Euclid: The Early Release Observations Lens Search Experiment

Fuente: arXiv

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Bibliographische Detailangaben
Hauptverfasser:	Barroso, J. A. Acevedo, O'Riordan, C. M., Clément, B., Tortora, C., Collett, T. E., Courbin, F., Gavazzi, R., Metcalf, R. B., Busillo, V., Andika, I. T., Cabanac, R., Courtois, H. M., Crook-Mansour, J., Delchambre, L., Despali, G., Ecker, L. R., Franco, A., Holloway, P., Jackson, N., Jahnke, K., Mahler, G., Marchetti, L., Matavulj, P., Melo, A., Meneghetti, M., Moustakas, L. A., Müller, O., Nucita, A. A., Paulino-Afonso, A., Pearson, J., Rojas, K., Scarlata, C., Schuldt, S., Serjeant, S., Sluse, D., Suyu, S. H., Vaccari, M., Verma, A., Vernardos, G., Walmsley, M., Bouy, H., Walth, G. L., Powell, D. M., Bolzonella, M., Cuillandre, J. -C., Kluge, M., Saifollahi, T., Schirmer, M., Stone, C., Acebron, A., Bazzanini, L., Díaz-Sánchez, A., Hogg, N. B., Koopmans, L. V. E., Kruk, S., Leuzzi, L., Manjón-García, A., Mannucci, F., Nagam, B. C., Pearce-Casey, R., Scharré, L., Wilde, J., Altieri, B., Amara, A., Andreon, S., Auricchio, N., Baccigalupi, C., Baldi, M., Balestra, A., Bardelli, S., Basset, A., Battaglia, P., Bender, R., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Caillat, A., Camera, S., Candini, G. P., Capobianco, V., Carbone, C., Carretero, J., Casas, S., Castellano, M., Castignani, G., Cavuoti, S., Cimatti, A., Colodro-Conde, C., Congedo, G., Conselice, C. J., Conversi, L., Copin, Y., Corcione, L., Cropper, M., Da Silva, A., Degaudenzi, H., De Lucia, G., Dinis, J., Dubath, F., Dupac, X., Dusini, S., Farina, M., Farrens, S., Ferriol, S., Frailis, M., Franceschi, E., Galeotta, S., Garilli, B., George, K., Gillard, W., Gillis, B., Giocoli, C., Gómez-Alvarez, P., Grazian, A., Grupp, F., Guzzo, L., Haugan, S. V. H., Hoekstra, H., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Jhabvala, M., Joachimi, B., Keihänen, E., Kermiche, S., Kiessling, A., Kubik, B., Kunz, M., Kurki-Suonio, H., Mignant, D. Le, Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Mainetti, G., Maiorano, E., Mansutti, O., Marcin, S., Marggraf, O., Martinelli, M., Martinet, N., Marulli, F., Massey, R., Medinaceli, E., Melchior, M., Mellier, Y., Merlin, E., Meylan, G., Moresco, M., Moscardini, L., Munari, E., Nakajima, R., Neissner, C., Nichol, R. C., Niemi, S. -M., Nightingale, J. W., 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., Rossetti, E., Saglia, R., Sakr, Z., Sánchez, A. G., Sapone, D., Schneider, P., Schrabback, T., Secroun, A., Seidel, G., Serrano, S., Sirignano, C., Sirri, G., Skottfelt, J., Stanco, L., Steinwagner, J., Tallada-Crespí, P., Tavagnacco, D., Taylor, A. N., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E. A., Valenziano, L., Vassallo, T., Wang, Y., Weller, J., Zucca, E., Burigana, C., Scottez, V., Viel, M., Scott, D., Vegetti, S.
