LOFT: A large observatory for x-ray timing

Fabio Muleri; M. Feroci; T. Belloni; J. Braga; S. Campana; T. Courvousier; M. Hernanz; R. Hudec; G. L. Israel; P. S. Ray; A. Santangelo; L. Stella; A. Vacchi; M. Van Der Klis; D. Walton; A. Zdziarski; J. M. Alvarez; A. Argan; G. Baldazzi; M. Barbera; G. Bertuccio; V. Bonvicini; E. Bozzo; R. Campana; A. Collura; G. Cusumano; E. Del Monte; J. W. Den Herder; S. Di Cosimo; G. Di Persio; Y. Evangelista; F. Fuschino; J. L. Galvez; P. Giommi; M. Grassi; P. Guttridge; J. J.M. In'T Zand; D. Kataria; D. Klochkov; C. Labanti; F. Lazzarotto; P. Malcovati; M. Marisaldi; M. Mastropietro; T. Mineo; E. Morelli; F. Muleri; P. Orleanski; B. Phlips; L. Picolli; M. Rapisarda; A. Rashevski; R. Remillard; A. Rubini; T. Schanz; A. Segreto; M. Stolarski; C. Tenzer; R. Wawrzaszek; C. Wilson-Hodge; B. Winter; G. Zampa; N. Zampa; A. Alpar; D. Altamirano; L. Amati; L. A. Antonelli; P. Attinà; C. Barbieri; L. Burderi; M. Bursa; G. A. Caliandro; P. Casella; D. Chakrabarty; A. Corongiu; E. Costa; S. Covino; S. Dall'Osso; F. D'Amico; C. Done; T. Di Salvo; A. Drago; D. De Martino; A. De Rosa; I. Donnarumma; M. Dovciak; U. Ertan; M. Falanga; R. Fender; F. Frontera; P. Ghandi; E. Gogus; W. Hermsen; J. Isern; J. Horak; P. Jonker; E. Kalemci; G. Kanbach; V. Karas; W. Kluzniak; K. Kokkotas; J. Krolik; N. Kylafis; J. Lattimer; D. Leahy; T. Maccarone; J. McClintock; M. Mendez; S. Mereghetti; R. Mignani; C. Miller; S. Mornick; S. Motta; T. Muñoz-Darias; A. Naletto; M. Orio; M. Orlandini; F. Ozel; L. Pacciani; S. Paltani; I. Papadakis; A. Papitto; A. Patruno; A. Pellizzoni; A. Possenti; D. Psaltis; N. Rea; P. Reig; P. Romano; M. Romanova; A. Shearer; P. Soffitta; N. Stergioulas; Z. Stuchlik; A. Tiengo; D. Torres; R. Turolla; S. Vercellone; A. Watts; K. Wood; L. Zampieri; S. Zane; A. Zezas; J. Ziolkowski

LOFT: A large observatory for x-ray timing

Fabio Muleri
, M. Feroci
, T. Belloni
, J. Braga
, S. Campana
, T. Courvousier
, M. Hernanz
, R. Hudec
, G. L. Israel
, P. S. Ray
, A. Santangelo
, L. Stella
, A. Vacchi
, M. Van Der Klis
, D. Walton
, A. Zdziarski
, J. M. Alvarez
, A. Argan
, G. Baldazzi
, M. Barbera

