Time series models of three sets of RXTE Observations of 4U 1543-47

dc.contributor.authorKoen, Chris
dc.date.accessioned2013-11-14T11:33:10Z
dc.date.available2013-11-14T11:33:10Z
dc.date.issued2013
dc.description.abstractThe X-ray nova 4U 1543−47 was in a different physical state (low/hard, high/soft, and very high) during the acquisition of each of the three time series analyzed in this paper. Standard time series models of the autoregressive moving average (ARMA) family are fitted to these series. The low/hard data can be adequately modeled by a simple low-order model with fixed coefficients, once the slowly varying mean count rate has been accounted for. The high/soft series requires a higher order model, or an ARMA model with variable coefficients. The very high state is characterized by a succession of “dips,” with roughly equal depths. These seem to appear independently of one another. The underlying stochastic series can again be modeled by an ARMA form, or roughly as the sum of an ARMA series and white noise. The structuring of each model in terms of short-lived aperiodic and “quasi-periodic” components is discussed.en_US
dc.description.accreditationWeb of Scienceen_US
dc.identifier.citationKoen, C (2013). Timw Series Models of Three sets of RXTE Observations of 4U 1543−47.The Astrophysical Journal. 765:53en_US
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/10566/814
dc.language.isoenen_US
dc.privacy.showsubmitterfalse
dc.publisherOxford University Pressen_US
dc.rights© 2013 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.urihttp://dx.doi.org/10.1088/0004-637X/765/1/53
dc.status.ispeerreviewedtrue
dc.subjectMethods: statisticalen_US
dc.subjectStars: individual: 4U 1543–47en_US
dc.subjectX-rays: individual: 4U 1543–47en_US
dc.titleTime series models of three sets of RXTE Observations of 4U 1543-47en_US
dc.typeArticleen_US

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