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Pulsar distances and the galactic distribution of free electrons
We describe a quantitative model for the distribution of free electrons in the Galaxy, with particular emphasis on its utility for estimating pulsar distances from dispersion measures. Contrary to… Expand
Further experimental tests of relativistic gravity using the binary pulsar PSR 1913+16
Fourteen-year observations of the binary pulsar PSR 1913 + 16 provided data consistent with a straightforward model allowing for the motion of the earth, special and general relativistic effects… Expand
High - precision timing of millisecond pulsars. 3: Long - term monitoring of PSRs B1855+09 and B1937+21
On the orbital period change of the binary pulsar PSR 1913+16
The theoretical significance of the raw observational parameter called the rate of orbital period change, P b obs , of the binary pulsar PSR 1913+16 is reexamined. It is shown that the current… Expand
Timing Measurements of the Relativistic Binary Pulsar PSR B1913+16
We present results of more than three decades of timing measurements of the first known binary pulsar, PSR B1913+16. Like most other pulsars, its rotational behavior over such long timescales is… Expand
Timing behavior of 96 radio pulsars
We present results from observations of 104 pulsars made between 1989 August and 1993 April, including timing solutions for 96 of them. Pulse profiles were recorded at four frequencies in the range… Expand
A search for low-luminosity pulsars.
The results of Phase I of the Princeton-NRAO pulsar survey, carried out at 390 MHz using the 92 m telescope at Green Bank, West Virginia, are presented. This search discovered 34 new pulsars and… Expand
The eclipsing millisecond pulsar PSR 1957 + 20
Information obtained over the past year on the eclipsing millisecond pulsar PSR 1957 + 20 and its orbiting companion is discussed. The pulsar is found to be similar in many ways to other millisecond… Expand
Princeton-Arecibo Declination-Strip Survey for Millisecond Pulsars. I.
Observations of the Crab pulsar and nebula by the EGRET telescope on the Compton Gamma-Ray Observatory
The Crab pulsar and nebula were observed three times in 1991 April to June by the Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma-Ray Observatory (CGRO): April 23 to May 7, May… Expand