| 18 | | * psastro fixes: |
| 19 | | * improve the test for the allowed order for a given number of stars, and make the requirements tighter. |
| 20 | | * iteratively remove clumps of objects in the raw and ref tables used for the astrometric match and analysis. This avoids catastrophic failures due to nebulosity and galaxies. |
| 21 | | * add a feature to require a single (closest) reference match in the fitting after the first N clipping iterations. This prevents solutions driven by outliers in crowded fields. |
| 22 | | * some minor tuning of the clipping radii for GPC1 |
| | 18 | * psastro fixes: |
| | 19 | * improve the test for the allowed order for a given number of stars, and make the requirements tighter. |
| | 20 | * iteratively remove clumps of objects in the raw and ref tables used for the astrometric match and analysis. This avoids catastrophic failures due to nebulosity and galaxies. |
| | 21 | * add a feature to require a single (closest) reference match in the fitting after the first N clipping iterations. This prevents solutions driven by outliers in crowded fields. |
| | 22 | * some minor tuning of the clipping radii for GPC1 |