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Galaxy power-spectrum responses and redshift-space super-sample effect · Around

2017

Galaxy power-spectrum responses and redshift-space super-sample effect

Li, Yin, Schmittfull, Marcel, Seljak, Uroš

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Understand

As a major source of cosmological information, galaxy clustering is susceptible to long-wavelength density and tidal fluctuations.

These long modes modulate the growth and expansion rate of local structures, shifting them in both amplitude and scale.
These effects are often named the growth and dilation effects, respectively.
In particular the dilation shifts the baryon acoustic oscillation (BAO) peak and breaks the assumption of the Alcock-Paczynski (AP) test.

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