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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

evidence

Establishes the 17 August 2017 binary neutron-star merger and the associated kilonova AT2017gfo in NGC 4993 at roughly 40 Mpc as a site of r-process nucleosynthesis. Volume and page numbers are deliberately not asserted because they were not confirmed. Ejecta mass estimates of 0.03-0.06 solar masses come from modelling papers summarised via search, not from this paper.

A evidence is not a place. Drawing it on a map would assert something about the world that no stored fact supports.

Evidence · 0

This object cites no evidence.

Timeline

No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.

Connections · 0
    Assembled narrative · 0

    This object does not clear the publishing floor: an assembled narrative needs a description and at least one cited piece of evidence.

    Observed changes · 0

    No public Signals are attached to this object. Signals show what changed and when it was observed — never a direction or a rank.

    Actions

    Read the assembled narrativeThis object has no public Experience: one needs a description and at least one cited piece of evidence.Continue in StudioOpen TwinTwin does not start a decision from this kind of object.ShareSaveSaved objects are part of the authenticated projection, which is declared and not yet built.

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