Zobrazeno 1 - 10
of 1 426
pro vyhledávání: '"Boggs, A E"'
Autor:
Aramaki, T., Boezio, M., Boggs, S. E., Bonvicini, V., Bridges, G., Campana, D., Craig, W. W., von Doetinchem, P., Everson, E., Fabris, L., Feldman, S., Fuke, H., Gahbauer, F., Gerrity, C., Ghislotti, L., Hailey, C. J., Hayashi, T., Kawachi, A., Kozai, M., Lazzaroni, P., Law, M., Lenni, A., Lowell, A., Manghisoni, M., Marcelli, N., Mizukoshi, K., Mocchiutti, E., Mochizuki, B., Mognet, S. A. I., Munakata, K., Munini, R., Okazaki, S., Olson, J., Ong, R. A., Osteria, G., Perez, K., Perfetto, F., Quinn, S., Re, V., Riceputi, E., Roach, B., Rogers, F., Ryan, J. L., Saffold, N., Scotti, V., Shimizu, Y., Shutt, K., Sparvoli, R., Stoessl, A., Tiberio, A., Vannuccini, E., Xiao, M., Yamatani, M., Yee, K., Yoshida, T., Zampa, G., Zeng, J., Zweerink, J.
Compilation of papers presented by the GAPS Collaboration at the 38th International Cosmic Ray Conference (ICRC), held July 26 through August 3, 2023 in Nagoya, Japan.
Externí odkaz:
http://arxiv.org/abs/2310.10181
Autor:
Boggs, Steven E., Pike, Sean N.
Charge trapping in germanium detectors will inevitably impact their excellent spectral performance. Disordered regions in the germanium crystal structure, either created in the material during processing or induced by radiation exposure, will affect
Externí odkaz:
http://arxiv.org/abs/2310.01312
Autor:
Tomsick, John A., Boggs, Steven E., Zoglauer, Andreas, Hartmann, Dieter, Ajello, Marco, Burns, Eric, Fryer, Chris, Karwin, Chris, Kierans, Carolyn, Lowell, Alexander, Malzac, Julien, Roberts, Jarred, Saint-Hilaire, Pascal, Shih, Albert, Siegert, Thomas, Sleator, Clio, Takahashi, Tadayuki, Tavecchio, Fabrizio, Wulf, Eric, Beechert, Jacqueline, Gulick, Hannah, Joens, Alyson, Lazar, Hadar, Neights, Eliza, Oliveros, Juan Carlos Martinez, Matsumoto, Shigeki, Melia, Tom, Yoneda, Hiroki, Amman, Mark, Bal, Dhruv, von Ballmoos, Peter, Bates, Hugh, Böttcher, Markus, Bulgarelli, Andrea, Cavazzuti, Elisabetta, Chang, Hsiang-Kuang, Chen, Claire, Chu, Che-Yen, Ciabattoni, Alex, Costamante, Luigi, Dreyer, Lente, Fioretti, Valentina, Fenu, Francesco, Gallego, Savitri, Ghirlanda, Giancarlo, Grove, Eric, Huang, Chien-You, Jean, Pierre, Khatiya, Nikita, Knödlseder, Jürgen, Krause, Martin, Leising, Mark, Lewis, Tiffany R., Lommler, Jan Peter, Marcotulli, Lea, Martinez-Castellanos, Israel, Mittal, Saurabh, Negro, Michela, Nussirat, Samer Al, Nakazawa, Kazuhiro, Oberlack, Uwe, Palmore, David, Panebianco, Gabriele, Parmiggiani, Nicolo, Parsotan, Tyler, Pike, Sean N., Rogers, Field, Schutte, Hester, Sheng, Yong, Smale, Alan P., Smith, Jacob, Trigg, Aaron, Venters, Tonia, Watanabe, Yu, Zhang, Haocheng
Publikováno v:
PoS(ICRC2023)745
The Compton Spectrometer and Imager (COSI) is a NASA Small Explorer (SMEX) satellite mission in development with a planned launch in 2027. COSI is a wide-field gamma-ray telescope designed to survey the entire sky at 0.2-5 MeV. It provides imaging, s
Externí odkaz:
http://arxiv.org/abs/2308.12362
Autor:
Martinez-Castellanos, Israel, Gallego, Savitri, Huang, Chien-You, Karwin, Chris, Kierans, Carolyn, Lommler, Jan Peter, Mittal, Saurabh, Negro, Michela, Neights, Eliza, Pike, Sean N., Sheng, Yong, Siegert, Thomas, Yoneda, Hiroki, Zoglauer, Andreas, Tomsick, John A., Boggs, Steven E., Hartmann, Dieter, Ajello, Marco, Burns, Eric, Fryer, Chris, Lowell, Alexander, Malzac, Julien, Roberts, Jarred, Saint-Hilaire, Pascal, Shih, Albert, Sleator, Clio, Takahashi, Tadayuki, Tavecchio, Fabrizio, Wulf, Eric, Beechert, Jacqueline, Gulick, Hannah, Joens, Alyson, Lazar, Hadar, Oliveros, Juan Carlos Martinez, Matsumoto, Shigeki, Melia, Tom, Amman, Mark, Bal, Dhruv, von Ballmoos, Peter, Bates, Hugh, Böttcher, Markus, Bulgarelli, Andrea, Cavazzuti, Elisabetta, Chang, Hsiang-Kuang, Chen, Claire, Chu, Che-Yen, Ciabattoni, Alex, Costamante, Luigi, Dreyer, Lente, Fioretti, Valentina, Fenu, Francesco, Ghirlanda, Giancarlo, Grove, Eric, Jean, Pierre, Khatiya, Nikita, Knödlseder, Jürgen, Krause, Martin, Leising, Mark, Lewis, Tiffany R., Marcotulli, Lea, Nussirat, Samer Al, Nakazawa, Kazuhiro, Oberlack, Uwe, Palmore, David, Panebianco, Gabriele, Parmiggiani, Nicolo, Parsotan, Tyler, Rogers, Field, Schutte, Hester, Smale, Alan P., Smith, Jacob, Trigg, Aaron, Venters, Tonia, Watanabe, Yu, Zhang, Haocheng
