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Hauptverfasser: Atek, H., Gavazzi, R., Weaver, J. R., Diego, J. M., Schrabback, T., Hatch, N. A., Aghanim, N., Dole, H., Hartley, W. G., Taamoli, S., Congedo, G., Jimenez-Teja, Y., Cuillandre, J. -C., Bañados, E., Belladitta, S., Bowler, R. A. A., Franco, M., Jauzac, M., Mahler, G., Richard, J., Rocci, P. -F., Serjeant, S., Toft, S., Abriola, D., Bergamini, P., Biviano, A., Dimauro, P., Ezziati, M., Golden-Marx, J. B., Grillo, C., Hughes, A. C. N., Kang, Y., Kneib, J. -P., Lombardi, M., Mamon, G. A., McPartland, C. J. R., Meneghetti, M., Miyatake, H., Montes, M., Mortlock, D. J., Oesch, P. A., Okabe, N., Rosati, P., Taylor, A. N., Tarsitano, F., Weller, J., Kluge, M., Laureijs, R., Paltani, S., Saifollahi, T., Schirmer, M., Stone, C., Mora, A., Altieri, B., Amara, A., Andreon, S., Auricchio, N., Baldi, M., Balestra, A., Bardelli, S., Basset, A., Bender, R., Bodendorf, C., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Candini, G. P., Capobianco, V., Carbone, C., Cardone, V. F., Carretero, J., Casas, S., Castander, F. J., Castellano, M., Cavuoti, S., Cimatti, A., Conselice, C. J., Conversi, L., Copin, Y., Corcione, L., Courbin, F., Courtois, H. M., Da Silva, A., Degaudenzi, H., Di Giorgio, A. M., Dinis, J., Douspis, M., Dubath, F., Dupac, X., Dusini, S., Ealet, A., Farina, M., Farrens, S., Ferriol, S., Fotopoulou, S., Frailis, M., Franceschi, E., Galeotta, S., Gillard, W., Gillis, B., Giocoli, C., Gómez-Alvarez, P., Grazian, A., Grupp, F., Guzzo, L., Hailey, M., Haugan, S. V. H., Hoar, J., Hoekstra, H., Holliman, M. S., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Hudelot, P., Jahnke, K., Jhabvala, M., Keihänen, E., Kermiche, S., Kiessling, A., Kitching, T., Kohley, R., Kubik, B., Kuijken, K., Kümmel, M., Kunz, M., Kurki-Suonio, H., Lahav, O., Mignant, D. Le, Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Maino, D., Maiorano, E., Mansutti, O., Marggraf, O., Markovic, K., Martinet, N., Marulli, F., Massey, R., Maurogordato, S., McCracken, H. J., Mei, S., Mellier, Y., Merlin, E., Meylan, G., Moresco, M., Moscardini, L., Nakajima, R., Nichol, R. C., Niemi, S. -M., Padilla, C., Paech, K., Pasian, F., Peacock, J. A., 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., Saglia, R., Sapone, D., Schneider, P., Secroun, A., Seidel, G., Serrano, S., Sirignano, C., Sirri, G., Skottfelt, J., Stanco, L., Tallada-Crespí, P., Teplitz, H. I., Tereno, I., Toledo-Moreo, R., Tutusaus, I., Valenziano, L., Vassallo, T., Kleijn, G. Verdoes, Veropalumbo, A., Wang, Y., Zucca, E., Baccigalupi, C., Burigana, C., Castignani, G., Sakr, Z., Scottez, V., Viel, M., Simon, P., Stern, D., Martín-Fleitas, J., Scott, D.
Format: Preprint
Veröffentlicht: 2024
Schlagworte:
Astrophysics of Galaxies
Online-Zugang:https://arxiv.org/abs/2405.13504
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author Atek, H.
Gavazzi, R.
Weaver, J. R.
Diego, J. M.
Schrabback, T.
