Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Lucas, Tammy J."'
Autor:
Satterthwaite, Thomas P., Ahmed, Zeeshan, Bae, Kyuyoung, Devlin, Mark, Dicker, Simon, Duff, Shannon M., Dutcher, Daniel, Haridas, Saianeesh K., Henderson, Shawn W., Hubmayr, Johannes, Johnson, Bradley R., Kofman, Anna, Lashner, Jack, Link, Michael J., Lucas, Tammy J., Manduca, Alex, Niemack, Michael D., Orlowski-Scherer, John, Pinsonneault-Marotte, Tristan, Silva-Feaver, Max, Staggs, Suzanne, Vavagiakis, Eve M., Wang, Yuhan, Zheng, Kaiwen
The Simons Observatory is a new ground-based cosmic microwave background experiment, which is currently being commissioned in Chile's Atacama Desert. During its survey, the observatory's small aperture telescopes will map 10% of the sky in bands cent
Externí odkaz:
http://arxiv.org/abs/2406.01844
Autor:
Sierra, Carlos E., Harrington, Kathleen, Sutariya, Shreya, Alford, Thomas, Kofman, Anna M., Chesmore, Grace E., Austermann, Jason E., Bazarko, Andrew, Beall, James A., Bhandarkar, Tanay, Devlin, Mark J., Dicker, Simon R., Dow, Peter N., Duff, Shannon M., Dutcher, Daniel, Galitzki, Nicholas, Golec, Joseph E., Groh, John C., Gudmundsson, Jon E., Haridas, Saianeesh K., Healy, Erin, Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Lessler, Claire S., Lew, Richard A., Link, Michael J., Lucas, Tammy J., McMahon, Jeffrey J., Moore, Jenna E., Nati, Federico, Niemack, Michael D., Schmitt, Benjamin L., Silva-Feaver, Max, Singh, Robinjeet, Sonka, Rita F., Thomas, Alex, Thornton, Robert J., Tsan, Tran, Ullom, Joel N., Van Lanen, Jeffrey L., Vavagiakis, Eve M., Vissers, Michael R., Wang, Yuhan, Zheng, Kaiwen
The Simons Observatory will map the temperature and polarization over half of the sky, at millimeter wavelengths in six spectral bands from the Atacama Desert in Chile. These data will provide new insights into the genesis, content, and history of ou
Externí odkaz:
http://arxiv.org/abs/2405.06868
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:
Duff, Shannon M., Austermann, Jason, Beall, James A., Daniel, David P., Hubmayr, Johannes, Jaehnig, Greg C., Johnson, Bradley R., Jones, Dante, Link, Michael J., Lucas, Tammy J., Sonka, Rita F., Staggs, Suzanne T., Ullom, Joel, Wang, Yuhan
The Simons Observatory (SO) is a cosmic microwave background instrumentation suite in the Atacama Desert of Chile. More than 65,000 polarization-sensitive transition-edge sensor (TES) bolometers will be fielded in the frequency range spanning 27 to 2
Externí odkaz:
http://arxiv.org/abs/2403.18225
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
Autor:
Healy, Erin, Ali, Aamir M., Arnold, Kam, Austermann, Jason E., Beall, James A., Bruno, Sarah Marie, Choi, Steve K., Connors, Jake, Cothar, Nicholas F., Dober, Bradley, Duff, Shannon M., Galitzki, Nicholas, Hilton, Gene, Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Johnson, Bradley R., Li, Yaqiong, Link, Michael J., Lucas, Tammy J., McCarrick, Heather, Niemack, Michael D., Silva-Feaver, Maximiliano, Sonka, Rita F., Staggs, Suzanne, Vavagiakis, Eve M., Vissers, Michael R., Wang, Yuhan, Westbrook, Benjamin, Wollack, Edward J., Xu, Zhilei, Zheng, Kaiwen
Publikováno v:
Proc. SPIE 11453, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, 1145317 (2020)
The Simons Observatory (SO) is a suite of instruments sensitive to temperature and polarization of the cosmic microwave background (CMB) to be located at Cerro Toco in the Atacama Desert in Chile. Five telescopes, one large aperture telescope and fou
Externí odkaz:
http://arxiv.org/abs/2204.05869
Autor:
