Zobrazeno 1 - 10
of 300
pro vyhledávání: '"Pitts Mark"'
Autor:
Wuu, Cheng-hsin, Zheng, Ningyuan, Ardisson, Scott, Bali, Rohan, Belko, Danielle, Brockmeyer, Eric, Evans, Lucas, Godisart, Timothy, Ha, Hyowon, Huang, Xuhua, Hypes, Alexander, Koska, Taylor, Krenn, Steven, Lombardi, Stephen, Luo, Xiaomin, McPhail, Kevyn, Millerschoen, Laura, Perdoch, Michal, Pitts, Mark, Richard, Alexander, Saragih, Jason, Saragih, Junko, Shiratori, Takaaki, Simon, Tomas, Stewart, Matt, Trimble, Autumn, Weng, Xinshuo, Whitewolf, David, Wu, Chenglei, Yu, Shoou-I, Sheikh, Yaser
Photorealistic avatars of human faces have come a long way in recent years, yet research along this area is limited by a lack of publicly available, high-quality datasets covering both, dense multi-view camera captures, and rich facial expressions of
Externí odkaz:
http://arxiv.org/abs/2207.11243
Autor:
Odell, George H.
Publikováno v:
Lithic Technology, 1998 Oct 01. 23(2), 147-148.
Externí odkaz:
https://www.jstor.org/stable/23273089
Autor:
Harrington, David, Ammons, Mark, Hunter, Lisa, Max, Claire, Hoffmann, Mark, Pitts, Mark, Armstrong, J. D.
Adaptive optics workbenches are fully functional optical systems that can be used to illustrate and teach a variety of concepts and cognitive processes. Four systems have been funded, designed and constructed by various institutions and people as par
Externí odkaz:
http://arxiv.org/abs/1009.4463
Autor:
Montgomery, Ryan, Harrington, David, Sonnett, Sarah, Pitts, Mark, Mostafanezhad, Isar, Foley, Mike, Laag, Eddie, Hunter, Lisa
We describe the design and elements of implementation of the Akamai Maui Short Course (AMSC). The AMSC contains four full inquiry activities each of which builds on those previous: Camera Obscura and Sun Shadows, Lenses and Refraction, Color and Ligh
Externí odkaz:
http://arxiv.org/abs/1009.4458
Autor:
Looper, Dagny L., Bochanski, John J., Burgasser, Adam J., Mohanty, Subhanjoy, Mamajek, Eric E., Faherty, Jacqueline K., West, Andrew A., Pitts, Mark A.
We report the discovery of TWA 30B, a wide (~3400 AU), co-moving M dwarf companion to the nearby (~42 pc) young star TWA 30. Companionship is confirmed from their statistically consistent proper motions and radial velocities, as well as a chance alig
Externí odkaz:
http://arxiv.org/abs/1008.4340
Autor:
Looper, Dagny L., Mohanty, Subhanjoy, Bochanski, John J., Burgasser, Adam J., Mamajek, Eric E., Herczeg, Gregory J., West, Andrew A., Faherty, Jacqueline K., Rayner, John, Pitts, Mark A., Kirkpatrick, J. Davy
TWA 30 is a remarkable young (7+/-3 Myr), low-mass (0.12+/-0.04 Msun), late-type star (M5+/-1) residing 42+/-2 pc away from the sun in the TW Hydrae Association. It shows strong outflow spectral signatures such as [S II], [O I], [O II], [O III], and
Externí odkaz:
http://arxiv.org/abs/1003.3447
Autor:
LaRocca-Pitts, Mark1 marklp@armc.org
Publikováno v:
Chaplaincy Today. 2009, Vol. 25 Issue 2, p45-45. 1p.
Publikováno v:
Billboard. 9/29/2018, Vol. 130 Issue 22, p68-69. 2p. 1 Color Photograph.
Akademický článek
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Autor:
LYLE, ASHLEY
Publikováno v:
Billboard. 10/13/2018, Vol. 130 Issue 23, p80-80. 1p. 2 Color Photographs.