All Figures

$\begin{figure} \par\includegraphics[angle=0,width=5.5cm,clip]{Ff231_f1.ps} \end{figure}$ Figure 1: The integrated profile of the PSR J1713+0747 at 8.35 GHz along with the profile at 1.41 GHz. The profiles have been aligned by timing model. Intensity of the profiles is shown in arbitrary units.
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In the text

$\begin{figure} \par\includegraphics[angle=0,width=5.5cm,clip]{Ff231_f2.ps} \end{figure}$ Figure 2: The integrated profile of the PSR B1855+09 at 8.35 GHz along with the profile at 1.41 GHz. The profiles have been aligned by timing model. Intensity of the profiles is shown in arbitrary units.
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In the text

$\begin{figure} \par\includegraphics[angle=0,width=5.5cm,clip]{Ff231_f3.ps} \end{figure}$ Figure 3: The integrated profile of the PSR J2145-0750 at 8.35 GHz along with the profile at 1.41 GHz. The profiles have been aligned by timing model. Intensity of the profiles is shown in arbitrary units.
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In the text

$\begin{figure} \par\includegraphics[angle=0,width=6.5cm,clip]{Ff231_f4.ps} \end{figure}$ Figure 4: Spectra of 3 millisecond pulsars together with a single power law fits and spectral indices. Diamonds denote 100 MHz data taken from Kuzmin and Losovsky (2001), circles denote data from 300 MHz to 4.85 GHz taken from Kramer et al. (1999) and references therein. Squares denote our 8.35 GHz observations and triangles show flux density upper limits calculated from our observations at 8.35 GHz.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{Ff231_f5.ps} \end{figure}$ Figure 5: Interpulse-to-Mainpulse amplitude ratios at different frequencies for B1855+09. Data at 104 MHz were taken from Kuzmin et al. (1990), data at 430 MHz, 1.4 GHz and 2.4 GHz from Thorsett & Stinebring (1990) and at 4.85 GHz from Kijak et al. (1997).
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In the text

$\begin{figure} \par\includegraphics[angle=0,width=5.5cm,clip]{Ff231_f1.ps} \end{figure}$	Figure 1: The integrated profile of the PSR J1713+0747 at 8.35 GHz along with the profile at 1.41 GHz. The profiles have been aligned by timing model. Intensity of the profiles is shown in arbitrary units.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=0,width=5.5cm,clip]{Ff231_f2.ps} \end{figure}$	Figure 2: The integrated profile of the PSR B1855+09 at 8.35 GHz along with the profile at 1.41 GHz. The profiles have been aligned by timing model. Intensity of the profiles is shown in arbitrary units.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=0,width=5.5cm,clip]{Ff231_f3.ps} \end{figure}$	Figure 3: The integrated profile of the PSR J2145-0750 at 8.35 GHz along with the profile at 1.41 GHz. The profiles have been aligned by timing model. Intensity of the profiles is shown in arbitrary units.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{Ff231_f5.ps} \end{figure}$	Figure 5: Interpulse-to-Mainpulse amplitude ratios at different frequencies for B1855+09. Data at 104 MHz were taken from Kuzmin et al. (1990), data at 430 MHz, 1.4 GHz and 2.4 GHz from Thorsett & Stinebring (1990) and at 4.85 GHz from Kijak et al. (1997).
Open with DEXTER