cmb.out

\BOOKMARK [1][-]{section.1}{Introduction}{}% 1
\BOOKMARK [2][-]{subsection.1.1}{Radio Astronomy}{section.1}% 2
\BOOKMARK [2][-]{subsection.1.2}{Cosmic Microwave Background}{section.1}% 3
\BOOKMARK [2][-]{subsection.1.3}{Atmospheric opacity}{section.1}% 4
\BOOKMARK [2][-]{subsection.1.4}{Brightness temperature}{section.1}% 5
\BOOKMARK [2][-]{subsection.1.5}{Radiative transfer}{section.1}% 6
\BOOKMARK [1][-]{section.2}{Observations}{}% 7
\BOOKMARK [2][-]{subsection.2.1}{Telescope}{section.2}% 8
\BOOKMARK [2][-]{subsection.2.2}{Calibrations}{section.2}% 9
\BOOKMARK [2][-]{subsection.2.3}{Observations}{section.2}% 10
\BOOKMARK [1][-]{section.3}{Data Reduction}{}% 11
\BOOKMARK [2][-]{subsection.3.1}{Determining the period}{section.3}% 12
\BOOKMARK [2][-]{subsection.3.2}{Determining the dispersion measure}{section.3}% 13
\BOOKMARK [2][-]{subsection.3.3}{Pulse Profile}{section.3}% 14
\BOOKMARK [1][-]{section.4}{Results}{}% 15
\BOOKMARK [2][-]{subsection.4.1}{Period}{section.4}% 16
\BOOKMARK [2][-]{subsection.4.2}{dispersion measure}{section.4}% 17
\BOOKMARK [2][-]{subsection.4.3}{Period change}{section.4}% 18
\BOOKMARK [1][-]{section.5}{Discussion}{}% 19
\BOOKMARK [2][-]{subsection.5.1}{Period}{section.5}% 20
\BOOKMARK [2][-]{subsection.5.2}{Period Change}{section.5}% 21
\BOOKMARK [2][-]{subsection.5.3}{Age of the pulsar}{section.5}% 22
\BOOKMARK [2][-]{subsection.5.4}{Magnetic field of the pulsar}{section.5}% 23
\BOOKMARK [2][-]{subsection.5.5}{Dispersion measure}{section.5}% 24
\BOOKMARK [2][-]{subsection.5.6}{Distance}{section.5}% 25
\BOOKMARK [1][-]{section.6}{Conclusions}{}% 26
\BOOKMARK [2][-]{subsection.6.1}{Errors}{section.6}% 27
\BOOKMARK [2][-]{subsection.6.2}{Comparison with other pulsars}{section.6}% 28
\BOOKMARK [2][-]{subsection.6.3}{Future experiments}{section.6}% 29