Optimizing astronomical observation strategies with Gnuastro 0.21's new pointing simulation tool and improving exposure mapping accuracy.

Optimizing astronomical observation strategies with Gnuastro 0.21's new pointing simulation tool and improving exposure mapping accuracy.

Optimizing astronomical observation strategies with Gnuastro 0.21's new pointing simulation tool and improving exposure mapping accuracy.

From the outside, Ukio may seem like a simple short-term rental business. But behind the scenes, there is a complex tool being built that…

Optimizing astronomical observation strategies with Gnuastro 0.21's new pointing simulation tool and improving exposure mapping accuracy.

Saving Tesla is no easy task.

Discover how Weekly Predictions revolutionizes crypto investing with Karim Chaib, founder of Dopamine, offering data-driven insights for informed decisions.

We probably won’t use these fancy data structures like linked lists, binary trees, AVL trees or whatever in our day-to-day work.

Exploring machine understanding of story dialogue via new tasks and dataset, improving coherence and speaker recognition in storytelling AI.

The heart loots what it wants

5/9/2024: Top 5 stories on the HackerNoon homepage!

An analysis of Meta’s master plan and OpenAI’s masterpiece

But accessibility options are nice to see

So, I’ve been navigating the realms of project management throughout my academic pursuit of an MBA, and let me tell you – it’s been quite the adventure! One approach that’s been making waves and…

The sustainable way out

Then-

Cyvers co-founder and CEO Deddy Lavid provides valuable insights into how AI algorithms can identify potential blockchain security threats.

Explore the power of CoinGecko's API with our guide on using real-time crypto data for trading, market analysis, and building applications.

Accretion flows in galactic nuclei involve magnetized plasma, and it has been long known that magnetic fields strongly perturb the energetics (Shvartsman 1971

Testing the accuracy of our method by numerically stimulating hydrodynamic spherical bondi accretion.

Our numerical scheme utilizes the GRMHD code KHARMA[1], a performance-portable C++ implementation based on iharm3D; iharm3D is itself an extension of HARM.