Automated scheduler for the SOXS instrument: design and performance
Laura Asquini, Marco Landoni, Dave Young, Laurent Marty, Stephen J., Smartt, Sergio Campana, Riccardo Claudi, Pietro Schipani, Jani Achren, Matteo, Aliverti, Jose A. Araiza Duran, Iair Arcavi, Federico Battaini, Andrea, Baruffolo, Sagi Ben Ami, Andrea Bianco, Alex Bichkovsky

TL;DR
This paper describes the development and initial testing of an automated, scalable scheduler for the SOXS instrument at ESO-NTT, designed to optimize transient observations without on-site astronomer presence.
Contribution
The paper introduces a new fully automated, scalable scheduler architecture for the SOXS instrument, capable of rapid response and weather adaptation, tailored for remote operation at ESO-NTT.
Findings
Scheduler is ready for on-site testing during commissioning.
Web interface and preliminary performance tests are described.
Architecture uses Docker, API Gateway, and Flask for scalability.
Abstract
We present the advancements in the development of the scheduler for the Son Of X-shooter instrument at the ESO-NTT 3.58-m telescope in La Silla, Chile. SOXS is designed as a single-object spectroscopic facility and features a high-efficiency spectrograph with two arms covering the spectral range of 350-2000 nm and a mean resolving power of approximately R=4500. It will conduct UV-visible and near-infrared follow-up observations of astrophysical transients, drawing from a broad pool of targets accessible through the streaming services of wide-field telescopes, both current and future, as well as high-energy satellites. The instrument will cater to various scientific objectives within the astrophysical community, each entailing specific requirements for observation planning. SOXS will operate at the European Southern Observatory (ESO) in La Silla, without the presence of astronomers on…
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