Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Henke, Doug"'
Autor:
Chapman, Scott C., Huber, Anthony I., Sinclair, Adrian K., Wheeler, Jordan D., Austermann, Jason E., Beall, James, Burgoyne, James, Choi, Steve K., Crites, Abigail, Duell, Cody J., Devina, Jesslyn, Gao, Jiansong, Fich, Mike, Henke, Doug, Herter, Terry, Johnstone, Doug, Knee, Lewis B. G., Niemack, Michael D., Rossi, Kayla M., Stacey, Gordon, Tsuchitori, Joel, Ullom, Joel, Van Lanen, Jeff, Vavagiakis, Eve M., Vissers, Michael, collaboration, the CCAT-prime
The Fred Young Submillimeter Telescope (FYST) at the Cerro-Chajnantor Atacama Telescope prime (CCAT- prime) Facility will host Prime-Cam as a powerful, first generation camera with imaging polarimeters working at several wavelengths and spectroscopic
Externí odkaz:
http://arxiv.org/abs/2208.10634
Autor:
Huber, Anthony I., Chapman, Scott C., Sinclair, Adrian K., Spencer, Locke D., Austermann, Jason E., Choi, Steve K., Devina, Jesslyn, Gallardo, Patricio A., Henke, Doug, Huber, Zachary B., Keller, Ben, Li, Yaqiong, Lin, Lawrence T., Niemack, Mike, Rossi, Kayla M., Vavagiakis, Eve M., Wheeler, Jordan D.
Prime-Cam is a first-generation instrument for the Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) Facility. The 850$~$GHz module for Prime-Cam will probe the highest frequency of all the instrument modules. We describe the parameter space of t
Externí odkaz:
http://arxiv.org/abs/2208.09560
Autor:
De Huang, Yau, Morata, Oscar, Koch, Patrick Michel, Kemper, Ciska, Hwang, Yuh-Jing, Chiong, Chau-Ching, Ho, Paul, Chu, You-Hua, Huang, Chi-Den, Liu, Ching-Tang, Hsieh, Fang-Chia, Tseng, Yen-Hsiang, Weng, Shou-Hsien, Ho, Chin-Ting, Chiang, Po-Han, Wu, Hsiao-Ling, Chang, Chih-Cheng, Jian, Shou-Ting, Lee, Chien-Feng, Lee, Yi-Wei, Iguchi, Satoru, Asayama, Shin'ichiro, Iono, Daisuke, Gonzalez, Alvaro, Effland, John, Saini, Kamaljeet, Pospieszalski, Marian, Henke, Doug, Yeung, Keith, Finger, Ricardo, Tapia, Valeria, Reyes, Nicolas
The Atacama Large Millimeter/submillimeter Array(ALMA) Band 1 receiver covers the 35-50 GHz frequency band. Development of prototype receivers, including the key components and subsystems has been completed and two sets of prototype receivers were fu
Externí odkaz:
http://arxiv.org/abs/1612.00893
Akademický článek
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Autor:
Salem Hesari, Sara, Henke, Doug, Knee, Lewis, Reshetov, Vlad, Veidt, Bruce, Jiang, Frank, Seyfollahi, Alireza, Wevers, Ivan, Kelly, Neal
The Radio Instrumentation Team (RIT) team at NRC Herzberg in Victoria, Canada, is developing a dual linear polarization, cryogenic radio astronomy receiver covering the frequency range of 30.5 to 50.5 GHz for the next generation Very Large Array (ngV
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c51c38b41f06cd757506c500a78d38a
Autor:
Henke, Doug, Groppi, Chris
Focal plane arrays (FPA), integrated into total power antennas, are noted as a desired technology for ALMA development during the 2030s. For full compatibility with ALMA, a dual-linear, sideband-separating (2SB) architecture is necessary. We report o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88d8b6f767a163beb33c8b55a68787e0
Publikováno v:
Sail; Jun/Jul2024, Vol. 55 Issue 5, p9-9, 1/3p, 1 Color Photograph
Autor:
Zmuidzinas, Jonas, Gao, Jian-Rong, Huang, Yau-De, Hwang, Yuh-Jing, Chiong, Chau-Ching, Yen, Hsi-Wei, Koch, Patrick Michel, Huang, Chi-Den, Liu, Bill, Chen, Cheng Lin, Tsai, Jwu Jiun, Hsiung, Wei-Ling, Chi, Li-Pin, Ho, Chin-Ting, Wang, Chao-Chin, Chien, Chen, Chu, You-Hua, Ho, Paul, Kemper, Francisca, Morata, Oscar, Gonzalez, Alvaro, Iguchi, Satoru, Uzawa, Yoshi, Iono, Daisuke, Nagai, Hiroshi, Effland, John, Saini, Kamaljeet, Pospieszalski, Marian, Henke, Doug, Yeung, Keith, Finger, Ricardo, Tapia, Valeria, Reyes, Nicolas, Siringo, Giorgio, Marconi, Gianni, Cabezas, Rodrigo
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12190 Issue: 1 p121900K-121900K-9, 1097110p
Autor:
Zmuidzinas, Jonas, Gao, Jian-Rong, Huber, Anthony I., Chapman, Scott C., Sinclair, Adrian K., Spencer, Locke D., Austermann, Jason E., Choi, Steve K., Devina, Jesslyn, Gallardo, Patricio A., Henke, Doug, Huber, Zachary B., Keller, Ben, Li, Yaqiong, Lin, Lawrence T., Niemack, Mike, Rossi, Kayla M., Vavagiakis, Eve M., Wheeler, Jordan D.
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12190 Issue: 1 p121901D-121901D-12, 12068212p
Autor:
Huang, Yau De Ted, Morata, Oscar, Koch, Patrick Michel, Kemper, Ciska, Hwang, Yuh Jing, Chiong, Chau Ching, Ho, Paul T.P., Chu, You Hua, Huang, Chi Den, Liu, Ching Tang, Hsieh, Fang Chia, Tseng, Yen Hsiang, Yang, Chia Hsiang, Tsay, Jinn Jy, Chang, Tsu, Ho, Chin Ting, Chiang, Po Han, Chang, Chih Cheng, Jian, Shou Ting, Hsu, Sung Po, Chien, Chen, Iguchi, Satoru, Asayama, Shin'ichiro, Iono, Daisuke, Gonzalez, Alvaro, Effland, John, Saini, Kamaljeet, Pospieszalski, Marian, Henke, Doug, Yeung, Keith, Finger, Ricardo, Tapia, Valeria, Reyes, Nicolas, Zmuidzinas, Jonas, Gao, Jian-Rong
Publikováno v:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
The Atacama Large Millimeter/submillimeter Array (ALMA) Band 1 receiver covers the frequency range of 35-50 GHz. An extension of up to 52 GHz is on a best-effort basis. A total of 73 units have to be built in two phases: 8 preproduction and then 65 p