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Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Schrabback, T., Congedo, G., Gavazzi, R., Hartley, W. G., Jansen, H., Kang, Y., Kleinebreil, F., Atek, H., Bertin, E., Cuillandre, J. -C., Diego, J. M., Grandis, S., Hoekstra, H., Kümmel, M., Linke, L., Miyatake, H., Okabe, N., Paltani, S., Schefer, M., Simon, P., Tarsitano, F., Taylor, A. N., Weaver, J. R., Bhatawdekar, R., Montes, M., Rosati, P., Toft, S., Altieri, B., Amara, A., Amendola, L., Andreon, S., Auricchio, N., Baccigalupi, C., Baldi, M., Balestra, A., Bardelli, S., Battaglia, P., Bender, R., Biviano, A., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Cañas-Herrera, G., Candini, G. P., Capobianco, V., Carbone, C., Cardone, V. F., Carretero, J., Casas, S., Castander, F. J., Castellano, M., Castignani, G., Cavuoti, S., Chambers, K. C., Cimatti, A., Colodro-Conde, C., Conselice, C. J., Conversi, L., Copin, Y., Costille, A., Courbin, F., Courtois, H. M., Cropper, M., Da Silva, A., Degaudenzi, H., De Lucia, G., Dole, H., Douspis, M., Dubath, F., Dupac, X., Dusini, S., Escoffier, S., Farina, M., Farinelli, R., Farrens, S., Faustini, F., Ferriol, S., Finelli, F., Fosalba, P., Frailis, M., Franceschi, E., Fumana, M., Galeotta, S., George, K., Gillard, W., Gillis, B., Giocoli, C., Gracia-Carpio, J., Grazian, A., Grupp, F., Haugan, S. V. H., Hoar, J., Holmes, W., Hook, I. M., Hormuth, F., Hornstrup, A., Hudelot, P., Jahnke, K., Jhabvala, M., Joachimi, B., Keihänen, E., Kermiche, S., Kilbinger, M., Kubik, B., Kuijken, K., Kunz, M., Kurki-Suonio, H., Laureijs, R., 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., Marcin, S., Marggraf, O., Martinelli, M., Martinet, N., Marulli, F., Massey, R. J., Maurogordato, S., Medinaceli, E., Mei, S., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Mohr, J. J., Mora, A., Moresco, M., Moscardini, L., Nakajima, R., Neissner, C., Nichol, R. C., Niemi, S. -M., Padilla, C., Pasian, F., Pedersen, K., Percival, W. J., Pettorino, V., Pires, S., Polenta, G., Poncet, M., Popa, L. A., Pozzetti, L., Raison, F., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rosset, C., Saglia, R., Sakr, Z., Sapone, D., Sartoris, B., Schirmer, M., Schneider, P., Secroun, A., Seidel, G., Seiffert, M., Serrano, S., Sirignano, C., Sirri, G., Mancini, A. Spurio, Stanco, L., Steinwagner, J., Tallada-Crespí, P., Tereno, I., Tessore, N., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E. A., Valenziano, L., Valiviita, J., Vassallo, T., Kleijn, G. Verdoes, Veropalumbo, A., Wang, Y., Weller, J., Zamorani, G., Zerbi, F. M., Zucca, E., Bolzonella, M., Burigana, C., Gabarra, L., Martín-Fleitas, J., Matthew, S., Pezzotta, A., Scottez, V., Sereno, M., Viel, M., Scott, D.
