Distribution is a ubiquitous data type in high energy physics
(HEP), many other sciences, and our daily life. When the space of
distributions is equipped with a suitable metric, previously ad-hoc
notions of similarity can now be formulated in a...
Conservative finite difference methods have proven extremely
robust and reliable for magnetohydrodynamics simulations of binary
neutron star mergers. However, finite difference methods are
generally less accurate and efficient than spectral methods...
A key challenge for the next decade of survey cosmology is
ensuring that the models for summary statistics they measure, such
as galaxy clustering and lensing, are sufficiently accurate in
light of the high degree of precision of these measurements...
The Evryscopes are a North-South pair of ultra-wide-field
telescopes with an instantaneous field of view covering 16,512
square degrees at 13.2"/pixel resolution. The Evryscopes observe
continuously at two-minute cadence to a depth of 15.5 in
g-band...
ALMA has spatially resolved dozens of protoplanetary discs,
discovering widespread signatures of young massive planets. To
translate these observations into quantitative measures of the
system, such as disc and planet masses, one must perform...
Galaxy clusters are the most massive gravitationally self-bound
objects in the Universe. These clusters form at the rare high peaks
of the primordial density fluctuations, and they subsequently trace
the growth of structure in the Universe as they...
