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