Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
Abstract
We present measurements of EG, a probe of gravity from large-scale structure, using BOSS LOWZ and CMASS spectroscopic samples, with lensing measurements from SDSS (galaxy lensing) and Planck (CMB lensing). Using SDSS lensing and the BOSS LOWZ sample, we measure (stat), ±0.026 (systematic), consistent with the predicted value from the Planck ΛCDM model, EG=0.46. Using CMB lensing, we measure (stat) for LOWZ (statistically consistent with galaxy lensing and Planck predictions) and (stat) for the CMASS sample, consistent with the Planck prediction of EG=0.40 given the higher redshift of the sample. We also study the redshift evolution of EG by splitting the LOWZ sample into two samples based on redshift, with results being consistent with model predictions. We estimate systematic uncertainties on the above $$\langle$$EG$$\rangle$$ numbers to be ~6% (when using galaxy-galaxy lensing) or ~3% (when using CMB lensing), subdominant to the quoted statistical errors. These systematic error budgets are dominated by observational systematics in galaxy-galaxy lensing and by theoretical modeling uncertainties, respectively. We do not estimate observational systematics in galaxy-CMB lensing cros-correlations.
- Authors:
-
- Carnegie Mellon Univ., Pittsburgh, PA (United States). McWilliams Center for Cosmology; Univ. of California, Berkeley, CA (United States). Berkeley Center for Cosmological Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. of Edinburgh, Scotland (United Kingdom). The Royal Observatory
- Carnegie Mellon Univ., Pittsburgh, PA (United States). McWilliams Center for Cosmology
- Univ. of California, Berkeley, CA (United States). Berkeley Center for Cosmological Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. Autonoma de Madrid (UAM), Cantoblanco, Madrid (Spain). Inst. de Fisica Teorica
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States). Berkeley Center for Cosmological Physics; Carnegie Mellon Univ., Pittsburgh, PA (United States). McWilliams Center for Cosmology
- Publication Date:
- Research Org.:
- Carnegie Mellon Univ., Pittsburgh, PA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); European Research Council (ERC); Carnegie Mellon University; Alfred P. Sloan Foundation; National Science Foundation (NSF)
- OSTI Identifier:
- 1755662
- Grant/Contract Number:
- SC0010118; 670193
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 482; Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; gravitational lensing: weak; large-scale structure of Universe; cosmology: observations
Citation Formats
Singh, Sukhdeep, Alam, Shadab, Mandelbaum, Rachel, Seljak, Uroš, Rodriguez-Torres, Sergio, and Ho, Shirley. Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy. United States: N. p., 2018.
Web. doi:10.1093/mnras/sty2681.
Singh, Sukhdeep, Alam, Shadab, Mandelbaum, Rachel, Seljak, Uroš, Rodriguez-Torres, Sergio, & Ho, Shirley. Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy. United States. https://doi.org/10.1093/mnras/sty2681
Singh, Sukhdeep, Alam, Shadab, Mandelbaum, Rachel, Seljak, Uroš, Rodriguez-Torres, Sergio, and Ho, Shirley. Thu .
"Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy". United States. https://doi.org/10.1093/mnras/sty2681. https://www.osti.gov/servlets/purl/1755662.
@article{osti_1755662,
title = {Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy},
author = {Singh, Sukhdeep and Alam, Shadab and Mandelbaum, Rachel and Seljak, Uroš and Rodriguez-Torres, Sergio and Ho, Shirley},
abstractNote = {We present measurements of EG, a probe of gravity from large-scale structure, using BOSS LOWZ and CMASS spectroscopic samples, with lensing measurements from SDSS (galaxy lensing) and Planck (CMB lensing). Using SDSS lensing and the BOSS LOWZ sample, we measure ⟨ E G ⟩ = 0.40 − 0.04 + 0.05 (stat), ±0.026 (systematic), consistent with the predicted value from the Planck ΛCDM model, EG=0.46. Using CMB lensing, we measure ⟨ E G ⟩ = 0.46 − 0.09 + 0.08 (stat) for LOWZ (statistically consistent with galaxy lensing and Planck predictions) and ⟨ E G ⟩ = 0.39 − 0.05 + 0.05 (stat) for the CMASS sample, consistent with the Planck prediction of EG=0.40 given the higher redshift of the sample. We also study the redshift evolution of EG by splitting the LOWZ sample into two samples based on redshift, with results being consistent with model predictions. We estimate systematic uncertainties on the above $\langle$EG$\rangle$ numbers to be ~6% (when using galaxy-galaxy lensing) or ~3% (when using CMB lensing), subdominant to the quoted statistical errors. These systematic error budgets are dominated by observational systematics in galaxy-galaxy lensing and by theoretical modeling uncertainties, respectively. We do not estimate observational systematics in galaxy-CMB lensing cros-correlations.},
doi = {10.1093/mnras/sty2681},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 482,
place = {United States},
year = {Thu Oct 04 00:00:00 EDT 2018},
month = {Thu Oct 04 00:00:00 EDT 2018}
}
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