X-RED: A satellite mission concept to detect early universe gamma ray bursts
|Title:||X-RED: A satellite mission concept to detect early universe gamma ray bursts||Authors:||Krumpe, Mirko; Coffey, Deirdre; Egger, Georg; et al.||Permanent link:||http://hdl.handle.net/10197/11163||Date:||18-Aug-2005||Online since:||2019-10-18T15:45:04Z||Abstract:||Gamma ray bursts (GRBs) are the most energetic eruptions known in the Universe. Instruments such as Compton-GRO/BATSE and the GRB monitor on BeppoSAX have detected more than 2700 GRBs and, although observational confirmation is still required, it is now generally accepted that many of these bursts are associated with the collapse of rapidly spinning massive stars to form black holes. Consequently, since first generation stars are expected to be very massive, GRBs are likely to have occurred in significant numbers at early epochs. X-red is a space mission concept designed to detect these extremely high redshifted GRBs, in order to probe the nature of the first generation of stars and hence the time of reionisation of the early Universe. We demonstrate that the gamma and x-ray luminosities of typical GRBs render them detectable up to extremely high redshifts (z ∼ 10 to 30), but that current missions such as HETE2 and SWIFT operate outside the observational range for detection of high redshift GRB afterglows. Therefore, to redress this, we present a complete mission design from the science case to the mission architecture and payload, the latter comprising three instruments, namely wide field x-ray cameras to detect high redshift gamma-rays, an x-ray focussing telescope to determine accurate coordinates and extract spectra, and an infrared spectrograph to observe the high redshift optical afterglow. The mission is expected to detect and identify for the first time GRBs with z > 10, thereby providing constraints on properties of the first generation of stars and the history of the early Universe.||metadata.dc.description.othersponsorship:||European Space Agency
Deutsches Zentrum für Luft- und Raumfahrt
|Type of material:||Conference Publication||Publisher:||SPIE||Copyright (published version):||2005 Society of Photo-Optical Instrumentation Engineers (SPIE)||Keywords:||GRB; First generation stars; Space mission; Pop III||DOI:||10.1117/12.616601||Other versions:||http://www.spie.org/conferences/programs/05/am/||Language:||en||Status of Item:||Peer reviewed||Is part of:||Siegmund, O.H.W. (ed.). UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIV||Conference Details:||Optics and Photonics 2005, San Diego, California United States of America, 31 July - 4 August 2005|
|Appears in Collections:||Physics Research Collection|
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