NOTES06.C TT0600WVL.DAT = BELL0600.DATT 7852 lines. A# = Laboratory intensity given in revised C 1 multiplet table, Moore (1970) NEW LINES, with mult # and lab obs'n 5040.752 0 -2.60 3.0 64086.920 83919.710 6.00 s2p3 3D 4f [5] 7.95 5040.735 S' 0.9 ?? C 18.01 P 5041.481 0 -2.00 1.0 64089.850 2.0 83919.760 6.00 s2p3 3D 4f [5] 7.95 5041.4455S -0.0355/S' 7.3 -C 1 18.01 A6 5041.796 0 -2.50 2.0 64090.950 3.0 83919.650 6.00 s2p3 3D 4f [5] 7.95 41.76 masked s' 27.7 FE(C 18.01 A6 5040.134 0 -2.50 2.0 64090.950 3.0 83926.220 6.00 s2p3 3D 4f [7] 7.95 5040.122 S' 1.4 C 1 18.01 A4 5017.090 0 -2.50 3.0 64086.920 84013. 6.00 s2p3 3D 4f'[5] 7.95 5017.045 C2 tt> tr 6631.809 10747 -0.548 2.5 32436.778 3.5 47511.458 13.00 3d 2D 12f 2F 4.02 31.773 T>> 0.2 ATM? 6631.809 10746 -1.849 2.5 32436.778 2.5 47511.458 13.00 3d 2D 12f 2F 4.02 masked/t 6696.185 10858 -1.576 1.5 32435.435 2.5 47365.189 13.00 3d 2D 11f 2F 4.02 masked/T 6696.788 10860 -1.421 2.5 32436.778 3.5 47365.189 13.00 3d 2D 11f 2F 4.02 n.o.? T=> tr 6696.788 10859 -2.722 2.5 32436.778 2.5 47365.189 13.00 3d 2D 11f 2F 4.02 -t 8p 2P and higher np terms not given by Martin & Zalubas (l979); high terms in general are listed to 3 decimal places, while M & Z give one or none. 1984 jun 17, B.Bell KP1301NUW.DAT = BELL1301.DAL ENS from C.W.Martin & R.Zalubas, 1979, J.Phys.& Chem.Ref.Data 8, 826-31, updated from E.Biemont & J.W.Brault, 1987, Physica Scripta 35, 286-295, THE SPECTRUM OF AL I AND AL II IN THE INFRARED; gf's from BW, NBS, WEI, & KP 3184 lines; 1 in Rev2 3900.66 A BW B.Warner, 1968, MN 140, 53-59, (theoretical) WEI A.W.Weiss, 1974, Phys.Rev.A 2, 1524-36, (theoretical). KP1302NUW.DAT = BELL1302.DAL ENS from C.W.Martin & R.Zalubas, 1979, J.Phys.& Chem.Ref.Data 8, 832-33; unchanged from KP1302.DAT. 372 lines KP1303 ENS from C.W.Martin & R.Zalubas, 1979, J.Phys.& Chem.Ref.Data 8, 834-37. KP1304NUW.DAT = BELL1304.DAL ENS from C.W.Martin & R.Zalubas, 1979, J.Phys.& Chem.Ref.Data 8, 838-42. 94 lines KP1305 ENS from C.W.Martin & R.Zalubas, 1979, J.Phys.& Chem.Ref.Data 8, 843-46 (3d,4d); 3d updated from M.C.Artru & V.Kaufman, 1980, J.Opt.Soc.Am. 70, 1130-35; (5d from AEL I, 1949 removed but saved as KP1305UPN.QQ) KP1401NUW.ENC = ENS from SHENSTONE (1961), updated from W.C.MARTIN & R.ZALUBAS, 1983, J.PHYS.& CHEM.REF.DATA 12, 342-46, SiII. KP1402NUW.ENC = BELL1402.DAL ENS from W.C.MARTIN & R.ZALUBAS, 1983, J.PHYS.