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4by Beck, Ivo, Angot, HĂ©lène, Baccarini, Andrea, Dada, Lubna, QuĂ©lĂ©ver, Lauriane, Jokinen, Tuija, Laurila, Tiia, Lampimäki, Markus, Bukowiecki, Nicolas, Boyer, Matthew, Gong, Xianda, Gysel-Beer, Martin, Petäjä, Tuukka, Wang, Jian, Schmale, Julia“... and particle concentrations in pristine environments. However, data from remote areas are often contaminated...”
Published in Atmospheric Measurement Techniques (2022)
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7by Grandis, S., Klein, M., Mohr, J. J., Bocquet, S., Paulus, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Benson, B. A., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Capasso, R., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Eifler, T. F., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., GarcĂa-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Ogando, R. C., Palmese, A., Paz-ChinchĂłn, F., Plazas, A. A., Romer, A. K., Roodman, A., Sanchez, E., Saro, A., Scarpine, V., Schubnell, M., Serrano, S., Sheldon, E., Smith, M., Stark, A. A., Suchyta, E., Swanson, M. C., Tarle, G., Thomas, D., Tucker, D. L., Varga, T. N., Weller, J., Wilkinson, R.“... reveals no clear evidence for MARD-Y3 contamination, SPT-SZ incompleteness or outlier fraction. Finally...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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8by Grandis, S., Klein, M., Mohr, J. J., Bocquet, S., Paulus, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Benson, B. A., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Capasso, R., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Eifler, T. F., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., GarcĂa-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Ogando, R. C., Palmese, A., Paz-ChinchĂłn, F., Plazas, A. A., Romer, A. K., Roodman, A., Sanchez, E., Saro, A., Scarpine, V., Schubnell, M., Serrano, S., Sheldon, E., Smith, M., Stark, A. A., Suchyta, E., Swanson, M. C., Tarle, G., Thomas, D., Tucker, D. L., Varga, T. N., Weller, J., Wilkinson, R.“... reveals no clear evidence for MARD-Y3 contamination, SPT-SZ incompleteness or outlier fraction. Finally...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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9by Grandis, S., Klein, M., Mohr, J. J., Bocquet, S., Paulus, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Benson, B. A., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Capasso, R., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Eifler, T. F., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., GarcĂa-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Ogando, R. C., Palmese, A., Paz-ChinchĂłn, F., Plazas, A. A., Romer, A. K., Roodman, A., Sanchez, E., Saro, A., Scarpine, V., Schubnell, M., Serrano, S., Sheldon, E., Smith, M., Stark, A. A., Suchyta, E., Swanson, M. C., Tarle, G., Thomas, D., Tucker, D. L., Varga, T. N., Weller, J., Wilkinson, R.“... reveals no clear evidence for MARD-Y3 contamination, SPT-SZ incompleteness or outlier fraction. Finally...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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11by Grandis, S., Mohr, J. J., Costanzi, M., Saro, A., Bocquet, S., Klein, M, Aguena, M., Allam, S., Annis, J., Ansarinejad, B., Bleem, L.“... contaminants. At a richness $\hat{λ}$ = 40, this population makes up >12% (97.5 percentile) of the total...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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12by Grandis, S., Mohr, J. J., Costanzi, M., Saro, A., Bocquet, S., Klein, M., Aguena, M., Allam, S., Annis, J., Ansarinejad, B., Bacon, D., Bertin, E., Bleem, L., Brooks, D., Burke, D. L., Carnero Rosel, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, A., da Costa, L. N., De Vincente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Everett, S., Ferrero, I., Floyd, B., Fosalba, P., Frieman, J., GarcĂa-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lahav, O., Lidman, C., Lima, M., Maia, M. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Myles, J., Ogando, R., Palmese, A., Paz-ChinchĂłn, F., Plazas, A. A., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Singh, P., Smith, M., Suchyta, E., Swanson, M. C., Tarle, G., Thomas, D., To, C., Weller, J., Wilkinson, R. D., Wu, H.“..., which we call contaminants. At a richness $\hat{\lambda }=40$, this population makes up ${\gt}12{{\ \rm...”
Published in Monthly Notices of the Royal Astronomical Society (2023)
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13by Grandis, S., Mohr, J. J., Costanzi, M., Saro, A., Bocquet, S., Klein, M., Aguena, M., Allam, S., Annis, J., Ansarinejad, B., Bacon, D., Bertin, E., Bleem, L., Brooks, D., Burke, D. L., Carnero Rosel, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, A., da Costa, L. N., De Vincente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Everett, S., Ferrero, I., Floyd, B., Fosalba, P., Frieman, J., GarcĂa-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lahav, O., Lidman, C., Lima, M., Maia, M. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Myles, J., Ogando, R., Palmese, A., Paz-ChinchĂłn, F., Plazas, A. A., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Singh, P., Smith, M., Suchyta, E., Swanson, M. C., Tarle, G., Thomas, D., To, C., Weller, J., Wilkinson, R. D., Wu, H.“...-mass objects not correctly accounted for by our richness-mass scatter model, which we call contaminants...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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14by Grandis, S., Mohr, J. J., Costanzi, M., Saro, A., Bocquet, S., Klein, M., Aguena, M., Allam, S., Annis, J., Ansarinejad, B., Bacon, D., Bertin, E., Bleem, L., Brooks, D., Burke, D. L., Carnero Rosel, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, A., da Costa, L. N., De Vincente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Everett, S., Ferrero, I., Floyd, B., Fosalba, P., Frieman, J., GarcĂa-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lahav, O., Lidman, C., Lima, M., Maia, M. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Myles, J., Ogando, R., Palmese, A., Paz-ChinchĂłn, F., Plazas, A. A., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Singh, P., Smith, M., Suchyta, E., Swanson, M. C., Tarle, G., Thomas, D., To, C., Weller, J., Wilkinson, R. D., Wu, H.“..., which we call contaminants. At a richness $\hat{\lambda }=40$, this population makes up ${\gt}12{{\ \rm...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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15by Grandis, S., Mohr, J. J., Costanzi, M., Saro, A., Bocquet, S., Klein, M., Aguena, M., Allam, S., Annis, J., Ansarinejad, B., Bacon, D., Bertin, E., Bleem, L., Brooks, D., Burke, D. L., Carnero Rosel, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, A., da Costa, L. N., De Vincente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Everett, S., Ferrero, I., Floyd, B., Fosalba, P., Frieman, J., GarcĂa-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lahav, O., Lidman, C., Lima, M., Maia, M. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Myles, J., Ogando, R., Palmese, A., Paz-ChinchĂłn, F., Plazas, A. A., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Singh, P., Smith, M., Suchyta, E., Swanson, M. C., Tarle, G., Thomas, D., To, C., Weller, J., Wilkinson, R. D., Wu, H.“..., which we call contaminants. At a richness $\hat{\lambda }=40$, this population makes up ${\gt}12{{\ \rm...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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16by Simmons, Mary Ann, Poston, Ted M., Tiller, Brett L., Stegen, Amanda, Hand, Kristine D., Brandenberger, Jill M.“... of the accumulation of Hanford-derived and environmental contaminants by resident goose populations....”
Published 2014
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18by Bæk, Edda, Hinton, Thomas G., Skuterud, Lavrans, Beasley, James C., Salbu, Brit, Baranwal, Vikas C., Lind, Ole Christian“... distribution of contaminants. Instead, most wildlife exposure data are estimated from model simulations...”
Published in Ecological Indicators (2023)
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