| Posters | ||||||||||||
| Ata | Metin | AIP Potsdam | Reconstruction of the cosmological Large-scale Structure with Bayesian statistics and biased tracers | |||||||||
| Autefage | Mathieu | AIP Potsdam | The impact of non-local halo/galaxy bias on baryon acoustic oscillations | |||||||||
| Bilicki | Maciej | Leiden Univ. | Observational Progress on All-Sky Large-scale Structure of the Universe | |||||||||
| Borzyszkowski | Mikolaj | Argelander-Institut fŸr Astronomie | Can we observe relativistic redshift-space distortions in forthcoming galaxy surveys? | |||||||||
| Cabass | Giovanni | La Sapienza - Univ. of Rome | Constraints on the Early and Late Integrated Sachs-Wolfe effects after Planck 2015 | |||||||||
| Carucci | Isabella Paola | SISSA, Trieste | The imprint of warm dark matter on the 21cm power spectrum: forecasts for SKA | |||||||||
| Chen | Song | Univ. Bielefeld | Fluctuations of radio galaxy number count | |||||||||
| Chiang | Chi-Ting | MPA | Position-dependent power spectrum | |||||||||
| Cole | Shaun | Durham Univ. | Large Scale Halo Light Cone Catalogues | |||||||||
| Compostella | Michele | MPA | A numerical perspective on helium reionization | |||||||||
| Fonseca | JosŽ | Univ. of the Western Cape | Beating cosmic variance: cross-correlating HI intensity mapping with galaxy surveys | |||||||||
| FŸhrer | Florian | Univ. Heidelberg | Higher-order massive neutrino perturbations in large-scale structure | |||||||||
| Garzilli | Antonella | Lorentz Institute, Leiden Univ. | Lyman alpha forest: warm IGM or warm dark matter? | |||||||||
| GrŸn | Daniel | LMU | Weak lensing by galaxy troughs in Dark Energy Survey Science Verification data | |||||||||
| Hawken | Adam | Osservatorio di Brera | Halo properties in f(R) cosmology | |||||||||
| Hoffmann | Kai | ICE (CSIC/IEEC) | Non-local bias contribution to third-order galaxy correlations | |||||||||
| Hu | Bin | Leiden Univ. | Effective field theory approach for dark energy and modified gravity | |||||||||
| Israel | Holger | Durham Univ. | Reconciling Planck cluster counts and cosmology?Chandra/XMM instrumental calibration and hydrostaticmass bias | |||||||||
| Izard | Albert | ICE, CSIC-IEEC | Towards fast and accurate massive mock making with Lagrangian methods | |||||||||
| Koda | Jun | INAF - Osservatorio Astronomico di Brera | Many mock catalogues for low-mass galaxies | |||||||||
| Koo | Hanwool | Seoul National Univ. | Constraining ΛCDM and Coupled Dark Energy by using the Spin Alignments in Galaxy Pairs | |||||||||
| Kopp | Michael | Univ. of Cyprus | Redshift space distortions with the truncated Zel'dovich approximation | |||||||||
| Kovacs | Andras | IFAE Barcelona | Cold imprint of supervoids in the Cosmic Microwave Background re-considered with Planck and BOSS DR10 | |||||||||
| Krzyszkowska | Jolanta | Heidelberg Institute for Theoretical Studies | Angular Momentum Properties of Haloes in the Illustris Simulation | |||||||||
| Lazeyras | Titouan | MPA | Precision measurement of the local bias of dark matter halos | |||||||||
| Li | Ming | NAOC | Optimization of kSZ measurements with a reconstructed cosmological flow field | |||||||||
| Lin | Chieh-An | CEA Saclay | A fast stochastic approach for cosmological constraints using weak-lensing peak counts | |||||||||
| Macaulay | Ed | Univ. of Queensland | Signals from Noise in the Hubble Diagram | |||||||||
| Markovic | Dida | ICG, Portsmouth | Simulating Spectroscopic Data for Euclid Galaxy Clustering | |||||||||
