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Notice about FITS format
Note that if you're uploading a FITS, only monochrome 8/16 bit FITS images are supported.

Blind parameters

Please choose a value between 0 .. 1200
Please choose a value between 0.20 .. 30.00
Please choose a value between 1.00 .. 30.00
Please choose a value between 0 .. 3
Please choose a value between 0 .. 3
Please choose a value between 1 .. 16

Help


Maximum number of stars to use:

The maximum number of stars to take from the image to be used in the solving process. The stars are picked in the order of magnitude, brighter/bigger stars first.

The more stars are used, the more calculations need to be made, but larger star counts also improves the chance of success especially with wide-field images.

Default value is 0, which lets the solver decide based on the number of stars detected in the image.

Minimum field radius (degrees):

The minimum field radius to try, in degrees. The search moves from large field radiuses to smaller ones, i.e. 8, 4, 2, 1, 0.5 degrees and so on. This is the minimum field radius to try.

The smaller the minimum radius, the more work needs to be done. The amount of work increases exponentially.

Default value is 0.5. For images that have a smaller field radius, this need to be lowered. There also needs to be sufficiently high quad densities in the quad database in order for very small field radiuses to be solvable.

Maximum field radius (degrees):

The maximum field radius to try, in degrees. The search moves from large field radiuses to smaller ones, i.e. 8, 4, 2, 1, 0.5 degrees and so on. This is the maximum field radius to try.

Default value is 8.

Include lower quad densities:

The catalog star -based quad database has been split into passes, with different quad densities per square degree. When searching for matches, the algorithm measures the image's quad density and then tries to use the best available database pass with the quad density as close as possible to the image's.

However it's likely that the densities are somewhere in between two passes. An offset of 1 will include one lower quad density database quad pass into the search. More passes can be included as well, but it's usually not very beneficial and it increases the number of calculations that needs to be made.

Default value is 1.

Include higher quad densities:

The catalog star -based quad database has been split into passes, with different quad densities per square degree. When searching for matches, the algorithm measures the image's quad density and then tries to use the best available database pass with the quad density as close as possible to the image's.

However it's likely that the densities are somewhere in between two passes. An offset of 1 will include one higher quad density database quad pass into the search. More passes can be included as well, but it's usually not very beneficial and it increases the number of calculations that needs to be made.

Default value is 1.

Database quad sampling:

Sampling allows the solver to use less database quads per run when trying to find matches. For example, with a sampling value of 4 only 1/4 of the quads available in the database are used per run in trying to find a solution. If a solution is not found with the first 1/4 of the quads, then it moves on to test the next 1/4 and so on.

Because a smaller number of calculation needs to be made per run, a sampled run is faster and may yield a result much faster - only a single potential quad match needs to be found in order to trigger a full matching operation, and if a solution is then found a lot of time has just been saved.

Default value is 6.

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