- 16 Oct, 2018 9 commits
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Chris Shallue authored
This applies mainly to scrambled data (NaN time values typically come with NaN flux values, which are removed anyway, but scrambing decouples NaN time values from NaN flux values). PiperOrigin-RevId: 209029696
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Alex Tamkin authored
Update configurations with label mapping for simulated data and new batch_size and learning_rate from vizier studies. PiperOrigin-RevId: 208902383
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Alex Tamkin authored
PiperOrigin-RevId: 208863882
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Alex Tamkin authored
PiperOrigin-RevId: 208862798
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Alex Tamkin authored
Ensure consistent argument order, change NaN processing to remove NaN times as well, and do so before scrambling PiperOrigin-RevId: 207804986
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Alex Tamkin authored
Modify processing pipeline to enable generation of scrambled lightcurves. Fix bugs to enable generation of inverted lightcurves. PiperOrigin-RevId: 207595688
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Chris Shallue authored
Inversion should be done *after* fitting a normalization curve to the stellar variability and dividing it away. Doing it before normalizing may result in unintentionally reversing the inversion. Therefore we remove the option to do it at this point. PiperOrigin-RevId: 207309650
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Chris Shallue authored
PiperOrigin-RevId: 205427760
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Chris Shallue authored
PiperOrigin-RevId: 205168785
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- 26 Jun, 2018 1 commit
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Billy Lamberta authored
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- 25 Jun, 2018 3 commits
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Chris Shallue authored
PiperOrigin-RevId: 202034593
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Chris Shallue authored
PiperOrigin-RevId: 202034513
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Chris Shallue authored
PiperOrigin-RevId: 201878162
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- 24 Jun, 2018 4 commits
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Chris Shallue authored
PiperOrigin-RevId: 201839789
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Chris Shallue authored
PiperOrigin-RevId: 201839334
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Chris Shallue authored
PiperOrigin-RevId: 201007094
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Chris Shallue authored
PiperOrigin-RevId: 201007073
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- 15 Jun, 2018 1 commit
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Chris Shallue authored
This subcase may pass or fail based on the version of pydl. PiperOrigin-RevId: 200736816
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- 14 Jun, 2018 4 commits
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Chris Shallue authored
PiperOrigin-RevId: 199887920
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Chris Shallue authored
PiperOrigin-RevId: 199862472
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Chris Shallue authored
- Return additional metadata about the spline fit: likelihood_term, penalty_term, bic. - Don't fit a spline to < 4 points. Previously, light curve segments with less than 4 points would be fit by a fake spline that fit the points exactly. - Better support for light curve segments with 0-2 points. PiperOrigin-RevId: 199858599
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Chris Shallue authored
PiperOrigin-RevId: 193054491
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- 16 Mar, 2018 7 commits
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Christopher Shallue authored
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Christopher Shallue authored
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Christopher Shallue authored
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Christopher Shallue authored
This is not a performance issue for the instances replaced because each instance is expected to iterate over zipped lists of < ~20 references to numpy arrays.
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Christopher Shallue authored
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Christopher Shallue authored
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Chris Shallue authored
PiperOrigin-RevId: 189060074
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- 09 Mar, 2018 2 commits
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Chris Shallue authored
PiperOrigin-RevId: 188503988
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Chris Shallue authored
PiperOrigin-RevId: 188502535
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- 05 Mar, 2018 2 commits
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Chris Shallue authored
PiperOrigin-RevId: 187887326
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Chris Shallue authored
PiperOrigin-RevId: 187400242
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- 28 Feb, 2018 3 commits
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Christopher Shallue authored
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Christopher Shallue authored
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Christopher Shallue authored
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- 23 Jan, 2018 1 commit
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Christopher Shallue authored
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