Baryonic acoustic oscillations from 21 cm intensity mapping: the Square Kilometre Array case by Villaescusa-Navarro, F, Alonso, D, Viel, M

The H I content of dark matter haloes at z ≈ 0 from ALFALFA by Obuljen, A, Alonso, D, Villaescusa-Navarro, F, Yoon, I, Jones, M

Cross-correlating 21cm intensity maps with Lyman Break Galaxies in the post-reionization era by Villaescusa-Navarro, F, Viel, M, Alonso, D, Datta, K, Bull, P, Santos, M

Lensing is low: Cosmology, galaxy formation, or new physics? by Leauthaud, A, Saito, S, Hilbert, S, Barreira, A, More, S, White, M, Alam, S, Behroozi, P, Bundy, K, Coupon, J, Erben, T, Heymans, C, Hildebrandt, H, Mandelbaum, R, Miller, L, Moraes, B, Pereira, M, Rodriguez-Torres, S, Schmidt, F, Shan, H, Viel, M, Villaescusa-Navarro, F

Beyond ΛCDM: Problems,solutions,and the road ahead by Bull, P, Akrami, Y, Adamek, J, Baker, T, Jiménez, J, Bentivegna, E, Camera, S, Clesse, S, Davis, JH, Di Dio, E, Enander, J, Heavens, A, Heisenberg, L, Hu, B, Llinares, C, Maartens, R, Mörtsell, E, Nadathur, S, Noller, J, Pasechnik, R, Pawlowski, MS, Pereira, TS, Quartin, M, Ricciardone, A, Riemer-Sørensen, S, Rinaldi, M, Sakstein, J, Saltas, ID, Salzano, V, Sawicki, I, Solomon, AR, Spolyar, D, Starkman, GD, Steer, D, Tereno, I, Verde, L, Villaescusa-Navarro, F, Von Strauss, M, Winther, HA

Cosmology with Phase 1 of the Square Kilometre Array Red Book 2018: technical specifications and performance forecasts by Bacon, DJ, Battye, RA, Bull, P, Camera, S, Ferreira, PG, Harrison, I, Parkinson, D, Pourtsidou, A, Santos, MG, Wolz, L, Abdalla, F, Akrami, Y, Alonso, D, Andrianomena, S, Ballardini, M, Bernal, JL, Bertacca, D, Bengaly, CAP, Bonaldi, A, Bonvin, C, Brown, ML, Chapman, E, Chen, S, Chen, X, Cunnington, S, Davis, TM, Dickinson, C, Fonseca, J, Grainge, K, Harper, S, Jarvis, MJ, Maartens, R, Maddox, N, Padmanabhan, H, Pritchard, JR, Raccanelli, A, Rivi, M, Roychowdhury, S, Sahlen, M, Schwarz, DJ, Siewert, TM, Viel, M, Villaescusa-Navarro, F, Xu, Y, Yamauchi, D, Zuntz, J, Square Kilometre Array Cosmology Science Working Group