Hatch, N. A.
Aghanim, N.
Dole, H.
Hartley, W. G.
Taamoli, S.
Congedo, G.
Jimenez-Teja, Y.
Cuillandre, J. -C.
Bañados, E.
Belladitta, S.
Bowler, R. A. A.
Franco, M.
Jauzac, M.
Mahler, G.
Richard, J.
Rocci, P. -F.
Serjeant, S.
Toft, S.
Abriola, D.
Bergamini, P.
Biviano, A.
Dimauro, P.
Ezziati, M.
Golden-Marx, J. B.
Grillo, C.
Hughes, A. C. N.
Kang, Y.
Kneib, J. -P.
Lombardi, M.
Mamon, G. A.
McPartland, C. J. R.
Meneghetti, M.
Miyatake, H.
Montes, M.
Mortlock, D. J.
Oesch, P. A.
Okabe, N.
Rosati, P.
Taylor, A. N.
Tarsitano, F.
Weller, J.
Kluge, M.
Laureijs, R.
Paltani, S.
Saifollahi, T.
Schirmer, M.
Stone, C.
Mora, A.
Altieri, B.
Amara, A.
Andreon, S.
Auricchio, N.
Baldi, M.
Balestra, A.
Bardelli, S.
Basset, A.
Bender, R.
Bodendorf, C.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Candini, G. P.
Capobianco, V.
Carbone, C.
Cardone, V. F.
Carretero, J.
Casas, S.
Castander, F. J.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Conselice, C. J.
Conversi, L.
Copin, Y.
Corcione, L.
Courbin, F.
Courtois, H. M.
Da Silva, A.
Degaudenzi, H.
Di Giorgio, A. M.
Dinis, J.
Douspis, M.
Dubath, F.
Dupac, X.
Dusini, S.
Ealet, A.
Farina, M.
Farrens, S.
Ferriol, S.
Fotopoulou, S.
Frailis, M.
Franceschi, E.
Galeotta, S.
Gillard, W.
Gillis, B.
Giocoli, C.
Gómez-Alvarez, P.
Grazian, A.
Grupp, F.
Guzzo, L.
Hailey, M.
Haugan, S. V. H.
Hoar, J.
Hoekstra, H.
Holliman, M. S.
Holmes, W.
Hook, I.
Hormuth, F.
Hornstrup, A.
Hudelot, P.
Jahnke, K.
Jhabvala, M.
Keihänen, E.
Kermiche, S.
Kiessling, A.
Kitching, T.
Kohley, R.
Kubik, B.
Kuijken, K.
Kümmel, M.
Kunz, M.
Kurki-Suonio, H.
Lahav, O.
Mignant, D. Le
Ligori, S.
Lilje, P. B.
Lindholm, V.
Lloro, I.
Maino, D.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Markovic, K.
Martinet, N.
Marulli, F.
Massey, R.
Maurogordato, S.
McCracken, H. J.
Mei, S.
Mellier, Y.
Merlin, E.
Meylan, G.
Moresco, M.
Moscardini, L.
Nakajima, R.
Nichol, R. C.
Niemi, S. -M.
Padilla, C.
Paech, K.
Pasian, F.
Peacock, J. A.
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.
Saglia, R.
Sapone, D.
Schneider, P.
Secroun, A.
Seidel, G.
Serrano, S.
Sirignano, C.
Sirri, G.
Skottfelt, J.
Stanco, L.
Tallada-Crespí, P.
Teplitz, H. I.
Tereno, I.
Toledo-Moreo, R.
Tutusaus, I.
Valenziano, L.
Vassallo, T.
Kleijn, G. Verdoes
Veropalumbo, A.
Wang, Y.
Zucca, E.
Baccigalupi, C.
Burigana, C.
Castignani, G.
Sakr, Z.
Scottez, V.
Viel, M.
Simon, P.
Stern, D.
Martín-Fleitas, J.
