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We're back with our latest edition of "Proof of AI Journals," by Proof of AI Lab.
In this Journal, our researcher Kevin Ros dives into how 2025 is the year of agentic AI, and Model Context Protocol (MCP) is quickly becoming the standard for connecting agents to tools like Slack, Uber, and Notion.
But there's a huge problem: authentication.
Each agent needs to authenticate with each tool individually.
If you're running 10 agents across 20 tools, that's 200 separate OAuth flows.
This leads to the M × N auth problem:
🔁 Redundant flows
🔓 Massive attack surface
🧱 No granular control over time, task, or scope
At Kite AI, we’re building a cryptographically secure transaction layer that solves this.
Agentic systems won’t scale until auth is reimagined, and we’re building that future. 🪁
It’s been exactly 2 weeks since we upgraded our Testnet to Testnet Ozone, and here are our metrics so far.
Huge thank you to all the Gkiters who’ve jumped in, tested, and shared feedback.
Your input is shaping what comes next - keep it coming! 🫡
How does a satellite antenna work for radar astronomy? 📡
Missed our latest article? Here's a quick recap:
Electromagnetic Principles and System Architecture
At its core, radar astronomy relies on the fundamental properties of electromagnetic waves. The process involves transmitting a beam toward a target and then analyzing the extremely weak echoes that return. The key components of a radar astronomy system include:
Transmitter:
High-powered transmitters (often up to 1 megawatt or more) generate either pulsed or continuous-wave signals. Pulsed systems provide excellent range resolution, while continuous-wave systems enable precise Doppler measurements. The transmitted power compensates for the rapid signal loss, which follows an inverse fourth-power law with distance.
Antenna (Radar Telescope):
Serving both as transmitter and receiver, large, high-gain antennas focus the radio beam and collect the faint echoes. Facilities such as the historic Arecibo Observatory, the Goldstone Solar System Radar, and Evpatoria Planetary Radar have utilized these techniques to achieve high-precision astrometric measurements and detailed imagery.
Propagation Channel:
As the radio waves traverse interplanetary space, their strength diminishes dramatically. This necessitates extremely sensitive receivers and sophisticated signal processing to extract meaningful data from echoes that may be millions of times weaker than the transmitted signal.
Receiver and Signal Processor:
State-of-the-art receivers, incorporating ultra-low-noise amplifiers and advanced digital signal processing (DSP) techniques (like coherent integration and matched filtering), capture and refine the weak return signals. These processes yield accurate measurements of distance, velocity, surface properties, and even subsurface structures.
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Introducing a brand new MilkyWay 🐄
The first moo-dular restaking portal for any chain.
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Breaking Down our Latest article written by @jefhsia
Pt 1 - Early Signals 📶
The Birth of Cosmic Communication The Advent of Radio Waves The story of interstellar communication begins with the discovery of radio waves, a form of electromagnetic radiation with wavelengths ranging from 1 millimeter to 100 kilometers. Traveling at the speed of light, radio waves became a cornerstone of human communication due to their ability to carry information through modulation techniques like AM (Amplitude Modulation) and FM (Frequency Modulation).