Result for 087F56939963A04B0E71A0B171D32EA7C66CAF53

Query result

Key Value
FileName./usr/lib64/python3.10/site-packages/ephem/tests/__pycache__/test_usno.cpython-310.opt-1.pyc
FileSize15237
MD59239903C79D0CB5B12D66239EC3C023C
SHA-1087F56939963A04B0E71A0B171D32EA7C66CAF53
SHA-256180A3F6E66E69C8859D22651514C89862E2CA8CCC2506FBB14891BDE6DE3071B
SSDEEP384:6xRxwNxwuxvpyWoLIwZstE0UqFpjhPxOFneKQSaq:/OiyHLyJDNPx2neG
TLSHT18D62D7C775935A52FE65F2B6C29822057519F33B2386822F751DF09E0FD05886AB36CC
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

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
MD51A8974E95D45675DC7A2DD23AEAB49B7
PackageArchaarch64
PackageDescriptionPyEphem 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.
PackageMaintainerneoclust <neoclust>
PackageNamepython3-ephem
PackageRelease1.mga9
PackageVersion4.1.3
SHA-1737B6A333408601B67D47CCB226C4E8AAC10D54B
SHA-2563C3CB6048B5480750012E3DDD1D1174E2930AFCA60C7AFE151ACBE3B9DBE64F0