Parents (Total: 29)

The searched file hash is included in 29 parent files which include package known and seen by metalookup. A sample is included below:

Key	Value
MD5	5760C8164B755E019C241913BEE79A6E
PackageArch	aarch64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	2.fc33
PackageVersion	9.1.2
SHA-1	03B2931B014ED6E01B915FB6B6803AB73445B53B
SHA-256	C4C3C21F0C7157857930512B5686918C089DE80F7448FFA4C8234D577EB62910

Key	Value
MD5	184DA5A0D30028CBB7439DFC81267816
PackageArch	aarch64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	2.fc34
PackageVersion	9.2.3
SHA-1	069E80563F8DABE96B8A616798220CD498C43A51
SHA-256	9B3CEDE7D9D50A0D7B0BB2E173829AAB0330D366E9DDA92444D1B2B704518BBB

Key	Value
MD5	989D580CAD0EF30EB993481B8558C370
PackageArch	x86_64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	6.el6
PackageVersion	6.0.1
SHA-1	07496002843D89F83D331CF5D38FC8471D137EFE
SHA-256	D29D72069547A508B6411AEA1B3594422E37C3040D1F8ACF85B508647012D04F

Key	Value
MD5	26FED91B243B7BBA03C583F9531E6DB0
PackageArch	ppc64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	6.el6
PackageVersion	6.0.1
SHA-1	07E899F13C7A9F0C75CD3675D44A89B842E56FF8
SHA-256	EDF1194DD74B2CF9C48380AF34DCAE4B78D24D5AAB69BBF3D3BE0267B00B053C

Key	Value
MD5	8B4B02FEA159184FD77967C2BCC9B9E9
PackageArch	ppc64le
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	3.fc24
PackageVersion	8.0.7
SHA-1	080329274C5CDD130CD890F8B376578419856099
SHA-256	CCBA3BB212A777ABDF076D691DB3523F674310FA02655EE22B6146CF926A19FE

Key	Value
MD5	C0DAA92C4A788F280B666B5CE7581BF1
PackageArch	x86_64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	1.el7
PackageVersion	7.3.4
SHA-1	0B3F32A668C8C623E14D9FC22D3521FE3871FF15
SHA-256	8AA572C32340B8E5EE10FCC46B0EEE5E8791C2011F42B9E9898974D74A241206

Key	Value
MD5	8262138BCEF179EEC0E48AD0C0EFF925
PackageArch	x86_64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	1.fc32
PackageVersion	9.1.0
SHA-1	0BD6AF2FFF99DF62A1F351DB5490A594530257DD
SHA-256	2AD4CA3A79DAD46623DF6C216286A09CC8AA983CFA9A51122BB5BAA461D1BFA3

Key	Value
MD5	5311DF0388F60D14478B4DBA21BFC7B0
PackageArch	ppc64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	1.fc20
PackageVersion	7.3.1
SHA-1	1389C19273340B4673E47C8CE8CFE55A25254AE2
SHA-256	F55F087825CA377056F99F144D4DAA14D578237F19EC34D785AB3A42BFF99F7E

Key	Value
MD5	E35AE7C3D4D4132BD6D9A191D1794B7E
PackageArch	s390x
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	1.fc21
PackageVersion	8.0.2
SHA-1	14473066A31102708DF1638F2A8C013061A8A679
SHA-256	0F8CDC715CBB31A9AE7FE17A2377C3A4BEF66581657EF2FAFFA7ABF6E447C471

Key	Value
MD5	6098749E6A2FCC0D661B539374519D35
PackageArch	aarch64
PackageDescription	The 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.
PackageMaintainer	Fedora Project
PackageName	ast
PackageRelease	3.fc24
PackageVersion	8.0.7
SHA-1	2B7F016104BD74ABD5DABCD95B2AF2BC2AF1B29E
SHA-256	4E436B0EFECE979D00F2440A927C67C0B76198FB241AD87B65A8D753AC8628EA