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Euclid Quick Data Release (Q1). The first Euclid view of Planck galaxy protocluster candidates at cosmic noon

Euclid Collaboration T. Dusserre H. Dole F. Sarron G. Castignani N. Ramos-Chernenko +495 lainnya
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[ABRIGED ABSTRACT] A large catalogue of candidate galaxy protoclusters with high star-formation rates was produced by the Planck collaboration. We search, in the first data release (Q1) of the Euclid survey, for the visible and infrared counterparts of the Planck galaxy protocluster candidates expected to be above $z>1.5$. Eight of them are in Euclid Q1. Our goal is to investigate the optical nature of these overdensities previously detected in the submillimetre wavelength range. We search for overdensities using the DETECTIFz algorithm, an overdensity finder based on Delaunay tessellation that uses photometric redshift probability distributions through Monte Carlo simulations. Focusing our search on the eight high-star forming Planck protocluster candidates, we find that two of them have one Euclid counterpart, and six have between two and four Euclid counterparts, which amounts to a total of 20 Euclid counterparts. These Euclid counterparts lie at photometric redshifts $1.4<z_{\rm ph}<2.7$ and 12 of them also have partial Herschel coverage. All detections have also been confirmed by at least one other independent protocluster detection algorithm. We study the colours, derived stellar masses and star-formation rates (SFRs) of the detected member galaxies of those protocluster candidate counterparts. We also estimate the total stellar masses, SFRs, and the halo mass lower limits for all Euclid protocluster candidates. We find that in the dark matter halo mass ($M_{\rm h}$) / redshift plane, these Planck and Euclid overdense regions lie in the region $12.6<\log_{10} (M_{\rm h}/M_\odot)<13.4$, $1.4<z<2.7$. This means that the halos of our objects are expected to have experienced a transition between cold flows in hot media to accretion of hot material.

Topik & Kata Kunci

Physics

Penulis (500)

E

Euclid Collaboration T. Dusserre

H

H. Dole

F

F. Sarron

G

G. Castignani

N

N. Ramos-Chernenko

N

N. Aghanim

A

A. Garic

I

I. Mellouki

N

N. Dagoneau

O

O. Chapuis

B

B. Frye

M

M. Polletta

H

H. Dannerbauer

M

M. Langer

L

L. Maurin

E

E. Soubrié

A

A. Biviano

S

S. Mei

N

N. Mai

B

B. Altieri

A

A. Amara

S

S. Andreon

N

N. Auricchio

C

C. Baccigalupi

M

M. Baldi

A

A. Balestra

S

S. Bardelli

P

P. Battaglia

A

A. Bonchi

D

D. Bonino

E

E. Branchini

M

M. Brescia

J

J. Brinchmann

S

S. Camera

G

G. Cañas-Herrera

V

V. Capobianco

C

C. Carbone

J

J. Carretero

S

S. Casas

M

M. Castellano

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S. Cavuoti

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K. Chambers

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A. Cimatti

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C. Colodro-Conde

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G. Congedo

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C. Conselice

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L. Conversi

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Y. Copin

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A. Costille

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F. Courbin

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H. Courtois

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M. Cropper

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G. D. Lucia

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A. Giorgio

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X. Dupac

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S. Dusini

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A. Ealet

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M. Farina

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D. S. U. Paris-Saclay

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Cnrs

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I. D. Spatiale

9

91405

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Orsay

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Institut de Recherche en Informatique de Toulouse

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U. Toulouse

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Toulouse Inp

U

UT3

3

31400 Toulouse

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Laboratoire Mcd

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Centre de Biologie Int'egrative

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I. Bologna

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V. G. 933

4

40129 Bologna

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Italy

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Instituto de Astrof'isica de Canarias

V

V'ia L'actea

3

38205 La Laguna

T

Tenerife

S

Spain.

D

D. Astrof'isica

U

U. L. Laguna

3

38200

L

L. Laguna

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Universit'e Paris-Saclay

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Cea

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D'epartement d''Electronique des D'etecteurs et d'Informatique Physique

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91191

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Gif-sur-Yvette

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Inria

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Department of AstronomySteward Observatory

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U. Arizona

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9. N. C. Avenue

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Tucson

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USA.

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2. viaBeirut

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7

7. Paris

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C. Laboratory

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Centre Pierre Binetruy

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IRL2007

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CPB-IN2P3

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Berkeley

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Esacesa

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Camino Bajo de Castillo

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Urb. Villafranca del Castillo

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28692 Villanueva de la Canada

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Madrid

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S. O. Mathematics

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U. Surrey

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Guildford

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Surrey

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20133 Milano

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Napoli

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F. Porto

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U. Torino

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I. Torino

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European Space AgencyESTEC

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2. Noordwijk

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The Netherlands.

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Institute Lorentz

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Leiden University

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2. NielsBohrweg

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L. Observatory

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Port d'Informaci'o Cient'ifica

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Campus Uab

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08193 Bellaterra

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Format Sitasi

APA MLA BibTeX
Dusserre, E.C.T., Dole, H., Sarron, F., Castignani, G., Ramos-Chernenko, N., Aghanim, N. et al. (2025). Euclid Quick Data Release (Q1). The first Euclid view of Planck galaxy protocluster candidates at cosmic noon. https://www.semanticscholar.org/paper/bc04a70393168b7dc1667c531cf5fd5326898446

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