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Toshifumi Futamase grad student 2001 Tohoku University
 (The Pursuit of Non-Gaussian Fluctuations in the Cosmic Microwave Background.)
David N. Spergel grad student 2001 Tohoku University (Physics Tree)
 (Co-Supervisor)
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Publications

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Park H, Komatsu E, Shapiro PR, et al. (2016) THE IMPACT OF NONLINEAR STRUCTURE FORMATION ON THE POWER SPECTRUM OF TRANSVERSE MOMENTUM FLUCTUATIONS AND THE KINETIC SUNYAEV-ZEL'DOVICH EFFECT Astrophysical Journal. 818
Jee I, Komatsu E, Suyu SH, et al. (2016) Time-delay cosmography: Increased leverage with angular diameter distances Journal of Cosmology and Astroparticle Physics. 2016
Giannantonio T, Komatsu E. (2015) Bayesian evidence of nonstandard inflation: Isocurvature perturbations and running spectral index Physical Review D - Particles, Fields, Gravitation and Cosmology. 91
Jee I, Komatsu E, Suyu SH. (2015) Measuring angular diameter distances of strong gravitational lenses Journal of Cosmology and Astroparticle Physics. 2015
Chiang CT, Wagner C, Sánchez AG, et al. (2015) Position-dependent correlation function from the SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 10 CMASS sample Journal of Cosmology and Astroparticle Physics. 2015
Wagner C, Schmidt F, Chiang CT, et al. (2015) The angle-averaged squeezed limit of nonlinear matter N-point functions Journal of Cosmology and Astroparticle Physics. 2015
Kunze KE, Komatsu E. (2015) Constraints on primordial magnetic fields from the optical depth of the cosmic microwave background Journal of Cosmology and Astroparticle Physics. 2015
Naruko A, Komatsu E, Yamaguchi M. (2015) Anisotropic inflation reexamined: Upper bound on broken rotational invariance during inflation Journal of Cosmology and Astroparticle Physics. 2015
Ando S, Benoit-Lévy A, Komatsu E. (2014) Mapping dark matter in the gamma-ray sky with galaxy catalogs Physical Review D - Particles, Fields, Gravitation and Cosmology. 90
Shi X, Komatsu E. (2014) Analytical model for non-thermal pressure in galaxy clusters Monthly Notices of the Royal Astronomical Society. 442: 521-532
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