Difference between revisions of "GRB220302A"

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(Analysis by Name (Institute - email))
(Analysis by Kenta)
 
(9 intermediate revisions by the same user not shown)
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== LST Observations ==
 
== LST Observations ==
  
* '''Dates of data-taking''':  
+
* '''Dates of data-taking''': 2022-03-02
** Date (time of observation h)
+
** '''2022-03-02'''
*** Zenith range (deg):
+
*** '''Zenith range (deg)''': 61 -> 52
*** Transmission9km:
+
*** '''Transmission9km''':
*** Observation condition: ''dark, moonlight, twilight, mixed, calima, ...''
+
*** '''Observation condition''': dark
*** Observation mode: ''e.g., ON, std or custom wobbles''
+
*** '''Observation mode''': std wobbles
*** Runs:  
+
*** '''Runs''': 7219 - 7221
*** Joint observations with MAGIC? : ''Yes/No''
+
*** '''Joint observations with MAGIC?''' : Yes
*** ELOG link:
+
*** '''ELOG link''': [http://www.lst1.iac.es/elog/LST+commissioning/2112 Logbook URL]
*** Important comments: ''delay, ...''
+
*** '''Important comments''': ''delay, ...''
  
== Analysis by Kenta (Institute - email) ==
+
== Analysis by Kenta ==
  
=== Data-taking information ===
+
=== Analysis configuration ===
  
* Overall selected observation time:
+
* '''Analyzer''': Kenta Terauchi (Kyoto Univ., email: terauchi.kenta.74s@st.kyoto-u.ac.jp)
* Selected runs:
 
* Position analyzed: ''RA, Dec''
 
  
=== Monte Carlo information ===
+
* '''Software versions''':
 +
**lstchain v0.9.2
  
* Link to MC files used:
+
* '''Cuts and parameters used''':  
** Particle types:
+
** intensity > 50
 +
** gammaness > 0.7
 +
** leakage < 0.2
  
=== DL1 data ===
+
* ''' DL1 files ''':
  
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 (lstchain v0.9.X)
  
'''Example''' :
+
/fefs/aswg/data/real/DL1/20220302/v0.9/tailcut84/dl1_LST-1.Run0{7219,7220,7221}.h5
  
Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)
+
* ''' Random Forest ''':
 +
src-indep (diffuse gamma, src_r<3deg, disp_norm)
 +
/fefs/aswg/data/models/20200629_prod5_trans_80/zenith_20deg/south_pointing/20220215_v0.9.1_prod5_trans_80_local_tailcut_8_4
  
* original DL1a files
+
* '''DL2 MC data for IRF''':
  
/fefs/aswg/data/real/DL1/20210808/v0.7.3/tailcut84/dl1_LST-1.Run0XXXX.XXXX.h5
+
* '''Overall selected observation time''': 48 min
/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
+
* '''Position analyzed''': 301.432, +49.389 (deg)
  
  /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/lstchain_standard_config.json
+
* '''Analysis/data problems''':
 
 
* 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 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 ===
 
 
 
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
 
 
 
=== High-level analysis ===
 
 
 
Please put any information about the production of higher level analysis here.
 
 
 
'''Example'''
 
 
 
* Science Tool: gammapy 0.18.2
 
* Point-like IRF, 1D analysis
 
 
 
== Analysis Results ==
 
 
 
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 ===
  
=== Significance map ===
+
* theta < 0.2
 +
* norm_range_theta2: 0.3 - 0.5
  
=== Excess map ===
 
  
=== Spectral results ===
+
{| align='center'
 +
| [[Image:GRB220302A_th2_Kenta.png|thumb|600px|center|alt=Theta2 plot for GRB220302A.|Theta2 plot for GRB220302A.]]
 +
|
 +
|}

Latest revision as of 11:14, 8 March 2022

Go back to Transient observation logbook.


Alert Information[edit]

  • Name/type of the alert: Name
  • GCN notice: https://gcn.gsfc.nasa.gov/other/1094950.swift
  • Triggered by: Swift-BAT
  • Alert coordinates:
    • RA: 20 05 44 (hh mm ss), Dec: +49 23 20 (dd mm ss)
    • RA, Dec in deg (ICRS): 301.432, +49.389
  • Alert arrival time: 2022-03-02 07:41:17 UTC
  • Other relevant information:
    • Redshift (z):

LST Observations[edit]

  • Dates of data-taking: 2022-03-02
    • 2022-03-02
      • Zenith range (deg): 61 -> 52
      • Transmission9km:
      • Observation condition: dark
      • Observation mode: std wobbles
      • Runs: 7219 - 7221
      • Joint observations with MAGIC? : Yes
      • ELOG link: Logbook URL
      • Important comments: delay, ...

Analysis by Kenta[edit]

Analysis configuration[edit]

  • Analyzer: Kenta Terauchi (Kyoto Univ., email: terauchi.kenta.74s@st.kyoto-u.ac.jp)
  • Software versions:
    • lstchain v0.9.2
  • Cuts and parameters used:
    • intensity > 50
    • gammaness > 0.7
    • leakage < 0.2
  • DL1 files :

Used DL1b files produced by LSTOSA (lstchain v0.9.X)

/fefs/aswg/data/real/DL1/20220302/v0.9/tailcut84/dl1_LST-1.Run0{7219,7220,7221}.h5
  • Random Forest :

src-indep (diffuse gamma, src_r<3deg, disp_norm)

/fefs/aswg/data/models/20200629_prod5_trans_80/zenith_20deg/south_pointing/20220215_v0.9.1_prod5_trans_80_local_tailcut_8_4
  • DL2 MC data for IRF:
  • Overall selected observation time: 48 min
  • Position analyzed: 301.432, +49.389 (deg)
  • Analysis/data problems:

Theta2 plot[edit]

  • theta < 0.2
  • norm_range_theta2: 0.3 - 0.5


Theta2 plot for GRB220302A.
Theta2 plot for GRB220302A.