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This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of gamma-ray bursts. For a summary, we refer to…

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of magnetospheres of isolated neutron stars.…

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of high-mass X-ray binaries and ultra-luminous…

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of active galactic nuclei. For a summary, we…

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of stellar flares. For a summary, we refer to…

高能天体物理现象 · 物理学 2015-01-13 S. A. Drake , E. Behar , J. G. Doyle , M. Güdel , K. Hamaguchi , A. F. Kowalski , T. Maccarone , R. A. Osten , U. Peretz , S. J. Wolk

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of radio-loud Active Galactic Nuclei. For a…

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of jetted tidal disruption events. For a…

高能天体物理现象 · 物理学 2015-01-13 E. M. Rossi , I. Donnarumma , R. Fender , P. Jonker , S. Komossa , Z. Paragi , I. Prandoni , L. Zampieri

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of the physics of accretion and ejection around…

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of high-energy radiation from thunderstorms and…

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of accreting white dwarfs. For a summary, we…

LOFT, the Large Observatory for X-ray Timing, is a new space mission concept devoted to observations of Galactic and extra-Galactic sources in the X-ray domain with the main goals of probing gravity theory in the very strong field…

天体物理仪器与方法 · 物理学 2019-08-14 E. Bozzo

LOFT, the large observatory for X-ray timing, is a new mission concept competing with other four candidates for a launch opportunity in 2022-2024. LOFT will be performing high-time resolution X-ray observations of compact objects, combining…

天体物理仪器与方法 · 物理学 2015-06-12 Tomaso M. Belloni , Enrico Bozzo

LOFT, the Large Observatory For X-ray Timing, is one of five ESA M3 candidate missions. It will address the Cosmic Vision theme: "Matter under Extreme Conditions". By coupling for the first time a huge collecting area for the detection of…

天体物理仪器与方法 · 物理学 2015-06-18 E. Bozzo , L. Stella , M. van der Klis , A. Watts , D. Barret , J. Wilms , P. Uttley , J. W. den Herder , M. Feroci

The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final down-selection for a launch slot in 2022-2024. Thanks to the unprecedented combination of effective area and…

