Several loggf values were modified to better fit high resolution observed stellar spectra with synthetic spectra. The used stars with references can be seen at STARS Cr II the modified lines Mn II the modified lines Mn III the modified lines Fe II the modified lines Ga I (31.00) both old (Kurucz) and modified lines from NIST Ga II (31.01) both modified and added lines Ga III (31.02) Added ion Ge II (32.01) both old (Kurucz) and modified lines from NIST As II (33.01) Added ion Y III (39.02) Added ion Zr II (40.01) both old (Kurucz) and modified loggf values Zr III (40.02) Added ion ( Ru II (44.01) both modified and added lines)-- On 28 Sept. 2017 this file was replaced in the linelist by gf4401.all from Kurucz ( Rh II (45.01) both modified and added lines)-- On 23 Sept. 2017 this file was replaced in the linelist by gf4501.all from Kurucz Pd II (46.01) the Kurucz file was replaced Ag II (47.01) all the lines are from NIST Cd II (48.01) both modified and added lines. In II (49.01) is the Kurucz file with a few modified loggf values. This linelist has still to be updated. Sn II (50.01) modified and added lines from 1250 to 3000 A. Xe I (54.00) Added ion: there are only three lines from NIST Xe II (54.01) Added ion Ce II (58.01) is the Kurucz file with modified loggf values from 3800 to 6900 A Ce III (58.02) Added ion Pr II (59.01) is the Kurucz file with modified loggf values from 3800 to 6200 A Pr III (59.02) Added ion for the optical region Nd II (60.01) is the Kurucz file with modified loggf values from 3800 to 6400 A Nd III (60.02) Added ion for the optical region Sm II (62.01) is the Kurucz file with modified loggf values from 3800 to 6400 A Eu III (63.02) Added ion Gd II (64.01) is the Kurucz file with modified loggf values from 3800 to 6900 A Tb II (65.01) is the Kurucz file with modified loggf values Tb III (65.02) Added ion Dy II (66.01) is the Kurucz file with modified loggf values from 3800 to 5700 A Dy III (66.02) Added ion Ho II (67.01) is the Kurucz file with modified loggf values Ho III (67.02) Added ion Er II (68.01) is the Kurucz file with modified loggf values from 3800 to 5900 A Er III (68.02) Added ion Tm II (69.01) is the Kurucz file with modified loggf values from 3040 to 5900 A Tm III (69.02) Added ion Yb II (70.01) is the Kurucz file with a few modified (from NIST) loggf values Yb III (70.02) added ion Os II (76.01) both modified and added lines Ir II (77.01) both modified and added lines Pt II (78.01) Added ion Pt III (78.02) Added ion Au II (79.01) Added ion Au III (79.02) Added ion Hg I (80.00) both modified (from NIST) and added lines Hg II (80.01) both modified (from NIST) and added lines Hg III (80.02) Added ion Tl II (81.01) Added ion Bi II (83.01) Added ion Th II (90.01) is the Kurucz file with some modified loggf values from 3900 to 6900 A Th III (90.02) Added ion We used the STIS-HST ultraviolet spectra of HD 175640 and HR 6000 to estimate the loggf changes for Mn II and Mn III. For several Cr II and Fe II lines the Kurucz log gf values were replaced by the Raassen and Uylings data (RU).