@article{10902/4844,
year = {2014},
month = {2},
url = {http://hdl.handle.net/10902/4844},
abstract = {We present initial results from the Jubilee Integrated Sachs-Wolfe (ISW) project, which models the expected Λ cold dark matter ISW effect in the Jubilee simulation. The simulation volume is (6 h−1 Gpc)3, allowing power on very large scales to be incorporated into the calculation. Haloes are resolved down to a mass of 1.5 × 1012 h−1 M⊙, which allows us to derive a catalogue of mock Luminous Red Galaxies (LRGs) for cross-correlation analysis with the ISW signal. We find the ISW effect observed on a projected sky to grow stronger at late times with the evolution of the ISW power spectrum matching expectations from linear theory. Maps of the gravitational-lensing effect are calculated using the same potential as for the ISW. We calculate the redshift dependence of the ISW–LRG cross-correlation signal for a full-sky survey with no noise considerations. For ℓ < 30, the signal is strongest for lower redshift bins (z ∼ 0.2–0.5), whereas for ℓ > 30, the signal is best observed with surveys covering z ∼ 0.6–1.0.},
publisher = {Oxford University Press},
publisher = {Royal Astronomical Society},
publisher = {Monthly Notices of the Royal Astronomical Society, vol. 438, iss.1, Pp.412-425 (2014)},
title = {The Jubilee ISW project – I. Simulated ISW and weak lensing maps and initial power spectra results},
author = {Watson, W. A. and Diego Rodríguez, José María and Gottlöber, S. and Iliev, I. T. and Knebe, A. and Martínez González, Enrique and Yepes, G. and Barreiro Vilas, Rita Belén and González Nuevo, Joaquín and Hotchkiss, S. and Marcos Caballero, Airam Eduardo and Nadathur, S. and Vielva Martínez, Patricio},
}