D'ORAZI, VALENTINAVALENTINAD'ORAZI0000-0001-9275-9492OLIVA, ErnestoErnestoOLIVA0000-0002-6040-5849BRAGAGLIA, AngelaAngelaBRAGAGLIA0000-0002-0474-0896FRASCA, AntonioAntonioFRASCA0000-0002-0338-7883SANNA, NicolettaNicolettaSANNA0000-0003-4486-6802BIAZZO, KatiaKatiaBIAZZO0000-0002-1892-2180Casali, G.G.Casali0000-0002-9123-0412DESIDERA, SilvanoSilvanoDESIDERA0000-0002-2662-3762LUCATELLO, SaraSaraLUCATELLO0000-0001-8808-0073MAGRINI, LAURALAURAMAGRINI0000-0001-8613-2589ORIGLIA, LiviaLiviaORIGLIA2021-11-162021-11-162020http://hdl.handle.net/20.500.12386/31088GIARPS (the simultaneous observing mode of the spectrographers GIANO and HARPS-N) at the 3.6m telescope TNG was used to target ten solar-type dwarfs in the Praesepe cluster (Table 1). Observations were carried out between December 2018 and January 2019. <P />The instrument configuration allows us to operate with the HARPS-N spectrograph (R=115000, λλ=3800-6900Å), and the GIANO-B near-infrared (NIR) spectrograph (R=50000, 0.97-2.5um). <P />Equivalent width for different species measured in 10 solar-type stars in Praesepe (table2.dat). <P />Stellar parameters and abundances is found in the table stars.dat (table 1 and 5 of the paper). <P />(2 data files).enDatabase10.26093/cds/vizier.36330038https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/633/A382020yCat..36330038DFIS/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