We present observations of a complete sub-sample of 20 radio galaxies from the Third Cambridge Catalog (3C) with redshift <0.3 obtained from VLT/MUSE optical integral field spectrograph. These data have been obtained as part of the survey MURALES (a MUse RAdio Loud Emission line Snapshot survey) with the main goal of exploring the Active Galactic Nuclei (AGN) feedback process in a sizeable sample of the most powerful radio sources at low redshift. We present the data analysis and, for each source, the resulting emission line images and the 2D gas velocity field. Thanks to their unprecedented depth (the median 3 sigma surface brightness limit in the emission line maps is 6X10^-18 erg s-1 cm-2 arcsec-2, these observations reveal emis...
From an optical spectroscopic survey of 3CR radiogalaxies (RGs) with z < 0.3, we discovered three ob...
We study the composition of the faint radio population selected from the VLA-COSMOS 3GHz Large Proje...
We discuss CO spectral line data of a volume-limited sample of 23 nearby (z<0.03) low luminosity rad...
We present observations of a complete sub-sample of 20 radio galaxies from the Third Cambridge Catal...
We report the first results of the MURALES survey, a complete program of MUSE observations of nearby...
This is the sixth paper presenting the results of the MUse RAdio Loud Emission line Snapshot survey ...
We present 19 nearby (z < 0.3) 3CR radio galaxies imaged at low and high excitation as part of a ...
We present HST/WFPC2 Linear Ramp Filter images of high surface brightness emission lines (either [OI...
We present Hubble Space Telescope WFPC2 Linear Ramp Filter images of high surface brightness emissio...
From an optical spectroscopic survey of 3CR radio galaxies with z<0.3, we discovered a new spectrosc...
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. T...
Context. There is growing observational evidence of active galactic nuclei (AGN) feedback on the int...
We explore the implications of our optical spectroscopic survey of 3CR radio sources with z < 0.3 fo...
Active galactic nuclei (AGNs) show episodic activity, which can be evident in galaxies that exhibit ...
From an optical spectroscopic survey of 3CR radiogalaxies (RGs) with z < 0.3, we discovered three ob...
We study the composition of the faint radio population selected from the VLA-COSMOS 3GHz Large Proje...
We discuss CO spectral line data of a volume-limited sample of 23 nearby (z<0.03) low luminosity rad...
We present observations of a complete sub-sample of 20 radio galaxies from the Third Cambridge Catal...
We report the first results of the MURALES survey, a complete program of MUSE observations of nearby...
This is the sixth paper presenting the results of the MUse RAdio Loud Emission line Snapshot survey ...
We present 19 nearby (z < 0.3) 3CR radio galaxies imaged at low and high excitation as part of a ...
We present HST/WFPC2 Linear Ramp Filter images of high surface brightness emission lines (either [OI...
We present Hubble Space Telescope WFPC2 Linear Ramp Filter images of high surface brightness emissio...
From an optical spectroscopic survey of 3CR radio galaxies with z<0.3, we discovered a new spectrosc...
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. T...
Context. There is growing observational evidence of active galactic nuclei (AGN) feedback on the int...
We explore the implications of our optical spectroscopic survey of 3CR radio sources with z < 0.3 fo...
Active galactic nuclei (AGNs) show episodic activity, which can be evident in galaxies that exhibit ...
From an optical spectroscopic survey of 3CR radiogalaxies (RGs) with z < 0.3, we discovered three ob...
We study the composition of the faint radio population selected from the VLA-COSMOS 3GHz Large Proje...
We discuss CO spectral line data of a volume-limited sample of 23 nearby (z<0.03) low luminosity rad...