Euclid data release: Q1

Euclid has a number of planned data releases to the world. The first one is the “Quick Data Release 1” or Q1 for short, that released 63.1 deg² of wide-survey science data on 19 March 2025. This release, containing approximately 26 million detections, is not a cosmology release but primarily aimed at a variety of astrophysical studies, providing VIS and NISP images, NISP spectroscopy, external ground-based data, catalogues, and masks. A total or seven technical publications and a supplement describe the content of the release. An overview is given in Euclid Collaboration: Aussel et al., 2025, “Euclid Quick Data Release (Q1) – Data release overview”. A constantly updated list of Q1 reference and science papers is given below. Complete information is available at ESA’s Q1 data release page, with a detailed description in the release’s Explanatory Supplement, and with a specific pointer to the Release Notes.

Basic data release information

Fields
Layout of the Q1 are covered (squares) and the future Euclid Deep Survey area (blue line). Source: EC: Aussel et al. (2025), Fig. 1
FieldQ1 area
[deg²]
DR3-depth area [deg²]RA
[deg]
Dec
[deg]
λ
[deg]
β
[deg]
DR3 visits
EDF-N22.920269.733+66.018258.690+89.44640
EDF-S28.12361.241–48.42336.493–66.59945
EDF-F12.11052.932–28.08840.772–45.39752
DC0.585.75–8.36785.05–31.73317 (Q1)

DC is the `Dark Cloud’, Lynd’s Catalogue of Dark Nebulae (LDN) 1641 in Orion A, observed as a guiding calibration field during Euclid commissioning.

Data products released
  • VIS and NISP calibrated single epoch image and 2d spectra frames
  • Merged (MER) mosaics stacked tiles of VIS and NISP images
  • Ground-based EXTernal calibrated Euclid images as MER stacked tiles in the g, r, i, and z bands
  • NISP calibrated coadded 1d spectra
  • Spectroscopic redshift catalogues
  • Catalogues of detections based on VIS with information in all bands
  • Masks for RMS, sky coverage, point-spread-functions, and more
Data access

Q1 data can be accessed through ESA’s Euclid Science Archive (https://eas.esac.esa.int/sas) where catalogues can be queried and a cutout service is available.

These data are also available through Python with the Euclid astroquery toolkit. Due to the large size of the FITS files we promote the use of the ESA Datalabs platform (https://datalabs.esa.int).

A subset of the data can be accessed through ESA Sky (https://sky.esa.int).

The data and their structure are described in the Q1 Data Product Description Document (DPDD).

A small cutout of the Dark Cloud, here in the center HOPS 221, a young stellar object with prominent outflows. The field is 7 arcmin wide. Source: EC: Aussel et al. (2025), Fig. 3

Q1 publications

Euclid Q1 overview, data products and processing:
Scientific results using Euclid Q1 data:

Updated: 2025-04-02, KJ