| Date |
Speaker |
Title |
Arxiv number |
| Dec 11 2019 |
Samuel Young |
Primordial Black Holes |
|
| Jan 8 2020 |
Alex Barreira |
Baryonic effects for weak lensing: II. Combination with X-ray data and
extended cosmologies |
arXiv:1911.08494 |
| Jan 8 2020 |
Ira Wolfson |
A Note on the Swampland Distance Conjecture |
arXiv:1911.09050 |
| Jan 22 2020 |
Martha Lippich |
Super-resolution emulator of
cosmological simulations using deep physical models |
arXiv:2001.05519 |
| Jan 22 2020 |
Minh Nguyen |
Large Scale Structure Reconstruction with Short-Wavelength Modes |
arXiv:2001.02780 |
| Jan 29 2020 |
Fabian Schmidt |
Cosmology from galaxy clustering via the EFT |
arXiv:1909.05277
arXiv:1909.05271 |
| Feb 5 2020 |
Ariel G. Sanchez |
Cosmology from large-scale structure: Constraining Lambda-CDM with BOSS |
arXiv:1909.11006 |
| Feb 5 2020 |
Sherry Suyu |
The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints |
arXiv:2001.09213 |
| Feb 12 2020 |
Rodrigo Voivodic |
Using the Marked Power Spectrum to Detect the Signature of Neutrinos in Large-Scale Structure |
arXiv:2001.11024 |
| Feb 12 2020 |
Giovanni Cabass |
Super-CMB fluctuations can resolve the Hubble tension |
arXiv:1905.02278 |
| Feb 19 2020 |
Laura Herold |
Is there an early Universe solution to the Hubble tension? |
arXiv:2002.06044 |
Feb 26 2020 |
Leila Mirzagholi |
Simulating the Cosmic Neutrino Background using Collisionless Hydrodynamics
|
arXiv:2002.04601 |
| Feb 26 2020 |
Daniel Farrow |
Angular Correlation Function Estimators Accounting for Contamination from Probabilistic Distance Measurements |
arXiv:1911.07832 |
| Mar 4 2020 |
Jiamin Hou |
Arrows of Time and Initial and Final Conditions in the Quantum Mechanics of Closed Systems Like the Universe |
arXiv:2002.07093 |
| Mar 4 2020 |
Agne Semenaite |
Neutrino effects on the morphology of cosmic large-scale structure |
arXiv:2002.08846 |
| Mar 11 2020 |
Linda Blot |
The Distinct Stellar-to-Halo Mass Relations of Satellite and Central
Galaxies:
Insights from the IllustrisTNG Simulations |
arXiv:2002.11119 |
| Mar 11 2020 |
Samuel Young |
Non-linear statistics of primordial black holes from gaussian curvature perturbations |
arXiv:1912.07072
arXiv:1912.04687 |
| Mar 18 2020 |
Alex Barreira |
Compensated Isocurvature Perturbations in the Galaxy Power Spectrum |
arXiv:2002.12931 |
| Mar 25 2020 |
Minh Nguyen |
Observational detection of correlation between galaxy spins and initial conditions |
arXiv:2003.04800 |
| Apr 1 2020 |
Fabian Schmidt |
Measuring the Tidal Response of Structure Formation: Anisotropic Separate Universe Simulations using TreePM |
arXiv:2003.06427 |
| Apr 1 2020 |
Martha Lippich |
What will it take to measure individual neutrino mass states using cosmology? |
arXiv:2003.03354 |
| Apr 8 2020 |
Sherry Suyu |
Constraints on compact dark matter with fast radio burst observations |
arXiv:2003.13349 |
| Apr 8 2020 |
Rodrigo Voivodic |
The Halo Void (Dust) Model of Large Scale Structure |
arXiv:2003.06411 |
| Apr 15 2020 |
Giovanni Cabass |
Induced superhorizon tensor perturbations from anisotropic non-Gaussianity |
arXiv:2001.00409 |
| Apr 15 2020 |
Laura Herold |
Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum |
arXiv:2003.08277 |
| Apr 22 2020 |
Linda Blot |
Clusters Have Edges: The Projected Phase SpaceStructure of SDSS redMaPPer Clusters |
arXiv:2003.11555 |
| Apr 22 2020 |
Daniel Farrow |
Voronoi volume function: A new probe of cosmology and galaxy evolution |
arXiv:2001.08760 |
| Apr 29 2020 |
Jiamin Hou |
Galaxy redshift-space bispectrum: the Importance of Being Anisotropic |
arXiv:2003.12075 |
| Apr 29 2020 |
Agne Semenaite |
Observing Baryonic Acoustic Oscillations in tomographic cosmic shear surveys |
arXiv:2004.03201 |
| May 6 2020 |
Andrea Pezzotta |
Does jackknife scale really matter for accurate large-scale structure covariances? |
arXiv:2004.13436 |
| May 13 2020 |
Samuel Young |
Dark matter and dark radiation from evaporating primordial black holes |
arXiv:2004.04740 |
| May 13 2020 |
Alex Barreira |
A hydrodynamical halo model for weak-lensing cross correlations |
arXiv:2005.00009 |
| May 20 2020 |
Jiamin Hou |
Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure |
arXiv:2004.02926 |
| May 20 2020 |
