Roman Observations Time Allocation Committee Final Report and Recommendations

dc.contributor.authorZasowski, Gail
dc.contributor.authorJha, Saurabh W.
dc.contributor.authorChomiuk, Laura
dc.contributor.authorFan, Xiaohui
dc.contributor.authorHickox, Ryan
dc.contributor.authorHuber, Dan
dc.contributor.authorKerins, Eamonn
dc.contributor.authorKobulnicky, Chip
dc.contributor.authorLauer, Tod
dc.contributor.authorSako, Masao
dc.contributor.authorShapley, Alice
dc.contributor.authorStephens, Denise
dc.contributor.authorWeinberg, David
dc.contributor.authorWilliams, Ben
dc.contributor.authorBarclay, Thomas
dc.date.accessioned2025-06-17T14:44:55Z
dc.date.available2025-06-17T14:44:55Z
dc.date.issued2025-04-24
dc.description.abstractThe Nancy Grace Roman Space Telescope is poised to revolutionize our scientific understanding of exoplanets, dark matter, dark energy, and general astrophysics, including through an innovative community approach to defining and executing sky surveys. The Roman Observations Time Allocation Committee (ROTAC) was convened to recommend time allocations for the three Core Community Surveys (CCS) using the Wide Field Instrument (WFI): the High Latitude Wide Area Survey, the High Latitude Time Domain Survey, and the Galactic Bulge Time Domain Survey, as well as balance the time allocation for the General Astrophysics Surveys. Each CCS had a corresponding Definition Committee that collected community input and designed proposals for a nominal (in-guide) survey, as well as underguide and overguide options with smaller and larger time allocations, respectively. These options explored different ways of fulfilling the mission science requirements while maximizing general astrophysics science goals enabled by the surveys. In this report, the ROTAC lays out its recommendations for the three CCS observing designs and the WFI time allotment for CCS (74.5%) and the General Astrophysics Surveys (25.5%).
dc.description.urihttps://arxiv.org/pdf/2505.10574
dc.format.extent165 pages
dc.genrereports
dc.genrepreprints
dc.identifierdoi:10.13016/m27xge-eksi
dc.identifier.urihttps://doi.org/10.48550/arXiv.2505.10574
dc.identifier.urihttp://hdl.handle.net/11603/38806
dc.language.isoen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rightsPublic Domain
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.titleRoman Observations Time Allocation Committee Final Report and Recommendations
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0001-7139-2724

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