Table 2
Percentiles of Slit/Smeas distribution for ten bright pulsars with HBA timing observations.
| 4 Sub-bands | 2 Sub-bands | Band-integrated | |||||
| 120 MHz | 139 MHz | 159 MHz | 178 MHz | 130 MHz | 168 MHz | 149 MHz | |
|
|
|||||||
| Median | 0.8 | 1.0 | 1.0 | 1.2 | 0.9 | 1.1 | 1.0 |
| 16th Percentile | 0.5 | 0.6 | 0.6 | 0.6 | 0.6 | 0.6 | 0.6 |
| 84th Percentile | 1.5 | 1.6 | 1.7 | 2.2 | 1.5 | 1.9 | 1.6 |
Notes. Slit is obtained from a fit through literature flux density values and Smeas is the HBA flux density. The 16th and 84th percentiles were used for estimating the uncertainty of a single flux density measurement (see text for details).
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