Fast Offline Analysis S240915b September 2024 P068

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Revision as of 22:27, 15 September 2024 by Hluciani (talk | contribs) (General analysis information)
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General information

  • Name of the source: S240915b
  • Brief description of the source: compact binary merger candidate. The classification of the GW signal is BBH (86%), NSBH (14%), Terrestrial (<1%), or BNS (<1%)
    • Object type :
    • Redshift (z) :
    • Other relevant information
    • RA: XXXXXX (hh mm ss), Dec: XXXXX (dd mm ss)
    • RA, Dec in deg (ICRS): 331.5, 73.1 (pointing coordinates)
  • Analysis by:
    • Helena Luciani (University of Trieste - helena.luciani@phd.units.it)

Data-taking information

  • Dates of data-taking: 2024-09-14
      • time of observations: 1.2 hours
      • ZD range (deg): 50 - 70
      • Observations:

20240914 : [19076, 19077]

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/DL1/20240911/v0.10/tailcut84/dl1_LST-1.Run19076.h5
/fefs/aswg/data/real/DL1/20240911/v0.10/tailcut84/dl1_LST-1.Run19077.h5

Monte Carlo information

  • All-sky MC production used: 20240131_allsky_v0.10.5_all_dec_base
  • Declination line (training): dec_6676


Random forest

Path to the models used:

/fefs/aswg/data/models/AllSky/20240131_allsky_v0.10.5_all_dec_base/dec_6676/