No. | Authors | Title (and PDF, as published) | Reference (journal and arXiv link) |
114 | J. Muir and D. Huterer | Peeling off the late Universe: Reconstructing the ISW map with galaxy surveys | arXiv:1604.06586 |
113 | E. J. Baxter, J. Clampitt, T. Giannantonio, S. Dodelson, B. Jain, D. Huterer et al. (DES collaboration) | Joint Measurement of Lensing-Galaxy Correlations Using SPT and DES SV Data | arXiv:1602.07384 |
112 | D.J. Schwarz, C.J. Copi, D. Huterer and G.D. Starkman | CMB Anomalies after Planck | arXiv:1510.07929 |
111 | M. Yoon and D. Huterer | Kinematic dipole detection with galaxy surveys: forecasts and requirements | Astrophys. J. 813, L18 (2015), arXiv:1509.05374 |
110 | D. Huterer, D. L. Shafer and F. Schmidt | No evidence for bulk velocity from type Ia supernovae | JCAP 12, 033 (2015), arXiv:1509.04708 |
109 | I. Jee, E. Komatsu, S. Suyu and D. Huterer | Time-delay Cosmography: Increased Leverage with Angular Diameter Distances | JCAP 04, 031 (2016), arXiv:1509.03310 |
108 | T. Giannantonio et al (DES collaboration) | CMB lensing tomography with the DES Science Verification galaxies | MNRAS 456, 3213 (2016), arXiv:1507.05551 |
107 | K.A. Hinton, A. Becker and D. Huterer | A User-Friendly Dark Energy Model Generator | arXiv:1506.05088 |
106 | D. Schwarz et al (10 authors) | Testing foundations of modern cosmology with SKA all-sky surveys | PoS AASKA14, 032 (2015), arXiv:1501.03820 |
105 | M. Alvarez et al (28 authors) | Testing Inflation with Large Scale Structure: Connecting Hopes with Reality | arXiv:1412.4671 |
104 | J. Bielefeld, D. Huterer and E. Linder | Cosmological Leverage from the Matter Power Spectrum in the Presence of Baryon and Nonlinear Effects | JCAP 1505, 023 (2015), arXiv:1411.3725 |
103 | E.J. Ruiz and D. Huterer | Banana Split: Testing the Dark Energy Consistency with Geometry and Growth | Phys. Rev. D 91, 063009 (2015), arXiv:1410.5832 |
102 | D. L. Shafer and D. Huterer | Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology | MNRAS 447, 2961 (2015), arXiv:1410.0035 |
101 | M. Yoon, D. Huterer, C. Gibelyou, A. Kovacs and I. Szapudi | Dipolar modulation in number counts of WISE-2MASS sources | MNRAS 445, L60 (2014), arXiv:1406.1187 |
100 | A. Evrard, P. Arnault, D. Huterer and A. Farahi | A Model for Multi-property Galaxy Cluster Statistics | MNRAS 441, 3562 (2014), arXiv:1403.1456 |
99 | D.L. Shafer and D. Huterer | Chasing the phantom: A closer look at type Ia supernovae and the dark energy equation of state | Phys. Rev. D 89, 063510 (2014), arXiv:1312.1688 |
98 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | Large-Scale Alignments from WMAP and Planck | MNRAS 449, 3458 (2015), arXiv:1311.4562 |
97 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | Lack of large-angle TT correlations persists in WMAP and Planck | MNRAS 451, 2978 (2015), arXiv:1310.3831 |
96 | B. Jain et al. | Novel Probes of Gravity and Dark Energy | arXiv:1309.5389 |
95 | S. Dodelson et al. | Dark Energy and CMB | Astropart. Phys., 63, 1 (2015), arXiv:1309.5386 |
94 | D. Huterer et al. | Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion | Astropart. Phys., 63, 23 (2015), arXiv:1309.5385 |
93 | J. Newman et al. | Spectroscopic Needs for Imaging Dark Energy Experiments: Photometric Redshift Training and Calibration | Astropart. Phys., 63, 81 (2015), arXiv:1309.5384 |
92 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | Large-Angle CMB Suppression and Polarisation Predictions | MNRAS 434, 3590 (2013), arXiv:1303.4786 |
91 | W. Fang, A. Becker, D. Huterer and E. Lim | Joint Minkowski Functionals and Bispectrum Constraints on Non-Gaussianity in the CMB | Phys. Rev. D 88, 041302 (2013), arXiv:1303.4381 |
