The z-GAL Pilot Program - data release December 01, 2020 

This public release contains all the uv-tables that were used for the
article "NOEMA redshift measurements of bright Herschel galaxies" by
Neri et al. 2020. 

CONTENTS

This public release contain spectral line and continuum uv-tables for
a sample of H-ATLAS selected SMGs observed with NOEMA band 1 (3mm) and
band 2 (2mm) between April 2018 and August 2019. The uv-tables are
provided in GILDAS and UVFITS format. Filenames are given according to
the following nomenclature:

 - 'source_id'-c-'center_frequency'.uvt               for continuum data
 - 'source_id'-'low_band_edge'-'high_band_edge.uvt    for line data

where 'source_id' is the name of the source in the Herschel Bright
Sources (HerBS) catalog, 'low_band_edge' is the frequency in MHz at
the lower end of the frequency range covered by the observations,
'high_band_edge' the frequency at the upper end, and 'center_frequency'
the reference frequency for the continuum as determined from the
line-free part of the spectrum.

Data reduction and calibration was made using the CLIC software
contained in the IRAM GILDAS package. The uv-tables provide
visibilities in units of Jy/beam and channels resampled from 2MHz to
channels of 16MHz. Tables with the native 2MHz spectral resolution are
available on request.

QUESTIONS and ACKNOWLEDGMENTS

If you have any questions about the data, please, contact us
(zgal@iram.fr). We also like to hear about any scientific use of the
data and would appreciate acknowledgment in publications or talks
using these data.