Difference between revisions of "Fast offline analysis GRB240811A August 2024 P067"
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==General information== | ==General information== | ||
− | * '''Name of the source''': | + | * '''Name of the source''': GRB240811A |
* '''Brief description of the source''': | * '''Brief description of the source''': | ||
− | ** Object type : | + | ** Object type : GRB |
− | ** Redshift (z) : | + | ** Redshift (z) : ? |
** Other relevant information | ** Other relevant information | ||
− | ** RA, Dec in deg (ICRS): | + | ** 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) |
Revision as of 15:18, 12 August 2024
Contents
General information
- 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
- Dates of data-taking: 2024-08-03, 2024-08-08
- ZD range (deg): --> 15-35 deg
- AZ range (deg): -->
- Transmission9km:
- Observation condition: dark
- Observation mode: std wobbles
- Observations:
'2024-08-03': [18412, 18413] 0.2 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
- 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
https://www.lst1.iac.es/datacheck/observation_overview/2024/08/run_summary_2024_08_08.pdf
General analysis information
- source-independent analysis
- lstchain version: v0.10.11
- 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/DL1/20240803/v0.10/tailcut84/dl1_LST-1.Run18413.h5 /fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18516.h5 /fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18517.h5 /fefs/aswg/data/real/DL1/20240808/v0.10/tailcut84/dl1_LST-1.Run18518.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
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_4822
Random forest
Path to the models used:
/fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_4822
DL2 data
Config file:
/fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_4822/lstchain_config_2024-01-31.json
Files in:
/fefs/aswg/workspace/ryuji.takeishi/FOA/WR140/DL2
DL3 data & IRF
"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/WR140/DL3
High-level analysis
- Gammapy 1.1
- 1D analysis (point-like IRF)
Analysis Results
Theta2 plot
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