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Table 2
Supernova remnant flux densities in the MeGaPluG pilot.
| Name | Radius (arcmin) | S400 MHz (Jy) Observed/expected | S650 MHz (Jy) Observed/expected |
|---|---|---|---|
| G29.6+0.1 | 3.3 | 0.39 ± 0.26/0.90 ± 0.14 | 0.28 ± 0.17/0.70 ± 0.16 |
| G29.7−0.3 | 2.7 | 17.2 ± 1.7/16.6 ± 1.9 | 10.7 ± 1.1/11.9 ± 2.0 |
| G31.9+0.0 | 4.5 | 39.2 ± 4.0/27.6 ± 2.9 | 24.0 ± 2.4/22.5 ± 3.1 |
| G32.8−0.1 | 11.5 | 10.1 ± 1.3/15.3 ± 1.7 | 3.6 ± 0.5/13.4 ± 1.8 |
| G33.2−0.6 | 9.2 | 1.7 ± 0.4 /4.2 ± 0.5 | 1.1 ± 0.2/3.6 ± 0.5 |
| G33.6+0.1 | 6.7 | 19.3 ± 2.1/20.4 ± 2.3 | 12.9 ± 1.3/16.0 ± 2.4 |
| G34.7−0.4 | 19.2 | 180 ± 18/319 ± 38 | 107 ± 11/262 ± 42 |
Notes. The expected flux densities in the two bands are calculated using the spectral indices derived in Dokara et al. (2023).
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