Author: "Ros, E." / Publication Year Range: Last 50 years / Publisher: edp sciences - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Ros, E."' showing total 279 results

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279 results on '"Ros, E."'

1. Very-long-baseline interferometry study of the flaring blazar TXS 1508+572 in the early Universe

Author: Benke, P., primary, Gokus, A., additional, Lisakov, M., additional, Gurvits, L.I., additional, Eppel, F., additional, Heßdorfer, J., additional, Kadler, M., additional, Kovalev, Y., additional, Ros, E., additional, and Rosch, F., additional
Published: 2024
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2. Ordered magnetic fields around the 3C 84 central black hole

Author: Paraschos, G. F., primary, Kim, J.-Y., additional, Wielgus, M., additional, Röder, J., additional, Krichbaum, T. P., additional, Ros, E., additional, Agudo, I., additional, Myserlis, I., additional, Moscibrodzka, M., additional, Traianou, E., additional, Zensus, J. A., additional, Blackburn, L., additional, Chan, C.-K., additional, Issaoun, S., additional, Janssen, M., additional, Johnson, M. D., additional, Fish, V. L., additional, Akiyama, K., additional, Alberdi, A., additional, Alef, W., additional, Algaba, J. C., additional, Anantua, R., additional, Asada, K., additional, Azulay, R., additional, Bach, U., additional, Baczko, A.-K., additional, Ball, D., additional, Baloković, M., additional, Barrett, J., additional, Bauböck, M., additional, Benson, B. A., additional, Bintley, D., additional, Blundell, R., additional, Bouman, K. L., additional, Bower, G. C., additional, Boyce, H., additional, Bremer, M., additional, Brinkerink, C. D., additional, Brissenden, R., additional, Britzen, S., additional, Broderick, A. E., additional, Broguiere, D., additional, Bronzwaer, T., additional, Bustamante, S., additional, Byun, D.-Y., additional, Carlstrom, J. E., additional, Ceccobello, C., additional, Chael, A., additional, Chang, D. O., additional, Chatterjee, K., additional, Chatterjee, S., additional, Chen, M. T., additional, Chen, Y., additional, Cheng, X., additional, Cho, I., additional, Christian, P., additional, Conroy, N. S., additional, Conway, J. E., additional, Cordes, J. M., additional, Crawford, T. M., additional, Crew, G. B., additional, Cruz-Osorio, A., additional, Cui, Y., additional, Dahale, R., additional, Davelaar, J., additional, De Laurentis, M., additional, Deane, R., additional, Dempsey, J., additional, Desvignes, G., additional, Dexter, J., additional, Dhruv, V., additional, Doeleman, S. S., additional, Dougal, S., additional, Dzib, S. A., additional, Eatough, R. P., additional, Emami, R., additional, Falcke, H., additional, Farah, J., additional, Fomalont, E., additional, Ford, H. A., additional, Foschi, M., additional, Fraga-Encinas, R., additional, Freeman, W. T., additional, Friberg, P., additional, Fromm, C. M., additional, Fuentes, A., additional, Galison, P., additional, Gammie, C. F., additional, García, R., additional, Gentaz, O., additional, Georgiev, B., additional, Goddi, C., additional, Gold, R., additional, Gómez-Ruiz, A. I., additional, Gómez, J. L., additional, Gu, M., additional, Gurwell, M., additional, Hada, K., additional, Haggard, D., additional, Haworth, K., additional, Hecht, M. H., additional, Hesper, R., additional, Heumann, D., additional, Ho, L. C., additional, Ho, P., additional, Honma, M., additional, Huang, C. L., additional, Huang, L., additional, Hughes, D. H., additional, Ikeda, S., additional, Impellizzeri, C. M. V., additional, Inoue, M., additional, James, D. J., additional, Jannuzi, B. T., additional, Jeter, B., additional, Jaing, W., additional, Jiménez-Rosales, A., additional, Jorstad, S., additional, Joshi, A. V., additional, Jung, T., additional, Karami, M., additional, Karuppusamy, R., additional, Kawashima, T., additional, Keating, G. K., additional, Kettenis, M., additional, Kim, D.-J., additional, Kim, J., additional, Kino, M., additional, Koay, J. Y., additional, Kocherlakota, P., additional, Kofuji, Y., additional, Koch, P. M., additional, Koyama, S., additional, Kramer, C., additional, Kramer, J. A., additional, Kramer, M., additional, Kuo, C.-Y., additional, La Bella, N., additional, Lauer, T. R., additional, Lee, D., additional, Lee, S.-S., additional, Leung, P. K., additional, Levis, A., additional, Li, Z., additional, Lico, R., additional, Lindahl, G., additional, Lindqvist, M., additional, Lisakov, M., additional, Liu, J., additional, Liu, K., additional, Liuzzo, E., additional, Lo, W.-P., additional, Lobanov, A. P., additional, Loinard, L., additional, Lonsdale, C. J., additional, Lowitz, A. E., additional, Lu, R.-S., additional, MacDonald, N. R., additional, Mao, J., additional, Marchili, N., additional, Markoff, S., additional, Marrone, D. P., additional, Marscher, A. P., additional, Martí-Vidal, I., additional, Matsushita, S., additional, Matthews, L. D., additional, Medeiros, L., additional, Menten, K. M., additional, Michalik, D., additional, Mizuno, I., additional, Mizuno, Y., additional, Moran, J. M., additional, Moriyama, K., additional, Mulaudzi, W., additional, Müller, C., additional, Müller, H., additional, Mus, A., additional, Musoke, G., additional, Nadolski, A., additional, Nagai, H., additional, Nagar, N. M., additional, Nakamura, M., additional, Narayanan, G., additional, Natarajan, I., additional, Nathanail, A., additional, Navarro Fuentes, S., additional, Neilsen, J., additional, Neri, R., additional, Ni, C., additional, Noutsos, A., additional, Nowak, M. A., additional, Oh, J., additional, Okino, H., additional, Olivares, H., additional, Ortiz-León, G. N., additional, Oyama, T., additional, Özel, F., additional, Palumbo, D. C. M., additional, Park, J., additional, Parsons, H., additional, Patel, N., additional, Pen, U.-L., additional, Piétu, V., additional, Plambeck, R., additional, PopStefanija, A., additional, Porth, O., additional, Pötzl, F. M., additional, Prather, B., additional, Preciado-López, J. A., additional, Psaltis, D., additional, Pu, H.-Y., additional, Ramakrishnan, V., additional, Rao, R., additional, Rawlings, M. G., additional, Raymond, A. W., additional, Rezzolla, L., additional, Ricarte, A., additional, Ripperda, B., additional, Roelofs, F., additional, Rogers, A., additional, Romero-Cañizales, C., additional, Roshanineshat, A., additional, Rottmann, H., additional, Roy, A. L., additional, Ruiz, I., additional, Ruszczyk, C., additional, Rygl, K. L. J., additional, Sánchez, S., additional, Sánchez-Argüelles, D., additional, Sánchez-Portal, M., additional, Sasada, M., additional, Satapathy, K., additional, Savolainen, T., additional, Schloerb, F. P., additional, Schonfeld, J., additional, Schuster, K., additional, Shao, L., additional, Shen, Z., additional, Small, D., additional, Sohn, B. W., additional, SooHoo, J., additional, Sosapanta Salas, L. D., additional, Souccar, K., additional, Sun, H., additional, Tazaki, F., additional, Tetarenko, A. J., additional, Tiede, P., additional, Tilanus, R. P. J., additional, Titus, M., additional, Torne, P., additional, Toscano, T., additional, Trent, T., additional, Trippe, S., additional, Turk, M., additional, van Bemmel, I., additional, van Langevelde, H. J., additional, van Rossum, D. R., additional, Vos, J., additional, Wagner, J., additional, Ward-Thompson, D., additional, Wardle, J., additional, Washington, J. E., additional, Weintroub, J., additional, Wharton, R., additional, Wiik, K., additional, Witzel, G., additional, Wondrak, M. F., additional, Wong, G. N., additional, Wu, Q., additional, Yadlapalli, N., additional, Yamaguchi, P., additional, Yfantis, A., additional, Yoon, D., additional, Young, A., additional, Young, K., additional, Younsi, Z., additional, Yu, W., additional, Yuan, F., additional, Yuan, Y.-F., additional, Zhang, S., additional, Zhao, G. Y., additional, and Zhao, S.-S., additional
Published: 2024
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3. First very long baseline interferometry detection of Fornax A.

Author: Paraschos, G. F., Wielgus, M., Benke, P., Mpisketzis, V., Rösch, F., Dasyra, K., Ros, E., Kadler, M., Ojha, R., Edwards, P. G., Hyland, L., Quick, J. F. H., and Weston, S.
Subjects: VERY long baseline interferometry, ASTROPHYSICAL jets, ACTIVE galactic nuclei, ACTIVE galaxies, BRIGHTNESS temperature
Abstract: Radio galaxies harbouring jetted active galactic nuclei are a frequent target of very long baseline interferometry (VLBI) because they play an essential role in our exploration of how jets form and propagate. Hence, only a few have not yet been detected with VLBI; Fornax A was one of the most famous examples. Here we present the first detection of the compact core region of Fornax A with VLBI. At 8.4 GHz the faint core is consistent with an unresolved point source. We constrained its flux density to be S0 = 47.5 − 62.3 mJy and its diameter to be D0min ≤ 70 μas. The high values of the measured brightness temperature (TB ≳ 1011 K) imply that the observed radiation is of non-thermal origin, likely associated with the synchrotron emission from the active galactic nucleus. We also investigated the possibility of a second radio source being present within the field of view. Adding a second Gaussian component to the geometrical model fit does not significantly improve the quality of the fit, and we therefore, conclude that our detection corresponds to the compact core of Fornax A. Analysis of the non-trivial closure phases provides evidence for the detection of a more extended flux density, on the angular scale of ∼4000 μas. Finally, the fractional circular polarisation of the core is consistent with zero, with a conservative upper limit being mcirc ≤ 4%. [ABSTRACT FROM AUTHOR]
Published: 2024
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4. TELAMON: Effelsberg monitoring of AGN jets with very-high-energy astroparticle emission. I. Program description and sample characterization

Author: Eppel, F., primary, Kadler, M., additional, Heßdörfer, J., additional, Benke, P., additional, Debbrecht, L., additional, Eich, J., additional, Gokus, A., additional, Hämmerich, S., additional, Kirchner, D., additional, Paraschos, G. F., additional, Rösch, F., additional, Schulga, W., additional, Sinapius, J., additional, Weber, P., additional, Bach, U., additional, Dorner, D., additional, Edwards, P. G., additional, Giroletti, M., additional, Kraus, A., additional, Hervet, O., additional, Koyama, S., additional, Krichbaum, T. P., additional, Mannheim, K., additional, Ros, E., additional, Zacharias, M., additional, and Zensus, J. A., additional
Published: 2024
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5. TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry. III. First-epoch S band images

Author: Benke, P., primary, Rösch, F., additional, Ros, E., additional, Kadler, M., additional, Ojha, R., additional, Edwards, P. G., additional, Horiuchi, S., additional, Hyland, L. J., additional, Phillips, C., additional, Quick, J. F. H., additional, Stevens, J., additional, Tzioumis, A. K., additional, and Weston, S., additional
Published: 2023
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6. From binary to singular: The AGN PSO J334.2028+1.4075 under the high-resolution scope

Author: Benke, P., primary, Gabányi, K. É., additional, Frey, S., additional, An, T., additional, Gurvits, L. I., additional, Kun, E., additional, Mohan, P., additional, Paragi, Z., additional, and Ros, E., additional
Published: 2023
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7. Radio jet precession in M 81*

Author: von Fellenberg, S. D., primary, Janssen, M., additional, Davelaar, J., additional, Zajaček, M., additional, Britzen, S., additional, Falcke, H., additional, Körding, E., additional, and Ros, E., additional
Published: 2023
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8. Time variability of the core-shift effect in the blazar 3C 454.3

Author: Chamani, W., primary, Savolainen, T., additional, Ros, E., additional, Kovalev, Y.Y., additional, Wiik, K., additional, Lähteenmäki, A., additional, Tornikoski, M., additional, and Tammi, J., additional
Published: 2023
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9. General relativistic effects and the near-infrared and X-ray variability of Sgr A* I

Author: von Fellenberg, S. D., primary, Witzel, G., additional, Bauböck, M., additional, Chung, H.-H., additional, Aimar, N., additional, Bordoni, M., additional, Drescher, A., additional, Eisenhauer, F., additional, Genzel, R., additional, Gillessen, S., additional, Marchili, N., additional, Paumard, T., additional, Perrin, G., additional, Ott, T., additional, Ribeiro, D. C., additional, Ros, E., additional, Vincent, F., additional, Widmann, F., additional, Willner, S. P., additional, and Anton Zensus, J., additional
Published: 2023
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10. Jet kinematics in the transversely stratified jet of 3C 84

Author: Paraschos, G. F., primary, Krichbaum, T. P., additional, Kim, J.-Y., additional, Hodgson, J. A., additional, Oh, J., additional, Ros, E., additional, Zensus, J. A., additional, Marscher, A. P., additional, Jorstad, S. G., additional, Gurwell, M. A., additional, Lähteenmäki, A., additional, Tornikoski, M., additional, Kiehlmann, S., additional, and Readhead, A. C. S., additional
Published: 2022
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11. Observing the inner parsec-scale region of candidate neutrino-emitting blazars

