Search Results - "Precup, N"

Design and Performance of the First BICEP Array Receiver by Schillaci, A., Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, Bischoff, C. A., Bock, J. J., Boenish, H., Bullock, E., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Dierickx, M., Duband, L., Fatigoni, S., Filippini, J. P., Hall, G., Halpern, M., Harrison, S., Henderson, S., Hildebrandt, S. R., Hilton, G. C., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Karpel, E., Kefeli, S., Kovac, J. M., Kuo, C. L., Lau, K., Megerian, K. G., Moncelsi, L., Namikawa, T., Nguyen, H. T., O’Brient, R., Palladino, S., Precup, N., Prouve, T., Pryke, C., Racine, B., Reintsema, C. D., Richter, S., Schmitt, B. L., Schwarz, R., Sheehy, C. D., Soliman, A., Germaine, T. St, Steinbach, B., Sudiwala, R. V., Thompson, K. L., Tucker, C., Turner, A. D., Umiltà, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wu, W. L. K., Yang, E., Yoon, K. W., Young, E., Yu, C., Zhang, C.

“…Branches of cosmic inflationary models, such as slow-roll inflation, predict a background of primordial gravitational waves that imprints a unique odd-parity…”
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Plastic Laminate Antireflective Coatings for Millimeter-Wave Optics in BICEP Array by Dierickx, M., Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Bischoff, C. A., Beck, D., Bock, J. J., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E., Duband, L., Eiben, M., Fatigoni, S., Filippini, J. P., Goeckner-Wald, N., Goldfinger, D. C., Grayson, J. A., Grimes, P., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S. R., Hilton, G. C., Hubmayr, J., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Kefeli, S., Kovac, J. M., Kuo, C. L., Lau, K., Leitch, E. M., Lennox, A., Megerian, K. G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H. T., O’Brient, R., Palladino, S., Petroff, M., Precup, N., Prouve, T., Pryke, C., Racine, B., Reintsema, C. D., Santalucia, D., Schillaci, A., Schmitt, B. L., Singari, B., Soliman, A., Germaine, T. St, Steinbach, B., Sudiwala, R. V., Thompson, K. L., Tucker, C., Turner, A. D., Umiltà, C., Verges, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wu, W. L. K., Yang, E., Yoon, K. W., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S.

“…The BICEP/ Keck series of experiments target the cosmic microwave background at degree-scale resolution from the South Pole. Over the next few years, the…”
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Characterizing the Sensitivity of 40 GHz TES Bolometers for BICEP Array by Zhang, C., Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, Bischoff, C. A., Bock, J. J., Boenish, H., Bullock, E., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Dierickx, M., Duband, L., Fatigoni, S., Filippini, J. P., Hall, G., Halpern, M., Harrison, S., Henderson, S., Hildebrandt, S. R., Hilton, G. C., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Karpel, E., Kefeli, S., Kovac, J. M., Kuo, C. L., Lau, K., Megerian, K. G., Moncelsi, L., Namikawa, T., Nguyen, H. T., O’Brient, R., Palladino, S., Precup, N., Prouvé, T., Pryke, C., Racine, B., Reintsema, C. D., Richter, S., Schillaci, A., Schmitt, B., Schwarz, R., Sheehy, C. D., Soliman, A., Germaine, T. St, Steinbach, B., Sudiwala, R. V., Thompson, K. L., Tucker, C., Turner, A. D., Umiltà, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wu, W. L. K., Yang, E., Yoon, K. W., Young, E., Yu, C.

