VizieR

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VizieR

  
J/A+A/702/A38
  NGC 4151 VHE spectral energy distribution (Abe+, 2025)
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2025A&A...702A..38A
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1.J/A+A/702/A38/figure1Squared angular distance ({theta}2) to the NGC 4151 position distribution shows the number of gamma-ray candidate events as a function of the squared angular separation between the reconstructed gamma-ray direction and the NGC 4151 position [profile](plot)
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(55 rows)
2.J/A+A/702/A38/table1Spectral energy distribution of Fig. 2 and Fig. 3, only MAGIC data (4 rows)

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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)theta2 deg2 Off-axis squared angle (phys.angSize)
  (1)Non  Number of ON events (meta.number)
  (1)Noff  Number of OFF events (meta.number)
  (1)DNoff  OFF events uncertainty (stat.error)
  (2)E283 TeV Energy (index = 2.83) (phys.energy)
  (2)E200 TeV Energy (index = 2.00) (phys.energy)
  (2)b_E TeV Energy bin width low (instr.bandwidth)
  (2)B_E TeV Energy bin width up (instr.bandwidth)
  (2)E2FE283 10-13TeV/cm2/sUpper limit on photon flux at E283 (phot.flux.density;em.gamma.hard)
  (2)E2FE200 10-13TeV/cm2/sUpper limit on photon flux at E200 (phot.flux.density;em.gamma.hard)

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