G. Bertuccio, V. Bonvicini, E. Bozzo, R. Campana, A. Collura, G. Cusumano, E. Del Monte, J. W. Den Herder, S. Di Cosimo, G. Di Persio, Y. Evangelista, F. Fuschino, J. L. Galvez, P. Giommi, M. Grassi, P. Guttridge, J. J.M. In'T Zand, D. Kataria, D. Klochkov, C. Labanti, F. Lazzarotto, P. Malcovati, M. Marisaldi, M. Mastropietro, T. Mineo, E. Morelli, F. Muleri, P. Orleanski, B. Phlips, L. Picolli, M. Rapisarda, A. Rashevski, R. Remillard, A. Rubini, T. Schanz, A. Segreto, M. Stolarski, C. Tenzer, R. Wawrzaszek, C. Wilson-Hodge, B. Winter, G. Zampa, N. Zampa, A. Alpar, D. Altamirano, L. Amati, L. A. Antonelli, P. Attinà, C. Barbieri, L. Burderi, M. Bursa, G. A. Caliandro, P. Casella, D. Chakrabarty, A. Corongiu, E. Costa, S. Covino, S. Dall'Osso, F. D'Amico, C. Done, T. Di Salvo, A. Drago, D. De Martino, A. De Rosa, I. Donnarumma, M. Dovciak, U. Ertan, M. Falanga, R. Fender, F. Frontera, P. Ghandi, E. Gogus, W. Hermsen, J. Isern, J. Horak, P. Jonker, E. Kalemci, G. Kanbach, V. Karas, W. Kluzniak, K. Kokkotas, J. Krolik, N. Kylafis, J. Lattimer, D. Leahy, T. Maccarone, J. McClintock, M. Mendez, S. Mereghetti, R. Mignani, C. Miller, S. Mornick, S. Motta, T. Muñoz-Darias, A. Naletto, M. Orio, M. Orlandini, F. Ozel, L. Pacciani, S. Paltani, I. Papadakis, A. Papitto, A. Patruno, A. Pellizzoni, A. Possenti, D. Psaltis, N. Rea, P. Reig, P. Romano, M. Romanova, A. Shearer, P. Soffitta, N. Stergioulas, Z. Stuchlik, A. Tiengo, D. Torres, R. Turolla, S. Vercellone, A. Watts, K. Wood, L. Zampieri, S. Zane, A. Zezas, J. Ziolkowski

Physics and Astronomy

National Institute for Astrophysics
Instituto Nacional de Pesquisas Espaciais
University of Geneva
Institute of Space Studies of Catalonia
Czech Technical University in Prague
NRL
University of Tübingen
National Institute for Nuclear Physics
University of Amsterdam
MSSL
N. Copernicus
LOFT

Research output: Contribution to journal › Conference article › peer-review

Abstract

LOFT (Large area Observatory For x-ray Timing) is an innovative mission submitted in response to the Cosmic Vision "Call for a Medium-size mission opportunity for a launch in 2022" recently issued by ESA. LOFT is an ideal candidate for the next generation of (extremely) large experiments for X-ray timing dedicated to the study of the physics of compact objects and to the understanding of the behavior of matter in strong gravitational fields. Recent developments in the field of large area monolithic silicon detectors allowed us to reach an effective area ∼12 m² (15 m² goal), more than a order of magnitude larger that RXTE/PCA, in the energy range 2-30 keV (1-40 keV goal). This Large Area Detector (LAD) will have both high timing resolution (<10 μs, 5 μs goal) and good spectral capabilities (<260 eV, <180 eV goal). A Wide Field Monitor (WFM), sensitive in the ∼1-50 keV energy range, will observe simultaneously more than a quarter of the sky in order to both discover and localize transient events and study their long term evolution.

Original language	English
Journal	Proceedings of Science
State	Published - 2010
Event	8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010 - Dublin Castle, Dublin, Ireland Duration: Sep 27 2010 → Sep 30 2010

Cite this

@article{5280ab4637ce4a408a45cd2e77a092e9,

title = "LOFT: A large observatory for x-ray timing",

abstract = "LOFT (Large area Observatory For x-ray Timing) is an innovative mission submitted in response to the Cosmic Vision {"}Call for a Medium-size mission opportunity for a launch in 2022{"} recently issued by ESA. LOFT is an ideal candidate for the next generation of (extremely) large experiments for X-ray timing dedicated to the study of the physics of compact objects and to the understanding of the behavior of matter in strong gravitational fields. Recent developments in the field of large area monolithic silicon detectors allowed us to reach an effective area ∼12 m2 (15 m2 goal), more than a order of magnitude larger that RXTE/PCA, in the energy range 2-30 keV (1-40 keV goal). This Large Area Detector (LAD) will have both high timing resolution (<10 μs, 5 μs goal) and good spectral capabilities (<260 eV, <180 eV goal). A Wide Field Monitor (WFM), sensitive in the ∼1-50 keV energy range, will observe simultaneously more than a quarter of the sky in order to both discover and localize transient events and study their long term evolution.",

