Oliver Philcox

All Publications

• Reanalyzing DESI DR1. III. Constraints on inflation from galaxy power spectra and bispectra PHYSICAL REVIEW D Chudaykin, A., Ivanov, M. M., Philcox, O. H. E. 2026; 113 (6)

  View details for DOI 10.1103/fhj3-6q4x

  View details for Web of Science ID 001721922000001

• Reanalyzing DESI DR1. I. ΛCDM constraints from the power spectrum and bispectrum PHYSICAL REVIEW D Chudaykin, A., Ivanov, M. M., Philcox, O. H. E. 2026; 113 (6)

  View details for DOI 10.1103/qsnt-dppc

  View details for Web of Science ID 001711188500001

• Quantum stress-energy at timelike boundaries: Testing a new beyond-ΛCDM parameter with cosmological data PHYSICAL REVIEW D Philcox, O. H. E., Silverstein, E., Torroba, G. 2026; 113 (4)

  View details for DOI 10.1103/162y-rmsv

  View details for Web of Science ID 001705986000006

• Modeling galaxy surveys with hybrid simulation-based inference PHYSICAL REVIEW D Zhang, G., Modi, C., Philcox, O. H. E. 2026; 113 (4)

  View details for DOI 10.1103/zj8s-v23z

  View details for Web of Science ID 001697993500003

• Wonderings on wiggly bispectra: Nonlinear evolution and reconstruction of oscillations in the squeezed bispectrum PHYSICAL REVIEW D Goldstein, S., Philcox, O. H. E., Fondi, E., Coulton, W. R. 2025; 112 (8)

  View details for DOI 10.1103/q8m3-vspd

  View details for Web of Science ID 001598985600006

• Suite of optimal and efficient power spectrum and bispectrum estimators for large-scale structure analyses PHYSICAL REVIEW D Philcox, O. H. E., Floss, T. 2025; 112 (6)

  View details for DOI 10.1103/rr6c-cf3s

  View details for Web of Science ID 001571301500005

• A Parameter-masked Mock Data Challenge for Beyond-two-point Galaxy Clustering Statistics ASTROPHYSICAL JOURNAL Krause, E., Kobayashi, Y., Salcedo, A. N., Ivanov, M. M., Abel, T., Akitsu, K., Angulo, R. E., Cabass, G., Contarini, S., Cuesta-Lazaro, C., Hahn, C., Hamaus, N., Jeong, D., Modi, C., Nguyen, N., Nishimichi, T., Paillas, E., Ibanez, M., Philcox, O. H. E., Pisani, A., Schmidt, F., Tanaka, S., Verza, G., Yuan, S., Zennaro, M. 2025; 990 (2)

  View details for DOI 10.3847/1538-4357/ad781d

  View details for Web of Science ID 001561554800001

• Searching for inflationary physics with the CMB trispectrum. II. Code and validation PHYSICAL REVIEW D Philcox, O. H. E. 2025; 111 (12)

  View details for DOI 10.1103/bprw-3zj1

  View details for Web of Science ID 001514484300016

• Searching for inflationary physics with the CMB trispectrum. I. Primordial theory and optimal estimators PHYSICAL REVIEW D Philcox, O. H. E. 2025; 111 (12)

  View details for DOI 10.1103/wkj2-q62t

  View details for Web of Science ID 001514484300011

• Searching for inflationary physics with the CMB trispectrum. III. Constraints from<i> Planck</i> PHYSICAL REVIEW D Philcox, O. H. E. 2025; 111 (12)

  View details for DOI 10.1103/y81z-g7th

  View details for Web of Science ID 001514484300005

• Integrated Sachs-Wolfe lensing bispectrum and trispectrum PHYSICAL REVIEW D Philcox, O. H. E., Hill, J. 2025; 111 (12)

  View details for DOI 10.1103/wsjw-32l6

  View details for Web of Science ID 001523437700011

• Non-Gaussianity beyond the scalar sector: A search for tensor and mixed tensor-scalar bispectra with Planck data PHYSICAL REVIEW D Philcox, O. H. E., Shiraishi, M. 2025; 111 (12)

  View details for DOI 10.1103/pb7x-lp19

  View details for Web of Science ID 001511064200008

• Searching for inflationary particle production in<i> Planck</i> data PHYSICAL REVIEW D Philcox, O. H. E., Kumar, S., Hill, J. 2025; 111 (10)

