J 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 (703 Slovakia, guarantor, belonging to the institution), Jakub ŘÍPA (203 Czech Republic, belonging to the institution), C. THÖNE, Filip MÜNZ (203 Czech Republic, belonging to the institution), Petr KURFÜRST (203 Czech Republic, belonging to the institution), M. JELÍNEK, Filip HROCH (203 Czech Republic, belonging to the institution), Jan BENÁČEK (203 Czech Republic), M. TOPINKA, G. LUKES-GERAKOPOULOS, Michal ZAJAČEK (703 Slovakia, belonging to the institution), Matúš LABAJ (703 Slovakia, belonging to the institution), Michal PRIŠEGEN (703 Slovakia, belonging to the institution), Jiří KRTIČKA (203 Czech Republic, belonging to the institution), J. MERC, A. PÁL, Ondřej PEJCHA (203 Czech Republic), 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

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

Netherlands

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

Impact factor

Impact factor: 10.300 in 2022

Organization unit

Faculty of Science

UT WoS

001157109500002

Keywords in English

UV space observatory; Kilonovae; Gamma-ray bursts; Supernovae

Tags

Tags

International impact, Reviewed
Změněno: 11/4/2024 10:24, Mgr. Marie Šípková, DiS.

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.

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