Difference between revisions of "Fast offline analysis GRB240811A August 2024 P067"

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(Created page with "==General information== * '''Name of the source''': WR 140 * '''Brief description of the source''': ** Object type : Wolf–Rayet star binary ** Redshift (z) : 0 ** Other rel...")
 
(Daily results)
 
(10 intermediate revisions by the same user not shown)
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==General information==
 
==General information==
* '''Name of the source''': WR 140
+
* '''Name of the source''': GRB240811A
 
* '''Brief description of the source''':  
 
* '''Brief description of the source''':  
** Object type : Wolf–Rayet star binary
+
** Object type : GRB
** Redshift (z) : 0
+
** Redshift (z) : ?
 
** Other relevant information  
 
** Other relevant information  
** RA, Dec in deg (ICRS):  305.1165658, 43.85452412
+
** RA, Dec in deg (ICRS):  226.3622, 28.8957
 
* Analysis by:
 
* Analysis by:
 
**Ryuji Takeishi (ICRR - take@icrr.u-tokyo.ac.jp)
 
**Ryuji Takeishi (ICRR - take@icrr.u-tokyo.ac.jp)
  
 
==Data-taking information==
 
==Data-taking information==
* '''Dates of data-taking''': 2024-08-03, 2024-08-08
+
* '''Dates of data-taking''': 2024-08-11
***ZD range (deg):  --> 15-35 deg
+
***ZD range (deg):  --> 30-50 deg
 
***AZ range (deg):  -->  
 
***AZ range (deg):  -->  
 
***Transmission9km:  
 
***Transmission9km:  
*** Observation condition: ''dark''
+
*** Observation condition: ''moon''
 
*** Observation mode: '' std wobbles''
 
*** Observation mode: '' std wobbles''
 
***Observations:
 
***Observations:
  
  '2024-08-03': [18412, 18413] 0.2 h
+
  '2024-08-11': [18574, 18575, 18576, 18577, 18578] 1.84 h
'2024-08-08': [18516, 18517, 18518, 18519, 18520, 18521, 18522] 2.2 h
 
  
*Data quality selection: cosmic rates are somewhat low. None of the runs survive the default dR/dI@442pe limit of 1.5. Likely due to high dust concentration
+
[[File:Quality_20240811_GRB240811A_Takeishi.png | 600 px]]
 +
 
 +
*Data quality selection: Almost runs did not survive the default dR/dI@442pe limit of 1.5. Likely due to high dust concentration. Since almost runs exceed dark NSB limit, we did both analyses with dark NSB MC and high NSB image cleaning MC.
 
*Joint observations with MAGIC? : yes
 
*Joint observations with MAGIC? : yes
*Information on data-taking (observations summaries): https://www.lst1.iac.es/datacheck/observation_overview/2024/08/run_summary_2024_08_03.pdf
+
*Information on data-taking (observations summaries): https://www.lst1.iac.es/datacheck/observation_overview/2024/08/run_summary_2024_08_11.pdf
https://www.lst1.iac.es/datacheck/observation_overview/2024/08/run_summary_2024_08_08.pdf
 
  
 
==General analysis information==
 
==General analysis information==
Line 31: Line 31:
 
* DL1b standard production (v0.10/tailcut84), run-wise merged files in:
 
* DL1b standard production (v0.10/tailcut84), run-wise merged files in:
  
  /fefs/aswg/data/real/DL1/20240803/v0.10/tailcut84/dl1_LST-1.Run18412.h5
+
  /fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18574.h5
  /fefs/aswg/data/real/DL1/20240803/v0.10/tailcut84/dl1_LST-1.Run18413.h5
+
  /fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18575.h5
  /fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18516.h5
+
  /fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18576.h5
  /fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18517.h5
+
  /fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18577.h5
  /fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18518.h5
+
  /fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18578.h5
/fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18519.h5
 
/fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18520.h5
 
/fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18521.h5
 
/fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18522.h5
 
  
 
==Monte Carlo information==
 
==Monte Carlo information==
 
Write below the MC production id among the existing MC
 
Write below the MC production id among the existing MC
 
* All-sky MC production used: 20240131_allsky_v0.10.5_all_dec_base
 
* All-sky MC production used: 20240131_allsky_v0.10.5_all_dec_base
** Declination line (training): dec_4822
+
** Declination line (training): dec_3476
 
+
High-NSB analysis:
 +
* All-sky MC production used: 20240229_dec34_nsb14
 +
** Declination line (training): dec_3476
  
 
===Random forest===
 
===Random forest===
 
Path to the models used:
 
Path to the models used:
  
  /fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_4822
+
  /fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_3476
 +
 
 +
High-NSB analysis:
 +
 
 +
/fefs/aswg/data/models/AllSky/20240229_dec34_nsb14/dec_3476
  
 
==DL2 data==
 
==DL2 data==
  
Config file:
+
Config file (standard):
  /fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_4822/lstchain_config_2024-01-31.json
+
  /fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_3476/lstchain_config_2024-01-31.json
 +
Config file (high-nsb):
 +
/fefs/aswg/data/models/AllSky/20240229_dec34_nsb14/dec_3476/llstchain_config_2024-02-29.json
  
