Accretion and obscuration in merger-dominated luminous red quasars
Discovery and analysis of dust-reddened type 1 quasars - Finding the missing link in quasar evolution
Evidence for Quasar Activity Triggered by Galaxy Mergers in HST Observations of Dust-reddened Quasars
Heavily obscured quasar host galaxies at z ~ 2 are discs, not major mergers
Host Galaxies of Young Dust-Reddened Quasars
Peering Through the Dust. II. XMM-Newton Observations of Two Additional FIRST-2MASS Red Quasars
Reddening and He I * l10830 Absorption Lines in Three Narrow-line Seyfert 1 Galaxies
Spitzer Observations of Young Red Quasars
The Black Hole Mass-Bulge Luminosity Relationship for Active Galactic Nuclei From Reverberation Mapping and Hubble Space Telescope Imaging
The host galaxies of FeLoBAL quasars at z ~ 0.9 are not dominated by recent major mergers
The radio spectra of reddened Two Micron All Sky Survey quasi-stellar objects: evidence for young radio jets
Instrument
ACS, ACS/WFC
Temporal Coverage
2005-04-18T01:13:48Z/2005-10-22T03:58:14Z
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, Lacy comma Mark D., 2006, 'The host galaxies of dust-reddened quasars', 1.0, European Space Agency, https://doi.org/10.5270/esa-wwp0867