Image de couverture de livre

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

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Klein, M., George, K., Mohr, J. J., Altieri, B., Amendola, L., Andreon, S., Auricchio, N., Baccigalupi, C., Baldi, M., Balestra, A., Bardelli, S., Biviano, A., Branchini, E., Brescia, M., Camera, S., Cañas-Herrera, G., Capobianco, V., Carbone, C., Carretero, J., Casas, S., Castellano, M., Castignani, G., Cavuoti, S., Chambers, K. C., Cimatti, A., Colodro-Conde, C., Congedo, G., Conversi, L., Copin, Y., Courbin, F., Courtois, H. M., Cropper, M., Da Silva, A., Degaudenzi, H., De Lucia, G., Dolding, C., Dole, H., Dubath, F., Ducret, F., Dupac, X., Dusini, S., Farina, M., Farinelli, R., Faustini, F., Ferriol, S., Finelli, F., Frailis, M., Franceschi, E., Fumana, M., Galeotta, S., Gillis, B., Giocoli, C., Gracia-Carpio, J., Grazian, A., Grupp, F., Haugan, S. V. H., Holmes, W., Hook, I. M., Hormuth, F., Hornstrup, A., Jahnke, K., Jhabvala, M., Keihänen, E., Kermiche, S., Kubik, B., Kümmel, M., Kunz, M., Kurki-Suonio, H., Brun, A. M. C. Le, Mignant, D. Le, Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Mainetti, G., Maino, D., Maiorano, E., Mansutti, O., Marggraf, O., Martinelli, M., Martinet, N., Marulli, F., Massey, R., Maurogordato, S., Medinaceli, E., Mei, S., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Moscardini, L., Nakajima, R., Neissner, C., Niemi, S. -M., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Percival, W. J., Pettorino, V., Pires, S., Polenta, G., Poncet, M., Popa, L. A., Pozzetti, L., Raison, F., Rebolo, R., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rosset, C., Rottgering, H. J. A., Saglia, R., Sakr, Z., Sapone, D., Schirmer, M., Schneider, P., Schrabback, T., Secroun, A., Sefusatti, E., Seidel, G., Serrano, S., Sirignano, C., Sirri, G., Stanco, L., Steinwagner, J., Tallada-Crespí, P., Taylor, A. N., Tereno, I., Toft, S., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valenziano, L., Valiviita, J., Vassallo, T., Veropalumbo, A., Wang, Y., Weller, J., Zerbi, F. M., Zucca, E., Burigana, C., Scottez, V., Sereno, M., Viel, M.
Format: Preprint
Publié: 2025
Sujets:
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
Accès en ligne:
Acceder al recurso
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866908419352428544
author Klein, M.
George, K.
Mohr, J. J.
Altieri, B.
Amendola, L.
Andreon, S.
Auricchio, N.
Baccigalupi, C.
Baldi, M.
Balestra, A.
Bardelli, S.
Biviano, A.
Branchini, E.
Brescia, M.
Camera, S.
Cañas-Herrera, G.
Capobianco, V.
Carbone, C.
Carretero, J.
Casas, S.
Castellano, M.
Castignani, G.
Cavuoti, S.
Chambers, K. C.
Cimatti, A.
Colodro-Conde, C.
Congedo, G.
Conversi, L.
Copin, Y.
Courbin, F.
Courtois, H. M.
Cropper, M.
Da Silva, A.
Degaudenzi, H.
De Lucia, G.
Dolding, C.
Dole, H.
Dubath, F.
Ducret, F.
Dupac, X.
Dusini, S.
Farina, M.
Farinelli, R.
Faustini, F.
Ferriol, S.
Finelli, F.
Frailis, M.
Franceschi, E.
Fumana, M.
Galeotta, S.
Gillis, B.
Giocoli, C.
Gracia-Carpio, J.
Grazian, A.
Grupp, F.
Haugan, S. V. H.
Holmes, W.
Hook, I. M.
Hormuth, F.
Hornstrup, A.
Jahnke, K.
Jhabvala, M.
Keihänen, E.
Kermiche, S.
Kubik, B.
Kümmel, M.
Kunz, M.
Kurki-Suonio, H.
Brun, A. M. C. Le
Mignant, D. Le
Ligori, S.
Lilje, P. B.
Lindholm, V.
Lloro, I.
Mainetti, G.
Maino, D.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Martinelli, M.
