The catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST by Prat, J, Zuntz, J, Chang, C, Tröster, T, Pedersen, E, García-García, C, Phillips-Longley, E, Sanchez, J, Alonso, D, Fang, X, Gawiser, E, Heitmann, K, Ishak, M, Jarvis, M, Kovacs, E, Larsen, P, Mao, Y-Y, Medina Varela, L, Paterno, M, Vitenti, SD, Zhang, Z

Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release by Nicola, A, Alonso, D, Sánchez, J, Slosar, A, Awan, H, Broussard, A, Dunkley, J, Gawiser, E, Gomes, Z, Mandelbaum, R, Miyatake, H, Newman, JA, Sevilla, I, Skinner, S, Wagoner, E

“…In terms of photometric redshift systematics, we show that additional care is needed in order to marginalize over uncertainties in the redshift distribution in galaxy clustering, even for samples of this small size, and that these uncertainties can be significantly constrained by including cross-bin correlations. …”

Reconstructing cosmic growth with kinetic Sunyaev-Zel’dovich observations in the era of stage IV experiments by Alonso, D, Louis, T, Bull, P, Ferreira, P

“…We describe a method for constraining the growth rate of structure to sub-1% precision out to z≈1, using a combination of galaxy cluster peculiar velocities measured using the kinetic Sunyaev-Zel'dovich (kSZ) effect, and the velocity field reconstructed from galaxy redshift surveys. …”

Galaxy bias in the era of LSST: perturbative bias expansions by Nicola, A, Hadzhiyska, B, Findlay, N, García-García, C, Alonso, D, Slosar, A, Guo, Z, Kokron, N, Angulo, R, Aviles, A, Blazek, J, Dunkley, J, Jain, B, Pellejero, M, Sullivan, J, Walter, CW, Zennaro, M

“…We consider a variety of different simulated galaxy samples and test the performance of the bias models in a tomographic joint analysis of LSST-Y10-like galaxy clustering, galaxy-galaxy-lensing and cosmic shear. …”

Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses by Mahony, C, Fortuna, MC, Joachimi, B, Korn, A, Hoekstra, H, Schmidt, SJ, Alonso, D, Singh, S, Ricci, M, Hildebrandt, H, Duncan, C, Johnston, H

“…In particular, we find that for the LSST gold sample (i < 25.3) including weak lensing magnification only improves the galaxy clustering constraint on.…”

Hefty enhancement of cosmological constraints from the DES Y1 data using a hybrid effective field theory approach to galaxy bias by Hadzhiyska, B, García-García, C, Alonso, D, Nicola, A, Slosar, A

“…We find that this model can explain the galaxy clustering and shear data up to wavenumbers k_max∼ 0.6 Mpc^-1. …”

Science-driven 3D data compression by Alonso, D

“…We apply this method to both weak lensing and galaxy clustering. In the case of galaxy clustering, we show that the resulting optimal basis is closely associated with the Fourier–Bessel basis, and that for certain observables, such as the effects of magnification bias or primordial non-Gaussianity, the bulk of the signal can be compressed into a small number of modes. …”

The impact of relativistic effects on cosmological parameter estimation by Lorenz, C, Alonso, D, Ferreira, P

“…In particular, we look at the magnification lensing contribution to galaxy clustering and general relativistic corrections to all observables. …”

LimberJack.jl: auto-differentiable methods for angular power spectra analyses by Ruiz-Zapatero, J, Alonso, D, García-García, C, Nicola, A, Mootoovaloo, A, Sullivan, JM, Bonici, M, Ferreira, PG

“…We present LimberJack.jl, a fully auto-differentiable code for cosmological analyses of 2 point auto- and cross-correlation measurements from galaxy clustering, CMB lensing and weak lensing data written in Julia. …”

Analytic marginalization of N(z) uncertainties in tomographic galaxy surveys by Hadzhiyska, B, Alonso, D, Nicola, A, Slosar, A

“…We showcase this method by applying it to the galaxy clustering measurements from the Hyper Suprime-Cam first data release. …”

Neutrino masses and beyond-ΛCDM cosmology with LSST and future CMB experiments by Mishra-Sharma, S, Alonso, D, Dunkley, J

“…We show how future CMB measurements can be combined with late-time measurements of galaxy clustering and cosmic shear from the Large Synoptic Survey Telescope to alleviate this degeneracy. …”

