J/A+A/689/A138ivo://CDS.VizieR/J/A+A/689/A138doi:10.26093/cds/vizier.36890138CDSNarloch W.Hajdu G.Pietrzynski G.Gieren W.Zgirski B.,Wielgorski P.Karczmarek P.Gorski M.Graczyk D.2024-11-29T20:05:24Z2024-09-09T09:04:07ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmilky-way-galaxyvariable-starsinfrared-photometryvisible-astronomybroad-band-photometryRR Lyrae stars are excellent tracers of the old population II due to their period-luminosity (PL) and period-luminosity-metallicity (PLZ) relations. While these relations have been investigated in detail in many photometric bands, there are few comprehensive studies about them in Sloan-like systems. We present PL and PLZ relations (as well as their counterparts in Wesenheit magnitudes) in the Sloan-Pan-STARSS gP1rP1iP1 bands obtained for Galactic RR Lyrae stars in the vincinity of the Sun. The data used in this paper were collected with the network of 40cm telescopes of the Las Cumbres Observatory, and geometric parallaxes were adopted from Gaia Data Release 3. We derived PL and PLZ relations separately for RRab and RRc-type stars, as well as for the mixed population of RRab+RRc stars. To our knowledge, these are the first PL and PLZ relations in the Sloan bands determined using RR Lyrae stars in the Galactic field.2024A&A...689A.138Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/689/A138CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/471/1446 : Ground-based proper motion of 12 nearby GC (Narloch+, 2017)J/A+A/647/A135 : 35 star clusters and fields in the SMC (Narloch+, 2021)J/A+A/666/A80 : Star clusters and fields in the LMC (Narloch+, 2022)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/689/A138https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/689/A138http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/689/A138https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/689/A138https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/689/A138http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/689/A138GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/689/A138/table1 (MW RR Lyr star and their main parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/689/A138/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/689/A138/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/689/A138/table1?GETtext/xml+votable180.050000true309.5628181-2.89028220.0055555555555555560/https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/689/A138?format=asciiOpticalInfrareddefaultJ/A+A/689/A138/table1MW RR Lyr star and their main parametersFileNamerName of the light curve file in rP1 band in subdirectory lcmeta.id;instr.bandpass;meta.filecharFileNameiName of the light curve file in iP1 band in subdirectory lcmeta.id;instr.bandpass;meta.filechar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLCShow the light curvesmeta.ref.urlcharType[RRab RRc] Type of RR Lyraemeta.codecharNameStar namemeta.id;meta.maincharn_Name[a*] Note on Name (1)meta.notecharPerPeriod adopted from AAVSO databasedtime.perioddoubleplxGaia DR3 parallax corrected with RUWEmaspos.parallax.trigfloate_plxGaia DR3 parallax errormasstat.error;pos.parallaxfloatRUWEGaia DR3 renormalized unit weight error RUWEstat.errorfloatGOFgoodness-of-fit from the Gaia DR3 catalogstat.fit.paramfloatSimbadSimbad column added by the CDSmeta.ref.urlcharE(B-V)Reddening value (2)magphot.color.excessfloate_E(B-V)Reddening value errormagstat.errorfloatgmeanIntensity-averaged mean Pan-STARRS gP1 magnitude from Fourier series fittingmagphot.mag;em.opt.Bfloate_gmeanIntensity-averaged mean Pan-STARRS gP1 magnitude errormagstat.errorfloatrmeanIntensity-averaged mean Pan-STARRS rP1 magnitude from Fourier series fittingmagphot.mag;em.opt.Rfloate_rmeanIntensity-averaged mean Pan-STARRS rP1 magnitude errormagstat.errorfloatimeanIntensity-averaged mean Pan-STARRS iP1 magnitude from Fourier series fittingmagphot.mag;em.opt.Ifloate_imeanIntensity-averaged mean Pan-STARRS iP1 magnitude errormagstat.errorfloat[Fe/H]? Adopted iron abundancephys.abund.Fefloatnullablee_[Fe/H]? Adopted iron abundance errorstat.error;phys.abund.Fefloatnullabler_[Fe/H][1/2]? Source of iron abundance (3)meta.refintnullableFileNamegName of the light curve file in gP1 band in subdirectory lcmeta.id;instr.bandpass;meta.filechar