# version of 2009 Jun 10, improve line precision so that 
# set line precision 6 can be used
# version of 2003 oct 27, cleaned up some lines whose wl had changed
#
# for information on the format of this file, see readme_LineList_dat.txt
# this is the standard list list, appropriate for dense gas like the BLR,
# which will use used if no name appears
#
# Begin CLOUDY grid output line list...
# 2 X-ray lines:
FeKa     1.78       Iron K-alpha line (near 6.4 keV)
o  8    18.9732     O VIII 19A H-like Lya
#
# UV lines: lambda > 600 Angstroms
mg10   609.793A     total Mg X 610
#inwd  609.793A     inward flux of Mg X 610
mg10   624.941A     total Mg X 625
#inwd  624.941A     inward flux of Mg X 625
totl   615     total of sum of both Mg X components
o  5   629.7A     total O V 630
s  4   655.072A     total S IV 655; level 2 line
n  3   678.210A     total N III 679; level 2 line
o  3   698.231     total O III 703; level 2 line
s  4   737.3     total S IV 737; level 2 line
n  3   752.112     total N III 764; level 2 line
n  4   765.1     total N IV 765
ne 8   770.404     total Ne VIII 770
ne 8   780.324     total Ne VIII 780
totl   774     total of sum of both Ne VIII component
#inwd   774     inward flux of sum of both Ne VIII components
s  5   786.473     total S V 786
o  4   789.4     total O IV 789
#inwd   789.4     inward flux of O IV 789
s  4   798.831     total S IV 799
O  2   833.802     total O II 834A
o  3   834.5     total O III 834
totl   895     total Ne VII] 895
s  6   933.378     total S VI 933
s  6   944.523     total S VI 944
p  4   950.661     total P IV 951; level 2 line
h  1   972.543     total Lyman-gamma 973
#inwd   972.543     inward flux of Lyman-gamma 973
c  3   977     total C III 977
#inwd   977     inward flux of C III 977
n  3   991     total N III 990
#inwd   991     inward flux of N III 990
h  1  1025.73     total Lyman-beta 1025
#inwd  1025.73     inward flux of Lyman-beta 1025
o  6  1031.93     total O VI 1032
o  6  1037.62     total O VI 1037
totl  1035     total of sum of both O VI components
#inwd  1035     inward flux of sum of both O VI components
he 2  1085.03     total He II Balmer-gamma 1085
n  2  1085     total N II 1085
s  4  1086.27     total S IV 1086; level 2 line
p  5  1121.30     total P V 1121; level 2 line
fe 3  1125.79     total Fe III 1122
ne 5  1141     total Ne V 1141
c  3  1176     total C III* 1176 (excited state)
#inwd  1176     inward flux of C III* 1176
s  3  1197.56     total S III 1198
totl  1198     total S V 1198
si 3  1207     total Si III 1207
inci  1215     incident continuum at 1215 Angstroms in units of nuF(nu)
H  1  1215.68     total Hydrogen Lyman-alpha 1215.67 
inwd  1215.68     inward flux of Lyman-alpha
he 2  1215.23     total He II Balmer-beta 1216
#inwd  1215.23     inward flux of He II Balmer-beta 1216
totl  1218     total of sum of O V] 1218 + [O V] 1218
#inwd  1218     inward flux of O V]
n  5  1239     total N V 1238.82
n  5  1243     total N V 1242.80
totl  1240     total of sum of both N V components
#inwd  1240     inward flux of sum of both N V components
s  2  1256     total S II 1256
si 2  1263.32     total Si II 1260 + 1263