Format:	Preprint
Publié:	2025
Sujets:	Cosmology and Nongalactic Astrophysics
Accès en ligne:	Acceder al recurso
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_version_	1866911628423856128
author	Schrabback, T. Congedo, G. Gavazzi, R. Hartley, W. G. Jansen, H. Kang, Y. Kleinebreil, F. Atek, H. Bertin, E. Cuillandre, J. -C. Diego, J. M. Grandis, S. Hoekstra, H. Kümmel, M. Linke, L. Miyatake, H. Okabe, N. Paltani, S. Schefer, M. Simon, P. Tarsitano, F. Taylor, A. N. Weaver, J. R. Bhatawdekar, R. Montes, M. Rosati, P. Toft, S. Altieri, B. Amara, A. Amendola, L. Andreon, S. Auricchio, N. Baccigalupi, C. Baldi, M. Balestra, A. Bardelli, S. Battaglia, P. Bender, R. Biviano, A. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Cañas-Herrera, G. Candini, G. P. Capobianco, V. Carbone, C. Cardone, V. F. Carretero, J. Casas, S. Castander, F. J. Castellano, M. Castignani, G. Cavuoti, S. Chambers, K. C. Cimatti, A. Colodro-Conde, C. Conselice, C. J. Conversi, L. Copin, Y. Costille, A. Courbin, F. Courtois, H. M. Cropper, M. Da Silva, A. Degaudenzi, H. De Lucia, G. Dole, H. Douspis, M. Dubath, F. Dupac, X. Dusini, S. Escoffier, S. Farina, M. Farinelli, R. Farrens, S. Faustini, F. Ferriol, S. Finelli, F. Fosalba, P. Frailis, M. Franceschi, E. Fumana, M. Galeotta, S. George, K. Gillard, W. Gillis, B. Giocoli, C. Gracia-Carpio, J. Grazian, A. Grupp, F. Haugan, S. V. H. Hoar, J. Holmes, W. Hook, I. M. Hormuth, F. Hornstrup, A. Hudelot, P. Jahnke, K. Jhabvala, M. Joachimi, B. Keihänen, E. Kermiche, S. Kilbinger, M. Kubik, B. Kuijken, K. Kunz, M. Kurki-Suonio, H. Laureijs, R. 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. Marcin, S. Marggraf, O. Martinelli, M. Martinet, N. Marulli, F. Massey, R. J. Maurogordato, S. Medinaceli, E. Mei, S. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Mohr, J. J. Mora, A. Moresco, M. Moscardini, L. Nakajima, R. Neissner, C. Nichol, R. C. Niemi, S. -M. Padilla, C. Pasian, F. Pedersen, K. Percival, W. J. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L. A. Pozzetti, L. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rosset, C. Saglia, R. Sakr, Z. Sapone, D. Sartoris, B. Schirmer, M. Schneider, P. Secroun, A. Seidel, G. Seiffert, M. Serrano, S. Sirignano, C. Sirri, G. Mancini, A. Spurio Stanco, L. Steinwagner, J. Tallada-Crespí, P. Tereno, I. Tessore, N. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Valiviita, J. Vassallo, T. Kleijn, G. Verdoes Veropalumbo, A. Wang, Y. Weller, J. Zamorani, G. Zerbi, F. M. Zucca, E. Bolzonella, M. Burigana, C. Gabarra, L. Martín-Fleitas, J. Matthew, S. Pezzotta, A. Scottez, V. Sereno, M. Viel, M. Scott, D.
author_facet	Schrabback, T. Congedo, G. Gavazzi, R. Hartley, W. G. Jansen, H. Kang, Y. Kleinebreil, F. Atek, H. Bertin, E. Cuillandre, J. -C. Diego, J. M. Grandis, S. Hoekstra, H. Kümmel, M. Linke, L. Miyatake, H. Okabe, N. Paltani, S. Schefer, M. Simon, P. Tarsitano, F. Taylor, A. N. Weaver, J. R. Bhatawdekar, R. Montes, M. Rosati, P. Toft, S. Altieri, B. Amara, A. Amendola, L. Andreon, S. Auricchio, N. Baccigalupi, C. Baldi, M. Balestra, A. Bardelli, S. Battaglia, P. Bender, R. Biviano, A. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Cañas-Herrera, G. Candini, G. P. Capobianco, V. Carbone, C. Cardone, V. F. Carretero, J. Casas, S. Castander, F. J. Castellano, M. Castignani, G. Cavuoti, S. Chambers, K. C. Cimatti, A. Colodro-Conde, C. Conselice, C. J. Conversi, L. Copin, Y. Costille, A. Courbin, F. Courtois, H. M. Cropper, M. Da Silva, A. Degaudenzi, H. De Lucia, G. Dole, H. Douspis, M. Dubath, F. Dupac, X. Dusini, S. Escoffier, S. Farina, M. Farinelli, R. Farrens, S. Faustini, F. Ferriol, S. Finelli, F. Fosalba, P. Frailis, M. Franceschi, E. Fumana, M. Galeotta, S. George, K. Gillard, W. Gillis, B. Giocoli, C. Gracia-Carpio, J. Grazian, A. Grupp, F. Haugan, S. V. H. Hoar, J. Holmes, W. Hook, I. M. Hormuth, F. Hornstrup, A. Hudelot, P. Jahnke, K. Jhabvala, M. Joachimi, B. Keihänen, E. Kermiche, S. Kilbinger, M. Kubik, B. Kuijken, K. Kunz, M. Kurki-Suonio, H. Laureijs, R. 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. Marcin, S. Marggraf, O. Martinelli, M. Martinet, N. Marulli, F. Massey, R. J. Maurogordato, S. Medinaceli, E. Mei, S. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Mohr, J. J. Mora, A. Moresco, M. Moscardini, L. Nakajima, R. Neissner, C. Nichol, R. C. Niemi, S. -M. Padilla, C. Pasian, F. Pedersen, K. Percival, W. J. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L. A. Pozzetti, L. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rosset, C. Saglia, R. Sakr, Z. Sapone, D. Sartoris, B. Schirmer, M. Schneider, P. Secroun, A. Seidel, G. Seiffert, M. Serrano, S. Sirignano, C. Sirri, G. Mancini, A. Spurio Stanco, L. Steinwagner, J. Tallada-Crespí, P. Tereno, I. Tessore, N. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Valiviita, J. Vassallo, T. Kleijn, G. Verdoes Veropalumbo, A. Wang, Y. Weller, J. Zamorani, G. Zerbi, F. M. Zucca, E. Bolzonella, M. Burigana, C. Gabarra, L. Martín-Fleitas, J. Matthew, S. Pezzotta, A. Scottez, V. Sereno, M. Viel, M. Scott, D.
contents	The Euclid space telescope of the European Space Agency (ESA) is designed to provide sensitive and accurate measurements of weak gravitational lensing distortions over wide areas on the sky. Here we present a weak gravitational lensing analysis of early Euclid observations obtained for the field around the massive galaxy cluster Abell 2390 as part of the Euclid Early Release Observations programme. We conduct galaxy shape measurements using three independent algorithms (LensMC, KSB+, and SourceXtractor++). Incorporating multi-band photometry from Euclid and Subaru/Suprime-Cam, we estimate photometric redshifts to preferentially select background sources from tomographic redshift bins, for which we calibrate the redshift distributions using the self-organising map approach and data from the Cosmic Evolution Survey (COSMOS). We quantify the residual cluster member contamination and correct for it in bins of photometric redshift and magnitude using their source density profiles, including corrections for source obscuration and magnification. We reconstruct the cluster mass distribution and jointly fit the tangential reduced shear profiles of the different tomographic bins with spherical Navarro--Frenk--White profile predictions to constrain the cluster mass, finding consistent results for the three shape catalogues and good agreement with earlier measurements. As an important validation test we compare these joint constraints to mass measurements obtained individually for the different tomographic bins, finding good consistency. More detailed constraints on the cluster properties are presented in a companion paper that additionally incorporates strong lensing measurements. Our analysis provides a first demonstration of the outstanding capabilities of Euclid for tomographic weak lensing measurements.
