Table 4.
Parameters of the 20 best candidates from the IRAM 30m Galactic centre survey excluding the Galactic centre magnetar PSR J1745−2900.
Pbary | σ | accel. | Epoch | Dataset |
---|---|---|---|---|
(ms) | (ms−2) | |||
452.0269 | 9.1 | 0.00 | 2016 Dec 22 | 3 mm* |
2354.2995 | 10.5 | 0.00 | 2016 Dec 22 | 2 mm |
9.3334 | 9.0 | 0.02 | 2017 Jan 02 | 3+2 mm |
2.5652 | 6.4 | 0.00 | 2017 Jan 02 | 3+2 mm* |
5746.5523 | 4.1 | −33.50 | 2017 Jan 23 | 3+2 mm |
29.0021 | 3.2 | 0.00 | 2017 Feb 14 | 3 mm |
23.9634 | 3.6 | −9.90 | 2017 Mar 01 | 3+2 mm |
12.1925 | 3.7 | 40.50 | 2017 Mar 01 | 3+2 mm |
5.7427 | 6.2 | 0.00 | 2017 Mar 10 | 2 mm |
3.8184 | 11.8 | 0.00 | 2017 Apr 18 | 3 mm |
3.8868 | 7.1 | 0.00 | 2017 May 18 | 3+2 mm* |
2.0782 | 5.9 | 0.00 | 2017 May 24 | 3 mm |
3.3240 | 6.1 | −0.24 | 2017 Jun 05 | 3+2 mm |
2.3460 | 7.0 | 0.05 | 2017 Nov 20 | 3 mm |
8.4191 | 7.5 | 0.04 | 2017 Nov 20 | 2 mm |
3485.2578 | 6.6 | 0.00 | 2017 Dec 18 | 3 mm* |
9.7925 | 2.2 | 0.00 | 2017 Dec 18 | 3 mm |
22.8158 | 2.8 | 0.00 | 2018 Jan 15 | 3 mm |
14.3172 | 8.5 | 0.02 | 2018 Jan 15 | 3 mm |
2.1344 | 5.6 | 0.00 | 2018 May 15 | 2 mm |
Notes. Columns indicate the barycentre spin period of the candidate (Pbary), the significance of the signal as given by PRESTO sifting.py (σ), the acceleration estimated by accelsearch (accel.), the epoch of the observation, and the frequency band (Dataset) that produced the candidate. An asterisk after the frequency band indicates the candidates shown in Fig. 5.
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