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J/A+A/537/A67  MESS: Multi-purpose Exoplanet Simulation System (Bonavita+, 2012)

A Monte Carlo tool for the statistical analysis and prediction of exoplanets search results. Bonavita M., Chauvin G., Desidera S., Gratton R., Janson M., Beuzit J.L., Kasper M., Mordasini C. <Astron. Astrophys. 537, A67 (2012)> =2012A&A...537A..67B
ADC_Keywords: Stars, double and multiple ; Planets Keywords: brown dwarfs - methods: statistical - methods: data analysis - planetary systems Abstract: The high number of planet discoveries made in the last years provides a good sample for statistical analysis, leading to some clues on the distributions of planet parameters, like masses and periods, at least in close proximity to the host star. We likely need to wait for the extremely large telescopes (ELTs) to have an overall view of the extrasolar planetary systems. In this context it would be useful to have a tool that can be used for the interpretation of the present results, and also to predict what the outcomes would be of the future instruments. For this reason we built MESS: a Monte Carlo simulation code which uses either the results of the statistical analysis of the properties of discovered planets, or the results of the planet formation theories, to build synthetic planet populations fully described in terms of frequency, orbital elements and physical properties. They can then be used to either test the consistency of their properties with the observed population of planets given different detection techniques or to actually predict the expected number of planets for future surveys. In addition to the code description, we present here some of its applications to actually probe the physical and orbital properties of a putative companion within the circumstellar disk of a given star and to test constrain the orbital distribution properties of a potential planet population around the members of the TW Hydrae association. Finally, using in its predictive mode, the synergy of future space and ground-based telescopes instrumentation has been investigated to identify the mass-period parameter space that will be probed in future surveys for giant and rocky planets. Description: All the IDL routines needed to run the MESS code are included, together with a script providing an example of its use, and all the necessary input files. Save all the file in the same directory, or add the directory where the .pro files are extracted to your IDL path. A step by step tutorial, further examples and newer versions of the code can be downloaded from www.messthecode.com Please send an email to for any suggestion/request. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file list.dat 90 6 List of files in prog subdirectory prog/* 0 6 All files related to the code
Byte-by-byte Description of file: list.dat
Bytes Format Units Label Explanations
1- 20 A20 --- FileName Name of the file in subdirectory prog 26- 90 A65 --- Title Title of the file
Acknowledgements: Mariangela Bonavita, mariangela.bonavita(at)gmail.com
(End) Patricia Vannier [CDS] 10-Nov-2011
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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