gully

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Great food for thought here, thanks!! One admittedly niche science case stems from the desire to register ancillary (e.g. ground-based spectroscopic) observations to space-based photometry, as in the case of...

Agreed to the themes here, and the point is taken about dilution--subtle aperture affects will matter, and EBs and other benchmarks would be great calibrators to spot-check. That's Tabby's star...

Demo of Tabby's star with custom and crude FFI zero point calibration: ![KIC_8462852_FFI_gully_vs_f3_demo](https://user-images.githubusercontent.com/860227/68791871-0b251380-05ff-11ea-80dd-e0540ccf5ad3.png) You can see the conspicuous channel-level offsets imperfectly corrected in at least one channel group. The overall...

A colleague was seeing a similar error that we diagnosed as the absence of the file `dm_deep_v1.2_vvcrit0.4_full_isos.h5` . When I send this file to the colleague and it is placed...

I'm experimenting with this now, I'll let you know if it sticks. :)

Ok, it seems like this worked. It's a minimal proof-of-concept, but with a little fixing-up it could be contributed back to the main repo, if desired. Notable demerits of the...

Code for above example: ``` python for mass in [0.02, 0.05, 0.1, 0.3, 0.6, 0.9, 1.2]: ev = bcah.evtrack(mass,dage=0.01, minage=6.0, maxage=9.9) plt.plot((ev['Teff']),ev['logL'],'.', alpha=0.5) for age in [6.0, 7.0, 8.0, 9.0,...

There's been some renewed interest from a few folks about Chabrier/Baraffe isochrones models. Here is the notebook that generated the figure above, and also makes an animation useful for talks...

Hi @timothydmorton ! I haven't tried this out since 2016 I think, so my hunch is that it won't work with version >= 2. The commits are linked here so...