001     601183
005     20240218030232.0
024 7 _ |a arXiv:2306.15080
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2024-00155
|2 datacite_doi
037 _ _ |a PUBDB-2024-00155
041 _ _ |a English
088 _ _ |a arXiv:2306.15080
|2 arXiv
100 1 _ |a Werner, N.
|0 P:(DE-HGF)0
|b 0
|e Corresponding author
245 _ _ |a Science with a small two-band UV-photometry mission I: Mission description and follow-up observations of stellar transients
260 _ _ |c 2023
336 7 _ |a Preprint
|b preprint
|m preprint
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|s 1706517960_3228871
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336 7 _ |a WORKING_PAPER
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336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
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500 _ _ |a Submitted to Space Science Reviews
520 _ _ |a This is the first in a collection of three papers introducing the science with an ultra-violet (UV) space telescope on an approximately 100 kg small satellite with a moderately fast re-pointing capability and a real-time alert communication system that is being studied for a Czech national space mission. The mission, called Quick Ultra-Violet Kilonova surveyor - QUVIK, will provide key follow-up capabilities to increase the discovery potential of gravitational wave observatories and future wide-field multi-wavelength surveys. The primary objective of the mission is the measurement of the UV brightness evolution of kilonovae, resulting from mergers of neutron stars, to distinguish between different explosion scenarios. The mission, which is designed to be complementary to the Ultraviolet Transient Astronomy Satellite - ULTRASAT, will also provide unique follow-up capabilities for other transients both in the near- and far-UV bands. Between the observations of transients, the satellite will target other objects described in this collection of papers, which demonstrates that a small and relatively affordable dedicated UV-space telescope can be transformative for many fields of astrophysics.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
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588 _ _ |a Dataset connected to arXivarXiv
693 _ _ |0 EXP:(DE-H253)ULTRASAT-20211201
|5 EXP:(DE-H253)ULTRASAT-20211201
|e Ultraviolet Transient Astronomy Satellite
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700 1 _ |a Řípa, J.
|0 P:(DE-HGF)0
|b 1
|e Corresponding author
700 1 _ |a Thöne, C.
|b 2
700 1 _ |a Münz, F.
|b 3
700 1 _ |a Kurfürst, P.
|b 4
700 1 _ |a Jelínek, M.
|b 5
700 1 _ |a Hroch, F.
|b 6
700 1 _ |a Benáček, J.
|b 7
700 1 _ |a Topinka, M.
|b 8
700 1 _ |a Lukes-Gerakopoulos, G.
|b 9
700 1 _ |a Zajaček, M.
|b 10
700 1 _ |a Labaj, M.
|b 11
700 1 _ |a Prišegen, M.
|b 12
700 1 _ |a Krtička, J.
|b 13
700 1 _ |a Merc, J.
|b 14
700 1 _ |a Pál, A.
|0 P:(DE-HGF)0
|b 15
700 1 _ |a Pejcha, O.
|b 16
700 1 _ |a Dániel, V.
|b 17
700 1 _ |a Jon, J.
|b 18
700 1 _ |a Šošovička, R.
|b 19
700 1 _ |a Gromeš, J.
|b 20
700 1 _ |a Václavík, J.
|b 21
700 1 _ |a Steiger, L.
|0 P:(DE-HGF)0
|b 22
700 1 _ |a Segiňák, J.
|b 23
700 1 _ |a Behar, E.
|b 24
700 1 _ |a Tarem, S.
|b 25
700 1 _ |a Salh, J.
|b 26
700 1 _ |a Reich, O.
|0 P:(DE-HGF)0
|b 27
700 1 _ |a Ben-Ami, S.
|b 28
700 1 _ |a Barschke, M. F.
|0 P:(DE-H253)PIP1091899
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|u desy
700 1 _ |a Berge, D.
|0 P:(DE-H253)PIP1080570
|b 30
|u desy
700 1 _ |a Tohuvavohu, A.
|b 31
700 1 _ |a Sivanandam, S.
|b 32
700 1 _ |a Bulla, M.
|b 33
700 1 _ |a Popov, S.
|b 34
700 1 _ |a Chang, Hsiang-Kuang
|b 35
856 4 _ |u https://arxiv.org/abs/2306.15080
856 4 _ |u https://bib-pubdb1.desy.de/record/601183/files/VfJEJk-2306.15080.pdf
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910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
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910 1 _ |a Deutsches Elektronen-Synchrotron
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913 1 _ |a DE-HGF
|b Forschungsbereich Materie
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914 1 _ |y 2023
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915 _ _ |a Creative Commons Attribution-ShareAlike CC BY-SA 4.0
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915 _ _ |a Published
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920 1 _ |0 I:(DE-H253)Z_GA-20210408
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980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a I:(DE-H253)Z_GA-20210408
980 _ _ |a UNRESTRICTED
980 1 _ |a FullTexts


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