@InProceedings{FerociBozzBragZwar:2016:StUp,
author = "Feroci, M. and Bozzo, E. and Braga, Jo{\~a}o and Zwart, F.",
affiliation = "{} and {} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "The LOFT mission concept: a status update",
booktitle = "Proceedings...",
year = "2016",
organization = "Space Telescopes and Instrumentation",
note = "Proceedings of SPIE, 9905",
abstract = "The Large Observatory For x-ray Timing (LOFT) is a mission concept
which was proposed to ESA as M3 and M4 candidate in the framework
of the Cosmic Vision 2015-2025 program. Thanks to the
unprecedented combination of effective area and spectral
resolution of its main instrument and the uniquely large field of
view of its wide field monitor, LOFT will be able to study the
behaviour of matter in extreme conditions such as the strong
gravitational field in the innermost regions close to black holes
and neutron stars and the supra-nuclear densities in the interiors
of neutron stars. The science payload is based on a Large Area
Detector (LAD, >8m2 effective area, 2-30 keV, 240 eV spectral
resolution, 1 degree collimated field of view) and a Wide Field
Monitor (WFM, 2-50 keV, 4 steradian field of view, 1 arcmin source
location accuracy, 300 eV spectral resolution). The WFM is
equipped with an on-board system for bright events (e.g., GRB)
localization. The trigger time and position of these events are
broadcast to the ground within 30 s from discovery. In this paper
we present the current technical and programmatic status of the
mission.",
conference-year = "25-27 July",
language = "en",
urlaccessdate = "12 maio 2024"
}