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.
|Original language||English (US)|
|Number of pages||3|
|Journal||Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment|
|State||Published - Mar 11 2004|
ASJC Scopus subject areas
- Nuclear and High Energy Physics