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Modify scale Y - X. Decrease max value of Y axis. Open Image. Increase max value of Y axis. Open Profile. Link series. Reset image thresholds. Apply same scale to all serie. Copy the active serie. Reverse Right/Left image. Paste the active serie. Display axis graduations.
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Modify scale Y - X Decrease max value of Y axis Open Image Increase max value of Y axis Open Profile Link series Reset image thresholds Apply same scale to all serie Copy the active serie Reverse Right/Left image Paste the active serie Display axis graduations Binning object Crop the profil to the selection Erase all except series Binning calibration lamp Move serie position in the list Reference to 1 the continuum, zone defined in the preferences Calibration 2 lines Calibration 3 lines and + Calculation on selection, calculations defined in the preference measure Division of a profil by another one Active serie Correction of atmospheric lines Call grapher GnuPlot Zoom/Cancel zoom on the zone selection Change color of the active serie Display database of elements Visual Spec - Quick Reference Card Short-cut Del/Suppr Delete the active serie, if temporary serie Ctrl+D Divide the active serie by another one Ctrl+E Database of element wavelength Ctrl+Q Console mode Ctrl+W Convert into fits "BeSS" Ctrl+T Spectral Type Ctrl+R Move serie Ctrl+I Window Infos... Ctrl+G Manage scale & graduations Ctrl+Z Interactive zoom Ctrl+L Spectra library Ctrl+F Smoothing filter "Low-Pass" Ctrl+C Copy Ctrl+V Paste Ctrl+B Paste format of the active profile Ctrl+N Reference the continuum to 1 Alt+selection profil Zoom on selection Ctrl + click sur série Automatic selection of line close by Formules Doppler: DV=c.Dl/l Rep: Iobs/Itheo + Extraction continuum Icorrinstru: Iobs/Rep Néon Véga Atmosphére
Visual Spec - Quick Reference Card Stellar Model Star Atmos file name coding- 450 is for the temperature, 4500°K- 45 if the gravity log(g)=4.5cm/s²- k4 is the microturbulence velocity, 4km/s- p00 is the metallicity ratio [M/H] which 0.0 for solar abundance or m05 for [M/H]=-0.5 for 0.32 times solar abundance or p05 for [M/H]=0.5 for 3.2 times solar abundance