LOFT: A large observatory for x-ray timing

F. 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; 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; 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; 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; E. Kalemci; G. Kanbach; V. Karas; W. Kluzniak; K. Kokkotas; N. Kylafis; J. Lattimer; D. Leahy; T. Maccarone; J. McClintock; M. Mendez; S. Mereghetti; R. Mignani; 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; L. Zampieri; S. Zane; A. Zezas; J. Ziolkowski

LOFT: A large observatory for x-ray timing

F. 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. BarberaG. 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, 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, 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, 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, E. Kalemci, G. Kanbach, V. Karas, W. Kluzniak, K. Kokkotas, N. Kylafis, J. Lattimer, D. Leahy, T. Maccarone, J. McClintock, M. Mendez, S. Mereghetti, R. Mignani, 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, L. Zampieri, S. Zane, A. Zezas, J. Ziolkowski

Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › 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
Title of host publication	8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010
Subtitle of host publication	Conference Proceedings
Publisher	Proceedings of Science
Publication status	Published - 30-Sept-2010
Event	8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010 - Dublin Castle, Dublin, Ireland Duration: 27-Sept-2010 → 30-Sept-2010

Publication series

Name	Proceedings of Science
ISSN (Print)	1824-8039

Conference

Conference	8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010
Country/Territory	Ireland
City	Dublin Castle, Dublin
Period	27/09/2010 → 30/09/2010

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Muleri, F., Feroci, M., Belloni, T., Braga, J., Campana, S., Courvousier, T., Hernanz, M., Hudec, R., Israel, G. L., Ray, P. S., Santangelo, A., Stella, L., Vacchi, A., Van Der Klis, M., Walton, D., Zdziarski, A., Alvarez, J. M., Argan, A., Baldazzi, G., ... Ziolkowski, J. (2010). LOFT: A large observatory for x-ray timing. In 8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010: Conference Proceedings Article Code 99182 (Proceedings of Science). Proceedings of Science.

@inproceedings{de9466c362f34dd2b3c1b65296c14f05,

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 = "F. 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 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 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 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 E. Kalemci and G. Kanbach and V. Karas and W. Kluzniak and K. Kokkotas 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 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 L. Zampieri and S. Zane and A. Zezas and J. Ziolkowski",

year = "2010",

month = sep,

day = "30",

language = "English",

series = "Proceedings of Science",

publisher = "Proceedings of Science",

booktitle = "8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010",

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, 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, 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, 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, Kalemci, E, Kanbach, G, Karas, V, Kluzniak, W, Kokkotas, K, Kylafis, N, Lattimer, J, Leahy, D, Maccarone, T, McClintock, J, Mendez, M, Mereghetti, S, Mignani, R, 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, Zampieri, L, Zane, S, Zezas, A & Ziolkowski, J 2010, LOFT: A large observatory for x-ray timing. in 8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010: Conference Proceedings., Code 99182, Proceedings of Science, Proceedings of Science, 8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010, Dublin Castle, Dublin, Ireland, 27/09/2010.

LOFT: A large observatory for x-ray timing. / Muleri, F.; Feroci, M.; Belloni, T. et al.
8th INTEGRAL Workshop on the Restless Gamma-Ray Universe, INTEGRAL 2010: Conference Proceedings. Proceedings of Science, 2010. Code 99182 (Proceedings of Science).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

TY - GEN

T1 - LOFT

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

AU - Muleri, F.

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 - 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 - 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 - 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 - Kalemci, E.

AU - Kanbach, G.

AU - Karas, V.

AU - Kluzniak, W.

AU - Kokkotas, K.

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 - 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 - Zampieri, L.

AU - Zane, S.

AU - Zezas, A.

AU - Ziolkowski, J.

PY - 2010/9/30

Y1 - 2010/9/30

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 - http://www.scopus.com/inward/record.url?scp=84884711533&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84884711533

T3 - Proceedings of Science

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

PB - Proceedings of Science

Y2 - 27 September 2010 through 30 September 2010

ER -

LOFT: A large observatory for x-ray timing

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