3 October 2007 EDGE: explorer of diffuse emission and gamma-ray burst explosions
Author Affiliations +
Abstract
How structures of various scales formed and evolved from the early Universe up to present time is a fundamental question of astrophysics. EDGE will trace the cosmic history of the baryons from the early generations of massive stars by Gamma-Ray Burst (GRB) explosions, through the period of galaxy cluster formation, down to the very low redshift Universe, when between a third and one half of the baryons are expected to reside in cosmic filaments undergoing gravitational collapse by dark matter (the so-called warm hot intragalactic medium). In addition EDGE, with its unprecedented capabilities, will provide key results in many important fields. These scientific goals are feasible with a medium class mission using existing technology combined with innovative instrumental and observational capabilities by: (a) observing with fast reaction Gamma-Ray Bursts with a high spectral resolution (R ~ 500). This enables the study of their (star-forming) environment and the use of GRBs as back lights of large scale cosmological structures; (b) observing and surveying extended sources (galaxy clusters, WHIM) with high sensitivity using two wide field of view X-ray telescopes (one with a high angular resolution and the other with a high spectral resolution). The mission concept includes four main instruments: a Wide-field Spectrometer with excellent energy resolution (3 eV at 0.6 keV), a Wide- Field Imager with high angular resolution (HPD 15") constant over the full 1.4 degree field of view, and a Wide Field Monitor with a FOV of 1/4 of the sky, which will trigger the fast repointing to the GRB. Extension of its energy response up to 1 MeV will be achieved with a GRB detector with no imaging capability. This mission is proposed to ESA as part of the Cosmic Vision call. We will briefly review the science drivers and describe in more detail the payload of this mission.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. W. den Herder, J. W. den Herder, L. Piro, L. Piro, T. Ohashi, T. Ohashi, L. Amati, L. Amati, J. Atteia, J. Atteia, S. Barthelmy, S. Barthelmy, M. Barbera, M. Barbera, D. Barret, D. Barret, S. Basso, S. Basso, M. Boer, M. Boer, S. Borgani, S. Borgani, O. Boyarskiy, O. Boyarskiy, E. Branchini, E. Branchini, G. Branduardi-Raymont, G. Branduardi-Raymont, M. Briggs, M. Briggs, G. Brunetti, G. Brunetti, C. Budtz-Jorgensenf, C. Budtz-Jorgensenf, D. Burrows, D. Burrows, S. Campana, S. Campana, E. Caroli, E. Caroli, G. Chincarini, G. Chincarini, F. Christensen, F. Christensen, M. Cocchi, M. Cocchi, A. Comastri, A. Comastri, A. Corsi, A. Corsi, V. Cotroneo, V. Cotroneo, P. Conconi, P. Conconi, L. Colasanti, L. Colasanti, G. Cusamano, G. Cusamano, A. de Rosa, A. de Rosa, M. Del Santo, M. Del Santo, S. Ettori, S. Ettori, Y. Ezoe, Y. Ezoe, L. Ferrari, L. Ferrari, M. Feroci, M. Feroci, M. Finger, M. Finger, G. Fishman, G. Fishman, R. Fujimoto, R. Fujimoto, M. Galeazzi, M. Galeazzi, A. Galli, A. Galli, F. Gatti, F. Gatti, N. Gehrels, N. Gehrels, B. Gendre, B. Gendre, G. Ghirlanda, G. Ghirlanda, G. Ghisellini, G. Ghisellini, P. Giommi, P. Giommi, M. Girardi, M. Girardi, L. Guzzo, L. Guzzo, F. Haardt, F. Haardt, I. Hepburn, I. Hepburn, W. Hermsen, W. Hermsen, H. Hoevers, H. Hoevers, A. Holland, A. Holland, J. In't Zand, J. In't Zand, Y. Ishisaki, Y. Ishisaki, H. Kawahara, H. Kawahara, N. Kawai, N. Kawai, J. Kaastra, J. Kaastra, M. Kippen, M. Kippen, P. A. J. de Korte, P. A. J. de Korte, C. Kouveliotou, C. Kouveliotou, A. Kusenko, A. Kusenko, C. Labanti, C. Labanti, R. Lieu, R. Lieu, C. Macculi, C. Macculi, K. Makishima, K. Makishima, G. Matt, G. Matt, P. Mazotta, P. Mazotta, D. McCammon, D. McCammon, M. Méndez, M. Méndez, T. Mineo, T. Mineo, S. Mitchell, S. Mitchell, K. Mitsuda, K. Mitsuda, S. Molendi, S. Molendi, L. Moscardini, L. Moscardini, R. Mushotzky, R. Mushotzky, L. Natalucci, L. Natalucci, F. Nicastro, F. Nicastro, P. O'Brien, P. O'Brien, J. Osborne, J. Osborne, F. Paerels, F. Paerels, M. Page, M. Page, S. Paltani, S. Paltani, G. Pareschi, G. Pareschi, E. Perinati, E. Perinati, C. Perola, C. Perola, T. Ponman, T. Ponman, A. Rasmussen, A. Rasmussen, M. Roncarelli, M. Roncarelli, P. Rosati, P. Rosati, O. Ruchayskiy, O. Ruchayskiy, E. Quadrini, E. Quadrini, I. Sakurai, I. Sakurai, R. Salvaterra, R. Salvaterra, S. Sasaki, S. Sasaki, G. Sato, G. Sato, J. Schaye, J. Schaye, J. Schmidtt, J. Schmidtt, S. Scioritino, S. Scioritino, M. Shaposhnikov, M. Shaposhnikov, K. Shinozaki, K. Shinozaki, D. Spiga, D. Spiga, Y. Suto, Y. Suto, G. Tagliaferri, G. Tagliaferri, T. Takahashi, T. Takahashi, Y. Takei, Y. Takei, Y. Tawara, Y. Tawara, P. Tozzi, P. Tozzi, H. Tsunemi, H. Tsunemi, T. Tsuru, T. Tsuru, P. Ubertini, P. Ubertini, E. Ursino, E. Ursino, M. Viel, M. Viel, J. Vink, J. Vink, N. White, N. White, R. Willingale, R. Willingale, R. Wijers, R. Wijers, K. Yoshikawa, K. Yoshikawa, N. Yamasaki, N. Yamasaki, } "EDGE: explorer of diffuse emission and gamma-ray burst explosions", Proc. SPIE 6688, Optics for EUV, X-Ray, and Gamma-Ray Astronomy III, 668805 (3 October 2007); doi: 10.1117/12.729457; https://doi.org/10.1117/12.729457
PROCEEDINGS
13 PAGES


SHARE
RELATED CONTENT

Xenia: cosmo-chemical evolution of the Universe
Proceedings of SPIE (July 29 2010)
The status of the Constellation-X mission
Proceedings of SPIE (September 17 2007)
X-ray astronomy with ultra-high-angular resolution
Proceedings of SPIE (October 10 2004)
NEW a mission to explore the warm hot intergalactic...
Proceedings of SPIE (June 12 2006)
Science with Generation-X
Proceedings of SPIE (July 14 2008)

Back to Top