Past Papers
Feb 27, 2025
Anmol Raina,”Cosmological Information Content of Betti Curves and k-nearest Neighbor Distributions” [Cosmological information content of Betti curves and $k$-nearest... ], @ Zoom, at 4:00pm
Feb 13, 2025
Nino Ephremidze, "Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure" [https://arxiv.org/abs/2502.02636], @ Zoom, at 4:00pm
Jan 30, 2025
Misha Rashkovetskyi, "Selecting samples of galaxies with fewer Fingers-of-God", [https://arxiv.org/abs/2501.10587] , @ Zoom, at 4:00pm
Dec 5, 2024
Gemma Zhang, "Learning Optimal and Interpretable Summary Statistics of Galaxy Catalogs with SBI", https://arxiv.org/abs/2411.08957, @ Zoom, at 5:00pm
Nov 7, 2024
Anmol Raina, "Disentangling the primordial nature of stochastic gravitational wave backgrounds with CMB spectral distortions", https://arxiv.org/abs/2309.02366, @ Zoom, at 5:00pm
Oct 24, 2024
Chandrika Chandrashekar, "Particle creation from non-geodesic trajectories in multifield inflation", https://arxiv.org/abs/2410.13843, @ Zoom, at 5:00pm
Oct 10, 2024
Nino Ephremidze, "Challenges to the Lambda CDM Cosmology",(https://arxiv.org/abs/2406.12106), @ Zoom, at 5:00pm
Sep 26, 2024
Catherine Petretti, "Searching for Dark Matter Interactions with ACT, SPT and DES", https://arxiv.org/abs/2409.06771, @ Zoom, at 5:00pm
Sep 12, 2024
Shu-Fan Chen, "The Atacama Cosmology Telescope: Multi-probe cosmology with unWISE galaxies and ACT DR6 CMB lensing", https://arxiv.org/abs/2409.02109 , @ Zoom, at 5:00pm
Apr 23, 2024
Aizhan Akhmetzhanova, "The Atacama Cosmology Telescope: Detection of Patchy Screening of the Cosmic Microwave Background", https://arxiv.org/abs/2401.13033 , @ Zoom, at 5:00pm
Mar 26, 2024
Anmol Raina, "Unveiling Neutrino Halos with CMB Lensing", https://arxiv.org/abs/2306.15715, @ Zoom, at 5:00pm
Mar 12, 2024
Prish Chakraborty, "The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing", https://arxiv.org/abs/2309.05659, @ Zoom, at 5:00pm
Feb 27, 2024
Chandrika Chandrashekar, "Dark Matter production during Warm Inflation via Freeze-In", https://arxiv.org/abs/2401.17371, @ Zoom, at 5:00pm
Feb 13, 2024
Arthur Tsang, "Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems using Recurrent Inference Machines", https://arxiv.org/abs/2301.04168, @ Zoom, at 5:00pm
Jan 30, 2024
Prof. Zachary Slepian
Title: Is Nature Its Own Mirror? Parity-Violation with Galaxy Quartets in BOSS
Abstract: Recently we have shown that the galaxy 4-point correlation function, which measures an excess of quartets of galaxies over random, is sensitive to parity violation in our universe’s large-scale structure. It is fundamentally 3D and thus has a handedness even after averaging over orientations, in contrast to galaxy pair and triplet correlations. With this new observable, we have detected parity violation at high statistical significance using the largest currently available sample, the SDSS Baryon Oscillation Spectroscopic Survey’s roughly 1 M galaxies. If confirmed by upcoming sky surveys such as DESI this would indicate new physics operant in the Universe’s earliest moments. In this talk I will discuss this result and the many systematics tests performed to test its robustness, as well as prospects for the future, especially with DESI data.
