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1by Alexandrou, Constantia, Leskovec, Luka, Meinel, Stefan, Negele, John, Paul, Srijit, Petschlies, Marcus, Pochinsky, Andrew, Rendon, Gumaro, Syritsyn, Sergey“... methods: a variational analysis as well as multiexponential matrix fits. We perform an analysis using...”
Published 2017
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2“... that fit empirical phase shifts remarkably well all the way up to the pion-production threshold...”
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3“... based on effective field theory allows us to systematically control theoretical errors. While the fits...”
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4by Penna-Lima, M., Bartlett, J. G., Rozo, E., Melin, J.-B., Merten, J., Evrard, A. E., Postman, M., Rykoff, E.“... to simultaneously fit an idealized CLASH selection function and the distribution between the measured observables...”
Published 2017
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5“... of the likelihood function. For the flat Lambda CDM model, the best fit is obtained with Omega(m) = 0.40(-0.09...”
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6by Cibirka, N., Cypriano, E. S., Brimioulle, F., Gruen, D., Erben, T., van Waerbeke, L., Miller, L., Finoguenov, A., Kirkpatrick, C., Henry, J. Patrick, Rykoff, E., Rozo, E., Dupke, R., Kneib, J.-P., Shan, H., Spinelli, P.“... a Bayesian analysis for the stacked profile and constrain the best-fitting NFW parameters M-200c...”
Published 2017
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7by Soergel, B., Flender, S., Story, K. T., Bleem, L., Giannantonio, T., Efstathiou, G., Rykoff, E., Benson, B. A., Crawford, T., Dodelson, S., Habib, S., Heitmann, K., Holder, G., Jain, B., Rozo, E., Saro, A., Weller, J., Abdalla, F. B., Allam, S., Annis, J., Armstrong, R., Benoit-Lévy, A., Bernstein, G. M., Carlstrom, J. E., Carnero Rosell, A., Carrasco Kind, M., Castander, F. J., Chiu, I., Chown, R., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., de Haan, T., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Holzapfel, W. L., Honscheid, K., James, D. J., Keisler, R., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Marshall, J. L., McDonald, M., Melchior, P., Miller, C. J., Miquel, R., Nord, B., Ogando, R., Omori, Y., Plazas, A. A., Rapetti, D., Reichardt, C. L., Romer, A. K., Roodman, A., Saliwanchik, B. R., Sanchez, E., Schubnell, M., Sevilla-Noarbe, I., Sheldon, E., Smith, R. C., Soares-Santos, M., Sobreira, F., Stark, A., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Vieira, J. D., Walker, A. R., Whitehorn, N.“... data. By fitting the pairwise kSZ signal to a theoretical template, we measure the average central...”
Published 2016
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8by Green, Jeremy, Hasan, Nesreen, Meinel, Stefan, Engelhardt, Michael, Krieg, Stefan, Laeuchli, Jesse, Negele, John, Orginos, Kostas, Pochinsky, Andrew, Syritsyn, Sergey“.... The form factor shapes are fit using the model-independent z expansion. From G(A)(q)(Q(2)), we determine...”
Published 2017
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9by Meinel, Stefan“... global fit and the Lambda(c) lifetime from experiments, this translates to branching fractions of B...”
Published 2017
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10by Li, Ran, Shan, Huanyuan, Kneib, Jean-Paul, Mo, Houjun, Rozo, Eduardo, Leauthaud, Alexie, Moustakas, John, Xie, Lizhi, Erben, Thomas, Van Waerbeke, Ludovic, Makler, Martin, Rykoff, Eli, Moraes, Bruno“...-star/h(-1) M-circle dot) < 12. The best-fitting subhalomass of the more massive satellite galaxy bin...”
Published 2016
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11“... a global fit to various Higgs search channels to obtain the 95% C.L. constraints on the model...”
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12by Kirk, D., Omori, Y., Benoit-Lévy, A., Cawthon, R., Chang, C., Larsen, P., Amara, A., Bacon, D., Crawford, T. M., Dodelson, S., Fosalba, P., Giannantonio, T., Holder, G., Jain, B., Kacprzak, T., Lahav, O., MacCrann, N., Nicola, A., Refregier, A., Sheldon, E., Story, K. T., Troxel, M. A., Vieira, J. D., Vikram, V., Zuntz, J., Abbott, T. M. C., Abdalla, F. B., Becker, M. R., Benson, B. A., Bernstein, G. M., Bernstein, R. A., Bleem, L. E., Bonnett, C., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Capozzi, D., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Evrard, A. E., Flaugher, B., Frieman, J., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Honscheid, K., James, D. J., Jarvis, M., Kent, S., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Martini, P., Melchior, P., Miller, C. J., Miquel, R., Nichol, R. C., Ogando, R., Plazas, A. A., Reichardt, C. L., Roodman, A., Rozo, E., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Sevilla-Noarbe, I., Simard, G., Smith, R. C., Soares-Santos, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Wechsler, R. H., Weller, J.“... to mass fluctuations at z similar to 0.44. Assuming the Planck 2015 best-fitting cosmology, the amplitude...”
Published 2016
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13by Melchior, P., Gruen, D., McClintock, T., Varga, T. N., Sheldon, E., Rozo, E., Amara, A., Becker, M. R., Benson, B. A., Bermeo, A., Bridle, S. L., Clampitt, J., Dietrich, J. P., Hartley, W. G., Hollowood, D., Jain, B., Jarvis, M., Jeltema, T., Kacprzak, T., MacCrann, N., Rykoff, E. S., Saro, A., Suchyta, E., Troxel, M. A., Zuntz, J., Bonnett, C., Plazas, A. A., Abbott, T. M. C., Abdalla, F. B., Annis, J., Benoit-Lévy, A., Bernstein, G. M., Bertin, E., Brooks, D., Buckley-Geer, E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cunha, C. E., D’Andrea, C. B., da Costa, L. N., Desai, S., Eifler, T. F., Flaugher, B., Fosalba, P., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruendl, R. A., Gschwend, J., Gutierrez, G., Honscheid, K., James, D. J., Kirk, D., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Martini, P., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Nichol, R. C., Ogando, R., Romer, A. K., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Smith, R. C., Soares-Santos, M., Sobreira, F., Swanson, M. E. C., Tarle, G., Thomas, D., Walker, A. R., Weller, J., Zhang, Y.“... <= lambda <= 180 and redshift 0.2 <= z <= 0.8, and fit the averaged mass density contrast profiles with a...”
Published 2017
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