Empirical multi-wavelength prediction method for Very High Energy Gamma-ray emitting BL Lacs




Ramazani VF, Lindfors E, Nilsson K

Gomboc, A

Symposium of the International-Astronomical-Union

2017

Proceedings of the International Astronomical Union

New Frontiers in Black Hole Astrophysics

NEW FRONTIERS IN BLACK HOLE ASTROPHYSICS

IAU SYMP P SERIES

IAU Symposium Proceedings Series

12

S324

239

240

2

1743-9213

DOIhttps://doi.org/10.1017/S1743921317001284



We present the most up-to-date and complete multi-wavelength correlation analysis on luminosity properties of TeV BL Lacs. Correlation function (power law or linear) parameters are calculated based on linear regression method. Using the lower energy luminosities of a sample of 182 non-TeV BL Lacs and the generated functions, minimum level of VHE gamma-ray emission was calculated for each non-TeV BL Lacs. This multi wavelength prediction method gives us a list of best candidates to be observed with current generation of Imaging Air Cherenkov Telescopes.



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