---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '22265'
abstract:
- lang: eng
  text: 'The well-known bimodality between star-forming discs and quiescent spheroids
    requires the existence of two main processes: galaxy quenching, causing the strong
    reduction of star formation, and morphological transformation, causing the transition
    from disc-dominated structures to bulge-dominated ones. In this paper, we aim
    to understand the link between these two processes and their relation with the
    stellar mass of galaxies and their local environment. Taking advantage of the
    first data released by the Euclid Collaboration, covering more than 60 deg2 with
    space-based imaging and photometry, we analyse a mass-complete sample of nearly
    one million galaxies in the range 0.25 < z < 1 with M* > 109.5 M⊙, using a combination
    of photometric and spectroscopic redshifts. We divide the sample into four sub-populations
    of galaxies, based on their star-formation activity (star-forming and quiescent)
    and morphology (disc-dominated and bulge-dominated). We then analyse the physical
    properties of these populations and their relative abundances in the stellar mass
    versus local density plane. Together with confirming the passivity-density relation
    and the morphology-density relation, we find that quiescent discy galaxies are
    more abundant in the low-mass regime of high-density environment where log10(1 + δ)
    > 1.3. At the same time, star-forming bulge-dominated galaxies are more common
    in field regions with log10(1 + δ) < 0.8, preferentially at high masses. Building
    on these results and interpreting them through comparison with simulations, we
    propose a scenario where the evolution of galaxies in the field significantly
    differs from that in higher-density environments. The morphological transformation
    in the majority of field galaxies takes place before the onset of quenching and
    is mainly driven by secular processes taking place within the main sequence, leading
    to the formation of star-forming bulge-dominated galaxies as intermediate-stage
    galaxies. Conversely, quenching of star formation precedes morphological transformation
    for most galaxies in higher-density environments. This causes the formation of
    quiescent disc-dominated galaxies before their transition into bulge-dominated
    ones.'
acknowledgement: 'FaGe, AnEn, EmDa, LoGa, SaQu, GaDe, MaTa, ChDe, LuPo acknowledge
  support from the ELSA project. “ELSA: Euclid Legacy Science Advanced analysis tools”
  (Grant Agreement no. 101135203) is funded by the European Union. Views and opinions
  expressed are however those of the author(s) only and do not necessarily reflect
  those of the European Union or Innovate UK. Neither the European Union nor the granting
  authority can be held responsible for them. UK participation is funded through the
  UK HORIZON guarantee scheme under Innovate UK grant 10093177. AnEn acknowledge support
  from the INAF MiniGrant 2023 “ADIEU: Anomaly Detections In EUclid”. CaLo acknowledges
  support by FCT-Fundação para a Ciência e a Tecnologia through grants UIDB/04434/2020
  DOI: 10.54499/UIDB/04434/2020, UIDP/04434/2020 DOI: 10.54499/UIDP/04434/2020. The
  Euclid Consortium acknowledges the European Space Agency and a number 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 detailed list is available on
  the Euclid website (www.euclid-ec.org). This work has made use of the Euclid Quick
  Release Q1 data from the Euclid mission of the European Space Agency (ESA), 2025,
  https://doi.org/10.57780/esa-2853f3b. This work has made use of CosmoHub, developed
  by PIC (maintained by IFAE and CIEMAT) in collaboration with ICE-CSIC. CosmoHub
  received funding from the Spanish government (MCIN/AEI/10.13039/501100011033), the
  EU NextGeneration/PRTR (PRTR-C17.I1), and the Generalitat de Catalunya. Based on
  data from UNIONS, a scientific collaboration using three Hawaii-based telescopes:
  CFHT, Pan-STARRS, and Subaru www.skysurvey.cc. Based on data from the Dark Energy
  Camera (DECam) on the Blanco 4-m Telescope at CTIO in Chile https://www.darkenergysurvey.org'
article_number: A12
article_processing_charge: Yes
article_type: original
arxiv: 1
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citation:
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  apa: 'Gentile, F., Daddi, E., Elbaz, D., Enia, A., Magnelli, B., Billand, J. B.,
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  chicago: 'Gentile, F., E. Daddi, D. Elbaz, A. Enia, B. Magnelli, J. B. Billand,
    P. Corcho-Caballero, et al. “Euclid Quick Data Release (Q1): XII. Quenching Precedes
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    bulge formation in dense environments but follows it in the field. Astronomy and
    Astrophysics. 711, A12.'
