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The latest results from the global mm-VLBI array. / Hodgson, Jeffrey A.; Krichbaum, Thomas P.; Marscher, Alan P.; Jorstad, Svetlana G.; Marti-Vidal, Ivan; Bremer, Michael; Lindqvist, Michael; De Vicente, Pablo; Zensus, Anton.

In: Proceedings of Science, Vol. 2012-October, 2012.

Research output: Contribution to journal › Conference article › peer-review

Harvard

Hodgson, JA, Krichbaum, TP, Marscher, AP, Jorstad, SG, Marti-Vidal, I, Bremer, M, Lindqvist, M, De Vicente, P & Zensus, A 2012, 'The latest results from the global mm-VLBI array', Proceedings of Science, vol. 2012-October.

APA

Hodgson, J. A., Krichbaum, T. P., Marscher, A. P., Jorstad, S. G., Marti-Vidal, I., Bremer, M., Lindqvist, M., De Vicente, P., & Zensus, A. (2012). The latest results from the global mm-VLBI array. Proceedings of Science, 2012-October.

Vancouver

Hodgson JA, Krichbaum TP, Marscher AP, Jorstad SG, Marti-Vidal I, Bremer M et al. The latest results from the global mm-VLBI array. Proceedings of Science. 2012;2012-October.

Author

Hodgson, Jeffrey A. ; Krichbaum, Thomas P. ; Marscher, Alan P. ; Jorstad, Svetlana G. ; Marti-Vidal, Ivan ; Bremer, Michael ; Lindqvist, Michael ; De Vicente, Pablo ; Zensus, Anton. / The latest results from the global mm-VLBI array. In: Proceedings of Science. 2012 ; Vol. 2012-October.

BibTeX

@article{f41e43bd294046d79bd5f95d560053fa,
title = "The latest results from the global mm-VLBI array",
abstract = "The Global mm-VLBI Array (GMVA) is the highest angular resolution imaging interferometer currently available as a common user facility. It is capable of angular resolutions on the order of 40 microarcseconds. Currently 14 stations in the United States and Europe participate in global 3 mm VLBI observations. The GMVA is used for continuum and spectroscopic imaging, probing the central regions of active galaxies and the origin of jets as these regions are typically not observable at longer wavelengths due to synchrotron self-absorption. In early 2012, fringes were detected to the three stations of the Korean VLBI Network (KVN), opening the possibility of extending the baseline coverage of the VLBI array to the East. In these proceedings, we will present recent images from a monitoring program of gamma-ray blazars using the GMVA, including the sources 3C454.3 and 0235+164, and an update of its current status and abilities.",
author = "Hodgson, {Jeffrey A.} and Krichbaum, {Thomas P.} and Marscher, {Alan P.} and Jorstad, {Svetlana G.} and Ivan Marti-Vidal and Michael Bremer and Michael Lindqvist and {De Vicente}, Pablo and Anton Zensus",
note = "Publisher Copyright: Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.; 11th European VLBI Network Symposium and Users Meeting, EVN Symposium 2012 ; Conference date: 09-10-2012 Through 12-10-2012",
year = "2012",
language = "English",
volume = "2012-October",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - The latest results from the global mm-VLBI array

AU - Hodgson, Jeffrey A.

AU - Krichbaum, Thomas P.

AU - Marscher, Alan P.

AU - Jorstad, Svetlana G.

AU - Marti-Vidal, Ivan

AU - Bremer, Michael

AU - Lindqvist, Michael

AU - De Vicente, Pablo

AU - Zensus, Anton

N1 - Publisher Copyright: Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

PY - 2012

Y1 - 2012

N2 - The Global mm-VLBI Array (GMVA) is the highest angular resolution imaging interferometer currently available as a common user facility. It is capable of angular resolutions on the order of 40 microarcseconds. Currently 14 stations in the United States and Europe participate in global 3 mm VLBI observations. The GMVA is used for continuum and spectroscopic imaging, probing the central regions of active galaxies and the origin of jets as these regions are typically not observable at longer wavelengths due to synchrotron self-absorption. In early 2012, fringes were detected to the three stations of the Korean VLBI Network (KVN), opening the possibility of extending the baseline coverage of the VLBI array to the East. In these proceedings, we will present recent images from a monitoring program of gamma-ray blazars using the GMVA, including the sources 3C454.3 and 0235+164, and an update of its current status and abilities.

AB - The Global mm-VLBI Array (GMVA) is the highest angular resolution imaging interferometer currently available as a common user facility. It is capable of angular resolutions on the order of 40 microarcseconds. Currently 14 stations in the United States and Europe participate in global 3 mm VLBI observations. The GMVA is used for continuum and spectroscopic imaging, probing the central regions of active galaxies and the origin of jets as these regions are typically not observable at longer wavelengths due to synchrotron self-absorption. In early 2012, fringes were detected to the three stations of the Korean VLBI Network (KVN), opening the possibility of extending the baseline coverage of the VLBI array to the East. In these proceedings, we will present recent images from a monitoring program of gamma-ray blazars using the GMVA, including the sources 3C454.3 and 0235+164, and an update of its current status and abilities.

UR - http://www.scopus.com/inward/record.url?scp=85052384150&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85052384150

VL - 2012-October

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

T2 - 11th European VLBI Network Symposium and Users Meeting, EVN Symposium 2012

Y2 - 9 October 2012 through 12 October 2012

ER -

ID: 88383735