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 These are some of the most important databases used by Cloudy:
 Many recombination coefficients were taken from http://amdpp.phys.strath.ac.uk/tamoc/RR/ and http://amdpp.phys.strath.ac.uk/tamoc/DR/
      and are based on the following papers:
        Badnell N. R., et al., A&A 406, 1151 (2003) [http://adsabs.harvard.edu/abs/2003A%26A...406.1151B]
        Badnell N. R., ApJS 167, 334 (2006) [http://adsabs.harvard.edu/abs/2006ApJS..167..334B]
 Much of the molecular emission data is from LAMDA as accessed on Dec. 18, 2010. This database is described in:
        Schoeier F.L., et al., A&A 432, 369 (2005) [http://adsabs.harvard.edu/abs/2005A%26A...432..369S]
      This database is in part based on the work of the following groups:
        JPL: Pickett H. M. et al., JQSRT, 60, 883 (1998). [http://adsabs.harvard.edu/abs/1998JQSRT..60..883P]
        CDMS: Mueller H. S. et al., A&A 370, L49 (2001). [http://adsabs.harvard.edu/abs/2001A%26A...370L..49M]
              Mueller H. S. et al., J. Mol. Struct. 742, 215 (2005). [http://adsabs.harvard.edu/abs/2005JMoSt.742..215M]
 Much of the ionic emission data is from version XXXX of CHIANTI. CHIANTI is a collaborative project involving the NRL (USA), the
      Universities of Florence (Italy) and Cambridge (UK), and George Mason University (USA). These papers describe Chianti:
        Dere K. P., et al., A&AS, 125, 149 (1997) [http://adsabs.harvard.edu/abs/1997A%26AS..125..149D]
        Landi E., et al., ApJ, 744, 99 (2012) [http://adsabs.harvard.edu/abs/2012ApJ...744...99L]
 Much of the H_2 data is from this web site: http://molat.obspm.fr/index.php?page=pages/Molecules/H2/H2can94.php. These data are
      described in:
        Abgrall H. et al., Can. J. Phys., 72, 856 (1994) [http://adsabs.harvard.edu/abs/1994CaJPh..72..856A]
        Wrathmall S. A. & Flower D. R., J. Phys. B, 40, 3221 (2007) [http://adsabs.harvard.edu/abs/2007JPhB...40.3221W]
 Please cite those papers that played a significant role in this calculation.