Search Results - "Pratt, G.W."

Estimation of the hydrostatic-to-lensing mass bias from resolved cluster masses by Muñoz-Echeverría, M., Macías-Pérez, J.F., Pratt, G.W., Pointecouteau, E., Bartalucci, I., De Petris, M., Ferragamo, A., Hanser, C., Kéruzoré, F., Mayet, F., Moyer-Anin, A., Paliwal, A., Perotto, L., Yepes, G.

“…We present a study on the bias of hydrostatic masses with respect to lensing mass estimates for a sample of 53 clusters in a redshift range between z = 0.05…”
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Cosmology with galaxy clusters: An improved multiwavelength analysis by Aymerich, G., Douspis, M., Pratt, G.W., Salvati, L., Soubrié, E., Andrade-Santos, F., Forman, W., Jones, C.

“…We provide a new scaling relation using a sample of clusters from a full re-observation by the X-ray Chandra telescope of the Planck ESZ catalogue, and compare…”
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Systematic effects on the upcoming NIKA2 LPSZ scaling relation by Moyer-Anin, A., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E.F.C., Ejlali, G., Gomez, A., Goupy, J., Hanser, C., Katsioli, S., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.F., Madden, S.C., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Muñoz-Echeverría, M., Paliwal, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G.W., Revéret, V., Rigby, A.J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Tucker, C.

“…In cluster cosmology, cluster masses are the main parameter of interest. They are needed to constrain cosmological parameters through the cluster number count…”
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The NIKA2 Sunyaev-Zeldovich Large Program: Precise galaxy cluster physics for an accurate cluster-based cosmology by Perotto, L., Adam, R., Ade, P., Ajeddig, H., André, P., Arnaud, M., Artis, E., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Ferragamo, A., Gomez, A., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.-F., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Muñoz-Echeverría, M., Paliwal, A., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G.W., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Yepes, G.

“…The NIKA2 Guaranteed-Time SZ Large Program (LPSZ) is dedicated to the high-angular resolution SZ mapping of a representative sample of 45 SZ-selected galaxy…”
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Cluster cosmology with the NIKA2 SZ Large Program by Mayet, F., Adam, R., Ade, P., André, P., Andrianasolo, A., Arnaud, M., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Bideaud, A., Bourrion, O., Calvo, M., Catalano, A., Comis, B., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E.F.C., Gomez, A., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.F., Mauskopf, P., Monfardini, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G.W., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Zylka, R.

“…The main limiting factor of cosmological analyses based on thermal Sunyaev-Zel’dovich (SZ) cluster statistics comes from the bias and systematic uncertainties…”
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NIKA: a mm camera for Sunyaev-Zel’dovich science in clusters of galaxies by Macías-Pérez, J.F., Adam, R., Ade, P., André, P., Andrianasolo, A., Aussel, H., Arnaud, M., Bartalucci, I., Beelen, A., Benoît, A., Bideaud, A., Bourrion, O., Calvo, M., Catalano, A., Comis, B., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E.F.C., Gomez, A., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Mauskopf, P., Mayet, F., Monfardini, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G.W., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Zylka, R.

“…Clusters of galaxies, the largest bound objects in the Universe, constitute a cosmological probe of choice, which is sensitive to both dark matter and dark…”
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A low-mass galaxy cluster as a test-case study for the NIKA2 SZ Large Program by Kéruzoré, F., Adam, R., Ade, P., André, P., Andrianasolo, A., Arnaud, M., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Bideaud, A., Bourrion, O., Calvo, M., Catalano, A., Comis, B., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E.F.C., Gomez, A., Goupy, J., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.F., Mauskopf, P., Mayet, F., Monfardini, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G.W., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Zylka, R.

“…High-resolution mapping of the hot gas in galaxy clusters is a key tool for cluster-based cosmological analyses. Taking advantage of the NIKA2 millimeter…”
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The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population by Pratt, G. W., Arnaud, M., Biviano, A., Eckert, D., Ettori, S., Nagai, D., Okabe, N., Reiprich, T. H.

