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08:45
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Registration (Royal Observatory of Edinburgh, Reception)
(until 09:15)
()
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09:15
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Welcome (Peacock)
(until 09:30)
()
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09:30
|
EFT of LSS
(until 10:30)
()
|
|
09:30
|
EFT of LSS (D'Amico)
()
|
|
10:00
|
EFT of LSS (Zhang)
()
|
|
10:30
|
--- Break ---
|
|
11:00
|
EFT of LSS
(until 12:30)
()
|
|
11:00
|
Integrated perturbation theory for scalar and tensor fields (Matsubara)
()
|
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11:30
|
Intrinsic alignments (Kokron)
()
|
|
12:00
|
The bispectrum in LPT (Chen)
()
|
|
|
09:00
|
Simulations and theory interplay
(until 10:34)
()
|
|
09:00
|
Fast numerical methods for cosmological inference from LSS (Hahn)
()
|
|
09:30
|
Hermes - Towards an Ultimate High-Performance Algorithm for Cosmic Statistics of Large Data Sets (Feng)
()
|
|
09:47
|
CLASS-OneLoop: Presentation and mock data analysis (Linde)
()
|
|
10:17
|
CLASS-OneLoop: Numerical Implementation and Outlook (Lesgourgues)
()
|
|
10:34
|
--- Break ---
|
|
11:04
|
Simulations and theory interplay
(until 12:38)
()
|
|
11:04
|
Predicting non-linear effects in matter clustering from changes in cosmology and baryons using multi-fidelity simulations (Conley)
()
|
|
11:21
|
The “Missing baryons” in the cosmic web—what is it? Where is it? How much? (Ma)
()
|
|
11:38
|
Hybrid Lagrangian models (Zennaro)
()
|
|
12:08
|
HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments (Maion)
()
|
|
|
09:00
|
Theory to observation
(until 10:30)
()
|
|
09:00
|
Building the EFT of LSS beyond the standard model (Castorina)
()
|
|
09:30
|
Large scale structure formation in theories with scale dependent linear growth (Aviles)
()
|
|
10:00
|
Issues for perturbative methods at higher redshift (White)
()
|
|
10:30
|
--- Break ---
|
|
11:00
|
Theory to observation
(until 12:30)
()
|
|
11:00
|
New tests of dark matter and inflation with BOSS using perturbation theory (Ivanov)
()
|
|
11:30
|
PNG in LSS modeling and analyses (Philcox)
()
|
|
12:00
|
Field level bias modeling, assembly bias, and primordial non-Gaussianity (Sullivan)
()
|
|
|
12:30
|
--- Lunch ---
|
|
13:30
|
EFT of LSS
(until 14:00)
()
|
|
13:30
|
Galaxy bias renormalization group (Rubira)
()
|
|
14:00
|
Panel led discussion: New domains for Perturbation Theory
()
|
|
14:30
|
field theory of cosmic structures
(until 15:00)
()
|
|
14:30
|
Optimal Transport Reconstruction of Large Scale Structures (Nikakhtar)
()
|
|
15:00
|
--- Break ---
|
|
15:30
|
field theory of cosmic structures
(until 16:30)
()
|
|
15:30
|
What makes a filament? (Feldbrugge)
()
|
|
16:00
|
The energy principle for the shape of protohaloes (Musso)
()
|
|
16:30
|
spotlights
()
|
|
17:00
|
--- reception ---
|
|
|
12:38
|
--- Lunch ---
|
|
13:38
|
Simulations and theory interplay
(until 14:55)
()
|
|
13:38
|
Extending Hybrid Models of structure formation (Pellejero)
()
|
|
14:08
|
Field-level emulation of cosmic structure formation with styled neural networks (Jamieson)
()
|
|
14:25
|
Perturbative Forward-Modeling of Large-Scale Structure for Field-Level Analysis and Beyond (Stadler)
()
|
|
14:55
|
--- Break ---
|
|
15:30
|
Simulations and theory interplay
(until 16:00)
()
|
|
15:30
|
How much information is left in galaxy clustering beyond the power spectrum? (Akitsu)
()
|
|
16:00
|
Panel led discussion: Simulations and theory
()
|
|
16:30
|
Panel led discussion: Status of numerical implementations of PT – What’s “done”? What are their strengths? What’s missing?
()
|
|
20:00
|
--- Conference dinner ---
|
|
|
12:30
|
--- Lunch ---
|
|
13:30
|
Panel led discussion: "Limits of pt, setting external priors, setting k_NL, how to squeeze info from LSS on small scales"
()
|
|
14:00
|
Observational steps
(until 15:00)
()
|
|
14:00
|
Emission line galaxies: local PNG bias (Desjacques)
()
|
|
14:30
|
Tomographic analysis with the weak lensing convergence one-point statistics (Castiblanco, presented by Harnois-Deraps)
()
|
|
15:00
|
--- Break ---
|
|
15:30
|
Observational steps
(until 16:30)
()
|
|
15:30
|
The Effective Field Theory of Large-Scale Structure and Multi-tracer (Voivodic)
()
|
|
16:00
|
Going beyond redshift-space distortions with the streaming model (Dam)
()
|
|
16:30
|
Panel or moderated discussion: Status of perturbation theory and priorities for addressing challenges to come given the amount of survey data coming in the next decade
()
|
|