& CHEM.REF.DATA 12, 347-52, SiIII. 1535 lines; log gf = BBCB, BW, KP, NBS, TZ. KP1403NUW.ENC = BELL1403.DAL ENS from W.C.MARTIN & R.ZALUBAS, 1983, J.PHYS.& CHEM.REF.DATA 12, 353--54, SiIV. 326 lines; log gf = KP. KP1404NUW.ENC = BELL1404.DAL ENS from W.C.MARTIN & R.ZALUBAS, 1983, J.PHYS.& CHEM.REF.DATA 12, 355-58, Si V. (incomplete, 3p, nd, nf) 134 lines; log gf = GL, GLBD, KP, NBS. KP1405NUW.ENC = BELL1405.DAL AEL ENS updated from W.C.MARTIN & R.ZALUBAS, 1983, J.PHYS.& CHEM. REF.DATA 12, 359-61, Si VI. 52 lines; log gf = KP, GLBD. MAR 88 NOTES1400.DAT Si 1: Significant CHANGES in upper energy levels Identif. old upn new upn Moore Brown et al. M & Z 6d 3D 2.0 62874.48 62774.99 +len * 6d 3P 2.0 62921.08? 63020.42 +len * 9s 3P 0.0 63579.44 63576.85 7d 3D 2.0 63714.40 63575.35 ** 7d 3P 2.0 63721.53 63770.28 7d 3P 1.0 63770.28 63844.65 7d 3P 0.0 63844.64 63863.80 8d 1P 1.0 64018.31 64020.42 10s 3P 1.0 64086.37 64085.87 8d 3D 2.0 64252.08? 64104.88 ** 8d 3P 0.0 64322.69 64358.52 10s 1P 1.0 64351.86 64376.18 9d 3F 4.0 64551.37 64550.37 L&W, M&Z 9d 3P 2.0 64616.74 64687.77 * 2PD N=9 10d 3P 2.0 84882.80 64916.64 * New values inserted, wavelengths recalculated by NEWWAVE; MERGPIERY rerun to fish for solar lines. l984 Jun B.Bell NEW LINES ADDED, OCT 84 4839.858 0 -2.50 1.0 40991.884 2.0 61647.875 14.00 p4s 1P 5f'[3] 5.08 39.884 Y-t T' 2.5 Y1(Si 17.12 A11 4851.539 0 -2.20 1.0 40991.884 2.0 61598.145 14.00 p4s 1P 5f'[5] 5.08 51.496 masked T' 6.8 V1(Si 17.11 A13 4551.812 0 -3.50 1.0 40991.884 2.0 62955.000 14.00 p4s 1P 6f'[5] 5.08 51.848 T' 0.2 V?(Si 17.19 A7 5128.034 0 -2.60 1.0 40991.884 1.0 60487.103 14.00 p4s 1P 6p 3D 5.08 28.0784S masked? T' 3.3 C2,NI 17.05A10 4921.727 0 -3.00 1.0 40991.884 2.0 61304.283 14.00 p4s 1P 5f [5] 5.08 21.785 masked T' 8.1 TI(Si 17.10 A1 5621.608 0 -2.50 1.0 40991.884 2.0 58775.451 14.00 p4s 1P 4f [5] 5.08 5621.6064S -0.0006 S 2.0 Si 17.01 A15 9464.767 0 -2.50 3.0 49933.755 2.0 60496.358 14.00 p3d 3F 6p 3D 6.19 64.83 t' 53 ATM 74.06 A4 6719.609 0 -2.50 4.0 50054.800 5.0 64932.510 14.00 p3d 3F 10f 3G 6.21 6719.62 s,N t' 3.1 Si 1 L&W 7012.612 0 -2.50 4.0 50054.800 5.0 64310.890 14.00 p3d 3F 9f 3G 6.21 6838.85 w t' 4.5 FE;Si 1 L&W NOTES1401.DAT TT1401: Twvl > SOLAR wvl e.g. 6347, 6371 A, 5978.9, 5957.5 A number of listed transitions correspond to no observed multiplet; also the