2026-10-09 APP 2.0.0-beta48 has been released !
This is mainly a bug fix release for the reported bugs in beta47. In addition it has a significant User Interface performance improvement noticable when you need to process 1000s of images in APP.
2026-10-03 APP 2.0.0-beta47 has been released !
This is a very big release... many code optimizations/rewrites, many parts of APP are much faster and more precise, especially star analysis and registration are much faster ! Big mosaics will go much faster 🙂
And we introduce a new preview filter, which includes the new Adaptive Deep Sky Stretch and a General Levels Stretch, this has been long over due. The old preview filter (the panel on the right side to stretch and preview your data) has not been updated for a couple of years and it is a critical part of any APP session.
Adaptive Deep Sky Stretch or ADSS is a much more intuitive stretch algorithm. It is also color preserving (which is a great new addition in itself ! ) which means that the highlights are no longer bleached, color is maintained from the linear data while stretching. You can simply stretch your data using the sky background level and signal width sliders which work much easier and more intuitive. You no longer need to fiddle with the old complicated sliders with zoom buttons. All the zoom buttons for the sliders are made redundant. And you can enter slider values in the slider value fields yourself. I will make a youtube video in the coming days to explain and fully introduce ADSS. Once the video is ready, it will be highlighted on the forum.
RGB Combine upgrade !. The RGB Combine Tool has been rewritten mostly. The tool is faster and easier to use and most importantly, the Luminance slider to inject a luminance channel or channels into the RGB composite is now working correctly. It no longer bleaches the RGB colors. Combined with the new ADSS preview, you will get much better and easier great composites with great color! I will also explain this in a new youtube video.
There is currently an initiative to make better use of the TIFF format for astronomy.
The idea is to save a FITS header in a standard way into a TIFF file. This makes conversion between TIFF and FITS possible without loosing header information.
The FITS header is stored in the description tag of the TIFF file.
The specification is here:
http://www.hnsky.org/astro-tiff.htm
Benefits:
- The TIFF compression algorithm makes the files smaller
- The files are readable by almost any image viewer.
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The standard way is intended to be used for light, dark, flat and flat-darks. These files are normally written in large quantities and compression and viewability makes sense.
Already some application developers are working on support. See the list at end of the specification in above webpage. For APP the only requirement would be to read TIFF and decode the tag description containing the header information in a string and decode information like date, exposure, gain, sensor temperature.
The specification is not set up as a replacement of FITS. It just propose better of use of the existing TIFF file format.
Han
www.hnsky.org
