We present radio Active Galactic Nuclei (AGN) luminosity functions over the redshift range 0.005 < z < 0.75. The sample from which the luminosity functions are constructed is an optical spectroscopic survey of radio galaxies, identified from matched Faint Images of the Radio Sky at Twenty-cm survey (FIRST) sources and Sloan Digital Sky Survey (SDSS) images. The radio AGN are separated into Low Excitation Radio Galaxies (LERGs) and High Excitation Radio Galaxies (HERGs) using the optical spectra. We derive radio luminosity functions for LERGs and HERGs separately in the three redshift bins (0.005 < z< 0.3, 0.3 < z < 0.5 and 0.5 < z <0.75). The radio luminosity functions can be well described by a double power-law. Assuming this double power...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies und...
We present a model to predict the luminosity function for radio galaxies and their linear size distr...
Exploring how radio-emitting active galactic nuclei (AGN) behave and evolve with time is critical fo...
We present radio Active Galactic Nuclei (AGN) luminosity functions over the redshift range 0.005 < z...
© 2016 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society...
© 2016 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society...
© 2016 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society...
This paper presents a study of the redshift evolution of radio-loud active galactic nuclei (AGN) as ...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies und...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies und...
MP, TM, KM, MJ, RJ and SF acknowledge support by the South African Square Kilometre Array Project an...
© 2018 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Socie...
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1....
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1...
We study the cosmic evolution of radio sources out to z ≃ 1.5 using a GMRT 610 MHz survey covering ∼...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies und...
We present a model to predict the luminosity function for radio galaxies and their linear size distr...
Exploring how radio-emitting active galactic nuclei (AGN) behave and evolve with time is critical fo...
We present radio Active Galactic Nuclei (AGN) luminosity functions over the redshift range 0.005 < z...
© 2016 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society...
© 2016 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society...
© 2016 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society...
This paper presents a study of the redshift evolution of radio-loud active galactic nuclei (AGN) as ...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies und...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies und...
MP, TM, KM, MJ, RJ and SF acknowledge support by the South African Square Kilometre Array Project an...
© 2018 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Socie...
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1....
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1...
We study the cosmic evolution of radio sources out to z ≃ 1.5 using a GMRT 610 MHz survey covering ∼...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies und...
We present a model to predict the luminosity function for radio galaxies and their linear size distr...
Exploring how radio-emitting active galactic nuclei (AGN) behave and evolve with time is critical fo...