Result for 1E8A90E637F386D187C43AEA792CF493225A05FD

Query result

Key Value
FileName./usr/lib/.build-id/cb/7f8d8443f0924de18b53dd35cb27f50def6ec0
FileSize90
MD58CE170A091EB5B4B84516A8041946B5C
SHA-11E8A90E637F386D187C43AEA792CF493225A05FD
SHA-256F10DB8977619769C401F347B7B977D15B6F6472FB81CE625C36246304F42C49B
SSDEEP3:gCD/9YJgLdWrzxOkLfVY5p:X/9YJgMrdOES5p
TLSHT161B0121481386520F941689A31040800D7411E95B3053E80B33C89B86C409580072B84
hashlookup:parent-total2
hashlookup:trust60

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Parents (Total: 2)

The searched file hash is included in 2 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
MD580120B84160CFFFE4863DA56E4A135E4
PackageArchi586
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.
PackageMaintainerumeabot <umeabot>
PackageNamepython3-ephem
PackageRelease2.mga9
PackageVersion4.1.1
SHA-15E9EFA34EB6A1AB1BAE5DBD7474779409EC1C1B5
SHA-2564407CC9B02D5457AB1FE238116760C2E023ACE0AEDADA124E7FE93F6AE455242
Key Value
MD55340D1965C68812A1D5ACE2912C6635C
PackageArchi586
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-101E36B85EFD4BD4040E69381B279EF795D812976
SHA-25657D96244E16D7BC4ABC7AA0963F39311998DEEDB36F43E7AA290F3E846366FB8