Mass Estimations of Supermassive Black Holes in Brightest Cluster Galaxies
Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296
Recoiling Supermassive Black Holes: A Search in the Nearby Universe
The Black Hole Mass of Abell 1836-BCG and Abell 3565-BCG
The High-Mass End of the Black Hole Mass Function: Mass Estimates in Brightest Cluster Galaxies
Instrument
ACS, ACS/HRC, STIS, STIS/CCD
Temporal Coverage
2003-08-16T05:51:47Z/2004-08-07T09:31:09Z
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, Ferrarese et al., 2007, 'The Upper End of the Supermassive Black Hole Mass Function: Pushing the 10 Billion Solar Mass Limit.', 1.0, European Space Agency, https://doi.org/10.5270/esa-n92m00l