A Complete Atlas of Recalibrated Hubble Space Telescope Faint Object Spectrograph Spectra of Active Galactic Nuclei and Quasars. I. Pre-COSTAR Spectra
Comparative Analysis of the High- and Low-Ionization Lines in the Broad-Line Region of Active Galactic Nuclei
Hubble Space Telescope STIS Spectroscopy of the Lya Emission Line in the Central Dominant Galaxies in A426, A1795, and A2597: Constraints on Clouds in the Intracluster Medium
Ly alpha Constraints on the Nature of the X-Ray--absorbing Medium in Cooling Flow Clusters
Observations of Far-UV Emission From NGC 1275 With the Hopkins Ultraviolet Telescope
Observations of O I and Ca II Emission Lines in Quasars: Implications for the Site of Fe II Line Emission
Revealing the Broad Line Region of NGC 1275: The Relationship to Jet Power
The HST ultraviolet spectrum of the nucleus of NGC 1275: Fermi-accelerated Lyalpha emission
The Redshifted Excess in Quasar C IV Broad Emission Lines
Instrument
FOS/BL
Temporal Coverage
1993-02-03T05:49:32Z/1993-02-03T12:43:26Z
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, Johnstone comma Roderick M., 1995, 'DETECTION OF ABSORPTION LINES FROM GAS IN THE COOLING FLOW IN THE PERSEUS CLUSTER', 1.0, European Space Agency, https://doi.org/10.5270/esa-uof3oxl