|
[0710.3588] A Comparison of Weak Lensing Measurements From Ground- and Space-Based Facilities
arxiv.org/abs/0710.3588 A Comparison of Weak Lensing Measurements From Ground- and Space-Based Facilities[0710.3586] Baryon oscillations in galaxy and matter power-spectrum covariance matrices
arxiv.org/abs/0710.3586 Baryon oscillations in galaxy and matter power-spectrum covariance matrices[0710.2371] Probing Non-Gaussianity In The Cosmic Microwave Background Anisotropies: One Point
arxiv.org/abs/0710.2371 Probing Non-Gaussianity In The Cosmic Microwave Background Anisotropies: One Point Distribution Function[0710.2262] A Method for Weak Lensing Flexion Analysis by the HOLICs Moment Approach
arxiv.org/abs/0710.2262 A Method for Weak Lensing Flexion Analysis by the HOLICs Moment ApproachAuthors:
Yuki Okura (1),
Keiichi Umetsu (2),
Toshifumi Futamase (1) ((1) Tohoku University, (2) ASIAA)
Precision of diffuse 21-cm lensingAuthors:
Tingting Lu (1),
Ue-Li Pen (2) ((1) Department of Astronomy and Astrophysics, University of Toronto, (2) CITA, University of Toronto) [0710.1198] Signature of the interaction between dark energy and dark matter in galaxy clusters
arxiv.org/abs/0710.1198 Signature of the interaction between dark energy and dark matter in galaxy clusters[0710.0373] To Bin or Not To Bin: Decorrelating the Cosmic Equation of State
arxiv.org/abs/0710.0373 To Bin or Not To Bin: Decorrelating the Cosmic Equation of State[0710.0440] The prospects for constraining dark energy with future X-ray cluster gas mass fraction
arxiv.org/abs/0710.0440 The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements[0709.4294] New constraints on dark energy from the observed growth of the most X-ray luminous
arxiv.org/abs/0709.4294 New constraints on dark energy from the observed growth of the most X-ray luminous galaxy clustersAuthors:
A. Mantz (1),
S. W. Allen (1),
H. Ebeling (2),
D. Rapetti (1) ((1) KIPAC, Stanford, (2) IfA, Hawaii) [0709.4029] Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain
arxiv.org/abs/0709.4029 Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark EnergyAuthors:
Andrew R. Zentner (University of Pittsburgh),
Douglas H. Rudd (University of Chicago),
Wayne Hu (University of Chicago) Baryon Acoustic Oscillation Intensity Mapping of Dark Energy[0709.3470] Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic mo
arxiv.org/abs/0709.3470 Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic modelsAuthors:
Geraint Harker (1,2),
Shaun Cole (1),
Adrian Jenkins (1) ((1) Durham University, (2) Kapteyn Institute) Photometric Redshifts and Photometry Errors[0709.2955] Baryonic Acoustic Oscillations in 21cm Emission: A Probe of Dark Energy out to High Reds
arxiv.org/abs/0709.2955 Baryonic Acoustic Oscillations in 21cm Emission: A Probe of Dark Energy out to High Redshifts[0709.2871] Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy Studies
arxiv.org/abs/0709.2871 Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy StudiesOn the Magnitude of Dark Energy Voids and Overdensities[0709.1692] Precision photometric redshift calibration for galaxy-galaxy weak lensing
arxiv.org/abs/0709.1692 Precision photometric redshift calibration for galaxy-galaxy weak lensingAuthors:
R. Mandelbaum,
U. Seljak,
C. M. Hirata,
S. Bardelli,
M. Bolzonella,
A. Bongiorno,
M. Carollo,
T. Contini,
B. Garilli,
A. Iovino,
P. Kampzcyk,
J.-P. Kneib,
C. Knobel,
D. C. Koo,
F. Lamareille,
O. Le Fevre,
J.-F. Leborgne,
S. J. Lilly,
C. Maier,
V. Mainieri,
M. Mignoli,
J. A. Newman,
P. A. Oesch,
E. Perez-Montero,
E. Ricciardelli,
M. Scodeggio,
J. Silverman,
L. Tasca
Weak lensing ellipticities in a strong lensing regime[0709.1159] Cross-correlation Weak Lensing of SDSS galaxy Clusters II: Cluster Density Profiles and
arxiv.org/abs/0709.1159 Cross-correlation Weak Lensing of SDSS galaxy Clusters II: Cluster Density Profiles and the Mass--Richness RelationBeyond two dark energy parametersAuthors:
