hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CUILLANDRE, J.-C | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | BERTIN, E | |
dc.contributor.author | BOLZONELLA, 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 | GWYN, S | |
dc.contributor.author | ISANI, S | |
dc.contributor.author | KLUGE, M | |
hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
dc.contributor.author | LAI, O | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [ObAS] | |
dc.contributor.author | LANÇON, A | |
dc.contributor.author | LANG, D.A | |
hal.structure.identifier | Agence Spatiale Européenne = European Space Agency [ESA] | |
dc.contributor.author | LAUREIJS, R | |
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 | ABDURRO'UF, M | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | AGHANIM, N | |
dc.contributor.author | ALTIERI, B | |
dc.contributor.author | ANNIBALI, F | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | ATEK, H | |
dc.contributor.author | AWAD, P | |
dc.contributor.author | BAES, M | |
dc.contributor.author | BAÑADOS, E | |
dc.contributor.author | BARRADO, D | |
dc.contributor.author | BELLADITTA, S | |
dc.contributor.author | BELOKUROV, V | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | BOSELLI, A | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | BOURNAUD, F | |
dc.contributor.author | BOVY, J | |
dc.contributor.author | BOWLER, R.A.A | |
dc.contributor.author | BUENADICHA, G | |
dc.contributor.author | BUITRAGO, F | |
dc.contributor.author | CANTIELLO, M | |
dc.contributor.author | CAROLLO, D | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CODIS, S | |
dc.contributor.author | COLLINS, M.L.M | |
dc.contributor.author | CONGEDO, G | |
dc.contributor.author | DALESSANDRO, E | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | DE LAPPARENT, V | |
dc.contributor.author | DE PAOLIS, F | |
dc.contributor.author | DIEGO, J.M | |
dc.contributor.author | DIMAURO, P | |
dc.contributor.author | DINIS, J | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | DOLE, Hervé | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [ObAS] | |
dc.contributor.author | DUC, P.-A | |
dc.contributor.author | ERKAL, D | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | EZZIATI, M | |
dc.contributor.author | FERGUSON, A.M.N | |
dc.contributor.author | FERRÉ-MATEU, A | |
dc.contributor.author | FRANCO, A | |
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 | GEORGE, K | |
hal.structure.identifier | Centre de Physique des Particules de Marseille [CPPM] | |
dc.contributor.author | GILLARD, W | |
dc.contributor.author | GOLDEN-MARX, J.B | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [ObAS] | |
dc.contributor.author | GOLDMAN, B | |
dc.contributor.author | GONZALEZ, A.H | |
dc.contributor.author | HABAS, R | |
dc.contributor.author | HARTLEY, W.G | |
dc.contributor.author | HATCH, N.A | |
dc.contributor.author | KOHLEY, R | |
dc.contributor.author | HOAR, J | |
dc.contributor.author | HOWELL, J.M | |
dc.contributor.author | HUNT, L.K | |
dc.contributor.author | JABLONKA, P | |
dc.contributor.author | JAUZAC, M | |
dc.contributor.author | KANG, Y | |
dc.contributor.author | KNAPEN, J.H | |
dc.contributor.author | KNEIB, J.-P | |
dc.contributor.author | KUZMA, P.B | |
dc.contributor.author | LARSEN, S.S | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [ObAS] | |
dc.contributor.author | MARCHAL, O | |
dc.contributor.author | MARTÍN-FLEITAS, J | |
dc.contributor.author | MARCOS-ARENAL, P | |
dc.contributor.author | MARLEAU, F.R | |
dc.contributor.author | MARTÍN, E.L | |
dc.contributor.author | MASSARI, D | |
dc.contributor.author | MCCONNACHIE, A.W | |
dc.contributor.author | MENEGHETTI, M | |
dc.contributor.author | MILUZIO, M | |
dc.contributor.author | CARRETERO, J. Miro | |
dc.contributor.author | MIYATAKE, H | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | MONDELIN, M | |
dc.contributor.author | MONTES, M | |
dc.contributor.author | MORA, A | |
dc.contributor.author | MÜLLER, O | |
dc.contributor.author | NALLY, C | |
hal.structure.identifier | Agence Spatiale Européenne = European Space Agency [ESA] | |
dc.contributor.author | NOESKE, K | |
dc.contributor.author | NUCITA, A.A | |
dc.contributor.author | OESCH, P.A | |
dc.contributor.author | OGURI, M | |
dc.contributor.author | PELETIER, R.F | |
dc.contributor.author | POULAIN, M | |
