Las Cumbres Observatory is the only globally-distributed network of robotically-controlled telescopes. In 2018, we launched a program to overhaul the procedures by which network problems are detected, diagnosed and resolved. The program fostered numerous improvements, including new software tools to monitor active telescopes, documentation of recovery procedures, and daily reviews of operations problems. The benefit to users has been an increase in on-sky hours. We discuss the improvements we have made over the past two years. We emphasize the implementation of procedures ensuring problems are promptly addressed and completely resolved. We present our workflow as a model for how to manage a system of interconnected telescopes.
Astrophysical phenomena occur on a range of timescales, and to properly characterize them, observations must be made at appropriate intervals on instrumentation determined by the scientific goals of the study. The traditional model of scheduling telescope time in blocks of consecutive nights and requiring the investigators to operate the instrument (either in person or remotely) is not optimal for this science. A queue-scheduled approach to time allocation can relieve the personal and financial burden of interactive observing runs. This is particularly powerful when requests for observations can be made through a programmatic interface, which provides not just a convenient tool for all astronomy programs, but also the opportunity to build fully automated observing programs. This will be an essential component of projects making follow-up observations for modern surveys that produce millions of alerts per night, as much of the science return will depend upon obtaining classification and characterization data rapidly and efficiently, as well as for coordination of observations across multiple facilities. The AEON Network is an initiative to build a programmatically accessible, queue-scheduled and user driven network of telescopes ideal for modern astronomical observing programs.
We report the development of MuSCAT3, a four channel simultaneous imager installed on the 2m Faulkes Telescope North at Haleakala Observatory on Maui, Hawai’i. MuSCAT3 has a capability of 4-color simultaneous imaging in g (400–550 nm), r (550–700 nm), i (700–820 nm), and zs (820–920 nm) bands with four independent 2048×2048 pixel CCDs, each having a field of view of 9.1×9.1 arcmin2 with a pixel scale of 0.27 arcsec per pixel. The development of MuSCAT3 started from September 2019, and MuSCAT3 achieved its first light on September 28th, 2020. The Las Cumbres Observatory started science operations of MuSCAT3 since November 4th, 2020, although a part of its capabilities are still limited.
Las Cumbres Observatory (LCOGT) has recently finished integrating the SOAR 4.1-meter telescope into its robotic telescope network. To achieve this, an observation request language was developed suitable for describing observations across a wide range of current and future telescope facilities and observing resources. A complete set of Application Programming Interfaces (APIs) were developed to allow any arbitrary observatory to utilize LCOGT’s observation management software, including interfaces to i) manage proposals, ii) retrieve and update a schedule of observations, iii) report the progress of ongoing observations, iv) propagate operational telemetry and v) receive science products. We describe our efforts, the experience gained, and the implications of this work on the Astronomical Event Observatory Network (AEON) initiative. We also introduce an alternate option for observation management in the open source Observatory Control System (OCS).
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