following multiplets/transifitons observed in the Lab are not in the file. JUN-1984, B.BELL transition E.P. Multiplet Number 14.01 s3p2 2D 3p3 2P 6.8 UV 13.06 2 lines * 14.01 s3p2 2D 3p3 2D 6.8 uv 13.05 2 lines ** 14.01 s3p2 2D 10p 2P 6.8 uv 13.03 14.01 s3p2 2D 9p 2P 6.8 uv 13.01 14.01 s3p2 2D 8f 2F 6.8 uv 13 14.01 s3p2 2D 8p 2P 6.8 uv 12.02 14.01 s3p2 2D 7f 2F 6.8 UV 12 * 14.01 s3p2 2D 4s 2P 6.8 UV 11.01 ** 14.01 s3p2 2D 6f 2F 6.8 UV 11 * 14.01 s3p2 2D 7p 2P 6.8 UV 10.02 14.01 s3p2 2D 6p 2P 6.8 UV 10.01 14.01 s3p2 2D 5f 2F 6.8 UV 10 14.01 s3p2 2D 3d 2D 6.8 UV 9.02 14.01 s3p2 2D 5p 2P 6.8 uv 9.01 14.01 s3p2 2S 3p3 2P 9.5 uv 15.04 ** 2 lines 14.01 3d 2D 4d' 2D 9.8 uv 18.06 14.01 3d 2D 3p3 2D 9.8 uv 18.05 14.01 3d 2D 3d' 2F 9.8 uv 18.04 ** 14.01 3d 2D 3d' 2F 9.8 uv 18.04 ** 14.01 3d 2D 4s' 2P 9.8 uv 18.01 3 lines 14.01 3d 2D 3d' 4F 9.8 uv 17.02 3 weak lines 14.01 s3p2 2P 3p3 2P 10.4 uv 28 14.01 s3p2 2P 3p3 2D 10.4 uv 27 ** 14.01 s3p2 2P 8p 2P 10.4 uv 26 14.01 s3p2 2P 7p 2P 10.4 uv 24 14.01 5s 2S 4s' 2P 12.1 uv 7.01 14.01 4d 2D 3d' 2F 12.5 7.10 14.01 4d 2D 4s' 2P 12.5 7.04 14.01 5p 2P sp4p 2P 12.8 7.25 14.01 sp3d 2D 4f' 4F 13.4 uv 33 14.01 sp3d 2D sp4p 2D 13.4 7.27 14.01 sp3d 2D sp4p 2D 13.4 7.26 14.01 sp3d 4F 4f' 2G 14.1 uv 36 14.01 sp3d 4F sp4p 4D 14.1 7.33 *** strong lab lines 14.01 sp4s 4P sp4p 4D 14.5 7.34 ** 14.01 sp4s 4P sp4p 4P 14.5 8 ** 14.01 sp4s 4P sp4p 4S 14.5 9 ** 14.01 4s' 2P sp4p 2S 15.0 11 14.01 3d' 4D 4f' 2F 15.4 12 * 14.01 3d' 4P 4f' 4F 15.4 16 * 14.01 3d' 4P 4f' 2F 15.4 15 * 14.01 8f 2F 4f' 4G 15.4 18 14.01 3d' 2F 4f' 4G 16.3 19 14.01 sp4p 4D 5d' 4F ? 16.3 26 14.01 sp4p 4D 4d' 4P 16.3 25 14.01 sp4p 4D 4d' 4D 16.3 24 * 14.01 sp4p 4D 4d' 4F 16.3 23 *** 14.01 sp4p 4D 5s' 4P 16.3 22 * 14.01 sp4p 2P 4d' 2P 16.4 28 14.01 sp4p 2P 4d' 2D 16.4 27 * 14.01 sp4p 4P 4d' 4P 16.6 31 * 14.01 sp4p 4P 4d' 4D 16.6 30 ** 14.01 sp4p 4P 5s' 4P 16.6 29 * 14.01 sp4p 4S 4d' 4P 16.7 32 ** 14.01 3p3 2D 4f' 2F ? 16.7 33 14.01 3p3 2D 4f' 4F 16.7 34 ADDED, DEC 84 - JAN 85 The minor adjustments in energy levels indicated by M&Z do not change wavelengths of Si 2. NEEDS RECALCULATION OF LOG gfs for new lines. NOTES1500.DAT KP1500 MARTIN (1959) found a number of unidenifiable P 1 lines in the infrared and wrote "It was a disappointment not to find more 4f and 5f terms. A strong exposure beyond 10,000A is needed to obtain transitions from 5f