Exploiting the full potential of photometric quasar surveys: Optimal power spectra through blind mitigation of systematics
Boris Leistedt, Hiranya V. Peiris

TL;DR
This paper introduces a new blind mode projection technique to optimally measure the angular power spectrum of photometric quasars, effectively mitigating systematics and enabling precise cosmological analyses.
Contribution
The authors develop an extended mode projection framework that robustly removes multiple systematics from power spectrum measurements in a blind manner.
Findings
Power spectra agree with theoretical models.
No significant residual systematics detected.
Method reduces need for aggressive data cuts.
Abstract
We present optimal measurements of the angular power spectrum of the XDQSOz catalogue of photometric quasars from the Sloan Digital Sky Survey. These measurements rely on a quadratic maximum likelihood estimator that simultaneously measures the auto- and cross-power spectra of four redshift samples, and provides minimum-variance, unbiased estimates even at the largest angular scales. Since photometric quasars are known to be strongly affected by systematics such as spatially-varying depth and stellar contamination, we introduce a new framework of extended mode projection to robustly mitigate the impact of systematics on the power spectrum measurements. This technique involves constructing template maps of potential systematics, decorrelating them on the sky, and projecting out modes which are significantly correlated with the data. Our method is able to simultaneously process several…
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