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Table F.2

Intermediate results for calculating the absolute positions reported in Table 3, and their associated uncertainties

α δ

tref = MJD 59554.0
psr. appr. A (22h22m05s.99997±0.11 mas) + [(3.67±0.01)−(0.51±0.11)-(0.19±0.07)] mas (−01°37′15″.7825±0.25 mas) + [(1.39±0.01)−(1.90±0.19)+(0.34±0.08)] mas
J2221 appr. B (22h22m06S00025 ±0.15 mas)+[(−0.53 ±0.01)-(1.43 ±0.10)+ (0.43±0.06)] mas (−01°37′15″.7804±0.38 mas)+[(−2.69±0.02) + (0.04±0.16)+(0.58±0.08)] mas
J2222 appr. B (22h22m06S00021 ±0.06 mas)+[(−0.22±0.03)-(0.45±0.11)-(0.18±0.07)] mas (−01°37′15″.7808±0.18 mas)+[(−0.54 ±0.06)-(1.82± 0.18)+(0.34± 0.08)] mas

tref = MJD 55743

J2221 appr. B (22h22m05s.96911 ±0.06 mas)+[(−0.53 ±0.01)−(1.43 ±0.10)+ (0.43 ±0.06)] mas (−01°37′15″.7242 ±0.15 mas)+[(−2.69±0.02) + (0.04±0.16)+(0.58±0.08)] mas
J2222 appr. B (22h22m05s.96910±0.01 mas)+[(−0.22±0.03)-(0.45±0.11)-(0.18±0.07)] mas (−01°37′15″.7244±0.03 mas)+[(−0.54±0.06)−(1.82±0.18)+(0.34±0.08)] mas

Notes. Identical to Table 3, the “psr. appr.”, “J2221 appr.” and “J2222 appr.” refer to the three approaches (to the absolute position of PSR J2222–0137) described in Sect. 5. Each absolute pulsar position is calculated from four terms in the round brackets. In all cases, the third term from the left refers to the core-shift-related position correction; and the fourth term is the position shift for aligning the off-beam calibrators to the RFC positions1.

(A)The first term from the left is the pulsar position obtained with the Multi-View strategy (see Sect. 3.1.2), while the second term removes the parallax effects (see Sect. 5).

(B)The first term from the left is the reference pulsar position xpsrPR$x_{{\rm{psr}}}^{{\rm{PR}}}$ derived with respect to the in-beam calibrator of use (i.e., J2221 for the J2221 approach, and J2222 for the J2222 approach). The second term aligns the reference point of the in-beam calibrator to the in-beam calibrator position determined with the Multi-View strategy (see Sect. 3.1.2).

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