“…The total mass of a galaxy cluster is one of its most fundamental properties. Together with the redshift, the mass links observation and theory, allowing us to…”
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The MADPSZ catalogue of Planck clusters over the DES region: extending to lower mass and higher redshift by Hernández-Lang, D., Mohr, J.J., Klein, M., Grandis, S., Melin, J.-B., Tarrío, P., Arnaud, M., Pratt, G.W., Abbott, T.M.C., Aguena, M., Alves, O., Andrade-Oliveira, F., Bacon, D., Bertin, E., Brooks, D., Burke, D.L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F.J., Costanzi, M., da Costa, L.N., Pereira, M.E.S., Desai, S., Diehl, H.T., Doel, P., Everett, S., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gruen, D., Gruendl, R.A., Gschwend, J., Gutierrez, G., Hinton, S.R., Hollowood, D.L., Honscheid, K., James, D.J., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A.A., Raveri, M., Rodriguez-Monroy, M., Romer, A.K., Scarpine, V., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Tarle, G., Thomas, D., Weaverdyck, N.

“…We present the first systematic follow-up of Planck Sunyaev-Zeldovich effect (SZE) selected candidates down to signal-to-noise (S/N) of 3 over the 5000 deg$^2$…”
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Unveiling the merger dynamics of the most massive MaDCoWS cluster at $z = 1.2$ from a multi-wavelength mapping of its intracluster medium properties by Ruppin, F., Mcdonald, M., Brodwin, M., Adam, R., Ade, P., André, P., Andrianasolo, A., Arnaud, M., Aussel, H., Bartalucci, I., Bautz, M.W., Beelen, A., Benoît, A., Bideaud, A., Bourrion, O., Calvo, M., Catalano, A., Comis, B., Decker, B., de Petris, M., Désert, F.-X., Doyle, S., Driessen, E.F.C., Eisenhardt, P.R.M., Gomez, A., Gonzalez, A.H., Goupy, J., Keruzore, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macias-Perez, J.F., Mauskopf, P., Mayet, F., Monfardini, A., Moravec, E., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G.W., Reveret, V., Ritacco, A., Romero, C., Roussel, H., Schuster, K., Shu, S., Sievers, A., Stanford, S.A., Stern, D., Tucker, C., Zylka, R.

“…The characterization of the Intra-Cluster Medium (ICM) properties of high-redshift galaxy clusters is fundamental to our understanding of large-scale structure…”
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The NIKA2 Sunyaev-Zeldovich Large Program: Sample and upcoming product public release by Perotto, L., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Barrena, R., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Ejlali, G., Ferragamo, A., Gomez, A., Goupy, J., Hanser, C., Katsioli, S., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.F., Madden, S. C., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Moyer-Anin, A., Muñoz-Echeverría, M., Paliwal, A., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G.W., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Tucker, C., Yepes, G.

“…The NIKA2 camera operating at the IRAM 30-m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zel’dovich effect towards galaxy…”
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The NIKA2 Sunyaev-Zeldovich Large Program by Perotto L., Adam R., Ade P., Ajeddig H., André P., Artis E., Aussel H., Barrena R., Bartalucci I., Beelen A., Benoît A., Berta S., Bing L., Bourrion O., Calvo M., Catalano A., De Petris M., Désert F.-X., Doyle S., Driessen E. F. C., Ejlali G., Ferragamo A., Gomez A., Goupy J., Hanser C., Katsioli S., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Madden S. C., Maury A., Mauskopf P., Mayet F., Monfardini A., Moyer-Anin A., Muñoz-Echeverría M., Paliwal A., Pisano G., Pointecouteau E., Ponthieu N., Pratt G.W., Revéret V., Rigby A. J., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Sievers A., Tucker C., Yepes G.

