booklet format - inaf iasf bologna

More documents

Recommendations

Info

Temporal Data Analysis A.A. 2011/2012 Declination ....... -6.06232986E+01 Experiment ........ XTE PCA Corrections applied: Vignetting - No ; Deadtime - No ; Bkgd - No ; Clock - Yes Selected Columns: 1- Time; 2- Y-axis; 3- Y-error; 4- Fractional exposure; File contains binned data. Name of the window file (’-’ for default window)[-] - Expected Start ... 10507.01351345407 (days) 0:19:27:562 (h:m:s:ms) Expected Stop .... 10510.83129123185 (days) 19:57: 3:562 (h:m:s:ms) Minimum Newbin Time 0.12500000 (s) for Maximum Newbin No.. 2638849 Default Newbin Time is: 645.00587 (s) (to have 1 Intv. of 512 Newbins) Type INDEF to accept the default value Newbin Time or negative rebinning[3600] 3600 Newbin Time ...... 3600.0000 (s) Maximum Newbin No. 92 Default Newbins per Interval are: 92 (giving 1 Interval of 92 Newbins) Type INDEF to accept the default value Number of Newbins/Interval[215] 92 Maximum of 1 Intvs. with 92 Newbins of 3600.00 (s) Name of output file[default] test Do you want to plot your results?[yes] yes Enter PGPLOT device[/xw] /xw 92 analysis results per interval Intv 1 Start 10507 0:49:27 Ser.1 Avg 3632. Chisq 0.7848E+08 Var 0.1568E+07 Newbs. 84 Min 224.6 Max 5219. expVar 1.423 Bins1873744 PLT> line step PLT> plot PLT> cpd cenx-3_long_lc.ps/cps PLT> plot PLT> quit 134 M.Orlandini
A.A. 2011/2012 Temporal Data Analysis In the top panel of Figure B.1 we show the light curve of the XTE/PCA observation, with data rebinned at 3600 s (that is, each bin corresponds to one hour of data). The “hole” is due to the eclipse of the X–ray pulsar by the optical companion. Figure B.1: Light curve of the X–ray binary pulsar Cen X–3 as observed by the PCA instrument aboard XTE. Top: data have been rebinned at 3600 s, in order to see the long-term behavior of the source (in this case the eclipse). Bottom: data have been rebinned at 0.125 s, in order to observe short-term variability, like the 4.8 s pulsation. By running again the lcurve program with a binning time of 0.125 s (the original time resolution of the data) we can see the single pulses, as shown in the bottom panel of Figure B.1. M.Orlandini 135
Page 1 and 2:
Temporal Data Analysis: Theory and
Page 3 and 4:
Course Outline Table of Contents Li
Page 5 and 6:
A.A. 2011/2012 Temporal Data Analys
Page 7 and 8:
List of Figures 1.1 Classification
Page 9 and 10:
List of Definitions 2.1 Even and od
Page 11 and 12:
List of Theorems 2.1 Convolution th
Page 13:
Part I Theory 1
Page 16 and 17:
Temporal Data Analysis A.A. 2011/20
Page 18 and 19:
Page 20 and 21:
Page 22 and 23:
Page 24 and 25:
Page 26 and 27:
Page 28 and 29:
Page 30 and 31:
Page 32 and 33:
Page 34 and 35:
Page 36 and 37:
Page 38 and 39:
Page 40 and 41:
Page 42 and 43:
Page 44 and 45:
Page 46 and 47:
Page 48 and 49:
Page 50 and 51:
Page 52 and 53:
Page 54 and 55:
Page 56 and 57:
Page 58 and 59:
Page 60 and 61:
Page 62 and 63:
Page 64 and 65:
Page 66 and 67:
Page 68 and 69:
Page 70 and 71:
Page 72 and 73:
Page 74 and 75:
Page 76 and 77:
Page 78 and 79:
Page 80 and 81:
Page 83 and 84:
Chapter5 Procedures for Analyzing R
Page 85 and 86:
Page 87 and 88:
Page 89 and 90:
Page 91 and 92:
Chapter6 Temporal Analysis in X-ray
Page 93 and 94:
Page 95 and 96: A.A. 2011/2012 Temporal Data Analys
Page 121 and 122: Chapter7 Bibliography Reference Tex
Page 123 and 124: AppendixA Examples Shown at the Bla
Page 145: AppendixB Practical Session on Timi
Page 179: A.A. 2011/2012 Temporal Data Analys
show all

booklet format - inaf iasf bologna

Create successful ePaper yourself

Delete template?

Save as template?