VIRAC2: NIR astrometry and time series photometry for 500M+ stars from the VVV and VVVX surveys

ABSTRACT We 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 $560~{\rm deg}^2$ of the Southern Galactic plane and bulge. The catalogue is complete at the $\gt 90$ per cent level for $11\lt K_s~{\rm mag}\lt 16$ sources, but extends to $K_s\approx {}17.5$ mag in most fields. Astrometric performance for $11\lt K_s~{\rm mag}\lt 14$ sources is typically $\approx {}0.37~{\rm mas~yr}^{-1}$ per dimension for proper motion, and $1~{\rm mas}$ for parallax. At $K_s=16$ the equivalent values are around $1.5~{\rm mas~yr}^{-1}$ and $5~{\rm mas}$. 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.

Publication Details

Journal
Apollo (University of Cambridge)
Published
2024-12-24
DOI
https://doi.org/10.17863/cam.114519
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

VIRAC2: NIR astrometry and time series photometry for 500M+ stars from the VVV and VVVX surveys

Apollo (University of Cambridge)
Stellar, planetary, and galactic studies
article

VIRAC2: NIR astrometry and time series photometry for 500M+ stars from the VVV and VVVX surveys

article en

Abstract

ABSTRACT We 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 $560~{\rm deg}^2$ of the Southern Galactic plane and bulge. The catalogue is complete at the $\gt 90$ per cent level for $11\lt K_s~{\rm mag}\lt 16$ sources, but extends to $K_s\approx {}17.5$ mag in most fields. Astrometric performance for $11\lt K_s~{\rm mag}\lt 14$ sources is typically $\approx {}0.37~{\rm mas~yr}^{-1}$ per dimension for proper motion, and $1~{\rm mas}$ for parallax. At $K_s=16$ the equivalent values are around $1.5~{\rm mas~yr}^{-1}$ and $5~{\rm mas}$. 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.

Apollo (University of Cambridge)
National Science Foundation, University of Hertfordshire, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Centro de Astrofísica y Tecnologías Afines, Agencia Nacional de Investigación y Desarrollo, Science and Technology Facilities Council
Openalex Percentile: Top 65%
Stellar, planetary, and galactic studies
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.