Config file:
/fefs/aswg/workspace/arnau.aguasca/scripts/lstMCpipe/v0.10.X/20230301_srcdep_galsource_min_413_tuned_nsb/lstchain_config_2023-03-01.json

Quality cuts optimization for detection (srcind)[edit]

Since the AllSky MC is a tailored production than the Fixed MC production, we cannot use high-zenith Crab observations to find the best cuts for detection. To do so, I found the best cuts (gammaness and theta) that minimise the sensitivity of MC gammas re-weightening the slope the the spectrum reported by MAGIC (Gamma = -3.7) and using OFF data from real OFF data (3 reflected OFF regions from runs 5890,5891,5892,5893, 5912,5913,5914,5915,5916,5917, 5942, 5943, 5944, 5945, 5970, 5971, 5972, 5973). I used a grid of gammaness and theta2 values. The best cuts are gammaness = 0.9 and theta2 = 0.01 deg2.

Theta2 plot[edit]

  • Right after the outburst (run id <= 5704)

File:Theta2 plot RSOph.pdf

  • After moon break (run id >= 5890)

File:Theta2 plot RSOph afterMoonBreak.pdf

DL3 data selection[edit]

  • - Quality cuts
 "EventSelector": {
   "filters": {
     "intensity": [50, Infinity],
     "width": [0, Infinity],
     "length": [0, Infinity],
     "r": [0, 1],
     "wl": [0.01, 1],
     "leakage_intensity_width_2": [0, 0.2],
     "event_type" : [32, 32]
   }
 },
 "DL3FixedCuts": {
   "gh_efficiency": 0.7,
   "theta_containment": 0.7,
   "alpha_containment": 0.7,
   "allowed_tels": [1]
 }

High-level analysis[edit]

  • Source-independent
    - IRF: point-like, single-offset, node interpolation.
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/DL3IRF-generated-configs/config_thetaChange_int50_leak0.2_gh0.9_geff0.7_th0.2_tc0.7_a15_ac0.68.json
- Produced DL3 files
/fefs/aswg/workspace/arnau.aguasca/Analysis/results/LST/real/DL3/RSOph/srcind/v0.9.14.dev79+g6a03d48.d20230508/tailcut84_dynclg_tNSBtoRSOph/AllSky_20221108_galsource_min_413_tuned_nsb_dec_min_413/int_50_lk_0.2_gh_dyn_0.7_th_dyn_0.7/interp_node/
  • Source-dependent
    - IRF: point-like, single-offset, nearest node.
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/DL3IRF-generated-configs/config_thetaChange_int50_leak0.2_gh0.9_geff0.5_th0.2_tc0.7_a15_ac0.7.json
- Produced DL3 files
/fefs/aswg/workspace/arnau.aguasca/Analysis/results/LST/real/DL3/RSOph/nearest_node/srcdep/v0.9.14.dev79+g6a03d48.d20230508/tailcut84_dynclg_tNSBtoRSOph/AllSky_20230301_srcdep_galsource_min_413_tuned_nsb_dec_min_413/int50_lk0.2_geff0.5_aeff0.7/


Analysis results src ind[edit]

  • The srcind high-level results will be used in the paper publication.
  • High-level analysis performed with gammapy-v1.0. Fitting process using the joint method in gammapy for the srcind results.
  • Spectral Energy distribution
  • 20210809
File:LST-1MAGICHESS SED RSOph 20210809 interp node srcind v0.9.14dev AllSkyMC.pdf
  • 20210810
File:LST-1MAGICHESS SED RSOph 20210810 interp node srcind v0.9.14dev AllSkyMC.pdf
  • 20210812
File:LST-1MAGICHESS SED RSOph 20210812 interp node srcind v0.9.14dev AllSkyMC.pdf
  • All data from Aug 9, 10 and 12
File:LST-1MAGIC SED RSOph 09to12 interp node srcind v0.9.14dev AllSkyMC.pdf
  • Light curve
  • Above E>100 GeV (MAGIC comparison)
File:LST-1MAGIC lightcurve RSOph interp node srcind v0.9.14dev AllSkyMC.pdf
  • Above E>250 GeV (HESS comparison)
File:LST-1HESS lightcurve RSOph interp node srcind v0.9.14dev AllSkyMC.pdf


Analysis results src dep[edit]

  • Comparison with srcind and srcdep
  • 20210809
File:Plot LST-1MAGICHESS SED RSOph final srcind&srcdep comparison 20210809.pdf
  • 20210810
File:Plot LST-1MAGICHESS SED RSOph final srcind&srcdep comparison 20210810.pdf
  • 20210812
File:Plot LST-1MAGICHESS SED RSOph final srcind&srcdep comparison 20210812.pdf
  • All data from Aug 9, 10 and 12
File:Plot LST-1MAGICHESS SED RSOph final srcind&srcdep comparison 09to12.pdf
  • Light curve
  • Above E>100 GeV (MAGIC comparison)
File:LST-1MAGIC lightcurve RSOph interp node srcind v0.9.14dev AllSkyMC.pdf
  • Above E>250 GeV (HESS comparison)
File:LST-1HESS lightcurve RSOph interp node srcind v0.9.14dev AllSkyMC.pdf
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