Parameter |
Description |
OUTNUMB |
Output starting number |
OUTPUTF |
Output generic name |
PLOTYP |
Type of plot (RATIO, MAGNITUDE) |
RADIUS |
Radius for cosmics rejection |
REBEND |
Final wavelength for rebinning |
REBMTD |
Rebinning method (LINEAR, QUADRATIC, SPLINE) |
REBOPT |
Rebin Option (YES/NO) |
REBSTP |
Wavelength step for rebinning |
REBSTRT |
Starting wavelength for rebinning |
RESPLOT |
Plot flag for response computation |
RESPONSE |
Response Image |
RESPOPT |
Response Correction Option (YES/NO) |
RESPTAB |
Intermediate Response Table |
RON |
Read-Out-Noise (ADU) |
ROTOPT |
Rotation Option (YES/NO) |
ROTSTART |
Y-start after rotation |
ROTSTEP |
Y-step after rotation |
SEAMTD |
Search centering method (GAUSS, GRAV, MAXI) |
SESSION |
Session name |
SHIFT |
Shift in pixels |
SIGMA |
Threshold for rejection of cosmics (std dev.) |
SKYMOD |
Mode of fitting |
SKYORD |
Orderfor sky fit |
SMOOTH |
Smoothing factor for spline fitting |
START |
start points of the raw image. |
STD |
Standard Star Spectrum |
STEP |
start points of the raw image. |
THRES |
Threshold for line detection (above local median) |
TOL |
tolerance in Angstroms for wavelength ident. |
TRIM |
Trim window (x1,y1,x2,y2) in pixels |
TRIMOPT |
Trim Option (YES/NO) |
TWODOPT |
Computes bivariate polynomial option. |
UPPSKY |
Lower, upper row number of upper sky |
WCENTER |
Central wavelength |
WIDTH |
Window size in X for line detection (pixels) |
WLC |
wavelength calibration image |
WLCMTD |
Wavelength calibration method (IDENT,GUESS) |
WLCNITER |
Minimum, Maximum number of iterations |
WRANG |
wavelength range to take from LINCAT |
YSTART |
Starting row for the calibration (pixel value) |
YSTEP |
Step in Y for line searching (pixels) |
YWIDTH |
Window size in Y for line detection (pixels) |