First results from the IllustrisTNG simulations: the galaxy colour bimodality
Dylan Nelson,Annalisa Pillepich,Volker Springel,Volker Springel,Rainer Weinberger,Lars Hernquist,Ruediger Pakmor,Shy Genel,Paul Torrey,Mark Vogelsberger,Guinevere Kauffmann,Federico Marinacci,Jill Naiman +12 more
TLDR
The first two simulations of the IllustrisTNG project were presented in this article, focusing on the optical colors of galaxies at low redshift, and the results showed that the simulated (g-r) colors of 10^9 10^11 Msun which redden at z < 1 accumulate on average ~25% of their final z=0 mass post-reddening; at the same time, ~18% of such massive galaxies acquire half or more of their last stellar mass while on the red sequence.Abstract:
We introduce the first two simulations of the IllustrisTNG project, a next generation of cosmological magnetohydrodynamical simulations, focusing on the optical colors of galaxies. We explore TNG100, a rerun of the original Illustris box, and TNG300, which includes 2x2500^3 resolution elements in a volume twenty times larger. Here we present first results on the galaxy color bimodality at low redshift. Accounting for the attenuation of stellar light by dust, we compare the simulated (g-r) colors of 10^9 10^11 Msun which redden at z<1 accumulate on average ~25% of their final z=0 mass post-reddening; at the same time, ~18% of such massive galaxies acquire half or more of their final stellar mass while on the red sequence.read more
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First results from the IllustrisTNG simulations: matter and galaxy clustering
Volker Springel,Volker Springel,Rüdiger Pakmor,Annalisa Pillepich,Rainer Weinberger,Dylan Nelson,Lars Hernquist,Mark Vogelsberger,Shy Genel,Shy Genel,Paul Torrey,Federico Marinacci,Jill Naiman +12 more
TL;DR: In this article, the authors used the IllustrisTNG simulations to study the non-linear correlation functions and power spectra of baryons, dark matter, galaxies and haloes over an exceptionally large range of scales.
Journal ArticleDOI
First results from the IllustrisTNG simulations: radio haloes and magnetic fields
Federico Marinacci,Mark Vogelsberger,Rüdiger Pakmor,Paul Torrey,Volker Springel,Volker Springel,Lars Hernquist,Dylan Nelson,Rainer Weinberger,Annalisa Pillepich,Jill Naiman,Shy Genel,Shy Genel +12 more
TL;DR: The IllustrisTNG project as mentioned in this paper is a suite of cosmological magnetohydrodynamical simulations performed with the moving-mesh code AREPO employing an updated Illustris galaxy formation model.
Journal ArticleDOI
The IllustrisTNG simulations: public data release
Dylan Nelson,Volker Springel,Volker Springel,Volker Springel,Annalisa Pillepich,Vicente Rodriguez-Gomez,Paul Torrey,Paul Torrey,Shy Genel,Mark Vogelsberger,Ruediger Pakmor,Ruediger Pakmor,Federico Marinacci,Federico Marinacci,Rainer Weinberger,Luke Zoltan Kelley,Mark R. Lovell,Mark R. Lovell,Benedikt Diemer,Lars Hernquist +19 more
TL;DR: The full public release of all data from the TNG100 and TNG300 simulations of the IllustrisTNG project is presented in this article, which includes a comprehensive model for galaxy formation physics, and each TNG simulation selfconsistently solves for the coupled evolution of dark matter, cosmic gas, luminous stars, and supermassive black holes from early time to the present day.
Journal ArticleDOI
First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback
Dylan Nelson,Annalisa Pillepich,Volker Springel,Volker Springel,Volker Springel,Rüdiger Pakmor,Rüdiger Pakmor,Rainer Weinberger,Shy Genel,Paul Torrey,Mark Vogelsberger,Federico Marinacci,Lars Hernquist +12 more
TL;DR: The TNG50 volume as mentioned in this paper is the third and final volume of the IllustrisTNG project, which includes a large-scale magnetohydrodynamical simulation of galaxy outflows driven by supernovae.
