Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science

The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and Time (LSST) in early to mid-2025. This multiband wide-field synoptic survey will transform our view of the solar system, with the discovery and monitoring of over five million small bodies. The final survey strategy ch...

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Published inThe Astrophysical journal. Supplement series Vol. 266; no. 2; pp. 22 - 89
Main Authors Schwamb, Megan E., Jones, R. Lynne, Yoachim, Peter, Volk, Kathryn, Dorsey, Rosemary C., Opitom, Cyrielle, Greenstreet, Sarah, Lister, Tim, Snodgrass, Colin, Bolin, Bryce T., Inno, Laura, Bannister, Michele T., Eggl, Siegfried, Solontoi, Michael, Kelley, Michael S. P., Jurić, Mario, Lin, Hsing Wen, Ragozzine, Darin, Bernardinelli, Pedro H., Chesley, Steven R., Daylan, Tansu, Ďurech, Josef, Fraser, Wesley C., Granvik, Mikael, Knight, Matthew M., Lisse, Carey M., Malhotra, Renu, Oldroyd, William J., Thirouin, Audrey, Ye, Quanzhi
Format Journal Article
LanguageEnglish
Published Saskatoon The American Astronomical Society 01.06.2023
American Astronomical Society
IOP Publishing
Subjects
Asteroids
ASTRONOMY AND ASTROPHYSICS
Comets
Dwarf planets
Interstellar objects
Interstellar space
Main belt asteroids
Near-Earth objects
Observatories
Onboard Space Systems
Optimization
Polls & surveys
Rymdtekniska system
Science
Simulation
Sky surveys
Small Solar System bodies
Solar system
Trans-Neptunian objects
Tuning
Online AccessGet full text
ISSN0067-0049
1538-4365
1538-4365
DOI10.3847/1538-4365/acc173

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Abstract The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and Time (LSST) in early to mid-2025. This multiband wide-field synoptic survey will transform our view of the solar system, with the discovery and monitoring of over five million small bodies. The final survey strategy chosen for LSST has direct implications on the discoverability and characterization of solar system minor planets and passing interstellar objects. Creating an inventory of the solar system is one of the four main LSST science drivers. The LSST observing cadence is a complex optimization problem that must balance the priorities and needs of all the key LSST science areas. To design the best LSST survey strategy, a series of operation simulations using the Rubin Observatory scheduler have been generated to explore the various options for tuning observing parameters and prioritizations. We explore the impact of the various simulated LSST observing strategies on studying the solar system's small body reservoirs. We examine what are the best observing scenarios and review what are the important considerations for maximizing LSST solar system science. In general, most of the LSST cadence simulations produce ±5% or less variations in our chosen key metrics, but a subset of the simulations significantly hinder science returns with much larger losses in the discovery and light-curve metrics.
NRC publication: Yes
AbstractList The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and Time (LSST) in early to mid-2025. This multiband wide-field synoptic survey will transform our view of the solar system, with the discovery and monitoring of over five million small bodies. The final survey strategy chosen for LSST has direct implications on the discoverability and characterization of solar system minor planets and passing interstellar objects. Creating an inventory of the solar system is one of the four main LSST science drivers. The LSST observing cadence is a complex optimization problem that must balance the priorities and needs of all the key LSST science areas. To design the best LSST survey strategy, a series of operation simulations using the Rubin Observatory scheduler have been generated to explore the various options for tuning observing parameters and prioritizations. We explore the impact of the various simulated LSST observing strategies on studying the solar system's small body reservoirs. We examine what are the best observing scenarios and review what are the important considerations for maximizing LSST solar system science. In general, most of the LSST cadence simulations produce ±5% or less variations in our chosen key metrics, but a subset of the simulations significantly hinder science returns with much larger losses in the discovery and light-curve metrics.
The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and Time (LSST) in early to mid-2025. This multiband wide-field synoptic survey will transform our view of the solar system, with the discovery and monitoring of over five million small bodies. The final survey strategy chosen for LSST has direct implications on the discoverability and characterization of solar system minor planets and passing interstellar objects. Creating an inventory of the solar system is one of the four main LSST science drivers. The LSST observing cadence is a complex optimization problem that must balance the priorities and needs of all the key LSST science areas. To design the best LSST survey strategy, a series of operation simulations using the Rubin Observatory scheduler have been generated to explore the various options for tuning observing parameters and prioritizations. We explore the impact of the various simulated LSST observing strategies on studying the solar system's small body reservoirs. We examine what are the best observing scenarios and review what are the important considerations for maximizing LSST solar system science. In general, most of the LSST cadence simulations produce +/- 5% or less variations in our chosen key metrics, but a subset of the simulations significantly hinder science returns with much larger losses in the discovery and light-curve metrics.
Author Malhotra, Renu
Opitom, Cyrielle
Dorsey, Rosemary C.
Schwamb, Megan E.
Solontoi, Michael
Chesley, Steven R.
Knight, Matthew M.
Lisse, Carey M.
Oldroyd, William J.
Bannister, Michele T.
Eggl, Siegfried
Kelley, Michael S. P.
Granvik, Mikael
Lister, Tim
Lin, Hsing Wen
Bernardinelli, Pedro H.
Ďurech, Josef
Ye, Quanzhi
Bolin, Bryce T.
Daylan, Tansu
Snodgrass, Colin
Inno, Laura
Yoachim, Peter
Greenstreet, Sarah
Ragozzine, Darin
Thirouin, Audrey
Jurić, Mario
Jones, R. Lynne
Fraser, Wesley C.
Volk, Kathryn
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CorporateAuthor SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
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  ident: apjsacc173bib192
  doi: 10.5281/zenodo.7374619
– volume: 493
  start-page: L129
  year: 2020
  ident: apjsacc173bib74
  publication-title: MNRAS
  doi: 10.1093/mnrasl/slaa025
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Snippet The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and Time (LSST) in early to mid-2025. This multiband wide-field synoptic survey...
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StartPage 22
SubjectTerms Asteroids
ASTRONOMY AND ASTROPHYSICS
Comets
Dwarf planets
Interstellar objects
Interstellar space
Main belt asteroids
Near-Earth objects
Observatories
Onboard Space Systems
Optimization
Polls & surveys
Rymdtekniska system
Science
Simulation
Sky surveys
Small Solar System bodies
Solar system
Trans-Neptunian objects
Tuning
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Title Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science
URI https://iopscience.iop.org/article/10.3847/1538-4365/acc173
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