Scott Sullivan (1),
Devdeep Sarkar (1),
Shahab Joudaki (1),
Alexandre Amblard (1),
Daniel Holz (2),
Asantha Cooray (1) ((1) UC Irvine, (2) LANL) Adiabatic instability in coupled dark energy-dark matter modelsDetecting Cosmic Strings in the CMB with the Canny AlgorithmWeak lensing goes bananas: What flexion really measures[0709.1106] Quantifying the Cosmic Web I: The large-scale halo ellipticity-ellipticity and elliptici
arxiv.org/abs/0709.1106 Quantifying the Cosmic Web I: The large-scale halo ellipticity-ellipticity and ellipticity-direction correlationsNeutrino Mass, Dark Energy, and the Linear Growth Factor[0708.4125] Comparing cosmic shear measures - Optimizing the Information content of cosmic shear dat
arxiv.org/abs/0708.4125 Comparing cosmic shear measures - Optimizing the Information content of cosmic shear data vectorsOn cosmological observables in a swiss-cheese universe[0704.3800] CMB polarization power spectra contributions from a network of cosmic strings
arxiv.org/abs/0704.3800 CMB polarization power spectra contributions from a network of cosmic strings[0708.3786] Temperature and Polarization CMB Maps from Primordial non-Gaussianities of the Local Typ
arxiv.org/abs/0708.3786 Temperature and Polarization CMB Maps from Primordial non-Gaussianities of the Local Type[0708.2989] Fast optimal CMB power spectrum estimation with Hamiltonian sampling
arxiv.org/abs/0708.2989 Fast optimal CMB power spectrum estimation with Hamiltonian samplingUsing Local Volume data to constrain Dark Matter dynamicsAuthors:
G. Lavaux (1),
R. Mohayaee (1),
S. Colombi (1),
R. B. Tully (2) ((1) IAP / Univ. Paris 6, (2) IfA, Univ. of Hawaii)
[0708.2340] Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fi
arxiv.org/abs/0708.2340 Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm[0708.1793] A sub-horizon framework for probing the relationship between the cosmological matter dis
arxiv.org/abs/0708.1793 A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations[0708.1367] A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
arxiv.org/abs/0708.1367 A Closure Theory for Non-linear Evolution of Cosmological Power Spectra[0708.1162] Small-Angle CMB Temperature Anisotropies Induced by Cosmic Strings
arxiv.org/abs/0708.1162 Small-Angle CMB Temperature Anisotropies Induced by Cosmic StringsAuthors:
Aurélien A. Fraisse (Princeton),
Christophe Ringeval (Louvain),
David N. Spergel (Princeton),
François R. Bouchet (IAP) [0708.0825] The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from th
arxiv.org/abs/0708.0825 The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from the Third Data Release Quasar Lens CatalogAuthors:
Masamune Oguri,
Naohisa Inada,
Michael A. Strauss,
Christopher S. Kochanek,
Gordon T. Richards,
Donald P. Schneider,
Robert H. Becker,
Masataka Fukugita,
Michael D. Gregg,
Patrick B. Hall,
Joseph F. Hennawi,
David E. Johnston,
Issha Kayo,
Charles R. Keeton,
Bartosz Pindor,
Min-Su Shin,
Edwin L. Turner,
Richard L. White,
Donald G. York,
Scott F. Anderson,
Neta A. Bahcall,
Robert J. Brunner,
Scott Burles,
Francisco J. Castander,
Kuenley Chiu,
Alejandro Clocchiatti,
Daniel Eisenstein,
Joshua A. Frieman,
Yozo Kawano,
Robert Lupton,
Tomoki Morokuma,
Hans-Walter Rix,
Ryan Scranton,
Erin Scott Sheldon Constraining Dark Energy Anisotropic Stress[0708.0387] Analysis of two-point statistics of cosmic shear: III. Covariances of shear measures mad
arxiv.org/abs/0708.0387 Analysis of two-point statistics of cosmic shear: III. Covariances of shear measures made easyAuthors:
B. Joachimi,
P. Schneider,
T. Eifler (Argelander-Institut für Astronomie, Universität Bonn) [0707.2968] Structure and evolution of Zel'dovich pancakes as probes of dark energy models
arxiv.org/abs/0707.2968 Structure and evolution of Zel'dovich pancakes as probes of dark energy modelsMicrolensing by Cosmic StringsAuthors:
Konrad Kuijken (1),
Xavier Siemens (2,3),
Tanmay Vachaspati (4) ((1) Leiden Observatory, Leiden University (2) LIGO Laboratory, CalTech (3) Theoretical Astrophysics, CalTech (4) CERCA, Dept of Physics, Case Western Reserve University) [0707.1594] Scale Transformations, Tree-level Perturbation Theory, and the Cosmological Matter Bispe
arxiv.org/abs/0707.1594 Scale Transformations, Tree-level Perturbation Theory, and the Cosmological Matter Bispectrum
Cosmic String Loops and Gravitational RadiationAuthors:
Joseph Polchinski Spherical Needlets for CMB Data AnalysisAuthors:
D. Marinucci,
D. Pietrobon,
A. Balbi,
P. Baldi,
P. Cabella,
G. Kerkyacharian,
P. Natoli,
D. Picard,
N. Vittorio Mapping Cosmological Observables to the Dark KineticsAuthors:
Sergei Bashinsky (Los Alamos) Dynamical Dark Energy or Simply Cosmic Curvature?Growing MatterAuthors:
Luca Amendola (INAF/OAR, Roma, Italy),
Marco Baldi (Max-Planck-Institut f. Astrophysics, Garching, Germany),
Christof Wetterich (Institute for Theoretical Physics, Heidelberg, Germany) [0706.2395] Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy
arxiv.org/abs/0706.2395 Combining Weak Lensing Tomography with Halo Clustering to Probe Dark EnergyCosmological Constraints on f(R) Acceleration ModelsChallenging the Cosmological ConstantAuthors:
Nemanja Kaloper [0706.1982] Limits on primordial power spectrum resolution: An inflationary flow analysis
arxiv.org/abs/0706.1982 Limits on primordial power spectrum resolution: An inflationary flow analysis[0706.1775] Galaxy-CMB Cross-Correlation as a Probe of Alternative Models of Gravity
arxiv.org/abs/0706.1775 Galaxy-CMB Cross-Correlation as a Probe of Alternative Models of GravityConditional Cumulants in Weakly Non-linear Regime[astro-ph/0610211] Information content in the halo-model dark-matter power spectrum II: Multiple cos
arxiv.org/abs/astro-ph/0610211 Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters[0706.0849] Imaging the Cosmic Matter Distribution using Gravitational Lensing of Pregalactic HI
arxiv.org/abs/0706.0849 Imaging the Cosmic Matter Distribution using Gravitational Lensing of Pregalactic HI[0706.0033] New constraints on dark energy from Chandra X-ray observations of the largest relaxed ga
arxiv.org/abs/0706.0033 New constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clustersAuthors:
S.W. Allen (1),
D.A. Rapetti (1),
R.W. Schmidt (2),
H. Ebeling (3),
G. Morris (1),
A.C. Fabian (4) ((1) KIPAC, Stanford, (2) Heidelberg, (3) Hawaii, (4) IoA, Cambridge) Evidence Of Dark Matter Annihilations In The WMAP Haze[0705.3455] BLOX: The Bonn Lensing, Optical, and X-ray selected galaxy clusters -- I. Cluster catalo
arxiv.org/abs/0705.3455 BLOX: The Bonn Lensing, Optical, and X-ray selected galaxy clusters -- I. Cluster catalog construction[0705.3323] Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
arxiv.org/abs/0705.3323 An improved cosmological bound on the thermal axion mass[astro-ph/0702040] Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM
arxiv.org/abs/astro-ph/0702040 Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology[0705.2380] A Covariant Road to Spatial Averaging in Cosmology : Scalar Corrections to the Cosmologi
arxiv.org/abs/0705.2380 A Covariant Road to Spatial Averaging in Cosmology : Scalar Corrections to the Cosmological EquationsAuthors:
Aseem Paranjape A Curvature Principle for the interaction between universesAuthors:
Orfeu Bertolami Black holes, information, and localityAuthors:
Steven B. Giddings [0705.2171] Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+
arxiv.org/abs/0705.2171 Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+17[0705.1906] The tension of cosmological magnetic fields as a contribution to dark energy
arxiv.org/abs/0705.1906 The tension of cosmological magnetic fields as a contribution to dark energy[0705.1955] Can we ever distinguish between quintessence and a cosmological constant?
