diff --git a/examples/Example.ipynb b/examples/Example.ipynb index d5deb07..ede4e77 100644 --- a/examples/Example.ipynb +++ b/examples/Example.ipynb @@ -463,7 +463,7 @@ "cell_type": "markdown", "metadata": {}, "source": [ - "Now we have a pretty good looking light curve! This light curve is just generated with the central pixel, so lets make a better aperture. We can do quick aperture photometry with tr.Make_lc(). If you provide no aperture, then it will use a 3x3 aperture at the centre of the image. If you want to give it a custom aperture, then you can either give it a list of coordinate pairs, referenced from the origin, or a boolean numpy array the same shape as the tpf images.In this case we know the source is at the centre, so the default aperture will work fine!\n", + "Now we have a pretty good looking light curve! This light curve is just generated with the central pixel, so lets make a better aperture. We can do quick aperture photometry with tr.make_lc(). If you provide no aperture, then it will use a 3x3 aperture at the centre of the image. If you want to give it a custom aperture, then you can either give it a list of coordinate pairs, referenced from the origin, or a boolean numpy array the same shape as the tpf images.In this case we know the source is at the centre, so the default aperture will work fine!\n", "\n", "Often we don't need the full cadence of the TESS FFIs, so we can bin the data to improve the signal to noise. Let's make two lightcurves, one with no binning and the other binned to 12, or 6 hours." ] @@ -474,8 +474,8 @@ "metadata": {}, "outputs": [], "source": [ - "lc = tr.Make_lc(tpf.astropy_time.mjd,flux,bin_size=0,normalise=False)\n", - "lc_bin = tr.Make_lc(tpf.astropy_time.mjd,flux,bin_size=12,normalise=False)" + "lc = tr.make_lc(tpf.astropy_time.mjd,flux,bin_size=0,normalise=False)\n", + "lc_bin = tr.make_lc(tpf.astropy_time.mjd,flux,bin_size=12,normalise=False)" ] }, { @@ -708,7 +708,7 @@ } ], "source": [ - "lc = tr.Make_lc(tpf.astropy_time.mjd,flux-ref,bin_size=12)\n", + "lc = tr.make_lc(tpf.astropy_time.mjd,flux-ref,bin_size=12)\n", "tr.Plotter(lc[0,:],lc[1,:])" ] },