Author: Nanci, C., primary, Giroletti, M., additional, Orienti, M., additional, Migliori, G., additional, Moldón, J., additional, Garrappa, S., additional, Kadler, M., additional, Ros, E., additional, Buson, S., additional, An, T., additional, Pérez-Torres, M. A., additional, D’Ammando, F., additional, Mohan, P., additional, Agudo, I., additional, Sohn, B. W., additional, Castro-Tirado, A. J., additional, and Zhang, Y., additional
Published: 2022
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12. Dual-high-frequency VLBI study of blazar-jet brightness-temperature gradients and collimation profiles

Author: Burd, P. R., primary, Kadler, M., additional, Mannheim, K., additional, Baczko, A.-K., additional, Ringholz, J., additional, and Ros, E., additional
Published: 2022
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13. Ambilateral collimation study of the twin-jets in NGC 1052

Author: Baczko, A.-K., primary, Ros, E., additional, Kadler, M., additional, Fromm, C. M., additional, Boccardi, B., additional, Perucho, M., additional, Krichbaum, T. P., additional, Burd, P. R., additional, and Zensus, J. A., additional
Published: 2022
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14. Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron

Author: Pötzl, F. M., primary, Lobanov, A. P., additional, Ros, E., additional, Gómez, J. L., additional, Bruni, G., additional, Bach, U., additional, Fuentes, A., additional, Gurvits, L. I., additional, Jauncey, D. L., additional, Kovalev, Y. Y., additional, Kravchenko, E. V., additional, Lisakov, M. M., additional, Savolainen, T., additional, Sokolovsky, K. V., additional, and Zensus, J. A., additional
Published: 2021
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15. Jet collimation in NGC 315 and other nearby AGN

Author: Boccardi, B., primary, Perucho, M., additional, Casadio, C., additional, Grandi, P., additional, Macconi, D., additional, Torresi, E., additional, Pellegrini, S., additional, Krichbaum, T. P., additional, Kadler, M., additional, Giovannini, G., additional, Karamanavis, V., additional, Ricci, L., additional, Madika, E., additional, Bach, U., additional, Ros, E., additional, Giroletti, M., additional, and Zensus, J. A., additional
Published: 2021
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16. Multiband RadioAstron space VLBI imaging of the jet in quasar S5 0836+710

Author: Ministerio de Economía y Competitividad (España), European Commission, Generalitat Valenciana, Academy of Finland, Russian Science Foundation, Alexander von Humboldt Foundation, Ministerio de Economía, Industria y Competitividad (España), European Cooperation in Science and Technology, Vega-García, L., Lobanov, A.P., Perucho, M., Bruni, G., Ros, E., Anderson, J. M., Agudo, Iván, Davis, R., Gómez, José L., Kovalev, Y. Y., Krichbaum, Thomas P., Lisakov, Mikhail M., Savolainen, T., Schinzel, F. K., Zensus, J. A., Ministerio de Economía y Competitividad (España), European Commission, Generalitat Valenciana, Academy of Finland, Russian Science Foundation, Alexander von Humboldt Foundation, Ministerio de Economía, Industria y Competitividad (España), European Cooperation in Science and Technology, Vega-García, L., Lobanov, A.P., Perucho, M., Bruni, G., Ros, E., Anderson, J. M., Agudo, Iván, Davis, R., Gómez, José L., Kovalev, Y. Y., Krichbaum, Thomas P., Lisakov, Mikhail M., Savolainen, T., Schinzel, F. K., and Zensus, J. A.
Abstract: Context Detailed studies of relativistic jets in active galactic nuclei (AGN) require high-fidelity imaging at the highest possible resolution. This can be achieved using very long baseline interferometry (VLBI) at radio frequencies, combining worldwide (global) VLBI arrays of radio telescopes with a space-borne antenna on board a satellite. Aims. We present multiwavelength images made of the radio emission in the powerful quasar S5 0836+710, obtained using a global VLBI array and the antenna Spektr-R of the RadioAstron mission of the Russian Space Agency, with the goal of studying the internal structure and physics of the relativistic jet in this object. Methods. The RadioAstron observations at wavelengths of 18 cm, 6 cm, and 1.3 cm are part of the Key Science Program for imaging radio emission in strong AGN. The internal structure of the jet is studied by analyzing transverse intensity profiles and modeling the structural patterns developing in the flow. Results. The RadioAstron images reveal a wealth of structural detail in the jet of S5 0836+710 on angular scales ranging from 0.02 mas to 200 mas. Brightness temperatures in excess of 1013 K are measured in the jet, requiring Doppler factors of 100 for reconciling them with the inverse Compton limit. Several oscillatory patterns are identified in the ridge line of the jet and can be explained in terms of the Kelvin Helmholtz (KH) instability. The oscillatory patterns are interpreted as the surface and body wavelengths of the helical mode of the KH instability. The interpretation provides estimates of the jet Mach number and of the ratio of the jet to the ambient density, which are found to be Mj 12 and 0:33. The ratio of the jet to the ambient density should be conservatively considered an upper limit because its estimate relies on approximations. © L. Vega-García et al. 2020
Published: 2020

17. SYMBA: An end-to-end VLBI synthetic data generation pipeline: Simulating Event Horizon Telescope observations of M 87

Author: Academy of Finland, European Commission, Alexander von Humboldt Foundation, John Templeton Foundation, China Scholarship Council, Comisión Nacional de Investigación Científica y Tecnológica (Chile), Consejo Nacional de Ciencia y Tecnología (México), European Research Council, Generalitat Valenciana, Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Gordon and Betty Moore Foundation, Istituto Nazionale di Fisica Nucleare, Japanese Government, Japan Society for the Promotion of Science, Chinese Academy of Sciences, Max Planck Society, Ministry of Science and Technology (Taiwan), National Aeronautics and Space Administration (US), National Science Foundation (US), National Natural Science Foundation of China, Natural Sciences and Engineering Research Council of Canada, National Research Foundation of Korea, Netherlands Organization for Scientific Research, National Research Foundation (South Africa), Russian Science Foundation, Ministero dell'Istruzione, dell'Università e della Ricerca, Roelofs, Freek, Janssen, M., Natarajan, I., Deane, Roger, Davelaar, J., Olivares, H., Porth, O., Paine, S. N., Bouman, Katherine L., Tilanus, R. P. J., van Bemmel, I. M., Schuster, K., Goddi, Ciriaco, Broderick, Avery E., Koay, J.Y, Ramakrishnan, V., Lobanov, A.P., Rawlings, M. G., Asada, Keiichi, Sánchez-Arguelles, D., Wong, G. N., Kim, J., Baloković, M., Roshanineshat, A., Ball, D., Hesper, R., Chatterjee, K., Titus, Michael A., Akiyama, Kazunori, Ruszczyk, Chester A., Inoue, M., Lee, S., Sasada, Mahito, Broguiere, D., Tazaki, F., Conway, J.E, Weintroub, Jonathan, Savolainen, T., Karuppusamy, R., MacDonald, N.R., Wagner, J., Young, K., Won Sohn, B., Noutsos, A., Medeiros, L., Barrett, John, van Langevelde, H. J., Zhao, Shan-Shan, Koch, P. M., Gentaz, O., Alberdi, Antxón, Ortiz-León, G. N., Wardle, J., Li, Z., Yuan, Y., Fraga-Encinas, R., Wu, Q., Fomalont, E., Falcke, H., Hada, Kazuhiro, Brinkerink, C. D., Young, A., Mao, J., Neri, Roberto, Bower, G.C., Ho, P., Chan, C., Zhao, G., Rogers, A., Patel, Nimesh, Carlstrom, J.E, Blackburn, Lindy, Christian, P., Mizuno, I., Kawashima, T., Preciado-López, J.A, Boland, W., Rottmann, H., Bremer, M., Ikeda, S., Chen, M., Jannuzi, B.T, Bronzwaer, T., James, D.J, Müller, C., Kino, Motoki, Dexter, J., Huang, C. L., Chael, A., Ni, C., Rezzolla, L., Dempsey, J., Kramer, C., Gammie, C.F, Cho, I., Trent, T., Rygl, K. L. J., Gómez, José L., Gu, M., Cui, Y., Gurwell, M., Piétu, V., Markoff, S., Shen, Z., De Laurentis, M., van Rossum, D. R., Desvignes, Gregory, Li, Y., Georgiev, B., Keating, G.K, Liu, K., Friberg, P., Lico, Rocco, Psaltis, D., Menten, K. M., Huang, L., Kuo, C., Galison, P., Ripperda, B., Toma, K., Marrone, Daniel P., Honma, M., Moscibrodzka, M., Jung, T., Gold, R., Baczko, A., Wex, N., Johnson, M. D., Ho, L. C., Younsi, Z., Liuzzo, Elisabetta, Jeter, B., Kramer, M., Small, D., Pen, U., Lauer, T.R, Byun, D., Jorstad, S., Traianou, E., Alef, W., Kettenis, Mark, Okino, H., Krichbaum, Thomas P., Prather, B., Lu, R., Wharton, R., Brissenden, R., Loinard, Laurent, Matthews, L.D., Koyama, S., Fish, Vincent L., Chatterjee, S., Martí-Vidal, Iván, Lo, W., Moriyama, K., Zensus, J. A., Sánchez, S., Cordes, J.M., Fromm, Christian M., Lonsdale, Colin J., Azulay, Rebecca, Mizuno, Y., Rose, M., Marscher, Alan P., Ros, E., Bintley, D., Shao, L., Narayanan, Gopal, Matsushita, S., Britzen, S., Doeleman, Sheperd S., Nakamura, M., SooHoo, J., Palumbo, Daniel C. M., Morán, J.M., Issaoun, Sara, García, R., Oyama, T., Nagai, H., PopStefanija, A., Chen, Y., Wielgus, Maciek, Hecht, M.H, Nagar, Neil M., Jiang, Wu, Narayan, Ramesh, Torne, P., Pesce, Dominic W., Tsuda, S., Trippe, S., Crew, Geoffrey B., Yuan, F., Raymond, Alexander W., Tiede, Paul, Özel, F., Eatough, R. P., Hughes, D. H., Rao, R., Zhu, Z., Ryan, B. R., Plambeck, R., Lindqvist, M., Karami, M., Roy, A.L., Schloerb, F. P., Pu, H., Academy of Finland, European Commission, Alexander von Humboldt Foundation, John Templeton Foundation, China Scholarship Council, Comisión Nacional de Investigación Científica y Tecnológica (Chile), Consejo Nacional de Ciencia y Tecnología (México), European Research Council, Generalitat Valenciana, Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Gordon and Betty Moore Foundation, Istituto Nazionale di Fisica Nucleare, Japanese Government, Japan Society for the Promotion of Science, Chinese Academy of Sciences, Max Planck Society, Ministry of Science and Technology (Taiwan), National Aeronautics and Space Administration (US), National Science Foundation (US), National Natural Science Foundation of China, Natural Sciences and Engineering Research Council of Canada, National Research Foundation of Korea, Netherlands Organization for Scientific Research, National Research Foundation (South Africa), Russian Science Foundation, Ministero dell'Istruzione, dell'Università e della Ricerca, Roelofs, Freek, Janssen, M., Natarajan, I., Deane, Roger, Davelaar, J., Olivares, H., Porth, O., Paine, S. N., Bouman, Katherine L., Tilanus, R. P. J., van Bemmel, I. M., Schuster, K., Goddi, Ciriaco, Broderick, Avery E., Koay, J.Y, Ramakrishnan, V., Lobanov, A.P., Rawlings, M. G., Asada, Keiichi, Sánchez-Arguelles, D., Wong, G. N., Kim, J., Baloković, M., Roshanineshat, A., Ball, D., Hesper, R., Chatterjee, K., Titus, Michael A., Akiyama, Kazunori, Ruszczyk, Chester A., Inoue, M., Lee, S., Sasada, Mahito, Broguiere, D., Tazaki, F., Conway, J.E, Weintroub, Jonathan, Savolainen, T., Karuppusamy, R., MacDonald, N.R., Wagner, J., Young, K., Won Sohn, B., Noutsos, A., Medeiros, L., Barrett, John, van Langevelde, H. J., Zhao, Shan-Shan, Koch, P. M., Gentaz, O., Alberdi, Antxón, Ortiz-León, G. N., Wardle, J., Li, Z., Yuan, Y., Fraga-Encinas, R., Wu, Q., Fomalont, E., Falcke, H., Hada, Kazuhiro, Brinkerink, C. D., Young, A., Mao, J., Neri, Roberto, Bower, G.C., Ho, P., Chan, C., Zhao, G., Rogers, A., Patel, Nimesh, Carlstrom, J.E, Blackburn, Lindy, Christian, P., Mizuno, I., Kawashima, T., Preciado-López, J.A, Boland, W., Rottmann, H., Bremer, M., Ikeda, S., Chen, M., Jannuzi, B.T, Bronzwaer, T., James, D.J, Müller, C., Kino, Motoki, Dexter, J., Huang, C. L., Chael, A., Ni, C., Rezzolla, L., Dempsey, J., Kramer, C., Gammie, C.F, Cho, I., Trent, T., Rygl, K. L. J., Gómez, José L., Gu, M., Cui, Y., Gurwell, M., Piétu, V., Markoff, S., Shen, Z., De Laurentis, M., van Rossum, D. R., Desvignes, Gregory, Li, Y., Georgiev, B., Keating, G.K, Liu, K., Friberg, P., Lico, Rocco, Psaltis, D., Menten, K. M., Huang, L., Kuo, C., Galison, P., Ripperda, B., Toma, K., Marrone, Daniel P., Honma, M., Moscibrodzka, M., Jung, T., Gold, R., Baczko, A., Wex, N., Johnson, M. D., Ho, L. C., Younsi, Z., Liuzzo, Elisabetta, Jeter, B., Kramer, M., Small, D., Pen, U., Lauer, T.R, Byun, D., Jorstad, S., Traianou, E., Alef, W., Kettenis, Mark, Okino, H., Krichbaum, Thomas P., Prather, B., Lu, R., Wharton, R., Brissenden, R., Loinard, Laurent, Matthews, L.D., Koyama, S., Fish, Vincent L., Chatterjee, S., Martí-Vidal, Iván, Lo, W., Moriyama, K., Zensus, J. A., Sánchez, S., Cordes, J.M., Fromm, Christian M., Lonsdale, Colin J., Azulay, Rebecca, Mizuno, Y., Rose, M., Marscher, Alan P., Ros, E., Bintley, D., Shao, L., Narayanan, Gopal, Matsushita, S., Britzen, S., Doeleman, Sheperd S., Nakamura, M., SooHoo, J., Palumbo, Daniel C. M., Morán, J.M., Issaoun, Sara, García, R., Oyama, T., Nagai, H., PopStefanija, A., Chen, Y., Wielgus, Maciek, Hecht, M.H, Nagar, Neil M., Jiang, Wu, Narayan, Ramesh, Torne, P., Pesce, Dominic W., Tsuda, S., Trippe, S., Crew, Geoffrey B., Yuan, F., Raymond, Alexander W., Tiede, Paul, Özel, F., Eatough, R. P., Hughes, D. H., Rao, R., Zhu, Z., Ryan, B. R., Plambeck, R., Lindqvist, M., Karami, M., Roy, A.L., Schloerb, F. P., and Pu, H.
Abstract: Context. Realistic synthetic observations of theoretical source models are essential for our understanding of real observational data. In using synthetic data, one can verify the extent to which source parameters can be recovered and evaluate how various data corruption effects can be calibrated. These studies are the most important when proposing observations of new sources, in the characterization of the capabilities of new or upgraded instruments, and when verifying model-based theoretical predictions in a direct comparison with observational data. Aims. We present the SYnthetic Measurement creator for long Baseline Arrays (SYMBA), a novel synthetic data generation pipeline for Very Long Baseline Interferometry (VLBI) observations. SYMBA takes into account several realistic atmospheric, instrumental, and calibration effects. Methods. We used SYMBA to create synthetic observations for the Event Horizon Telescope (EHT), a millimetre VLBI array, which has recently captured the first image of a black hole shadow. After testing SYMBA with simple source and corruption models, we study the importance of including all corruption and calibration effects, compared to the addition of thermal noise only. Using synthetic data based on two example general relativistic magnetohydrodynamics (GRMHD) model images of M 87, we performed case studies to assess the image quality that can be obtained with the current and future EHT array for different weather conditions. Results. Our synthetic observations show that the effects of atmospheric and instrumental corruptions on the measured visibilities are significant. Despite these effects, we demonstrate how the overall structure of our GRMHD source models can be recovered robustly with the EHT2017 array after performing calibration steps, which include fringe fitting, a priori amplitude and network calibration, and self-calibration. With the planned addition of new stations to the EHT array in the coming years, images could be reconstr
Published: 2020

