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Farnocchia, D.Reddy, V.
Bauer, J.M.
Warner, E.M.
Micheli, M.
Payne, M.J.
Farnham, T.
Kelley, M.S.
Balam, D.D.
Barkov, A.P.
Berteşteanu, D.
Birlan, M.
Bolin, B.T.
Brucker, M.J.
Buzzi, L.
Chambers, K.C.
Demetz, L.
Djupvik, A.A.
Elenin, L.
Fini, P.
Flynn, R.
Galli, G.
Gao, X.
Gȩdek, M.
Granvik, M.
Hasubick, W.
Ivanov, A.L.
Ivanov, V.A.
Ivanova, N.V.
Jaques, C.
Kasikov, A.
Kim, M.-J.
Lane, D.
Lee, H.-J.
Li, B.
Li, F.
Lister, T.
Lysenko, V.E.
Magnier, E.A.
Mahomed, N.
McCormick, J.
Moon, D.
Nastasi, A.
Nedelcu, D.A.
Neue, G.
Petrescu, E.
Popescu, M.
Prosperi, E.
Reszelewski, R.
Roh, D.-G.
Romanov, F.D.
Santana-Ros, T.
Schmalz, A.
Schmalz, S.
Scotti, J.V.
Seaman, R.
Sioulas, N.
Sonka, A.B.
Tholen, D.J.
Trelia, M.M.
Wainscoat, R.
Wang, X.
Wells, G.
Weryk, R.
Yakovenko, N.A.
Ye, Q.
Yim, H.-S.
Zhai, C.
Zhang, C.
Zhao, H.
Zhu, T.
Żołnowski, M.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2022-07-13
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Institute of PhysicsCitation
Chang, C. L., & Fang, M. (2020, June). E-Learning and online instructions of higher education during the 2019 novel coronavirus diseases (COVID-19) epidemic. In Journal of Physics: Conference Series (Vol. 1574, No. 1, p. 012166). IOP Publishing.Journal
Planetary Science JournalRights
© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
As part of the International Asteroid Warning Network's observational exercises, we conducted a campaign to observe near-Earth asteroid 2019 XS around its close approach to Earth on 2021 November 9. The goal of the campaign was to characterize errors in the observation times reported to the Minor Planet Center, which become an increasingly important consideration as astrometric accuracy improves and more fast-moving asteroids are observed. As part of the exercise, a total of 957 astrometric observations of 2019 XS during the encounter were reported and subsequently were analyzed to obtain the corresponding residuals. While the timing errors are typically smaller than 1 s, the reported times appear to be negatively biased, i.e., they are generally earlier than they should be. We also compared the observer-provided position uncertainty with the cross-track residuals, which are independent of timing errors. A large fraction of the estimated uncertainties appear to be optimistic, especially when <0 2. We compiled individual reports for each observer to help identify and remove the root cause of any possible timing error and improve the uncertainty quantification process. We suggest possible sources of timing errors and describe a simple procedure to derive reliable, conservative position uncertainties. © 2022. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
2632-3338Version
Final published versionae974a485f413a2113503eed53cd6c53
10.3847/PSJ/ac7224
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Except where otherwise noted, this item's license is described as © 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.