Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Burgoyne, James"'
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:
Freundt, Rodrigo, Li, Yaqiong, Henke, Doug, Austermann, Jason, Burgoyne, James R., Chapman, Scott, Choi, Steve K., Duell, Cody J., Huber, Zach, Niemack, Michael, Nikola, Thomas, Lin, Lawrence, Riechers, Dominik A., Stacey, Gordon, Vaskuri, Anna K., Vavagiakis, Eve M., Wheeler, Jordan, Zou, Bugao
Publikováno v:
Proc. SPIE 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII, 131020U (16 August 2024)
The Epoch of Reionization Spectrometer (EoR-Spec) is an upcoming Line Intensity Mapping (LIM) instrument designed to study the evolution of the early universe (z = 3.5 to 8) by probing the redshifted [CII] 158 $\mu$m fine-structure line from aggregat
Externí odkaz:
http://arxiv.org/abs/2409.05979
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:
Sinclair, Adrian K., Burgoyne, James, Huber, Anthony I., Murphy, Colin, Choi, Steve K., Duell, Cody J., Huber, Zachary B., Li, Yaqiong, Chapman, Scott C., Niemack, Michael D., Nikola, Thomas, Vavagiakis, Eve M., Walker, Samantha, Wheeler, Jordan D., Austermann, Jason, Lin, Lawrence, Xie, Ruixuan, Zou, Bugao, Mauskopf, Philip D.
The Fred Young Submillimeter Telescope (FYST), on Cerro Chajnantor in the Atacama desert of Chile, will conduct wide-field and small deep-field surveys of the sky with more than 100,000 detectors on the Prime-Cam instrument. Kinetic inductance detect
Externí odkaz:
http://arxiv.org/abs/2406.14892
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:
Burgoyne, James R., Sinclair, Adrian K., Chapman, Scott C., Choi, Steve K., Duell, Cody J., Huber, Anthony I., Huber, Zachary B., Keller, Ben, Lin, Lawrence, Niemack, Michael D., Scott, Douglas, Vavagiakis, Eve M., Walker, Samantha, Xie, Matt, collaboration, the CCAT
We outline the development of the readout software for the Prime-Cam and Mod-Cam instruments on the CCAT Fred Young Submillimeter Telescope (FYST), primecam_readout. The instruments feature lumped-element kinetic inductance detector (LEKID) arrays dr
Externí odkaz:
http://arxiv.org/abs/2406.01858
Autor:
Spilker, Justin S., Phadke, Kedar A., Aravena, Manuel, Archipley, Melanie, Bayliss, Matthew B., Birkin, Jack E., Bethermin, Matthieu, Burgoyne, James, Cathey, Jared, Chapman, Scott C., Dahle, Hakon, Gonzalez, Anthony H., Gururajan, Gayathri, Hayward, Christopher C., Hezaveh, Yashar D., Hill, Ryley, Hutchison, Taylor A., Kim, Keunho J., Kim, Seonwoo, Law, David, Legin, Ronan, Malkan, Matthew A., Marrone, Daniel P., Murphy, Eric J., Narayanan, Desika, Navarre, Alex, Olivier, Grace M., Rich, Jeffrey A., Rigby, Jane R., Reuter, Cassie, Rhoads, James E., Sharon, Keren, Smith, J. D. T., Solimano, Manuel, Sulzenauer, Nikolaus, Vieira, Joaquin D., Weiss, Axel, Whitaker, Katherine E.
Dust grains absorb half of the radiation emitted by stars throughout the history of the universe, re-emitting this energy at infrared wavelengths. Polycyclic aromatic hydrocarbons (PAHs) are large organic molecules that trace millimeter-size dust gra
Externí odkaz:
http://arxiv.org/abs/2306.03152
Autor:
Sinclair, Adrian K., Burgoyne, James R., Li, Yaqiong, Duell, Cody, Chapman, Scott C., Huber, Anthony I., Xie, Ruixuan
We demonstrate a prototype kinetic inductance detector (KID) readout system that uses less than 10 mW per pixel. The CCAT-prime RFSoC based readout is capable of reading four independent detector networks of up to 1000 KIDs each. The power dissipatio
Externí odkaz:
http://arxiv.org/abs/2305.00928
Autor:
Chapman, Scott C., Hill, Ryley, Aravena, Manuel, Archipley, Melanie, Babul, Arif, Burgoyne, James, Canning, Rebecca E. A., De Breuck, Carlos, Gonzalez, Anthony H., Hayward, Christopher C., Kim, Seon Woo, Malkan, Matt, Marrone, Dan P., McIntyre, Vincent, Murphy, Eric, Pass, Emily, Perry, Ryan W., Phadke, Kedar A., Rennehan, Douglas, Reuter, Cassie, Rotermund, Kaja M., Scott, Douglas, Seymour, Nick, Solimano, Manuel, Spilker, Justin, Stark, Anthony A., Sulzenauer, Nikolaus, Tothill, Nick, Vieira, Joaquin D., Vizgan, David, Wang, George, Weiss, Axel
We have observed the z=4.3 protocluster SPT2349-56 with ATCA with the aim of detecting radio-loud active galactic nuclei (AGN) amongst the ~30 submillimeter galaxies identified in the structure. We detect the central complex of SMGs at 2.2\,GHz with
Externí odkaz:
http://arxiv.org/abs/2301.01375
Autor:
Apostolovski, Yordanka, Aravena, Manuel, Anguita, Timo, Bethermin, Matthieu, Burgoyne, James, Chapman, Scott, De Breuck, Carlos, Gonzalez, Anthony, Gronke, Max, Guaita, Lucia, Hezaveh, Yashar, Hill, Ryley, Jarugula, Sreevani, Johnston, Evelyn, Malkan, Matt, Narayanan, Desika, Reuter, Cassie, Solimano, Manuel, Spilker, Justin, Sulzenauer, Nikolaus, Vieira, Joaquin, Vizgan, David, Weiß, Axel
Context. Deep spectroscopic surveys with the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed that some of the brightest infrared sources in the sky correspond to concentrations of dusty star-forming galaxies (DSFG) at high redshift.
Externí odkaz:
http://arxiv.org/abs/2301.01328