Evidence for a sign change of the ISW effect in the very recent Universe? Hot voids and cold overdensities at z < 0.03

Open Access

Fig. A.5.

Maximum detection level (calculated as in Figure 8) for void temperatures measured in norther galactic hemisphere only (upper left), southern galactic hemisphere only (upper right), lower redshift shell z < 0.02 only (lower left) and higher redshift shell 0.02 < z < 0.03 only (lower right).

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