<i>Euclid</i>preparation
L. GabarraDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyC. ManciniINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, ItalyL. Rodriguez MuñozDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyL. BisigelloDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyC. SirignanoDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyM. ScodeggioINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, ItalyM. TaliaDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyS DusiniINFN-Padova, Via Marzolo 8, 35131 Padova, ItalyW. GillardAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, FranceB. R. GranettINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, ItalyE. MaioranoINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyM. MorescoDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyL. PaganinDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146 Genova, ItalyE. PalazziINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyL. PozzettiINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyA. RenziDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyE. RossettiDipartimento di Fisica e Astronomia, Universita di Bologna, Via Gobetti 93/2, 40129 Bologna, ItalyD. VerganiINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyV. AllevatoINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyG. CastignaniDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyB. DeDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyM. FumanaINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, ItalyK. GangaUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, FranceB. GarilliINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, ItalyM. HirschmannINAF - Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyF. La FrancaDepartment of Mathematics and Physics, Roma Tre University, Via della Vasca Navale 84, 00146 Rome, ItalyC. LaigleInstitut d’Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, FranceF PassalacquaDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyM. SchirmerMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, GermanyL. StancoINFN-Padova, Via Marzolo 8, 35131 Padova, ItalyA. TrojaDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyL. Y. Aaron YungNASA Goddard Space Flight Center, Greenbelt, MD 20771, USAG. ZamoraniINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyJ. ZoubianAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, FranceS AnselmiDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyF OppizziDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyG VerzaDipartimento di Fisica e Astronomia “G. Galilei”, Universitá di Padova, Via Marzolo 8, 35131 Padova, ItalyN. AghanimUniversité Paris-Saclay, CNRS, Institut d’astrophysique spatiale, 91405 Orsay, FranceA. AmaraInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UKN. AuricchioINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyMarco BaldiDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyR. BenderMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyC BodendorfMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyD. BoninoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), ItalyE. BranchiniDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146 Genova, ItalyM. BresciaJ. BrinchmannInstituto de Astrofisica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, PortugalS. CameraDipartimento di Fisica, Universitâ degli Studi di Torino, Via P. Giuria 1, 10125 Torino, ItalyV. CapobiancoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), ItalyC. CarboneINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, ItalyJ. CarreteroInstitut de Fisica d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), SpainF. J. CastanderInstitut d’Estudis Espacials de Catalunya (IEEC), Carrer Gran Capitá 2-4, 08034 Barcelona, SpainM. CastellanoINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, ItalyS. CavuotiINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyR. CledassouCentre National d’Etudes Spatiales - Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, FranceG. CongedoInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UKChristopher J. ConseliceJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UKL ConversiESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Canada, Madrid, SpainY. CopinCentre National de la Recherche ScientifiqueL. CorcioneINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), ItalyA. CostilleAix-Marseille Université, CNRS, CNES, LAM, Marseille, FranceF. CourbinInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, SwitzerlandA. Da SilvaDepartamento de Fisica, Faculdade de Ciências, Universidade de Lisboa, Edificio C8, Campo Grande, 1749-016 Lisboa, PortugalH. DegaudenziDepartment of Astronomy, University of Geneva, ch. d’Ecogia 16, 1290 Versoix, SwitzerlandJ. DinisDepartamento de Fisica, Faculdade de Ciências, Universidade de Lisboa, Edificio C8, Campo Grande, 1749-016 Lisboa, PortugalF. DubathDepartment of Astronomy, University of Geneva, ch. d’Ecogia 16, 1290 Versoix, SwitzerlandX. DupacESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Canada, Madrid, SpainA. EaletUniversity of Lyon, Univ. Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, 69622 Villeurbanne, FranceS. FarrensUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, Astrophysique, Instrumentation et Modélisation Paris-Saclay, 91191 Gif-sur-Yvette, FranceS. FerriolUniversity of Lyon, Univ. Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, 69622 Villeurbanne, FranceM. FrailisINAF - Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyE. FranceschiINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyP. FranzettiINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, ItalyS. GaleottaINAF - Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyB. GillisInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UKC. GiocoliINAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyA. GrazianINAF-Osservatorio Astronomico di Padova, Via dell’Osservatorio 5, 35122 Padova, ItalyF. GruppMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyL. GuzzoDipartimento di Fisica “Aldo Pontremoli”, Universitâ degli Studi di Milano, Via Celoria 16, 20133 Milano, ItalyW HolmesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USAA. HornstrupCosmic Dawn Center (DAWN), DenmarkP. HudelotInstitut d’Astrophysique de Paris, 98bis Boulevard Arago, 75014 Paris, FranceK. JahnkęMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, GermanyM. KümmelUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyS. KermicheAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, FranceA. KiesslingJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USAM. KilbingerUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, Astrophysique, Instrumentation et Modélisation Paris-Saclay, 91191 Gif-sur-Yvette, FranceT. KitchingMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UKR. KohleyESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Canada, Madrid, SpainB. KubikUniversity of Lyon, Univ. Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, 69622 Villeurbanne, FranceM. KunzUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 1211 Genève 4, SwitzerlandH. Kurki‐SuonioDepartment of Physics, PO Box 64, 00014 University of Helsinki, FinlandS. LigoriINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), ItalyP. B. LiljeInstitute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, NorwayI. LloroNOVA optical infrared instrumentation group at ASTRON, Oude Hoogeveensedijk 4, 7991PD, Dwingeloo, The NetherlandsO. MansuttiINAF - Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyO. MarggrafArgelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, GermanyK. MarkovičJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USAF. MarulliDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy
2023en
ABI
Аннотация
This work focusses on the pilot run of a simulation campaign aimed at investigating the spectroscopic capabilities of the Euclid Near-Infrared Spectrometer and Photometer (NISP), in terms of continuum and emission line detection in the context of galaxy evolutionary studies. To this purpose, we constructed, emulated, and analysed the spectra of 4992 star-forming galaxies at 0.3 ≤ z ≤ 2.5 using the NISP pixel-level simulator. We built the spectral library starting from public multi-wavelength galaxy catalogues, with value-added information on spectral energy distribution (SED) fitting results, and stellar population templates from Bruzual & Charlot (2003, MNRAS, 344, 1000). Rest-frame optical and near-IR nebular emission lines were included using empirical and theoretical relations. Dust attenuation was treated using the Calzetti extinction law accounting for the differential attenuation in line-emitting regions with respect to the stellar continuum. The NISP simulator was configured including instrumental and astrophysical sources of noise such as the dark current, read-out noise, zodiacal background, and out-of-field stray light. In this preliminary study, we avoided contamination due to the overlap of the slitless spectra. For this purpose, we located the galaxies on a grid and simulated only the first order spectra. We inferred the 3.5 σ NISP red grism spectroscopic detection limit of the continuum measured in the H band for star-forming galaxies with a median disk half-light radius of 0.″4 at magnitude H = 19.5 ± 0.2 AB mag for the Euclid Wide Survey and at H = 20.8 ± 0.6 AB mag for the Euclid Deep Survey. We found a very good agreement with the red grism emission line detection limit requirement for the Wide and Deep surveys. We characterised the effect of the galaxy shape on the detection capability of the red grism and highlighted the degradation of the quality of the extracted spectra as the disk size increased. In particular, we found that the extracted emission line signal-to-noise ratio (S/N) drops by ~45% when the disk size ranges from 0.″25 to 1″. These trends lead to a correlation between the emission line S/N and the stellar mass of the galaxy and we demonstrate the effect in a stacking analysis unveiling emission lines otherwise too faint to detect.
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