18. Sub-milliarcsecond imaging of a bright flare and ejection event in the extragalactic jet 3C 111

Author: Schulz, R., primary, Kadler, M., additional, Ros, E., additional, Perucho, M., additional, Krichbaum, T. P., additional, Agudo, I., additional, Beuchert, T., additional, Lindqvist, M., additional, Mannheim, K., additional, Wilms, J., additional, and Zensus, J. A., additional
Published: 2020
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19. Multiband RadioAstron space VLBI imaging of the jet in quasar S5 0836+710

Author: Vega-García, L., primary, Lobanov, A. P., additional, Perucho, M., additional, Bruni, G., additional, Ros, E., additional, Anderson, J. M., additional, Agudo, I., additional, Davis, R., additional, Gómez, J. L., additional, Kovalev, Y. Y., additional, Krichbaum, T. P., additional, Lisakov, M., additional, Savolainen, T., additional, Schinzel, F. K., additional, and Zensus, J. A., additional
Published: 2020
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20. γ-ray emission in radio galaxies under the VLBI scope

Author: Angioni, R., primary, Ros, E., additional, Kadler, M., additional, Ojha, R., additional, Müller, C., additional, Edwards, P. G., additional, Burd, P. R., additional, Carpenter, B., additional, Dutka, M. S., additional, Gulyaev, S., additional, Hase, H., additional, Horiuchi, S., additional, Krauß, F., additional, Lovell, J. E. J., additional, Natusch, T., additional, Phillips, C., additional, Plötz, C., additional, Quick, J. F. H., additional, Rösch, F., additional, Schulz, R., additional, Stevens, J., additional, Tzioumis, A. K., additional, Weston, S., additional, Wilms, J., additional, and Zensus, J. A., additional
Published: 2020
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21. SYMBA: An end-to-end VLBI synthetic data generation pipeline

Author: Roelofs, F., primary, Janssen, M., additional, Natarajan, I., additional, Deane, R., additional, Davelaar, J., additional, Olivares, H., additional, Porth, O., additional, Paine, S. N., additional, Bouman, K. L., additional, Tilanus, R. P. J., additional, van Bemmel, I. M., additional, Falcke, H., additional, Akiyama, K., additional, Alberdi, A., additional, Alef, W., additional, Asada, K., additional, Azulay, R., additional, Baczko, A., additional, Ball, D., additional, Baloković, M., additional, Barrett, J., additional, Bintley, D., additional, Blackburn, L., additional, Boland, W., additional, Bower, G. C., additional, Bremer, M., additional, Brinkerink, C. D., additional, Brissenden, R., additional, Britzen, S., additional, Broderick, A. E., additional, Broguiere, D., additional, Bronzwaer, T., additional, Byun, D., additional, Carlstrom, J. E., additional, Chael, A., additional, Chan, C., additional, Chatterjee, S., additional, Chatterjee, K., additional, Chen, M., additional, Chen, Y., additional, Cho, I., additional, Christian, P., additional, Conway, J. E., additional, Cordes, J. M., additional, Crew, G. B., additional, Cui, Y., additional, De Laurentis, M., additional, Dempsey, J., additional, Desvignes, G., additional, Dexter, J., additional, Doeleman, S. S., additional, Eatough, R. P., additional, Fish, V. L., additional, Fomalont, E., additional, Fraga-Encinas, R., additional, Friberg, P., additional, Fromm, C. M., additional, Gómez, J. L., additional, Galison, P., additional, Gammie, C. F., additional, García, R., additional, Gentaz, O., additional, Georgiev, B., additional, Goddi, C., additional, Gold, R., additional, Gu, M., additional, Gurwell, M., additional, Hada, K., additional, Hecht, M. H., additional, Hesper, R., additional, Ho, L. C., additional, Ho, P., additional, Honma, M., additional, Huang, C. L., additional, Huang, L., additional, Hughes, D. H., additional, Ikeda, S., additional, Inoue, M., additional, Issaoun, S., additional, James, D. J., additional, Jannuzi, B. T., additional, Jeter, B., additional, Jiang, W., additional, Johnson, M. D., additional, Jorstad, S., additional, Jung, T., additional, Karami, M., additional, Karuppusamy, R., additional, Kawashima, T., additional, Keating, G. K., additional, Kettenis, M., additional, Kim, J., additional, Kino, M., additional, Koay, J. Y., additional, Koch, P. M., additional, Koyama, S., additional, Kramer, M., additional, Kramer, C., additional, Krichbaum, T. P., additional, Kuo, C., additional, Lauer, T. R., additional, Lee, S., additional, Li, Y., additional, Li, Z., additional, Lindqvist, M., additional, Lico, R., additional, Liu, K., additional, Liuzzo, E., additional, Lo, W., additional, Lobanov, A. P., additional, Loinard, L., additional, Lonsdale, C., additional, Lu, R., additional, MacDonald, N. R., additional, Mao, J., additional, Markoff, S., additional, Marrone, D. P., additional, Marscher, A. P., additional, Martí-Vidal, I., additional, Matsushita, S., additional, Matthews, L. D., additional, Medeiros, L., additional, Menten, K. M., additional, Mizuno, Y., additional, Mizuno, I., additional, Moran, J. M., additional, Moriyama, K., additional, Moscibrodzka, M., additional, Müller, C., additional, Nagai, H., additional, Nagar, N. M., additional, Nakamura, M., additional, Narayan, R., additional, Narayanan, G., additional, Neri, R., additional, Ni, C., additional, Noutsos, A., additional, Okino, H., additional, Ortiz-León, G. N., additional, Oyama, T., additional, Özel, F., additional, Palumbo, D. C. M., additional, Patel, N., additional, Pen, U., additional, Pesce, D. W., additional, Piétu, V., additional, Plambeck, R., additional, PopStefanija, A., additional, Prather, B., additional, Preciado-López, J. A., additional, Psaltis, D., additional, Pu, H., additional, Ramakrishnan, V., additional, Rao, R., additional, Rawlings, M. G., additional, Raymond, A. W., additional, Rezzolla, L., additional, Ripperda, B., additional, Rogers, A., additional, Ros, E., additional, Rose, M., additional, Roshanineshat, A., additional, Rottmann, H., additional, Roy, A. L., additional, Ruszczyk, C., additional, Ryan, B. R., additional, Rygl, K. L. J., additional, Sánchez, S., additional, Sánchez-Arguelles, D., additional, Sasada, M., additional, Savolainen, T., additional, Schloerb, F. P., additional, Schuster, K., additional, Shao, L., additional, Shen, Z., additional, Small, D., additional, Won Sohn, B., additional, SooHoo, J., additional, Tazaki, F., additional, Tiede, P., additional, Titus, M., additional, Toma, K., additional, Torne, P., additional, Traianou, E., additional, Trent, T., additional, Trippe, S., additional, Tsuda, S., additional, van Langevelde, H. J., additional, van Rossum, D. R., additional, Wagner, J., additional, Wardle, J., additional, Weintroub, J., additional, Wex, N., additional, Wharton, R., additional, Wielgus, M., additional, Wong, G. N., additional, Wu, Q., additional, Young, A., additional, Young, K., additional, Younsi, Z., additional, Yuan, F., additional, Yuan, Y., additional, Zensus, J. A., additional, Zhao, G., additional, Zhao, S., additional, and Zhu, Z., additional
Published: 2020
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22. Localizing the γ-ray emitting region in the blazar TXS 2013+370

Author: Traianou, E., primary, Krichbaum, T. P., additional, Boccardi, B., additional, Angioni, R., additional, Rani, B., additional, Liu, J., additional, Ros, E., additional, Bach, U., additional, Sokolovsky, K. V., additional, Lisakov, M. M., additional, Kiehlmann, S., additional, Gurwell, M., additional, and Zensus, J. A., additional
Published: 2020
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23. Apparent superluminal core expansion and limb brightening in the candidate neutrino blazar TXS 0506+056

Author: Ros, E., primary, Kadler, M., additional, Perucho, M., additional, Boccardi, B., additional, Cao, H.-M., additional, Giroletti, M., additional, Krauß, F., additional, and Ojha, R., additional
Published: 2019
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24. X-ray monitoring of the radio and γ-ray loud Narrow-Line Seyfert 1 Galaxy PKS2004–447

Author: Kreikenbohm A., Kadler M., Wilms J., Schulz R., Müller C., Ojha R., Ros E., Mannheim K., and Elsässer D.
Subjects: Physics, QC1-999
Abstract: We present preliminary results of the X-ray analysis of XMM-Newton and Swift observations as part of a multi-wavelength monitoring campaign in 2012 of the radio-loud narrow line Seyfert 1 galaxy PKS 2004–447. The source was recently detected in γ-rays by Fermi/LAT among only four other galaxies of that type. The 0:5 – 10 keV X-ray spectrum is well-described by a simple absorbed powerlaw (Γ ∼ 1.6). The source brightness exhibits variability on timescales of months to years with indications for spectral variability, which follows a “bluer-when-brighter” behaviour, similar to blazars.
Published: 2013
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25. The jet of the Low Luminosity AGN of M81

Author: Alberdi A., Martí-Vidal I., Marcaide J.M., Guirado J.C., Pérez-Torres M.A., Ros E., and Brunthaler A.
Subjects: Physics, QC1-999
Abstract: In this contribution, we summarize our main results of a big campaign of global VLBI observations of the AGN in M81 (M81*) phase-referenced to the radio supernova SN 1993J. Thanks to the precise multi-epoch and multi-frequency astrometry, we have determined the normalized core-shift of the relativistic jet of M81* and estimated both the magnetic field and the particle density at the jet base. We have also found evidence of jet precession in M81* coming from the systematic time evolution of the jet orientation correlated with changes in the overall flux density.
Published: 2013
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26. ANTARES constrains a blazar origin of two IceCube PeV neutrino events

