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The design of the wide field monitor for LOFT

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00481973" target="_blank" >RIV/67985815:_____/14:00481973 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1117/12.2055885" target="_blank" >http://dx.doi.org/10.1117/12.2055885</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1117/12.2055885" target="_blank" >10.1117/12.2055885</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The design of the wide field monitor for LOFT

  • Original language description

    LOFT (Large Observatory For x-ray Timing) is one of the ESA M3 missions selected within the Cosmic Vision program in 2011 to carry out an assessment phase study and compete for a launch opportunity in 2022-2024. The phase-A studies of all M3 missions were completed at the end of 2013. LOFT is designed to carry on-board two instruments with sensitivity in the 2-50 keV range: a 10 m(2) class Large Area Detector (LAD) with a < 1 degrees collimated FoV and a wide field monitor (WFM) making use of coded masks and providing an instantaneous coverage of more than 1/3 of the sky. The prime goal of the WFM will be to detect transient sources to be observed by the LAD. However, thanks to its unique combination of a wide field of view (FoV) and energy resolution (better than 500 eV), the WFM will be also an excellent monitoring instrument to study the long term variability of many classes of X-ray sources. The WFM consists of 10 independent and identical coded mask cameras arranged in 5 pairs to provide the desired sky coverage. We provide here an overview of the instrument design, configuration, and capabilities of the LOFT WFM. The compact and modular design of the WFM could easily make the instrument concept adaptable for other missions.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray

  • ISBN

    9780819496126

  • ISSN

    0277-786X

  • e-ISSN

  • Number of pages

    20

  • Pages from-to

    "91442V/1"-"91442V/20"

  • Publisher name

    SPIE

  • Place of publication

    Bellingham

  • Event location

    Montreal

  • Event date

    Jun 22, 2014

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000354529100086