Martinet, N.
Marulli, F.
Massey, R.
Maurogordato, S.
Medinaceli, E.
Mei, S.
Mellier, Y.
Meneghetti, M.
Merlin, E.
Meylan, G.
Moscardini, L.
Nakajima, R.
Neissner, C.
Niemi, S. -M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Percival, W. J.
Pettorino, V.
Pires, S.
Polenta, G.
Poncet, M.
Popa, L. A.
Pozzetti, L.
Raison, F.
Rebolo, R.
Renzi, A.
Rhodes, J.
Riccio, G.
Romelli, E.
Roncarelli, M.
Rosset, C.
Rottgering, H. J. A.
Saglia, R.
Sakr, Z.
Sapone, D.
Schirmer, M.
Schneider, P.
Schrabback, T.
Secroun, A.
Sefusatti, E.
Seidel, G.
Serrano, S.
Sirignano, C.
Sirri, G.
Stanco, L.
Steinwagner, J.
Tallada-Crespí, P.
Taylor, A. N.
Tereno, I.
Toft, S.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, I.
Valenziano, L.
Valiviita, J.
Vassallo, T.
Veropalumbo, A.
Wang, Y.
Weller, J.
Zerbi, F. M.
Zucca, E.
Burigana, C.
Scottez, V.
Sereno, M.
Viel, M.
author_facet Klein, M.
George, K.
Mohr, J. J.
Altieri, B.
Amendola, L.
Andreon, S.
Auricchio, N.
Baccigalupi, C.
Baldi, M.
Balestra, A.
Bardelli, S.
Biviano, A.
Branchini, E.
Brescia, M.
Camera, S.
Cañas-Herrera, G.
Capobianco, V.
Carbone, C.
Carretero, J.
Casas, S.
Castellano, M.
Castignani, G.
Cavuoti, S.
Chambers, K. C.
Cimatti, A.
Colodro-Conde, C.
Congedo, G.
Conversi, L.
Copin, Y.
Courbin, F.
Courtois, H. M.
Cropper, M.
Da Silva, A.
Degaudenzi, H.
De Lucia, G.
Dolding, C.
Dole, H.
Dubath, F.
Ducret, F.
Dupac, X.
Dusini, S.
Farina, M.
Farinelli, R.
Faustini, F.
Ferriol, S.
Finelli, F.
Frailis, M.
Franceschi, E.
Fumana, M.
Galeotta, S.
Gillis, B.
Giocoli, C.
Gracia-Carpio, J.
Grazian, A.
Grupp, F.
Haugan, S. V. H.
Holmes, W.
Hook, I. M.
Hormuth, F.
Hornstrup, A.
Jahnke, K.
Jhabvala, M.
Keihänen, E.
Kermiche, S.
Kubik, B.
Kümmel, M.
Kunz, M.
Kurki-Suonio, H.
Brun, A. M. C. Le
Mignant, D. Le
Ligori, S.
Lilje, P. B.
Lindholm, V.
Lloro, I.
Mainetti, G.
Maino, D.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Martinelli, M.
Martinet, N.
Marulli, F.
Massey, R.
Maurogordato, S.
Medinaceli, E.
Mei, S.
Mellier, Y.
Meneghetti, M.
Merlin, E.
Meylan, G.
Moscardini, L.
Nakajima, R.
Neissner, C.
Niemi, S. -M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Percival, W. J.
Pettorino, V.
Pires, S.
Polenta, G.
Poncet, M.
Popa, L. A.
Pozzetti, L.
Raison, F.
Rebolo, R.
Renzi, A.
Rhodes, J.
Riccio, G.
Romelli, E.
Roncarelli, M.
Rosset, C.
Rottgering, H. J. A.
Saglia, R.
Sakr, Z.
Sapone, D.
Schirmer, M.
Schneider, P.
Schrabback, T.
Secroun, A.
Sefusatti, E.
Seidel, G.
Serrano, S.
Sirignano, C.
Sirri, G.
Stanco, L.
Steinwagner, J.
Tallada-Crespí, P.
Taylor, A. N.
Tereno, I.
Toft, S.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, I.
Valenziano, L.
Valiviita, J.
Vassallo, T.
Veropalumbo, A.
Wang, Y.
Weller, J.
Zerbi, F. M.
Zucca, E.
Burigana, C.
Scottez, V.
Sereno, M.
