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Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission

Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
We present the Flagship galaxy mock, a simulated catalogue of billions of galaxies designed to support the scientific exploitation of the Euclid mission. Euclid is a medium-class mission of the European Space Agency optimised to determine the properties of dark matter and dark energy on the largest scales of the Universe. It probes structure formation over more than 10 billion years primarily from the combination of weak gravitational lensing and galaxy clustering data. The breadth of Euclid’s data will also foster a wide variety of scientific analyses. The Flagship simulation was developed to provide a realistic approximation to the galaxies that will be observed by Euclid and used in its scientific exploitation. We ran a state-of-the-art N-body simulation with four trillion particles, producing a lightcone on the fly. From the dark matter particles, we produced a catalogue of 16 billion haloes in one octant of the sky in the lightcone up to redshift z = 3. We then populated these haloes with mock galaxies using a halo occupation distribution and abundance-matching approach, calibrating the free parameters of the galaxy mock against observed correlations and other basic galaxy properties. Modelled galaxy properties include luminosity and flux in several bands, redshifts, positions and velocities, spectral energy distributions, shapes and sizes, stellar masses, star formation rates, metallicities, emission line fluxes, and lensing properties. We selected a final sample of 3.4 billion galaxies with a magnitude cut of HE < 26, where we are complete. We have performed a comprehensive set of validation tests to check the similarity to observational data and theoretical models. In particular, our catalogue is able to closely reproduce the main characteristics of the weak lensing and galaxy clustering samples to be used in the mission main cosmological analysis. Moreover, given its depth and completeness, this new galaxy mock also provides the community with a powerful tool for developing a wide range of scientific analyses beyond the Euclid mission.
astro-ph.CO, galaxies: evolution, catalogs, large-scale structure of Universe, cosmology: observations, gravitational lensing: weak
0004-6361
Castander, F.J.
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Fosalba, P.
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Stadel, J.
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Potter, D.
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Carretero, J.
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Tallada-Crespí, P.
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Pozzetti, L.
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Bolzonella, M.
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Mamon, G.A.
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Blot, L.
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Hoffmann, K.
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Huertas-Company, M.
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Monaco, P.
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Gonzalez, E.J.
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Lucia, G. De
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Scarlata, C.
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Breton, M.-A.
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Linke, L.
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Viglione, C.
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Li, S.-S.
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Zhai, Z.
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Baghkhani, Z.
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Pardede, K.
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Neissner, C.
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Teyssier, R.
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Crocce, M.
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Tutusaus, I.
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Miller, L.
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Congedo, G.
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Biviano, A.
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Hirschmann, M.
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Pezzotta, A.
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Aussel, H.
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Hoekstra, H.
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Kitching, T.
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Percival, W.J.
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Guzzo, L.
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Mellier, Y.
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Oesch, P.A.
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Bowler, R.A.A.
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Bruton, S.
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Allevato, V.
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Gonzalez-Perez, V.
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Manera, M.
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Avila, S.
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Kovács, A.
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Aghanim, N.
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Altieri, B.
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Shankar, F.
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Euclid Collaboration
Castander, F.J.
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Fosalba, P.
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Stadel, J.
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Potter, D.
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Carretero, J.
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Tallada-Crespí, P.
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Pozzetti, L.
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Bolzonella, M.
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Mamon, G.A.
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Blot, L.
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Hoffmann, K.
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Huertas-Company, M.
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Monaco, P.
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Gonzalez, E.J.
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Lucia, G. De
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Scarlata, C.
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Breton, M.-A.
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Linke, L.
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Viglione, C.
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Li, S.-S.
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Zhai, Z.
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Baghkhani, Z.
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Pardede, K.
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Neissner, C.
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Teyssier, R.
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Crocce, M.
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Tutusaus, I.
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Miller, L.
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Congedo, G.
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Biviano, A.
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Hirschmann, M.
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Pezzotta, A.
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Aussel, H.
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Hoekstra, H.
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Kitching, T.
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Percival, W.J.
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Guzzo, L.
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Mellier, Y.
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Oesch, P.A.
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Bowler, R.A.A.
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Bruton, S.
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Allevato, V.
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Gonzalez-Perez, V.
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Manera, M.
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Avila, S.
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Kovács, A.
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Aghanim, N.
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Altieri, B.
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Shankar, F.
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Euclid Collaboration (2025) Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission. A&A, 697, [A5]. (doi:10.1051/0004-6361/202450853).

