William T. Reach

TL;DR: In this article, the authors used the archival SOFIA/HAWC+ polarimetric data observed toward Ophiuchus (Oph) A cloud hosted by a B association star at 89 and 154 µm and found that the fractional polarization of thermal dust emission first increases with grain temperature and then decreases once the grain temperature exceeds µm 25-32 K. The latter trend differs from the prediction of the popular RAdiative Torques (RATs) alignment theory which implies a monotonic increase of the polarization fraction with thegrain temperature.

TL;DR: In this article, an infrared color discrimination tool was used to distinguish between solar system objects and extrasolar sources using the First Look Survey-Ecliptic Plane Component (FLS-EPC) data set.

TL;DR: Pan-STARRS (Pan-2012 K1) as discussed by the authors is a dynamically new Oort Cloud comet, conducted with NASA's Stratospheric Observatory for Infrared Astronomy facility (+FORCAST) in 2014 June.

TL;DR: In this article, the authors present new calculations of grain trajectories and the resultant grain density distribution for small ISDGs propagating through the heliosphere, using three-dimensional (3-D) magnetohydrodynamic/kinetic models designed to match data on the shape of the termination shock and the relative deflection of interstellar neutral H and He flowing into the helIosphere.