Supernova remnants in the vicinity of PSR J1734−3333. The black circles represent SNRs from the Green (2019) catalogue, and SNR G354.8−0.8 is in green. The diameter of each circle is given by the size of the SNR listed in the catalogue. The blue dot shows the current location of the pulsar, and the horizontal dashed lines show where the pulsar would have been at each labelled time in the past considering a proper motion μ_δ = −29 mas yr⁻¹. The shaded regions mark the possible location of the pulsar in the past considering also a proper motion in RA, for which we used the 1-σ range μ_α ∈ [0, 20] mas yr⁻¹ (dark shading) and the 2-σ range μ_α ∈ [ − 10, 30] mas yr⁻¹ (light shading).