Titlebook: Astronomical Time Series; Proceedings of The F Dan Maoz,Amiel Sternberg,Elia M. Leibowitz Conference proceedings 1997 Springer Science+Busi

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书目名称Astronomical Time Series影响因子(影响力)




书目名称Astronomical Time Series影响因子(影响力)学科排名




书目名称Astronomical Time Series网络公开度




书目名称Astronomical Time Series网络公开度学科排名




书目名称Astronomical Time Series被引频次




书目名称Astronomical Time Series被引频次学科排名




书目名称Astronomical Time Series年度引用




书目名称Astronomical Time Series年度引用学科排名




书目名称Astronomical Time Series读者反馈




书目名称Astronomical Time Series读者反馈学科排名

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Observations of Millisecond Pulsars on Time Scales from 10 Nanoseconds to 10 Yearsthe discovery of pulsars, which produce arguably the most famous astronomical time series (Hewish .., 1968). The diversity and richness of science that has developed from observations of pulsars could never have been foreseen by their discoverers. Most of this science is deduced from detailed studie

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Microlensing: Current Results and Future Prospectsalf that required to explain the dark matter, but the estimated MACHO mass (~ 0.4 M.) is most consistent with stars that should have been seen. Toward the bulge, the total mass is consistent with that given by dynamical estimates of the bulge mass, but the observed timescales seem to require that a

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Image Subtraction in Time Series Analysis: Application to Microlensing and Light Echoeserture photometry). Often the field containing the source is extremely crowded, or the source is extended. We describe techniques that we have developed in order to follow changes in such sources, utilizing the technique of image subtraction. In this way the stable flux in a field can be subtracted

舔食

Desperately Seeking Non-Gaussianitynity, therefore, than in the light curve of 0957+561, the gravitational lens that, until recently, had yielded frustratingly inconsistent determinations of its lag. We discuss the difficulties in measuring deviations from Gaussianity in weakly nonstationary processes (such as 1/. noise or random wal

平息

Friction

Reverberation Mapping and the Physics of Active Galactic Nuclei, enabled mapping of the gas distribution around the central black hole, and are starting to resolve the continuum source structure. This review describes the recent and successful campaigns of the International AGN Watch consortium, outlines the theoretical background of reverberation mapping and t

liposuction

Echo Mapping of X-Ray Binaries and Active Galactic Nuclei). In these systems radiation from a compact variable source drives responses in the surrounding medium. We outline maximum entropy techniques used to find smooth delay maps that fit incomplete and noisy measurements of the driving and responding lightcurves. In AGNs, erratically variable ionizing f

Radiation