90 | H.-Y. Wu and D. Huterer | Impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering | MNRAS 434, 2256 (2013), arXiv:1303.0835 |
89 | D. Huterer, C. Cunha, and and W. Fang | Calibration errors unleashed: effects on cosmological parameters and requirements for large-scale structure surveys | MNRAS 432, 2945 (2013), arXiv:1211.1015 |
88 | A. Becker and D. Huterer | First constraints on the running of non-Gaussianity | Phys. Rev. Lett. 109, 121302 (2012), arXiv:1207.5788 |
87 | E.J. Ruiz, D.L. Shafer, D. Huterer, and A. Conley | Principal components of dark energy with SNLS supernovae: the effects of systematic errors | Phys. Rev. D 86, 103004 (2012), arXiv:1207.4781 |
86 | C. Cunha, D. Huterer, H. Lin, M. Busha and R. Wechsler | Spectroscopic failures in photometric redshift calibration: cosmological biases and survey requirements | MNRAS 444, 129 (2014), arXiv:1207.3347 |
85 | A. Becker, D. Huterer, and K. Kadota | Constraining Scale-Dependent Non-Gaussianity with Future Large-Scale Structure and the CMB | JCAP 1212:034 (2012), arXiv:1206.6165 |
84 | C. Gibelyou and D. Huterer | Dipoles in the Sky | MNRAS 427, 1994 (2012), arXiv:1205.6476 |
83 | G.D. Starkman, C.J. Copi, D. Huterer and D.J. Schwarz | The Oddly Quiet Universe: How the CMB Challenges Cosmology's Standard Model | arXiv:1201.2459 |
82 | C. Cunha, D. Huterer, M. Busha and R. Wechsler | Sample variance in photometric redshift calibration: cosmological biases and survey requirements | MNRAS 423, 909 (2012), arXiv:1109.5691 |
81 | D. Schlegel et al. (142 authors) | The BigBOSS Experiment | arXiv:1106.1706 |
80 | E. Calabrese, D. Huterer, E.V. Linder, A. Melchiorri, and L. Pagano | Limits on Dark Radiation, Early Dark Energy, and Relativistic Degrees of Freedom | Phys. Rev. D 83, 023504 (2011), arXiv:1103.4132 |
79 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | Bias in low-multipole CMB reconstructions | MNRAS 418, 505 (2011), arXiv:1103.3505 |
78 | M. March, R. Trotta, L. Amendola and D. Huterer | Robustness to systematics for future dark energy probes | MNRAS 415, 143 (2011), arXiv:1101.1521 |
77 | D. Huterer, E. Komatsu and S. Shandera | Testing the Gaussianity and Statistical Isotropy of the Universe (Editorial article) | Advances in Astronomy vol. 2010, Article ID 697147 (2010), arXiv:1012.3744 |
76 | M. Mortonson, W. Hu and D. Huterer | Simultaneous Falsification of LambdaCDM and Quintessence with Massive, Distant Clusters | Phys. Rev. D 83, 023015 (2011), arXiv:1011.0004 |
75 | E. Calabrese, R. de Putter, D. Huterer, E.V. Linder and A. Melchiorri | Future CMB Constraints on Early, Cold, or Stressed Dark Energy | Phys. Rev. D 83, 023011 (2011), arXiv:1010.5612 |
74 | S. Shandera, N. Dalal and D. Huterer | A generalized local ansatz and its effect on halo bias | JCAP 1103:017 (2011), arXiv:1010.3722 |
73 | D. Huterer | The Accelerating Universe | arXiv:1010.1162 |
72 | C. Zunckel, D. Huterer, and G.D. Starkman | Testing the statistical isotropy of large scale structure with multipole vectors | Phys. Rev. D 84, 043005 (2011), arXiv:1009.4701 |
71 | A. Becker, D. Huterer, and K. Kadota | Scale-Dependent Non-Gaussianity as a Generalization of the Local Model | JCAP 1101:006 (2011), arXiv:1009.4189 |
70 | C. Gibelyou, D. Huterer, and W. Fang | Detectability of large-scale power suppression in the galaxy distribution | Phys. Rev. D 82, 123009 (2010), arXiv:1007.0757 |
69 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | Large-Angle Anomalies in the CMB | Advances in Astronomy vol. 2010, Article ID 847541 (2010), arXiv:1004.5602 |