arxiv.org/abs/0705.1955 Can we ever distinguish between quintessence and a cosmological constant?[0705.1437] Photo-z for weak lensing tomography from space: the role of optical and near-IR photomet
arxiv.org/abs/0705.1437 Photo-z for weak lensing tomography from space: the role of optical and near-IR photometry[0705.0533] A combined analysis of Lyman-alpha forest, 3D Weak Lensing and WMAP year three data
arxiv.org/abs/0705.0533 A combined analysis of Lyman-alpha forest, 3D Weak Lensing and WMAP year three data[0705.0358] Comparison of weak lensing masses and X-ray properties of galaxy clusters
arxiv.org/abs/0705.0358 Comparison of weak lensing masses and X-ray properties of galaxy clustersAuthors:
Henk Hoekstra
[0705.0163] Probing dark energy with cluster counts and cosmic shear power spectra: including the fu
arxiv.org/abs/0705.0163 Probing dark energy with cluster counts and cosmic shear power spectra: including the full covariance[0705.0343] The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity
arxiv.org/abs/0705.0343 The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity and non-linear galaxy bias[0705.0166] Dark energy constraints from cosmic shear power spectra: impact of intrinsic alignments
arxiv.org/abs/0705.0166 Dark energy constraints from cosmic shear power spectra: impact of intrinsic alignments on photometric redshift requirements[0704.3657] Probability Density of the Multipole Vectors for a Gaussian Cosmic Microwave Background
arxiv.org/abs/0704.3657 Probability Density of the Multipole Vectors for a Gaussian Cosmic Microwave BackgroundTowards observable signatures of other bubble universesMapping the Cosmological Confidence Ball SurfaceFundamental Plane of Sunyaev-Zeldovich clustersAuthors:
Niayesh Afshordi (ITC, Harvard) Measuring the dark side (with weak lensing)[0704.2350] The time evolution of cosmological redshift in non-standard dark energy models
arxiv.org/abs/0704.2350 The time evolution of cosmological redshift in non-standard dark energy modelsA discriminating probe of gravity at cosmological scalesAuthors:
Pengjie Zhang (SHAO),
Michele Liguori (Cambridge),
Rachel Bean (Cornell),
Scott Dodelson (Fermilab/Chicago) [astro-ph/0703741] Effects of Baryons and Dissipation on the Matter Power Spectrum
arxiv.org/abs/astro-ph/0703741 Effects of Baryons and Dissipation on the Matter Power SpectrumAuthors: Douglas H. Rudd, Andrew R. Zentner, Andrey V. Kravtsov (KICP, U.Chicago)
[astro-ph/0608351] The impact of neutrino masses on the determination of dark energy properties
arxiv.org/abs/astro-ph/0608351
[astro-ph/0608480] The Cluster Mass Function from Weak Gravitational Lensing
arxiv.org/abs/astro-ph/0608480
[astro-ph/0608549] The Atacama Cosmology Telescope Project: A Progress Report
arxiv.org/abs/astro-ph/0608549
[astro-ph/0608691] Non-Gaussianity of the density distribution in accelerating universes II:N-body s
arxiv.org/abs/astro-ph/0608691
[astro-ph/0608679] Efficient Cosmological Parameter Estimation with Hamiltonian Monte Carlo
arxiv.org/abs/astro-ph/0608679
[astro-ph/0608686] New Constraints on the Variable Equation of State Parameter from X-Ray Gas Mass F
arxiv.org/abs/astro-ph/0608686
[astro-ph/0608635] Measuring the matter density using baryon oscillations in the SDSS
arxiv.org/abs/astro-ph/0608635
[astro-ph/0608643] The Shear TEsting Programme 2: Factors affecting high precision weak lensing anal
arxiv.org/abs/astro-ph/0608643
[astro-ph/0609124] Primordial non-Gaussianity and Dark Energy constraints from Cluster Surveys
arxiv.org/abs/astro-ph/0609124
[astro-ph/0609354] Probing Dark Energy with Baryonic Acoustic Oscillations at High Redshifts
arxiv.org/abs/astro-ph/0609354
[astro-ph/0609547] The Scale Dependence of Halo and Galaxy Bias: Effects in Real Space
arxiv.org/abs/astro-ph/0609547
[astro-ph/0609543] Determining the expansion history of the universe with the three dimensional cosm
arxiv.org/abs/astro-ph/0609543
[astro-ph/0609507] Importance of Supernovae at z<0.1 for Probing Dark Energy
arxiv.org/abs/astro-ph/0609507
[astro-ph/0610054] Higher Order Contributions to the 21 cm Power Spectrum
arxiv.org/abs/astro-ph/0610054
