A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Predictions of the LSST Solar System Yield: Discovery Rates and Characterizations of Centaurs
Tekijät: Murtagh, Joseph; Schwamb, Megan E.; Merritt, Stephanie R.; Bernardinelli, Pedro H.; Kurlander, Jacob A.; Cornwall, Samuel; Juric, Mario; Fedorets, Grigori; Holman, Matthew J.; Eggl, Siegfried; Nesvorny, David; Volk, Kathryn; Jones, R. Lynne; Yoachim, Peter; Moeyens, Joachim; Kubica, Jeremy; Oldag, Drew; West, Maxine; Chandler, Colin Orion
Kustantaja: American Astronomical Society
Kustannuspaikka: BRISTOL
Julkaisuvuosi: 2025
Lehti:: The Astronomical Journal
Tietokannassa oleva lehden nimi: The Astronomical Journal
Lehden akronyymi: ASTRON J
Artikkelin numero: 98
Vuosikerta: 170
Numero: 2
Sivujen määrä: 18
ISSN: 0004-6256
eISSN: 1538-3881
DOI: https://doi.org/10.3847/1538-3881/ade1db
Verkko-osoite: https://doi.org/10.3847/1538-3881/ade1db
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/499425801
The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will start by the end of 2025 and operate for 10 yr, offering billions of observations of the southern night sky. One of its main science goals is to create an inventory of the solar system, allowing for a more detailed understanding of small-body populations, including the Centaurs, which will benefit from the survey's high cadence and depth. In this paper, we establish the first discovery limits for Centaurs throughout the LSST's decade-long operation using the best available dynamical models. Using the survey simulator Sorcha, we predict a roughly 7-fold increase in Centaurs in the Minor Planet Center (MPC) database, reaching similar to 1200-2000 (dependent on definition) by the end of the survey- about 50% of which are expected within the first 2 yr. Approximately 30-50 Centaurs will be observed twice as frequently, as they fall within one of the LSST's Deep Drilling Fields (DDF) for on average only up to 2 months. Outside of the DDFs, Centaurs will receive similar to 200 observations across the ugrizy filter range, facilitating searches for cometary-like activity through point-spread function extension analysis, as well as fitting light curves and phase curves for color determination. Regardless of definition, over 200 Centaurs will achieve high-quality color measurements across at least three filters in the LSST's six filters. These observations will also provide over 300 well-defined phase curves in the griz bands, improving absolute magnitude measurements to a precision of 0.2 mag.
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Julkaisussa olevat rahoitustiedot:
This work was supported by a LSST Discovery Alliance LINCC Frameworks Incubator grant [2023-SFF-LFI-01-Schwamb]. Support was provided by Schmidt Sciences. J.M. acknowledges support from the Department for the Economy (DfE) Northern Ireland postgraduate studentship scheme and travel support from the STFC for UK participation in LSST through grant ST/S006206/1. M.E.S. and S.R.M. acknowledge support in part from UK Science and Technology Facilities Council (STFC) grants ST/V000691/1 and ST/X001253/1. M.J., P.H.B., and J.A.K. acknowledge the support from the University of Washington College of Arts and Sciences, Department of Astronomy, and the DiRAC Institute. The DiRAC Institute is supported through generous gifts from the Charles and Lisa Simonyi Fund for Arts and Sciences and the Washington Research Foundation. M.J. wishes to acknowledge the support of the Washington Research Foundation Data Science Term Chair fund and the University of Washington Provost's Initiative in Data-Intensive Discovery. J.M and J.A.K. thank the LSST-DA Data Science Fellowship Program, which is funded by LSST-DA, the Brinson Foundation, and the Moore Foundation; their participation in the program has benefited this work. K.V. acknowledges support from NASA (grants 80NSSC23K1169 and 80NSSC23K0886). S.C. and S.E. acknowledge support by the National Science Foundation through award AST-2307570. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the authors and do not necessarily reflect the views of the National Science Foundation.
