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- W3157560264 abstract "Abstract The coming decades will establish the exploration of the gravitational wave (GW) Universe over a broad frequency range by ground and space interferometers. Meanwhile, wide-field, high-cadence and sensitive surveys will span the electromagnetic spectrum from radio all the way up to TeV, as well as the high-energy neutrino window. Among the numerous classes of transients, γ –ray bursts (GRBs) have direct links with most of the hot topics that will be addressed, such as the strong gravity regime, relativistic shocks, particle acceleration processes, equation of state of matter at nuclear density, and nucleosynthesis of heavy elements, just to mention a few. Other recently discovered classes of transients that are observed throughout cosmological distances include fast radio bursts (FRBs), fast blue optical transients (FBOTs), and other unidentified high-energy transients. Here we discuss how these topics can be addressed by a mission called ASTENA (Advanced Surveyor of Transient Events and Nuclear Astrophysics, see Frontera et al. 18). Its payload combines two instruments: (i) an array of wide-field monitors with imaging, spectroscopic, and polarimetric capabilities (WFM-IS); (ii) a narrow field telescope (NFT) based on a Laue lens operating in the 50–600 keV range with unprecedented angular resolution, polarimetric capabilities, and sensitivity." @default.
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- W3157560264 date "2021-04-23" @default.
- W3157560264 modified "2023-10-14" @default.
- W3157560264 title "A deep study of the high–energy transient sky" @default.
- W3157560264 cites W1604181701 @default.
- W3157560264 cites W1671599381 @default.
- W3157560264 cites W1687099926 @default.
- W3157560264 cites W1800321366 @default.
- W3157560264 cites W1870452575 @default.
- W3157560264 cites W1896972225 @default.
- W3157560264 cites W1919092116 @default.
- W3157560264 cites W1926824859 @default.
- W3157560264 cites W1964094621 @default.
- W3157560264 cites W1969193795 @default.
- W3157560264 cites W1993926965 @default.
- W3157560264 cites W1999369474 @default.
- W3157560264 cites W2007462702 @default.
- W3157560264 cites W2019058521 @default.
- W3157560264 cites W2029058495 @default.
- W3157560264 cites W2036423640 @default.
- W3157560264 cites W2053831110 @default.
- W3157560264 cites W2054582333 @default.
- W3157560264 cites W2060428341 @default.
- W3157560264 cites W2085754661 @default.
- W3157560264 cites W2086090890 @default.
- W3157560264 cites W2088506860 @default.
- W3157560264 cites W2090351667 @default.
- W3157560264 cites W2091106378 @default.
- W3157560264 cites W2110750342 @default.
- W3157560264 cites W2119844661 @default.
- W3157560264 cites W2136034398 @default.
- W3157560264 cites W2142983177 @default.
- W3157560264 cites W2264947362 @default.
- W3157560264 cites W2266746071 @default.
- W3157560264 cites W2287311144 @default.
- W3157560264 cites W2289905436 @default.
- W3157560264 cites W2414784202 @default.
- W3157560264 cites W2535836947 @default.
- W3157560264 cites W2554258215 @default.
- W3157560264 cites W2563744641 @default.
- W3157560264 cites W2571196594 @default.
- W3157560264 cites W2588788050 @default.
- W3157560264 cites W2609092435 @default.
- W3157560264 cites W272492758 @default.
- W3157560264 cites W2736990389 @default.
- W3157560264 cites W2766627241 @default.
- W3157560264 cites W2789384355 @default.
- W3157560264 cites W2887659426 @default.
- W3157560264 cites W2913685602 @default.
- W3157560264 cites W2945676005 @default.
- W3157560264 cites W2951253092 @default.
- W3157560264 cites W2955902629 @default.
- W3157560264 cites W2963005990 @default.
- W3157560264 cites W2996986362 @default.
- W3157560264 cites W3098099874 @default.
- W3157560264 cites W3098235040 @default.
- W3157560264 cites W3098898103 @default.
- W3157560264 cites W3099600050 @default.
- W3157560264 cites W3100115589 @default.
- W3157560264 cites W3100453682 @default.
- W3157560264 cites W3100494927 @default.
- W3157560264 cites W3101193009 @default.
- W3157560264 cites W3101536471 @default.
- W3157560264 cites W3101677407 @default.
- W3157560264 cites W3101879206 @default.
- W3157560264 cites W3102009706 @default.
- W3157560264 cites W3102074216 @default.