“…The BICEP/Keck (BK) experiment aims to detect the imprint of primordial gravitational waves in the cosmic microwave background polarization, which would be…”
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Optical Design and Characterization of 40-GHz Detector and Module for the BICEP Array by Soliman, A., Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, Bischoff, C. A., Bock, J. J., Boenish, H., Bullock, E., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Dierickx, M., Duband, L., Fatigoni, S., Filippini, J. P., Hall, G., Halpern, M., Harrison, S., Henderson, S., Hildebrandt, S. R., Hilton, G. C., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Karpel, E., Kefeli, S., Kovac, J. M., Kuo, C. L., Lau, K., Megerian, K. G., Moncelsi, L., Namikawa, T., Nguyen, H. T., O’Brient, R., Palladino, S., Prouve, T., Precup, N., Pryke, C., Racine, B., Reintsema, C. D., Richter, S., Schmitt, B., Schwarz, R., Sheehy, C. D., Schillaci, A., Germaine, T. St, Steinbach, B., Sudiwala, R. V., Thompson, K. L., Tucker, C., Turner, A. D., Umiltà, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wu, W. L. K., Yang, E., Yoon, K. W., Young, E., Yu, C., Zhang, C.

“…Families of cosmic inflation models predict a primordial gravitational-wave background that imprints B-mode polarization pattern in the cosmic microwave…”
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BICEP Array: 150 GHz Detector Module Development by Schillaci, Alessandro, Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Bischoff, C. A., Beck, D., Bock, J. J., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E., Dierickx, M., Duband, L., Eiben, M., Fatigoni, S., Filippini, J. P., Giannakopoulos, C., Goeckner-Wald, N., Goldfinger, D., Grayson, J. A., Grimes, P., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S. R., Hilton, G. C., Hubmayr, J., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Kefeli, S., Kovac, J. M., Kuo, C. L., Lau, K., Leitch, E. M., Lennox, A., Megerian, K. G., Miller, O. Y., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H. T., O’Brient, R., Palladino, S., Petroff, M., Precup, N., Prouve, T., Pryke, C., Racine, B., Reintsema, C. D., Schmitt, B. L., Singari, B., Soliman, A., Germaine, T. St, Steinbach, B., Sudiwala, R. V., Thompson, K. L., Tucker, C., Turner, A. D., Umiltà, C., Verges, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wu, W. L. K., Yang, E., Yoon, K. W., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S.

“…The Background Imaging of Cosmic Extragalactic Polarization (BICEP)/Keck (BK) collaboration is currently leading the quest for the highest-sensitivity…”
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Constraining Inflation with the BICEP/Keck CMB Polarization Experiments by Collaboration, The BICEP/Keck, :, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Beck, D, Bock, J. J, Boenish, H, Buza, V, CheshireIV, J. R, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Denison, E. V, Dierickx, M, Duband, L, Eiben, M, Elwood, B, Fatigoni, S, Filippini, J. P, Gao, M, Giannakopoulos, C, Goeckner-Wald, N, Goldfinger, D. C, Grayson, J, Grimes, P, Hall, G, Halal, G, Halpern, M, Hand, E, Harrison, S, Henderson, S, Hubmayr, J, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Kefeli, S, Kovac, J. M, Kuo, C L, Lau, K, Lennox, A, Liu, T, Megerian, K. G, Minutolo, L, Moncelsi, L, Nakato, Y, Namikawa, T, Nguyen, H. T, O'Brient, R, Palladino, S, Petroff, M, Polish, A, Precup, N, Prouve, T, Pryke, C, Racine, B, Reintsema, C. D, Romand, T, Salatino, M, Schillaci, A, Schmitt, B. L, Singari, B, Soliman, A, Germaine, T. St, Steiger, A, Steinbach, B, Sudiwala, R. V, Thompson, K. L, Tucker, C, Turner, A. D, Vergès, C, Vieregg, A. G, Wandui, A, Weber, A. C, Willmert, J, Wu, W. L. K, Yang, H, Yoon, K. W, Young, E, Yu, C, Zeng, L, Zhang, C, Zhang, S

