FLITECAM has two observing configurations: solo configuration and “FLIPO” configuration, which is the co-mounting of FLITECAM with the optical instrument HIPO (PI E. We present a performance report for FLITECAM, a 1-5 μm imager and spectrograph, upon its acceptance and delivery to SOFIA (Stratospheric Observatory for Infrared Astronomy). Projects in development include an upgrade to the telescope control system on the Keck I telescope, the blue channel of the Keck Cosmic Web Imager, the red channel of the Keck Cosmic Web Imager, the Keck Planet Finder, a deployable tertiary mirror for the Keck I telescope, an upgrade to the imager of OSIRIS, a major upgrade to the NIRSPEC instrument, and a fiber feed from the Keck II AO system to NIRSPEC. Projects recently completed include a new laser for the Keck II AO system, the upgrade of the spectrograph detector in the OSIRIS instrument, and the upgrade to the telescope control system on the Keck II telescope. We also describe the expected performance of projects currently in the development or construction phases. In this paper we describe the performance of recently completed new instruments, instrument upgrades, and infrastructure upgrade projects.

Our science driven strategic plan guides these developments and informs our plans for the future. Keck Observatory is committed to maintaining the scientific leadership of our observing community by matching our observers' skills and passions in their fields of astronomical science with a continuing dedication by the Observatory and its collaborators to the development of state of the art instrumentation and systems. Active management, cost to completion and risk policy are in place.

The Programme follows a roadmap that foresees one new instrument/project or one upgrade starting every year. Finally, two new Multi Object Spectrographs projects have started, one for the VLT (MOONS), one for the 4M VISTA telescope (4MOST), and two new instruments for La Silla, (SOXS and NIRPS) fully funded by the community, are being agreed. The mid-IR imager and spectrograph VISIR has been upgraded, and a major upgrade of the CRIRES spectrograph is under way. The Adapative Optics Facility is moving towards completion, as well as the high resolution spectrograph ESPRESSO and the VLTI second generation instrument MATISSE. The VLT second generation instruments KMOS, MUSE and SPHERE have been delivered and are in operations, GRAVITY is under commissioning at the renewed VLTI facility. The Paranal Instrumentation Programme is responsible for planning and delivering the instruments and the associated infrastructure needed to keep the VLT and La Silla Observatories at the forefront of ground-based astronomy.

Airborne by Constance Sharper