Astra: an open-source fully autonomous robotic observatory control software

arXiv:2607.12898 · astro-ph.IM, astro-ph.EP · Submitted 2026-07-14 · Read on arXiv

Peter P. Pedersen, David Degen, Lionel Garcia, Urs Schroffenegger, Daniel Sebastian, Sebastián Zúñiga-Fernández, Brice-Olivier Demory, Elsa Ducrot, Michaël Gillon, Matthew J. Hooton, Clàudia Janó-Muñoz, James McCormac, Mathilde Timmermans, Amaury H. M. J. Triaud, Didier Queloz

astro-ph.IM, astro-ph.EP

Submitted: 2026-07-14

Comments: 16 pages, 3 figures, proceedings of SPIE Astronomical Telescopes + Instrumentation 2026, 14155-116

Code: https://github.com/ppp-one/astra

License: http://creativecommons.org/licenses/by/4.0/

The gist: Robotic and autonomous observatories are critical for modern time-domain and high-cadence astronomical surveys.

Terminology

Abstract

Robotic and autonomous observatories are critical for modern time-domain and high-cadence astronomical surveys. The operation of these facilities requires complex software coordination to manage hardware, schedule observations, and ensure safety. However, existing observatory control software are often proprietary and platform-locked or require complex message-brokering infrastructure. Here we present Astra (Automated Survey observaTory Robotised with Alpaca): an open-source, cross-platform Python system for the sustained, fully autonomous operation of astronomical observatories, requiring no external message-broker infrastructure. Astra controls observatory hardware via the ASCOM Alpaca protocol, and executes prescheduled observatory actions under continuous safety supervision. Its multi-device actions include plate-solve-based pointing correction with a local Gaia--2MASS catalogue fallback, PID-controlled autoguiding, and autofocus. A FastAPI web service provides a browser UI, REST and WebSocket APIs for real-time status, image previews, and SQLite-backed telemetry and logs. Astra has run in fully unattended production since January 2024, scaling to six telescopes across three facilities: the SPECULOOS-South network (4 times 1,m class, Chile), SAINT-EX (1,m class, Mexico), and the ETH Observatory (0.5,m class, Switzerland), with no schedule aborts attributable to Astra software. Across the SPECULOOS-South network, it achieves sub-arcsecond autoguiding (0.11 median pointing scatter) and plate-solve failure rates below 1% on three of the four telescopes (3% on the narrowest-field unit), demonstrating that an open, standards-based software stack can meet the reliability demands of production survey astronomy.

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