This work presents results from the European Space Agency (ESA) space mission Euclid. Euclid data are being processed by the Euclid Consortium.
The Euclid Consortium acknowledges the European Space Agency and a num- ber of agencies and institutes that have supported the development of Euclid, in particular the Agenzia Spaziale Italiana, the Austrian Forschungsförderungsgesellschaft funded through BMK, the Belgian Science Policy, the Canadian Euclid Consortium, the Deutsches Zentrum für Luft- und Raumfahrt, the DTU Space and the Niels Bohr Institute in Denmark, the French Centre National d’Etudes Spatiales, the Fundação para a Ciência e a Tecnologia, the Hungarian Academy of Sciences, the Ministerio de Ciencia, Innovación y Universidades, the National Aeronautics and Space Administration, the National Astronomical Observatory of Japan, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Research Council of Finland, the Romanian Space Agency, the State Secretariat for Education, Research, and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and de- tailed list is available on the Euclid web site www.euclid-ec.org/
The Euclid mission website is https://www.cosmos.esa.int/euclid. The Euclid archive website is https://eas.esac.esa.int/sas/.
Based on data from UNIONS, a scientific collaboration using three Hawaii-based telescopes: CFHT, Pan-STARRS and Subaru www.skysurvey.cc
This work is also based on
data from the Dark Energy Camera (DECam) on the Blanco 4-m Telescope
at CTIO in Chile https://www.darkenergysurvey.org.
This work uses results from the ESA mission Gaia,
whose data are being processed by the Gaia Data Processing and
Analysis Consortium https://www.cosmos.esa.int/gaia
We are honoured and grateful for the opportunity of observing the Universe from Maunakea and Haleakala, which both have cultural, historical, and natural significance in Hawaii.
In case of errors or omissions, please contact the Euclid Helpdesk.