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 Pilot Program DSFGs from Stanley et al. (2023) ================================================================================ Byte-by-byte Description of file: datafile5.txt -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- ID Source identifier 11- 15 F5.3 --- zspec z-GAL-based spectroscopic redshift of galaxies 17- 20 F4.2 mJy Speak Peak flux density of CO(1-0) line 22- 25 F4.2 mJy e_Speak Uncertainty in Speak 27- 30 I4 km/s DeltaV ? FWHM line width of CO(1-0) line 32- 34 I3 km/s e_DeltaV Uncertainty in DeltaV 36- 40 F5.3 Jy.km/s I ? Line flux of CO(1-0) line 42- 46 F5.3 Jy.km/s e_I Uncertainty in I 48- 50 F3.1 10+11.K.km/s.pc2 muL' Integrated line luminosity of CO(1-0) line * gravitational lensing factor 52- 54 F3.1 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 10+11solMass muMass Mass of molecular hydrogen * gravitational lensing factor (3) 63- 65 F3.1 10+11solMass e_muMass Uncertainty in muMass 67- 67 A1 --- f_muMass [l] Flag on muMass (1) 69- 71 I3 Myr tau Gas depletion time 73- 75 I3 Myr e_tau Uncertainty in tau 77- 80 F4.1 GHz nuCont-IF1 First intermediate frequency band continuum central frequency 82- 85 F4.1 GHz nuCont-IF2 ? Second intermediate frequency band continuum central frequency 87- 87 A1 --- l_SCont-IF1 Limit flag on SCont-IF1 89- 93 F5.3 mJy SCont-IF1 IF1 band continuum flux density (2) 95- 99 F5.3 mJy e_SCont-IF1 ? Uncertainty in SCont-IF1 101-101 A1 --- l_SCont-IF2 Limit flag on SCont-IF2 103-106 F4.2 mJy SCont-IF2 ? IF2 band continuum flux density (2) 108-111 F4.2 mJy e_SCont-IF2 ? Uncertainty in SCont-IF2 113-113 I1 --- 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. The signatures of their lensed nature can be seen in Berta et al. (2021) [2021A&A...646A.122B]; Stanley et al. (2023) [2023ApJ...945...24S]. Note (2): 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. -------------------------------------------------------------------------------- HerBS-34 2.633 0.7 0.12 593 112 0.44 0.11 1.5 0.4 6.0 1.6 150 40 32.0 < 0.03 4 HerBS-43a 3.212 0.3 0.06 1166 249 0.37 0.10 1.7 0.5 6.8 2.0 200 70 22.2 0.024 0.007 5 HerBS-43b 4.054 0.08 0.03 744 290 0.064 0.033 0.4 0.2 1.6 0.8 110 50 22.2 0.019 0.003 5 HerBS-44 2.927 0.95 0.14 377 63 0.38 0.08 1.5 0.3 6.0 1.2 50 10 29.2 38.5 < 0.05 < 0.08 6 HerBS-54 2.442 0.8 0.11 1087 176 0.92 0.19 2.7 0.6 10.8 2.4 450 110 33.1 0.072 0.13 5 HerBS-58 2.084 2.12 0.32 363 64 0.82 0.19 1.8 0.4 7.2 1.6 410 90 28.8 37.3 < 0.04 < 0.06 4 HerBS-70E 2.308 0.49 0.09 622 130 0.32 0.09 0.9 0.2 3.6 0.8 90 30 27.1 34.8 0.60 0.02 0.47 0.02 4 HerBS-70W 2.311 0.83 0.15 197 39 0.17 0.04 0.5 0.1 2.0 0.4 230 120 27.1 34.8 < 0.03 < 0.03 5 HerBS-79 2.078 1.24 0.17 787 125 1.04 0.22 2.3 0.5 l 9.2 2.0 l 510 120 28.7 37.5 < 0.03 < 0.04 5 HerBS-89a 2.949 0.64 0.09 1586 247 1.08 0.22 4.4 0.9 l 17.6 3.6 l 610 130 29.2 38.5 < 0.06 < 0.15 5 HerBS-95E 2.972 0.2 0.04 658 137 0.14 0.04 0.6 0.2 2.4 0.8 210 80 29.0 38.5 < 0.02 < 0.06 5 HerBS-95W 2.973 0.95 0.12 522 76 0.52 0.10 2.2 0.4 8.8 1.6 550 120 29.0 38.5 < 0.02 < 0.06 7 HerBS-113 2.787 1.46 0.21 497 81 0.77 0.16 2.9 0.6 l 11.6 2.4 l 390 90 30.4 38.5 < 0.05 < 0.07 4 HerBS-154 3.707 0.95 0.11 384 54 0.39 0.07 2.3 0.4 l 9.2 1.6 l 120 30 19.2 24.4 < 0.07 < 0.03 5