A multiwavelength false-color image of the “Toothbrush” cluster of galaxies, 1RXS J0603.3+4214. The intensity in red shows the radio emission, blue is X -ray, and the background color composite is optical emission. Astronomers studying the cluster with new radio observations combined with other wavelengths have been able to confirm the galaxy merger scenario and estimate the magnetic field strength in the shocks. Credit: van Weeren et al.

Phase-folded unbinned HATSouth light curves for HATS-50 (upper left), HATS-51 (upper right), HATS-52 (lower left) and HATS-53 (lower right). In each case we show two panels. The top panel shows the full light curve, while the bottom panel shows the light curve zoomed-in on the transit. The solid lines show the model fits to the light curves. The dark filled circles in the bottom panels show the light curves binned in phase with a bin size of 0.002. Credit: Henning et al. 2017.

Comparison of microRNA extraction using nanowires versus conventional collection (a) Scatterplot comparing normalized intensities of microRNAs extracted with the nanowire device versus conventional collection by ultracentrifugation. (b) Histogram showing the frequency of microRNA species at different fluorescent intensities collected by nanowires (red) and ultracentrifugation (blue). Both the scatterplot and histogram analyses show a notably greater abundance of extracted microRNAs using the nanowire technology. © Takao Yasui

The economic impact of SOEC, developed by Professor Guntae Kim in September, 2016. Credit: UNIST