Analysis BLLac Oct 2022

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

• Dates of data-taking:
  • 2022-10-20 ( h)
    • ZD: 16 - 42 deg
    • Transmission9km: n/a
    • Runs: 9753, 9754, 9755, 9756, 9757, 9758, 9759, 9760, 9761
    • Joint observations with MAGIC
    • https://www.lst1.iac.es/datacheck/observation_overview/2022/10/CameraDailyCheck20221020.pdf

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
• tailcut 8-4 (with cleaning based on pedestal RMS)

DL3 data selection

• intensity > 30
• r: [0, 1 ]
• wl: [0.05, 1]
• leakage_intensity_width_2: [0, 0.2 ]
• fixed_gh_cut: 0.7
• fixed_theta_cut: 0.2

High-level analysis

• Science Tool: gammapy 0.18.2 (+ bugfix https://github.com/gammapy/gammapy/pull/3374)

Significance of the detection

1 Off reflected position
Theta2 cut: 0.04 deg

• Squares: Background
• Circles: Signal events

Stacked

• List of runs: [5219, 5220, 5229, 5230, 5231, 5232, 5233, 5234, 5235, 5251, 5252]
• Observation time: 2.46 h
• Number of ON events: 881
• Number of OFF events: 616 +/- 25
• Excess: 265 +/- 39
• Li&Ma significance: 6.9 sigma

Spectral analysis

Effective area

Migration Matrix and exposure

• 2021-07-10

• PowerLaw fit:
  • index: 3.5 +/- 0.2
  • E_ref: 0.1 TeV
  • amplitude: 1.3 +/- 0.2 10^-9 cm-2 s-1 TeV-1

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