Fabian Schmidt |
Violent expiratory events: On coughing and sneezing |
ResearchGate:262983673 |
| May 27 2020 |
Martha Lippich |
Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Shape of the Matter Power Spectrum |
arXiv:2004.01424 |
| May 27 2020 |
Linda Blot |
Beware of commonly used approximations II: estimating systematic biases in the best-fit parameters |
arXiv:2005.09666 |
| Jun 3 2020 |
Rodrigo Voivodic |
Model independent measurement of the growth rate from the consistency relations of the LSS |
arXiv:2005.09574 |
| Jun 10 2020 |
|
particlesforjustice.org |
|
| Jun 17 2020 |
Giovanni Cabass |
Impact of transforming to Conformal Fermi Coordinates on Quasi-Single Field Non-Gaussianity |
arXiv:2004.06126 |
| Jun 17 2020 |
Daniel Farrow |
Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions |
arXiv:2006.05383 |
| Jun 24 2020 |
Minh Nguyen |
Observation of Excess Electronic Recoil Events in XENON1T |
arXiv:2006.09721 |
| Jun 24 2020 |
Agne Semenaite |
Minimising the impact of scale-dependent galaxy bias on the joint cosmological analysis of large scale structures |
arXiv:2004.07811 |
| Jul 1 2020 |
Andrea Pezotta |
Testing one-loop galaxy bias - I. Power spectrum |
arXiv:2006.09729 |
| Jul 8 2020 |
Laura Herold |
J-PLUS: Unveiling the brightest-end of the Lya luminosity function at 2.0 < z < 3.3 over 1000 deg^2 |
arXiv:2006.15084 |
| Jul 8 2020 |
Daniel Farrow |
Searching for dark energy in the matter-dominated era |
arXiv:2007.02865 |
| Jul 15 2020 |
Elisa Ferreira |
Constraining Early Dark Energy with Large-Scale Structure |
arXiv:2006.11235 |
| Jul 15 2020 |
Sherry Suyu |
TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles |
arXiv:2007.02941 |
| Jul 22 2020 |
Ira Wolfson |
Measuring the spectrum of primordial gravitational waves with CMB, PTA and Laser Interferometers |
arXiv:2007.04241 |
| Jul 22 2020 |
Agne Semenaite |
Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing |
arXiv:2007.04007 |
| Jul 29 2020 |
Minh Nguyen |
Direct detection of the kinetic Sunyaev-Zel'dovich effect in galaxy clusters |
arXiv:2007.02952 |
| Jul 29 2020 |
Fabian Schmidt |
Information content in the redshift-space galaxy power spectrum and bispectrum |
arXiv:2007.04340 |
| Sep 9 2020 |
Sam Young |
The impact on distant fly-bys on the rate of binary primordial black hole mergers |
arXiv:2006.15023 |
| Sep 16 2020 |
Jiamin Hou |
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2 |
arXiv:2007.08998 |
| Martha Lippich |
Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections |
arXiv:2009.03311 |
| Sep 30 2020 |
Andrea Pezzotta |
Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey |
arXiv:2008.05991 |
| Laura Herold |
Cosmological constraints from BOSS with analytic covariance matrices |
arXiv:2009.00622 |
| Oct 7 2020 |
Daniel Farrow |
Cosmological 3D HI Gas Map with HETDEX Lya Emitters and eBOSS QSOs at z=2: IGM-Galaxy/QSO Connection and a ~40-Mpc Scale Giant HII Bubble Candidate |
arXiv:2009.07285 |
| Oct 14 2020 |
Sherry Suyu |
First measurement of the Hubble parameter from bright binary black hole GW190521
Hubble Constant Measurement with GW190521 as an Eccentric Black Hole Merger |
arXiv:2009.14199
arXiv:2009.14247 |
| Elisa Ferreira |
Why reducing the cosmic sound horizon can not fully resolve the Hubble tension |
arXiv:2010.04158 |
| Oct 21 2020 |
Agne Semenaite |
The End of Galaxy Surveys |
arXiv:2010.06064 |
| Alex Barreira |
On the "Lensing is Low" of BOSS Galaxies |
arXiv:2010.01143 |
| Nov 4 2020 |
Marta Monelli |
Polarizations of CMB and the Hubble tension |
arXiv:2010.12164 |
| Vyoma Muralidhara |
A Test of the Cosmological Principle with Quasars |
arXiv:2009.14826 |
| Nov 11 2020 |
Dragan Huterer |
Cosmology with dropout selection: Straw-man surveys and CMB lensing |
arXiv:1904.13378 |
| Elisa Ferreira |
Probing Dark Matter Self-interaction with Ultra-faint Dwarf Galaxies |
arXiv:2008.02529 |
| Nov 18 2020 |
Sten Delos |
Constraints on the Epoch of Dark Matter Formation from Milky Way Satellites |
arXiv:2010.01137 |
| Ippei Obata |
BICEP / Keck Array XII: Constraints on axion-like polarization oscillations in the cosmic microwave background |
arXiv:2011.03483 |
| Nov 25 2020 |
Giovanni Arico |
Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way |
arXiv:2011.08865 |
| Dec 9 2020 |
Ariel Sanchez |
Improved two-point correlation function estimates using glass-like distributions as a reference sample |
arXiv:2011.05747 |
| Linda Blot |
Cosmological Model Parameter Dependence of the Matter Power Spectrum Covariance from the DEUS-PUR Cosmo Simulations |
arXiv:2007.14984 |
| Dec 16 2020 |
Chris Byrohl |
Constraining Reionization in Progress at z=5.7 with Lyman-Alpha Emitters: Voids, Peaks, and Cosmic Variance |
arXiv:2011.03559 |
| |
|
2021 |
|
Jan 13 2021 |
Andrija Kostić |
Modeling Galaxies in Redshift Space at the Field Level |
arXiv:2012.03334 |
| Jan 20 2021 |
Agnė Semėnaitė |
Assessing tension metrics with Dark Energy Survey and Planck data |
arXiv:2012.09554 |
| Andrea Pezzotta 2021 |
Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons |
arXiv:2009.14225 |
| Jan 27 2021 |
Laura Herold |
Hockey-stick dark energy is not a solution to the H0 crisis |
arXiv:2101.08641 |
| Daniel Farrow |
Cosmological constraints from line intensity mapping with interlopers |
arXiv:2001.10792 |
| Feb 3 2021 |
Akin Yildirim |
The Hubble Constant from Infrared Surface Brightness Fluctuation Distances |
arXiv:2101.02221 |
| Minh Nguyen |
A new approach to observational cosmology using the scattering transform |
arXiv:2006.08561 |
| Feb 10 2021 |
Minh Nguyen |
New Interpretable Statistics for Large Scale Structure Analysis and Generation |
arXiv:2006.06298 |
| Alex Barreira |
Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias |
arXiv:2012.04637 |
| Feb 17 2021 |
Marta Monelli |
Constraining reionization with the first measurement of the CMB optical depth fluctuation - Compton-y cross-correlation |
arXiv:2102.00975 |
| Sam Young |
Extreme-Value Distributions and Primordial Black-Hole Formation |
arXiv:2101.10340 |
| Feb 24 2021 |
Angelo Caravano |
Lattice Simulations of Inflation |
arXiv:2102.06378 |
| Sten Delos |
Probing Small-Scale Power Spectra with Pulsar Timing Arrays |
arXiv:2012.09857 |
| Mar 3 2021 |
Fabian Schmidt |
Testing one-loop galaxy bias: joint analysis of power spectrum and bispectrum |
arXiv:2101.06902 |
| Ariel Sanchez |
Redshift-space distortions with split densities |
arXiv:2101.09854 |
| Mar 10 2021 |
Martha Lippich |
Information Content of Higher-Order Galaxy Correlation Functions |
arXiv:2102.01696 |
| Chris Byrohl |
The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift |
arXiv:2102.05516 |
| Mar 17 2021 |
Luisa Lucie-Smith |
Andromeda XXI - a dwarf galaxy in a low density dark matter halo |
arXiv:2102.11890 |
| Mar 24 2021 |
Paolo Campeti |
Comparing multi-field primordial feature models with the Planck data |
arXiv:2103.03025 |
| Vyoma Muralidhara |
Constraining the cosmic UV background at z>3 with MUSE Lyman-alpha emission observations |
arXiv:2103.09250 |
| Mar 31 2021 |
Elisa Ferreira |
The imprint of ultralight vector fields on gravitational wave propagation |
arXiv:2012.07505 |
| Ippei Obata |
Self-gravitating Vector Dark Matter |
arXiv:2101.07265 |
| Apr 14 2021 |
Minh Nguyen |
Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias |
arXiv:2103.09820 |
| Apr 21 2021 |
Nam Tran (Boston University) |
Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppm |
arXiv:2104.03181 |
| Agnė Semėnaitė |
When is tension just a fluctuation? How noisy data affects model comparison |
arXiv:2103.09820 |
| Apr 28 2021 |
Peter Stoffer (Universität Wien) |
The anomalous magnetic moment of the muon in the Standard Model |
arXiv:2006.04822 |
| May 5 2021 |
Andrija Kostić |
Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data |
arXiv:2011.00910 |
| Andrea Pezotta |
Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear |
arXiv:2010.12382 |
| May 12 2021 |
Laura Herold |
Beyond Yamamoto: Anisotropic Power Spectra and Correlation Functions with Pairwise Lines-of-Sight |
arXiv:2102.08384 |
| May 19 2021 |
Daniel Farrow |
Correcting correlation functions for redshift-dependent interloper contamination |
arXiv:2104.04613 |
| Jun 2 2021 |
Sam Young |
The Formation Probability of Primordial Black Holes |
arXiv:2105.07810 |
| Jun 9 2021 |
Luisa Lucie-Smith |
The Hubble Tension Bites the Dust: Sensitivity of the Hubble Constant Determination to Cepheid Color Calibration |