 
Files in:
 
Files in:
  
  /fefs/aswg/workspace/ryuji.takeishi/FOA/WR140/DL2
+
  /fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/DL2
 +
/fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/NSB14/DL2
  
 
==DL3 data & IRF==
 
==DL3 data & IRF==
Line 89: Line 94:
 
Files in:
 
Files in:
  
  /fefs/aswg/workspace/ryuji.takeishi/FOA/WR140/DL3
+
  /fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/DL3
 +
/fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/NSB14/DL3
  
 
==High-level analysis==
 
==High-level analysis==
Line 109: Line 115:
 
=== Daily results ===
 
=== Daily results ===
  
2024-08-03: No detection
+
Dark NSB image cleaning: No detection
[[File:20240803_WR140_Takeishi.png|500 px]]
+
[[File:Theta2_20240811_GRB240811A_Takeishi.png|500 px]]
  
2024-08-08: No detection
+
High NSB image cleaning: No detection
[[File:Theta2_20240808_WR140_Takeishi.png|500 px]]
+
[[File:Theta2_20240811_GRB240811A_highNSB_Takeishi.png|500 px]]
  
 
=== Significance and Excess sky maps ===
 
=== Significance and Excess sky maps ===

Latest revision as of 15:40, 12 August 2024

General information[edit]

  • Name of the source: GRB240811A
  • Brief description of the source:
    • Object type : GRB
    • Redshift (z) : ?
    • Other relevant information
    • RA, Dec in deg (ICRS): 226.3622, 28.8957
  • Analysis by:
    • Ryuji Takeishi (ICRR - take@icrr.u-tokyo.ac.jp)

Data-taking information[edit]

  • Dates of data-taking: 2024-08-11
      • ZD range (deg): --> 30-50 deg
      • AZ range (deg): -->
      • Transmission9km:
      • Observation condition: moon
      • Observation mode: std wobbles
      • Observations:
'2024-08-11': [18574, 18575, 18576, 18577, 18578] 1.84 h

Quality 20240811 GRB240811A Takeishi.png

General analysis information[edit]

  • source-independent analysis
  • lstchain version: v0.10.11
  • DL1b standard production (v0.10/tailcut84), run-wise merged files in:
/fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18574.h5
/fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18575.h5
/fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18576.h5
/fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18577.h5
/fefs/aswg/data/real/DL1/20240811/v0.10/tailcut84/dl1_LST-1.Run18578.h5

Monte Carlo information[edit]

Write below the MC production id among the existing MC

  • All-sky MC production used: 20240131_allsky_v0.10.5_all_dec_base
    • Declination line (training): dec_3476

High-NSB analysis:

  • All-sky MC production used: 20240229_dec34_nsb14
    • Declination line (training): dec_3476

Random forest[edit]

Path to the models used:

/fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_3476

High-NSB analysis:

/fefs/aswg/data/models/AllSky/20240229_dec34_nsb14/dec_3476

DL2 data[edit]

Config file (standard):

/fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_3476/lstchain_config_2024-01-31.json

Config file (high-nsb):

/fefs/aswg/data/models/AllSky/20240229_dec34_nsb14/dec_3476/llstchain_config_2024-02-29.json

Files in:

/fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/DL2
/fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/NSB14/DL2

DL3 data & IRF[edit]

 "EventSelector": {
   "filters": {
     "intensity": [50, Infinity],
     "width": [0, Infinity],
     "length": [0, Infinity],
     "r": [0, 1],
     "wl": [0.01, 1],
     "leakage_intensity_width_2": [0, 1],
     "event_type": [32, 32]
   }
 },
 "DL3Cuts": {
   "min_event_p_en_bin": 100,
   "min_gh_cut": 0.1,
   "max_gh_cut": 0.98,
   "min_theta_cut": 0.1,
   "max_theta_cut": 0.32,
   "fill_theta_cut": 0.32,
   "allowed_tels": [1]
 },
  • 70 % efficiency for both gammaness and theta gamma-ray selection cuts
  • Point-like IRF

Files in:

/fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/DL3
/fefs/aswg/workspace/ryuji.takeishi/FOA/GRB240811A/NSB14/DL3

High-level analysis[edit]

  • Gammapy 1.1
  • 1D analysis (point-like IRF)

Analysis Results[edit]

Theta2 plot[edit]

Settings:

  • Theta2 cut for signal extraction: 0.04 deg2
  • Normalization range: 0.1 - 0.4 deg2
  • Number of off positions: 3
  • Energy range: 100 GeV - 10 TeV

Daily results[edit]

Dark NSB image cleaning: No detection Theta2 20240811 GRB240811A Takeishi.png

High NSB image cleaning: No detection Theta2 20240811 GRB240811A highNSB Takeishi.png

Significance and Excess sky maps[edit]

Spectral results[edit]

Light curve[edit]