Comparison of the active galactic nuclei Baldwin effect with the modified Baldwin effect of the ultraviolet-optical emission lines in a single sample
Detection of low-metallicity warm plasma in a galaxy overdensity environment at z ~ 0.2
Evidence of a type 1/type 2 dichotomy in the correlation between quasar optical polarization and host-galaxy/extended emission position angles
NICMOS Observations of Low-Redshift Quasar Host Galaxies
Quasars and Ultraluminous Infrared Galaxies: At the Limit?
Rehabilitating C IV-based black hole mass estimates in quasars
The behaviour of quasar C IV emission-line properties with orientation
The Next Generation Atlas of Quasar Spectral Energy Distributions from Radio to X-Rays
The orientation dependence of quasar single-epoch black hole mass scaling relationships
The orientation dependence of quasar spectral energy distributions
Instrument
NICMOS, NICMOS/NIC1, NICMOS/NIC2, NICMOS/NIC3
Temporal Coverage
1997-09-24T01:27:23Z/1998-04-04T11:50:02Z
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, McLeod comma Kim, 1999, 'The Relation Between Quasar Luminosity and Host Galaxy Mass', 1.0, European Space Agency, https://doi.org/10.5270/esa-vb5cypj
