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The Large Observatory for X-ray Timing (LOFT)

Journal article
Authors M. Feroci
L. Stella
M. van der Klis
T. J. L. Courvoisier
M. Hernanz
R. Hudec
A. Santangelo
D. Walton
A. Zdziarski
D. Barret
T. Belloni
J. Braga
S. Brandt
C. Budtz-Jorgensen
S. Campana
J. W. den Herder
J. Huovelin
G. L. Israel
M. Pohl
P. Ray
A. Vacchi
S. Zane
A. Argan
P. Attina
G. Bertuccio
E. Bozzo
R. Campana
D. Chakrabarty
E. Costa
A. De Rosa
E. Del Monte
S. Di Cosimo
I. Donnarumma
Y. Evangelista
D. Haas
P. Jonker
S. Korpela
C. Labanti
P. Malcovati
R. Mignani
F. Muleri
M. Rapisarda
A. Rashevsky
N. Rea
A. Rubini
C. Tenzer
C. Wilson-Hodge
B. Winter
K. Wood
G. Zampa
N. Zampa
Marek A Abramowicz
M. A. Alpar
D. Altamirano
J. M. Alvarez
L. Amati
C. Amoros
L. A. Antonelli
R. Artigue
P. Azzarello
M. Bachetti
G. Baldazzi
M. Barbera
C. Barbieri
S. Basa
A. Baykal
R. Belmont
L. Boirin
V. Bonvicini
L. Burderi
M. Bursa
C. Cabanac
E. Cackett
G. A. Caliandro
P. Casella
S. Chaty
J. Chenevez
M. J. Coe
A. Collura
A. Corongiu
S. Covino
G. Cusumano
F. D'Amico
S. Dall'Osso
D. De Martino
G. De Paris
G. Di Persio
T. Di Salvo
C. Done
M. Dovciak
A. Drago
U. Ertan
S. Fabiani
M. Falanga
R. Fender
P. Ferrando
D. D. Ferreira
G. Fraser
F. Frontera
F. Fuschino
J. L. Galvez
P. Gandhi
P. Giommi
O. Godet
E. Gogus
A. Goldwurm
D. Gotz
M. Grassi
P. Guttridge
P. Hakala
G. Henri
W. Hermsen
J. Horak
A. Hornstrup
J. J. M. in't Zand
J. Isern
E. Kalemci
G. Kanbach
V. Karas
D. Kataria
T. Kennedy
D. Klochkov
W. Kluzniak
K. Kokkotas
I. Kreykenbohm
J. Krolik
L. Kuiper
I. Kuvvetli
N. Kylafis
J. M. Lattimer
F. Lazzarotto
D. Leahy
F. Lebrun
D. Lin
N. Lund
T. Maccarone
J. Malzac
M. Marisaldi
A. Martindale
M. Mastropietro
J. McClintock
I. McHardy
M. Mendez
S. Mereghetti
M. C. Miller
T. Mineo
E. Morelli
S. Morsink
C. Motch
S. Motta
T. Munoz-Darias
G. Naletto
V. Neustroev
J. Nevalainen
J. F. Olive
M. Orio
M. Orlandini
P. Orleanski
F. Ozel
L. Pacciani
S. Paltani
I. Papadakis
A. Papitto
A. Patruno
A. Pellizzoni
V. Petracek
J. Petri
P. O. Petrucci
B. Phlips
L. Picolli
A. Possenti
D. Psaltis
D. Rambaud
P. Reig
R. Remillard
J. Rodriguez
P. Romano
M. Romanova
T. Schanz
C. Schmid
A. Segreto
A. Shearer
A. Smith
P. J. Smith
P. Soffitta
N. Stergioulas
M. Stolarski
Z. Stuchlik
A. Tiengo
D. Torres
G. Torok
R. Turolla
P. Uttley
S. Vaughan
S. Vercellone
R. Waters
A. Watts
R. Wawrzaszek
N. Webb
J. Wilms
L. Zampieri
A. Zezas
J. Ziolkowski
Published in Experimental Astronomy
Volume 34
Issue 2
Pages 415-444
ISSN 0922-6435
Publication year 2012
Published at Department of Physics (GU)
Pages 415-444
Language en
Keywords Missions, X-ray timing, compact objects, black holes, neutron stars, silicon drift detector, black-hole, proportional counter, oscillations, alice, constraints, superagile, discovery, binaries, equation
Subject categories Astronomy


High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultradense matter and to black hole masses and spins. A 10 m(2)-class instrument in combination with good spectral resolution is required to exploit the relevant diagnostics and answer two of the fundamental questions of the European Space Agency (ESA) Cosmic Vision Theme "Matter under extreme conditions", namely: does matter orbiting close to the event horizon follow the predictions of general relativity? What is the equation of state of matter in neutron stars? The Large Observatory For X-ray Timing (LOFT), selected by ESA as one of the four Cosmic Vision M3 candidate missions to undergo an assessment phase, will revolutionise the study of collapsed objects in our galaxy and of the brightest supermassive black holes in active galactic nuclei. Thanks to an innovative design and the development of large-area monolithic silicon drift detectors, the Large Area Detector (LAD) on board LOFT will achieve an effective area of similar to 12 m(2) (more than an order of magnitude larger than any spaceborne predecessor) in the 2-30 keV range (up to 50 keV in expanded mode), yet still fits a conventional platform and small/medium-class launcher. With this large area and a spectral resolution of < 260 eV, LOFT will yield unprecedented information on strongly curved spacetimes and matter under extreme conditions of pressure and magnetic field strength.

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