Results 141 to 150 of about 85,255 (272)

The radio loud narrow-line quasar SDSSJ172206.03+565451.6

open access: green, 2005
S. Komossa   +5 more
openalex   +1 more source

Powerful Nuclear Outflows and Circumgalactic Medium Shocks Driven by the Most Luminous Known Obscured Quasar in the Universe

open access: yesThe Astrophysical Journal
We report integral field spectroscopy observations with the Near-Infrared Spectrograph on board the James Webb Space Telescope, targeting the 60 kpc environment surrounding the most luminous obscured quasar known at z = 4.6.
Andrey Vayner   +20 more
doaj   +1 more source

Galaxy and Mass Assembly (GAMA). The Properties of Quasar Host Galaxies: Star Formation Histories and Stellar Populations

open access: yesThe Astrophysical Journal
We investigated the star formation history and stellar populations of a sample of 205 Type I quasar host galaxies (0.1 < z < 0.35) and compared them with normal (nonactive) galaxies of the same mass and redshift within the volume of the Galaxy and Mass ...
Maria B. Stone   +7 more
doaj   +1 more source

Large-scale surveys of the quasar proximity effect

open access: yesThe Open Journal of Astrophysics
The UV radiation from high redshift quasars causes a local deficit in the neutral hydrogen absorption (Lyman-alpha forest) in their spectra, known as the proximity effect.
Rupert Croft   +8 more
doaj   +1 more source

Measuring the scale of cosmic homogeneity with SDSS-IV DR14 quasars [PDF]

open access: green, 2018
Rodrigo S. Gonçalves   +4 more
openalex   +1 more source

Astro2020 Science White Paper: A New Era for X-ray Lensing Studies of Quasars and Galaxies [PDF]

open access: green, 2019
G. Chartas   +4 more
openalex   +1 more source

A panchromatic view of infrared quasars: excess star formation and radio emission in the most heavily obscured systems [PDF]

open access: green, 2022
Carolina Andonie   +15 more
openalex   +1 more source

An Energetics of Quasar [PDF]

open access: yesProgress of Theoretical Physics, 1965
openaire   +1 more source

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