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Showing 61 - 80 results of 1,085 for search '"dark energy"', query time: 0.28s Refine Results
  1. 61
    ...Galaxy cluster surveys will be a powerful probe of dark energy. At the same time, cluster...
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  2. 62
    ...Galaxy cluster surveys will be a powerful probe of dark energy. At the same time, cluster...
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  3. 63
    ...The Dark Energy Survey (DES; operations 2009-2015) will address the nature of dark energy using...
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  4. 64
    ...Galaxy cluster surveys will be a powerful probe of dark energy. At the same time, cluster abundance...
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  5. 65
    ... place significant constraints on the evolution of the dark energy equation of state, $w=w(a)$. We...
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  6. 66
    ...The Dark Energy Survey (DES; operations 2009-2015) will address the nature of dark energy using...
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  7. 67
    ... degree of statistical confidence. Secondly, in order to attempt distinguish the different dark energy...
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  8. 68
  9. 69
    ... cosmologies with dynamical evolution of the dark energy. Particular attention is paid to models with a...
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  10. 70
    ...We present new limits on early dark energy (EDE) from the cosmic microwave background (CMB) using...
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  11. 71
  12. 72
    ...We present new limits on early dark energy (EDE) from the cosmic microwave background (CMB) using...
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  13. 73
    ... place significant constraints on the evolution of the dark energy equation of state, $w=w(a)$. We...
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  14. 74
    by Lima, Marcos, Hu, Wayne
    Published in Physical Review D (2007)
    ...The ability to constrain dark energy from the evolution of galaxy cluster counts is limited...
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  15. 75
    ...Galaxy cluster surveys will be a powerful probe of dark energy. At the same time, cluster abundance...
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  16. 76
    ... cosmologies with dynamical evolution of the dark energy. Particular attention is paid to models with a...
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  17. 77
  18. 78
    ... the different dark energy models from the expectations of $\Lambda$CDM, we analyze the predicted cluster-size...
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  19. 79
    by Omori, Y, Giannantonio, T, Porredon, A, Baxter, EJ, Chang, C, Crocce, M, Fosalba, P, Alarcon, A, Banik, N, Blazek, J, Bleem, LE, Bridle, SL, Cawthon, R, Choi, A, Chown, R, Crawford, T, Dodelson, S, Drlica-Wagner, A, Eifler, TF, Elvin-Poole, J, Friedrich, O, Gruen, D, Holder, GP, Huterer, D, Jain, B, Jarvis, M, Kirk, D, Kokron, N, Krause, E, MacCrann, N, Muir, J, Prat, J, Reichardt, CL, Ross, AJ, Rozo, E, Rykoff, ES, Sanchez, C, Secco, LF, Simard, G, Wechsler, RH, Zuntz, J, Abbott, TMC, Abdalla, FB, Allam, S, Avila, S, Aylor, K, Benson, BA, Bernstein, GM, Bertin, E, Bianchini, F, Brooks, D, Buckley-Geer, E, Burke, DL, Carlstrom, JE, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Castander, FJ, Chang, CL, Cho, H-M, Crites, AT, Cunha, CE, da Costa, LN, de Haan, T, Davis, C, De Vicente, J, Desai, S, Diehl, HT, Dietrich, JP, Dobbs, MA, Everett, WB, Doel, P, Estrada, J, Flaugher, B, Frieman, J, Garcia-Bellido, J, Gaztanaga, E, Gerdes, DW, George, EM, Gruendl, RA, Gschwend, J, Gutierrez, G, Halverson, NW, Harrington, NL, Hartley, WG, Hollowood, DL, Holzapfel, WL, Honscheid, K, Hou, Z, Hoyle, B, Hrubes, JD, James, DJ, Jeltema, T, Kuehn, K, Kuropatkin, N, Lee, AT, Leitch, EM, Lima, M, Luong-Van, D, Manzotti, A, Marrone, DP, Marshall, JL, McMahon, JJ, Melchior, P, Menanteau, F, Meyer, SS, Miller, CJ, Miquel, R, Mocanu, LM, Mohr, JJ, Natoli, T, Padin, S, Plazas, AA, Pryke, C, Romer, AK, Roodman, A, Ruhl, JE, Sanchez, E, Scarpine, V, Schaffer, KK, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Shirokoff, E, Smith, M, Soares-Santos, M, Sobreira, F, Staniszewski, Z, Stark, AA, Story, KT, Suchyta, E, Swanson, MEC, Tarle, G, Thomas, D, Troxel, MA, Vanderlinde, K, Vieira, JD, Walker, AR, Wu, WLK, Zahn, O
    Published in Physical Review D (2019)
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  20. 80
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