
Therefore, before formal observations begin, research teams must first construct a "simulated telescope" to fully simulate the entire observation process. Only after verifying the feasibility of the plan can they proceed to use real equipment to gaze into deep space.
Qwen Office has the privilege of serving as the underlying support platform for this simulation system.
02
How does the simulation system work?
Qwen Office assists relevant research teams at the National Astronomical Observatories in building a digital simulation system for large-aperture scientific-grade telescopes. It integrates information about various telescope components, sensor statuses, and observational environmental conditions into standardized MCP interfaces, enabling intelligent agents (Agents) to monitor and access them in real time.
This is akin to converting each part of the telescope into a row of "universal sockets," allowing Agents to plug in and use instantly—enabling not only real-time status checks but also remote control of equipment.
Two specialized models operate collaboratively under its coordination:
Cross-survey transient alignment timing model: Identifies candidate targets of extremely early supernovae from multiple public sky survey datasets, answering the question of "what to observe";
Short-term local weather forecasting model: Assesses real-time observing conditions, providing guidance on "how to observe."
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