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@ARTICLE{Werner:602690,
      author       = {Werner, N. and Řípa, J. and Thöne, C. and Münz, F. and
                      Kurfürst, P. and Jelínek, M. and Hroch, F. and Benáček,
                      J. and Topinka, M. and Lukes-Gerakopoulos, G. and Zajaček,
                      M. and Labaj, M. and Prišegen, M. and Krtička, J. and
                      Merc, J. and Pál, A. and Pejcha, O. and Dániel, V. and
                      Jon, J. and Šošovička, R. and Gromeš, J. and Václavík,
                      J. and Steiger, L. and Segiňák, J. and Behar, E. and
                      Tarem, S. and Salh, J. and Reich, O. and Ben-Ami, S. and
                      Barschke, M. F. and Berge, D. and Tohuvavohu, A. and
                      Sivanandam, S. and Bulla, M. and Popov, S. and Chang,
                      Hsiang-Kuang},
      title        = {{S}cience with a small two-band {UV}-photometry mission
                      {I}: {M}ission description and follow-up observations of
                      stellar transients},
      journal      = {Space science reviews},
      volume       = {220},
      number       = {1},
      issn         = {0038-6308},
      address      = {Dordrecht [u.a.]},
      publisher    = {Springer Science + Business Media B.V},
      reportid     = {PUBDB-2024-00736, arXiv:2306.15080},
      pages        = {11},
      year         = {2023},
      abstract     = {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.},
      keywords     = {UV space observatory (autogen) / Kilonovae (autogen) /
                      Gamma-ray bursts (autogen) / Supernovae (autogen)},
      cin          = {$Z_GA$},
      ddc          = {600},
      cid          = {$I:(DE-H253)Z_GA-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)ULTRASAT-20211201},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2306.15080},
      howpublished = {arXiv:2306.15080},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2306.15080;\%\%$},
      UT           = {WOS:001157109500002},
      doi          = {10.1007/s11214-024-01048-3},
      url          = {https://bib-pubdb1.desy.de/record/602690},
}