“…The NIKA2 camera operating at the IRAM 30-m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zel’dovich effect towards galaxy…”
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PHEMTO: The Polarimetric High Energy Modular Telescope Observatory by Laurent, P., Acero, F., Beckmann, V., Brandt, S., Cangemi, F., Civitani, M., Clavel, M., Coleiro, A., Curado, R., Ferrando, P., Ferrigno, C., Frontera, F., Gastaldello, F., Gotz, D., Gouiffes, C., Grinberg, V., Hanlon, L., Hartmann, D., Maggi, P., Marin, F., Meuris, A., Okajima, T., Pareschi, G., Pratt, G. W., Rea, N., Rodriguez, J., Rossetti, M., Spiga, D., Virgili, E., Zane, S.

“…Based upon dual focusing techniques, the Polarimetric High-Energy Modular Telescope Observatory (PHEMTO) is designed to have performance several orders of…”
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Multi-probe analysis of the galaxy cluster CL J1226.9+3332: Hydrostatic mass and hydrostatic-to-lensing bias by Muñoz-Echeverría, M., Adam, R., Ade, P., Ajeddig, H., André, P., Arnaud, M., Artis, E., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Ferragamo, A., Gomez, A., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.-F., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Paliwal, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G. W., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Yepes, G.

“…We present a multi-probe analysis of the well-known galaxy cluster CL J1226.9+3332 as a proof of concept for multi-wavelength studies within the framework of…”
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The LPSZ-CLASH galaxy cluster sample: Combining lensing and hydrostatic mass estimates by Muñoz-Echeverría, M., Adam, R., Ade, P., Ajeddig, H., André, P., Arnaud, M., Artis, E., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Ferragamo, A., Gomez, A., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.-F., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Paliwal, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G. W., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Yepes, G.

“…Starting from the clusters included in the NIKA sample and in the NIKA2 Sunyaev-Zel’dovich Large Program (LPSZ) we have selected a sample of six common objects…”
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PSZ2 G091: A massive double cluster at z ~ 0.822 observed by the NIKA2 camera by Artis, E., Adam, R., Ade, P., Ajeddig, H., André, P., Arnaud, M., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Ferragamo, A., Gomez, A., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.-F., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Muñoz-Echeverría, M., Paliwal, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G. W., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Yepes, G.

“…PSZ2 G091.83+26.11 is a massive galaxy cluster with M 500 = 7:43 × 10 14 M ⊙ at z = 0:822. This object exhibits a complex morphology with a clear bimodality…”
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The use of ultrasound in vivo to determine acute change in the mechanical properties of bone following intense physical activity by Rubin, C T, Pratt, G W, Porter, A L, Lanyon, L E, Poss, R

“…The velocity of ultrasound was measured transcutaneously across the patella and tibia in 98 volunteers both before and after running the 26 mile Boston…”
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Mapping the gas thermodynamic properties of the massive cluster merger MOO J1142+1527 at z = 1.2 by Ruppin, F., Adam, R., Ade, P., André, P., Andrianasolo, A., Arnaud, M., Aussel, H., Bartalucci, I., Bautz, M.W., Beelen, A., Benoît, A., Bideaud, A., Bourrion, O., Brodwin, M., Calvo, M., Catalano, A., Comis, B., Decker, B., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Eisenhardt, P. R. M., Gomez, A., Gonzalez, A. H., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J.F., Mauskopf, P., Mayet, F., McDonald, M., Monfardini, A., Moravec, E., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G. W., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Schuster, K., Shu, S., Sievers, A., Stanford, S. A., Stern, D., Tucker, C., Zylka, R.

“…We present the results of the analysis of the very massive cluster MOO J1142+1527 at a redshift z = 1.2 based on high angular resolution NIKA2…”
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Sorption of water, sodium sulfate, and water-soluble alcohols by [potato and corn] starch granules in aqueous suspension by BeMiller, J.N, Pratt, G.W

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Merging clusters of galaxies observed with XMM-Newton by Belsole, E., Sauvageot, J.-L., Pratt, G.W., Bourdin, H.

“…We present results from the XMM-Newton observations of our ongoing program on merging clusters. To date three clusters have been observed, covering the…”
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