中文
相关论文

相关论文: AGAMA: Action-based galaxy modelling architecture

200 篇论文

The Simulation Environment for Atomistic and Molecular Modeling (SEAMM) is an open-source software package written in Python that provides a graphical interface for setting up, executing, and analyzing molecular and materials simulations.…

ATHENA is an open source Python package for reduction in parameter space. It implements several advanced numerical analysis techniques such as Active Subspaces (AS), Kernel-based Active Subspaces (KAS), and Nonlinear Level-set Learning…

数值分析 · 数学 2022-04-19 Francesco Romor , Marco Tezzele , Gianluigi Rozza

Angle-action coordinates are used to study the relic of an N-body simulation of a self-gravitating satellite galaxy that was released on a short-period orbit within the disc of the Galaxy. Satellite stars that lie within 1.5 kpc of the Sun…

天体物理学 · 物理学 2009-11-13 Paul J. McMillan , James J. Binney

AI coding assistants like GitHub Copilot are rapidly transforming software development, but their safety remains deeply uncertain-especially in high-stakes domains like cybersecurity. Current red-teaming tools often rely on fixed benchmarks…

To advance our understanding of the evolution of the interstellar medium (ISM) of our Galaxy, numerical models of Milky Way (MW) type galaxies are widely used. However, most models only vaguely resemble the MW (e.g. in total mass), and…

In external galaxies, some galaxies have higher activities of star formation and central supermassive black holes. The interstellar medium in those galaxies can be heated by different mechanisms such as UV-heating, X-ray heating, cosmic-ray…

星系天体物理 · 物理学 2018-09-12 Nanase Harada

We present Magma, a foundation model that serves multimodal AI agentic tasks in both the digital and physical worlds. Magma is a significant extension of vision-language (VL) models in that it not only retains the VL understanding ability…

计算机视觉与模式识别 · 计算机科学 2025-02-19 Jianwei Yang , Reuben Tan , Qianhui Wu , Ruijie Zheng , Baolin Peng , Yongyuan Liang , Yu Gu , Mu Cai , Seonghyeon Ye , Joel Jang , Yuquan Deng , Lars Liden , Jianfeng Gao

Magnetic activity in the atmospheres of stars produces a number of spectroscopic signatures that are visible in the shape and strength of spectral lines. These signatures can be used to access, among other things, the variability of the…

天体物理仪器与方法 · 物理学 2018-11-29 J. Gomes da Silva , P. Figueira , N. C. Santos , J. P. Faria

Spatially-resolved studies of the kinematics of galaxies provide crucial insights into their assembly and evolution, enabling to infer the properties of the dark matter halos, derive the impact of feedback on the ISM, characterize the…

Aims. Galaxy mass models based on simple and analytical functions for the density and potential pairs have been widely proposed in the literature. Disk models constrained by kinematic data alone give information on the global disk structure…

星系天体物理 · 物理学 2016-10-05 D. A. Barros , J. R. D. Lépine , W. S. Dias

We describe a numerical implementation of star formation in disk galaxies, in which the conversion of cooling gas to stars in the multiphase interstellar medium is governed by the rate at which molecular clouds are formed and destroyed. In…

天体物理学 · 物理学 2008-11-26 C. M. Booth , T. Theuns , T. Okamoto

The Ca II H & K lines are strong chromospheric diagnostics that can be used to determine the temperature stratification and magnetic structure of the solar atmosphere. The Atacama Large Millimetre/Submillimetre Array (ALMA) offers…

太阳与恒星天体物理 · 物理学 2024-05-09 Sneha Pandit , Sven Wedemeyer , Mats Carlsson

Astronomical software is now a fact of daily life for all hands-on members of our community. Purpose-built software for data reduction and modeling tasks becomes ever more critical as we handle larger amounts of data and simulations.…

The Dark Sky Simulations are an ongoing series of cosmological N-body simulations designed to provide a quantitative and accessible model of the evolution of the large-scale Universe. Such models are essential for many aspects of the study…

宇宙学与河外天体物理 · 物理学 2014-07-10 Samuel W. Skillman , Michael S. Warren , Matthew J. Turk , Risa H. Wechsler , Daniel E. Holz , P. M. Sutter

The effect of angular momentum on galaxy formation and evolution has been studied for several decades. Our recent two papers using IllustrisTNG-100 simulation have revealed the acquisition path of the angular momentum from large-scale…

星系天体物理 · 物理学 2023-12-01 Sen Wang , Dandan Xu , Shengdong Lu , Cheng Li

From a carefully selected sample of $52\,089$ galaxies and $10\,429$ groups, we investigate the variation of the low-redshift galaxy stellar mass function (GSMF) in the equatorial Galaxy And Mass Assembly (GAMA) dataset as a function of…

星系天体物理 · 物理学 2025-03-28 A. Sbaffoni , J. Liske , S. P. Driver , A. S. G. Robotham , E. N. Taylor

Agent-based modeling is a computational dynamic modeling technique that may be less familiar to some readers. Agent-based modeling seeks to understand the behaviour of complex systems by situating agents in an environment and studying the…

多智能体系统 · 计算机科学 2023-04-19 G. Wade McDonald , Nathaniel D. Osgood

ABACUS (Atomic-orbital Based Ab-initio Computation at USTC) is an open-source software for first-principles electronic structure calculations and molecular dynamics simulations. It mainly features density functional theory (DFT) and…

A tutorial of the Mathematica package CGAlgebra, for conformal geometric algebra calculations is presented. Using rule-based programming, the 5-dimensional conformal geometric algebra is implemented and defined functions simplify the…

数学软件 · 计算机科学 2022-07-01 E. Alejandra Ortiz-Duran , Jose L. Aragon

Agent based modelling is a simulation method in which autonomous agents interact with their environment and one another, given a predefined set of rules. It is an integral method for modelling and simulating complex systems, such as…

多智能体系统 · 计算机科学 2022-01-10 George Datseris , Ali R. Vahdati , Timothy C. DuBois
‹ 上一页 1 8 9 10 下一页 ›