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 |
Jan 13 |
Andrija Kostic |
Modeling Galaxies in Redshift Space at the Field Level |
arXiv:2012.03334 |
Jan 20 |
Agne Semenaite |
Assessing tension metrics with Dark Energy Survey and Planck data |
arXiv:2012.09554 |
Andrea Pezzotta |
Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons |
arXiv:2009.14225 |
Jan 27 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
Luisa Lucie-Smith |
Andromeda XXI - a dwarf galaxy in a low density dark matter halo |
arXiv:2102.11890 |
Mar 24 |
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 |
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 |
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 |
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 |
Peter Stoffer (Universität Wien) |
The anomalous magnetic moment of the muon in the Standard Model |
arXiv:2006.04822 |
May 5 |
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 |
Laura Herold |
Beyond Yamamoto: Anisotropic Power Spectra and Correlation Functions with Pairwise Lines-of-Sight |
arXiv:2102.08384 |
May 19 |
Daniel Farrow |
Correcting correlation functions for redshift-dependent interloper contamination |
arXiv:2104.04613 |
Jun 2 |
Sam Young |
The Formation Probability of Primordial Black Holes |
arXiv:2105.07810 |
Jun 9 |
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 |
Marta Monelli |
The Origin of Parity Violation in Polarized Dust Emission and Implications for Cosmic Birefringence |
arXiv:2105.00120 |
Jun 23 |
Sten Delos |
The Milky Way satellite velocity function is a sharp probe of small-scale structure problems |
arXiv:2106.0905 |
Jul 14 |
Dragan Huterer |
Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing |
arXiv:2105.13549 |
Jul 21 |
Simon May |
Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics |
arXiv:2101.01828 |
Jul 28 |
Oliver Friedrich |
The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise |
arXiv:2107.02300 |
Sep 15 |
Fabian Schmidt |
Covariant Decomposition of The Nonlinear Galaxy Number Counts and Their Monopole |
arXiv:2106.15139 |
Sep 22 |
Martha Lippich |
A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample |
arXiv:2108.01670 |
Sep 29 |
Chris Byrohl |
The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-alpha emitters at 3.3 < z < 6 |
arXiv:2107.03723 |
Oct 6 |
Paolo Campeti |
Testing the Early Universe with Anisotropies of the Gravitational Wave Background |
arXiv:2109.03077 |
Oct 13 |
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 |
Luisa Lucie-Smith |
Capturing the physics of MaNGA galaxies with self-supervised Machine Learning |
arXiv:2104.08292 |
Oct 27 |
Ippei Obata |
Cosmic birefringence tomography and calibration-independence with reionization signals in the CMB |
arXiv:2108.09287 |
Nov 3 |
Angelo Caravano |
Lattice Simulations of Abelian Gauge Fields coupled to Axion during Inflation |
arXiv:2110.10695 |
Nov 10 |
Sherry Suyu |
A Jovian analogue orbiting a white dwarf star |
arXiv:2110.07934 |
Nov 17 |
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 |
Henrique Rubira |
Resonant excitation of the axion field during the QCD phase transition |
arXiv:2110.13157 |
Dec 1 |
Julia Stadler |
On the impact of lensing magnification on redshift-space galaxy clustering analysis |
arXiv:2110.10421 |
Dec 8 |
Elisabeth Krause (Un. of Arizona) |
Lensing discussion |
arXiv:2111.09898 |
Dec 15 |
Agnė Semėnaitė |
Joint Cambridge-Munich Journal Club |
arXiv:2111.03156 |
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 Kostic |
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 |
Andrea Pezzotta |
COMET: Clustering Observables Modelled by Emulated perturbation Theory |
arXiv:2208.01070 |
Nov. 9 |
Alex Barreira |
Constraints on primordial non-Gaussianity from halo bias measured through CMB lensing cross-correlations |
arXiv:2210.01049 |
Nov. 16 |
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 |
Vyoma Muralidhara |
Big bang nucleosynthesis and early dark energy in light of the EMPRESS Yp results and the H0 tension |
arXiv:2211.04087 |
Nov. 30 |
- |
**No Journal Club** |
|
Dec. 07 |
Laura Herold |
A new constraint on Early Dark Energy using the Profile Likelihood |
arXiv:2210.16296
arXiv:2112.12140 |
Dec. 14 |
Andrea Fiorilli |
Testing the accuracy of likelihoods for cluster abundance cosmology |
arXiv:2210.11093 |
Dec. 21 |
- |
**No Journal Club** |
|
|
|
2023 |
|
Jan. 11 |
Luisa Lucie-Smith |
Non-parametric Lagrangian biasing from the insights of neural nets |
arXiv:2212.08095 |
Jan. 18 |
Fabian Schmidt |
Consistency tests of field level inference with EFT likelihood |
arXiv:2212.07875 |
Jan. 25 |
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. 01 |
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. 08 |
|
Wheel session |
|
Feb. 15 |
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 |
Paolo Campeti |
