Results 31 to 40 of about 12,482 (163)
The rise and fall of little red dots could be driven by the environment
The little red dot (LRD) paradigm comprises three main unknowns that are intrinsically connected: (1) What is the nature of these sources? (2) How do they form? (3) How do they evolve?
Mérida Rosa M. +11 more
doaj +1 more source
A Raster-oriented Method for Creating Eclipse Maps
Traditional total solar eclipse maps based on 19th-century calculation methods do not take full advantage of important refinements recently made possible by fast computers and high-resolution digital elevation models of both the Earth and the Moon ...
Ernie Wright, C. Alex Young
doaj +1 more source
Thermal Radiation Transport with Tensor Trains
We present a novel tensor network algorithm to solve the time-dependent, gray thermal radiation transport equation. The method invokes a tensor train (TT) decomposition for the specific intensity.
Alex A. Gorodetsky +6 more
doaj +1 more source
Searches for continuous-wave gravitational radiation in data collected by modern long-baseline interferometers, such as the Laser Interferometer Gravitational-wave Observatory (LIGO), the Virgo interferometer, and the Kamioka Gravitational Wave Detector,
P. Clearwater +3 more
doaj +1 more source
Solar magnetic tornadoes are dynamic, spiral-shaped plasma structures characterized by helical magnetic fields and rotating plasma flows in the solar atmosphere.
Mark I. Blumenau +3 more
doaj +1 more source
Proton–proton fusion in lattice effective field theory
The proton–proton fusion rate is calculated at low energy in a lattice effective field theory (EFT) formulation. The strong and the Coulomb interactions are treated non-perturbatively at leading order in the EFT.
Gautam Rupak, Pranaam Ravi
doaj +1 more source
Astronomy Data And Computing Services - Upskilling the Australian astronomy community
The Astronomy Data And Computing Services (ADACS) initiative has been working with the Australian astronomy community for just over 3 years now. Our vision is to deliver astronomy-focused training, support and expertise to maximise the scientific return on investments in astronomical data & computing infrastructure.
openaire +1 more source
MLody—Deep Learning–generated Polarized Synchrotron Coefficients
Polarized synchrotron emission is a fundamental process in high-energy astrophysics, particularly in the environments around black holes and pulsars. Accurate modeling of this emission requires precise computation of the emission, absorption, rotation ...
J. Davelaar
doaj +1 more source
Probing the star formation main sequence down to 107 M⊙ at 1 < z < 9
The main sequence of star-forming galaxies (SFGMS or MS) is a fundamental scaling relation that provides a global framework for studying galaxy formation and evolution, as well as an insight into the complex star formation histories (SFHs) of individual ...
Mérida Rosa M. +14 more
doaj +1 more source
The “Chimera”: An Off-The-Shelf CPU/GPGPU/FPGA Hybrid Computing Platform
The nature of modern astronomy means that a number of interesting problems exhibit a substantial computational bound and this situation is gradually worsening.
Ra Inta, David J. Bowman, Susan M. Scott
doaj +1 more source