“…The BICEP/$\textit{Keck}$ (BK) series of cosmic microwave background (CMB) polarization experiments has, over the past decade and a half, produced a series of…”
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2022 Upgrade and Improved Low Frequency Camera Sensitivity for CMB Observation at the South Pole by Soliman, A, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Beck, D, Bock, J. J, Buza, V, Cheshire, J, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A. J, Denison, E. V, Dierickx, M. I, Duband, L, Eiben, M, Fatigoni, S, Filippini, J. P, Giannakopoulos, C, Goeckner-Wald, N, Goldfinger, D. C, Grayson, J, Grimes, P. K, Hall, G, Halal, G, Halpern, M, Hand, E, Harrison, S. A, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hubmayr, J, Hui, H, Irwin, K. D, Kangh, J, Karkare, K. S, Kefeli, S, Kovac, J. M, Kuo, C. L, Lau, K, Leitch, E. M, Lennox, A, Liu, T, Megerian, K. G, Minutolo, L, Moncelsi, L, Nakato, Y, Namikawa, T, Nguyen, H. T, O'Brient, R, Palladino, S, Petroff, M. A, Precup, N, Prouve, T, Pryke, C, Racine, B, Reintsema, C. D, Salatino, M, Schillaci, A, Schmitt, B. L, Singari, B, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Thompson, K. L, Tsai, C, Tucker, C, Turner, A. D, Umiltà, C, Vergès, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wu, W. L. K, Yang, H, Yoon, K. W, Young, E, Yu, C, Zeng, L, Zhang, C, Zhang, S

“…Constraining the Galactic foregrounds with multi-frequency Cosmic Microwave Background (CMB) observations is an essential step towards ultimately reaching the…”
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BICEP Array: 150 GHz detector module development by Schillaci, A, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Beck, D, Bock, J. J, Buza, V, Cheshire, J, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Denison, E, Dierickx, M, Duband, L, Eiben, M, Fatigoni, S, Filippini, J. P, Giannakopoulos, C, Goeckner-Wald, N, Goldfinger, D, Grayson, J. A, Grimes, P, Hall, G, Halal, G, Halpern, M, Hand, E, Harrison, S, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hubmayr, J, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Kefeli, S, Kovac, J. M, Kuo, C. L, Lau, K, Leitch, E. M, Lennox, A, Megerian, K. G, Miller, O. Y, Minutolo, L, Moncelsi, L, Nakato, Y, Namikawa, T, Nguyen, H. T, Brient, R. O', Palladino, S, Petroff, M, Precup, N, Prouve, T, Pryke, C, Racine, B, Reintsema, C. D, Schmitt, B. L, Singari, B, Soliman, A, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Thompson, K. L, Tucker, C, Turner, A. D, Umiltá, C, Verges, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C, Zeng, L, Zhang, C, Zhang, S

“…The BICEP/Keck Collaboration is currently leading the quest to the highest sensitivity measurements of the polarized CMB anisotropies on degree scale with a…”
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Analysis of Temperature-to-Polarization Leakage in BICEP3 and Keck CMB Data from 2016 to 2018 by Collaboration, The BICEP/Keck, :, Germaine, T. St, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Bock, J. J, Boenish, H, Bullock, E, Buza, V, Cheshire, J. R, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Denison, E, Dierickx, M, Duband, L, Eiben, M, Fatigoni, S, Filippini, J. P, Fliescher, S, Goeckner-Wald, N, Goldfinger, D. C, Grayson, J. A, Grimes, P, Hall, G, Halpern, M, Harrison, S. A, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hubmayr, J, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Karpel, E, Kefeli, S, Kernasovskiy, S. A, Kovac, J. M, Kuo, C. L, Lau, K, Leitch, E. M, Megerian, K. G, Minutolo, L, Moncelsi, L, Nakato, Y, Namikawa, T, Nguyen, H. T, O'Brient, R, OgburnIV, R. W, Palladino, S, Precup, N, Prouve, T, Pryke, C, Racine, B, Reintsema, C. D, Richter, S, Schillaci, A, Schmitt, B. L, Schwarz, R, Sheehy, C. D, Soliman, A, Steinbach, B, Sudiwala, R. V, Teply, G. P, Thompson, K. L, Tolan, J. E, Tucker, C, Turner, A. D, Umiltà, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wong, C. L, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C, Zeng, L, Zhang, C, Zhang, S

