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Perhaps observing a widening divergence between observation and theory, the authors declared that "it seems unlikely that this test of relativistic gravity will be improved significantly."<ref>J. M. Weisberg and J. H. Taylor, ''[http://arxiv.org/PS_cache/astro-ph/pdf/0407/0407149v1.pdf Relativistic Binary Pulsar B1913+16: Thirty Years of Observations and Analysis]'' (July 7, 2004).</ref>
 
Perhaps observing a widening divergence between observation and theory, the authors declared that "it seems unlikely that this test of relativistic gravity will be improved significantly."<ref>J. M. Weisberg and J. H. Taylor, ''[http://arxiv.org/PS_cache/astro-ph/pdf/0407/0407149v1.pdf Relativistic Binary Pulsar B1913+16: Thirty Years of Observations and Analysis]'' (July 7, 2004).</ref>
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No data observed after 2003 have been published about this binary pulsar, which suggests that the data have diverged even further from the predictions of the [[General Theory of Relativity]].  It would be easy to post the data on the internet for the public to view and draw their own conclusions.
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No data observed after 2003 have been published about this binary pulsar, which suggests either that the data have diverged even further from the predictions of the [[General Theory of Relativity]] or that the pulsar has not been observed since 2003.  It would be easy to post the data on the internet for the public to view and draw their own conclusions.
    
==References==
 
==References==
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