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

PyCOOL - a Cosmological Object-Oriented Lattice code written in Python

PyMorph: Automated Galaxy Structural Parameter Estimation using Python

QSO Selection Algorithm Using Time Variability and Machine Learning: Selection of 1,620 QSO Candidates from MACHO LMC Database

Quantifying Spectral Features of Type Ia Supernovae

Quasometry, Its Use and Purpose

QUBIC, a bolometric interferometer to measure the B modes of the CMB

QUBIC: The QU Bolometric Interferometer for Cosmology

Query Driven Visualization

Query Driven Visualization of Astronomical Catalogs

R&D Status of Nuclear Emulsion For Directional Dark Matter Search

R&D studies for the development of a compact transmitter able to mimic the acoustic signature of a UHE neutrino interaction