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The Astrophysical JournalWe report the identification of a quasar overdensity in the BOSSJ0210 field, dubbed the Cosmic Himalayas, consisting of 11 quasars at z = 2.16−2.20, the densest overdensity of quasars (17 σ ) in the ∼10,000 deg ^2 of the Sloan Digital Sky Survey (SDSS ...
Yongming Liang +29 more
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The Low-Mass End of the MBH/Mhost Relation in Quasars
Advances in Astronomy, 2012 The MBH-Mhost relation in quasars has been probed only in a limited parameter space, namely, at MBH∼109 M⊙ and Mhost∼1012 M⊙. Here we present a study of 26 quasars laying in the low-mass end of the relation, down to MBH∼107 M⊙.
Roberto Decarli +5 more
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Symposium - International Astronomical Union, 1972 I report here work done at Jodrell Bank by Mr John Gilbert and myself at a wavelength of 49 cm, on the degree of linear polarization, m49. For most sources the polarization is considerably reduced from its short wavelength value. We presume that most of this depolarization is by Faraday rotation, or rather by Faraday dispersion, between different parts
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A Search for Low-energy Gamma-rays from the Quasar 3C286 [PDF]
, 1965 D. J. Adams, R. R. Hillier, A.F. Janes
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Quasars and Their Host Galaxies [PDF]
, 2006 This review attempts to describe developments in the fields of quasar and quasar host galaxies in the past five. In this time period, the Sloan and 2dF quasar surveys have added several tens of thousands of quasars, with Sloan quasars being found to z>6. Obscured, or partially obscured quasars have begun to be found in significant numbers.
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The Detection Rate of Associated Mg ii Absorption Lines in Quasars Depends on Their Radio Emission
The Astrophysical JournalIn active galactic nuclei, jet-driven feedback plays a significant role in influencing the properties of gas within their host galaxy and the circumgalactic medium.
Zhi-Fu Chen, Luis C. Ho
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