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ping @amcody @barentsen and I all talked about this idea. We want to be able to hand-in priors on RA and Dec, and have the priors update with spacecraft induced...

Here's a *very rough pseudocode* of what Geert suggested: ```python scene = SceneModel(stars=[StarPrior(ra, dec, pos_uncertaity, flux), StarPrior(ra, dec, flux), ..], background_prior=UniformPrior()) scene.fit(tpf) ```

Hello! :wave: Yay! Glad this demo/tutorial is in the right direction. Some of the impetus for this feature has been slightly subdued-we now programmatically query the [HET Observability website](https://het.as.utexas.edu/HET/hetweb/ProgramPrep/hetdexcalendar.html) and...

Regarding TESS-- the observations I had in mind are contemporaneous with TESS, and so the TESS observability serves as a "constraint" as such. But I suppose the key idea is...

It looks like you're trying to fit with just two parameters-- Temperature and surface gravity, and excluding metallicity. The `PHOENIXGridInterfaceNoAlpha` expects 3 parameters. In order to achieve your desired outcome...

There is experimental code to do inference on binaries [here](https://github.com/gully/Starfish/blob/mix_model_omega2/scripts/star_binary.py), but it's basically untested, and has known bugs. I'll be revamping this code eventually, so I invite you to subscribe...

It seems like there's a resonance feature that reorders the wavelengths at one index location: ![vac_air_demo](https://cloud.githubusercontent.com/assets/860227/23523464/daa829f8-ff3b-11e6-8ed8-897466332830.png) Not sure how to handle this, though these are exceptionally short wavelengths, so it's...

I actually just implemented [wavelength-dependent spectral resolution](https://github.com/gully/Starfish/blob/mix_model_omega2/Starfish/grid_tools.py#L787) for the SpeX Prism mode, which [varies in spectral resolution by a factor of ~2.5](http://irtfweb.ifa.hawaii.edu/~spex/uprism_R.jpg). I added a method to the relevant instrumental...

Update: >in principle we could divide by a taper to get back high frequency structure, meaning that we would support either over- or under- estimates of the spectral resolution! I...

I experimented with custom terminal output, namely aligning the sample positions and printing accept/reject in a single line. Looks like this: