TESSELLATE: Piecing Together the Variable Sky With TESS

dc.contributor.authorRoxburgh, Hugh
dc.contributor.authorRidden-Harper, Ryan
dc.contributor.authorMoore, Andrew
dc.contributor.authorMontilla, Clarinda
dc.contributor.authorLeicester, Brayden
dc.contributor.authorLane, Zachary G.
dc.contributor.authorFreeburn, James
dc.contributor.authorRest, Armin
dc.contributor.authorBannister, Michele T.
dc.contributor.authorRidden-Harper, Andrew R.
dc.contributor.authorHubley, Lancia
dc.contributor.authorWang, Qinan
dc.contributor.authorHounsell, Rebekah
dc.contributor.authorCooke, Jeff
dc.contributor.authorCoulter, Dave A.
dc.contributor.authorFausnaugh, Michael M.
dc.date.accessioned2025-04-01T14:55:09Z
dc.date.available2025-04-01T14:55:09Z
dc.date.issued2025-02-24
dc.description.abstractWe present TESSELLATE, a dedicated pipeline for performing an untargeted search documenting all variable phenomena captured by the TESS space telescope. Building on the TESSreduce difference imaging pipeline, TESSELLATE extracts calibrated and reduced photometric data for every full frame image in the TESS archive. Using this data, we systematically identify transient, variable and non-sidereal signals across timescales ranging from minutes to weeks. The high cadence and wide field of view of TESS enables us to conduct a comprehensive search of the entire sky to a depth of ~17 mi. Based on the volumetric rates for known fast transients, we expect there to be numerous Fast Blue Optical Transients and Gamma Ray Burst afterglows present in the existing TESS dataset. Beyond transients, TESSELLATE can also identify new variable stars and exoplanet candidates, and recover known asteroids. We classify events using machine learning techniques and the work of citizen scientists via the Zooniverse Cosmic Cataclysms project. Finally, we introduce the TESSELLATE Sky Survey: a complete, open catalog of the variable sky observed by TESS.
dc.description.sponsorshipH.R. is supported by an Australian Government Research Training Program (RTP) Scholarship. R.R.H., A.M, C.M, and Z.G.L. are supported by the Royal Society of New Zealand, Te Ap?arangi through the Marsden Fund Fast Start Grant M1255. R.R.H is also supported by the Rutherford Foundation Postdoctoral Fellowship RFT-UOC2203-PD. M.T.B. appreciates support by the Rutherford Discovery Fellowships from New Zealand Government funding, administered by the Royal Society Te Ap?arangi. We thank the Zooniverse beta testers for Cosmic Cataclysms, in particular the users: Marcossilva, Wirg78, nathancbell, Kutchkutchela, InoSenpai, skraczek, As1310, Mayahn, jklingele, Gammapat, julienlg, remaap24, cesanjerry, captaincat, Barbalbero, andre.andrade, Enriquepa, jrukmini, cosmicTaryn, mprasad, Brbljusa, Tamerciftci; and project translators: InoSenpai, aglr, Michael Moons-654, Cledison Marcos da Silva. This work was performed on the OzSTAR national facility at Swinburne University of Technology. The OzSTAR program receives funding in part from the Astronomy National Collaborative Research Infrastructure Strategy (NCRIS) allocation provided by the Australian Government, and from the Victorian Higher Education State Investment Fund (VHESIF) provided by the Victorian Government.
dc.description.urihttp://arxiv.org/abs/2502.16905
dc.format.extent18 pages
dc.genrejournal articles
dc.genrepreprints
dc.identifierdoi:10.13016/m2loqi-czdu
dc.identifier.urihttps://doi.org/10.48550/arXiv.2502.16905
dc.identifier.urihttp://hdl.handle.net/11603/37864
dc.language.isoen
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.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectAstrophysics - High Energy Astrophysical Phenomena
dc.subjectAstrophysics - Solar and Stellar Astrophysics
dc.subjectAstrophysics - Earth and Planetary Astrophysics
dc.subjectAstrophysics - Instrumentation and Methods for Astrophysics
dc.titleTESSELLATE: Piecing Together the Variable Sky With TESS
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0002-0476-4206

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