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1by Stern, C., Dietrich, J., Bocquet, S., Applegate, D., Mohr, J., Bridle, S., Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M., Zuntz, J., Benson, B., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T., Abdalla, F., Avila, S., Bertin, E., Brooks, D., Burke, D., Rosell, A., Carretero, J., Castander, F., D’Andrea, C., da Costa, L., Davis, C., Vicente, J., Diehl, H., Doel, P., Estrada, J., Evrard, A., Flaugher, B., Fosalba, P., Frieman, J., Garc´ıa-Bellido, J., Gaztanaga, E., Gruendl, R., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A., Romer, A., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R., Sobreira, F., Suchyta, E., Swanson, M., Tarle, G., Walker, A.“... imply lower cluster masses than measured in previous work with and without WL, although...”
Published in Monthly Notices of the Royal Astronomical Society (2019)
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2by Stern, C., Dietrich, J.P., Bocquet, S., Applegate, D., Mohr, J.J., Bridle, S.L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M.A., Zuntz, J., Benson, B.A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C.L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T.M.C., Abdalla, F.B., Avila, S., Bertin, E., Brooks, D., Burke, D.L., Carnero Rosell, A., Carretero, J., Castander, F.J., D'Andrea, C.B., Da Costa, L.N., Davis, C., De Vicente, J., Diehl, H.T., Doel, P., Estrada, J., Evrard, A.E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R.A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T.“... masses than measured in previous work with and without WL, although the uncertainties are large. The WL...”
Published in Monthly Notices of the Royal Astronomical Society (2019)
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3by Stern, C., Dietrich, J. P., Bocquet, S., Applegate, D., Mohr, J. J., Bridle, S. L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M. A., Zuntz, J., Benson, B. A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C. L. Saliwanchik, Schrabback, T., Gupta, N., Abbott, T. M. C., Abdalla, F. B., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carretero, J., Castander, F. J., D'Andrea, C. B., da Costa, L. N., Davis, C., De Vicente, J., Diehl, H. T., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Walker, A. R., DES Collaboration, SPT Collaboration“...}. Results in both cases imply lower cluster masses than measured in previous work with and without WL...”
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4by Stern, C., Dietrich, J. P., Bocquet, S., Applegate, D., Mohr, J. J., Bridle, S. L., Kind, M. Carrasco, Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M. A., Zuntz, J., Benson, B. A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C. L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T. M. C., Abdalla, F. B., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Carretero, J., Castander, F. J., D'Andrea, C. B., da Costa, L. N., Davis, C., De Vicente, J., Diehl, H. T., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Walker, A. R.“... masses than measured in previous work with and without WL, although the uncertainties are large. The WL...”
Published in Monthly Notices of the Royal Astronomical Society (2018)
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5by Stern, C., Dietrich, J. P., Bocquet, S., Applegate, D., Mohr, J. J., Bridle, S. L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M. A., Zuntz, J., Benson, B. A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C. L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T. M. C., Abdalla, F. B., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carretero, J., Castander, F. J., D’Andrea, C. B., da Costa, L. N., Davis, C., De Vicente, J., Diehl, H. T., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Walker, A. R.“... masses than measured in previous work with and without WL, although the uncertainties are large. The WL...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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6by Stern, C., Dietrich, J. P., Bocquet, S., Applegate, D., Mohr, J. J., Bridle, S. L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M. A., Zuntz, J., Benson, B. A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C. L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T. C., Abdalla, F. B., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carretero, J., Castander, F. J., D’Andrea, C. B., da Costa, L. N., Davis, C., De Vicente, J., Diehl, H. T., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. C., Tarle, G., Walker, A. R.“... masses than measured in previous work with and without WL, although the uncertainties are large. The WL...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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7by Stern, C., Dietrich, J. P., Bocquet, S., Applegate, D., Mohr, J. J., Bridle, S. L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M. A., Zuntz, J., Benson, B. A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C. L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T. M. C., Abdalla, F. B., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carretero, J., Castander, F. J., D’Andrea, C. B., da Costa, L. N., Davis, C., De Vicente, J., Diehl, H. T., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Walker, A. R.“... work with and without WL, although the uncertainties are large. The WL derived value of B SZ is ≈20 per...”
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8by Stern, C., Dietrich, J.P., Bocquet, S., Applegate, D., Mohr, J.J., Bridle, S.L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M.A., Zuntz, J., Benson, B.A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C.L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T.M.C., Abdalla, F.B., Avila, S., Bertin, E., Brooks, D., Burke, D.L., Carnero Rosell, A., Carretero, J., Castander, F.J., d'Andrea, C.B., da Costa, L.N., Davis, C., de Vicente, J., Diehl, H.T., Doel, P., Estrada, J., Evrard, A.E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R.A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T.“... masses than measured in previous work with and without WL, although the uncertainties are large. The WL...”
Published in Monthly Notices of the Royal Astronomical Society (2019)
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9by Stern, C., Dietrich, J.P., Bocquet, S., Applegate, D., Mohr, J.J., Bridle, S.L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M.A., Zuntz, J., Benson, B.A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C.L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T.M.C., Abdalla, F.B., Avila, S., Bertin, E., Brooks, D., Burke, D.L., Carnero Rosell, A., Carretero, J., Castander, F.J., d'Andrea, C.B., da Costa, L.N., Davis, C., de Vicente, J., Diehl, H.T., Doel, P., Estrada, J., Evrard, A.E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R.A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M.A.G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A.A., Romer, A.K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R.C., Sobreira, F., Suchyta, E., Swanson, M.E.C., Tarle, G., Walker, A.R.“... masses than measured in previous work with and without WL, although the uncertainties are large. The WL...”
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10by Stern, C., Dietrich, J.P., Bocquet, S., Applegate, D., Mohr, J.J., Bridle, S.L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M.A., Zuntz, J., Benson, B.A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C.L., Saliwanchik, B., Schrabback, T., Gupta, N., Abbott, T.M.C., Abdalla, F.B., Avila, S., Bertin, E., Brooks, D., Burke, D.L., Carnero Rosell, A., Carretero, J., Castander, F.J., d'Andrea, C.B., da Costa, L.N., Davis, C., de Vicente, J., Diehl, H.T., Doel, P., Estrada, J., Evrard, A.E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R.A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M.A.G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A.A., Romer, A.K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R.C., Sobreira, F., Suchyta, E., Swanson, M.E.C., Tarle, G., Walker, A.R.“... masses than measured in previous work with and without WL, although the uncertainties are large. The WL...”
Published in Monthly Notices of the Royal Astronomical Society (2019)
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