Scott, D.
author_facet Atek, H.
Gavazzi, R.
Weaver, J. R.
Diego, J. M.
Schrabback, T.
Hatch, N. A.
Aghanim, N.
Dole, H.
Hartley, W. G.
Taamoli, S.
Congedo, G.
Jimenez-Teja, Y.
Cuillandre, J. -C.
Bañados, E.
Belladitta, S.
Bowler, R. A. A.
Franco, M.
Jauzac, M.
Mahler, G.
Richard, J.
Rocci, P. -F.
Serjeant, S.
Toft, S.
Abriola, D.
Bergamini, P.
Biviano, A.
Dimauro, P.
Ezziati, M.
Golden-Marx, J. B.
Grillo, C.
Hughes, A. C. N.
Kang, Y.
Kneib, J. -P.
Lombardi, M.
Mamon, G. A.
McPartland, C. J. R.
Meneghetti, M.
Miyatake, H.
Montes, M.
Mortlock, D. J.
Oesch, P. A.
Okabe, N.
Rosati, P.
Taylor, A. N.
Tarsitano, F.
Weller, J.
Kluge, M.
Laureijs, R.
Paltani, S.
Saifollahi, T.
Schirmer, M.
Stone, C.
Mora, A.
Altieri, B.
Amara, A.
Andreon, S.
Auricchio, N.
Baldi, M.
Balestra, A.
Bardelli, S.
Basset, A.
Bender, R.
Bodendorf, C.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Candini, G. P.
Capobianco, V.
Carbone, C.
Cardone, V. F.
Carretero, J.
Casas, S.
Castander, F. J.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Conselice, C. J.
Conversi, L.
Copin, Y.
Corcione, L.
Courbin, F.
Courtois, H. M.
Da Silva, A.
Degaudenzi, H.
Di Giorgio, A. M.
Dinis, J.
Douspis, M.
Dubath, F.
Dupac, X.
Dusini, S.
Ealet, A.
Farina, M.
Farrens, S.
Ferriol, S.
Fotopoulou, S.
Frailis, M.
Franceschi, E.
Galeotta, S.
Gillard, W.
Gillis, B.
Giocoli, C.
Gómez-Alvarez, P.
Grazian, A.
Grupp, F.
Guzzo, L.
Hailey, M.
Haugan, S. V. H.
Hoar, J.
Hoekstra, H.
Holliman, M. S.
Holmes, W.
Hook, I.
Hormuth, F.
Hornstrup, A.
Hudelot, P.
Jahnke, K.
Jhabvala, M.
Keihänen, E.
Kermiche, S.
Kiessling, A.
Kitching, T.
Kohley, R.
Kubik, B.
Kuijken, K.
Kümmel, M.
Kunz, M.
Kurki-Suonio, H.
Lahav, O.
Mignant, D. Le
Ligori, S.
Lilje, P. B.
Lindholm, V.
Lloro, I.
Maino, D.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Markovic, K.
Martinet, N.
Marulli, F.
Massey, R.
Maurogordato, S.
McCracken, H. J.
Mei, S.
Mellier, Y.
Merlin, E.
Meylan, G.
Moresco, M.
Moscardini, L.
Nakajima, R.
Nichol, R. C.
Niemi, S. -M.
Padilla, C.
Paech, K.
Pasian, F.
Peacock, J. A.
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.
Saglia, R.
Sapone, D.
Schneider, P.
Secroun, A.
Seidel, G.
Serrano, S.
Sirignano, C.
Sirri, G.
Skottfelt, J.
Stanco, L.
Tallada-Crespí, P.
Teplitz, H. I.
Tereno, I.
Toledo-Moreo, R.
Tutusaus, I.
Valenziano, L.
Vassallo, T.
Kleijn, G. Verdoes
Veropalumbo, A.
Wang, Y.
Zucca, E.
Baccigalupi, C.
