The Design of the CCAT-prime Epoch of Reionization Spectrometer Instrument

@article{Cothard2020TheDO,
  title={The Design of the CCAT-prime Epoch of Reionization Spectrometer Instrument},
  author={Nicholas F. Cothard and Steve K. Choi and Cody J. Duell and Terry L. Herter and J. Hubmayr and Jeff J. McMahon and Michael D. Niemack and Thomas Nikola and Carlos E. Sierra and Gordon J. Stacey and Eve M. Vavagiakis and Edward J. Wollack and Bugao Zou},
  journal={Journal of Low Temperature Physics},
  year={2020},
  volume={199},
  pages={898-907}
}
The epoch of reionization spectrometer (EoR-Spec) is an instrument module for the Prime-Cam receiver of the 6-m aperture CCAT-prime Telescope at 5600 m in Chile. EoR-Spec will perform 158 $$\upmu $$ μ m [CII] line intensity mapping of star-forming regions at redshifts between 3.5 and 8 (420–210 GHz), tracing the evolution of structure during early galaxy formation. At lower redshifts, EoR-Spec will observe galaxies near the period of peak star formation—when most stars in today’s universe were… 

CCAT-prime: the optical design for the Epoch of reionization spectrometer

The Epoch of Reionization Spectrometer (EoR-Spec) will be an instrument module for the Prime-Cam receiver on the CCAT-prime Collaboration’s Fred Young Submillimeter Telescope (FYST), a 6-m primary

CCAT-prime: the design of the epoch of reionization spectrometer detector arrays

The epoch of reionization spectrometer (EoR-Spec) is an instrument module that will be deployed in the Prime-Cam receiver on the Fred Young Submillimeter Telescope (FYST), which is a 6m off-axis

CCAT-prime: the epoch reionization spectrometer for primce-cam on FYST

The Fred Young Submillimeter Telescope (FYST), which is the telescope of the CCAT-prime project, will be located at 5600 m near the summit of Cerro Chajnantor in northern Chile, and will host the

Sensitivity of the Prime-Cam Instrument on the CCAT-Prime Telescope

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

CCAT-prime/FYST: a status report on the ultra-widefield submillimeter observatory on Cerro Chajnantor

We report on the CCAT-prime Project, including the science program, the Fred Young Submillimeter Telescope (FYST), its instrumentation, and the schedule. FYST is a 6-m telescope sited at 5600 m

CCAT-prime: the design and characterization of the silicon mirrors for the Fabry-Perot interferometer in the Epoch of reionization spectrometer

The Epoch of Reionization Spectrometer (EoR-Spec) is one of the instrument modules to be installed in the Prime-Cam receiver of the Fred Young Submillimeter Telescope (FYST). This six-meter aperture

The ALMA Spectroscopic Survey in the HUDF: A Search for [C ii] Emitters at 6 ≤ z ≤ 8

The Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Band 6 scan (212–272 GHz) covers potential [C ii] emission in galaxies at 6 ≤ z ≤

Implications of the z > 5 Lyman-α forest for the 21-cm power spectrum from the epoch of reionization

Our understanding of the intergalactic medium at redshifts z = 5–6 has improved considerably in the last few years due to the discovery of quasars with z > 6 that enable Lyman-α forest studies at

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The South Pole Telescope Summertime Line Intensity Mapper (SPT-SLIM) is a pathfinder experiment that will demonstrate the use of on-chip filter-bank spectrometers for mm-wave line intensity mapping

CCAT-prime: Designs and status of the first light 280 GHz MKID array and mod-cam receiver

  • C. DuellE. Vavagiakis B. Zou
  • Physics
    Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
  • 2020
The CCAT-prime project's first light array will be deployed in Mod-Cam, a single-module testbed and first light cryostat, on the Fred Young Submillimeter Telescope (FYST) in Chile's high Atacama

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