| Key | Value |
|---|---|
| FileName | ./usr/lib64/python3.10/site-packages/ephem/tests/__pycache__/test_usno.cpython-310.opt-1.pyc |
| FileSize | 15237 |
| MD5 | 9239903C79D0CB5B12D66239EC3C023C |
| SHA-1 | 087F56939963A04B0E71A0B171D32EA7C66CAF53 |
| SHA-256 | 180A3F6E66E69C8859D22651514C89862E2CA8CCC2506FBB14891BDE6DE3071B |
| SSDEEP | 384:6xRxwNxwuxvpyWoLIwZstE0UqFpjhPxOFneKQSaq:/OiyHLyJDNPx2neG |
| TLSH | T18D62D7C775935A52FE65F2B6C29822057519F33B2386822F751DF09E0FD05886AB36CC |
| hashlookup:parent-total | 1 |
| hashlookup:trust | 55 |
The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:
| Key | Value |
|---|---|
| MD5 | 1A8974E95D45675DC7A2DD23AEAB49B7 |
| PackageArch | aarch64 |
| PackageDescription | PyEphem provides scientific-grade astronomical computations for the Python programming language. Given a date and location on the Earth’s surface, it can compute the positions of the Sun and Moon, of the planets and their moons, and of any asteroids, comets, or earth satellites whose orbital elements the user can provide. Additional functions are provided to compute the angular separation between two objects in the sky, to determine the constellation in which an object lies, and to find the times at which an object rises, transits, and sets on a particular day. The numerical routines that lie behind PyEphem are those from the wonderful XEphem astronomy application, whose author, Elwood Downey, generously gave permission for us to use them as the basis for PyEphem. |
| PackageMaintainer | neoclust <neoclust> |
| PackageName | python3-ephem |
| PackageRelease | 1.mga9 |
| PackageVersion | 4.1.3 |
| SHA-1 | 737B6A333408601B67D47CCB226C4E8AAC10D54B |
| SHA-256 | 3C3CB6048B5480750012E3DDD1D1174E2930AFCA60C7AFE151ACBE3B9DBE64F0 |