Date | Speaker | Title | Arxiv number |
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Sep. 25 | Matteo Esposito | Evolution Mapping II: Describing Statistics of the Non-Linear Cosmic Velocity Field | arXiv:2406.08539 |
Wheel | HOD-informed prior for EFT-based full-shape analyses of LSS | arXiv:2409.12937 | |
Oct. 2 | Jeong-In Moon | The Hubble Tension in our own Backyard: DESI and the Nearness of the Coma Cluster | arXiv:2409.14546 |
Wheel | DESI constraints on alpha-attractor inflationary models Using dust to constrain dark matter models |
arXiv:2410.00827 arXiv:2409.14780 |
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Oct. 9 | Luisa Lucie-Smith | The causal effect of cosmic filaments on dark matter halos | arXiv:2409.13010 |
Wheel | 2D watershed void clustering for probing the cosmic large-scale structure The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles |
arXiv:2410.04898 arXiv:409.15513 |
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Oct. 16 | Andrea Pezzotta | DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS | arXiv:2410.08163 |
Wheel | Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior | arXiv:2410.08998 | |
Oct. 23 | Andrea Fiorilli | Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy | arXiv:2410.10616 |
Wheel | The Affleck-Dine Curvaton | arXiv:2410.13712 | |
Oct. 30 | Jiamin Hou | Parity-breaking galaxy 4-point function from lensing by chiral gravitational waves | arXiv:2408.03994 |
Wheel | FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structure On the spatial distribution of the Large-Scale structure: An Unsupervised search for Parity Violation |
arXiv:2410.19905 arXiv:2410.16030 |
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Nov. 6 | ** CANCELLED ** | ||
Nov. 13 | Safak Celik | FIMP Dark Matter in bulk viscous non-standard cosmologies | arXiv:2411.05590 |
Wheel | |||
Nov. 20 | Sofia Contarini | A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity | arXiv:2410.21457 |
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Nov. 27 | Fabian Schmidt | Structure formation with primordial black holes: collisional dynamics, binaries, and gravitational waves | arXiv:2410.01876 |
Wheel | Cross-Correlating the Universe: The Gravitational Wave Background and Large-Scale Structure | arXiv:2411.00532 | |
Dec. 4 | Sha Azyzy | Kinetic Gauge Friction in Natural Inflation | arXiv:2411.19892 |
Wheel | Simulation-based inference has its own Dodelson-Schneider effect (but it knows that it does) | arXiv:2412.02311 | |
Dec. 11 | Ivana Nikolac | Constraining the phase shift of relativistic species in DESI BAOs | arXiv:2412.05990 |
Wheel | Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing | arXiv:2412.07765 | |
Dec. 18 | ** We're on a break ** | ||
Dec. 25 | ** MERRY CHRISTMAS** | ||
Jan. 1 | ** HAPPY NEW YEAR ** | ||
Jan. 8 | ** We're still on a break ** | ||
Jan. 15 | Drew Jamieson | Probing primordial non-Gaussianity by reconstructing the initial conditions | arXiv:2412.00968 |
Wheel | Cosmological Constraints using the Void Size Function Data from BOSS DR16 | arXiv:2501.07817 | |
Jan. 22 | Noemi Anau Montel | Tests for model misspecification in simulation-based inference: from local distortions to global model checks | arXiv:2412.15100 |
Wheel | Impact of particle production during inflation on the detection of CMB B-mode polarization Boosting Supermassive Black Hole Growth in the Early Universe by Fuzzy Dark Matter Solitons |
arXiv:2501.08592 arXiv:2501.09098v1 |
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Jan. 29 | Beatriz Tucci | Refining local-type primordial non-Gaussianity: Sharpened bϕ constraints through bias expansion | arXiv:2501.14873 |
Wheel | Gamma-Ray Observations of Galaxy Clusters Strongly Constrain Dark Matter Annihilation in Prompt Cusps | arXiv:2501.14865 | |
Feb. 5 | Alejandro Perez-Fernandez | Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions | arXiv:2501.18597 |
Feb. 12 | Toshiki Kurita | Selecting samples of galaxies with fewer Fingers-of-God | arXiv:2501.10587 |
Wheel | Cosmological Inference with Cosmic Voids and Neural Network Emulators | arXiv:2502.05262 | |
Feb. 19 | Jed Homer | Simulation-based inference has its own Dodelson-Schneider effect (but it knows that it does) | arXiv:2412.02311 |
Feb. 26 | Adri Duivenvoorden | Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models | arXiv:22502.13243 |
Wheel | Learning the Universe: 3 h^-1 Gpc Tests of a Field Level N-body Simulation Emulator SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport |
arXiv:2502.13242 arXiv:2502.17553 |
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March 5 | Matteo Esposito | ||
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March 12 | Andrea Fiorilli | ||
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March 19 | Jeongin Moon | ||
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March 26 | Ivana Nikolac | ||
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April 2 | Jiamin Hou | ||
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April 9 | Harry (Hsiang-Ming) Huang | ||
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April 16 | Andrea Pezzotta | ||
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April 23 | Safak Celik | ||
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April 30 | Sofia Contarini | ||
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May 7 | Fabian Schmidt | ||
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May 14 | Sha Azyzy | ||
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