KStars v3.7.6 is released on 2025.04.01 for Windows, MacOS & Linux. It's a bi-monthly bug-fix release with a couple of exciting features.
Scheduler Plans Visualized
Hy Murveit added a graph to the Scheduler page that displays visually the scheduler's plans--the same plans described in the log at the bottom of that page, and partially described in the scheduler's table. You can see altitude graphs for all the scheduler jobs, which are highlighted in green when that job is planned to be active. The next two nights of the plan can be accessed using buttons to the right (and left) of the graph. The graph can be enlarged or hidden by sliding the "splitter" handle above it up or down.
PHD2 & Internal Guider RMS
Many users reported differences between the RMS value reported by Ekos internal guider vs PHD2. This is not a new issue as there was a difference in RMS calculations ever since Ekos Guider module was developed over a decade ago. In this release, we updated the internal Guider RMS calculations to use the same algorithm used by PHD2. This way, there is now a more consistent metric to judge the performance of the two guider systems.
Weather Scheduler Integration
Weather station integration with the scheduler was improved. The weather enforcement is now global and not per job. If weather enforcement is enabled, you can adjust the Grace Period (default 10 minutes) in cases where the scheduler cannot be started due to a weather Alert or Warning.
When a weather warning is received, existing jobs can continue to execute but new jobs will not be executed until the weather situation improves. Upon detecting a weather hazard, the scheduler execute a Soft shutdown mode where it can park the mount and dome, but still retains connection with INDI drivers to continue monitoring the weather situation. If the weather does not improve by the Grace Period, it then commences a full shutdown of the observatory. Otherwise, it should resume the job from where it was left.
Contrast Based Focusing
John Evans added an option to allow focusing on non-star fields by using various contrast based algorithms. This is suitable for Lunar, Solar and planetary imaging.
Autofocus Optimization
John Evans added an option has been added to Focus that allows an Autofocus run to re-use a previous successful Autofocus result if the previous AF run occurred within a user-defined time period, say <10mins ago. This can speed up certain situations when using the Scheduler where multiple Autofocus requests can happen within a short period of time.
Imaging Planner Improvements
Hy Murveit pushed a new Imaging Planner catalog release along with improvements to the KStars Imaging Planner.
It should now start up much more quickly on first use, or first use after a catalog upgrade.
There were stability improvements.
The catalog was extended to include 770 objects.
Upgrade to KStars 3.7.6, use Data -> Download New Data to get the latest Imaging Planner catalog, and run Load Catalog in the Imaging Planner tool to take advantage of all these improvements.
Quick Go & Rotate
Added support to Go and Rotate in Framing Assistant. This would command fast go to target and then followed by rotation to match position angle indicated. Simply adjust the Position Angle to your desired angle then command Ekos to solve and rotate in one go.
Scheduler Coordinates Flexibility
Wolfgang Reissenberger introduced enhancements for handling target coordinates in the scheduler module:
Add an option to switch the target coordinates between J2000 and JNow. This is interesting for those cases where the user wants to enter the coordinates manually, but has the coordinates only in JNow - for example when taking them over from the align module.
Add a "use the current target" button. Currently, there is only an option to take over the current skymap center.
Furthermore, during the time where the moon is visible, it should be possible to schedule only those jobs that are not disturbed by moonlight (e.g. H-alpha captures). To enable this, a new optional constraint is introduced where the maximal moon altitude could be set.
Use PHD2-scheme graph
Toni Schriber modified the internal guider chart to use PHD2-scheme (RA/DEC) for graph of guide mount drift. This should help comparisons between PHD2 and internal guider more consistent.
KStars v3.7.5 is released on 2025.02.03 for Windows, MacOS & Linux. It's a bi-monthly bug-fix release with a couple of exciting features. Here are the release notes organized by developer.
Jasem Mutlaq
Added dome slit visualization on sky map. Specify the Dome Measurement parameters in the INDI Dome driver to see a live dome slit overlay in the Sky Map.
Implemented generic DBus methods for KStars options
Added SchedulerSleeping event
Added mutex protection for multi-threaded resources
Enhanced scheduler loading and settings management
Improved filter manager operations
Fixed video subframing. Up to 50x improvement in subframed video feeds.
Fixed multiple profile editor issues
Added VSCode development setup support
Hy Murveit
Fixed DMS delta angle calculation
Added mandatory settle to PAA
Improved imaging planner stability
Fixed pierside placeholder directory usage
Added START_AT scheduler test
Fixed Abell planetary nebula lookup
Enhanced PAA adjustment estimation
Wolfgang Reissenberger
Implemented video sequence capture. Preliminary support for capturing Video files as regular sequences in the Capture module. Great news for EAA.
