Results 91 to 100 of about 85,255 (272)

Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8

open access: yes, 2015
We study the dependence of quasar clustering on quasar luminosity and black hole mass by measuring the angular overdensity of photometrically selected galaxies imaged by WISE about z $\sim$ 0.8 quasars from SDSS.
Eisenstein, Daniel J.   +1 more
core   +1 more source

Spectroscopy along Multiple, Lensed Sightlines through Outflowing Winds in the Quasar SDSS J1029+2623 [PDF]

open access: yes, 2012
We study the origin of absorption features on the blue side of the C IV broad emission line of the large-separation lensed quasar SDSS J1029+2623 at z_em ~ 2.197.
Gandhi, Poshak   +5 more
core   +3 more sources

Adenosine A2A Receptors Control the Mis‐Localization of Aquaporin‐4 in Rats Subject to Repeated Restraint Stress

open access: yesJournal of Neurochemistry, Volume 170, Issue 4, April 2026.
Restraint stress triggers anxiety, along with a loss of polarization and coverage of aquaporin‐4 (AQP4) in astrocytes of the frontal cortex; these effects are attenuated by blockade of adenosine A2A receptors. ABSTRACT Repeated stress triggers anxiety accompanied by a deregulation of cortical glucocorticoid receptors, which is relieved by blocking ...
Liliana Dias   +5 more
wiley   +1 more source

The Extremely Luminous Quasar Survey (ELQS) in the SDSS footprint I.: Infrared Based Candidate Selection

open access: yes, 2017
Studies of the most luminous quasars at high redshift directly probe the evolution of the most massive black holes in the early Universe and their connection to massive galaxy formation.
Fan, Xiaohui   +6 more
core   +1 more source

The Extremely Luminous Quasar Survey in the Pan-STARRS 1 Footprint (PS-ELQS) [PDF]

open access: yes, 2019
We present the results of the Extremely Luminous Quasar Survey in the $3\pi$ survey of the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS; PS1).
Fan, Xiaohui   +9 more
core   +2 more sources

Surveying the Onset and Evolution of Supermassive Black Holes at High-z with AXIS

open access: yesUniverse
The nature and origin of supermassive black holes (SMBHs) remain an open matter of debate within the scientific community. While various theoretical scenarios have been proposed, each with specific observational signatures, the lack of sufficiently ...
Nico Cappelluti   +9 more
doaj   +1 more source

Work in Progress: Use of Wood‐Based Inserts in Injection Molding

open access: yesEngineering Reports, Volume 8, Issue 3, March 2026.
The study investigates the suitability of wood‐based mold inserts for the production of small series in polymer injection molding, showing that specially modified materials like laminated beech and compressed bamboo are more promising than natural woods. The results indicate that reproducible components can be produced with these tools. ABSTRACT In the
David Grundmann   +6 more
wiley   +1 more source

The Subaru high-z quasar survey: discovery of faint z~6 quasars

open access: yes, 2014
We present the discovery of one or two extremely faint z~6 quasars in 6.5 deg^2 utilizing a unique capability of the wide-field imaging of the Subaru/Suprime-Cam.
Furusawa, Hisanori   +11 more
core   +1 more source

Anisotropy Analysis of Bamboo and Tooth Using 4‐Angle Polarization Micro‐Spectroscopy

open access: yesNano Select, Volume 7, Issue 3, March 2026.
Super‐resolution via orientation: spatial distribution of specific molecular vibrations are revealed at 1/20 of the diffraction limit. ABSTRACT To investigate the anisotropic properties of biomaterials, two distinct classes are considered as follows: polymer‐based (cellulose in plants) and crystalline‐based (enamel in teeth), each demonstrating ...
Meguya Ryu   +8 more
wiley   +1 more source

Probing the faint end of the quasar luminosity function at z ~ 4 in the COSMOS field [PDF]

open access: yes, 2010
We searched for quasars that are ~ 3 mag fainter than the SDSS quasars in the redshift range 3.7 < z < 4.7 in the COSMOS field to constrain the faint end of the quasar luminosity function.
Boyle   +26 more
core   +2 more sources

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