Using atmospheric composition as a metric for detecting life on habitable planets

Using Biogenic Sulfur Gases as Remotely Detectable Biosignatures on Anoxic Planets

Using Case Studies in Calculus-based Physics

Using causal models to distinguish between neurogenesis-dependent and -independent effects on behaviour

Using Differential Ion Mobility as a Conformational Filter to Simplify Spectra of Biomolecular Ions

Using Edible Models to Communicate Principles of Comet Science: Assembling Amino Acids from Simpler Molecules

Using Electrical Impedance Spectroscopy to Detect Water in Planetary Regoliths

Using FISH-SIMS to Study Marine Methane Oxidation Coupled to the Reduction of Metal Oxides, a Plausible Microbial Metabolism for Subsurface Mars

Using graph concepts to understand the organization of complex systems

Using invariants for phylogenetic tree construction

Using profiles based on hydropathy properties to define essential regions for splicing

Using the Abitibi Greenstone Belt to understand Martian hydrothermal systems and the potential for biosignature preservation in high temperature aqueous environments

Using the tangle: a consistent construction of phylogenetic distance matrices for quartets

Utilization of inorganic substrata and production of organic substances by non-differentiated plant tissue cultures cultivated in low magnetic field

Utilizing active mid-infrared microspectrometry for in situ analysis of cryptoendolithic microbial communities of Battleship Promontory, Dry Valleys, Antarctica

Utilizing of protein splicing phenomenon for optimization of obtaining and purification of the recombinant human growth hormone

Utilizing the information content in two-state trajectories

UV habitability and dM stars: an approach for evaluation of biological survival

UV Photochemistry of DNA In Vitro and in Bacillus subtilis Spores at Earth-Ambient and Low Atmospheric Pressure: Implications for Spore Survival on Other Planets or Moons in the Solar System

UV photolysis of polyynes at λ=254 nm and at λ>222 nm