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Journal Club

The Cosmology Journal Club is a series of weekly informal discussions by faculty, postdocs and graduate students of recent papers published or posted on the arXiv.  The scope is meant to be very broad but the papers should somehow be related to cosmology.  We are hoping theorists, experimentalists and observers from both the Physics and the Astronomy Departments will drop by.

Each volunteer should present a paper very briefly (~5 min), and then the rest can weigh in with comments, questions and complaints (~5 min).  The goal is to keep the entire process very informal.  Our plan is to post on this web page the papers to be discussed a few days beforehand so participants can read through them if they want.  Last-minute suggestions are welcome.

The Journal Club is held every Monday (unless otherwise noted) from 12:30 - 1:30.  Please feel free to bring along your lunch.  It takes place in 5242 Chamberlin Hall. All Faculty, postdocs, researchers, graduate and undergraduate students with an interest in Cosmology and Astrophysics are welcome to listen, suggest and present!

If you have questions or comments about this Journal Club, would like to propose a topic or volunteer to introduce a paper, please email Hojin Yoo(hyoo6@wisc.edu) . 

Upcoming Papers

2013

May.06 - August.31

Summer Break

Previous Papers

2013

May.06

  • New Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IGM at z=7.7 arXiv:1304.4991
  • Primordial Non-Gaussianity and Reionization arXiv:1304.8049
  • Apr.29

  • Dark Matter Search Results Using the Silicon Detectors of CDMS II arXiv:1304.4279
  • Low-Mass Dark-Matter Hint from CDMS II, Higgs Boson at LHC, and Darkon Models arXiv:1304.6058
  • The unbearable lightness of being: CDMS versus XENON arXiv:1304.6066
  • Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure arXiv:1304.6984
  • Apr.22

  • Planck 2013 results support the simplest cyclic models arXiv:1304.3122
  • Apr.15

  • First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5-350 GeV PRL 110, 141102 (2013)
  • A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy arXiv:1301.0446
  • A kinematic study of the Andromeda dwarf spheroidal system arXiv:1302.6590
  • Inflationary paradigm in trouble after Planck2013arXiv:1304.2785
  • Apr.8

  • Planck 2013 results. XVI. Cosmological parameters arXiv:1303.5076
  • Planck 2013 results. XV. CMB power spectra and likelihood arXiv:1303.5075
  • and additional 26 Planck papers...(volunteers are welcome) arXiv:planck2013
  • The Origin of the WMAP Quadrupole arXiv:1003.1073
  • Improved CMB Map from WMAP Data arXiv:0907.2731
  • Apr.1

    Cancelled (NOT a joke on April Fools'day!!!)

    Mar.18

  • Scintillation of Liquid Helium for Low-Energy Nuclear Recoils arXiv:1303.3858v1
  • Bayesian analysis of anisotropic cosmologies: Bianchi VIIh and WMAP arXiv:1303.3409
  • Double-Disk Dark Matter arXiv:1303.1521v1
  • Mar.11

  • Limits on spin-independent couplings of WIMP dark matter with a p-type point-contact germanium detector arXiv:1303.0925
  • Precise Measurements of Primordial Power Spectrum with 21 cm Fluctuations arXiv:1303.1688
  • Why multi-tracer surveys beat cosmic variance arXiv:1302.5444
  • Mar.4

  • Two Emission Mechanisms in the Fermi Bubbles: A Possible Signal of Annihilating Dark Matter arXiv:1302.6589
  • THE FUNDAMENTAL MULTI-BASELINE MODE-MIXING FOREGROUND IN 21 CM EOR OBSERVATIONS arXiv:1301.3126
  • A Concept for A Dark Matter Detector Using Liquid Helium-4 arXiv:1302.0534
  • Feb.25

  • Perturbed Recombination from Dark Matter AnnihilationarXiv:1302.4753
  • Seeking Inflation Fossils in the Cosmic Microwave Background arXiv:1302.1868
  • Feb.18

  • Seeking Inflation Fossils in the Cosmic Microwave Background arXiv:1302.1868
  • Laboratory search for a quintessence field arXiv:1302.1579
  • Feb.11

  • Searching for Spurious Solar and Sky Lines in the Fermi-LAT Spectrum arXiv:1302.0427
  • Cosmological Parameters from Pre-Planck CMB Measurements arXiv:1302.1841
  • A Brief History of Curvature arXiv:1302.1201v1
  • All-Sky Interferometry with Spherical Harmonic Transit Telescopes arXiv:1302.0327
  • Feb.04

