Dwarf Spheroidal Galaxies in the M101 Group and Behind it
Luminosity Functions and Host-to-host Scatter of Dwarf Satellite Systems in the Local Volume
The impact of satellite trails on Hubble Space Telescope observations
The M 101 galaxy group as a node in a nearby cosmic filament
The M101 Satellite Luminosity Function and the Halo-Halo Scatter among Local Volume Hosts
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2017-05-11T19:24:17Z/2017-10-07T05:34:22Z
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, Crnojevic comma Denija, 2018, 'An extremely asymmetric dwarf satellite distribution around M101', 1.0, European Space Agency, https://doi.org/10.5270/esa-95a6dgr