S
S. Palladino
Researcher at University of Cincinnati
Publications - 7
Citations - 141
S. Palladino is an academic researcher from University of Cincinnati. The author has contributed to research in topics: Cosmic microwave background & South Pole Telescope. The author has an hindex of 4, co-authored 7 publications receiving 111 citations. Previous affiliations of S. Palladino include University of Toronto.
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Proceedings ArticleDOI
BICEP Array: A multi-frequency degree-scale CMB polarimeter
Howard Hui,Peter A. R. Ade,Zeeshan Ahmed,Randol W. Aikin,Kate D. Alexander,Denis Barkats,S. J. Benton,Colin A. Bischoff,James J. Bock,R. Bowens-Rubin,Justus A. Brevik,I. Buder,E. Bullock,Victor Buza,Jake Connors,J. Cornelison,B. P. Crill,M. Crumrine,Marion Dierickx,L. Duband,Cora Dvorkin,Jeffrey P. Filippini,S. Fliescher,J. A. Grayson,G. Hall,Mark Halpern,Sarah M. Harrison,S. R. Hildebrandt,Gene C. Hilton,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,J. P. Kaufman,Brian Keating,S. Kefeli,S. A. Kernasovskiy,John M Kovac,C. L. Kuo,Kam Y. Lau,N. A. Larsen,E. M. Leitch,M. Lueker,K. G. Megerian,Lorenzo Moncelsi,T. Namikawa,Calvin B. Netterfield,H. T. Nguyen,Roger O'Brient,R. W. Ogburn,S. Palladino,C. Pryke,B. Racine,S. Richter,R. Schwarz,Alessandro Schillaci,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Z. K. Staniszewski,Bryan Steinbach,Rashmikant V. Sudiwala,G. P. Teply,K. L. Thompson,J. E. Tolan,Carole Tucker,A. D. Turner,C. Umiltà,Abigail G. Vieregg,A. Wandui,A. C. Weber,Donald V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,Eui-Hyeok Yang,Ki Won Yoon,C. Zhang +77 more
TL;DR: The Bicep Array as discussed by the authors is the latest multi-frequency instrument in the BICEp/Keck Array program, consisting of four 550mm aperture refractive telescopes observing the polarization of the cosmic microwave background (CMB) at 30/40, 95, 150 and 220/270 GHz with over 30,000 detectors.
Proceedings ArticleDOI
BICEP Array: a multi-frequency degree-scale CMB polarimeter
Howard Hui,Peter A. R. Ade,Zeeshan Ahmed,Randol W. Aikin,Kate D. Alexander,Denis Barkats,S. J. Benton,Colin A. Bischoff,James J. Bock,R. Bowens-Rubin,Justus A. Brevik,I. Buder,E. Bullock,Victor Buza,Jake Connors,J. Cornelison,B. P. Crill,M. Crumrine,Marion Dierickx,L. Duband,Cora Dvorkin,Jeffrey P. Filippini,S. Fliescher,J. A. Grayson,G. Hall,Mark Halpern,Sarah M. Harrison,S. R. Hildebrandt,Gene C. Hilton,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,J. P. Kaufman,Brian Keating,S. Kefeli,S. A. Kernasovskiy,John M Kovac,C. L. Kuo,Kam Y. Lau,N. A. Larsen,E. M. Leitch,M. Lueker,K. G. Megerian,Lorenzo Moncelsi,T. Namikawa,Calvin B. Netterfield,H. T. Nguyen,Roger O'Brient,R. W. Ogburn,S. Palladino,C. Pryke,B. Racine,S. Richter,R. Schwarz,Alessandro Schillaci,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Z. K. Staniszewski,Bryan Steinbach,Rashmikant V. Sudiwala,G. P. Teply,K. L. Thompson,J. E. Tolan,Carole Tucker,A. D. Turner,C. Umiltà,Abigail G. Vieregg,A. Wandui,A. C. Weber,Donald V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,Eui-Hyeok Yang,Ki Won Yoon,C. Zhang +77 more
TL;DR: The BICEP Array as mentioned in this paper is the newest multi-frequency instrument in the BiceP/Keck Array program, consisting of four 550 mm aperture refractive telescopes observing the polarization of the cosmic microwave background (CMB) at 30/40, 95, 150 and 220/270 GHz with over 30,000 detectors.
