Las Cumbres Observatory (LCOGT) operates a global network of robotic 0.4, 1.0, and 2.0-meter telescopes to facilitate scientific research and education in time-domain astronomy. LCOGT’s flagship educational program, Global Sky Partners (GSP), awards up to 1500 hours per year of telescope time to individuals and organizations that run their own, fully supported, educational programs. The GSP has a presence in 40 countries and 45% of the Partners target under-served, under-represented, and developing world audiences. The degradation and obsolescence of the original 0.4-meter telescope network prompted LCOGT to update the fleet of 10 telescopes to a new system consisting of predominantly off-the-shelf products. New PlaneWave DeltaRho 350 telescopes with Gemini Focuser/Rotators, LCOGT filter wheels, and QHY600 CMOS cameras, complement the original, custom-built mount. The deployment of all ten telescopes was completed in March 2024. We describe the design and performance of this new system and its components. We comment on modifications made to the QHY600 cameras, as well as on the treatment of random telegraph noise of its CMOS detectors within our data processing system BANZAI. The new telescope network supports the GSP program as well as multiple key science projects, including follow-up observations for the TESS satellite mission.
Las Cumbres Observatory global telescope (LCOGT) is a unique worldwide network of dynamically scheduled, fully robotic optical telescopes, purpose built for time domain astronomy. The LCOGT network enters its second decade of operations in 2024. A flood of transient alerts are expected from the Vera C. Rubin Legacy Survey of Space and Time (LSST) and multimessenger observatories. In 2023 LCOGT will complete the northern hemisphere 1-m telescope ring, currently four telescopes at McDonald and Teide Observatories, with the addition of two 1-m telescopes at Ali Observatory in Tibet. The southern ring is complete at the Siding Spring, Cerro Tololo and the South African Astronomical Observatories. LCOGT is an active partner in the Astrophysical Event Observatory Network (AEON) with NOIRLab facilities (Gemini Observatory, SOAR Observatory, and the Community Science and Data Center), to develop the infrastructure to efficiently carry out astronomical observations in the Vera C. Rubin Observatory LSST era. While the global pandemic has provided multiple operational challenges, hardware and software projects currently underway will make LCOGT an even more powerful transient follow-up facility in its second decade of operations.
Las Cumbres Observatory (LCOGT) operates a network of more than 25 telescopes that are globally distributed over seven sites. Despite the COVID-19 pandemic restricting travel to most of those sites since March 2020, LCOGT achieved several significant operational milestones: (i) We deployed a new multi-channel imager (MuSCAT3) at Haleakala Observatory. (ii) We installed two new 1-meter telescopes at Teide Observatory. (iii) We performed essential maintenance with local staff at the sites. The latter included opening two of the NRES spectrograph’s thermal and pressure enclosures - a task traditionally executed by trained LCOGT personnel only. We discuss the evolution of LCOGT’s paradigm for maintenance. Sustaining observatory operations increasingly relied on local observatory staff, of various skill levels and capabilities, to execute the highest priority work with remote support. We made this possible with extensive planning, being sensitive to local conditions, and bringing in expertise to support and guide in real-time via extended Zoom sessions.
The operation of robotic telescopes at remote locations without supervision by local staff is a specific challenge for Las Cumbres Observatory’s (LCOGT) global network, where more than 25 telescopes are operated at seven globally distributed sites. LCOGT personnel typically visits each site every 18 months for general maintenance and upgrade tasks, whereas minor failures are handled by local site support staff. LCOGT is making efforts to quantitatively inform decisions about scheduling preventative maintenance tasks and to provide tools to assist with failure diagnostic and response. For example, all night-time observations from all telescopes are analyzed to quantify the telescopes’ throughput; these data, updated daily and looking back more than four years, are used to inform the cadence of telescope mirror washing and recoating. Further examples of utilizing every day’s science data are presented, including monitoring the readnoise of more than 25 CCD cameras which has enabled the early detection of a failing CCD controller. Telemetry from all installations is collected in a no-SQL database (Opensearch) ∗ and presented to various stakeholders via the visualization tools Kibana and Grafana† . These utilities are used to diagnose problems in preprogrammed views, e.g., to detect acute issues or long-term degradation in the fleet of Cryotiger cooling systems. Telemetry data and performance metrics have always been collected at LCOGT. Making those data consistent, accessible, and easy to use for all stakeholders at LCOGT made the deluge of information usable in the daily observatory operation routine.
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.
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 Global Telescope Network (LCOGT) has built the Network of Robotic Echelle Spectrographs (NRES), consisting of four identical, high-resolution optical spectrographs, each fiber-fed simultaneously by up to two 1-meter telescopes and a calibration source. Two units have been installed and are currently executing scientific observations. A third unit has been installed and is presently in commissioning. A fourth unit has been shipped to site and will be installed in mid 2018. Operating on four separate continents in both the Northern and Southern hemispheres, these instruments comprise a globally-distributed, autonomous spectrograph facility for stellar classification and high-precision radial velocity of bright stars. Simulations suggest we will achieve long-term radial velocity precision of 3 m/s in less than an hour for stars with V < 12. Radial velocity precision of 75 m/s has already been demonstrated with our automatic data-processing pipeline across multiple sites. Work is ongoing to improve several NRES system components including telescope control (robotic source acquisition in particular) and the data-processing pipeline. In this document we briefly overview the NRES design, its purpose and goals, results achieved to date in the field, and the ongoing development effort to improve instrument performance.
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