  • The Galactic Wind Haze and its gamma-spectrum arXiv:1301.4405v1
  • OPENING THE 21CM EOR WINDOW: MEASUREMENTS OF FOREGROUND ISOLATION WITH PAPER arXiv:1301.7099v1
  • Density Profiles of CDM Microhalos and their Implications for Annihilation Boost Factors arXiv:1302.0003
  • Jan.28

  • Low energy cosmic ray positron fraction explained by charge-sign dependent solar modulation arXiv:1211.6905
  • A refined foreground-corrected limit on the HI power spectrum at z = 8.6 from the GMRT Epoch of Reionization Experiment arXiv:1301.5906
  • Violation of non-Gaussianity consistency relation in a single field inflationary model arXiv:1210.3692
  • Jan.18

  • Extremely metal-poor gas at a redshift of 7 arXiv:1212.0548
  • COMPRESSED SENSING FOR APERTURE SYNTHESIS IMAGING http://www.ece.ucsb.edu/~psen/Papers/ICIP10_ApertureSynthesisImaging.pdf
  • XMASS detector arXiv:1301.2815
  • Light WIMP search in XMASS arXiv:1211.5404
  • Jan.11

  • Is a tabletop search for Planck scale signals feasible? arXiv:1211.3816v2
  • The Atacama Cosmology Telescope: Temperature and Gravitational Lensing Power Spectrum Measurements from Three Seasons of Data arXiv:1301.1037
  • Solving Large Scale Structure in Ten Easy Steps with COLA arXiv:1301.0322
  • Jan.18

  • Extremely metal-poor gas at a redshift of 7 arXiv:1212.0548
  • COMPRESSED SENSING FOR APERTURE SYNTHESIS IMAGING http://www.ece.ucsb.edu/~psen/Papers/ICIP10_ApertureSynthesisImaging.pdf
  • XMASS detector arXiv:1301.2815
  • Light WIMP search in XMASS arXiv:1211.5404
  • 2012

    Jan.04

  • Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results arXiv:1212.5226
  • Sparsely Sampling the Sky: A Bayesian Experimental Design Approach arXiv:1212.3194
  • Is a tabletop search for Planck scale signals feasible? arXiv:1211.3816v2
  • A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey arXiv:1210.7231
  • Dec.14

  • Identifying Ionized Regions in Noisy Redshifted 21 cm Data Sets arXiv:1212.2656
  • Dark Radiation and Decaying Matter arXiv:1212.1472v1
  • THE ABUNDANCE OF STAR-FORMING GALAXIES IN THE REDSHIFT RANGE 8.5 TO 12: NEW RESULTS FROM THE 2012 HUBBLE ULTRA DEEP FIELD CAMPAIGN arXiv:1211.6804v1
  • Dec.07

  • Will Nonlinear Peculiar Velocity and Inhomogeneous Reionization Spoil 21cm Cosmology from the Epoch of Reionization? arXiv:1211.2036
  • Self-Calibration of CMB Polarization Experiments arXiv:1211.5734
  • Search for ultra high energy cosmic ray sources. FRI radio galaxy Centaurus A arXiv:1212.1402
  • Equivalence Principle Violation in Weakly Vainshtein-Screened Systems arXiv:1212.0831
  • Nov.30

  • Global 21cm signal experiments: a designer's guide arXiv:1211.3743
  • Astrophysical searches for a hidden-photon signal in the radio regime arXiv:1211.6268v1
  • Nov.16

  • A Fast Method for Power Spectrum and Foreground Analysis for 21 cm Cosmology arXiv:1211.2232
  • Search for Gamma-ray Spectral Lines in the Milky Way Diffuse with the Fermi Large Area Telescope ppt, blog
  • Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz arXiv:1112.5004
  • Testing standard and non-standard neutrino physics with cosmological data arXiv:1211.2154v1
  • Nov.09

  • Direct detection of self-interacting dark matter arXiv:1211.1377
  • Cross-correlations as a carbon monoxide detector arXiv:1211.1397
  • Nov.02

  • Near-infrared background anisotropies from diffuse intrahalo light of galaxies arXiv:1210.6031
  • The Imprint of the Extragalactic Background Light in the Gamma-Ray Spectra of Blazars Science DOI: 10.1126/science.1227160
  • Celestial Ephemerides in an Expanding Universe arXiv:1207.3873
  • Oct.26

