Publications (115)
Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the SDSS: stellar mass, luminosity, morphology, and environment dependencies
Rachel Mandelbaum, Uros Seljak, Guinevere Kauffmann +2
The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey
Patrick McDonald, Uros Seljak, Scott Burles +8
Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
Teppei Okumura, Uros Seljak, Zvonimir Vlah +1
Signatures of First Stars in Galaxy Surveys: Multi-Tracer Analysis of the Supersonic Relative Velocity Effect and the Constraints from the BOSS Power Spectrum Measurements
Jaiyul Yoo, Uros Seljak
Lensing Induced Cluster Signatures in Cosmic Microwave Background
Uros Seljak, Matias Zaldarriaga
Galaxy Bias and non-Linear Structure Formation in General Relativity
Tobias Baldauf, Uros Seljak, Leonardo Senatore +1
Intrinsic alignment-lensing interference as a contaminant of cosmic shear
Christopher M. Hirata, Uros Seljak
Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications
Shirley Ho, Antonio Cuesta, Hee-Jong Seo +37
Cluster Density Profiles as a Test of Modified Gravity
Lucas Lombriser, Fabian Schmidt, Tobias Baldauf +3
Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints
Uros Seljak, Anze Slosar, Patrick McDonald
Galaxy-galaxy weak lensing in SDSS: intrinsic alignments and shear calibration errors
Christopher M. Hirata, Rachel Mandelbaum, Uros Seljak +9
Rees-Sciama Effect in a CDM Universe
Uros Seljak
Simulating Weak Lensing by Clusters and Large-Scale Structure
Bhuvnesh Jain, Uros Seljak, Simon White
Prospects for ACT: simulations, power spectrum, and non-Gaussian analysis
Kevin M. Huffenberger, Uros Seljak
Cluster abundance normalization from observed mass-temperature relation
Uros Seljak
Reconstruction of lensing from the cosmic microwave background polarization
Christopher M. Hirata, Uros Seljak
Galaxy-dark matter correlations applied to galaxy-galaxy lensing: predictions from the semi-analytic galaxy formation models
Jacek Guzik, Uros Seljak
Joint Analysis of Gravitational Lensing, Clustering and Abundance: Toward the Unification of Large-Scale Structure Analysis
Jaiyul Yoo, Uros Seljak
Gravitational lensing as a contaminant of the gravity wave signal in CMB
Uros Seljak, Christopher M. Hirata
Evidence for Quadratic Tidal Tensor Bias from the Halo Bispectrum
Tobias Baldauf, Uros Seljak, Vincent Desjacques +1
A Two-Fluid Approximation for Calculating the Cosmic Microwave Background Anisotropies
Uros Seljak
Sunyaev-Zeldovich effect from hydrodynamical simulations: maps and low order statistics
Uros Seljak, Juan Burwell, Ue-Li Pen
Primordial non-Gaussianity in the Bispectrum of the Halo Density Field
Tobias Baldauf, Uros Seljak, Leonardo Senatore
Shear calibration biases in weak lensing surveys
Christopher M. Hirata, Uros Seljak
Amplitude of Primeval Fluctuations from Cosmological Mass Density Reconstructions
Uros Seljak, Edmund Bertschinger
Optimizing BAO measurements with non-linear transformations of Lyman-alpha forest
Xinkang Wang, Andreu Font-Ribera, Uros Seljak
Redshift space bias and beta from the halo model
Uros Seljak
Large Scale Structure Effects on the Gravitational Lens Image Positions and Time Delay
Uros Seljak
On Estimating the QSO Transmission Power Spectrum
Lam Hui, Scott Burles, Uros Seljak +3
Halo Concentration and the Dark Matter Power Spectrum
Kevin M. Huffenberger, Uros Seljak
Density profiles of galaxy groups and clusters from SDSS galaxy-galaxy weak lensing
Rachel Mandelbaum, Uros Seljak, Richard J. Cool +3
The Scalar, Vector and Tensor Contributions to CMB anisotropies from Cosmic Defects
Neil Turok, Ue-Li Pen, Uros Seljak
GRAVITATIONAL LENSING EFFECT ON COSMIC MICROWAVE BACKGROUND ANISOTROPIES: A POWER SPECTRUM APPROACH
Uros Seljak