“…Proc. SPIE 11453, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, 114532E (15 December 2020) The BICEP/Keck Array…”
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Observing low elevation sky and the CMB Cold Spot with BICEP3 at the South Pole by Kang, J, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Bock, J. J, Boenish, H, Bullock, E, Buza, V, Cheshire, J. R, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Denison, E, Dierickx, M, Duband, L, Eiben, M, Fatigoni, S, Filippini, J. P, Fliescher, S, Goeckner-Wald, N, Goldfinger, D. C, Grayson, J. A, Grimes, P, Hall, G, Halpern, M, Harrison, S. A, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hubmayr, J, Hui, H, Irwin, K. D, Karkare, K. S, Karpel, E, Kefeli, S, Kernasovskiy, S. A, Kovac, J. M, Kuo, C. L, Lau, K, Leitch, E. M, Megerian, K. G, Minutolo, L, Moncelsi, L, Nakato, Y, Namikawa, T, Nguyen, H. T, O'Brient, R, OgburnIV, R. W, Palladino, S, Precup, N, Prouve, T, Pryke, C, Racine, B, Reintsema, C. D, Richter, S, Schillaci, A, Schmitt, B. L, Schwarz, R, Sheehy, C. D, Soliman, A, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Teply, G. P, Thompson, K. L, Tolan, J. E, Tucker, C, Turner, A. D, Umiltà, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wong, C. L, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C, Zeng, L, Zhang, C, Zhang, S

“…Proc. SPIE 11453, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, 114532D (13 December 2020) BICEP3 is a 520 mm…”
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Polarization Calibration of the BICEP3 CMB polarimeter at the South Pole by Cornelison, J, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Bock, J. J, Boenish, H, Bullock, E, Buza, V, Cheshire, J. R, Connors, J, Crumrine, M, Cukierman, A, Denison, E, Dierickx, M, Duband, L, Eiben, M, Fatigoni, S, Filippini, J. P, Fliescher, S, Goeckner-Wald, N, Goldfinger, D. C, Grayson, J. A, Grimes, P, Hall, G, Halpern, M, Harrison, S. A, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hubmayr, J, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Karpel, E, Kefeli, S, Kernasovskiy, S. A, Kovac, J. M, Kuo, C. L, Lau, K, Leitch, E. M, Megerian, K. G, Minutolo, L, Moncelsi, L, Nakato, Y, Namikawa, T, Nguyen, H. T, O'Brient, R, OgburnIV, R. W, Palladino, S, Precup, N, Prouve, T, Pryke, C, Racine, B, Reintsema, C. D, Richter, S, Schillaci, A, Schmitt, B. L, Schwarz, R, Sheehy, C. D, Soliman, A, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Teply, G. P, Thompson, K. L, Tolan, J. E, Tucker, C, Turner, A. D, Umiltà, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wong, C. L, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C, Zeng, L, Zhang, C, Zhang, S

“…The BICEP3 CMB Polarimeter is a small-aperture refracting telescope located at the South Pole and is specifically designed to search for the possible signature…”
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Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole by Moncelsi, L, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Bock, J. J, Buza, V, Cheshire, J, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Denison, E. V, Dierickx, M, Duband, L, Eiben, M, Fatigoni, S, Filippini, J. P, Goeckner-Wald, N, Goldfinger, D. C, Grayson, J, Grimes, P, Hall, G, Halpern, M, Harrison, S, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hubmayr, J, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Kefeli, S, Kovac, J. M, Kuo, C. L, Lau, K, Leitch, E. M, Megerian, K. G, Minutolo, L, Nakato, Y, Namikawa, T, Nguyen, H. T, O'Brient, R, Palladino, S, Precup, N, Prouve, T, Pryke, C, Racine, B, Reintsema, C. D, Schillaci, A, Schmitt, B. L, Soliman, A, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Thompson, K. L, Tucker, C, Turner, A. D, Umiltà, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C, Zeng, L, Zhang, C, Zhang, S