author = "Fabio Muleri and M. Feroci and T. Belloni and J. Braga and S. Campana and T. Courvousier and M. Hernanz and R. Hudec and Israel, \{G. L.\} and Ray, \{P. S.\} and A. Santangelo and L. Stella and A. Vacchi and \{Van Der Klis\}, M. and D. Walton and A. Zdziarski and Alvarez, \{J. M.\} and A. Argan and G. Baldazzi and M. Barbera and G. Bertuccio and V. Bonvicini and E. Bozzo and R. Campana and A. Collura and G. Cusumano and \{Del Monte\}, E. and \{Den Herder\}, \{J. W.\} and \{Di Cosimo\}, S. and \{Di Persio\}, G. and Y. Evangelista and F. Fuschino and Galvez, \{J. L.\} and P. Giommi and M. Grassi and P. Guttridge and \{In'T Zand\}, \{J. J.M.\} and D. Kataria and D. Klochkov and C. Labanti and F. Lazzarotto and P. Malcovati and M. Marisaldi and M. Mastropietro and T. Mineo and E. Morelli and F. Muleri and P. Orleanski and B. Phlips and L. Picolli and M. Rapisarda and A. Rashevski and R. Remillard and A. Rubini and T. Schanz and A. Segreto and M. Stolarski and C. Tenzer and R. Wawrzaszek and C. Wilson-Hodge and B. Winter and G. Zampa and N. Zampa and A. Alpar and D. Altamirano and L. Amati and Antonelli, \{L. A.\} and P. Attin{\`a} and C. Barbieri and L. Burderi and M. Bursa and Caliandro, \{G. A.\} and P. Casella and D. Chakrabarty and A. Corongiu and E. Costa and S. Covino and S. Dall'Osso and F. D'Amico and C. Done and \{Di Salvo\}, T. and A. Drago and \{De Martino\}, D. and \{De Rosa\}, A. and I. Donnarumma and M. Dovciak and U. Ertan and M. Falanga and R. Fender and F. Frontera and P. Ghandi and E. Gogus and W. Hermsen and J. Isern and J. Horak and P. Jonker and E. Kalemci and G. Kanbach and V. Karas and W. Kluzniak and K. Kokkotas and J. Krolik and N. Kylafis and J. Lattimer and D. Leahy and T. Maccarone and J. McClintock and M. Mendez and S. Mereghetti and R. Mignani and C. Miller and S. Mornick and S. Motta and T. Mu{\~n}oz-Darias and A. Naletto and M. Orio and M. Orlandini and F. Ozel and L. Pacciani and S. Paltani and I. Papadakis and A. Papitto and A. Patruno and A. Pellizzoni and A. Possenti and D. Psaltis and N. Rea and P. Reig and P. Romano and M. Romanova and A. Shearer and P. Soffitta and N. Stergioulas and Z. Stuchlik and A. Tiengo and D. Torres and R. Turolla and S. Vercellone and A. Watts and K. Wood and L. Zampieri and S. Zane and A. Zezas and J. Ziolkowski",

year = "2010",

language = "English",

journal = "Proceedings of Science",

issn = "1824-8039",

note = "8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010 ; Conference date: 27-09-2010 Through 30-09-2010",