arXiv:2105.11461 |
| Alex Barreira |
Cosmological constraints from unWISE and Planck CMB lensing tomography |
arXiv:2105.03421 |
| Jun 16 2021 |
Marta Monelli |
The Origin of Parity Violation in Polarized Dust Emission and Implications for Cosmic Birefringence |
arXiv:2105.00120 |
| Jun 23 2021 |
Sten Delos |
The Milky Way satellite velocity function is a sharp probe of small-scale structure problems |
arXiv:2106.0905 |
| Jul 14 2021 |
Dragan Huterer (University of Michigan) |
Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing |
arXiv:2105.13549 |
| Jul 21 2021 |
Simon May |
Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics |
arXiv:2101.01828 |
| Jul 28 2021 |
Oliver Friedrich |
The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise |
arXiv:2107.02300 |
| Sep 15 2021 |
Fabian Schmidt |
Covariant Decomposition of The Nonlinear Galaxy Number Counts and Their Monopole |
arXiv:2106.15139 |
| Sep 22 2021 |
Martha Lippich |
A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample |
arXiv:2108.01670 |
| Sep 29 2021 |
Chris Byrohl |
The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-alpha emitters at 3.3 < z < 6 |
arXiv:2107.03723 |
| Oct 6 2021 |
Paolo Campeti |
Testing the Early Universe with Anisotropies of the Gravitational Wave Background |
arXiv:2109.03077 |
| Oct 13 2021 |
Vyoma Muralidhara |
Cross-correlation of the Polarizations of the 21-cm and Cosmic Microwave Backgrounds |
arXiv:2110.01619 |
| Alexandre Barthelemy |
Probability distribution function of the aperture mass field with large deviation theory |
arXiv:2012.03831 |
| Oct 20 2021 |
Luisa Lucie-Smith |
Capturing the physics of MaNGA galaxies with self-supervised Machine Learning |
arXiv:2104.08292 |
| Oct 27 2021 |
Ippei Obata |
Cosmic birefringence tomography and calibration-independence with reionization signals in the CMB |
arXiv:2108.09287 |
| Nov 3 2021 |
Angelo Caravano |
Lattice Simulations of Abelian Gauge Fields coupled to Axion during Inflation |
arXiv:2110.10695 |
| Nov 10 2021 |
Sherry Suyu |
A Jovian analogue orbiting a white dwarf star |
arXiv:2110.07934 |
| Nov 17 2021 |
Drew Jamieson |
The Covariance of Squeezed Bispectrum Configurations |
arXiv:2111.05887 |
| Elena de la Hoz, Patricia Diego-Palazuelos |
Determination of Polarization Angles in CMB Experiments and Application to CMB Component Separation Analyses |
arXiv:2110.14328 |
| Nov 24 2021 |
Henrique Rubira |
Resonant excitation of the axion field during the QCD phase transition |
arXiv:2110.13157 |
| Dec 1 2021 |
Julia Stadler |
On the impact of lensing magnification on redshift-space galaxy clustering analysis |
arXiv:2110.10421 |
| Dec 8 2021 |
Elisabeth Krause (Un. of Arizona) |
Lensing discussion |
arXiv:2111.09898 |
| Dec 15 2021 |
Agnė Semėnaitė |
Joint Cambridge-Munich Journal Club |
arXiv:2111.03156 |
| |
|
2022 |
|
| Jan 19 |
Laura Herold |
New Early Dark Energy is compatible with current LSS data |
arXiv:2009.00006 |
| Feb 2 |
Andrija Kostić |
The BOSS DR12 Full-Shape Cosmology: LCDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole |
arXiv:2112.04515 |
| Feb 9 |
Andrea Pezotta |
Combined full shape analysis of BOSS galaxies and eBOSS quasars using an iterative emulator |
arXiv:2201.04679 |
| Feb 16 |
Daniel Farrow |
AbacusHOD: A highly efficient extended multi-tracer HOD framework and its application to BOSS and eBOSS data |
arXiv:2110.11412 |
| Feb 23 |
Alex Barreira |
The clustering of galaxies in the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Primordial non-Gaussianity in Fourier Space |
arXiv:2106.13725 |
| Mar 9 |
Vyoma Muralidhara |
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics |
arXiv:2202.07680 |
| Mar 16 |
Agnė Semėnaitė |
Consistent lensing and clustering in a low-S8 Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000 |
arXiv:2202.07440 |
| Eiichiro Komatsu |
New physics from polarised light of the cosmic microwave background |
arXiv:2202.13919 |
| Mar 23 |
Fabian Schmidt |
Not so fuzzy: excluding FDM with sizes and stellar kinematics of ultra-faint dwarf galaxies |
arXiv:2203.05750 |
| Mar 30 |
Sten Delos |
Small-scale structure in vector dark matter |
arXiv:2203.11935 |
| Apr 6 |
Paolo Campeti |
Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices |
arXiv:2202.05949 |
| Apr 13 |
Ippei Obata |
Cosmic Birefringence: Cross-Spectra and Cross-Bispectra with CMB Anisotropies |
arXiv:2202.04584 |
| Apr 20 |
Luisa Lucie-Smith |
From Images to Dark Matter: End-To-End Inference of Substructure From Hundreds of Strong Gravitational Lenses |
arXiv:2203.00690 |
| May 4 |
Julia Stadler |
Wavelet Moments for Cosmological Parameter Estimation |
arXiv:2204.07646 |
| May 11 |
Anik Halder |
JOINT CAMBRIDGE-MUNICH JOURNAL CLUB |
arXiv:2201.05607 |
| May 25 |
Beatriz Tucci |
Can we actually constrain fNL using the scale-dependent bias effect? An illustration of the impact of galaxy bias uncertainties using the BOSS DR12 galaxy power spectrum |
arXiv:2205.05673 |
| Angelo Caravano |
Cosmological Bootstrap in Slow Motion |
arXiv:2205.10340 |
| Jun 1 |
Sam Goldstein |
Determining the Hubble Constant without the Sound Horizon: A 3.6% Constraint on H0 from Galaxy Surveys, CMB Lensing and Supernovae |
arXiv:2204.02984 |
| Jun 8 |
Linda Blot |
Galaxy Cluster Statistics in Modified Gravity Cosmologies |
arXiv:2205.13015 |
| Jun 15 |
Sherry Suyu |
The AGEL Survey: Spectroscopic Confirmation of Strong Gravitational Lenses in the DES and DECaLS Fields Selected Using Convolutional Neural Network |
arXiv:2205.05307 |
| Jun 22 |
Maja Lujan Niemeyer |
HI intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies |
arXiv:2206.01579 |
| Jun 29 |
Marta Monelli |
CMB spectral distortions revisited: a new take on ? distortions and primordial non-Gaussianities from FIRAS data |
arXiv:2206.02762 |
| Oct. 12 |
Wheel only |
|
|
| Oct. 19 |
Matteo Esposito |
The JWST High Redshift Observations and Primordial Non-Gaussianity |
arXiv:2210.04812 |
| Oct. 26 |
Andrija Kostić |
The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching |
arXiv:2210.10059
arXiv:2210.10075 |
| Nov 2 2022 |
Andrea Pezzotta |
COMET: Clustering Observables Modelled by Emulated perturbation Theory |
arXiv:2208.01070 |
| Nov 9 2022 |
Alex Barreira |
Constraints on primordial non-Gaussianity from halo bias measured through CMB lensing cross-correlations |
arXiv:2210.01049 |
| Nov 16 2022 |
Jose Luis Bernal |
The deconvolved distribution estimator: enhancing reionisation-era CO line-intensity mapping analyses with a cross-correlation analogue for one-point statistics
Characteristic Functions for Cosmological Cross-Correlations |
arXiv:2210.14890
arXiv:2210.14902 |
| Nov 23 2022 |
Vyoma Muralidhara |
Big bang nucleosynthesis and early dark energy in light of the EMPRESS Yp results and the H0 tension |
arXiv:2211.04087 |
| Dec 7 2022 |
Laura Herold |
A new constraint on Early Dark Energy using the Profile Likelihood |
arXiv:2210.16296
arXiv:2112.12140 |
| Dec 14 2022 |
Andrea Fiorilli |
Testing the accuracy of likelihoods for cluster abundance cosmology |
arXiv:2210.11093 |
| |
|
2023 |
|
| Jan 11 2023 |
Luisa Lucie-Smith |
Non-parametric Lagrangian biasing from the insights of neural nets |
arXiv:2212.08095 |
| Jan 18 2023 |
Fabian Schmidt |
Consistency tests of field level inference with EFT likelihood |
arXiv:2212.07875 |
| Jan 25 2023 |
Ziyang Chen |
Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data |
arXiv:2301.02186 |
| Feb 1 2023 |
Alejandra Melo |
TDCOSMO. XIII. Improved Hubble constant measurement from lensing time delays using spatially resolved stellar kinematics of the lens galaxy |
arXiv:2301.02656 |
| Feb 15 2023 |
Carlos Correa |
Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids |
arXiv:2212.06849 |
| Feb 22 2023 |
Paolo Campeti |
Inference of the optical depth to reionization τ from Planck CMB maps with convolutional neural networks |
arXiv:2301.09634 |
| Mar 1 2023 |
Sten Delos |
Observational Evidence for Cosmological Coupling of Black Holes and its Implications for an Astrophysical Source of Dark Energy |
arXiv:2302.07878 |
| Mar 8 2023 |
Beatriz Tucci |
Robust field-level likelihood-free inference with galaxies |
arXiv:2302.14101 |
| Mar 15 2023 |
Julia Stadler |
Higher-order statistics of the large-scale structure from photometric redshifts |
arXiv:2301.03581 |
| Mar 22 2023 |
Linda Blot |
DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons |
arXiv:2303.05537 |
| Mar 29 2023 |
