A Jet Model for the Broadband Spectrum Of the Seyfert 1 Galaxy NGC 4051
Characterizing Transition Temperature Gas in the Galactic Corona
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
Far Ultraviolet Spectroscopic Explorer Spectroscopy of Absorption and Emission Lines from the Narrow-Line Seyfert 1 Galaxy NGC 4051
Feedback from Mass Outflows in Nearby Active Galactic Nuclei. I. Ultraviolet and X-Ray Absorbers
High-Resolution X-Ray and Ultraviolet Spectroscopy of the Complex Intrinsic Absorption in NGC 4051 with Chandra and the Hubble Space Telescope
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Observations of Outflowing Ultraviolet Absorbers in NGC 4051 with the Cosmic Origins Spectrograph
The Milky Way halo as a QSO absorption-line system. New results from an HST/STIS absorption-line catalogue of Galactic high-velocity clouds
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-03-24T21:32:15Z/2000-03-25T03:02:57Z
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, Brandt comma William Nielsen, 2006, 'Coordinated STIS/AXAF Spectroscopy of UV/X-ray Absorption in the Seyfert 1 Galaxy NGC 4051', 1.0, European Space Agency, https://doi.org/10.5270/esa-2327hc0
