GRB INVESTIGATIONS BY ESA GAIA AND LOFT

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F13%3A00212322" target="_blank" >RIV/68407700:21230/13:00212322 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.14311/AP.2013.53.0799" target="_blank" >https://doi.org/10.14311/AP.2013.53.0799</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.14311/AP.2013.53.0799" target="_blank" >10.14311/AP.2013.53.0799</a>

Jazyk výsledku

angličtina

Název v původním jazyce

GRB INVESTIGATIONS BY ESA GAIA AND LOFT

Popis výsledku v původním jazyce

The possibility of studying GRBs with the ESA Gaia and LOFT missions is briefly addressed. The ESA Gaia satellite to be launched in November 2013 will focus on high precision astrometry of stars and all objects down to limiting magnitude 20. The satellite will also provide photometric and spectral information and hence important inputs for various branches of astrophysics, including the study of GRBs and related optical afterglows (OAs) and optical transients (OTs). The strength of Gaia in GRB analyses will be the fine spectral resolution (spectro-photometry and ultra-low dispersion spectroscopy), which will allow the correct classication of related triggers. An interesting feature of Gaia BP and RP instruments will be the study of highly redshifted triggers. Similarly, the low dispersion spectroscopy provided by various plate surveys can also supply valuable data for investigations of high-energy sources. The ESA LOFT candidate mission, now in the assessment study phase, will also be able to detect and be used in the study of GRBs, with emphasis on low-energy (X-ray) emission

Název v anglickém jazyce

GRB INVESTIGATIONS BY ESA GAIA AND LOFT

Popis výsledku anglicky

The possibility of studying GRBs with the ESA Gaia and LOFT missions is briefly addressed. The ESA Gaia satellite to be launched in November 2013 will focus on high precision astrometry of stars and all objects down to limiting magnitude 20. The satellite will also provide photometric and spectral information and hence important inputs for various branches of astrophysics, including the study of GRBs and related optical afterglows (OAs) and optical transients (OTs). The strength of Gaia in GRB analyses will be the fine spectral resolution (spectro-photometry and ultra-low dispersion spectroscopy), which will allow the correct classication of related triggers. An interesting feature of Gaia BP and RP instruments will be the study of highly redshifted triggers. Similarly, the low dispersion spectroscopy provided by various plate surveys can also supply valuable data for investigations of high-energy sources. The ESA LOFT candidate mission, now in the assessment study phase, will also be able to detect and be used in the study of GRBs, with emphasis on low-energy (X-ray) emission

Druh

J_SC - Článek v periodiku v databázi SCOPUS

CEP obor

—

OECD FORD obor

20201 - Electrical and electronic engineering

Projekt

<a href="/cs/project/GA102%2F09%2F0997" target="_blank" >GA102/09/0997: Automatická detekce a obrazová analýza optické emise kosmických gama záblesků</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2013

Kód důvěrnosti údajů

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

Název periodika

Acta Polytechnica

ISSN

1210-2709

e-ISSN

1805-2363

Svazek periodika

53

Číslo periodika v rámci svazku

Supplement

Stát vydavatele periodika

CZ - Česká republika

Počet stran výsledku

4

Strana od-do

799-802

Kód UT WoS článku

000433673300059

EID výsledku v databázi Scopus

2-s2.0-84896860703