By Jeffrey D. Scargle (auth.), Dan Maoz, Amiel Sternberg, Elia M. Leibowitz (eds.)
ELlA M. LEIBOWITZ Director, clever Observatory Chair, clinical Organizing Committee The foreign symposium on "Astronomical Time sequence" used to be held on the Tel Aviv collage campus in Tel Aviv, from December 30 1996 to January 11997. It used to be prepared with the intention to have fun the twenty fifth anniversary of the Florence and George clever Observatory (WO) operated via Tel Aviv collage. the positioning of the 1 meter telescope of the observatory is close to the city of Mitzpe-Ramon, a few 220 km south of Tel Aviv, on the heart of the Israeli Negev highland. there have been significant purposes for the alternative of Time sequence because the sub ject subject for our symposium. One is principally inquisitive about the subject material itself, and one is said relatively to the clever Observatory. there's rarely any doubt that astronomical time sequence are one of the such a lot historical thoughts in human civilization and tradition. you'll even say that astronomical time sequence preceeded astronomy itself, because the effect of the day /night cycle in the world is one of the first and such a lot primary impact that provoke a. person, or, actually, such a lot residing creatures on the earth. An echo of this concept. may be heard within the Biblical tale of construction, the place the idea that of evening and day preceeds the production of the astronomical objects.
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Extra resources for Astronomical Time Series: Proceedings of The Florence and George Wise Observatory 25th Anniversary Symposium held in Tel-Aviv, Israel, 30 December 1996–1 January 1997
T. & Flannery, B. , Cambridge:Cambridge University Priestley, M. , 1988, Nonlinear and Non-Stationary Time Series Analysis, London:Academic Qian, S. , 1996, Joint Time-Frequency Analysis: Methods and Applications, Englewood Cliffs NJ:Prentice Hall Reilly, D. O. Box 563, Hartboro PA USA SAS/ETS Users' Guide, 1993, SAS Institute, SAS Campus Drive, Cary NC 27513 USA Scargle, J. , 1984, in Statistical Challenges in Modern Astronomy (E. Feigelson and G. J. ), NY:Springer, p. , Crutchfield, J. , 1993, Astrophys.
Flexibility of data analysis than have been possible before. 1, pulsar observations have traditionally been made using hardware filter banks, which take a band-limited signal and produce time series for numerous frequency channels, which are then each squared to yield power time series, which are sampled. Appropriate delays are then added to the digitized channels to dedisperse. , 1992). Timing resolution can be limited by the sampling rate, or by the residual dispersion smearing within individual channels.
Long-Term High-Precision Timing of Millisecond Pulsars In this section we review recent results of long-term, high-precision millisecond pulsar timing experiments. 1. 1. PSRs B1855+09 and B1937+21 Long-term, high precision millisecond pulsar timing has been done at the 305-m dish at Arecibo, Puerto Rico since the discovery of millisecond pulsars. Bi-weekly timing observations for two of the first discovered millisecond pulsars, PSRs B1855+09 and B1937+21, are described in detail in Kaspi, Taylor and Ryba (1994).
Astronomical Time Series: Proceedings of The Florence and George Wise Observatory 25th Anniversary Symposium held in Tel-Aviv, Israel, 30 December 1996–1 January 1997 by Jeffrey D. Scargle (auth.), Dan Maoz, Amiel Sternberg, Elia M. Leibowitz (eds.)