Title: Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6 Authors: Prajapati P., Riechers D., Cox P., Weiss A., Saintonge A., Jones B., Bakx T.J.L.C., Berta S., van der Werf P., Neri R., Butler K.M., Cooray A., Ismail D., Baker A.J., Borsato E., Harris A., Ivison R., Lehnert M., Marchetti L., Messias H., Omont A., Vlahakis C., Yang C. Table: Vz-GAL (this work): CO(2–1) Line and Underlying Continuum Properties ================================================================================ Byte-by-byte Description of file: datafile4.txt -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- ID Source identifier 11- 16 F6.4 --- zspec z-GAL-based spectroscopic redshift of galaxies 18- 21 F4.2 mJy Speak Peak flux density of CO(2-1) line 23- 26 F4.2 mJy e_Speak Uncertainty in Speak 28- 30 I3 km/s DeltaV FWHM line width of CO(2-1) line 32- 34 I3 km/s e_DeltaV Uncertainty in DeltaV 36- 39 F4.2 Jy.km/s I Line flux of CO(2-1) line 41- 44 F4.2 Jy.km/s e_I Uncertainty in I 46- 49 F4.2 10+11.K.km/s.pc2 muL' Integrated line luminosity of CO(2-1) line * gravitational lensing factor 51- 54 F4.2 10+11.K.km/s.pc2 e_muL' ? Uncertainty in muL' 56- 56 A1 --- f_muL' [l] Flag on muL' (1) 58- 61 F4.1 GHz nuCont-IF1 First intermediate frequency band continuum central frequency 63- 63 A1 --- f_nuCont-IF1 [*] Flag on nuCont-IF1 (2) 65- 68 F4.1 GHz nuCont-IF2 ? Second intermediate frequency band continuum central frequency 70- 70 A1 --- l_SCont-IF1 Limit flag on SCont-IF1 72- 75 F4.2 mJy SCont-IF1 IF1 band continuum flux density (3) 77- 80 F4.2 mJy e_SCont-IF1 ? Uncertainty in SCont-IF1 82- 82 A1 --- l_SCont-IF2 Limit flag on SCont-IF2 84- 87 F4.2 mJy SCont-IF2 ? IF2 band continuum flux density (3) 89- 90 I2 --- Sig Line significance in {sigma}; rms noise of the moment-0 map of the line -------------------------------------------------------------------------------- Note (1): l = Line luminosities and gas masses of lensed DSFG candidates. Many of these targets have known lensing factor {mu} > 1 from Borsato et al. (2024) [2024AMRAS.528.6222B]. Note (2): * = CASA tclean mfs-mode-based net central frequency for a combined continuum of individual IF1 and IF2 detections at two different central frequencies. Note (3): For continuum non-detections (SNR < 2), we provide the 3{sigma}_c_ upper-limits on the continuum flux densities (assuming an unresolved emission within a beam), where {sigma}_c_ is the rms noise of a given continuum map. -------------------------------------------------------------------------------- HeLMS-19 4.6880 4.29 0.45 288 35 1.31 0.21 2.76 0.44 l 41.1 0.87 0.10 5 HeLMS-24 4.9841 2.26 0.14 691 50 1.66 0.16 3.83 0.37 34.4 * 0.09 0.02 11 HeLMS-27 3.7652 2.07 0.56 599 189 1.32 0.12 1.95 0.18 l 43.0 48.2 < 0.14 < 0.35 2 HeLMS-36 3.9802 0.78 0.15 309 67 0.26 0.07 0.42 0.11 45.6 < 0.15 3 HeLMS-45 5.3998 1.06 0.10 515 56 0.58 0.08 1.51 0.21 28.2 36.1 < 0.09 < 0.18 8 HerS-11 4.6618 1.66 0.17 462 55 0.82 0.13 1.70 0.27 41.2 < 0.19 7 HerBS-78 3.7344 0.95 0.29 639 224 0.65 0.06 0.96 0.10 48.1 < 0.18 3 HerBS-177 3.9625 1.49 0.23 593 104 0.94 0.10 1.52 0.15 l 45.9 < 0.13 5 HerBS-179 3.9423 1.23 0.38 385 137 0.50 0.05 0.80 0.10 46.1 < 0.19 2 HerBS-185 4.3238 0.97 0.15 469 83 0.48 0.11 0.90 0.20 l 42.7 < 0.17 4