format	Preprint
id	arxiv_https___arxiv_org_abs_2507_07629
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390 Schrabback, T. Congedo, G. Gavazzi, R. Hartley, W. G. Jansen, H. Kang, Y. Kleinebreil, F. Atek, H. Bertin, E. Cuillandre, J. -C. Diego, J. M. Grandis, S. Hoekstra, H. Kümmel, M. Linke, L. Miyatake, H. Okabe, N. Paltani, S. Schefer, M. Simon, P. Tarsitano, F. Taylor, A. N. Weaver, J. R. Bhatawdekar, R. Montes, M. Rosati, P. Toft, S. Altieri, B. Amara, A. Amendola, L. Andreon, S. Auricchio, N. Baccigalupi, C. Baldi, M. Balestra, A. Bardelli, S. Battaglia, P. Bender, R. Biviano, A. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Cañas-Herrera, G. Candini, G. P. Capobianco, V. Carbone, C. Cardone, V. F. Carretero, J. Casas, S. Castander, F. J. Castellano, M. Castignani, G. Cavuoti, S. Chambers, K. C. Cimatti, A. Colodro-Conde, C. Conselice, C. J. Conversi, L. Copin, Y. Costille, A. Courbin, F. Courtois, H. M. Cropper, M. Da Silva, A. Degaudenzi, H. De Lucia, G. Dole, H. Douspis, M. Dubath, F. Dupac, X. Dusini, S. Escoffier, S. Farina, M. Farinelli, R. Farrens, S. Faustini, F. Ferriol, S. Finelli, F. Fosalba, P. Frailis, M. Franceschi, E. Fumana, M. Galeotta, S. George, K. Gillard, W. Gillis, B. Giocoli, C. Gracia-Carpio, J. Grazian, A. Grupp, F. Haugan, S. V. H. Hoar, J. Holmes, W. Hook, I. M. Hormuth, F. Hornstrup, A. Hudelot, P. Jahnke, K. Jhabvala, M. Joachimi, B. Keihänen, E. Kermiche, S. Kilbinger, M. Kubik, B. Kuijken, K. Kunz, M. Kurki-Suonio, H. Laureijs, R. 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. Marcin, S. Marggraf, O. Martinelli, M. Martinet, N. Marulli, F. Massey, R. J. Maurogordato, S. Medinaceli, E. Mei, S. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Mohr, J. J. Mora, A. Moresco, M. Moscardini, L. Nakajima, R. Neissner, C. Nichol, R. C. Niemi, S. -M. Padilla, C. Pasian, F. Pedersen, K. Percival, W. J. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L. A. Pozzetti, L. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rosset, C. Saglia, R. Sakr, Z. Sapone, D. Sartoris, B. Schirmer, M. Schneider, P. Secroun, A. Seidel, G. Seiffert, M. Serrano, S. Sirignano, C. Sirri, G. Mancini, A. Spurio Stanco, L. Steinwagner, J. Tallada-Crespí, P. Tereno, I. Tessore, N. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Valiviita, J. Vassallo, T. Kleijn, G. Verdoes Veropalumbo, A. Wang, Y. Weller, J. Zamorani, G. Zerbi, F. M. Zucca, E. Bolzonella, M. Burigana, C. Gabarra, L. Martín-Fleitas, J. Matthew, S. Pezzotta, A. Scottez, V. Sereno, M. Viel, M. Scott, D. Cosmology and Nongalactic Astrophysics The Euclid space telescope of the European Space Agency (ESA) is designed to provide sensitive and accurate measurements of weak gravitational lensing distortions over wide areas on the sky. Here we present a weak gravitational lensing analysis of early Euclid observations obtained for the field around the massive galaxy cluster Abell 2390 as part of the Euclid Early Release Observations programme. We conduct galaxy shape measurements using three independent algorithms (LensMC, KSB+, and SourceXtractor++). Incorporating multi-band photometry from Euclid and Subaru/Suprime-Cam, we estimate photometric redshifts to preferentially select background sources from tomographic redshift bins, for which we calibrate the redshift distributions using the self-organising map approach and data from the Cosmic Evolution Survey (COSMOS). We quantify the residual cluster member contamination and correct for it in bins of photometric redshift and magnitude using their source density profiles, including corrections for source obscuration and magnification. We reconstruct the cluster mass distribution and jointly fit the tangential reduced shear profiles of the different tomographic bins with spherical Navarro--Frenk--White profile predictions to constrain the cluster mass, finding consistent results for the three shape catalogues and good agreement with earlier measurements. As an important validation test we compare these joint constraints to mass measurements obtained individually for the different tomographic bins, finding good consistency. More detailed constraints on the cluster properties are presented in a companion paper that additionally incorporates strong lensing measurements. Our analysis provides a first demonstration of the outstanding capabilities of Euclid for tomographic weak lensing measurements.
title	Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
topic	Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2507.07629