  • SPTpol: an instrument for CMB polarization measurements with the South Pole Telescope arXiv:1210.4970
  • Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies arXiv:1210.4562
  • CMB constraints on light dark matter candidates arXiv:1210.6845
  • Oct.19

  • Do the Herschel cold clouds in the Galactic halo embody its dark matter? arXiv:1210.0489
  • Testing MOND Over a Wide Acceleration Range in X-Ray Ellipticals arXiv:1205.1308
  • Oct.12

  • A Sensitivity and Array-Configuration Study for Measuring the Power Spectrum of 21cm Emission from Reionization, arXiv:1103.2135
  • The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts, arXiv:1210.2413
  • Characterizing Foreground for redshifted 21-cm radiation: 150 MHz GMRT observations, arXiv:1208.1617
  • THE IMPACT OF THE SUPERSONIC BARYON-DARK MATTER VELOCITY DIFFERENCE ON THE Z~20 21CM BACKGROUND, arXiv:1204.1345
  • CMB Power Asymmetry from Non-Gaussian Modulation, arXiv:1210.2965
  • Oct.05

  • CONSTRAINTS ON DARK MATTER ANNIHILATION IN CLUSTERS OF GALAXIES FROM DIFFUSE RADIO EMISSION, arXiv:1210.0872
  • Reionization and the Cosmic Dawn with the Square Kilometre Array, arXiv:1210.0197
  • THE FORMATION OF THE FIRST COSMIC STRUCTURES AND THE PHYSICS OF THE Z~20 UNIVERSE, arXiv:1204.1344
  • Sep.28

  • Constraints on the Shape of the Milky Way Dark Matter Halo from Jeans Equations Applied to SDSS Data, arXiv:1209.2708
  • The effect of massive neutrinos on the matter power spectrum, arXiv:1006.0689
  • Fermi-LAT gamma-ray signal from Earth Limb, systematic detector effects and their implications for the 130 GeV gamma-ray excess, arXiv:1209.4548
  • Is the 130 GeV Line Real? A Search for Systematics in the Fermi-LAT Data, arXiv:1209.4562
  • Sep.21

  • THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III, arXiv:1208.0022
  • The large-scale cross-correlation of Damped Lyman Alpha Systems with the Lyman Alpha Forest: First Measurements from BOSS, arXiv:1209.4596
  • Foreground Removal using fastica: A Showcase of LOFAR-EoR, arXiv:1201.2190
  • CMB power spectrum parameter degeneracies in the era of precision cosmology, arXiv:1201.3654
  • Sep.14

  • The 21cm forest in the diffuse IGM as seen by LOFAR, arXiv:1209.2615
  • Dark energy fifth forces in torsion pendulum experiments, arXiv:1209.0211
  • GRAVITATIONAL FIELD EQUATIONS AND THEORY OF DARK MATTER AND DARK ENERGY, arXiv:1206.5078
  • Sep.07

  • Measuring neutrino masses with a future galaxy survey, arXiv:1209.1043
  • Measurement of 21 cm brightness fluctuations at z~0.8 in cross-correlation, arXiv:1208.0331
  • HI intensity mapping : a single dish approach, arXiv:1209.0343
  • Aug.3

  • Dark Matter Results from 225 Live Days of XENON100 Data, arXiv:1207.5988
  • DOUBLE GAMMA-RAY LINES FROM UNASSOCIATED FERMI-LAT SOURCES, arXiv:1207.7060v1
  • Theoretical bounds on the tensor-to-scalar ratio, arXiv:1208.0210
  • Revealing Cosmic Rotation, arXiv:1207.6640
  • Jul.27

  • Handedness asymmetry of spiral galaxies with z<0.3 shows cosmic parity violation and a dipole axis, arXiv:1207.5464v1
  • Detection of a Gamma-Ray Source in the Galactic Center Consistent with Extended Emission from Dark Matter Annihilation and Concentrated Astrophysical Emission, arXiv:1207.6047
  • First constraints on the running of non-Gaussianity, arXiv:1207.5788
  • Jul.20

  • An evidence for indirect detection of dark matter from galaxy clusters in Fermi-LAT data, arXiv:1207.4466
  • The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies, arXiv:1206.6945
  • Detection of dark galaxies and circum-galactic filaments fluorescently illuminated by a quasar at z=2.4, arXiv:1204.5753
  • Cosmic Tides, arXiv:1202.5804
  • Jul.13

