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CODE_OF_CONDUCT.html

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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/exception_report/wfc3_exception_report.html">Exception Report Checklist - WFC3</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/calwf3_v1.0_cte/calwf3_with_v1.0_PCTE.html">Processing WFC3/UVIS Data with <code class="docutils literal notranslate"><span class="pre">calwf3</span></code> Using the v1.0 CTE-Correction</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/persistence/wfc3_ir_persistence.html">Masking Persistence in WFC3/IR Images</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html">Analyzing WFC3/UVIS G280 Exoplanet Transit Observations</a></li>
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</ul>
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</details></li>
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<li class="toctree-l1 has-children"><a class="reference internal" href="notebooks/WFC3/ir_tvb.html">WFC3/IR Time Variable Background (TVB)</a><details><summary><span class="toctree-toggle" role="presentation"><i class="fa-solid fa-chevron-down"></i></span></summary><ul>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/mast_api_psf/download_psf_cutouts.html">Downloading WFC3 and WFPC2 PSF Cutouts from MAST</a></li>
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</ul>
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</details></li>
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<li class="toctree-l1 has-children"><a class="reference internal" href="notebooks/WFC3/grism_spectroscopy.html">Grism Spectroscopy</a><details><summary><span class="toctree-toggle" role="presentation"><i class="fa-solid fa-chevron-down"></i></span></summary><ul>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html">Analyzing WFC3/UVIS G280 Exoplanet Transit Observations</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_IR_extraction/slitlessutils_IR_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/IR</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_UVIS_fullframe_extraction/slitlessutils_UVIS_fullframe_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/UVIS Full-Frame</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_UVIS_subarray_extraction/slitlessutils_UVIS_subarray_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/UVIS Subarrays</a></li>
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</ul>
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</details></li>
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</ul>
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</div>

CONTRIBUTING.html

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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/exception_report/wfc3_exception_report.html">Exception Report Checklist - WFC3</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/calwf3_v1.0_cte/calwf3_with_v1.0_PCTE.html">Processing WFC3/UVIS Data with <code class="docutils literal notranslate"><span class="pre">calwf3</span></code> Using the v1.0 CTE-Correction</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/persistence/wfc3_ir_persistence.html">Masking Persistence in WFC3/IR Images</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html">Analyzing WFC3/UVIS G280 Exoplanet Transit Observations</a></li>
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</ul>
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</details></li>
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<li class="toctree-l1 has-children"><a class="reference internal" href="notebooks/WFC3/ir_tvb.html">WFC3/IR Time Variable Background (TVB)</a><details><summary><span class="toctree-toggle" role="presentation"><i class="fa-solid fa-chevron-down"></i></span></summary><ul>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/mast_api_psf/download_psf_cutouts.html">Downloading WFC3 and WFPC2 PSF Cutouts from MAST</a></li>
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</ul>
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</details></li>
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<li class="toctree-l1 has-children"><a class="reference internal" href="notebooks/WFC3/grism_spectroscopy.html">Grism Spectroscopy</a><details><summary><span class="toctree-toggle" role="presentation"><i class="fa-solid fa-chevron-down"></i></span></summary><ul>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html">Analyzing WFC3/UVIS G280 Exoplanet Transit Observations</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_IR_extraction/slitlessutils_IR_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/IR</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_UVIS_fullframe_extraction/slitlessutils_UVIS_fullframe_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/UVIS Full-Frame</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_UVIS_subarray_extraction/slitlessutils_UVIS_subarray_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/UVIS Subarrays</a></li>
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</ul>
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</details></li>
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</ul>
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</div>

