The Javalambre Photometric Local Universe Survey (J-PLUS) is a 12-band photometric survey using the 83-cm JAST telescope. Data Release 3 includes 47.4 million...
J-PLUS: Spectroscopic validation of Hα emission line maps in spatially resolved galaxies
Aims. We present a dedicated automated pipeline to construct spatially resolved emission Hα+[NII] maps and to derive the spectral energy distributions (SEDs) in...
J-PLUS: The Javalambre Photometric Local Universe Survey
The Javalambre Photometric Local Universe Survey (J-PLUS ) is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the...
J-PLUS: Uncovering a large population of extreme [OIII] emitters in the local Universe
Context. Over the past decades, several studies have discovered a population of galaxies that undergo very strong star formation events. They are called extreme...
Jansky VLA observations of synchrotron emitting optical hotspots of 3C 227 and 3C 445 radio galaxies
We report results on deep Jansky Very Large Array (VLA) A-configuration observations at 22 GHz of the hotspots of the radio galaxies 3C 227 and 3C 445...
Jet-induced molecular gas excitation and turbulence in the Teacup
In order to investigate the impact of radio jets on the interstellar medium (ISM) of galaxies hosting active galactic nuclei (AGN), we present subarcsecond...
Jets from Subparsec to Kiloparsec Scales: A Physical Connection
The Chandra discovery of bright X-ray emission from kiloparsec-scale jets allows insight into the physical parameters of the jet flow at large scales. At the...
Joint gas and stellar dynamical models of WLM: an isolated dwarf galaxy within a cored, prolate DM halo
We present multitracer dynamical models of the low-mass (M * ∼ 10 7), isolated dwarf irregular galaxy WLM in order to simultaneously constrain the inner slope...
Joint gas and stellar dynamical models of WLM: an isolated dwarf galaxy within a cored, prolate DM halo
We present multitracer dynamical models of the low-mass (M * ∼ 10 7), isolated dwarf irregular galaxy WLM in order to simultaneously constrain the inner slope...