Euclid Quick Data Release (Q1): First visual morphology catalogue
Authors/Creators
Contributors
Research groups:
Description
Interactive visualiser at euclid.streamlit.app.
Contents
- Catalogue (
morphology_catalog.csv/parquet)- List of ID columns and morphology columns
- List of morphology questions and answers available
- List of additional columns copied from MER (flux, ellipticity, area, etc.)
- Extra physical measurements (
extra_physical_measurements.parquet)
- Images (
cutouts...tar)
Full documentation is available here. Below is a summary.
1. Catalogue (morphology_catalog.csv/parquet)
The morphology catalogue covers galaxies which are either bright or extended. Specifically, it includes galaxies matching one of the following criteria:
- segmentation area > 700 pixels, or...
- VIS < 20.5 AND segmentation area > 200 pixels
The measurements were made by Zoobot foundation models, finetuned on Euclid galaxies using the responses of Galaxy Zoo volunteers.
Our models were trained using galaxies from the selection cuts above but with the first option requiring 1200 pixels. Therefore, galaxies between 700 and 1200 pixels in area are may have less reliable measurements.
The catalogue file is morphology_catalogue (.parquet or .csv, the contents are identical). It includes the following columns:
| release_name | Always Q1_R1, for now |
| tile_index | Euclid tile index i.e. which MER tile hosts this galaxy |
| object_id | Euclid object id i.e. the MER catalogue identifier for this galaxy |
| segmentation_map_id | Alternative Euclid identifier. The first 9 digits are the tile index, the other digits match the internal segmentation id of the source. |
| right_ascension | in degrees, from the MER catalogue |
| declination | in degrees, from the MER catalogue |
| {question}_{answer}_fraction | e.g. smooth-or-featured_smooth_fraction. The fraction of volunteers expected to give this answer to this morphology question. Probably the morphology columns you want. |
| {question}_{answer}_dirichlet | e.g. smooth-or-featured_smooth_dirichlet. The concentration for a Dirichlet distribution (useful for uncertainties). See the paper. |
| warning_galaxy_fails_training_cuts | Marks galaxies between 700px and 1200px, where performance may be lower. See above. |
| cutout_width_arcsec | Width (and height) of cutout in arcseconds |
The following questions and answers are available.
| Question | Answer | Notes |
| smooth-or-featured | smooth | May include face-on lenticulars, which are better identified with e.g. Sersic indices |
| how-rounded | round | |
| how-rounded | in-between | |
| how-rounded | cigar-shaped | |
| smooth-or-featured | featured-or-disk | The question branch most commonly used by researchers |
| disk-edge-on | yes | |
| edge-on-bulge | boxy | |
| edge-on-bulge | none | |
| edge-on-bulge | rounded | |
| disk-edge-on | no | |
| has-spiral-arms | yes | |
| spiral-winding | tight | |
| spiral-winding | medium | |
| spiral-winding | loose | |
| spiral-arm-count | 1 | |
| spiral-arm-count | 2 | |
| spiral-arm-count | 3 | |
| spiral-arm-count | 4 | |
| spiral-arm-count | more-than-4 | Often overlaps with cant-tell |
| spiral-arm-count | cant-tell | Often overlaps with more-than-4 |
| has-spiral-arms | no | |
| bar | strong | Bar strength is a mix of length and width |
| bar | weak | |
| bar | no | |
| bulge-size | dominant | |
| bulge-size | large | |
| bulge-size | moderate | |
| bulge-size | small | |
| bulge-size | none | |
| smooth-or-featured | problem | |
| problem | star | |
| problem | zoom | i.e. bad zoom, a cutout which is too wide |
| problem | artifact | |
| artifact | satellite | |
| artifact | scattered | |
| artifact | diffraction | |
| artifact | ray | |
| artifact | saturation | |
| artifact | other | |
| artifact | ghost | Dichrotic ghosts |
| merging | none | |
| merging | minor_disturbance | |
| merging | major_disturbance | Primarily obvious tidal tails and similar features |
| merging | merger | Primarily "dramatic" ongoing mergers |
| clumps | yes | Not recommended; we are building clump-specific models |
| clumps | no | Not recommended; we are building clump-specific models |
For convenience, we have also copied over some useful MER catalogue columns. The schema for the full MER catalogue is here. Additionally, Euclid also makes available many other tables with e.g. photometric redshifts, estimated masses, etc. These are documented here. All fluxes are in micro-janskies (uJy).
| segmentation_area | Number of pixels included in SourceExtractor++ mask of galaxy (0.1 arcsec/pixel). |
| flux_segmentation | Total VIS flux inside the segmentation mask above. |
| mag_segmentation | As above, converted to magnitude. ```mag = -2.5*log10(flux[muJy])+23.9```. Not technically in MER catalogue. |
| flux_detection_total | VIS flux measured within a Kron aperture in the detection image. FLUX_AUTO in SourceExtractor. |
| flux_vis_1fwhm_aper | VIS flux within an aperture of radius 1 FWHM. |
| mumax_minus_mag | A star/galaxy diagnostic. The morphology catalogue uses the recommended filter MUMAX_MINUS_MAG>=-2.6 to reject stars. |
| mu_max | Peak surface brightness above the background in the detection band (directly from SExtractor) |
| ellipticity | A parametrization of how stretched an object is in the detection band (VIS, here), computed from the minor and major axes of the object itself (directly from SExtractor). [I assume this is the major/minor axis ratio] |
| kron_radius | Major semi-axis (in pixels) of the elliptical aperture used for total (Kron) aperture photometry on the detection image |
1b Useful Physical Measurements (useful_physical_measurements.parquet)
(added 29th March 2025)
People often want to combine morphology with physical measurements like redshift, stellar mass, etc. This table includes these columns. You can cross-match to the morphology catalog using object_id.
