S2DFS: analysis of temporal changes of drifting subpulses

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Table 1:

The details of the analysed pulsars.
Name	Date	$\nu$	P₀	$N_{\rm pulses}$	P₃	P₂
PSR	[MJD/dd.mm.yy]	[MHZ]	[s]		[P₀]	[deg]
B0031-07	51780/24.08.2000	328	0.9430	7666	$6.7\pm 0.1$	$\rm -21.9^{+0.2}_{-0.1}$
	53239/22.08.2004	1380		1204	$8.3\pm 0.3$	$\rm -40^{+2}_{-50}$
B1819-22	53182/26.06.2004	328	1.8743	1095	$16.9\pm 0.6$	$\rm -17^{+2}_{-6}$
	53188/02.07.2004	1380		1096	$9.8\pm 0.6$	$\rm -9.1^{+0.1}_{-1.0}$
B1944+17	52706/08.03.2003	328	0.4406	3990	$13.5\pm 0.9$	$\rm -30^{+5}_{-10}$
	51977/09.03.2001	1380		2056	$13\pm 0.5$	$\rm -11.7^{+0.3}_{-0.3}$

The last two columns hold results presented in the work of Weltevrede et al. (2006,2007).

Source LaTeX | All tables | In the text

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