Astrometry in crowded fields towards the Galactic bulge
Chemically Dissected Rotation Curves of the Galactic Bulge from Main-sequence Proper Motions
First Detection of the White Dwarf Cooling Sequence of the Galactic Bulge
Microlensing Constraints on the Mass of Single Stars from HST Astrometric Measurements
New Insights on the Galactic Bulge Initial Mass Function
New variable stars towards the Galactic Bulge - I. The bright regime
Predicted trends in Milky Way bulge proper motion rotation curves: future prospects for HST and LSST
The impact of satellite trails on Hubble Space Telescope observations
The White Dwarf Cooling Sequence of the Galactic Bulge
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2011-10-20T20:41:18Z/2012-10-24T15:02:40Z
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, Sahu et al., 2013, 'Detecting and Measuring the Masses of Isolated Black Holes and Neutron Stars through Astrometric Microlensing', 1.0, European Space Agency, https://doi.org/10.5270/esa-vp2rcjh