Primordial non-Gaussianity with $\mu$-type and $y$-type spectral distortions: exploiting Cosmic Microwave Background polarization and dealing with secondary sources

R. Mehrem, J. T. Londergan, and M. H. Macfarlane, Analytic expressions for integrals of products of spherical bessel functions

1991

Earlier work this paper cites.

PhD thesis, UC, Berkeley, 1995

W. T. Hu, Wandering in the Background: A CMB Explorer · 1995

Earlier work this paper cites.

A. Cooray, Integrated sachs-wolfe effect: Large scale structure correlation

2002

Earlier work this paper cites.

E. Komatsu and U. Seljak, The Sunyaev-Zel’dovich angular power spectrum as a probe of cosmological parameters

2002

Earlier work this paper cites.

M. Liguori, S. Matarrese, and L. Moscardini, High-resolution simulations of cosmic microwave background non-gaussian maps in spherical coordinates

2003

Earlier work this paper cites.

N. Bartolo, S. Matarrese, and A. Riotto, On nonGaussianity in the curvaton scenario

2004

Earlier work this paper cites.

N. Dalal, O. Dore, D. Huterer, and A. Shirokov, The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects

Original

2008

Earlier work this paper cites.

S. Matarrese and L. Verde, The effect of primordial non-Gaussianity on halo bias

Original

2008

Earlier work this paper cites.

J. L. Tinker, A. V. Kravtsov, A. Klypin, et al., Toward a halo mass function for precision cosmology: The Limits of universality

Original

2008

Earlier work this paper cites.

J. L. Tinker, B. E. Robertson, A. V. Kravtsov, et al., The Large-scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Original

2010

Earlier work this paper cites.

C. T. Byrnes, M. Gerstenlauer, S. Nurmi, G. Tasinato, and D. Wands, Scale-dependent non-Gaussianity probes inflationary physics

Original

2010

Earlier work this paper cites.

N. Taburet, C. Hernández-Monteagudo, N. Aghanim, M. Douspis, and R. A. Sunyaev, The ISW-tSZ cross-correlation: integrated Sachs-Wolfe extraction out of pure cosmic microwave background data

Original

2011

Earlier work this paper cites.

E. Pajer and M. Zaldarriaga, A New Window on Primordial non-Gaussianity

Original

2012

Earlier work this paper cites.

J. Ganc and E. Komatsu, Scale-dependent bias of galaxies and mu-type distortion of the cosmic microwave background spectrum from single-field inflation with a modified initial state

Original

2012

Cited alongside, same era.

N. Battaglia, J. R. Bond, C. Pfrommer, and J. L. Sievers, On the Cluster Physics of Sunyaev-Zel’dovich Surveys II: Deconstructing the Thermal SZ Power Spectrum

Original

2012

Cited alongside, same era.

A. Becker and D. Huterer, First constraints on the running of non-Gaussianity

Original

2012

Cited alongside, same era.

M. Biagetti, H. Perrier, A. Riotto, and V. Desjacques, Testing the running of non-Gaussianity through the CMB μ \mu -distortion and the halo bias

Original

2013

Cited alongside, same era.

G. W. Pettinari, C. Fidler, R. Crittenden, K. Koyama, and D. Wands, The intrinsic bispectrum of the cosmic microwave background

J. C. Hill and D. N. Spergel, Detection of thermal SZ-CMB lensing cross-correlation in Planck nominal mission data

Original

2014

Later among the works it cites.

L. Van Waerbeke, G. Hinshaw, and N. Murray, Detection of warm and diffuse baryons in large scale structure from the cross-correlation of gravitational lensing and the thermal Sunyaev-Zeldovich effect

Original

2014

Later among the works it cites.

A. Ota, T. Sekiguchi, Y. Tada, and S. Yokoyama, Anisotropic CMB distortions from non-Gaussian isocurvature perturbations

Original

2015

Later among the works it cites.

M. Shiraishi, M. Liguori, N. Bartolo, and S. Matarrese, Measuring primordial anisotropic correlators with CMB spectral distortions

Original

2015

Later among the works it cites.

R. Emami, E. Dimastrogiovanni, J. Chluba, and M. Kamionkowski, Probing the scale dependence of non-Gaussianity with spectral distortions of the cosmic microwave background