Black Hole Mass Estimates Based on C IV are Consistent with Those Based on the Balmer Lines
Measuring Microlensing Using Spectra of Multiply Lensed Quasars
New database for a sample of optically bright lensed quasars in the northern hemisphere
Properties of Active Galactic Nuclei and Galaxies: Spectral Energy Distributions, Luminosity Functions and Black Hole Masses
Revealing the structure of the lensed quasar Q 0957+561. III. Constraints on the size of the broad-line region
The dark halo of the main lens galaxy in QSO 0957 + 561
The influence of gravitational lensing on the spectra of lensed quasi-stellar objects
Ultraviolet Structure in the Lensed QSO 0957+561
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
1999-04-15T05:59:37Z/2000-06-03T00:55:21Z
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, Cohen comma Ross D., 2001, 'A Unique Measurement of the Dust-to-Gas Ratio in an Absorption Line System', 1.0, European Space Agency, https://doi.org/10.5270/esa-gg8frcc