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Update help and translation

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Dušan Poizl
2024-10-02 11:52:35 +02:00
parent 258553a6bb
commit 06b3dbc1bb
14 changed files with 1878 additions and 575 deletions
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@@ -122,6 +122,8 @@ V skripte je dostupný globálny objekt nazvaný <b>core</b> ktorý má nasledov
<li><b>getFloat(label = "", value = 0, decimals = 3)</b> ukáže diálog pre získanie reálneho čísla. Prvý parameter je textový popis. Druhý parameter je východzia hodnota. Tretí parameter je počet desatinných miest.
Obydva parametre sú voliteľné. Vracia zadané číslo alebo ak je stlačené tlačidlo zrušiť vráti Undefined.</li>
<li><b>getItem(items)</b> ukáže dialog pre výber jednej hodnoty z poľa hodnôt. Vracia vybranú hodnotu ako String alebo ak je stlačené tlačidlo zrušiť vráti Undefined.</li>
<li><b>setStartingSolution(solution)</b> with this you can set starting point and image scale. It accepth object with attributes "ra", "dec", "pixscale".
Same object as returned by <i>File.solve()</i> method. You can also call it without paramer in which case it will clear any previously set values.</li>
</ul>
<h4>File</h4>
@@ -175,6 +177,14 @@ for(file of convertedFiles)// now we can iterate over the files
<li><b>stats()</b> calculate basic images statistics and return them as object with attributes "mean", "stddev", "median", "min", "max" and "mad".
<pre>let s = file.stats();
core.log("Median value is " + s.median);</pre></li>
<li><b>solve(updateHeader)</b> this method will run plate solving on this image and will return solution in form of object with these attributes "ra" and "dec" which are center coordinates of image
"fieldWidth" and "fieldHeight" which is FOV of image in arcseconds, "orientation" is degrees east of north, "pixscale" scale of image in arcseconds per pixel,
"parity" true false value if the image was flipped in vertical direction, "raError" and "decError" deviation from starting point.
When updateHeader is set to true it update FITS header for file with this solution. Default value is false.</li>
<li><b>extractStars(hfr)</b> extract stars will run extraction of stars. When parameter hfr is set to true it will fit HFR on every star.
It return array of objects representing extracted stars. Each object in array
will have these attributes "x" and "y" pixel coordinates of center of star, "mag" relative magnitude of star, "flux" total flux, "peak" peak value of star, "HFR" half flux radius of star,
"a" and "b" semi major and minor axis of star, "theta" angle of orientation of the star, "ra" and "dec" coordinates of star, "numPixels" number of pixel occupied by the star in image.</li>
</ul>
<h4>FITSRecordModify</h4>