title BLR model, density 1e09 cm-3, flux of H-ion phots 1e20 cm2 s-1 c c commands controlling continuum ========= table agn phi(h) 22 c c commands for density & abundances ========= hden 9 c c commands controlling geometry ========= stop column density 23 c c other commands for details ========= init "c84.ini" iterate convergence c these are to try to speed things up no level2 lines c c commands controlling output ========= normalize to "totl" 1216 100 print line faint 1 // get rid of lots of faint lines save performance "blr_n09_p22.per" save monitors "blr_n09_p22.asr" last save overview "blr_n09_p22.ovr" last save dr "blr_n09_p22.dr" last save convergence reason "blr_n09_p22.cvr" c c commands giving the monitors ========= // strong blr lines // //total of sum of both O VI comp // >>chng 06 feb 03, from 3.579 to 4.515, guess dr to Badnell mean // >>chng 06 apr 22, from 4.515 to 4.675, RP use Badnell DR for He-like // >>chng 06 nov 29, from 4.675 to 4.714, Badnell DR turned on // >>chng 07 jan 20, from 4.714 to 4.754, e2 bug // >>chng 07 may 21, from 4.754 to 4.725, fix bug in He-like DR extrapolation // >>chng 10 aug 08, from 4.725 to 4.725, drift down // >>chng 11 sep 15, from 4.71 to 4.745, Chianti for Fe moderate to high ions // >>chng 11 nov 16, from 4.745 to 4.78, adjust newmole monitors monitor line luminosity "totl" 1035 4.78 // //total Hydrogen Lyman-alpha 1215.67 // >>chng 06 feb 03, from 6.259 to 6.764, guess dr to Badnell mean // >>chng 06 nov 29, from 6.764 to 6.811, Badnell DR turned on // >>chng 09 jun 28, from 6.811 to 6.78, check convergence of outward Hb // >>chng 09 jul 27, from 6.78 to 6.824, rm test on outward Hb - will create ticket on problems // >>chng 11 sep 15, from 6.824 to 6.863, Chianti for Fe moderate to high ions monitor line luminosity "totl" 1216 6.863 // //total of sum of both N V comp // >>chng 06 feb 03, from 1.613 to 2.647, guess dr to Badnell mean // >>chng 06 apr 22, from 2.647 to 2.851, RP use Badnell DR for He-like // >>chng 06 nov 29, from 2.851 to 2.894, Badnell DR turned on // >>chng 07 jan 20, from 2.894 to 2.921, e2 bug // >>chng 07 may 21, from 2.921 to 2.884, fix bug in He-like DR extrapolation // >>chng 11 sep 15, from 2.884 to 2.91, Chianti for Fe moderate to high ions // >>chng 11 nov 16, from 2.91 to 2.96, adjust newmole monitors monitor line luminosity "totl" 1240 2.96 // // >>chng 09 jun 28, from 1 to 4.215, check convergence of outward Hb // >>chng 11 sep 15, from 4.215 to 4.244, Chianti for Fe moderate to high ions monitor line luminosity "H 1" 4861 4.244, // // >>chng 09 jun 28, from 1 to 3.914, check convergence of outward Hb // >>chng 11 sep 15, from 3.914 to 3.943, Chianti for Fe moderate to high ions monitor line luminosity "Inwd" 4861 3.943, // //total He II Balmer-alpha 1640 // >>chng 06 feb 03, from 5.513 to 5.974, guess dr to Badnell mean // >>chng 06 nov 29, from 5.974 to 6.017, Badnell DR turned on // >>chng 07 oct 22, from 6.017 to 5.606, resolve l-levels of h-like sequence // >>chng 08 dec 13, from 5.606 to 5.584, merging newsolvers branch // >>chng 11 sep 15, from 5.584 to 5.62, Chianti for Fe moderate to high ions monitor line luminosity "he 2" 1640 5.62 // // >>chng 08 dec 08, from 4 to 3, upper limit -> equals (r2515) // >>chng 09 jun 28, from 3 to 4, check convergence outward Hb // >>chng 09 jul 27, from 4 to 3, rm test on outward Hb - will create ticket on problems monitor niter 3 error 0.01 // // >>chng 06 feb 03, from 7.020 to 6.628, guess dr to Badnell mean // >>chng 06 nov 29, from 6.628 to 6.591, Badnell DR turned on // >>chng 11 sep 15, from 6.591 to 6.557, Chianti for Fe moderate to high ions monitor hydrogen 2 temperature 6.557 // // >>chng 03 dec 07, from 280 to 330, dr resolve metal changes // >>chng 05 dec 22, from 330 to 20 (13), very hot, why did it ever need 330? // >>chng 08 dec 08, from 20 to 15, upper limit -> equals (r2515) // >>chng 09 jun 15, from 15 to 37, gradual approach to outer edge monitor nzone 37 // c blr_n09_p22.in c class blr c ======================================== This is one of the models that sample the LOC plane.