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000601184 088__ $$2arXiv$$aarXiv:2208.00159
000601184 1001_ $$0P:(DE-HGF)0$$aBen-Ami, Sagi$$b0$$eCorresponding author
000601184 1112_ $$aSpace Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray$$cMontréal$$d2022-07-17 - 2022-07-23$$wCanada
000601184 245__ $$aThe scientific payload of the Ultraviolet Transient Astronomy Satellite (ULTRASAT)
000601184 250__ $$aPart One of Two Parts
000601184 260__ $$aBellingham, Wash.$$bSPIE$$c2022
000601184 29510 $$aSpace Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray : [Proceedings] - SPIE, 2022. - ISBN 97815106534369781510653443 - doi:10.1117/12.2629850
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000601184 500__ $$aPresented in the SPIE Astronomical Telescopes + Instrumentation 2022
000601184 520__ $$aThe Ultraviolet Transient Astronomy Satellite (ULTRASAT) is a space-borne near UV telescope with an unprecedented large field of view (200 deg2 ). The mission, led by the Weizmann Institute of Science and the Israel Space Agency in collaboration with DESY (Helmholtz association, Germany) and NASA (USA), is fully funded and expected to be launched to a geostationary transfer orbit in Q2/Q3 of 2025. With a grasp 300 times larger than GALEX, the most sensitive UV satellite to date, ULTRASAT will revolutionize our understanding of the hot transient universe, as well as of flaring galactic sources. We describe the mission payload, the optical design and the choice of materials allowing us to achieve a point spread function of ∼ 10 arcsec across the FoV, and the detector assembly. We detail the mitigation techniques implemented to suppress out-of-band flux and reduce stray light, detector properties including measured quantum efficiency of scout (prototype) detectors, and expected performance (limiting magnitude) for various objects.
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000601184 7001_ $$aShvartzvald, Yossi$$b1
000601184 7001_ $$aWaxman, Eli$$b2
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000601184 7001_ $$aAlgranatti, Viktor M.$$b5
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000601184 7001_ $$aKüsters, Daniel$$b30
000601184 7001_ $$aLiran, Tuvia$$b31
000601184 7001_ $$aMiron-Salomon, Yonit$$b32
000601184 7001_ $$aMor, Zohar$$b33
000601184 7001_ $$aNir, Aharon$$b34
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000601184 7001_ $$0P:(DE-H253)PIP1017590$$aPorelli, Andrea$$b37$$udesy
000601184 7001_ $$aSagiv, Ilan$$b38
000601184 7001_ $$0P:(DE-H253)PIP1091245$$aSchliwinski, Julian$$b39
000601184 7001_ $$aSprecher, Tuvia$$b40
000601184 7001_ $$0P:(DE-H253)PIP1085659$$aDe Simone, Nicola$$b41$$udesy
000601184 7001_ $$aStern, Nir$$b42
000601184 7001_ $$aStone, Nicholas C.$$b43
000601184 7001_ $$aTrakhtenbrot, Benjamin$$b44
000601184 7001_ $$0P:(DE-H253)PIP1091983$$aVasilev, Mikhail$$b45$$udesy
000601184 7001_ $$0P:(DE-H253)PIP1091973$$aWatson, Jason J.$$b46$$udesy
000601184 7001_ $$0P:(DE-H253)PIP1087269$$aZappon, Francesco$$b47$$udesy
000601184 7001_ $$aden Herder, Jan-Willem A.$$b48$$eEditor
000601184 7001_ $$aNakazawa, Kazuhiro$$b49$$eEditor
000601184 7001_ $$aNikzad, Shouleh$$b50$$eEditor
000601184 773__ $$0PERI:(DE-600)2398361-9$$a10.1117/12.2629850$$p1218105$$tProceedings of SPIE$$v12181$$x0038-7355$$y2022
000601184 7870_ $$0PUBDB-2024-00195$$aBen-Ami, Sagi et.al.$$d2023$$iIsParent$$rarXiv:2208.00159$$tThe scientific payload of the Ultraviolet Transient Astronomy Satellite (ULTRASAT)
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