Fabian Schmidt |
The halo model for cosmology: a pedagogical review |
arXiv:2303.08752 |
| Apr 5 2023 |
Marta Monelli |
Do the CMB Temperature Fluctuations Conserve Parity? |
arXiv:2303.12106 |
| Apr 19 2023 |
Vyoma Muralidhara |
The period-luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for H0 |
arXiv:2304.01671 |
| Apr 26 2023 |
Sara Maleubre |
Void-Finding Systematics using Crossing Numbers |
arXiv:2302.05469 |
| May 3 2023 |
Andrea Pezzotta |
The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps |
arXiv:2304.12338 |
| May 10 2023 |
Emil Brinch Holm |
Special Seminar: A Frequentist's Guide to LambdaCDM Extensions |
arXiv:2211.01935
arXiv:2205.13628 |
| May 17 2023 |
Matteo Esposito |
COVMOS: A new Monte Carlo approach for galaxy clustering analysis |
arXiv:2211.13590 |
| May 24 2023 |
Laurence Gong |
Cambridge-Munich joint journal club: Cosmology from the integrated shear 3-point correlation function: simulated likelihood analyses with machine-learning emulators |
arXiv:2304.01187 |
| May 31 2023 |
Ivana Babić |
Cosmological constraints with the linear point from the BOSS survey |
arXiv:2303.10661 |
| Jun 7 2023 |
Vyoma Muralidhara |
Robustness of Baryon Acoustic Oscillations Measurements with Photometric Redshift Uncertainties |
arXiv:2306.01696 |
| Jun 14 2023 |
Beatriz Tucci |
EFTofLSS meets simulation-based inference: σ8 from biased tracers |
arXiv:2310.03741 |
| Jun. 21 - Sep. 06 |
- |
** Summer Break ** |
|
| Sep 6 2023 |
Matteo Esposito |
Late Time Modification of Structure Growth and the S8 Tension |
arXiv:2308.16183 |
| Sep 20 2023 |
Julia Stadler |
Data Compression and Inference in Cosmology with Self-Supervised Machine Learning |
arXiv:2308.09751 |
| Oct. 04 |
Carlos Correa |
AI-assisted super-resolution cosmological simulations |
arXiv:2010.06608
arXiv:2105.01016
arXiv:2305.12222 |
| Oct 11 2023 |
Beatriz Tucci |
Sensitivity Analysis of Simulation-Based Inference for Galaxy Clustering |
arXiv:2309.15071 |
| Wheel |
The position-dependent matter density probability distribution function
Cosmological constraints from density-split clustering in the BOSS CMASS galaxy sample |
arXiv:2010.07235
arXiv:2309.16541 |
| Oct 18 2023 |
Andrea Fiorilli |
Cosmological parameters derived from the final (PR4) Planck data release |
arXiv:2309.10034 |
| Wheel |
Robust cosmological inference from non-linear scales with k-th nearest neighbor statistics |
arXiv:2310.04501 |
| Oct 25 2023 |
Luisa Lucie-Smith |
Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with Cosmic Microwave Background |
arXiv:2310.07642 |
| Wheel |
The 2-point correlation function covariance with fewer mocks
Creating Jackknife and Bootstrap estimates of the covariance matrix for the two-point correlation function |
arXiv:2306.16332
arXiv:2109.07071 |
| Nov 8 2023 |
Andrea Pezzotta |
Full Shape Cosmology Analysis from BOSS in configuration space using Neural Network Acceleration |
arXiv:2310.17834 |
| Nov 15 2023 |
Ivana Babić |
On the range of validity of perturbative models for galaxy clustering and its uncertainty |
arXiv:2311.04608 |
| Nov 22 2023 |
Şafak Çelik |
Cosmological constraints on light but massive relics |
arXiv:2107.09664 |
| Wheel |
Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform |
arXiv:2310.16116 |
| Nov 29 2023 |
Fabian Schmidt |
Direct signatures of the formation time of galaxies |
arXiv:2307.11409 |
| Wheel |
Constraining Baryonic Physics with DES Y1 and Planck data -- Combining Galaxy Clustering, Weak Lensing, and CMB Lensing
5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM |
arXiv:2311.08047
arXiv:2311.16377 |
| Dec 6 2023 |
Vyoma Muralidhara |
Detection of the CMB lensing -- galaxy bispectrum |
arXiv:2311.04213 |
| Andrea Pezzotta |
Euclid preparation. TBD. Galaxy power spectrum modelling in real space |
arXiv:2312.00679 |
| |
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2024 |
|
| Jan 17 2024 |
Ivana Nikolac |
Massive black hole binaries in LISA: constraining cosmological parameters at high redshifts |
arXiv:2312.04632 |
| Wheel |
Bayesian Inference of Initial Conditions from Non-Linear Cosmic Structures using Field-Level Emulators |
arXiv:2312.09271 |
| Jan 24 2024 |
Sofia Contarini |
