Bibcode
Feroci, M.; den Herder, J. W.; Bozzo, E.; Barret, D.; Brandt, S.; Hernanz, M.; van der Klis, M.; Pohl, M.; Santangelo, A.; Stella, L.; Watts, A.; Wilms, J.; Zane, S.; Ahangarianabhari, M.; Albertus, C.; Alford, M.; Alpar, A.; Altamirano, D.; Alvarez, L.; Amati, L.; Amoros, C.; Andersson, N.; Antonelli, A.; Argan, A.; Artigue, R.; Artigues, B.; Atteia, J.-L.; Azzarello, P.; Bakala, P.; Baldazzi, G.; Balman, S.; Barbera, M.; van Baren, C.; Bhattacharyya, S.; Baykal, A.; Belloni, T.; Bernardini, F.; Bertuccio, G.; Bianchi, S.; Bianchini, A.; Binko, P.; Blay, P.; Bocchino, F.; Bodin, P.; Bombaci, I.; Bonnet Bidaud, J.-M.; Boutloukos, S.; Bradley, L.; Braga, J.; Brown, E.; Bucciantini, N.; Burderi, L.; Burgay, M.; Bursa, M.; Budtz-Jørgensen, C.; Cackett, E.; Cadoux, F. R.; Caïs, P.; Caliandro, G. A.; Campana, R.; Campana, S.; Capitanio, F.; Casares, J.; Casella, P.; Castro-Tirado, A. J.; Cavazzuti, E.; Cerda-Duran, P.; Chakrabarty, D.; Château, F.; Chenevez, J.; Coker, J.; Cole, R.; Collura, A.; Cornelisse, R.; Courvoisier, T.; Cros, A.; Cumming, A.; Cusumano, G.; D'Ai, A.; D'Elia, V.; Del Monte, E.; de Luca, A.; de Martino, D.; Dercksen, J. P. C.; de Pasquale, M.; De Rosa, A.; Del Santo, M.; Di Cosimo, S.; Diebold, S.; Di Salvo, T.; Donnarumma, I.; Drago, A.; Durant, M.; Emmanoulopoulos, D.; Erkut, M. H.; Esposito, P.; Evangelista, Y.; Fabian, A.; Falanga, M.; Favre, Y. et al.
Bibliographical reference
Proceedings of the SPIE, Volume 9144, id. 91442T 20 pp. (2014).
Advertised on:
7
2014
Citations
25
Refereed citations
16
Description
The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3
Cosmic Vision framework and participated in the final downselection for
a launch slot in 2022-2024. Thanks to the unprecedented combination of
effective area and spectral resolution of its main instrument, LOFT will
study the behaviour of matter under extreme conditions, such as the
strong gravitational field in the innermost regions of accretion flows
close to black holes and neutron stars, and the supranuclear densities
in the interior of neutron stars. The science payload is based on a
Large Area Detector (LAD, 10 m2 effective area, 2-30 keV,
240 eV spectral resolution, 1° 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 status of the
mission at the end of its Phase A study.
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