Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Karen Byrum"'
Autor:
J. A. Sobrin, Thomas Cecil, E. V. Denison, S. S. Meyer, Kent D. Irwin, Peter A. R. Ade, W. L. Holzapfel, K. T. Story, K. Vanderlinde, A. E. Lowitz, V. Novosad, Donna Kubik, Aled Jones, John E. Carlstrom, G. I. Noble, Lincoln Bryant, Jason W. Henning, T. de Haan, Ki Won Yoon, Volodymyr Yefremenko, Nathan Whitehorn, Zeeshan Ahmed, T. Natoli, N. L. Harrington, Gene C. Hilton, Robert Gardner, Amy N. Bender, Carole Tucker, Jason Gallicchio, E. M. Leitch, C. L. Chang, A. E. Gambrel, W. B. Everett, A. Foster, Adrian T. Lee, D. Howe, D. Dutcher, Antony A. Stark, M. Jonas, Aritoki Suzuki, J. E. Ruhl, J. Stephen, Trupti Khaire, D. Riebel, Bradford Benson, J. F. Cliche, Joshua Montgomery, H. M. Cho, Ari Cukierman, Graeme Smecher, Z. Pan, Alexandra S. Rahlin, R. Basu Thakur, Matt Dobbs, K. R. Ferguson, Faustin Carter, Andrew Nadolski, Junjia Ding, Adam Anderson, M. R. Young, N. W. Halverson, Leila R. Vale, Oliver Jeong, Chao-Lin Kuo, Keith L. Thompson, John Groh, Karen Byrum, John E. Pearson, P. Paschos, N. Huang, A. Gilbert, J. Fu, A. M. Kofman, Jessica Avva, R. Guyser, Stephen Padin, C. M. Posada, Steve Kuhlmann, Joaquin Vieira, S. Guns, Daniel Michalik, Gensheng Wang, W. Quan, Erik Shirokoff, Peter S. Barry, A. H. Harke-Hosemann, H. T. Nguyen, M. Korman, J. T. Sayre
Publikováno v:
Journal of Low Temperature Physics. 199:182-191
Frequency-domain multiplexing (fMux) is an established technique for the readout of large arrays of transition edge sensor (TES) bolometers. Each TES in a multiplexing module has a unique AC voltage bias that is selected by a resonant filter. This sc
Autor:
M. Korman, Kent D. Irwin, W. L. Holzapfel, J. E. Ruhl, H. M. Cho, Ari Cukierman, V. Novosad, Donna Kubik, C. L. Chang, A. E. Gambrel, Alexandra S. Rahlin, Matt Dobbs, K. Vanderlinde, Keith L. Thompson, D. Howe, M. R. Young, Karen Byrum, Thomas Cecil, R. Basu Thakur, Erik Shirokoff, P. Paschos, Aled Jones, Peter A. R. Ade, Zeeshan Ahmed, Amy N. Bender, Ki Won Yoon, A. H. Harke-Hosemann, K. T. Story, A. E. Lowitz, H. T. Nguyen, D. Dutcher, Antony A. Stark, J. A. Sobrin, J. Stephen, Jason Gallicchio, Lincoln Bryant, Jason W. Henning, J. T. Sayre, S. S. Meyer, Volodymyr Yefremenko, Nathan Whitehorn, John E. Pearson, Peter S. Barry, N. L. Harrington, T. Natoli, Andrew Nadolski, Jessica Avva, G. I. Noble, Carole Tucker, R. Guyser, Stephen Padin, Trupti Khaire, N. Huang, A. Foster, Joshua Montgomery, A. Gilbert, C. M. Posada, Bradford Benson, Robert Gardner, J. F. Cliche, Steve Kuhlmann, Gene C. Hilton, Joaquin Vieira, Chao-Lin Kuo, S. Guns, Graeme Smecher, W. B. Everett, N. W. Halverson, Daniel Michalik, Gensheng Wang, John Groh, J. Fu, E. V. Denison, W. Quan, A. M. Kofman, M. Jonas, Leila R. Vale, Adrian T. Lee, Aritoki Suzuki, Faustin Carter, Junjia Ding, John E. Carlstrom, T. de Haan, E. M. Leitch, D. Riebel, Oliver Jeong, Z. Pan, K. R. Ferguson, Adam Anderson