68 | D. Sarkar, D. Huterer, C.J. Copi, G.D. Starkman and D.J. Schwarz | Missing Power vs low-l Alignments in the Cosmic Microwave Background: No Correlation in the Standard Cosmological Model | Astropart. Phys., 34, 591 (2010), arXiv:1004.3784 |
67 | M. Mortonson, D. Huterer and W. Hu | Figures of merit for present and future dark energy probes | Phys. Rev. D 82, 063004 (2010), arXiv:1004.0236 |
66 | C. Cunha, D. Huterer, and O. Doré | Primordial non-Gaussianity from the covariance of galaxy cluster counts | Phys. Rev. D 82, 023004 (2010), arXiv:1003.2416 |
65 | A.P. Hearin, A.R. Zentner, Z. Ma, and D. Huterer | A General Study of The Influence of Catastrophic Photometric Redshift Errors on Cosmology with Cosmic Shear Tomography | Astrophys. J. 720, 1351 (2010), arXiv:1002.3383 |
64 | R. de Putter, D. Huterer and E. Linder | Measuring the Speed of Dark: Detecting Dark Energy Perturbations | Phys. Rev. D 81, 103513 (2010), arXiv:1002.1311 |
63 | D. Huterer | Weak lensing, dark matter and dark energy | Gen. Rel. Grav. 42, 2177 (2010), arXiv:1001.1758 |
62 | M. Mortonson, W. Hu and D. Huterer | Testable dark energy predictions from current data | Phys. Rev. D 81, 063007 (2010), arXiv:0912.3816 |
61 | R. Zhang and D. Huterer | Disks in the sky: A reassessment of the WMAP "cold spot" | Astropart. Phys., 33, 69 (2010), arXiv:0908.3988 |
60 | M. Mortonson, W. Hu and D. Huterer | Hiding dark energy transitions at low redshift | Phys. Rev. D 80, 067301 (2009), arXiv:0908.1408 |
59 | C. Cunha, D. Huterer and J. Frieman | Constraining Dark Energy with Clusters: Complementarity with Other Probes | Phys. Rev. D 80, 063532 (2009), arXiv:0904.1589 |
58 | G. Bernstein and D. Huterer | Catastrophic photometric redshift errors: weak lensing survey requirements | MNRAS 401, 1399 (2010), arXiv:0902.2782 |
57 | D. Huterer | The Road to Dark Energy | Mod. Phys. Lett 23, 1346 (2008) |
56 | A. Albrecht et al (the FoMSWG - Figure of Merit Science Working Group) | Findings of the Joint Dark Energy Mission Figure of Merit Science Working Group | arXiv:0901.0721 |
55 | M. Mortonson, W. Hu and D. Huterer | Falsifying Paradigms for Cosmic Acceleration | Phys. Rev. D 79, 023004 (2009), arXiv:0810.1744 |
54 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | No large-angle correlations on the non-Galactic microwave sky | MNRAS 399, 295 (2009), arXiv:0808.3767 |
53 | K.M. Smith and D. Huterer | No Evidence for the Cold Spot in the NVSS Radio Survey | MNRAS 403, 2 (2010), arXiv:0805.2751 |
52 | J. Frieman, M. Turner and D. Huterer | Dark Energy and the Accelerating Universe | Ann. Rev. Astron. Astrophys. 46, 385 (2008), arXiv:0803.0982 |
51 | G. Zhao, D. Huterer and X. Zhang | High-resolution temporal constraints on the dynamics of dark energy | Phys. Rev. D 77, 121302 (2008), arXiv:0712.2277 |
50 | N. Dalal, O. Doré, D. Huterer and A. Shirokov | The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects | Phys. Rev. D 77, 123514 (2008), arXiv:0710.4560 |
49 | M.S.Turner and D. Huterer | Cosmic Acceleration, Dark Energy and Fundamental Physics | J. Phys. Soc. Jpn. 76, 111015 (2007), arXiv:0706.2186 |
48 | L.M. Krauss, K. Jones-Smith and D. Huterer | Dark Energy, a Cosmological Constant and Type Ia Supernovae | New J. Phys. 9, 141 (2007), astro-ph/0701692 |
47 | P.-S. Corasaniti, D. Huterer and A. Melchiorri | Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test | Phys. Rev. D 75, 062001 (2007), astro-ph/0701433 |
46 | D. Huterer and H.V. Peiris | Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables | Phys. Rev. D 75, 083503 (2007), astro-ph/0610427 |
