BIANCHI, SIMONESIMONEBIANCHI0000-0002-3879-6038Giovanardi, C.C.Giovanardi0000-0003-4486-6802Smith, M. W. L.M. W. L.Smith0000-0003-1734-8356Fritz, J.J.Fritz0000-0002-9384-846XDavies, J. I.J. I.Davies0000-0001-9162-2371Haynes, M. P.M. P.HaynesGiovanelli, R.R.GiovanelliBaes, M.M.BaesBocchio, M.M.BocchioBoissier, S.S.BoissierBoquien, M.M.BoquienBoselli, A.A.BoselliCASASOLA, VIVIANAVIVIANACASASOLAClark, C. J. R.C. J. R.Clarkde Looze, I.I.de Loozedi Serego Alighieri, S.S.di Serego AlighieriGrossi, M.M.GrossiJones, A. P.A. P.JonesHughes, T. M.T. M.HughesHUNT, Leslie KippLeslie KippHUNTMadden, S.S.MaddenMAGRINI, LAURALAURAMAGRINIPappalardo, C.C.PappalardoYsard, N.N.YsardZIBETTI, StefanoStefanoZIBETTI2020-05-042020-05-042016http://hdl.handle.net/20.500.12386/24430Images of the Virgo cirrus in the atomic gas HI emission and in the dust emission at 250um from Herschel-SPIRE. Two images are provided for HI emission from low velocity (LVC; -20km/s<v<100km/s) and intermediate velocity (IVC; -100km/s<v<-20km/s) clouds. The images are the same presented in the left and mid panels of Fig. 3 in the paper. Three images are provided at 250um: the observations, with large scale offsets removed; the model, obtained from the emissivity values derived in the paper and the two atomic gas maps; the residuals between observations and models. The three images have been obtained from observations/model/residuals for each of the four HeViCS fields, and combined in a single large scale map after removing field-to-field offsets; they are the same presented in Fig. 8 of the paper. In all cases the resolution is 4.8'.enDatabasehttps://cdsarc.unistra.fr/viz-bin/cat/J/A%2bA/597/A1302016yCat..35970130BFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation