Final performances of the X-ray Mirrors of the JET-X telescope

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dc.creatorPoretti, E.
dc.creatorCampana, S.
dc.creatorCitterio, O.
dc.creatorConconi, P.
dc.creatorGhigo, M.
dc.creatorMazzoleni, F.
dc.creatorTagliaferri, G.
dc.creatorCusumano, G.
dc.creatorLa Rosa, G.
dc.creatorBrauninger, W.
dc.creatorBurkert, W.
dc.creatorCastelli, C. M.
dc.creatorWillingale, R.
dc.date1997-11-04
dc.date.accessioned2026-07-07T02:24:55Z
dc.date.available2026-07-07T02:24:55Z
dc.descriptionThe Joint European Telesscope (JET-X) is one of the core scientific instruments of the SPECTRUM-X-Gamma mission. JET-X was designed to study X-ray emissions in the band 0.3-10 KeV. Its angular resolution is better than 20 arcsec; the values of the effective areas are 161 cm2 at 1.5 KeV and 69 cm2 at 8 Kev (for one telescope). The value of the HEW circle in function of the off-axis angle is presented; it is found to be below 20 arcsec at 1.5 Kev and around 23 arcsec at 8 KeV up to an off-axis angle of 12 arcmin.
dc.description2 pages, 1 ps figure. To be published in the Proceedings of the IAU Symposium 188 THE HOT UNIVERSE, held in Kyoto (August 26-30, 1997) in occasion of the XXIII IAU General Assembly
dc.identifierhttps://arxiv.org/abs/astro-ph/9711027
dc.identifierhttp://arxiv.org/abs/astro-ph/9711027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11739
dc.subjectAstrophysics
dc.titleFinal performances of the X-ray Mirrors of the JET-X telescope
dc.typetext

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