DOI: 10.5281/zenodo.15106473
title: Euclid Quick Data Release (Q1): First visual morphology catalogue

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:



df['file_loc'] = df['tile_index'].astype(str) + '_' + df['object_id'].astype(str).str.replace('-', 'NEG') + '_.jpg'

 

Cutouts...tar has images of every galaxy, as shown to the model. These are the VIS+Y images also shown to the volunteers. 

 

Volunteers were also able to inspect two other processing versions. Fig 3 in the Q1 visual morphology paper shows an example galaxy in all three versions. Only the VIS+Y images are included here for now.

 


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.