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Table 2

Overview of the EPTA DR2 25 pulsar data set.

Pulsar Jname Telescopes MJD range Tspan (yr) NTOA Median σTOA (µs) wrms (µs) wrms, whitened (µs)
P L S C
J0030+0451 EFF, LT, NRT, WSRT, LEAP 51275–59294 22.0 4069 3.40 6.07 2.85 2.30
J0613−0200(*) EFF, LT, NRT, WSRT, LEAP 50931–59293 22.9 2909 7.40 1.43 6.16 2.47 1.06
J0751+1807(*) EFF, LT, NRT, WSRT, LEAP 50460–59294 24.2 3613 2.22 4.43 2.12 1.50
J0900−3144 LT, NRT 54286–59269 13.6 6064 2.95 8.92 4.28 2.60
J1012+5307(*) EFF, LT, NRT, WSRT, LEAP 50647–59295 23.7 5325 3.77 1.76 5.59 4.78 1.28 1.02
J1022+1001(*) EFF, LT, NRT, WSRT, LEAP 50361–59294 24.5 2445 11.3 2.19 4.42 2.99 1.78 1.56
J1024−0719 EFF, LT, NRT, WSRT, LEAP 50841–59294 23.1 2522 2.38 7.64 1.10 1.02
J1455−3330 LT, NRT 53375–59117 15.7 2815 7.23 17.8 2.52 2.46
J1600−3053(*) EFF, LT, NRT, WSRT, LEAP 53998–59230 14.3 2982 0.48 1.50 2.68 0.37
J1640+2224 EFF, LT, NRT, WSRT, LEAP 50459–59385 24.4 2006 3.57 7.65 1.13 1.10
J1713+0747(*) EFF, LT, NRT, WSRT, LEAP 50360–59295 24.5 5003 3.13 0.32 0.54 0.67 0.43 0.20
J1730−2304 EFF, LT, NRT 53397–59279 16.1 1315 1.57 7.26 1.00 0.83
J1738+0333 EFF, LT, NRT, WSRT 54103–59259 14.1 1019 4.31 2.90 2.33
J1744−1134(*) EFF, LT, NRT, WSRT, LEAP 50460–59230 24.0 1946 3.60 0.90 2.29 1.15 1.01 0.56
J1751−2857 LT, NRT 53746–59111 14.7 398 3.17 3.73 2.34
J1801−1417 LT, NRT 54206–59214 13.7 449 4.09 3.94 2.46
J1804−2717 LT, NRT 53766–59145 14.7 723 5.94 1.80 1.63
J1843−1113 EFF, LT, NRT, WSRT 53156–59293 16.8 893 1.37 2.64 3.47 0.81
J1857+0943(*) EFF, LT, NRT, WSRT, LEAP 50458–59258 24.1 1540 1.70 4.05 6.85 1.38 1.05
J1909−3744(*) NRT 53368–59115 15.7 2503 0.29 0.57 0.73 0.14
J1910+1256 LT, NRT 53725–59282 15.2 538 2.65 2.03 1.77
J1911+1347 EFF, LT, NRT 54095–59282 14.2 882 1.22 1.36 1.06 0.75
J1918−0642 EFF, LT, NRT, WSRT, LEAP 52095–59294 19.7 1361 2.04 4.14 1.78 1.31
J2124−3358(*) LT, NRT 53365–59213 16.0 2018 3.70 12.6 2.24 2.17
J2322+2057 EFF, LT, NRT 53905–59268 14.7 804 10.9 4.08 4.08

Notes. The columns represent the name of the pulsar, the telescopes that have collected the data, the number of TOAs, the timespan Tspan of the data set, the median σTOA in each frequency band, the weighted rms (wrms) of the timing residuals, and the weighted rms after subtracting both red and DM noise (i.e. of the whitened residuals). The corresponding frequency coverage for the P, L, S, and C bands is 0.3–1.0, 1.0–2.0, 2.0–4.0, and 4.0–8.0 GHz, respectively. The asterisk next to the pulsar name denotes that this pulsar is also included in the InPTA data release (also see Appendix A).

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