Results 131 to 140 of about 6,949,336 (206)

Color-redshift relations and photometric redshift estimations of quasars in large sky surveys

open access: yes, 2004
With a recently constructed composite quasar spectrum and the chi(2) minimization technique, we describe a general method for estimating the photometric redshifts of a large sample of quasars by deriving theoretical color-redshift relations and comparing
Zhang, W, Wu, XB, Zhou, X
core  

Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913. [PDF]

open access: yesNat Commun, 2022
Ginolfi M   +20 more
europepmc   +1 more source

First rest-frame infrared spectrum of a z > 7 quasar: MIRI-MRS observations of J1120+0641

open access: yes, 2023
Bosman S   +31 more
europepmc   +1 more source

The Ellis-Baldwin test. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci
Secrest NJ.
europepmc   +1 more source

Selections of High Redshift Quasars with Multi-wavelength Data

open access: yes, 2015
학위논문(박사)--서울대학교 대학원 :자연과학대학 물리·천문학부,2015. 8. 임명신.High redshift quasars (z > 5) hold keys to understanding the evolution of the universe in its early stage.
전이슬
core  

Challenges and opportunities for time-delay cosmography with multi-messenger gravitational lensing. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci
Birrer S   +4 more
europepmc   +1 more source

{\Lambda}CDM-Rastall cosmology revisited: constraints from a recent Quasars datasample

open access: yes
In this paper we study the impact of a recent quasar datasample in the constraint of the free parameters of an extension of general relativity. As a ruler to test, we use Rastall gravity in the context of background cosmology being a simple extension to ...
Hernández-Almada, Alberto   +4 more
core  

VLBI imaging of extremely high redshift quasars at 5 GHz

open access: yes, 1999
. We present very long baseline interferometry (VLBI) images of ten very high redshift (z ? 3) quasars at 5 GHz. The sources 0004+139, 0830+101, 0906+041, 0938+119 and 1500+045 were observed in September 1992 using a global VLBI array, while 0046+063 ...
Frey, S.   +15 more
core  

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