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<ri:Resource created="2010-11-20T13:37:02Z" status="active" updated="2026-08-03T07:24:34Z" 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>3.6 years of DIRBE NIR stellar light curves</title><shortName>J/ApJS/190/203</shortName><identifier>ivo://CDS.VizieR/J/ApJS/190/203</identifier><altIdentifier>doi:10.26093/cds/vizier.21900203</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Price S.D.</name></creator><creator><name>Smith B.J.</name></creator><creator><name>Kuchar T.A.</name></creator><creator><name>Mizuno D.R.</name></creator><creator><name>Kraemer K.E.</name></creator><date role="Updated">2026-08-03T07:24:34Z</date><date role="Created">2010-11-20T13:37:02Z</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>infrared-photometry</subject><subject>variable-stars</subject><description>The weekly averaged near-infrared fluxes for 2652 stars were extracted from the cold and warm era all-sky maps of the Diffuse Infrared Background Experiment (DIRBE). Since the DIRBE program only archived the individual Calibrated Infrared Observations for the 10 month cold era mission, the weekly averaged fluxes were all that were available for the warm era. The steps required to extract stellar fluxes are described as are the adjustments that were necessary to correct the results for several systematic effects. The observations are at a cadence of once a week for 3.6 years (~1300 days), providing continuous sampling on variable stars that span the entire period for the longest fundamental pulsators. The stars are divided into three categories: those with large amplitude of variability, smaller amplitude variables, and sources whose near-infrared brightness do not vary according to our classification criteria. We show examples of the results and the value of the added baseline in determining the phase lag between the visible and infrared.</description><source format="bibcode">2010ApJS..190..203P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/190/203</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/J/ApJ/500/554">J/ApJ/500/554 : COBE DIRBE IR photometry (Odenwald+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/154/673">J/ApJS/154/673 : COBE DIRBE Point Source Catalog (Smith+, 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48212 48222 48229 48250 48269 48297 48301 48328 48330 48344 48464 48466 48480-48481 48515-48516 48572 48589 48596 48617 48650 48676 48715 48731 48753 48773 48821 48894 48903 48992 48999 49002 49041 49045 49081 49113 49123 49136</spatial><spectral>3.780835296817751e-20 1.7778042830267053e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/190/203?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/190/203/var</name><description>data for variables and candidate variables (table 1 and 2 of the paper)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name (G2) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>F1.25</name><description>? Average DIRBE 1.25 micron flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.J;stat.mean</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F1.25</name><description>? Number of 1.25 micron observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P1.25</name><description>? Period of the 1.25 micron light curve</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>A1.25</name><description>? Amplitude of the 1.25 micron light curve (2)</description><unit>Jy</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F2.2</name><description>? Average DIRBE 2.2 micron flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F2.2</name><description>? Number of 2.2 micron observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P2.2</name><description>? Period of the 2.2 micron light curve</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>A2.2</name><description>? Amplitude of the 2.2 micron light curve (2)</description><unit>Jy</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F3.5</name><description>? Average DIRBE 3.5 micron flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F3.5</name><description>? Number of 3.5 micron observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P3.5</name><description>? Period of the 3.5 micron light curve</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>A3.5</name><description>? Amplitude of the 3.5 micron light curve (2)</description><unit>Jy</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F4.9</name><description>? Average DIRBE 4.9 micron flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F4.9</name><description>? Number of 4.9 micron observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Var</name><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>DIRBE</name><description>DIRBE name (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>P4.9</name><description>? Period of the 4.9 micron light curve</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>A4.9</name><description>? Amplitude of the 4.9 micron light curve (2)</description><unit>Jy</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Com</name><description>[ABCF, ] Additional comment(s) (G3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>LC</name><description>Plot the light curve(s)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position, from DIRBE name (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position, from DIRBE name (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJS/190/203/table3</name><description>DIRBE non-variables</description><column><name>e_F3.5</name><description>? The 1{sigma} uncertainty in F3.5</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F3.5</name><description>? Number of 3.5 micron observations (1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F4.9</name><description>? Average DIRBE DIRBE 4.9 micron flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F4.9</name><description>? The 1{sigma} uncertainty in F4.9</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F4.9</name><description>? Number of 4.9 micron observations (1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Com</name><description>[ABCF, ] Additional comment(s) (G3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>LC</name><description>Plot the light curve(s)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>DIRBE</name><description>DIRBE name (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Other name (G2)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>F1.25</name><description>? Average DIRBE 1.25 micron flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.J;stat.mean</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F1.25</name><description>? The 1{sigma} uncertainty in F1.25</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F1.25</name><description>? Number of 1.25 micron observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F2.2</name><description>? Average DIRBE 2.2 micron flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F2.2</name><description>? The 1{sigma} uncertainty in F2.2</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_F2.2</name><description>? Number of 2.2 micron observations (1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F3.5</name><description>? Average DIRBE 3.5 micron flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>