Description |
To place tighter constraints on the physics of the early Universe, its expansion history and the nature of gravity, a better understanding of the nature of the bias between observable and dark matter will be needed. The workshop will be an occasion to present and discuss the most recent developments in the understanding of this bias, along with insights from recent observations. |
Material
Workshop on Galaxy Bias: Non-linear, Non-local and Non-Gaussian | (smr 2491)
Go to day
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08:30 - 09:30
Registration & Administrative Formalities
Location: Adriatico Guest House (Lower Level 1) - 08:30 Registration & Administrative Formalities 1h0'
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09:30 - 10:00
Bias and the formation of dark-matter halos
Location: Adriatico Guest House Giambiagi Lecture Hall -
09:30
Bias and the formation of dark-matter halos
30'
Speaker: C. Porciani (Bonn University)
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09:30
Bias and the formation of dark-matter halos
30'
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10:00 - 10:30
Bias: a personal cook book
Location: Adriatico Guest House Giambiagi Lecture Hall -
10:00
Bias: a personal cook book
30'
Speaker: V. Desjacques (University of Geneva)
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10:00
Bias: a personal cook book
30'
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10:30 - 11:15
Coffee Break
Location: Adriatico Guest House Cafeteria - 10:30 Coffee Break 45'
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11:15 - 11:45
Peak-Background Split, Renormalization, and Galaxy Clustering
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:15
Peak-Background Split, Renormalization, and Galaxy Clustering
30'
Speaker: F. Schmidt (Max-Planck-Institute for Astrophysics) Material: slides
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11:15
Peak-Background Split, Renormalization, and Galaxy Clustering
30'
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11:45 - 12:15
Excursion sets with correlated steps: mass function, non-Gaussianity and bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:45
Excursion sets with correlated steps: mass function, non-Gaussianity and bias
30'
Speaker: M. Musso (Université Catholique de Louvain) Material: slides
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11:45
Excursion sets with correlated steps: mass function, non-Gaussianity and bias
30'
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12:15 - 12:45
Exploring the scale dependence of Lagrangian bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
12:15
Exploring the scale dependence of Lagrangian bias
30'
Speaker: A. Paranjape (ETH Zurich) Material: slides
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12:15
Exploring the scale dependence of Lagrangian bias
30'
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12:45 - 14:15
Lunch Break
Location: Adriatico Guest House Cafeteria - 12:45 Lunch Break 1h30'
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14:15 - 14:45
Measuring galaxy bias with position-dependent power spectrum
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:15
Measuring galaxy bias with position-dependent power spectrum
30'
Speaker: C. Wagner (Max-Planck-Institute for Astrophysics)
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14:15
Measuring galaxy bias with position-dependent power spectrum
30'
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14:45 - 15:15
An 'unbiased' measurement of the matter density parameter Omega_m from VIPERS PDR-1 (z~1)
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:45
An 'unbiased' measurement of the matter density parameter Omega_m from VIPERS PDR-1 (z~1)
30'
Speaker: J. Bel (OA Brera) Material: slides
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14:45
An 'unbiased' measurement of the matter density parameter Omega_m from VIPERS PDR-1 (z~1)
30'
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15:15 - 16:00
Coffee Break
Location: Adriatico Guest House Cafeteria - 15:15 Coffee Break 45'
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16:00 - 16:30
Measuring the growth of matter density fluctuations with third-order galaxy correlations
Location: Adriatico Guest House Giambiagi Lecture Hall -
16:00
Measuring the growth of matter density fluctuations with third-order galaxy correlations
30'
Speaker: K. Hoffmann (ICE Barcellona) Material: slides
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16:00
Measuring the growth of matter density fluctuations with third-order galaxy correlations
30'
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16:30 - 17:00
Measuring the CMASS galaxy bias using the bispectrum technique
Location: Adriatico Guest House Giambiagi Lecture Hall -
16:30
Measuring the CMASS galaxy bias using the bispectrum technique
30'
Speaker: H. Gil-Marin (University of Portsmouth) Material: slides
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16:30
Measuring the CMASS galaxy bias using the bispectrum technique
30'
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19:00 - 21:00
RECEPTION
Location: Adriatico Guest House Cafeteria - 19:00 RECEPTION 2h0'
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08:30 - 09:30
Registration & Administrative Formalities
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09:30 - 10:00
The SHAM approach to modelling galaxy bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
09:30
The SHAM approach to modelling galaxy bias
30'
Speaker: S. Cole (Durham University) Material: slides
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09:30
The SHAM approach to modelling galaxy bias
30'
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10:00 - 10:30
Are the halo occupation predictions consistent with large scale clustering of galaxies in simularions?
Location: Adriatico Guest House Giambiagi Lecture Hall -
10:00
Are the halo occupation predictions consistent with large scale clustering of galaxies in simularions?
