Bayesian age and mass estimates for transiting planet host stars
Source code, makefile and README for installation of software used for the analysis in Maxted, Serenelli & Southworth, "Bayesian mass and age estimates for transiting exoplanet host stars", A&A 575, 36, 2015.
Manuel, tables et logiciels de navigation astronomique
SSynth is a package of scientific software consisting of shell scripts and fortran source code for efficiently calculating a model stellar spectrum using the standard LTE, homogenous, and plane parallel approximations.
RT is the world's fastest and most accurate simulation of astrophysical radiative transfer. RT includes C++ implementations of the Mersenne Twister and R250/521 RNGs, and the best-known BSP traversal algorithm.
XAudine : Linux control command software,GUI and device drivers for operating Audine astronomy CCD camera.
Implementation in Python of some of the statistical methods provided by "asurv", the survival analysis software.
simulation of objects in space with classical mechanics
astronx simulates the motion of mass-centres in cartesian space. The mass-centres interact solely through gravity. astronx uses the Bulirsch-Stoer extrapolation algorithm with adaptive stepsize to integrate the newtonian equations of motion.
PARAMESH is a package of Fortran 90 subroutines designed to provide an application developer with an easy route to extend an existing serial code which uses a logically cartesian structured mesh into a parallel code with adaptive mesh refinement(AMR).
This is a project to prove the existence of space travel by observing the international space station. This will include some history about non-believers, maths and a program to calculate the heigth and velocity of the ISS.
This library is a Fortran 95 gnuplot interface for some Unix like OS'es. This provides some routines that enables direct access of a child gnuplot session from a Fortran 95 program. You will need a copy of fortranposix to make this work.
Data, catalogues and code for analyzing the Sloan Digital Sky Survey (SDSS) Quasar data. The resources presented here were published by Ross et al. in the Astrophysical Journal, 2009, Vol. , / .
SIGPROC - a collection of signal processing programs developed for pulsar data reduction has been developed and maintained since 1999. The package is used to search for and visualize the presence of pulsed signals in noisy radio astronomy data.
Working group working in the compilation and development of tools for stellar evolution
PSRPOP - a package to simulate radio pulsar populations has been undergoing development and use since 2003. The package is used to infer the underlying properties of pulsars and help make predictions for future surveys.
OpenWD is a scientific project to develop state-of-the-art models of white dwarf stars, to draw upon the collective expertise of astronomers around the world, and to facilitate comparisons between evolutionary and pulsational studies of white dwarf stars
FreeEOS is a Fortran library for calculating the equation of state using an efficient free-energy minimization technique that is suitable for physical conditions in stellar interiors.