000079565 001__ 79565
000079565 005__ 20200117212654.0
000079565 0247_ $$2doi$$a10.1093/mnras/sty2541
000079565 0248_ $$2sideral$$a108644
000079565 037__ $$aART-2018-108644
000079565 041__ $$aeng
000079565 100__ $$aDella Valle, M.
000079565 245__ $$aGW170817: implications for the local kilonova rate and for surveys from ground-based facilities
000079565 260__ $$c2018
000079565 5060_ $$aAccess copy available to the general public$$fUnrestricted
000079565 5203_ $$aWe compute the local rate of events similar to GRB 170817A, which has been recently found to be associated with a kilonova (KN) outburst. Our analysis finds an observed rate of such events of RKN~352+810-281 Gpc-3¿yr-1. After comparing at their face values this density of sGRB outbursts with the much higher density of binary neutron star (BNS) mergers of 1540+3200-1220 Gpc-3¿yr-1, estimated by LIGO–Virgo collaboration, one can conclude, admittedly with large uncertainty that either only a minor fraction of BNS mergers produces short gamma-ray bursts (sGRB)/KN events or the sGRBs associated with BNS mergers are beamed and observable under viewing angles as large as ¿ ¿ 40°. Finally, we provide preliminary estimates of the number of sGRB/KN events detected by future surveys carried out with present/future ground-based/space facilities, such as LSST, VST, ZTF, SKA, and THESEUS.
000079565 540__ $$9info:eu-repo/semantics/openAccess$$aAll rights reserved$$uhttp://www.europeana.eu/rights/rr-f/
000079565 590__ $$a5.231$$b2018
000079565 591__ $$aASTRONOMY & ASTROPHYSICS$$b15 / 69 = 0.217$$c2018$$dQ1$$eT1
000079565 592__ $$a2.422$$b2018
000079565 593__ $$aSpace and Planetary Science$$c2018$$dQ1
000079565 593__ $$aAstronomy and Astrophysics$$c2018$$dQ1
000079565 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000079565 700__ $$aGuetta, D.
000079565 700__ $$aCappellaro, E.
000079565 700__ $$aAmati, L.
000079565 700__ $$aBotticella, M.T.
000079565 700__ $$aBranchesi, M.
000079565 700__ $$aBrocato, E.
000079565 700__ $$aIzzo, L.
000079565 700__ $$0(orcid)0000-0001-5654-0266$$aPerez-Torres, M.A.$$uUniversidad de Zaragoza
000079565 700__ $$aStratta, G.
000079565 7102_ $$12004$$2405$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física Teórica
000079565 773__ $$g481, 4 (2018), 4355-4360$$pMon. not. R. Astron. Soc.$$tMonthly Notices of the Royal Astronomical Society$$x0035-8711
000079565 8564_ $$s192225$$uhttps://zaguan.unizar.es/record/79565/files/texto_completo.pdf$$yVersión publicada
000079565 8564_ $$s109902$$uhttps://zaguan.unizar.es/record/79565/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000079565 909CO $$ooai:zaguan.unizar.es:79565$$particulos$$pdriver
000079565 951__ $$a2020-01-17-21:22:03
000079565 980__ $$aARTICLE