Mostrar el registro sencillo del ítem
Euclid: The Early Release Observations Lens Search Experiment
dc.contributor.author | ACEVEDO BARROSO, J.A | |
dc.contributor.author | O'RIORDAN, C.M | |
dc.contributor.author | CLÉMENT, B | |
dc.contributor.author | TORTORA, C | |
dc.contributor.author | COLLETT, T.E | |
dc.contributor.author | COURBIN, F | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | GAVAZZI, R | |
dc.contributor.author | METCALF, R.B | |
dc.contributor.author | BUSILLO, V | |
dc.contributor.author | ANDIKA, I.T | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | CABANAC, R | |
hal.structure.identifier | Institut de Physique des 2 Infinis de Lyon [IP2I Lyon] | |
dc.contributor.author | COURTOIS, H.M | |
dc.contributor.author | CROOK-MANSOUR, J | |
dc.contributor.author | DELCHAMBRE, L | |
dc.contributor.author | DESPALI, G | |
dc.contributor.author | ECKER, L.R | |
dc.contributor.author | FRANCO, A | |
dc.contributor.author | HOLLOWAY, P | |
dc.contributor.author | JACKSON, N | |
dc.contributor.author | JAHNKE, K | |
dc.contributor.author | MAHLER, G | |
dc.contributor.author | MARCHETTI, L | |
dc.contributor.author | MATAVULJ, P | |
dc.contributor.author | MELO, A | |
dc.contributor.author | MENEGHETTI, M | |
dc.contributor.author | MOUSTAKAS, L.A | |
dc.contributor.author | MÜLLER, O | |
dc.contributor.author | NUCITA, A.A | |
dc.contributor.author | PAULINO-AFONSO, A | |
dc.contributor.author | PEARSON, J | |
dc.contributor.author | ROJAS, K | |
dc.contributor.author | SCARLATA, C | |
dc.contributor.author | SCHULDT, S | |
dc.contributor.author | SERJEANT, S | |
dc.contributor.author | SLUSE, D | |
dc.contributor.author | SUYU, S.H | |
dc.contributor.author | VACCARI, M | |
dc.contributor.author | VERMA, A | |
dc.contributor.author | VERNARDOS, G | |
dc.contributor.author | WALMSLEY, M | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
hal.structure.identifier | Institut universitaire de France [IUF] | |
dc.contributor.author | BOUY, H | |
dc.contributor.author | WALTH, G.L | |
dc.contributor.author | POWELL, D.M | |
dc.contributor.author | BOLZONELLA, M | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CUILLANDRE, J.-C | |
dc.contributor.author | KLUGE, M | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [ObAS] | |
dc.contributor.author | SAIFOLLAHI, T | |
dc.contributor.author | SCHIRMER, M | |
dc.contributor.author | STONE, C | |
dc.contributor.author | ACEBRON, A | |
dc.contributor.author | BAZZANINI, L | |
dc.contributor.author | DÍAZ-SÁNCHEZ, A | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | HOGG, N.B | |
dc.contributor.author | KOOPMANS, L.V.E | |
dc.contributor.author | KRUK, S | |
dc.contributor.author | LEUZZI, L | |
dc.contributor.author | MANJÓN-GARCÍA, A | |
dc.contributor.author | MANNUCCI, F | |
dc.contributor.author | NAGAM, B.C | |
dc.contributor.author | PEARCE-CASEY, R | |
dc.contributor.author | SCHARRÉ, L | |
dc.contributor.author | WILDE, J | |
dc.contributor.author | ALTIERI, B | |
dc.contributor.author | AMARA, A | |
dc.contributor.author | ANDREON, S | |
dc.contributor.author | AURICCHIO, N | |
dc.contributor.author | BACCIGALUPI, C | |
dc.contributor.author | BALDI, M | |
dc.contributor.author | BALESTRA, A | |
dc.contributor.author | BARDELLI, S | |
hal.structure.identifier | Centre National d'Études Spatiales [Toulouse] [CNES] | |
dc.contributor.author | BASSET, A | |
dc.contributor.author | BATTAGLIA, P | |
dc.contributor.author | BENDER, R | |
dc.contributor.author | BONINO, D | |
dc.contributor.author | BRANCHINI, E | |
dc.contributor.author | BRESCIA, M | |
dc.contributor.author | BRINCHMANN, J | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | CAILLAT, A | |
dc.contributor.author | CAMERA, S | |
dc.contributor.author | CANDINI, G.P | |
dc.contributor.author | CAPOBIANCO, V | |
dc.contributor.author | CARBONE, C | |
dc.contributor.author | CARRETERO, J | |
dc.contributor.author | CASAS, S | |
dc.contributor.author | CASTELLANO, M | |