[astro-ph/0610007] Separating the Weak Lensing and Kinetic SZ Effects from CMB Temperature Maps
arxiv.org/abs/astro-ph/0610007
[astro-ph/0610257] 21-cm Background Anisotropies Can Discern Primordial Non-Gaussianity from Slow-Ro
arxiv.org/abs/astro-ph/0610257
[astro-ph/0610284] Cosmological constraints from COMBO-17 using 3D weak lensing
arxiv.org/abs/astro-ph/0610284
[astro-ph/0610294] A potentially pure test of cosmic geometry: galaxy clusters and the real space Al
arxiv.org/abs/astro-ph/0610294
[astro-ph/0610336] How well can (renormalized) perturbation theory predict dark matter clustering pr
arxiv.org/abs/astro-ph/0610336
[astro-ph/0610764] Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data
arxiv.org/abs/astro-ph/0610764
[astro-ph/0610762] Topology of structure in the Sloan Digital Sky Survey: model testing
arxiv.org/abs/astro-ph/0610762
[astro-ph/0610922] Cosmic Neutrino Bound on the Dark Matter Annihilation Rate in the Late Universe
arxiv.org/abs/astro-ph/0610922
[astro-ph/0611093] Direct Reconstruction of the Dark Energy Scalar-Field Potential
arxiv.org/abs/astro-ph/0611093
[astro-ph/0611159] How Tomographic Cosmic Shear Maps Lead to Constraints on Dark Energy Properties
arxiv.org/abs/astro-ph/0611159
[astro-ph/0611284] Some impacts of quintessence models on cosmic structure formation
arxiv.org/abs/astro-ph/0611284
[astro-ph/0611274] The Cross-Correlation of High-Redshift 21 cm and Galaxy Surveys
arxiv.org/abs/astro-ph/0611274
[astro-ph/0611313] Statistical analysis of galaxy surveys - III: The non-linear clustering of red an
arxiv.org/abs/astro-ph/0611313
[astro-ph/0611353] Late Forming Dark Matter in Theories of Neutrino Dark Energy
arxiv.org/abs/astro-ph/0611353
[astro-ph/0611454] The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth
arxiv.org/abs/astro-ph/0611454
[astro-ph/0606568] Measuring dark energy properties with 3D cosmic shear
arxiv.org/abs/astro-ph/0606568
[astro-ph/0611514] Complex Physics in Cluster Cores: Showstopper for the Use of Clusters for Cosmolo
arxiv.org/abs/astro-ph/0611514
[astro-ph/0611541] The Physics and Early History of the Intergalactic Medium
arxiv.org/abs/astro-ph/0611541
[astro-ph/0611695] Holography and the scale-invariance of density fluctuations
arxiv.org/abs/astro-ph/0611695
[astro-ph/0611744] Gravitational lensing by cosmic strings: what we learn from the CSL-1 case
arxiv.org/abs/astro-ph/0611744
[astro-ph/0611801] Measuring Dark Energy with the Wide-Field Multi-Object Spectrograph (WFMOS)
arxiv.org/abs/astro-ph/0611801
[astro-ph/0607284] Primordial Non-Gaussianity and Analytical Formula for Minkowski Functionals of th
arxiv.org/abs/astro-ph/0607284
[astro-ph/0609413] Clustering of dark matter tracers: renormalizing the bias parameters
arxiv.org/abs/astro-ph/0609413
[astro-ph/0611849] Large-N expansions applied to gravitational clustering
arxiv.org/abs/astro-ph/0611849
[astro-ph/0611913] A Statistical Study of Weak Lensing by Triaxial Dark Matter Halos: Consequences f
arxiv.org/abs/astro-ph/0611913
[astro-ph/0612123] Evolution of the Non-Linear Galaxy Bias up to Redshift z=1.5
arxiv.org/abs/astro-ph/0612123
[gr-qc/0612031] Tunneling probability for the birth of an asymptotically DeSitter universe
arxiv.org/abs/gr-qc/0612031
[astro-ph/0612187] Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations
arxiv.org/abs/astro-ph/0612187
[astro-ph/0612555] Cosmological Constraints from Galaxy Cluster Velocity Statistics
arxiv.org/abs/astro-ph/0612555
[astro-ph/0612569] Constraining f(R) Gravity as a Scalar Tensor Theory
arxiv.org/abs/astro-ph/0612569
[astro-ph/0612662] Probing inflation with CMB polarization : weak lensing effect on the covariance o
arxiv.org/abs/astro-ph/0612662
[astro-ph/0612773] The matter power spectrum as a tool to discriminate dark matterr-dark energy inte
arxiv.org/abs/astro-ph/0612773
[astro-ph/0607458] Modified-Source Gravity and Cosmological Structure Formation
arxiv.org/abs/astro-ph/0607458
[astro-ph/0701113] Information criteria for astrophysical model selection
arxiv.org/abs/astro-ph/0701113
[hep-th/0606020] Strings, Branes and Cosmology: What can we hope to learn?
