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Related papers: LOFT: Large Observatory For X-ray Timing

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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…

Instrumentation and Methods for Astrophysics · Physics 2015-06-23 S. Zane

The Large Observatory for X-ray Timing (LOFT) is one of the four candidate ESA M3 missions considered for launch in the 2022 time-frame. It is specifically designed to perform fast X-ray timing and probe the status of the matter near black…

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…

Instrumentation and Methods for Astrophysics · Physics 2015-05-28 M. Feroci , the LOFT Consortium

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…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 E. Bozzo , J. W. den Herder , M. Feroci , L. Stella

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…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 E. Bozzo

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…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 M. Hernanz

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…

Instrumentation and Methods for Astrophysics · Physics 2015-06-12 Tomaso M. Belloni , Enrico Bozzo

LOFT (Large Observatory for X-ray Timing) is one of the five candidates that were considered by ESA as an M3 mission (with launch in 2022-2024) and has been studied during an extensive assessment phase. It is specifically designed to…

The high time resolution observations of the X-ray sky hold the key to a number of diagnostics of fundamental physics, some of which are unaccessible to other types of investigations, such as those based on imaging and spectroscopy.…

Large Observatory For X-ray Timing (LOFT) is a next generation X-ray telescope selected by European Space Agency as one of the space mission concepts within the ``Cosmic Vision'' programme. The Large Area Detector on board of LOFT will be a…

Cosmology and Nongalactic Astrophysics · Physics 2014-12-31 A. Neronov , A. Boyarsky , D. Iakubovskyi , O. Ruchayskiy

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…

Instrumentation and Methods for Astrophysics · Physics 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…

Instrumentation and Methods for Astrophysics · Physics 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

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…

Instrumentation and Methods for Astrophysics · Physics 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

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…

Instrumentation and Methods for Astrophysics · Physics 2012-10-09 E. Bozzo , P. Esposito , P. Romano

The Large Observatory For X-ray Timing (LOFT) is an innovative medium-class mission selected for an assessment phase in the framework of the ESA M3 Cosmic Vision call. LOFT is intended to answer fundamental questions about the behaviour of…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 R. Campana , M. Feroci , E. Del Monte , S. Brandt , C. Budtz-Jørgensen , N. Lund , J. Alvarez , M. Hernanz , E. Perinati

LOFT (Large Observatory For x-ray Timing) is one of the four missions selected in 2011 for assessment study for the ESA M3 mission in the Cosmic Vision program, expected to be launched in 2024. The LOFT mission will carry two instruments…

LOFT (Large Observatory for X-ray Timing) is an X-ray timing observatory that, with four other candidates, was considered by ESA as an M3 mission (with launch in 2022-2024) and has been studied during an extensive assessment phase. Its…

The Large Observatory for X-ray Timing (LOFT) is one of the four candidate ESA M3 missions considered for launch in the time-frame of 2022. It is specifically designed to perform fast X-ray timing and probe the status of the matter near…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 S. Suchy , P. Uter , C. Tenzer , A. Santangelo , A. Argan , M. Feroci , T. E. Kennedy , P. J. Smith , D. Walton , S. Zane , J. Portell , E. García-Berro

The Large Observatory for X-ray Timing (LOFT) is one of the five candidates that were considered by ESA as an M3 mission (with launch in 2022-2024). It is specifically designed to exploit the diagnostics of very rapid X-ray flux and…

Instrumentation and Methods for Astrophysics · Physics 2014-08-29 Y. Evangelista , I. Donnarumma , R. Campana , C. Schmid , M. Feroci

The Large Observatory for X-ray Timing (LOFT) was one of the M3 missions selected for the phase A study in the ESA's Cosmic Vision program. LOFT is designed to perform high-time-resolution X-ray observations of black holes and neutron…

Instrumentation and Methods for Astrophysics · Physics 2014-08-29 M. Barbera , B. Winter , J. Coker , M. Feroci , T. Kennedy , D. Walton , S. Zane
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