Journal ArticleDOI
First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time
Annalisa Pillepich,Dylan Nelson,Volker Springel,Rüdiger Pakmor,Paul Torrey,Rainer Weinberger,Mark Vogelsberger,Federico Marinacci,Federico Marinacci,Shy Genel,Arjen van der Wel,Arjen van der Wel,Lars Hernquist +12 more
TL;DR: In this paper, the authors present a new cosmological, magnetohydrodynamical simulation for galaxy formation, TNG50, which reaches a numerical resolution typical of zoom-in simulations, with a baryonic element mass of 8.5 x 10(4) M-circle dot and an average cell size of 70-140pc in the star-forming regions of galaxies.
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Planck 2015 results - XIII. Cosmological parameters
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TL;DR: In this article, the authors present a cosmological analysis based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation.
Journal ArticleDOI
Planck 2015 results. XIII. Cosmological parameters
Peter A. R. Ade,Nabila Aghanim,Monique Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,James G. Bartlett,N. Bartolo,E. Battaner,Richard A. Battye,K. Benabed,Alain Benoit,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,J. J. Bock,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,François R. Bouchet,F. Boulanger,M. Bucher,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,A. Catalano,Anthony Challinor,A. Chamballu,Ranga-Ram Chary,H. C. Chiang,Jens Chluba,P. R. Christensen,Sarah E. Church,David L. Clements,S. Colombi,L. P. L. Colombo,C. Combet,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,Jacques Delabrouille,F.-X. Désert,E. Di Valentino,Clive Dickinson,Jose M. Diego,Klaus Dolag,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,A. Ducout,Jo Dunkley,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Ensslin,H. K. Eriksen,Marzieh Farhang,James R. Fergusson,Fabio Finelli,Olivier Forni,M. Frailis,A. A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,S. Galli,K. Ganga,C. Gauthier,Martina Gerbino,Tuhin Ghosh,M. Giard,Y. Giraud-Héraud,Elena Giusarma,E. Gjerløw,J. González-Nuevo,Krzysztof M. Gorski,Serge Gratton,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,Jan Hamann,F. K. Hansen,Duncan Hanson,D. L. Harrison,George Helou,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Zhiqi Huang,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,Lloyd Knox,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,J. P. Leahy,R. Leonardi,Julien Lesgourgues,François Levrier,Antony Lewis,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,G. Maggio,Davide Maino,N. Mandolesi,A. Mangilli,A. Marchini,Peter G. Martin,M. Martinelli,E. Martínez-González,Silvia Masi,Sabino Matarrese,Pasquale Mazzotta,P. McGehee,Peter Meinhold,Alessandro Melchiorri,J.-B. Melin,L. Mendes,A. Mennella,M. Migliaccio,M. Millea,S. Mitra,M.-A. Miville-Deschênes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Adam Moss,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,C. A. Oxborrow,F. Paci,L. Pagano,F. Pajot,R. Paladini,Daniela Paoletti,Bruce Partridge,F. Pasian,G. Patanchon,T. J. Pearson,O. Perdereau,L. Perotto,Francesca Perrotta,Valeria Pettorino,F. Piacentini,M. Piat,E. Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,G. Polenta,L. Popa,G. W. Pratt,G. Prézeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,William T. Reach,Rafael Rebolo,M. Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,Graca Rocha,C. Rosset,M. Rossetti,G. Roudier,B. Rouillé d'Orfeuil,Michael Rowan-Robinson,Jose Alberto Rubino-Martin,Ben Rusholme,Najla Said,Valentina Salvatelli,L. Salvati,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,Michael Seiffert,Paolo Serra,E. P. S. Shellard,Locke D. Spencer,M. Spinelli,V. Stolyarov,R. Stompor,R. Sudiwala,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,T. Trombetti,M. Tucci,J. Tuovinen,M. Turler,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,B. Van Tent,P. Vielva,Fabrizio Villa,L. A. Wade,Benjamin D. Wandelt,Ingunn Kathrine Wehus,Martin White,Simon D. M. White,Althea Wilkinson,D. Yvon,Andrea Zacchei,Andrea Zonca +260 more
TL;DR: In this paper, the authors present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB, which are consistent with the six-parameter inflationary LCDM cosmology.
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