Towards cosmology with Void Lensing: how to find voids sensitive to weak-lensing and numerically interpret them |
arXiv:2311.14586 |
| Jan 31 2024 |
Matteo Esposito |
SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos |
arXiv:2401.02075 |
| Feb 07 2024 |
Toshiki Kurita |
Analysis of BOSS Galaxy Data with Weighted Skew-Spectra |
arXiv:2401.13036 |
| Feb 14 2024 |
Julia Stadler |
A point cloud approach to generative modeling for galaxy surveys at the field level |
arXiv:2311.17141 |
| Wheel |
The SRG/eROSITA All-Sky Survey: Cosmology Constraints from Cluster Abundances in the Western Galactic Hemisphere |
arXiv:2402.08458 |
| Feb 21 2024 |
Alejandro Perez-Fernandez |
CLASS-OneLoop: Accurate and Unbiased Inference from Spectroscopic Galaxy Surveys |
arXiv:2402.09778 |
| Wheel |
Cosmological constraints from the Chandra-Planck galaxy cluster sample |
arXiv:2402.04006v1 |
| Feb 28 2024 |
Andrea Fiorilli |
The universal multiplicity function: counting halos and voids |
arXiv:2401.14451 |
| Mar 6 2024 |
Vittorio Ghirardini |
The SRG/eROSITA All-Sky Survey: Cosmology Constraints from Cluster Abundances in the Western Galactic Hemisphere |
arXiv:2402.08458 |
| Mar 13 2024 |
Beatriz Tucci |
Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS |
arXiv:2402.13310 |
| Mar 20 2024 |
Jeong-In Moon |
Examining Lyman-alpha Emitters through MillenniumTNG in anticipation of
DESI-II |
arXiv:2403.02414 |
| Apr 3 2024 |
Luisa Lucie-Smith |
Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3
cosmic shear two-point correlations on small scales: the S8 tension
remains present |
arXiv:2403.20323 |
| Apr 10 2024 |
Ivana Babić |
DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon
Acoustic Oscillations |
arXiv:2404.03002 |
| Wheel |
Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback
Cosmic Web Classification through Stochastic Topological Ranking |
arXiv:2404.06098v1
arXiv:2404.0112424v1 |
| Apr 17 2024 |
Drew Jamieson |
Bounds on galaxy stochasticity from halo occupation distribution modeling |
arXiv:2404.04252v1 |
| Wheel |
Does DESI 2024 Confirm ΛCDM?
Deep Learning for Cosmological Parameter Inference from Dark Matter Halo Density Field |
arXiv:2404.08633
arXiv:2404.09483 |
| Apr 24 2024 |
Şafak Çelik |
Minimal decaying dark matter: from cosmological tensions to neutrino signatures |
arXiv:2403.15543 |
| May 8 2024 |
Fabian Schmidt |
A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics |
arXiv:2405.02252 |
| May 15 2024 |
Andrea Pezzotta |
Power spectrum multipoles and clustering wedges during the Epoch of Reionization |
arXiv:2405.05414 |
| May 29 2024 |
Ivana Nikolac |
DESI constraints on varying electron mass model and axion-like early dark energy |
arXiv:2405.11869 |
| Jun 5 2024 |
Sofia Contarini |
Fast simulation mapping: from standard to modified gravity cosmologies using the bias assignment method |
arXiv:2405.10319 |
| Wheel |
Improving cosmological analyses of HI clustering by reducing stochastic noise
Dwarf galaxies imply dark matter is heavier than 2.2x10^-21eV |
arXiv:2405.18559
arXiv:2405.20374 |
| Jun 12 2024 |
Toshiki Kurita |
The Atacama Cosmology Telescope: DR6 Gravitational Lensing and SDSS BOSS cross-correlation measurement and constraints on gravity with the EG statistic |
arXiv:2405.12795 |
| Wheel |
The New Worlds Simulations: Large-scale Simulations across Three Cosmologies |
arXiv:2406.07276v1 |
| Jun 19 2024 |
Julia Stadler |
Probabilistic Lagrangian bias estimators and the cumulant bias expansion |
arXiv:2407.01524 |
| Jul 10 2024 |
Ivana Babić |
Straightening the Ruler: Field-Level Inference of the BAO Scale with LEFTfield |
arXiv:2405.01950 |
| Sep 25 2024 |
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 2024 |
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 |
| Oct 9 2024 |
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
|
| Oct 16 2024 |
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 2024 |
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 2024 |
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 |
| Nov 13 2024 |
Şafak Çelik |
FIMP Dark Matter in bulk viscous non-standard cosmologies |
arXiv:2411.05590 |
| Nov 20 |
Sofia Contarini |
A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity |
arXiv:2410.21457 |
