Black Hole Mass Measurements of Early-type Galaxies NGC 1380 and NGC 6861 through ALMA and HST Observations and Gas-dynamical Modeling
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
Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
Near-infrared surface brightness fluctuation measurements with the Hubble Space Telescopes WFC3/IR channel
Optical and Infrared Photometry of Globular Clusters in NGC 1399: Evidence for Color-Metallicity Nonlinearity
Recoiling Supermassive Black Holes: A Search in the Nearby Universe
The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
Instrument
WFC3, WFC3/IR
Temporal Coverage
2009-12-10T00:11:23Z/2010-07-20T12:15:41Z
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., 2011, 'Calibration of Surface Brightness Fluctuations for WFC3/IR', 1.0, European Space Agency, https://doi.org/10.5270/esa-gm67egk