Fixed focus options
Improved remote directory handling
Fixed flats with wall position
Enhanced filter wheel integration
John Evans
Enabled focuser controls when camera disconnected
Improved focus measure framing
Fixed focus advisor code warnings
Updated aberration inspector functionality
Toni Schriber
Fixed overshooting cosine in CachingDms calculation
Implemented calibration reuse after rotation. Guide calibration data can now be re-used between sessions after rotation.
Ben Cooksley
Removed CMake trace/debug logs from CI runs
György Balló
Set window icon
Oliver Kellogg
Fixed typo in FITS Viewer configuration
Akarsh Simha
Fixed right-click popup menu on deep stars
Technical Highlights
Improved capture sequence stability: Set 5-minute timeout for transient operations (dome motion, mount parking/unparking, dust cap operations, focusing, filter wheel changes) to prevent indefinite sequence stalling.
Improved mount rotation processing
Enhanced scheduler loading mechanism
Added mutex protection for multi-threaded resources
KStars v3.7.4 is released on 2024.12.05 for Windows, MacOS & Linux. It's a bi-monthly bug-fix release with a couple of exciting features.
Imaging Planner
Hy Murveit added a brand new Imaging Planner in KStars to facilitate imaging.
The Imaging Planner tool helps users choose which objects to image. Users can download catalogs of recommended objects, or possibly create and share their own catalogs. The tool computes when the objects in a read-in catalog may be imaged on the selected night given constraints such as minimum altitude, terrain and moon separation.
It can sort the objects along several different dimensions including the number of hours an object may be imaged tonight (given the users geography, constraints and possibly artificial horizon), its peak altitude, distance from the moon, constellation, name and type. Objects can also be filtered out for several reasons (e.g. type of object, whether it was previously imaged, keywords the user has added, whether the object has been selected, user not interested, etc).
This tool helps users research the objects by showing small images of the objects, showing the objects' sky locations on the skymap, and by providing links to follow to internet sites with more information and images. It allows users to attach notes and links to objects, and select certain of them for further consideration. This tool can be used in conjunction with the Ekos imager or any other imaging tool. It does not currently directly interact with the actual imager; it only helps the user decide what to image.
Simbad Integration with FITSViewer
John Evans added a new, experimental feature to the FITSViewer that allows the user to dynamically query the SIMBAD astronomical database and highlight the results on the image in the FITSViewer. The user draws a circle on the image and the objects within that circle are then displayed in a table and on the image.
It is possible to filter by object type and click through to the Simbad / CDS or NED websites for more information about the objects.
This is an interesting tool to see what is in your image, be it a subframe whilst you are imaging or a completed image that you have reloaded into the FITSViewer.
In order to use the feature you will need an internet connection to access the online Simbad database and an image must have WCS enabled within the FITSViewer. For the most accurate results, plate solve the image with the build-in FITSViewer plate solver. The feature is controlled by a toggle in the FITSViewer options.
New Focus Measures
John Evans introduced a new contrast based focusing algorithm suited for solar and planetary imaging.
4 new focus measures have been added to the Focus Module to complement the existing measures of HFR, FWHM, etc. · StdDev. This is similar conceptually to the Fourier Algorithm but is simpler. It uses an algorithm based on the standard deviation of the pixels in the image as the measure of focus. It can be used on star fields. · Contrast based measures use algorithms that can be found in other areas of image processing and uses the contrast of texture in the image in various way as a measure of focus. The following measures are available:
o Sobel o Laplassian o Canny
These measures require some form of extended object in the image so will not work on star fields. They are intended for Solar, Lunar and planetary focusing.
These algorithms can be used on the whole image or with the existing mask features, or with a user-defined region-of-interest that is used in single-star mode for star based focusing measures.
This new feature requires the openCV library to be installed (a standard installation is fine). This library is not installed by default with Kstars so anyone wishing to use these features will need to first install openCV and then rebuild Kstars on their system. It will not be available with pre-built executables.
KStars v3.7.3 is released on 2024.10.03 for Windows, MacOS & Linux. It's a bi-monthly bug-fix release with a couple of exciting features.
Extension Interface
Ed Lee contributed the Extension Interface for KStars.
Extensions are small programs that can be added to interact with KStars/Ekos/INDI in order to provide extra functions and features. Extensions are separate from KStars. They are not provided as part of this software. Only a means to call them is provided for convenience. Make sure that you understand the requirements and risks of using an extension.
