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
Hubble Space Telescope Wide Field Camera 3 Identifies an r p = 1 Kpc Dual Active Galactic Nucleus in the Minor Galaxy Merger SDSS J0924+0510 at z = 0.1495
Merger-driven Fueling of Active Galactic Nuclei: Six Dual and Offset AGNs Discovered with Chandra and Hubble Space Telescope Observations
Multiwavelength observations of the triple-peaked AGN Mrk 622
Strange quasar candidates with abnormal astrometric characteristics from Gaia EDR3 and SDSS (SQUAB-II): optical identifications
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 Origin of Double-peaked Narrow Lines in Active Galactic Nuclei. I. Very Large Array Detections of Dual AGNs and AGN Outflows
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-10-29T12:28:30Z/2012-08-25T08:05:29Z
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, Liu comma Xin, 2012, 'The Frequency and Demographics of Dual Active Galactic Nuclei', 1.0, European Space Agency, https://doi.org/10.5270/esa-u7w3hyx