30'
Speaker: A. Pujol Vallribera (ICE Barcellona) Material: slides
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10:00
Are the halo occupation predictions consistent with large scale clustering of galaxies in simularions?
30'
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10:30 - 11:15
Coffee Break
Location: Adriatico Guest House Cafeteria - 10:30 Coffee Break 45'
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11:15 - 11:45
Large-scale Cosmic Structures and Clusters of Galaxies in HectoMAP
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:15
Large-scale Cosmic Structures and Clusters of Galaxies in HectoMAP
30'
Speaker: A. Diaferio (University of Torino) Material: slides
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11:15
Large-scale Cosmic Structures and Clusters of Galaxies in HectoMAP
30'
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11:45 - 12:15
Using dark matter halos to reconstruct the cosmic density field
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:45
Using dark matter halos to reconstruct the cosmic density field
30'
Speaker: H. Mo (UMass Amherst)
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11:45
Using dark matter halos to reconstruct the cosmic density field
30'
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12:15 - 12:45
Mapping the cosmic web: the environment of galaxy birth
Location: Adriatico Guest House Giambiagi Lecture Hall -
12:15
Mapping the cosmic web: the environment of galaxy birth
30'
Speaker: B. Jones (University of Groningen)
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12:15
Mapping the cosmic web: the environment of galaxy birth
30'
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12:45 - 14:15
Lunch Break
Location: Adriatico Guest House Cafeteria - 12:45 Lunch Break 1h30'
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14:15 - 14:45
Nonlocal Halo Bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:15
Nonlocal Halo Bias
30'
Speaker: K.C. Chan (University of Geneva) Material: slides
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14:15
Nonlocal Halo Bias
30'
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14:45 - 15:15
Understanding higher-order non-local bias by combining the power spectrum with the bispectrum
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:45
Understanding higher-order non-local bias by combining the power spectrum with the bispectrum
30'
Speaker: S. Saito (University of Tokyo)
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14:45
Understanding higher-order non-local bias by combining the power spectrum with the bispectrum
30'
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15:15 - 16:00
Coffee Break
Location: Adriatico Guest House Cafeteria - 15:15 Coffee Break 45'
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16:00 - 16:30
The Imprint of Initial Conditions on Halo Bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
16:00
The Imprint of Initial Conditions on Halo Bias
30'
Speaker: T. Baldauf (IAS, Princeton)
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16:00
The Imprint of Initial Conditions on Halo Bias
30'
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16:30 - 17:00
Non-Local Bias factors: Theory vs simulations
Location: Adriatico Guest House Giambiagi Lecture Hall -
16:30
Non-Local Bias factors: Theory vs simulations
30'
Speaker: M. Biagetti (Universite de Geneve) Material: slides
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16:30
Non-Local Bias factors: Theory vs simulations
30'
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09:30 - 10:00
The SHAM approach to modelling galaxy bias
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09:30 - 10:00
Cosmology with galaxy bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
09:30
Cosmology with galaxy bias
30'
Speaker: E. Gaztañaga (ICE Barcellona) Material: slides
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09:30
Cosmology with galaxy bias
30'
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10:00 - 10:30
The effect of baryons on the distribution of matter
Location: Adriatico Guest House Giambiagi Lecture Hall -
10:00
The effect of baryons on the distribution of matter
30'
Speaker: J. Schaye (Leiden University)
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10:00
The effect of baryons on the distribution of matter
30'
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10:30 - 11:15
Coffee Break
Location: Adriatico Guest House Cafeteria - 10:30 Coffee Break 45'
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11:15 - 11:45
The effects of baryons on the halo mass function
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:15
The effects of baryons on the halo mass function
30'
Speaker: W. Cui (OA Trieste) Material: slides
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11:15
The effects of baryons on the halo mass function
30'
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11:45 - 12:15
Distribution of cool gas around luminous red galaxies
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:45
Distribution of cool gas around luminous red galaxies
30'
Speaker: G.B. Zhu (Johns Hopkins University)
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11:45
Distribution of cool gas around luminous red galaxies
30'
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12:15 - 12:45
Assembly bias in models and observations
Location: Adriatico Guest House Giambiagi Lecture Hall -
12:15
Assembly bias in models and observations
30'
Speaker: N. Padilla (Pontificia Universidad Católica de Chile) Material: slides
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12:15
Assembly bias in models and observations
30'
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12:45 - 14:15
Lunch Break
Location: Adriatico Guest House Cafeteria - 12:45 Lunch Break 1h30'
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14:15 - 14:45
The dynamical aspect of halo/galaxy bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:15