FireCapture launcher (FC_launcher): disconnects the current primary camera INDI driver and launches FireCapture. Upon close restarts the INDI driver.
KStars Backup (KS_backup): provides a GUI for the archiving and restoration of KStars/INDI (and optionally others) configuration directories to/from .tar.gz archives/
Sirial_EEA: provides live stacking of the preview job from the Capture Module and displays it auto-stretched in the Ekos preview window.
Each extension must have a companion configuration file also located in the extensions directory, named the same as the executable with the addition of a .conf eg: an extension named example must also have a configuration file named example.conf A configuration file is a plain text file that provides configuration settings to the extension program and usage information to the user. A configuration file is only valid if it contains a line starting with: minimum_kstars_version=x.y.z The x.y.z is the minimum release of KStars that the extension is designed/tested against. This value is checked against the current KStars KSTARS_VERSION macro defined in version.h and must be equal or lower for the extension to be considered valid. The extension should also check that this minimum_kstars_version string matches what it expects.
Optionally each extension can also provide an icon file for display in the Extension drop down list. Again the naming should match the extension executable with a valid file extension (.jpg, .bmp, .gif, .png or .svg) and be placed in the same extensions directory. A default icon is used for any extension that does not provide it's own icon.
Several new DBus functions/signals are added to enable general extension use and for a specific upcoming extension.
Multi-Target Scheduler
Wolfgang Reissenberger continued the development of multi-camera acquisition and now scheduling with many exciting updates!
Multi-Camera Scheduling
With this new release it is possible to create and run schedules for two or more optical trains in parallel within the same KStars instance. All mount related events like slewing, dithering, alignment and meridian flip are synchronized, i.e. capturing on all optical trains takes these events into account.
Lead and follower jobs
If you want to run capturing on multiple optical trains in parallel, you need to decide, which of the optical trains is the lead job, which defines the target and the scheduling criteria. All other optical trains will be follower jobs, for which only the capture sequence to be used is relevant.
Job Synchronization
Ekos ensures that no mount motion happens while one of the optical trains is capturing to avoid star trails.
In case of dithering, the capture module decides what to do as soon as dithering is requested, depending on the setup of the lead job. If the remaining capture time of a follower train is more than 50% of the lead job exposure time, capturing of the follower train is stopped and restarted after dithering. If the remaining capture time is less than 50%, the Capture module waits for the follower to finish its capture.
For the meridian flip and re-alignment: both are controlled by the lead job. All running follower capturing sequences are stopped and restarted after a successful completion of the respective action.
Recommendations
The lead job should have the longest exposure times, especially if dithering is used.
If you use re-focusing, consider to not suspend guiding during focusing, since the other optical train might capture in parallel.
Configure the same optical train in the Align module that you use in the lead job. This is important if you use the re-alignment check option of the scheduler.
Do not use the Force re-alignment before re-starting jobs, since each new iteration of the lead job stops capturing of the follower trains. Consider using Verify captured image position every n frames instead, since this option triggers re-alignment only if it is necessary.
Adhoc focus with Multi-Camera setups
Wolfgang Reissenberger added support for simultaneous parallel focusing when you are running multi-camera setup. It would be a good idea to disable Suspend Guiding so that guiding is unaffected when focusing operation commences.
Invent Multi-Star Guide Star
Hy Murveit introduced an experimental Multi-Star parameter. In the original (conservative) multi-star guiding implementation, although many stars contributed to the computed guiding drift computation, there still was one more important star that anchored the scheme.
With this change, all the guide stars contribute equally to the guiding calculations. This removes the risk that an unfortunate selection of a double star for the more-important main guide star would degrade performance.
KStars v3.7.2 is released on 2024.08.03 for Windows, MacOS & Linux. It's a bi-monthly bug-fix release with a couple of exciting features.
A few members of the KStars development team were enjoying their summer holidays over the past few weeks, but we still have a couple of exciting features in this release!
Multi-Camera Support
Wolfgang Reissenberger devoted countless hours to bring this complex feature that required lots of architectural changes in Ekos. If you have double rigs (or even more), we have a new great feature: multi camera support! If you have more than one optical train on your mount, you now will be able to run capture sequences for each of your optical trains in parallel from the same KStars instance. You simply need to create an optical train for each of your telescopes on your mount, create camera tabs for each optical train, create their own sequence and let them run in parallel.
