Nature - 15.08.2019
Letter https://doi.org/10.1038/s41586-019-1389-7 A fast radio burst localized to a massive galaxy V. ravi1,2*, M. Catha^3 , L. D ...
Letter reSeArCH The spectrum (Fig. 3 ) indicates stellar absorption features at a redshift of 0.660(2). A single emission line, ...
reSeArCH Letter The properties of PSO J20 7 + 72 are in tension with FRB progeni- tor models developed on the basis of the host ...
Letter reSeArCH MeThods The DSA-10 instrument. The Deep Synoptic Array 10-element prototype (DSA-10) is an array of ten 4.5-m ra ...
reSeArCH Letter We verified the efficacy of our localization procedure using a selection of meth- ods. First, no substantial pha ...
Letter reSeArCH Conroy, C., Gunn, J. E. & White, M. The propagation of uncertainties in stellar population synthesis modeli ...
reSeArCH Letter Extended Data Fig. 1 | DSA-10 images. Dirty and deconvolved images are shown of two bright point-sources and FRB ...
Letter reSeArCH Extended Data Fig. 2 | Visibility phases measured for two bright point-sources and FRB 190523. Only data on base ...
reSeArCH Letter Extended Data Fig. 3 | Recovered positions of J1927 + 7358 on 12 separate days. Each position was derived from 5 ...
Letter reSeArCH extended data Table 1 | ITRF coordinates for the ten dsA-10 antennas ...
Letter https://doi.org/10.1038/s41586-019-1470-2 The formation of Jupiter’s diluted core by a giant impact Shang-Fei Liu1,2*, Ya ...
reSeArCH Letter The impact results in little mass loss (see Table 1 ), but Jupiter’s initial core is completely disrupted. Duri ...
Letter reSeArCH A gradual accretion of planetesimals along with the runaway gas accre- tion may also produce a diluted core^15 , ...
reSeArCH Letter MeThods A statistical N-body study of embryo collisions. We investigate the statistics of collisions between an ...
Letter reSeArCH affected by the choice of a H-He EOS model because the impact causes only a small change in internal energy insi ...
reSeArCH Letter Jupiter with a diluted core (models H-4.5 and H-4.5-rock). If the heavy elements are represented by rock (SiO 2 ...
Letter reSeArCH 0 0.2 0.4 0.6 0.8 1 InwardMergeOutwardEscape InwardMergeOutwardEscape InwardMergeOutwardEscape InwardMergeOutwar ...
reSeArCH Letter 0 102030405060708090 0 25 50 75 100 0 2 4 6 8 Collision angle N tgrow=0.1 Myr, k=10.0 Probabilit y(%) f=1.0 0 10 ...
Letter reSeArCH Density ( g cm-3 ) 10 -4 10 -3 10 -2 10 -1 100101 3,302.0 s 4,801.0 s 6,301.0 s 39,705.0 s a b c d Extended Data ...
reSeArCH Letter 0.0 0.2 0.4 0.6 0.8 1.0 -1×10^41 0 1×10^41 2×10^41 3×10^41 4×10^41 5×10^41 6×10^41 Radius[RJ] Δ E internal [ergs ...
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