  View details for DOI 10.1103/PhysRevD.111.103523

  View details for Web of Science ID 001494567200002

• BOSS constraints on massive particles during inflation: The cosmological collider in action PHYSICAL REVIEW D Cabass, G., Philcox, O. H. E., Ivanov, M. M., Akitsu, K., Chen, S., Simonovi, M., Zaldarriaga, M. 2025; 111 (6)

  View details for DOI 10.1103/PhysRevD.111.063510

  View details for Web of Science ID 001458949100008

• Could sample variance be responsible for the parity-violating signal seen in the Baryon Oscillation Spectroscopic Survey? PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES Philcox, O. E., Ereza, J. 2025; 383 (2290): 20240034

  Abstract

  Recent works have uncovered an excess signal in the parity-odd four-point correlation function measured from the Baryon Oscillation Spectroscopic Survey (BOSS) galaxy catalogue. If physical in origin, this could indicate new parity-breaking processes in inflation. At heart, these studies compare the observed four-point correlator with the distribution obtained from parity-conserving mock galaxy surveys; if the simulations underestimate the covariance of the data, noise fluctuations may be misinterpreted as a signal. To test this, we reanalyse the BOSS CMASS parity-odd dataset with the noise distribution model using the newly developed GLAM-Uchuu suite of mocks. These comprise full [Formula: see text]-body simulations that follow the evolution of [Formula: see text] dark matter particles and represent a significant upgrade compared with the formerly used MultiDark-Patchy mocks, which were based on an alternative (non [Formula: see text]-body) gravity solver. We find no significant evidence for parity-violation (with a baseline detection significance of [Formula: see text]), suggesting that the former signal ([Formula: see text] with our data cuts) could be caused by an underestimation of the covariance in MultiDark-Patchy. The significant differences between results obtained with the two sets of BOSS-calibrated galaxy catalogues (whose covariances differ at the [Formula: see text] level) showcase the heightened sensitivity of beyond-two-point analyses to nonlinear effects and indicate that previous constraints may suffer from large systematic uncertainties.This article is part of the discussion meeting issue 'Challenging the standard cosmological model'.

  View details for DOI 10.1098/rsta.2024.0034

  View details for Web of Science ID 001428238700006

  View details for PubMedID 39938550

  View details for PubMedCentralID PMC12169525

• Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering PHYSICAL REVIEW LETTERS Chen, S., Ivanov, M. M., Philcox, O. H. E., Wenzl, L. 2024; 133 (23): 231001

  Abstract

  We present a new perturbative full-shape analysis of BOSS galaxy clustering data, including the full combination of the galaxy power spectrum and bispectrum multipoles, baryon acoustic oscillations, and cross-correlations with the gravitational lensing of cosmic microwave background measured from Planck. Assuming the ΛCDM model, we constrain the matter density fraction Ω_{m}=0.3138±0.0086, the Hubble constant H_{0}=68.23±0.78  km s^{-1} Mpc^{-1}, and the mass fluctuation amplitude σ_{8}=0.688±0.026 (equivalent to S_{8}=0.703±0.029). Cosmic structure at low redshifts appears suppressed with respect to the Planck ΛCDM concordance model at 4.5σ. We explore the implications of this dataset for the recent DESI BAO preference for dynamical dark energy (DDE): the BOSS data combine with DESI BAO and PantheonPlus supernovae competitively compared to the CMB, yielding no preference for DDE, but the same ∼10% suppression of structure, with dark energy being consistent with a cosmological constant at 68% CL. Our results suggest that either the data contains residual systematics, or more model-building efforts may be required to restore cosmological concordance.

  View details for DOI 10.1103/PhysRevLett.133.231001

  View details for Web of Science ID 001376943000002

  View details for PubMedID 39714644

• Intermediate mass-range particles from small scales: Nonperturbative techniques for cosmological collider physics from large-scale structure surveys PHYSICAL REVIEW D Goldstein, S., Philcox, O. H. E., Hill, J., Hui, L. 2024; 110 (8)

  View details for DOI 10.1103/PhysRevD.110.083516

  View details for Web of Science ID 001339038100007

• The 3D Lyman-α forest power spectrum from eBOSS DR16 MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY de Belsunce, R., Philcox, O. H. E., Irsic, V., McDonald, P., Guy, J., Palanque-Delabrouille, N. 2024; 533 (3): 3756-3770

  View details for DOI 10.1093/mnras/stae2035

  View details for Web of Science ID 001306863900002

• Testing parity symmetry with the polarized cosmic microwave background PHYSICAL REVIEW D Philcox, O. H. E., Shiraishi, M. 2024; 109 (8)

