The Mira-Titan Universe. II. Matter Power Spectrum Emulation
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Hal Finkel | Earl Lawrence | David Higdon | Derek Bingham | Katrin Heitmann | Adrian Pope | Nicholas Frontiere | Salman Habib | Juliana Kwan | D. Higdon | D. Bingham | A. Pope | S. Habib | K. Heitmann | E. Lawrence | J. Kwan | H. Finkel | N. Frontiere | Amol Upadhye | A. Upadhye
[1] Daniel Thomas,et al. Cosmology from large-scale galaxy clustering and galaxy-galaxy lensing with dark energy survey science verification data , 2016, 1604.07871.
[2] Yin Li,et al. Quintessential scale dependence from separate universe simulations , 2016, 1609.01701.
[3] Yin Li,et al. Separating the Universe into real and fake energy densities , 2016 .
[4] T. Prusti,et al. Kinematics of symmetric Galactic longitudes to probe the spiral arms of the Milky Way with Gaia , 2016, 1602.07687.
[5] C. Heymans,et al. Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces , 2016, 1602.02154.
[6] L. Casarini,et al. Extending the Coyote emulator to dark energy models with standard w0-wa parametrization of the equation of state , 2016, 1601.07230.
[7] C. B. D'Andrea,et al. Cosmology from cosmic shear with Dark Energy Survey science verification data , 2015, 1507.05552.
[8] Hal Finkel,et al. HACC: Simulating Sky Surveys on State-of-the-Art Supercomputing Architectures , 2014, 1410.2805.
[9] Hal Finkel,et al. THE MIRA–TITAN UNIVERSE: PRECISION PREDICTIONS FOR DARK ENERGY SURVEYS , 2015, 1508.02654.
[10] Shahab Joudaki,et al. An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models , 2015, 1505.07833.
[11] J. Harnois-Déraps,et al. Precision reconstruction of the cold dark matter-neutrino relative velocity from N -body simulations , 2015, 1503.07480.
[12] S. Bridle,et al. Cosmic Discordance: Are Planck CMB and CFHTLenS weak lensing measurements out of tune? , 2014, 1408.4742.
[13] Scott Dodelson,et al. Accounting for baryonic effects in cosmic shear tomography: determining a minimal set of nuisance parameters using PCA , 2014, 1405.7423.
[14] Hal Finkel,et al. COSMIC EMULATION: FAST PREDICTIONS FOR THE GALAXY POWER SPECTRUM , 2013, 1311.6444.
[15] Mark Trodden,et al. Beyond the Cosmological Standard Model , 2014, 1407.0059.
[16] H. Hoekstra,et al. 3D cosmic shear: cosmology from CFHTLenS , 2014, 1401.6842.
[17] Shaun A. Thomas,et al. pkann – II. A non-linear matter power spectrum interpolator developed using artificial neural networks , 2013, 1312.2101.
[18] R. Biswas,et al. Large-scale structure formation with massive neutrinos and dynamical dark energy , 2013, 1309.5872.
[19] C. A. Oxborrow,et al. Planck 2013 results. XVI. Cosmological parameters , 2013, 1303.5076.
[20] Earl Lawrence,et al. THE COYOTE UNIVERSE EXTENDED: PRECISION EMULATION OF THE MATTER POWER SPECTRUM , 2013, 1304.7849.
[21] Scott Dodelson,et al. Accounting for Baryons in Cosmological Constraints from Cosmic Shear , 2012, 1212.1177.
[22] Katrin Heitmann,et al. COSMIC EMULATION: THE CONCENTRATION–MASS RELATION FOR wCDM UNIVERSES , 2012, 1210.1576.
[23] G. Bruce Berriman,et al. Astrophysics Source Code Library , 2012, ArXiv.
[24] Takahiro Nishimichi,et al. REVISING THE HALOFIT MODEL FOR THE NONLINEAR MATTER POWER SPECTRUM , 2012, 1208.2701.
[25] Daniel Thomas,et al. The clustering of galaxies in the sdss-iii baryon oscillation spectroscopic survey: Baryon acoustic oscillations in the data release 9 spectroscopic galaxy sample , 2012, 1312.4877.
[26] Steven Bergner,et al. Making choices in multi-dimensional parameter spaces , 2011 .
[27] M. Viel,et al. Massive neutrinos and the non‐linear matter power spectrum , 2011, 1109.4416.
[28] H. Feldman,et al. The effect of massive neutrinos on the matter power spectrum , 2010, 1006.0689.
[29] Jonathan L. Feng. Dark Matter Candidates from Particle Physics and Methods of Detection , 2010, 1003.0904.
[30] Earl Lawrence,et al. THE COYOTE UNIVERSE. III. SIMULATION SUITE AND PRECISION EMULATOR FOR THE NONLINEAR MATTER POWER SPECTRUM , 2009, 0912.4490.
[31] M. Kamionkowski,et al. The Physics of Cosmic Acceleration , 2009, 0903.0866.
[32] David Higdon,et al. THE COYOTE UNIVERSE. II. COSMOLOGICAL MODELS AND PRECISION EMULATION OF THE NONLINEAR MATTER POWER SPECTRUM , 2009, 0902.0429.
[33] D. Higdon,et al. THE COYOTE UNIVERSE. I. PRECISION DETERMINATION OF THE NONLINEAR MATTER POWER SPECTRUM , 2008, 0812.1052.
[34] D. Higdon,et al. Cosmic calibration: Constraints from the matter power spectrum and the cosmic microwave background , 2007, astro-ph/0702348.
[35] E. Linder. Exploring the expansion history of the universe. , 2002, Physical review letters.
[36] J. Peacock,et al. Stable clustering, the halo model and non-linear cosmological power spectra , 2002, astro-ph/0207664.
[37] M. Chevallier,et al. ACCELERATING UNIVERSES WITH SCALING DARK MATTER , 2000, gr-qc/0009008.
[38] A. Lewis,et al. Efficient computation of CMB anisotropies in closed FRW models , 1999, astro-ph/9911177.
[39] G. Murante,et al. Cluster Mass Function in Mixed Models , 1999, astro-ph/9905281.
[40] J. Holtzman,et al. Structure formation with cold plus hot dark matter , 1993, astro-ph/9305011.