Viel, M.
contents 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 $1<z<2$ as effectively as current optical surveys at $z<0.6$, significantly enhancing high-redshift confirmation. SZE-selected samples will thus greatly benefit from Euclid overlap. Among five known high-$z$ SZE clusters in Q1, we identify the highest-redshift jellyfish galaxy candidate to date, EUCLJ035330.86$-$504347.6 in SPT-CLJ0353$-$5043 ($z=1.32$), two massive star-forming galaxies near ACT-CLJ0350.0$-$4819 ($z=1.46$), and strong lensing features in SPT-CLJ0353$-$5043 and SPT-CLJ0421$-$4845.
format Preprint
id arxiv_https___arxiv_org_abs_2506_19566
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle 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
Klein, M.
George, K.
Mohr, J. J.
Altieri, B.
Amendola, L.
Andreon, S.
Auricchio, N.
Baccigalupi, C.
Baldi, M.
Balestra, A.
Bardelli, S.
Biviano, A.
Branchini, E.
Brescia, M.
Camera, S.
Cañas-Herrera, G.
Capobianco, V.
Carbone, C.
Carretero, J.
Casas, S.
Castellano, M.
Castignani, G.
Cavuoti, S.
Chambers, K. C.
Cimatti, A.
Colodro-Conde, C.
Congedo, G.
Conversi, L.
Copin, Y.
Courbin, F.
Courtois, H. M.
Cropper, M.
Da Silva, A.
Degaudenzi, H.
De Lucia, G.
Dolding, C.
Dole, H.
Dubath, F.
Ducret, F.
Dupac, X.
Dusini, S.
Farina, M.
Farinelli, R.
Faustini, F.
Ferriol, S.
Finelli, F.
Frailis, M.
Franceschi, E.
Fumana, M.
Galeotta, S.
Gillis, B.
Giocoli, C.
Gracia-Carpio, J.
Grazian, A.
Grupp, F.
Haugan, S. V. H.
Holmes, W.
Hook, I. M.
Hormuth, F.
Hornstrup, A.
Jahnke, K.
Jhabvala, M.
Keihänen, E.
Kermiche, S.
Kubik, B.
Kümmel, M.
Kunz, M.
Kurki-Suonio, H.
Brun, A. M. C. Le
Mignant, D. Le
Ligori, S.
Lilje, P. B.
Lindholm, V.
Lloro, I.
Mainetti, G.
Maino, D.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Martinelli, M.
Martinet, N.
Marulli, F.
Massey, R.
Maurogordato, S.
Medinaceli, E.
Mei, S.
Mellier, Y.
Meneghetti, M.
Merlin, E.
Meylan, G.
Moscardini, L.
Nakajima, R.
Neissner, C.
Niemi, S. -M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Percival, W. J.
Pettorino, V.
Pires, S.
Polenta, G.
Poncet, M.
Popa, L. A.
Pozzetti, L.
Raison, F.
Rebolo, R.
Renzi, A.
Rhodes, J.
Riccio, G.
Romelli, E.
Roncarelli, M.
Rosset, C.
Rottgering, H. J. A.
Saglia, R.
Sakr, Z.
Sapone, D.
Schirmer, M.
Schneider, P.
Schrabback, T.
Secroun, A.
Sefusatti, E.
Seidel, G.
Serrano, S.
Sirignano, C.
Sirri, G.
Stanco, L.
Steinwagner, J.
Tallada-Crespí, P.
Taylor, A. N.
Tereno, I.
Toft, S.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, I.
Valenziano, L.
Valiviita, J.
Vassallo, T.
Veropalumbo, A.
Wang, Y.
Weller, J.
Zerbi, F. M.
Zucca, E.
Burigana, C.
Scottez, V.
Sereno, M.
Viel, M.
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
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 $1<z<2$ as effectively as current optical surveys at $z<0.6$, significantly enhancing high-redshift confirmation. SZE-selected samples will thus greatly benefit from Euclid overlap. Among five known high-$z$ SZE clusters in Q1, we identify the highest-redshift jellyfish galaxy candidate to date, EUCLJ035330.86$-$504347.6 in SPT-CLJ0353$-$5043 ($z=1.32$), two massive star-forming galaxies near ACT-CLJ0350.0$-$4819 ($z=1.46$), and strong lensing features in SPT-CLJ0353$-$5043 and SPT-CLJ0421$-$4845.
title 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
topic Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2506.19566

Documents similaires