Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-27T07:35:45.388Z Has data issue: false hasContentIssue false
  • English
  • Français

GRBs and Lobster Eye X-Ray Telescopes

Published online by Cambridge University Press:  22 July 2013

R. Hudec ,
L. Pina ,
V. Marsikova  and
A. Inneman
R. Hudec
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, 251 65 Ondřejov, Czech Republic Czech Technical University in Prague, Faculty of Electrical Engineering, Prague, Czech Republic
L. Pina
Affiliation:
Czech Technical University in Prague, Faculty of Nuclear Science, Prague, Czech Republic
V. Marsikova
Affiliation:
Rigaku Innovative Techniologies Europe, Prague, Czech Republic
A. Inneman
Affiliation:
Rigaku Innovative Techniologies Europe, Prague, Czech Republic
Get access

Abstract

A large majority of GRBs exhibit X-ray emission. In addition, a dedicated separate groupof GRB, the XRFs, exists which emission dominates in the X-ray spectral range. And thethird group of GRB related objects (yet hypothetical) are the group of off-axis observedGRBs (orphan afterglows). These facts justify the consideration of an independentexperiment for monitoring, detection and analyses of GRBs and others fast X-ray transientsin X-rays. We will present and discuss such experiment based on wide-field X-raytelescopes of Lobster Eye type. We show that the wide field and fine sensitivity ofLobster Eye X-ray All-Sky Monitor make such instruments important tools in study ofGRBs.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 61: Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe , 2013 , pp. 611 - 615
Copyright
© EAS, EDP Sciences 2013

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Amati, L., Frontera, F., in’t Zand, J.J.M., et al., 2004, A&A, 426, 415
Angel, J.R.P., 1979, ApJ, 364, 233
De Pasquale, M., Piro, L., Perna, R., et al., 2003, ApJ, 592, 1018 CrossRef
Fraser, G.W., Brunton, A.N., Bannister, N.P., et al., 2002, Proc. SPIE, 4497, 115 CrossRef
Frontera, F., Amati, L., in ’t Zand, J.J.M., et al., 2004, ApJ, 616, 1078 CrossRef
Gorenstein, P., 1998, Proc. SPIE, 3444, 382 CrossRef
Inneman, A., Hudec, R., & Pina, L., 2000, Proc. SPIE, 4138, 94 CrossRef
Inneman, A., Hudec, R., Pina, L., et al., 1999, Proc. SPIE, 3766, 72 CrossRef
Priedhorsky, W.C., Peele, A.G., & Nugent, K.A., 1996, MNRAS, 279, 733 CrossRef
Schmidt, W.K.H., 1975, Nucl. Instr. Meth., 127, 285 CrossRef
Sveda, L., Hudec, R., Pina, L., et al., 2005, in Cosmic Explosions, Springer Proceedings in Physics, Vol. 99, ed. J.M. Marcaide & K.W. Weiler, 197
Sveda, L., Hudec, R., Pina, L., et al., 2009, in EUV and X-Ray Optics: Synergy between Laboratory and Space, ed. R. Hudec & L. Pina, Proceedings of the SPIE, Vol. 7360, p. 73600F, 10
Tichy, V., Sveda, L., Marsik, J., et al., 2009a, Baltic Astron., 18, 369
Tichy, V., Hromcik, M., Hudec, R., et al., 2009b, Baltic Astron., 18, 362
Tichy, V., Barbera, M., Collura, A., et al., 2011, Nucl. Instr. Meth. Phys. Res. A, 633, id. 169