  View details for DOI 10.1103/PhysRevD.109.083514

  View details for Web of Science ID 001224785000006

• What can galaxy shapes tell us about physics beyond the standard model? PHYSICAL REVIEW D Philcox, O. H. E., Konig, M. J., Alexander, S., Spergel, D. N. 2024; 109 (6)

  View details for DOI 10.1103/PhysRevD.109.063541

  View details for Web of Science ID 001195489900007

• Testing graviton parity and Gaussianity with Planck T-, E-, and B-mode bispectra PHYSICAL REVIEW D Philcox, O. H. E., Shiraishi, M. 2024; 109 (6)

  View details for DOI 10.1103/PhysRevD.109.063522

  View details for Web of Science ID 001195813300001

• Consistently constraining fNL with the squeezed lensing bispectrum using consistency relations PHYSICAL REVIEW D Goldstein, S., Philcox, O. H. E., Hill, J., Esposito, A., Hui, L. 2024; 109 (4)

  View details for DOI 10.1103/PhysRevD.109.043515

  View details for Web of Science ID 001172759700001

• Signatures of a parity-violating universe PHYSICAL REVIEW D Coulton, W. R., Philcox, O. H. E., Villaescusa-Navarro, F. 2024; 109 (2)

  View details for DOI 10.1103/PhysRevD.109.023531

  View details for Web of Science ID 001174885400008

• Do the CMB Temperature Fluctuations Conserve Parity? PHYSICAL REVIEW LETTERS Philcox, O. H. E. 2023; 131 (18): 181001

  Abstract

  Observations of the cosmic microwave background (CMB) have cemented the notion that the large-scale Universe is both statistically homogeneous and isotropic. But is it invariant also under reflections? To probe this we require parity-sensitive statistics: for scalar observables, the simplest is the trispectrum. We make the first measurements of the parity-odd scalar CMB, focusing on the large-scale (2<ℓ<510) temperature anisotropies measured by Planck. This is facilitated by new quasi-maximum-likelihood estimators for binned correlators, which account for mask convolution and leakage between even- and odd-parity components, and achieve ideal variances within ≈20%. We perform a blind test for parity violation by comparing a χ^{2} statistic from Planck to theoretical expectations, using two suites of simulations to account for the possible likelihood non-Gaussianity and residual foregrounds. We find consistency at the ≈0.4σ level, yielding no evidence for novel early-Universe phenomena. The measured trispectra allow for a wealth of new physics to be constrained; here, we use them to constrain eight primordial models, including ghost inflation, cosmological collider scenarios, and Chern-Simons gauge fields. We find no signatures of new physics, with a maximal detection significance of 2.0σ. Our results also indicate that the recent parity excesses seen in the BOSS galaxy survey are not primordial in origin, given that the CMB dataset contains roughly 250× more primordial modes, and is far easier to interpret, given the linear physics, Gaussian statistics, and accurate mocks. Tighter CMB constraints can be wrought by including smaller scales (though rotational invariance washes out the flat-sky limit) and adding polarization data.

  View details for DOI 10.1103/PhysRevLett.131.181001

  View details for Web of Science ID 001640051900001

  View details for PubMedID 37977606

• Parity-violating trispectrum from Chern-Simons gravity JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS Creque-Sarbinowski, C., Alexander, S., Kamionkowski, M., Philcox, O. 2023

  View details for DOI 10.1088/1475-7516/2023/11/029

  View details for Web of Science ID 001167989300004

• Optimal estimation of the binned mask-free power spectrum, bispectrum, and trispectrum on the full sky: Tensor edition PHYSICAL REVIEW D Philcox, O. H. E. 2023; 108 (6)

  View details for DOI 10.1103/PhysRevD.108.063506

  View details for Web of Science ID 001070819500002

• Optimal estimation of the binned mask-free power spectrum, bispectrum, and trispectrum on the full sky: Scalar edition PHYSICAL REVIEW D Philcox, O. H. E. 2023; 107 (12)

  View details for DOI 10.1103/PhysRevD.107.123516

  View details for Web of Science ID 001055203300005

• Ultra-light axions and the S8 tension: joint constraints from the cosmic microwave background and galaxy clustering JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS Rogers, K. K., Hlozek, R., Lague, A., Ivanov, M. M., Philcox, O. H. E., Cabass, G., Akitsu, K., Marsh, D. J. E. 2023

  View details for DOI 10.1088/1475-7516/2023/06/023

  View details for Web of Science ID 001025474200002

• Accurate estimation of angular power spectra for maps with correlated masks PHYSICAL REVIEW D Surrao, K. M., Philcox, O. H. E., Hill, J. 2023; 107 (8)

