Progress with the LOFAR Imaging Pipeline

Progressive Prediction of Turbulence Using Wave-Front Sensor Data in Adaptive Optics Using Data Mining

Propagation of Aberrations through Phase Induced Amplitude Apodization coronagraph

Properties of a Variable-delay Polarization Modulator

Prospects for accurate distance measurements of pulsars with the SKA: enabling fundamental physics

Prospects of Search for Solar Axions with Mass over 1 eV and Hidden Sector Photons

Protection of existing and potential observatory sites: Triennial report 2009-2012 of IAU Commission 50

Proto-Model of an Infrared Wide-Field Off-Axis Telescope

ProtoEXIST: Advanced Prototype CZT Coded Aperture Telescopes for EXIST

Prototyping scalable digital signal processing systems for radio astronomy using dataflow models

PSDF: Particle Stream Data Format for N-Body Simulations

Pseudo-Newtonian Potentials for Nearly Parabolic Orbits

PSRCHIVE and PSRFITS: Definition of the Stokes Parameters and Instrumental Basis Conventions

Public Perception of Astronomers: Revered, Reviled and Ridiculed

Pulsar science with the Five hundred metre Aperture Spherical Telescope

Pulsar Science with the Green Bank 43m Telescope

Pulsar timing analysis in the presence of correlated noise

Pulsars with the Australian Square Kilometre Array Pathfinder

Pupil remapping for high contrast astronomy: results from an optical testbed

Pushing the limit of instrument capabilities