Distance, Energy, and Variability of Quasar Outflows: Two HST/COS Epochs of LBQS 1206+1052
HST/COS Observations of Quasar Outflows in the 500-1050 A Rest Frame. III. Four Similar Outflows in 2MASS J1051+1247 with Enough Energy to Be Major Contributors to AGN Feedback
HST/COS Observations of Quasar Outflows in the 500-1050 A Rest Frame. II. The Most Energetic Quasar Outflow Measured to Date
HST/COS Observations of Quasar Outflows in the 500-1050 A Rest Frame. I. The Most Energetic Outflows in the Universe and Other Discoveries
HST/COS Observations of Quasar Outflows in the 500-1050 A Rest Frame. IV. The Largest Broad Absorption Line Acceleration
HST/COS Observations of Quasar Outflows in the 500-1050 A Rest Frame. VI. Wide, Energetic Outflows in SDSS J0755+2306
HST/COS Observations of Quasar Outflows in the 500-1050 A Rest Frame. V. Richness of Physical Diagnostics and Ionization Potential-dependent Velocity Shift in PKS J0352-0711
HST/COS Observations of Quasar Outflows in the 500-1050 SRest Frame. VII. Distances and Energetics for 11 Outflows in Five Quasars
Probing the physicochemical properties of the Leo Ring and the Leo I group
The contribution of quasar absorption outflows to AGN feedback
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2017-05-13T15:52:56Z/2018-01-04T22:40:01Z
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, Arav comma Nahum, 2019, 'Deciphering Quasar Outflows and Measuring their Contribution to AGN Feedback', 1.0, European Space Agency, https://doi.org/10.5270/esa-92hm09z