Euclid: Photometric redshift calibration with the clustering redshifts technique
本文证明,利用来自 BOSS、DESI 和 Euclid NISP 的小尺度角聚类及光谱参考样本的聚类红移技术,通过优化流程并解决如单晕星系分布等偏差,能够成功约束 Euclid 成相分组的平均红移,以满足任务对σ(⟨z⟩)<0.002(1+z)的严格精度要求。
原作者: W. d'Assignies (Institut de Física d'Altes Energies), M. Manera (Serra Húnter Fellow, Departament de Física, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, Institut de Física d'Altes Energies), C. Padilla (Institut de Física d'Altes Energies), O. Ilbert (Aix-Marseille Université, CNRS, CNES, LAM, Marseille, France), H. Hildebrandt (Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute), L. Reynolds (Institut de Física d'Altes Energies, Departament de Física, Universitat Autònoma de Barcelona, 08193 Bellaterra), J. Chaves-Montero (Institut de Física d'Altes Energies), A. H. Wright (Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute), P. Tallada-Crespí (Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Port d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra), M. Eriksen (Institut de Física d'Altes Energies, Port d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra), J. Carretero (Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Port d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra), W. Roster (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), Y. Kang (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), K. Naidoo (Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK), R. Miquel (Institut de Física d'Altes Energies, Institució Catalana de Recerca i Estudis Avançats), B. Altieri (ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain), A. Amara (School of Mathematics and Physics, University of Surrey, Guildford, Surrey, GU2 7XH, UK), S. Andreon (INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy), N. Auricchio (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), C. Baccigalupi (IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, INFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, SISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy), D. Bagot (Centre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France), M. Baldi (Dipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), A. Balestra (INAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy), S. Bardelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), P. Battaglia (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), A. Biviano (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy), E. Branchini (Dipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, Italy, INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy), M. Brescia (Department of Physics "E. Pancini", University Federico II, Via Cinthia 6, 80126, Napoli, Italy, INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy), S. Camera (Dipartimento di Fisica, Università degli Studi di Torino, Via P. Giuria 1, 10125 Torino, Italy, INFN-Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy, INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), V. Capobianco (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), C. Carbone (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), V. F. Cardone (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, INFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy), S. Casas (Institute for Theoretical Particle Physics and Cosmology), F. J. Castander (Institute of Space Sciences, Institut d'Estudis Espacials de Catalunya), M. Castellano (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), G. Castignani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), S. Cavuoti (INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, INFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy), K. C. Chambers (Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA), A. Cimatti (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), C. Colodro-Conde (Instituto de Astrofísica de Canarias, Vía Láctea, 38205 La Laguna, Tenerife, Spain), G. Congedo (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), C. J. Conselice (Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK), L. Conversi (European Space Agency/ESRIN, Largo Galileo Galilei 1, 00044 Frascati, Roma, Italy, ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain), Y. Copin (Université Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), F. Courbin (Institut de Ciències del Cosmos, Institució Catalana de Recerca i Estudis Avançats), H. M. Courtois (UCB Lyon 1, CNRS/IN2P3, IUF, IP2I Lyon, 4 rue Enrico Fermi, 69622 Villeurbanne, France), M. Crocce (Institute of Space Sciences, Institut d'Estudis Espacials de Catalunya), A. Da Silva (Departamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, Portugal, Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal), H. Degaudenzi (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), S. de la Torre (Aix-Marseille Université, CNRS, CNES, LAM, Marseille, France), G. De Lucia (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), M. Douspis (Université Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France), X. Dupac (ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain), A. Ealet (Université Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), S. Escoffier (Aix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France), M. Farina (INAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy), F. Faustini (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, Space Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy), S. Ferriol (Université Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), F. Finelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy), P. Fosalba (Institut d'Estudis Espacials de Catalunya, Institute of Space Sciences), S. Fotopoulou (School of Physics, HH Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol, BS8 1TL, UK), M. Frailis (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), E. Franceschi (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. Fumana (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), S. Galeotta (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), K. George (Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany), B. Gillis (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), C. Giocoli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), P. Gómez-Alvarez (FRACTAL S.L.N.E., calle Tulipán 2, Portal 13 1A, 28231, Las Rozas de Madrid, Spain, ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain), J. Gracia-Carpio (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), A. Grazian (INAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy), F. Grupp (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany), W. Holmes (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), I. M. Hook (Department of Physics, Lancaster University, Lancaster, LA1 4YB, UK), A. Hornstrup (Technical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark, Cosmic Dawn Center), K. Jahnke (Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany), M. Jhabvala (NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA), B. Joachimi (Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK), E. Keihänen (Department of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland), S. Kermiche (Aix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France), A. Kiessling (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), B. Kubik (Université Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), M. Kümmel (Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany), M. Kunz (Université de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, CH-1211 Genève 4, Switzerland), H. Kurki-Suonio (Department of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland), O. Lahav (Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK), A. M. C. Le Brun (Laboratoire d'etude de l'Univers et des phenomenes eXtremes, Observatoire de Paris, Université PSL, Sorbonne Université, CNRS, 92190 Meudon, France), S. Ligori (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), P. B. Lilje (Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway), V. Lindholm (Department of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland), I. Lloro (SKA Observatory, Jodrell Bank, Lower Withington, Macclesfield, Cheshire SK11 9FT, UK), G. Mainetti (Centre de Calcul de l'IN2P3/CNRS, 21 avenue Pierre de Coubertin 69627 Villeurbanne Cedex, France), D. Maino (Dipartimento di Fisica "Aldo Pontremoli", Università degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy, INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, INFN-Sezione di Milano, Via Celoria 16, 20133 Milano, Italy), E. Maiorano (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), O. Mansutti (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), S. Marcin (University of Applied Sciences and Arts of Northwestern Switzerland, School of Computer Science, 5210 Windisch, Switzerland), O. Marggraf (Universität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany), K. Markovic (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), M. Martinelli (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, INFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy), N. Martinet (Aix-Marseille Université, CNRS, CNES, LAM, Marseille, France), F. Marulli (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), R. Massey (Department of Physics, Institute for Computational Cosmology, Durham University, South Road, Durham, DH1 3LE, UK), D. C. Masters (Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA), E. Medinaceli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), S. Mei (Université Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, CNRS-UCB International Research Laboratory, Centre Pierre Binétruy, IRL2007, CPB-IN2P3, Berkeley, USA), M. Melchior (University of Applied Sciences and Arts of Northwestern Switzerland, School of Engineering, 5210 Windisch, Switzerland), Y. Mellier (Institut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, France, Institut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France), M. Meneghetti (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), E. Merlin (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), G. Meylan (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne), A. Mora (Telespazio UK S.L. for European Space Agency), M. Moresco (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), L. Moscardini (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), C. Neissner (Institut de Física d'Altes Energies, Port d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra), S. -M. Niemi (European Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands), S. Paltani (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), F. Pasian (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), K. Pedersen (DARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark), V. Pettorino (European Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands), S. Pires (Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France), G. Polenta (Space Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy), M. Poncet (Centre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France), L. A. Popa (Institute of Space Science, Str. Atomistilor, nr. 409 Măgurele, Ilfov, 077125, Romania), L. Pozzetti (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), F. Raison (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), R. Rebolo (Instituto de Astrofísica de Canarias, Vía Láctea, 38205 La Laguna, Tenerife, Spain, Consejo Superior de Investigaciones Cientificas, Calle Serrano 117, 28006 Madrid, Spain, Universidad de La Laguna, Departamento de Astrofísica, 38206 La Laguna, Tenerife, Spain), A. Renzi (Dipartimento di Fisica e Astronomia "G. Galilei", Università di Padova, Via Marzolo 8, 35131 Padova, Italy, INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), J. Rhodes (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), G. Riccio (INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy), E. Romelli (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), M. Roncarelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), E. Rossetti (Dipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy), R. Saglia (Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), Z. Sakr (Institut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany, Institut de Recherche en Astrophysique et Planétologie, Université St Joseph, Faculty of Sciences, Beirut, Lebanon), D. Sapone (Departamento de Física, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile), B. Sartoris (Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), J. A. Schewtschenko (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), P. Schneider (Universität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany), T. Schrabback (Universität Innsbruck, Institut für Astro- und Teilchenphysik, Technikerstr. 