Excess noise from scattered light poses a persistent challenge in the analysis of data gravitational wave detectors such as LIGO. We integrate physically motivated model for behavior these "glitches" into standard Bayesian pipeline used science. This allows inference free parameters this model, and subtraction models to produce glitch-free versions data. show that is an effective discriminator ...

We review recent progress in high-resolution imaging of scattered light from disks around young stellar objects. Many new disks have been discovered or imaged in scattered light, and improved instrumentation and observing techniques have led to better disk images at optical, near-infrared, and thermal-infrared wavelengths. Multi-wavelength datasets are particularly valuable, as dust particle pr...

We describe a single-shot method to differentiate unscattered and scattered components of light transmission through a heterogeneous translucent material. Directly-transmitted components travel in a straight line from the light source, while scattered components originate from multiple scattering centers in the volume. Computer vision methods deal with participating media via 2D contrast enhanc...