The Large Area Detector of LOFT: the Large Observatory for X-ray Timing
S. Zane (1), D. Walton (1), T. Kennedy (1), M. Feroci (2), J.-W. Den, Herder (3), M. Ahangarianabhari (4), A. Argan (5), P. Azzarello (6), G., Baldazzi (7), M. Barbera (23,24), D. Barret (8), G. Bertuccio (4), P. Bodin, (9), E. Bozzo (6), L. Bradley (1), F. Cadoux (10)

TL;DR
LOFT's Large Area Detector was designed for fast X-ray timing near black holes and neutron stars, offering unprecedented variability studies, but was not selected for launch despite a robust design.
Contribution
The paper presents the detailed design and capabilities of the LAD instrument, highlighting its potential for revolutionizing X-ray variability studies.
Findings
LAD has a 10 m² effective area operating in 2-30 keV range.
The instrument can perform millisecond X-ray timing.
The design is robust and ready for future ESA proposals.
Abstract
LOFT (Large Observatory for X-ray Timing) is one of the five candidates that were considered by ESA as an M3 mission (with launch in 2022-2024) and has been studied during an extensive assessment phase. It is specifically designed to perform fast X-ray timing and probe the status of the matter near black holes and neutron stars. Its pointed instrument is the Large Area Detector (LAD), a 10 m 2 -class instrument operating in the 2-30keV range, which holds the capability to revolutionise studies of variability from X-ray sources on the millisecond time scales. The LAD instrument has now completed the assessment phase but was not down-selected for launch. However, during the assessment, most of the trade-offs have been closed leading to a robust and well documented design that will be re- proposed in future ESA calls. In this talk, we will summarize the characteristics of the LAD design…
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