Add to ORKGWe summarize the results of an X-ray spectroscopic survey of radio-loud AGNs observed with ASCA, using proprietary and archival data (public up to 1998 September). We briefly compare our results with those obtained for radio-quiet AGNs studied by other authors, and with the predictions of unified models
We report ROSAT X-ray observations of two powerful radio galaxies. 3C 280 provides evidence for a mi...
none10siWe present the results from new ~15 ks Chandra-ACIS and 4.9 GHz Very Large Array (VLA) obser...
Radio-loud AGN (> 10 22 W Hz-1 at 1.4 GHz) will be the dominant bright source population detected wi...
We present a uniform and systematic analysis of the 0.6-10 keV X-ray spectra of radio-loud active ga...
We have conducted 22 GHz radio imaging at 1 arcsec resolution of 100 low-redshift AGN selected at 1...
We present the result of 27 ASCA observations of 26 radio-quiet quasars (RQQs) from the PG survey. A...
We present results of a complete radio follow-up obtained with the VLA and ATCA radio telescopes dow...
The current paradigm for radio-quiet AGNs is reviewed, taking into account new results from recent l...
Context. When can an active galactic nucleus (AGN) be considered radio loud (RL)? Following the esta...
This recently expired grant has supported the work of the PI, his students, and his collaborators on...
Super massive black holes (SMBH) are thought to be ubiquitously hosted in massive galaxies. They may...
In a previous paper we showed that the radio sources selected by combining large area radio and opt...
Context. X-ray emission from active galactic nuclei (AGN) is dominated by the accretion disk around ...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASPWe present...
Over recent years there has been mounting evidence that accreting supermassive black holes in active...
We report ROSAT X-ray observations of two powerful radio galaxies. 3C 280 provides evidence for a mi...
none10siWe present the results from new ~15 ks Chandra-ACIS and 4.9 GHz Very Large Array (VLA) obser...
Radio-loud AGN (> 10 22 W Hz-1 at 1.4 GHz) will be the dominant bright source population detected wi...
We present a uniform and systematic analysis of the 0.6-10 keV X-ray spectra of radio-loud active ga...
We have conducted 22 GHz radio imaging at 1 arcsec resolution of 100 low-redshift AGN selected at 1...
We present the result of 27 ASCA observations of 26 radio-quiet quasars (RQQs) from the PG survey. A...
We present results of a complete radio follow-up obtained with the VLA and ATCA radio telescopes dow...
The current paradigm for radio-quiet AGNs is reviewed, taking into account new results from recent l...
Context. When can an active galactic nucleus (AGN) be considered radio loud (RL)? Following the esta...
This recently expired grant has supported the work of the PI, his students, and his collaborators on...
Super massive black holes (SMBH) are thought to be ubiquitously hosted in massive galaxies. They may...
In a previous paper we showed that the radio sources selected by combining large area radio and opt...
Context. X-ray emission from active galactic nuclei (AGN) is dominated by the accretion disk around ...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASPWe present...
Over recent years there has been mounting evidence that accreting supermassive black holes in active...
We report ROSAT X-ray observations of two powerful radio galaxies. 3C 280 provides evidence for a mi...
none10siWe present the results from new ~15 ks Chandra-ACIS and 4.9 GHz Very Large Array (VLA) obser...
Radio-loud AGN (> 10 22 W Hz-1 at 1.4 GHz) will be the dominant bright source population detected wi...