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Table 2.

Geometry of MSC pulsars derived using both methods.

PSR αRVM β αρW Prof_mid ϕ0 Δϕ rem−BCW rem/RLC Ref.
(deg) (deg) (deg) (deg) (deg) (deg) (km)
J0729−1448 62±8 −4.8±0.4 65 24 + 14 $ 65^{+14}_{-24} $ −5.3 4.7±0.2 10.0 525 0.044 1
J0742−2822 77±5 6.4±0.2 78 13 + 12 $ 78^{+12}_{-13} $ 4.9 10.1±0.1 5.2 180 0.023 2
J0922+0638 (17±7) (−2.1±0.8) ( 78 13 + 12 ) $ (78^{+12}_{-13}) $ 2
J0953+0755 (103.9±0.4) (24.2±0.1) ( 46 18 + 5 ) $ (46^{+5}_{-18}) $ 2
J1121−5444 (172±5) (−0.4±0.2) 60 12 + 6 $ 60^{+6}_{-12} $ −0.7 2.1±0.1 2.8 100 0.012 1
J1141−3322 (8±4) (−0.5±0.3) 45 13 + 3 $ 45^{+3}_{-13} $ 1.4 −2.2±0.1 −3.6 <0 1
J1705−3950 (48±5) (19±2) ( 29 8 + 4 ) $ (29^{+4}_{-8}) $ 1
J1741−3927 24±7 4±1 60 12 + 6 $ 60^{+6}_{-12} $ −0.2 −1.0±0.1 −0.8 <0 1
J1820−0427 (12±7) (−0.8±0.4) 68 19 + 14 $ 68^{+14}_{-19} $ 0.5 −1.0±0.1 −1.5 <0 2
J1825−0935 83.8±0.2 −4.3±0.1 68 19 + 14 $ 68^{+14}_{-19} $ 0.0 −7.0±0.1 −7.0 <0 2
J1844+1454 (173±5) (−0.4±0.2) 78 13 + 12 $ 78^{+12}_{-13} $ 4.6 9.1±0.1 4.5 1195 0.020 1
J1905+0709 29±8 −6±1 20 6 + 2 $ 20^{+2}_{-6} $ −1.9 −0.3±0.2 1.6 215 0.007 2
J1909+0007 74±9 −2.9±0.2 67 19 + 13 $ 67^{+13}_{-19} $ −0.9 −1.6±0.2 −0.7 <0 2
J1932+2220 41±8 −3.9±0.7 ( 64 18 + 12 ) $ (64^{+12}_{-18}) $ 2
J2043+2740 123±7 7.9±0.8 64 18 + 12 $ 64^{+12}_{-18} $ 3.9 13.3±0.3 9.4 190 0.041 2

Notes. We list αRVM, βRVM, and αρW and their respective uncertainties, the profile midpoint, the PPA centroid as measured from RVM fits, ϕ0, the resulting BCW delay, Δϕ, and the inferred emission height in km and RLC units. References. Note that negative delays, Δϕ, are not expected in the BCW model. For those cases we indicate this with ‘<0’ for the emission height. Values in brackets reflect the results of fits that we do not consider to be reliable but note that even in such cases the PPA centroid is often well defined (see text for details). (1) Basu et al. (2024); (2) SSW.

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