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Autori principali:	Kadler, M., Riechers, D. A., Agarwal, J., Baczko, A. -K., Beuther, H., Bigiel, F., Birnstiel, T., Boccardi, B., Bomans, D. J., Boogaard, L., Braun, T. T., Britzen, S., Brüggen, M., Brunthaler, A., Caselli, P., Elsässer, D., von Fellenberg, S., Flock, M., Fromm, C. M., Fuhrmann, L., Hartogh, P., Hoeft, M., Keenan, R. P., Kovalev, Y., Kreckel, K., Livingston, J., Lobanov, A. P., Müller, H., Ros, E., Schilke, P., De Simone, M., Spitler, L., Ueda, T., Vardoulaki, E., Vegetti, S., Weis, K., Wendel, C., Xu, M. H., Zhao, G. -Y., Albrecht, M., Basu, A., Tjus, J. Becker, Bernhart, S., Blum, J., Bonnassieux, E., Bredendiek, C., van Delden, M., Di Gennaro, G., Enders, A., Eppel, F., Hase, H., Hoang, D., Hugentobler, U., Kaasinen, M., Krupp, N., Kun, E., Laubach, M., Lin, Y., Mannheim, K., Menten, K. M., Perkuhn, R., Pohl, N., Powell, D. M., Rezzolla, L., Ricci, L., Schinnerer, E., Schmidt, K., Schöpfel, J., Stanko, S., Stein, M., Sulzenauer, N., Taziaux, S., Tursunov, A., Walter, F., Weiss, A., Witzel, G., Wolf, S., Zensus, J. A., Mus, A., Toth, L. V., Alberdi, A., Benisty, M., Cox, P., Guirado, J. C., Johnson, M. D., Juvela, M., Neeleman, M., Pashchenko, I. N., Torres, M. A. Pérez, Perraut, K., Zajacek, M.
Natura:	Preprint
Pubblicazione:	2023
Soggetti:	Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics Earth and Planetary Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Accesso online:	https://arxiv.org/abs/2311.10056
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_version_	1866929390703607808
author	Kadler, M. Riechers, D. A. Agarwal, J. Baczko, A. -K. Beuther, H. Bigiel, F. Birnstiel, T. Boccardi, B. Bomans, D. J. Boogaard, L. Braun, T. T. Britzen, S. Brüggen, M. Brunthaler, A. Caselli, P. Elsässer, D. von Fellenberg, S. Flock, M. Fromm, C. M. Fuhrmann, L. Hartogh, P. Hoeft, M. Keenan, R. P. Kovalev, Y. Kreckel, K. Livingston, J. Lobanov, A. P. Müller, H. Ros, E. Schilke, P. De Simone, M. Spitler, L. Ueda, T. Vardoulaki, E. Vegetti, S. Weis, K. Wendel, C. Xu, M. H. Zhao, G. -Y. Albrecht, M. Basu, A. Tjus, J. Becker Bernhart, S. Blum, J. Bonnassieux, E. Bredendiek, C. van Delden, M. Di Gennaro, G. Enders, A. Eppel, F. Hase, H. Hoang, D. Hugentobler, U. Kaasinen, M. Krupp, N. Kun, E. Laubach, M. Lin, Y. Mannheim, K. Menten, K. M. Perkuhn, R. Pohl, N. Powell, D. M. Rezzolla, L. Ricci, L. Schinnerer, E. Schmidt, K. Schöpfel, J. Stanko, S. Stein, M. Sulzenauer, N. Taziaux, S. Tursunov, A. Walter, F. Weiss, A. Witzel, G. Wolf, S. Zensus, J. A. Mus, A. Toth, L. V. Alberdi, A. Benisty, M. Cox, P. Guirado, J. C. Johnson, M. D. Juvela, M. Neeleman, M. Pashchenko, I. N. Torres, M. A. Pérez Perraut, K. Zajacek, M.
author_facet	Kadler, M. Riechers, D. A. Agarwal, J. Baczko, A. -K. Beuther, H. Bigiel, F. Birnstiel, T. Boccardi, B. Bomans, D. J. Boogaard, L. Braun, T. T. Britzen, S. Brüggen, M. Brunthaler, A. Caselli, P. Elsässer, D. von Fellenberg, S. Flock, M. Fromm, C. M. Fuhrmann, L. Hartogh, P. Hoeft, M. Keenan, R. P. Kovalev, Y. Kreckel, K. Livingston, J. Lobanov, A. P. Müller, H. Ros, E. Schilke, P. De Simone, M. Spitler, L. Ueda, T. Vardoulaki, E. Vegetti, S. Weis, K. Wendel, C. Xu, M. H. Zhao, G. -Y. Albrecht, M. Basu, A. Tjus, J. Becker Bernhart, S. Blum, J. Bonnassieux, E. Bredendiek, C. van Delden, M. Di Gennaro, G. Enders, A. Eppel, F. Hase, H. Hoang, D. Hugentobler, U. Kaasinen, M. Krupp, N. Kun, E. Laubach, M. Lin, Y. Mannheim, K. Menten, K. M. Perkuhn, R. Pohl, N. Powell, D. M. Rezzolla, L. Ricci, L. Schinnerer, E. Schmidt, K. Schöpfel, J. Stanko, S. Stein, M. Sulzenauer, N. Taziaux, S. Tursunov, A. Walter, F. Weiss, A. Witzel, G. Wolf, S. Zensus, J. A. Mus, A. Toth, L. V. Alberdi, A. Benisty, M. Cox, P. Guirado, J. C. Johnson, M. D. Juvela, M. Neeleman, M. Pashchenko, I. N. Torres, M. A. Pérez Perraut, K. Zajacek, M.
