GALACTICNUCLEUS: A high angular resolution JHKs imaging survey of the Galactic centre. I. Methodology, performance, and near-infrared extinction towards the Galactic centre
Near-infrared variability study of the central 2.3 x 2.3 arcmin2 of the Galactic Centre - II. Identification of RR Lyrae stars in the Milky Way nuclear star cluster
Near-infrared variability study of the central 2.3 arcmin x 2.3 arcmin of the Galactic Centre - I. Catalogue of variable sources
Stellar Populations in the Central 0.5 pc of Our Galaxy. III. The Dynamical Substructures
The Nuclear Star Cluster and Nuclear Stellar Disk of the Milky Way: Different Stellar Populations and Star Formation Histories
Instrument
WFC3, WFC3/IR
Temporal Coverage
2014-02-06T21:08:46Z/2014-02-07T04:15:58Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Do comma Tuan, 2015, 'Measuring the physical properties of the Milky Way nuclear star cluster with proper motions', 1.0, European Space Agency, https://doi.org/10.5270/esa-5d0nxe8