Extensive Globular Cluster Systems Associated with Ultra Diffuse Galaxies in the Coma Cluster
Identifying the Variety of Jovian X-Ray Auroral Structures: Tying the Morphology of X-Ray Emissions to Associated Magnetospheric Dynamics
Implications for galaxy formation models from observations of globular clusters around ultra-diffuse galaxies
Multi-resolution Filtering: An Empirical Method for Isolating Faint, Extended Emission in Dragonfly Data and Other Low Resolution Images
Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. II. Constraints on Fuzzy Dark Matter
Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. I. Observations, Kinematics, and Cold Dark Matter Halo Fits
Still at odds with conventional galaxy evolution: the star formation history of ultradiffuse galaxy Dragonfly 44
The impact of satellite trails on Hubble Space Telescope observations
The number of globular clusters around the iconic UDG DF44 is as expected for dwarf galaxies
Ultraviolet and X-ray properties of Comas ultra-diffuse galaxies
Instrument
ACS/WFC, WFC3/UVIS
Temporal Coverage
2017-04-16T15:01:53Z/2017-04-23T13:04:21Z
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, van Dokkum et al., 2018, 'Imaging of three Ultra Diffuse Galaxies with measured stellar kinematics', 1.0, European Space Agency, https://doi.org/10.5270/esa-3yavpv7