XO1.README TITLE MODEL FOR XO-1 GSC 02041-01657 TEFF 5750. GRAV 4.53 ABUND [-0.058] VTURB 0.541 - 1.982 km/s HE 0.089 VROTATION 1.11 km/s Wavelength, flux, continuum triplets in vacuum nm and in ergs/cm**2/s/ster/nm (WL(I)=FIRSTWL*(1.D0+1.D0/RESOLUTION)**(I-1),I=1,NWL) FIRSTWL 89.90014024 LASTWL 300300.04016128 RESOLUTION 500000 (actually resolving power) NWL 4056924 89.90014024 2.580E-06 2.580E-06 89.90032004 2.580E-06 2.580E-06 89.90049984 2.580E-06 2.580E-06 300298.83896472 4.328E-03 4.328E-03 300299.43956240 4.328E-03 4.328E-03 300300.04016128 4.328E-03 4.328E-03 The spectrum was computed with the same lines that were used to compute the ATLAS12 model. Lines with good wavelengths should match features in an observed spectrum. The predicted lines can have a large wavelength uncertainty. The 500000 resolving power spectrum was instrumentally broadened with a gaussian to smaller resolving powers at the same wavelengths using program BROADEN. The broadened spectra were then resampled at the center of an odd number of points using program RESAMPLE. The new points are uniformly spaced in doppler space. Intensity spectra at 17 angles, mu = 1.,.9,.8,.7,.6,.5,.4,.3,.25,.2,.15,.125,.1,.075,.05,.025,.01 blocks = 512b IXO1P.DAT01 301100 IXO1P.DAT02 301100 IXO1P.DAT03 301100 IXO1P.DAT04 301100 IXO1P.DAT05 301100 IXO1P.DAT06 301100 IXO1P.DAT07 301100 IXO1P.DAT08 301100 IXO1P.DAT09 301100 IXO1P.DAT10 301100 IXO1P.DAT11 301100 IXO1P.DAT12 301100 IXO1P.DAT13 301100 IXO1P.DAT15 301100 IXO1P.DAT16 301100 IXO1P.DAT17 301100 Flux spectra with rotation velocity 1.11 km/s resolving power | resampling blocks = 512B | RXO1P.100000RESAM3 100367 RXO1P.10000RESAM25 12044 RXO1P.1000RESAM251 1200 RXO1P.100RESAM2501 121 RXO1P.20000RESAM13 23162 RXO1P.2000RESAM125 2409 RXO1P.200RESAM1251 241 RXO1P.30000RESAM9 33456 RXO1P.3000RESAM83 3628 RXO1P.300RESAM833 9125 RXO1P.500000 301100 RXO1P.50000RESAM5 60220 RXO1P.5000RESAM51 5904 RXO1P.500RESAM501 601 MODXO1.DAT input model AM058T5750G453KVD.DAT ATLAS12 model