45 | D. Huterer and E.V. Linder | Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy | Phys. Rev. D 75, 023519 (2007), astro-ph/0608681 |
44 | D. Huterer | Mysteries at Universe's Largest Observable Scales | New Astronomy Reviews 50, 868 (2006), astro-ph/0608318 |
43 | W. Hu, D. Huterer and K. Smith | Supernovae, Lensed CMB and Dark Energy | Astrophys. J. Lett. 650, L13 (2006), astro-ph/0607316 |
42 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3 | Phys. Rev. D 75, 023507 (2007), astro-ph/0605135 |
41 | A. Cooray, D. Huterer and D. Holz | Problems with Small Area Surveys: Lensing Covariance of Supernova Distance Measurements | Phys. Rev. Lett. 96, 021301 (2006), astro-ph/0509581 |
40 | A. Cooray, D. Holz and D. Huterer | Cosmology from supernova magnification maps | Astrophys. J. 637, L77 (2006), astro-ph/0509579 |
39 | C. Gordon, W. Hu, D. Huterer and T. Crawford, | Spontaneous Isotropy Breaking: A Mechanism for CMB Multipole Alignments | Phys. Rev. D, 72, 103002 (2005), astro-ph/0509301 |
38 | C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman | On the large-angle anomalies of the microwave sky | MNRAS 367, 79 (2006), astro-ph/0508047 |
37 | SNAP collaboration | Probing Dark Energy via Weak Gravitational Lensing with the SuperNova Acceleration Probe (SNAP) | White paper to the Dark Energy Task Force astro-ph/0507460 |
36 | SNAP collaboration | Supernova Acceleration Probe: Studying Dark Energy with Type Ia Supernovae | White paper to the Dark Energy Task Force astro-ph/0507459 |
35 | SNAP collaboration | Seeing the Nature of the Accelerating Physics: It's a SNAP | White paper to the Dark Energy Task Force astro-ph/0507458 |
34 | Z. Ma, W. Hu and D. Huterer | Effect of Photometric Redshift Errors on Weak Lensing Tomography | Astrophys. J., 636, 21 (2006), astro-ph/0506614 |
33 | D. Huterer, M. Takada, G. Bernstein and B. Jain | Systematic Errors in Future Weak Lensing Surveys: Requirements and Prospects for Self-Calibration | MNRAS 366, 101 (2006), astro-ph/0506030 |
32 | E. V. Linder and D. Huterer | How many dark energy parameters? | Phys. Rev. D., 72, 043509 (2005) astro-ph/0505330 |
31 | D. Huterer and M. White | Nulling Tomography with Weak Gravitational Lensing | Phys. Rev. D., 72, 043002 (2005) astro-ph/0501451 |
30 | D. Huterer and M. Takada | Calibrating the Nonlinear Matter Power Spectrum: Requirements for Future Weak Lensing Surveys | Astropart. Phys., 23, 369 (2005), astro-ph/0412142 |
29 | D. Huterer and T. Vachaspati | Distribution of Singularities in the Cosmic Microwave Background Polarization | Phys. Rev. D., 72, 043004 (2005) astro-ph/0405474 |
28 | SNAP collaboration | Supernova / Acceleration Probe: A Satellite Experiment to Study the Nature of the Dark Energy | PASP (submitted) astro-ph/0405232 |
27 | D. Huterer, C.R. Keeton and C.-P. Ma | Effects of Ellipticity and Shear on Gravitational Lens Statistics | Astrophys. J., 624, 34 (2005), astro-ph/0405040 |
26 | D. Huterer and A. Cooray | Uncorrelated Estimates of Dark Energy Evolution | Phys. Rev. D, 71, 023506 (2005), astro-ph/0404062 |
25 | D.J. Schwarz, G.D. Starkman, D. Huterer and C.J. Copi | Is the low-ell microwave background cosmic? | Phys. Rev. Lett., 93, 221301 (2004), astro-ph/0403353 |
24 | D. Huterer, A. Kim, L.M. Krauss and T. Broderick | Redshift Accuracy Requirements for Future Supernova and Number Count Surveys | Astrophys. J., 615, 595 (2004), astro-ph/0402002 |
23 | C.J. Copi, D. Huterer and G.D. Starkman | Multipole Vectors---a new representation of the CMB sky and evidence for statistical anisotropy or non-Gaussianity at 2 <= l <= 8 | Phys. Rev. D, 70, 043515 (2004), astro-ph/0310511 |