25/8, 6020 Innsbruck, Austria), A. Secroun (Aix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France), E. Sefusatti (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, INFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy), G. Seidel (Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany), M. Seiffert (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), S. Serrano (Institut d'Estudis Espacials de Catalunya, Satlantis, University Science Park, Sede Bld 48940, Leioa-Bilbao, Spain, Institute of Space Sciences), P. Simon (Universität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany), C. Sirignano (Dipartimento di Fisica e Astronomia "G. Galilei", Università di Padova, Via Marzolo 8, 35131 Padova, Italy, INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), G. Sirri (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), A. Spurio Mancini (Department of Physics, Royal Holloway, University of London, TW20 0EX, UK), L. Stanco (INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), J. Steinwagner (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), D. Tavagnacco (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), A. N. Taylor (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), H. I. Teplitz (Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA), I. Tereno (Departamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, Portugal, Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal), N. Tessore (Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK), S. Toft (Cosmic Dawn Center, Niels Bohr Institute, University of Copenhagen, Jagtvej 128, 2200 Copenhagen, Denmark), R. Toledo-Moreo (Universidad Politécnica de Cartagena, Departamento de Electrónica y Tecnología de Computadoras, Plaza del Hospital 1, 30202 Cartagena, Spain), F. Torradeflot (Port d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas), A. Tsyganov (Centre for Information Technology, University of Groningen, P.O. Box 11044, 9700 CA Groningen, The Netherlands), I. Tutusaus (Institut de Recherche en Astrophysique et Planétologie), L. Valenziano (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy), J. Valiviita (Department of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland), T. Vassallo (Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), G. Verdoes Kleijn (Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands), Y. Wang (Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA), J. Weller (Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), G. Zamorani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), E. Zucca (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. Bolzonella (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), C. Burigana (INAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, Italy, INFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy), L. Gabarra (Department of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK), J. Martín-Fleitas (Aurora Technology for European Space Agency), I. Risso (INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, and INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy), V. Scottez (Institut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, France, ICL, Junia, Université Catholique de Lille, LITL, 59000 Lille, France), M. Viel (IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, SISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy, INFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, ICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy)