Publikováno v:
Journal of Low Temperature Physics. 199:320-329
SPT-3G is a polarization-sensitive receiver, installed on the South Pole Telescope, that measures the anisotropy of the cosmic microwave background (CMB) from degree to arcminute scales. The receiver consists of ten 150~mm-diameter detector wafers, c
Autor:
Faustin Carter, S. E. Kuhlmann, Junjia Ding, Gene C. Hilton, J. C. Hood, A. T. Lee, M. Millea, Erik Shirokoff, Oliver Jeong, N. W. Halverson, Thomas Cecil, John E. Pearson, G. I. Noble, John E. Carlstrom, E. V. Denison, B. Thorne, K. Prabhu, C. L. Kuo, François R. Bouchet, M. Korman, Federico Bianchini, K. Dibert, S. Padin, Ethan Anderes, Neil Goeckner-Wald, D. Riebel, J. E. Ruhl, Jason W. Henning, Nikhel Gupta, N. Huang, M. Rouble, M. Jonas, RB Thakur, K. L. Thompson, J. T. Sayre, C. Tucker, A. A. Stark, A. Lowitz, M. A. Dobbs, N. L. Harrington, Z. Pan, Karen Byrum, A. H. Harke-Hosemann, C. Lu, Srinivasan Raghunathan, B. Riedel, C. L. Chang, A. Cukierman, Andreas Bender, Z. Ahmed, K. Aylor, E. M. Leitch, Alexandra S. Rahlin, S. Guns, J. A. Sobrin, K. W. Yoon, D. Howe, P. Chaubal, Young, Graeme Smecher, C. Umilta, J. F. Cliche, T. de Haan, Silvia Galli, H. Nguyen, Lloyd Knox, T. Natoli, K. Vanderlinde, T. M. Crawford, J. Fu, P. Paschos, S. S. Meyer, Christian L. Reichardt, H-M. Cho, L. R. Vale, A. Foster, K. T. Story, Karim Benabed, E. Hivon, E. Schiappucci, Anthony P. Jones, Andrew Nadolski, Lindsey Bleem, Jessica Avva, Peter S. Barry, L. Balkenhol, Bradford Benson, Yefremenko, R. Guyser, R. Gualtieri, C. M. Posada, Chang Feng, G. P. Holder, A. M. Kofman, Daniel Michalik, Novosad, J. D. Vieira, C. Daley, Gensheng Wang, W. L. Holzapfel, W. Quan, K. R. Ferguson, Adam Anderson, Gang Chen, Nathan Whitehorn, Robert Gardner, M. Archipley, Y. Omori, A. Suzuki, Lincoln Bryant, D. Dutcher, T.-L. Chou, Trupti Khaire, Joshua Montgomery, J. Stephen, A. E. Gambrel, Kent D. Irwin, W. L. K. Wu, Donna Kubik, P. A. R. Ade, W. B. Everett
Publikováno v:
Physical Review D. 104
We present measurements of the $E$-mode ($EE$) polarization power spectrum and temperature-$E$-mode ($TE$) cross-power spectrum of the cosmic microwave background using data collected by SPT-3G, the latest instrument installed on the South Pole Teles
Autor:
Gagik Tovmassian, F. Di Pierro, V. Masone, M. Ambrosio, C. B. Adams, N. La Palombara, A. Brill, Amy Furniss, K. Meagher, Marcos Santander, Nicola Giglietto, Olivier Hervet, Wystan Benbow, C. Bonavolontà, S. I. Mognet, Maria Ionica, A. Bouvier, S. P. Wakely, Vladimir Vassiliev, F. R. Pantaleo, Fernando Garfias, Alasdair E. Gent, Akira Okumura, S. Loporchio, A. Kuznetsov, J. Thornhill, J. H. Buckley, R. A. Cameron, L. Stiaccini, E. Fiandrini, E. Pueschel, S. Schlenstedt, R. J. White, L. Di Venere, Thomas Meures, G. Ambrosi, Arturo Iriarte, Daniel Nieto, M. Valentino, Riccardo