The LOFT Ground Segment
E. Bozzo (a), A. Antonelli (b), A. Argan (c), D. Barret (d, r), P., Binko (a), S. Brandt (e), E. Cavazzuti (b), T. Courvoisier (a), J.W. den, Herder (f), M. Feroci (g, q), C. Ferrigno (a), P. Giommi (b), D. G\"otz (h),, L. Guy (a), M. Hernanz (i), J.J.M. in't Zand (f)

TL;DR
The LOFT mission aimed to study X-ray timing using two instruments, with a detailed ground segment plan for data collection, processing, and distribution, despite not being selected for launch.
Contribution
This paper provides a comprehensive overview of the planned LOFT ground segment organization and data management strategies.
Findings
Detailed design of LOFT ground operations
Data flow and archiving plans established
Mission design remained robust despite non-selection
Abstract
LOFT, the Large Observatory For X-ray Timing, was one of the ESA M3 mission candidates that completed their assessment phase at the end of 2013. LOFT is equipped with two instruments, the Large Area Detector (LAD) and the Wide Field Monitor (WFM). The LAD performs pointed observations of several targets per orbit (~90 minutes), providing roughly ~80 GB of proprietary data per day (the proprietary period will be 12 months). The WFM continuously monitors about 1/3 of the sky at a time and provides data for about ~100 sources a day, resulting in a total of ~20 GB of additional telemetry. The LOFT Burst alert System additionally identifies on-board bright impulsive events (e.g., Gamma-ray Bursts, GRBs) and broadcasts the corresponding position and trigger time to the ground using a dedicated system of ~15 VHF receivers. All WFM data are planned to be made public immediately. In this…
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