Starfish

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Currently all the links point to `iancze/Starfish` so we'll need to update those. GitHub is really kind and will automatically redirect links so nothing is broken, yet, but going through...

mileslucas

Issues running the example WASP14: pca problem

11

Hi! I installed Starfish in my laptop computer (Ubuntu 16.04). I followed the instructions and had no issues until trying to follow the example for WASP14. The error appear when...

AngelicaJara

Different local kernels

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_The problem:_ Not all residual spectrum outliers originate solely from line strength mismatches. In general, line _width_ mismatches or line center shifts will be present in the residual spectrum as...

gully

Version 0.3 Roadmap

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Version 0.2 is out, so version 0.3 roadmap is here. :rocket: Simple goals for this release: - [x] Air/vacuum instrument class support #57 - [ ] Enhanced terminal output during...

gully

Priors on the normalization of the global and emulator covariance matrix

1

The normalization of the global covariance is described by a free parameter `logAmp` (the actual normalization is `(10**logAmp)**2`). But if such normalization is much higher than the median value of...

zjzhang42

Rewriting the Habib Likelihood Equation

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@iancze @gully I would love some help on this. So the Habib likelihood function is great for comparing fitting the GP hyperparameters to the spectra, but I've been wondering if...

mileslucas

Pickling in parallel.py

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I'm not sure what the history of `parallel.py` is, but I tried running it with some data files and I ran into the issues that nothing would work as is...

mileslucas

Priors on stellar parameters

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## Priors on stellar parameters _The problem:_ I suspect that a common use case might resemble the following scenario: A user would like to force the value of a parameter...

gully

Spectra storage format specification

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I would like to use this as a discussion point for fleshing out a data format spec for use in Starfish. This also pertains to #21. Spurred on by a...

iancze

New physics mean model extension: veiling from circumstellar disk

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I am adding a new module to support inferences of an emission component from circumstellar disks. My assumptions for the purpose of this implementation are: 1. The emission component is...

gully