Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg SPT-SZ and Planck Gravitational Lensing Map
arXiv:1712.07541 · doi:10.3847/1538-4357/aac264
Abstract
We report constraints on cosmological parameters from the angular power spectrum of a cosmic microwave background (CMB) gravitational lensing potential map created using temperature data from 2500 deg of South Pole Telescope (SPT) data supplemented with data from Planck in the same sky region, with the statistical power in the combined map primarily from the SPT data. We fit the corresponding lensing angular power spectrum to a model including cold dark matter and a cosmological constant (CDM), and to models with single-parameter extensions to CDM. We find constraints that are comparable to and consistent with constraints found using the full-sky Planck CMB lensing data. Specifically, we find from the lensing data alone with relatively weak priors placed on the other CDM parameters. In combination with primary CMB data from Planck, we explore single-parameter extensions to the CDM model. We find or eV both at 95% confidence, all in good agreement with results that include the lensing potential as measured by Planck over the full sky. We include two independent free parameters that scale the effect of lensing on the CMB: , which scales the lensing power spectrum in both the lens reconstruction power and in the smearing of the acoustic peaks, and , which scales only the amplitude of the CMB lensing reconstruction power spectrum. We find for the lensing map made from combined SPT and Planck temperature data, indicating that the amount of lensing is in excellent agreement with what is expected from the observed CMB angular power spectrum when not including the information from smearing of the acoustic peaks.
12 pages, 7 figures, submitted to ApJ, typo in bandpower table corrected
References in corpus (4)
Cited by in corpus (23)
- Planck 2018 results. VIII. Gravitational lensing
- Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies
- Dark Energy Survey Year 1 Results: Constraints on Intrinsic Alignments and their Colour Dependence from Galaxy Clustering and Weak Lensing
- First Cosmological Constraint on the Effective Theory of Dark Matter-Proton Interactions
- Constraints on Cosmological Parameters from the 500 deg SPTpol Lensing Power Spectrum
- A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
- Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
- CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
- On the effect of non-Gaussian lensing deflections on CMB lensing measurements
- Maps of the Southern Millimeter-wave Sky from Combined 2500 deg SPT-SZ and Planck Temperature Data
- Microwave Spectro-Polarimetry of Matter and Radiation across Space and Time
- Planck residuals anomaly as a fingerprint of alternative scenarios to inflation
- Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
- Lensing power spectrum of the Cosmic Microwave Background with deep polarization experiments
- Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
- Deconstructing the Planck TT Power Spectrum to Constrain Deviations from CDM
- Lensing covariance on cut sky and SPT-Planck lensing tensions
- How much primordial tensor mode is allowed?
- Sourced fluctuations in generic slow contraction
- Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
- Detecting deviations from Gaussianity in high-redshift CMB lensing maps
- Understanding CMB physics through the exploration of exotic cosmological models: a classroom study using CLASS
- Constraining Power of Wavelet vs. Power Spectrum Statistics for CMB Lensing and Weak Lensing with Learned Binning