Absolute emission altitude of pulsars: PSRs B1839+09, B1916+14, and B2111+46

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Table 1:

Core emission geometry parameters of PSRs B1839+09, B1916+14 and B2111+46.
Pulsar	$\nu$	$\delta\phi'_{\rm core}$	$\delta\phi'_{\rm PPAIP}$	$r_{\rm core}$	$r_{\rm core}$	$\chi^2$	SR	$s/s_{\rm lof}$
PSR B	(MHz)	( $^\circ$ )	( $^\circ$ )	(km)^a	$(\%~~ r_{\rm LC})$		(%)^b	foot value
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
1839+09	1418	$-0.32\pm0.07$	$0.32\pm0.01$	$50\pm5$	$0.28\pm0.0 3$	102 .	100	$0.51\pm0.03$
1916+14	1418	$-0.23\pm0.02$	$0.23\pm0.01$	$95\pm4$	$0.20\pm0.01$	28.25	94	$0.26\pm0.01$
2111+46	610	$-1.33\pm0.02$	$1.33\pm0.20$	$503\pm38$	$1.04\pm0.08$	5.7	100	$0.13\pm0.00$
	1408	$-0.23\pm0.08$	$0.23\pm0.29$	$83\pm54$	$0.17\pm0.11$	2.05	95	$0.51\pm0.17$

Notes. ^(a) Emission heights computed using the exact formula (G05). ^(b) The percentage of the standardized residuals (SR) with value of -2 and +2.

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