Sorcha: Optimized Solar System Ephemeris Generation

Fuente: arXiv
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Autori principali: Holman, Matthew J., Bernardinelli, Pedro H., Schwamb, Megan E., Jurić, Mario, Oldag, Drew, West, Maxine, Napier, Kevin J., Merritt, Stephanie R., Fedorets, Grigori, Cornwall, Samuel, Kurlander, Jacob A., Eggl, Siegfried, Kubica, Jeremy, Kiker, Kathleen, Murtagh, Joseph, Naidu, Shantanu P., Chandler, Colin Orion
Natura: Preprint
Pubblicazione: 2025
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author Holman, Matthew J.
Bernardinelli, Pedro H.
Schwamb, Megan E.
Jurić, Mario
Oldag, Drew
West, Maxine
Napier, Kevin J.
Merritt, Stephanie R.
Fedorets, Grigori
Cornwall, Samuel
Kurlander, Jacob A.
Eggl, Siegfried
Kubica, Jeremy
Kiker, Kathleen
Murtagh, Joseph
Naidu, Shantanu P.
Chandler, Colin Orion
author_facet Holman, Matthew J.
Bernardinelli, Pedro H.
Schwamb, Megan E.
Jurić, Mario
Oldag, Drew
West, Maxine
Napier, Kevin J.
Merritt, Stephanie R.
Fedorets, Grigori
Cornwall, Samuel
Kurlander, Jacob A.
Eggl, Siegfried
Kubica, Jeremy
Kiker, Kathleen
Murtagh, Joseph
Naidu, Shantanu P.
Chandler, Colin Orion
contents Sorcha is a solar system survey simulator built for the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) and future large-scale wide-field surveys. Over the ten-year survey, the LSST is expected to collect roughly a billion observations of minor planets. The task of a solar system survey simulator is to take a set of input objects (described by orbits and physical properties) and determine what a real or hypothetical survey would have discovered. Existing survey simulators have a computational bottleneck in determining which input objects lie in each survey field, making them infeasible for LSST data scales. Sorcha can swiftly, efficiently, and accurately calculate the on-sky positions for sets of millions of input orbits and surveys with millions of visits, identifying which exposures these objects cross, in order for later stages of the software to make detailed estimates of the apparent magnitude and detectability of those input small bodies. In this paper, we provide the full details of the algorithm and software behind Sorcha's ephemeris generator. Like many of Sorcha's components, its ephemeris generator can be easily used for other surveys.
format Preprint
id arxiv_https___arxiv_org_abs_2506_02140
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Sorcha: Optimized Solar System Ephemeris Generation
Holman, Matthew J.
Bernardinelli, Pedro H.
Schwamb, Megan E.
Jurić, Mario
Oldag, Drew
West, Maxine
Napier, Kevin J.
Merritt, Stephanie R.
Fedorets, Grigori
Cornwall, Samuel
Kurlander, Jacob A.
Eggl, Siegfried
Kubica, Jeremy
Kiker, Kathleen
Murtagh, Joseph
Naidu, Shantanu P.
Chandler, Colin Orion
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Computational Physics
Sorcha is a solar system survey simulator built for the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) and future large-scale wide-field surveys. Over the ten-year survey, the LSST is expected to collect roughly a billion observations of minor planets. The task of a solar system survey simulator is to take a set of input objects (described by orbits and physical properties) and determine what a real or hypothetical survey would have discovered. Existing survey simulators have a computational bottleneck in determining which input objects lie in each survey field, making them infeasible for LSST data scales. Sorcha can swiftly, efficiently, and accurately calculate the on-sky positions for sets of millions of input orbits and surveys with millions of visits, identifying which exposures these objects cross, in order for later stages of the software to make detailed estimates of the apparent magnitude and detectability of those input small bodies. In this paper, we provide the full details of the algorithm and software behind Sorcha's ephemeris generator. Like many of Sorcha's components, its ephemeris generator can be easily used for other surveys.
title Sorcha: Optimized Solar System Ephemeris Generation
topic Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Computational Physics
url https://arxiv.org/abs/2506.02140