no code implementations • 3 Feb 2021 • Kathleen Harrington, Carlos Sierra, Grace Chesmore, Shreya Sutariya, Aamir M. Ali, Steve K. Choi, Nicholas F. Cothard, Simon Dicker, Nicholas Galitzki, Shuay-Pwu Patty Ho, Anna M. Kofman, Brian J. Koopman, Jack Lashner, Jeff McMahon, Michael D. Niemack, John Orlowski-Scherer, Joseph Seibert, Max Silva-Feaver, Eve M. Vavagiakis, Zhilei Xu, Ningfeng Zhu
The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes and one large-aperture telescope, which will observe from the Atacama Desert in Chile.
Instrumentation and Methods for Astrophysics
no code implementations • 25 Jan 2021 • Joseph E. Golec, Jeffrey J. McMahon, Aamir M. Ali, Simon Dicker, Nicholas Galitzki, Kathleen Harrington, Benjamin Westbrook, Edward J. Wollack, Zhilei Xu, Ningfeng Zhu
The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes and one large-aperture telescope, which will observe from the Atacama Desert in Chile.
Instrumentation and Methods for Astrophysics
no code implementations • 18 Dec 2020 • Brian J. Koopman, Jack Lashner, Lauren J. Saunders, Matthew Hasselfield, Tanay Bhandarkar, Sanah Bhimani, Steve K. Choi, Cody J. Duell, Nicholas Galitzki, Kathleen Harrington, Adam D. Hincks, Shuay-Pwu Patty Ho, Laura Newburgh, Christian L. Reichardt, Joseph Seibert, Jacob Spisak, Benjamin Westbrook, Zhilei Xu, Ningfeng Zhu
To meet this need, we have designed and built an open-sourced platform for distributed system management, called the Observatory Control System (ocs).
Instrumentation and Methods for Astrophysics
no code implementations • 15 Dec 2020 • Matthew A. Petroff, John W. Appel, Charles L. Bennett, Michael K. Brewer, Manwei Chan, David T. Chuss, Joseph Cleary, Jullianna Denes Couto, Sumit Dahal, Joseph R. Eimer, Thomas Essinger-Hileman, Pedro Fluxá Rojas, Kathleen Harrington, Jeffrey Iuliano, Tobias A. Marriage, Nathan J. Miller, Deniz Augusto Nunes Valle, Duncan J. Watts, Zhilei Xu
The Cosmology Large Angular Scale Surveyor (CLASS) is an array of polarization-sensitive millimeter wave telescopes that observes ~70% of the sky at frequency bands centered near 40GHz, 90GHz, 150GHz, and 220GHz from the Atacama desert of northern Chile.
Instrumentation and Methods for Astrophysics
1 code implementation • 4 Nov 2019 • Matthew A. Petroff, Joseph R. Eimer, Kathleen Harrington, Aamir Ali, John W. Appel, Charles L. Bennett, Michael K. Brewer, Ricardo Bustos, Manwei Chan, David T. Chuss, Joseph Cleary, Jullianna Denes Couto, Sumit Dahal, Rolando Dünner, Thomas Essinger-Hileman, Pedro Fluxá Rojas, Dominik Gothe, Jeffrey Iuliano, Tobias A. Marriage, Nathan J. Miller, Carolina Núñez, Ivan L. Padilla, Lucas Parker, Rodrigo Reeves, Karwan Rostem, Deniz Augusto Nunes Valle, Duncan J. Watts, Janet L. Weiland, Edward J. Wollack, Zhilei Xu
Then, using two years of observations at 32. 3 GHz to 43. 7 GHz from the CLASS Q-band telescope, we present a detection of this signal and compare the observed signal to that predicted by the model.
Instrumentation and Methods for Astrophysics
