Stardock Trial version. User rating User Rating 6. Fences is a program that helps you organize your desktop, and can hide your icons when they're not in use. A "Fence", a term coined by this program, is an icon group on your desktop. Fences is an add-on to your desktop, not a replacement. We don't have any change log information yet for version 1.
Sometimes publishers take a little while to make this information available, so please check back in a few days to see if it has been updated. If you have any changelog info you can share with us, we'd love to hear from you! Head over to our Contact page and let us know. It does this by grouping by type: folders, files and icons that are grouped by expandable and highly custom. This is a known bug, and it's mentioned in the original post.
There should be a fix soon, so don't feel the need to delete your precious apps right away ;-. There's also a rare bug report about apps with 3 or more digits in the name causing a problem with Crackulous, but so far that's not been confirmed. Make sure you address your crashing in the official Crackulous crashing topic. But how do I crack apps without buying them? You don't. Every single app that's ever been cracked has been legitimately purchased by the cracker. Part of the cracking method requires you to run the app on your iDevice before it's cracked, and the only way to do that is by buying it and downloading it legitimately.
Makes you think twice before you start spamming the requests board, doesn't it? Don't know how to do that? This, my friends, is why we have a Tutorials section here at Hackulous ;- Take some initiative and search for it! The image is then saved in the working directory with a unique name containing the capture timestamp. Version 1. You can choose the type of snapshot you want: a file on the disk, or in memory in the clipboard. The star detection algorithm, which serves both global registration and astrometric resolution, has been modified to improve performance and reliability.
It detects fewer false positives that could distort the alignments and estimates the profiles of the stars to resolve the PSF on a box of size adapted to each. Compared to the previous version, there should be less need to adjust the dynamic PSF settings for Siril to register the images. Star detection comparison between version 0.
A side effect of this improvement, and not the least, is the reduction in overall registration processing time. This performance gain is also quite spectacular for monochrome images as can be seen in the following illustrations. Performance report for a sequence of color images. The comparison is made in 16 and 32bits for versions 0. Version 0. Performance report for a sequence of monochrome images.
For global registration, it is now possible to choose the number of degrees of freedom of the transformation that sends the image to be registered to the reference image. By default, the transformation is a homography , which admits a certain number of distortions between the 2 images. But for sequences of images in which one would expect little or no distortion, this projection has too many degrees of freedom and one may wish to test more rigid projections, which will result in less interpolation.
For this purpose, it is now possible to choose a translation 1 translation along each axis , a similarity 2 translations, 1 rotation and 1 scale or an affinity the same with shearing in addition. Depending on the chosen type, the transformation which sends the image to be registered on the reference image is calculated on 2, 4, 6 or 8 degrees of freedom.
The higher the number of degrees, the more deformation the transformation admits between the 2 images. A new tool integrates the already substantial panoply of Siril analysis tools. It is used to analyze the image and indicate to the user whether or not the sensor is tilted relative to the optical axis.
The latter is represented by a quadrilateral with at each vertex, the value of the FWHM used for the calculation. The image is divided into 4 equal parts in which the FWHMs are calculated. Then the FWHM of the central zone is also calculated. A sensor with zero tilt would be represented by a square with all the FWHM values identical.
There are two ways to use this new feature:. In fact, the greater the number of stars used in the calculation, the more reliable the result of the analysis. Warning: for the result to make sense, it is preferable to run this command on a sub and not a stacking result.
A pre-processed image just demosaiced for color sensors is therefore ideal. Moreover, the drawn quadrilateral has its proportions exaggerated, in order to be more visible on the screen.
In the toolbar has been added a button to perform a quick photometry of the stars. Simply select this button to change the image selection mode, then click on a star. The result of the photometry appears instantly.
Its value is calculated in dB , but for more understanding, it is associated with 6 levels of notation:.
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