Table 1
Integrated flux density of SNR G315.4-2.3.
| ν (MHz) | Sν (Jy) | Telescope | Reference |
|---|---|---|---|
| 408 | 86±9 a | MOST | 1 |
| 843 | 22.7±1.4 b | MOST | 2 |
| 1335 | 15.4±1.0 | MeerKAT | 3 |
| 1340 | 28±3 a | ATCA | 4 |
| 1410 | 30±3 a | Murriyang | 5 |
| 2200 | 21.7±1.1 | ATCA | 6 |
| 2400 | 24.3±1.0 b | Murriyang | 7 |
| 2650 | 20±2 a | Murriyang | 5 |
| 4850 | 10.1±0.5 b | Murriyang | 8 |
| 5000 | 18.2±1.8 a | Murriyang | 1 |
Notes. (1) Caswell et al. (1975); (2) Whiteoak & Green (1996); (3) Cotton et al. (2024); (4) Dickel et al. (2001); (5) Hill (1967); (6) this paper; (7) Duncan et al. (1995); (8) Condon et al. (1993). MOST: Molonglo Observatory Synthesis Telescope; Murriyang: Parkes 64 m telescope. (α)The uncertainty was not provided in the literature and we used a relative uncertainty of 10%. (b) We measured the integrated flux density from the survey maps.
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