A low frequency study of PSRs B1133+16, B1112+50, and B0031−07

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Table 1

Observation details and telescope parameters.

Pulsar	Period	Date	Duration	N_pulses	Band^a	T_sys	N_bins ^b	Δt^b	S_min ^c
	s	dd/mm/yy	min		MHz	K		μs	Jy

B1133+16.........	1.187913065936	23/11/08	280	~13 701	110–180	400	2048	809	9.0
B0031−07.........	0.942950994559	02/11/08	360	~22 758	110–180	400	2048	580	10.7
B1112+50.........	1.656439759937	01/10/08	570	~14 286	110–180	400	2048	460	12.0

Notes.

^(a)

The pulsar signal was recorded from eight 2.5 MHz bands centred at 116.75, 130, 139.75, 142.25, 147.50, 156, 163.50, and 173.75 MHz.

^(b)

Δt is the effective time resolution of the pulses with N_bins across the pulse period.

^(c)

S_min is the minimum detectable signal per time sample based on a 30% aperture efficiency.

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