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Using the most recent releases of WISE and Planck data, we perform updatedmeasurements of the bias and typical dark matter halo mass of infrared-selectedobscured and unobscured quasars, using the angular autocorrelation function andcosmic microwave background (CMB) lensing cross-correlations. Since our recentwork of this kind, the WISE Allwise catalogue was released with improvedphotometry, and the Planck mission was completed and released improvedproducts. These new data provide a more reliable measurement of the quasar biasand provide an opportunity to explore the role of changing survey pipelines inresults downstream. We present a comparison of IR color-selected quasars, splitinto obscured and unobscured populations based on optical-IR colors, selectedfrom two versions of the WISE data. Which combination of data is used impactsthe final results, particularly for obscured quasars, both because ofmitigation of some systematics and because the newer catalogue provides aslightly different sample. We show that Allwise data is superior in severalways, though there may be some systematic trends with Moon contamination thatwere not present in the previous catalogue. We opt currently for the mostconservative sample that meet our selection criteria in both the previous andnew WISE catalogues. We measure a higher bias and halo mass for obscuredquasars ($b_{\textrm{obsc}} \sim 2.1$, $b_{\textrm{unob}} \sim 1.8$) --- atodds with simple orientation models --- but at a reduced significance($\sim$1.5$\sigma$) as compared to our work with previous survey data.

Updated measurements of the dark matter halo masses of obscured quasars with improved WISE and Planck data