Table 3
List of the 27 non-detected MSPs.
| PSR | P | DM | Binary? | WSRT | BSA | LOFAR | Epoch | T obs |
|
KL01 flux density | Ref. |
| (ms) | (pc cm-3) | detected? | detected? | ObsID | (MJD) | (min) | (mJy) | (mJy at 102 MHz) | |||
|
|
|||||||||||
| J0023+0923 | 3 .050 | 14 .326 | BW | ... | ... | L84514 | 56 311.679 | 20 | 4 | ... | 1 |
| L155443 | 56 473.224 | 20 | |||||||||
| J0340+4130 | 3 .299 | 49 .575 | Isolated | ... | ... | L85586 | 56 318.785 | 20 | 3 | ... | 9 |
| L155441 | 56 473.360 | 20 | |||||||||
| J0613−0200 | 3 .062 | 38 .781 | He WD | n | y | L81271 | 56 289.007 | 20 | 5 | 240 ± 100 | 1 |
| L155440 | 56 473.467 | 20 | |||||||||
| J1327−0755 | 2 .678 | 27 .912 | He WD | ... | ... | L243060 | 56 907.580 | 20 | 5 | ... | 29 |
| J1400−1438∗ | 3 .084 | 4 .928 | He WD | ... | ... | L173398 | 56 533.626 | 20 | 10 | ... | 42 |
| J1455−3330 | 7 .987 | 13 .562 | He WD | ... | ... | L85908 | 56 322.243 | 20 | 60 | ... | 1 |
| J1551−0658 | 7 .09 | 21 .6 | Binary? | ... | ... | L227493 | 56 789.992 | 20 | 7 | ... | 30 |
| J1600−3053 | 3 .598 | 52 .317 | He WD | ... | ... | L146215 | 56 456.919 | 20 | 70 | ... | 1 |
| J1614−2230 | 3 .151 | 34 .487 | CO WD | ... | ... | L85907 | 56 322.269 | 20 | 25 | ... | 25 |
| B1620−26 | 11 .076 | 62 .865 | He WD+UL | ... | y | L85906 | 56 322.285 | 20 | 40 | 450 ± 200 § | 1 |
| J1643−1224 | 4 .622 | 62 .377 | He WD | ... | ... | L81278 | 56 286.424 | 20 | 15 | ... | 1 |
| L85231 | 56 315.324 | 20 | |||||||||
| J1646−2142 | 5 .85 | 29 .8 | Binary | ... | ... | L227491 | 56 787.043 | 20 | 30 | ... | 31 |
| J1719−1438 | 5 .79 | 36 .862 | UL/Carbon WD? | ... | ... | L249812 | 56 964.547 | 20 | 15 | ... | 32, 33 |
| J1721−2457 | 3 .497 | 47 .758 | Isolated | ... | ... | L249814 | 56 964.562 | 20 | 45 | ... | 34, 35 |
| J1741+1351 | 3 .747 | 24 .0 | He WD | ... | ... | L81281 | 56 281.492 | 20 | 4 | ... | 26 |
| L83025 | 56 304.456 | 20 | |||||||||
| J1745+1017 | 2 .652 | 23 .970 | BW? | ... | ... | L249816 | 56 964.576 | 20 | 4 | ... | 36 |
| J1751−2857 | 3 .915 | 42 .808 | He WD | ... | ... | L249818 | 56 964.591 | 20 | 220 | ... | 37 |
| J1804−2717 | 9 .343 | 24 .674 | He WD | ... | ... | L249820 | 56 964.606 | 20 | 110 | ... | 38, 39 |
| J1828+0625 | 3 .63 | 22 .4 | Binary | ... | ... | L249822 | 56 964.620 | 20 | 6 | ... | 31 |
| J1832−0836 | 2 .719 | 28 .18 | Isolated | ... | ... | L249824 | 56 964.635 | 20 | 40 | ... | 40 |
| J1903+0327 | 2 .150 | 297 .548 | MS | ... | ... | L85596 | 56 318.440 | 20 | 20 | ... | 1 |
| J1910+1256 | 4 .984 | 38 .097 | He WD | ... | ... | L85595 | 56 318.456 | 20 | 10 | ... | 1 |
| J1911+1347 | 4 .626 | 30 .99 | Isolated | ... | ... | L243072 | 56 907.790 | 20 | 5 | ... | 41 |
| J1949+3106 | 13 .138 | 164 .126 | CO WD | ... | ... | L85593 | 56 318.487 | 20 | 4 | ... | 27 |
| J2010−1323 | 5 .223 | 22 .181 | Isolated | ... | ... | L84520 | 56 311.490 | 20 | 15 | ... | 1 |
| J2017+0603 | 2 .896 | 23 .918 | He WD | ... | ... | L85591 | 56 318.520 | 20 | 5 | ... | 19 |
| J2229+2643 | 2 .978 | 23 .019 | He WD | ... | y | L84517 | 56 311.587 | 20 | 3 | 60 ± 30 | 28 |
Notes. Column descriptions are the same as in Table 2. is the upper limit on the mean flux density and taken as three times the nominal error of the mean flux density measurements. Flux densities by Kuzmin & Losovsky (2001, KL01) are at 102 or 111 MHz. Some of the pulsars were attempted twice.
Observations were done both at 102 and 111 MHz, and it is not clear for which frequency the flux densities were reported.
The catalogued position of PSR J1400−1438 was about 6′ off from the position derived from over three years of timing with the GBT (J. Swiggum, priv. comm.). We detected this MSP in a recent LOFAR observation using the updated coordinates. The average profile, effective pulse width and flux density measurement for this MSP will be presented elsewhere.
Reference. (1) Desvignes & et al. (2015); (9) J. Hessels (priv. comm.); (19) Cognard et al. (2011); (25) Demorest et al. (2010); (26) Jacoby et al. (2007); (27) Deneva et al. (2012); (28) Wolszczan et al. (2000); (29) Boyles et al. (2013); (30) Hessels et al. (2011); (31) Ray et al. (2012); (32) Ng et al. (2014); (33) Bailes et al. (2011); (34) Edwards & Bailes (2001); (35) Janssen et al. (2010); (36) Barr et al. (2013b); (37) Stairs et al. (2005); (38) Hobbs et al. (2004b); (39) Lorimer et al. (1996); (40) Burgay et al. (2013); (41) Lorimer et al. (2006); (42) Rosen et al. (2013).
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