Confirmation of general relativity on large scales from weak lensing and galaxy velocities
Reinabelle Reyes, Rachel Mandelbaum, Uros Seljak +4
Correlations in the Lyman alpha forest: testing the gravitational instability paradigm
Matias Zaldarriaga, Uros Seljak, Lam Hui
The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey
III Collaboration, Christopher P. Ahn, Rachael Alexandroff +224
Limits on the Density of Compact Objects from High Redshift Supernovae
Uros Seljak, Daniel E. Holz
Ellipticity of dark matter halos with galaxy-galaxy weak lensing
Rachel Mandelbaum, Christopher M. Hirata, Tamara Broderick +2
Seeing in the dark -- II. Cosmic shear in the Sloan Digital Sky Survey
Eric M. Huff, Tim Eifler, Christopher M. Hirata +3
Cross-correlation of CMB with large-scale structure: weak gravitational lensing
Christopher M. Hirata, Nikhil Padmanabhan, Uros Seljak +2
An All-Sky Analysis of Polarization in the Microwave Background
Matias Zaldarriaga, Uros Seljak
Maximum-Likelihood Analysis of the COBE Angular Correlation Function
Uros Seljak, Edmund Bertschinger
The Shear TEsting Programme 2: Factors affecting high precision weak lensing analyses
Richard Massey, Catherine Heymans, Joel Berge +28
Polarization of Microwave Background: Statistical and Physical Properties
Uros Seljak, Matias Zaldarriaga
Direct Signature of Evolving Gravitational Potential from Cosmic Microwave Background
Uros Seljak, Matias Zaldarriaga
Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
Nico Hamaus, Uros Seljak, Vincent Desjacques
Primordial non-Gaussianity in the large scale structure of the Universe
Vincent Desjacques, Uros Seljak
Weak Lensing Reconstruction and Power Spectrum Estimation: Minimum Variance Methods
Uros Seljak
Measuring primordial non-gaussianity without cosmic variance
Uros Seljak
Going beyond the Kaiser redshift-space distortion formula: a full general relativistic account of the effects and their detectability in galaxy clustering
Jaiyul Yoo, Nico Hamaus, Uros Seljak +1
Detection of large scale intrinsic ellipticity-density correlation from the Sloan Digital Sky Survey and implications for weak lensing surveys
Rachel Mandelbaum, Christopher M. Hirata, Mustapha Ishak +2
A Line of Sight Approach to Cosmic Microwave Background Anisotropies
Uros Seljak, Matias Zaldarriaga
Distribution function approach to redshift space distortions. Part II: N-body simulations
Teppei Okumura, Uros Seljak, Patrick McDonald +1
Impact of Scale Dependent Bias and Nonlinear Structure Growth on the ISW Effect: Angular Power Spectra
Robert E. Smith, Carlos Hernandez-Monteagudo, Uros Seljak
Measuring Dark Matter Power Spectrum from Cosmic Microwave Background
Uros Seljak, Matias Zaldarriaga
Sunyaev-Zeldovich effect in WMAP and its effect on cosmological parameters
Kevin M. Huffenberger, Uros Seljak, Alexey Makarov
Analyzing weak lensing of the cosmic microwave background using the likelihood function
Christopher M. Hirata, Uros Seljak
Primordial non-Gaussianity from the large scale structure
Vincent Desjacques, Uros Seljak
Testing the tidal alignment model of galaxy intrinsic alignment
Jonathan Blazek, Matthew McQuinn, Uros Seljak
Assessing the effects of foregrounds and sky removal in WMAP
Anze Slosar, Uros Seljak
Signature of Gravity Waves in Polarization of the Microwave Background
Uros Seljak, Matias Zaldarriaga
Weak Lensing and CMB: Parameter forecasts including a running spectral index
Mustapha Ishak, Christopher M. Hirata, Patrick McDonald +1
An algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering
Tobias Baldauf, Robert E. Smith, Uros Seljak +1
Cosmography and Power Spectrum Estimation: a Unified Approach
Uros Seljak
21 cm Intensity Mapping
Jeffrey B. Peterson, Roy Aleksan, Reza Ansari +37
