Results 241 to 250 of about 120,169 (292)

Achieving GPT-4o level performance in astronomy with a specialized 8B-parameter large language model. [PDF]

open access: yesSci Rep
de Haan T   +8 more
europepmc   +1 more source

Atom Addition Formation of Thionylimide (HNSO) on Interstellar Dust Grains: Chemical Routes Requiring Oxygen and Nitrogen Atom Surface Diffusion. [PDF]

open access: yesACS Earth Space Chem
Del Valle JC   +6 more
europepmc   +1 more source

Discs no more: the morphology of low-mass simulated galaxies in FIREbox. [PDF]

open access: yesMon Not R Astron Soc
Benavides JA   +11 more
europepmc   +1 more source

X-ray absorption spectroscopy of FeH+ to aid its identification in astrochemical environments.

open access: yesChem Commun (Camb)
Jin S   +10 more
europepmc   +1 more source

Visualizing many-particle astronomical simulations

ACM SIGGRAPH 2007 posters, 2007
Astronomers often work on many-particle systems. For example, the Earth had been formed from millions of planetesimals, and a galaxy contains hundreds of billions of stars. We have developed a GUI visualization tool specialized for astronomical many-particle simulations.
Takaaki Takeda, Toshiyuki Takahei
openaire   +1 more source

MAISIE: a multipurpose astronomical instrument simulator environment

SPIE Proceedings, 2016
Astronomical instruments often need simulators to preview their data products and test their data reduction pipelines. Instrument simulators have tended to be purpose-built with a single instrument in mind, and at- tempting to reuse one of these simulators for a different purpose is often a slow and difficult task.
Alan O'Brien   +3 more
openaire   +1 more source

Conceptualizing astronomical scale: Virtual simulations on handheld tablet computers reverse misconceptions

Computers & Education, 2014
Matthew H. Schneps   +5 more
openaire   +3 more sources

Optimizing Numerical Simulations of Colliding Galaxies. II. Comparing Simulations to Astronomical Observations

Research Notes of the AAS, 2020
Abstract Our research focuses on determining the dynamical orbital parameters associated with galaxy collisions. We are accomplishing this by optimizing numerical models of galactic interactions with astronomical observations of colliding galaxies and measuring the uncertainty in the parameter space of these models. This paper will focus
Matthew Ogden   +4 more
openaire   +1 more source

Numerical simulation of astronomical observations with ISO-LWS

Il Nuovo Cimento C, 1993
The purpose of this work is the numerical simulation of the ISO-LWS spectrometer output with a computer code aiming at obtaining data similar as far as possible to those to be gained during the mission. With such data the processing and analysis programmes will be tested in order to assess the instrument capabilities and limits.
E. Tommasi, P. Saraceno, R. Orfei
openaire   +1 more source

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