Result for 169F0C6AC27F5E7089546CF26257CF938EE0EB15

Query result

Key Value
FileName./usr/lib/python3.10/site-packages/ephem/__pycache__/cities.cpython-310.pyc
FileSize8952
MD59973DB596D4EE291C82C53867ABF1B1E
SHA-1169F0C6AC27F5E7089546CF26257CF938EE0EB15
SHA-256A34CA8127516CB603636A6C71BF8D64C34BF5FDFFC60127D3A22CFD6CD3BB22E
SSDEEP192:yG33HMJC52OxN4VL9QPRRXtlxk9Rm8i0CtX61Eou4okkxKRkaLRkqU:yO3lEEmPQpRXtrk9Rm8t1EZPkkERkis
TLSHT1BE026EC84B5290C1E241F13F9562CC9D6661A2EFB31934C097ECB2F42DE3E489E27982
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
MD528648970FEE5B74BCAF3440DD3275D77
PackageArcharmv7hl
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-104FF49D41D51ABA9D569C14B1DEA47E5179721EB
SHA-256755938854A158ED98309F5DBEC9A404FDF3B142247DA71A45483CF72F2811575