Characterizing Transition Temperature Gas in the Galactic Corona
C II Radiative Cooling of the Diffuse Gas in the Milky Way
High-Velocity Line Emission in the Narrow-Line Region of NGC 4151
M31 Globular Clusters in the Hubble Space Telescope Archive. I. Cluster Detection and Completeness
M31 Globular Clusters in the Hubble Space Telescope Archive. II. Structural Parameters
Mass Outflow from the Nucleus of the Seyfert 1 Galaxy NGC 4151
Measurement of black hole masses in active galactic nuclei
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
Probing the Ionization Structure of the Narrow-Line Region in the Seyfert 1 Galaxy NGC 4151
Simultaneous Ultraviolet and X-Ray Observations of the Seyfert Galaxy NGC 4151. II. Physical Conditions in the UV Absorbers
Space Telescope Imaging Spectrograph Echelle Observations of NGC 4151: Variable Ionization of the Intrinsic UV Absorbers
Space Telescope Imaging Spectrograph Echelle Observations of the Seyfert Galaxy NGC 4151: Physical Conditions in the Ultraviolet Absorbers
The Milky Way halo as a QSO absorption-line system. New results from an HST/STIS absorption-line catalogue of Galactic high-velocity clouds
The non-constant slope of the C IV Baldwin effect in NGC 4151
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.
