AGN STORM 2. VIII. Investigating the Narrow Absorption Lines in Mrk 817 Using HST-COS Observations
Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
Calibrating C-IV-based Black Hole Mass Estimators
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Diagnosing galactic feedback with line broadening in the low-redshift Lya forest
Extending the Calibration of C IV-based Single-epoch Black Hole Mass Estimators for Active Galactic Nuclei
HST/COS Observations of Galactic High-velocity Clouds: Four Active Galactic Nucleus Sight Lines through Complex C
Nearby Galaxy Filaments and the Ly-alpha Forest: Confronting Simulations and the UV Background with Observations
The Chemical Properties of Low-redshift QSOs
The effect of stellar and AGN feedback on the low-redshift Lyman a forest in the Sherwood simulation suite
The Low-redshift Intergalactic Medium as Seen in Archival Legacy HST/STIS and FUSE Data
Ultraviolet and X-ray Variability of the Seyfert 1.5 Galaxy Markarian 817
Instrument
COS, COS/FUV, WFC3, WFC3/UVIS
Temporal Coverage
2009-08-02T07:57:42Z/2009-08-04T03:33:53Z
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.
