- 04 Apr, 2017 1 commit
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Robert Lancaster authored
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- 03 Apr, 2017 1 commit
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Script Kiddy authored
In case of conflict in i18n, keep the version of the branch "ours" To resolve a particular conflict, "git checkout --ours path/to/file.desktop"
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- 02 Apr, 2017 3 commits
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Robert Lancaster authored
I was working on the Whats Interesting tool because I think it has a lot of potential. I added photos and descriptions to the list. I added photos to the detail view. I also changed some of the layouts. And finally I added a telescope slew button.
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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- 31 Mar, 2017 2 commits
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Jasem Mutlaq authored
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Jasem Mutlaq authored
Detect if flat image is already saturated before calculating fitting. Only utilize polynomial fitting if we have 4 or more points since it can quite unreliable at low counts
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- 29 Mar, 2017 3 commits
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Csaba Kertész authored
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Yuri Chornoivan authored
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Yuri Chornoivan authored
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- 28 Mar, 2017 1 commit
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Jasem Mutlaq authored
Initial work for Image Guiding algorithm by Bob Majewski. All guide images must be explicitly converted to floats and then partitioned into NxN regions before sending them to the algorithm
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- 27 Mar, 2017 2 commits
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Jasem Mutlaq authored
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Robert Lancaster authored
I found the drawing issue that was making the horizontal bar for different pixel heights of the window. It took me some time to dig up what exactly was causing the black line. But I finally did. It was a result of clipping that was taking place in Skymapqdraw.cpp: // Set Clipping QPainterPath path; path.addPolygon(m_SkyMap->projector()->clipPoly()); psky.setClipPath(path); psky.setClipping(true); Which was based upon some code in Projector.cpp in the method void Projector::updateClipPoly() The issue was that in creating the clip path, it was stepping around the circle from 0 to 180 degrees and then from 0 to -180 degrees. As a result, it created not a circular clipping region but two semicircular clipping regions. I painted the path so that I could clearly see what was going on: Then I tried reversing the direction for the second half circle from -180 to 0. This did not work, it produced an unbounded clipping region. But then I tried doing a full circular path from 0 to 360. This not only gave a circular path, it worked perfectly for the clipping region and fixed the problem. Now what I don’t know is whether the reason for two separate half circles was based upon some issue with the sincos method accurately calculating the other half of the circle. The reason I suspect this is because someone went to a lot of trouble to write two separate loops that are nearly identical. As far as I can tell, this method works, please check for me. CCMAIL:kstars-devel@kde.org
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- 26 Mar, 2017 3 commits
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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Robert Lancaster authored
This patch should allow the remote solver to print its solutions nicely in the table the same way the online and the local solver already do. It also adds an autoscale button for the solutions graph.
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- 25 Mar, 2017 5 commits
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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Jasem Mutlaq authored
Read indidrivers.xml as the first file. Silenty ignore replicas. Do not allow device manager to start INDI services for remote drivers
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Jasem Mutlaq authored
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Jasem Mutlaq authored
Create INDI driver entries regardless of what is currently install. Drivers that are not locally available are treated as remote-only drivers
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- 24 Mar, 2017 1 commit
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Jasem Mutlaq authored
Do not process WCS on loading if we plan to create a WCS file. Make loadWCS asynchronous and use signal to proceed in the chain
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- 23 Mar, 2017 3 commits
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Jasem Mutlaq authored
Do not make thumbnail selector dependent on detail dialog since it can be used also in observing list
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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- 22 Mar, 2017 3 commits
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Jasem Mutlaq authored
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Valentin Boettcher authored
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Yuri Chornoivan authored
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- 21 Mar, 2017 7 commits
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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Jasem Mutlaq authored
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Valentin Boettcher authored
I've constructed a request to JPL myself and got out a csv of several hundred megabytes, which is certainly not suitable for KStars. Looking at the differences between my query and the one in KStars, I found some extra parameters, which had not been included in my one: c1_item=Ai and c1_op=%3C and c1_value=12. That basicly means, that JPL filters the asteroids for the ones which have an parameter 'H' (absolute magnitude) smaller than 12, which means that they are 'visible'. Added "Waiting for Server Response" to filedownloder class to improve usability. CCMAIL:kstars-devel@kde.org
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- 20 Mar, 2017 4 commits
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Jasem Mutlaq authored
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Jasem Mutlaq authored
Add support for observers in capture module. Observer names are sent to INDI CCD driver where they are recorded in the FITS header. Furthermore, target name is also sent to the CCD driver to be recorded as OBJECT
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Jasem Mutlaq authored
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Robert Lancaster authored
Here is a patch that will add a sort function to the mount modeling tool that will start with the point that is currently closest to the telescope and then sort the rest of the points by the minimal distance after the previous point. Also I added a check to see if Goto Nothing is selected in the align module and if so, a warning is issued when the user tries to start the modeling tool. CCMAIL:kstars-devel@kde.org
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- 19 Mar, 2017 1 commit
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Jasem Mutlaq authored
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