α-attractor dark energy in view of next-generation cosmological surveys by García-García, C, Ruíz-Lapuente, P, Alonso, D, Zumalacárregui, M

“…We systematically account for the constraining power of SNIa from WFIRST, BAO from DESI and WFIRST, galaxy clustering and shear from LSST and Stage-4 CMB experiments. …”

Core Cosmology Library: Precision cosmological predictions for LSST by Chisari, N, Alonso, D, Krause, E, Leonard, C, Bull, P, Neveu, J, Villarreal, A, Singh, S, McClintock, T, Ellison, J, Du, Z, Zuntz, J, Mead, A, Joudaki, S, Lorenz, C, Tröster, T, Sanchez, J, Lanusse, F, Ishak, M, Hlozek, R, Blazek, J, Campagne, J, Almoubayyed, H, Eifler, T, Kirby, M, Kirkby, D, Plaszczynski, S, Slosar, A, Vrastil, M, Wagoner, E

“…As a result, predictions for correlation functions of galaxy clustering, galaxy–galaxy lensing, and cosmic shear are demonstrated to be within a fraction of the expected statistical uncertainty of the observables for the models and in the range of scales of interest to LSST. …”

The growth of density perturbations in the last ∼10 billion years from tomographic large-scale structure data by Garcia-Garcia, C, Ruiz Zapatero, J, Alonso, D, Bellini, E, Ferreira, P, Mueller, E, Nicola, A, Ruiz-Lapuente, P

“…To do so, we decouple the linear growth of density inhomogeneities from the background expansion, and constrain its redshift dependence making use of a combination of 6 different data sets, including cosmic shear, galaxy clustering and CMB lensing. We analyze these data under a consistent harmonic-space angular power spectrum-based pipeline. …”

Disconnected pseudo-Cℓ covariances for projected large-scale structure data by García-García, C, Alonso, D, Bellini, E

“…The disconnected part of the power spectrum covariance matrix (also known as the "Gaussian" covariance) is the dominant contribution on large scales for galaxy clustering and weak lensing datasets. The presence of a complicated sky mask causes non-trivial correlations between different Fourier/harmonic modes, which must be accurately characterized in order to obtain reliable cosmological constraints. …”

Constraining cosmology with the Gaia-unWISE Quasar Catalog and CMB lensing: structure growth by Alonso, D, Fabbian, G, Storey-Fisher, K, Eilers, A-C, Garcia-Garcia, C, Hogg, D, Rix, HW

“…Our constraints are competitive with those from state-of-the-art 3×2-point analyses, but arise from a range of scales and redshifts that is highly complementary to those covered by cosmic shear data and most galaxy clustering samples. This, coupled with the unprecedented combination of volume and redshift precision achieved by Quaia, allows us to break the usual degeneracy between Ωm and σ8.…”

MeerKLASS: MeerKAT large area synoptic survey by Santos, MG, Cluver, M, Hilton, M, Jarvis, M, Jozsa, GIG, Leeuw, L, Smirnov, O, Taylor, R, Abdalla, F, Afonso, J, Alonso, D, Bacon, D, Bassett, BA, Bernardi, G, Bull, P, Camera, S, Chiang, HC, Colafrancesco, S, Ferreira, PG, Fonseca, J, Heyden, KVD, Heywood, I, Knowles, K, Lochner, M, Ma, Y-Z, Maartens, R, Makhathini, S, Moodley, K, Pourtsidou, A, Prescott, M, Sievers, J, Spekkens, K, Vaccari, M, Weltman, A, Whittam, I, Witzemann, A, Wolz, L, Zwart, JTL

“…Finally, the same survey will supply unique information for a range of other science applications, including a large statistical investigation of galaxy clusters as well as produce a rotation measure map across a huge swathe of the sky. …”