Wide Angle Effects in Future Galaxy Surveys
Jaiyul Yoo, Uros Seljak
Numerical Investigations of Weak Lensing by Large-Scale Structure
Bhuvnesh Jain, Uros Seljak, Simon White
Precision cluster mass determination from weak lensing
Rachel Mandelbaum, Uros Seljak, Tobias Baldauf +1
Minimizing the stochasticity of halos in large-scale structure surveys
Nico Hamaus, Uros Seljak, Vincent Desjacques +2
Ray Tracing Simulations of Weak Lensing by Large-Scale Structure
Bhuvnesh Jain, Uros Seljak, Simon White
A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing
Rachel Mandelbaum, Uros Seljak
Measuring Polarization In Cosmic Microwave Background
Uros Seljak
Detectability of tensor modes in the presence of foregrounds
Mihail Amarie, Christopher Hirata, Uros Seljak
Power Spectra in Global Defect Theories of Cosmic Structure Formation
Ue-Li Pen, Uros Seljak, Neil Turok
Correlation of CMB with large-scale structure: II. Weak lensing
Christopher M. Hirata, Shirley Ho, Nikhil Padmanabhan +2
Separating intrinsic alignment and galaxy-galaxy lensing
Jonathan Blazek, Rachel Mandelbaum, Uros Seljak +1
How to measure redshift-space distortions without sample variance
Patrick McDonald, Uros Seljak
Halo mass - concentration relation from weak lensing
Rachel Mandelbaum, Uros Seljak, Christopher M. Hirata
Supersonic Relative Velocity Effect on the Baryonic Acoustic Oscillation Measurements
Jaiyul Yoo, Neal Dalal, Uros Seljak
Systematic errors in weak lensing: application to SDSS galaxy-galaxy weak lensing
Rachel Mandelbaum, Christopher M. Hirata, Uros Seljak +6
CMBFAST for spatially closed universes
Matias Zaldarriaga, Uros Seljak
Bias, redshift space distortions and primordial nongaussianity of nonlinear transformations: application to Lyman alpha forest
Uros Seljak
Constraints on f(R) gravity from probing the large-scale structure
Lucas Lombriser, Anze Slosar, Uros Seljak +1
Cosmological constraints from the CMB and Ly-alpha forest revisited
Uros Seljak, Patrick McDonald, Alexey Makarov
Cosmological Model Predictions for Weak Lensing: Linear and Nonlinear Regimes
Bhuvnesh Jain, Uros Seljak
Can sterile neutrinos be the dark matter?
Uros Seljak, Alexey Makarov, Patrick McDonald +1
Calibrating Photometric Redshifts of Luminous Red Galaxies
Nikhil Padmanabhan, Tamas Budavari, David J. Schlegel +20
Distribution function approach to redshift space distortions
Uros Seljak, Patrick McDonald
Large scale bias and stochasticity of halos and dark matter
Uros Seljak, Michael S. Warren
Lensing effect on polarization in microwave background: extracting convergence power spectrum
Jacek Guzik, Uros Seljak, Matias Zaldarriaga
Can superhorizon cosmological perturbations explain the acceleration of the universe?
Christopher M. Hirata, Uros Seljak
Cosmological Constraints on DGP Braneworld Gravity with Brane Tension
Lucas Lombriser, Wayne Hu, Wenjuan Fang +1
B polarization of cosmic microwave background as a tracer of strings
Uros Seljak, Anze Slosar
Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
Vincent Desjacques, Uros Seljak
Integral Solution for the Microwave Background Anisotropies in Non-fl at Universes
Matias Zaldarriaga, Uros Seljak, Edmund Bertschinger
Galaxy Mass and Luminosity Scaling Laws Determined by Weak Gravitational Lensing
Timothy A. McKay, Erin Scott Sheldon, Judith Racusin +18
Constraining the dark energy with Ly-alpha forest
Uros Seljak, Rachel Mandelbaum, Patrick McDonald
Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
Shirley Ho, Christopher M. Hirata, Nikhil Padmanabhan +2
Polarization of the Microwave Background in Defect Models
Uros Seljak, Ue-Li Pen, Neil Turok
Constraints on local primordial non-Gaussianity from large scale structure
Anze Slosar, Christopher Hirata, Uros Seljak +2