contents	The Next Generation Very Large Array (ngVLA) is a planned radio interferometer providing unprecedented sensitivity at wavelengths between 21 cm and 3 mm. Its 263 antenna element array will be spatially distributed across North America to enable both superb low surface brightness recovery and sub-milliarcsecond angular resolution imaging. The project was developed by the international astronomy community under the lead of the National Radio Astronomy Observatory (NRAO), and is anticipated to be built between 2027 and 2037. Two workshops have been held in 2022 and 2023 with the goal to discuss and consolidate the scientific interests in the ngVLA within the German astronomical community. This community paper constitutes a collection of 48 science ideas which the German community aims to pursue with the ngVLA in the 2030s. This is not a complete list and the ideas are not developed at the level of a "Science Book", such that the present document is mainly meant provide a basis for further discussion within the community. As such, additional contributions are welcome, and will be considered for inclusion in future revisions.
format	Preprint
id	arxiv_https___arxiv_org_abs_2311_10056
institution	arXiv
publishDate	2023
record_format	arxiv
spellingShingle	A Collection of German Science Interests in the Next Generation Very Large Array Kadler, M. Riechers, D. A. Agarwal, J. Baczko, A. -K. Beuther, H. Bigiel, F. Birnstiel, T. Boccardi, B. Bomans, D. J. Boogaard, L. Braun, T. T. Britzen, S. Brüggen, M. Brunthaler, A. Caselli, P. Elsässer, D. von Fellenberg, S. Flock, M. Fromm, C. M. Fuhrmann, L. Hartogh, P. Hoeft, M. Keenan, R. P. Kovalev, Y. Kreckel, K. Livingston, J. Lobanov, A. P. Müller, H. Ros, E. Schilke, P. De Simone, M. Spitler, L. Ueda, T. Vardoulaki, E. Vegetti, S. Weis, K. Wendel, C. Xu, M. H. Zhao, G. -Y. Albrecht, M. Basu, A. Tjus, J. Becker Bernhart, S. Blum, J. Bonnassieux, E. Bredendiek, C. van Delden, M. Di Gennaro, G. Enders, A. Eppel, F. Hase, H. Hoang, D. Hugentobler, U. Kaasinen, M. Krupp, N. Kun, E. Laubach, M. Lin, Y. Mannheim, K. Menten, K. M. Perkuhn, R. Pohl, N. Powell, D. M. Rezzolla, L. Ricci, L. Schinnerer, E. Schmidt, K. Schöpfel, J. Stanko, S. Stein, M. Sulzenauer, N. Taziaux, S. Tursunov, A. Walter, F. Weiss, A. Witzel, G. Wolf, S. Zensus, J. A. Mus, A. Toth, L. V. Alberdi, A. Benisty, M. Cox, P. Guirado, J. C. Johnson, M. D. Juvela, M. Neeleman, M. Pashchenko, I. N. Torres, M. A. Pérez Perraut, K. Zajacek, M. Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics Earth and Planetary Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics The Next Generation Very Large Array (ngVLA) is a planned radio interferometer providing unprecedented sensitivity at wavelengths between 21 cm and 3 mm. Its 263 antenna element array will be spatially distributed across North America to enable both superb low surface brightness recovery and sub-milliarcsecond angular resolution imaging. The project was developed by the international astronomy community under the lead of the National Radio Astronomy Observatory (NRAO), and is anticipated to be built between 2027 and 2037. Two workshops have been held in 2022 and 2023 with the goal to discuss and consolidate the scientific interests in the ngVLA within the German astronomical community. This community paper constitutes a collection of 48 science ideas which the German community aims to pursue with the ngVLA in the 2030s. This is not a complete list and the ideas are not developed at the level of a "Science Book", such that the present document is mainly meant provide a basis for further discussion within the community. As such, additional contributions are welcome, and will be considered for inclusion in future revisions.
title	A Collection of German Science Interests in the Next Generation Very Large Array
topic	Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics Earth and Planetary Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
url	https://arxiv.org/abs/2311.10056

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