Line identifications
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This lists the contents of blrLineList.dat, the list of emission lines usually predicted for BLR calculations.  

#
# this is the list of lines that will be pulled out of the loc calculations
# and saved as predictions
# it is meant to be edited and viewed by a human
# the selection of lines is appropriate for a dense gas, as in the BLR
#
# the list was trundated 99dec09 so that number of lines, with feii bands 
# included, does not exceed the 256 row limit of Excel
#
# comments can appear anywhere and begin with a # in col 1
#
# data lines do not have a # in col 1, but have the 4-char label
# in 1-4 followed by an integer wavelength
#
# comments can appear after the wavelength
#
# Begin CLOUDY grid output line list...
# 2 X-ray lines:
FeKa 2 Iron K-alpha line (near 6.4 keV)
o 8 19 O VIII 19A H-like Lya
#
# UV lines: lambda > 600 Angstroms
mg10 610 total Mg X 610
#inwd 610 inward flux of Mg X 610
mg10 625 total Mg X 625
#inwd 625 inward flux of Mg X 625
totl 615 total of sum of both Mg X components
o 5 630 total O V 630
s 4 655 total S IV 655; level 2 line
n 3 678 total N III 679; level 2 line
o 3 698 total O III 703; level 2 line
s 4 737 total S IV 737; level 2 line
n 3 752 total N III 764; level 2 line
n 4 765 total N IV 765
ne 8 770 total Ne VIII 770
ne 8 780 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 total S V 786
o 4 789 total O IV 789
#inwd 789 inward flux of O IV 789
s 4 799 total S IV 799
O 2 834 total O II 834A
o 3 835 total O III 834
totl 895 total Ne VII] 895
s 6 933 total S VI 933
s 6 944 total S VI 944
totl 933 total of sum of both S VI components
p 4 951 total P IV 951; level 2 line
h 1 973 total Lyman-gamma 973
#inwd 972 inward flux of Lyman-gamma 973
c 3 977 total C III 977
#inwd 977 inward flux of C III 977
n 3 990 total N III 990
#inwd 990 inward flux of N III 990
h 1 1026 total Lyman-beta 1025
#inwd 1025 inward flux of Lyman-beta 1025
o 6 1032 total O VI 1032
o 6 1037 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 total He II Balmer-gamma 1085
n 2 1085 total N II 1085
s 4 1086 total S IV 1086; level 2 line
p 5 1121 total P V 1121; level 2 line
fe 3 1122 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 1194 total S III 1194
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)
totl 1216 total Hydrogen Lyman-alpha 1215.67 
inwd 1216 inward flux of Lyman-alpha
he 2 1215 total He II Balmer-beta 1216
inwd 1215 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 1260 total Si II 1260 + 1263
6lev 1304 total O I 1302 + 1305 
si 2 1305 total Si II 1305
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
o 4 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]
s 4 1406 total S IV 1406
totl 1486 total of sum of N IV] 1486 + [N IV]
inwd 1488 inward flux of N IV]
si 2 1527 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 1671 total Al II 1670.8; level 2 line
s 3 1720 total S III 1720
n 3 1750 total N III] 1750 (all components; not computed seperately)
inwd 1750 inward flux of N III]
fe 2 1787 total Fe II 1787 (probably selectively excited)
si 2 1808 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]
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 2140 total sum of N II] 2139.01, 2142.77
c 2 2326 total C II] 2324.69 + 2328.12
si 2 2335 total Si II] 2335
totl 2665 total of sum of Al II] 2669 + [Al II] 
mg 2 2796 total Mg II 2796 of the doublet
mg 2 2804 total Mg II 2804 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 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)
totl 3889 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 4102 total H-delta
inwd 4102 inward flux of H-delta
h 1 4340 total H-gamma
inwd 4340 inward flux of H-gamma
ca b 4471 total He I 4471, case B approximation
he 2 4686 total He II 4686 (Paschen-alpha)
inwd 4686 inward flux of He II 4686
totl 4861 total H-beta 4861
inwd 4861 inward flux of H-beta 4861
totl 5876 total He I 5876
inwd 5876 inward flux of He I 5876
na 1 5895 total Na ID 5895
h 1 6563 total H-alpha 6563
inwd 6563 inward flux of H-alpha 6563
#
# near IR emission lines and continua
k 1 7745 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 10830 total He I 10,830A
h 1 18 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 1100
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 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 11186
nFnu 8220
nFnu 8205
nFnu 6209
nFnu 4885
nFnu 3649
nFnu 3644
nFnu 2392
nFnu 2071
nFnu 2052
nFnu 1793
nFnu 1585
#
# 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
nFnu 1356
nFnu 1297
nFnu 1262
nFnu 1218
nFnu 1196
nFnu 1175
nFnu 1143
nFnu 1113
nFnu 1103
nFnu 1073
nFnu 1064
nFnu 1035
nFnu 1000
nFnu 913
nFnu 911
nFnu 760
nFnu 701
nFnu 608
nFnu 575
nFnu 505
nFnu 503
nFnu 399
#
# 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 11186
#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 913
#InwT 911
#InwT 760
#InwT 701
#InwT 608
#InwT 575
#InwT 505
#InwT 503
#InwT 399
# End of CLOUDY grid output...

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Last changed 04/05/03.
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Copyright 1978-2003 Gary J. Ferland