Format:	Preprint
Veröffentlicht:	2024
Schlagworte:	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
Online-Zugang:	Acceder al recurso
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author	Barroso, J. A. Acevedo O'Riordan, C. M. Clément, B. Tortora, C. Collett, T. E. Courbin, F. Gavazzi, R. Metcalf, R. B. Busillo, V. Andika, I. T. Cabanac, R. Courtois, H. M. Crook-Mansour, J. Delchambre, L. Despali, G. Ecker, L. R. Franco, A. Holloway, P. Jackson, N. Jahnke, K. Mahler, G. Marchetti, L. Matavulj, P. Melo, A. Meneghetti, M. Moustakas, L. A. Müller, O. Nucita, A. A. Paulino-Afonso, A. Pearson, J. Rojas, K. Scarlata, C. Schuldt, S. Serjeant, S. Sluse, D. Suyu, S. H. Vaccari, M. Verma, A. Vernardos, G. Walmsley, M. Bouy, H. Walth, G. L. Powell, D. M. Bolzonella, M. Cuillandre, J. -C. Kluge, M. Saifollahi, T. Schirmer, M. Stone, C. Acebron, A. Bazzanini, L. Díaz-Sánchez, A. Hogg, N. B. Koopmans, L. V. E. Kruk, S. Leuzzi, L. Manjón-García, A. Mannucci, F. Nagam, B. C. Pearce-Casey, R. Scharré, L. Wilde, J. Altieri, B. Amara, A. Andreon, S. Auricchio, N. Baccigalupi, C. Baldi, M. Balestra, A. Bardelli, S. Basset, A. Battaglia, P. Bender, R. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Caillat, A. Camera, S. Candini, G. P. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Castignani, G. Cavuoti, S. Cimatti, A. Colodro-Conde, C. Congedo, G. Conselice, C. J. Conversi, L. Copin, Y. Corcione, L. Cropper, M. Da Silva, A. Degaudenzi, H. De Lucia, G. Dinis, J. Dubath, F. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Frailis, M. Franceschi, E. Galeotta, S. Garilli, B. George, K. Gillard, W. Gillis, B. Giocoli, C. Gómez-Alvarez, P. Grazian, A. Grupp, F. Guzzo, L. Haugan, S. V. H. Hoekstra, H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Jhabvala, M. Joachimi, B. Keihänen, E. Kermiche, S. Kiessling, A. Kubik, B. Kunz, M. Kurki-Suonio, H. Mignant, D. Le Ligori, S. Lilje, P. B. Lindholm, V. Lloro, I. Mainetti, G. Maiorano, E. Mansutti, O. Marcin, S. Marggraf, O. Martinelli, M. Martinet, N. Marulli, F. Massey, R. Medinaceli, E. Melchior, M. Mellier, Y. Merlin, E. Meylan, G. Moresco, M. Moscardini, L. Munari, E. Nakajima, R. Neissner, C. Nichol, R. C. Niemi, S. -M. Nightingale, J. W. 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. Rossetti, E. Saglia, R. Sakr, Z. Sánchez, A. G. Sapone, D. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Skottfelt, J. Stanco, L. Steinwagner, J. Tallada-Crespí, P. Tavagnacco, D. Taylor, A. N. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Vassallo, T. Wang, Y. Weller, J. Zucca, E. Burigana, C. Scottez, V. Viel, M. Scott, D. Vegetti, S.
author_facet	Barroso, J. A. Acevedo O'Riordan, C. M. Clément, B. Tortora, C. Collett, T. E. Courbin, F. Gavazzi, R. Metcalf, R. B. Busillo, V. Andika, I. T. Cabanac, R. Courtois, H. M. Crook-Mansour, J. Delchambre, L. Despali, G. Ecker, L. R. Franco, A. Holloway, P. Jackson, N. Jahnke, K. Mahler, G. Marchetti, L. Matavulj, P. Melo, A. Meneghetti, M. Moustakas, L. A. Müller, O. Nucita, A. A. Paulino-Afonso, A. Pearson, J. Rojas, K. Scarlata, C. Schuldt, S. Serjeant, S. Sluse, D. Suyu, S. H. Vaccari, M. Verma, A. Vernardos, G. Walmsley, M. Bouy, H. Walth, G. L. Powell, D. M. Bolzonella, M. Cuillandre, J. -C. Kluge, M. Saifollahi, T. Schirmer, M. Stone, C. Acebron, A. Bazzanini, L. Díaz-Sánchez, A. Hogg, N. B. Koopmans, L. V. E. Kruk, S. Leuzzi, L. Manjón-García, A. Mannucci, F. Nagam, B. C. Pearce-Casey, R. Scharré, L. Wilde, J. Altieri, B. Amara, A. Andreon, S. Auricchio, N. Baccigalupi, C. Baldi, M. Balestra, A. Bardelli, S. Basset, A. Battaglia, P. Bender, R. