O2 Muu julkaisu
Empirical multi-wavelength prediction method for Very High Energy Gamma-ray emitting BL Lacs
Tekijät: Ramazani VF, Lindfors E, Nilsson K
Toimittaja: Gomboc, A
Konferenssin vakiintunut nimi: Symposium of the International-Astronomical-Union
Julkaisuvuosi: 2017
Journal: Proceedings of the International Astronomical Union
Kokoomateoksen nimi: New Frontiers in Black Hole Astrophysics
Tietokannassa oleva lehden nimi: NEW FRONTIERS IN BLACK HOLE ASTROPHYSICS
Lehden akronyymi: IAU SYMP P SERIES
Sarjan nimi: IAU Symposium Proceedings Series
Vuosikerta: 12
Numero: S324
Aloitussivu: 239
Lopetussivu: 240
Sivujen määrä: 2
ISSN: 1743-9213
DOI: https://doi.org/10.1017/S1743921317001284
Tiivistelmä
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.
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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