Ninety-seven Eclipsing Quadruple Star Candidates Discovered in TESS Full-frame Images

dc.contributor.authorKostov, Veselin B.
dc.contributor.authorPowell, Brian P.
dc.contributor.authorRappaport, Saul A.
dc.contributor.authorBorkovits, Tamás
dc.contributor.authorBarclay, Thomas
dc.contributor.authoret al
dc.date.accessioned2022-05-31T23:17:47Z
dc.date.available2022-05-31T23:17:47Z
dc.date.issued2022-04-13
dc.descriptionAuthors: Veselin B. Kostov,Brian P. Powell, Saul A. Rappaport, Tamás Borkovits, Robert Gagliano, Thomas L. Jacobs, Martti H. Kristiansen, Daryll M. LaCourse, Mark Omohundro, Jerome Orosz, Allan R. Schmitt, Hans M. Schwengeler, Ivan A. Terentev, Guillermo Torres, Thomas Barclay,, Adam H. Friedman, Ethan Kruse, Greg Olmschenk,, Andrew Vanderburg, and William Welshen_US
dc.description.abstractWe present a catalog of 97 uniformly vetted candidates for quadruple star systems. The candidates were identified in TESS full-frame image data from sectors 1–42 through a combination of machine-learning techniques and visual examination, with major contributions from a dedicated group of citizen scientists. All targets exhibit two sets of eclipses with two different periods, both of which pass photocenter tests confirming that the eclipses are on target. This catalog outlines the statistical properties of the sample, nearly doubles the number of known multiply eclipsing quadruple systems, and provides the basis for detailed future studies of individual systems. Several important discoveries have already resulted from this effort, including the first sextuply eclipsing sextuple stellar system and the first transiting circumbinary planet detected from one sector of TESS data.en_US
dc.description.sponsorshipWe thank the referee for the insightful comments which helped improve this article. This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Funding for the TESS mission is provided by NASA's Science Mission directorate. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Center for Climate Simulation (NCCS) at Goddard Space Flight Center. Personnel directly supporting this effort were Mark L. Carroll, Laura E. Carriere, Ellen M. Salmon, Nicko D. Acks, Matthew J. Stroud, Bruce E. Pfaff, Lyn E. Gerner, Timothy M. Burch, and Savannah L. Strong. This research has made use of the Exoplanet Follow-up Observation Program website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. This research is based on observations made with the Galaxy Evolution Explorer, obtained from the MAST data archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. T.B. acknowledges the financial support of the Hungarian National Research, Development and Innovation Office—NKFIH grant KH-130372. V.B.K. is thankful for support from NASA grants 80NSSC21K0631 and 80NSSC21K0351. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products.en_US
dc.description.urihttps://iopscience.iop.org/article/10.3847/1538-4365/ac5458en_US
dc.format.extent27 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2l8f3-mern
dc.identifier.citationKostov, Veselin B. et al. Ninety-seven Eclipsing Quadruple Star Candidates Discovered in TESS Full-frame Images. The Astrophysical Journal Supplement Series 259, (Apr. 13, 2022, no. 2.). https://doi.org/10.3847/1538-4365/ac5458en_US
dc.identifier.urihttps://doi.org/10.3847/1538-4365/ac5458
dc.identifier.urihttp://hdl.handle.net/11603/24773
dc.language.isoen_USen_US
dc.publisherIOP Scienceen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
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.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleNinety-seven Eclipsing Quadruple Star Candidates Discovered in TESS Full-frame Imagesen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0001-7139-2724en_US

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