“…A detection of curl-type ($B$-mode) polarization of the primary CMB would be direct evidence for the inflationary paradigm of the origin of the Universe. The…”
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Design and performance of the first BICEP Array receiver by Schillaci, A, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Bock, J. J, Boenish, H, Bullock, E, Buza, V, Cheshire, J, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Dierickx, M, Duband, L, Fatigoni, S, Filippini, J. P, Hall, G, Halpern, M, Harrison, S, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Karpel, E, Kefeli, S, Kovac, J. M, Kuo, C. L, Lau, K, Megerian, K. G, Moncelsi, L, Namikawa, T, Nguyen, H. T, O'Brient, R, Palladino, S, Precup, N, Prouvé, T, Pryke, C, Racine, B, Reintsema, C. D, Richter, S, Schmitt, B, Schwarz, R, Sheehy, C. D, Soliman, A, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Thompson, K. L, Tucker, C, Turner, A. D, Umiltà, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C, Zhang, C

“…Branches of cosmic inflationary models, such as slow-roll inflation, predict a background of primordial gravitational waves that imprints a unique odd-parity…”
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Characterizing the Sensitivity of 40 GHz TES Bolometers for BICEP Array by Zhang, C, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Bock, J. J, Boenish, H, Bullock, E, Buza, V, Cheshire, J, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Dierickx, M, Duband, L, Fatigoni, S, Filippini, J. P, Hall, G, Halpern, M, Harrison, S, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Karpel, E, Kefeli, S, Kovac, J. M, Kuo, C. L, Lau, K, Megerian, K. G, Moncelsi, L, Namikawa, T, Nguyen, H. T, O'Brient, R, Palladino, S, Precup, N, Prouvé, T, Pryke, C, Racine, B, Reintsema, C. D, Richter, S, Schillaci, A, Schmitt, B, Schwarz, R, Sheehy, C. D, Soliman, A, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Thompson, K. L, Tucker, C, Turner, A. D, Umiltà, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C

“…The BICEP/Keck (BK) experiment aims to detect the imprint of primordial gravitational waves in the Cosmic Microwave Background polarization, which would be…”
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Optical Design and Characterization of 40-GHz Detector and Module for the BICEP Array by Soliman, A, Ade, P. A. R, Ahmed, Z, Amiri, M, Barkats, D, Thakur, R. Basu, Bischoff, C. A, Bock, J. J, Boenish, H, Bullock, E, Buza, V, Cheshire, J, Connors, J, Cornelison, J, Crumrine, M, Cukierman, A, Dierickx, M, Duband, L, Fatigoni, S, Filippini, J. P, Hall, G, Halpern, M, Harrison, S, Henderson, S, Hildebrandt, S. R, Hilton, G. C, Hui, H, Irwin, K. D, Kang, J, Karkare, K. S, Karpel, E, Kefeli, S, Kovac, J. M, Kuo, C. L, Lau, K, Megerian, K. G, Moncelsi, L, Namikawa, T, Nguyen, H. T, OBrient, R, Palladino, S, Prouve, T, Precup, N, Pryke, C, Racine, B, Reintsema, C. D, Richter, S, Schmitt, B, Schwarz, R, Sheehy, C. D, Schillaci, A, Germaine, T. St, Steinbach, B, Sudiwala, R. V, Thompson, K. L, Tucker, C, Turner, A. D, Umilta, C, Vieregg, A. G, Wandui, A, Weber, A. C, Wiebe, D. V, Willmert, J, Wu, W. L. K, Yang, E, Yoon, K. W, Young, E, Yu, C, Zhang, C

“…Families of cosmic inflation models predict a primordial gravitational-wave background that imprints B-mode polarization pattern in the Cosmic Microwave…”
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Treatment with antibiotics and chemotherapeutics by Precup, N

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Side effects from treatment with antibiotics and chemotherapeutics by Cilţea, E, Precup, N

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