The following bolometric correction tables have been calculated from COMA07/SPHREAD03 spectra based on COMARCS04 hydrostatic models. Reddening due to circumstellar dust is not included. Each of the 36 tables contains a photometric system including different filters. If a certain filter curve is not covered by the synthetic spectra (below 4444 and above 250000A) a value of -999999 is listed for the bolometric correction. Details concerning the photometric systems are given in Marigo, P., Girardi, L., Bressan, A., et al., 2008A&A...482..883M and in http://stev.oapd.inaf.it/~lgirardi/cmd_2.1/photsys.html .
Synthetic spectrophotometry for C-rich giants (Aringer+, 2009)
MARIGO, PAOLA;
2009
Abstract
The following bolometric correction tables have been calculated from COMA07/SPHREAD03 spectra based on COMARCS04 hydrostatic models. Reddening due to circumstellar dust is not included. Each of the 36 tables contains a photometric system including different filters. If a certain filter curve is not covered by the synthetic spectra (below 4444 and above 250000A) a value of -999999 is listed for the bolometric correction. Details concerning the photometric systems are given in Marigo, P., Girardi, L., Bressan, A., et al., 2008A&A...482..883M and in http://stev.oapd.inaf.it/~lgirardi/cmd_2.1/photsys.html .
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