The dynamical aspect of halo/galaxy bias
30'
Speaker: A. Faltenbacher (Wits University Johannesburg) Material: slides
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14:15
The dynamical aspect of halo/galaxy bias
30'
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14:45 - 15:15
A consistency relation for galaxies
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:45
A consistency relation for galaxies
30'
Speaker: M. Simonovic (SISSA)
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14:45
A consistency relation for galaxies
30'
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15:15 - 16:00
Coffee Break
Location: Adriatico Guest House Cafeteria - 15:15 Coffee Break 45'
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16:00 - 16:30
Measuring nonlinear galaxy bias from counts in cells at z~1
Location: Adriatico Guest House Giambiagi Lecture Hall -
16:00
Measuring nonlinear galaxy bias from counts in cells at z~1
30'
Speaker: E. Branchini (University Roma Tre) Material: slides
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16:00
Measuring nonlinear galaxy bias from counts in cells at z~1
30'
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16:30 - 17:00
Modelling the Halo/Galaxy Bias with the full nonlinear information in the mass
density field
Location: Adriatico Guest House Giambiagi Lecture Hall -
16:30
Modelling the Halo/Galaxy Bias with the full nonlinear information in the mass
density field
30'
Speaker: J.E. Pollack (University of Bonn)
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16:30
Modelling the Halo/Galaxy Bias with the full nonlinear information in the mass
density field
30'
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20:00 - 22:00
Outside Dinner - Ristorante ANTICO PANADA
Via Rossini, 8/D - 34132 Trieste - tel: 0403476286 If you wish to attend - it is mandatory to confirm your participation by e-mail (smr2491@ictp.it). Further details will be provided during the Workshop.
Location: - 20:00 Outside Dinner - Ristorante ANTICO PANADA 2h0'
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09:30 - 10:00
Cosmology with galaxy bias
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09:30 - 10:00
The multiple faces of galaxy bias
Location: Adriatico Guest House Giambiagi Lecture Hall -
09:30
The multiple faces of galaxy bias
30'
Speaker: U. Seljak (Berkeley University) Material: slides
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09:30
The multiple faces of galaxy bias
30'
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10:00 - 10:30
Integrated PT and its applications
Location: Adriatico Guest House Giambiagi Lecture Hall -
10:00
Integrated PT and its applications
30'
Speaker: T. Matsubara (Nagoya University) Material: slides
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10:00
Integrated PT and its applications
30'
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10:30 - 11:15
Coffee Break
Location: Adriatico Guest House Cafeteria - 10:30 Coffee Break 45'
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11:15 - 11:45
Modeling the galaxy distribution in redshiftspace with perturbation theory and stochastic halo biasing
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:15
Modeling the galaxy distribution in redshiftspace with perturbation theory and stochastic halo biasing
30'
Speaker: F. Kitaura (Leibniz Institute for Astrophysics in Potsdam) Material: slides
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11:15
Modeling the galaxy distribution in redshiftspace with perturbation theory and stochastic halo biasing
30'
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11:45 - 12:15
Distribution function approach to redshift space distortions of dark matter halos
Location: Adriatico Guest House Giambiagi Lecture Hall -
11:45
Distribution function approach to redshift space distortions of dark matter halos
30'
Speaker: Z. Vlah (University of Zurich)
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11:45
Distribution function approach to redshift space distortions of dark matter halos
30'
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12:15 - 12:45
Using spatial clustering to estimate redshift distributions
Location: Adriatico Guest House Giambiagi Lecture Hall -
12:15
Using spatial clustering to estimate redshift distributions
30'
Speaker: B. Ménard (Johns Hopkins University) Material: slides
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12:15
Using spatial clustering to estimate redshift distributions
30'
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12:45 - 14:15
Lunch Break
Location: Adriatico Guest House Cafeteria - 12:45 Lunch Break 1h30'
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14:15 - 14:45
Halo abundances and clustering with massive neutrinos
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:15
Halo abundances and clustering with massive neutrinos
30'
Speaker: E. Castorina (SISSA)
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14:15
Halo abundances and clustering with massive neutrinos
30'
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14:45 - 15:15
Clustering properties in cosmologies with massive neutrinos
Location: Adriatico Guest House Giambiagi Lecture Hall -
14:45
Clustering properties in cosmologies with massive neutrinos
30'
Speaker: F.A. Villaescusa Navarro (OA Trieste)
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14:45
Clustering properties in cosmologies with massive neutrinos
30'
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15:15 - 15:20
Distribution of Certificates of Attendance
IN MAIL BOXES
Location: Adriatico Guest House Giambiagi Lecture Hall - 15:15 Distribution of Certificates of Attendance 5'
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15:20 - 16:00
Get-Together Drink
Location: Adriatico Guest House (Terrace) - 15:20 Get-Together Drink 40'
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09:30 - 10:00
The multiple faces of galaxy bias