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

L. Piro; L. Colasanti; G. Gandolfi; L. Pacciani; A. De Rosa; D. Hampai; E. Costa; M. Feroci; P. Soffitta; F. Gatti; D. Pergolesi; R. Vaccarone; M. Orio; A. Ferrari; E. Trussoni; D. McCammon; W. T. Sanders; F. S. Porter; R. L. Kelley; C. K. Stahle; E. Figueroa; A. Szymkowiak; M. Galeazzi

doi:10.1016/j.nima.2003.11.257

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

L. Piro, L. Colasanti^*, G. Gandolfi, L. Pacciani, A. De Rosa, D. Hampai, E. Costa, M. Feroci, P. Soffitta, F. Gatti, D. Pergolesi, R. Vaccarone, M. Orio, A. Ferrari, E. Trussoni, D. McCammon, W. T. Sanders, F. S. Porter, R. L. Kelley, C. K. StahleE. Figueroa, A. Szymkowiak, M. Galeazzi

^*Corresponding author for this work

Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

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.

Original language	English (US)
Pages (from-to)	376-378
Number of pages	3
Journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	520
Issue number	1-3
DOIs	https://doi.org/10.1016/j.nima.2003.11.257
State	Published - Mar 11 2004

Keywords

GRB
Microcalorimeters
WHIM

ASJC Scopus subject areas

Nuclear and High Energy Physics
Instrumentation

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10.1016/j.nima.2003.11.257

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Piro, L., Colasanti, L., Gandolfi, G., Pacciani, L., De Rosa, A., Hampai, D., Costa, E., Feroci, M., Soffitta, P., Gatti, F., Pergolesi, D., Vaccarone, R., Orio, M., Ferrari, A., Trussoni, E., McCammon, D., Sanders, W. T., Porter, F. S., Kelley, R. L., ... Galeazzi, M. (2004). X-ray survey with microcalorimeters: From GRB in the far universe to diffuse emission in our galaxy. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 520(1-3), 376-378. https://doi.org/10.1016/j.nima.2003.11.257

Piro, L. ; Colasanti, L. ; Gandolfi, G. ; Pacciani, L. ; De Rosa, A. ; Hampai, D. ; Costa, E. ; Feroci, M. ; Soffitta, P. ; Gatti, F. ; Pergolesi, D. ; Vaccarone, R. ; Orio, M. ; Ferrari, A. ; Trussoni, E. ; McCammon, D. ; Sanders, W. T. ; Porter, F. S. ; Kelley, R. L. ; Stahle, C. K. ; Figueroa, E. ; Szymkowiak, A. ; Galeazzi, M. / X-ray survey with microcalorimeters : From GRB in the far universe to diffuse emission in our galaxy. In: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2004 ; Vol. 520, No. 1-3. pp. 376-378.

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title = "X-ray survey with microcalorimeters: From GRB in the far universe to diffuse emission in our galaxy",

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.",

keywords = "GRB, Microcalorimeters, WHIM",

author = "L. Piro and L. Colasanti and G. Gandolfi and L. Pacciani and {De Rosa}, A. and D. Hampai and E. Costa and M. Feroci and P. Soffitta and F. Gatti and D. Pergolesi and R. Vaccarone and M. Orio and A. Ferrari and E. Trussoni and D. McCammon and Sanders, {W. T.} and Porter, {F. S.} and Kelley, {R. L.} and Stahle, {C. K.} and E. Figueroa and A. Szymkowiak and M. Galeazzi",

year = "2004",

month = mar,

day = "11",

doi = "10.1016/j.nima.2003.11.257",

language = "English (US)",

volume = "520",

pages = "376--378",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

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Piro, L, Colasanti, L, Gandolfi, G, Pacciani, L, De Rosa, A, Hampai, D, Costa, E, Feroci, M, Soffitta, P, Gatti, F, Pergolesi, D, Vaccarone, R, Orio, M, Ferrari, A, Trussoni, E, McCammon, D, Sanders, WT, Porter, FS, Kelley, RL, Stahle, CK, Figueroa, E, Szymkowiak, A & Galeazzi, M 2004, 'X-ray survey with microcalorimeters: From GRB in the far universe to diffuse emission in our galaxy', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 520, no. 1-3, pp. 376-378. https://doi.org/10.1016/j.nima.2003.11.257

X-ray survey with microcalorimeters : From GRB in the far universe to diffuse emission in our galaxy. / Piro, L.; Colasanti, L.; Gandolfi, G.; Pacciani, L.; De Rosa, A.; Hampai, D.; Costa, E.; Feroci, M.; Soffitta, P.; Gatti, F.; Pergolesi, D.; Vaccarone, R.; Orio, M.; Ferrari, A.; Trussoni, E.; McCammon, D.; Sanders, W. T.; Porter, F. S.; Kelley, R. L.; Stahle, C. K.; Figueroa, E.; Szymkowiak, A.; Galeazzi, M.

In: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol. 520, No. 1-3, 11.03.2004, p. 376-378.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

T1 - X-ray survey with microcalorimeters

T2 - From GRB in the far universe to diffuse emission in our galaxy

AU - Piro, L.

AU - Colasanti, L.

AU - Gandolfi, G.

AU - Pacciani, L.

AU - De Rosa, A.

AU - Hampai, D.

AU - Costa, E.

AU - Feroci, M.

AU - Soffitta, P.

AU - Gatti, F.

AU - Pergolesi, D.

AU - Vaccarone, R.

AU - Orio, M.

AU - Ferrari, A.

AU - Trussoni, E.

AU - McCammon, D.

AU - Sanders, W. T.

AU - Porter, F. S.

AU - Kelley, R. L.

AU - Stahle, C. K.

AU - Figueroa, E.

AU - Szymkowiak, A.

AU - Galeazzi, M.

PY - 2004/3/11

Y1 - 2004/3/11

N2 - 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.

AB - 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.

KW - GRB

KW - Microcalorimeters

KW - WHIM

UR - http://www.scopus.com/inward/record.url?scp=12144288451&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=12144288451&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2003.11.257

DO - 10.1016/j.nima.2003.11.257

M3 - Article

AN - SCOPUS:12144288451

VL - 520

SP - 376

EP - 378

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

SN - 0168-9002

IS - 1-3

ER -

Piro L, Colasanti L, Gandolfi G, Pacciani L, De Rosa A, Hampai D et al. X-ray survey with microcalorimeters: From GRB in the far universe to diffuse emission in our galaxy. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2004 Mar 11;520(1-3):376-378. https://doi.org/10.1016/j.nima.2003.11.257

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

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Keywords

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