The Simons Observatory: science goals and forecasts by Ade, P, Alonso, D, Aguirre, J, Ahmed, Z, Aiola, S, Ali, A, Alvarez, MA, Arnold, K, Ashton, P, Austermann, J, Awan, H, Baccigalupi, C, Baildon, T, Barron, D, Battaglia, N, Battye, R, Baxter, E, Bazarko, A, Beall, JA, Bean, R, Beck, D, Beckman, S, Beringue, B, Bianchini, F, Boada, S, Boettger, D, Bond, JR, Borrill, J, Brown, ML, Bruno, SM, Bryan, S, Calabrese, E, Calafut, V, Calisse, P, Carron, J, Challinor, A, Chesmore, G, Chinone, Y, Chluba, J, Cho, H-MS, Choi, S, Coppi, G, Cothard, NF, Coughlin, K, Crichton, D, Crowley, KD, Crowley, KT, Cukierman, A, D'Ewart, JM, Dunner, R, De Haan, T, Devlin, M, Dicker, S, Didier, J, Dobbs, M, Dober, B, Duell, CJ, Duff, S, Duivenvoorden, A, Dunkley, J, Dusatko, J, Fabbian, G, Feeney, S, Ferraro, S, Fluxa, P, Freese, K, Frisch, JC, Frolov, A, Fuller, G, Fuzia, B, Galitzki, N, Ghersi, JTG, Gao, J, Gawiser, E, Gerbino, M, Gluscevic, V, Goeckner-Wald, N, Golec, J, Green, D, Grigorian, A, Groh, J, Groppi, C, Guan, Y, Gudmundsson, JE, Han, D, Hargrave, P, Hasegawa, M, Hasselfield, M, Hattori, M, Haynes, V, Hazumi, M, He, Y, Healy, E, Henderson, SW, Hervias-Caimapo, C, Hill, CA, Hill, JC, Hilton, G, Hilton, M, Hincks, AD, Hinshaw, G, Hlozek, R, Ho, S, Ho, S-PP, Howe, L, Huang, Z, Hubmayr, J, Huffenberger, K, Hughes, JP, Ijjas, A, Ikape, M, Irwin, K, Jaffe, AH, Jain, B, Jeong, O, Kaneko, D, Karpel, ED, Katayama, N, Keating, B, Kernasovskiy, SS, Keskitalo, R, Kisner, T, Kiuchi, K, Klein, J, Knowles, K, Koopman, B, Kosowsky, A, Krachmalnicoff, N, Kuenstner, SE, Kuo, C-L, Kusaka, A, Lashner, J, Lee, A, Lee, E, Leon, D, Leung, JS-Y, Lewis, A, Li, Y, Li, Z, Limon, M, Linder, E, Lopez-Caraballo, C, Louis, T, Lowry, L, Lungu, M, Madhavacheril, M, Mak, D, Maldonado, F, Mani, H, Mates, B, Matsuda, F, Maurin, L, Mauskopf, P, May, A, McCallum, N, McKenney, C, McMahon, J, Meerburg, PD, Meyers, J, Miller, A, Mirmelstein, M, Moodley, K, Munchmeyer, M, Munson, C, Naess, S, Nati, F, Navaroli, M, Newburgh, L, Nguyen, HN, Niemack, M, Nishino, H, Orlowski-Scherer, J, Page, L, Partridge, B, Peloton, J, Perrotta, F, Piccirillo, L, Pisano, G, Poletti, D, Puddu, R, Puglisi, G, Raum, C, Reichardt, CL, Remazeilles, M, Rephaeli, Y, Riechers, D, Rojas, F, Roy, A, Sadeh, S, Sakurail, Y, Salatino, M, Rao, MS, Schaan, E, Schmittfull, M, Sehgal, N, Seibert, J, Seljak, U, Sherwin, B, Shimon, M, Sierra, C, Sievers, J, Sikhosana, P, Silva-Feaver, M, Simon, SM, Sinclair, A, Siritanasak, P, Smith, K, Smith, SR, Spergel, D, Staggs, ST, Stein, G, Stevens, JR, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Teply, G, Thomas, DB, Thorne, B, Thornton, R, Trac, H, Tsai, C, Tucker, C, Ullom, J, Vagnozzi, S, Van Engelen, A, Van Lanen, J, Van Winkle, DD, Vavagiakis, EM, Verges, C, Vissers, M, Wagoner, K, Walker, S, Ward, J, Westbrook, B, Whitehorn, N, Williams, J, Williams, J, Wollack, EJ, Xu, Z, Yu, B, Yu, C, Zago, F, Zhang, H, Zhu, N, The Simons Observatory collaboration

“…The survey will also provide a legacy catalog of 16,000 galaxy clusters and more than 20,000 extragalactic sources.…”