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<ri:Resource created="2023-11-07T10:47:55Z" status="active" updated="2026-08-03T07:30:23Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>New periodic signals detected in TESS</title><shortName>J/MNRAS/499/4011</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/499/4011</identifier><altIdentifier>doi:10.26093/cds/vizier/bg-fk-3xb</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chakraborty J.</name></creator><creator><name>Wheeler A.</name></creator><creator><name>Kipping D.</name></creator><date role="Updated">2026-08-03T07:30:23Z</date><date role="Created">2023-11-07T10:47:55Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>eclipsing-binary-stars</subject><subject>multiple-stars</subject><subject>effective-temperature</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>We apply the weirddetector, a non-parametric signal detection algorithm based on phase dispersion minimization, in a search for low duty-cycle periodic signals in the Transiting Exoplanet Survey Satellite (TESS) photometry. Our approach, in contrast to commonly used model-based approaches specifically for flagging transits, eclipsing binaries, or other similarly periodic events, makes minimal assumptions about the shape of a periodic signal, with the goal of finding 'weird' signals of unexpected or arbitrary shape. In total, 248301 TESS sources from the first-year Southern sky survey are run through the weirddetector, of which we manually inspect the top 21500 for periodicity. To minimize false-positives, we here only report on the upper decile in terms of signal score, a sample for which we obtain 97% recall of TESS eclipsing binaries and 62% of the TOIs. In our sample, we find 377 previously unreported periodic signals, for which we make a first-pass assignment that 26 are ultra-short periods (&lt;0.3d), 313 are likely eclipsing binaries, 28 appear planet-like, and 10 are miscellaneous signals.</description><source format="bibcode">2020MNRAS.499.4011C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/499/4011</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 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