Fix PDC language in LightCurveFile tutorial per JS recommendation
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- "Kepler light curves from MAST have some level of processing (more details [here](https://arxiv.org/pdf/1207.3093.pdf)) and allow you to access the two kinds of flux; the **SAP** flux and the **PDCSAP** flux. SAP flux is Simple Aperture Photometry flux, the same as we made in the [previous tutorial](http://lightkurve.keplerscience.org/tutorials/1.03-what-are-lightcurves.html). PDCSAP is the Pre-search Data Conditioning SAP flux. Long term trends have been removed from this data using so-called Cotrending Basis Vectors (CBVs). PDCSAP flux is usually slightly cleaner data than the SAP flux and will have fewer long term trends.\n",
+ "Kepler light curves from MAST have some level of processing (more details [here](https://arxiv.org/pdf/1207.3093.pdf)) and allow you to access the two kinds of flux; the **SAP** flux and the **PDCSAP** flux. SAP flux is Simple Aperture Photometry flux, the same as we made in the [previous tutorial](http://lightkurve.keplerscience.org/tutorials/1.03-what-are-lightcurves.html). PDCSAP is the Pre-search Data Conditioning SAP flux. Long term trends have been removed from this data using so-called Cotrending Basis Vectors (CBVs). PDCSAP flux is usually cleaner data than the SAP flux and will have fewer systematic trends.\n",
"\n",
"We can read in a light curve file from the Kepler mission using `KeplerLightCurveFile`. We can use the `search_lightcurvefile()` function to fetch them from the data archive:"
]
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- "version": "3.7.3"
+ "version": "3.7.4"
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