README.html

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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/exception_report/wfc3_exception_report.html">Exception Report Checklist - WFC3</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/calwf3_v1.0_cte/calwf3_with_v1.0_PCTE.html">Processing WFC3/UVIS Data with <code class="docutils literal notranslate"><span class="pre">calwf3</span></code> Using the v1.0 CTE-Correction</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/persistence/wfc3_ir_persistence.html">Masking Persistence in WFC3/IR Images</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html">Analyzing WFC3/UVIS G280 Exoplanet Transit Observations</a></li>
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</ul>
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</details></li>
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<li class="toctree-l1 has-children"><a class="reference internal" href="notebooks/WFC3/ir_tvb.html">WFC3/IR Time Variable Background (TVB)</a><details><summary><span class="toctree-toggle" role="presentation"><i class="fa-solid fa-chevron-down"></i></span></summary><ul>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/mast_api_psf/download_psf_cutouts.html">Downloading WFC3 and WFPC2 PSF Cutouts from MAST</a></li>
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</ul>
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</details></li>
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<li class="toctree-l1 has-children"><a class="reference internal" href="notebooks/WFC3/grism_spectroscopy.html">Grism Spectroscopy</a><details><summary><span class="toctree-toggle" role="presentation"><i class="fa-solid fa-chevron-down"></i></span></summary><ul>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html">Analyzing WFC3/UVIS G280 Exoplanet Transit Observations</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_IR_extraction/slitlessutils_IR_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/IR</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_UVIS_fullframe_extraction/slitlessutils_UVIS_fullframe_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/UVIS Full-Frame</a></li>
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<li class="toctree-l2"><a class="reference internal" href="notebooks/WFC3/slitlessutils_UVIS_subarray_extraction/slitlessutils_UVIS_subarray_extraction.html"><code class="docutils literal notranslate"><span class="pre">Slitlessutils</span></code> Cookbook: Spectral Extraction for WFC3/UVIS Subarrays</a></li>
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</ul>
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</details></li>
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</ul>
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_sources/notebooks/WFC3/README.md

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WFC3 Notebooks is the primary repository for analyzing data from the
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[Wide Field Camera 3](https://www.stsci.edu/hst/instrumentation/wfc3) on the
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Hubble Space Telescope. The Jupyter notebooks include tools for general data analysis,
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WFC3/IR time variable background (TVB), photometry and point spread function (PSF) modeling. This repository contains the
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WFC3/IR time variable background (TVB), photometry, and point spread function (PSF) modeling. This repository contains the
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complementary notebooks mentioned in the [WFC3 Data Handbook](https://hst-docs.stsci.edu/wfc3dhb).
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These notebooks include:
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- [Exception Report Checklist - WFC3](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/exception_report/wfc3_exception_report.html)
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- [Processing WFC3/UVIS Data with `calwf3` Using the v1.0 CTE-Correction](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/calwf3_v1.0_cte/calwf3_with_v1.0_PCTE.html)
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- [Masking Persistence in WFC3/IR Images](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/persistence/wfc3_ir_persistence.html)
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- [Analyzing WFC3/UVIS G280 Exoplanet Transit Observations](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html)
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WFC3/IR Time Variable Background (TVB):
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- [WFC3/IR IMA Visualization Tools with an Example of Time Variable Background](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/ir_ima_visualization/IR_IMA_Visualization_with_an_Example_of_Time_Variable_Background.html)
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- [HST WFC3 Point Spread Function Modeling](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/point_spread_function/hst_point_spread_function.html)
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- [Downloading WFC3 and WFPC2 PSF Cutouts from MAST](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/mast_api_psf/download_psf_cutouts.html)
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Grism Spectroscopy:
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- [Analyzing WFC3/UVIS G280 Exoplanet Transit Observations](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/uvis_g280_transit/G280_Exoplanet_Transits.html)
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- [`Slitlessutils` Cookbook: Spectral Extraction for WFC3/IR](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/slitlessutils_IR_extraction/slitlessutils_IR_extraction.html)
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- [`Slitlessutils` Cookbook: Spectral Extraction for WFC3/UVIS Full-Frame](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/slitlessutils_UVIS_fullframe_extraction/slitlessutils_UVIS_fullframe_extraction.html)
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- [`Slitlessutils` Cookbook: Spectral Extraction for WFC3/UVIS Subarray](https://spacetelescope.github.io/hst_notebooks/notebooks/WFC3/slitlessutils_UVIS_subarray_extraction/slitlessutils_UVIS_subarray_extraction.html)
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See the [WFC3 Instrument Handbook](https://hst-docs.stsci.edu/wfc3ihb),
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[WFC3 Data Handbook](https://hst-docs.stsci.edu/wfc3dhb),
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[wfc3tools](https://github.com/spacetelescope/wfc3tools), and
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## Contributing
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New contributions and feedback are very welcomed! Please open a new [issue](https://github.com/spacetelescope/hst_notebooks/issues) or new pull request for bugs, feedback, or new features you would like to see. If there is an issue you would like to work on, please leave a comment and we will be happy to assist. Questions can also be sent to the WFC3 team through the [HST Help Desk](https://stsci.service-now.com/hst).
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New contributions and feedback are very welcome! Please open a new [issue](https://github.com/spacetelescope/hst_notebooks/issues) or new pull request for bugs, feedback, or new features you would like to see. If there is an issue you would like to work on, please leave a comment and we will be happy to assist. Questions can also be sent to the WFC3 team through the [HST Help Desk](https://stsci.service-now.com/hst).
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WFC3 Notebooks follows the
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WFC3 Notebooks follow the
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[Astropy Code of Conduct](https://www.astropy.org/code_of_conduct.html)
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and strives to provide a welcoming community to all of our users and
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contributors.
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Want more information about how to make a contribution? Take a look at
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the the `astropy`
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the `astropy`
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[contributing](https://www.astropy.org/contribute.html)
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and [developer](https://docs.astropy.org/en/stable/index.html#developer-documentation)
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documentation.

