The μ–z diagram (Figure 1) plots the observed internal proper motion μ versus redshift z for 32 extragalactic radio sources associated with active galactic nuclei. The observed points fall below an upper bound which decreases with redshift; there is a statistically significant anticorrelation between redshift and internal proper motion
The definitive version is available at www.blackwell-synergy.com Copyright Blackwell Publishing DOI ...
A remarkable correlation is found in radio-loud quasars and BLLacs when the directly observed angula...
Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range z > ...
The μ–z diagram (Figure 1) plots the observed internal proper motion μ versus redshift z for 32 extr...
Research in observational cosmology; gives a more refined analysis of data set considered in Jackson...
Radio-loud quasars at high redshift (z ≥ 4) are rare objects in the universe and rarely observed wit...
The comparison of redshift-distance relationship for high and low-redshift supernovae revealed the s...
Highly accreting quasars are possible cosmological probes, as their Eddington ratio is expected to s...
The Cosmological Principle is part of the foundation that underpins the standard model of the Univer...
The cosmological concordance model (ΛCDM) well accounts for a wealth of observations, from the exist...
Abstract. The envelope function in the largest angular size-redshift diagram for quasars is shown to...
Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range at $...
Context. Ultra-compact structure in radio sources (especially in quasars that can be observed up to ...
This paper is aimed at verifying the predictions of relativistic beaming and orientation based unifi...
In this work, a theoretical model is developed for explanation of temporal evolution of extragalacti...
The definitive version is available at www.blackwell-synergy.com Copyright Blackwell Publishing DOI ...
A remarkable correlation is found in radio-loud quasars and BLLacs when the directly observed angula...
Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range z > ...
The μ–z diagram (Figure 1) plots the observed internal proper motion μ versus redshift z for 32 extr...
Research in observational cosmology; gives a more refined analysis of data set considered in Jackson...
Radio-loud quasars at high redshift (z ≥ 4) are rare objects in the universe and rarely observed wit...
The comparison of redshift-distance relationship for high and low-redshift supernovae revealed the s...
Highly accreting quasars are possible cosmological probes, as their Eddington ratio is expected to s...
The Cosmological Principle is part of the foundation that underpins the standard model of the Univer...
The cosmological concordance model (ΛCDM) well accounts for a wealth of observations, from the exist...
Abstract. The envelope function in the largest angular size-redshift diagram for quasars is shown to...
Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range at $...
Context. Ultra-compact structure in radio sources (especially in quasars that can be observed up to ...
This paper is aimed at verifying the predictions of relativistic beaming and orientation based unifi...
In this work, a theoretical model is developed for explanation of temporal evolution of extragalacti...
The definitive version is available at www.blackwell-synergy.com Copyright Blackwell Publishing DOI ...
A remarkable correlation is found in radio-loud quasars and BLLacs when the directly observed angula...
Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range z > ...