A Uniform Analysis of the Lya Forest at z = 0-5. III. Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
A Uniform Analysis of the Lya Forest at z = 0-5. IV. The Clustering and Evolution of Clouds at z <= 1.7
Emission Line Properties of Active Galactic Nuclei from a pre-COSTAR Faint Object Spectrograph Hubble Space Telescope Spectral Atlas
Evidence of a Strong N V/C IV Correlation between Emission and Absorption Lines in Active Galactic Nuclei
Hubble Space Telescope and Ground-based Observations of I Zw 1 and Mrk 486 and the Variability of Polarization in Radio-quiet Active Galactic Nuclei
Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
On the weak Lya emission line of BL Lacertae objects
SDSS J094533.99+100950.1 - the remarkable weak emission line quasar
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Ultraviolet interstellar linear polarization. IV. Cross-calibration between the Wisconsin ultraviolet photo-polarimeter experiment and the faint object spectrograph.
Instrument
FOS/BL
Temporal Coverage
1992-12-05T21:39:17Z/1993-04-07T05:42:17Z
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, Angel comma Roger, 1994, 'SPECTROPOLARIMETRY OF QSOS, BLAZARS AND AGN AUGMENTATION: CYCLE 2 OBSERVATIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-avxa5j2