arxiv.org/abs/hep-th/0606020
[astro-ph/0701276] Cluster Mass Estimators from CMB Temperature and Polarization Lensing
arxiv.org/abs/astro-ph/0701276
[astro-ph/0701338] Bayesian Evidence for a Cosmological Constant using new High-Redshift Supernovae
arxiv.org/abs/astro-ph/0701338
[astro-ph/0701380] New Constraints on Oscillations in the Primordial Spectrum of Inflationary Pertur
arxiv.org/abs/astro-ph/0701380
[astro-ph/0701376] Science with the next generation of radio surveys from LOFAR to the SKA
arxiv.org/abs/astro-ph/0701376
[astro-ph/0701510] Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined wit
arxiv.org/abs/astro-ph/0701510
[astro-ph/0701782] Probing the Largest Cosmological Scales with the CMB-Velocity Correlation
arxiv.org/abs/astro-ph/0701782
[astro-ph/0702015] Probing the Coupling between Dark Components of the Universe
arxiv.org/abs/astro-ph/0702015
[astro-ph/0702031] Testing the reliability of weak lensing cluster detections
arxiv.org/abs/astro-ph/0702031
[astro-ph/0702078] Measuring dark energy with the shear triplet statistics
arxiv.org/abs/astro-ph/0702078
[astro-ph/0702113] Constraining the Nature of Dark Energy using the SKA
arxiv.org/abs/astro-ph/0702113
[astro-ph/0702223] Fitting CMB data with cosmic strings and inflation
arxiv.org/abs/astro-ph/0702223
[astro-ph/0702314] Determining neutrino properties using future galaxy redshift surveys
arxiv.org/abs/astro-ph/0702314
[astro-ph/0702381] Extension of the standard cosmological model: anisotropy, rotation, and magnetic
arxiv.org/abs/astro-ph/0702381
[astro-ph/0702584] SDSS Galaxy Clustering: Luminosity & Color Dependence and Stochasticity
arxiv.org/abs/astro-ph/0702584
[astro-ph/0702664] Evolution of the Pancaking Effect in a LCDM Cosmology
arxiv.org/abs/astro-ph/0702664
[astro-ph/0703202] Constraints on the Sound Speed of Dynamical Dark Energy
arxiv.org/abs/astro-ph/0703202
[astro-ph/0703191] On model selection forecasting, Dark Energy and modified gravity
arxiv.org/abs/astro-ph/0703191
[astro-ph/0703285] Comment on `Tainted evidence: cosmological model selection versus fitting', by Er
arxiv.org/abs/astro-ph/0703285
[astro-ph/0703375] Constraints on a New Post-General Relativity Cosmological Parameter
arxiv.org/abs/astro-ph/0703375
[astro-ph/0703372] Joint Analysis of Cluster Observations: I. Mass Profile of Abell 478 from Combine
arxiv.org/abs/astro-ph/0703372
[astro-ph/0703462] Dark Energy-Dark Matter Interaction and the Violation of the Equivalence Principl
arxiv.org/abs/astro-ph/0703462
[astro-ph/0703570] Cosmological Constraints From the 100 Square Degree Weak Lensing Survey
arxiv.org/abs/astro-ph/0703570
[astro-ph/0703571] Cosmological Constraints from SDSS maxBCG Cluster Abundances
arxiv.org/abs/astro-ph/0703571
[hep-th/0703027] Degravitation of the Cosmological Constant and Graviton Width
arxiv.org/abs/hep-th/0703027
[hep-th/0703215] Cosmic 21-cm Fluctuations as a Probe of Fundamental Physics
arxiv.org/abs/hep-th/0703215
|