The scientific payload of the Ultraviolet Transient Astronomy Satellite (ULTRASAT)

The Ultraviolet Transient Astronomy Satellite (ULTRASAT) is a space-borne near UV telescope with an unprecedented large field of view (200 sq. deg.). The mission, led by the Weizmann Institute of Science and the Israel Space Agency in collaboration with DESY (Helmholtz association, Germany) and NASA...

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Bibliographic Details
Published in:arXiv.org 2023-03
Main Authors: Ben-Ami, Sagi, Shvartzvald, Yossi, Waxman, Eli, Netzer, Udi, Yaniv, Yoram, Algranatti, Viktor M, Gal-Yam, Avishay, Lapid, Ofer, Ofek, Eran, Topaz, Jeremy, Arcavi, Iair, Arooj Asif, Azaria, Shlomi, Bahalul, Eran, Barschke, Merlin F, Bastian-Querner, Benjamin, Berge, David, Berlea, Vlad D, Buhler, Rolf, Dittmar, Louise, Gelman, Anatoly, Giavitto, Gianluca, Guttman, Or, Haces Crespo, Juan M, Heilbrunn, Daniel, Kachergincky, Arik, Kaipachery, Nirmal, Kowalski, Marek, Kulkarni, Shrinivasrao R, Kumar, Shashank, Kusters, Daniel, Tuvia Liran, Miron-Salomon, Yonit, Mor, Zohar, Nir, Aharon, Nitzan, Gadi, Philipp, Sebastian, Porelli, Andrea, Sagiv, Ilan, Schliwinski, Julian, Sprecher, Tuvia, De Simone, Nicola, Stern, Nir, Stone, Nicholas C, Trakhtenbrot, Benny, Vasilev, Mikhail, Watson, Jason J, Zappon, Francesco
Format: Article
Language:English
Subjects:
Object recognition
Optical design
Point spread functions
Quantum efficiency
Transfer orbits
Ultraviolet astronomy
Online Access:Get full text
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Summary:The Ultraviolet Transient Astronomy Satellite (ULTRASAT) is a space-borne near UV telescope with an unprecedented large field of view (200 sq. deg.). 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 Q2/3 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 ~10arcsec 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.
ISSN:2331-8422