Bono, G.G.BonoNonino, M.M.NoninoFabrizio, MicheleMicheleFabrizioBuonanno, R.R.Buonanno2020-09-172020-09-172017-01-01https://hdl.handle.net/20.500.13025/5462VizieR On-line Data Catalog J/ApJ/830/126. Originally published in 2016ApJ...830..126FTo constrain the Carina kinematical structure, we adopted data collected at four spectrographs mounted at the Very Large Telescope (VLT) of the European Southern Observatory (ESO). The spectral resolution of data ranges from 600 to 40000, allowing us to obtain accurate RVs up to the horizontal branch (HB) magnitude level (V~21.5mag). (1 data file).Galaxies spectraRadial velocitiesPhotometry UBVRIStars horizontal branchStars giant Comment table2.dat 2748x88 Radial velocities of spectroscopic targetshttp://adsabs.harvard.edu/abs/2017yCat..18300126F2017yCat..18300126F