Rate of correct detection of periodic signal with the Gaia satellite

Monthly Notices of the Royal Astronomical Society

Volumn 361, Issue 4, 2005, Pages 1136-1144

  Eyer, L ^a,b   Mignard, F ^c  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b PRINCETON UNIVERSITY OBSERVATORY   (United States)

^c CNRS   (France)

Author keywords

Methods: numerical; Space vehicles: instruments; Stars: variables: other; Surveys; Techniques: miscellaneous

Indexed keywords

GAMMA RAYS; NUMERICAL METHODS; PHOTOMETRY; SATELLITES; SIGNAL TO NOISE RATIO;

'CURRENT; EUROPEAN SPACE AGENCY; GAIA SATELLITE; METHOD: NUMERICAL; PERFORMANCE; PERIODIC SIGNAL; SPACE VEHICLES: INSTRUMENTS; STAR: VARIABLE: OTHER; STARS: VARIABLES; TECHNIQUE: MISCELLANEOUS;

STARS;

EID: 23944481851     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09266.x     Document Type: Review

References (8)

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3. Eyer L., Grenon M., 1997, ESA SP-402, 467
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5. Mignard F., 2001, A Practical Scanning Law for Gaia Simulations, Technical Note GAIA-FM-010
6. Perryman M. A. C. et al., 2001, A&A, 369, 339
7. Pourbaix D., Jancart S., 2003, in Munari U., ed., ASP Conf. Ser. Vol. 298, Gaia Spectroscopy, Science and Technology. Astron. Soc. Pac., San Francisco, p. 345
8. Press W. H., Teukolsky S. A., Vetterling W. T., Flannery B. P., 1992, Numerical Recipes in FORTRAN. Cambridge Univ. Press, Cambridge