EPSC Abstracts
Vol. 18, EPSC-DPS2025-979, 2025, updated on 09 Jul 2025
https://doi.org/10.5194/epsc-dps2025-979
EPSC-DPS Joint Meeting 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Layup: orbit fitting at LSST Scale
Pedro H. Bernardinelli1, Matthew Holman2, Meg Schwamb3, Kevin Napier2,4, Thomas Ruch4, Joseph Murtagh3, Ryan Lyttle3, Rahil Makadia5, Drew Oldag1,6, Max West1,6, Wilson Beebe1,6, Hanno Rein7, Carrie Holt8, Siegfried Eggl5, Colin Chandler1,6, Jeremy Kubica6,9, and Mario Juric1
Pedro H. Bernardinelli et al.
  • 1University of Washington, United States of America (phbern@uw.edu)
  • 2Center for Astrophysics | Harvard & Smithsonian
  • 3Astrophysics Research Centre, Queen’s University Belfast
  • 4University of Michigan
  • 5Department of Aerospace Engineering, University of Illinois at Urbana-Champaign
  • 6LSST Interdisciplinary Network for Collaboration and Computing
  • 7Department of Physical and Environmental Sciences, University of Toronto at Scarborough
  • 8Las Cumbres Observatory
  • 9McWilliams Center for Cosmology and Astrophysics, Department of Physics, Carnegie Mellon University

Starting later this year, the Vera C. Rubin’s Observatory’s Legacy Survey of Space and Time (LSST) will begin discovering millions of new Solar System objects, ranging from the closest near-Earth asteroids to the most distant trans-Neptunian objects.  Fitting the orbits of those objects (the process of taking the observed on-sky positions and velocities of newly discovered moving Solar System objects and transforming them into orbital parameters) is essential to LSST Solar System science.  To address this challenge, we present Layup, a modern and open-source orbit fitting software suite built in Python and C++, driven with the ephemeris quality orbit integrator ASSIST (Holman et al 2023) and built in collaboration with the LINCC Framework team of software engineers, as part of their Incubator program. In addition to handling the large data volume expected from LSST, Layup also has the capability to handle observations from shift-and-stack and ranging data, routines for converting orbits and uncertainties across different formats, and a special-purpose integrator to derive cometary semi-major axes upon entry in the planetary region, as well as accurate, publication quality visualization tools.



How to cite: Bernardinelli, P. H., Holman, M., Schwamb, M., Napier, K., Ruch, T., Murtagh, J., Lyttle, R., Makadia, R., Oldag, D., West, M., Beebe, W., Rein, H., Holt, C., Eggl, S., Chandler, C., Kubica, J., and Juric, M.: Layup: orbit fitting at LSST Scale, EPSC-DPS Joint Meeting 2025, Helsinki, Finland, 7–12 Sep 2025, EPSC-DPS2025-979, https://doi.org/10.5194/epsc-dps2025-979, 2025.