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Table 2.

Properties of the detected bursts.

Burst ID TOA ϕ Δt Sν Fν E
[MJD] [ms] [Jy] [Jy ms] [1037 erg] [MHz ms−1]
SRT-P-01 59162.8253243218 0.5870 19 ± 2 3.1 ± 0.8 48 ± 16 8 ± 2.5 N.A.
SRT-P-02 59162.8343320911 0.5875 14.0 ± 0.5 12.2 ± 3.0 139 ± 43 24 ± 7 −9.7 ± 0.6
SRT-P-03 59162.8567440946 0.5889 13.2 ± 0.5 11.7 ± 2.9 125 ± 39 21 ± 6 −11.4 ± 0.6
SRT-P-04 59162.8665428914 0.5895 23 ± 2 3.2 ± 0.8 61 ± 20 10 ± 2 N.A.
SRT-P-05 59162.8752448474 0.5900 18 ± 2 5.3 ± 1.5 77 ± 29 13 ± 3 N.A.
59162.8752449374 0.5900 23 ± 1 5.3 ± 1.5 98 ± 27 17 ± 3 N.A.
SRT-P-06 59162.9481096844 0.5945 14 ± 2 5.5 ± 1.4 62 ± 23 10 ± 6 N.A.
SRT-P-07 59162.9513861530 0.5947 23 ± 4 2.7 ± 0.7 50 ± 20 8 ± 1 N.A.
SRT-P-08 59162.9515615864 0.5947 20 ± 2 3.0 ± 0.7 49 ± 17 8 ± 1 N.A.
SRT-P-09 59162.9661486339 0.5956 12 ± 2 2.3 ± 0.6 22 ± 9 4 ± 3 N.A.
SRT-P-10 59194.7961833830 0.5448 9 ± 2 2.1 ± 0.6 15 ± 7 3 ± 1 N.A.
SRT-P-11 59244.9407380909 0.6155 22 ± 2 5.2 ± 1.3 92 ± 21 16 ± 2 −11.3 ± 0.6
SRT-P-12 59244.9503715983 0.6160 18.1 ± 0.9 11.8 ± 2.9 172 ± 55 29 ± 6 −10.7 ± 0.6
SRT-P-13 59244.9559004303 0.6164 12 ± 1 7.3 ± 1.9 70 ± 27 12 ± 3 N.A.
SRT-P-14 59258.8293625230 0.4660 16 ± 2 4.9 ± 1.3 64 ± 23 10 ± 2 N.A.
uGMRT-01 59441.0257263218 0.6231 20 ± 2 0.8 ± 0.2 8.9 ± 0.8 2.1 ± 0.2 −5.9 ± 0.5
uGMRT-02 59441.0453208005 0.6243 9.2 ± 0.7 0.6 ± 0.2 2.8 ± 0.9 0.3 ± 0.1 N.A.
uGMRT-03 59441.0575323455 0.6250 20.8 ± 0.6 7.9 ± 0.2 84 ± 3 36 ± 1 −10.5 ± 0.5
uGMRT-04 59441.0622128892 0.6254 7.6 ± 0.8 0.4 ± 0.4 2.5 ± 0.7 0.6 ± 0.1 N.A.
uGMRT-05 59441.0665624511 0.6256 6 ± 1 0.4 ± 0.1 0.6 ± 0.1 0.06 ± 0.01 N.A.
uGMRT-06 59441.0944839544 0.6273 16 ± 4 1.3 ± 1.2 7.9 ± 2.3 0.8 ± 0.2 N.A.
uGMRT-07 59441.1011067833 0.6277 15 ± 8 0.2 ± 0.1 0.9 ± 0.8 0.2 ± 0.2 N.A.

Notes. The second column reports the barycentric time of arrival (TOA) at infinite frequency (TDB units, DE405 ephemeris, TAI clock, DM-delay constant 2.41 × 10−16 pc cm−3 s, reference frequencies for the DM correction are 375.875 MHz for SRT-P and 500 MHz for uGMRT). The TOAs have been computed via the Tempo2 software (Hobbs et al. 2006). The third column contains the bursts phase ϕ (see Sect. 3.1.2). The fourth column reports the FWHM width Δt of the bursts. Sν, Fν, E are respectively the peak flux density, the fluence density and the isotropic energy of the bursts. The last column reports the linear drift rate of the bursts (for the bursts for which it was not possible to assess this value, i.e. a drift was not present, a N.A. value is reported).

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