Laser-produced transient tin plasmas are the sources of extreme ultraviolet (EUV) light at
13.5 nm wavelength for next-generation nanolithography, enabling the continued …

A long-standing paradigm in astrophysics is that collisions—or mergers—of two neutron
stars form highly relativistic and collimated outflows (jets) that power γ-ray bursts of short …

With the first direct detection of merging black holes in 2015, the era of gravitational wave
(GW) astrophysics began. A complete picture of compact object mergers, however, requires …

We report the discovery and monitoring of the near-infrared counterpart (AT2017gfo) of a
binary neutron-star merger event detected as a gravitational wave source by Advanced …

The 2017 detection of the inspiral and merger of two neutron stars in gravitational waves
and gamma rays was accompanied by a quickly reddening transient. Such a transient was …

The electromagnetic transients accompanying compact binary mergers (γ-ray bursts,
afterglows and 'macronovae') are crucial to pinpoint the sky location of gravitational wave …

We present a new, publicly available set of Los Alamos OPLIB opacity tables for the
elements hydrogen through zinc. Our tables are computed using the Los Alamos ATOMIC …

Spectral line-shape models are an important part of understanding high-energy-density
(HED) plasmas. Models are needed for calculating opacity of materials and can serve as …

Extreme ultraviolet (EUV) lithography is currently entering high-volume manufacturing to
enable the continued miniaturization of semiconductor devices. The required EUV light, at …

The electromagnetic observations of GW170817 were able to dramatically increase our
understanding of neutron star mergers beyond what we learned from gravitational waves …