levels to the knon term 3d 4D. The finding of these levels should then allow the completion of the 3d and 5f quartets, since many of the unclassified lines in the region 8000-8400A must belong to the multiplets 3d 4F - 5f 4(DFG)o." Problems resolved by SVENDENIUS, Nils, (l980) Physica Scripta 22, 240-287, THE SPECTRUM AND TERM ANALYSIS OF NEUTRAL PHOSPHORUS, P I. (1800 P I Transitions measured and classified, giving a total of 282 energy levels, about 180 of which are new; source for AEL1500.DAT, and revision of KP1500.DAT (and many new lines added thereto). MOST NEW LINES lacking GF; assigned gf = ES, estimated from lab intensities (in general correlation betwwen log gf and lab intensities appears poor). TYPOS in published energy levels: term publ=NS=MZM should be (publ values give wrong WVLs) 3.5 4p 4D 65788.455 65787.455 1.5 5p 4D 75351.512 75353.512 1219 lines; log gf ? KP1501NUW.ENC = BELL1501.DAL ENS updaed from W.C.Martin, R.Zalubas, & A.Musgrove, 1985, J.Phys.& Chem.Ref.Data 14, 762-67, (primarily from SVENDENIUS, Nils, C.E.Magnusson, & P.O.Zetterberg (l983) Physica Scripta 27, 339-363, THE SPECTRUM OF SINGLY IONIZED PHOSPHORUS, P II. (900 P II lines, 500-12,000A, measured and classified, giving a total of 159 energy levels, updating Martin(l959). Major changes 129626.000 p5p 3P 1.0 to 5p 3P 1.0 130173.43 130174.300 p5p 3P 2.0 to 130399.78 139410.200 p5d 1D 2.0 to 5d 1D 2.0 139212.72 and 5d 3D 2.0 139622.67 (log gf = GUES) 141958.40 p5d 1P 1.0 to 5d 1P 1.0 141487.87 ADJUSTMENTS GIVE SOME NEW LINES WITH OLD GFs; (in general correlation betwwen log gf and lab intensities appears poor). 1066 lines, log gf from KP, MRB, NBS, SMTH (& GUES) MRB=M.H.Miller, R.A, Roig, and R.D. Bengtson. 1971, Phys. Rev. A, 1709-1722. KP1502NUW.ENC = BELL1502.DAL ENS from W.C.Martin, R.Zalubas, & A.Musgrove, 1985, J.Phys.& Chem.Ref.Data 14, 768-771; log gf KP, LKI, NBS; 163 lines. KP1503NUW.ENC = BELL1503.DAL ENS in accord with W.C.Martin, R.Zalubas, & A.Musgrove, 1985, J.Phys.& Chem.Ref. Data 14, 772-777; log gf BW, KP, NBS; KP1504NUW.ENC = BELL1504.DAL ENS updated from W.C.Martin, R.Zalubas, & A.Musgrove, 1985, J.Phys.& Chem.Ref. Data 14, 778-79; log gf KP; 221 lines. KP1505NUW.ENC = BELL1505.DAL ENS updated from W.C.Martin, R.Zalubas, & A.Musgrove, 1985, J.Phys.