ALMA Observations of Multiple CO and C Lines toward the Active Galactic Nucleus of NGC 7469: An X-Ray-dominated Region Caught in the Act
ALMA resolves giant molecular clouds in a tidal dwarf galaxy
Black Hole-Galaxy Scaling Relationships for Active Galactic Nuclei with Reverberation Masses
Black hole mass measurement using ALMA observations of CI and CO emissions in the Seyfert 1 galaxy NGC 7469
H I Spectroscopy of Reverberation-mapped Active Galactic Nuclei
Significant Suppression of Star Formation in Radio-quiet AGN Host Galaxies with Kiloparsec-scale Radio Structures
Spectroscopic Indication of a Centi-parsec Supermassive Black Hole Binary in the Galactic Center of NGC 5548
The Black Hole Mass of NGC 4151 from Stellar Dynamical Modeling
The BRAVE Program. I. Improved Bulge Stellar Velocity Dispersion Estimates for a Sample of Active Galaxies
The impact of satellite trails on Hubble Space Telescope observations
Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-mapped AGNs
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2009-11-10T08:04:56Z/2010-07-17T16:15:05Z
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, Bentz et al., 2011, 'The Black Hole Mass - Bulge Luminosity Relationship for the Nearest Reverberation-Mapped AGNs', 1.0, European Space Agency, https://doi.org/10.5270/esa-9970v1m