Fig. 1

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Large-field global view toward SNR G150.3+4.5. The upper panel shows an integrated intensity map derived from the 12CO emission with a velocity range between −60 and 15 km s−1 (3σ = 4.7 K km s−1). The purple dashed contours represent the Urumqi λ 6 cm radio continuum emission (Gao & Han 2014), and the purple ellipse shows the size of the remnant in the 6 cm radio observations. The contours run at 3.0 + n × 3.0 mK (n = 1, 2,… 5). The orange and green circles represent the very high energy source 1LHAASO J0428+5531 (Cao et al. 2024), with orange indicating KM2A component and green denoting the WCDA component. The red circles represent two SNR candidates G151.2+2.9 (Kerton et al. 2007) and G149.5+3.2 (Gerbrandt et al. 2014). The bottom panel depicts the average spectra of the regions marked in the upper panel with the rectangle, with the spectra of 12CO (blue) and 13CO (red). The annotations on the spectra pinpoint the velocity ranges of individual components.
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