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Towards the ultimate in Time precision: BIPM17 corrections #8130

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@mhvk

Talking to @luojing1211 from PINT (and mostly to remind ourselves), one additional correction that pulsar timing people make happens for conversion to TT -- which appears to have different versions, the most current being TT(BIPM17) [1]. It can be the difference between pulsar timing arrays detecting gravitational waves or not... We should follow the BIPM, though may need to think about how to ensure that one can also use pure-ERFA/SOFA.

[1] ftp://ftp2.bipm.org/pub/tai/ttbipm/TTBIPM.17

EDIT: link to BIPM sercive responsible for this: https://www.bipm.org/en/bipm-services/timescales/

p.s. Related precision issues: improve interpolation in IERS tables (#1803) and GPS-UTC corrections (#2134)

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  1. pllim commented on Nov 15, 2018

    @pllim
    Member

    To ensure future accessibility to the cited work, is there a proper reference other than FTP link? If so, please also include that in this issue. Thanks!

  2. mhvk commented on Nov 15, 2018

    @mhvk
    ContributorAuthor

    @pllim - OK, added link to BIPM time service above (it works in conjunction with IAU). Let me also ping @taldcroft to think about what should be default. Options:

    1. Always "best possible", i.e., use most recent TT(BIPM) (as we do for IERS). Files are not very big, but it means that results might very slightly change (10s of ns level) with time.
    2. Default to "builtin" ERFA/SOFAR (as we do for coordinate transformations, but not for UT1), i.e., have some context manager or so to define which TT one uses.
    3. Have context manager, but default to "best possible".

    I think we need the context manager, and would go for a default of "best possible".

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