Author/Authors :
Piro، نويسنده , , L. and Colasanti، نويسنده , , L. and Gandolfi، نويسنده , , G. and Pacciani، نويسنده , , L. and De Rosa، نويسنده , , A. and Hampai، نويسنده , , D. and Costa، نويسنده , , E. and Feroci، نويسنده , , M. and Soffitta، نويسنده , , P. and Gatti، نويسنده , , F. and Pergolesi، نويسنده , , D. and Vaccarone، نويسنده , , R. and Orio، نويسنده , , M. and Ferrari، نويسنده , , A. and Trussoni، نويسنده , , E. and McCammon، نويسنده , , D. and Sanders، نويسنده , , W.T. and Porter، نويسنده , , F.S. and Kelley، نويسنده , , R.L. and Stahle، نويسنده , , C.K. and Figueroa، نويسنده , , E. and Szymkowiak، نويسنده , , A. and Galeazzi، نويسنده , , M.، نويسنده ,
Abstract :
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.
