Application of a Bayesian Method to Absorption Spectral-Line Finding in Simulated ASKAP Data

Application of Bayesian model averaging to measurements of the primordial power spectrum

Application of cross correlations between CMB and large scale structure to constraints on the primordial non-Gaussianity

Application of slingshot model to the giant radio galaxy DA240 (Brief : DA 240 in slingshot model)

Application of the Kolmogorov-Smirnov test to CMB data: Is the universe really weakly random?

Application of XFaster power spectrum and likelihood estimator to Planck

Applications of Bayesian model averaging to the curvature and size of the Universe

Applications of Cosmological Perturbation Theory

Applications of the IGIMF-theory to the astrophysics of galaxies

Applying MOG to lensing: Einstein rings, Abell 520 and the Bullet Cluster

Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations

Applying the Analytic Theory of Colliding Ring Galaxies

Approximate Analytic Spectra of Reionized CMB Anisotropies and Polarization generated by Relic Gravitational Waves

ArborZ: Photometric Redshifts Using Boosted Decision Trees

ARCADE 2 Measurement of the Extra-Galactic Sky Temperature at 3-90 GHz

Archipelagian Cosmology: Dynamics and Observables in a Universe with Discretized Matter Content

ARCRAIDER II: Arc search in a sample of non-Abell clusters

Are $^{12}$CO lines good indicators of the star formation rate in galaxies?

Are Active Galactic Nuclei the Solution to the Excess Cosmic Radio Background at 1.4 GHz?

Are all perturbations created equal? An analysis of the WMAP 5- and 7-year data without inflationary prejudice