Calibration of the XRT-SOLARB flat mirror samples at the XACT Facility of INAF-OAPA

Marco Barbera; Giovanni Peres; Leon Golub; null Weber; null Golub; null Varisco; null Cosmo; null Artale; null Cheimets; null De Luca; null Collura; null Bookbinder; null Barbera; Giovanni Peres; null Di Cicca

Calibration of the XRT-SOLARB flat mirror samples at the XACT Facility of INAF-OAPA

Marco Barbera, Giovanni Peres, Leon Golub, Weber, Golub, Varisco, Cosmo, Artale, Cheimets, De Luca, Collura, Bookbinder, Barbera, Giovanni Peres, Di Cicca

Fisica e Chimica - Emilio Segrè

Risultato della ricerca: Other › peer review

3 Citazioni (Scopus)

Abstract

The X-Ray Telescope (XRT) experiment on-board the Japanese satellite SOLAR-B (launch in 2006) is equipped with amodified Wolter I grazing incidence X-ray telescope (focal length 2700 mm) to image the full Sun at ~ 1.5" angularresolution onto a 2048 x 2048 back illuminated CCD focal plane detector. The X-ray telescope consisting of one singlereflecting shell is coated with ion beam sputtered Iridium over a binding layer of Chromium to provide nearly 5 squarecentimetres effective area at 60 Å. We present preliminary results of X-ray calibrations of the XRT flat mirror samplesperformed at the X-ray Astronomy Calibration and Testing (XACT) facility of INAF-OAPA. We describe theinstrumental set-up, the adopted measurement technique, and present the measured reflectivity vs. angle of incidence atfew energies.

Lingua originale	English
Pagine	440-448
Numero di pagine	9
Stato di pubblicazione	Published - 2004

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

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@conference{e5a89aaffe7b409990c841b46cbdd93d,

title = "Calibration of the XRT-SOLARB flat mirror samples at the XACT Facility of INAF-OAPA",

abstract = "The X-Ray Telescope (XRT) experiment on-board the Japanese satellite SOLAR-B (launch in 2006) is equipped with amodified Wolter I grazing incidence X-ray telescope (focal length 2700 mm) to image the full Sun at ~ 1.5{"} angularresolution onto a 2048 x 2048 back illuminated CCD focal plane detector. The X-ray telescope consisting of one singlereflecting shell is coated with ion beam sputtered Iridium over a binding layer of Chromium to provide nearly 5 squarecentimetres effective area at 60 {\AA}. We present preliminary results of X-ray calibrations of the XRT flat mirror samplesperformed at the X-ray Astronomy Calibration and Testing (XACT) facility of INAF-OAPA. We describe theinstrumental set-up, the adopted measurement technique, and present the measured reflectivity vs. angle of incidence atfew energies.",

keywords = "Calibration, Grazing incidence optics, Instrumentation, X-ray Astronomy, Calibration, Grazing incidence optics, Instrumentation, X-ray Astronomy",

author = "Marco Barbera and Giovanni Peres and Leon Golub and Weber and Golub and Varisco and Cosmo and Artale and Cheimets and {De Luca} and Collura and Bookbinder and Barbera and Giovanni Peres and {Di Cicca}",

year = "2004",

language = "English",

pages = "440--448",

}

TY - CONF

T1 - Calibration of the XRT-SOLARB flat mirror samples at the XACT Facility of INAF-OAPA

AU - Barbera, Marco

AU - Peres, Giovanni

AU - Golub, Leon

AU - Weber, null

AU - Golub, null

AU - Varisco, null

AU - Cosmo, null

AU - Artale, null

AU - Cheimets, null

AU - De Luca, null

AU - Collura, null

AU - Bookbinder, null

AU - Barbera, null

AU - Peres, Giovanni

AU - Di Cicca, null

PY - 2004

Y1 - 2004

N2 - The X-Ray Telescope (XRT) experiment on-board the Japanese satellite SOLAR-B (launch in 2006) is equipped with amodified Wolter I grazing incidence X-ray telescope (focal length 2700 mm) to image the full Sun at ~ 1.5" angularresolution onto a 2048 x 2048 back illuminated CCD focal plane detector. The X-ray telescope consisting of one singlereflecting shell is coated with ion beam sputtered Iridium over a binding layer of Chromium to provide nearly 5 squarecentimetres effective area at 60 Å. We present preliminary results of X-ray calibrations of the XRT flat mirror samplesperformed at the X-ray Astronomy Calibration and Testing (XACT) facility of INAF-OAPA. We describe theinstrumental set-up, the adopted measurement technique, and present the measured reflectivity vs. angle of incidence atfew energies.

AB - The X-Ray Telescope (XRT) experiment on-board the Japanese satellite SOLAR-B (launch in 2006) is equipped with amodified Wolter I grazing incidence X-ray telescope (focal length 2700 mm) to image the full Sun at ~ 1.5" angularresolution onto a 2048 x 2048 back illuminated CCD focal plane detector. The X-ray telescope consisting of one singlereflecting shell is coated with ion beam sputtered Iridium over a binding layer of Chromium to provide nearly 5 squarecentimetres effective area at 60 Å. We present preliminary results of X-ray calibrations of the XRT flat mirror samplesperformed at the X-ray Astronomy Calibration and Testing (XACT) facility of INAF-OAPA. We describe theinstrumental set-up, the adopted measurement technique, and present the measured reflectivity vs. angle of incidence atfew energies.

KW - Calibration

KW - Grazing incidence optics

KW - Instrumentation

KW - X-ray Astronomy

KW - Calibration

KW - Grazing incidence optics

KW - Instrumentation

KW - X-ray Astronomy

UR - http://hdl.handle.net/10447/30222

M3 - Other

SP - 440

EP - 448

ER -