diff --git a/kstars/ekos/align/opsastrometry.ui b/kstars/ekos/align/opsastrometry.ui index 6ecbfd960..7cdbee559 100644 --- a/kstars/ekos/align/opsastrometry.ui +++ b/kstars/ekos/align/opsastrometry.ui @@ -1,739 +1,714 @@ OpsAstrometry 0 0 536 480 Basic Options 0 <p>This option should <b>ONLY</b> be checked if your astrometry.net version is 0.67 or earlier. Uncheck for any versions greater than 0.67</p> --no-fits2fits Check this option if your image does not have much nebulosity. If it does have strong nebulosity, uncheck it. --resort true This will prevent the solver from looking at an already existing WCS Header before blindly trying to solve the image. It is recommended to keep it checked. --no-verify false Detect parity and reuse it to speed up solver. parity - - - false - - - Prevents creation of unnecessary files unused by Ekos. - - - --no-plots - - - false - - - - - - - false + + + Qt::Horizontal - + - 50 - 16777215 + 40 + 20 - - Overwrite already generated files. It must be checked to prevent solver failure. - - - -O - - - false - - + Imaging Options <p>The units of the imager scale bounds above.</p> <ul> <li>dw: degree width</li> <li>aw: arcminute width</li> <li>app: arcsecs per pixel</li> </ul> units Qt::AlignCenter 22 22 22 22 Update Image Scale Bounds from the currently active camera and telescope combination. false 30 16777215 The high end of the imager scale, calculated as a little bigger than the longer dimension of the image. H 110 16777215 <p>The units of the imager scale bounds above.</p> <ul> <li>dw: degree width</li> <li>aw: arcminute width</li> <li>app: arcsecs per pixel</li> </ul> 0 dw aw app 2 16 2 Downsample the image to shrink its size and speed up the solver. Down Sample false Set image scale to speed up solver as it does not have to search index files of different image scales. Use Scale false false 30 16777215 The lower end of the imager scale, calculated as a little smaller than the shorter dimension of the image. L 3 0.000000000000000 999.000000000000000 30.000000000000000 false Downsample the image to shrink its size and speed up the solver. downsample Qt::AlignCenter 3 0.000000000000000 999.000000000000000 40.000000000000000 The high end of the imager scale, calculated as a little bigger than the longer dimension of the image. High Qt::AlignCenter Automatically update image scale values when CCD and/or Mount parameters are updated. Auto Update true 0 0 22 22 22 22 Image Scale Auto Update is turned off. :/icons/AlignWarning.svg true Qt::AlignCenter false 30 16777215 <p>The units of the imager scale bounds above.</p> <ul> <li>dw: degree width</li> <li>aw: arcminute width</li> </ul> u The lower end of the imager scale, calculated as a little smaller than the shorter dimension of the image. Low Qt::AlignCenter Qt::Horizontal 40 20 Position Options Set estimated position to speed up astrometry solver as it does not have to search in other areas of the sky. Use Position false false 30 16777215 The Search Radius for the Estimated Telescope/Image Field Position in degrees. 5 1.000000000000000 360.000000000000000 30.000000000000000 false 30 16777215 The RA of the Estimated Telescope/Image Field Position in hh:mm:ss notation 3 The DEC of the Estimated Telescope/Image Field Position in dd:mm:ss notation DEC true The RA of the Estimated Telescope/Image Field Position in hh:mm:ss notation The RA of the Estimated Telescope/Image Field Position in hh:mm:ss notation RA 22 22 22 22 Update coordinates to the current telescope position Qt::Horizontal 40 20 The Search Radius for the Estimated Telescope/Image Field Position in degrees. Radius true 70 0 The DEC of the Estimated Telescope/Image Field Position in dd:mm:ss notation false 30 16777215 The DEC of the Estimated Telescope/Image Field Position in dd:mm:ss notation 4 Automatically update position coordinates when mount completes slewing. Auto Update true 0 0 22 22 22 22 Position Auto Update is turned off. :/icons/AlignWarning.svg true Qt::AlignCenter Do not use Sync when Slew to Target is selected. Use differential slewing to correct for discrepancies. This is useful on some mounts (e.g. Paramount). Use differential slewing instead of syncing Custom: Additional optional astrometry.net options. Qt::Vertical 20 40 dmsBox QLineEdit
widgets/dmsbox.h
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