McCarrick, Heather, Healy, Erin, Ahmed, Zeeshan, Arnold, Kam, Atkins, Zachary, Austermann, Jason E., Bhandarkar, Tanay, Beall, Jim A., Bruno, Sarah Marie, Choi, Steve K., Connors, Jake, Cothard, Nicholas F., Crowley, Kevin D., Dicker, Simon, Dober, Bradley, Duell, Cody J., Duff, Shannon M., Dutcher, Daniel, Frisch, Josef C., Galitzki, Nicholas, Gralla, Megan B., Gudmundsson, Jon E., Henderson, Shawn W., Hilton, Gene C., Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Kofman, Anna M., Kusaka, Akito, Lashner, Jack, Lee, Adrian T., Li, Yaqiong, Link, Michael J., Lucas, Tammy J., Lungu, Marius, Mates, J. A. B., McMahon, Jeffrey J., Niemack, Michael D., Orlowski-Scherer, John, Seibert, Joseph, Silva-Feaver, Maximiliano, Simon, Sara M., Staggs, Suzanne, Suzuki, Aritoki, Terasaki, Tomoki, Ullom, Joel N., Vavagiakis, Eve M., Vale, Leila R., Van Lanen, Jeff, Vissers, Michael R., Wang, Yuhan, Wollack, Edward J., Xu, Zhilei, Young, Edward, Yu, Cyndia, Zheng, Kaiwen, Zhu, Ningfeng
Publikováno v:
2021 ApJ 922 38
Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducting transition-edge sensor (TES) bolometers tiled densely into ever lar
Externí odkaz:
http://arxiv.org/abs/2106.14797
Autor:
Xu, Zhilei, Adachi, Shunsuke, Ade, Peter, Beall, J. A., Bhandarkar, Tanay, Bond, J. Richard, Chesmore, Grace E., Chinone, Yuji, Choi, Steve K., Connors, Jake A., Coppi, Gabriele, Cothard, Nicholas F., Crowley, Kevin D., Devlin, Mark, Dicker, Simon, Dober, Bradley, Duff, Shannon M., Galitzki, Nicholas, Gallardo, Patricio A., Golec, Joseph E., Gudmundsson, Jon E., Haridas, Saianeesh K., Harrington, Kathleen, Hervias-Caimapo, Carlos, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Kaneko, Daisuke, Kofman, Anna M., Koopman, Brian J., Lashner, Jack, Limon, Michele, Link, Michael J., Lucas, Tammy J., Matsuda, Frederick, McCarrick, Heather, Nati, Federico, Niemack, Michael D., Orlowski-Scherer, John, Piccirillo, Lucio, Sarmiento, Karen Perez, Schaan, Emmanuel, Silva-Feaver, Maximiliano, Sonka, Rita, Sutariya, Shreya, Tajima, Osamu, Teply, Grant P., Terasaki, Tomoki, Thornton, Robert, Tucker, Carole, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Walker, Samantha, Whipps, Zachary, Wollack, Edward J., Zannoni, Mario, Zhu, Ningfeng, Zonca, Andrea
Publikováno v:
Research Notes AAS, 5, 100 (2021)
The Simons Observatory (SO) is a Cosmic Microwave Background (CMB) experiment to observe the microwave sky in six frequency bands from 30GHz to 290GHz. The Observatory -- at $\sim$5200m altitude -- comprises three Small Aperture Telescopes (SATs) and
Externí odkaz:
http://arxiv.org/abs/2104.09511
Autor:
Zhu, Ningfeng, Bhandarkar, Tanay, Coppi, Gabriele, Kofman, Anna M., Orlowski-Scherer, John L., Xu, Zhilei, Adachi, Shunsuke, Ade, Peter, Aiola, Simone, Austermann, Jason, Bazarko, Andrew O., Beall, James A., Bhimani, Sanah, Bond, J. Richard, Chesmore, Grace E., Choi, Steve K., Connors, Jake, Cothard, Nicholas F., Devlin, Mark, Dicker, Simon, Dober, Bradley, Duell, Cody J., Duff, Shannon M., Dünner, Rolando, Fabbian, Giulio, Galitzki, Nicholas, Gallardo, Patricio A., Golec, Joseph E., Haridas, Saianeesh K., Harrington, Kathleen, Healy, Erin, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Keatin, Brian, Kiuchi, Kenji, Koopman, Brian J., Lashner, Jack, Lee, Adrian T., Li, Yaqiong, Limon, Michele, Link, Michael, Lucas, Tammy J, McCarrick, Heather, Moore, Jenna, Nati, Federico, Newburgh, Laura B., Niemack, Michael D., Pierpaoli, Elena, Randall, Michael J., Sarmiento, Karen Perez, Saunders, Lauren J., Seibert, Joseph, Sierra, Carlos, Sonka, Rita, Spisak, Jacob, Sutariya, Shreya, Tajima, Osamu, Teply, Grant P., Thornton, Robert J., Tsan, Tran, Tucker, Carole, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Walker, Samantha, Westbrook, Benjamin, Wollack, Edward J., Zannoni, Mario
The Simons Observatory (SO) Large Aperture Telescope Receiver (LATR) will be coupled to the Large Aperture Telescope located at an elevation of 5,200 m on Cerro Toco in Chile. The resulting instrument will produce arcminute-resolution millimeter-wave
Externí odkaz:
http://arxiv.org/abs/2103.02747
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