Nov 21, 2023
Prish Chakraborty, "Positivity from Cosmological Correlators", https://arxiv.org/abs/2310.02490, @ Zoom, at 5:00pm
Nov 7, 2023
Chandrika Chandrashekar, "Multifield ultralight dark matter", https://arxiv.org/abs/2301.07114, @ Zoom, at 5:00pm
Oct 24, 2023
Anmol Raina, "Consistently constraining fNL with the squeezed lensing bispectrum using consistency relations", https://arxiv.org/abs/2310.12959, @ Zoom, at 5:00pm
Oct 10, 2023
Wenzer Qin
Title: Probing exotic energy injection with the CMB and early star formation
Abstract: Dark matter interactions with Standard Model particles can inject energy at early times, altering the standard evolution of the early universe. In particular, this energy injection can perturb the spectrum of the cosmic microwave background (CMB) away from that of a perfect blackbody, alter the CMB anisotropy spectrum, and affect processes by which the first stars form. For this study, I will discuss recent work to upgrade the DarkHistory code package to more carefully track interactions among low energy electrons, hydrogen atoms, and radiation, in order to accurately compute the evolution of the CMB spectral distortion in the presence of Dark Matter energy injection. I will show results for the contribution to the spectral distortions from redshifts z < 3000 for arbitrary energy injection scenarios, new CMB anisotropy constraints on light dark matter, as well as the effect of exotic energy injection on early star formation.
Sep 26, 2023
Theo Simon
Title: Constraining cosmological models with the effective field theory of large-scale structures
Abstract: In this talk, I will present the paradigm of the effective field theory of large-scale structures (EFTofLSS) and how it can be used to constrain cosmological models. First, I will discuss the consistency of this theory and its predictive power, and then I will present the constraints of the EFTofLSS applied to BOSS and eBOSS data on the LCDM model. Finally, I will mention the constraints from this theory on early dark energy, a model that potentially resolves the Hubble tension, and on decaying cold dark matter, a model that possibly resolves the S8 tension.
May 16, 2023
Prof. Cumrun Vafa, @ Zoom, at 5:00pm
Title: Quantum Gravity and A Unification of the Dark Sector
Abstract: In this talk I apply consistency conditions of quantum gravity to the dark sector. Motivated by the smallness of the dark energy combined with other experimental data, one is naturally led to a corner of the quantum gravity landscape with one extra mesoscopic dimension in the micron range. Interestingly this also leads to graviton excitations in the 5th dimension as an unavoidable candidate for the dark matter. Moreover TCC conjecture applied to the late time cosmology motivates specific initial conditions in this scenario, leading to the right abundance of dark matter gravitons and an explanation of the cosmological coincidence problem. We show how this novel dark matter scenario may also resolve the S8 tension.
May 2, 2023
Shu-Fan Chen, "Field-level inference of cosmic shear with intrinsic alignments and baryons", https://arxiv.org/abs/2304.04785, @ Zoom, at 5:00pm
Apr 18, 2023
Aizhan Akhmetzhanova, "Cosmology with 6 parameters in the Stage-IV era: efficient marginalisation over nuisance parameters”, https://arxiv.org/abs/2301.11895, @ Zoom, at 5:00pm
Apr 4, 2023
Chandrika Chandrashekar, “Do the CMB Temperature Fluctuations Conserve Parity?", https://arxiv.org/abs/2303.12106, @ Zoom, at 5:00pm
Mar 6, 2023
Gemma Zhang, “Beyond Gaussian Noise: A Generalized Approach to Likelihood Analysis with non-Gaussian Noise”, https://arxiv.org/abs/2302.03046, @ Zoom, at 5:00pm
Feb 21, 2023
Alex Johnson, “S8 Tension in the Context of Dark Matter-Baryon Scattering", https://arxiv.org/abs/2301.08260 , @ Zoom, at 5:00pm
Feb 7, 2023
Georgios Valogiannis, “Constraints on S8 from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS”, https://arxiv.org/abs/2301.08692 , @ Zoom, at 5:00pm
Jan 24, 2023
Anmol Raina, "Detecting deviations from Gaussianity in high-redshift CMB lensing maps", https://arxiv.org/abs/2211.09617, @ Zoom, at 5:00pm
Nov 29, 2022
Katie Fraser, "A lower bound on dark matter mass, https://arxiv.org/abs/2211.09775 , @ Zoom, at 5:00pm
Nov 15, 2022
Carol Cuesta-Lazaro, "Constraining nuLCDM with density-split clustering", https://arxiv.org/abs/2209.04310 , @ Zoom, at 5:00pm
Nov 8, 2022
Gabriela Sato-Polito (External Speaker from Johns Hopkins), "Cosmology and astrophysics with the extragalactic light: background and fluctuations", @ Zoom, at 4:00pm & Lyman 330
Abstract:
The aggregate light emitted by all extragalactic sources can be measured either as an absolute intensity or through its spatial fluctuations; these are known as line-intensity mapping (LIM) when a particular line transition is targeted. I will discuss how these measurements can be used both to investigate the presence of speculative sources of radiation, such as decaying dark matter, and learn about galaxy evolution. I then focus on intensity mapping and discuss how the unique characteristics of these measurements (e.g. wide redshift coverage, sensitivity to faint sources, and mapping speed) may enable a variety of scientific goals, some of the challenges in realizing them and promising future directions.
