000262329 001__ 262329
000262329 005__ 20190619220136.0
000262329 022__ $$a0035-8711
000262329 022__ $$a1365-2966
000262329 02470 $$a000449616200081$$2isi
000262329 0247_ $$a10.1093/mnras/sty1939$$2doi
000262329 037__ $$aARTICLE
000262329 245__ $$aDark Energy Survey Year 1 Results: A Precise H-0 Estimate from DES Y1, BAO, and D/H Data
000262329 260__ $$c2018$$aOxford$$bOXFORD UNIV PRESS
000262329 269__ $$a2018-11-01
000262329 336__ $$aJournal Articles
000262329 520__ $$aWe combine Dark Energy Survey Year 1 clustering and weak lensing data with baryon acoustic oscillations and Big Bang nucleosynthesis experiments to constrain the Hubble constant. Assuming a flat Lambda CDM model with minimal neutrino mass (Sigma m(v), = 0.06 eV), we find H-0 = 67.4(-1.2)(+1.1) km s(-1) Mpc(-1) (68 per cent CL). This result is completely independent of Hubble constant measurements based on the distance ladder, cosmic microwave background anisotropies (both temperature and polarization), and strong lensing constraints. There are now five data sets that: (a) have no shared observational systematics; and (b) each constrains the Hubble constant with fractional uncertainty at the few-per cent level. We compare these five independent estimates, and find that, as a set, the differences between them are significant at the 2.5 sigma level (chi(2)/dof = 24/11, probability to exceed = 1.1 per cent). Having set the threshold for consistency at 30 sigma we combine all five data sets to arrive at H-0 = 69.3(-0.6)(+0.4) km s(-1) Mpc(-1).
000262329 650__ $$aAstronomy & Astrophysics
000262329 650__ $$aAstronomy & Astrophysics
000262329 6531_ $$acosmological parameters
000262329 6531_ $$acosmology: observations
000262329 6531_ $$adistance scale
000262329 6531_ $$abaryon acoustic-oscillations
000262329 6531_ $$acosmological parameter constraints
000262329 6531_ $$ahubble constant
000262329 6531_ $$adistance ladder
000262329 6531_ $$agalaxy sample
000262329 6531_ $$asdss dr7
000262329 6531_ $$amodel
000262329 700__ $$aAbbott, T. M. C.
000262329 700__ $$aAbdalla, F. B.
000262329 700__ $$aAnnis, J.
000262329 700__ $$aBechtol, K.
000262329 700__ $$g276121$$0250390$$aBlazek, J.
000262329 700__ $$aBenson, B. A.
000262329 700__ $$aBernstein, R. A.
000262329 700__ $$aBernstein, G. M.
000262329 700__ $$aBertin, E.
000262329 700__ $$aBrooks, D.
000262329 700__ $$aBurke, D. L.
000262329 700__ $$aCarnero Rosell, A.
000262329 700__ $$aCarrasco Kind, M.
000262329 700__ $$aCarretero, J.
000262329 700__ $$aCastander, F. J.
000262329 700__ $$aChang, C. L.
000262329 700__ $$aCrawford, T. M.
000262329 700__ $$aCunha, C. E.
000262329 700__ $$aD'Andrea, C. B.
000262329 700__ $$ada Costa, L. N.
000262329 700__ $$aDavis, C.
000262329 700__ $$aDeRose, J.
000262329 700__ $$aDesai, S.
000262329 700__ $$aDiehl, H. T.
000262329 700__ $$aDietrich, J. P.
000262329 700__ $$aDoel, P.
000262329 700__ $$aDrlica-Wagner, A.
000262329 700__ $$aEvrard, A. E.
000262329 700__ $$g104110$$0244407$$aFernandez, E.
000262329 700__ $$aFlaugher, B.
000262329 700__ $$aFosalba, P.
000262329 700__ $$aFrieman, J.
000262329 700__ $$aGarcia-Bellido, J.
000262329 700__ $$aGaztanaga, E.
000262329 700__ $$aGerdes, D. W.
000262329 700__ $$aGiannantonio, T.
000262329 700__ $$aGruen, D.
000262329 700__ $$aGruendl, R. A.
000262329 700__ $$aGschwend, J.
000262329 700__ $$aGutierrez, G.
000262329 700__ $$aHartley, W. G.
000262329 700__ $$aHenning, J. W.
000262329 700__ $$aHonscheid, K.
000262329 700__ $$aHoyle, B.
000262329 700__ $$aHuterer, D.
000262329 700__ $$aJain, B.
000262329 700__ $$aJames, D. J.
000262329 700__ $$aJarvis, M.
000262329 700__ $$aJeltema, T.
000262329 700__ $$aJohnson, M. D.
000262329 700__ $$aJohnson, M. W. G.
000262329 700__ $$aKrause, E.
000262329 700__ $$aKuehn, K.
000262329 700__ $$aKuhlmann, S.
000262329 700__ $$aKuropatkin, N.
000262329 700__ $$aLahav, O.
000262329 700__ $$aLiddle, A. R.
000262329 700__ $$g274501$$0250244$$aLima, M.
000262329 700__ $$aLin, H.
000262329 700__ $$aMacCrann, N.
000262329 700__ $$aMaia, M. A. G.
000262329 700__ $$aManzotti, A.
000262329 700__ $$aMarch, M.
000262329 700__ $$aMarshall, J. L.
000262329 700__ $$aMiquel, R.
000262329 700__ $$aMohr, J. J.
000262329 700__ $$aNatoli, T.
000262329 700__ $$aNugent, P.
000262329 700__ $$aOgando, R. L. C.
000262329 700__ $$aPark, Y.
000262329 700__ $$aPlazas, A. A.
000262329 700__ $$aReichardt, C. L.
000262329 700__ $$aReil, K.
000262329 700__ $$aRoodman, A.
000262329 700__ $$g251584$$0248569$$aRoss, A. J.
000262329 700__ $$aRozo, E.
000262329 700__ $$aRykoff, E. S.
000262329 700__ $$g106339$$0241512$$aSanchez, E.
000262329 700__ $$aScarpine, V.
000262329 700__ $$aSchubnell, M.
000262329 700__ $$aScolnic, D.
000262329 700__ $$aSevilla-Noarbe, I.
000262329 700__ $$aSheldon, E.
000262329 700__ $$g206098$$0244159$$aSmith, M.
000262329 700__ $$aSmith, R. C.
000262329 700__ $$aSoares-Santos, M.
000262329 700__ $$aSobreira, F.
000262329 700__ $$aSuchyta, E.
000262329 700__ $$aTarle, G.
000262329 700__ $$aThomas, D.
000262329 700__ $$aTroxel, M. A.
000262329 700__ $$aWalker, A. R.
000262329 700__ $$aWechsler, R. H.
000262329 700__ $$aWeller, J.
000262329 700__ $$aWester, W.
000262329 700__ $$aWu, W. L. K.
000262329 700__ $$aZuntz, J.
000262329 773__ $$k3$$j480$$q3879-3888$$tMonthly Notices Of The Royal Astronomical Society
000262329 8560_ $$fyves.revaz@epfl.ch
000262329 909C0 $$zPasquier, Simon$$0252365$$yApproved$$pLASTRO$$xU10933$$myves.revaz@epfl.ch
000262329 909CO $$particle$$ooai:infoscience.epfl.ch:262329$$pSB
000262329 961__ $$afantin.reichler@epfl.ch
000262329 973__ $$aEPFL$$sPUBLISHED$$rREVIEWED
000262329 980__ $$aARTICLE
000262329 980__ $$aWoS
000262329 981__ $$aoverwrite