Record type: Article

Abstract

We present the Flagship galaxy mock, a simulated catalogue of billions of galaxies designed to support the scientific exploitation of the Euclid mission. Euclid is a medium-class mission of the European Space Agency optimised to determine the properties of dark matter and dark energy on the largest scales of the Universe. It probes structure formation over more than 10 billion years primarily from the combination of weak gravitational lensing and galaxy clustering data. The breadth of Euclid’s data will also foster a wide variety of scientific analyses. The Flagship simulation was developed to provide a realistic approximation to the galaxies that will be observed by Euclid and used in its scientific exploitation. We ran a state-of-the-art N-body simulation with four trillion particles, producing a lightcone on the fly. From the dark matter particles, we produced a catalogue of 16 billion haloes in one octant of the sky in the lightcone up to redshift z = 3. We then populated these haloes with mock galaxies using a halo occupation distribution and abundance-matching approach, calibrating the free parameters of the galaxy mock against observed correlations and other basic galaxy properties. Modelled galaxy properties include luminosity and flux in several bands, redshifts, positions and velocities, spectral energy distributions, shapes and sizes, stellar masses, star formation rates, metallicities, emission line fluxes, and lensing properties. We selected a final sample of 3.4 billion galaxies with a magnitude cut of HE < 26, where we are complete. We have performed a comprehensive set of validation tests to check the similarity to observational data and theoretical models. In particular, our catalogue is able to closely reproduce the main characteristics of the weak lensing and galaxy clustering samples to be used in the mission main cosmological analysis. Moreover, given its depth and completeness, this new galaxy mock also provides the community with a powerful tool for developing a wide range of scientific analyses beyond the Euclid mission.

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2405.13495v1 - Accepted Manuscript
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Accepted/In Press date: 19 December 2024
Published date: 30 April 2025
Additional Information: Paper submitted as part of the A&A special issue `Euclid on Sky', which contains Euclid key reference papers and first results from the Euclid Early Release Observations
Keywords: astro-ph.CO, galaxies: evolution, catalogs, large-scale structure of Universe, cosmology: observations, gravitational lensing: weak

Identifiers

Local EPrints ID: 502623
URI: http://eprints.soton.ac.uk/id/eprint/502623
ISSN: 0004-6361
PURE UUID: 9023db21-b3a7-4edb-95a2-f83ff3d58434

Catalogue record

Date deposited: 02 Jul 2025 16:34
Last modified: 10 Sep 2025 11:02

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Contributors

Author: F.J. Castander
Author: P. Fosalba
Author: J. Stadel
Author: D. Potter
Author: J. Carretero
Author: P. Tallada-Crespí
Author: L. Pozzetti
Author: M. Bolzonella
Author: G.A. Mamon
Author: L. Blot
Author: K. Hoffmann
Author: M. Huertas-Company
Author: P. Monaco
Author: E.J. Gonzalez
Author: G. De Lucia
Author: C. Scarlata
Author: M.-A. Breton
Author: L. Linke
Author: C. Viglione
Author: S.-S. Li
Author: Z. Zhai
Author: Z. Baghkhani
Author: K. Pardede
Author: C. Neissner
Author: R. Teyssier
Author: M. Crocce
Author: I. Tutusaus
Author: L. Miller
Author: G. Congedo
Author: A. Biviano
Author: M. Hirschmann
Author: A. Pezzotta
Author: H. Aussel
Author: H. Hoekstra
Author: T. Kitching
Author: W.J. Percival
Author: L. Guzzo
Author: Y. Mellier
Author: P.A. Oesch
Author: R.A.A. Bowler
Author: S. Bruton
Author: V. Allevato
Author: V. Gonzalez-Perez
Author: M. Manera
Author: S. Avila
Author: A. Kovács
Author: N. Aghanim
Author: B. Altieri
Author: F. Shankar
Corporate Author: Euclid Collaboration

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