  View details for DOI 10.1103/PhysRevD.107.083521

  View details for Web of Science ID 000975806700004

• Constraining single-field inflation with MegaMapper PHYSICS LETTERS B Cabass, G., Ivanov, M. M., Philcox, O. H. E., Simonovic, M., Zaldarriaga, M. 2023; 841

  View details for DOI 10.1016/j.physletb.2023.137912

  View details for Web of Science ID 000984229400001

• Cosmology with the galaxy bispectrum multipoles: Optimal estimation and application to BOSS data PHYSICAL REVIEW D Ivanov, M. M., Philcox, O. H. E., Cabass, G., Nishimichi, T., Simonovic, M., Zaldarriaga, M. 2023; 107 (8)

  View details for DOI 10.1103/PhysRevD.107.083515

  View details for Web of Science ID 000974677700007

• The CAMELS Project: Public Data Release ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES Villaescusa-Navarro, F., Genel, S., Angles-Alcazar, D., Perez, L. A., Villanueva-Domingo, P., Wadekar, D., Shao, H., Mohammad, F. G., Hassan, S., Moser, E., Lau, E. T., Valle, L., Nicola, A., Thiele, L., Jo, Y., Philcox, O. H. E., Oppenheimer, B. D., Tillman, M., Hahn, C., Kaushal, N., Pisani, A., Gebhardt, M., Delgado, A., Caliendo, J., Kreisch, C., Wong, K. W. K., Coulton, W. R., Eickenberg, M., Parimbelli, G., Ni, Y., Steinwandel, U. P., La Torre, V., Dave, R., Battaglia, N., Nagai, D., Spergel, D. N., Hernquist, L., Burkhart, B., Narayanan, D., Wandelt, B., Somerville, R. S., Bryan, G. L., Viel, M., Li, Y., Irsic, V., Kraljic, K., Marinacci, F., Vogelsberger, M. 2023; 265 (2)

  View details for DOI 10.3847/1538-4365/acbf47

  View details for Web of Science ID 000964876300001

• A uniform spherical goat (problem): explicit solution for homologous collapse's radial evolution in time MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Slepian, Z., Philcox, O. H. E. 2023; 522 (1): L42-L45

  View details for DOI 10.1093/mnrasl/slac153

  View details for Web of Science ID 001066034100009

• Disordered Heterogeneous Universe: Galaxy Distribution and Clustering across Length Scales PHYSICAL REVIEW X Philcox, O. H. E., Torquato, S. 2023; 13 (1)

  View details for DOI 10.1103/PhysRevX.13.011038

  View details for Web of Science ID 000957629400001

• Colliders and ghosts: Constraining inflation with the parity-odd galaxy four-point function PHYSICAL REVIEW D Cabas, G., Ivanov, M. M., Philcox, O. H. E. 2023; 107 (2)

  View details for DOI 10.1103/PhysRevD.107.023523

  View details for Web of Science ID 000925057300007

• Squeezing f_NL out of the matter bispectrum with consistency relations PHYSICAL REVIEW D Goldstein, S., Esposito, A., Philcox, O. H. E., Hui, L., Hill, J., Scoccimarro, R., Abitbol, M. H. 2022; 106 (12)

  View details for DOI 10.1103/PhysRevD.106.123525

  View details for Web of Science ID 000910921600012

• Novel cosmological tests from combining galaxy lensing and the polarized Sunyaev-Zel'dovich effect PHYSICAL REVIEW D Philcox, O. H. E., Johnson, M. C. 2022; 106 (8)

  View details for DOI 10.1103/PhysRevD.106.083501

  View details for Web of Science ID 000879331700001

• Determining the Hubble constant without the sound horizon: A 3.6% constraint on <i>H</i>₀ from galaxy surveys, CMB lensing, and supernovae PHYSICAL REVIEW D Philcox, O. H. E., Farren, G. S., Sherwin, B. D., Baxter, E. J., Brout, D. J. 2022; 106 (6)

  View details for DOI 10.1103/PhysRevD.106.063530

  View details for Web of Science ID 000870044300009

• Probing parity violation with the four-point correlation function of BOSS galaxies PHYSICAL REVIEW D Philcox, O. H. E. 2022; 106 (6)

  View details for DOI 10.1103/PhysRevD.106.063501

  View details for Web of Science ID 000863110800002

• Cosmology with the redshift-space galaxy bispectrum monopole at one-loop order PHYSICAL REVIEW D Philcox, O. H. E., Ivanov, M. M., Cabass, G., Simonovic, M., Zaldarriaga, M., Nishimichi, T. 2022; 106 (4)