原始论文采用 CC BY 4.0 许可(http://creativecommons.org/licenses/by/4.0/)。 ✨ 这是对下方论文的AI生成解释。它不是由作者撰写或认可的。如需技术准确性,请参阅原始论文。 阅读完整免责声明
想象一下,欧几里得空间望远镜就像一台巨大的高速相机,正在拍摄宇宙中数十亿个星系的全景照片。为了理解宇宙的故事——它如何膨胀、暗能量如何运作、以及暗物质如何将其维系在一起——科学家们不仅需要知道这些星系“在哪里”,还需要知道它们“有多远”。
在天文学中,距离是通过“红移”来测量的(即随着宇宙膨胀,来自星系的光被拉伸的程度)。然而,要获得每一个单独星系的精确距离,就像试图在拥挤的体育场里采访每一个人一样:既太慢又太昂贵。因此,天文学家使用一种基于星系颜色的“最佳猜测”方法(测光红移)。但这些猜测可能模糊不清,就像在雾中拍摄的照片。
本文介绍了一种利用成团红移(clustering-redshifts)技术来驱散这种迷雾的新锐方法。
核心思想:“派对客人”类比
把宇宙想象成一个巨大的派对。
- 测光星系是我们从远处能看到的客人,但我们不知道他们确切是谁或来自哪里。我们只知道他们在房间里。
- 光谱星系是一小群经过彻底采访的贵宾。我们知道他们确切的姓名、年龄和家乡(即他们的精确距离)。
问题在于:我们有一大群“神秘客人”(测光星系),需要弄清楚他们的平均年龄和距离。我们无法采访他们所有人。
成团红移的解决方案:
我们不采访神秘客人,而是观察他们如何站在贵宾旁边。
- 如果一个神秘客人正站在一位来自“红移镇 1"的贵宾旁边,那么该神秘客人很可能也来自“红移镇 1"。
- 如果他们站在一位来自“红移镇 2"的贵宾附近,那么他们很可能也来自那里。
通过测量神秘客人在不同距离处围绕已知贵宾聚集的紧密程度,我们可以统计性地重建整个群体的真实距离分布。
本文做了什么
作者们不仅仅是理论推演;他们构建了一个巨大的虚拟宇宙(称为"Flagship 2 模拟”),以测试该方法是否足以满足欧几里得任务的需求。他们创造了一个包含 4 万亿粒子和数十亿个星系的假想宇宙,然后在其上运行“成团”测试,看是否能恢复出真实的距离。
以下是主要发现,以简单的方式解释:
1. “单晕”问题(“家庭单元”问题)
在非常小的尺度上,星系通常生活在群体或“晕”中(就像住在同一所房子里的家庭)。有时,不同类型的星系(如红色和蓝色星系)在这些微小的家庭单元内并不很好地混合。
- 解决方法:团队发现,如果观察靠得太近的星系(小于 150 万光年),由于这些家庭动态的影响,数学计算会变得混乱且不准确。他们决定忽略“近距离邻居”,只观察距离稍远的星系。这使得结果更加清晰。
2. 找到正确的“变焦”级别
就像拍照一样,你需要合适的变焦级别。
- 变焦过大:你会看到太多的噪音和家庭怪癖(单晕问题)。
- 变焦过小:你会失去区分贵宾与人群所需的细节。
- 最佳点:他们发现,观察150 万到 500 万光年之间的尺度是完美的平衡点。这为他们提供了最清晰的信号,同时没有噪音。
3. 修正“偏差”(权重问题)
在这个类比中,某些类型的星系比其他星系更“重”(聚集性更强)。如果不考虑这种权重,你的距离计算就会出错。
- 创新点:本文介绍了一种新的、更好的方法来测量这些“神秘客人”的这种“权重”(星系偏差)。他们测试了几种方法,发现其中一种(称为M3)的效果几乎与完全知晓真实距离一样好。这就像拥有一台非常精准的秤,可以在不单独称重的情况下称量神秘客人的重量。
4. 结果:达成目标
欧几里得任务有一条严格的规定:任何星系组的平均距离猜测必须准确到极小的误差范围内(小于距离的 0.2%)。
- 裁决:使用他们优化的方法,团队成功达到了这一目标。他们能够以高精度重建星系的真实距离分布。事实上,他们的结果优于先前的尝试,证明了这种“派对客人”方法是稳健的,并且已准备好处理真实的欧几里得数据。
为什么这很重要
这篇论文本质上是对一种关键工具的“压力测试”。在真实的欧几里得望远镜数据到来之前,科学家们需要知道:我们能否信任这种成团方法给出正确的答案?
答案是肯定的。他们表明,通过仔细选择要比较的星系,忽略“太近”的星系,并使用一种新的数据加权方法,他们可以以解决暗能量和暗物质之谜所需的精度来绘制宇宙结构图。
简而言之:他们构建了一个虚拟宇宙,测试了一种通过观察星系如何聚集来测量宇宙距离的新方法,修正了发现的错误,并证明了该方法的精度足以帮助我们理解宇宙的命运。
技术摘要:Euclid 任务:基于 Flagship 2 模拟的成团红移技术的光度红移校准性能
问题陈述
成像巡天(如 Euclid)所推导的宇宙学约束的精度,关键依赖于对星系分层样本红移分布 n(z) 的准确估计。具体而言,平均红移的不确定度 σ(⟨z⟩) 必须在 68% 置信度下低于 0.002(1+z),以满足 Euclid 的科学要求。虽然光谱红移非常精确,但对于成像巡天中数十亿个星系而言,获取其光谱红移的成本过高。光度红移(photo-z)提供了一种解决方案,但存在颜色与红移之间的简并性以及代表性训练样本的局限性。成团红移(clustering-z)技术提供了一种替代方案,它通过光度样本与具有可靠红移的光谱样本之间的角互相关,统计推断红移分布。然而,先前的研究(例如 Naidoo 等人 2023)指出了残留的系统偏差,特别是在高红移处,并强调了测量光度星系偏倚和建模小尺度成团效应方面的挑战。
方法论
本研究利用 Euclid Flagship 2 模拟(Castander 等人 2025)中的 5000 平方度模拟数据,评估了成团红移技术的有效性。作者生成了 Euclid 光度星系、Euclid NISP 光谱星系以及外部光谱示踪体(BOSS、DESI 和 4MOST)的逼真模拟样本。
方法论包括:
- 流程优化:作者测试了成团红移流程的各个组件,包括不同的角关联估计量、尺度范围和加权方案。
- 偏倚校正:主要重点是开发和测试测量光度星系偏倚(bp)的新方法,这是该技术的主要限制。他们引入了方法 M3 和 M4,在更小的光度红移区间内测量偏倚并插值其演化,将这些方法与现有方法(M0–M2)以及使用真实红移的理想化“完全校正”(M5)进行了比较。
- 系统误差分析:本研究调查了多种系统偏差来源:
- 小尺度效应:单晕机制(one-halo regime)和非线性星系 - 晕连接对互相关的影响。
- 建模近似:比较了光谱红移分布的狄拉克(Dirac)、Limber 单区间和“三区间”近似。
- 物理效应:引力透镜放大效应和红移空间畸变(RSD)的影响。
- 红移重构:采用两种不同的方法从离散测量中提取矩(⟨z⟩ 和 σz):参数化的“移位 - 拉伸”模型(SSM)和非参数化的抑制高斯过程(SGP)方法。
主要贡献
- 最佳尺度范围:作者确定投影尺度范围 1.5<rp<5 Mpc 为最佳。该范围避免了单晕机制(rp<1.5 Mpc 会因星系 - 晕物理引入偏差),同时保持足够的信噪比(SNR),并且与主要宇宙学分析所使用的尺度保持区分。
- 光度偏倚测量:本文引入并验证了方法 M3,该方法在较大的光度红移区间(Δzphoto=0.1)内测量光度偏倚并拟合红移演化。该方法的性能与理想化的 M5(使用真实红移)相当,并显著优于之前的部分校正方法。
- 光谱切片:研究确定了最佳的光谱红移切片为 Δz≈0.05,在需要足够的数据点与由区间建模及放大等物理效应引入的系统误差之间取得了平衡。
- 估计量选择:作者主张使用积分对计数估计量(公式 57),即积分数据 - 随机对计数之比,而非积分计数之比,发现其具有更好的掩模校正效果和更直接的加权解释。
- 示踪体分离:本文建议在特定红移处的互相关中使用单一类型的光谱示踪体(例如发射线星系 ELGs 或亮红星系 LRGs),以避免因不同的星系 - 晕连接属性(例如红蓝星系之间的“一致性”效应)而产生的偏差。
结果
- 精度:优化后的流程成功约束了所有十个分层样本(最高至 zphoto=1.6)的平均红移和标准差。
- 要求满足情况:使用 SSM 方法,该方法在所有区间和天区均达到或超过了 Euclid 对 σ(⟨z⟩)<0.002(1+z) 的要求。保守的 SGP 方法产生了可比的结果,但在特定区间(1、3 和 7)显示出略大的偏差,不过考虑到模拟约束,这些偏差仍在可接受范围内。
- 偏差抑制:研究确定了“单区间近似”(忽略与相邻光谱切片的关联)和单晕机制是偏差的主要来源。通过将尺度限制在 >1.5 Mpc 并使用 M3 偏倚校正,这些偏差被降低至符合要求水平。
- 与先前工作的比较:结果表明,相较于先前的 Flagship 1 研究(Naidoo 等人 2023),本研究取得了显著改进,实现了更低的平均红移偏差和更严格的约束。这一改进归因于更大的模拟体积、优化的尺度范围、新的偏倚校正方法以及光谱示踪体的分离。
意义
本文声称,成团红移技术是 Euclid 任务红移校准的一个稳健且可行的核心组成部分。研究表明,利用优化的流程和逼真的模拟数据,该技术能够满足 Euclid 弱引力透镜和星系成团分析所需的严格精度要求。作者强调,虽然当前结果较为乐观(依赖于模拟和特定的偏倚校正),但对系统源(如单晕效应和闯入者)的识别以及缓解策略的开发,为实际数据分析提供了清晰的前进路径。这项工作建立了一个基准框架(尺度范围、偏倚校正、示踪体选择),可应用于真实的 Euclid 数据,以确保宇宙学约束的准确性。
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