This new feature may also be used in combination with the scheduler: in this release, the scheduler itself will control the first camera. On top of that, you could configure additional cameras in the capture tab which could execute their own capture sequences. Enhancing the scheduler such that it could control multiple optical trains in parallel is already under development and will be part of one of the next releases. So stay tuned!
Focus Advisor v4
John Evans refactored the Focus Advisor to make it simpler while still offering a lot of insight on parameters tuning. It is now more accessible to new users and has added functionality to optimize values for 2 of the more difficult Focus parameters: Step Size and Backlash (or AF Overscan).
In addition, Focus Advisor contains a convenience tool to locate stars by searching the range of motion of the focuser and another convenience tool to highlight differences between current Focus parameter settings and those recommended by Focus Advisor.
KStars v3.7.0 is released on 2024.04.05 for Windows, MacOS & Linux. It's a bi-monthly bug-fix release with a couple of exciting features.
CI & CD Infrastructure
We say goodbye to KDE's binary factory as we transition to fully use Gitlab's CI/CD pipelines to build, test, and publish KStars. Over the last two months, Eric Dejouhanet worked with the KDE's Craft & System admin teams to transition KStars pipelines to the new framework.
Short status on pipelines:
Merge requests run the custom build and the CI builds
Master runs the CI build (though there could be other things we run, such as CVE scans)
Craft recipes are run from the last commit of the master or release branch, they require "build" and "build-and-test-stable" to be run manually beforehand.
Publishing to Microsoft store is available after the Windows Craft is run.
This is still an ongoing process and we hope to have this process fully automated by 3.7.1 release where we will automatically publish latest releases for both stable and master branches.
Donut Buster
Rejoice Newtonian, SCT, and RC owners! With KStars new Donut Buster feature, your donut focusing woes might be something of the past. John Evans implemented this experimental feature to help protect against outliers that might affect your autofocus routine. In addition to that, the Focus Advisor is now automatically applied when creating new profiles. Based on the type of equipment you have in your optical train, the Focus Advisor would try to guess the optimal focus settings for your setup. Both features are experimental and would benefit from your feedback.
Custom Views
Akarsh Simha introduced the ability to orient the sky map to match the view through any instrument.
A view is a collection of settings: the orientation of the sky map, how the orientation changes as the sky map is panned, whether it is mirrored or not, and optionally the field-of-view to set the map to.
If no views are defined, KStars introduces a set of standard / "demo" views by default. Existing views can be edited and new views can be added using the "Edit Views..." interface. They can also be re-ordered in the interface. The ordering of the views in the "Edit Views..." dialog defines the order in which views will be cycled through using the keyboard shortcuts Shift + Page Up and Shift + Page Down. Thus, you can set up the views for easily switching between naked eye / finder scope / telescope views for easy star-hopping.
Furthermore, there is a new option in the View menu that enables mirroring the sky map so as to be able to match the view through an erecting prism used for example on a Schmidt-Cassegrain or Refracting type telescope.
The rotation feature overlay now also marks East in addition to north and zenith, so as to know easily whether the display is mirrored or not.
Blinking
Hy Murveit added a very useful Blinking feature to the FITS Viewer tool. This adds several ways to blink; that is, compare multiple images.
In Analyze, one can now move from one session to the next (forward or backward). Keyboard shortcuts are provided for that.
Another set of keyboard shortcuts both advance and show the next image in the same FITS Viewer.
Thus, for example, one can advance through all the captured images of the evening, showing all the captures on the FITS Viewer by repeating a keyboard shortcut.
A useful complement to this might be adding the ability to delete bad captures, but for now that will have to wait for a rainy day.
In the FITS Viewer, the Open File menu command (both in the main KStars top menu, and in the FITS Viewer menu) now allows multiple files to be selected. If they are then the files are opened in individual tabs.
Shift-selecting would select files from the first to the shift-clicked file. Clearly one wouldn't want to select 100 files resulting in 100 tabs, but this can be used to, e.g. compare 10 images.
Going along with the above, keyboard shortcuts have been added to move to the next or previous FITS Viewer tab, Also helpful to the above is a new command to zoom in/out all tabs (not just the current one).
There is a new Blink Directory menu command (in both menus, as above) which will open a single tab with a list of all the images below the directory selected (that is, both in that directory, and in directories below it). It initially displays the first image, but new commands work in that tab to switch to displaying the next (or previous) image file in the list. This could be used to blink hundreds of files.
