* * This file contains the data for calculating light curves in filters. * The columns of the table -- with an example -- are: * * Specific * Filter Effective Intensity * Name Log g Temperature at mu = 1 a b * * B 4.5 5775 3.750e+6 0.99 -0.17 * * * Filter Name: any of the standard names, UBVRIJHK. * Log g: log of the gravity in cgs units. * Effective Temp: in degrees K. * Specific Intensity: in cgs units: ergs/cm^2/sec/A/steradian * a and b: quadratic limb darkening coefficients. * * The limb darkening law used by the program is * I(mu) = I(mu=1) * ( 1 - a*(1-mu) - b*(1-mu)^2) * * All columns in the table must be present, even if zero. * * Only those lines with filters requested by file "starpars" * and with values of log( g ) within 0.1 of those requested * by "starpars" are read and stored by the program. The * program interpolates in temperature but not in log( g ). * Comment lines begin with an asterisk. * * * The following adapted from solar tables in Allen, AQ, 3rd ed. U 4.5 5775 2.23e+6 0.78 0.10 B 4.5 5775 3.86e+6 0.65 0.17 V 4.5 5775 3.40e+6 0.47 0.23 H 4.5 5775 4.03e+5 0.15 0.20 K 4.5 5775 1.42e+5 0.09 0.17 * The following lines were calculated by C. Froning * from a stellar atmosphere code. H 4.5 2000 53173.9 -0.020 0.606 H 4.5 2500 71483.4 0.003 0.451 H 4.5 3000 95903.6 0.022 0.321 H 4.5 3500 138765. 0.048 0.299 H 4.5 4000 237193. 0.171 0.368 H 4.5 4500 290133. 0.146 0.398 K 4.5 2000 32535.5 -0.164 0.735 K 4.5 2500 38843.7 -0.001 0.294 K 4.5 3000 47115.8 0.011 0.235 K 4.5 3500 62386.3 0.030 0.240 K 4.5 4000 90181.2 0.118 0.310 K 4.5 4500 104593. 0.124 0.315