WorldCat Identities

Bailes, M. (Matthew)

Overview
Works: 16 works in 34 publications in 1 language and 248 library holdings
Genres: Conference papers and proceedings  Observations 
Roles: Editor, Author, Other
Classifications: QB843.P8, 523.8874
Publication Timeline
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Most widely held works about M Bailes
 
Most widely held works by M Bailes
Pulsars, problems and progress : IAU Colloquium 160 : proceedings held at the Research Centre for Theoretical Astrophysics, University of Sydney, Australia, 8-12 January 1996 by IAU Colloquium( Book )

3 editions published in 1996 in English and held by 114 WorldCat member libraries worldwide

Pulsars : problems and progress, IAU Colloquium 160 : proceedings held at the Research Centre for Theoretical Astrophysics, University of Sydney, Australia, 8-12 January 1996 by Union astronomique internationale( Book )

2 editions published in 1996 in English and held by 3 WorldCat member libraries worldwide

Pulsars: problems and progress by International Astronomical Union( Book )

2 editions published in 1996 in English and held by 3 WorldCat member libraries worldwide

Implications of a VLBI distance to the double pulsar J0737-3039A/B by A. T Deller( Book )

2 editions published in 2009 in English and held by 2 WorldCat member libraries worldwide

"The double pulsar J0737-3039A/B is a unique system with which to test gravitational theories in the strong-field regime. However, the accuracy of such tests will be limited by knowledge of the distance and relative motion of the system. Here we present very long baseline interferometry (VLBI) observations which reveal that the distance to PSR J0737-3039A/B is 1150-160+220 parsecs, more than double previous estimates, and confirm its low transverse velocity (~9 kilometers per second). Combined with a decade of pulsar timing, these results will allow tests of gravitational radiation emission theories at the 0.01% uncertainty level, putting stringent constraints on theories that predict dipolar gravitational radiation. They also allow insight into the system's formation and the source of its high-energy emission."
Transformation of a star into a planet in a millisecond pulsar binary by M Bailes( Book )

1 edition published in 2011 in English and held by 1 WorldCat member library worldwide

Wide-band profile domain pulsar timing analysis( )

1 edition published in 2016 in English and held by 1 WorldCat member library worldwide

Abstract We extend profile domain pulsar timing to incorporate wide-band effects such as frequency-dependent profile evolution and broad-band shape variation in the pulse profile. We also incorporate models for temporal variations in both pulse width and in the separation in phase of the main pulse and interpulse. We perform the analysis with both nested sampling and Hamiltonian Monte Carlo methods. In the latter case, we introduce a new parametrization of the posterior that is extremely efficient in the low signal-to-noise regime and can be readily applied to a wide range of scientific problems. We apply this methodology to a series of simulations, and to between seven and nine years of observations for PSRs J1713+0747, J1744−1134 and J1909−3744 with frequency coverage that spans 700–3600Mhz. We use a smooth model for profile evolution across the full frequency range, and compare smooth and piecewise models for the temporal variations in dispersion measure (DM). We find that the profile domain framework consistently results in improved timing precision compared to the standard analysis paradigm by as much as 40percent for timing parameters. Incorporating smoothness in the DM variations into the model further improves timing precision by as much as 30percent. For PSR J1713+0747, we also detect pulse shape variation uncorrelated between epochs, which we attribute to variation intrinsic to the pulsar at a level consistent with previously published analyses. Not accounting for this shape variation biases the measured arrival times at the level of ∼30ns, the same order of magnitude as the expected shift due to gravitational waves in the pulsar timing band
Timing Studies of Radio Pulsars by Setnam L Shemar( Book )

1 edition published in 1991 in English and held by 1 WorldCat member library worldwide

The origin of pulsar velocities by M Bailes( )

1 edition published in 1989 in English and held by 1 WorldCat member library worldwide

Optical detection of the companion of the millisecond pulsar J0437-4715 by J. F Bell( Book )

1 edition published in 1993 in English and held by 1 WorldCat member library worldwide

The High Time Resolution Universe Pulsar Survey – XIII. PSR J1757−1854, the most accelerated binary pulsar( )

1 edition published in 2018 in English and held by 1 WorldCat member library worldwide

The SUrvey for Pulsars and Extragalactic Radio Bursts – III. Polarization properties of FRBs 160102 and 151230( )

1 edition published in 2018 in English and held by 1 WorldCat member library worldwide

Abstract We report on the polarization properties of two fast radio bursts (FRBs): 151230 and 160102 discovered in the SUrvey for Pulsars and Extragalactic Radio Bursts (SUPERB) at the Parkes Radio Telescope. FRB 151230 is observed to be 6 ± 11 per cent circularly polarized and 35 ± 13 per cent linearly polarized with a rotation measure (RM) consistent with zero. Conversely, FRB 160102 is observed to have a circular polarization fraction of 30 ± 11 per cent, linear polarization fraction of 84 ± 15 per cent for RM = −221(6) radm, and the highest measured dispersion measure (2596.1 ± 0.3 pc cm) for an FRB to date. We examine possible progenitor models for FRB 160102 in extragalactic, non-cosmological and cosmological scenarios. After accounting for the Galactic foreground contribution, we estimate the intrinsic RM to be −256(9) rad m in the low-redshift case and ∼−2.4×10 rad m in the high-redshift case. We assess the relative likeliness of these scenarios and how each can be tested. We also place constraints on the scattering measure and study the impact of scattering on the signal’s polarization position angle
A test of general relativity from the three-dimensional orbital geometry of a binary pulsar by W Van Straten( )

1 edition published in 2001 in English and held by 0 WorldCat member libraries worldwide

 
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Alternative Names
Bailes, M.

Bailes, Matthew

Languages
English (34)