Open Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202452111]


Issue
A&A
Volume 711, July 2026
Article Number C2
Number of page(s) 1
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/202661330e
Published online 16 July 2026

In the published paper, Eq. (4) correctly included the cosmological time-dilation factor, (1 + z), in the conversion from proper motion to apparent jet speed. However, this factor was inadvertently omitted in the numerical calculation. Since the adopted redshift is z = 0.42, the apparent speeds derived from Eq. (4) should be multiplied by 1 + z = 1.42. Accordingly, the affected numerical values in the Abstract, main text, Table 2, and Fig. 12 should be revised as described below.

Including the proper redshift correction (1 + z), the corrected apparent speeds are βapp = 1.103 ± 0.056, 6.702 ± 0.615, 7.774 ± 16.139, and 7.293 ± 50.427 for the C1, C2, C3, and C4 components, respectively. Therefore, references to C1 as a “subluminal” component, or to its “subluminal speed,” should be replaced by “slow-moving” or “slow-moving, mildly superluminal.” The historical apparent speeds quoted from the literature for comparison should also be corrected by the same factor: the historical maximum (4.8c) and median (3.1c) speeds at 15 GHz should be revised to 6.78c and 4.41c, respectively, and the historical maximum (4.5c) and median (3.6c) speeds at 43 GHz should be revised to 6.25c and 4.94c, respectively. Thus, the corrected apparent speed of C2, βapp = 6.70 ± 0.62, still remains comparable to the historical maximum apparent speeds reported for PKS 0735+178. The corresponding corrected minimum Lorentz factors are Γmin = 1.49 ± 0.04 and 6.78 ± 0.61 for C1 and C2, respectively. For C2, the corrected critical viewing angle, variability Lorentz factor, and variability viewing angle are θc = (8.49 ± 0.77)°, Γvar = 6.82 ± 0.63, and θvar = (7.52 ± 3.50)°, respectively. These corrected values are listed in Table 1.

For the comparison with δ ≃ 30, the required viewing angle and Lorentz factor of C2 should be changed from θ ≃ 0.6° and Γ ≃ 15.4 to θ ≃ 0.81° and Γ ≃ 15.76, respectively. Accordingly, the viewing-angle change for C2 discussed in the original paper should be revised from θ ≃ 0.6°-6.8° to θ ≃ 0.8°-7.5°. The corresponding updates are reflected in the corrected Fig. 12. Using the corrected viewing angle, the deprojected distance of the apparent C1–C2 passage region from the very long baseline interferometry core should be revised from 6.05 ± 3.65 pc to 5.49 ± 2.58 pc. Accordingly, the distance quoted as ≳6.5 pc should be revised to ≳5.5 pc.

These numerical corrections do not affect the fitted component positions, angular proper motions, ejection epoch of C2, or inferred C1–C2 passage time, as these quantities were determined directly from the angular motions. The main observational results of the paper – a temporal coincidence between the apparent C1–C2 passage and IceCube-211208A – are therefore valid, and the scientific conclusions of the paper remain unchanged.


© The Authors 2026

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All Tables

Table 1

Corrected numerical values.

All Figures

Thumbnail: Fig. 12 Refer to the following caption and surrounding text. Fig. 12

Corrected version of Fig. 12 in the original paper. The gray shaded region has been updated to reflect the corrected apparent speed of C2.

In the text

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