  • The unusual smoothness of the extragalactic unresolved radio background, arXiv:1207.0856
  • A filament of dark matter between two clusters of galaxies, arXiv:1207.0809
  • By Dawn's Early Light: CMB Polarization Impact on Cosmological Constraints, arXiv:1207.1105
  • Jul.06

  • New Dark Matter Detectors using DNA for Nanometer Tracking, arXiv:1206.6809
  • The unusual smoothness of the extragalactic unresolved radio background, arXiv:1207.0856
  • Is a co-rotating Dark Disk a threat to Dark Matter Directional Detection ?, arXiv:1207.1050
  • Jun.22

  • Force-Free Gravitational Redshift: Proposed Gravitational Aharonov-Bohm experiment, arXiv:1109.4887
  • The Fast Fourier Transform Telescope, arXiv:0805.4414
  • Stable bounce and inflation in non-local higher derivative cosmology, arXiv:1206.6374
  • Jun.22

  • Prospects for weak lensing studies with new radio telescopes, arXiv:1206.4437
  • On the Use of Ly-alpha Emitters as Probes of Reionization, arXiv:1206.4028
  • Determination of neutrino mass hierarchy by 21 cm line and CMB B-mode polarization observations, arXiv:1205.5223
  • Jun.15

  • Strong Evidence for Gamma-ray Lines from the Inner Galaxy, arXiv:1206.1616
  • Jun.08

  • Optical Intensity Interferometry with the Cherenkov Telescope Array, arXiv:1204.3624
  • The 21cm radiation from minihalos as a probe of small primordial non-Gaussianity, arXiv:1205.6799
  • On the local dark matter density, arXiv:1205.4033v1
  • Kinematical and chemical vertical structure of the Galactic thick disk II. A lack of dark matter in the solar neighborhood, arXiv:1204.3924v1
  • Intensity Mapping with the 21-cm and Lyman Alpha Lines, arXiv:1206.0143v1
  • May.11

  • A closer look at CMB constraints on WIMP dark matter, arXiv:1201.3939
  • Influence of synchrotron self-absorption on the 21cm experiments, arXiv:1205.1113
  • Do we have a Theory of Early Universe Cosmology?, arXiv:1204.6108
  • May.04

  • GAMMA-RAY LINES IN THE FERMI DATA: IS IT A BUBBLE?, arXiv:1204.6047
  • CMB polarization anisotropies from cosmological reionization: extension to B-modes, arXiv:1205.0463
  • Apr.27

  • No evidence of dark matter in the solar neighborhood, arXiv:1204.3919
  • Galileons on Trial, arXiv:1204.4314
  • An absence of neutrinos associated with cosmic-ray acceleration in gamma-ray bursts, Nature (19 April 2012)
  • Apr.20

  • An absence of neutrinos associated with cosmic-ray acceleration in gamma-ray bursts, Nature (19 April 2012)
  • Optical Intensity Interferometry with the Cherenkov Telescope Array , arXiv:1204.3624
  • Apr.13

  • The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function, arXiv:1203.6616
  • The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample, arXiv:1203.6594
  • The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of potential systematics, arXiv:1203.6499
  • A Tentative Gamma-Ray Line from Dark Matter Annihilation at the Fermi Large Area Telescope, arXiv:1204.2797
  • Mar.30

  • Detection of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel'dovich Effect, arXiv:1203.4219
  • The Optimal Cosmic Epoch for Precision Cosmology, arXiv:1203.2622
  • Quantum Gravity Constraints on Inflation, arXiv:1203.5476
  • Mar.23

  • The Missing Massive Satellites of the Milky Way, arXiv:1203.4097
  • Spatial Curvature Falsifies Eternal Inflation, arXiv:1202.5037
  • Mar.16

    This week's meeting cancelled!!!