Paoletti, Q. Feng, S. J. Fegan, A. Boiano, V. J. Guarino, David Kieda, G. Hughes, Julien Rousselle, G. Sironi, Justin Vandenbroucke, V. Vagelli, R. Shang, Enrico Giro, B. A. W. Mode, T. B. Humensky, A. Petrashyk, W. Jin, Maria Magdalena González, N. Otte, M. Caprai, Stefan Funk, M. Bitossi, D. Ribeiro, Karen Byrum, B. Bertucci, G. Pareschi, Andrea Rugliancich, Manel Errando, D. Depaoli, E. Roache, J. Ruíz-Díaz-Soto, T. C. Arlen, Michael Schneider, Jason John Watson, T. Nguyen, B. Stevenson, Jonathan Biteau, L. Tosti, Reshmi Mukherjee, David A. Williams, Jonathan S. Lapington, P. Kaaret, C. A. Johnson, Elisabetta Bissaldi, Gordon T. Richards, P. Fortin, Carla Aramo, Francesco Giordano, Salvo Scuderi, G. M. Foote, Hiroyasu Tajima, Richard Bose, Jamie Holder, R. Halliday, P. Yu, Rodolfo Canestrari, Ruben Alfaro, D. Ross, A. Zink, P. Wilcox, P. I. Batista, Matthew Wood, P. T. Reynolds, B. Kim, F. Licciulli, L. P. Taylor, A. M. Brown, M. Capasso, Corbin Covault
Publikováno v:
Astropart.Phys.
Astropart.Phys., 2021, 128, pp.102562. ⟨10.1016/j.astropartphys.2021.102562⟩
Astropart.Phys., 2021, 128, pp.102562. ⟨10.1016/j.astropartphys.2021.102562⟩
The Schwarzschild-Couder Telescope (SCT) is a telescope concept proposed for the Cherenkov Telescope Array. It employs a dual-mirror optical design to remove comatic aberrations over an $8^{\circ}$ field of view, and a high-density silicon photomulti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2965e10347bb20f743cfe163247b513f
http://hdl.handle.net/2318/1877441
http://hdl.handle.net/2318/1877441
Autor:
C. Aramo, Thomas Brian Humensky, Giovanni Pareschi, L. Stiaccini, Carmela Bonavolontà, A. Rugliancich, M. Caprai, E. Fiandrini, David Kieda, Daniel Nieto, A. Furniss, M. Bitossi, G. Sironi, S. J. Fegan, Wystan Benbow, B. Stevenson, C. Adams, Markus Garczarczyk, Justin Vandenbroucke, Riccardo Paoletti, B. Kim, Elisabetta Bissaldi, L. Di Venere, A. Petrashyk, R. A. Cameron, M. Valentino, Vladimir Vassiliev, Gagik Tovmassian, A. Boiano, S. Loporchio, Corbin Covault, Nicola Giglietto, P. Wilcox, A. Iriarte, Francesco Giordano, Reshmi Mukherjee, F. Garfias, A. Brill, S. P. Wakely, T. Meures, P. Kaarat, R. Shang, Michele Limon, K. Powell, Marcos Santander, B. A. W. Mode, F. R. Pantaleo, D. A. Williams, Julien Rousselle, G. Hughes, O. Hervet, V. Masone, R. Halliday, R. Bose, Q. Feng, Jade Powell, J. H. Buckley, Salvo Scuderi, S. Schlenstedt, M. Ambrosio, Peter Y. Yu, M. Capasso, Akira Okumura, F. Licciulli, A. Gent, J. Ruíz-Díaz-Soto, L. P. Taylor, B. Bertucci, M. Ionica, N. Otte, D. Ribeiro, E. Roache, N. La Palombara, Giovanni Ambrosi, W. Jin, Karen Byrum, L. Tosti, Ruben Alfaro, Maria Magdalena González, V. Vagelli
Publikováno v:
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Optics + Photonics 2020 Digital Forum
SPIE Optics + Photonics 2020 Digital Forum, Aug 2020, Online Conference, United States. pp.1148805, ⟨10.1117/12.2568134⟩