dc.contributor.author | CASTIGNANI, G | |
dc.contributor.author | CAVUOTI, S | |
dc.contributor.author | CIMATTI, A | |
dc.contributor.author | COLODRO-CONDE, C | |
dc.contributor.author | CONGEDO, G | |
dc.contributor.author | CONSELICE, C.J | |
dc.contributor.author | CONVERSI, L | |
hal.structure.identifier | Institut de Physique des 2 Infinis de Lyon [IP2I Lyon] | |
dc.contributor.author | COPIN, Y | |
dc.contributor.author | CORCIONE, L | |
dc.contributor.author | CROPPER, M | |
dc.contributor.author | DA SILVA, A | |
dc.contributor.author | DEGAUDENZI, H | |
dc.contributor.author | DE LUCIA, G | |
dc.contributor.author | DINIS, J | |
dc.contributor.author | DUBATH, F | |
dc.contributor.author | DUPAC, X | |
dc.contributor.author | DUSINI, S | |
dc.contributor.author | FARINA, M | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | FARRENS, S | |
hal.structure.identifier | Institut de Physique des 2 Infinis de Lyon [IP2I Lyon] | |
dc.contributor.author | FERRIOL, S | |
dc.contributor.author | FRAILIS, M | |
dc.contributor.author | FRANCESCHI, E | |
dc.contributor.author | GALEOTTA, S | |
dc.contributor.author | GARILLI, B | |
dc.contributor.author | GEORGE, K | |
hal.structure.identifier | Centre de Physique des Particules de Marseille [CPPM] | |
dc.contributor.author | GILLARD, W | |
dc.contributor.author | GILLIS, B | |
dc.contributor.author | GIOCOLI, C | |
dc.contributor.author | GÓMEZ-ALVAREZ, P | |
dc.contributor.author | GRAZIAN, A | |
dc.contributor.author | GRUPP, F | |
dc.contributor.author | GUZZO, L | |
dc.contributor.author | HAUGAN, S.V.H | |
dc.contributor.author | HOEKSTRA, H | |
dc.contributor.author | HOLMES, W | |
dc.contributor.author | HOOK, I | |
dc.contributor.author | HORMUTH, F | |
dc.contributor.author | HORNSTRUP, A | |
dc.contributor.author | JHABVALA, M | |
dc.contributor.author | JOACHIMI, B | |
dc.contributor.author | KEIHÄNEN, E | |
hal.structure.identifier | Centre de Physique des Particules de Marseille [CPPM] | |
dc.contributor.author | KERMICHE, S | |
dc.contributor.author | KIESSLING, A | |
hal.structure.identifier | Institut de Physique des 2 Infinis de Lyon [IP2I Lyon] | |
dc.contributor.author | KUBIK, B | |
dc.contributor.author | KUNZ, M | |
dc.contributor.author | KURKI-SUONIO, H | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | LE MIGNANT, D | |
dc.contributor.author | LIGORI, S | |
dc.contributor.author | LILJE, P.B | |
dc.contributor.author | LINDHOLM, V | |
dc.contributor.author | LLORO, I | |
hal.structure.identifier | Centre de Calcul de l'IN2P3 [CC-IN2P3] | |
dc.contributor.author | MAINETTI, G | |
dc.contributor.author | MAIORANO, E | |
dc.contributor.author | MANSUTTI, O | |
dc.contributor.author | MARCIN, S | |
dc.contributor.author | MARGGRAF, O | |
dc.contributor.author | MARTINELLI, M | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | MARTINET, N | |
dc.contributor.author | MARULLI, F | |
dc.contributor.author | MASSEY, R | |
dc.contributor.author | MEDINACELI, E | |
dc.contributor.author | MELCHIOR, M | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | MELLIER, Y | |
dc.contributor.author | MERLIN, E | |
dc.contributor.author | MEYLAN, G | |
dc.contributor.author | MORESCO, M | |
dc.contributor.author | MOSCARDINI, L | |
dc.contributor.author | MUNARI, E | |
dc.contributor.author | NAKAJIMA, R | |
dc.contributor.author | NEISSNER, C | |
dc.contributor.author | NICHOL, R.C | |
hal.structure.identifier | Agence Spatiale Européenne = European Space Agency [ESA] | |
dc.contributor.author | NIEMI, S.-M | |
dc.contributor.author | NIGHTINGALE, J.W | |
dc.contributor.author | PADILLA, C | |
dc.contributor.author | PALTANI, S | |
dc.contributor.author | PASIAN, F | |
dc.contributor.author | PEDERSEN, K | |
dc.contributor.author | PERCIVAL, W.J | |
hal.structure.identifier | Agence Spatiale Européenne = European Space Agency [ESA] | |
dc.contributor.author | PETTORINO, V | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | PIRES, S | |
