Euclid: Quick Data Release (Q1) -- Watching ICM-selected galaxy clusters with Euclid eyes -- prospects of Euclid data in the context of large SZ and X-ray based surveys Article Swipe
Mary Beth Klein
,
Koshy George
,
J. J. Mohr
,
B Altieri
,
Luca Amendola
,
S. Andreon
,
N. Auricchio
,
C. Baccigalupi
,
Marco Baldi
,
A. Balestra
,
S. Bardelli
,
A. Biviano
,
E. Branchini
,
M. Brescia
,
S. Camera
,
G Cañas-Herrera
,
V. Capobianco
,
R. Maoli
,
J. Carretero
,
Santiago Casas
,
M. G. Castellano
,
G. Castignani
,
S. Cavuoti
,
K. C. Chambers
,
A. Cimatti
,
C. Colodro-Conde
,
G. Congedo
,
L. Conversi
,
Y. Copin
,
F. Courbin
,
H. M. Courtois
,
M Cropper
,
A. Da Silva
,
H. Degaudenzi
,
G. De Lucia
,
C. Dolding
,
H. Dole
,
F. Dubath
,
Franck Ducret
,
X Dupac
,
S. Dusini
,
M. Farina
,
R. Farinelli
,
F Faustini
,
S. Ferriol
,
F. Finelli⋆
,
M. Frailis
,
E. Franceschi
,
M. Fumana
,
S. Galeotta
,
B. Gillis
,
C. Giocoli
,
J. Graciá‐Carpio
,
A. Grazian
,
F. Grupp
,
S. V. H. Haugan
,
W. Holmes
,
I. Hook
,
F Hormuth
,
S. Andreon
,
K. Jahnkę
,
M. Jhabvala
,
Marco Baldi
,
S. Kermiche
,
B. Kubik
,
M Kümmel
,
M. Kunz
,
H. Kurki-Suonio
,
A.M.C Le Brun
,
D. Le Mignant
,
S. Ligori
,
P. B. Lilje
,
V. Lindholm
,
I. Lloro
,
G. Mainetti
,
Donatella Biagi
,
G. Meylan
,
O. Mansutti
,
O. Marggraf
,
M. Martinelli
,
N. Martinet
,
F. Marulli
,
R. Massey
,
S. Maurogordato
,
E. Medinaceli
,
V. Pettorino
,
Y. Mellier
,
M. Meneghetti
,
E. Merlin
,
G. Meylan
,
L. Moscardini
,
R. Nakajima
,
C. Neissner
,
S.-M Niemi
,
C. Padilla
,
S. Paltani
,
F. Pasian
,
K. Pedersen
,
Will J. Percival
,
V. Pettorino
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2506.19566
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2506.19566
Galaxy clusters detected through their X-ray emission or Sunyaev--Zeldovich effect (SZE), both produced by the intra-cluster medium (ICM), are key probes in cosmological and astrophysical studies. To maximise the scientific return of such surveys, complementary data are required for cluster confirmation and redshift estimation. This is typically provided by wide-field optical and infrared surveys, which are increasingly challenged by ongoing and future ICM-selected samples. In particular, at high redshifts ($z>1$) probed by upcoming SZE-selected samples, current large surveys may be insufficient for reliable confirmation. Deep, high-resolution infrared surveys like Euclid will thus be essential for confirming most high-redshift clusters. We present an analysis of the first sizeable Euclid dataset (Q1), overlapping with several ICM-selected cluster samples. We apply an adaptation of the MCMF cluster confirmation tool to estimate key properties, including redshift and richness, and to predict Euclid's capabilities for high-redshift cluster confirmation. We find promising performance, particularly at high redshifts, while richness estimates at low redshifts ($z<0.4$) are currently limited by Q1 data quality but should improve with future releases. Using MCMF runs on random lines of sight, we predict that Euclid will confirm clusters at $1
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- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2506.19566
- https://arxiv.org/pdf/2506.19566
- OA Status
- green
- OpenAlex ID
- https://openalex.org/W4414684254
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- Title
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Euclid: Quick Data Release (Q1) -- Watching ICM-selected galaxy clusters with Euclid eyes -- prospects of Euclid data in the context of large SZ and X-ray based surveysWork title
- Type
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
- Publication date
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2025-06-24Full publication date if available
- Authors
-
Mary Beth Klein, Koshy George, J. J. Mohr, B Altieri, Luca Amendola, S. Andreon, N. Auricchio, C. Baccigalupi, Marco Baldi, A. Balestra, S. Bardelli, A. Biviano, E. Branchini, M. Brescia, S. Camera, G Cañas-Herrera, V. Capobianco, R. Maoli, J. Carretero, Santiago Casas, M. G. Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A. Cimatti, C. Colodro-Conde, G. Congedo, L. Conversi, Y. Copin, F. Courbin, H. M. Courtois, M Cropper, A. Da Silva, H. Degaudenzi, G. De Lucia, C. Dolding, H. Dole, F. Dubath, Franck Ducret, X Dupac, S. Dusini, M. Farina, R. Farinelli, F Faustini, S. Ferriol, F. Finelli⋆, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, B. Gillis, C. Giocoli, J. Graciá‐Carpio, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, I. Hook, F Hormuth, S. Andreon, K. Jahnkę, M. Jhabvala, Marco Baldi, S. Kermiche, B. Kubik, M Kümmel, M. Kunz, H. Kurki-Suonio, A.M.C Le Brun, D. Le Mignant, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, G. Mainetti, Donatella Biagi, G. Meylan, O. Mansutti, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R. Massey, S. Maurogordato, E. Medinaceli, V. Pettorino, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, L. Moscardini, R. Nakajima, C. Neissner, S.-M Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, Will J. Percival, V. PettorinoList of authors in order
- Landing page
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https://arxiv.org/abs/2506.19566Publisher landing page
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https://arxiv.org/pdf/2506.19566Direct link to full text PDF
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YesWhether a free full text is available
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greenOpen access status per OpenAlex
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https://arxiv.org/pdf/2506.19566Direct OA link when available
- Cited by
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0Total citation count in OpenAlex
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| abstract_inverted_index.confirmation. | 83, 142 |
| abstract_inverted_index.high-redshift | 97, 140 |
| abstract_inverted_index.intra-cluster | 15 |
| abstract_inverted_index.high-resolution | 85 |
| abstract_inverted_index.Sunyaev--Zeldovich | 8 |
| cited_by_percentile_year | |
| countries_distinct_count | 1 |
| institutions_distinct_count | 147 |
| citation_normalized_percentile |