Zobrazeno 1 - 10
of 12 140
pro vyhledávání: '"Lawrence, T"'
Autor:
Middleton, Alicia, Choi, Steve K., Walker, Samantha, Austermann, Jason, Burgoyne, James R., Butler, Victoria, Chapman, Scott C., Crites, Abigail T., Duell, Cody J., Freundt, Rodrigo G., Huber, Anthony I., Huber, Zachary B., Hubmayr, Johannes, Keller, Ben, Lin, Lawrence T., Niemack, Michael D., Patel, Darshan, Sinclair, Adrian K., Smith, Ema, Vaskuri, Anna, Vavagiakis, Eve M., Vissers, Michael, Wang, Yuhan, Wheeler, Jordan
Prime-Cam, one of the primary instruments for the Fred Young Submillimeter Telescope (FYST) developed by the CCAT Collaboration, will house up to seven instrument modules, with the first operating at 280 GHz. Each module will include three arrays of
Externí odkaz:
http://arxiv.org/abs/2410.21396
Autor:
Duell, Cody J., Austermann, Jason, Burgoyne, James R., Chapman, Scott C., Choi, Steve K., Crites, Abigail T., Freundt, Rodrigo G., Huber, Anthony I., Huber, Zachary B., Hubmayr, Johannes, Keller, Ben, Lin, Lawrence T., Middleton, Alicia M., Murphy, Colin C., Niemack, Michael D., Nikola, Thomas, Patel, Darshan, Sinclair, Adrian K., Smith, Ema, Stacey, Gordon J., Vaskuri, Anna, Vavagiakis, Eve M., Vissers, Michael, Walker, Samantha, Wheeler, Jordan
Publikováno v:
Proc. SPIE 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII, 131021O (16 August 2024)
Prime-Cam, a first-generation science instrument for the Atacama-based Fred Young Submillimeter Telescope, is being built by the CCAT Collaboration to observe at millimeter and submillimeter wavelengths using kinetic inductance detectors (KIDs). Prim
Externí odkaz:
http://arxiv.org/abs/2409.02271
Autor:
Huber, Zachary B., Lin, Lawrence T., Vavagiakis, Eve M., Freundt, Rodrigo G., Butler, Victoria, Chapman, Scott C., Choi, Steve K., Crites, Abigail T., Duell, Cody J., Gallardo, Patricio A., Huber, Anthony I., Keller, Ben, Middleton, Alicia, Niemack, Michael D., Nikola, Thomas, Orlowski-Scherer, John, Smith, Ema, Stacey, Gordon, Walker, Samantha, Zou, Bugao
Prime-Cam is a first-generation science instrument for the CCAT Observatory's six-meter aperture Fred Young Submillimeter Telescope (FYST). FYST's crossed-Dragone design provides high optical throughput to take advantage of its unique site at 5600 m
Externí odkaz:
http://arxiv.org/abs/2407.20873
Autor:
Gascard, Thomas J. L. J., Wang, Yi, Gudmundsson, Jon E., Vavagiakis, Eve M., Duell, Cody J., Huber, Zachary B., Lin, Lawrence T., Niemack, Michael D., Freundt, Rodrigo G.
Current and future experiments observing the cosmic microwave background require a detailed understanding of optical performance at cryogenic temperatures. Pre-deployment analysis of optics can be performed in custom-engineered cryogenic test beds, s
Externí odkaz:
http://arxiv.org/abs/2407.04613
Autor:
Duell, Cody J., Austermann, Jason, Beall, James, Burgoyne, James R., Chapman, Scott C., Choi, Steve K., Freundt, Rodrigo G., Gao, Jiansong, Groppi, Christopher, Huber, Anthony I., Huber, Zachary B., Hubmayr, Johannes, Keller, Ben, Li, Yaqiong, Lin, Lawrence T., Matthewson, Justin, Mauskopf, Philip, Middleton, Alicia, Murphy, Colin C., Niemack, Michael D., Nikola, Thomas, Sinclair, Adrian K., Smith, Ema, van Lanen, Jeff, Vaskuri, Anna, Vavagiakis, Eve M., Vissers, Michael, Walker, Samantha, Wheeler, Jordan, Zou, Bugao
The CCAT Collaboration's six-meter Fred Young Submillimeter Telescope is scheduled to begin observing in the Chilean Atacama in 2025, targeting a variety of science goals throughout cosmic history. Prime-Cam is a 1.8-meter diameter cryostat that will
Externí odkaz:
http://arxiv.org/abs/2406.06828
Autor:
Galitzki, Nicholas, Tsan, Tran, Spisak, Jake, Randall, Michael, Silva-Feaver, Max, Seibert, Joseph, Lashner, Jacob, Adachi, Shunsuke, Adkins, Sean M., Alford, Thomas, Arnold, Kam, Ashton, Peter C., Austermann, Jason E., Baccigalupi, Carlo, Bazarko, Andrew, Beall, James A., Bhimani, Sanah, Bixler, Bryce, Coppi, Gabriele, Corbett, Lance, Crowley, Kevin D., Crowley, Kevin T., Day-Weiss, Samuel, Dicker, Simon, Dow, Peter N., Duell, Cody J., Duff, Shannon M., Gerras, Remington G., Groh, John C., Gudmundsson, Jon E., Harrington, Kathleen, Hasegawa, Masaya, Healy, Erin, Henderson, Shawn W., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Keating, Brian, Keller, Ben, Kiuchi, Kenji, Kofman, Anna M., Koopman, Brian J., Kusaka, Akito, Lee, Adrian T., Lew, Richard A., Lin, Lawrence T., Link, Michael J, Lucas, Tammy J., Lungu, Marius, Mangu, Aashrita, McMahon, Jeffrey J, Miller, Amber D., Moore, Jenna E., Morshed, Magdy, Nakata, Hironobu, Nati, Federico, Newburgh, Laura B., Nguyen, David V., Niemack, Michael D., Page, Lyman A., Sakaguri, Kana, Sakurai, Yuki, Rao, Mayuri Sathyanarayana, Saunders, Lauren J., Shroyer, Jordan E., Sugiyama, Junna, Tajima, Osamu, Takeuchi, Atsuto, Bua, Refilwe Tanah, Teply, Grant, Terasaki, Tomoki, Ullom, Joel N., Van Lanen, Jeffrey L., Vavagiakis, Eve M., Vissers, Michael R, Walters, Liam, Wang, Yuhan, Xu, Zhilei, Yamada, Kyohei, Zheng, Kaiwen
The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5,200 m in the Atacama Desert in Chile. The SO SATs will cover six spectral bands betwee
Externí odkaz:
http://arxiv.org/abs/2405.05550
Autor:
Dutcher, Daniel, Duff, Shannon M., Groh, John C., Healy, Erin, Hubmayr, Johannes, Johnson, Bradley R., Jones, Dante, Keller, Ben, Lin, Lawrence T., Link, Michael J., Lucas, Tammy J., Morgan, Samuel, Seino, Yudai, Sonka, Rita F., Staggs, Suzanne T., Wang, Yuhan, Zheng, Kaiwen
The Simons Observatory (SO) is a cosmic microwave background instrumentation suite being deployed in the Atacama Desert in northern Chile. The telescopes within SO use three types of dichroic transition-edge sensor (TES) detector arrays, with the 90
Externí odkaz:
http://arxiv.org/abs/2311.05583