_sources/notebooks/WFC3/general_tools.md

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sufficiently dithered to step over the observed persistence artifacts,
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AstroDrizzle may be used to exclude those flagged pixels when combining the FLT
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## Analyzing WFC3/UVIS G280 Exoplanet Transit Observations
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We present the reduction and analysis of exoplanet transit observations of the
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hot Jupiter HAT-P-41b taken with the WFC3/UVIS G280 grism. The notebook
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demonstrates source finding, background subtraction, cosmic ray rejection,
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subarray embedding, spectral trace fitting, spectum extraction, and light curve
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generation.
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![STScI Logo](../../_static/stsci_header.png)
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# Grism Spectroscopy
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Here are brief descriptions of the WFC3 Notebooks for grism spectroscopy
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analysis.
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## Analyzing WFC3/UVIS G280 Exoplanet Transit Observations
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We present the reduction and analysis of exoplanet transit observations of the
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hot Jupiter HAT-P-41b taken with the WFC3/UVIS G280 grism. The notebook
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demonstrates source finding, background subtraction, cosmic ray rejection,
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subarray embedding, spectral trace fitting, spectrum extraction, and light curve
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generation.
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## Slitlessutils Cookbook: Spectral Extraction for WFC3/IR
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This notebook demonstrates an end-to-end workflow for extracting 1D spectra from
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G102 or G141 data using `slitlessutils`. This example guides users through the
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recommended procedure for analyzing slitless data, including downloading data,
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preparing direct and dispersed images, performing background subtraction, and
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executing the traditional extraction mode.
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## Slitlessutils Cookbook: Spectral Extraction for WFC3/UVIS Full-Frame
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This notebook demonstrates an end-to-end workflow for extracting 1D spectra from
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G280 full-frame data using `slitlessutils`. This example guides users through the
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recommended procedure for analyzing slitless data, including downloading data,
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preparing direct and dispersed images, performing background subtraction, and
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executing the traditional extraction mode.
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## Slitlessutils Cookbook: Spectral Extraction for WFC3/UVIS Subarray
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This notebook demonstrates an end-to-end workflow for extracting 1D spectra from
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G280 subarray data using `slitlessutils`. This example guides users through the
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recommended procedure for analyzing slitless data, including downloading data,
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preparing direct and dispersed images, performing background subtraction, and
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executing the traditional extraction mode.

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