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Use SpectrumDM service in 5_Euclid_intro_SPE_catalog.md
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tutorials/euclid_access/5_Euclid_intro_SPE_catalog.md

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@@ -159,7 +159,7 @@ We specify the following conditions on our search:
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- Signal to noise ratio column (_gf = gaussian fit) should be greater than 5
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- We want to detect H-alpha.
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- We choose in which tileID to search, usign the tileID from the first notebook.
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- Choose spectroscopic redshift (spe_z) beween 1.4 and 1.6 and spe_z_prob greater than 0.999
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- Choose spectroscopic redshift (spe_z) between 1.4 and 1.6 and spe_z_prob greater than 0.999
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- H-alpha line flux should be more than 2x10^16 erg s^-1 cm^-2
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- Join the lines and galaxy candidates tables on object_id and spe_rank
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@@ -208,23 +208,19 @@ result_table2 = Irsa.query_tap(adql_object).to_qtable()
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### The following steps to read in the spectrum follows the 3_Euclid_intro_1D_spectra notebook.
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This involves reading in the spectrum without readin in the full FITS file, just pulling the extension we want.
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```{code-cell} ipython3
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file_uri = urllib.parse.urljoin(Irsa.tap_url, result_table2['uri'][0])
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file_uri
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spectrum_path = urllib.parse.urljoin(Irsa.tap_url, result_table2['path'][0])
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spectrum_path
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```
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```{code-cell} ipython3
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with fits.open(file_uri) as hdul:
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spectrum = QTable.read(hdul[result_table2['hdu'][0]], format='fits')
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spec_header = hdul[result_table2['hdu'][0]].header
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spectrum = QTable.read(spectrum_path)
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```
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### Now the data are read in, plot the spectrum with the H-alpha line labeled
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```{tip}
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As we use astropy.visualization's ``quantity_support``, matplotlib automatically picks up the axis units from the quantitites we plot.
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As we use astropy.visualization's ``quantity_support``, matplotlib automatically picks up the axis units from the quantities we plot.
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```
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```{code-cell} ipython3
@@ -248,8 +244,8 @@ plt.title(f'Object ID {obj_id}')
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## About this Notebook
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**Author**: Tiffany Meshkat, Anahita Alavi, Anastasia Laity, Andreas Faisst, Brigitta Sipőcz, Dan Masters, Harry Teplitz, Jaladh Singhal, Shoubaneh Hemmati, Vandana Desai
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**Author**: Tiffany Meshkat, Anahita Alavi, Anastasia Laity, Andreas Faisst, Brigitta Sipőcz, Dan Masters, Harry Teplitz, Jaladh Singhal, Shoubaneh Hemmati, Vandana Desai, Troy Raen
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**Updated**: 2025-03-31
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**Updated**: 2025-09-23
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**Contact:** [the IRSA Helpdesk](https://irsa.ipac.caltech.edu/docs/help_desk.html) with questions or reporting problems.

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