Initial commit for trunk

.gitignore

+.*
+!.gitignore
+*.o
+*.lo
+*.a
+*.so
+*~
+\#*\#
+*.dep
+*.gch
+# LaTeX temporary files
+*.aux
+*.log
+*.bbl
+*.blg
+*.lof
+*.lot
+*.out
+*.toc
+*.exe
+
+

.hgignore

+
+# Automatically generated by `hgimportsvn`
+syntax:glob
+.svn
+*.o
+*.lo
+*.a
+*.so
+*~
+\#*\#
+*.dep
+*.gch
+# LaTeX temporary files
+*.aux
+*.log
+*.bbl
+*.blg
+*.lof
+*.lot
+*.out
+*.toc
+*.exe
+
+

data/0m010.szd

+# size distribution file for single sized grain
+2010403 # magic number for version control
+ssize  # choices are SSIZE, POWER, EXP1, EXP2, EXP3
+0.010  # grain size (micron)

data/0m100.szd

+# size distribution file for single sized grain
+2010403 # magic number for version control
+ssize  # choices are SSIZE, POWER, EXP1, EXP2, EXP3
+0.100  # grain size (micron)

data/1m000.szd

+# size distribution file for single sized grain
+2010403 # magic number for version control
+ssize  # choices are SSIZE, POWER, EXP1, EXP2, EXP3
+1.000  # grain size (micron)

data/FeII_bands.ini

+9 6 11
+# the above is a version number and must appear as the first line - 
+# it is used to confirm that this is the correct file
+# for the current version of the code
+#
+# change log 
+# 9 6 11, change 2798 band to 2797 to avoid collision with label for MgII
+# 9 5 30, add Baldwin et al 2004 FeII UV band, all ID strengs now " bounded
+#
+# the large FeII atom predicts far too many lines to be grasped by a human
+# under most circumstances.  The bands defined in this file provide a way to
+# collapse the FeII spectrum into a smaller group of lines.
+#
+# These bands will be entered into the main emission line 
+# printout with line label "Fe2b", 
+# They will have a wavelength given by the first number on the following lines.
+# The second pair of numbers are bounds for summing over the 
+# predicted FeII emission spectrum.
+# Lines are included if their wavelengths are ge lower, le upper bounds
+# these are all vacuum wavelengths 
+#
+# data in this file is read in by routine FeIICreate, which calls
+# FeIIBandsCreate, all into is put into
+# structure FeII_Bands[n][3]
+# The data structure FeII is in cddrive.h
+#
+# The number of wavelength bands is deduced on the fly by reading this file
+# and stored as FillnBands.
+# There is no limit to the number of bands in this file.
+#
+# The first number should be entered as an integer because
+# it will be converted to an
+# integer in the printout.  The remaining numbers are floats.
+# All numbers must be greater than 0 and the third number must be 
+# larger than the second.
+#
+# Any line with a "#" in col 1 is a comment and totally ignored,
+# These comment lines can occur anywhere within this file.
+# Any line that does not have a "#" in col 1 must contain three numbers.  
+#
+# The file ends with end of file, and must contain comments or valid data
+# up to that point
+#
+# the order of the bands in this file can be changed, and the 
+# bands will appear in exactly this order in the standard printout
+#
+# these are very broad bands
+1500  1000  2000  "very broad FeII band"
+2500  2000  3000  "very broad FeII band"
+5000  4000  6000  "very broad FeII band"
+7000  6000  7800  "break in excitation beyond 7800 - Lya casecades above 7800"
+10000 7800  30000 "should be dominated by cascades after pump"
+#
+# these are the little bands, which pick up individual features
+1067  1000  1133    
+1120  1070  1170  
+1148  1133  1163    "UV10"
+1212  1163  1260    "under Lya+NV"
+1270  1260  1280    "UV9"
+1295  1280  1310    "Lya  cascades"
+1330  1310  1350    
+1365  1350  1380    "Lya  cascades"
+1450  1400  1500  
+1485  1380  1590    
+1550  1500  1600  
+1615  1590  1640     "UV8, UV43"
+1650  1600  1700  
+1670  1640  1700     "UV68, UV40"
+1740  1700  1780     "misc."
+1787  1780  1793     "UV191"
+1822  1793  1850     "misc."
+1870  1850  1890     "Lya  cascades (blue wing of C III])"
+1930  1890  1970     "under CIII]"
+2090  1970  2210     "misc. (see Grandi, year)"
+2355  2280  2430     "UV2, UV3, UV35, UV36, spike in Baldwin+04 spike to gap ratio"
+2430  2200  2660     "UV bump defined in Baldwin et al. 2004"  
+2445  2240  2650     "UV band used by Baldwin et al. 2004"
+2495  2430  2560     "Lya  cascades, gap in Baldwin+04 Spike to gap ratio"
+2610  2560  2660     "UV1, UV64, spike in Baldwin+04 spike to gap ratio"
+2695  2660  2730     "UV62, UV63 (avoid Mg II)"
+2758  2730  2785     "UV62, UV63 under Mg II"
+2780  2660  2900  
+2797  2785  2810      "misc. under Mg II"
+2840  2810  2870      "Lya  cascades under Mg II"
+2935  2870  3000      "UV60, UV61, UV78"
+2960  2900  3025  
+3050  3000  3100    
+3180  3025  3330  
+3250  3100  3400      "1,6,7"
+3590  3400  3780    
+3910  3780  4040      "3, 29"
+4060  4040  4080    
+4255  4080  4430      "27, 28 (blend w/ Hg, Hd)"
+4558  4430  4685      "37, 38"
+4600  4450  4750      "first Fe II opt band used in Baldwin+04"
+4743  4685  4800    
+4855  4800  4910      "under Hb"
+4920  4750  5080  
+4975  4910  5040      "42"
+4971  4924  5018      "blend with Hb, [OIII]"
+5070  5040  5100      "under Hb, [OIII]"
+5143  5100  5185      "5169 only, avoids Hb, [OIII]"
+5270  5080  5460      "second Fe II opt band used in Baldwin+04"
+5318  5185  5450      "48, 49"
+5540  5450  5630      "55"
+5865  5630  6100    
+6265  6100  6430      "40, 74"
+6565  6430  6700      "under Ha +[NII]"
+6910  6700  7120    
+7445  7120  7770      "72, 73"
+7785  7770  7800    
+8625  7800  9450      "Lya cascades"
+10325 9450  11200     "Lya cascades"
+18890 16780 21000     "Lya cascades"
+22000 21000 23000     "Lya cascades"