000601183 001__ 601183
000601183 005__ 20240218030232.0
000601183 0247_ $$2arXiv$$aarXiv:2306.15080
000601183 0247_ $$2datacite_doi$$a10.3204/PUBDB-2024-00155
000601183 037__ $$aPUBDB-2024-00155
000601183 041__ $$aEnglish
000601183 088__ $$2arXiv$$aarXiv:2306.15080
000601183 1001_ $$0P:(DE-HGF)0$$aWerner, N.$$b0$$eCorresponding author
000601183 245__ $$aScience with a small two-band UV-photometry mission I: Mission description and follow-up observations of stellar transients
000601183 260__ $$c2023
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000601183 500__ $$aSubmitted to Space Science Reviews
000601183 520__ $$aThis 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.
000601183 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000601183 588__ $$aDataset connected to arXivarXiv
000601183 693__ $$0EXP:(DE-H253)ULTRASAT-20211201$$5EXP:(DE-H253)ULTRASAT-20211201$$eUltraviolet Transient Astronomy Satellite$$x0
000601183 7001_ $$0P:(DE-HGF)0$$aŘípa, J.$$b1$$eCorresponding author
000601183 7001_ $$aThöne, C.$$b2
000601183 7001_ $$aMünz, F.$$b3
000601183 7001_ $$aKurfürst, P.$$b4
000601183 7001_ $$aJelínek, M.$$b5
000601183 7001_ $$aHroch, F.$$b6
000601183 7001_ $$aBenáček, J.$$b7
000601183 7001_ $$aTopinka, M.$$b8
000601183 7001_ $$aLukes-Gerakopoulos, G.$$b9
000601183 7001_ $$aZajaček, M.$$b10
000601183 7001_ $$aLabaj, M.$$b11
000601183 7001_ $$aPrišegen, M.$$b12
000601183 7001_ $$aKrtička, J.$$b13
000601183 7001_ $$aMerc, J.$$b14
000601183 7001_ $$0P:(DE-HGF)0$$aPál, A.$$b15
000601183 7001_ $$aPejcha, O.$$b16
000601183 7001_ $$aDániel, V.$$b17
000601183 7001_ $$aJon, J.$$b18
000601183 7001_ $$aŠošovička, R.$$b19
000601183 7001_ $$aGromeš, J.$$b20
000601183 7001_ $$aVáclavík, J.$$b21
000601183 7001_ $$0P:(DE-HGF)0$$aSteiger, L.$$b22
000601183 7001_ $$aSegiňák, J.$$b23
000601183 7001_ $$aBehar, E.$$b24
000601183 7001_ $$aTarem, S.$$b25
000601183 7001_ $$aSalh, J.$$b26
000601183 7001_ $$0P:(DE-HGF)0$$aReich, O.$$b27
000601183 7001_ $$aBen-Ami, S.$$b28
000601183 7001_ $$0P:(DE-H253)PIP1091899$$aBarschke, M. F.$$b29$$udesy
000601183 7001_ $$0P:(DE-H253)PIP1080570$$aBerge, D.$$b30$$udesy
000601183 7001_ $$aTohuvavohu, A.$$b31
000601183 7001_ $$aSivanandam, S.$$b32
000601183 7001_ $$aBulla, M.$$b33
000601183 7001_ $$aPopov, S.$$b34
000601183 7001_ $$aChang, Hsiang-Kuang$$b35
000601183 8564_ $$uhttps://arxiv.org/abs/2306.15080
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000601183 9141_ $$y2023
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