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Copy file name to clipboardExpand all lines: tutorials/firefly/NEOWISE_light_curve_demo.md
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name: python3
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<aid="top"></a>
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# Finding Light Curves of Solar System Objects
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***
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## Learning Goals
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By the end of this tutorial, you will:
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You can re-initizialize the viewer to return to a clean slate with [`reinit_viewer`](https://caltech-ipac.github.io/firefly_client/api/firefly_client.FireflyClient.html#firefly_client.FireflyClient.reinit_viewer).
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```{code-cell} ipython3
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# fc.reinit_viewer(); # The semi-colon suppresses the output of the method when ran
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# fc.reinit_viewer(); # The semi-colon suppresses the output of the method when ran
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```
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## Step 2
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You will notice that there are colored squares that signify where the object was observed based on the RA and Dec given in the catalog.
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Alternatively, we can queue a HiPS image using the method [`show_hips`](https://caltech-ipac.github.io/firefly_client/api/firefly_client.FireflyClient.html#firefly_client.FireflyClient.show_hips). However, this method requires target coordinates for the object you want to analyze.
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```{code-cell} ipython3
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r = fc.add_cell(2, 2, 2, 2, 'catalog-image', 'target')
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if r['success']:
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fc.show_coverage();
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```
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Alternatively, we can queue a HiPS image using the method [`show_hips`](https://caltech-ipac.github.io/firefly_client/api/firefly_client.FireflyClient.html#firefly_client.FireflyClient.show_hips). However, this method requires target coordinates for the object you want to analyze.
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