Oct 18, 2022
Çağan Şengül, "Galactic satellite systems in CDM, WDM and SIDM", https://arxiv.org/abs/2208.07376 , @ Zoom, at 4:00pm
Oct 4, 2022
Benjamin Schmitt, Overview of the CMB-S4 experiment, @ Zoom, at 5:00pm
Sep 20, 2022
Miranda Eiben, “Evidence for Line-of-Sight Frequency Decorrelation of Polarized Dust Emission in Planck Data" https://arxiv.org/abs/2101.09291, @ Zoom, at 5:00pm
Apr 26, 2022
Siddharth Mishra-Sharma, “Gravitationally Lensed Black Hole Emission Tomography" https://arxiv.org/abs/2204.03715, @ Zoom, at 5:00pm
Apr 12, 2022
Claire Lamman, “Tidal alignments as a contaminant of redshift space distortions" https://ui.adsabs.harvard.edu/abs/2009MNRAS.399.1074H/abstract , @ Zoom, at 5:00pm
Mar 29, 2022
Sebastian Wagner-Carena (External Speaker from Stanford), "From Images to Dark Matter: End-to-End Inference of Substructure from Hundreds of Strong Gravitational Lenses", @ Zoom, at 5:00pm
Abstract:
Constraining the distribution of small-scale structure in our universe allows us to probe alternatives to the cold dark matter paradigm. Strong gravitational lensing offers a unique window into small dark matter halos because these halos impart a gravitational lensing signal even if they do not host luminous galaxies. We create large datasets of strong lensing images with realistic low-mass halos, Hubble Space Telescope (HST) observational effects, and galaxy light from HST's COSMOS field. Using a simulation-based inference pipeline, we train a neural posterior estimator of the subhalo mass function (SHMF) and place constraints on populations of lenses generated using a separate set of galaxy sources. We find that by combining our network with a hierarchical inference framework, we can both reliably infer the SHMF across a variety of configurations and scale efficiently to populations with hundreds of lenses. By conducting precise inference on large and complex simulated datasets, our method lays a foundation for extracting dark matter constraints from the next generation of wide-field optical imaging surveys.
SPRING BREAK
Mar 1, 2022
Mila Chadayammuri (CfA), "The Importance of Being Interpretable: Toward An Understandable Machine Learning Encoder for Galaxy Cluster Cosmology", @ Zoom, at 5:00pm
Feb 15, 2022
Georges Obied, "A Tale of Two U(1)'s: Kinetic Mixing from Lattice WGC States", @ Zoom, at 5:00pm
Feb 1, 2022
Çağan Şengül, "Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy cluster" , https://arxiv.org/abs/2110.06232 @ Zoom, at 5:00pm
Dec 7, 2021
Prish Chakraborty , "The Information Content of Projected Galaxy Fields" , https://arxiv.org/abs/2111.13702 @ Zoom, at 5:0
Nov 23, 2021
Sihao Cheng (External Speaker from Johns Hopkins) presented:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.499.5902C/abstract
https://ui.adsabs.harvard.edu/abs/2021MNRAS.507.1012C/abstract
Abstract:
Patterns and complex textures are ubiquitous in astronomical data but challenging to quantify. I will present a new powerful statistic called the “scattering transform”. It borrows ideas from convolutional neural nets (CNNs) while retaining the advantages of traditional statistics. As an example, I will show its application to weak lensing cosmology, where it outperforms classic statistics and is on a par with CNNs. I will also show interesting visual interpretations of the scattering transform and its advantages for practical data analysis. I argue that the scattering transform provides a powerful new approach in cosmology and beyond.
