Zobrazeno 1 - 10
of 42
pro vyhledávání: '"Oliver H. E. Philcox"'
Publikováno v:
Physical Review X, Vol 13, Iss 1, p 011038 (2023)
The studies of disordered heterogeneous media and galaxy cosmology share a common goal: analyzing the disordered distribution of particles and/or building blocks at microscales to predict physical properties of the medium at macroscales, whether it b
Externí odkaz:
https://doaj.org/article/60e86a50c99f40ccb6a271ef47fd6e89
Autor:
Francisco Villaescusa-Navarro, Shy Genel, Daniel Anglés-Alcázar, Lucia A. Perez, Pablo Villanueva-Domingo, Digvijay Wadekar, Helen Shao, Faizan G. Mohammad, Sultan Hassan, Emily Moser, Erwin T. Lau, Luis Fernando Machado Poletti Valle, Andrina Nicola, Leander Thiele, Yongseok Jo, Oliver H. E. Philcox, Benjamin D. Oppenheimer, Megan Tillman, ChangHoon Hahn, Neerav Kaushal, Alice Pisani, Matthew Gebhardt, Ana Maria Delgado, Joyce Caliendo, Christina Kreisch, Kaze W. K. Wong, William R. Coulton, Michael Eickenberg, Gabriele Parimbelli, Yueying Ni, Ulrich P. Steinwandel, Valentina La Torre, Romeel Dave, Nicholas Battaglia, Daisuke Nagai, David N. Spergel, Lars Hernquist, Blakesley Burkhart, Desika Narayanan, Benjamin Wandelt, Rachel S. Somerville, Greg L. Bryan, Matteo Viel, Yin Li, Vid Irsic, Katarina Kraljic, Federico Marinacci, Mark Vogelsberger
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 265, Iss 2, p 54 (2023)
The Cosmology and Astrophysics with Machine Learning Simulations (CAMELS) project was developed to combine cosmology with astrophysics through thousands of cosmological hydrodynamic simulations and machine learning. CAMELS contains 4233 cosmological
Externí odkaz:
https://doaj.org/article/3325626d077745a3abeb937b84af2f24
Autor:
Zachary Slepian, Oliver H E Philcox
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 522:L42-L45
The homologous collapse from rest of a uniform density sphere under its self gravity is a well-known toy model for the formation dynamics of astronomical objects ranging from stars to galaxies. Equally well-known is that the evolution of the radius w
The widely used MASTER approach for angular power spectrum estimation was developed as a fast $C_{\ell}$ estimator on limited regions of the sky. This method expresses the power spectrum of a masked map ("pseudo-$C_\ell$") in terms of the power spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e88ef9364f469ec2dbbce9605afad1d2
http://arxiv.org/abs/2302.05436
http://arxiv.org/abs/2302.05436
Autor:
Oliver H E, Philcox, Zachary, Slepian
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America. 119(33)
We present efficient algorithms for computing the
Autor:
Mikhail M. Ivanov, Oliver H. E. Philcox, Giovanni Cabass, Takahiro Nishimichi, Marko Simonović, Matias Zaldarriaga
We present a framework for self-consistent cosmological analyses of the full-shape anisotropic bispectrum, including the quadrupole $(\ell=2)$ and hexadecapole $(\ell=4)$ moments. This features a novel window-free algorithm for extracting the latter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7e3d8d3a1499a2df3f2e59f9c4f0097
http://arxiv.org/abs/2302.04414
http://arxiv.org/abs/2302.04414
Publikováno v:
Physical Review D. 107
Could new physics break the mirror symmetry of the Universe? Utilizing recent measurements of the parity-odd four-point correlation function of BOSS galaxies, we probe the physics of inflation by placing constraints on the amplitude of a number of pa
Autor:
Zachary Slepian, Robert N. Cahn, Jiamin Hou, Craig Warner, Daniel J. Eisenstein, Oliver H. E. Philcox
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 509:2457-2481
We present a new algorithm for efficiently computing the N-point correlation functions (NPCFs) of a 3D density field for arbitrary N. This can be applied both to a discrete spectroscopic galaxy survey and a continuous field. By expanding the statisti
Publikováno v:
Physical Review D. 106
The polarized Sunyaev-Zel'dovich (pSZ) effect is sourced by the Thomson scattering of CMB photons from distant free electrons and yields a novel view of the CMB quadrupole throughout the observable Universe. Galaxy shear measures the shape distortion
Publikováno v:
Physical Review D. 106