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<ri:Resource created="2017-08-04T16:35:47Z" status="active" updated="2025-06-13T15:25:00Z" 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>SDSS-III/APOGEE. II. The multi-epoch ABE sample</title><shortName>J/AJ/153/174</shortName><identifier>ivo://CDS.VizieR/J/AJ/153/174</identifier><altIdentifier>doi:10.26093/cds/vizier.51530174</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chojnowski S.D.</name></creator><creator><name>Wisniewski J.P.</name></creator><creator><name>Whelan D.G.</name></creator><creator><name>Labadie-Bartz J.,Borges Fernandes M.</name></creator><creator><name>Lin C.-C.</name></creator><creator><name>Majewski S.R.</name></creator><creator><name>Stringfellow G.S.,Mennickent R.E.</name></creator><creator><name>Roman-Lopes A.</name></creator><creator><name>Tang B.</name></creator><creator><name>Hearty F.R.</name></creator><creator><name>Holtzman J.A.,Pepper J.</name></creator><creator><name>Zasowski G.</name></creator><date role="Updated">2018-12-19T06:10:25Z</date><date role="Created">2017-08-04T16:35:47Z</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>emission-line-stars</subject><subject>line-intensities</subject><subject>radial-velocity</subject><description>We report on the H-band spectral variability of classical Be stars observed over the course of the Apache Point Galactic Evolution Experiment (APOGEE), one of four subsurveys comprising SDSS-III. As described in the first paper of this series, the APOGEE B-type emission-line (ABE) star sample was culled from the large number of blue stars observed as telluric standards during APOGEE observations. In this paper, we explore the multi-epoch ABE sample, consisting of 1100 spectra for 213 stars. These "snapshots" of the circumstellar disk activity have revealed a wealth of temporal variability including, but not limited to, gradual disappearance of the line emission and vice versa over both short and long timescales. Other forms of variability include variation in emission strength, emission peak intensity ratios, and emission peak separations. We also analyze radial velocities (RVs) of the emission lines for a subsample of 162 stars with sufficiently strong features, and we discuss on a case-by-case basis whether the RV variability exhibited by some stars is caused by binary motion versus dynamical processes in the circumstellar disks. Ten systems are identified as convincing candidates for binary Be stars with as of yet undetected companions.</description><source format="bibcode">2017AJ....153..174C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/153/174</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/V/137">V/137 : Extended Hipparcos Compilation (XHIP) (Anderson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/7">J/AJ/149/7 : SDSS-III/APOGEE. I. Be stars (Chojnowski+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/786/120">J/ApJ/786/120 : Spectropolarimetry of classical Be stars (Draper+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/1306">J/ApJ/709/1306 : Spectropolarimetry of 60 Cyg and {pi} Aqr (Wisniewski+, 2010)</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/MNRAS/371/252">J/MNRAS/371/252 : Southern B and Be stars (Levenhagen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/415/145">J/A+A/415/145 : Radial velocities of 16 stars in NGC 6913 (Boeche+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/912">J/A+A/368/912 : Polarization and rotational vel. of Be stars (Yudin, 2001)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/153/174</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/153/174</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/153/174</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/153/174</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/153/174</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ABE</name><description>Identifier of the Apache Point Observatory Galactic Evolution Experiment (APOGEE) B-type emission-line (ABE) star (running number) (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>PapI</name><description>Display the data from Paper I (Chojnowski et al. 2015, Cat. J/AJ/149/7)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>New</name><description>Indicates an additional new Be star from APOGEE1 (table1)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Nobs</name><description>[2/30] Number of APOGEE observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MJD0</name><description>[55702/56812] Modified Julian Date (MJD) of first APOGEE observation (JD-2400000.5)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>dJD</name><description>[1/1862] Observational baseline ({Delta}JD)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>&lt;S/N&gt;</name><description>[46/800] Mean Signal-to-Noise ratio</description><ucd>stat.snr;stat.mean</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VType</name><description>Variability classification (1)</description><ucd>meta.code.class;src.var</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>&lt;PSep&gt;</name><description>[0/629]? Mean Br11 peak separation (G2)</description><unit>km/s</unit><ucd>phys.veloc;arith.diff;stat.mean</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PAmp</name><description>[0/128]? Scatter (maximum minus minimum) in Br11 peak separation</description><unit>km/s</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>&lt;EW&gt;</name><description>[-17/6] Mean Br11 equivalent width W_Br11_ (in {AA}) (G3)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_&lt;EW&gt;</name><description>[0/2.93] Standard deviation ({sigma}) in &lt;EW&gt; (in {AA})</description><unit>0.1nm</unit><ucd>stat.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EWAmp</name><description>[0.01/8.37] Scatter (maximum minus minimum) in Br11 equivalent width (in {AA})</description><unit>0.1nm</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>&lt;RV&gt;</name><description>[-93/76.6]? 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