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<ri:Resource created="2022-09-28T08:36:49Z" status="active" updated="2025-05-19T09:50:00Z" 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>Classifying Be Star Variability with TESS I.</title><shortName>J/AJ/163/226</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/226</identifier><altIdentifier>doi:10.26093/cds/vizier.51630226</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Labadie-Bartz J.</name></creator><creator><name>Carciofi A.C.</name></creator><creator><name>Henrique de Amorim T.</name></creator><creator><name>Rubio A.,Luiz Figueiredo A.</name></creator><creator><name>Ticiani dos Santos P.</name></creator><creator><name>Thomson-Paressant K.</name></creator><date role="Updated">2022-10-12T12:15:46Z</date><date role="Created">2022-09-28T08:36:49Z</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>be-stars</subject><subject>variable-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>TESS photometry is analyzed for 430 classical Be stars observed in the first year of the mission. The often complex and diverse variability of each object in this sample is classified to obtain an understanding of the behavior of this class as a population. Ninety-seven percent of the systems are variable above the noise level, with timescales spanning nearly the entire range of what is accessible with TESS, from tens of minutes to tens of days. The variability seen with TESS is summarized as follows. Nearly every system contains multiple periodic signals in the frequency regime between about 0.5 and 4/day. One or more groups of closely spaced frequencies is the most common feature, present in 87% of the sample. Among the Be stars with brightening events that are characteristic of mass ejection episodes (18% of the full sample, or 31% of early-type stars), all have at least one frequency group, and the majority of these (83%) show a concurrent temporary amplitude enhancement in one or more frequency groups. About one-third (34%) of the sample is dominated by longer-term trends (timescales &gt;2day). Low-frequency stochastic signals are prominent in about 25% of the sample, with varying degrees of intensity. Higher-frequency signals (6&lt;f&lt;15/day) are sometimes seen (in 15% of the sample) and in most cases likely reflect p-mode pulsation. In rare cases (~3%), even higher frequencies beyond the traditional p-mode regime (f&gt;15/day) are observed.</description><source format="bibcode">2022AJ....163..226L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/226</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/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/17">III/17 : Early-Type Emission-Line Stars (Wackerling 1970)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/67">III/67 : Catalogue of Be stars (Jaschek+, 1982)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/135">III/135 : Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/10">IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/276">I/276 : Tycho Double Star Catalogue (TDSC) (Fabricius+ 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/260">III/260 : General Catalogue of Ap and Am stars (Renson+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/107/1556">J/AJ/107/1556 : Late B-type stars classification (Garrison+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/104/315">J/A+AS/104/315 : Member of Herbig Ae/Be stellar group (The+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/135">J/ApJS/99/135 : Rotation and Spectral Peculiarities (Abt+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/304/235">J/A+A/304/235 : UBV Photometry of phi Per (Bozic+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/378/861">J/A+A/378/861 : Spectroscopy of Be stars (Chauville+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/912">J/A+A/368/912 : Polarization &amp; rotational veloc. of Be stars (Yudin, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/2039">J/AJ/124/2039 : LMC Blue variable stars from MACHO (Keller+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/409/275">J/A+A/409/275 : Rotation and magnetic field in omega Ori (Neiner+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/54/207">J/AcA/54/207 : Ephemerids of eclipsing binaries (Kreiner, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2659">J/AJ/127/2659 : CHANDRA observations of NGC 2264 (Ramirez+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/440/305">J/A+A/440/305 : Fundamental param. of fast-rotating B stars (Fremat+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/158/193">J/ApJS/158/193 : Catalog of Galactic {beta} Cephei stars (Stankov+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/NewA/10.325">J/other/NewA/10.325 : 2MASS observations of Be stars (Zhang+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/451/1053">J/A+A/451/1053 : Fundamental parameters of Be stars (Fremat+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/647/1375">J/ApJ/647/1375 : BV light curves of {gamma} Cas (Smith+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/652/458">J/ApJ/652/458 : BVRH{alpha} photom. candidates Be stars (Wisniewski+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/1280">J/ApJ/686/1280 : Discovery hot subdwarf companion to FY CMa (Peters+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/477/917">J/A+A/477/917 : Beta Cephei stars in the ASAS-3 data. 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