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High-resolution X-ray spectroscopy with microcalorimeters L. Piro

High-resolution X-ray spectroscopy with microcalorimeters L. Piro. Some key scientific drivers: GRB engine and progenitors: X-ray lines and absorption features Outflowing plasmas in the Galaxy and the boundary with the local cluster X-Ray Cosmology: GRB and WHIM (Cosmology section).

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High-resolution X-ray spectroscopy with microcalorimeters L. Piro

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  1. High-resolution X-ray spectroscopy with microcalorimetersL. Piro • Some key scientific drivers: • GRB engine and progenitors: X-ray lines and absorption features • Outflowing plasmas in the Galaxy and the boundary with the local cluster • X-Ray Cosmology: GRB and WHIM (Cosmology section)

  2. X-ray Iron features in GRB • GB970508 (Piro et al 1999) • GB000214 (Antonelli et al 2000) • GB991216 (Piro et al 2000) • GB990705 (Amati et al 2000) • GB980828 (Yoshida et al 1999)

  3. Study of local and intergalactic medium in primeval galaxies with GRB with XEUS • Study of the metallicity of the ISM of a host galaxy of a GRB at z=5 through X-ray edges • The Fe line in a GRB like GB970508 but at z=5

  4. TES Al-Ag multi-layer High purity Si glued on a Sn absorber Electro – thermal links to the heat bath Polycrystalline Sn energy absorber TES (Transition Edge Sensor) microcalorimeters We are developing, in collaboration with Genova University, TES devices with the goal of conforming to XEUS specs First single pixel prototype already working with DE=16 eV at 6 keV, we are now improved tecniques and are confident to achieve the target DE=4 eV in the next year Multi-pixel prototype design under development

  5. TES microcalorimeter program • TES microcalorimeters are the next generation X-ray spectroscopy devices, and have been selected as focal plane instruments for ambitious astrophysical missions like XEUS (ESA) and Con-X (NASA). Groups developing these devices are NASA/Goddard, Wisconsin Uni. , NIST, SRON. • We have set up a collaboration with Genova University, that has built up a longstanding experience on micro-calorimeters for basic physics applications. After the realization and test of a first prototype of TES detector, we have realized a 2nd batch (currently under testing) and foresee to achieve in 1 year a 4-5 eV resolution @ 6 keV. We have already started the design of a prototype of a position sensitive detector, that we plan to realize in 2 years (pending funds availability) • The final goal is to identify the techniques for the realization of a detector to the XEUS requirements. • Manpower: IASF(Roma) 3 research staff, 1 phd student, 3 technicians: manpower for 2002: 25 men-months; Universita Genova: 2 research staff, 4 phd/fellows, 2 technicians: 42 man-months in 2002. Similar manpower in 2003. • Most of the activities are currently carried out with INFN and EU funds devoted to basic physics applications. In order to develop detectors compliant to the astrophysical requirements we estimate a budget of about 1000 keuro in 3 years. Proposals to support this activity are and will be submitted to ASI, EU, CNR, MIUR.

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