Table 16.
Stability of the NEFD estimates.
Data set | Method | A1 | A3 | A1 and A3 | A2 |
---|---|---|---|---|---|
HLS J0918+5142 | Deep int. | 46.6 | 38.4 | 30.4 | 8.5 |
Scatter | 45.7 | 36.3 | 28.5 | 8.2 | |
N2R9 | Scatter | 47.0 | 36.9 | 28.8 | 8.4 |
N2R12 | 47.3 | 36.4 | 30.2 | 8.5 | |
N2R14 | 47.3 | 39.8 | 30.9 | 9.3 | |
Combined | 47.2 | 37.9 | 30.1 | 8.8 |
Notes. Top-of-atmosphere NEFD in mJy s1/2 for the two methods described in the text, which are the deep integration (labelled “Deep int”) and the scatter method (“Scatter”), and using two different data sets, HLS J0918+5142 and all sub-Jy sources acquired during the reference observation campaigns. The results given in the last row are based on more than a thousand scans (202, 481, and 430 scans during N2R9, N2R12, and N2R14, respectively).
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