Standard

Multiwavelength Observations of 6 FSRQ in 2008-2012. / Troitskiy, I. S.; Morozova, D. A.; Jorstad, S. G.; Larionov, V. M.; Marscher, A. P.; Agudo, I.; Blinov, D. A.; Smith, P. S.

Proceedings of the International Astronomical Union, IAU Symposium. 2014. p. 249-251.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research

Harvard

Troitskiy, IS, Morozova, DA, Jorstad, SG, Larionov, VM, Marscher, AP, Agudo, I, Blinov, DA & Smith, PS 2014, Multiwavelength Observations of 6 FSRQ in 2008-2012. in Proceedings of the International Astronomical Union, IAU Symposium. pp. 249-251.

APA

Troitskiy, I. S., Morozova, D. A., Jorstad, S. G., Larionov, V. M., Marscher, A. P., Agudo, I., Blinov, D. A., & Smith, P. S. (2014). Multiwavelength Observations of 6 FSRQ in 2008-2012. In Proceedings of the International Astronomical Union, IAU Symposium (pp. 249-251)

Vancouver

Troitskiy IS, Morozova DA, Jorstad SG, Larionov VM, Marscher AP, Agudo I et al. Multiwavelength Observations of 6 FSRQ in 2008-2012. In Proceedings of the International Astronomical Union, IAU Symposium. 2014. p. 249-251

Author

Troitskiy, I. S. ; Morozova, D. A. ; Jorstad, S. G. ; Larionov, V. M. ; Marscher, A. P. ; Agudo, I. ; Blinov, D. A. ; Smith, P. S. / Multiwavelength Observations of 6 FSRQ in 2008-2012. Proceedings of the International Astronomical Union, IAU Symposium. 2014. pp. 249-251

BibTeX

@inproceedings{c80d283bd3a649eab3a10279eb38d102,
title = "Multiwavelength Observations of 6 FSRQ in 2008-2012",
abstract = "We present results of 4 years of VLBA monitoring along with γ-ray and optical R-band photometric observations of 6 blazars (0420-014, 1156+295, 1222+216, PKS 1510-089, 1633+382 and CTA 102). We have analyzed total intensity images obtained with the VLBA at 43 GHz and investigated kinematic evolution of the pc-scale jets of the sources. For all sources we compare flux variations in the VLBI core and bright superluminal knots with γ-ray and optical light curves. The majority of γ-ray flares are coincident with the appearance of a new superluminal knot and/or a flare in the millimeter-wave core and at optical wavelengths. These results support the conclusion that for many flares in blazars the region of the enhanced γ-ray and optical emission is located in the vicinity or downstream of the mm-wave VLBI core.",
author = "Troitskiy, {I. S.} and Morozova, {D. A.} and Jorstad, {S. G.} and Larionov, {V. M.} and Marscher, {A. P.} and I. Agudo and Blinov, {D. A.} and Smith, {P. S.}",
year = "2014",
language = "English",
pages = "249--251",
booktitle = "Proceedings of the International Astronomical Union, IAU Symposium",

}

RIS

TY - GEN

T1 - Multiwavelength Observations of 6 FSRQ in 2008-2012

AU - Troitskiy, I. S.

AU - Morozova, D. A.

AU - Jorstad, S. G.

AU - Larionov, V. M.

AU - Marscher, A. P.

AU - Agudo, I.

AU - Blinov, D. A.

AU - Smith, P. S.

PY - 2014

Y1 - 2014

N2 - We present results of 4 years of VLBA monitoring along with γ-ray and optical R-band photometric observations of 6 blazars (0420-014, 1156+295, 1222+216, PKS 1510-089, 1633+382 and CTA 102). We have analyzed total intensity images obtained with the VLBA at 43 GHz and investigated kinematic evolution of the pc-scale jets of the sources. For all sources we compare flux variations in the VLBI core and bright superluminal knots with γ-ray and optical light curves. The majority of γ-ray flares are coincident with the appearance of a new superluminal knot and/or a flare in the millimeter-wave core and at optical wavelengths. These results support the conclusion that for many flares in blazars the region of the enhanced γ-ray and optical emission is located in the vicinity or downstream of the mm-wave VLBI core.

AB - We present results of 4 years of VLBA monitoring along with γ-ray and optical R-band photometric observations of 6 blazars (0420-014, 1156+295, 1222+216, PKS 1510-089, 1633+382 and CTA 102). We have analyzed total intensity images obtained with the VLBA at 43 GHz and investigated kinematic evolution of the pc-scale jets of the sources. For all sources we compare flux variations in the VLBI core and bright superluminal knots with γ-ray and optical light curves. The majority of γ-ray flares are coincident with the appearance of a new superluminal knot and/or a flare in the millimeter-wave core and at optical wavelengths. These results support the conclusion that for many flares in blazars the region of the enhanced γ-ray and optical emission is located in the vicinity or downstream of the mm-wave VLBI core.

M3 - Conference contribution

SP - 249

EP - 251

BT - Proceedings of the International Astronomical Union, IAU Symposium

ER -

ID: 4700990