/
Past Papers

Past Papers

Feb 27, 2025

Feb 13, 2025

Jan 30, 2025

Dec 5, 2024

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  

Oct 10, 2024  

Sep 26, 2024  

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  

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 

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 

Nov 7, 2023 

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 

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

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

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

Nov 29, 2022

Nov 15, 2022

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

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

Apr 12, 2022

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 

 

Nov 23, 2021 

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 

Sep 28, 2021 

Sep 14, 2021 

Apr 27, 2021 

  • Nakai, Suzuki, Takahashi, Yamada, Gravitational Waves and Dark Radiation from Dark Phase Transition: Connecting NANOGrav Pulsar Timing Data and Hubble Tensionarxiv.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 Telescopearxiv.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 Bispectraarxiv.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 galaxiesarxiv.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 Clusteringarxiv.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 Dataarxiv.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 halosarxiv.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 metacalibrationarxiv.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 polarisationarxiv.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 matterarxiv.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 Emissivityarxiv.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 clustersarxiv.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 Lamppostarxiv.org/2007.13750 (presented by Linda Xu) @ Zoom, at 4:00

Jul 24, 2020

Jul 7, 2020 

  • Cheng et al., Allys et al., A new approach to observational cosmology using the scattering transformarxiv.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 inflationarXiv:2005.08998 (presented by Arthur Tsang) @ Zoom, at 4:00

May 12, 2020 

  • Jedamzik, Pogosian, Relieving the Hubble Tension with Primordial Magnetic FieldsarXiv:2004.09487 (presented by Georges Obied) @ Zoom, at 5:30

Apr 28, 2020 

  • Wu, Motloch, Raveri, Hubble constant tension between CMB lensing and BAO measurementsarXiv:2004.10207 (presented by Arthur Tsang) @ Zoom, at 5:30

Apr 14, 2020 

  • Barreira, Cabass, Lozanov, Schmidt, Compensated Isocurvature Perturbations in the Galaxy Power SpectrumarXiv: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 SeesawarXiv: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 tensionarXiv: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 TensionarXiV: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 learningarXiV:1909.02005 (presented by Arthur Tsang) @ Lyman 330

Sep 3, 2019

  • Jeong, Kamionkowski, Gravitational waves, CMB polarization, and the Hubble tensionarXiV: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 DatasetarXiV:1904.01640 (presented by Tyler St Germaine)

May 14, 2019

  • Alexander, Bramburger, Mc Donough, Dark Disk Substructure and Superfluid Dark MatterarXiV:1901.03694 (presented by Evan McDonough)

May 7, 2019

  • Linde, On the problem of initial conditions for inflationarXiV: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 subhaloesarXiV: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 LambdaCDMarXiV: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 AnisotropyarXiV: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 matricesarXiV:1901.05019 (presented by Sihan Yuan)

Mar 5, 2019

  • Coulton, Spergel : The bispectrum of polarized galactic foregroundsarXiV:1901.04515 (presented by Ben Racine)

Feb 19, 2019

  • Ribli, Pataki, Matilla, Hsu, Haiman, Csabai: Weak lensing cosmology with convolutional neural networks on noisy dataarXiV: 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 BurstsarXiV:1901.02418  (presented by Nicholas DePorzio)

Jan 22, 2019

  • Raveri, Hu, Sethi : Swampland Conjectures and Late-Time CosmologyarXiV:1812.10448  (presented by Georges Obied)

Nov 27, 2018

  • Poulin, Smith, Karwal, Kamionkowski: Early Dark Energy Can Resolve The Hubble TensionarXiV: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, POLARBEARarXiV:1809.06556 (presented by James Cornelison)

Oct 9, 2018

  • Bender, SPT collaboration, Year two instrument status of the SPT-3G cosmic microwave background receiverarXiV: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 simplearXiV: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 DecayarXiV: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 StructurearXiV:1803.11539  (presented by Linda Xu)

Mar 27, 2018

  • M. Pospelov et al, New Physics in the Rayleigh-Jeans Tail of the CMBarXiV: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 ParticlesarXiv: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-CalibrationarXiv: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 spectrumarXiv:1511.00055 (presented by Georges Obied)

Mar 8, 2017

  • J. Carron, A. Lewis, A. Challinor, Internal delensing of Planck CMB temperature and polarizationarXiv: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 HerschelarXiv: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 grismarXiv: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 neutrinosarXiv: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 regimearXiv: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 THzarXiv:1605.04920 (presented by Ioana Zelko)

Nov 9, 2016

  • A. Kogut, D.J. Fixsen, Foreground Bias From Parametric Models of Far-IR Dust EmissionarXiv:1607.02150 (presented by Tansu Daylan)

Oct 26, 2016

  • P. D. Meerburg, M. Munchmeyer, J. B. Munoz, X. Chen, Prospects for Cosmological Collider PhysicsarXiv:1610.06559 (presented by Xingang Chen)

Oct 12, 2016

  • T. Louis et al, The Atacama Cosmology Telescope: two-season ACTPol spectra and parametersarXiv:1610.02360 (presented by Victor Buza)

Sep 28, 2016

  • C. Heinrich, V. Miranda, W. Hu, Complete Reionization Constraints from Planck 2015 PolarizationarXiv:1609.04788 (presented by Georges Obied)

Sep 14, 2016

  • R. Caldwell, C. Hirata, M. Kamionkowski, Dust polarization and ISM turbulencearXiv:1608.08138 (presented by Azadeh Moradinejad)

Related content

New Paper Suggestions
New Paper Suggestions
More like this
Cosmology Journal Club Home
Cosmology Journal Club Home
More like this
PSF to Cosmology projects
PSF to Cosmology projects
More like this
Weekly Group Meeting schedule
Weekly Group Meeting schedule
More like this
DOE proposal 2020
DOE proposal 2020
More like this
LIGO galaxy catalog
LIGO galaxy catalog
More like this

Copyright © 2024 The President and Fellows of Harvard College * Accessibility * Support * Request Access * Terms of Use