Author: Adrián Martínez, S., Albert, A., André, M., Anton, G., Ardid, M., Aubert, J. J., Baret, B., Barrios, J., Basa, S., Bertin, V., Biagi, S., Bogazzi, C., Bormuth, R., Bou Cabo, M., Bouwhuis, M. C., Bruijn, R., Brunner, J., Busto, J., Capone, Antonio, Caramete, L., Carr, J., Chiarusi, T., Circella, M., Coniglione, R., Core, L., Costantini, H., Coyle, P., Creusot, A., De Rosa, G., Dekeyser, I., Deschamps, A., DE BONIS, Giulia, Distefano, C., Donzaud, C., Dornic, D., Dorosti, Q., Drouhin, D., Dumas, A., Eberl, T., Enzenhöfer, A., Escoffier, S., Fehn, K., Felis, I., Fermani, Paolo, Folger, F., Fusco, L. A., Galatà, S., Gay, P., Geißelsöder, S., Geyer, K., Giordano, V., Gleixner, A., Gřómez González, J. P., Graf, K., Guillard, G., van Haren, H., Heijboer, A. J., Hello, Y., Hernández Rey, J. J., Herold, B., Herrero, A., Hößl, J., Hofestädt, J., Hugon, C., James, C. W., de Jong, M., Kalekin, O., Katz, U., Kießling, D., Kooijman, P., Kouchner, A., Kulikovskiy, V., Lahmann, R., Lambard, E., Lambard, G., Lefèvre, D., Leonora, E., Loehner, H., Loucatos, S., Mangano, S., Marcelin, M., Margiotta, A., Martínez Mora, J. A., Martini, S., Mathieu, A., Michael, T., Migliozzi, P., Neff, M., Nezri, E., Palioselitis, D., Păvăląs, G. E., Pellegrino, C., Perrina, Chiara, Piattelli, P., Popa, V., Pradier, T., Racca, C., Riccobene, G., Richter, R., Roensch, K., Rostovtsev, A., Saldaña, M., Samtleben, D. F. E., Sánchez Losa, . A., Sanguineti, M., Sapienza, P., Schmid, J., Schnabel, J., Schulte, S., Schüssler, F., Seitz, T., Sieger, C., Spies, A., Spurio, M., Steijger, J. J. M., Stolarczyk, T. h., Taiuti, M., Tamburini, C., Tayalati, Y., Trovato, A., Vallage, B., Vallée, C., Van Elewyck, V., Visser, E., Vivolo, D., Wagner, S., de Wolf, E., Yatkin, K., Yepes, H., Zornoza, J. D., Zúñiga, J., Krauß, F., Kadler, M., Mannheim, . K., Schulz, R., Trüstedt, J., Wilms, J., Ojha, R., Ros, E., Baumgartner, W., Beuchert, T., Blanchard, J., Bürkel, C., Carpenter, B., Edwards, P. G., Eisenacher Glawion, D., Elsässer, D., Fritsch, U., Gehrels, N., Gräfe, C., Großberger, C., Hase, H., Horiuchi, S., Kappes, A., Kreikenbohm, A., Kreykenbohm, I., Langejahn, M., Leiter, K., Litzinger, E., Lovell, J. E. J., Müller, C., Phillips, C., Plötz, C., Quick, J., Steinbring, T., Stevens, J., Thompson, D. J., Tzioumis, A. K., Research unit Nuclear & Hadron Physics, Institut d’Investigació per a la Gestió Integrada de Zones Costaneres (IGIC), Universitat Politècnica de València (UPV), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Laboratory of Applied Bioacoustics (LAB-UPC), Universidad Polytecnica de Cataluña (UPC), Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut méditerranéen d'océanologie (MIO), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Aix Marseille Université (AMU)-Institut de Recherche pour le Développement (IRD), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université Paris-Sud - Paris 11 (UP11), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut Pluridisciplinaire Hubert Curien (IPHC), Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), The ANTARES Collaboration, The TANAMI Collaboration, Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), KM3NeT (IHEF, IoP, FNWI), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Département de Physique des Particules (ex SPP) (DPhP), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Adrián Martínez, S., Albert, A., André, M., Anton, G., Ardid, M., Aubert, J. J., Baret, B., Barrios, J., Basa, S., Bertin, V., Biagi, S., Bogazzi, C., Bormuth, R., Bou Cabo, M., Bouwhuis, M. C., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Chiarusi, T., Circella, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., DE ROSA, Gianfranca, Dekeyser, I., Deschamps, A., De Bonis, G., Distefano, C., Donzaud, C., Dornic, D., Dorosti, Q., Drouhin, D., Dumas, A., Eberl, T., Enzenhöfer, A., Escoffier, S., Fehn, K., Felis, I., Fermani, P., Folger, F., Fusco, L. A., Galatà, S., Gay, P., Geißelsöder, S., Geyer, K., Giordano, V., Gleixner, A., Gómez González, J. P., Gracia Ruiz, R., Graf, K., van Haren, H., Heijboer, A. J., Hello, Y., Hernández Rey, J. J., Herrero, A., Hößl, J., Hofestädt, J., Hugon, C., W. James, C., de Jong, M., Kalekin, O., Katz, U., Kießling, D., Kooijman, P., Kouchner, A., Kulikovskiy, V., Lahmann, R., Lattuada, D., Lefèvre, D., Leonora, E., Loehner, H., Loucatos, S., Mangano, S., Marcelin, M., Margiotta, A., Martínez Mora, J. A., Martini, S., Mathieu, A., Michael, T., Migliozzi, P., Neff, M., Nezri, E., Palioselitis, D., Păvălaş, G. E., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Racca, C., Riccobene, G., Richter, R., Roensch, K., Rostovtsev, A., Saldaña, M., Samtleben, D. F. E., Sánchez Losa, A., Sanguineti, M., Sapienza, P., Schmid, J., Schnabel, J., Schulte, S., Schüssler, F., Seitz, T., Sieger, C., Spies, A., Spurio, M., Steijger, J. J. M., Stolarczyk, T. h., Taiuti, M., Tamburini, C., Tayalati, Y., Trovato, A., Tselengidou, M., Tönnis, C., Vallage, B., Vallée, C., Van Elewyck, V., Visser, E., Vivolo, Daniele, Wagner, S., de Wolf, E., Yepes, H., Zornoza, J. D., Zúñiga, J., Krauß, F., Kadler, M., Mannheim, K., Schulz, R., Trüstedt, J., Wilms, J., Ojha, R., Ros, E., Baumgartner, W., Beuchert, T., Blanchard, J., Bürkel, C., Carpenter, B., Edwards, P. G., Eisenacher Glawion, D., Elsässer, D., Fritsch, U., Gehrels, N., Gräfe, C., Großberger, C., Hase, H., Horiuchi, S., Kappes, A., Kreikenbohm, A., Kreykenbohm, I., Langejahn, M., Leiter, K., Litzinger, E., Lovell, J. E. J., Müller, C., Phillips, C., Plötz, C., Quick, J., Steinbring, T., Stevens, J., Thompson, D. J., Tzioumis, A. K., Adrian-Martinez, S, Albert, A, Andre, M, Anton, G, Ardid, M, Aubert, Jj, Baret, B, Barrios, J, Basa, S, Bertin, V, Biagi, S, Bogazzi, C, Bormuth, R, Bou-Cabo, M, Bouwhuis, Mc, Brujin, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Cane, J, Chiarusim, T, Circella, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, De Rosa, G, Dekeyser, I, Deschamps, A, De Bonis, G, Distefano, C, Donzaud, C, Dornic, D, Dorosti, Q, Drouhin, D, Dumas, A, Eberl, T, Enzenhofer, A, Escoffier, S, Fehn, K, Felis, I, Fermani, P, Folger, F, Fusco, La, Galata, S, Gay, P, Geisselsoder, S, Geyer, K, Giordano, V, Gleixner, A, Gomez-Gonzalez, Jp, Gracia-Ruiz, R, Graf, K, van Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Herrero, A, Hossl, J, Hofestadt, J, Hugon, C, James, Cw, de Jong, M, Kalekin, O, Katz, U, Kiessling, D, Kooijman, P, Kouchner, A, Kulikovskiy, V, Lahmann, R, Lattuada, D, Lefevre, D, Leonora, E, Loehner, H, Loucatos, S, Mangano, S, Marcelin, M, Margiotta, A, Martinez-Mora, Ja, Martini, S, Mathieu, A, Michael, T, Migliozzi, P, Neff, M, Nezri, E, Palioselitis, D, Pavalas, Ge, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Richter, R, Roensch, K, Rostovtsev, A, Saldana, M, Samtleben, Dfe, Sanchez-Losa, A, Sanguineti, M, Sapienza, P, Schmid, J, Schnabel, J, Schulte, S, Schussler, F, Seitz, T, Sieger, C, Spies, A, Spurio, M, Steijger, Jjm, Stolarczyk, T, Taiuti, M, Tamburini, C, Tayalati, Y, Trovato, A, Tselengidou, M, Tonnis, C, Vallage, B, Vallee, C, Van Elewyck, V, Visser, E, Vivolo, D, Wagner, S, de Wolf, E, Yepes, H, Zornoza, Jd, Zuniga, J, Krauss, F, Kadler, M, Mannheim, K, Schulz, R, Trustedt, J, Wilms, J, Ojha, R, Ros, E, Baumgartner, W, Beuchert, T, Blanchard, J, Burke, C, Carpenter, B, Edwards, Pg, Glawion, De, Elsasser, D, Fritsch, U, Gehrels, N, Grafe, C, Grossberger, C, Hase, H, Horiuchi, S, Kappes, A, Kreikenbohm, A, Kreykenbohm, I, Langejahn, M, Leiter, K, Litzinger, E, Lovell, Jej, Muller, C, Phillips, C, Plotz, C, Quick, J, Steinbring, T, Stevens, J, Thompson, Dj, Tzioumis, Ak, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Adrián-Martínez, S, Aubert, J.-J., Bou-Cabo, M., Bouwhuis, M.C., De Rosa, G., Fusco, L.A., Gómez-González, J.P., Gracia-Ruiz, R., Van Haren, H., Heijboer, A.J., Hernández-Rey, J.J., James, C.W., De Jong, M., Martínez-Mora, J.A., Pəvəlaş, G.E., Samtleben, D.F.E., Sánchez-Losa, A., Steijger, J.J.M., Stolarczyk, Th., Vivolo, D., De Wolf, E., Zornoza, J.D., Edwards, P.G., Lovell, J.E.J., Thompson, D.J., Tzioumis, A.K., Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Adrian-Martinez, S., Andre, M., Aubert, J. -J., Enzenhofer, A., Galata, S., Geisselsoder, S., Gomez-Gonzalez, J. P., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., James, C. W., Kiessling, D., Lefevre, D., Martinez-Mora, J. A., Pevelas, G. E., Saldana, M., Sanchez-Losa, A., Schussler, F., Tonnis, C., Vallee, C., Zuniga, J., Krauss, F., Trustedt, J., Burkel, C., Elsasser, D., Grafe, C., Grossberger, C., Muller, C., and Plotz, C.
Subjects: Astrofísica, active [Galaxies], Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Flux, FOS: Physical sciences, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, Spectral line, 0103 physical sciences, Neutrino, Galaxies: active, Neutrinos, Quasars: general, Neutrins, Blazar, 010303 astronomy & astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Muon, Cosmologia, 010308 nuclear & particles physics, Física, Astronomy and Astrophysics, general [Quasars], Astronomy and Astrophysic, Neutrino astrophysics, Quasars general, Cosmology, neutrinos – galaxies: active – quasars: general, Space and Planetary Science, Galaxies active, Col·lisions (Física nuclear), Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], FISICA APLICADA, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, MATEMATICA APLICADA, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Event (particle physics)
Abstract: Context. The source(s) of the neutrino excess reported by the IceCube Collaboration is unknown. The TANAMI Collaboration recently reported on the multiwavelength emission of six bright, variable blazars which are positionally coincident with two of the most energetic IceCube events. Objects like these are prime candidates to be the source of the highest-energy cosmic rays, and thus of associated neutrino emission. Aims. We present an analysis of neutrino emission from the six blazars using observations with the ANTARES neutrino telescope. Methods. The standard methods of the ANTARES candidate list search are applied to six years of data to search for an excess of muons and hence their neutrino progenitors from the directions of the six blazars described by the TANAMI Collaboration, and which are possibly associated with two IceCube events. Monte Carlo simulations of the detector response to both signal and background particle fluxes are used to estimate the sensitivity of this analysis for different possible source neutrino spectra. A maximum-likelihood approach, using the reconstructed energies and arrival directions of through-going muons, is used to identify events with properties consistent with a blazar origin. Results. Both blazars predicted to be the most neutrino-bright in the TANAMI sample (1653-329 and 1714-336) have a signal flux fitted by the likelihood analysis corresponding to approximately one event. This observation is consistent with the blazar-origin hypothesis of the IceCube event IC 14 for a broad range of blazar spectra, although an atmospheric origin cannot be excluded. No ANTARES events are observed from any of the other four blazars, including the three associated with IceCube event IC20. This excludes at a 90% confidence level the possibility that this event was produced by these blazars unless the neutrino spectrum is flatter than -2.4., The authors would like to thank A. Kappes for helpful discussions regarding the IceCube analysis. The ANTARES authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'enegie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. The TANAMI authors acknowledge support and partial funding by the Deutsche Forschungsgemeinschaft grant WI 1860-10/1 (TANAMI) and GRK 1147, Deutsches Zentrum fur Luft- und Raumfahrt grant 50 OR1311/50 OR1303/50 OR1401, the Spanish MINECO project AYA2012-38491-C02-01, the Generalitat Valenciana project PROMETEOII/2014/057, the COST MP0905 action "Black Holes in a Violent Universe" and the Helmholtz Alliance for Astroparticle Physics (HAP).
Published: 2015

