Standard

Very long baseline polarimetric monitoring at 15 GHz of the TeV blazar Markarian 421. / Lico, R.; Casadio, C.; Gómez, J.L.; Giroletti, M.; Orienti, M.; Giovannini, G.; Blasi, M.G.; Cotton, W.; Edwards, P.G.; Fuhrmann, L.; Jorstad, S.; Kino, M.; Kovalev, Y.Y.; Krichbaum, T.P.; Marscher, A.; Paneque, D.; Perez-Torres, M.A.; Piner, G.; Sokolovsky, K.V.

EPJ Web of Conferences. 2013.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции › научная

Harvard

Lico, R, Casadio, C, Gómez, JL, Giroletti, M, Orienti, M, Giovannini, G, Blasi, MG, Cotton, W, Edwards, PG, Fuhrmann, L, Jorstad, S, Kino, M, Kovalev, YY, Krichbaum, TP, Marscher, A, Paneque, D, Perez-Torres, MA, Piner, G & Sokolovsky, KV 2013, Very long baseline polarimetric monitoring at 15 GHz of the TeV blazar Markarian 421. в EPJ Web of Conferences. https://doi.org/10.1051/epjconf/20136107004

APA

Lico, R., Casadio, C., Gómez, J. L., Giroletti, M., Orienti, M., Giovannini, G., Blasi, M. G., Cotton, W., Edwards, P. G., Fuhrmann, L., Jorstad, S., Kino, M., Kovalev, Y. Y., Krichbaum, T. P., Marscher, A., Paneque, D., Perez-Torres, M. A., Piner, G., & Sokolovsky, K. V. (2013). Very long baseline polarimetric monitoring at 15 GHz of the TeV blazar Markarian 421. в EPJ Web of Conferences https://doi.org/10.1051/epjconf/20136107004

Vancouver

Lico R, Casadio C, Gómez JL, Giroletti M, Orienti M, Giovannini G и пр. Very long baseline polarimetric monitoring at 15 GHz of the TeV blazar Markarian 421. в EPJ Web of Conferences. 2013 https://doi.org/10.1051/epjconf/20136107004

Author

Lico, R. ; Casadio, C. ; Gómez, J.L. ; Giroletti, M. ; Orienti, M. ; Giovannini, G. ; Blasi, M.G. ; Cotton, W. ; Edwards, P.G. ; Fuhrmann, L. ; Jorstad, S. ; Kino, M. ; Kovalev, Y.Y. ; Krichbaum, T.P. ; Marscher, A. ; Paneque, D. ; Perez-Torres, M.A. ; Piner, G. ; Sokolovsky, K.V. / Very long baseline polarimetric monitoring at 15 GHz of the TeV blazar Markarian 421. EPJ Web of Conferences. 2013.

BibTeX

@inproceedings{9bca2dc4e58749b489883a9ba4768472,
title = "Very long baseline polarimetric monitoring at 15 GHz of the TeV blazar Markarian 421",
abstract = "Thanks to high resolution radio observations it is possible to obtain a direct imaging of the innermost regions of Active Galactic Nuclei; in particular, it is possible to investigate about the jet's morphology and any proper motions, and the time evolution of physical parameters, such as flux densities and spectral index. Furthermore, with the study of the polarization properties, it is possible to obtain important information about the magnetic field structure and the emission mechanisms. In this work we present recent results about the nearby (z=0.031) TeV blazar Mrk 421. We analyzed data obtained with the Very Long Baseline Array (VLBA),both in total and polarized intensity, at twelve epochs (one observation per month from January to December 2011) at 15, 24 and 43 GHz, in the context of a broadband campaign from the radio to gamma-ray. We investigate the inner jet structure on parsec scale through the study of model-fit components for each epoch. At these frequencies the source shows a compact (about 0.1",
author = "R. Lico and C. Casadio and J.L. G{\'o}mez and M. Giroletti and M. Orienti and G. Giovannini and M.G. Blasi and W. Cotton and P.G. Edwards and L. Fuhrmann and S. Jorstad and M. Kino and Y.Y. Kovalev and T.P. Krichbaum and A. Marscher and D. Paneque and M.A. Perez-Torres and G. Piner and K.V. Sokolovsky",
year = "2013",
doi = "10.1051/epjconf/20136107004",
language = "English",
booktitle = "EPJ Web of Conferences",

}

RIS

TY - GEN

T1 - Very long baseline polarimetric monitoring at 15 GHz of the TeV blazar Markarian 421

AU - Lico, R.

AU - Casadio, C.

AU - Gómez, J.L.

AU - Giroletti, M.

AU - Orienti, M.

AU - Giovannini, G.

AU - Blasi, M.G.

AU - Cotton, W.

AU - Edwards, P.G.

AU - Fuhrmann, L.

AU - Jorstad, S.

AU - Kino, M.

AU - Kovalev, Y.Y.

AU - Krichbaum, T.P.

AU - Marscher, A.

AU - Paneque, D.

AU - Perez-Torres, M.A.

AU - Piner, G.

AU - Sokolovsky, K.V.

PY - 2013

Y1 - 2013

N2 - Thanks to high resolution radio observations it is possible to obtain a direct imaging of the innermost regions of Active Galactic Nuclei; in particular, it is possible to investigate about the jet's morphology and any proper motions, and the time evolution of physical parameters, such as flux densities and spectral index. Furthermore, with the study of the polarization properties, it is possible to obtain important information about the magnetic field structure and the emission mechanisms. In this work we present recent results about the nearby (z=0.031) TeV blazar Mrk 421. We analyzed data obtained with the Very Long Baseline Array (VLBA),both in total and polarized intensity, at twelve epochs (one observation per month from January to December 2011) at 15, 24 and 43 GHz, in the context of a broadband campaign from the radio to gamma-ray. We investigate the inner jet structure on parsec scale through the study of model-fit components for each epoch. At these frequencies the source shows a compact (about 0.1

AB - Thanks to high resolution radio observations it is possible to obtain a direct imaging of the innermost regions of Active Galactic Nuclei; in particular, it is possible to investigate about the jet's morphology and any proper motions, and the time evolution of physical parameters, such as flux densities and spectral index. Furthermore, with the study of the polarization properties, it is possible to obtain important information about the magnetic field structure and the emission mechanisms. In this work we present recent results about the nearby (z=0.031) TeV blazar Mrk 421. We analyzed data obtained with the Very Long Baseline Array (VLBA),both in total and polarized intensity, at twelve epochs (one observation per month from January to December 2011) at 15, 24 and 43 GHz, in the context of a broadband campaign from the radio to gamma-ray. We investigate the inner jet structure on parsec scale through the study of model-fit components for each epoch. At these frequencies the source shows a compact (about 0.1

U2 - 10.1051/epjconf/20136107004

DO - 10.1051/epjconf/20136107004

M3 - Conference contribution

BT - EPJ Web of Conferences

ER -

ID: 7412610