Burigana, C.
Castignani, G.
Sakr, Z.
Scottez, V.
Viel, M.
Simon, P.
Stern, D.
Martín-Fleitas, J.
Scott, D.
contents We present the first analysis of the Euclid Early Release Observations (ERO) program that targets fields around two lensing clusters, Abell 2390 and Abell 2764. We use VIS and NISP imaging to produce photometric catalogs for a total of $\sim 500\,000$ objects. The imaging data reach a $5\,σ$ typical depth in the range 25.1-25.4 AB in the NISP bands, and 27.1-27.3 AB in the VIS band. Using the Lyman-break method in combination with photometric redshifts, we identify $30$ Lyman-break galaxy (LBG) candidates at $z>6$ and 139 extremely red sources (ERSs), most likely at lower redshift. The deeper VIS imaging compared to NISP means we can routinely identify high-redshift Lyman breaks of the order of $3$ magnitudes, which reduces contamination by brown dwarf stars and low-redshift galaxies. Spectroscopic follow-up campaigns of such bright sources will help constrain both the bright end of the ultraviolet galaxy luminosity function and the quasar luminosity function at $z>6$, and constrain the physical nature of these objects. Additionally, we have performed a combined strong lensing and weak lensing analysis of A2390, and demonstrate how Euclid will contribute to better constraining the virial mass of galaxy clusters. From these data, we also identify optical and near-infrared counterparts of known $z>0.6$ clusters, which exhibit strong lensing features, establishing the ability of Euclid to characterize high-redshift clusters. Finally, we provide a glimpse of Euclid's ability to map the intracluster light out to larger radii than current facilities, enabling a better understanding of the cluster assembly history and mapping of the dark matter distribution. This initial dataset illustrates the diverse spectrum of legacy science that will be enabled by the Euclid survey.
format Preprint
id arxiv_https___arxiv_org_abs_2405_13504
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Euclid: Early Release Observations -- A preview of the Euclid era through a galaxy cluster magnifying lens
Atek, H.
Gavazzi, R.
Weaver, J. R.
Diego, J. M.
Schrabback, T.
Hatch, N. A.
Aghanim, N.
Dole, H.
Hartley, W. G.
Taamoli, S.
Congedo, G.
Jimenez-Teja, Y.
Cuillandre, J. -C.
Bañados, E.
Belladitta, S.
Bowler, R. A. A.
Franco, M.
Jauzac, M.
Mahler, G.
Richard, J.
Rocci, P. -F.
Serjeant, S.
Toft, S.
Abriola, D.
Bergamini, P.
Biviano, A.
Dimauro, P.
Ezziati, M.
Golden-Marx, J. B.
Grillo, C.
Hughes, A. C. N.
Kang, Y.
Kneib, J. -P.
Lombardi, M.
Mamon, G. A.
McPartland, C. J. R.
Meneghetti, M.
Miyatake, H.
Montes, M.
Mortlock, D. J.
Oesch, P. A.
Okabe, N.
Rosati, P.
Taylor, A. N.
Tarsitano, F.
Weller, J.
Kluge, M.
Laureijs, R.
Paltani, S.
Saifollahi, T.
Schirmer, M.
Stone, C.
Mora, A.
Altieri, B.
Amara, A.
Andreon, S.
Auricchio, N.
Baldi, M.
Balestra, A.
Bardelli, S.
Basset, A.
Bender, R.
Bodendorf, C.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Candini, G. P.
Capobianco, V.
Carbone, C.
Cardone, V. F.
Carretero, J.
Casas, S.
Castander, F. J.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Conselice, C. J.
Conversi, L.
Copin, Y.
Corcione, L.
Courbin, F.
Courtois, H. M.
Da Silva, A.
Degaudenzi, H.
Di Giorgio, A. M.
Dinis, J.
Douspis, M.
Dubath, F.
Dupac, X.
Dusini, S.
