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Timestamp:
09/20/06 04:19:25 (2 years ago)
Author:
gary
Message:

data files - some sort of version mismatch had crept in - these are needed to get smoke test to runall.pl

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  • branches/newmole/data/bands_continuum.dat

    r452 r505  
    1 6 2 13   
     16 8 7   
     2# MAGIC NUMBER 
    23# the above is a version number and must appear as the first line -  
    34# it is used to confirm that this is the correct file 
     
    56# it is the currnet date, y mm dd 
    67# search for "bands_continuum magic number here" in cont_createpointers.c 
    7 # version 6 2 13, add PAH bands 
     8#  
     9# VERSION CHANGE LOG 
     10# 6 2 13, add PAH bands 
     11#  
     12# 6 8 7 NA made several adjustments to bands, following changed 
     13#       FIR, from 42.5 -122.5 mic to 40 - 500 mic,  
     14#       TIR, from 3.-1100 to 500-3100 mic, centroid from 550 to 1800 mic  
     15#       NIRa upper bound from 5.0 to 4.0 mic  
     16#       NMIR upper bound from 42.5 to 40 mic 
     17#       added TALL 1.0, 1e-5 to 1e4 microns 
     18#       series of IRAS bands 
     19# 
     20# N.B. THIS FILE MUST BE KEPT PARALLEL WITH DOCUMENTATION 
     21# table of bands is given in Part 3 of Hazy, in chapter lines.doc "the emission lines" 
     22# section Continua under "the main emission-line printout"  
    823# 
    924# the vars are 
     
    2237# the emission-line stack in the main output 
    2338# 
     39# LINE FORMAT 
    2440# each line that does not begin with a # must  
    2541# fully specifies an entry into the emission-line stack 
     
    2945# the integrated intensity in the output. It appears as the "line label" 
    3046# in the main output 
     47# 
     48# The 5th char must be a space 
    3149# 
    3250# The first number is the mean wavelength of the band and will appear 
     
    3856# All numbers must be greater than 0 and the third number must be  
    3957# larger than the second. 
     58# 
     59# EXAMPLE 
     60# LABL wl  wl1  wl2 
     61# where LABL is the 4 char label that will appear in the emission-line stack 
     62# wl is the wavelength that will appear in the stack 
     63# wl1 and wl2 are the lower and upper bounds to the band 
    4064# 
    4165# NB ALL WAVELENGTHS *MUST* BE IN MICRONS 
     
    6185#>>refer        cont    band Helou, G, Khan, I. R., Malek, L., & 
    6286#>>refercont    Boehmer, L. 1988, ApJS, 68, 151 
    63 FIR 83m 42.5m 122.5m  
     87FIR  83m 40m 500m  
    6488# this is the TIR band described by 
    6589#>>refer        cont    band Helou, G. & Dale, D. A. 2002, ApJ, 576, 159 
    66 TIR 550m 3.0m 1100.0m 
     90TIR  1800m 500m 3100.0m 
    6791## this is the lower range to the NIR band defined on the IPAC website 
    6892#>>refer        cont    band http://www.ipac.caltech.edu/Outreach/Edu/Regions/irregions.html 
    69 NIRa 2.85m 0.7m 5.0m 
     93NIRa 2.85m 0.7m 40m 
    7094# this is the upper range to the NIR band defined on the IPAC website 
    7195#>>refer        cont    band http://www.ipac.caltech.edu/Outreach/Edu/Regions/irregions.html 
     
    78102MIRb 22.5m 5.0m 40.0m 
    79103# this is the micron band with wavelengths less than FIR 
    80 NMIR 21.75m 0.7m 42.5m 
     104NMIR 21.75m 0.7m 40m 
    81105# this is the micron band with wavelengths greater than FIR 
    82106TFIR 611.25m 122.5m 1100.0m 
     
    84108TALL 1.0m 0.00001m 10000.0m 
    85109# 
     110# Here are the IRAS 1, 2, 3, and 4 bands at 12, 25, 60, and 100 microns.  The definition of these bands come from 
     111#>>refer        cont    band    S.Satyapal      private communication 
     112# The labeling convention of these bands follows that given in  
     113#>>refer        cont    band    Malhotra et al. 2001, ApJ, 561, 766 
     114# in which the labels were just the letter "F" followed by the wavelength 
     115F12  12m 8.5m 15m 
     116F25  25m 19m 30m 
     117F60  60m 40m 80m 
     118F100 100m 83m 120m 
    86119# DEFINE PAH EMISSION BANDS HERE PAHC is the continuum associated with the various PAH features 
    87120# NB - NA adjusted these bands so that the continuum can be removed from the PAH energy 
     
    92125#  
    93126# 3.3 microns 
    94 PAH 3.3m 3.25m 3.35m 
     127PAH  3.3m 3.25m 3.35m 
    95128PAHC 3.2m 3.15m 3.25m 
    96129# 6.2 microns 
    97 PAH 6.2m 5.9m 6.4m 
     130PAH  6.2m 5.9m 6.4m 
    98131PAHC 5.65m 5.4m 5.9m 
    99132# 7.9 microns 
    100 PAH 7.9m 7.4m 8.4m 
     133PAH  7.9m 7.4m 8.4m 
    101134PAHC 6.9m 6.4m 7.4m 
    102135# 11.3 microns 
    103 PAH 11.3m 11.1m 11.5m 
     136PAH  11.3m 11.1m 11.5m 
    104137PAHC 10.9m 10.7m 11.1m 
    105138# 11.8 microns 
    106 PAH 11.8m 11.6m 12.3m 
     139PAH  11.8m 11.6m 12.3m 
    107140PAHC 12.65m 12.3m 13.0m 
    108141# 13.3 microns 
    109 PAH 13.3m 12.9m 13.7m 
     142PAH  13.3m 12.9m 13.7m 
    110143PAHC 14.1m 13.7m 14.5m 
    111144# this is a test - the Balmer continuum