ATOMS


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).