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## Images
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-[MER Mosaics](1_Euclid_intro_MER_images.md) — Retrieve both a full MER mosaic image and multi-wavelength cutouts, then subtract the background from the cutouts and extract sources.
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```{card}
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:link: 1_Euclid_intro_MER_images.md
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:header: **MER Mosaics**
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Retrieve both a full MER mosaic image and multi-wavelength cutouts, then subtract the background from the cutouts and extract sources.
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```
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## Spectra
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-[SIR 1D Spectra](3_Euclid_intro_1D_spectra.md) — Load a galaxy spectrum and plot it. Understand the wavelength, flux, and mask values.
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```{card}
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:link: 3_Euclid_intro_1D_spectra.md
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:header: **SIR 1D Spectra**
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Load a galaxy spectrum and plot it. Understand the wavelength, flux, and mask values.
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```
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## Catalogs
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-[MER Catalogs](2_Euclid_intro_MER_catalog.md) — Explore the columns in the MER final catalog, query for stars, and create a color-magnitude diagram.
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-[PHZ Catalogs](4_Euclid_intro_PHZ_catalog.md) — Join the PHZ and MER catalogs and do a box search for galaxies with quality redshifts, load a MER mosaic cutout of the box, and plot the cutout with the catalog results overlaid.
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Then plot the SIR spectrum of the brightest galaxy and look at a MER mosaic cutout of the galaxy in Firefly.
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-[SPE Catalogs](5_Euclid_intro_SPE_catalog.md) — Join the SPE and MER catalogs and query for galaxies with H-alpha line detections, then plot the SIR spectrum of a galaxy with a high SNR H-alpha line measurement.
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-**Merged Objects HATS Catalog** — This product was created by IRSA and contains the Euclid MER, PHZ, and SPE catalogs in a single [HATS](https://hats.readthedocs.io/en/latest/) catalog.
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-[Introduction](../parquet-catalog-demos/euclid-q1-hats/1-euclid-q1-hats-intro.md) — Understand the content and format of the Euclid Q1 Merged Objects HATS Catalog, then perform a basic query.
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-[Magnitudes](../parquet-catalog-demos/euclid-q1-hats/4-euclid-q1-hats-magnitudes.md) — 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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````{grid} 1 1 2 2
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```{card}
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:link: 2_Euclid_intro_MER_catalog.md
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:header: **MER Catalogs**
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Explore the columns in the MER final catalog, query for stars, and create a color-magnitude diagram.
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```
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```{card}
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:link: 5_Euclid_intro_SPE_catalog.md
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:header: **SPE Catalogs**
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Join the SPE and MER catalogs and query for galaxies with H-alpha line detections, then plot the SIR spectrum of a galaxy with a high SNR H-alpha line measurement.
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```
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```{card}
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:link: 4_Euclid_intro_PHZ_catalog.md
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:header: **PHZ Catalogs**
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Join the PHZ and MER catalogs and do a box search for galaxies with quality redshifts, load a MER mosaic cutout of the box, and plot the cutout with the catalog results overlaid.
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Then plot the SIR spectrum of the brightest galaxy and look at a MER mosaic cutout of the galaxy in Firefly.
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```
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````
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### Merged Objects HATS Catalog
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This product was created by IRSA and contains the Euclid MER, PHZ, and SPE catalogs in a single [HATS](https://hats.readthedocs.io/en/latest/) catalog.
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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```
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````
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## Special Topics
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-[Cloud Access](../cloud_access/euclid-cloud-access.md) — Browse the on-cloud copy of Q1, then efficiently retrieve a MER mosaic cutout and a SIR spectrum.
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-[Early Release Observations (ERO) - Star Clusters](Euclid_ERO.md) (deprecated; ERO is superseded by Q1) — Create multi-wavelength ERO image cutouts of a globular cluster, extract sources, and measure photometry.
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Then load Gaia sources at the location of the globular cluster, match with Euclid ERO catalogs, and visualize the results with Firefly.
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````{grid} 1 1 2 2
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```{card}
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:link: ../cloud_access/euclid-cloud-access.md
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:header: **Cloud Access**
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Browse the on-cloud copy of Q1, then efficiently retrieve a MER mosaic cutout and a SIR spectrum.
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```
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```{card}
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:link: Euclid_ERO.md
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:header: **ERO Star Clusters**
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[*Deprecated; ERO is superseded by Q1*] Create multi-wavelength ERO (Early Release Observations) image cutouts of a globular cluster, extract sources, and measure photometry.
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Then load Gaia sources at the location of the globular cluster, match with Euclid ERO catalogs, and visualize the results with Firefly.
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