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The Future Of The Arecibo Observatory: The Next Generation Arecibo Telescope

Anish Roshi, D. and Aponte, N. and Araya, E. and Arce, H. and Baker, L. A. and Baan, W. and Becker, T. M. and Breakall, J. K. and Brown, R. G. and Brum, C. G. M. and Busch, M. and Campbell, D. B. and Cohen, T. and Cordova, F. and Deneva, J. S. and Devogele, M. and Dolch, T. and Fernandez-Rodriguez, F. O. and Ghosh, T. and Goldsmith, P. F. and Gurvits, L. I. and Haynes, M. and Heiles, C. and Hessel, J. W. T. and Hickson, D. and Isham, B. and Kerr, R. B. and Kelly, J. and Kiriazes, J. J. and Lautenbach, J. and Lebron, M. and Lewandowska, N. and Magnani, L. and Manoharan, P. K. and Margot, J. L. and Marshall, S. E. and McGilvray, A. K. and Mendez, A. and Minchin, R. and Negron, V. and Nolan, M. C. and Olmi, L. and Paganelli, F. and Palliyaguru, N. T. and Pantoja, C. A. and Paragi, Z. and Parshley, S. C. and Peek, J. E. G. and Perera, B. B. P. and Perillat, P. and Pinilla-Alonso, N. and Quintero, L. and Radovan, H. and Raizada, S. and Robishaw, T. and Route, M. and Salter, C. J. and Santoni, A. and Santos, P. and Sau, S. and Selvaraj, D. and Smith, A. J. and Sulzer, M. and Vaddi, S. and Vargas, F. and Venditti, F. C. F. and Venkataraman, A. and Verkouter, H. and Virkki, A. K. and Vishwas, A. and Weinreb, S. and Werthimer, D. and Wolszczan, A. and Zambrano-Marin, L. F. (2021) The Future Of The Arecibo Observatory: The Next Generation Arecibo Telescope. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20210520-150021870

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Abstract

The Arecibo Observatory (AO) is a multidisciplinary research and education facility that is recognized worldwide as a leading facility in astronomy, planetary, and atmospheric and space sciences. AO's cornerstone research instrument was the 305-m William E. Gordon telescope. On December 1, 2020, the 305-m telescope collapsed and was irreparably damaged. In the three weeks following the collapse, AO's scientific and engineering staff and the AO users community initiated extensive discussions on the future of the observatory. The community is in overwhelming agreement that there is a need to build an enhanced, next-generation radar-radio telescope at the AO site. From these discussions, we established the set of science requirements the new facility should enable. These requirements can be summarized briefly as: 5 MW of continuous wave transmitter power at 2 - 6 GHz, 10 MW of peak transmitter power at 430 MHz (also at 220MHz under consideration), zenith angle coverage 0 to 48 deg, frequency coverage 0.2 to 30 GHz and increased Field-of-View. These requirements determine the unique specifications of the proposed new instrument. The telescope design concept we suggest consists of a compact array of fixed dishes on a tiltable, plate-like structure with a collecting area equivalent to a 300m dish. This concept, referred to as the Next Generation Arecibo Telescope (NGAT), meets all of the desired specifications and provides significant new science capabilities to all three research groups at AO. This whitepaper presents a sample of the wide variety of the science that can be achieved with the NGAT, the details of the telescope design concept and the need for the new telescope to be located at the AO site. We also discuss other AO science activities that interlock with the NGAT in the white paper.


Item Type:Report or Paper (White Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/2103.01367arXivDiscussion Paper
ORCID:
AuthorORCID
Goldsmith, P. F.0000-0002-6622-8396
Weinreb, S.0000-0002-9353-6204
Additional Information:We are grateful to the Arecibo Observatory users’ community for the invaluable support, comments, and discussion that helped us to write this white paper with a short notice. Special thanks to Joanna Rankin from University of Vermont, who led the organization of the AO’s user community and Pia Salter for her enthusiastic support to the effort for Arecibo telescope reconstruction. We thank the technical staff of the AO, as well as Dr. Shaffer and the UNC-URSI community for their suggestions and inputs while preparing the white paper. We also greatly appreciate valuable input from Gordon Lacy, Mohammad Islam, and Dean Chalmers at NRC Canada; Peter Dewdney from SKA; Larry D’Addario from Caltech; Anthony van Eyken from SRI International; Alex Kraus from MPIFR, Bonn; Chip Cohen from Fractal Antenna Systems; Tim Bastian from NRAO, Timothy Kennedy from the NASA Johnson Space Center and Catherine Neish from Western University. A huge thanks to B. Serna, SwRI, Texas, for helping with the formatting of the whitepaper.
Record Number:CaltechAUTHORS:20210520-150021870
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210520-150021870
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:109227
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:24 May 2021 14:13
Last Modified:24 May 2021 14:13

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