Table 1
Different observational setups used in this work.
| Observation | Pointings | Beams/P | FoV/P | Res. | t int | BW | f | N ch | t samp | Coh. | R d |
| deg2 | ° | min | MHz | MHz | ms | TB/h | |||||
|
|
|||||||||||
| LPPS survey | 246 | 7 | 75 | 3.7 | 57 | 6.8 | 142 | 560 | 0.655 | I | 0.09 |
| LOTAS survey | 206 | 19 | 3.9 | 0.5a | 17 | 48 | 143 | 3904 | 1.3 | C | 0.8 |
| LOTAS confirmation | − | 61−217 | − | <0.1 | 27 | 80 | 150 | 6576 | 0.49 | C | 12−42 |
| LOTAS timing | − | 1 | − | − | 15−30 | 80 | 150 | 6576 | 1.3 | C | 0.07 |
Notes. Listed are the number of pointings over the survey; the number of beams per pointing Beams/P, the field of view per pointing FoV/P, the angular resolution (FWHM of each beam), integration time tint, bandwidth BW, central frequency f, number of channels Nch, sampling time tsamp, whether beamforming was (I)ncoherent or (C)oherent, and the data rate Rd.
With the 2011 beam-former, beams at higher declinations were spaced more closely in right ascension (Sect. 4.2.1 in C13).
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