Difference between revisions of "GRB230512A"

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* Position analyzed: ''RA, Dec''
 
* Position analyzed: ''RA, Dec''
  
=== Monte Carlo information ===
 
 
* Link to MC files used:
 
** Particle types:
 
  
 
=== DL1 data ===
 
=== 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.
+
Used DL1b files produced by LSTOSA
 
 
'''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/
 
 
 
* 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/data/real/DL1/20230512/v0.9/tailcut84/
/fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/Run0XXXX
 
  
=== Random forest ===
 
 
Please include the path to the RF files used or your specific .json files used in producing your RFs and for which source analysis (source dependent or independent), and variables 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 ===
 
=== DL2 data ===
  
Information about your DL2 data and settings such as: specifc versions of lstchain, specfic .json version used.
+
* Random forest:  
 
 
'''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'''
 
  
* Science Tool: gammapy 0.18.2
+
XXXXXXXXXXXXX
* Point-like IRF, 1D analysis
 
  
== Analysis Results ==
+
* lstchain v0.9.12 with config file
 +
XXXXXXXXXXXXX
  
Please place higher-level analysis results (Spectra, SkyMaps, Lightcurves, etc) here.
 
If the alert was observed for several nights please add plots for each night separately and all data together.
 
  
=== Theta2 plot ===
+
=== Theta2 plot from DL2===
  
=== Significance map ===
+
*Cuts and parameters used:
 +
**intensity > 50
 +
**gammaness > 0.8
 +
**Theta2_global_cut=0.04
 +
**leakage < 0.2
 +
** norm_range_theta2_min=0.3   
 +
** norm_range_theta2_max=0.5
  
=== Excess map ===
+
{| align='center'
 +
| [[Image: Theta2_DL2_plot_GRB230512A.png |thumb|600px|center|alt=Theta2 plot for GRB130512A.|Theta2 plot for GRB230512A.]]
 +
|}
  
=== Spectral results ===
+
----

Revision as of 15:31, 13 May 2023

Go back to Transient Working Group.


Alert Information

  • Name/type of the alert: Name
  • GCN notice: https://gcn.nasa.gov/circulars/33778
  • Triggered by: Fermi GBM (but alert from TH by Fermi-LAT)
  • Alert coordinates (From Fermi-LAT):
    • RA: 19 41 36.00 (hh mm ss), Dec: +38 24 00.00 (dd mm ss)
    • RA, Dec in deg (ICRS): 295.4, 38.4
  • Alert arrival time: 06:27:45 UT
  • Other relevant information:
    • Redshift (z): n/a

Multi-wavelength Observations

Timeline
T0+ Instrument Outcome Outcome specific value (flux/UL/...) Comment Link
0-300 s after the GBM trigger Fermi-LAT Detection (1.0 ± 0.3) E-05 ph/cm2/s The highest-energy photon is a 1.7 GeV https://gcn.nasa.gov/circulars/33780
45.5 - 57.3 ks Swift-XRT No aparent detection Nine uncatalogued X-ray sources have been detected However none of them is above the RASS limit or shows definitive signs of fading. https://gcn.nasa.gov/circulars/33789
2 hours Zwicky Transient Facility No aparent detection Two sources were found within the 95% localization region These are likely unrelated as they fall outside the LAT localization https://gcn.nasa.gov/circulars/33784


LST Observations

  • * Dates of data-taking: 2023-05-12
    • 2023-05-12 (4.1 h)
      • Zenith range (deg): 62 - 15
      • Transmission9km: n/a
      • Observation condition: dark, moonlight, high level of dust, moderate cloudiness
      • Observation mode: std wobbles
      • Runs: 12962 - 12973
      • Joint observations with MAGIC? : Yes
      • ELOG link: [1]
      • Important comments: '

Analysis by Arnau Aguasca-Cabot (UB - arnau.aguasca@fqa.ub.edu)

Data-taking information

  • Overall selected observation time:
  • Selected runs:
  • Position analyzed: RA, Dec


DL1 data

Used DL1b files produced by LSTOSA

/fefs/aswg/data/real/DL1/20230512/v0.9/tailcut84/


DL2 data

  • Random forest:
XXXXXXXXXXXXX
  • lstchain v0.9.12 with config file
XXXXXXXXXXXXX


Theta2 plot from DL2

  • Cuts and parameters used:
    • intensity > 50
    • gammaness > 0.8
    • Theta2_global_cut=0.04
    • leakage < 0.2
    • norm_range_theta2_min=0.3
    • norm_range_theta2_max=0.5
Theta2 plot for GRB130512A.
Theta2 plot for GRB230512A.