& Chem.Ref. Data 14, 780-82; log gf KP, NBS; 9 lines. JUNE 88 B.BELL NOTES16.S KP1600NUW.ENC = BELL1600.DAL ENS from NBS preprint (APR 1985), based primarily on Kaufman 1982 & (WVL 1157-2169A) & Jakobsson 1966 (WVL 9212-34270A); nd 5D levels not adequately resolved for n >4, calculated from solar wvl's (KP1600UPN.5D): j 4d 5d 6d 7d 8d 4.0 74973.25 78270.06 79992.10 80995.30 81628.70 3.0 74974.17 78270.42 79992.35 80995.35 81628.75 2.0 74975.22 78270.76 79992.45 80995.40 81628.80 1.0 74976.14 78271.00 79992.55 0.0 74976.68 78271.20 79992.60 log gf from KP, NBS, & LW (6,7,8d) 834 lines, 128 solar (KP1600SUN.SUN) SEP 88 KP1600NUW.DALENC = BELL1600.DAL ENS further updated from W.C.Martin, R.Zalubas, & A.Musgrove, 1990, ENERGY LEVELS OF SULFUR, S I... preprint (nd 5D levels remain inadequately resolved); log gf from KP, NBS, & LW (6,7,8d), FOS, GUES. PUNCHL900,...950.SRT 16.00 revised in wvl, GUES gf's to solar j 4d 5d 6d 7d 8d 4.0 74973.14 78270.10 79992.15 80995.28 81628.70 3.0 74974.10 78270.52 79992.32 80995.35* 81628.75* 2.0 74975.19 78270.99 79992.50 80995.40* 81628.80* 1.0 74976.06 78271.09* 79992.55* * not in table 0.0 74976.61 78271.09* 79992.60* also * 4s' 3dD 76842.867 old BELL1600.DAL has damping from NBS; BELL1600.DALA has solar data, no damping. JAN 90 KP1601NUW.ENC = BELL1601.DAL ENS from AEL updated from J.E.Pettersson, 1983, Physica Scripta 28, 421-434 (involving major energy changes for 5p et al, given log gf GUES); log gf BSMB, BW, KP, MWRB, NBS, & GUES; 742 lines. ESP NEEDS RECALCULATION KP1602NUW.ENC = BELL1602.DAL ENS from AEL; log gf KP, BSMS, FIX, NORM, NBS; 191 lines. KP1603NUW.ENC = BELL1603.DAL ENS from AEL (except quartets, from ??, updated from Kelly (1987); log gf KP, IL; 75 lines. KP1604NUW.ENC = BELL1604.DAL ENS from AEL updated from I.Joelsson, P.O.Zetterberg & C.E.Magnusson, 1981 Physica Scripta 23, 1087-95; log gf KP, NBS; 41 lines. KP1605NUW.ENC = BELL1605.DAL ENS from AEL updated from I.Joelsson, P.O.Zetterberg, & C.E.Magnusson, 1979, Physica Scripta 20, 145-150; log gf KP; 152 lines. JULY 88 * * * * * * * UPN 4d 5D OLD, differing from values in other appearances of 4d 5D: 8670.281 252 -0.880 1.0 63445.115 0.0 74975.600 16.00 4p 5P 4d 5D 7.87 8670.20 -0.081 t = 0.9 S 1 6 A1 8670.724 253 -0.530 1.0 63445.115 1.0 74975.010 16.00 4p 5P 4d 5D 7.87 8670.6090S -0.1150 T>= 1.4 S 1 6 A2 8671.386 254 -0.640 1.0 63445.115 2.0 74974.130 16.00 4p 5P 4d 5D 7.87 8671.308 -0.193 