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dc.contributor.authorSmith, Leigh C.
dc.contributor.authorLucas, Philip W.
dc.contributor.authorKoposov, Sergey E.
dc.contributor.authorGonzález-Fernández, Carlos
dc.contributor.authorAlonso-García, Javier
dc.contributor.authorMinniti, Dante
dc.contributor.authorSanders, Jason L.
dc.contributor.authorBedin, Luigi R.
dc.contributor.authorBelokurov, Vasily
dc.contributor.authorEvans, N. Wyn
dc.contributor.authorHempel, Maren
dc.contributor.authorIvanov, Valentin D.
dc.contributor.authorKurtev, Radostin G.
dc.contributor.authorSaito, Roberto K.
dc.date.accessioned2025-01-20T13:00:02Z
dc.date.available2025-01-20T13:00:02Z
dc.date.issued2025-02-28
dc.identifier.citationSmith , L C , Lucas , P W , Koposov , S E , González-Fernández , C , Alonso-García , J , Minniti , D , Sanders , J L , Bedin , L R , Belokurov , V , Evans , N W , Hempel , M , Ivanov , V D , Kurtev , R G & Saito , R K 2025 , ' Virac2: NIR Astrometry and Time Series Photometry for 500M+ Stars from the VVV and VVVX Surveys ' , Monthly Notices of the Royal Astronomical Society , vol. 536 , no. 4 , stae2797 , pp. 3707–3738 . https://doi.org/10.1093/mnras/stae2797
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/2501.06295v1
dc.identifier.urihttp://hdl.handle.net/2299/28720
dc.description© 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an open access article distributed under the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
dc.description.abstractWe present VIRAC2, a catalogue of positions, proper motions, parallaxes and Z, Y, J, H, and K_s near-infrared photometric time series of 545 346 537 unique stars. The catalogue is based on a point spread function fitting reduction of nearly a decade of VISTA VVV and VVVX images, which cover 560 deg^2 of the Southern Galactic plane and bulge. The catalogue is complete at the >90 per cent level for <Ks mag<1 11<Ks<16 sources, but extends to Ks≈17.5 mag in most fields. Astrometric performance for 11<Ks mag<14 sources is typically ≈0.37 mas yr−1per dimension for proper motion, and 1 mas for parallax. At Ks=16 the equivalent values are around 1.5 mas yr−1and 5 mas. These uncertainties are validated against Gaia DR3 and Hubble Space Telescope astrometry. The complete catalogues are available via the ESO archive. We perform an initial search of the catalogue for nearby ultracool dwarf candidates. In total we find 26 new sources whose parallaxes place them within 50 parsecs of the Sun. Among them we find two high-confidence T dwarfs and a number of other sources that appear to lie close to the L/T transition.en
dc.format.extent32
dc.format.extent5914119
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.GA
dc.subjectastro-ph.SR
dc.titleVirac2: NIR Astrometry and Time Series Photometry for 500M+ Stars from the VVV and VVVX Surveysen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionCentre for Future Societies Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1093/mnras/stae2797
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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