{"article_type":"original","date_published":"2016-11-02T00:00:00Z","language":[{"iso":"eng"}],"issue":"10","day":"02","status":"public","main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1608.03169"}],"date_created":"2024-09-06T07:47:04Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","author":[{"full_name":"Liu, Jia","first_name":"Jia","last_name":"Liu"},{"last_name":"Hill","full_name":"Hill, J. Colin","first_name":"J. Colin"},{"first_name":"Blake D.","full_name":"Sherwin, Blake D.","last_name":"Sherwin"},{"first_name":"Andrea","full_name":"Petri, Andrea","last_name":"Petri"},{"last_name":"Böhm","first_name":"Vanessa","full_name":"Böhm, Vanessa"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán","full_name":"Haiman, Zoltán"}],"publisher":"American Physical Society","type":"journal_article","oa_version":"Preprint","citation":{"apa":"Liu, J., Hill, J. C., Sherwin, B. D., Petri, A., Böhm, V., &#38; Haiman, Z. (2016). CMB lensing beyond the power spectrum: Cosmological constraints from the one-point probability distribution function and peak counts. <i>Physical Review D</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevd.94.103501\">https://doi.org/10.1103/physrevd.94.103501</a>","chicago":"Liu, Jia, J. Colin Hill, Blake D. Sherwin, Andrea Petri, Vanessa Böhm, and Zoltán Haiman. “CMB Lensing beyond the Power Spectrum: Cosmological Constraints from the One-Point Probability Distribution Function and Peak Counts.” <i>Physical Review D</i>. American Physical Society, 2016. <a href=\"https://doi.org/10.1103/physrevd.94.103501\">https://doi.org/10.1103/physrevd.94.103501</a>.","short":"J. Liu, J.C. Hill, B.D. Sherwin, A. Petri, V. Böhm, Z. Haiman, Physical Review D 94 (2016).","ama":"Liu J, Hill JC, Sherwin BD, Petri A, Böhm V, Haiman Z. CMB lensing beyond the power spectrum: Cosmological constraints from the one-point probability distribution function and peak counts. <i>Physical Review D</i>. 2016;94(10). doi:<a href=\"https://doi.org/10.1103/physrevd.94.103501\">10.1103/physrevd.94.103501</a>","ieee":"J. Liu, J. C. Hill, B. D. Sherwin, A. Petri, V. Böhm, and Z. Haiman, “CMB lensing beyond the power spectrum: Cosmological constraints from the one-point probability distribution function and peak counts,” <i>Physical Review D</i>, vol. 94, no. 10. American Physical Society, 2016.","ista":"Liu J, Hill JC, Sherwin BD, Petri A, Böhm V, Haiman Z. 2016. CMB lensing beyond the power spectrum: Cosmological constraints from the one-point probability distribution function and peak counts. Physical Review D. 94(10), 103501.","mla":"Liu, Jia, et al. “CMB Lensing beyond the Power Spectrum: Cosmological Constraints from the One-Point Probability Distribution Function and Peak Counts.” <i>Physical Review D</i>, vol. 94, no. 10, 103501, American Physical Society, 2016, doi:<a href=\"https://doi.org/10.1103/physrevd.94.103501\">10.1103/physrevd.94.103501</a>."},"date_updated":"2024-09-25T08:01:19Z","article_number":"103501","publication_identifier":{"issn":["2470-0010","2470-0029"]},"year":"2016","publication":"Physical Review D","doi":"10.1103/physrevd.94.103501","quality_controlled":"1","scopus_import":"1","month":"11","oa":1,"title":"CMB lensing beyond the power spectrum: Cosmological constraints from the one-point probability distribution function and peak counts","volume":94,"_id":"17669","extern":"1","article_processing_charge":"No","publication_status":"published","abstract":[{"lang":"eng","text":"Unprecedentedly precise cosmic microwave background (CMB) data are expected from ongoing and near-future CMB Stage-III and IV surveys, which will yield reconstructed CMB lensing maps with effective resolution approaching several arcminutes. The small-scale CMB lensing fluctuations receive non-negligible contributions from nonlinear structure in the late-time density field. These fluctuations are not fully characterized by traditional two-point statistics, such as the power spectrum. Here, we use N-body ray-tracing simulations of CMB lensing maps to examine two higher-order statistics: the lensing convergence one-point probability distribution function (PDF) and peak counts. We show that these statistics contain significant information not captured by the two-point function, and provide specific forecasts for the ongoing Stage-III Advanced Atacama Cosmology Telescope (AdvACT) experiment. Considering only the temperature-based reconstruction estimator, we forecast 9σ (PDF) and 6σ (peaks) detections of these statistics with AdvACT. Our simulation pipeline fully accounts for the non-Gaussianity of the lensing reconstruction noise, which is significant and cannot be neglected. Combining the power spectrum, PDF, and peak counts for AdvACT will tighten cosmological constraints in the Ωm-σ8 plane by ≈30%, compared to using the power spectrum alone."}],"external_id":{"arxiv":["1608.03169"]},"intvolume":"        94"}