Publikováno v:
Martinez, Israel. The cosipy library: COSI's high-level analysis software. PoS ICRC2023 (2023) 444-858
The Compton Spectrometer and Imager (COSI) is a selected Small Explorer (SMEX) mission launching in 2027. It consists of a large field-of-view Compton telescope that will probe with increased sensitivity the under-explored MeV gamma-ray sky (0.2-5 Me
Externí odkaz:
http://arxiv.org/abs/2308.11436
Autor:
Pike, Sean N., Boggs, Steven E., Beechert, Jacqueline, Roberts, Jarred, Shih, Albert Y., Tomsick, John A., Zoglauer, Andreas
We present measurements of electron and hole trapping in three COSI germanium cross-strip detectors. By characterizing the relative charge collection efficiency (CCE) as a function of interaction depth, we show that intrinsic trapping of both electro
Externí odkaz:
http://arxiv.org/abs/2306.08778
Autor:
Boggs, Steven E., Pike, Sean N.
In an ideal germanium detector, fully-absorbed monoenergetic gamma-rays will appear in the measured spectrum as a narrow peak, broadened into a Gaussian of width determined only by the statistical properties of charge cloud generation and the electro
Externí odkaz:
http://arxiv.org/abs/2305.01544
Autor:
Boggs, Steven E.
When a $\gamma$-ray interacts in a semiconductor detector, the resulting electron-hole charge clouds drift towards their respective electrodes for signal collection. These charge clouds will expand over time due to both thermal diffusion and mutual e
Externí odkaz:
http://arxiv.org/abs/2304.09713
Autor:
Beechert, Jacqueline, Lazar, Hadar, Boggs, Steven E., Brandt, Terri J., Chang, Yi-Chi, Chu, Che-Yen, Gulick, Hannah, Kierans, Carolyn, Lowell, Alexander, Pellegrini, Nicholas, Roberts, Jarred M., Siegert, Thomas, Sleator, Clio, Tomsick, John A., Zoglauer, Andreas
The Compton Spectrometer and Imager (COSI) is a balloon-borne soft $\gamma$-ray telescope (0.2-5 MeV) designed to study astrophysical sources. COSI employs a compact Compton telescope design and is comprised of twelve high-purity germanium semiconduc
Externí odkaz:
http://arxiv.org/abs/2203.00695
Autor:
Beechert, Jacqueline, Siegert, Thomas, Tomsick, John A., Zoglauer, Andreas, Boggs, Steven E., Brandt, Terri J., Gulick, Hannah, Jean, Pierre, Kierans, Carolyn, Lazar, Hadar, Lowell, Alexander, Roberts, Jarred M., Sleator, Clio, von Ballmoos, Peter
The Compton Spectrometer and Imager (COSI) is a balloon-borne compact Compton telescope designed to survey the 0.2-5 MeV sky. COSI's energy resolution of $\sim$0.2% at 1.8 MeV, single-photon reconstruction, and wide field of view make it capable of s
Externí odkaz:
http://arxiv.org/abs/2202.11713
Autor:
Tomsick, John A., Boggs, Steven E., Zoglauer, Andreas, Wulf, Eric, Mitchell, Lee, Phlips, Bernard, Sleator, Clio, Brandt, Terri, Shih, Albert, Roberts, Jarred, Jean, Pierre, von Ballmoos, Peter, Oliveros, Juan Martinez, Smale, Alan, Kierans, Carolyn, Hartmann, Dieter, Leising, Mark, Ajello, Marco, Burns, Eric, Fryer, Chris, Saint-Hilaire, Pascal, Malzac, Julien, Tavecchio, Fabrizio, Fioretti, Valentina, Bulgarelli, Andrea, Ghirlanda, Giancarlo, Chang, Hsiang-Kuang, Takahashi, Tadayuki, Nakazawa, Kazuhiro, Matsumoto, Shigeki, Melia, Tom, Siegert, Thomas, Lowell, Alexander, Lazar, Hadar, Beechert, Jacqueline, Gulick, Hannah
The Compton Spectrometer and Imager (COSI) is a 0.2-5 MeV Compton telescope capable of imaging, spectroscopy, and polarimetry of astrophysical sources. Such capabilities are made possible by COSI's germanium cross-strip detectors, which provide high
Externí odkaz:
http://arxiv.org/abs/2109.10403