A Second Galaxy Missing Dark Matter in the NGC 1052 Group
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group
The Dragonfly Nearby Galaxies Survey. II. Ultra-Diffuse Galaxies near the Elliptical Galaxy NGC 5485
The Dragonfly Nearby Galaxies Survey. V. HST/ACS Observations of 23 Low Surface Brightness Objects in the Fields of NGC 1052, NGC 1084, M96, and NGC 4258
The impact of satellite trails on Hubble Space Telescope observations
The M 101 galaxy group as a node in a nearby cosmic filament
Using Surface Brightness Fluctuations to Study Nearby Satellite Galaxy Systems: Calibration and Methodology
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2015-04-02T01:45:26Z/2015-09-07T18:40:27Z
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, van Dokkum et al., 2016, 'Distances and stellar populations of seven low surface brightness galaxies in the field of M101', 1.0, European Space Agency, https://doi.org/10.5270/esa-ewnfg0o