Nov 9, 2021
Stephen Chen (External Speaker from Berkeley) presented his latest research:
Abstract:
Spectroscopic surveys are a powerful cosmological probe, encoding information about structure formation and the geometry of the universe in the 3D distribution of galaxies. Upcoming surveys like DESI, which will increase the number of measured galaxy redshifts by an order of magnitude, will test our ability to use this information while providing opportunities to test fundamental physics in unprecedented ways. In this talk I will discuss our recent work on a new method to combine the two main prongs of these surveys--redshift-space distortions and BAO--within the framework of Lagrangian perturbation theory. As an illustrative example, I will discuss the application of this method to data from the BOSS survey, obtaining cosmological constraints that are competitive but consistent with primary CMB and lensing measurements. I will also discuss future prospects for perturbation theory analyses of large-scale structure, for example by jointly analyzing spectroscopic and lensing surveys.
Oct 26, 2021
Ted Macioce (External Speaker from Caltech) presented his latest research on the kSZ effect:
Abstract:
Measuring the kinetic Sunyaev-Zel’dovich (kSZ) effect is a promising technique to constrain both cosmic growth and galaxy cluster formation. Detecting the kSZ effect in massive galaxy clusters will become increasingly feasible as millimeter-wave telescopes gain sensitivity and resolving power over multiple frequency bands. While such kSZ measurements will have unprecedented sensitivity, they will also be contaminated by emission from dusty star-forming galaxies, primary anisotropies of the cosmic microwave background (CMB), and the typically dominant thermal SZ signal, making analysis efforts difficult. Current kSZ forecasts account for these contaminants in a simplified way, relying on assumptions that may not apply in the high-resolution regime. Moreover, they typically use Fisher matrix analyses, which cannot give a fully accurate description of the degeneracies among the physical parameters describing the cluster. We present a new mock observation and analysis pipeline for kSZ images that uses more detailed noise models and more sophisticated analysis methods to extract peculiar velocities, temperatures, and optical depths more accurately. With these mock observations, we will inform the designs of next-generation millimeter telescopes targeting kSZ observations by identifying the optimal instrumentation choices for both cosmological and cluster-scale constraints. The software pipeline we develop will also be directly usable as an analysis tool once observations from such telescopes become available.
Oct 12, 2021
Arthur Tsang, Neural Physical Engines for Inferring the Halo Mass Distribution Function https://arxiv.org/abs/1909.06379. @ Zoom, at 5:0
Sep 28, 2021
Misha Rashkovetskyi , Small-scale Clumping at Recombination and the Hubble Tension https://arxiv.org/abs/2108.02747 . @ Zoom, at 5:0
Sep 14, 2021
Siddharth Mishra-Sharma, Inferring CDM Substructure Using Global Astrometry Beyond the Power Spectrum.https://arxiv.org/abs/2110.01620 @ Zoom, at 5:00
Apr 27, 2021
Nakai, Suzuki, Takahashi, Yamada, Gravitational Waves and Dark Radiation from Dark Phase Transition: Connecting NANOGrav Pulsar Timing Data and Hubble Tension, arxiv.org/2009.09754 (presented by Nick DePorzio) @ Zoom, at 5:00
Apr 13, 2021
SPIDER Collaboration, A Constraint on Primordial B-Modes from the First Flight of the SPIDER Balloon-Borne Telescope, arxiv.org/2103.13334 (presented by Jeffrey Filippini) @ Zoom, at 5:00
Mar 30, 2021
Chen, Lee, Dvorkin, Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra, arxiv.org/2103.01229 (presented by Shu-Fan Chen) @ Zoom, at 5:00
Mar 2, 2021