dc.contributor.author | POLENTA, G | |
hal.structure.identifier | Centre National d'Études Spatiales [Toulouse] [CNES] | |
dc.contributor.author | PONCET, M | |
dc.contributor.author | POPA, L.A | |
dc.contributor.author | POZZETTI, L | |
dc.contributor.author | RAISON, F | |
dc.contributor.author | REBOLO, R | |
dc.contributor.author | RENZI, A | |
dc.contributor.author | RHODES, J | |
dc.contributor.author | RICCIO, G | |
dc.contributor.author | ROMELLI, E | |
dc.contributor.author | RONCARELLI, M | |
dc.contributor.author | ROSSETTI, E | |
dc.contributor.author | SAGLIA, R | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | SAKR, Z | |
dc.contributor.author | SÁNCHEZ, A.G | |
dc.contributor.author | SAPONE, D | |
dc.contributor.author | SCHNEIDER, P | |
dc.contributor.author | SCHRABBACK, T | |
hal.structure.identifier | Centre de Physique des Particules de Marseille [CPPM] | |
dc.contributor.author | SECROUN, A | |
dc.contributor.author | SEIDEL, G | |
dc.contributor.author | SERRANO, S | |
dc.contributor.author | SIRIGNANO, C | |
dc.contributor.author | SIRRI, G | |
dc.contributor.author | SKOTTFELT, J | |
dc.contributor.author | STANCO, L | |
dc.contributor.author | STEINWAGNER, J | |
dc.contributor.author | TALLADA-CRESPÍ, P | |
dc.contributor.author | TAVAGNACCO, D | |
dc.contributor.author | TAYLOR, A.N | |
dc.contributor.author | TERENO, I | |
dc.contributor.author | TOLEDO-MOREO, R | |
dc.contributor.author | TORRADEFLOT, F | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | TUTUSAUS, I | |
dc.contributor.author | VALENTIJN, E.A | |
dc.contributor.author | VALENZIANO, L | |
dc.contributor.author | VASSALLO, T | |
dc.contributor.author | WANG, Y | |
dc.contributor.author | WELLER, J | |
dc.contributor.author | ZUCCA, E | |
dc.contributor.author | BURIGANA, C | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
hal.structure.identifier | Laboratoire Paul Painlevé - UMR 8524 [LPP] | |
dc.contributor.author | SCOTTEZ, V | |
dc.contributor.author | VIEL, M | |
dc.date.accessioned | 2024-08-28T02:09:18Z | |
dc.date.available | 2024-08-28T02:09:18Z | |
dc.identifier.uri | https://oskar-bordeaux.fr/handle/20.500.12278/201337 | |
dc.description.abstractEn | We investigate the ability of the Euclid telescope to detect galaxy-scale gravitational lenses. To do so, we perform a systematic visual inspection of the $0.7\,\rm{deg}^2$ Euclid ERO data towards the Perseus cluster using both the high-resolution VIS $I_{\scriptscriptstyle\rm E}$ band, and the lower resolution NISP bands. We inspect every extended source brighter than magnitude $23$ in $I_{\scriptscriptstyle\rm E}$ with $41$ expert human classifiers. This amounts to $12\,086$ stamps of $10^{\prime\prime}\,\times\,10^{\prime\prime}$. We find $3$ grade A and $13$ grade B candidates. We assess 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 $0.\!\!^{\prime\prime}68\,<\,\theta_\mathrm{E}\,<1.\!\!^{\prime\prime}24$, 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 data set, our results corroborate the promise that Euclid will ultimately deliver a sample of around $10^5$ galaxy-scale lenses. | |
dc.language.iso | en | |
dc.title.en | Euclid: The Early Release Observations Lens Search Experiment | |
dc.type | Document de travail - Pré-publication | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph] | |
dc.identifier.arxiv | 2408.06217 | |
bordeaux.hal.laboratories | Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804 | * |
bordeaux.institution | Université de Bordeaux | |
bordeaux.institution | CNRS | |
hal.identifier | hal-04679199 | |
hal.version | 1 | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-04679199v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=ACEVEDO%20BARROSO,%20J.A&O'RIORDAN,%20C.M&CL%C3%89MENT,%20B&TORTORA,%20C&COLLETT,%20T.E&rft.genre=preprint |
Archivos en el ítem
Archivos | Tamaño | Formato | Ver |
---|---|---|---|
No hay archivos asociados a este ítem. |