X-ray survey with microcalorimeters: from GRB in the far universe to diffuse emission in our galaxy

Details X-ray survey with microcalorimeters: from GRB in the far universe to diffuse emission in our galaxy X-ray survey with microcalorimeters: from GRB in the far universe to diffuse emission in our galaxy

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004nimpa.520..376p&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 520, Issue 1-3, p. 376-378.

Physics

Microcalorimeters, Grb, Whim

Scientific paper

IMBOSS is an experiment based on X-ray microcalorimeters and aimed to perform a high spectral resolution all-sky survey. One of the primary scientific goals is the observation of the baryon ``missing'' matter at z<2. This is expected to be in the form of a warm-hot medium emitting in soft X-rays. We aim to detect and study the WHIM via X-ray emission lines. Another key goal is the detection of X-ray features in the prompt emission of GRBs, ultimately leading to a measurement of z for those class of GRBs still embedded in the mystery. Finally, a high-resolution spectroscopy survey will clarify the origin of the many components thought to make up the diffuse galactic X-ray emission.

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