Denzel, Mukherjee, Saha, A new strategy for matching observed and simulated lensing galaxies, arxiv.org/2102.10114 (presented by Arthur Tsang) @ Zoom, at 5:00
Feb 16, 2021
Liu, Valogiannis, Battaglia, Bean, Constraints on f(R) and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering, arxiv.org/2101.08728 (presented by Georgios Valogiannis) @ Zoom, at 5:00
Feb 2, 2021
Minami, Komatsu, New Extraction of the Cosmic Birefringence from the Planck 2018 Polarisation Data, arxiv.org/2011.11254 (presented by Clara Vergès) @ Zoom, at 5:00
Jan 19, 2021
Jamieson, Loverde, Position-dependent Voronoi probability distribution functions for matter and halos, arxiv.org/2012.10508 (presented by Çağan Şengül) @ Zoom, at 5:00
Dec 15, 2020
Kannawadi, Rosenberg, Hoekstra, Mitigating the effects of undersampling in weak lensing shear estimation with metacalibration, arxiv.org/2010.04164 (presented by Arthur Tsang) @ Zoom, at 5:00
Dec 1, 2020
Lizancos, Challinor, Carron, Impact of internal-delensing biases on searches for primordial B-modes of CMB polarisation, arxiv.org/2007.01622 (presented by Anton Lizancos) @ Zoom, at 5:00
Oct 13, 2020
Boruah et al., Peculiar velocities in the local Universe: comparison of different models and the implications for Ho and dark matter, arxiv.org/2010.01119 (presented by Sasha Brownsberger) @ Zoom, at 5:00
Sep 29, 2020
Zelko, Finkbeiner, Implications of Grain Size Distribution and Composition for the Correlation Between Dust Extinction and Emissivity, arxiv.org/2009.11869 (presented by Ioana Zelko) @ Zoom, at 5:00
Sep 15, 2020
Meneghetti et al., An excess of small-scale gravitational lenses observed in galaxy clusters, arxiv.org/2009.04471 (presented by Ana Diaz Rivero) @ Zoom, at 5:00
Aug 4, 2020
Buch et al., Dark Matter Substructure under the Electron Scattering Lamppost, arxiv.org/2007.13750 (presented by Linda Xu) @ Zoom, at 4:00
Jul 24, 2020
eBOSS Collaboration, The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey, arxiv.org/2007.08991, 2007.08993, 2007.08994, 2007.08995 (presented by Nick DePorzio) @ Zoom, at 4:00
Jul 7, 2020
Cheng et al., Allys et al., A new approach to observational cosmology using the scattering transform, arxiv.org/2006.08561 and arxiv.org/2006.06298 (presented by Maya Burhanpurkar) @ Zoom, at 4:00
Jun 9, 2020
Domenech, Chen, Kamionkowski, Loeb, Lensing anomaly as a fingerprint of alternative scenarios to inflation, arXiv:2005.08998 (presented by Arthur Tsang) @ Zoom, at 4:00
May 12, 2020
Jedamzik, Pogosian, Relieving the Hubble Tension with Primordial Magnetic Fields, arXiv:2004.09487 (presented by Georges Obied) @ Zoom, at 5:30
Apr 28, 2020
Wu, Motloch, Raveri, Hubble constant tension between CMB lensing and BAO measurements, arXiv:2004.10207 (presented by Arthur Tsang) @ Zoom, at 5:30
Apr 14, 2020
Barreira, Cabass, Lozanov, Schmidt, Compensated Isocurvature Perturbations in the Galaxy Power Spectrum, arXiv:2002.12931 (presented by Shu-Fan Chen) @ Zoom, at 5:30
Mar 31, 2020
He, Ma, Zheng, Resolving Hubble Tension by Self-Interacting Neutrinos with Dirac Seesaw, arXiv:2003.12057 (presented by Nick DePorzio) @ Zoom, at 5:30
Mar 17, 2020
Pandey, Raveri, Jain, A model independent comparison of supernova and strong lensing cosmography: implications for the Hubble constant tension, arXiv:1912.04325 (presented by Ana Diaz) @ Zoom, at 5:30
Mar 3, 2020
List, Lewis, A unified framework for 21cm tomography sample generation and parameter inference with Progressively Growing GANs, arXiV:2002.07940 (presented by Julian Munoz) @ Lyman 330, at 5:30
Feb 18, 2020
Dai et al., Asymmetric Surface Brightness Structure of Lensed Arc in SDSS J1226+2152: A Case for Dark Matter Substructure, arXiV:2001.00261 (presented by Çağan Şengül) @ M-340, at 5:45
Feb 4, 2020
