Difference between revisions of "GRB241029A"

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(Data-taking information)
(Cross-check)
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*Data quality selection: runs 19376 and 19377 failed default dR/dI rate and were not included
 
*Data quality selection: runs 19376 and 19377 failed default dR/dI rate and were not included
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Note: run 19380 was cut from high-level analysis as elapsed_time < 300s
  
 
===General analysis information===
 
===General analysis information===

Revision as of 17:02, 30 October 2024

Alert Information

  • Name/type of the alert: GRB 241029A
  • GCN circular: [1]
  • Astro-COLIBRI: [2]
  • Triggered by: SVOM/ECLAIRs
  • Alert coordinates:
    • RA: 21 41 18.48 (hh mm ss), Dec: 5 5 9.6 (dd mm ss)
    • RA, Dec in deg (ICRS): 325.327deg, 5.086deg
  • Alert arrival time: 2024-10-29 02:19:53UTC
  • Other relevant information:
    • GCN notices + circulars: [3]
    • Redshift (z): z = 1.072 (OSIRIS@GTC, GCN #37950 [4])

LST Observations

  • Dates of data-taking: 2024-10-29
    • 2024-10-29
      • Zenith range (deg): 26 --> 40
      • Transmission9km: tbd
      • Observation condition: dark
      • Observation mode: std wobbles
      • Runs: 19377 - 19382
      • Joint observations with MAGIC? : yes (19377 - 19382)
      • ELOG link:[ https://www.lst1.iac.es/elog/LST+commissioning/3632]
      • Important comments:

Fast analysis

  • Analysis by:
    • Analyzer 1 name (Roger Grau - rgrau@ifae.es)
    • Analyzer 2 Tora T. H. Arnesen (IAC - tora.arnesen@iac.es)

Data-taking information

  • Dates of data-taking: 2024-10-29
    • Date (time of observation h) 2024-10-29: 1.488 h
      • ZD range (deg): 22-42
      • Observations: (see example below)
2024-10-29: [19377 19378 19379 19381 19382]
  • Data quality selection: 19376, 19380 runs did not survive the data quality selection (max NSB std: 2.3)

Cross-check

  • Dates of data-taking: 2024-10-29
    • Date (time of observation h) 2024-10-29: 1.27 h
      • ZD range (deg): 24-42
      • Observations: (see example below)
2024-10-29: [19378 19379 19380 19381 19382]
  • Data quality selection: runs 19376 and 19377 failed default dR/dI rate and were not included

Note: run 19380 was cut from high-level analysis as elapsed_time < 300s

General analysis information

  • source-independent analysis
  • lstchain version: v0.10.12
  • DL1b standard production (v0.10/tailcut84), run-wise merged files in:
/fefs/aswg/data/real/DL1/YYYYMMDD/v0.10/tailcut84/dl1_LST-1.Run?????.h5


Monte Carlo information

  • All-sky MC production used: 20240131_allsky_v0.10.5_all_dec_base
  • Declination line (training): dec_931

Random forest

Path to the models used:

/fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_931

DL2 data

The config file to produce the DL2 files must be the one used to produce the RF models. Should be located together with model's files.


Files in:

/fefs/aswg/workspace/roger.grau/fast_oa_Oct_2024/GRB241029A/DL2


DL3 data & IRF

Files in:

/fefs/aswg/workspace/roger.grau/fast_oa_Oct_2024/GRB241029A/DL3

Configuration used for producing IRF/DL3 files (you can leave standard settings):

 "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 energy-dependent cuts
  • Point-like IRF.


High-level analysis and results

Analysis settings

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

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: 0.01 - 10 TeV

Daily results

  • 2024-10-29: No detection
Error creating thumbnail: File missing

General information

General analysis information

Monte Carlo information

Random forest

DL2 data

DL3 data & IRF

High-level analysis

Analysis Results

Theta2 plot

Daily results

Stacked observations

Significance and Excess sky maps

Spectral results