  View details for DOI 10.1103/PhysRevD.106.043530

  View details for Web of Science ID 000861232600008

• Efficient computation of <i>N</i>-point correlation functions in <i>D</i> dimensions PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA Philcox, O. H. E., Slepian, Z. 2022; 119 (33): e2111366119

  Abstract

  We present efficient algorithms for computing the N-point correlation functions (NPCFs) of random fields in arbitrary D-dimensional homogeneous and isotropic spaces. Such statistics appear throughout the physical sciences and provide a natural tool to describe stochastic processes. Typically, algorithms for computing the NPCF components have [Formula: see text] complexity (for a dataset containing n particles); their application is thus computationally infeasible unless N is small. By projecting the statistic onto a suitably defined angular basis, we show that the estimators can be written in a separable form, with complexity [Formula: see text] or [Formula: see text] if evaluated using a Fast Fourier Transform on a grid of size [Formula: see text]. Our decomposition is built upon the D-dimensional hyperspherical harmonics; these form a complete basis on the [Formula: see text] sphere and are intrinsically related to angular momentum operators. Concatenation of [Formula: see text] such harmonics gives states of definite combined angular momentum, forming a natural separable basis for the NPCF. As N and D grow, the number of basis components quickly becomes large, providing a practical limitation to this (and all other) approaches: However, the dimensionality is greatly reduced in the presence of symmetries; for example, isotropic correlation functions require only states of zero combined angular momentum. We provide a Julia package implementing our estimators and show how they can be applied to a variety of scenarios within cosmology and fluid dynamics. The efficiency of such estimators will allow higher-order correlators to become a standard tool in the analysis of random fields.

  View details for DOI 10.1073/pnas.2111366119

  View details for Web of Science ID 000891285100003

  View details for PubMedID 35939667

  View details for PubMedCentralID PMC9388109

• Constraints on multifield inflation from the BOSS galaxy survey PHYSICAL REVIEW D Cabass, G., Ivanov, M. M., Philcox, O. H. E., Simonovic, M., Zaldarriaga, M. 2022; 106 (4)

  View details for DOI 10.1103/PhysRevD.106.043506

  View details for Web of Science ID 000836423100005

• Analytic Gaussian covariance matrices for galaxy <i>N</i>-point correlation functions PHYSICAL REVIEW D Hou, J., Cahn, R. N., Philcox, O. H. E., Slepian, Z. 2022; 106 (4)

  View details for DOI 10.1103/PhysRevD.106.043515

  View details for Web of Science ID 000883063700003

• Constraints on Single-Field Inflation from the BOSS Galaxy Survey PHYSICAL REVIEW LETTERS Cabass, G., Ivanov, M. M., Philcox, O. H. E., Simonovi, M., Zaldarriaga, M. 2022; 129 (2): 021301

  Abstract

  Nonlocal primordial non-Gaussianity (NLPNG) is a smoking gun of interactions in single-field inflationary models and can be written as a combination of the equilateral and orthogonal templates. We present the first constraints on these from the redshift-space galaxy power spectra and bispectra of the BOSS data. These are the first such measurements independent of the cosmic microwave background fluctuations. We perform a consistent analysis that includes all necessary nonlinear corrections generated by NLPNG and vary all relevant cosmological and nuisance parameters in a global fit to the data. Our conservative analysis yields joint limits on the amplitudes of the equilateral and orthogonal shapes, f_{NL}^{equil}=940±600 and f_{NL}^{ortho}=-170±170 (both at 68% CL). These can be used to derive constraints on coefficients of the effective single-field inflationary Lagrangian; in particular, we find that the sound speed of inflaton fluctuations has the bound c_{s}≥0.013 at 95% CL. Fixing the quadratic galaxy bias and cosmological parameters, the constraints can be tightened to f_{NL}^{equil}=260±300 and f_{NL}^{ortho}=-23±120 (68% CL).

