A Dual Black Hole Associated with Obscured and Unobscured AGNs: CXO J101527.2+625911
A Potential Recoiling Supermassive Black Hole, CXO J101527.2+625911
A weak lensing comparability study of galaxy mergers that host AGNs.
Comparing and Calibrating Black Hole Mass Estimators for Distant Active Galactic Nuclei
Cosmic Evolution of Black Holes and Spheroids. III. The MBH-s* Relation in the Last Six Billion Years
Cosmic Evolution of Black Holes and Spheroids. II. Scaling Relations at z=0.36
Cosmic Evolution of Black Holes and Spheroids. I. The MBH-s Relation at z = 0.36
Cosmic Evolution of Black Holes and Spheroids. V. The Relation between Black Hole Mass and Host Galaxy Luminosity for a Sample of 79 Active Galaxies
Merger-driven Growth of Intermediate-mass Black Holes: Constraints from Hubble Space Telescope Imaging of Hyper-luminous X-Ray Sources
Post-starburst quasars: bridging the gap between post-starburst galaxies and quasars
Stronger Constraints on the Evolution of the M BH-{\sigma }_{* } Relation up to z ~ 0.6
The Connection between 3.3 mm Polycyclic Aromatic Hydrocarbon Emission and Active Galactic Nucleus Activity
The impact of satellite trails on Hubble Space Telescope observations
Variability of Moderate-Luminosity Active Galactic Nuclei at z = 0.36
Instrument
ACS, ACS/WFC
Temporal Coverage
2004-08-11T01:02:32Z/2004-12-10T00:37:40Z
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, Treu comma Tommaso L., 2005, 'Co-evolution of spheroids and black holes', 1.0, European Space Agency, https://doi.org/10.5270/esa-xq82nux