| Nov 27 2024 |
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 2024 |
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 2024 |
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 |
| |
|
2025 |
|
| Jan 15 2025 |
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 2025 |
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
|
| Jan 29 2025 |
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 2025 |
Alejandro Perez-Fernandez |
Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions |
arXiv:2501.18597 |
| Feb 12 2025 |
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 2025 |
Jed Homer (USM/LMU) |
Simulation-based inference has its own Dodelson-Schneider effect (but it knows that it does) |
arXiv:2412.02311 |
| Feb. 26 2025 |
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
|
| March 5 2025 |
Matteo Esposito |
Illustrating the consequences of a misuse of sigma8 in cosmology |
arXiv:2501.11571 |
| Mar 12 2025 |
Andrea Fiorilli |
Simulation-Based Priors without Simulations: an Analytic Perspective on EFT Parameters of Galaxies |
arXiv:2503.07270 |
| Wheel |
Excursion Sets with a "Perfect" Collapse Model |
arXiv:2503.07735v1 |
| Mar 19 2025 |
Jeongin Moon |
The Spectroscopic Stage-5 Experiment |
arXiv:2503.07923 |
| Wheel |
Does dark matter fall in the same way as standard model particles? A direct constraint of Euler's equation with cosmological data
How many simulations do we need for simulation-based inference in cosmology?
|
arXiv:2502.12843
arXiv:2503.13755
|
| Mar 26 2025 |
Ivana Nikolac |
DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints |
arXiv:2503.14738 |
| Apr 2 |
Sofia Contarini |
Weak-lensing tunnel voids in simulated light-cones: a new pipeline to investigate modified gravity and massive neutrinos signatures |
arXiv:2504.02041 |
| Apr 9 2025 |
Jiamin Hou |
Anatomy of parity-violating trispectra in galaxy surveys |
arXiv:2504.02931 |
| Wheel |
Has ACT measured radiative corrections to the tree-level Higgs-like inflation? |
arXiv:2504.06002 |
| Apr 16 2025 |
Harry (Hsiang-Ming) Huang |
Bootstrapping LSS perturbation theory beyond third order |
arXiv:2504.01078 |
| Wheel |
Implications of distance duality violation for the H0 tension and evolving dark energy |
arXiv:2504.10464 |
| Apr 30 2025 |
Şafak Çelik |
Anchors no more: Using peculiar velocities to constrain H0 and the primordial Universe without calibrators |
arXiv:2504.10453 |
| Wheel |
Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data
Effective Field Theory of Chiral Gravitational Waves |
arXiv:2504.18464
arXiv:2504.19059 |
| May 7 2025 |
Sha Azyzy |
Hubble-induced phase transitions in the Standard Model and beyond |
arXiv:2505.00900 |
| May 14 2025 |
Boris Bolliet (University of Cambridge) |
Extracting cosmological information from the abundance of galaxy clusters with simulation-based inference |
arXiv:2504.10230 |
| May 21 2025 |
Fabian Schmidt |
Forward vs Backward: Improving BAO Constraints with Field-Level Inference |
arXiv:2505.13588 |
| Wheel |
Vlasov Perturbation Theory applied to ΛCDM
Hunting axion dark matter signatures in low-frequency terrestrial magnetic fields |
arXiv:2505.02907
arXiv:2504.06653 |
| May 28 2025 |
Fumihiro Naokawa (University of Tokyo) |
Universal profile for cosmic birefringence tomography with radio galaxies |
arXiv:2504.06709 |
| Jun 4 2025 |
Noemi Anau Montel |
Field-Level Comparison and Robustness Analysis of Cosmological N-Body Simulations |
arXiv:2505.13620 |
| Jun 11 2025 |
Alejandro Perez-Fernandez |
Renormalized Perturbation Theory at field level: the LSS Bootstrap in GridSPT |
arXiv:2506.07105 |
| Wheel |
A novel test of gravity: Does spacetime geometry track matter density?
Can a Dark Inferno Melt Earth's Core? |
arXiv:2506.04387
arXiv:2505.24070 |
| Jul 2 2025 |
* wheel day * |
Going beyond S8: fast inference of the matter power spectrum from weak-lensing surveys |
arXiv:2506.16434 |
| Jul 9 2025 |
Adri Duivenvoorden |
EMPRESS. XV. A New Determination of the Primordial Helium Abundance Suggesting a Moderately Low Y_P Value |
arXiv:2506.24050 |
| Jul 16 - Sep 8 |
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** Summer Break ** |
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