PANCINO, ELENAELENAPANCINO0000-0002-0845-6171Britavskiy, N.N.Britavskiy0000-0003-0788-5879ROMANO, DonatellaDonatellaROMANO0000-0001-9206-9723Cacciari, C.C.CacciariMucciarelli, A.A.MucciarelliCLEMENTINI, GisellaGisellaCLEMENTINI2020-03-042020-03-042015http://hdl.handle.net/20.500.12386/23108Equivalent widths and atomic data of the absorption lines used in the abundance analysis, for each separate exposure at different phases. <P />Observations of 15 RR Lyrae stars (DR And, X Ari, TW Boo, RZ Cam, RX Cet, U Com, RV CrB, SW CVn, UZ CVn, AE Dra, SZ Gem, VX Her, DH Hya, TU UMa, and RV UMa) and one BL Her star (UY Eri) were carried out with SARG@TNG, operated on the island of La Palma, Spain, during two separate runs in 2009 March and between September and November. <P />Eight stars (SW Aqr, TW Cap, DH Hya, V Ind, SS Leo, V716 Oph, BK Tuc, and UV Vir) were observed with UVES@VLT, between 2009 April and August in service mode. <P />(3 data files). <P />enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/447/24042015yCat..74472404PFIS/05 - ASTRONOMIA E ASTROFISICA