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tutorials/notebooks/FITS-cubes/FITS-cubes.ipynb

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"\n",
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"This tutorial will walk you though a simple visual analysis of the Small Magellanic Cloud (SMC) using HI 21cm emission and a Herschel 250 micron map. We will learn how to read in data from vizier, query and download matching data from Herschel using astroquery, and plot the resulting images in a multitude of ways. \n",
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"\n",
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"The primary libraries we will be using are: [astroquery](http://www.astropy.org/astroquery/), [spectral_cube](https://spectral-cube.readthedocs.io/en/latest/), [reproject](https://reproject.readthedocs.io/en/stable/#), [matplotlib](https://matplotlib.org/), and [aplpy](https://aplpy.github.io/)) They can be installed using conda and pip:\n",
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"The primary libraries we will be using are: [astroquery](http://www.astropy.org/astroquery/), [spectral_cube](https://spectral-cube.readthedocs.io/en/latest/), [reproject](https://reproject.readthedocs.io/en/stable/#), [matplotlib](https://matplotlib.org/), and [aplpy](https://aplpy.github.io/)) \n",
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"\n",
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"They can be installed using conda:\n",
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"- `conda install -c astropy astroquery`\n",
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"- `conda install spectral-cube`\n",
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"- `conda install reproject`\n",
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"- `conda install aplpy`"
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"- `conda install -c astropy spectral-cube`\n",
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"- `conda install -c astropy reproject`\n",
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"- `conda install -c astropy aplpy`\n",
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"\n",
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"Alternatively, if you don't use conda, you can use pip."
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]
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},
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{
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"ax.set_ylim(y_lim)"
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]
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},
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{
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"cell_type": "markdown",
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"metadata": {},
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"source": [
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"## Add some TRY and CHALLENGE items here to wrap things up"
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]
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},
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{
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"cell_type": "markdown",
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"metadata": {
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"The real power of reproject is in actually changing the map projection used to display the data. This is done by creating a WCS object that contains a different projection type such as `CTYPE : 'RA---CAR' 'DEC--CAR'` as opposed to `CTYPE : 'RA---TAN' 'DEC--TAN'`. \n",
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"\n",
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"## Challenge:\n",
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"### Use [reproject](https://reproject.readthedocs.io/en/stable/#) and WCS to create a new WCS object in a different map projection and see distortions in the image can change. "
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"\n",
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"Use [reproject](https://reproject.readthedocs.io/en/stable/#) and WCS to create a new WCS object in a different map projection and see distortions in the image can change. "
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]
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],
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"metadata": {
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"kernelspec": {
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"display_name": "Python [default]",
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"display_name": "Python 2",
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"language": "python",
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"name": "python3"
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"name": "python2"
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},
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"language_info": {
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"codemirror_mode": {
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"name": "ipython",
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"version": 3
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"version": 2
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},
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"file_extension": ".py",
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"mimetype": "text/x-python",
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"name": "python",
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"nbconvert_exporter": "python",
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"pygments_lexer": "ipython3",
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"version": "3.6.2"
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"pygments_lexer": "ipython2",
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"version": "2.7.13"
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}
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},
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"nbformat": 4,

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