Ivanov, Simonovic, Zaldarriaga, Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data, arXiv:1912.08208 (presented by Hayden Lee) @ Lyman 330, at 5:30
Oct 29, 2019
Baushev, Pilipenko, The central cusps in dark matter halos: fact or fiction? arXiV:1808.03088 (presented by Çağan Şengül) @ M-340, at 5:45
Oct 22, 2019
Lin, Mack, Hou, Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model arXiV:1910.02978 (presented by Sasha Brownsberger) @ Lyman 330, at 5:30
Oct 1, 2019
Capparelli, Caldwell, Melchiorri, Cosmic Birefringence Test of the Hubble Tension, arXiV:1909.04621 (presented by Linda Xu) @ M-340, at 5:45
Sep 17, 2019
Brehmer, Mishra-Sharma, Hermans, Louppe, Cranmeri, Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning, arXiV:1909.02005 (presented by Arthur Tsang) @ Lyman 330
Sep 3, 2019
Jeong, Kamionkowski, Gravitational waves, CMB polarization, and the Hubble tension, arXiV:1908.06100 (presented by Benjamin Racine) @ 160 concord avenue, room M-340
May 28, 2019
Keck Array and BICEP2 Collaborations, BICEP2 / Keck Array XI: Beam Characterization and Temperature-to-Polarization Leakage in the BK15 Dataset, arXiV:1904.01640 (presented by Tyler St Germaine)
May 14, 2019
Alexander, Bramburger, Mc Donough, Dark Disk Substructure and Superfluid Dark Matter, arXiV:1901.03694 (presented by Evan McDonough)
May 7, 2019
Linde, On the problem of initial conditions for inflation, arXiV:1710.04278 (presented by Çağan Şengül, moved from April 30)
Apr 16, 2019
Li, Frenk, Cole, Wang, Gao, Projection effects in the strong lensing study of subhaloes, arXiV:1612.06227 (presented by Arthur Tsang)
Apr 2, 2019
Riess, Casertano, Yuan, Macri, Scolnic, Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM, arXiV:1903.07603 (presented by Linda Xu)
Mar 18, 2019
Special Monday Journal Club / Seminar: Philcox, Sherwin, van Engelen, Detection and Removal of CMB B-mode Dust Foregrounds with Signatures of Statistical Anisotropy, arXiV:1805.09177 (presented by Oliver Philcox in M-340 at 160 Concord Ave)
Mar 19, 2019
Yuan, Eisenstein, Decorrelating the errors of the galaxy correlation function with compact transformation matrices, arXiV:1901.05019 (presented by Sihan Yuan)
Mar 5, 2019
Coulton, Spergel : The bispectrum of polarized galactic foregrounds, arXiV:1901.04515 (presented by Ben Racine)
Feb 19, 2019
Ribli, Pataki, Matilla, Hsu, Haiman, Csabai: Weak lensing cosmology with convolutional neural networks on noisy data, arXiV: 1902.03663 (presented by Ana Diaz Rivero)
Feb 5, 2019
Madhavacheril, Battaglia, Smith, Sievers : Cosmology with kSZ: breaking the optical depth degeneracy with Fast Radio Bursts, arXiV:1901.02418 (presented by Nicholas DePorzio)
Jan 22, 2019
Raveri, Hu, Sethi : Swampland Conjectures and Late-Time Cosmology, arXiV:1812.10448 (presented by Georges Obied)
Nov 27, 2018
Poulin, Smith, Karwal, Kamionkowski: Early Dark Energy Can Resolve The Hubble Tension, arXiV:1811.04083 (presented by Linda Xu)
Nov 13, 2018
Hadzhiyska, Spergel, Dunkley: A Small-Scale Modification to the Lensing Kernel, arXiV:1711.03168
Hadzhiyska, Spergel: Measuring the Duration of Last Scattering, arXiV:1808.04083
(presented by Boryana Hadzhiyska)
Oct 30, 2018
Shanks, Hogarth, Metcalfe: GAIA Cepheid parallaxes and ‘Local Hole’ relieve H0 tension, arXiV:1810.02595
Riess, Casertano, Kenworthy, Scolnic, Macri: Seven Problems with the Claims Related to the Hubble Tension in arXiv:1810.02595, arXiV:1810.03526
Shanks, Hogarth, Metcalfe: H0 Tension: Response to Riess et al arXiv:1810.03526, arXiV:1810.07628
(presented by Ana Diaz Rivero)
Oct 16, 2018
Satoru Takakura et al, Measurements of tropospheric ice clouds with a ground-based CMB polarization experiment, POLARBEAR, arXiV:1809.06556 (presented by James Cornelison)
Oct 9, 2018
Bender, SPT collaboration, Year two instrument status of the SPT-3G cosmic microwave background receiver, arXiV:1809.00036 (presented by James Cornelison)
