Table 1
Integrated flux densities on SNR G46.8–0.3 used to construct the radio continuum spectrum of the source presented in Fig. 2.
| Frequency (MHz) | Scaled flux (Jy) | Reference |
|---|---|---|
| 30.9 | 93.9 ± 18.8 (*) | Kassim(1988) |
| 38 | 100 ±15 (*) | Holden & Caswell (1969) |
| 83 | 57.7 ± 9.9 | Kovalenko et al. (1994a) |
| 88 | 70.9 ± 8.9 | This work (GLEAM) |
| 111 | 54.1 ± 9.8 | Kovalenko et al. (1994a) |
| 118 | 55.0 ± 6.2 | This work (GLEAM) |
| 155 | 41.5 ± 4.6 | This work (GLEAM) |
| 178 | 42.6 ± 6.4 | Holden & Caswell (1969) |
| 200 | 33.5 ± 3.4 | This work (GLEAM) |
| 400 | 28.0 ± 5.6 (†) | Downes (1971) |
| 408 | 22.7 ± 4.5 | Holden & Caswell (1969) |
| 610 | 22.9 ± 2.3 (†) | Moran(1965) |
| 610 | 21.5 ± 3.2 | Holden & Caswell (1969) |
| 960 | 16.0 ± 1.6 | Trushkin (1996) |
| 1400 | 17.0 ± 3.4 (†) | Downes (1971) |
| 1400 | 16.7 ± 2.5 | Holden & Caswell (1969) |
| 1414 | 17.7 ± 1.8 | Altenhoff et al. (1970) |
| 1420 | 15.9 ± 1.6 | This work (THOR+VGPS) |
| 1465 | 13.3 ± 0.1 | Dubner et al. (1996) |
| 2695 | 11.0 ± 1.1 | Altenhoff et al. (1970) |
| 2700 | 9.9 ± 1.5 | Day et al. (1970) |
| 2730 | 10.0 ± 0.9 | Willis (1973) |
| 3900 | 8.7 ± 0.9 | Trushkin (1996) |
| 4800 | 6.9 ± 0.2 | Sun et al. (2011) |
| 4850 | 6.9 ± 0.4 | Condon et al. (1989) |
| 4850 | 7.2 ± 0.4 | This work (GB6) |
| 5000 | 6.6 ± 0.7 | Caswell & Clark (1975) |
| 5000 | 5.6 ± 0.6 | Angerhofer et al. (1977) |
| 10300 | 4.0 ± 0.8 | This work (NRO) |
| 11 200 | 5.1 ± 0.5 | Trushkin (1996) |
Notes. Fluxes were set to the absolute scale of Perley & Butler (2017) (see text for details). (*)No correction factor was applied to bring the measurement to the Perley & Butler (2017) scale because the corresponding frequency is outside its 50 MHz–50 GHz validity range.(†) A correction to the absolute scale of Perley & Butler (2017) was not applied due to the lack of information on the flux density calibrator source.
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