Galaxy formation and evolution

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Identification of old tidal dwarfs near early-type galaxies from deep imaging and HI observations

(2014)

Authors:

Pierre-Alain Duc, Sanjaya Paudel, Richard M McDermid, Jean-Charles Cuillandre, Paolo Serra, Frédéric Bournaud, Michele Cappellari, Eric Emsellem
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Salpeter normalization of the Stellar Initial Mass Function for massive galaxies at z~1

(2014)

Authors:

Shravan Shetty, Michele Cappellari
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The stellar IMF in early-type galaxies from a non-degenerate set of optical line indices

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 438:2 (2014) 1483-1499

Authors:

Chiara Spiniello, Scott Trager, Léon VE Koopmans, Charlie Conroy
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Milli-arcsecond properties of 10C sources in the Lockman Hole

ArXiv 1402.2553 (2014)

Authors:

Imogen H Whittam, Julia M Riley, David A Green
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Dancing in the dark: galactic properties trace spin swings along the cosmic web

ArXiv 1402.1165 (2014)

Authors:

Yohan Dubois, Christophe Pichon, Charlotte Welker, Damien Le Borgne, Julien Devriendt, Clotilde Laigle, Sandrine Codis, Dmitry Pogosyan, Stéphane Arnouts, Karim Benabed, Emmanuel Bertin, Jeremy Blaizot, François Bouchet, Jean-François Cardoso, Stéphane Colombi, Valérie de Lapparent, Vincent Desjacques, Raphaël Gavazzi, Susan Kassin, Taysun Kimm, Henry McCracken, Bruno Milliard, Sébastien Peirani, Simon Prunet, Stéphane Rouberol, Joseph Silk, Adrianne Slyz, Thierry Sousbie, Romain Teyssier, Laurence Tresse, Marie Treyer, Didier Vibert, Marta Volonteri

Abstract:

A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments above redshift 1.2. The analysis of more than 150 000 galaxies per time step in the redshift range 1.2
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