27. Using evolutionary algorithms to model relativistic jets

Author: Fromm, C. M., primary, Younsi, Z., additional, Baczko, A., additional, Mizuno, Y., additional, Porth, O., additional, Perucho, M., additional, Olivares, H., additional, Nathanail, A., additional, Angelakis, E., additional, Ros, E., additional, Zensus, J. A., additional, and Rezzolla, L., additional
Published: 2019
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28. Gamma-ray emission in radio galaxies under the VLBI scope

Author: Angioni, R., primary, Ros, E., additional, Kadler, M., additional, Ojha, R., additional, Müller, C., additional, Edwards, P. G., additional, Burd, P. R., additional, Carpenter, B., additional, Dutka, M. S., additional, Gulyaev, S., additional, Hase, H., additional, Horiuchi, S., additional, Krauß, F., additional, Lovell, J. E. J., additional, Natusch, T., additional, Phillips, C., additional, Plötz, C., additional, Quick, J. F. H., additional, Rösch, F., additional, Schulz, R., additional, Stevens, J., additional, Tzioumis, A. K., additional, Weston, S., additional, Wilms, J., additional, and Zensus, J. A., additional
Published: 2019
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29. Asymmetric jet production in the active galactic nucleus of NGC 1052

Author: Baczko, A.-K., primary, Schulz, R., additional, Kadler, M., additional, Ros, E., additional, Perucho, M., additional, Fromm, C. M., additional, and Wilms, J., additional
Published: 2019
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30. Spatially resolved origin of millimeter-wave linear polarization in the nuclear region of 3C 84

Author: Kim, J.-Y., primary, Krichbaum, T. P., additional, Marscher, A. P., additional, Jorstad, S. G., additional, Agudo, I., additional, Thum, C., additional, Hodgson, J. A., additional, MacDonald, N. R., additional, Ros, E., additional, Lu, R.-S., additional, Bremer, M., additional, de Vicente, P., additional, Lindqvist, M., additional, Trippe, S., additional, and Zensus, J. A., additional
Published: 2019
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31. VLBA polarimetric monitoring of 3C 111

Author: Ministerio de Economía y Competitividad (España), European Commission, Generalitat Valenciana, Russian Foundation for Basic Research, Alexander von Humboldt Foundation, Academy of Finland, Junta de Andalucía, Beuchert, T., Kadler, M., Perucho, M., Großberger, C., Schulz, R., Agudo, Iván, Casadio, Carolina, Gómez, José L., Gurwell, M., Homan, D., Kovalev, Y. Y., Lister, Matthew L., Markoff, S., Molina, Sol, Pushkarev, A.B., Ros, E., Savolainen, T., Steinbring, T., Thum, C., Wilms, J., Ministerio de Economía y Competitividad (España), European Commission, Generalitat Valenciana, Russian Foundation for Basic Research, Alexander von Humboldt Foundation, Academy of Finland, Junta de Andalucía, Beuchert, T., Kadler, M., Perucho, M., Großberger, C., Schulz, R., Agudo, Iván, Casadio, Carolina, Gómez, José L., Gurwell, M., Homan, D., Kovalev, Y. Y., Lister, Matthew L., Markoff, S., Molina, Sol, Pushkarev, A.B., Ros, E., Savolainen, T., Steinbring, T., Thum, C., and Wilms, J.
Abstract: Context. While studies of large samples of jets of active galactic nuclei (AGN) are important in order to establish a global picture, dedicated single-source studies are an invaluable tool for probing crucial processes within jets on parsec scales. These processes involve in particular the formation and geometry of the jet magnetic field as well as the flow itself. Aims. We aim to better understand the dynamics within relativistic magneto-hydrodynamical flows in the extreme environment and close vicinity of supermassive black holes. Methods. We analyze the peculiar radio galaxy 3C 111, for which long-Term polarimetric observations are available. We make use of the high spatial resolution of the VLBA network and the MOJAVE monitoring program, which provides high data quality also for single sources and allows us to study jet dynamics on parsec scales in full polarization with an evenly sampled time-domain. While electric vectors can probe the underlying magnetic field, other properties of the jet such as the variable (polarized) flux density, feature size, and brightness temperature, can give valuable insights into the flow itself. We complement the VLBA data with data from the IRAM 30-m Telescope as well as the SMA. Results. We observe a complex evolution of the polarized jet. The electric vector position angles (EVPAs) of features traveling down the jet perform a large rotation of &180across a distance of about 20 pc. As opposed to this smooth swing, the EVPAs are strongly variable within the first parsecs of the jet.We find an overall tendency towards transverse EVPAs across the jet with a local anomaly of aligned vectors in between. The polarized flux density increases rapidly at that distance and eventually saturates towards the outermost observable regions. The transverse extent of the flow suddenly decreases simultaneously to a jump in brightness temperature around where we observe the EVPAs to turn into alignment with the jet flow. Also the gradient of the fe
Published: 2018

32. Extended X-ray emission in PKS 1718-649

Author: Beuchert, T., Rodríguez-Ardila, A., Moss, V., Schulz, R., Kadler, M., Wilms, J., Angioni, R., Callingham, J., Gräfe, C., Krauß, F., Kreikenbohm, A., Langejahn, M., Leiter, K., Maccagni, F., Müller, C., Ojha, R., Ros, E., Tingay, Steven, Beuchert, T., Rodríguez-Ardila, A., Moss, V., Schulz, R., Kadler, M., Wilms, J., Angioni, R., Callingham, J., Gräfe, C., Krauß, F., Kreikenbohm, A., Langejahn, M., Leiter, K., Maccagni, F., Müller, C., Ojha, R., Ros, E., and Tingay, Steven
Abstract: © ESO 2018. PKS 1718-649 is one of the closest and most comprehensively studied candidates of a young active galactic nucleus (AGN) that is still embedded in its optical host galaxy. The compact radio structure, with a maximal extent of a few parsecs, makes it a member of the group of compact symmetric objects (CSO). Its environment imposes a turnover of the radio synchrotron spectrum towards lower frequencies, also classifying PKS 1718-649 as gigahertz-peaked radio spectrum (GPS) source. Its close proximity has allowed the first detection of extended X-ray emission in a GPS/CSO source with Chandra that is for the most part unrelated to nuclear feedback. However, not much is known about the nature of this emission. By co-adding all archival Chandra data and complementing these datasets with the large effective area of XMM-Newton, we are able to study the detailed physics of the environment of PKS 1718-649. Not only can we confirm that the bulk of the kiloparsec-scale environment emits in the soft X-rays, but we also identify the emitting gas to form a hot, collisionally ionized medium. While the feedback of the central AGN still seems to be constrained to the inner few parsecs, we argue that supernovae are capable of producing the observed large-scale X-ray emission at a rate inferred from its estimated star formation rate.
Published: 2018

33. TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry - II. Additional Sources

Author: Müller, C., Kadler, M., Ojha, R., Schulz, R., Trüstedt, J., Edwards, P., Ros, E., Carpenter, B., Angioni, R., Blanchard, J., Böck, M., Burd, P., Dörr, M., Dutka, M., Eberl, T., Gulyaev, S., Hase, H., Horiuchi, S., Katz, U., Krauß, F., Lovell, J., Natusch, T., Nesci, R., Phillips, C., Plötz, C., Pursimo, T., Quick, J., Stevens, J., Thompson, D., Tingay, Steven, Tzioumis, A., Weston, S., Wilms, J., Zensus, J., Müller, C., Kadler, M., Ojha, R., Schulz, R., Trüstedt, J., Edwards, P., Ros, E., Carpenter, B., Angioni, R., Blanchard, J., Böck, M., Burd, P., Dörr, M., Dutka, M., Eberl, T., Gulyaev, S., Hase, H., Horiuchi, S., Katz, U., Krauß, F., Lovell, J., Natusch, T., Nesci, R., Phillips, C., Plötz, C., Pursimo, T., Quick, J., Stevens, J., Thompson, D., Tingay, Steven, Tzioumis, A., Weston, S., Wilms, J., and Zensus, J.
Abstract: TANAMI is a multiwavelength program monitoring active galactic nuclei (AGN) south of -30deg declination including high-resolution Very Long Baseline Interferometry (VLBI) imaging, radio, optical/UV, X-ray and gamma-ray studies. We have previously published first-epoch 8.4GHz VLBI images of the parsec-scale structure of the initial sample. In this paper, we present images of 39 additional sources. The full sample comprises most of the radio- and gamma-ray brightest AGN in the southern quarter of the sky, overlapping with the region from which high-energy (>100TeV) neutrino events have been found. We characterize the parsec-scale radio properties of the jets and compare with the quasi-simultaneous Fermi/LAT gamma-ray data. Furthermore, we study the jet properties of sources which are in positional coincidence with high-energy neutrino events as compared to the full sample. We test the positional agreement of high-energy neutrino events with various AGN samples. Our observations yield the first images of many jets below -30deg declination at milliarcsecond resolution. We find that gamma-ray loud TANAMI sources tend to be more compact on parsec-scales and have higher core brightness temperatures than gamma-ray faint jets, indicating higher Doppler factors. No significant structural difference is found between sources in positional coincidence with high-energy neutrino events and other TANAMI jets. The 22 gamma-ray brightest AGN in the TANAMI sky show only a weak positional agreement with high-energy neutrinos demonstrating that the >100TeV IceCube signal is not simply dominated by a small number of the $\gamma$-ray brightest blazars. Instead, a larger number of sources have to contribute to the signal with each individual source having only a small Poisson probability for producing an event in multi-year integrations of current neutrino detectors.
Published: 2018

34. Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron

Author: Bruni, G., Gómez Fernández, J. L., Casadio, C., Lobanov, A., Kovalev, Y.Y., Sokolovsky, K.V., Lisakov, Mikhail M., Bach, U., Marscher, A., Jorstad, S., Anderson, J.M., Krichbaum, Thomas P., Savolainen, T., Vega-Garciá, L., Fuentes, A., Zensus, J.A., Alberdi, Antxón, Lee, S.S., Lu, R.S., Pérez-Torres, Miguel A., Ros, E., Alexander von Humboldt Foundation, National Research Foundation of Korea, National Aeronautics and Space Administration (US), Generalitat Valenciana, Ministerio de Economía y Competitividad (España), Academy of Finland, Max-Planck-Institut für Radioastronomie, Instituto de Astrofísica de Andalucía, Lebedev Physical Institute, Boston University, St. Petersburg State University, GFZ German Research Centre for Geosciences, Metsähovi Radio Observatory, Korea Astronomy and Space Science Institute, Department of Electronics and Nanoengineering, Aalto-yliopisto, and Aalto University
Subjects: magnetic fields [galaxies], Galaxies: magnetic fields, Galaxies: jets, Astrophysics::High Energy Astrophysical Phenomena, active [galaxies], jets [galaxies], Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxies: active, Astrophysics::Galaxy Astrophysics
Abstract: RadioAstron is a 10 m orbiting radio telescope mounted on the Spektr-R satellite, launched in 2011, performing Space Very Long Baseline Interferometry (SVLBI) observations supported by a global ground array of radio telescopes. With an apogee of ∼350 000 km, it is offering for the first time the possibility to perform μas-resolution imaging in the cm-band. Aims. The RadioAstron active galactic nuclei (AGN) polarization Key Science Project (KSP) aims at exploiting the unprecedented angular resolution provided by RadioAstron to study jet launching/collimation and magnetic-field configuration in AGN jets. The targets of our KSP are some of the most powerful blazars in the sky. Methods. We present observations at 22 GHz of 3C 273, performed in 2014, designed to reach a maximum baseline of approximately nine Earth diameters. Reaching an angular resolution of 0.3 mas, we study a particularly low-activity state of the source, and estimate the nuclear region brightness temperature, comparing with the extreme one detected one year before during the RadioAstron early science period. We also make use of the VLBA-BU-BLAZAR survey data, at 43 GHz, to study the kinematics of the jet in a ∼1.5-yr time window. Results. We find that the nuclear brightness temperature is two orders of magnitude lower than the exceptionally high value detected in 2013 with RadioAstron at the same frequency (1.4 × 10 13 K, source-frame), and even one order of magnitude lower than the equipartition value. The kinematics analysis at 43 GHz shows that a new component was ejected ∼2 months after the 2013 epoch, visible also in our 22 GHz map presented here. Consequently this was located upstream of the core during the brightness temperature peak. Fermi-LAT observations for the period 2010â '2014 do not show any Î 3-ray flare in conjunction with the passage of the new component by the core at 43 GHz. Conclusions. These observations confirm that the previously detected extreme brightness temperature in 3C 273, exceeding the inverse Compton limit, is a short-lived phenomenon caused by a temporary departure from equipartition. Thus, the availability of interferometric baselines capable of providing μas angular resolution does not systematically imply measured brightness temperatures over the known physical limits for astrophysical sources.© 2017 ESO., Scientific results from data presented in this publication are derived from the EVN project code GA030C (ground array), and from the RadioAstron mission project code RAKS04C (space segment). J.L.G. and A.F. acknowledge support by the Spanish Ministry of Economy and Competitiveness grants AYA2013-40825-P and AYA2016-80889-P. A. A. and M.A.P.T. acknowledge support by the Spanish MINECO through grants AYA2012-38491-C02-02 and AYA2015-63939-C2-1-P, cofunded with FEDER funds. E.R. acknowledges support from the Spanish MINECO through grants AYA2012-38491-C02-01 and AYA2015-63939-C2-2-P and from the Generalitat Valenciana grant PROMETEOII/2014/057. T.S. was funded by the Academy of Finland projects 274477 and 284495. The research at Boston University was supported in part by NASA Fermi Guest Investigator grant NNX14AQ58G. S.S.L. was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIP) (No. NRF-2016R1C1B2006697). Y. Y. K. was supported in part by the Alexander von Humboldt Foundation. This research has made use of data from the OVRO 40-m monitoring program (Richards et al. 2011) which is supported in part by NASA grants NNX08AW31G, NNX11A043G, and NNX14AQ89G and NSF grants AST-0808050 and AST-1109911.
Published: 2017

