Result for 09C53F2F8DB0C24747E965281AE4221A0AF12661

Query result

Key Value
FileName./usr/lib64/python2.7/site-packages/ephem/tests/test_angles.pyo
FileSize3254
MD5532A0F60C62B19004A26CEF1D1543841
SHA-109C53F2F8DB0C24747E965281AE4221A0AF12661
SHA-256B4628CD753BFE071403F0B8FDF5F15AE1C0102ADF0B69EC8BDEB4B59EDE6F781
SSDEEP96:5gysTgPiigjFudJrDx5rt8vvQ6izargWv1l3Zxl13gSLH:vdCFurgCg1RT
TLSHT1EB619DC1B3A75D4AE8F508B591A0125BFA64E0B3750067C1526C203FAD9C7AAC9BBBC1
hashlookup:parent-total2
hashlookup:trust60

Network graph view

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
MD54AAC3F466621DD864716BBB0F79D2AA8
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.
PackageMaintainershlomif <shlomif>
PackageNamepython-ephem
PackageRelease4.mga7
PackageVersion3.7.6.0
SHA-1D76828413EA337B005070893766F9DA727633524
SHA-25684C0EF1E1702AA966BF070BBDF05B61C66F7B3A7097A89D1551C157EB0BD92C0
Key Value
MD5894C086B6A71A2E1038A6261C577C03D
PackageArchx86_64
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.
PackageMaintainershlomif <shlomif>
PackageNamepython-ephem
PackageRelease4.mga7
PackageVersion3.7.6.0
SHA-13A085053842CD2A584ADFC73D39E1E908EB8629B
SHA-2565710C4859E78747F5826D940B8D434DD9E3E817C02EC7972B359B1779BBB9835