    Mar.9

  • Relic gravitational waves from light primordial black holes, arXiv:1105.2303
  • Cosmological Constant: A Lesson from Bose-Einstein Condensates, PRL
  • Mar.2

  • Cosmology without cosmic variance, arXiv:1104.3862
  • A new probe of the small-scale primordial power spectrum: astrometric microlensing by ultracompact minihalos, arXiv:1202.1284
  • Feb.24

  • A closer look at CMB constraints on WIMP dark matter, arXiv:1201.3939
  • Axion Dark Matter and Cosmological Parameters,PRL.
  • Feb.17

  • Dark Matter Detection with Polarized Detectors, arXiv:1202.1807
  • Generating zeta with non-Abelian Vector Fields, arXiv:1202.3133
  • Feb.10

  • Observational Probes of Cosmic Acceleration, arXiv:1201.2434
  • Bayesian power spectrum analysis of interferometric data, arXiv:1109.4640
  • Feb.03

  • Gravitational detection of a low-mass dark satellite at cosmological distance, arXiv:1201.3643
  • Observational Consequences of Dark Energy Decay, arXiv:1202.0107
  • CMB at 2x2 order: The dissipation of primordial acoustic waves and the observable part of the associated energy release, arXiv:1202.0057
  • A New Window on Primordial non-Gaussianity, arXiv:1201.5375
  • Jan. 27

  • The Empirical Case For 10 GeV Dark Matter, arXiv:1201.1303
  • Cosmological CPT Violation and CMB Polarization Measurements, arXiv:1201.4457
  • 2011

    Dec. 2

  • Non-Thermal Dark Matter Mimicing An Additional Neutrino Species In The Early Universe, arXiv:1111.6599
  • Searching for hidden mirror symmetries in CMB fluctuations from WMAP 7 year maps, arXiv:1111.5362
  • The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations, arXiv:1108.2635
  • 2011

    Nov. 18

  • Detection of Pristine Gas Two Billion Years After the Big Bang, sciencexpress
  • MIMAC: A micro-tpc matrix project for directional detection of dark matter, arXiv:1111.1566
  • Reconstruction of Gravitational Lensing Using WMAP 7-Year Data, arXiv:1111.2371
  • Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB, arXiv:1111.2544
  • Nov. 11

  • MIMAC: A micro-tpc matrix project for directional detection of dark matter, arXiv:1111.1566
  • Neutrino mass in cosmology: status and prospects, arXiv:1111.1436
  • Effect of Population III Multiplicity on Dark Star Formation, arXiv:1111.1527
  • Nov. 4

  • The Directional Dark Matter Detector, arXiv:1110.3401v1
  • A measurement of secondary cosmic microwave background anisotropies with two years of South Pole Telescope observations, arXiv:1111.0932
  • Bayesian Cluster Finder: Clusters in the CFHTLS Archive Research Survey, arXiv:1111.0013
  • Re-ionizing the Universe without Stars, arXiv:1106.5546v2
  • Oct. 28

  • The Directional Dark Matter Detector, arXiv:1110.3401v1
  • Analysis of WMAP 7-year Temperature Data: Astrophysics of the Galactic Haze, arXiv:1110.5418
  • Toward A Consistent Picture For CRESST, CoGeNT and DAMA, arXiv:1110.5338
  • Oct. 21

  • (Mis-)Interpreting supernovae observations in a lumpy universe, arXiv:1109.2484
  • Systematics in lensing reconstruction: Dark matter rings in the sky? arXiv:1110.3979
  • Prospects for determination of thermal history after inflation with future gravitational wave detectors,arXiv:1110.4169
  • Oct. 14

  • Cosmological Measurements with Forthcoming Radio Continuum Surveys, arXiv:1108.0930v1
  • The TIANSHAN Radio Experiment for Neutrino Detection, arXiv:1007.4359v3
  • Oct. 07

  • Precision cosmography with stacked voids, arXiv:1110.0345
  • Dark Matter implications of the Fermi-LAT measurement of anisotropies in the diffuse gamma-ray background: status report, arXiv:1110.0324
  • Does Bose-Einstein condensation of CMB photons cancel #distortions created by dissipation of sound waves in the early Universe?, arXiv:1110.0475
  • Sep. 30

    Sep. 23

    • Measurement of the neutrino velocity with the OPERA detector in the CNGS beam, arXiv:1109.4897
    • Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements, arXiv:1105.0419
    • Detection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope, arXiv:1103.2124

    Sep. 16

    • Results from 730 kg days of the CRESST-II Dark Matter Search, arXiv:1109.0702
    • Intensity Mapping with Carbon Monoxide Emission Lines and the Redshifted 21 cm Line, arXiv:1104.4800

     

     

     

     


    Last updated: 09/07/2011
     

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