}

Muleri, F, Feroci, M, Belloni, T, Braga, J, Campana, S, Courvousier, T, Hernanz, M, Hudec, R, Israel, GL, Ray, PS, Santangelo, A, Stella, L, Vacchi, A, Van Der Klis, M, Walton, D, Zdziarski, A, Alvarez, JM, Argan, A, Baldazzi, G, Barbera, M, Bertuccio, G, Bonvicini, V, Bozzo, E, Campana, R, Collura, A, Cusumano, G, Del Monte, E, Den Herder, JW, Di Cosimo, S, Di Persio, G, Evangelista, Y, Fuschino, F, Galvez, JL, Giommi, P, Grassi, M, Guttridge, P, In'T Zand, JJM, Kataria, D, Klochkov, D, Labanti, C, Lazzarotto, F, Malcovati, P, Marisaldi, M, Mastropietro, M, Mineo, T, Morelli, E, Muleri, F, Orleanski, P, Phlips, B, Picolli, L, Rapisarda, M, Rashevski, A, Remillard, R, Rubini, A, Schanz, T, Segreto, A, Stolarski, M, Tenzer, C, Wawrzaszek, R, Wilson-Hodge, C, Winter, B, Zampa, G, Zampa, N, Alpar, A, Altamirano, D, Amati, L, Antonelli, LA, Attinà, P, Barbieri, C, Burderi, L, Bursa, M, Caliandro, GA, Casella, P, Chakrabarty, D, Corongiu, A, Costa, E, Covino, S, Dall'Osso, S, D'Amico, F, Done, C, Di Salvo, T, Drago, A, De Martino, D, De Rosa, A, Donnarumma, I, Dovciak, M, Ertan, U, Falanga, M, Fender, R, Frontera, F, Ghandi, P, Gogus, E, Hermsen, W, Isern, J, Horak, J, Jonker, P, Kalemci, E, Kanbach, G, Karas, V, Kluzniak, W, Kokkotas, K, Krolik, J, Kylafis, N, Lattimer, J, Leahy, D, Maccarone, T, McClintock, J, Mendez, M, Mereghetti, S, Mignani, R, Miller, C, Mornick, S, Motta, S, Muñoz-Darias, T, Naletto, A, Orio, M, Orlandini, M, Ozel, F, Pacciani, L, Paltani, S, Papadakis, I, Papitto, A, Patruno, A, Pellizzoni, A, Possenti, A, Psaltis, D, Rea, N, Reig, P, Romano, P, Romanova, M, Shearer, A, Soffitta, P, Stergioulas, N, Stuchlik, Z, Tiengo, A, Torres, D, Turolla, R, Vercellone, S, Watts, A, Wood, K, Zampieri, L, Zane, S, Zezas, A & Ziolkowski, J 2010, 'LOFT: A large observatory for x-ray timing', Proceedings of Science.

TY - JOUR

T1 - LOFT

T2 - 8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010

AU - Muleri, Fabio

AU - Feroci, M.

AU - Belloni, T.

AU - Braga, J.

AU - Campana, S.

AU - Courvousier, T.

AU - Hernanz, M.

AU - Hudec, R.

AU - Israel, G. L.

AU - Ray, P. S.

AU - Santangelo, A.

AU - Stella, L.

AU - Vacchi, A.

AU - Van Der Klis, M.

AU - Walton, D.

AU - Zdziarski, A.

AU - Alvarez, J. M.

AU - Argan, A.

AU - Baldazzi, G.

AU - Barbera, M.

AU - Bertuccio, G.

AU - Bonvicini, V.

AU - Bozzo, E.

AU - Campana, R.

AU - Collura, A.

AU - Cusumano, G.

AU - Del Monte, E.

AU - Den Herder, J. W.

AU - Di Cosimo, S.

AU - Di Persio, G.

AU - Evangelista, Y.

AU - Fuschino, F.

AU - Galvez, J. L.

AU - Giommi, P.

AU - Grassi, M.

AU - Guttridge, P.

AU - In'T Zand, J. J.M.

AU - Kataria, D.

AU - Klochkov, D.

AU - Labanti, C.

AU - Lazzarotto, F.

AU - Malcovati, P.

AU - Marisaldi, M.

AU - Mastropietro, M.

AU - Mineo, T.

AU - Morelli, E.

AU - Muleri, F.

AU - Orleanski, P.

AU - Phlips, B.

AU - Picolli, L.

AU - Rapisarda, M.

AU - Rashevski, A.

AU - Remillard, R.

AU - Rubini, A.

AU - Schanz, T.

AU - Segreto, A.

AU - Stolarski, M.

AU - Tenzer, C.

AU - Wawrzaszek, R.

AU - Wilson-Hodge, C.

AU - Winter, B.

AU - Zampa, G.

AU - Zampa, N.

AU - Alpar, A.

AU - Altamirano, D.

AU - Amati, L.

AU - Antonelli, L. A.

AU - Attinà, P.

AU - Barbieri, C.

AU - Burderi, L.

AU - Bursa, M.

AU - Caliandro, G. A.

AU - Casella, P.

AU - Chakrabarty, D.

AU - Corongiu, A.

