Python and XML for Agile Scientific Computing
To set up a mock data challenge, the authors needed to string together a lot of existing and new code. In the mock LISA data challenges (MLDCs; http:// astrogravs.nasa.gov/docs/mldc), the challengers distribute several simulated LISA data sets to challenge participants; the data include GW signals f...
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| Published in | Computing in science & engineering Vol. 10; no. 1; pp. 80 - 87 |
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| Main Authors | , |
| Format | Journal Article |
| Language | English |
| Published |
New York
IEEE
01.01.2008
The Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subjects | |
| Online Access | Get full text |
| ISSN | 1521-9615 1558-366X |
| DOI | 10.1109/MCSE.2008.20 |
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| Abstract | To set up a mock data challenge, the authors needed to string together a lot of existing and new code. In the mock LISA data challenges (MLDCs; http:// astrogravs.nasa.gov/docs/mldc), the challengers distribute several simulated LISA data sets to challenge participants; the data include GW signals from sources of undisclosed parameters as well as realistic instrument noise. Participants must analyze the data and report their estimates for the GW source parameters. These challenges are meant to be blind tests but not really contests: their greatest benefit comes from the quantitative comparison of results, analysis methods, and algorithm implementations. The laser interferometer space antenna (LISA), a space-borne GW observatory planned jointly by NASA and the European Space Agency, will assuredly detect a wide variety of GW sources throughout the universe, thanks mostly to the quietness of the space environment and to LISA's very long 5-million-km baseline. |
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| AbstractList | To set up a mock data challenge, the authors needed to string together a lot of existing and new code. In the mock LISA data challenges (MLDCs; http:// astrogravs.nasa.gov/docs/mldc), the challengers distribute several simulated LISA data sets to challenge participants; the data include GW signals from sources of undisclosed parameters as well as realistic instrument noise. Participants must analyze the data and report their estimates for the GW source parameters. These challenges are meant to be blind tests but not really contests: their greatest benefit comes from the quantitative comparison of results, analysis methods, and algorithm implementations. The laser interferometer space antenna (LISA), a space-borne GW observatory planned jointly by NASA and the European Space Agency, will assuredly detect a wide variety of GW sources throughout the universe, thanks mostly to the quietness of the space environment and to LISA's very long 5-million-km baseline. |
| Author | Vallisneri, Michele Babak, Stanislav |
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| Cites_doi | 10.1109/MCSE.2007.58 10.1109/MCISE.2003.1182968 10.1109/MCISE.2004.1267615 10.1109/MCISE.2004.1255825 10.1145/1272457.1272461 10.1088/0264-9381/24/19/S18 |
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| References | ref7 Baker (ref1) 2007 ref3 (ref4) 2007; 9 ref6 ref5 ref2 Kangasharju (s1ref1) 2007 |
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| Snippet | To set up a mock data challenge, the authors needed to string together a lot of existing and new code. In the mock LISA data challenges (MLDCs; http://... |
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| SubjectTerms | agile computing Algorithm design and analysis Algorithms Antennas Blinds Computation Computational modeling Computer simulation Data analysis Extensible Markup Language Instruments Interferometers Laser noise NASA Observatories Python Scientific computing scientific programming Space environment Testing XML |
| Title | Python and XML for Agile Scientific Computing |
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