Result for 08A01ABFA691B631445B93B804ADE6FCD142FB28

Query result

Key Value
FileName./usr/bin/gyoto
FileSize133776
MD5B9291DCD1B6E041C7B6E43CDD18D9AE9
SHA-108A01ABFA691B631445B93B804ADE6FCD142FB28
SHA-2564EED664F48B785BDDAF43C8E15F305960F1448FD6D0F583BBA08D6139446AC1C
SSDEEP3072:mzXXz5sWMSu/AmK7HFZVVsZZdmKQ4ni+bX+7FD5olF11Fl1156iKi6C7iHKe:mzXRmKJhsZZdmBOi0X+BD5olF11Fl11N
TLSHT1A9D3A503BB849D23C8DBCC71481EC20113FEAC8D639A7717355587BC6D566CEAD67A88
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
FileSize128902
MD54D6EB9E02ADE48A72259E367A3E21305
PackageDescriptionGeneral relativistic ray-tracing command-line interface Gyoto is a framework for computing geodesics in curved space-times. The gyoto utility program uses this framework to compute images of astronomical objects in the vicinity of compact objects (e.g. black-holes). Such images are distorted by strong gravitational lensing. The gyoto program takes a scenery description in XML format, computes this scenery using relativistic ray-tracing, and saves the result in FITS format. . This package contains the `gyoto' command-line utility. More complex uses of the Gyoto framework can be achieved using the yorick-gyoto, python-gyoto or python3-gyoto packages. Gyoto can be extended with plug-ins (see libgyoto6-dev). . MPI parallelization requires the mpi-default-bin package.
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamegyoto-bin
PackageSectionscience
PackageVersion1.2.0-2
SHA-15A9FC82D06C7E244B257B86CC81C94150E141781
SHA-2567FE2F42D37554A8F954E4CD6968E805212FE618EB1457E64A86AF1F26096E885