  View details for DOI 10.1103/PhysRevLett.129.021301

  View details for Web of Science ID 000828087900023

  View details for PubMedID 35867436

• Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies JOURNAL OF HIGH ENERGY ASTROPHYSICS Abdalla, E., Abellan, G., Aboubrahim, A., Agnello, A., Akarsu, O., Akrami, Y., Alestas, G., Aloni, D., Amendola, L., Anchordoqui, L. A., Anderson, R. I., Arendse, N., Asgari, M., Ballardini, M., Bargerx, V., Basilakos, S., Batista, R. C., Battistelli, E. S., Battye, R., Benetti, M., Benisty, D., Berlin, A., de Bernardis, P., Berti, E., Bidenko, B., Birrer, S., Blakeslee, J. P., Boddy, K. K., Bom, C. R., Bonilla, A., Borghi, N., Bouchet, F. R., Braglia, M., Buchert, T., Buckley-Geer, E., Calabrese, E., Caldwell, R. R., Camarena, D., Capozziello, S., Casertano, S., Chen, A., Chen, G., Chen, H., Chluba, J., Chudaykin, A., Cicoli, M., Copi, C. J., Courbin, F., Cyr-Racine, F., Czerny, B., Dainotti, M., D'Amico, G., Davis, A., Perez, J., de Haro, J., Delabrouille, J., Denton, P. B., Dhawan, S., Dienes, K. R., Di Valentino, E., Du, P., Eckert, D., Escamilla-Rivera, C., Ferte, A., Finelli, F., Fosalba, P., Freedman, W. L., Frusciante, N., Gaztanaga, E., Giare, W., Giusarma, E., Gomez-Valent, A., Handley, W., Harrison, I., Hart, L., Hazra, D., Heavens, A., Heinesen, A., Hildebrandt, H., Hill, J., Hogg, N. B., Holz, D. E., Hooper, D. C., Hosseininejad, N., Huterer, D., Ishak, M., Ivanov, M. M., Jaffe, A. H., Jang, I., Jedamzik, K., Jimenez, R., Joseph, M., Joudaki, S., Kamionkowski, M., Karwal, T., Kazantzidis, L., Keeley, R. E., Klasen, M., Komatsu, E., Koopmans, L. V. E., Kumar, S., Lamagna, L., Dn, R., Lee, C., Lesgourgues, J., Said, J., Lewis, T. R., L'Huillier, B., Lucca, M., Maartens, R., Macri, L. M., Marfatia, D., Marra, V., Martins, C. P., Masi, S., Matarrese, S., Mazumdar, A., Melchiorri, A., Mena, O., Mersini-Houghton, L., Mertens, J., Milakovic, D., Minami, Y., Miranda, V., Moreno-Pulido, C., Moresco, M., Mota, D. F., Mottola, E., Mozzon, S., Muir, J., Mukherjee, A., Mukherjee, S., Naselsky, P., Nath, P., Nesseris, S., Niedermann, F., Notari, A., Nunes, R. C., Colgain, E. O., Owens, K. A., Ozulker, E., Pace, F., Paliathanasis, A., Palmese, A., Pan, S., Paoletti, D., Bergliaffa, S., Perivolaropoulos, L., Pesce, D. W., Pettorino, V., Philcox, O. H. E., Pogosian, L., Poulin, V., Poulot, G., Raveri, M., Reid, M. J., Renzi, F., Riess, A. G., Sabla, V., Salucci, P., Salzano, V., Saridakis, E. N., Sathyaprakash, B. S., Schmaltz, M., Schoneberg, N., Scolnic, D., Sen, A. A., Sehgal, N., Shafieloo, A., Sheikh-Jabbari, M. M., Silk, J., Silvestri, A., Skaraj, F., Sloth, M. S., Soares-Santos, M., Peracaula, J., Songsheng, Y., Soriano, J. F., Staicova, D., Starkman, G. D., Szapudi, I., Teixeira, E. M., Thomas, B., Treu, T., Trott, E., van de Ruck, C., Vazquez, J., Verde, L., Visinelli, L., Wang, D., Wang, J., Wang, S., Watkins, R., Watson, S., Webb, J. K., Weiner, N., Weltman, A., Witte, S. J., Wojtak, R., Yadav, A., Yang, W., Zhao, G., Zumalacarregui, M. 2022; 34: 49-211

  View details for DOI 10.1016/j.jheap.2022.04.002

  View details for Web of Science ID 000807122400002

• Precision analysis of the redshift-space galaxy bispectrum PHYSICAL REVIEW D Ivanov, M. M., Philcox, O. H. E., Nishimichi, T., Simonovic, M., Takada, M., Zaldarriaga, M. 2022; 105 (6)

  View details for DOI 10.1103/PhysRevD.105.063512

  View details for Web of Science ID 000770875800005

• Determining the Hubble constant without the sound horizon: Perspectives PHYSICAL REVIEW D Farren, G. S., Philcox, O. H. E., Sherwin, B. D. 2022; 105 (6)

