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

Published online by Cambridge University Press:  23 June 2017

V. Fallah Ramazani ,
E. Lindfors  and
K. Nilsson
V. Fallah Ramazani
Affiliation:
Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Finland
E. Lindfors
Affiliation:
Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Finland
K. Nilsson
Affiliation:
FINCA (Finnish Center for Astronomy with ESO), University of Turku, Finland
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Abstract

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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.

Keywords

BL LacsVHE gamma-ray
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 239 - 240
Copyright
Copyright © International Astronomical Union 2017