22 | D. Huterer and C.-P. Ma | Constraints on Dark Energy and the Inner Cluster Mass Profile from Strong Lensing Statistics | Astrophys. J. Lett., 600, L7 (2004), astro-ph/0307301 |
21 | D. Huterer and T. Vachaspati | Gravitational Lensing by Cosmic Strings in the Era of Wide-Field Surveys | Phys. Rev. D., 68, 041301 (2003), astro-ph/0305006 |
20 | J. Rhodes et al. (SNAP collaboration) | Weak Lensing from Space I: Prospects for the Supernova/Acceleration Probe | Astropart. Phys., 20, 377 (2004), astro-ph/0304417 |
19 | A. Cooray, D. Huterer and D. Baumann | Growth Rate of Large Scale Structure as a Powerful Probe of Dark Energy | Phys. Rev. D. 69 027301 (2004), astro-ph/0304268 |
18 | A.N. Davis, D. Huterer and L.M. Krauss | Strong lensing constraints on the velocity dispersion and density profile of elliptical galaxies | MNRAS 344 1029 (2003), astro-ph/0210494 |
17 | E. V. Linder and D. Huterer | Why Supernovae at z>1 are needed to Probe Dark Energy | Phys. Rev. D. 67 081303 (2003), astro-ph/0208138 |
16 | J.A. Frieman, D. Huterer, E.V. Linder and M.S. Turner | Probing Dark Energy with Supernovae: Exploiting Complementarity with the Cosmic Microwave Background | Phys. Rev. D. 67 083505 (2003), astro-ph/0208100 |
15 | D. Huterer and G.D. Starkman | Parameterization of Dark-Energy Properties: a Principal-Component Approach | Phys. Rev. Lett. 90 031301 (2003), astro-ph/0207517 |
14 | D. Huterer and M. White | Weak Lensing as a Calibrator of the Cluster Mass-Temperature Relation | Astrophys. J. Lett. 578 L95 (2002), astro-ph/0206292 |
13 | D. Huterer, G.D. Starkman and M. Trodden | Is the Universe Inflating? Dark Energy and the Future of the Universe | Phys. Rev. D. 66 043511 (2002) astro-ph/0202256 |
12 | D. Huterer | Weak Lensing and Dark Energy | Phys. Rev. D. 65 063001 (2002) astro-ph/0106399 |
11 | A. Cooray, W. Hu, D. Huterer and M. Joffre | Measuring Angular Diameter Distances through Halo Clustering | Astrophys. J. 557 L7 (2001), astro-ph/0105061 |
10 | D. Huterer, E.V. Linder and J. Weller | Constraints on Dark Energy and Its Models | Yellow Book on Dark Energy, SNOWMASS 2001, eds. E. V. Linder |
9 | D. Huterer and M.S. Turner | Constraining the Properties of Dark Energy | proceedings of 20th Texas Symposium on Relavistic Astrophysics astro-ph/0103175 |
8 | D. Huterer and M.S. Turner | Probing Dark Energy: Methods and Strategies | Phys. Rev. D. 64 123527 (2001), astro-ph/0012510 |
7 | D. Huterer, L. Knox and R.C. Nichol | The Angular Power Spectrum of EDSGC galaxies | Astrophys. J. 555 547 (2001), astro-ph/0011069 |
6 | D. Huterer and M.S. Turner | Optimal Supernova Search Strategies | proceedings of Dark Matter 2000, ed. D. Cline astro-ph/0006419 |
5 | D. Huterer and M.S. Turner | On the Degree of Scale Invariance of Inflationary Perturbations | Phys. Rev. D. 62 063503 (1999), astro-ph/9908157 |
4 | D. Huterer and M.S. Turner | Prospects for Probing the Dark Energy via Supernova Distance Measurements | Phys. Rev. D. 60 081301 (1999), astro-ph/9808133 |
3 | A.R. Cooray and D. Huterer | Gravitational Lensing as a Probe of Quintessence | Astrophys. J. 513 L95 (1999), astro-ph/9901097 |
2 | D. Huterer, K.I. Paularena and A. Szabo, | Observation and Analysis of Selected IMP 8 and WIND Bow Shock Crossings in Late 1994 | J. Geophys. Res. 102 A9 19761 (1997) |
1 | D. Huterer, D.D. Sasselov and P.L. Schechter | Distances to Nearby Galaxies: Combining Fragmentary Data Using Four Different Methods | Astron. J. 110 2705 (1995), astro-ph/9508122 |