Program LINLTE.FOR (LINFOR)
Fine analysis and spectrum synthesis of stellar spectra
Input files:
Stellar Physics
These files are required to control LINFOR.
- ATM.DAT from
ATMOS
-
Model atmosphere
- LINE.DAT
-
Line data and commands -- the actual control file
- FALT.DAT
-
Convolution (German: Faltung) data and output control of spectrum
synthesis (file only needed for synthesis)
- DEPART.DAT from NLTE system
-
Departure coefficients for given element (file only needed if NLTE
calculations requested)
- OBS.OUT
-
Observed spectrum (needed only for spectrum fits)
- LIMITS.DAT
-
Wavelength regions for spectrum fits (not strictly required as it is
written/updated by LINFOR)
Broadening Tables
These files are needed only if corresponding calculations are requested
in LINE.DAT.
- VCS.DAT
-
Stark broadening tables for hydrogen (VCS theory)
- VCSSB.DAT
-
Stark broadening tables for He II (VCS theory following Schöning and Butler).
- BCSS_HE1.DAT and BCSS_4471.DAT
-
Broadening tables for He I (Barnard, Cooper, Shamey). Both files are
needed.
- BWB.DAT
-
Broadening tables for He I (Beauchamp)
Output files:
- FOR003.DAT in UNIX usually fort.3; FORTRAN
channel number 3
-
Line printer output of results
- PLOT.OUT
-
Synthetic spectrum (optional)
- LIMITS.DAT
-
Wavelength regions for spectrum fits (written/updated by LINFOR)