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Update allwise to best practices and follow template
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---
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jupytext:
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text_representation:
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extension: .md
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format_name: myst
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format_version: 0.13
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jupytext_version: 1.19.1
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kernelspec:
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name: python3
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display_name: python3
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language: python
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---
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# Searching for AllWISE Atlas Images
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## Learning Goals
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By the end of this tutorial, you will:
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* Learn how to access IRSA's WISE AllWISE Atlas (L3a) coadded images via the Simple Image Access (SIA) service.
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* identify which of IRSA's AllWISE Atlas images cover a specified coordinate.
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* Visualize one of the identified images using Forefly.
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* Create and display a cutout of the downloaded image.
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## Introduction
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The AllWISE program builds upon the work of the successful Wide-field Infrared Survey Explorer mission [(WISE; Wright et al. 2010)](http://adsabs.harvard.edu/abs/2010AJ....140.1868W) by combining data from the WISE cryogenic and NEOWISE [(Mainzer et al. 2011 ApJ, 731, 53)](http://adsabs.harvard.edu/abs/2011ApJ...731...53M) post-cryogenic survey phases to form the a comprehensive view of the full mid-infrared sky. The AllWISE Images Atlas is comprised of 18,240 4-band calibrated 1.56°x1.56° FITS images, depth-of-coverage and noise maps, and image metadata produced by coadding nearly 7.9 million Single-exposure images from all survey phases. For more information about the WISE mission, see:
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https://irsa.ipac.caltech.edu/Missions/wise.html
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The [NASA/IPAC Infrared Science Archive (IRSA)](https://irsa.ipac.caltech.edu) at Caltech is the archive for AllWISE images and catalogs. The AllWISE Atlas images that are the subject of this tutorial are made accessible via the [International Virtual Observatory Alliance (IVOA)](https://ivoa.net) [Simple Image Access (SIA)](https://wiki.ivoa.net/internal/IVOA/SiaInterface/SIA-V2-Analysis.pdf) protocol.
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```{note}
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IRSA supports both SIA v1 and SIA v2 protocols. The version used depends on the specific dataset. This IRSA [website](https://irsa.ipac.caltech.edu/ibe/sia.html) provides information on which version each service uses and how to access them. Further information on how to access IRSA data with different techniques is available [here](https://irsa.ipac.caltech.edu/docs/program_interface/api_images.html)
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```
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## Imports
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- `astropy.coordinates` for defining coordinates
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- `astropy.nddata` for creating an image cutout
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- `astropy.wcs` for interpreting the World Coordinate System header keywords of a fits file
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- `astropy.units` for attaching units to numbers passed to the SIA service
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- `matplotlib.pyplot` for plotting
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- `astropy.io` to manipulate FITS files
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- `firefly_client` for visuzlizing images
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- `astroquery/ipac.irsa` for data access
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```{code-cell} ipython3
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# Uncomment the next line to install dependencies if needed.
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%pip install matplotlib astropy jupyter_firefly_extensions
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```
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```{code-cell} ipython3
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from astropy.coordinates import SkyCoord
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from astropy.nddata import Cutout2D
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from astropy.wcs import WCS
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import astropy.units as u
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import matplotlib.pyplot as plt
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from astropy.io import fits
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from firefly_client import FireflyClient
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from astroquery.ipac.irsa import Irsa
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```
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## 1. Define the target
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Define coordinates of a bright star
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```{code-cell} ipython3
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ra = 314.30417
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dec = 77.595559
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pos = SkyCoord(ra=ra, dec=dec, unit='deg')
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```
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## 2. Discover AllWISE Atlas images
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IRSA provides Simple Image Access (SIA) services for various datasets. A list of available datasets and their access URLs can be found at:
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https://irsa.ipac.caltech.edu/ibe/sia.html
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This tutorial uses SIA v2 for AllWISE Atlas images.
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```{code-cell} ipython3
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names = Irsa.list_collections(filter="allwise")
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names
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# We see from the resulting table that the dataset collection we are interested in is called "wise_allwise"
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```
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## 3. Search for images
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```{code-cell} ipython3
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#get a table of all images within 1 arcsecond of our target position
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dataset_name = names['collection'][0]
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im_table = Irsa.query_sia(pos=(pos, 1 * u.arcsec), collection=dataset_name)
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```
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Inspect the table that is returned
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```{code-cell} ipython3
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im_table
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```
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```{code-cell} ipython3
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im_table.colnames
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```
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```{code-cell} ipython3
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# Let's look at the values in one of the columns
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im_table['energy_bandpassname']
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```
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## 4.Locate and visualize an image of interest
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Let's search the image results for the W3 band image.
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```{code-cell} ipython3
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# You can put the URL from the column "access_url" into a browser to download the file.
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# Or you can work with it in Python, as shown below.
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w3_mask = im_table['energy_bandpassname'] == 'W3'
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w3_table = im_table[w3_mask]
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# Lets look at the access_url of the first one:
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image_url = w3_table['access_url'][0]
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image_url
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```
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```{code-cell} ipython3
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#Use Astropy to examine the header of the URL from the previous step.
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hdulist = fits.open(image_url)
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hdulist.info()
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```
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Download the image and open it in Astropy
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```{code-cell} ipython3
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## 7. Visualize a SPHEREx Spectral Image MEF using the Firefly Python Client.
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# We will use the open-source astronomy data visualization software Firefly.
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# Firefly has a Python client.
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#Open a Firefly viewer in a tab within jupyterlab.
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fc = FireflyClient.make_client(url="https://irsa.ipac.caltech.edu/irsaviewer")
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fc = FireflyClient.make_lab_client()
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# Visualize an image by sending its URL to the viewer.
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fc.show_fits_image(file_input=image_url,
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plot_id="image",
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Title="Image"
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)
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#Try use the interactive tools in the viewer to explore the data.
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```
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## 5. Extract a cutout and plot it
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```{code-cell} ipython3
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data = hdulist[0].data
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wcs = WCS(hdulist[0].header)
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# make 1' x 1' cutout
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cutout = Cutout2D(data, position=pos, size=1 * u.arcmin, wcs=wcs)
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# display
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plt.figure()
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plt.imshow(cutout.data, origin='lower')
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plt.colorbar()
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```
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***
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## Acknowledgements
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- [Caltech/IPAC-IRSA](https://irsa.ipac.caltech.edu/)
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## About this notebook
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## About this notebook
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**Authors:** IRSA Data Science Team, including Troy Raen, Brigitta Sipőcz, Jessica Krick, Andreas Faisst, Jaladh Singhal, Vandana Desai, Dave Shupe
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**Updated:** 16 February 2026
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**Contact:** [IRSA Helpdesk](https://irsa.ipac.caltech.edu/docs/help_desk.html) with questions or problems.
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**Runtime:** As of the date above, this notebook takes about 20 seconds to run to completion on a machine with 8GB RAM and 4 CPU.
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This runtime is dependent on archive servers which means runtime will vary for users.
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## Citations
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If you use `astropy` for published research, please cite the authors. Follow these links for more information about citing `astropy`:
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* [Citing `astropy`](https://www.astropy.org/acknowledging.html)
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Please include the following in any published material that makes use of the WISE data products:
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"This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration."
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Please also cite the dataset Digital Object Identifier (DOI): [10.26131/IRSA153](https://www.ipac.caltech.edu/doi/irsa/10.26131/IRSA153)

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