URSO, Riccardo GiovanniRiccardo GiovanniURSO0000-0001-6926-1434PALUMBO, Maria ElisabettaMaria ElisabettaPALUMBO0000-0002-1216-7831Ceccarelli, C.C.Ceccarelli0000-0002-9122-491XBalucani, N.N.Balucani0000-0003-1859-3070Bottinelli, S.S.Bottinelli0000-0002-3688-160XCODELLA, CLAUDIOCLAUDIOCODELLA0000-0003-4864-2806FONTANI, FRANCESCOFRANCESCOFONTANI0000-0003-1514-3074LETO, PAOLOPAOLOLETO0000-0003-0348-3418TRIGILIO, CORRADOCORRADOTRIGILIO0000-0002-6972-8388Vastel, C.C.Vastel0000-0002-7288-4613Bachiller, R.R.BachillerBARATTA, GiuseppeGiuseppeBARATTABUEMI, CARLA SIMONACARLA SIMONABUEMICaux, E.E.CauxJaber Al-Edhari, A.A.Jaber Al-EdhariLefloch, B.B.LeflochLopez-Sepulcre, A.A.Lopez-SepulcreUMANA, Grazia Maria GloriaGrazia Maria GloriaUMANATESTI, LeonardoLeonardoTESTI2022-11-212022-11-212019http://hdl.handle.net/20.500.12386/32729Data reported in Figure 1 correspond to newly detected C<SUB>2</SUB>O and lines towards: L1544 (panels A, B, C, D, E and F); L1498 (panels G and H); and Elias 18 (panels I and J). Each panel reports the molecule and its transition. The detection reported in panel G (performed with the Noto-32m telescope) was acquired with a lower resolution than that used for the observations reported in the other panels (IRAM-30m telescope). For clarity we give a larger VLSR scale that allows a better evaluation of the baseline. <P />Table 1 and Table 2 in the paper report information on the spectroscopic parameters and telescope used. <P />Further details are given in Section 2 in the paper. <P />Files are given in FITS and ASCII format for each panel. <P />(3 data files).enDatabase10.26093/cds/vizier.36280072https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/628/A722019yCat..36280072UFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation