Deriving pulsar pair-production multiplicities from pulsar wind nebulae using H.E.S.S. and LHAASO observations

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Table 2

Estimates of the maximum and minimum values of the lower limit for ⟨κ⟩ for the H.E.S.S./ATNF sample.

ATNF name	Ė_t	⟨κ⟩_min	⟨κ⟩_max
ATNF name	(×10³⁶erg/s)	(Dimensionless)	(Dimensionless)
J1833–1034	33.9	884	4430
J1513–5908	17.0	802	938
J1930+1852	12.0	374	464
J1420–6048	10.0	130	495
J1846–0258	8.13	1030	1060
J0835–4510	6.92	173	333
J1838–0655	5.50	98	349
J1418–6058	4.90	107	159
J1357–6429	3.09	109	128
J1826–1334	2.82	72	119
J1119–6127	2.29	268	273
J1301–6305	1.70	64	73
J1747–2809	42.7	1880	59 185
J1617–5055	15.8	316	1072
J1023–5746	11.0	304	435
J1856+0245	4.57	80	191
J1640–4631	4.37	351	386
J1709–4429	3.39	89	145
J1907+0602	2.82	57	90
J1016–5857	2.57	42	65
J1803–2137	2.19	85	111
J1809–1917	1.82	26	61
J1718–3825	1.29	13	39
J1028–5819	0.832	6	12
J1833–0827	0.575	5	12
J1857+0143	0.447	8	10

Notes. ⟨κ⟩_min assumes a P₀ of 10 ms and ⟨κ⟩_max assumes a P₀ of 50 ms. This corresponds to the entire vertical range as shown in Fig. 1.

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