Zobrazeno 1 - 10
of 498
pro vyhledávání: '"Miller Nathan P"'
Autor:
Caputo, Regina, Kierans, Carolyn, Cannady, Nicholas, Falcone, Abe, Fukazawa, Yasushi, Jadhav, Manoj, Kerr, Matthew, Kirschner, Nicholas, Kumar, Kavic, Laviron, Adrien, Leys, Richard, Liceaga-Indart, Iker, McEnery, Julie, Metcalfe, Jessica, Metzler, Zachary, Miller, Nathan, Mitchell, John, Parker, Lucas, Peric, Ivan, Perkins, Jeremy, Phlips, Bernard, Racusin, Judith, Sasaki, Makoto, Segal, Kenneth N., Shy, Daniel, Steinhebel, Amanda L., Striebig, Nicolas, Suda, Yusuke, Tajima, Hiroyasu, Valverde, Janeth, Violette, Daniel P., Woolf, Richard, Zoglauer, Andreas
Publikováno v:
Proceedings Volume 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray; 130932L (2024)
Many questions posed in the Astro2020 Decadal survey in both the New Messengers and New Physics and the Cosmic Ecosystems science themes require a gamma-ray mission with capabilities exceeding those of existing (e.g. Fermi, Swift) and planned (e.g. C
Externí odkaz:
http://arxiv.org/abs/2412.02562
Autor:
Gunderson, Sean J., Gayley, Kenneth G., Huenemoerder, David P., Pradhan, Pragati, Miller, Nathan A.
We fit the high resolution \textit{Chandra} X-ray spectra of the O supergiant $\zeta$ Puppis using the variable boundary condition (VBC) line model to test the stability of its mass-loss rate between two epochs of observation: 2000 March and 2018 Jul
Externí odkaz:
http://arxiv.org/abs/2402.13032
Autor:
Li, Yunyang, Eimer, Joseph, Osumi, Keisuke, Appel, John, Brewer, Michael, Ali, Aamir, Bennett, Charles, Bruno, Sarah Marie, Bustos, Ricardo, Chuss, David, Cleary, Joseph, Couto, Jullianna, Dahal, Sumit, Datta, Rahul, Denis, Kevin, Dunner, Rolando, Inostroza, Francisco Raul Espinoza, Essinger-Hileman, Thomas, Fluxa, Pedro, Harrington, Kathleen, Iuliano, Jeffrey, Karakla, John, Marriage, Tobias, Miller, Nathan, Novack, Sasha, Núñez, Carolina, Petroff, Matthew, Reeves, Rodrigo, Rostem, Karwan, Shi, Rui, Valle, Deniz, Watts, Duncan, Weiland, J., Wollack, Edward, Xu, Zhilei, Zeng, Lingzhen
The Cosmology Large Angular Scale Surveyor (CLASS) is a telescope array that observes the cosmic microwave background over 75\% of the sky from the Atacama Desert, Chile, at frequency bands centered near 40, 90, 150, and 220~GHz. This paper describes
Externí odkaz:
http://arxiv.org/abs/2305.01045
Autor:
Joo, Rocío, McDonald, Gavin, Miller, Nathan, Kroodsma, David, Farthing, Courtney, Belhabib, Dyhia, Hochberg, Timothy
Many fishing vessels use forced labor, but identifying vessels that engage in this practice is challenging because few are regularly inspected. We developed a positive-unlabeled learning algorithm using vessel characteristics and movement patterns to
Externí odkaz:
http://arxiv.org/abs/2302.10987
Autor:
Shi, Rui, Marriage, Tobias A., Appel, John W., Bennett, Charles L., Chuss, David T., Cleary, Joseph, Eimer, Joseph, Dahal, Sumit, Datta, Rahul, Espinoza, Francisco, Li, Yunyang, Miller, Nathan J., Núñez, Carolina, Padilla, Ivan L., Petroff, Matthew A., Valle, Deniz A. N., Wollack, Edward J., Xu, Zhilei
Publikováno v:
The Astrophysical Journal, 945:79 (20pp), 2023 March 1
In this paper, we explore the power of the cosmic microwave background (CMB) polarization (E-mode) data to corroborate four potential anomalies in CMB temperature data: the lack of large angular-scale correlations, the alignment of the quadrupole and
Externí odkaz:
http://arxiv.org/abs/2206.05920
Autor:
Gunderson, Sean J., Gayley, Kenneth G., Pradhan, Pragati, Huenemoerder, David P., Miller, Nathan A.
