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Variability of the counterpart to the gamma-ray blazar GT0106+613

Published online by Cambridge University Press:  24 March 2015

Pedro L. Luque-Escamilla ,
J. Martí ,
E. Ramírez-Valenzuela ,
A. J. Muñoz-Arjonilla  and
J. M. Paredes
Pedro L. Luque-Escamilla
Affiliation:
Dept. Ingeniería Mecánica y Minera, Universidad de Jaén, E.P.S. Jaén, Campus Las Lagunillas, s/n, 23700, Jaén, Spain email: [email protected] Grupo de Investigación FAEG, Univ. de Jaén, Campus Las Lagunillas s/n, 23071 Jaén, Spain email: [email protected]
J. Martí
Affiliation:
Dept. Fsica, Universidad de Jaén, E.P.S. Jaén, Campus Las Lagunillas, s/n, 23700, Jaén, Spain email: [email protected] Grupo de Investigación FAEG, Univ. de Jaén, Campus Las Lagunillas s/n, 23071 Jaén, Spain email: [email protected]
E. Ramírez-Valenzuela
Affiliation:
Instituto de Astrofísica de Andalucía, CSIC, Avda. Vía Láctea
A. J. Muñoz-Arjonilla
Affiliation:
Grupo de Investigación FAEG, Univ. de Jaén, Campus Las Lagunillas s/n, 23071 Jaén, Spain email: [email protected]
J. M. Paredes
Affiliation:
Departament dAstronomia i Meteorologia, Institut de Ciències del Cosmos (ICC), Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, E-08028, Barcelona, Spain. email: [email protected]
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Abstract

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We present the optical/infrared counterpart to GT0106+613, a transient gamma-ray source believed to be a blazar. Long-term differential photometry and satellite information was used to confirm the variability in optical/infrared wavelengths, correlated with gamma-ray flares from the source. An intense optical flare with no counterpart in gamma-rays is also remarkable.

Keywords

gamma rays: observationsquasars: individual (J0109+6134)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S313: Extragalactic jets from every angle , September 2014 , pp. 87 - 88
Copyright
Copyright © International Astronomical Union 2015 

References

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