Table 2.
Pulsars discovered or independently re-discovered (detected) in the TULIPP survey.
| LoTSS source | Pulsar name | P | p | DM | RM | Discovery notes |
|---|---|---|---|---|---|---|
| (s) | (%) | (pc cm−3) | (rad m−2) | |||
| Discoveries | ||||||
| ILT J104937.86+582217.6 | PSR J1049+5822 | 0.7276 | 61L | 12.364(1) | 3.9(1) | TULIPP (this work) |
| ILT J160218.82+390101.5 | PSR J1602+3901 | 0.003708 | 5|V| | 17.2590(2) | – | TULIPP (this work) |
| Detections | ||||||
| ILT J022042.11+362655.7 | PSR J0220+3626 | 1.029 | 4|V| | 45.422(5) | – | LPA (Tyul’bashev et al. 2016) |
| ILT J074212.22+411015.0 | PSR J0742+4110 | 0.003139 | − | 20.814(1) | – | GBNCC (Stovall et al. 2014) |
| ILT J163035.93+355042.5 | PSR J1630+3550 | 0.003229 | 28L | 17.45494(8) | 8.5(1) | AO327 (Deneva et al. 2013) |
| ILT J221227.42+245034.4 | PSR J2212+2450 | 0.003907 | − | 25.213(1) | – | AO327 (Deneva et al. 2013) |
| ILT J222741.76+303820.8 | PSR J2227+3038 | 0.8424 | 23L 10|V| | 19.961(6) | −59.4(1) | Arecibo (Camilo et al. 1996) |
Notes. Pulse period is presented to four significant figures. The fractional polarisation, p, is given for sources that have sufficient a signal-to-noise ratios to be measured using the beam-formed observations, where L denotes linear and |V| absolute circular polarisations (the systematic uncertainties are expected to be ≈5 − 10%; Noutsos et al. 2015). DM and RM measurements using the beam-formed observations are also provided. These are the mean values obtained from the beam-formed data.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.