27,079 research outputs found
Enabling pulsar and fast transient searches using coherent dedispersion
We present an implementation of the coherent dedispersion algorithm capable
of dedispersing high-time-resolution radio observations to many different
dispersion measures (DMs). This approach allows the removal of the dispersive
effects of the interstellar medium and enables searches for pulsed emission
from pulsars and other millisecond-duration transients at low observing
frequencies and/or high DMs where time broadening of the signal due to
dispersive smearing would otherwise severely reduce the sensitivity. The
implementation, called 'cdmt', for Coherent Dispersion Measure Trials, exploits
the parallel processing capability of general-purpose graphics processing units
to accelerate the computations. We describe the coherent dedispersion algorithm
and detail how cdmt implements the algorithm to efficiently compute many
coherent DM trials. We present the concept of a semi-coherent dedispersion
search, where coherently dedispersed trials at coarsely separated DMs are
subsequently incoherently dedispersed at finer steps in DM. The software is
used in an ongoing LOFAR pilot survey to test the feasibility of performing
semi-coherent dedispersion searches for millisecond pulsars at 135MHz. This
pilot survey has led to the discovery of a radio millisecond pulsar -- the
first at these low frequencies. This is the first time that such a broad and
comprehensive search in DM-space has been done using coherent dedispersion, and
we argue that future low-frequency pulsar searches using this approach are both
scientifically compelling and feasible. Finally, we compare the performance of
cdmt with other available alternatives.Comment: 8 pages, 7 figures, submitted to Astronomy and Computin
LOFAR discovery of the fastest-spinning millisecond pulsar in the Galactic field
We report the discovery of PSR J09520607, a 707-Hz binary millisecond
pulsar which is now the fastest-spinning neutron star known in the Galactic
field (i.e., outside of a globular cluster). PSR J09520607 was found using
LOFAR at a central observing frequency of 135 MHz, well below the 300 MHz to 3
GHz frequencies typically used in pulsar searches. The discovery is part of an
ongoing LOFAR survey targeting unassociated Fermi Large Area Telescope
-ray sources. PSR J09520607 is in a 6.42-hr orbit around a very
low-mass companion ( M) and we identify a
strongly variable optical source, modulated at the orbital period of the
pulsar, as the binary companion. The light curve of the companion varies by 1.6
mag from at maximum to , indicating that it is
irradiated by the pulsar wind. Swift observations place a 3- upper
limit on the keV X-ray luminosity of erg
s (using the 0.97 kpc distance inferred from the dispersion measure).
Though no eclipses of the radio pulsar are observed, the properties of the
system classify it as a black widow binary. The radio pulsed spectrum of PSR
J09520607, as determined through flux density measurements at 150 and 350
MHz, is extremely steep with (where ).
We discuss the growing evidence that the fastest-spinning radio pulsars have
exceptionally steep radio spectra, as well as the prospects for finding more
sources like PSR J09520607.Comment: 9 pages, 3 figures, 1 table, published in ApJ letter
A Search for Sub-Millisecond Pulsars
We have conducted a search of 19 southern Galactic globular clusters for
sub-millisecond pulsars at 660 MHz with the Parkes 64-m radio telescope. To
minimize dispersion smearing we used the CPSR baseband recorder, which samples
the 20 MHz observing band at the Nyquist rate. By possessing a complete
description of the signal we could synthesize an optimal filterbank in
software, and in the case of globular clusters of known dispersion measure,
much of the dispersion could be removed using coherent techniques. This allowed
for very high time resolution (25.6 us in most cases), making our searches in
general sensitive to sub-millisecond pulsars with flux densities greater than
about 3 mJy at 50 cm. No new pulsars were discovered, placing important
constraints on the proportion of pulsars with very short spin periods in these
clusters.Comment: 8 pages, 3 figures, to appear in Ap
Searching for Millisecond Pulsars: Surveys, Techniques and Prospects
Searches for millisecond pulsars (which we here loosely define as those with
periods 20 ms) in the Galactic field have undergone a renaissance in the
past five years. New or recently refurbished radio telescopes utilizing cooled
receivers and state-of-the art digital data acquisition systems are carrying
out surveys of the entire sky at a variety of radio frequencies. Targeted
searches for millisecond pulsars in point sources identified by the {\it Fermi}
Gamma-ray Space Telescope have proved phenomenally successful, with over 50
discoveries in the past five years. The current sample of millisecond pulsars
now numbers almost 200 and, for the first time in 25 years, now outnumbers
their counterparts in Galactic globular clusters. While many of these searches
are motivated to find pulsars which form part of pulsar timing arrays, a wide
variety of interesting systems are now being found. Following a brief overview
of the millisecond pulsar phenomenon, we describe these searches and present
some of the highlights of the new discoveries in the past decade. We conclude
with predictions and prospects for ongoing and future surveys.Comment: 16 pages, 3 figures, accepted for publication in Classical and
Quantum gravit
Realfast: Real-Time, Commensal Fast Transient Surveys with the Very Large Array
Radio interferometers have the ability to precisely localize and better
characterize the properties of sources. This ability is having a powerful
impact on the study of fast radio transients, where a few milliseconds of data
is enough to pinpoint a source at cosmological distances. However, recording
interferometric data at millisecond cadence produces a terabyte-per-hour data
stream that strains networks, computing systems, and archives. This challenge
mirrors that of other domains of science, where the science scope is limited by
the computational architecture as much as the physical processes at play. Here,
we present a solution to this problem in the context of radio transients:
realfast, a commensal, fast transient search system at the Jansky Very Large
Array. Realfast uses a novel architecture to distribute fast-sampled
interferometric data to a 32-node, 64-GPU cluster for real-time imaging and
transient detection. By detecting transients in situ, we can trigger the
recording of data for those rare, brief instants when the event occurs and
reduce the recorded data volume by a factor of 1000. This makes it possible to
commensally search a data stream that would otherwise be impossible to record.
This system will search for millisecond transients in more than 1000 hours of
data per year, potentially localizing several Fast Radio Bursts, pulsars, and
other sources of impulsive radio emission. We describe the science scope for
realfast, the system design, expected outcomes, and ways real-time analysis can
help in other fields of astrophysics.Comment: Accepted to ApJS Special Issue on Data; 11 pages, 4 figure
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