Publikováno v:
MNRAS 513 2 (2022) 2663-2672
We fit a new line shape model to \textit{Chandra} X-ray spectra of the O supergiant $\zeta$ Puppis to test the robustness of mass-loss rates derived from X-ray wind line profiles against different assumed heating models. Our goal is to track the hot
Externí odkaz:
http://arxiv.org/abs/2206.05219
Autor:
Dahal, Sumit, Appel, John W., Datta, Rahul, Brewer, Michael K., Ali, Aamir, Bennett, Charles L., Bustos, Ricardo, Chan, Manwei, Chuss, David T., Cleary, Joseph, Couto, Jullianna D., Denis, Kevin L., Dünner, Rolando, Eimer, Joseph, Espinoza, Francisco, Essinger-Hileman, Thomas, Golec, Joseph E., Harrington, Kathleen, Helson, Kyle, Iuliano, Jeffrey, Karakla, John, Li, Yunyang, Marriage, Tobias A., McMahon, Jeffrey J., Miller, Nathan J., Novack, Sasha, Núñez, Carolina, Osumi, Keisuke, Padilla, Ivan L., Palma, Gonzalo A., Parker, Lucas, Petroff, Matthew A., Reeves, Rodrigo, Rhoades, Gary, Rostem, Karwan, Valle, Deniz A. N., Watts, Duncan J., Weiland, Janet L., Wollack, Edward J., Xu, Zhilei
Publikováno v:
The Astrophysical Journal, 926:33 (9pp), 2022 February 10
The Cosmology Large Angular Scale Surveyor (CLASS) observes the polarized cosmic microwave background (CMB) over the angular scales of 1$^\circ \lesssim \theta \leq$ 90$^\circ$ with the aim of characterizing primordial gravitational waves and cosmic
Externí odkaz:
http://arxiv.org/abs/2107.08022
Publikováno v:
Sci Rep 11, 23391 (2021)
In this work, we present a Quantum Hopfield Associative Memory (QHAM) and demonstrate its capabilities in simulation and hardware using IBM Quantum Experience. The QHAM is based on a quantum neuron design which can be utilized for many different mach
Externí odkaz:
http://arxiv.org/abs/2105.11590
Autor:
Harrington, Kathleen, Datta, Rahul, Osumi, Keisuke, Ali, Aamir, Appel, John W., Bennett, Charles L., Brewer, Michael K., Bustos, Ricardo, Chan, Manwei, Chuss, David T., Cleary, Joseph, Couto, Jullianna Denes, Dahal, Sumit, Dünner, Rolando, Eimer, Joseph R., Essinger-Hileman, Thomas, Hubmayr, Johannes, Inostroza, Francisco Raul Espinoza, Iuliano, Jeffrey, Karakla, John, Li, Yunyang, Marriage, Tobias A., Miller, Nathan J., Núñez, Carolina, Padilla, Ivan L., Parker, Lucas, Petroff, Matthew A., Márquez, Bastian Pradenas, Reeves, Rodrigo, Rojas, Pedro Fluxá, Rostem, Karwan, Valle, Deniz Augusto Nunes, Watts, Duncan J., Weiland, Janet L., Wollack, Edward J., Xu, Zhilei
Publikováno v:
2021 ApJ 922 212
The Cosmology Large Angular Scale Surveyor (CLASS) is a four-telescope array observing the largest angular scales ($2 \lesssim \ell \lesssim 200$) of the cosmic microwave background (CMB) polarization. These scales encode information about reionizati
Externí odkaz:
http://arxiv.org/abs/2101.00034
Autor:
Petroff, Matthew A., Appel, John W., Bennett, Charles L., Brewer, Michael K., Chan, Manwei, Chuss, David T., Cleary, Joseph, Couto, Jullianna Denes, Dahal, Sumit, Eimer, Joseph R., Essinger-Hileman, Thomas, Rojas, Pedro Fluxá, Harrington, Kathleen, Iuliano, Jeffrey, Marriage, Tobias A., Miller, Nathan J., Valle, Deniz Augusto Nunes, Watts, Duncan J., Xu, Zhilei
Publikováno v:
Proc. SPIE 11452, Software and Cyberinfrastructure for Astronomy VI, 114521O (13 December 2020)
The Cosmology Large Angular Scale Surveyor (CLASS) is an array of polarization-sensitive millimeter wave telescopes that observes ~70% of the sky at frequency bands centered near 40GHz, 90GHz, 150GHz, and 220GHz from the Atacama desert of northern Ch
Externí odkaz:
http://arxiv.org/abs/2012.08433