Table 1: Parameters of several nearby old pulsars.
Pulsar Age Distance^* Parallax^* $\mu_\alpha^*$ $\mu_\delta^*$ v $_{\perp}^*$ log( $\dot{E}$ ) Optical band Magnitude

log ( $\tau$ ) pc mas mas yr^-1 mas yr^-1 km s^-1 ergs s^-1

PSR B1929+10 6.49 331(10) 3.02(9) 94.8 43 163(5) 33.59 F342W 26.8^a

PSR B1133+16 6.70 350(20) 2.80(16) -73.95 368.05 631(38) 31.94 - 28.1^d

PSR B0950+08 7.24 262(5) 3.82(7) -2.09 29.5 36.6(7) 32.74 B 27.07^b

PSR J0108-1431 8.23 60-130 - <26 <78 <50₁₃₀ 30.75 B >28.6^c

**Table 1:** Parameters of several nearby old pulsars.
Pulsar	Age	Distance^*	Parallax^*	$\mu_\alpha^*$	$\mu_\delta^*$	v $_{\perp}^*$	log( $\dot{E}$ )	Optical band	Magnitude
	log ( $\tau$ )	pc	mas	mas yr^-1	mas yr^-1	km s^-1	ergs s^-1
PSR B1929+10	6.49	331(10)	3.02(9)	94.8	43	163(5)	33.59	F342W	26.8^a
PSR B1133+16	6.70	350(20)	2.80(16)	-73.95	368.05	631(38)	31.94	-	28.1^d
PSR B0950+08	7.24	262(5)	3.82(7)	-2.09	29.5	36.6(7)	32.74	B	27.07^b
PSR J0108-1431	8.23	60-130	-	<26	<78	<50₁₃₀	30.75	B	>28.6^c

^* Brisken et al. (2002); ^a Pavlov et al. (1996); ^b Zharikov et al. (2002,2004); ^c Mignani et al. (2003); ^d this paper.

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