Deep Hubble Space Telescope Photometry of Large Magellanic Cloud and Milky Way Ultrafaint Dwarfs: A Careful Look into the Magnitude-Size Relation
Inhomogeneous Galactic chemical evolution: modelling ultra-faint dwarf galaxies of the Large Magellanic Cloud
Metallicity Distribution Functions of 13 Ultra-faint Dwarf Galaxy Candidates from Hubble Space Telescope Narrowband Imaging
Reconciling Observed and Simulated Stellar Halo Masses
Structural Parameters and Possible Association of the Ultra-faint Dwarfs Pegasus III and Pisces II from Deep Hubble Space Telescope Photometry
The impact of satellite trails on Hubble Space Telescope observations
The origin of ultra diffuse galaxies: stellar feedback and quenching
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2016-09-26T12:26:01Z/2018-04-09T19:11:27Z
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, Kallivayalil comma Nitya, 2018, 'Milky Way Cosmology: Laying the Foundation for Full 6-D Dynamical Mapping of the Nearby Universe', 1.0, European Space Agency, https://doi.org/10.5270/esa-p7ty0ge