The columns are copied from the Science Archive Service database and are grouped by the origin table. They are:
MER columns (flux, shape)
MER morphology columns (CAS, Gini, Sersic profiles)
PHZ (Photometric redshift)
PP ("p"hysical "p"arameters inc. stellar mass, star formation rate, luminosity, an alternative photometric redshift)
Below is a full schema. The descriptions are summarised from the Q1 Data Product Description Document.
| flux_detection_total | |
| flux_y_1fwhm_aper |
Y (Euclid) equivalent of flux_vis_1fwhm_aper, above |
| flux_j_1fwhm_aper |
J (Euclid) equivalent of flux_vis_1fwhm_aper, above |
| flux_h_1fwhm_aper | H (Euclid) equivalent of flux_vis_1fwhm_aper, above |
| flux_i_ext_decam_1fwhm_aper | I (DECam, ground-based) equivalent of flux_vis_1fwhm_aper, above. Only filled where Legacy Survey DECam observations are available. |
| flux_r_ext_decam_1fwhm_aper | R (DECam, ground-based) equivalent of flux_vis_1fwhm_aper, above. Only filled where Legacy Survey DECam observations are available. |
| flux_g_ext_decam_1fwhm_aper | G (DECam, ground-based) equivalent of flux_vis_1fwhm_aper, above. Only filled where Legacy Survey DECam observations are available. |
| flux_z_ext_decam_1fwhm_aper | Z (DECam, ground-based) equivalent of flux_vis_1fwhm_aper, above. Only filled where Legacy Survey DECam observations are available. |
|
semimajor_axis |
Semi-major axis of the ellipse describing the object shape, in pixels |
|
position_angle |
Position angle of the ellipse describing the object shape, in degrees and using a counter-clockwise NE-SW convention; |
|
det_quality_flag |
|
|
concentration |
C of CAS. As in Conselice 2003 (cite papers within this review). |
|
asymmetry |
A of CAS. As in Conselice 2003 (cite papers within this review). |
|
smoothness |
S of CAS. As in Conselice 2003 (cite papers within this review). |
|
gini |
Measure of light concentration, in analogy to wealth concentration in an economy. See Lotz, Primack & Madau 2004. |
|
moment_20 |
aka M20. See Lotz, Primack & Madau 2004. |
|
sersic_sersic_vis_index |
From SourceExtractor++. See Quilley 2025. |
|
sersic_visnir_flags |
"Flags from the VISNIR fit" |
|
phz_median |
Redshift from PHZ (nearest neighbour matching with "NNPZ" code). Recommended (better match to DESI spec-z). |
|
phz_flags |
0 => OK, 1 => NNPZ flag: no close neighbor, 10 not VIS detected, 11 missing band, 12 too faint |
|
phz_pp_median_redshift |
Redshift from physical parameter fit. Not recommended (worse match to DESI spec-z). |
|
phz_pp_median_stellarmass |
Stellar mass from physical parameter fit. In log10(stellar mass in solar masses) |
|
phys_param_flags |
"A 64 bit integer containing the flags of the physical parameters processing (TBD)" |
|
phz_pp_median_luminosity |
Luminosity from physical parameter fit? Not documented. |
|
phz_pp_median_sfr |
Star formation rate from physical parameter fit. In log10(stellar mass in solar masses) |
object_id, right_ascension, declination
2. Images
We are sharing the original cutout images as shown to Galaxy Zoo volunteers. The images are named like {tile_index}_{object_id}.jpg, where the negative sign ('-') in object id is replaced with 'NEG' to avoid path issues. You can construct the file paths from the morphology catalogue. For example:
The VIS+Y images are composites with VIS in the blue channel and Y in the red channel (and the median of VIS and Y in the green channel, but this isn't visible). They use an arcinsh stretch, with the stretch designed to balance the contribution from each band.
The VIS only images are black-and-white, and also use an arcsinh stretch.
The VIS LSB images use a more complicated stretch to highlight LSB features. This is not included yet on Zenodo.
Full details of the image processing are in the Q1 visual morphology paper.
Files
morphology_catalogue.csv
Files
(8.7 GB)
| Name | Size | Download all |
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md5:1acad78f1e9883e765beff508233894d
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3.7 GB | Download |
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md5:4cec21cfb799c1861ea9701bed5a8980
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3.8 GB | Download |
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md5:652e4546c63085c37539a9e9664f64e2
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601.4 MB | Preview Download |
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md5:79e7880d5989e05ec23205782c30025a
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97.3 MB | Download |
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md5:d007c08ccb52450d542eca13591118bf
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337.8 MB | Download |
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md5:a43e3edfe6df3ef0ad9bd10da67d3dae
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138.6 MB | Download |
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md5:2bdaea95a50fdddbccbff2e7b1a05996
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67.7 MB | Download |
Additional details
Dates
- Available
-
2025-03-19Initial public release
Software
- Programming language
- Python