Ealet, A.
Farina, M.
Farrens, S.
Ferriol, S.
Fotopoulou, S.
Frailis, M.
Franceschi, E.
Galeotta, S.
Gillard, W.
Gillis, B.
Giocoli, C.
Gómez-Alvarez, P.
Grazian, A.
Grupp, F.
Guzzo, L.
Hailey, M.
Haugan, S. V. H.
Hoar, J.
Hoekstra, H.
Holliman, M. S.
Holmes, W.
Hook, I.
Hormuth, F.
Hornstrup, A.
Hudelot, P.
Jahnke, K.
Jhabvala, M.
Keihänen, E.
Kermiche, S.
Kiessling, A.
Kitching, T.
Kohley, R.
Kubik, B.
Kuijken, K.
Kümmel, M.
Kunz, M.
Kurki-Suonio, H.
Lahav, O.
Mignant, D. Le
Ligori, S.
Lilje, P. B.
Lindholm, V.
Lloro, I.
Maino, D.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Markovic, K.
Martinet, N.
Marulli, F.
Massey, R.
Maurogordato, S.
McCracken, H. J.
Mei, S.
Mellier, Y.
Merlin, E.
Meylan, G.
Moresco, M.
Moscardini, L.
Nakajima, R.
Nichol, R. C.
Niemi, S. -M.
Padilla, C.
Paech, K.
Pasian, F.
Peacock, J. A.
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.
Saglia, R.
Sapone, D.
Schneider, P.
Secroun, A.
Seidel, G.
Serrano, S.
Sirignano, C.
Sirri, G.
Skottfelt, J.
Stanco, L.
Tallada-Crespí, P.
Teplitz, H. I.
Tereno, I.
Toledo-Moreo, R.
Tutusaus, I.
Valenziano, L.
Vassallo, T.
Kleijn, G. Verdoes
Veropalumbo, A.
Wang, Y.
Zucca, E.
Baccigalupi, C.
Burigana, C.
Castignani, G.
Sakr, Z.
Scottez, V.
Viel, M.
Simon, P.
Stern, D.
Martín-Fleitas, J.
Scott, D.
Astrophysics of Galaxies
We present the first analysis of the Euclid Early Release Observations (ERO) program that targets fields around two lensing clusters, Abell 2390 and Abell 2764. We use VIS and NISP imaging to produce photometric catalogs for a total of $\sim 500\,000$ objects. The imaging data reach a $5\,σ$ typical depth in the range 25.1-25.4 AB in the NISP bands, and 27.1-27.3 AB in the VIS band. Using the Lyman-break method in combination with photometric redshifts, we identify $30$ Lyman-break galaxy (LBG) candidates at $z>6$ and 139 extremely red sources (ERSs), most likely at lower redshift. The deeper VIS imaging compared to NISP means we can routinely identify high-redshift Lyman breaks of the order of $3$ magnitudes, which reduces contamination by brown dwarf stars and low-redshift galaxies. Spectroscopic follow-up campaigns of such bright sources will help constrain both the bright end of the ultraviolet galaxy luminosity function and the quasar luminosity function at $z>6$, and constrain the physical nature of these objects. Additionally, we have performed a combined strong lensing and weak lensing analysis of A2390, and demonstrate how Euclid will contribute to better constraining the virial mass of galaxy clusters. From these data, we also identify optical and near-infrared counterparts of known $z>0.6$ clusters, which exhibit strong lensing features, establishing the ability of Euclid to characterize high-redshift clusters. Finally, we provide a glimpse of Euclid's ability to map the intracluster light out to larger radii than current facilities, enabling a better understanding of the cluster assembly history and mapping of the dark matter distribution. This initial dataset illustrates the diverse spectrum of legacy science that will be enabled by the Euclid survey.
title Euclid: Early Release Observations -- A preview of the Euclid era through a galaxy cluster magnifying lens
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2405.13504

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