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Very-long-baseline interferometry study of the flaring blazar TXS 1508+572 in the early Universe
| Indexado |
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| DOI | 10.1051/0004-6361/202450153 | ||||
| Año | 2024 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
In this case, however, the core region was also affected by the flare as the core shift stays consistent throughout the observations.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Benke, P. | - |
Max Planck Inst Radioastron - Alemania
Julius Maximilians Univ Wurzburg - Alemania Max Planck Institute for Radio Astronomy - Alemania Julius-Maximilians-Universität Würzburg - Alemania |
| 2 | Gokus, A. | - |
Washington Univ St Louis - Estados Unidos
McDonnell Center for the Space Sciences - Estados Unidos |
| 3 | Lisakov, Mikhail | Hombre |
Max Planck Inst Radioastron - Alemania
Pontificia Universidad Católica de Valparaíso - Chile Lebedev Phys Inst - Rusia Max Planck Institute for Radio Astronomy - Alemania P.N. Lebedev Physical Institute of the Russian Academy of Sciences - Rusia |
| 4 | Gurvits, L. I. | - |
Joint Inst VLBI ERIC - Países Bajos
Delft Univ Technol - Países Bajos Joint Institute for VLBI ERIC - Países Bajos Faculteit Luchtvaart- en Ruimtevaarttechniek, TU Delft - Países Bajos |
| 5 | Eppel, F. | - |
Max Planck Inst Radioastron - Alemania
Julius Maximilians Univ Wurzburg - Alemania Max Planck Institute for Radio Astronomy - Alemania Julius-Maximilians-Universität Würzburg - Alemania |
| 6 | Hessdoerfer, J. | - |
Max Planck Inst Radioastron - Alemania
Julius Maximilians Univ Wurzburg - Alemania |
| 6 | HeBdörfer, J. | - |
Max Planck Institute for Radio Astronomy - Alemania
Julius-Maximilians-Universität Würzburg - Alemania |
| 7 | Kadler, M. | Hombre |
Julius Maximilians Univ Wurzburg - Alemania
Julius-Maximilians-Universität Würzburg - Alemania |
| 8 | Kovalev, Y. Y. | Hombre |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania |
| 9 | Rossi, E. | Hombre |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania |
| 10 | Roesch, F. | - |
Max Planck Inst Radioastron - Alemania
Julius Maximilians Univ Wurzburg - Alemania Max Planck Institute for Radio Astronomy - Alemania Julius-Maximilians-Universität Würzburg - Alemania |
| Fuente |
|---|
| Deutsche Forschungsgemeinschaft |
| European Research Council |
| Deutsche Forschungsgemeinschaft (DFG) |
| European Research Council (ERC) |
| International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne |
| Universities of Bonn and Cologne |
| European Union’s Horizon2020 research and innovation programme |
| International Max Planck Research School for Environmental, Cellular and Molecular Microbiology |
| VLBA |
| Agradecimiento |
|---|
| The authors thank the anonymous referee for useful comments that helped to improve the manuscript. The data were obtained at VLBA within the proposal BG281. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work made use of the Swinburne University of Technology software correlator, developed as part of the Australian Major National Research Facilities Programme and operated under license. This research was supported through a PhD grant from the International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne. This publication is part of the M2FINDERS project which has received funding from the European Research Council (ERC) under the European Union's Horizon2020 Research and Innovation Programme (grant agreement No. 101018682). F.E., J.H., M.K., and F.R. acknowledge support from the Deutsche Forschungsgemeinschaft (DFG, grants 447572188, 434448349, 465409577). |
| The authors thank the anonymous referee for useful comments that helped to improve the manuscript. The data were obtained at VLBA within the proposal BG281. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work made use of the Swinburne University of Technology software correlator, developed as part of the Australian Major National Research Facilities Programme and operated under license. This research was supported through a PhD grant from the International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne. This publication is part of the M2FINDERS project which has received funding from the European Research Council (ERC) under the European Union\u2019s Horizon2020 Research and Innovation Programme (grant agreement No. 101018682). F.E., J.H., M.K., and F.R. acknowledge support from the Deutsche Forschungsgemeinschaft (DFG, grants 447572188, 434448349, 465409577). |
