Result for 94028E985554263168FA22C6A4128ED10EC6EF6F

Query result

Key Value
FileName./etc/ld.so.conf.d/ast_i386.conf
FileSize13
MD5FD664DF1FB3B1194F3F47D27B57BA315
SHA-194028E985554263168FA22C6A4128ED10EC6EF6F
SHA-2564C26387699CF6CE130CC380D82F9926E03EA6525883C46168651E1C27691FFFC
SSDEEP3:A+Jn:Agn
TLSH
hashlookup:parent-total12
hashlookup:trust100

Network graph view

Parents (Total: 12)

The searched file hash is included in 12 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
MD576802EE876EB512E7301186FEE73F0F8
PackageArchi686
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease1.fc32
PackageVersion9.1.0
SHA-1C398932EDFE8C409D9506FB32BC1DD1D1587A90A
SHA-256988F25861F19DF80C98AD1FDAD906E131ABC51242FB3310D64CF99E7BDBA9F69
Key Value
MD5F35E877150382B2B0D063C485E01982D
PackageArchi686
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease6.el6
PackageVersion6.0.1
SHA-1F90CC456A471A37DE987F74994D4CF1FB670465E
SHA-2566F986ED8CC7A233204C1DBDBA6389AD1668B79428F50487E440FC46EBD85F197
Key Value
MD58563E49C3089B45AD0874C4131B53542
PackageArchppc
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease1.fc20
PackageVersion7.3.1
SHA-1DBF74B134EFCA9AEF23B58389DD89E50374B4D7E
SHA-2565DED7508E15282B2CB93733DD3A2FA35EA564401322626B95F44C010D25206C7
Key Value
MD5BF9368BB6CA474D7F07866CBE97C8C8A
PackageArchi686
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease2.fc33
PackageVersion9.1.2
SHA-142EE2F6750816FB9B727D031D142428355477103
SHA-25638D67843B205D0D56735BF280A4177D13F6D54861FAFE12E0DC33B986CECD93B
Key Value
MD5E87BAC5A9F6D0494A0D7AA5539785052
PackageArchs390
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease1.fc21
PackageVersion8.0.2
SHA-1DA833DE135CF960453EF20420E120E4621EE3C13
SHA-256C9AF868F4038422AA6A2D97A581CEC4A4A3C09AFA79E7A377C836A0BD29BC473
Key Value
MD56D438374C1CCB1D63A87B8A87BB55EE3
PackageArchs390
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease1.fc20
PackageVersion7.3.1
SHA-1B2877814A6DD14D4085DA470911BA5764D927B29
SHA-25666A5CB76B8B1901C5F26A9FACA362B5303F0BA5FC6B1C4A3B97E691658F64285
Key Value
MD5E470B2F50703234DE973A9424160B09A
PackageArchs390
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease1.fc23
PackageVersion8.0.5
SHA-1228B267BAE2F777201A8617DFDD65CC32218A85D
SHA-2560B866A73EF2ECA46714CE2DA20E61AC78CE9ECCD2A3B47CCE480D88A30B0A5BE
Key Value
MD5EE54C5647FC496780F07987375F84F03
PackageArcharmv7hl
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease2.fc33
PackageVersion9.1.2
SHA-1CE83783689AABE24B32C090261E5DA962D85D90F
SHA-256C1E7A9A22B9E11A6666003D759062403B64CC18907FD6F97E330F1BF2CC6B6DB
Key Value
MD59C6B55686C77051ECD12B4E47654A667
PackageArchs390
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease1.fc22
PackageVersion8.0.2
SHA-111A69F8CE1EBCFC63CEAA1708400A30C9D94F0A1
SHA-256182F752E1FE93E786D29F599111583849F71729424563F5E8510B02CBC76A535
Key Value
MD532DD1124452D749F931AC3A2A98D5C57
PackageArchi686
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease2.fc34
PackageVersion9.2.3
SHA-168A7D5D1040FE5BE4E4D79ACFB9610F14A63965C
SHA-256C84A798BC691E0865E497D374CA1F84811633A7A83A12975028160C7858EB736
Key Value
MD504336281A4B9F4A80DDBB666538F62C6
PackageArcharmv7hl
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease2.fc34
PackageVersion9.2.3
SHA-1D2BC564229B0F21F162DCE69BEAFA313836416CE
SHA-256D6DDA123F4E9B03EC72A7DE5971469C36696EA34D8246FEC959A837DB7BCE58D
Key Value
MD5D48F5C1B08DC4D0BE975A579E57FB21C
PackageArcharmv7hl
PackageDescriptionThe AST library provides a comprehensive range of facilities for attaching world coordinate systems to astronomical data, for retrieving and interpreting that information and for generating graphical output based on it. It's main selling points are: * Ease of use. * Facilities for generating plots of generalized non-linear, potentially discontinuous 2-D or 3-D coordinate systems, with detailed control of the appearance of the plot. * Facilities for converting transparently between different coordinate systems, including a wide range of celestial, spectral and time coordinate systems. * Facilities for searching a general collection of connected coordinate systems for a coordinate system with any given set of characteristics. * Allows code for handling WCS information to be written in a general way without regard to the specific nature of the coordinate systems being handled (i.e. whether they represent sky positions, spectral positions, focal plane positions, pixel positions, etc). * Flexible system for saving and retrieving WCS information, including (but not limited to) a range of different popular FITS descriptions. * Written in C but has interfaces for C, Fortran, Java (via JNI), Perl, and UNIX shell. * Extensive documentation.
PackageMaintainerFedora Project
PackageNameast
PackageRelease1.fc32
PackageVersion9.1.0
SHA-15F38521DC855FE0D877EA6B883998FF31760B114
SHA-256A5639DD7C3BB8423B1CF871023919FF634FE7C2F737F54BE7022BFC9398A8478