  mla: 'Gentile, F., et al. “Euclid Quick Data Release (Q1): XII. Quenching Precedes
    Bulge Formation in Dense Environments but Follows It in the Field.” <i>Astronomy
    and Astrophysics</i>, vol. 711, A12, EDP Sciences, 2026, doi:<a href="https://doi.org/10.1051/0004-6361/202557633">10.1051/0004-6361/202557633</a>.'
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    C.M. Gutierrez, A. Hall, S. Hemmati, H. Hildebrandt, J. Hjorth, J.J.E. Kajava,
    Y. Kang, V. Kansal, D. Karagiannis, K. Kiiveri, J. Kim, C.C. Kirkpatrick, S. Kruk,
    L. Legrand, M. Lembo, F. Lepori, G. Leroy, G.F. Lesci, J. Lesgourgues, L. Leuzzi,
    T.I. Liaudat, A. Loureiro, J. Macias-Perez, E.A. Magnier, F. Mannucci, R. Maoli,
    C.J.A.P. Martins, L. Maurin, M. Miluzio, P. Monaco, C. Moretti, G. Morgante, K.
    Naidoo, A. Navarro-Alsina, S. Nesseris, D. Paoletti, F. Passalacqua, K. Paterson,
    L. Patrizii, A. Pisani, D. Potter, M. Radovich, G. Rodighiero, S. Sacquegna, M.
    Sahlén, D.B. Sanders, E. Sarpa, C. Scarlata, A. Schneider, M. Schultheis, D. Sciotti,
    E. Sellentin, L.C. Smith, S.A. Stanford, K. Tanidis, G. Testera, R. Teyssier,
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    Vielzeuf, N.A. Walton, Astronomy and Astrophysics 711 (2026).
das_tickbox: '1'
dataavailabilitystatement: 'This work has made use of the Euclid Quick Release Q1
  data from the Euclid mission of the European Space Agency (ESA), 2025, https://doi.org/10.57780/esa-2853f3b.
  This work has made use of CosmoHub, developed by PIC (maintained by IFAE and CIEMAT)
  in collaboration with ICE-CSIC. CosmoHub received funding from the Spanish government
  (MCIN/AEI/10.13039/501100011033), the EU NextGeneration/PRTR (PRTR-C17.I1), and
  the Generalitat de Catalunya. Based on data from UNIONS, a scientific collaboration
  using three Hawaii-based telescopes: CFHT, Pan-STARRS, and Subaru www.skysurvey.cc.
  Based on data from the Dark Energy Camera (DECam) on the Blanco 4-m Telescope at
  CTIO in Chile https://www.darkenergysurvey.org'
date_created: 2026-07-12T22:02:18Z
date_published: 2026-07-01T00:00:00Z
date_updated: 2026-07-13T08:43:41Z
day: '01'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.1051/0004-6361/202557633
external_id:
  arxiv:
  - '2511.02964'
file:
- access_level: open_access
  checksum: 29c087abb97eed26d4aa2a19bbb46666
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  creator: dernst
  date_created: 2026-07-13T08:42:10Z
  date_updated: 2026-07-13T08:42:10Z
  file_id: '22277'
  file_name: 2026_AstronomyAstrophysics_Euclid.pdf
  file_size: 3482066
  relation: main_file
  success: 1
file_date_updated: 2026-07-13T08:42:10Z
has_accepted_license: '1'
intvolume: '       711'
keyword:
- 'galaxies: evolution'
- 'galaxies: interactions'
- 'galaxies: statistics'
language:
- iso: eng
month: '07'
oa: 1
oa_version: Published Version
publication: Astronomy and Astrophysics
publication_identifier:
  eissn:
  - 1432-0746
  issn:
  - 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
researchdata_availability: no
scopus_import: '1'
status: public
supplementarymaterial: no
title: 'Euclid Quick Data Release (Q1): XII. Quenching precedes bulge formation in
  dense environments but follows it in the field'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 711
year: '2026'
...