天体物理仪器与方法 · 物理学 2014-09-01 M. Feroci , J. W. den Herder , E. Bozzo , D. Barret , S. Brandt , M. Hernanz , M. van der Klis , M. Pohl , A. Santangelo , L. Stella , A. Watts , J. Wilms , S. Zane , M. Ahangarianabhari , C. Albertus , M. Alford , A. Alpar , D. Altamirano , L. Alvarez , L. Amati , C. Amoros , N. Andersson , A. Antonelli , A. Argan , R. Artigue , B. Artigues , J. -L. Atteia , P. Azzarello , P. Bakala , G. Baldazzi , S. Balman , M. Barbera , C. van Baren , S. Bhattacharyya , A. Baykal , T. Belloni , F. Bernardini , G. Bertuccio , S. Bianchi , A. Bianchini , P. Binko , P. Blay , F. Bocchino , P. Bodin , I. Bombaci , J. -M. Bonnet Bidaud , S. Boutloukos , L. Bradley , J. Braga , E. Brown , N. Bucciantini , L. Burderi , M. Burgay , M. Bursa , C. Budtz-Jørgensen , E. Cackett , F. R. Cadoux , P. Cais , G. A. Caliandro , R. Campana , S. Campana , F. Capitanio , J. Casares , P. Casella , A. J. Castro-Tirado , E. Cavazzuti , P. Cerda-Duran , D. Chakrabarty , F. Château , J. Chenevez , J. Coker , R. Cole , A. Collura , R. Cornelisse , T. Courvoisier , A. Cros , A. Cumming , G. Cusumano , A. D'Aì , V. D'Elia , E. Del Monte , A. De Luca , D. De Martino , J. P. C. Dercksen , M. De Pasquale , A. De Rosa , M. Del Santo , S. Di Cosimo , S. Diebold , T. Di Salvo , I. Donnarumma , A. Drago , M. Durant , D. Emmanoulopoulos , M. H. Erkut , P. Esposito , Y. Evangelista , A. Fabian , M. Falanga , Y. Favre , C. Feldman , V. Ferrari , C. Ferrigno , M. Finger , M. H. Finger , G. W. Fraser , M. Frericks , F. Fuschino , M. Gabler , D. K. Galloway , J. L. Galvez Sanchez , E. Garcia-Berro , B. Gendre , S. Gezari , A. B. Giles , M. Gilfanov , P. Giommi , G. Giovannini , M. Giroletti , E. Gogus , A. Goldwurm , K. Goluchová , D. Götz , C. Gouiffes , M. Grassi , P. Groot , M. Gschwender , L. Gualtieri , C. Guidorzi , L. Guy , D. Haas , P. Haensel , M. Hailey , F. Hansen , D. H. Hartmann , C. A. Haswell , K. Hebeler , A. Heger , W. Hermsen , J. Homan , A. Hornstrup , R. Hudec , J. Huovelin , A. Ingram , J. J. M. in't Zand , G. Israel , K. Iwasawa , L. Izzo , H. M. Jacobs , F. Jetter , T. Johannsen , H. M. Jacobs , P. Jonker , J. Josè , P. Kaaret , G. Kanbach , V. Karas , D. Karelin , D. Kataria , L. Keek , T. Kennedy , D. Klochkov , W. Kluzniak , K. Kokkotas , S. Korpela , C. Kouveliotou , I. Kreykenbohm , L. M. Kuiper , I. Kuvvetli , C. Labanti , D. Lai , F. K. Lamb , P. P. Laubert , F. Lebrun , D. Lin , D. Linder , G. Lodato , F. Longo , N. Lund , T. J. Maccarone , D. Macera , S. Maestre , S. Mahmoodifar , D. Maier , P. Malcovati , I. Mandel , V. Mangano , A. Manousakis , M. Marisaldi , A. Markowitz , A. Martindale , G. Matt , I. M. McHardy , A. Melatos , M. Mendez , S. Mereghetti , M. Michalska , S. Migliari , R. Mignani , M. C. Miller , J. M. Miller , T. Mineo , G. Miniutti , S. Morsink , C. Motch , S. Motta , M. Mouchet , G. Mouret , J. Mulačová , F. Muleri , T. Muñoz-Darias , I. Negueruela , J. Neilsen , A. J. Norton , M. Nowak , P. O'Brien , P. E. H. Olsen , M. Orienti , M. Orio , M. Orlandini , P. Orleanski , J. P. Osborne , R. Osten , F. Ozel , L. Pacciani , M. Paolillo , A. Papitto , J. M. Paredes , A. Patruno , B. Paul , E. Perinati , A. Pellizzoni , A. V. Penacchioni , M. A. Perez , V. Petracek , C. Pittori , J. Pons , J. Portell , A. Possenti , J. Poutanen , M. Prakash , P. Le Provost , D. Psaltis , D. Rambaud , P. Ramon , G. Ramsay , M. Rapisarda , A. Rachevski , I. Rashevskaya , P. S. Ray , N. Rea , S. Reddy , P. Reig , M. Reina Aranda , R. Remillard , C. Reynolds , L. Rezzolla , M. Ribo , R. de la Rie , A. Riggio , A. Rios , P. Rodríguez- Gil , J. Rodriguez , R. Rohlfs , P. Romano , E. M. R. Rossi , A. Rozanska , A. Rousseau , F. Ryde , L. Sabau-Graziati , G. Sala , R. Salvaterra , A. Sanna , J. Sandberg , S. Scaringi , S. Schanne , J. Schee , C. Schmid , S. Shore , R. Schneider , A. Schwenk , A. D. Schwope , J. -Y. Seyler , A. Shearer , A. Smith , D. M. Smith , P. J. Smith , V. Sochora , P. Soffitta , P. Soleri , A. Spencer , B. Stappers , A. W. Steiner , N. Stergioulas , G. Stratta , T. E. Strohmayer , Z. Stuchlik , S. Suchy , V. Sulemainov , T. Takahashi , F. Tamburini , T. Tauris , C. Tenzer , L. Tolos , F. Tombesi , J. Tomsick , G. Torok , J. M. Torrejon , D. F. Torres , A. Tramacere , A. Trois , R. Turolla , S. Turriziani , P. Uter , P. Uttley , A. Vacchi , P. Varniere , S. Vaughan , S. Vercellone , V. Vrba , D. Walton , S. Watanabe , R. Wawrzaszek , N. Webb , N. Weinberg , H. Wende , P. Wheatley , R. Wijers , R. Wijnands , M. Wille , C. A. Wilson-Hodge , B. Winter , K. Wood , G. Zampa , N. Zampa , L. Zampieri , L. Zdunik , A. Zdziarski , B. Zhang , F. Zwart , M. Ayre , T. Boenke , C. Corral van Damme , E. Kuulkers , D. Lumb

LOFT, the large observatory for X-ray timing, was selected by the European Space Agency (ESA) in February 2011 as one of four medium size mission concepts for the Cosmic Vision program that will compete for a launch opportunity in the early…

天体物理仪器与方法 · 物理学 2012-10-09 E. Bozzo , P. Esposito , P. Romano

The Large Observatory For X-ray Timing, LOFT, was selected by the European Space Agency as one of the four Cosmic Vision M3 candidate missions to compete for a launch opportunity at the start of the 2020s. Thanks to an innovative design and…

天体物理仪器与方法 · 物理学 2019-08-14 E. Bozzo , J. W. den Herder , M. Feroci , L. Stella

LOFT is one of the four medium mission candidates (M3), selected by ESA in the framework of the Cosmic Vision Programme (2015-2025), for feasibility study. If approved by ESA in 2014, its launch is foreseen in 2022-2024. LOFT is being…

天体物理仪器与方法 · 物理学 2019-08-13 M. Hernanz

High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultra-dense matter and to black hole masses and spins. A 10 m^2-class instrument in combination with good…

天体物理仪器与方法 · 物理学 2015-05-28 M. Feroci , the LOFT Consortium

LOFT (the Large Observatory for X-ray Timing), is a mission concept that was considered by ESA as a candidate for an M3 mission and has been studied during an extended >2-years long assessment phase. The mission was specifically designed to…

