nIFTy cosmology: comparison of galaxy formation models

作者: Daniel Cunnama , Gabriella De Lucia , Julien E. Devriendt , Pascal J. Elahi , Andreea Font

DOI: 10.1093/MNRAS/STV1149

关键词: Dark matterStar formationCosmologyGalaxyHalo occupation distributionGalaxy formation and evolutionAstronomyCalibration (statistics)PhysicsAstrophysicsStellar mass

摘要: We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 halo occupation distribution for based upon the same cosmological simulation merger tree information derived from it. The participating codes have proven to be very successful in their own right but they all been calibrated independently using various observational data sets, stellar models, trees. In this paper, we apply them without recalibration leads wide variety predictions mass function, specific star rates, stellar-to-halo ratios, abundance orphan galaxies. scatter is much larger than seen previous studies primarily because used outside native environment within which are well tested calibrated. purpose ‘nIFTy models’ bring together as many modellers possible investigate common approach model calibration. This paper provides unified description presents initial, uncalibrated baseline our future where will develop calibration framework address extent that reduces here.

参考文章(310)
Rachel S. Somerville, Rudy C. Gilmore, Joel R. Primack, Alberto Domínguez, Galaxy Properties from the Ultra-violet to the Far-Infrared: Lambda-CDM models confront observations arXiv: Cosmology and Nongalactic Astrophysics. ,(2011) , 10.1111/J.1365-2966.2012.20490.X
M. Viola, P. Monaco, S. Borgani, G. Murante, L. Tornatore, How does gas cool in DM halos arXiv: Astrophysics. ,(2007) , 10.1111/J.1365-2966.2007.12598.X
Gabriella De Lucia, Fabio Fontanot, David Wilman, Pierluigi Monaco, Times, environments and channels of bulge formation in a LambdaCDM cosmology arXiv: Cosmology and Nongalactic Astrophysics. ,(2011) , 10.1111/J.1365-2966.2011.18475.X
A. V. Macciò, S. Gottlöber, A. A. Dutton, J. C. Muñoz-Cuartas, The Redshift Evolution of LCDM Halo Parameters: Concentration, Spin, and Shape arXiv: Cosmology and Nongalactic Astrophysics. ,(2010) , 10.1111/J.1365-2966.2010.17704.X
J. B. Hyde, M. Bernardi, R. K. Sheth, A. Pizzella, E. Tundo, On the inconsistency between the black hole mass function inferred from M_bh-sigma and M_bh-L correlation arXiv: Astrophysics. ,(2006) , 10.1086/518225
James Binney, Scott Tremaine, Galactic Dynamics: Second Edition Galactic Dynamics: Second Edition. ,(2008) , 10.1515/9781400828722
V. Gonzalez-Perez, C. G. Lacey, C. M. Baugh, C. D. P. Lagos, J. Helly, D. J. R. Campbell, P. D. Mitchell, How sensitive are predicted galaxy luminosities to the choice of stellar population synthesis model Monthly Notices of the Royal Astronomical Society. ,vol. 439, pp. 264- 283 ,(2014) , 10.1093/MNRAS/STT2410
Joel R. Primack, Rudy C. Gilmore, Rudy C. Gilmore, Alberto Domínguez, Alberto Domínguez, Rachel S. Somerville, Rachel S. Somerville, Galaxy properties from the ultraviolet to the far‐infrared: Λ cold dark matter models confront observations Monthly Notices of the Royal Astronomical Society. ,vol. 423, pp. 1992- 2015 ,(2012) , 10.1111/J.1365-2966.2012.20490.X
Hannah Parkinson, Shaun Cole, John Helly, Generating dark matter halo merger trees Monthly Notices of the Royal Astronomical Society. ,vol. 383, pp. 557- 564 ,(2007) , 10.1111/J.1365-2966.2007.12517.X