Jun 26, 2018
L. E. Ibanez, V. Martin-Lozano, I. Valenzuela, Constraining Neutrino Masses, the Cosmological Constant and BSM Physics from the Weak Gravity Conjecture, arXiV:1706.05392 (presented by Georges Obied)
May 15, 2018
Anna Ijjas & Paul J. Steinhardt, Bouncing Cosmology made simple, arXiV:1803.01961 (presented by Victor Buza)
May 1, 2018
Hongwan Liu: special Journal Club "seminar" about the recent Edges result: Too Hot, Too Cold or Just Right? Implications of a 21-cm Signal for Dark Matter Annihilation and Decay, arXiV:1803.09739
Apr 24, 2018
Duncan J. Watts et al, A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment’s Sample-Variance Limited E-Mode Measurement, arXiV:1801.01481 (presented by Lingzhen Zeng)
Apr 10, 2018
E. Castorina et al, Primordial non-Gaussianities and zero bias tracers of the Large Scale Structure, arXiV:1803.11539 (presented by Linda Xu)
Mar 27, 2018
M. Pospelov et al, New Physics in the Rayleigh-Jeans Tail of the CMB, arXiV:1803.07048 (presented by Julian Muñoz)
Feb 27, 2018
S. Vagnozzi et al, Constraints on the sum of the neutrino masses in dynamical dark energy models with w(z)≥−1 are tighter than those obtained in ΛCDM, arXiv:1801.08553 (presented by Ana Diaz Rivero)
Feb 13, 2018
N. Krachmalnicoff et al, The S-PASS view of polarized Galactic Synchrotron at 2.3 GHz as a contaminant to CMB observations, arXiv:1802.01145 (presented by Benjamin Racine)
Jan 30, 2018
Dizgah, Lee, Muñoz, Dvorkin, Galaxy Bispectrum from Massive Spinning Particles, arXiv:1801.07265 (presented by Azadeh Moradinezhad Dizgah)
Apr 19, 2017
TBD (presented by Tyler St. Germaine)
Apr 5, 2017
Abitbol, Hill, and Johnson, Foreground-Induced Biases in CMB Polarimeter Self-Calibration, arXiv:1512.06834 (presented by James Cornelison)
Mar 22, 2017
G. E. Addison , Y. Huang , D. J. Watts et al, Quantifying discordance in the 2015 Planck CMB spectrum, arXiv:1511.00055 (presented by Georges Obied)
Mar 8, 2017
J. Carron, A. Lewis, A. Challinor, Internal delensing of Planck CMB temperature and polarization, arXiv:1701.01712 (presented by Victor Buza)
Feb 22, 2017
A. Manzotti, K. T. Story, W. L. K. Wu et al, CMB Polarization B-mode Delensing with SPTpol and Herschel, arXiv:1701.04396 (presented by Kirit Karkare)
Feb 8, 2017
Nierenberg et al, Probing dark matter substructure in the gravitational lens HE0435-1223 with the WFC3 grism, arXiv:1701.05188 (presented by Ana Diaz Rivero)
Jan 25, 2017
Castorina et al, DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos, arXiv:1505.07148 (presented by Nina Maksimova)
Dec 14, 2016
M. Lewandowski, A. Maleknejad, L. Senatore, An effective description of dark matter and dark energy in the mildly non-linear regime, arXiv:1611.07966 (presented by Sruthi Narayanan)
Dec 7, 2016
Zheng et al, An Improved Model of Diffuse Galactic Radio Emission from 10 MHz to 5 THz, arXiv:1605.04920 (presented by Ioana Zelko)
Nov 9, 2016
A. Kogut, D.J. Fixsen, Foreground Bias From Parametric Models of Far-IR Dust Emission, arXiv:1607.02150 (presented by Tansu Daylan)
Oct 26, 2016
P. D. Meerburg, M. Munchmeyer, J. B. Munoz, X. Chen, Prospects for Cosmological Collider Physics, arXiv:1610.06559 (presented by Xingang Chen)
Oct 12, 2016
T. Louis et al, The Atacama Cosmology Telescope: two-season ACTPol spectra and parameters, arXiv:1610.02360 (presented by Victor Buza)
Sep 28, 2016
C. Heinrich, V. Miranda, W. Hu, Complete Reionization Constraints from Planck 2015 Polarization, arXiv:1609.04788 (presented by Georges Obied)
Sep 14, 2016
R. Caldwell, C. Hirata, M. Kamionkowski, Dust polarization and ISM turbulence, arXiv:1608.08138 (presented by Azadeh Moradinejad)
Related content
Copyright © 2024 The President and Fellows of Harvard College * Accessibility * Support * Request Access * Terms of Use