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Related papers: LEXT: a lobster eye optic for Gamow

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The Microchannel X-ray Telescope (MXT) is one of four instruments on the Space-based multi-band astronomical Variable Objects Monitor (SVOM) satellite mission, launched on the 22nd June 2024. The MXT is a narrow-field-optimised, lobster eye…

Instrumentation and Methods for Astrophysics · Physics 2026-05-12 Charly Feldman , James Pearson , Gillian Butcher , Richard Willingale , Paul O'Brien , Julian Osborne , Karine Mercier , Jean-Michel Le Duigou , Diego Gotz

As a novel X-ray focusing technology, lobster eye micro-pore optics (MPO) feature both a wide observing field of view and true imaging capability, promising sky monitoring with significantly improved sensitivity and spatial resolution in…

The Microchannel X-ray Telescope (MXT) will be the first focusing X-ray telescope based on a "Lobster-Eye" optical design to be flown on Sino-French mission SVOM. SVOM will be dedicated to the study of Gamma-Ray Bursts and more generally…

The Photo-z InfraRed Telescope (PIRT) is an instrument on the Gamow Explorer, currently proposed for a NASA Astrophysics Medium Explorer. PIRT works in tandem with a companion wide-field instrument, the Lobster Eye X-ray Telescope (LEXT),…

We present the Micro-channel X-ray Telescope (MXT), a new narrow-field (about 1{\deg}) telescope that will be flying on the Sino-French SVOM mission dedicated to Gamma-Ray Burst science, scheduled for launch in 2021. MXT is based on square…

Lobster-ISS is an X-ray all-sky monitor experiment selected by ESA two years ago for a Phase A study (now almost completed) for a future flight (2009) aboard the Columbus Exposed Payload Facility of the International Space Station. The main…

The Lobster Eye Imager for Astronomy (LEIA), a pathfinder of the Wide-field X-ray Telescope of the Einstein Probe (EP) mission, was successfully launched onboard the SATech-01 satellite of the Chinese Academy of Sciences on 27 July 2022. In…

Instrumentation and Methods for Astrophysics · Physics 2023-08-02 Z. X. Ling , X. J. Sun , C. Zhang , S. L. Sun , G. Jin , S. N. Zhang , X. F. Zhang , J. B. Chang , F. S. Chen , Y. F. Chen , Z. W. Cheng , W. Fu , Y. X. Han , H. Li , J. F. Li , Y. Li , Z. D. Li , P. R. Liu , Y. H. Lv , X. H. Ma , Y. J. Tang , C. B. Wang , R. J. Xie , Y. L. Xue , A. L. Yan , Q. Zhang , C. Y. Bao , H. B. Cai , H. Q. Cheng , C. Z. Cui , Y. F. Dai , D. W. Fan , H. B. Hu , J. W. Hu , M. H. Huang , Z. Q. Jia , C. C. Jin , D. Y. Li , J. Q. Li , H. Y. Liu , M. J. Liu , Y. Liu , H. W. Pan , Y. L. Qiu , M. Sugizaki , H. Sun , W. X. Wang , Y. L. Wang , Q. Y. Wu , X. P. Xu , Y. F. Xu , H. N. Yang , X. Yang , B. Zhang , M. Zhang , W. D. Zhang , Z. Zhang , D. H. Zhao , X. Q. Cong , B. W. Jiang , L. H. Li , X. B. Qiu , J. N. Sun , D. T. Su , J. Wang , C. Wu , Z. Xu , X. M. Yang , S. K. Zhang , Z. Zhang , N. Zhang , Y. F. Zhu , H. Y. Ban , X. Z. Bi , Z. M. Cai , W. Chen , X. Chen , Y. H. Chen , Y. Cui , X. L. Duan , Z. G Feng , Y. Gao , J. W. He , T. He , J. J. Huang , F. Li , J. S. Li , T. J. Li , T. T. Li , H. Q. Liu , L. Liu , R. Liu , S. Liu , N. Meng , Q. Shi , A. T. Sun , Y. M. Wang , Y. B. Wang , H. C. Wu , D. X Xu , Y. Q Yang , Y. Yang , X. S. Yu , K. X. Zhang , Y. L. Zhang , Y. H. Zhang , Y. T. Zhang , H. Zhou , X. C. Zhu , J. S. Cheng , L. Qin , L. Wang , Q. L. Wang , M. Bai , R. L. Gao , Z. Ji , Y. R. Liu , F. L. Ma , Y. J. Shi , J. Su , Y. Y. Tan , J. Z. Tong , H. T. Xu , C. B. Xue , G. F. Xue , W. Yuan

The Transient High Energy Sources and Early Universe Surveyor is an ESA M5 candidate mission currently in Phase A, with Launch in $\sim$2032. The aim of the mission is to complete a Gamma Ray Burst survey and monitor transient X-ray events.…

The next large NASA mission in the field of gamma-ray astronomy, GLAST, is scheduled for launch in 2007. Aside from the main instrument LAT (Large-Area Telescope), a gamma-ray telescope for the energy range between 20 MeV and > 100 GeV, a…

We report on results of the on-ground X-ray calibration of the Lobster Eye Imager for Astronomy (LEIA), an experimental space wide-field (18.6*18.6 square degrees) X-ray telescope built from novel lobster eye mirco-pore optics. LEIA was…

The Gamma-ray Large Area Space Telescope (GLAST) is a space-based observatory scheduled to launch in October 2007 with two instruments: (1) the GLAST Burst Monitor (GBM), sensitive to photon energies between 8 keV and 25 MeV and optimized…

Astrophysics · Physics 2008-11-26 Jennifer E. Carson

The localization of X-ray counterparts to gravitational wave events requires a telescope with accurate localization capability in a field of view comparable to the region constrained by the gravitational wave detectors. In the context of a…

Instrumentation and Methods for Astrophysics · Physics 2025-10-07 John Rankin , Sergio Campana , Giovanni Pareschi , Daniele Spiga , Stefano Basso , Marta Maria Civitani , Paolo Conconi , Vincenzo Cotroneo

This chapter describes the history, principles, and recent developments of large field of view X-ray optics based on lobster eye designs. Most of grazing incidence (reflective) X-ray imaging systems used in astronomy and other applications,…

Instrumentation and Methods for Astrophysics · Physics 2023-04-05 Rene Hudec , Charly Feldman

Galactic Exoplanet Survey Telescope (GEST) was proposed for a discovery mission to search for microlensing terrestrial planets toward the Galactic bulge and also Kuiper Belt Objects (KBOs) that are believed to hold vital information of the…

Astrophysics · Physics 2009-11-06 Sun Hong Rhie

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

Lobster eye telescopes are ideal monitors to detect X-ray transients, because they could observe celestial objects over a wide field of view in X-ray band. However, images obtained by lobster eye telescopes are modified by their unique…

Instrumentation and Methods for Astrophysics · Physics 2023-02-08 Peng Jia , Wenbo Liu , Yuan Liu , Haiwu Pan

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

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…

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