hal.structure.identifier | Centre de Recherche Astrophysique de Lyon [CRAL] | |
dc.contributor.author | QUILLEY, L | |
hal.structure.identifier | Agence Spatiale Européenne = European Space Agency [ESA] | |
dc.contributor.author | RACCA, G.D | |
dc.contributor.author | REJKUBA, M | |
dc.contributor.author | RHODES, J | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | ROCCI, P.-F | |
dc.contributor.author | ROMÁN, J | |
dc.contributor.author | SACQUEGNA, S | |
dc.contributor.author | SAREMI, E | |
dc.contributor.author | SCARAMELLA, R | |
dc.contributor.author | SCHINNERER, E | |
dc.contributor.author | SERJEANT, S | |
dc.contributor.author | SOLA, E | |
hal.structure.identifier | Université de Lille, Sciences et Technologies | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | SORCE, J.G | |
dc.contributor.author | TARSITANO, F | |
dc.contributor.author | TERENO, I | |
dc.contributor.author | TOFT, S | |
dc.contributor.author | TORTORA, C | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [ObAS] | |
dc.contributor.author | URBANO, M | |
dc.contributor.author | VENHOLA, A | |
hal.structure.identifier | Observatoire astronomique de Strasbourg [ObAS] | |
dc.contributor.author | VOGGEL, K | |
dc.contributor.author | WEAVER, J.R | |
dc.contributor.author | XU, X | |
dc.contributor.author | ŽERJAL, M | |
dc.contributor.author | ZÖLLER, R | |
dc.contributor.author | ANDREON, S | |
dc.contributor.author | AURICCHIO, N | |
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 | BENDER, R | |
dc.contributor.author | BODENDORF, C | |
dc.contributor.author | BRANCHINI, E | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | BRAU-NOGUE, S | |
dc.contributor.author | BRESCIA, M | |
dc.contributor.author | BRINCHMANN, J | |
dc.contributor.author | CAMERA, S | |
dc.contributor.author | CAPOBIANCO, V | |
dc.contributor.author | CARBONE, C | |
dc.contributor.author | CARRETERO, J | |
dc.contributor.author | CASAS, S | |
dc.contributor.author | CASTANDER, F.J | |
dc.contributor.author | CASTELLANO, M | |
dc.contributor.author | CAVUOTI, S | |
dc.contributor.author | CIMATTI, A | |
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 | COURBIN, F | |
hal.structure.identifier | Institut de Physique des 2 Infinis de Lyon [IP2I Lyon] | |
dc.contributor.author | COURTOIS, H.M | |
dc.contributor.author | CROPPER, M | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | CUBY, J.-G | |
dc.contributor.author | DA SILVA, A | |
dc.contributor.author | DEGAUDENZI, H | |
dc.contributor.author | DI GIORGIO, A.M | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | DOUSPIS, Marian | |
dc.contributor.author | DUNCAN, C.A.J | |
dc.contributor.author | DUPAC, X | |
dc.contributor.author | DUSINI, S | |
dc.contributor.author | FABRICIUS, M | |
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 | FOTOPOULOU, S | |
dc.contributor.author | FRAILIS, M | |
dc.contributor.author | FRANCESCHI, E | |
dc.contributor.author | GALEOTTA, S | |
dc.contributor.author | GARILLI, B | |
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 | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | HUDELOT, P | |
dc.contributor.author | JAHNKE, K | |
dc.contributor.author | JHABVALA, M | |
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 | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | KILBINGER, M | |
dc.contributor.author | KITCHING, T | |
hal.structure.identifier | Institut de Physique des 2 Infinis de Lyon [IP2I Lyon] | |
dc.contributor.author | KUBIK, B | |
dc.contributor.author | KUIJKEN, K | |
dc.contributor.author | KÜMMEL, M | |
dc.contributor.author | KUNZ, M | |
dc.contributor.author | KURKI-SUONIO, H | |
dc.contributor.author | LAHAV, O | |
dc.contributor.author | LIGORI, S | |
dc.contributor.author | LILJE, P.B | |
dc.contributor.author | LINDHOLM, V | |
dc.contributor.author | LLORO, I | |
dc.contributor.author | MAINO, D | |
dc.contributor.author | MAIORANO, E | |
dc.contributor.author | MANSUTTI, O | |
dc.contributor.author | MARGGRAF, O | |
dc.contributor.author | MARKOVIC, K | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | MARTINET, N | |
dc.contributor.author | MARULLI, F | |
dc.contributor.author | MASSEY, R | |
hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
dc.contributor.author | MAUROGORDATO, S | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | MCCRACKEN, H.J | |