35. The limb-brightened jet of M87 down to the 7 Schwarzschild radii scale

Author: Kim, J.-Y., primary, Krichbaum, T. P., additional, Lu, R.-S., additional, Ros, E., additional, Bach, U., additional, Bremer, M., additional, de Vicente, P., additional, Lindqvist, M., additional, and Zensus, J. A., additional
Published: 2018
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36. Extended X-ray emission in PKS 1718−649

Author: Beuchert, T., primary, Rodríguez-Ardila, A., additional, Moss, V. A., additional, Schulz, R., additional, Kadler, M., additional, Wilms, J., additional, Angioni, R., additional, Callingham, J. R., additional, Gräfe, C., additional, Krauß, F., additional, Kreikenbohm, A., additional, Langejahn, M., additional, Leiter, K., additional, Maccagni, F. M., additional, Müller, C., additional, Ojha, R., additional, Ros, E., additional, and Tingay, S. J., additional
Published: 2018
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37. VLBA polarimetric monitoring of 3C 111

Author: Beuchert, T., primary, Kadler, M., additional, Perucho, M., additional, Großberger, C., additional, Schulz, R., additional, Agudo, I., additional, Casadio, C., additional, Gómez, J. L., additional, Gurwell, M., additional, Homan, D., additional, Kovalev, Y. Y., additional, Lister, M. L., additional, Markoff, S., additional, Molina, S. N., additional, Pushkarev, A. B., additional, Ros, E., additional, Savolainen, T., additional, Steinbring, T., additional, Thum, C., additional, and Wilms, J., additional
Published: 2018
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38. TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry

Author: Müller, C., primary, Kadler, M., additional, Ojha, R., additional, Schulz, R., additional, Trüstedt, J., additional, Edwards, P. G., additional, Ros, E., additional, Carpenter, B., additional, Angioni, R., additional, Blanchard, J., additional, Böck, M., additional, Burd, P. R., additional, Dörr, M., additional, Dutka, M. S., additional, Eberl, T., additional, Gulyaev, S., additional, Hase, H., additional, Horiuchi, S., additional, Katz, U., additional, Krauß, F., additional, Lovell, J. E. J., additional, Natusch, T., additional, Nesci, R., additional, Phillips, C., additional, Plötz, C., additional, Pursimo, T., additional, Quick, J. F. H., additional, Stevens, J., additional, Thompson, D. J., additional, Tingay, S. J., additional, Tzioumis, A. K., additional, Weston, S., additional, Wilms, J., additional, and Zensus, J. A., additional
Published: 2018
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39. Jet-torus connection in radio galaxies

Author: Fromm, C. M., primary, Perucho, M., additional, Porth, O., additional, Younsi, Z., additional, Ros, E., additional, Mizuno, Y., additional, Zensus, J. A., additional, and Rezzolla, L., additional
Published: 2018
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40. First multi-wavelength campaign on the gamma-ray-loud active galaxy IC 310

Author: Ahnen, M. L. (M. L.), Ansoldi, S. (S.), Antonelli, L. A. (L. A.), Arcaro, C. (C.), Babic, A. (A.), Banerjee, B. (B.), Bangale, P. (P.), de Almeida, U. B. (U. Barres), Barrio, J. A. (J. A.), Becerra Gonzalez, J. (J.), Bednarek, W. (W.), Bernardini, E. (E.), Berti, A. (A.), Biasuzzi, B. (B.), Biland, A. (A.), Blanch, O. (O.), Bonnefoy, S. (S.), Bonnoli, G. (G.), Borracci, F. (F.), Bretz, T. (T.), Carosi, R. (R.), Carosi, A. (A.), Chatterjee, A. (A.), Colin, P. (P.), Colombo, E. (E.), Contreras, J. L. (J. L.), Cortina, J. (J.), Covino, S. (S.), Cumani, P. (P.), Da Vela, P. (P.), Dazzi, F. (F.), De Angelis, A. (A.), De Lotto, B. (B.), de Ona Wilhelmi, E. (E.), Di Pierro, F. (F.), Doert, M. (M.), Dominguez, A. (A.), Prester, D. D. (D. Dominis), Dorner, D. (D.), Doro, M. (M.), Einecke, S. (S.), Glawion, D. E. (D. Eisenacher), Elsaesser, D. (D.), Engelkemeier, M. (M.), Ramazani, V. F. (V. Fallah), Fernandez-Barral, A. (A.), Fidalgo, D. (D.), Fonseca, M. V. (M. V.), Font, L. (L.), Fruck, C. (C.), Galindo, D. (D.), Lopez, R. J. (R. J. Garcia), Garczarczyk, M. (M.), Gaug, M. (M.), Giammaria, P. (P.), Godinovic, N. (N.), Gora, D. (D.), Guberman, D. (D.), Hadasch, D. (D.), Hahn, A. (A.), Hassan, T. (T.), Hayashida, M. (M.), Herrera, J. (J.), Hose, J. (J.), Hrupec, D. (D.), Hughes, G. (G.), Idec, W. (W.), Ishio, K. (K.), Kodani, K. (K.), Konno, Y. (Y.), Kubo, H. (H.), Kushida, J. (J.), Lelas, D. (D.), Lindfors, E. (E.), Lombardi, S. (S.), Longo, F. (F.), Lopez, M. (M.), Majumdar, P. (P.), Makariev, M. (M.), Mallot, K. (K.), Maneva, G. (G.), Manganaro, M. (M.), Mannheim, K. (K.), Maraschi, L. (L.), Mariotti, M. (M.), Martinez, M. (M.), Mazin, D. (D.), Menzel, U. (U.), Mirzoyan, R. (R.), Moralejo, A. (A.), Moretti, E. (E.), Nakajima, D. (D.), Neustroev, V. (V.), Niedzwiecki, A. (A.), Rosillo, M. N. (M. Nievas), Nilsson, K. (K.), Nishijima, K. (K.), Noda, K. (K.), Nogues, L. (L.), Nothe, M. (M.), Paiano, S. (S.), Palacio, J. (J.), Palatiello, M. (M.), Paneque, D. (D.), Paoletti, R. (R.), Paredes, J. M. (J. M.), Paredes-Fortuny, X. (X.), Pedaletti, G. (G.), Peresano, M. (M.), Perri, L. (L.), Persic, M. (M.), Poutanen, J. (J.), Moroni, P. G. (P. G. Prada), Prandini, E. (E.), Puljak, I. (I.), Garcia, J. R. (J. R.), Reichardt, I. (I.), Rhode, W. (W.), Ribo, M. (M.), Rico, J. (J.), Saito, T. (T.), Satalecka, K. (K.), Schroeder, S. (S.), Schweizer, T. (T.), Shore, S. N. (S. N.), Sillanpaa, A. (A.), Sitarek, J. (J.), Snidaric, I. (I.), Sobczynska, D. (D.), Stamerra, A. (A.), Strzys, M. (M.), Suric, T. (T.), Takalo, L. (L.), Tavecchio, F. (F.), Temnikov, P. (P.), Terzic, T. (T.), Tescaro, D. (D.), Teshima, M. (M.), Torres, D. F. (D. F.), Torres-Alba, N. (N.), Toyama, T. (T.), Treves, A. (A.), Vanzo, G. (G.), Vazquez Acosta, M. (M.), Vovk, I. (I.), Ward, J. E. (J. E.), Will, M. (M.), Wu, M. H. (M. H.), Krauss, F. (F.), Schulz, R. (R.), Kadler, M. (M.), Wilms, J. (J.), Ros, E. (E.), Bach, U. (U.), Beuchert, T. (T.), Langejahn, M. (M.), Wendel, C. (C.), Gehrels, N. (N.), Baumgartner, W. H. (W. H.), Markwardt, C. B. (C. B.), Muller, C. (C.), Grinberg, V. (V.), Hovatta, T. (T.), Magill, J. (J.), Ahnen, M. L. (M. L.), Ansoldi, S. (S.), Antonelli, L. A. (L. A.), Arcaro, C. (C.), Babic, A. (A.), Banerjee, B. (B.), Bangale, P. (P.), de Almeida, U. B. (U. Barres), Barrio, J. A. (J. A.), Becerra Gonzalez, J. (J.), Bednarek, W. (W.), Bernardini, E. (E.), Berti, A. (A.), Biasuzzi, B. (B.), Biland, A. (A.), Blanch, O. (O.), Bonnefoy, S. (S.), Bonnoli, G. (G.), Borracci, F. (F.), Bretz, T. (T.), Carosi, R. (R.), Carosi, A. (A.), Chatterjee, A. (A.), Colin, P. (P.), Colombo, E. (E.), Contreras, J. L. (J. L.), Cortina, J. (J.), Covino, S. (S.), Cumani, P. (P.), Da Vela, P. (P.), Dazzi, F. (F.), De Angelis, A. (A.), De Lotto, B. (B.), de Ona Wilhelmi, E. (E.), Di Pierro, F. (F.), Doert, M. (M.), Dominguez, A. (A.), Prester, D. D. (D. Dominis), Dorner, D. (D.), Doro, M. (M.), Einecke, S. (S.), Glawion, D. E. (D. Eisenacher), Elsaesser, D. (D.), Engelkemeier, M. (M.), Ramazani, V. F. (V. Fallah), Fernandez-Barral, A. (A.), Fidalgo, D. (D.), Fonseca, M. V. (M. V.), Font, L. (L.), Fruck, C. (C.), Galindo, D. (D.), Lopez, R. J. (R. J. Garcia), Garczarczyk, M. (M.), Gaug, M. (M.), Giammaria, P. (P.), Godinovic, N. (N.), Gora, D. (D.), Guberman, D. (D.), Hadasch, D. (D.), Hahn, A. (A.), Hassan, T. (T.), Hayashida, M. (M.), Herrera, J. (J.), Hose, J. (J.), Hrupec, D. (D.), Hughes, G. (G.), Idec, W. (W.), Ishio, K. (K.), Kodani, K. (K.), Konno, Y. (Y.), Kubo, H. (H.), Kushida, J. (J.), Lelas, D. (D.), Lindfors, E. (E.), Lombardi, S. (S.), Longo, F. (F.), Lopez, M. (M.), Majumdar, P. (P.), Makariev, M. (M.), Mallot, K. (K.), Maneva, G. (G.), Manganaro, M. (M.), Mannheim, K. (K.), Maraschi, L. (L.), Mariotti, M. (M.), Martinez, M. (M.), Mazin, D. (D.), Menzel, U. (U.), Mirzoyan, R. (R.), Moralejo, A. (A.), Moretti, E. (E.), Nakajima, D. (D.), Neustroev, V. (V.), Niedzwiecki, A. (A.), Rosillo, M. N. (M. Nievas), Nilsson, K. (K.), Nishijima, K. (K.), Noda, K. (K.), Nogues, L. (L.), Nothe, M. (M.), Paiano, S. (S.), Palacio, J. (J.), Palatiello, M. (M.), Paneque, D. (D.), Paoletti, R. (R.), Paredes, J. M. (J. M.), Paredes-Fortuny, X. (X.), Pedaletti, G. (G.), Peresano, M. (M.), Perri, L. (L.), Persic, M. (M.), Poutanen, J. (J.), Moroni, P. G. (P. G. Prada), Prandini, E. (E.), Puljak, I. (I.), Garcia, J. R. (J. R.), Reichardt, I. (I.), Rhode, W. (W.), Ribo, M. (M.), Rico, J. (J.), Saito, T. (T.), Satalecka, K. (K.), Schroeder, S. (S.), Schweizer, T. (T.), Shore, S. N. (S. N.), Sillanpaa, A. (A.), Sitarek, J. (J.), Snidaric, I. (I.), Sobczynska, D. (D.), Stamerra, A. (A.), Strzys, M. (M.), Suric, T. (T.), Takalo, L. (L.), Tavecchio, F. (F.), Temnikov, P. (P.), Terzic, T. (T.), Tescaro, D. (D.), Teshima, M. (M.), Torres, D. F. (D. F.), Torres-Alba, N. (N.), Toyama, T. (T.), Treves, A. (A.), Vanzo, G. (G.), Vazquez Acosta, M. (M.), Vovk, I. (I.), Ward, J. E. (J. E.), Will, M. (M.), Wu, M. H. (M. H.), Krauss, F. (F.), Schulz, R. (R.), Kadler, M. (M.), Wilms, J. (J.), Ros, E. (E.), Bach, U. (U.), Beuchert, T. (T.), Langejahn, M. (M.), Wendel, C. (C.), Gehrels, N. (N.), Baumgartner, W. H. (W. H.), Markwardt, C. B. (C. B.), Muller, C. (C.), Grinberg, V. (V.), Hovatta, T. (T.), and Magill, J. (J.)
Abstract: Context: The extragalactic very-high-energy gamma-ray sky is rich in blazars. These are jetted active galactic nuclei that are viewed at a small angle to the line-of-sight. Only a handful of objects viewed at a larger angle are so far known to emit above 100 GeV. Multi-wavelength studies of such objects up to the highest energies provide new insights into the particle and radiation processes of active galactic nuclei. Aims: We aim to report the results from the first multi-wavelength campaign observing the TeV detected nucleus of the active galaxy IC 310, whose jet is observed at a moderate viewing angle of 10°−20°. Methods: The multi-instrument campaign was conducted between 2012 November and 2013 January, and involved observations with MAGIC, Fermi, INTEGRAL, Swift, OVRO, MOJAVE and EVN. These observations were complemented with archival data from the AllWISE and 2MASS catalogs. A one-zone synchrotron self-Compton model was applied to describe the broadband spectral energy distribution. Results: IC 310 showed an extraordinary TeV flare at the beginning of the campaign, followed by a low, but still detectable TeV flux. Compared to previous measurements in this energy range, the spectral shape was found to be steeper during the low emission state. Simultaneous observations in the soft X-ray band showed an enhanced energy flux state and a harder-when-brighter spectral shape behavior. No strong correlated flux variability was found in other frequency regimes. The broadband spectral energy distribution obtained from these observations supports the hypothesis of a double-hump structure. Conclusions: The harder-when-brighter trend in the X-ray and VHE emission, observed for the first time during this campaign, is consistent with the behavior expected from a synchrotron self-Compton scenario. The contemporaneous broadband spectral energy distribution is well described with a one-zone synchrotron self-Compton model using parameters that are comparable to those fou
Published: 2017

