Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile
Jodrell Bank Pulsar Group

@uom_pulsars

We are the Jodrell Bank Pulsars and Time Domain Astrophysics Group @officialUoM.

#Pulsars, #FastRadioBursts, #Exoplanets, #Novae

ID: 1219284492055142401

linkhttps://bit.ly/38GXBly calendar_today20-01-2020 15:45:43

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Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

09:33:52 UTC. Now observing the intermittent pulsar PSR B1931+24 with the Mark II telescope. Rotation period: 0.8 s Age: 2 MYr Distance: 4.6 kpc

09:33:52 UTC. Now observing the intermittent pulsar PSR B1931+24 with the Mark II telescope.

Rotation period: 0.8 s
Age: 2 MYr
Distance: 4.6 kpc
Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

14:52:52 UTC. Now observing the mode-switching pulsar PSR B0329+54 with the Mark II telescope. Rotation period: 0.7 s Age: 6 MYr Distance: 1.0 kpc

14:52:52 UTC. Now observing the mode-switching pulsar PSR B0329+54 with the Mark II telescope.

Rotation period: 0.7 s
Age: 6 MYr
Distance: 1.0 kpc
Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

15:12:57 UTC. Now observing the young glitching pulsar PSR J0631+1036 with the Mark II telescope. Rotation period: 0.3 s Age: 44 kYr Distance: 2.1 kpc

15:12:57 UTC. Now observing the young glitching pulsar PSR J0631+1036 with the Mark II telescope.

Rotation period: 0.3 s
Age: 44 kYr
Distance: 2.1 kpc
Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

17:02:19 UTC. Now observing the Crab pulsar PSR B0531+21 with the Mark II telescope. Rotation period: 33.4 ms Age: 1 kYr Distance: 2.0 kpc

17:02:19 UTC. Now observing the Crab pulsar PSR B0531+21 with the Mark II telescope.

Rotation period: 33.4 ms
Age: 1 kYr
Distance: 2.0 kpc
Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

19:22:07 UTC. Now observing the mode-switching pulsar PSR B1540-06 with the Mark II telescope. Rotation period: 0.7 s Age: 13 MYr Distance: 3.2 kpc

19:22:07 UTC. Now observing the mode-switching pulsar PSR B1540-06 with the Mark II telescope.

Rotation period: 0.7 s
Age: 13 MYr
Distance: 3.2 kpc
Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

19:52:01 UTC. Now observing the binary millisecond pulsar PSR J1713+0747 with the Mark II telescope. Rotation period: 4.6 ms Age: 8490 MYr Distance: 1.2 kpc Companion: White dwarf

19:52:01 UTC. Now observing the binary millisecond pulsar PSR J1713+0747 with the Mark II telescope.

Rotation period: 4.6 ms
Age: 8490 MYr
Distance: 1.2 kpc
Companion: White dwarf
Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

21:21:42 UTC. Now observing the millisecond pulsar PSR B1937+21 with the Mark II telescope. Rotation period: 1.6 ms Age: 235 MYr Distance: 3.5 kpc

21:21:42 UTC. Now observing the millisecond pulsar PSR B1937+21 with the Mark II telescope.

Rotation period: 1.6 ms
Age: 235 MYr
Distance: 3.5 kpc
Jodrell Bank Pulsar Group (@uom_pulsars) 's Twitter Profile Photo

Michael Keith of UoM Physics & Astronomy, and his PhD student Iuliana Niţu (Iuliana Nițu) have investigated the effects of quasi-periodicities in the timing noise of pulsars, on how well we can measure their timing parameters. Released on arXiv.org today -> arxiv.org/abs/2306.03529

Michael Keith of <a href="/UoMPhysics/">UoM Physics & Astronomy</a>, and his PhD student Iuliana Niţu (<a href="/iulicn29/">Iuliana Nițu</a>) have investigated the effects of quasi-periodicities in the timing noise of pulsars, on how well we can measure their timing parameters. Released on <a href="/arxiv/">arXiv.org</a> today -&gt; arxiv.org/abs/2306.03529