The Large Observatory for X-ray Timing

D 2014

The Large Observatory for X-ray Timing

ABRAMOWICZ, Marek; Pavel BAKALA; Zdeněk STUCHLÍK a Gabriel TÖRÖK

Základní údaje

Originální název

The Large Observatory for X-ray Timing

Autoři

ABRAMOWICZ, Marek; Pavel BAKALA; Zdeněk STUCHLÍK a Gabriel TÖRÖK

Vydání

Bellingham, Washington, Proc. SPIE Vol. 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 20 s. 2014

Nakladatel

SPIE

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

ISBN

978-0-8194-9612-6

ISSN

DOI

https://doi.org/10.1117/12.2055913

UT WoS

000354529100085

EID Scopus

2-s2.0-84922526544

Klíčová slova anglicky

X-ray timing;compact objects;X-ray spectroscopy;X-ray imaging;X-ray detectors;microchannel plates

Štítky

FÚ, sbornik

Příznaky

Mezinárodní význam

Změněno: 7. 4. 2021 15:19, Mgr. Pavlína Jalůvková

Anotace

V originále

The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final downselection for a launch slot in 2022-2024. Thanks to the unprecedented combination of effective area and spectral resolutionof its main instrument, LOFT will study the behaviour of matter under extreme conditions, such as the strong gravitational field in the innermost regions of accretion flows close to black holes and neutron stars, and the supranuclear densities in the interior of neutron stars. The science payload is based on a Large Area Detector (LAD, 10 m^2 effective area, 2-30 keV, 240 eV spectral resolution, 1^circ collimated field of view) and a Wide Field Monitor (WFM, 2-50 keV, 4 steradian field of view, 1 arcmin source location accuracy, 300 eV spectral resolution). The WFM is equipped with an on-board system for bright events (e.g. GRB) localization. The trigger time and position of these events are broadcast to the ground within 30 s from dis

Citovat

ABRAMOWICZ, Marek; Pavel BAKALA; Zdeněk STUCHLÍK a Gabriel TÖRÖK. The Large Observatory for X-ray Timing. In Proc. SPIE Vol. 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. Bellingham, Washington: SPIE, 2014, 20 s. ISBN 978-0-8194-9612-6. Dostupné z: https://doi.org/10.1117/12.2055913.

@inproceedings{42723,
   author = {Abramowicz, Marek and Bakala, Pavel and Stuchlík, Zdeněk and Török, Gabriel},
   address = {Bellingham, Washington},
   booktitle = {Proc. SPIE Vol. 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray},
   doi = {https://doi.org/10.1117/12.2055913},
   keywords = {X-ray timing;compact objects;X-ray spectroscopy;X-ray imaging;X-ray detectors;microchannel plates},
   language = {eng},
   location = {Bellingham, Washington},
   isbn = {978-0-8194-9612-6},
   publisher = {SPIE},
   title = {The Large Observatory for X-ray Timing},
   url = {http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1893955},
   year = {2014}
}

TY  - CONF
ID  - 42723
AU  - Abramowicz, Marek - Bakala, Pavel - Stuchlík, Zdeněk - Török, Gabriel
PY  - 2014
TI  - The Large Observatory for X-ray Timing
PB  - SPIE
CY  - Bellingham, Washington
SN  - 9780819496126
KW  - X-ray timing;compact objects;X-ray spectroscopy;X-ray imaging;X-ray detectors;microchannel plates
UR  - http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1893955
N2  - The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final downselection for a launch slot in 2022-2024. Thanks to the unprecedented combination of effective area and spectral resolutionof its main instrument, LOFT will study the behaviour of matter under extreme conditions, such as the strong gravitational field in the innermost regions of accretion flows close to black holes and neutron stars, and the supranuclear densities in the interior of neutron stars. The science payload is based on a Large Area Detector (LAD, 10 m^2 effective area, 2-30 keV, 240 eV spectral resolution, 1^circ collimated field of view) and a Wide Field Monitor (WFM, 2-50 keV, 4 steradian field of view, 1 arcmin source location accuracy, 300 eV spectral resolution). The WFM is equipped with an on-board system for bright events (e.g. GRB) localization. The trigger time and position of these events are broadcast to the ground within 30 s from dis
ER  -

ABRAMOWICZ, Marek; Pavel BAKALA; Zdeněk STUCHLÍK a Gabriel TÖRÖK. The Large Observatory for X-ray Timing. In \textit{Proc. SPIE Vol. 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray}. Bellingham, Washington: SPIE, 2014, 20 s. ISBN~978-0-8194-9612-6. Dostupné z: https://doi.org/10.1117/12.2055913.

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