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- W3094691796 abstract "We study the cross correlation of damped Ly$alpha$ systems (DLAs) and their background quasars, using the most updated DLA catalog and the Planck 2018 CMB lensing convergence field. Our measurement suggests that the DLA bias $b_{rm DLA}$ is smaller than $3.1$, corresponding to $log(M/M_odot h^{-1})leq 12.3$ at a confidence of $90%$. These constraints are broadly consistent with Alonso et al. (2018) and previous measurements by cross-correlation between DLAs and the Ly$alpha$ forest (e.g. Font-Ribera et al. 2012; Perez-Rafols et al. 2018). Further, our results demonstrate the potential of obtaining a more precise measurement of the halo mass of high-redshift sources using next generation CMB experiments with a higher angular resolution. The python-based codes and data products of our analysis are available at https://github.com/LittleLin1999/CMB-lensingxDLA." @default.
- W3094691796 created "2020-11-09" @default.
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- W3094691796 date "2020-12-28" @default.
- W3094691796 modified "2023-10-16" @default.
- W3094691796 title "Constraining the Halo Mass of Damped Ly<i>α</i> Absorption Systems (DLAs) at <i>z</i> = 2–3.5 Using the Quasar-CMB Lensing Cross-correlation" @default.
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- W3094691796 doi "https://doi.org/10.3847/1538-4357/abc620" @default.
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