ALMA Observations of a Candidate Molecular Outflow in an Obscured Quasar
A Second Look at 12 Candidate Dual AGNs Using BAYMAX
Dual AGN Candidates with Double-peaked O III Lines Matching that of Confirmed Dual AGNs
Extended X-Ray Emission from a Quasar-driven Superbubble
Merger-driven Fueling of Active Galactic Nuclei: Six Dual and Offset AGNs Discovered with Chandra and Hubble Space Telescope Observations
Observational Constraints on Correlated Star Formation and Active Galactic Nuclei in Late-stage Galaxy Mergers
Spatially Resolved UV Diagnostics of AGN Feedback: Radiation Pressure Dominates in a Prototypical Quasar-driven Superwind
The diverse cold molecular gas contents, morphologies, and kinematics of type-2 quasars as seen by ALMA
The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei. IV. Association with Galaxy Mergers
The Quasar Feedback Survey: revealing the interplay of jets, winds, and emission-line gas in type 2 quasars with radio polarization
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-11-01T09:01:48Z/2012-11-21T02:43:13Z
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, Comerford et al., 2013, 'Identifying Analogs of NGC 6240: Galaxies with Dual Supermassive Black Holes', 1.0, European Space Agency, https://doi.org/10.5270/esa-mdsmdbi
