MATA — An AO system, fully developed in-house

What is MATA (Module for Adaptive Telescope Astronomy at Lulin)

A non-invasive, cost-effective natural guide star AO prototype for the Lulin One-meter Telescope — turning the LOT from a light bucket into a sharp eye, and laying the groundwork for AO on Taiwan's larger telescopes. AO corrects the blurring of starlight by atmospheric turbulence in real time, letting a ground-based telescope approach the sharpness of a space-based one. MATA brings this capability to the LOT as a compact natural guide star (NGS) system whose optics, hardware integration, and control software are all developed within the TARA / ASIAA OIR team. It is designed to be non-invasive to the host telescope and cost-effective enough to serve as a working testbed. This is the first step toward a domestic AO capability that can feed into TP2m, Subaru, and GMT.

Wavefront Sensor
Detector
Low readout noise
Frame rate
> 1 kHz readout
Deformable Mirror
Actuators
12 × 12
Response
Short settling
Real-time Control
Software
In-house RTC
Latency Goal
Total < 2 ms
Performance
Bands
Red-optimized i & z
Resolution
0.2″ – 0.3″

System breakdown

Six development tracks

MATA is built across six tightly coupled subsystems, each developed and tested within the team.

Wavefront Reconstruction

Shack–Hartmann reconstruction algorithm, validated against real Subaru AO data.

AO Real-time Control Interface

Live control GUI (V2.0) with WFS spots, slopes, phase reconstruction, and DM response.

DM Controller

Control software complete; in-house low-latency driver being implemented with the new DM.

Optical & Mechanical Design

Compact 50 × 50 cm bench layout; optomechanics with the IAA OIR and NCU Lulin team.

Simulations

End-to-end turbulence and closed-loop modelling (HCIPy) across guide-star brightness.

Subsystem Testing & Integration

Bench integration and closed-loop stability verification ahead of on-sky runs.

Schedule

2026 roadmap

From bench design to first light on the Lulin sky.

2026 Q1
  • Optical & mechanical design
  • New DM & WFS camera ready
  • Simulations
2026 Q2–Q3
  • Subsystem verification
  • Closed-loop stability testing
  • End-to-end latency < 2 ms
2026 Q4
  • Lulin on-sky engineering runs

MATA is not just an instrument — it is a proof of concept for the TARA operational model.

  • Integrates domestic resources and optimizes existing facilities for global competitiveness.
  • Transforms the LOT from a light bucket into a sharp eye, securing a unique niche for a 1-m telescope in the global network.
  • Serves as a pathfinder for AO on TP2m, Robo-AO-like systems, and 3–4 m class telescopes.
  • Builds the people, methods, and partnerships behind Taiwan's entry into the GMT era.

People

Contact & collaborators

Contact Person

Dr. Po-Chieh Yu

TARA Scientist · TARA / ASIAA

pcyu@asiaa.sinica.edu.tw

Collaborators

S.-Y. Wang C. Baranec M. Kimura Y.-C. Chang C.-Y. Chou B.-J. Wang P.-J. Huang H.-Y. Chen S.-F. Hsu H.-C. Lin W.-P. Chen

Partner Institutions / Group

ASIAA OIR IANCU IfA — Robo-AO-2