  View details for DOI 10.1103/PhysRevD.105.063503

  View details for Web of Science ID 000767152100001

• Cosmological constraints without nonlinear redshift-space distortions PHYSICAL REVIEW D Ivanov, M. M., Philcox, O. H. E., Simonovic, M., Zaldarriaga, M., Nischimichi, T., Takada, M. 2022; 105 (4)

  View details for DOI 10.1103/PhysRevD.105.043531

  View details for Web of Science ID 000761169800003

• BOSS DR12 full-shape cosmology: ΛCDM constraints from the large-scale galaxy power spectrum and bispectrum monopole PHYSICAL REVIEW D Philcox, O. H. E., Ivanov, M. M. 2022; 105 (4)

  View details for DOI 10.1103/PhysRevD.105.043517

  View details for Web of Science ID 000761170400007

• Cosmology without window functions. II. Cubic estimators for the galaxy bispectrum PHYSICAL REVIEW D Philcox, O. H. E. 2021; 104 (12)

  View details for DOI 10.1103/PhysRevD.104.123529

  View details for Web of Science ID 000731839200012

• encore: an <i>O</i> (<i>N</i>_g<SUP>2</SUP>) estimator for galaxy <i>N</i>-point correlation functions MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Philcox, O. H. E., Slepian, Z., Hou, J., Warner, C., Cahn, R. N., Eisenstein, D. J. 2022; 509 (2): 2457-2481

  View details for DOI 10.1093/mnras/stab3025

  View details for Web of Science ID 000728381700062

• An exact integral-to-sum relation for products of Bessel functions PROCEEDINGS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES Philcox, O. H. E., Slepian, Z. 2021; 477 (2253)

  View details for DOI 10.1098/rspa.2021.0376

  View details for Web of Science ID 000691540400003

• Kepler's Goat Herd: An exact solution to Kepler's equation for elliptical orbits MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Philcox, O. H. E., Goodman, J., Slepian, Z. 2021; 506 (4): 6111-6116

  View details for DOI 10.1093/mnras/stab1296

  View details for Web of Science ID 000705339100100

• The CAMELS Project: Cosmology and Astrophysics with Machine-learning Simulations ASTROPHYSICAL JOURNAL Villaescusa-Navarro, F., Angles-Alcazar, D., Genel, S., Spergel, D. N., Somerville, R. S., Dave, R., Pillepich, A., Hernquist, L., Nelson, D., Torrey, P., Narayanan, D., Li, Y., Philcox, O., La Torre, V., Delgado, A., Ho, S., Hassan, S., Burkhart, B., Wadekar, D., Battaglia, N., Contardo, G., Bryan, G. L. 2021; 915 (1)

  View details for DOI 10.3847/1538-4357/abf7ba

  View details for Web of Science ID 000670421000001

• Beyond the Yamamoto approximation: Anisotropic power spectra and correlation functions with pairwise lines of sight PHYSICAL REVIEW D Philcox, O. H. E., Slepian, Z. 2021; 103 (12)

  View details for DOI 10.1103/PhysRevD.103.123509

  View details for Web of Science ID 000661800000004

• Cosmology without window functions: Quadratic estimators for the galaxy power spectrum PHYSICAL REVIEW D Philcox, O. H. E. 2021; 103 (10)

  View details for DOI 10.1103/PhysRevD.103.103504

  View details for Web of Science ID 000655874500002

• Modeling galaxies in redshift space at the field level JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS Schmittfull, M., Simonovic, M., Ivanov, M. M., Philcox, O. H. E., Zaldarriaga, M. 2021

  View details for DOI 10.1088/1475-7516/2021/05/059

  View details for Web of Science ID 000654421200039

• Modeling the marked spectrum of matter and biased tracers in real- and redshift-space JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS Philcox, O. H. E., Aviles, A., Massara, E. 2021

  View details for DOI 10.1088/1475-7516/2021/03/038

  View details for Web of Science ID 000636717400033

• Fewer mocks and less noise: Reducing the dimensionality of cosmological observables with subspace projections PHYSICAL REVIEW D Philcox, O. H. E., Ivanov, M. M., Zaldarriaga, M., Simonovic, M., Schmittfull, M. 2021; 103 (4)

  View details for DOI 10.1103/PhysRevD.103.043508

  View details for Web of Science ID 000614624300001

• Determining the Hubble constant without the sound horizon: Measurements from galaxy surveys PHYSICAL REVIEW D Philcox, O. H. E., Sherwin, B. D., Farren, G. S., Baxter, E. J. 2021; 103 (2)

