
CCAT-prime Collaboration: Science Goals and Forecasts with Prime …
2022年12月16日 · Prime-Cam is one of two instruments planned for FYST and will provide unprecedented spectroscopic and broadband measurement capabilities to address important astrophysical questions ranging from Big Bang cosmology through reionization and the formation of the first galaxies to star formation within our own Milky Way.
The Simons Observatory: Science Goals and Forecasts for the …
7 小时之前 · CCAT-Prime Collaboration et al. (2023) CCAT-Prime Collaboration, et al. 2023, arXiv:2107.10364, Ap. J. Supp., 264, 7, CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
Sensitivity of the Prime-Cam Instrument on the CCAT-prime …
2019年8月27日 · CCAT-prime is a new 6 m crossed Dragone telescope designed to characterize the Cosmic Microwave Background (CMB) polarization and foregrounds, measure the Sunyaev-Zel'dovich effects of galaxy clusters, map the [CII] emission intensity from the Epoch of Reionization (EoR), and monitor accretion luminosity over multi-year timescales of hundreds of...
CCAT Observatory
Rendering of CCAT site and telescope. The Fred Young Submillimeter Telescope (FYST) will be a 6-meter (20 feet) diameter telescope designed to operate at submillimeter to millimeter wavelengths and located at an exceptional site at 5600 meters (18,400 feet) on Cerro Chajnantor overlooking the ALMA array.
CCAT-Prime Science • GEco: Star formation in the Milky Way, the Magellanicclouds and other nearby galaxies through submmspectroscopy and photometry • kSZ: Probing of the nature of dark energy, gravity on large scales and neutrino mass sum through kinetic SZ effect –Polarization foregrounds: Galactic dust science & CMB polncorrections
Prime-Cam: A first-light instrument for the CCAT-prime telescope
2018年6月29日 · We present an overview of the motivation and design of Prime-Cam, a first-light instrument for CCAT-prime. Prime-Cam will house seven instrument modules in a 1.8 meter diameter cryostat, cooled by a dilution refrigerator.
CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime …
2022年8月10日 · We describe the first light 280 GHz MKID array for Prime-Cam and present its initial laboratory characterization. In particular, we show a measurement that is an important first step of an array postprocessing method for improving yield and the effect of …
CCAT-prime (CCAT-p) will be a 6-meter diameter, 10-micron surface precision telescope operating at submillimeter to millimeter wavelengths and sited at 5600 meters elevation on Cerro Chajnantor in the Atacama Desert of northern Chile. The novel optical design (see figure below) will deliver a high-
CCAT-prime: Design and status of the Prime-Cam and Mod-Cam …
CCAT-prime will address a suite of science goals, from Big Bang cosmology to star formation and galaxy evolution over cosmic time. Prime-Cam, a first-generation science instrument for FYST, will deliver over ten times greater sub-mm mapping speed than current and near-term facilities for unprecedented mm and sub-mm broadband and spectroscopic ...
CCAT-prime: design of the Mod-Cam receiver and 280 GHz MKID …
2022年8月31日 · Prime-Cam, a first-generation science instrument for FYST, will deliver over ten times greater mapping speed than current and near-term facilities for unprecedented 280–850 GHz broadband and spectroscopic measurements …