| Massara | Elena | SISSA | Modelling the LSS in massive neutrino cosmologies | |||||||||
| Merson | Alex | UCL | Halo detection via large-scale Bayesian inference | |||||||||
| Monna | Anna | MPE/USM | Constraining the galaxy mass content in the core of clusters through strong lensing and velocity dispersion measurements | |||||||||
| Moraes | Bruno | UCL | Measuring the angular power spectrum and cross-correlations of BOSS data | |||||||||
| Muir | Jessica | Univ. of Michigan | The impact of LSS survey systematics on ISW signal reconstruction | |||||||||
| Musso | Marcello | Univ. of Pennsylvania | Modelling halo statistics | |||||||||
| Osato | Ken | Univ. of Tokyo | Investigating the sigma8 tension by the cross-correlation of tSZ and cosmic shear | |||||||||
| Paz | Dante | Instituto de Astronom’a Te—rica y Experimental | Reducing the impact of covariance uncertainties on statistical inferences of cosmological parameters | |||||||||
| Pezzotta | Andrea | INAF - Osservatorio Astronomico di Brera | Clustering with multiple galaxy populations in VIPERS | |||||||||
| Pujol | Arnau | ICE, Barcelona | Halo clustering: enviroment versus mass | |||||||||
| Rau | Markus Michael | USM | Low Bias Lensing and Large Scale Structure Measurements using Machine Learning photometric redshift PDF reconstruction | |||||||||
| Renneby | Malin | Universe Cluster / LMU | Cosmological rescaling and weak lensing observables | |||||||||
| Roth | Nina | UCL | Towards controlled experiments in galaxy formation | |||||||||
| Schaan | Emmanuel | Princeton Univ. | Kinematic Sunyaev-Zel'dovich effect and constraints on the missing baryons | |||||||||
| Seehars | Sebastian | ETH ZŸrich | Simulating H I Intensity Maps at Low Redshifts: Covariance of the Angular Power Spectrum | |||||||||
| Sekiguchi | Toyokazu | Univ. of Helsinki | Structure formation in decaying dark matter | |||||||||
| Shafer | Daniel | Univ. of Michigan | Multiplicative errors in the galaxy power spectrum | |||||||||
| Shim | Junsup | Seoul National Univ. | Observational evidence of the bridge effect of void filaments | |||||||||
| Shirasaki | Masato | NAOJ | Probing cosmology with weak lensing selected clusters | |||||||||
| Singh | Sukhdeep | Carnegie Mellon Univ. | Intrinsic Alignments of Galaxies | |||||||||
| Sšrgel | Bjšrn | IoA, Cambridge | The kinematic SZ effect from DES galaxy clusters and high-resolution CMB maps | |||||||||
| Sorce | Jenny | AIP Potsdam | Cosmicflows observations give us CLUES to matter distribution | |||||||||
| Sugiyama | Naonori | Univ. of Tokyo | Analytical approach to density-weighted velocity correlation function of Large-Scape Structure | |||||||||
| Thomas | Daniel | Univ. of Cyprus | The non-linear relativistic universe | |||||||||
| Umehata | Hideki | ESO | Dusty starbursts and AGNs in a z=3.1 protocluster revealed by ALMA | |||||||||
| Wiegand | Alexander | CfA, Harvard | Minkowski functionals as a tracer of cosmic inhomogeneity | |||||||||
| Wilson | Michael | Univ. of Edinburgh | Clipping the wings of non-linear structure | |||||||||
| Wolz | Laura | Univ. of Melbourne | Intensity Mapping Cross-Correlations: Connecting the Largest Scales to Galaxy Evolution | |||||||||
| Xavier | Henrique | UCL | Fast full sky simulations of correlated lognormal fields | |||||||||
| Yoon | Mijin | Univ. of Michigan | Kinematic dipole detection with galaxy surveys | |||||||||
| Ziparo | Felicia | Univ. of Birmingham | LoCuSS: Exploring the selection of faint, blue, background galaxies for cluster weak-lensing | |||||||||