Journal ArticleDOI
Design and Performance of the First BICEP Array Receiver
Alessandro Schillaci,Peter A. R. Ade,Zeeshan Ahmed,Mandana Amiri,Denis Barkats,R. Basu Thakur,Colin A. Bischoff,James J. Bock,H. Boenish,E. Bullock,Victor Buza,J. Cheshire,Jake Connors,J. Cornelison,M. Crumrine,A. Cukierman,Marion Dierickx,Lionel Duband,S. Fatigoni,Jeffrey P. Filippini,G. Hall,Mark Halpern,Sarah M. Harrison,S. Henderson,Sergi R. Hildebrandt,Gene C. Hilton,Howard Hui,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,S. Kefeli,John M Kovac,Chao-Lin Kuo,King Tong Lau,K. G. Megerian,Lorenzo Moncelsi,Toshiya Namikawa,H. T. Nguyen,Roger O'Brient,S. Palladino,N. Precup,T. Prouvé,C. Pryke,B. Racine,Carl D. Reintsema,S. Richter,Benjamin L. Schmitt,R. Schwarz,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Bryan Steinbach,Rashmikant V. Sudiwala,Keith L. Thompson,Carole Tucker,Anthony D. Turner,C. Umiltà,Abigail G. Vieregg,A. Wandui,A. C. Weber,Donald V. Wiebe,J. Willmert,W. L. K. Wu,Eui-Hyeok Yang,Ki Won Yoon,Edward D. Young,Che-Hang Yu,Chao Zhang +68 more
TL;DR: The BICEP/Keck (BK) experiment targets this primordial signature, the amplitude of which is parameterized by the tensor-to-scalar ratio r, by observing the polarized microwave sky through the exceptionally clean and stable atmosphere at the South Pole as discussed by the authors.
Proceedings ArticleDOI
Ultra-thin large-aperture vacuum windows for millimeter wavelengths receivers
Denis Barkats,Marion Dierickx,John M Kovac,Chris Pentacoff,Peter A. R. Ade,Zeeshan Ahmed,Randol W. Aikin,Kate D. Alexander,S. J. Benton,Colin A. Bischoff,J. J. Bock,R. Bowens-Rubin,Justus A. Brevik,I. Buder,E. Bullock,Victor Buza,J. Connors,J. Cornelison,B. P. Crill,M. Crumrine,L. Duband,Cora Dvorkin,Jeffrey P. Filippini,S. Fliescher,J. A. Grayson,G. Hall,Mark Halpern,S. A. Harrison,S. R. Hildebrandt,G. C. Hilton,Howard Hui,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,J. P. Kaufman,B. G. Keating,S. Kefeli,S. A. Kernasovskiy,C. L. Kuo,K. Lau,N. A. Larsen,E. M. Leitch,M. Lueker,K. G. Megerian,Lorenzo Moncelsi,T. Namikawa,H. T. Nguyen,Roger O'Brient,R. W. Ogburn,S. Palladino,C. Pryke,B. Racine,S. Richter,R. Schwarz,Alessandro Schillaci,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Z. K. Staniszewski,Bryan Steinbach,R. V. Sudiwala,Grant Teply,K. L. Thompson,J. E. Tolan,Carole Tucker,A. D. Turner,C. Umiltà,Abigail G. Vieregg,A. Wandui,A. C. Weber,D. V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,Hong Yang,K. W. Yoon,C. Zhang +77 more
TL;DR: In this article, the suitability of high-modulus polyethylene windows for ground-based CMB experiments was investigated for ground and future receivers in the Bicep/Keck Array program.
Journal ArticleDOI
Characterizing the Sensitivity of 40 GHz TES Bolometers for BICEP Array
Chao Zhang,P. A. R. Ade,Zeeshan Ahmed,Mandana Amiri,Denis Barkats,R. Basu Thakur,Colin A. Bischoff,James J. Bock,H. Boenish,E. Bullock,Victor Buza,J. Cheshire,Jake Connors,J. Cornelison,M. Crumrine,A. Cukierman,Marion Dierickx,Lionel Duband,S. Fatigoni,Jeffrey P. Filippini,G. Hall,Mark Halpern,Sarah M. Harrison,S. Henderson,Sergi R. Hildebrandt,Gene C. Hilton,Howard Hui,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,S. Kefeli,John M Kovac,Chao-Lin Kuo,King Tong Lau,K. G. Megerian,Lorenzo Moncelsi,Toshiya Namikawa,H. T. Nguyen,Roger O'Brient,S. Palladino,N. Precup,T. Prouvé,C. Pryke,B. Racine,Carl D. Reintsema,S. Richter,Alessandro Schillaci,Benjamin L. Schmitt,R. Schwarz,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Bryan Steinbach,Rashmikant V. Sudiwala,Keith L. Thompson,Carole Tucker,Anthony D. Turner,C. Umiltà,Abigail G. Vieregg,A. Wandui,A. C. Weber,Donald V. Wiebe,J. Willmert,W. L. K. Wu,Eui-Hyeok Yang,Ki Won Yoon,E. Young,Che-Hang Yu +68 more
TL;DR: The 30/40 GHz detector of the BICEP/Keck Array as mentioned in this paper achieved a per bolometer NEP including all noise components of $2.07\times 10^{-17}\,\mathrm{W}/\sqrt{\hbox{Hz}}.