The Astrophysical Journal, 825:24 (13pp), 2016 July 1 doi:10.3847/0004-637X/825/1/24 © 2016. The American Astronomical Society. All rights reserved. TOWARD A TOMOGRAPHIC ANALYSIS OF THE CROSS-CORRELATION BETWEEN PLANCK CMB LENSING AND H-ATLAS GALAXIES F. Bianchini1,2,3, A. Lapi1,2,3,4, M. Calabrese1,5, P. Bielewicz1,6, J. Gonzalez-Nuevo7, C. Baccigalupi1,2, L. Danese1, G. de Zotti1,8, N. Bourne9, A. Cooray10, L. Dunne9,11,12, S. Eales11, and E. Valiante11 1 Astrophysics Sector, SISSA, Via Bonomea 265, I-34136 Trieste, Italy;
[email protected] 2 INFN—Sezione di Trieste, Via Valerio 2, I-34127 Trieste, Italy 3 INAF—Osservatorio Astronomico di Trieste, via Tiepolo 11, I-34131, Trieste, Italy 4 Dipartimento di Fisica, Università “Tor Vergata,” Via della Ricerca Scientifica 1, I-00133 Roma, Italy 5 INAF, Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 (LC), Italy 6 Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland 7 Departamento de Física, Universidad de Oviedo, C. Calvo Sotelo s/n, E-33007 Oviedo, Spain 8 INAF—Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy 9 Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK 10 Department of Physics and Astronomy, University of California, Irvine CA 92697, USA 11 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, UK 12 Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, 8140, New Zealand Received 2015 November 16; revised 2016 April 28; accepted 2016 April 29; published 2016 June 27 ABSTRACT We present an improved and extended analysis of the cross-correlation between the map of the cosmic microwave background (CMB) lensing potential derived from the Planck mission data and the high-redshift galaxies detected by the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) in the photometric redshift range zph 1.5.