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Table 1.

Parameters of the observed pulsars and observational setup of the observations in the LC3_036 proposal.

J1412+7922 J1958+2846 J1932+1916 J1907+0919
Right ascension, α (J2000) 14 12 56 19 58 40 19 32 20 19 07 14.33
Declination, δ (J2000) +79 22 04 +28 45 54 +19 16 39 +09 19 20.1
Period, P (s) 0.05919907107 0.29038924475 0.208214903876 5.198346
Period derivative, (s s−1) 3.29134×10−15 2.12038×10−13 9.31735×10−14 9.2×10−11
Epoch (MJD) 58150(a) 54800(b) 55214(c) 53628(d)
LOFAR ObsID L257877 L258545 L259173 L216886
Obs. date (MJD) 57038 57046 57068 56755
Sample time (ms) 0.16384 1.31072 1.31072 0.65536
Test pulsar detected B1322+83 B1952+29 B1933+16 B1907+10
Periodic flux density (mJy at GHz) < 4 at 0.385(e) < 2.0 at 0.15(g) < 2.9 at 0.15(g) 50 at 0.111(h)
< 0.05 at 1.36(f) < 0.005 at 1.51(b) < 0.075 at 1.4(c) < 0.4 at 0.43(i)
< 0.3 at 1.38(e) < 0.3 at 1.41(i)
< 0.012 @ 1.95(j)
LOFAR periodic sensitivity Slim,p (mJy) 0.26 ± 0.13 0.53 ± 0.26 0.73 ± 0.36 1.39 ± 0.69
LOFAR single pulse sensitivity Slim,sp (Jy) 1.47 ± 0.73 1.35 ± 0.68 2.20 ± 1.10 0.84 ± 0.82

Notes. The beam of each observation was centered on the reported pulsar coordinates. The bottom rows list the earlier periodicity and single-pulse search limits. The upper limits from Frail et al. (2016) described in the main text are period-averaged flux densities and are not listed here. The last row lists the limits from the current work for S/N = 5, with errors of 50% (Bilous et al. 2016).

References. (a)Bogdanov et al. (2019), (b)Ray et al. (2011), (c)Pletsch et al. (2013), (d)Mereghetti et al. (2006), (e)Hessels et al. (2007), (f)Zane et al. (2011), (g)Grießmeier et al. (2021), (h)Shitov et al. (2000), (i)Lorimer & Xilouris (2000), (j)Lazarus et al. (2012).

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