AU - Costa, E.

AU - Covino, S.

AU - Dall'Osso, S.

AU - D'Amico, F.

AU - Done, C.

AU - Di Salvo, T.

AU - Drago, A.

AU - De Martino, D.

AU - De Rosa, A.

AU - Donnarumma, I.

AU - Dovciak, M.

AU - Ertan, U.

AU - Falanga, M.

AU - Fender, R.

AU - Frontera, F.

AU - Ghandi, P.

AU - Gogus, E.

AU - Hermsen, W.

AU - Isern, J.

AU - Horak, J.

AU - Jonker, P.

AU - Kalemci, E.

AU - Kanbach, G.

AU - Karas, V.

AU - Kluzniak, W.

AU - Kokkotas, K.

AU - Krolik, J.

AU - Kylafis, N.

AU - Lattimer, J.

AU - Leahy, D.

AU - Maccarone, T.

AU - McClintock, J.

AU - Mendez, M.

AU - Mereghetti, S.

AU - Mignani, R.

AU - Miller, C.

AU - Mornick, S.

AU - Motta, S.

AU - Muñoz-Darias, T.

AU - Naletto, A.

AU - Orio, M.

AU - Orlandini, M.

AU - Ozel, F.

AU - Pacciani, L.

AU - Paltani, S.

AU - Papadakis, I.

AU - Papitto, A.

AU - Patruno, A.

AU - Pellizzoni, A.

AU - Possenti, A.

AU - Psaltis, D.

AU - Rea, N.

AU - Reig, P.

AU - Romano, P.

AU - Romanova, M.

AU - Shearer, A.

AU - Soffitta, P.

AU - Stergioulas, N.

AU - Stuchlik, Z.

AU - Tiengo, A.

AU - Torres, D.

AU - Turolla, R.

AU - Vercellone, S.

AU - Watts, A.

AU - Wood, K.

AU - Zampieri, L.

AU - Zane, S.

AU - Zezas, A.

AU - Ziolkowski, J.

PY - 2010

Y1 - 2010

N2 - LOFT (Large area Observatory For x-ray Timing) is an innovative mission submitted in response to the Cosmic Vision "Call for a Medium-size mission opportunity for a launch in 2022" recently issued by ESA. LOFT is an ideal candidate for the next generation of (extremely) large experiments for X-ray timing dedicated to the study of the physics of compact objects and to the understanding of the behavior of matter in strong gravitational fields. Recent developments in the field of large area monolithic silicon detectors allowed us to reach an effective area ∼12 m2 (15 m2 goal), more than a order of magnitude larger that RXTE/PCA, in the energy range 2-30 keV (1-40 keV goal). This Large Area Detector (LAD) will have both high timing resolution (<10 μs, 5 μs goal) and good spectral capabilities (<260 eV, <180 eV goal). A Wide Field Monitor (WFM), sensitive in the ∼1-50 keV energy range, will observe simultaneously more than a quarter of the sky in order to both discover and localize transient events and study their long term evolution.

AB - LOFT (Large area Observatory For x-ray Timing) is an innovative mission submitted in response to the Cosmic Vision "Call for a Medium-size mission opportunity for a launch in 2022" recently issued by ESA. LOFT is an ideal candidate for the next generation of (extremely) large experiments for X-ray timing dedicated to the study of the physics of compact objects and to the understanding of the behavior of matter in strong gravitational fields. Recent developments in the field of large area monolithic silicon detectors allowed us to reach an effective area ∼12 m2 (15 m2 goal), more than a order of magnitude larger that RXTE/PCA, in the energy range 2-30 keV (1-40 keV goal). This Large Area Detector (LAD) will have both high timing resolution (<10 μs, 5 μs goal) and good spectral capabilities (<260 eV, <180 eV goal). A Wide Field Monitor (WFM), sensitive in the ∼1-50 keV energy range, will observe simultaneously more than a quarter of the sky in order to both discover and localize transient events and study their long term evolution.

UR - https://www.scopus.com/pages/publications/84884711533

M3 - Conference article

AN - SCOPUS:84884711533

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

Y2 - 27 September 2010 through 30 September 2010

ER -

LOFT: A large observatory for x-ray timing

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