Perturbations of a Cosmological Model and Angular Variations of the Microwave Background
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January 1967
Small scale integrated Sachs-Wolfe effect
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July 1994
A correlation between the cosmic microwave background and large-scale structure in the Universe
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January 2004
Detection of the Integrated Sachs-Wolfe and Sunyaev-Zeldovich Effects from the Cosmic Microwave Background-Galaxy Correlation
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October 2003
First Year Wilkinson Microwave Anisotropy Probe Observations: Dark Energy Induced Correlation with Radio Sources
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Constraining dark energy with cross-correlated CMB and large scale structure data
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Correlating the CMB with luminous red galaxies: The integrated Sachs-Wolfe effect
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August 2005
Cross-correlation of the cosmic microwave background and radio galaxies in real, harmonic and wavelet spaces: detection of the integrated Sachs-Wolfe effect and dark energy constraints
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January 2006
Detection of the integrated Sachs-Wolfe effect and corresponding dark energy constraints made with directional spherical wavelets
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April 2007
High redshift detection of the integrated Sachs-Wolfe effect
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September 2006
Error analysis in cross-correlation of sky maps: application to the Integrated Sachs-Wolfe detection
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November 2007
Cross-correlation of 2MASS and WMAP 3: implications for the integrated Sachs-Wolfe effect
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May 2007
Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
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June 2008
Correlation of CMB with large-scale structure. I. Integrated Sachs-Wolfe tomography and cosmological implications
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August 2008
The high redshift Integrated Sachs-Wolfe effect
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September 2009
The significance of the integrated Sachs-Wolfe effect revisited: The significance of the ISW effect revisited
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October 2012
Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
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October 2014
Planck 2015 results : XXI. The integrated Sachs-Wolfe effect
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September 2016
CMB anomalies after Planck
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August 2016
Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimation
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April 2013
Planck 2015 results : XVII. Constraints on primordial non-Gaussianity
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A Linear Filter to Reconstruct the ISW Effect From CMB and LSS Observations
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October 2008
A map of the Integrated Sachs-Wolfe Signal from Luminous red Galaxies
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July 2009
An estimate of the local integrated Sachs-Wolfe signal and its impact on cosmic microwave background anomalies: The local ISW signal and CMB anomalies
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June 2010
Integrated Sachs-Wolfe effect map recovery from NVSS and WMAP 7-yr data
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January 2013
Removal of two large-scale cosmic microwave background anomalies after subtraction of the integrated Sachs-Wolfe effect
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August 2013
Mapping the integrated Sachs-Wolfe effect
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December 2014
The integrated Sachs–Wolfe signal from BOSS superstructures
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October 2015
Reconstructing the integrated Sachs-Wolfe map with galaxy surveys
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August 2016
On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
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February 2016
Systematic Effects in Large-Scale Angular Power Spectra of Photometric Quasars and Implications for Constraining Primordial Non-Gaussianity
Pullen, Anthony R.; Hirata, Christopher M.
Publications of the Astronomical Society of the Pacific, Vol. 125, Issue 928
https://doi.org/10.1086/671189
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June 2013
Clustering of Sloan Digital sky Survey iii Photometric Luminous Galaxies: the Measurement, Systematics, and Cosmological Implications
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November 2012
Sloan Digital Sky Survey III photometric quasar clustering: probing the initial conditions of the Universe
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May 2015
Constraining the initial conditions of the Universe using large scale structure
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February 2014
Improved primordial non-Gaussianity constraints from measurements of galaxy clustering and the integrated Sachs-Wolfe effect
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January 2014
Characterizing unknown systematics in large scale structure surveys
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April 2014
The SDSS-III Baryonic Oscillation Spectroscopic Survey: constraints on the integrated Sachs–Wolfe effect
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December 2013
Excess Clustering on Large Scales in the MegaZ DR7 Photometric Redshift Survey
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June 2011
Measurement of the angular correlation function of radio galaxies from the NRAO VLA Sky Survey
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January 2002
Revisiting the WMAP-NVSS angular cross correlation. A skeptic's view
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September 2010
Analysis of Systematic Effects and Statistical Uncertainties in Angular Clustering of Galaxies from Early Sloan Digital Sky Survey Data
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November 2002
Ameliorating systematic uncertainties in the angular clustering of galaxies: a study using the SDSS-III: Ameliorating systematic uncertainties in w(θ)
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September 2011
Estimating the large-scale angular power spectrum in the presence of systematics: a case study of Sloan Digital Sky Survey quasars
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September 2013
Exploiting the full potential of photometric quasar surveys: optimal power spectra through blind mitigation of systematics
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August 2014
Unbiased methods for removing systematics from galaxy clustering measurements
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December 2015
Testing lsst Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics
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September 2016
Unbiased pseudo- C ℓ power spectrum estimation with mode projection
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October 2016
No galaxy left behind: accurate measurements with the faintest objects in the Dark Energy Survey
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January 2016
Calibration errors unleashed: effects on cosmological parameters and requirements for large-scale structure surveys
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May 2013
Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
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January 2015
HEALPix: A Framework for High‐Resolution Discretization and Fast Analysis of Data Distributed on the Sphere
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April 2005
Integrated Sachs-Wolfe effect in cross-correlation: The observer's manual
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Optimising large galaxy surveys for ISW detection
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April 2008
Constraining cosmology with shear peak statistics: tomographic analysis
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Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models
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August 2000
Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters
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September 2016
Planck 2015 results : XV. Gravitational lensing
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September 2016
An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
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February 2008
Measuring the integrated Sachs-Wolfe effect
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September 2011
Measuring dark energy clustering with CMB-galaxy correlations
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December 2004
Optimal integrated Sachs-Wolfe detection and joint likelihood for cosmological parameter estimation
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December 2008
Improved dark energy detection through the polarization-assisted cross correlation of the cosmic microwave background with radio sources
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March 2011
Why your model parameter confidences might be too optimistic. Unbiased estimation of the inverse covariance matrix
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December 2006
Putting the precision in precision cosmology: How accurate should your data covariance matrix be?
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May 2013
Constraining dark energy with cross-correlated CMB and Large Scale Structure data
text
January 2005