Software
MARS DR2 for Pixinsight Released
Monday, June 22, 2026
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Russ Scritchfield |
Discover how the new MARS DR2 database is advancing gradient correction in PixInsight, offering expanded sky coverage and deeper reference images for astrophotography.
The field of astrophotography and image processing continues to evolve with the second data release of the MARS database, officially available for download through the PixInsight Software Distribution System. This release is designed to seamlessly replace the previous iteration of the database, bringing substantial improvements to the Multiscale Gradient Correction tool. Users can configure the gradient correction tool to utilize the updated database alongside existing resources, streamlining their workflow for greater accuracy. Gradient correction remains one of the most critical steps in astronomical image processing, as it involves the removal of unwanted light signals, such as light pollution or natural skyglow, which can obscure faint celestial details. By relying on a highly objective and meticulously compiled database, photographers can achieve more authentic and reliable representations of the night sky.
The defining improvement in this release is its vastly expanded sky coverage, which directly addresses limitations encountered in earlier versions. The database provides comprehensive coverage of the entire Northern hemisphere in broadband. For narrowband imaging, the coverage extends up to a declination of positive seventy five degrees. Furthermore, the project has broadened its reach beyond the Northern hemisphere, expanding into Southern declinations down to negative fifteen degrees. This expanded coverage is crucial for users who process images captured during the late winter and spring months, seasons that were previously challenging due to a lack of comprehensive reference data. For example, the updated database allows for highly accurate corrections on deep space regions such as the Virgo cluster of galaxies. The source material notes a specific instance where an eighteen hour exposure captured with a 400mm lens revealed faint residual structures, such as stellar streams originating from interacting galaxies, which were preserved and accurately rendered after applying the correction. By providing a reliable reference across such a vast area of the sky, the tool allows users to objectively correct gradients even in images that are entirely filled by large nebulae, ensuring that actual structural details of the objects are not mistakenly removed during the correction process.
Capabilities of the PixInsight MARS DR2 Update for Gradient Correction
The creation of this comprehensive database represents a massive observational and computational effort aimed at achieving the most objective gradient correction currently available to the astrophotography community. The sheer volume of data acquired and processed underscores the dedication required to build such a robust tool. The survey encompasses a total of 1,347 hours of exposure time, gathered across 226 separate nights of observation. This data was collected using a variety of filters, specifically red, green, blue, hydrogen alpha, and doubly ionized oxygen, ensuring a wide spectral range for accurate color and narrowband correction. To maintain the highest possible quality standards, approximately seventy three thousand individual images were subjected to rigorous visual inspection using the Blink tool. This meticulous quality control process ensures that no defective or compromised images are allowed to enter the preprocessing pipeline, thereby protecting the integrity of the final database.
The raw data accumulated for this project reached a staggering 8.4 TB (Terrabyte), which expanded to 12.2 TB during the preprocessing phase. Processing this monumental amount of data necessitated the use of specialized, high performance computing hardware. The project utilized a dedicated server equipped with a 96 core processor, 768 GB (Gigabyte) of RAM, and 64 TB of NVMe storage to handle the intensive preprocessing and database generation tasks. The resulting database is significantly deeper than its predecessor. When the tool corrects gradients, it integrates all the individual master images that cover the specific field of the target image. This integration process creates an incredibly deep reference image. Depending on the specific field and the number of available masters, the new database is two to six times deeper in narrowband and broadband red, green, and blue channels compared to the previous release. Even more impressively, it can be up to eighteen times deeper when using the luminance band. This unprecedented depth is expected to be more than sufficient to accurately correct the vast majority of images produced by the community, allowing for the extraction of even the faintest signals without introducing artifacts or false gradients.
Future of the PixInsight MARS DR2 Update for Gradient Correction
The practical applications of this deep reference data are demonstrated through various examples from the survey. Examination of regions like the Andromeda Galaxy and the Pegasus constellation reveals incredibly faint structures, such as tidal streams and prominent cirrus clouds. Furthermore, the removal of the continuum from broadband filters allows for the clear visualization of faint planetary nebulae and massive supernova remnants, which appear highly detailed against a properly corrected background. Objects that were once exceptionally difficult to process cleanly can now be handled with a much higher degree of confidence and objectivity. Looking ahead, the project shows no signs of slowing down. The team plans to continue acquiring images from the Northern hemisphere for at least another full year, further densifying the data and improving the reference models. The future roadmap includes expanding the overall coverage by incorporating additional data sources and beginning development on a new mosaic generation tool based on this vast repository of objective sky data.
- DRAFT COPY ONLY -