41. Young, active radio stars in the AB Doradus moving group

Author: Ministerio de Economía y Competitividad (España), Generalitat Valenciana, Azulay, R., Guirado, J.C., Marcaide, J.M., Martí-Vidal, Iván, Ros, E., Tognelli, E., Hormuth, F., Ortiz, José Luis, Ministerio de Economía y Competitividad (España), Generalitat Valenciana, Azulay, R., Guirado, J.C., Marcaide, J.M., Martí-Vidal, Iván, Ros, E., Tognelli, E., Hormuth, F., and Ortiz, José Luis
Abstract: Context. Precise determination of stellar masses is necessary to test the validity of pre-main-sequence (PMS) stellar evolutionary models, whose predictions are in disagreement with measurements for masses below 1.2 M. To improve such a test, and based on our previous studies, we selected the AB Doradus moving group (AB Dor-MG) as the best-suited association on which to apply radio-based high-precision astrometric techniques to study binary systems. Aims. We seek to determine precise estimates of the masses of a set of stars belonging to the AB Dor-MG using radio and infrared observations. Methods. We observed in phase-reference mode with the Very Large Array (VLA) at 5 GHz and with the European VLBI Network (EVN) at 8.4 GHz the stars HD 160934, EK Dra, PW And, and LO Peg. We also observed some of these stars with the near-infrared CCD AstraLux camera at the Calar Alto observatory to complement the radio observations. Results. We determine model-independent dynamical masses of both components of the star HD 160934, A and c, which are 0.70 ± 0.07 M and 0.45 ± 0.04 M, respectively. We revised the orbital parameters of EK Dra and we determine a sum of the masses of the system of 1.38 ± 0.08 M. We also explored the binarity of the stars LO Peg and PW And. Conclusions. We found observational evidence that PMS evolutionary models underpredict the mass of PMS stars by 10%-40%, as previously reported by other authors. We also inferred that the origin of the radio emission must be similar in all observed stars, that is, extreme magnetic activity of the stellar corona that triggers gyrosynchrotron emission from non-Thermal, accelerated electrons. © ESO, 2017.
Published: 2017

42. Radio and gamma-ray properties of extragalactic jets from the TANAMI sample

Author: Böck, M., Kadler, M., Müller, C., Tosti, G., Bastieri, D., Burnett, T., Carpenter, B., Cavazzuti, E., Dutka, M., Blanchard, J., Edwards, P. G., Hase, H., Horiuchi, S., Jauncey, D. L., Krauß, F., Lister, M. L., Lovell, J. E. J., Lott, B., Murphy, D. W., Phillips, C., Plötz, C., Pursimo, T., Quick, J., Ros, E., Taylor, G., Thompson, D. J., Tingay, S. J., Tzioumis, A., and Zensus, J. A.
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: The TANAMI program has been observing parsec-scale radio jets of southern (declination south of − 30°) γ-ray bright AGN, simultaneously with Fermi/LAT monitoring of their γ-ray emission, via high-resolution radio imaging with Very Long Baseline Interferometry techniques. We present the radio and γ-rayproperties of the TANAMI sources based on one year of contemporaneous TANAMI and Fermi/LAT data. A large fraction (72%) of the TANAMI sample can be associated with bright γ-ray sources for this time range. Association rates differ for different optical classes with all BL Lacs, 76% of quasars, and just 17% of galaxies detected by the LAT. Upper limits were established on the γ-ray flux from TANAMI sources not detected by LAT. This analysis led to the identification of three new Fermi sources whose detection was later confirmed. The γ-ray and radio luminosities are related by Lγ ∝ Lᵣ⁰·⁸⁹±⁰·⁰⁴. The brightness temperatures of the radio cores increase with the average γ-ray luminosity and the presence of brightness temperatures above the inverse Compton limit implies strong Doppler boosting in those sources. The undetected sources have lower γ/radio luminosity ratios and lower contemporaneous brightness temperatures. Unless the Fermi/LAT-undetected blazars are much γ-ray-fainter than the Fermi/LAT-detected sources, their γ-ray luminosity should not be significantly lower than the upper limits calculated here.
Published: 2016
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43. The AB Doradus system revisited: The dynamical mass of AB Dor A/C

Author: Azulay, R., primary, Guirado, J. C., additional, Marcaide, J. M., additional, Martí-Vidal, I., additional, Ros, E., additional, Tognelli, E., additional, Jauncey, D. L., additional, Lestrade, J.-F., additional, and Reynolds, J. E., additional
Published: 2017
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44. Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron

Author: Bruni, G., primary, Gómez, J. L., additional, Casadio, C., additional, Lobanov, A., additional, Kovalev, Y. Y., additional, Sokolovsky, K. V., additional, Lisakov, M. M., additional, Bach, U., additional, Marscher, A., additional, Jorstad, S., additional, Anderson, J. M., additional, Krichbaum, T. P., additional, Savolainen, T., additional, Vega-García, L., additional, Fuentes, A., additional, Zensus, J. A., additional, Alberdi, A., additional, Lee, S.-S., additional, Lu, R.-S., additional, Pérez-Torres, M., additional, and Ros, E., additional
Published: 2017
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45. First multi-wavelength campaign on the gamma-ray-loud active galaxy IC 310

Author: Ahnen, M. L., primary, Ansoldi, S., additional, Antonelli, L. A., additional, Arcaro, C., additional, Babić, A., additional, Banerjee, B., additional, Bangale, P., additional, Barres de Almeida, U., additional, Barrio, J. A., additional, Becerra González, J., additional, Bednarek, W., additional, Bernardini, E., additional, Berti, A., additional, Biasuzzi, B., additional, Biland, A., additional, Blanch, O., additional, Bonnefoy, S., additional, Bonnoli, G., additional, Borracci, F., additional, Bretz, T., additional, Carosi, R., additional, Carosi, A., additional, Chatterjee, A., additional, Colin, P., additional, Colombo, E., additional, Contreras, J. L., additional, Cortina, J., additional, Covino, S., additional, Cumani, P., additional, Da Vela, P., additional, Dazzi, F., additional, De Angelis, A., additional, De Lotto, B., additional, de Oña Wilhelmi, E., additional, Di Pierro, F., additional, Doert, M., additional, Domínguez, A., additional, Dominis Prester, D., additional, Dorner, D., additional, Doro, M., additional, Einecke, S., additional, Eisenacher Glawion, D., additional, Elsaesser, D., additional, Engelkemeier, M., additional, Fallah Ramazani, V., additional, Fernández-Barral, A., additional, Fidalgo, D., additional, Fonseca, M. V., additional, Font, L., additional, Fruck, C., additional, Galindo, D., additional, García López, R. J., additional, Garczarczyk, M., additional, Gaug, M., additional, Giammaria, P., additional, Godinović, N., additional, Gora, D., additional, Guberman, D., additional, Hadasch, D., additional, Hahn, A., additional, Hassan, T., additional, Hayashida, M., additional, Herrera, J., additional, Hose, J., additional, Hrupec, D., additional, Hughes, G., additional, Idec, W., additional, Ishio, K., additional, Kodani, K., additional, Konno, Y., additional, Kubo, H., additional, Kushida, J., additional, Lelas, D., additional, Lindfors, E., additional, Lombardi, S., additional, Longo, F., additional, López, M., additional, Majumdar, P., additional, Makariev, M., additional, Mallot, K., additional, Maneva, G., additional, Manganaro, M., additional, Mannheim, K., additional, Maraschi, L., additional, Mariotti, M., additional, Martínez, M., additional, Mazin, D., additional, Menzel, U., additional, Mirzoyan, R., additional, Moralejo, A., additional, Moretti, E., additional, Nakajima, D., additional, Neustroev, V., additional, Niedzwiecki, A., additional, Nievas Rosillo, M., additional, Nilsson, K., additional, Nishijima, K., additional, Noda, K., additional, Nogués, L., additional, Nöthe, M., additional, Paiano, S., additional, Palacio, J., additional, Palatiello, M., additional, Paneque, D., additional, Paoletti, R., additional, Paredes, J. M., additional, Paredes-Fortuny, X., additional, Pedaletti, G., additional, Peresano, M., additional, Perri, L., additional, Persic, M., additional, Poutanen, J., additional, Prada Moroni, P. G., additional, Prandini, E., additional, Puljak, I., additional, Garcia, J. R., additional, Reichardt, I., additional, Rhode, W., additional, Ribó, M., additional, Rico, J., additional, Saito, T., additional, Satalecka, K., additional, Schroeder, S., additional, Schweizer, T., additional, Shore, S. N., additional, Sillanpää, A., additional, Sitarek, J., additional, Snidaric, I., additional, Sobczynska, D., additional, Stamerra, A., additional, Strzys, M., additional, Surić, T., additional, Takalo, L., additional, Tavecchio, F., additional, Temnikov, P., additional, Terzić, T., additional, Tescaro, D., additional, Teshima, M., additional, Torres, D. F., additional, Torres-Albà, N., additional, Toyama, T., additional, Treves, A., additional, Vanzo, G., additional, Vazquez Acosta, M., additional, Vovk, I., additional, Ward, J. E., additional, Will, M., additional, Wu, M. H., additional, Krauß, F., additional, Schulz, R., additional, Kadler, M., additional, Wilms, J., additional, Ros, E., additional, Bach, U., additional, Beuchert, T., additional, Langejahn, M., additional, Wendel, C., additional, Gehrels, N., additional, Baumgartner, W. H., additional, Markwardt, C. B., additional, Müller, C., additional, Grinberg, V., additional, Hovatta, T., additional, and Magill, J., additional
Published: 2017
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46. Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

