# Joseph E. McEwen

## Publications Authored By Joseph E. McEwen

**Authors:**Metin Ata, Falk Baumgarten, Julian Bautista, Florian Beutler, Dmitry Bizyaev, Michael R. Blanton, Jonathan A. Blazek, Adam S. Bolton, Jonathan Brinkmann, Joel R. Brownstein, Etienne Burtin, Chia-Hsun Chuang, Johan Comparat, Kyle S. Dawson, Axel de la Macorra, Wei Du, Helion du Mas des Bourboux, Daniel J. Eisenstein, Hector Gil-Marin, Katie Grabowski, Julien Guy, Nick Hand, Shirley Ho, Timothy A. Hutchinson, Mikhail M. Ivanov, Francisco-Shu Kitaura, Jean-Paul Kneib, Pierre Laurent, Jean-Marc Le Goff, Joseph E. McEwen, Eva-Maria Mueller, Adam D. Myers, Jeffrey A. Newman, Nathalie Palanque-Delabrouille, Kaike Pan, Isabelle Paris, Marcos Pellejero-Ibanez, Will J. Percival, Patrick Petitjean, Francisco Prada, Abhishek Prakash, Sergio A. Rodriguez-Torres, Ashley J. Ross, Graziano Rossi, Rossana Ruggeri, Ariel G. Sanchez, Siddharth Satpathy, David J. Schlegel, Donald P. Schneider, Hee-Jong Seo, Anze Slosar, Alina Streblyanska, Jeremy L. Tinker, Rita Tojeiro, Mariana Vargas Magana, M. Vivek, Yuting Wang, Christophe Yeche, Liang Yu, Pauline Zarrouk, Cheng Zhao, Gong-Bo Zhao, Fangzhou Zhu

**Category:**Cosmology and Nongalactic Astrophysics

We present measurements of the Baryon Acoustic Oscillation (BAO) scale in redshift-space using the clustering of quasars. We consider a sample of 147,000 quasars from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) distributed over 2044 square degrees with redshifts $0.8 < z < 2. Read More

Cosmological perturbation theory is a powerful tool to predict the statistics of large-scale structure in the weakly non-linear regime, but even at 1-loop order it results in computationally expensive mode-coupling integrals. Here we present a fast algorithm for computing 1-loop power spectra of quantities that depend on the observer's orientation, thereby generalizing the FAST-PT framework (McEwen et al., 2016) that was originally developed for scalars such as the matter density. Read More

**Authors:**Zachary Slepian, Daniel J. Eisenstein, Jonathan A. Blazek, Joel R. Brownstein, Chia-Hsun Chuang, Héctor Gil-Marín, Shirley Ho, Francisco-Shu Kitaura, Joseph E. McEwen, Will J. Percival, Ashley J. Ross, Graziano Rossi, Hee-Jong Seo, Anže Slosar, Mariana Vargas-Magaña

**Category:**Cosmology and Nongalactic Astrophysics

We search for a galaxy clustering bias due to a modulation of galaxy number with the baryon-dark matter relative velocity resulting from recombination-era physics. We find no detected signal and place the constraint $b_v < 0.01$ on the relative velocity bias for the CMASS galaxies. Read More

We present a novel algorithm, FAST-PT, for performing convolution or mode-coupling integrals that appear in nonlinear cosmological perturbation theory. The algorithm uses several properties of gravitational structure formation -- the locality of the dark matter equations and the scale invariance of the problem -- as well as Fast Fourier Transforms to describe the input power spectrum as a superposition of power laws. This yields extremely fast performance, enabling mode-coupling integral computations fast enough to embed in Monte Carlo Markov Chain parameter estimation. Read More

The combination of galaxy-galaxy lensing (GGL) and galaxy clustering is a promising route to measuring the amplitude of matter clustering and testing modified gravity theories of cosmic acceleration. Halo occupation distribution (HOD) modeling can extend the approach down to nonlinear scales, but galaxy assembly bias could introduce systematic errors by causing the HOD to vary with large scale environment at fixed halo mass. We investigate this problem using the mock galaxy catalogs created by Hearin & Watson (2013, HW13), which exhibit significant assembly bias because galaxy luminosity is tied to halo peak circular velocity and galaxy colour is tied to halo formation time. Read More

At the epoch of decoupling, cosmic baryons had supersonic velocities relative to the dark matter that were coherent on large scales. These velocities subsequently slow the growth of small-scale structure and, via feedback processes, can influence the formation of larger galaxies. We examine the effect of streaming velocities on the galaxy correlation function, including all leading-order contributions for the first time. Read More

We examine the statistics of the low-redshift Lyman-alpha forest from smoothed particle hydrodynamic simulations in light of recent improvements in the estimated evolution of the cosmic ultraviolet background (UVB) and recent observations from the Cosmic Origins Spectrograph (COS). We find that the value of the metagalactic photoionization rate required by our simulations to match the observed properties of the low-redshift Lyman-alpha forest is a factor of 5 larger than the value predicted by state-of-the art models for the evolution of this quantity. This mismatch results in the mean flux decrement of the Lyman-alpha forest being underpredicted by at least a factor of 2 (a 10-sigma discrepancy with observations) and a column density distribution of Lyman-alpha forest absorbers systematically and significantly elevated compared to observations over nearly two decades in column density. Read More

**Category:**Nuclear Theory

A formalism is presented that allows an asymptotically exact solution of non-relativistic and semi-relativistic two-body problems with infinitely rising confining potentials. We consider both linear and quadratic confinement. The additional short-range terms are expanded in a Coulomb-Sturmian basis. Read More