SPIE Optics + Photonics 2020 Digital Forum
SPIE Optics + Photonics 2020 Digital Forum, Aug 2020, Online Conference, United States. pp.1148805, ⟨10.1117/12.2568134⟩
For the first time in the history of ground-based $\gamma$-ray astronomy, the on-axis performance of the dual mirror, aspheric, aplanatic Schwarzschild-Couder optical system has been demonstrated in a $9.7$-m aperture imaging atmospheric Cherenkov te
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be68bcd2dd71ff9f9bc59e96834cf248
https://hal.archives-ouvertes.fr/hal-03047620
https://hal.archives-ouvertes.fr/hal-03047620
Autor:
Bonnie Fleming, Ian Shipsey, Marcel Demarteau, James Fast, Sunil Golwala, Young-Kee Kim, Abraham Seiden, James Hirschauer, Gabriella Sciolla, Ornella Palamara, Kate Scholberg, Jodi Cooley, Dan McKinsey, Clarence Chang, Brenna Flaugher, Sarah Demers, Monica Pepe-Altarelli, Francesco Lanni, Roger Rusack, Roxanne Guenette, Jocelyn Monroe, Lindley Winslow, Peter Krizan, Andrew Geraci, Kent Irwin, Gabriella Carini, Mitch Newcomer, Marina Artuso, Carl Haber, Darin Acosta, Tulika Bose, Michael Begel, Meenakshi Narain, Daniel Dwyer, Amy Connolly, Andrew Sonnenschein, Reyco Henning, Kyle Dawson, Laura Newburgh, Matthew Reece, Nicola Serra, Nural Akchurin, Sarah Eno, Paolo Rumerio, Renyuan Zhu, Jennifer Raaf, Andrea Pocar, Jonathan Asaadi, Hugh Lippincott, Graham Giovanetti, Adriana Lita, Felix Sefkow, Gretchen Campbell, Alexander Sushkov, Ronald Walsworth, Anna Grassellino, Angelo Dragone, Maurice Garcia-Sciveres, Terri Shaw, Julia Thom-Levy, Alessandro Tricoli, Petra Merkel, Wesley Ketchum, Jinlong Zhang, Paul O'Connor, Georgia Karagiorgi, Christie Ashton, Lali Chaterjee, Peter Lee, Donald Hornback, Helmut Marsiske, Michelle Shinn, Karen Byrum, Glen Crawford, Elaine Lessner, Donna Nevels, Gulshan Rai, Kathy Turner, Randall Ruchti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d08ddd948d3fd90a110367ca47401052
https://doi.org/10.2172/1659761
https://doi.org/10.2172/1659761
Autor:
Frank Krennrich, Gary Drake, Karen Byrum, J. D. Eisch, Amanda Weinstein, John S. Anderson, Hugh Dickinson
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 891:6-17
It is anticipated that forthcoming, next generation, atmospheric Cherenkov telescope arrays will include a number of medium-sized telescopes that are constructed using a dual-mirror Schwarzschild-Couder configuration. These telescopes will sample a w
Autor:
Dean Walters, Lei Xia, Ranjan Dharmapalan, Edward May, Robert Wagner, Anil U. Mane, Jingbo Wang, Huyue Zhao, Marcel Demarteau, Junqi Xie, Karen Byrum, Jeffrey W. Elam
Publikováno v:
IEEE Transactions on Nuclear Science. 64:1871-1879
Microchannel plate photodetectors, capable of picosecond time resolution and sub-mm spatial resolution, are a perfect candidate for the next generation of photodetectors for precision timing measurements. Argonne National Laboratory is producing low-
