Přehled o publikaci
2024
Science with a Small Two-Band UV-Photometry Mission I: Mission Description and Follow-up Observations of Stellar Transients
WERNER, Norbert; Jakub ŘÍPA; C. THÖNE; Filip MÜNZ; Petr KURFÜRST et. al.Basic information
Original name
Science with a Small Two-Band UV-Photometry Mission I: Mission Description and Follow-up Observations of Stellar Transients
Authors
WERNER, Norbert; Jakub ŘÍPA; C. THÖNE; Filip MÜNZ; Petr KURFÜRST; M. JELÍNEK; Filip HROCH; Jan BENÁČEK; M. TOPINKA; G. LUKES-GERAKOPOULOS; Michal ZAJAČEK; Matúš LABAJ; Michal PRIŠEGEN; Jiří KRTIČKA; J. MERC; A. PÁL; Ondřej PEJCHA; V. DÁNIEL; J. JON; R. ŠOŠOVIČKA; J. GROMEŠ; J. VÁCLAVÍK; L. STEIGER; J. SEGIŇÁK; E. BEHAR; S. TAREM; J. SALH; O. REICH; S. BEN-AMI; M. F. BARSCHKE; D. BERGE; A. TOHUVAVOHU; S. SIVANANDAM; M. BULLA; S. POPOV and Hsiang-Kuang CHANG
Edition
Space Science Reviews, Springer, 2024, 0038-6308
Other information
Language
English
Type of outcome
Article in a journal
Country of publisher
Netherlands
Confidentiality degree
is not subject to a state or trade secret
Organization
Přírodovědecká fakulta – Repository – Repository
UT WoS
001157109500002
EID Scopus
2-s2.0-85184246559
Keywords in English
UV space observatory; Kilonovae; Gamma-ray bursts; Supernovae
Changed: 12/4/2024 04:08, RNDr. Daniel Jakubík
Abstract
V originále
This is the first in a collection of three papers introducing the science with an ultra-violet (UV) space telescope on an approximately 130 kg small satellite with a moderately fast re-pointing capability and a real-time alert communication system approved 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.