Black Hole Mass Measurements of Early-type Galaxies NGC 1380 and NGC 6861 through ALMA and HST Observations and Gas-dynamical Modeling
Circumnuclear Dust in Luminous Early-type Galaxies. I. Sample Properties and Stellar Luminosity Models
Gas-dynamical Mass Measurements of the Supermassive Black Holes in the Early-type Galaxies NGC 4786 and NGC 5193 from ALMA and HST Observations
Instrument
WFC3/IR, WFC3/UVIS
Temporal Coverage
2018-04-03T19:33:06Z/2019-04-27T23:15:48Z
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, Boizelle comma Benjamin, 2019, 'Stellar Luminosity Profiles for Precision Measurements of Black Hole Mass in Early-Type Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-pjipjdw