天体物理仪器与方法 · 物理学 2015-06-23 S. Zane

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is currently planned for between 2022 and 2024. LOFT is designed to…

天体物理仪器与方法 · 物理学 2015-06-11 M. Feroci , J. W. den Herder , E. Bozzo , D. Barret , S. Brandt , M. Hernanz , M. van der Klis , M. Pohl , A. Santangelo , L. Stella , A. Watts , J. Wilms , S. Zane , M. Ahangarianabhari , A. Alpar , D. Altamirano , L. Alvarez , L. Amati , C. Amoros , N. Andersson , A. Antonelli , A. Argan , R. Artigue , P. Azzarello , G. Baldazzi , S. Balman , M. Barbera , T. Belloni , G. Bertuccio , S. Bianchi , A. Bianchini , P. Bodin , J. -M. Bonnet Bidaud , S. Boutloukos , J. Braga , E. Brown , N. Bucciantini , L. Burderi , M. Bursa , C. Budtz-Jørgensen , E. Cackett , F. R. Cadoux , P. Cais , G. A. Caliandro , R. Campana , S. Campana , P. Casella , D. Chakrabarty , J. Chenevez , J. Coker , R. Cole , A. Collura , T. Courvoisier , A. Cros , A. Cumming , G. Cusumano , A. D'Aì , V. D'Elia , E. Del Monte , D. De Martino , A. De Rosa , S. Di Cosimo , S. Diebold , T. Di Salvo , I. Donnarumma , A. Drago , M. Durant , D. Emmanoulopoulos , Y. Evangelista , A. Fabian , M. Falanga , Y. Favre , C. Feldman , C. Ferrigno , M. H. Finger , G. W. Fraser , F. Fuschino , D. K. Galloway , J. L. Galvez Sanchez , E. Garcia-Berro , B. Gendre , S. Gezari , A. B. Giles , M. Gilfanov , P. Giommi , G. Giovannini , M. Giroletti , A. Goldwurm , D. Götz , C. Gouiffes , M. Grassi , P. Groot C. Guidorzi , D. Haas , F. Hansen , D. H. Hartmann , C. A. Haswe , A. Heger , J. Homan , A. Hornstrup , R. Hudec , J. Huovelin , A. Ingram , J. J. M. in't Zand , J. Isern , G. Israe , L. Izzo , P. Jonker , P. Kaaret , V. Karas , D. Karelin , D. Kataria , L. Keek , T. Kennedy , D. Klochkov , W. Kluzniak , K. Kokkotas , S. Korpela , C. Kouveliotou , I. Kreykenbohm , L. M. Kuiper , I. Kuvvetli , C. Labanti , D. Lai , F. K. Lamb , F. Lebrun , D. Lin , D. Linder , G. Lodato , F. Longo , N. Lund , T. J. Maccarone , D. Macera , D. Maier , P. Malcovati , V. Mangano , A. Manousakis , M. Marisaldi , A. Markowitz , A. Martindale , G. Matt , I. M. McHardy , A. Melatos , M. Mendez , S. Migliari , R. Mignani , M. C. Miller , J. M. Miller , T. Mineo , G. Miniutti , S. Morsink , C. Motch , S. Motta , M. Mouchet , F. Muleri , A. J. Norton , M. Nowak , P. O'Brien , M. Orienti , M. Orio , M. Orlandini , P. Orleanski , J. P. Osborne , R. Osten , F. Ozel , L. Pacciani , A. Papitto , B. Paul , E. Perinati , V. Petracek , J. Portell , J. Poutanen , D. Psaltis , D. Rambaud , G. Ramsay , M. Rapisarda , A. Rachevski , P. S. Ray , N. Rea , S. Reddy , P. Reig , M. Reina Aranda , R. Remillard , C. Reynolds , P. Rodríguez-Gil , J. Rodriguez , P. Romano , E. M. R. Rossi , F. Ryde , L. Sabau-Graziati , G. Sala , R. Salvaterra , A. Sanna , S. Schanne , J. Schee , C. Schmid , A. Schwenk , A. D. Schwope , J. -Y. Seyler , A. Shearer , A. Smith , D. M. Smith , P. J. Smith , V. Sochora , P. Soffitta , P. Soleri , B. Stappers , B. Stelzer , N. Stergioulas , G. Stratta , T. E. Strohmayer , Z. Stuchlik , S. Suchy , V. Sulemainov , T. Takahashi , F. Tamburini , C. Tenzer , L. Tolos , G. Torok , J. M. Torrejon , D. F. Torres , A. Tramacere , A. Trois , S. Turriziani , P. Uter , P. Uttley , A. Vacchi , P. Varniere , S. Vaughan , S. Vercellone , V. Vrba , D. Walton , S. Watanabe , R. Wawrzaszek , N. Webb , N. Weinberg , H. Wende , P. Wheatley , R. Wijers , R. Wijnands , M. Wille , C. A. Wilson-Hodge , B. Winter , K. Wood , G. Zampa , N. Zampa , L. Zampieri , A. Zdziarski , B. Zhang
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