6lev  1304     total O I 1302 + 1305  
si 2  1307.66     total Si II 1308
c  2  1335     total C II 1335 + 1336
si 4  1394     total Si IV 1394
si 4  1403     total Si IV 1403
totl  1397     total of sum of both Si IV components
#inwd  1397     inward flux of sum of both Si IV components
totl  1402     total O IV] 1402; 5 components to line: 
#
# 1397.2, 1399.77, 1401.16, 1404.81, 1407.39 --- not computed individually
#inwd  1402    inward flux of O IV]
totl  1406     total S IV 1406
totl  1486     total of sum of N IV] 1486 + [N IV]
N  4  1485     most forbidden of the pair
#N  4 1486      stonger of the pair, at high density this will be the same as total	
#inwd  1488     inward flux of N IV]
si 2  1531     total Si II 1527 + 1533
c  4  1548     total C IV 1548.19
c  4  1551     total C IV 1550.77
totl  1549     total of sum of both C IV components
inwd  1549     inward flux of sum of both C IV components
he 2  1640     total He II Balmer-alpha 1640
inwd  1640     inward flux of He II Balmer-alpha 1640
o  3  1661     total O III] 1661
#inwd  1661     inward flux of O III] 1661
o  3  1666     total O III] 1666
#inwd  1666     inward flux of O III] 1666
totl  1665     total of sum of both O III] components
al 2  1670.79     total Al II 1670.8; level 2 line
s  3  1720     total S III 1720
totl  1750     total N III] 1750 (all components; not computed seperately)
#inwd  1750     inward flux of N III]
fe 2  1786     total Fe II 1787 (probably selectively excited)
si 2  1813.99     total Si II 1814 (1808.0 + 1816.9 + 1817.5)
al 3  1855     total Al III 1855
al 3  1863     total Al III 1863
totl  1860     total sum of both Al III components
#inwd  1860     inward flux of sum of both Al III components
totl  1888     total of sum of Si III] 1892 + [Si III]
Si 3  1883     the most forbidden of the doublet
#inwd  1892     inward flux of Si III] 1892
totl  1909     total of sum of C III] 1908.73 + [C III]
#inwd  1910     inward flux of C III] 1908.73
n  2  2141     total sum of N II] 2139.01, 2142.77
o  3  2321     single line from 5-level atom
totl  2326     total C II] 2324.69 + 2328.12
totl  2335     total Si II] 2335
totl  2665     total of sum of Al II] 2669 + [Al II] 2660
al 2  2660     emission from most forbidden line of multiplet
mg 2  2795.53     total Mg II 2796 of the doublet
mg 2  2802.71     total Mg II 2803 of the doublet
totl  2798     total of sum of both Mg II components
inwd  2798     inward flux of sum of both Mg II components
#
# optical emission lines and continua
he 2  3203.30     total He II Paschen-beta line
BA C     0     total of integrated H balmer continuum
BaC   3646     total nuFnu of Balmer jump at 3646 (the head)
#h  1  3835     total H-7 (H-Balmer)
He 1  3888.63     total H-6 (H-Balmer)
ca2k  3934     total Ca II 3934 emission
ca2h  3969     total Ca II 3969 emission
#h  1  3970     total H-epsilon
h  1  4101.76     total H-delta
#inwd  4101.76     inward flux of H-delta
h  1  4340.49     total H-gamma
#inwd  4340.49     inward flux of H-gamma
ca b  4471.49     total He I 4471, case B approximation
he 2  4686.01     total He II 4686 (Paschen-alpha)
