Sam Lee

On the possible workaround for explicitly passing `cenfunc` and `stdfunc` parameters to `sigma_clip()`, I did a bit of due diligence on the mapping required. One thing that stood out is...

> The reason we encounter MaskedQuantity in Lightkurve is because the astropy.table.QTable class uses MaskedQuantity objects in place of MaskedColumn as of AstroPy v5.0. I first thought it might be...

@ceb will this PR support MAST case, where the MAST service uses a long-running polling mechanism such that the raw http response from MAST is really just a status code,...

@ceb Thanks for the clarification.

Something strange is going on. If I do a river plot using TESS only data, i.e., `tlc` in the example, the result plot looks okay. ```python river_tess = tlc.fold(bls.period_at_max_power, bls.transit_time_at_max_power).plot_river(method='sigma');...

Context on why I tried to remove `flux_err` in the first place. I try to do a plot of a lightcurve with 2 different flavors of flux (in the same...

What you suggested make sense - A more helping error / error message would be an improvement.

1. For `LightCurve` objects, it is indeed limited by an upstream astropy issue. If my memory serves me right, the crux of the issue is `Quantity` doesn't support masking. 2....

Additionally, we should be able to take care of the BTJD conversion, something like the following: ```python # given a df lc = lk.TessLightCurve.from_pandas(df) ``` @bmorris3 In your use case,...

@bmorris3 I wonder if the round-trip exercise is about playing around with the API or has some concrete use cases. Conceivably, we could make it work by changing `LightCurve.to_pandas()` so...