TNG50 shows galactic outflow mass loading is non-monotonic with stellar mass, rising rapidly above 10^10.5 Msun due to black hole feedback, and produces fast multi-phase outflows with emergent collimation.
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A bias-controlled quasar sample of ~2000 objects demonstrates that the X-ray-to-UV luminosity relation remains constant from redshift 0.7 to 5.
The paper advocates for a high-S/N UV spectroscopic survey of quasars to produce a legacy archive enabling detailed CGM, IGM, Milky Way, and AGN outflow studies.
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First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
TNG50 shows galactic outflow mass loading is non-monotonic with stellar mass, rising rapidly above 10^10.5 Msun due to black hole feedback, and produces fast multi-phase outflows with emergent collimation.
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The X-ray-to-UV relation does not evolve in homogeneous quasar samples
A bias-controlled quasar sample of ~2000 objects demonstrates that the X-ray-to-UV luminosity relation remains constant from redshift 0.7 to 5.
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High-S/N Quasar Observations with HST/COS: Deep Fields for Spectroscopy
The paper advocates for a high-S/N UV spectroscopic survey of quasars to produce a legacy archive enabling detailed CGM, IGM, Milky Way, and AGN outflow studies.