dc.contributor.author | MEDINACELI, E | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | MELLIER, Y | |
dc.contributor.author | MEYLAN, G | |
dc.contributor.author | MOHR, J.J | |
dc.contributor.author | MORESCO, M | |
dc.contributor.author | MOSCARDINI, L | |
dc.contributor.author | MUNARI, E | |
dc.contributor.author | NAKAJIMA, R | |
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 | PADILLA, C | |
dc.contributor.author | PALTANI, S | |
dc.contributor.author | PASIAN, F | |
dc.contributor.author | PEACOCK, J.A | |
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 | REFREGIER, A | |
dc.contributor.author | RENZI, A | |
dc.contributor.author | RICCIO, G | |
dc.contributor.author | RIX, Hans-Walter | |
dc.contributor.author | ROMELLI, E | |
dc.contributor.author | RONCARELLI, M | |
dc.contributor.author | ROSSETTI, E | |
dc.contributor.author | SAGLIA, R | |
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 | TALLADA-CRESPÍ, P | |
dc.contributor.author | TAYLOR, A.N | |
dc.contributor.author | TEPLITZ, H.I | |
dc.contributor.author | TOLEDO-MOREO, R | |
dc.contributor.author | TSYGANOV, A | |
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 | KLEIJN, G. Verdoes | |
dc.contributor.author | WANG, Y | |
dc.contributor.author | WELLER, J | |
dc.contributor.author | WILLIAMS, O.R | |
dc.contributor.author | ZAMORANI, G | |
dc.contributor.author | ZUCCA, E | |
dc.contributor.author | BACCIGALUPI, C | |
dc.contributor.author | BURIGANA, C | |
hal.structure.identifier | Centre National d'Études Spatiales [Toulouse] [CNES] | |
dc.contributor.author | CASENOVE, P | |
dc.contributor.author | LIEBING, P | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
hal.structure.identifier | JUNIA [JUNIA] | |
dc.contributor.author | SCOTTEZ, V | |
dc.contributor.author | SIMON, P | |
dc.contributor.author | SCOTT, D | |
dc.description.abstractEn | The Euclid ERO showcase Euclid's capabilities in advance of its main mission, targeting 17 astronomical objects, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions. A total of 24 hours observing time was allocated in the early months of operation, engaging the scientific community through an early public data release. We describe the development of the ERO pipeline to create visually compelling images while simultaneously meeting the scientific demands within months of launch, leveraging a pragmatic, data-driven development strategy. The pipeline's key requirements are to preserve the image quality and to provide flux calibration and photometry for compact and extended sources. The pipeline's five pillars are: removal of instrumental signatures; astrometric calibration; photometric calibration; image stacking; and the production of science-ready catalogues for both the VIS and NISP instruments. We report a PSF with a full width at half maximum of 0.16" in the optical and 0.49" in the three NIR bands. Our VIS mean absolute flux calibration is accurate to about 1%, and 10% for NISP due to a limited calibration set; both instruments have considerable colour terms. The median depth is 25.3 and 23.2 AB mag with a SNR of 10 for galaxies, and 27.1 and 24.5 AB mag at an SNR of 5 for point sources for VIS and NISP, respectively. Euclid's ability to observe diffuse emission is exceptional due to its extended PSF nearly matching a pure diffraction halo, the best ever achieved by a wide-field, high-resolution imaging telescope. Euclid offers unparalleled capabilities for exploring the LSB Universe across all scales, also opening a new observational window in the NIR. Median surface-brightness levels of 29.9 and 28.3 AB mag per square arcsec are achieved for VIS and NISP, respectively, for detecting a 10 arcsec x 10 arcsec extended feature at the 1 sigma level. | |
dc.language.iso | en | |
dc.rights.uri | http://creativecommons.org/licenses/by-sa/ | |
dc.title.en | Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometry | |
dc.type | Document de travail - Pré-publication | |
dc.subject.hal | Physique [physics]/Physique [physics]/Instrumentations et Détecteurs [physics.ins-det] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph] | |
dc.identifier.arxiv | 2405.13496 | |
hal.identifier | hal-04592901 | |
hal.version | 1 | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-04592901v1 | |
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