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Diffstat (limited to 'gnu/packages/astronomy.scm')
| -rw-r--r-- | gnu/packages/astronomy.scm | 28 |
1 files changed, 28 insertions, 0 deletions
diff --git a/gnu/packages/astronomy.scm b/gnu/packages/astronomy.scm index df3131646b..de37d6b2e6 100644 --- a/gnu/packages/astronomy.scm +++ b/gnu/packages/astronomy.scm @@ -8168,6 +8168,34 @@ Moon position, etc.") any arbitrary astrometric projection defined in the WCS standard.") (license license:gpl3+))) +(define-public tempo + (package + (name "tempo") + (version "13.103") + (source + (origin + (method url-fetch) + (uri (string-append "mirror://sourceforge/tempo/tempo-" + version ".tar.gz")) + (sha256 + (base32 "1ghml56sd7rhwymrlqlvj3g12hjyqvk2sjl08rqlf5y7dwdp0nvl")))) + (build-system gnu-build-system) + (native-inputs + (list gfortran)) + (home-page "https://github.com/nanograv/tempo") + (synopsis "Pulsar timing data analysis program") + (description + "Tempo analyzes pulsar timing data. Pulse times of arrival (TOAs), +pulsar model parameters, and coded instructions are read from one or more +input files. The TOAs are fitted by a pulse timing model incorporating +transformation to the solar-system barycenter, pulsar rotation and spin-down +and, where necessary, one of several binary models. Program output includes +parameter values and uncertainties, residual pulse arrival times, chi-squared +statistics, and the covariance matrix of the model. In prediction +mode,ephemerides of pulse phase behavior (in the form of polynomial +expansions) are calculated from input timing models.") + (license license:gpl2+))) + (define-public unsio ;; There is no versioned tag, use the latest commit. (let ((commit "25e52468298e1194c9726ef5dba9d5fbb46870f5") |