inwd  4686.01     inward flux of He II 4686
H  1  4861.36     total H-beta 4861
inwd  4861.36     inward flux of H-beta 4861
He 1  5875.61     total He I 5876
#inwd  5875.61     inward flux of He I 5876
na 1  5891.94     total Na ID 5892
h  1  6562.85     total H-alpha 6563
#inwd  6562.85     inward flux of H-alpha 6563
#
# near IR emission lines and continua
k  1  7676.23     total K I 7745
6lev  8446     total O I 8446
ca2x  8498     total Ca II 8498
ca2y  8542     total Ca II 8542
ca2z  8662     total Ca II 8662
PA C     0     total of integrated H Paschen continuum
totl 10829.9     total He I 10,830A, all three lines within multiplet
h  1   1.87511m    total H Paschen-alpha
#
# The following 11 "lines" represent emission by a "6-level" Fe II atom
# of Hamann & Ferland, a modification of the Wills, Netzer, and Wills.
# See HAZY for some details.
fe 2  6200
fe 2  4300
fe 2  2400
fe 2  1080
fe 2  1500     
fe 2 11500
fe 2  2500
fe 2  2300
fe 2  8900
fe 2  1216     pumping of the Fe II atom via H Lya 1216
fe2c     0     cooling from the Fe II atom
#
# Some high critical density forbidden lines
ne 5  3426     total [Ne V] 3426
ne 3  3869     total [Ne III] 3869
totl  4363     total [O III] 4363
o  3  5007     total [O III] 5007
Fe14  5303     total [Fe XIV] 5303
o  1  5577     total [O I] 5577
Fe 7  6087     total [Fe VII] 6087
o  1  6300     total [O I] 6300
Fe10  6375     total [Fe X] 6375
Fe11  7892.30     total [Fe XI] 7892
#
# an optical incident continuum bin in units of nuFnu
inci  4860     incident continuum at 4860 Angstroms in units of nuF(nu)
#
# The following are the total non-line emission from the cloud 
# (diffuse + reflected continuum) at a given wavelength in Angstroms.
# All have units of nuF(nu).
nFnu 122.4m  microns 
#
nFnu  8329.68   A
nFnu  8078.61 
nFnu  6209.66 
nFnu  4885.36
nFnu  3704.34
nFnu  3587.67 
nFnu  2392.03
nFnu  2071.34
nFnu  2052.68 
nFnu  1793.44
nFnu  1585.12
#
# In optically thick clouds of significant H I columns, Lya "Rayleigh
# scattering" of incident continuum becomes important beginning here and
# extending down to the Lyman limit.
#
nFnu  1458.33
nFnu  1356.96  
nFnu  1297.29
nFnu  1262.79  
nFnu  1218.08
nFnu  1196.33
nFnu  1175.06
nFnu  1143.64  
nFnu  1113.22
nFnu  1103.23
nFnu  1073.86  
nFnu  1064.34
nFnu  1035.92  
nFnu  1000
nFnu   925.144
nFnu   897.8  
nFnu   760.023
nFnu   701.514  
nFnu   608.160
nFnu   575.146
nFnu   511.948  
nFnu   496.874  
nFnu   399.153
#
# The following are the inward directed non-line emission from the cloud 
# (diffuse + reflected continuum) at a given wavelength in Angstroms.
# All have units of nuF(nu).
#
#InwT 1.119m
#InwT  8220
#InwT  8205
#InwT  6209
#InwT  4885
#InwT  3649
#InwT  3644
#InwT  2392
#InwT  2071
#InwT  2052
#InwT  1793
#InwT  1585
#InwT  1458
#InwT  1356
#InwT  1297
#InwT  1262
#InwT  1218
#InwT  1196
#InwT  1175
#InwT  1143
#InwT  1113
#InwT  1103
#InwT  1073
#InwT  1064
#InwT  1035
#InwT  1000
#InwT   897.8
#InwT   925.1
#InwT   760
#InwT   701.5
#InwT   608.2
#InwT   575.1
#InwT   399.2
#
# lines from he-like ions
#>>chng 06 aug 17, mean wl of multiplet now used
TOTL  5484.32A Li 2
TOTL  3721.72A Be 3
TOTL  2824.03A B  4
TOTL  2275.25A C  5
TOTL  1903.86A N  6
TOTL  1633.92A O  7
TOTL  1408.98A F  8
TOTL  1266.26A Ne 9
TOTL  1134.43A Na 10
TOTL  1025.02A Mg 11
# end dense line list
# the file ends with the end of file, or a cr in the first col