  View details for DOI 10.1103/PhysRevD.103.023538

  View details for Web of Science ID 000613143200002

• A faster Fourier transform? Computing small-scale power spectra and bispectra for cosmological simulations in <i>O</i>(<i>N</i><SUP>2</SUP>) time MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Philcox, O. H. E. 2021; 501 (3): 4004-4034

  View details for DOI 10.1093/mnras/staa3882

  View details for Web of Science ID 000610549500064

• The clustering of the SDSS-IV extended baryon oscillation spectroscopic survey DR16 luminous red galaxy and emission-line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Wang, Y., Zhao, G., Zhao, C., Philcox, O. H. E., Alam, S., Tamone, A., de Mattia, A., Ross, A. J., Raichoor, A., Burtin, E., Paviot, R., de la Torre, S., Percival, W. J., Dawson, K. S., Gil-Marin, H., Bautista, J. E., Hou, J., Koyama, K., Peacock, J. A., Ruhlmann-Kleider, V., des Bourboux, H., Chuang, C., Comparat, J., Escoffier, S., Kneib, J., Mueller, E., Newman, J. A., Rossi, G., Shafieloo, A., Schneider, D. P. 2020; 498 (3): 3470–83

  View details for DOI 10.1093/mnras/staa2593

  View details for Web of Science ID 000587752500030

• Nonlinear perturbation theory extension of the Boltzmann code CLASS PHYSICAL REVIEW D Chudaykin, A., Ivanov, M. M., Philcox, O. H. E., Simonovic, M. 2020; 102 (6)

  View details for DOI 10.1103/PhysRevD.102.063533

  View details for Web of Science ID 000573183700006

• What does the marked power spectrum measure? Insights from perturbation theory PHYSICAL REVIEW D Philcox, O. H. E., Massara, E., Spergel, D. N. 2020; 102 (4)

  View details for DOI 10.1103/PhysRevD.102.043516

  View details for Web of Science ID 000558593800003

• Effective halo model: Creating a physical and accurate model of the matter power spectrum and cluster counts PHYSICAL REVIEW D Philcox, O. H. E., Spergel, D. N., Villaescusa-Navarro, F. 2020; 101 (12)

  View details for DOI 10.1103/PhysRevD.101.123520

  View details for Web of Science ID 000540912900005

• Combining full-shape and BAO analyses of galaxy power spectra: a 1.6% CMB-independent constraint on <i>H</i>₀ JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS Philcox, O. H. E., Ivanov, M. M., Simonovic, M., Zaldarriaga, M. 2020

  View details for DOI 10.1088/1475-7516/2020/05/032

  View details for Web of Science ID 000535391600033

• Computing the small-scale galaxy power spectrum and bispectrum in configuration space MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Philcox, O. H. E., Eisenstein, D. J. 2020; 492 (1): 1214-1242

  View details for DOI 10.1093/mnras/stz3335

  View details for Web of Science ID 000512329900095

• RASCALC: a jackknife approach to estimating single- and multitracer galaxy covariance matrices MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Philcox, O. H. E., Eisenstein, D. J., O'Conne, R., Wiegand, A. 2020; 491 (3): 3290-3317

  View details for DOI 10.1093/mnras/stz3218

  View details for Web of Science ID 000512306500016

• Inferring Galactic Parameters from Chemical Abundances: A Multi-star Approach ASTROPHYSICAL JOURNAL Philcox, O. H. E., Rybizki, J. 2019; 887 (1)

  View details for DOI 10.3847/1538-4357/ab5186

  View details for Web of Science ID 000506001500009

• Estimating covariance matrices for two- and three-point correlation function moments in Arbitrary Survey Geometries MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Philcox, O. H. E., Eisenstein, D. J. 2019; 490 (4): 5931-5951

  View details for DOI 10.1093/mnras/stz2896

  View details for Web of Science ID 000504000300109

• Detection and removal of B-mode dust foregrounds with signatures of statistical anisotropy MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Philcox, O. H. E., Sherwin, B. D., van Engelen, A. 2018; 479 (4): 5577-5595

  View details for DOI 10.1093/mnras/sty1769

  View details for Web of Science ID 000441383700092

• On the Optimal Choice of Nucleosynthetic Yields, Initial Mass Function, and Number of SNe Ia for Chemical Evolution Modeling ASTROPHYSICAL JOURNAL Philcox, O., Rybizki, J., Gutcke, T. A. 2018; 861 (1)

  View details for DOI 10.3847/1538-4357/aac6e4

  View details for Web of Science ID 000436925600004