Open Access
Table 1
Integrated flux densities over the full extent of Kes 17 that we used to construct the radio continuum spectrum of the remnant shown in Fig. 1.
| Frequency (MHz) | Integrated flux (Jy) | Reference |
|---|---|---|
| 88 | 43.9 ± 5.2 | This work (GLEAM) |
| 118 | 39.3 ± 4.2 | This work (GLEAM) |
| 155 | 32.0 ± 4.0 | This work (GLEAM) |
| 408 | 21.4 ± 2.2 | Shaver & Goss (1970a) |
| 408 | 24.0 ± 3.7 | Kesteven (1968) |
| 408 | 21.4 ± 3.3 | Green (1974) |
| 843 | 18.0 ± 1.8 (†) | Whiteoak & Green (1996) |
| 1400 | 10.9 ± 0.14 (†) | Gelfand et al. (2013) |
| 1420 | 11.2 ± 0.7 (†) | This work (SGPS) |
| 2303 | 11.1 ± 1.6 (†) | This work (S-PASS) |
| 5000 | 6.7 ± 0.7 | Shaver & Goss (1970b) |
| 5000 | 6.8 ± 0.7 | Milne (1969) |
| 5000 | 6.9 ± 1.4 | Milne & Dickel (1975) |
| 8800 | 6.3 ± 1.3 | Dickel et al. (1973) |
Notes.(†) Measurements not corrected for the absolute flux scale of Perley & Butler (2017) because information on the primary flux calibration is lacking.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.