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The ISW imprints of voids and superclusters on the CMB

Published online by Cambridge University Press:  12 October 2016

S. Hotchkiss*
Affiliation:
Department of Physics and Astronomy, University of Sussex, Falmer, Brighton, BN1 9QH, UK
S. Nadathur
Affiliation:
Department of Physics, University of Helsinki and Helsinki Institute of Physics, P.O. Box 64, FIN-00014, University of Helsinki, Finland
S. Gottlöber
Affiliation:
Leibniz-Institute for Astrophysics, An der Sternwarte 16, D-14482 Potsdam, Germany
I. T. Iliev
Affiliation:
Department of Physics and Astronomy, University of Sussex, Falmer, Brighton, BN1 9QH, UK
A. Knebe
Affiliation:
Departamento de Física Teórica, Modulo C-XI, Facultad de Ciencias, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, Spain
W. A. Watson
Affiliation:
Department of Physics and Astronomy, University of Sussex, Falmer, Brighton, BN1 9QH, UK
G. Yepes
Affiliation:
Departamento de Física Teórica, Modulo C-XI, Facultad de Ciencias, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, Spain
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Abstract

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We examine the stacked integrated Sachs-Wolfe (ISW) imprints on the CMB along the lines of sight of voids and superclusters in galaxy surveys, using the Jubilee ISW simulation and mock luminous red galaxy (LRG) catalogues. We show that the expected signal in the concordance \Lam CDM model is much smaller than the primary anisotropies arising at the last scattering surface and therefore any currently claimed detections of such an imprint cannot be caused by the ISW effect in \Lam CDM. We look for the existence of such a signal in the Planck CMB using a catalogue of voids and superclusters from the Sloan Digital Sky Survey (SDSS), but find a result completely consistent with \Lam CDM – i.e., a null detection.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Cai, Y.-C., Cole, S., Jenkins, A., & Frenk, C. S., 2010, MNRAS, 407, 201 Google Scholar
Cai, Y.-C., Neyrinck, M. C., Szapudi, I., Cole, S., & Frenk, C. S., 2013, ApJ, 786, 110 Google Scholar
Dunkley, J., et al., 2009, ApJS, 180, 306 CrossRefGoogle Scholar
Flender, S., Hotchkiss, S., & Nadathur, S., 2013, JCAP, 1302, 013 CrossRefGoogle Scholar
Granett, B. R., Neyrinck, M. C., & Szapudi, I., 2008, ApJ, 683, L99 CrossRefGoogle Scholar
Granett, B. R., Neyrinck, M. C., & Szapudi, I., 2009, ApJ, 701, 414 Google Scholar
Hernández-Monteagudo, C. & Smith, R. E., 2013, MNRAS, 435, 1094 Google Scholar
Hotchkiss, S. et al., 2014, MNRAS in press, arXiv:1405.3552Google Scholar
Hunt, P. & Sarkar, S., 2010, MNRAS, 401, 547 Google Scholar
Ilić, S., Langer, M., & Douspis, M., 2013, A&A, 556, A51 Google Scholar
Kazin, E. A. et al., 2010, ApJ, 710, 1444 CrossRefGoogle Scholar
Nadathur, S. & Hotchkiss, S., 2014, MNRAS, 440, 1248 Google Scholar
Nadathur, S., Hotchkiss, S., & Sarkar, S., 2012, JCAP, 1206, 042 CrossRefGoogle Scholar
Neyrinck, M. C., 2008, MNRAS, 386, 2101 Google Scholar
Planck Collaboration et al., 2013b, ArXiv e-prints, 1303.5079Google Scholar
Planck Collaboration et al., 2013a, ArXiv e-prints, 1303.5062Google Scholar
Watson, W. A. et al., 2014, MNRAS, 438, 412 Google Scholar
Zheng, Z., Zehavi, I., Eisenstein, D. J., Weinberg, D. H., & Jing, Y., 2009, ApJ, 707, 554 CrossRefGoogle Scholar