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2017

Unbiased clustering estimation in the presence of missing observations

Bianchi, Davide, Percival, Will J.

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In order to be efficient, spectroscopic galaxy redshift surveys do not obtain redshifts for all galaxies in the population targeted.

The missing galaxies are often clustered, commonly leading to a lower proportion of successful observations in dense regions.
One example is the close-pair issue for SDSS spectroscopic galaxy surveys, which have a deficit of pairs of observed galaxies with angular separation closer than the hardware limit on placing neighbouring fibers.
Spatially clustered missing observations will exist in the next generations of surveys.

Unbiased clustering estimation in the presence of missing observations · Around

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