S2DFS: analysis of temporal changes of drifting subpulses

M. Serylak; B. W. Stappers; P. Weltevrede

doi:10.1051/0004-6361/200912453

Home

All issues

Volume 506 / No 2 (November I 2009)

A&A, 506 2 (2009) 865-874

Full HTML

Highlight

Free Access

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

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.