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Caillat, A. Camera, S. Candini, G. P. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Castignani, G. Cavuoti, S. Cimatti, A. Colodro-Conde, C. Congedo, G. Conselice, C. J. Conversi, L. Copin, Y. Corcione, L. Cropper, M. Da Silva, A. Degaudenzi, H. De Lucia, G. Dinis, J. Dubath, F. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Frailis, M. Franceschi, E. Galeotta, S. Garilli, B. George, K. Gillard, W. Gillis, B. Giocoli, C. Gómez-Alvarez, P. Grazian, A. Grupp, F. Guzzo, L. Haugan, S. V. H. Hoekstra, H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Jhabvala, M. Joachimi, B. Keihänen, E. Kermiche, S. Kiessling, A. Kubik, B. Kunz, M. Kurki-Suonio, H. Mignant, D. Le Ligori, S. Lilje, P. B. Lindholm, V. Lloro, I. Mainetti, G. Maiorano, E. Mansutti, O. Marcin, S. Marggraf, O. Martinelli, M. Martinet, N. Marulli, F. Massey, R. Medinaceli, E. Melchior, M. Mellier, Y. Merlin, E. Meylan, G. Moresco, M. Moscardini, L. Munari, E. Nakajima, R. Neissner, C. Nichol, R. C. Niemi, S. -M. Nightingale, J. W. 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. Rossetti, E. Saglia, R. Sakr, Z. Sánchez, A. G. Sapone, D. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Skottfelt, J. Stanco, L. Steinwagner, J. Tallada-Crespí, P. Tavagnacco, D. Taylor, A. N. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Vassallo, T. Wang, Y. Weller, J. Zucca, E. Burigana, C. Scottez, V. Viel, M. Scott, D. Vegetti, S.
contents	We investigated the ability of the Euclid telescope to detect galaxy-scale gravitational lenses. To do so, we performed a systematic visual inspection of the $0.7\,\rm{deg}^2$ Euclid Early Release Observations data towards the Perseus cluster using both the high-resolution $I_{\scriptscriptstyle\rm E}$ band and the lower-resolution $Y_{\scriptscriptstyle\rm E}$, $J_{\scriptscriptstyle\rm E}$, $H_{\scriptscriptstyle\rm E}$ bands. Each extended source brighter than magnitude 23 in $I_{\scriptscriptstyle\rm E}$ was inspected by 41 expert human classifiers. This amounts to $12\,086$ stamps of $10^{\prime\prime}\,\times\,10^{\prime\prime}$. We found $3$ grade A and $13$ grade B candidates. We assessed the validity of these $16$ candidates by modelling them and checking that they are consistent with a single source lensed by a plausible mass distribution. Five of the candidates pass this check, five others are rejected by the modelling, and six are inconclusive. Extrapolating from the five successfully modelled candidates, we infer that the full $14\,000\,{\rm deg}^2$ of the Euclid Wide Survey should contain $100\,000^{+70\,000}_{-30\,000}$ galaxy-galaxy lenses that are both discoverable through visual inspection and have valid lens models. This is consistent with theoretical forecasts of $170\,000$ discoverable galaxy-galaxy lenses in Euclid. Our five modelled lenses have Einstein radii in the range $0.\!\!^{\prime\prime}68\,<\,θ_\mathrm{E}\,<1.\!\!^{\prime\prime}24$, but their Einstein radius distribution is on the higher side when compared to theoretical forecasts. This suggests that our methodology is likely missing small-Einstein-radius systems. Whilst it is implausible to visually inspect the full Euclid dataset, our results corroborate the promise that Euclid will ultimately deliver a sample of around $10^5$ galaxy-scale lenses.
