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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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@@ -133,6 +133,8 @@ Le deuxième paramètre est la valeur par défaut dans la zone de saisie. Les de
<li><b>getFloat(label = "", value = 0, decimals = 3)</b> affiche une boîte de dialogue avec une zone de saisie pour récupérer une valeur décimale. Le texte passé dans le premier argument est utilisé comme label de description.
Le deuxième paramètre est la valeur par défaut dans la zone de saisie. Les trois paramètres sont facultatifs. Lorsque vous appuyez sur Annuler, il renvoie Undefined.</li>
<li><b>getItem(items)</b> affiche une boîte de dialogue de sélection qui permet de sélectionner un élément dans un tableau d'éléments. Lorsque vous appuyez sur Annuler, il renvoie 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>
@@ -185,6 +187,14 @@ for(file of convertedFiles)// now we can iterate over the files
<li><b>stats()</b> calculer les statistiques d'images de base et les renvoyer sous forme d'objet avec des attributs "mean", "stddev", "median", "min", "max" et "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>