Hot NH3 Spectra for Astrophysical Applications
Hot stars and interferometry
How achromatic is the stellar scintillation on large telescopes?
How and Why to do VLBI on GPS
How can we distinguish transient pulsars from SETI beacons?
How to Make an Atomic Blog in Your Own Kitchen. Summary of the Workshop: Uncertainties in Atomic Data and How They Propagate in Chemical Abundances
How well do STARLAB and NBODY compare? II: Hardware and accuracy
How well do STARLAB and NBODY4 compare? I: Simple models
How Will Astronomy Archives Survive The Data Tsunami?
Hurst parameter analysis of radio pulsar timing noise
Hydrodynamic simulations with the Godunov SPH
Hydrodynamics of Hypersonic Jets: Experiments and Numerical Simulations
HYPERION: An open-source parallelized three-dimensional dust continuum radiative transfer code
IceCube Collaboration Contributions to ARENA 2010
IceCube's In-Ice Radio Extension: Status and Results
IceCube3--a new window on the Universe
Identification of Dark Matter with directional detection
Identification of important VO spectral services benefiting from deployment on the Grid
Identification of noise artifacts in searches for long-duration gravitational-wave transients
Identifying Patterns on Cosmic Ray Maps with Wavelets on the Sphere