학술논문
z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [I] Overview
Document Type
Working Paper
Author
Cox, P.; Neri, R.; Berta, S.; Ismail, D.; Stanley, F.; Young, A.; Jin, S.; Bakx, T.; Beelen, A.; Dannerbauer, H.; Krips, M.; Lehnert, M.; Omont, A.; Riechers, D. A.; Baker, A. J.; Bendo, G.; Borsato, E.; Buat, V.; Butler, K.; Chartab, N.; Cooray, A.; Dye, S.; Eales, S.; Gavazzi, R.; Hughes, D.; Ivison, R.; Jones, B. M.; Marchetti, L.; Messias, H.; Nanni, A.; Negrello, M.; Perez-Fournon, I.; Serjeant, S.; Urquhart, S.; Vlahakis, C.; Weiss, A.; van der Werf, P.; Yang, C.
Source
A&A 678, A26 (2023)
Subject
Language
Abstract
(Abridged) Using the IRAM NOEMA interferometer, we measures the redshifts of 126 bright galaxies detected in the Herschel H-ATLAS, HeLMS, and HerS surveys. We report reliable spectroscopic redshifts for a total of 124 of the Herschel-selected galaxies. The redshifts are estimated from scans of the 3 and 2-mm bands (and, in one case, the 1-mm band) and are based on the detection of at least two emission lines. Together with the Pilot Programme (Neri et al. 2020), including spectroscopic redshifts of 11 sources, our survey has derived precise redshifts for 135 bright Herschel-selected galaxies, making it the largest sample of high-z galaxies with robust redshifts to date. Most emission lines detected are from 12CO (mainly from J=2-1 to 5-4), with some sources seen in [CI] and H2O emission lines. The spectroscopic redshifts are in the range 0.8