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update notebooks to lcviz 0.4.2 #5

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Aug 23, 2024
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update notebooks to lcviz 0.4.2 #5

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13 changes: 6 additions & 7 deletions mult_ephem_RR-Lyr.ipynb
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Original file line number Diff line number Diff line change
Expand Up @@ -9,8 +9,8 @@
"\n",
"[RR Lyrae](https://en.wikipedia.org/wiki/RR_Lyrae) is the prototype of a class of variable stars with radial pulsations. The pulsation period is related to the stellar luminosity, and a second, lower frequency variation can be seen on longer timescales, known as the [Blazkho effect](https://en.wikipedia.org/wiki/Blazhko_effect). \n",
"\n",
"* **Last Updated**: March 7, 2024\n",
"* **lcviz version**: 0.2.0\n",
"* **Last Updated**: August 21, 2024\n",
"* **lcviz version**: 0.4.2\n",
"\n",
"RR Lyrae itself was in the Kepler field, so let's load one Kepler Quarter of long-cadence observations, and inspect the periods:"
]
Expand Down Expand Up @@ -69,7 +69,7 @@
"plot_options = lcviz.plugins['Plot Options']\n",
"freq_analysis = lcviz.plugins['Frequency Analysis']\n",
"freq_analysis.auto_range = False\n",
"freq_analysis.xunit.selected = 'period'\n",
"freq_analysis.xunit = 'period'\n",
"\n",
"lcviz.show()"
]
Expand Down Expand Up @@ -151,12 +151,11 @@
"metadata": {},
"outputs": [],
"source": [
"for viewer in lcviz.app.get_viewer_reference_names():\n",
"for viewer in plot_options.viewer.choices:\n",
" plot_options.viewer = viewer\n",
" plot_options.layer = lcviz.app.data_collection[0].label\n",
" plot_options.marker_color_mode = 'Linear'\n",
" plot_options.marker_colormap = 'Viridis'\n",
" plot_options._obj.marker_color_col_value = 'phase:blazkho'"
" plot_options.marker_color_col = 'phase:blazkho'"
]
},
{
Expand Down Expand Up @@ -184,7 +183,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
"version": "3.11.3"
"version": "3.11.9"
}
},
"nbformat": 4,
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6 changes: 3 additions & 3 deletions mult_ephem_kic_2835289.ipynb
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Expand Up @@ -9,8 +9,8 @@
"\n",
"This notebook loads the Kepler light curve for a eclipsing triple system (KIC 2835289) containing a binary with ellipsoidal variations and a third star on an eccentric orbit. We use lcviz to flatten the light curve, and phase-fold on both orbital periods.\n",
"\n",
"* **Last Updated**: March 7, 2024\n",
"* **lcviz version**: 0.2.0"
"* **Last Updated**: August 21, 2024\n",
"* **lcviz version**: 0.4.2"
]
},
{
Expand Down Expand Up @@ -264,7 +264,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
"version": "3.11.3"
"version": "3.11.9"
}
},
"nbformat": 4,
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16 changes: 7 additions & 9 deletions short_cadence_phase_curve_HAT-P-7.ipynb
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Expand Up @@ -9,8 +9,8 @@
"\n",
"HAT-P-7 b ([Pál et al. 2008](https://ui.adsabs.harvard.edu/abs/2008ApJ...680.1450P/abstract)) is a hot Jupiter orbiting a bright F6V host in the Kepler field. Let's take a look at short cadence (one-minute) Kepler observations from the first three Kepler quarters to see the secondary eclipse of the planet, when the planet's flux disappears as the planet is eclipsed by the host star.\n",
"\n",
"* **Last Updated**: March 7, 2024\n",
"* **lcviz version**: 0.2.0\n",
"* **Last Updated**: August 21, 2024\n",
"* **lcviz version**: 0.4.2\n",
"\n",
"First we download the observations with `lightkurve`:"
]
Expand Down Expand Up @@ -156,25 +156,23 @@
},
"outputs": [],
"source": [
"viewer = lcviz.app.get_viewer('flux-vs-phase:default')\n",
"viewer.state.y_min = 0.99993\n",
"viewer.state.y_max = 1.00005\n",
"lcviz.viewers['flux-vs-phase:default'].set_limits(y_min=0.99993, y_max=1.00005)\n",
"\n",
"plot_options = lcviz.plugins['Plot Options']\n",
"plot_options.viewer = 'flux-vs-phase:default'\n",
"plot_options.layer = 'HAT-P-7'\n",
"plot_options.layer = 'HAT-P-7 Q3'\n",
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Suggested change
"plot_options.layer = 'HAT-P-7 Q3'\n",
"plot_options.layer = 'HAT-P-7'\n",

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hmmm are you on main or 0.4.2? I am pretty sure I ran this through and the quarter was appended to the input data-label. (0.4.x does not have spacetelescope/lcviz#120)

"plot_options.marker_opacity = 0.1\n",
"plot_options.marker_size = 1\n",
"\n",
"plot_options.layer = 'binned HAT-P-7:default'\n",
"plot_options.layer = 'binned HAT-P-7 Q3:default'\n",
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Suggested change
"plot_options.layer = 'binned HAT-P-7 Q3:default'\n",
"plot_options.layer = 'binned HAT-P-7:default'\n",

"plot_options.marker_size = 50\n",
"plot_options.marker_color = 'r'"
]
},
{
"cell_type": "code",
"execution_count": null,
"id": "5e851e0a-c4e0-48a3-9701-b6c1928e7fc5",
"id": "496237ce-a773-4f42-b2c3-ae81d329c3fb",
"metadata": {},
"outputs": [],
"source": []
Expand All @@ -196,7 +194,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
"version": "3.11.3"
"version": "3.11.9"
}
},
"nbformat": 4,
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