… The observations presented in this thesis were all made at observing frequencies between
400 MHz and 1400 MHz. in the range where pulse fluxes are strongest and the emissions …

… the Princeton Mark IV data acquisition system at 610 MHz (Stairs, Taylor, & Thorsett
Exploratory observations were 1998). made in January and February, followed by a concentrated …

… For the new postupgrade data that we introduce here, we observed with a ‘‘ coherent ’’
system: the Princeton Mark IV instrument (Stairs et al. 2000a). For each sense of circular …

We report on the discovery of a binary pulsar, PSR J1740—3052, during the Parkes multibeam
survey. Timing observations of the 570-ms pulsar at Jodrell Bank and Parkes show that it …

We present a large sample of high-precision, coherently dedispersed polarization profiles of
millisecond pulsars (MSPs) at frequencies between 410 and 1414 MHz. These data include …

… In this paper we describe the Princeton Mark IV system, a baseband recorder developed
primarily for pulsar astronomy and optimized for use with the Arecibo telescope; within the next …

… We used and fixed the Mark III DM bin derived by Stairs et al. (1998) due to systematic errors
they found in the Mark III 430 MHz TOAs, which we discarded from this study. The results of …

Pre-detection, or``coherent,''dedispersion is a powerful technique which completely eliminates
the effects of dispersive smearing on pulsar profiles, greatly increasing the precision of …

We present a new timing solution for PSR B1534+12, based on coherently-dedispersed
observations at Jodrell Bank and, recently, Arecibo. The new data have resulted in improved …

Neutron stars provide insight into the structure of matter at extreme densities, the validity of
gravitational theories near strongly self-gravitating objects, and QED phenomena in high …