AGN winds as probes of cosmic feedback: the case of Mrk 509
Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
Calibrating C-IV-based Black Hole Mass Estimators
Characterizing the UV and X-ray Outflow in Mrk 509
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Extending the Calibration of C IV-based Single-epoch Black Hole Mass Estimators for Active Galactic Nuclei
Galactic-scale Absorption Outflow in the Low-luminosity Quasar IRAS F04250-5718: Hubble Space Telescope/Cosmic Origins Spectrograph Observations
Multiwavelength campaign on Mrk 509. II. Analysis of high-quality Reflection Grating Spectrometer spectra
Multiwavelength campaign on Mrk 509. I. Variability and spectral energy distribution
Multiwavelength campaign on Mrk 509. IV. Optical-UV-X-ray variability and the nature of the soft X-ray excess
Multiwavelength Campaign on Mrk 509 IX. Lower Limit on the Distance of the Absorber from HST COS and STIS Spectroscopy
Multiwavelength campaign on Mrk 509. IX. The Galactic foreground
Multiwavelength campaign on Mrk 509. V. Chandra-LETGS observation of the ionized absorber
Multiwavelength campaign on Mrk 509. VI. HST/COS observations of the far-ultraviolet spectrum
Multiwavelength campaign on Mrk 509. VIII. Location of the X-ray absorber
Multiwavelength campaign on Mrk 509. VII. Relative abundances of the warm absorber
Multiwavelength campaign on Mrk 509. XII. Broad band spectral analysis
Multiwavelength campaign on Mrk 509. XIV. Chandra HETGS spectra
Multiwavelength campaign on Mrk 509. X. Lower limit on the distance of the absorber from HST COS and STIS spectroscopy
Multiwavelength campaign on Mrk 509. XV. Global modeling of the broad emission lines in the optical, UV, and X-ray bands
Multiwavelength campaign on Mrk 509. XVI. Continued HST/COS monitoring of the far-ultraviolet spectrum
New Measurements of the Lya Forest Continuum and Effective Optical Depth with LyCAN and DESI Y1 Data
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
The Low-redshift Intergalactic Medium as Seen in Archival Legacy HST/STIS and FUSE Data
Winds in Mrk 509: A Common Origin for the X-ray and UV Ionized Gas?
Instrument
COS, COS/FUV
Temporal Coverage
2009-12-10T02:48:40Z/2009-12-11T09:38:33Z
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.
