Comparing Globular Cluster System Properties with Host Galaxy Environment
Connecting Infrared Surface Brightness Fluctuation Distances to Type Ia Supernova Hosts: Testing the Top Rung of the Distance Ladder
Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
Probing within the Bondi radius of the ultramassive black hole in NGC 1600
The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
The impact of satellite trails on Hubble Space Telescope observations
The MASSIVE Survey XIV--Stellar Velocity Profiles and Kinematic Misalignments from 200 pc to 20 kpc in Massive Early-type Galaxies
Instrument
ACS/WFC, WFC3/IR, WFC3/UVIS
Temporal Coverage
2017-12-21T09:47:30Z/2020-03-04T02:39:37Z
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, Blakeslee et al., 2020, 'MASSIVE+: The Growth Histories of MASSIVE Survey Galaxies from their Globular Cluster Colors', 1.0, European Space Agency, https://doi.org/10.5270/esa-m6yf9bo