9 research outputs found
MeerTRAP: Twelve Galactic fast transients detected in a real-time, commensal MeerKAT survey
MeerTRAP is a real-time untargeted search project using the MeerKAT telescope
to find single pulses from fast radio transients and pulsars. It is performed
commensally with the MeerKAT large survey projects (LSPs), using data from up
to 64 of MeerKAT's 13.96~m dishes to form hundreds of coherent beams on sky,
each of which is processed in real time to search for millisecond-duration
pulses. We present the first twelve Galactic sources discovered by MeerTRAP,
with DMs in the range of 33--381~pc~cm. One source may be Galactic or
extragalactic depending on the Galactic electron density model assumed.
Follow-up observations performed with the MeerKAT, Lovell, and Parkes radio
telescopes have detected repeat pulses from seven of the twelve sources. Pulse
periods have been determined for four sources. Another four sources could be
localised to the arcsecond-level using a novel implementation of the tied-array
beam localisation method.Comment: 16 pages, 14 figure
FRB 20210405I: a nearby Fast Radio Burst localised to sub-arcsecond precision with MeerKAT
We present the first sub-arcsecond localised Fast Radio Burst (FRB) detected
using MeerKAT. FRB 20210405I was detected in the incoherent beam using the
MeerTRAP pipeline on 2021 April 05 with a signal to noise ratio of 140.8 and a
dispersion measure of 565.17 pc cm. It was detected while MeerTRAP was
observing commensally with the ThunderKAT large survey project, and was
sufficiently bright that we could use the ThunderKAT 8s images to localise the
FRB. Two different models of the dispersion measure in the Milky Way and halo
suggest that the source is either right at the edge of the Galaxy, or outside.
This highlights the uncertainty in the Milky Way dispersion measure models,
particularly in the Galactic Plane, and the uncertainty of Milky Way halo
models. Further investigation and modelling of these uncertainties will be
facilitated by future detections and localisations of nearby FRBs. We use the
combined localisation, dispersion measure, scattering, specific luminosity and
chance coincidence probability information to find that the origin is most
likely extra-galactic and identify the likely host galaxy of the FRB: 2MASS
J17012494932475. Using SALT spectroscopy and archival observations of the
field, we find that the host is a disk/spiral galaxy at a redshift of
.Comment: 15 pages, 4 tables, 10 figures. Accepted to MNRA
FRB 20210405I: the first Fast Radio Burst sub-arcsecond localised with MeerKAT
International audienceWe present the first sub-arcsecond localised Fast Radio Burst (FRB) detected using MeerKAT. The FRB, FRB 20210405I, was detected in the incoherent beam using the MeerTRAP pipeline on 2021 April 05 with a signal to noise ratio of 140.8 and a dispersion measure of 565.17 pc cm. It was detected while MeerTRAP was observing commensally with the ThunderKAT large survey project, and was sufficiently bright that we could use the ThunderKAT 8s images to localise the FRB. Two different models of the dispersion measure in the Milky Way and halo suggest that the source is either right at the edge of the Galaxy, or outside. However, we use the combined localisation, dispersion measure, scattering, specific luminosity and chance coincidence probability information to find that the origin is most likely extragalactic and identify the likely host galaxy of the FRB: 2MASS J17012494932475. Using SALT spectroscopy and archival observations of the field, we find that the host is a disk/spiral galaxy at a redshift of
Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds
The radio-emitting neutron star population encompasses objects with spin
periods ranging from milliseconds to tens of seconds. As they age and spin more
slowly, their radio emission is expected to cease. We present the discovery of
an ultra-long period radio-emitting neutron star, J0901-4046, with spin
properties distinct from the known spin and magnetic-decay powered neutron
stars. With a spin-period of 75.88 s, a characteristic age of 5.3 Myr, and a
narrow pulse duty-cycle, it is uncertain how radio emission is generated and
challenges our current understanding of how these systems evolve. The radio
emission has unique spectro-temporal properties such as quasi-periodicity and
partial nulling that provide important clues to the emission mechanism.
Detecting similar sources is observationally challenging, which implies a
larger undetected population. Our discovery establishes the existence of
ultra-long period neutron stars, suggesting a possible connection to the
evolution of highly magnetized neutron stars, ultra-long period magnetars, and
fast radio burstsComment: Published in Nature Astronomy -
https://www.nature.com/articles/s41550-022-01688-
Discoveries and Timing of Pulsars in NGC 6440
Using the MeerKAT radio telescope, a series of observations have been
conducted to time the known pulsars and search for new pulsars in the globular
cluster NGC 6440. As a result, two pulsars have been discovered, NGC 6440G and
NGC 6440H, one of which is isolated and the other a non-eclipsing (at
frequencies above 962 MHz) "Black Widow", with a very low mass companion
(M > 0.006 M). It joins the other binary pulsars discovered
so far in this cluster which all have low companion masses (M < 0.30
M). We present the results of long-term timing solutions obtained
using data from both Green Bank and MeerKAT telescopes for these two new
pulsars and an analysis of the pulsars NGC 6440C and NGC 6440D. For the
isolated pulsar NGC 6440C, we searched for planets using a Markov Chain Monte
Carlo technique. We find evidence for significant unmodelled variations but
they cannot be well modelled as planets nor as part of a power-law red-noise
process. Studies of the eclipses of the "Redback" pulsar NGC 6440D at two
different frequency bands reveal a frequency dependence with longer and
asymmetric eclipses at lower frequencies (962-1283 MHz).Comment: 14 pages, 10 figures, 4 tables. Accepted for publication in MNRA