Autor:
Shaul Hanany, Georges Obied, J. Colin Hill, Thomas Cecil, Keith L. Thompson, Adam Anderson, Michael L. Brown, Doug Johnstone, Lorenzo Moncelsi, Erminia Calabrese, Howard Hui, Haruki Nishino, Sara M. Simon, James Kerby, Theodore Kisner, K. T. Story, Moritz Münchmeyer, Aritoki Suzuki, Joseph J. Mohr, Adrian T. Lee, Bradley R. Johnson, Sanah Bhimani, W. C. Jones, A. E. Lowitz, Nathan Whitehorn, Valentine Novosad, Marcelo A. Alvarez, Anze Slosar, Kam Arnold, Kevork N. Abazajian, Mustafa A. Amin, Evan Grohs, Abigail G. Vieregg, Siavash Yasini, Mathew S. Madhavacheril, Julien Carron, Ritoban Basu Thakur, Jean-Baptiste Melin, Shawn W. Henderson, Asantha Cooray, Chris Stoughton, Peter Timbie, Matteo Bonato, Ki Won Yoon, Blakesley Burkhart, Salman Habib, T. Natoli, Jacques Delabrouille, Carlo Baccigalupi, Victor Guarino, Steven W. Allen, Kathy Bailey, Aurelien A. Fraisse, Osamu Tajima, Silvia Galli, Denis Barkats, Antony Lewis, Ari Cukierman, Johannes Hubmayr, Marilena LoVerde, Erik Shirokoff, G. P. Holder, James G. Bartlett, James Yeck, Dale Li, N. W. Halverson, Graeme E. Addison, Adam Mantz, Matthieu Tristram, Laura Newburgh, Sarah Shandera, Alessandro Schillaci, Lindsey Bleem, Raphael Flauger, Marcel Schmittfull, S. Pandey, Kent D. Irwin, N. Kurita, Gregory S. Tucker, Matthew Hasselfield, Reijo Keskitalo, Levon Pogosian, Rachel S. Somerville, C. D. Sheehy, Srini Rajagopalan, Jesse Treu, Giuseppe Puglisi, Eric J. Baxter, John M Kovac, Emmanuel Schaan, Marcel Demarteau, Akito Kusaka, Suzanne T. Staggs, Kirit Karkare, Josquin Errard, Thomas Essinger-Hileman, Anne Lähteenmäki, Mattia Negrello, Toshiya Namikawa, Zhilei Xu, Mark Halpern, Simone Ferraro, Edo Berger, François R. Bouchet, Zeeshan Ahmed, Frederick Matsuda, Joseph Eimer, Alexandra S. Rahlin, W. L. Kimmy Wu, Giulio Fabbian, Chao-Lin Kuo, Christian L. Reichardt, Marius Millea, Stephen Padin, A. T. Crites, Joel Meyers, William Edwards, R. Gualtieri, Jason W. Henning, Arthur Kosowsky, Edward J. Wollack, W. L. Holzapfel, Michael D. Niemack, John E. Carlstrom, Rachel Bean, Cora Dvorkin, Ely D. Kovetz, David Alonso, Nicholas Battaglia, Sean Bryan, Gianfranco De Zotti, Anthony Challinor, Graca Rocha, Federico Nati, Jeffrey P. Filippini, Katrin Heitmann, Eric V. Linder, Antony A. Stark, Martin Nordby, Grant Teply, Benjamin Saliwanchik, Peter Adshead, P. Daniel Meerburg, Victoria Calafut, Francis-Yan Cyr-Racine, M.E. Huffer, Chris Bebek, Lloyd Knox, Masashi Hazumi, Eleonora Di Valentino, Natalie A. Roe, Nicholas Galitzki, Masaya Hasegawa, Sarah Kernovsky, Victor Buza, Darcy Barron, C. Pryke, Tijmen de Haan, Tony Mroczkowski, Vera Gluscevic, Andrea Zonca, Daniel Green, Kimberly K. Boddy, Srinivasan Raghunathan, Jeff McMahon, J. E. Ruhl, Steve Kuhlmann, Blake D. Sherwin, Joaquin Vieira, Peter S. Barry, Daisuke Nagai, Karen Byrum, Neelima Sehgal, Murdock Gilchriese, Marco Raveri, M. Tomasi, Douglas Scott, James