The analysis of indexed astronomical time series – X. Significance testing of O − C data
| dc.contributor.author | Koen, Chris | |
| dc.date.accessioned | 2013-12-02T12:36:28Z | |
| dc.date.available | 2013-12-02T12:36:28Z | |
| dc.date.issued | 2006 | |
| dc.description.abstract | It is assumed that O − C (‘observed minus calculated’) values of periodic variable stars are determined by three processes, namely measurement errors, random cycle-to-cycle jitter in the period, and possibly long-term changes in the mean period. By modelling the latter as a random walk, the covariances of all O − C values can be calculated. The covariances can then be used to estimate unknown model parameters, and to choose between alternative models. Pseudo-residuals which could be used in model fit assessment are also defined. The theory is illustrated by four applications to spotted stars in eclipsing binaries. | en_US |
| dc.description.accreditation | Web of Science | en_US |
| dc.identifier.citation | Koen, C. (2006). The analysis of indexed astronomical time series – X. Significance testing of O − C data. Monthly Notices of the Royal Astronomical Society, 365(2): 489-495 | en_US |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.uri | http://hdl.handle.net/10566/893 | |
| dc.language.iso | en | en_US |
| dc.privacy.showsubmitter | false | |
| dc.publisher | Oxford University Press | en_US |
| dc.rights | © 2005 Copyright Oxford University Press. This file may be freely used for educational purposes, as long as it is not altered in any way. Acknowledgement of the authors and the source is required. | |
| dc.source.uri | http://dx.doi.org/10.1111/j.1365-2966.2005.09719.x | |
| dc.status.ispeerreviewed | true | |
| dc.subject | Methods: data analysis | en_US |
| dc.subject | Methods: statistical | en_US |
| dc.subject | Stars: variables: other | en_US |
| dc.title | The analysis of indexed astronomical time series – X. Significance testing of O − C data | en_US |
| dc.type | Article | en_US |