We present here the first results from the Chandra ERA (Environments of Radio-loud AGN) Large Project, characterizing the cluster environments of a sample of 26 radio-loud active galactic nuclei (AGNs) at z ∼ 0.5 that covers three decades of radio luminosity. This is the first systematic X-ray environmental study at a single epoch, and has allowed us to examine the relationship between radio luminosity and cluster environment without the problems ofMalmquist bias.We have found a weak correlation between radio luminosity and host cluster X-ray luminosity, as well as tentative evidence that this correlation is driven by the subpopulation of low-excitation radio galaxies, with high-excitation radio galaxies showing no significant correla...
none10siWe present the results from new ~15 ks Chandra-ACIS and 4.9 GHz Very Large Array (VLA) obser...
Our understanding of how active galactic nucleus feedback operates in galaxy clusters has improved i...
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1....
Copyright IAURadio-loud AGN play an important role in galaxy evolution. We need to understand their ...
The interactions between radio-loud AGN and their environments play an important rôle in galaxy and ...
In this study, we investigate 89 radio galaxies that are spectroscopically confirmed to be members o...
This thesis contains the first systematic X-ray investigation of the relationships between the prope...
An understanding of the relationship betwe...
The spatial clustering amplitude (B_{gq}) is determined for a sample of 44 powerful AGN at z~0.2. No...
Context. Several problems with the process of galaxy formation are still open. One of them is the ro...
Low frequency radio astronomy allows us to observe the fainter and older synchrotron emission from t...
none7siFirst-ranked galaxies in clusters, usually referred to as brightest cluster galaxies (BCGs), ...
We study the cosmic evolution of radio sources out to z ≃ 1.5 using a GMRT 610 MHz survey covering ∼...
We discuss the optical properties, X-ray detections and active galactic nucleus (AGN) populations of...
Context. The mechanism of radio emission in radio-quiet (RQ) active galactic nuclei (AGNs) is still ...
none10siWe present the results from new ~15 ks Chandra-ACIS and 4.9 GHz Very Large Array (VLA) obser...
Our understanding of how active galactic nucleus feedback operates in galaxy clusters has improved i...
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1....
Copyright IAURadio-loud AGN play an important role in galaxy evolution. We need to understand their ...
The interactions between radio-loud AGN and their environments play an important rôle in galaxy and ...
In this study, we investigate 89 radio galaxies that are spectroscopically confirmed to be members o...
This thesis contains the first systematic X-ray investigation of the relationships between the prope...
An understanding of the relationship betwe...
The spatial clustering amplitude (B_{gq}) is determined for a sample of 44 powerful AGN at z~0.2. No...
Context. Several problems with the process of galaxy formation are still open. One of them is the ro...
Low frequency radio astronomy allows us to observe the fainter and older synchrotron emission from t...
none7siFirst-ranked galaxies in clusters, usually referred to as brightest cluster galaxies (BCGs), ...
We study the cosmic evolution of radio sources out to z ≃ 1.5 using a GMRT 610 MHz survey covering ∼...
We discuss the optical properties, X-ray detections and active galactic nucleus (AGN) populations of...
Context. The mechanism of radio emission in radio-quiet (RQ) active galactic nuclei (AGNs) is still ...
none10siWe present the results from new ~15 ks Chandra-ACIS and 4.9 GHz Very Large Array (VLA) obser...
Our understanding of how active galactic nucleus feedback operates in galaxy clusters has improved i...
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1....