Impact of different temperature profiles and disc-to-star mass ratios on the disk's surface density profile when it reaches equilibrium
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Updated
Feb 5, 2023 - TeX
Impact of different temperature profiles and disc-to-star mass ratios on the disk's surface density profile when it reaches equilibrium
This easy-to-use program brings a new amazing Astronomy Picture of the Day (APOD) directly to your desktop every day!
Code of my Master's Thesis for Lund University with the title "Efficient discovery of binary stars".
Solutions to some problems in ``Bayesian Methods in Cosmology'' article
Ovaj sudar je bio posmatran u vremenskom periodu od milijardu godina (10^9 ) koliko obično traju sudari dve galaksije. Ispitan je slučaj sudara dve identične, spiralne galaksije, koje su, dok su bile izolovane, bile stabilne. Galaksije su predstavljene N-body sistemom. Algoritam koji je koriscen ima vremensku slozenost θ(n^2)
a galaxy cluster catalogue obtained in directions of SZcat by applying deep learning method to ACT+Planck maps
My personal academic website.
Tools for 21cm Fisher forecasts with 21cmFAST
A framework for building deep learning models and pipelines for astrophysics applications.
GTRPy is a GUI based application that allows users to perform Tensor and 6 different type of field operations in both 3D and 4D
C++17 N-body Barnes-Hut on heterogeneous hardware architectures
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