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The High Time Resolution Universe Survey - XI. Discovery of five recycled pulsars and the optical detectability of survey white dwarf companions
S. D. Bates, D. Thornton, M. Bailes +20
We present the discovery of a further five recycled pulsar systems in the mid-Galactic latitude portion of the High Time Resolution Universe (HTRU) Survey. The pulsars have rotatio…
Arecibo Pulsar Survey Using ALFA. III. Precursor Survey and Population Synthesis
J. K. Swiggum, D. R. Lorimer, M. A. McLaughlin +33
The Pulsar Arecibo L-band Feed Array (PALFA) Survey uses the ALFA 7-beam receiver to search both inner and outer Galactic sectors visible from Arecibo ($32^{\circ}\lesssim \ell \le…
The High Time Resolution Universe Survey - IX: Polarimetry of long-period pulsars
C. Tiburzi, S. Johnston, M. Bailes +16
We present a polarimetric analysis of 49 long-period pulsars discovered as part of the High Time Resolution Universe (HTRU) southern survey. The sources exhibit the typical charact…
Goals, Strategies and First Discoveries of AO327, the Arecibo All-Sky 327 MHz Drift Pulsar Survey
J. S. Deneva, K. Stovall, M. A. McLaughlin +5
We report initial results from AO327, a drift survey for pulsars with the Arecibo telescope at 327 MHz. The first phase of AO327 will cover the sky at declinations of -1 to 28 degr…
The High Time Resolution Universe Pulsar Survey VIII: The Galactic millisecond pulsar population
L. Levin, M. Bailes, B. R. Barsdell +17
We have used millisecond pulsars (MSPs) from the southern High Time Resolution Universe (HTRU) intermediate latitude survey area to simulate the distribution and total population o…
The pulsar spectral index distribution
Samuel D. Bates, Duncan R. Lorimer, Joris P. W. Verbiest
The flux density spectra of radio pulsars are known to be steep and, to first order, described by a power-law relationship of the form S_ν \propto ν^α, where S_ν is the flux densit…