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Copy file name to clipboardExpand all lines: tutorials/euclid_access/euclid.md
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@@ -6,6 +6,11 @@ It carries two instruments: the VISible instrument (VIS) and the Near-Infrared S
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[Quick Release 1 (Q1)](https://irsa.ipac.caltech.edu/data/Euclid/docs/overview_q1.html) was released in March 2025 and consists of approximately 35 TB of imaging, spectroscopy, and catalogs, covering four non-contiguous fields totaling 63 square degrees.
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Data products include MERged mosaics of calibrated and stacked frames; combined infrared spectra (SIR); and catalogs of MER objects, photometric redshifts and classifications (PHZ), and spectroscopic redshifts and line measurements (SPE).
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Data products include:
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- MER (merged) mosaic images of calibrated and stacked frames;
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- SIR combined infrared spectra;
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- Catalogs of MER objects, photometric redshifts and classifications (PHZ), and spectroscopic redshifts and line measurements (SPE);
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- Merged Objects Catalog (created by IRSA) containing the MER, PHZ, and SPE catalogs in a single HATS Catalog.
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Explore the columns in the MER final catalog, query for stars, and create a color-magnitude diagram.
Join the PHZ and MER catalogs to query galaxies with quality redshifts in a box region, create MER mosaic cutouts with catalog overlays, and plot the brightest galaxy's SIR spectrum.
Introduction: Understand the content and format of the Euclid Q1 Merged Objects HATS Catalog, then perform a basic query.
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Join the PHZ and MER catalogs to query galaxies with quality redshifts in a box region, create MER mosaic cutouts with catalog overlays, and plot the brightest galaxy's SIR spectrum.
Magnitudes: Review the types of flux measurements available, load template-fit and aperture magnitudes, and plot distributions and comparisons for different object types.
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```{card}
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Create multi-wavelength ERO image cutouts of a globular cluster, extract sources, and measure photometry. Match Gaia sources with Euclid ERO catalogs, then visualize with Firefly.
Review the types of flux measurements available, load template-fit and aperture magnitudes, and plot distributions and comparisons for different object types.
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