format	Preprint
id	arxiv_https___arxiv_org_abs_2408_06217
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Euclid: The Early Release Observations Lens Search Experiment Barroso, J. A. Acevedo O'Riordan, C. M. Clément, B. Tortora, C. Collett, T. E. Courbin, F. Gavazzi, R. Metcalf, R. B. Busillo, V. Andika, I. T. Cabanac, R. Courtois, H. M. Crook-Mansour, J. Delchambre, L. Despali, G. Ecker, L. R. Franco, A. Holloway, P. Jackson, N. Jahnke, K. Mahler, G. Marchetti, L. Matavulj, P. Melo, A. Meneghetti, M. Moustakas, L. A. Müller, O. Nucita, A. A. Paulino-Afonso, A. Pearson, J. Rojas, K. Scarlata, C. Schuldt, S. Serjeant, S. Sluse, D. Suyu, S. H. Vaccari, M. Verma, A. Vernardos, G. Walmsley, M. Bouy, H. Walth, G. L. Powell, D. M. Bolzonella, M. Cuillandre, J. -C. Kluge, M. Saifollahi, T. Schirmer, M. Stone, C. Acebron, A. Bazzanini, L. Díaz-Sánchez, A. Hogg, N. B. Koopmans, L. V. E. Kruk, S. Leuzzi, L. Manjón-García, A. Mannucci, F. Nagam, B. C. Pearce-Casey, R. Scharré, L. Wilde, J. Altieri, B. Amara, A. Andreon, S. Auricchio, N. Baccigalupi, C. Baldi, M. Balestra, A. Bardelli, S. Basset, A. Battaglia, P. Bender, R. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Caillat, A. Camera, S. Candini, G. P. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Castignani, G. Cavuoti, S. Cimatti, A. Colodro-Conde, C. Congedo, G. Conselice, C. J. Conversi, L. Copin, Y. Corcione, L. Cropper, M. Da Silva, A. Degaudenzi, H. De Lucia, G. Dinis, J. Dubath, F. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Frailis, M. Franceschi, E. Galeotta, S. Garilli, B. George, K. Gillard, W. Gillis, B. Giocoli, C. Gómez-Alvarez, P. Grazian, A. Grupp, F. Guzzo, L. Haugan, S. V. H. Hoekstra, H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Jhabvala, M. Joachimi, B. Keihänen, E. Kermiche, S. Kiessling, A. Kubik, B. Kunz, M. Kurki-Suonio, H. Mignant, D. Le Ligori, S. Lilje, P. B. Lindholm, V. Lloro, I. Mainetti, G. Maiorano, E. Mansutti, O. Marcin, S. Marggraf, O. Martinelli, M. Martinet, N. Marulli, F. Massey, R. Medinaceli, E. Melchior, M. Mellier, Y. Merlin, E. Meylan, G. Moresco, M. Moscardini, L. Munari, E. Nakajima, R. Neissner, C. Nichol, R. C. Niemi, S. -M. Nightingale, J. W. 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. Rossetti, E. Saglia, R. Sakr, Z. Sánchez, A. G. Sapone, D. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Skottfelt, J. Stanco, L. Steinwagner, J. Tallada-Crespí, P. Tavagnacco, D. Taylor, A. N. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Vassallo, T. Wang, Y. Weller, J. Zucca, E. Burigana, C. Scottez, V. Viel, M. Scott, D. Vegetti, S. Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics We investigated the ability of the Euclid telescope to detect galaxy-scale gravitational lenses. To do so, we performed a systematic visual inspection of the $0.7\,\rm{deg}^2$ Euclid Early Release Observations data towards the Perseus cluster using both the high-resolution $I_{\scriptscriptstyle\rm E}$ band and the lower-resolution $Y_{\scriptscriptstyle\rm E}$, $J_{\scriptscriptstyle\rm E}$, $H_{\scriptscriptstyle\rm E}$ bands. Each extended source brighter than magnitude 23 in $I_{\scriptscriptstyle\rm E}$ was inspected by 41 expert human classifiers. This amounts to $12\,086$ stamps of $10^{\prime\prime}\,\times\,10^{\prime\prime}$. We found $3$ grade A and $13$ grade B candidates. We assessed the validity of these $16$ candidates by modelling them and checking that they are consistent with a single source lensed by a plausible mass distribution. Five of the candidates pass this check, five others are rejected by the modelling, and six are inconclusive. Extrapolating from the five successfully modelled candidates, we infer that the full $14\,000\,{\rm deg}^2$ of the Euclid Wide Survey should contain $100\,000^{+70\,000}_{-30\,000}$ galaxy-galaxy lenses that are both discoverable through visual inspection and have valid lens models. This is consistent with theoretical forecasts of $170\,000$ discoverable galaxy-galaxy lenses in Euclid. Our five modelled lenses have Einstein radii in the range $0.\!\!^{\prime\prime}68\,<\,θ_\mathrm{E}\,<1.\!\!^{\prime\prime}24$, but their Einstein radius distribution is on the higher side when compared to theoretical forecasts. This suggests that our methodology is likely missing small-Einstein-radius systems. Whilst it is implausible to visually inspect the full Euclid dataset, our results corroborate the promise that Euclid will ultimately deliver a sample of around $10^5$ galaxy-scale lenses.
title	Euclid: The Early Release Observations Lens Search Experiment
topic	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2408.06217