The LSST Cadence Impact on Non-time-critical Eclipsing Binary Science

The Legacy Survey of Space and Time (LSST) is slated to commence in 2025 at the Vera Rubin Observatory. One of the crucial parts of preparing the survey is the choice of observing cadence in an effort to optimize auxiliary science goals while maintaining the core project requirements. Here we look a...

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Main Authors: Andrej Prša, Peter Yoachim, Lynne Jones
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Online Access:https://doi.org/10.3847/1538-4365/acda31
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author Andrej Prša
Peter Yoachim
Lynne Jones
author_facet Andrej Prša
Peter Yoachim
Lynne Jones
author_sort Andrej Prša
collection DOAJ
description The Legacy Survey of Space and Time (LSST) is slated to commence in 2025 at the Vera Rubin Observatory. One of the crucial parts of preparing the survey is the choice of observing cadence in an effort to optimize auxiliary science goals while maintaining the core project requirements. Here we look at the impact of proposed cadences, encoded in different operation simulations (opsims), on non-time-critical eclipsing binary science. This is particularly pertinent because LSST is the first large-scale survey that will provide us with color information in addition to high-precision coverage of faint targets. We study the differences between the baseline opsim v2.1 and the latest opsim v3.0 runs. We find that all runs provide sufficient data coverage to enable in-depth studies in the field of eclipsing binaries, and that there are no adverse impacts from any proposed opsim modification studied here.
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spelling doaj.art-a04a141b98164897844d0b61fa4551442023-09-03T12:27:22ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492023-01-0126722210.3847/1538-4365/acda31The LSST Cadence Impact on Non-time-critical Eclipsing Binary ScienceAndrej Prša0https://orcid.org/0000-0002-1913-0281Peter Yoachim1https://orcid.org/0000-0003-2874-6464Lynne Jones2https://orcid.org/0000-0001-5916-0031Villanova University , Department of Astrophysics and Planetary Sciences, 800 Lancaster Ave., Villanova, PA 19085, USA ; aprsa@villanova.eduDepartment of Astronomy and the DiRAC Institute, University of Washington , Seattle, WA, USAAerotek / Rubin Observatory , Victoria, BC, CanadaThe Legacy Survey of Space and Time (LSST) is slated to commence in 2025 at the Vera Rubin Observatory. One of the crucial parts of preparing the survey is the choice of observing cadence in an effort to optimize auxiliary science goals while maintaining the core project requirements. Here we look at the impact of proposed cadences, encoded in different operation simulations (opsims), on non-time-critical eclipsing binary science. This is particularly pertinent because LSST is the first large-scale survey that will provide us with color information in addition to high-precision coverage of faint targets. We study the differences between the baseline opsim v2.1 and the latest opsim v3.0 runs. We find that all runs provide sufficient data coverage to enable in-depth studies in the field of eclipsing binaries, and that there are no adverse impacts from any proposed opsim modification studied here.https://doi.org/10.3847/1538-4365/acda31Optical astronomyEclipsing binary starsOptical observatories
spellingShingle Andrej Prša
Peter Yoachim
Lynne Jones
The LSST Cadence Impact on Non-time-critical Eclipsing Binary Science
The Astrophysical Journal Supplement Series
Optical astronomy
Eclipsing binary stars
Optical observatories
title The LSST Cadence Impact on Non-time-critical Eclipsing Binary Science
title_full The LSST Cadence Impact on Non-time-critical Eclipsing Binary Science
title_fullStr The LSST Cadence Impact on Non-time-critical Eclipsing Binary Science
title_full_unstemmed The LSST Cadence Impact on Non-time-critical Eclipsing Binary Science
title_short The LSST Cadence Impact on Non-time-critical Eclipsing Binary Science
title_sort lsst cadence impact on non time critical eclipsing binary science
topic Optical astronomy
Eclipsing binary stars
Optical observatories
url https://doi.org/10.3847/1538-4365/acda31
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