Analysis BLLac Oct 2022

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Revision as of 11:09, 27 October 2022 by Nozaki (talk | contribs) (Data-taking information)
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BL Lacertae flare Oct 2022

General information

  • Name of the source: BL Lacertae
  • Brief description of the source:
    • IBL / LBL
    • highly variable
    • z = 0.069
    • RA: 22 02 43.3 (hh mm ss), Dec: +42 16 40 (dd mm ss)
    • RA, Dec in deg (ICRS): 330.68038, 42.277772

Data-taking information

DL1 data

Standard run-wise data files produced by LSTOSA.

  • tailcut 8-4 (with cleaning based on pedestal RMS)
/fefs/aswg/data/real/DL1/20221020/v0.9/tailcut84/


Fast analysis by Seiya Nozaki (source-dependent analysis)

DL2 data

  • lstchain v0.9.6
  • source-dependent

Significance of the detection

  • 1 Off reflected position
  • cut
    • intensity > 100
    • gammaness > 0.7
    • alpha < 10
  • statistics
    • Number of ON events: 128864
    • Number of OFF events: 113599
    • Excess: 15265
    • Li&Ma significance: 31 sigma

Alpha BLLac 20221020 SNozaki.png

DL3 analysis

  • gammapy 0.20.1
  • cut
    • intensity > 0
    • r: [0, 1]
    • wl: [0.01, 1]
    • event_type = 32
    • 70% efficiency gammaness cut (min_gh_cut=0.1, max_gh_cut=0.95
    • 70% efficiency gammaness cut (min_alpha_cut=1, min_alpha_cut=20)
  • 2022-10-20 (SED)

SED BLLac 20221020 SNozaki.png

  • 2022-10-20 (LC)
    • > 100 GeV: (6.29 +/- 0.20) x 1E-10 / (cm2 s)

LC BLLac 20221020 SNozaki.png



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