Author: Ahnen, M. L., primary, Ansoldi, S., additional, Antonelli, L. A., additional, Antoranz, P., additional, Babic, A., additional, Banerjee, B., additional, Bangale, P., additional, Barres de Almeida, U., additional, Barrio, J. A., additional, Becerra González, J., additional, Bednarek, W., additional, Bernardini, E., additional, Berti, A., additional, Biasuzzi, B., additional, Biland, A., additional, Blanch, O., additional, Bonnefoy, S., additional, Bonnoli, G., additional, Borracci, F., additional, Bretz, T., additional, Buson, S., additional, Carosi, A., additional, Chatterjee, A., additional, Clavero, R., additional, Colin, P., additional, Colombo, E., additional, Contreras, J. L., additional, Cortina, J., additional, Covino, S., additional, Da Vela, P., additional, Dazzi, F., additional, De Angelis, A., additional, De Lotto, B., additional, de Oña Wilhelmi, E., additional, Di Pierro, F., additional, Doert, M., additional, Domínguez, A., additional, Dominis Prester, D., additional, Dorner, D., additional, Doro, M., additional, Einecke, S., additional, Eisenacher Glawion, D., additional, Elsaesser, D., additional, Engelkemeier, M., additional, Fallah Ramazani, V., additional, Fernández-Barral, A., additional, Fidalgo, D., additional, Fonseca, M. V., additional, Font, L., additional, Frantzen, K., additional, Fruck, C., additional, Galindo, D., additional, García López, R. J., additional, Garczarczyk, M., additional, Garrido Terrats, D., additional, Gaug, M., additional, Giammaria, P., additional, Godinović, N., additional, González Muñoz, A., additional, Gora, D., additional, Guberman, D., additional, Hadasch, D., additional, Hahn, A., additional, Hanabata, Y., additional, Hayashida, M., additional, Herrera, J., additional, Hose, J., additional, Hrupec, D., additional, Hughes, G., additional, Idec, W., additional, Kodani, K., additional, Konno, Y., additional, Kubo, H., additional, Kushida, J., additional, La Barbera, A., additional, Lelas, D., additional, Lindfors, E., additional, Lombardi, S., additional, Longo, F., additional, López, M., additional, López-Coto, R., additional, Majumdar, P., additional, Makariev, M., additional, Mallot, K., additional, Maneva, G., additional, Manganaro, M., additional, Mannheim, K., additional, Maraschi, L., additional, Marcote, B., additional, Mariotti, M., additional, Martínez, M., additional, Mazin, D., additional, Menzel, U., additional, Miranda, J. M., additional, Mirzoyan, R., additional, Moralejo, A., additional, Moretti, E., additional, Nakajima, D., additional, Neustroev, V., additional, Niedzwiecki, A., additional, Nievas Rosillo, M., additional, Nilsson, K., additional, Nishijima, K., additional, Noda, K., additional, Nogués, L., additional, Overkemping, A., additional, Paiano, S., additional, Palacio, J., additional, Palatiello, M., additional, Paneque, D., additional, Paoletti, R., additional, Paredes, J. M., additional, Paredes-Fortuny, X., additional, Pedaletti, G., additional, Peresano, M., additional, Perri, L., additional, Persic, M., additional, Poutanen, J., additional, Prada Moroni, P. G., additional, Prandini, E., additional, Puljak, I., additional, Reichardt, I., additional, Rhode, W., additional, Ribó, M., additional, Rico, J., additional, Rodriguez Garcia, J., additional, Saito, T., additional, Satalecka, K., additional, Schröder, S., additional, Schultz, C., additional, Schweizer, T., additional, Shore, S. N., additional, Sillanpää, A., additional, Sitarek, J., additional, Snidaric, I., additional, Sobczynska, D., additional, Stamerra, A., additional, Steinbring, T., additional, Strzys, M., additional, Surić, T., additional, Takalo, L., additional, Tavecchio, F., additional, Temnikov, P., additional, Terzić, T., additional, Tescaro, D., additional, Teshima, M., additional, Thaele, J., additional, Torres, D. F., additional, Toyama, T., additional, Treves, A., additional, Vanzo, G., additional, Verguilov, V., additional, Vovk, I., additional, Ward, J. E., additional, Will, M., additional, Wu, M. H., additional, Zanin, R., additional, Abeysekara, A. U., additional, Archambault, S., additional, Archer, A., additional, Benbow, W., additional, Bird, R., additional, Buchovecky, M., additional, Buckley, J. H., additional, Bugaev, V., additional, Connolly, M. P., additional, Cui, W., additional, Dickinson, H. J., additional, Falcone, A., additional, Feng, Q., additional, Finley, J. P., additional, Fleischhack, H., additional, Flinders, A., additional, Fortson, L., additional, Gillanders, G. H., additional, Griffin, S., additional, Grube, J., additional, Hütten, M., additional, Hanna, D., additional, Holder, J., additional, Humensky, T. B., additional, Kaaret, P., additional, Kar, P., additional, Kelley-Hoskins, N., additional, Kertzman, M., additional, Kieda, D., additional, Krause, M., additional, Krennrich, F., additional, Lang, M. J., additional, Maier, G., additional, McCann, A., additional, Moriarty, P., additional, Mukherjee, R., additional, Nieto, D., additional, O’Brien, S., additional, Ong, R. A., additional, Otte, N., additional, Park, N., additional, Perkins, J., additional, Pichel, A., additional, Pohl, M., additional, Popkow, A., additional, Pueschel, E., additional, Quinn, J., additional, Ragan, K., additional, Reynolds, P. T., additional, Richards, G. T., additional, Roache, E., additional, Rovero, A. C., additional, Rulten, C., additional, Sadeh, I., additional, Santander, M., additional, Sembroski, G. H., additional, Shahinyan, K., additional, Telezhinsky, I., additional, Tucci, J. V., additional, Tyler, J., additional, Wakely, S. P., additional, Weinstein, A., additional, Wilcox, P., additional, Wilhelm, A., additional, Williams, D. A., additional, Zitzer, B., additional, Razzaque, S., additional, Villata, M., additional, Raiteri, C. M., additional, Aller, H. D., additional, Aller, M. F., additional, Larionov, V. M., additional, Arkharov, A. A., additional, Blinov, D. A., additional, Efimova, N. V., additional, Grishina, T. S., additional, Hagen-Thorn, V. A., additional, Kopatskaya, E. N., additional, Larionova, L. V., additional, Larionova, E. G., additional, Morozova, D. A., additional, Troitsky, I. S., additional, Ligustri, R., additional, Calcidese, P., additional, Berdyugin, A., additional, Kurtanidze, O. M., additional, Nikolashvili, M. G., additional, Kimeridze, G. N., additional, Sigua, L. A., additional, Kurtanidze, S. O., additional, Chigladze, R. A., additional, Chen, W. P., additional, Koptelova, E., additional, Sakamoto, T., additional, Sadun, A. C., additional, Moody, J. W., additional, Pace, C., additional, Pearson, R., additional, Yatsu, Y., additional, Mori, Y., additional, Carraminyana, A., additional, Carrasco, L., additional, de la Fuente, E., additional, Norris, J. P., additional, Smith, P. S., additional, Wehrle, A., additional, Gurwell, M. A., additional, Zook, A., additional, Pagani, C., additional, Perri, M., additional, Capalbi, M., additional, Cesarini, A., additional, Krimm, H. A., additional, Kovalev, Y. Y., additional, Kovalev, Yu. A., additional, Ros, E., additional, Pushkarev, A. B., additional, Lister, M. L., additional, Sokolovsky, K. V., additional, Kadler, M., additional, Piner, G., additional, Lähteenmäki, A., additional, Tornikoski, M., additional, Angelakis, E., additional, Krichbaum, T. P., additional, Nestoras, I., additional, Fuhrmann, L., additional, Zensus, J. A., additional, Cassaro, P., additional, Orlati, A., additional, Maccaferri, G., additional, Leto, P., additional, Giroletti, M., additional, Richards, J. L., additional, Max-Moerbeck, W., additional, and Readhead, A. C. S., additional
Published: 2017
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47. Young, active radio stars in the AB Doradus moving group

Author: Azulay, R., primary, Guirado, J. C., additional, Marcaide, J. M., additional, Martí-Vidal, I., additional, Ros, E., additional, Tognelli, E., additional, Hormuth, F., additional, and Ortiz, J. L., additional
Published: 2017
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48. Absolute kinematics of radio-source components in the complete S5 polar cap sample

Author: Martí-Vidal, I., primary, Abellán, F. J., additional, Marcaide, J. M., additional, Guirado, J. C., additional, Pérez-Torres, M. A., additional, and Ros, E., additional
Published: 2016
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49. Discovery of off-axis jet structure of TeV blazar Mrk 501 with mm-VLBI

Author: Giroletti, M., Giovannini, G., Orienti, M., Ros, E., Savolainen, T., Krichbaum, T. P., Perez-Torres, M. A., Koyama, Shoko, Kino, Motoki, Doi, Akihiro, Hada, Kazuhiro, Niinuma, Kotaro, Nagai, Hiroshi, ITA, DEU, ESP, FIN, JPN, Junta de Andalucía, Ministerio de Economía y Competitividad (España), Japan Society for the Promotion of Science, Koyama, S., Kino, M., Giroletti, M., Doi, A., Giovannini, G., Orienti, M., Hada, K., Ros, E., Niinuma, K., Nagai, H., Savolainen, T., Krichbaum, T. P., Pérez-Torres, M. Á., Max-Planck-Institut für Radioastronomie, Korea Astronomy and Space Science Institute, INAF Istituto di Radioastronomia, Japan Aerospace Exploration Agency, National Astronomical Observatory of Japan, Yamaguchi University, Metsähovi Radio Observatory, Centro de Estudios de la Física del Cosmos de Aragón, Aalto-yliopisto, and Aalto University
Subjects: Astrofísica, active [Galaxies], 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Flux, Context (language use), galaxies [Radio continuum], Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Radio continuum: galaxies, individual: Markarian 501 [BL Lacertae objects], 0103 physical sciences, Very-long-baseline interferometry, Blazar, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Very Long Baseline Array, 0105 earth and related environmental sciences, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Jet (fluid), Spectral index, BL Lacertae objects: individual: Markarian 501, galaxies: active, galaxies: jets, radio continuum: galaxies, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Galaxies: active, Astrophysics - Astrophysics of Galaxies, BL Lacertae objects: individual: Markarian 501, Galaxies: jets, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astronomia, jets [Galaxies], Millimeter, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Context. High-resolution millimeter wave very-long-baseline interferometry (mm-VLBI) is an ideal tool for probing the structure at the base of extragalactic jets in detail. The TeV blazar Mrk 501 is one of the best targets among BL Lac objects for studying the nature of off-axis jet structures because it shows different jet position angles at different scales. Aims. The aim of this study is to investigate the properties of the off-axis jet structure through high-resolution mm-VLBI images at the jet base and physical parameters such as kinematics, flux densities, and spectral indices. Methods. We performed Very Long Baseline Array (VLBA) observations over six epochs from 2012 February to 2013 February at 43 GHz. Quasi-simultaneous Global Millimeter VLBI Array (GMVA) observations at 86 GHz were performed in May 2012. Results. We discover a new jet component at the northeast direction from the core in all the images at 43 and 86 GHz. The new component shows the off-axis location from the persistent jet extending to the southeast. The 43 GHz images reveal that the scattering of the positions of the NE component is within ∼0.2 mas. The 86 GHz data reveals a jet component located 0.75 mas southeast of the radio core. We also discuss the spectral indices between 43 and 86 GHz, where the northeast component has steeper spectral index and the southeast component has comparable or flatter index than the radio core does. © ESO, 2016., This work was partially supported by Grant-in-Aid for Scientific Research, KAKENHI 24340042 (A.D.) and 2450240 (M.K.) from the Japan Society for the Promotion of Science (JSPS). E.R. and M.A.P.T. acknowledge partial support from the Spanish MINECO through projects AYA-2012-38491-C02-01 and AYA-2012-38491-C02-02. E.R. also acknowledges partial support from the Generalitat Valenciana through project PROMETEOII/2014/057.
Published: 2016

50. Discovery of off-axis jet structure of TeV blazar Mrk 501 with mm-VLBI

Author: Junta de Andalucía, Ministerio de Economía y Competitividad (España), Japan Society for the Promotion of Science, Koyama, S., Kino, Motoki, Giroletti, M., Doi, A., Giovannini, G., Orienti, M., Hada, Kazuhiro, Ros, E., Niinuma, K., Nagai, H., Savolainen, T., Krichbaum, Thomas P., Pérez-Torres, Miguel A., Junta de Andalucía, Ministerio de Economía y Competitividad (España), Japan Society for the Promotion of Science, Koyama, S., Kino, Motoki, Giroletti, M., Doi, A., Giovannini, G., Orienti, M., Hada, Kazuhiro, Ros, E., Niinuma, K., Nagai, H., Savolainen, T., Krichbaum, Thomas P., and Pérez-Torres, Miguel A.
Abstract: Context. High-resolution millimeter wave very-long-baseline interferometry (mm-VLBI) is an ideal tool for probing the structure at the base of extragalactic jets in detail. The TeV blazar Mrk 501 is one of the best targets among BL Lac objects for studying the nature of off-axis jet structures because it shows different jet position angles at different scales. Aims. The aim of this study is to investigate the properties of the off-axis jet structure through high-resolution mm-VLBI images at the jet base and physical parameters such as kinematics, flux densities, and spectral indices. Methods. We performed Very Long Baseline Array (VLBA) observations over six epochs from 2012 February to 2013 February at 43 GHz. Quasi-simultaneous Global Millimeter VLBI Array (GMVA) observations at 86 GHz were performed in May 2012. Results. We discover a new jet component at the northeast direction from the core in all the images at 43 and 86 GHz. The new component shows the off-axis location from the persistent jet extending to the southeast. The 43 GHz images reveal that the scattering of the positions of the NE component is within ∼0.2 mas. The 86 GHz data reveals a jet component located 0.75 mas southeast of the radio core. We also discuss the spectral indices between 43 and 86 GHz, where the northeast component has steeper spectral index and the southeast component has comparable or flatter index than the radio core does. © ESO, 2016.
Published: 2016

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