Inference of the optical depth to reionization τ from Planck CMB maps with convolutional neural networks |
arXiv:2301.09634 |
Mar. 01 |
Sten Delos |
Observational Evidence for Cosmological Coupling of Black Holes and its Implications for an Astrophysical Source of Dark Energy |
arXiv:2302.07878 |
Mar. 08 |
Beatriz Tucci |
Robust field-level likelihood-free inference with galaxies |
arXiv:2302.14101 |
Mar. 15 |
Julia Stadler |
Higher-order statistics of the large-scale structure from photometric redshifts |
arXiv:2301.03581 |
Mar. 22 |
Linda Blot |
DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons |
arXiv:2303.05537 |
Mar. 29 |
Fabian Schmidt |
The halo model for cosmology: a pedagogical review |
arXiv:2303.08752 |
Apr. 05 |
Marta Monelli |
Do the CMB Temperature Fluctuations Conserve Parity? |
arXiv:2303.12106 |
Apr. 12 |
- |
** No Journal Club ** |
|
Apr. 19 |
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 |
Sara Maleubre |
Void-Finding Systematics using Crossing Numbers |
arXiv:2302.05469 |
May 03 |
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 |
Emil Brinch Holm |
Special Seminar: A Frequentist's Guide to LambdaCDM Extensions |
arXiv:2211.01935
arXiv:2205.13628 |
May 17 |
Matteo Esposito |
COVMOS: A new Monte Carlo approach for galaxy clustering analysis |
arXiv:2211.13590 |
May 24 |
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 |
Ivana Babic |
Cosmological constraints with the linear point from the BOSS survey |
arXiv:2303.10661 |
Jun. 07 |
Vyoma Muralidhara |
Robustness of Baryon Acoustic Oscillations Measurements with Photometric Redshift Uncertainties |
arXiv:2306.01696 |
Jun. 14 |
Beatriz Tucci |
EFTofLSS meets simulation-based inference: σ8 from biased tracers |
TBA |
Jun. 21 - Sep. 06 |
- |
** Summer Break ** |
|
Sep. 06 |
Matteo Esposito |
Late Time Modification of Structure Growth and the S8 Tension |
arXiv:2308.16183 |
Sep. 13 |
- |
** No Journal club ** |
|
Sep. 20 |
Julia Stadler |
Data Compression and Inference in Cosmology with Self-Supervised Machine Learning |
arXiv:2308.09751 |
Sep. 27 |
- |
** No Journal club ** |
|
Oct. 04 |
Carlos Correa |
AI-assisted super-resolution cosmological simulations |
arXiv:2010.06608
arXiv:2105.01016
arXiv:2305.12222 |
Oct. 11 |
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 |
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 |
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. 01 |
- |
** No Journal club: Public holiday ** |
|
Nov. 08 |
Andrea Pezzotta |
Full Shape Cosmology Analysis from BOSS in configuration space using Neural Network Acceleration |
arXiv:2310.17834 |
Nov. 15 |
Ivana Babic |
On the range of validity of perturbative models for galaxy clustering and its uncertainty |
arXiv:2311.04608 |
Nov. 22 |
Safak Celik |
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 |
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. 06 |
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 |
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 |
Matteo Esposito |
SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos |
arXiv:2401.02075 |
Feb. 07 |
Toshiki Kurita |
Analysis of BOSS Galaxy Data with Weighted Skew-Spectra |
arXiv:2401.13036 |
Feb. 14 |
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 |
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 |
Andrea Fiorilli |
The universal multiplicity function: counting halos and voids |
arXiv:2401.14451 |
Mar. 06 |
Vittorio Ghirardini |
The SRG/eROSITA All-Sky Survey: Cosmology Constraints from Cluster Abundances in the Western Galactic Hemisphere |
arXiv:2402.08458 |
Mar. 13 |
Beatriz Tucci |
Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS |
arXiv:2402.13310 |
Mar. 20 |
Jeong-In Moon |
Examining Lyman-alpha Emitters through MillenniumTNG in anticipation of
DESI-II |
arXiv:2403.02414 |
Apr. 3 |
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 |
Ivana Babic |
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 |
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 |
Safak Celik |
Minimal decaying dark matter: from cosmological tensions to neutrino signatures |
arXiv:2403.15543 |
May 08 |
Fabian Schmidt |
A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics |
arXiv:2405.02252 |
May 15 |
Andrea Pezzotta |
Power spectrum multipoles and clustering wedges during the Epoch of Reionization |
arXiv:2405.05414 |
May 29 |
Ivana Nikolac |
DESI constraints on varying electron mass model and axion-like early dark energy |
arXiv:2405.11869 |
Jun. 05 |
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 |
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 |
Julia Stadler |
Probabilistic Lagrangian bias estimators and the cumulant bias expansion |
arXiv:2407.01524 |
July 10 |
Ivana Babic |
Straightening the Ruler: Field-Level Inference of the BAO Scale with LEFTfield |
arXiv:2405.01950 |