J. Bock, Martin White, Chang Feng, Ken Ganga, Martina Gerbino, Suvodip Mukherjee, Radek Stompor, Gensheng Wang, B. Racine, Mark Reichanadter, Paul O'Connor, Alexander van Engelen, Kevin M. Huffenberger, Maria Salatino, Kathleen Harrington, Nobuhiko Katayama, Bradford Benson, Daniel Grin, Colin A. Bischoff, Charles R. Lawrence, Mark Vogelsberger, Shannon M. Duff, Scott Watson, Sebastian Bocquet, C. Umiltà, Andrei V. Frolov, C. L. Chang, Johanna Nagy, J. Richard Bond, Philip Daniel Mauskopf, B. Flaugher, Robert R. Caldwell, Mark J. Devlin, Renée Hlozek, Anirban Roy, Elena Pierpaoli, Amy N. Bender, Bruce Partridge, E. Y. Young, Matt Dobbs, Julian Borrill, Adriaan J. Duivenvoorden, Yuji Chinone, Mathieu Remazeilles, T. M. Crawford, Jon E. Gudmundsson, Hsiao-Mei Sherry Cho, Gunther Haller
We provide an overview of the science case, instrument configuration and project plan for the next-generation ground-based cosmic microwave background experiment CMB-S4, for consideration by the 2020 Decadal Survey.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4e75dab97e9c1c9aa7bed99b69ce0dca
https://doi.org/10.2172/1556957
https://doi.org/10.2172/1556957
Autor:
N. Kuklev, H. M. Cho, Faustin Carter, Junjia Ding, Gene C. Hilton, E. V. Denison, N. Huang, V. G. Yefremenko, Christian L. Reichardt, Peter S. Barry, K. L. Thompson, Alexandra S. Rahlin, Z. Pan, Gilbert Holder, A. A. Stark, N. W. Halverson, T. de Haan, R. Basu Thakur, Chihway Chang, Kent D. Irwin, N. L. Harrington, John Groh, W. L. Holzapfel, Q. Y. Tang, Jessica Avva, A. Cukierman, John E. Carlstrom, Donna Kubik, T. Natoli, A. E. Lowitz, John E. Pearson, Stephen Padin, Bradford Benson, J. E. Ruhl, Jason W. Henning, W. B. Everett, Carole Tucker, Leila R. Vale, A. Foster, Daniel Michalik, Thomas Cecil, Gensheng Wang, Jason E. Austermann, Valentine Novosad, J. A. Sobrin, K. W. Yoon, Oliver Jeong, H. Nguyen, Graeme Smecher, Lindsey Bleem, Amy N. Bender, S. S. Meyer, R. N. Gannon, Karen Byrum, L. J. Saunders, J. F. Cliche, D. Dutcher, C. M. Posada, M. R. Young, K. Vanderlinde, I. Shirley, Steve Kuhlmann, Matt Dobbs, Joaquin Vieira, Lloyd Knox, G. I. Noble, A. M. Kofman, C. L. Kuo, T. M. Crawford, M. Jonas, Aritoki Suzuki, Zeeshan Ahmed, Peter A. R. Ade, K. T. Story, Nathan Whitehorn, Trupti Khaire, Joshua Montgomery, A. J. Gilbert, Adam Anderson, J. T. Sayre, A. H. Harke-Hosemann, E. M. Leitch, M. Korman, Erik Shirokoff, Aaron Lee, Andrew Nadolski
A new receiver for the South Pole Telescope, SPT-3G, was deployed in early 2017 to map the cosmic microwave background at 95, 150, and 220 GHz with ∼ \ud ∼\ud 16,000 detectors, 10 times more than its predecessor SPTpol. The increase in detector c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c218f17bf9ef2759dbd8aca4420bbb1
https://orca.cardiff.ac.uk/id/eprint/113385/1/LTD17_proc_aanderson.pdf
https://orca.cardiff.ac.uk/id/eprint/113385/1/LTD17_proc_aanderson.pdf