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09:00
The Full-Shape analayis of the Dark Energy Spectroscopic Instrument data release 1
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Gil-Marin
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09:30
Towards an optimal marked correlation function analysis for the detection of modified gravity
-
Martin Kärcher
(University of Milan)
-
10:00
CNN-Enhanced Zel’dovich Reconstruction for BAO analysis in Large-Scale Structure Surveys
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Edoardo Maragliano
(University of Genoa, INFN)
-
11:00
Modelling the distribution of galaxy multi-tracers through cosmic time
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Ginevra Favole
(Instituto de Astrofísica de Canarias)
-
11:30
Indicator Power Spectra
-
Istvan Szapudi
(Institute for Astronomy, University of Hawaii)
-
12:00
The clustering of dark matter haloes in alternative cosmological models
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Massimiliano Romanello
(Università di Bologna)
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12:30
De-noising cosmological covariance matrices using Rotational Invariant estimators
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Antonio Farina
(Istituto Nazionale di Astrofisica (INAF))
-
14:30
Measuring higher-order correlation functions in current and future galaxy surveys
-
Slepian
-
15:00
Cosmology from Large Scale full-shape analyses combining 2PCF and 3PCF
-
Massimo Guidi
(University of Bologna)
-
15:30
Consistent Clustering Analysis in Configuration and Fourier Space
-
Alfonso Veropalumbo
(Istituto Nazionale di Astrofisica (INAF))
-
16:30
Toward a full-shape analysis of the galaxy anisotropic 3-point correlation function at the BAO scale
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Kristers Nagainis
(University of Latvia Institute of Astronomy)
-
17:00
TBD
-
Michele Ennio Maria Moresco
(Istituto Nazionale di Astrofisica (INAF))
Michele Moresco
(University of Bologna)
-
17:30
The BAO linear point as cosmic ruler: tests and applications to the Euclid mission
-
Angelo Ferrari
(INFN - Bologna)
