S. Carniani

Author notes These authors contributed equally: B. E. Robertson, S. Tacchella. Authors and Affiliations Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA, USA B. E. Robertson & K. A. Suess Kavli Institute for Cosmology, University of Cambridge, Cambridge, UK S. Tacchella, M. Curti, F. D’Eugenio, T. J. Looser, R. Maiolino, H. Übler, J. Witstok & L. Sandles Cavendish Laboratory, University of Cambridge, Cambridge, UK S. Tacchella, M. Curti, F. D’Eugenio, T. J. Looser, R. Maiolino, H.

The optical integral field spectroscopic data were retrieved from the European Southern Observatory (ESO) archive and were obtained with the MUSE spectrometer at the ESO’s VLT with an on-source integration time of 52?min. The wavelength coverage is from 0.46??m to 0.93??m and the spectral resolution varies from R?=?2,000 to R?=?4,000 across the wavelength range. The seeing during the observations was only about 2.5?.