Difference between revisions of "GRB221009A src-ind analysis dark conditions"
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=General information= | =General information= | ||
| − | This wiki web page shows the analysis of GRB221009A data recorded in dark conditions and in mild moon conditions using the source-independent analysis. For the analysis of GRB221009A for runs in moon conditions go to | + | This wiki web page shows the analysis of GRB221009A data recorded in dark conditions and in mild moon conditions using the source-independent analysis. |
| + | |||
| + | For the analysis of GRB221009A for runs in moon conditions go to the following page: [https://www.lst1.iac.es/wiki/index.php/GRB221009A_src-ind_analysis_moon GRB221009A_src-ind_analysis_moon] | ||
| + | |||
| + | The wiki page with the summary of the current results of the src-ind moon analysis (as of February 8th) for the discussion with LST-Reco conveners is the following: [https://www.lst1.iac.es/wiki/index.php/Source-independent_strong_moon_analysis_results_for_discussion_(not_updated)] | ||
| + | |||
| + | * Slides presented at the GRB221009A meetings about the source-independent dark/mild-moon analysis: | ||
| + | : [https://indico.cta-observatory.org/event/4414/#2-source-independent-data-anal Start and Dark analysis I] | ||
| + | : [https://indico.cta-observatory.org/event/4433/#3-source-independent-data-anal Dark analysis II] | ||
| + | : [https://indico.cta-observatory.org/event/4521/#3-source-independent-data-anal Dark analysis III] | ||
| + | : [https://indico.cta-observatory.org/event/4522/#3-source-independent-data-anal Moon analysis IV] | ||
| + | : [https://indico.cta-observatory.org/event/4590/#3-source-independent-data-anal Moon analysis V] | ||
Revision as of 11:39, 3 March 2023
Back to the Data analysis page
Go back to Transient Working Group.
Go Back to Gamma-Ray Bursts (GRBs).
Go back to GRB221009A.
- Analysis by A. Aguasca-Cabot (Universitat de Barcelona - arnau.aguasca@fqa.ub.edu)
Contents
General information
This wiki web page shows the analysis of GRB221009A data recorded in dark conditions and in mild moon conditions using the source-independent analysis.
For the analysis of GRB221009A for runs in moon conditions go to the following page: GRB221009A_src-ind_analysis_moon
The wiki page with the summary of the current results of the src-ind moon analysis (as of February 8th) for the discussion with LST-Reco conveners is the following: [1]
- Slides presented at the GRB221009A meetings about the source-independent dark/mild-moon analysis:
Dark analysis
Monte Carlo information
- Link to MC files used: /fefs/aswg/data/mc/DL1/AllSky/20221027_v0.9.9_crab_tuned/*
- Particle types: The standard ones for the AllSky MC production.
- DEC Band (deg): dec_2276
DL1 data
Please include your settings to produce your DL1a and DL1b files. This includes whether you use LSTOSA, specific versions of lstchain, dllab scripts, cleaning levels, and calibration information.
Example :
Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)
- original DL1a files
/fefs/aswg/data/real/DL1/20210808/v0.7.3/tailcut84/dl1_LST-1.Run0XXXX.XXXX.h5 /fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/XXX/zenith_20deg/south_pointing/20210416_v0.7.3_prod5_trans_80_local_taicut_8_4/
- lstchain v0.7.5
- real data: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning
/fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/lstchain_standard_config.json
- MC: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning, PSF+NSB tuning
"image_modifier": {
"increase_nsb": true,
"extra_noise_in_dim_pixels": 0.74,
"extra_bias_in_dim_pixels": 0.38,
"transition_charge": 8,
"extra_noise_in_bright_pixels": 0.052,
"increase_psf": true,
"smeared_light_fraction": 0.125
},
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/lstchain_dl1ab_tune_MC_to_BLLac_config.json
- Produced DL1b files
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/data/ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/Run0XXXX
Random forest
Please include your specific .json files used in producing your RFs and for which source analysis (source dependent or independent), and variabules used in the RF.
Example
- lstchain-0.7.6.dev242+g2086cb9
- source-indep (diffuse gamma, src_r<3deg, disp_norm)
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/RF/lstchain_standard_config.json
- source-dep
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/RF/lstchain_src_dep_config.json
DL2 data
Information about your DL2 data and settings such as: specifc versions of lstchain, specfic .json version used.
Example:
- lstchain-0.7.6.dev242+g2086cb9
- source-indep
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/DL2/data/ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcindep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5
- source-dep
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/DL2/data/ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcdep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5
DL3 data selection
Information about your DL3 data selection.
Example
- intensity > 50
- r: [0, 1 ]
- wl: [0.1, 1 ]
- leakage_intensity_width_2: [0, 0.2 ]
- source-indep
- fixed_gh_cut: 0.3
- fixed_theta_cut: 0.2
- source-dep
- fixed_gh_cut: 0.7
- fixed_alpha_cut: 10
High-level analysis
Please put any information about the production of higher level analysis here.
Example
- lstchain to generate source-dep IRF, DL3
- Science Tool: gammapy 0.18.2
- point-like IRF, 1D analysis
Analysis Results
Please place higher-level analysis results (Spectra, SkyMaps, Lightcurves, etc) here.