T = 0.7 S 1 6 A1 8679.063 255 -1.000 2.0 63456.192 1.0 74975.010 16.00 4p 5P 4d 5D 7.87 8678.9346S -0.1284 t=< 0.9 S 1 6 A1 8679.726 256 -0.410 2.0 63456.192 2.0 74974.130 16.00 4p 5P 4d 5D 7.87 8679.646 -0.08bl T < 4.7 FEp/S 6 A2 8680.577 257 -0.210 2.0 63456.192 3.0 74973.000 16.00 4p 5P 4d 5D 7.87 8670.4182S -0.1588 T>= 2.9 S 1 6 A8 8693.243 258 -1.370 3.0 63474.101 2.0 74974.130 16.00 4p 5P 4d 5D 7.87 8693.15 -0.093 t = 0.4 S 1 6 A1 8694.097 259 -0.510 3.0 63474.101 3.0 74973.000 16.00 4p 5P 4d 5D 7.87 8693.9437S -0.1533 T>= 2.0 S 1 6 A3 8694.815 260 0.080 3.0 63474.101 4.0 74972.050 16.00 4p 5P 4d 5D 7.87 8694.6444S -0.1706 T>= 3.9 S 1 6 A10 Changed to UPNs in accord with other appearances of 4d 5D, giving less discordant wavelengths: 8670.130 0252 -0.880 1.0 63445.115 0.0 74975.800 16.00 4p 5P 4d 5D 7.87 8670.20 0.070 t = 0.9 S 1 6 A1 8670.574 0253 -0.530 1.0 63445.115 1.0 74975.210 16.00 4p 5P 4d 5D 7.87 8670.6090S 0.0350 T>= 1.4 S 1 6 A2 8671.236 0254 -0.640 1.0 63445.115 2.0 74974.330 16.00 4p 5P 4d 5D 7.87 8671.308 0.072 T = 0.7 S 1 6 A1 8678.912 0255 -1.000 2.0 63456.192 1.0 74975.210 16.00 4p 5P 4d 5D 7.87 8678.9346S 0.0226 t=< 0.9 S 1 6 A1 8679.575 0256 -0.410 2.0 63456.192 2.0 74974.330 16.00 4p 5P 4d 5D 7.87 8679.646 0.07bl T < 4.7 FEp/S 6 A2 8680.426 0257 -0.210 2.0 63456.192 3.0 74973.200 16.00 4p 5P 4d 5D 7.87 8670.4182S -0.0078 T>= 2.9 S 1 6 A8 8693.091 0258 -1.370 3.0 63474.101 2.0 74974.330 16.00 4p 5P 4d 5D 7.87 8693.15 0.059 t = 0.4 S 1 6 A1 8693.946 0259 -0.510 3.0 63474.101 3.0 74973.200 16.00 4p 5P 4d 5D 7.87 8693.9437S -0.0023 T>= 2.0 S 1 6 A3 8694.664 0260 0.080 3.0 63474.101 4.0 74972.250 16.00 4p 5P 4d 5D 7.87 8694.6444S -0.0196 T>= 3.9 S 1 6 A10 See KP16004D.5D NOV 84 ENS MARTIN ET AL 1990 8670.235 252 -0.880 1.0 63446.065 0.0 74976.610 16.00 4p 5P 4d 5D 7.87 8670.20 -0.035 t = 0.9 S 1 6 A1 8670.649 253 -0.530 1.0 63446.065 1.0 74976.060 16.00 4p 5P 4d 5D 7.87 8670.6090S -0.0400 T>= 1.4 S 1 6 A2 8671.303 254 -0.640 1.0 63446.065 2.0 74975.190 16.00 4p 5P 4d 5D 7.87 8671.308 0.005 T = 0.7 S 1 6 A1 8678.987 255 -1.000 2.0 63457.142 1.0 74976.060 16.00 4p 5P 4d 5D 7.87 8678.9346S -0.0524 t=< 0.9 S 1 6 A1 8679.643 256 -0.410 2.0 63457.142 2.0 74975.190 16.00 4p 5P 4d 5D 7.87 8679.646 -0.00bl T < 4.7 FEp/S 6 A2 8680.464 257 -0.210 2.0 63457.142 3.0 74974.100 16.00 4p 5P 4d 5D 7.87 8670.4182S -0.0458 T>= 2.9 S 1 6 A8 8693.159 258 -1.370 3.0 63475.051 2.0 74975.190 16.00 4p 5P 4d 5D 7.87 8693.15 -0.009 t = 0.4 S 1 6 A1 8693.983 259 -0.510 3.0 63475.051 3.0 74974.100 16.00 4p 5P 4d 5D 7.87 8693.9437S -0.0402 T>= 2.0 S 1 6 A3 8694.709 260 0.080 3.0 63475.051 4.0 74973.140 16.00 4p 5P 4d 5D 7.87 8694.6444S -0.0646 T>= 3.9 S 1 6 A10 JAN 90 Y.N.Joshi, M.Mazzoni, A.Nencioni, W.H.Parkinson and A.Cantu, 1987, J.Phys.B 20, 1203-13, PHOYOABSORPTION SPECTRUM OF ATOMIC SULPHUR (1220-840A, various series). NOTES17.CL KP1700NUW.DAT = BELL1700.DAL ENS from L.J.Radziemski,jr. & V.Kaufman, 1969, JOSA 59, 424-443; log gf KP; 3491 lines. KP1701NUW.ENC = BELL1701.DAL ENS updated from L.J.Radziemski & V.Kaufman, 1974, JOSA 64, 366-89 (some large changes, some deleted = KP1701ENS.NOT, WVLs recalculated); log gf KP, NBS (no damping data); 1450 lines. KP1702NUW.ENC = BELL1702.DAL ENS from AEL; log gf KP; 720 lines. KP1703WVL.DAT = BELL1703.DAL ENS from AEL; log gf KP, NBS; 134 lines. KP1704WVL.DAT = BELL1704.DAL ENS from AEL; log gf KP; 71 lines JULY 88 NOTES18.AR KP1800NUW.ENC = BELL1800.DAL ENS from AEL, updated from L.Minnhagen, 1973 JOSA 63, 1185-98; log gf KP, NBS, AS, DC, LI, WA; 3555 lines. KP1801NUW.ENC = BELL1801.DAL ENS from L.Minnhagen, 1963, Arkiv f.Fisik, 25, 203-284, updated from G.Norlen, 1973, Physica Scripta 8, 249-68 (Table VII, p.266-7) and L.Minnhagen, 1971, JOSA 61, 1257- 62 (lowest levels); j's energies reversed for nf' and ng' series, except 5f' [3] and 5g' [2] (only one available); log gf KP, GO, L, T; 6982 lines. KP1802NUW.ENC = BELL1802.DAL ENS from AEL (4p" corrected); log gf KP, CDD, NBS, RSS; 1008 lines. KP1803NUW.ENC = BELL1803.DAL ENS from AEL & NBS; log gf KP, NBS; 149 lines. KP1804NUW.ENC ENS from AEL & NBS; log gf AYM, KP; 56 lines. JULY 88 NOTES19.K KP1901NUW.ENC = BELL1901.DAL ENS from AEL updated from C.Corliss & J.Sugar, 1979, J.Phys.Chem.Ref.Data 8, 1126-27, K II; log gf 67 lines. KP1902NUW.ENC = BELL1902.DAL ENS from AEL updated from C.Corliss & J.Sugar, 1979, J.Phys.Chem.Ref.Data 8, 1128, K III; log gf KP; 232 lines. KP1903NUW.ENC = BELL1903.DAL ENS from AEL updated from C.Corliss & J.Sugar, 1979, J.Phys.Chem.Ref.Data 8, 1129, K IV; log gf KP; 65 lines. KP1904NUW.ENC = BELL1904.DAL ENS from AEL updated from C.Corliss & J.Sugar, 1979, J.Phys.Chem.Ref.Data 8, 1130, K V; log gf KP; 126 lines. JULY 88