Sky Flats
Dušan Poizl added an option to capturing sky flats. When shooting flats at sky it often end up in never-ending loop of adjusting exposure because intensity of light change and calculation of exposure break down. Adjust the tolerance to 2000 ADU to higher for a better chance at capturing sky flats.
Scheduler Refactor
Wolfgang Reissenberger continues with his work on Separating Business Logic from UI in Scheduler. Over the years the Scheduler has grown to one of the most complex classes. With this release we refactored the Scheduler class and separated the UI from the underlying state model and its business logic. This opens the door for future development of new scheduling features and a much modular approach towards more flexible sequencing approaches.
Standalone Editor
To add any job to the scheduler, you need at minimum the following:
Target
Sequence File
The sequence file contains all your sequence settings (e.g. Capture 20x15 LRGB images). To create this file, you first need to add sequence job in the Capture module and then save the corresponding sequence. While this facilitates re-usability across different sessions, some users wanted to create sequence on-the-fly in the scheduler.
Hy Murveit developed the standalone sequence editor in the scheduler module where it relies on settings saved from your last astrophotography session. Now it's easier than ever to plan scheduler jobs without having Ekos or your equipment profile running!
KStars v3.6.8 is released on 2023.12.03 for Windows, MacOS & Linux. It's a bi-monthly bug-fix release with a couple of exciting features.
Aberration Inspector
John Evans introduces the very exciting Aberration Inspector tool. The Aberration Inspector is a tool that makes use of Autofocus to analyze backfocus and sensor tilt in the connected optical train. It solves up to 9 virtual tiles on the sensor as defined by the existing Mosaic Mask.
The information is then used to analyze:
Back focus.
Sensor Tilt.
There are 4 sections:
V-curve for the each tile.
Table of data detailing the curve fitting results.
Analysis of back focus and tilt.
3D Surface graphic to explain the Petzval Surface intersection with the sensor.
This release provides display only functionality. In future it would be possible to add functionality to offer recommendations for adjustments using Octopi, PhotonCage, etc.
Sub-exposure Calculator
Joseph McGee continues to add improvements and fixes for the Sub-exposure calculator. For usability, the window is now re-sizeable, an issue with the display of tool tips was corrected, and an indicator has been added for the sensor type of the selected camera (Mono / Color). For functionality: the upper limit of the Noise Increase input parameter was increased, support was added for cameras with non-variable read noise, (cameras with CCD sensors).
Several new camera data files were added to the KStars source code repository, and a function to allow direct direct download of camera files from the repository was enabled. (Note: users who have created their own camera data files, may wish set the file attribute to read-only, and/or make a back up copy in case of an accidental over-write from the download function if the camera file has the same name).
A new experimental graphical tool to determine an appropriate number of sub-exposures for integration was added. This tool allows the selection of an exposure time to noise ratio for a stacked image; the tool will compute the number of sub-exposures required to achieve that value.
Hy Murveit added a very useful feature to the FITS Viewer: a built-in solver!
The FITS Viewer Solver is used to plate-solve the image loaded in the FITS Viewer's tab. It only works with the internal StellarSolver. You get the RA and DEC coordinates for the center of the image, the image's scale, the angle of rotation, and the number of stars detected in the image. Its main use case is debugging plate-solving issues in Ekos, though the information displayed can be generally useful. The controls and displays are described below.
This adds a new tool inside the splitter on the FITS Viewer. It plate-solves the displayed image, and allows the user to experiment with a number of plate-solving parameters, and thus help debug plate-solving issues.
How to test it out?
Open the sliding panel on the left part way, click on Plate Solving, and resize the windows appropriately.
Experiment with the parameters available (Use Scale, Use Position, the scale and RA/DEC positions, choose a profile and/or edit it)
Click Solve, and the image is solved and the solution presented in the Scale and RA & DEC and Angle boxes.
If you enable "Mark Stars" above the image window, you will also see the stars that were detected.
Quality of Life improvements
Make "Set Coordinates Manually" dialog more intuitive.
Telescope name specified in the optical trains are now saved in the FITS header (the mount name was saved before).
New placeholders for ISO, binning and pure exposure time added.
Add a new not-default scheduler option to disable greedy scheduling.
Reduce latency between captures, especially when guiding / dithering.
Fix issue with differential slewing.
Separate Business Logic from UI in Scheduler.
Fix bug in estimating job time, capture delays were misinterpreted.
Fixed guide start deviation was not saved properly in esq file.
Bugfix in one-pulse dither. Dither pulses were going the wrong way.
Fix Scheduler hangs when Focus does not signal Autofocus start failure.