Christopher Groppi
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View article: CCAT: Readout of over 10,000 280 GHz KIDs in Mod-Cam using RFSoC Electronics
CCAT: Readout of over 10,000 280 GHz KIDs in Mod-Cam using RFSoC Electronics Open
Over the past decade, kinetic inductance detectors (KIDs) have emerged as a viable superconducting technology for astrophysics at millimeter and submillimeter wavelengths. KIDs spanning 210 - 850 GHz across seven instrument modules will be…
View article: CCAT: Mod-Cam Readout Overview and Flexible Stripline Performance
CCAT: Mod-Cam Readout Overview and Flexible Stripline Performance Open
The CCAT Observatory's first-light and commissioning instrument, Mod-Cam, is nearing readiness for deployment to the Fred Young Submillimeter Telescope (FYST) in the Atacama Desert in northern Chile. In-lab testing of Mod-Cam and the first…
View article: CCAT: Mod-Cam Cryogenic Performance and its Impact on 280 GHz KID Array Noise
CCAT: Mod-Cam Cryogenic Performance and its Impact on 280 GHz KID Array Noise Open
The CCAT Observatory's Fred Young Submillimeter Telescope (FYST) is designed to observe submillimeter astronomical signals with high precision, using receivers fielding state-of-the-art kinetic inductance detector (KID) arrays. Mod-Cam, a …
View article: CCAT: Comparisons of 280 GHz TiN and Al Kinetic Inductance Detector Arrays
CCAT: Comparisons of 280 GHz TiN and Al Kinetic Inductance Detector Arrays Open
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 cryosta…
View article: Cosmic Ray Susceptibility of the Terahertz Intensity Mapper Detector Arrays
Cosmic Ray Susceptibility of the Terahertz Intensity Mapper Detector Arrays Open
View article: CONCERTO: Instrument and status
CONCERTO: Instrument and status Open
CONCERTO (CarbON CII line in post-rEionization and ReionizaTiOn) is a low-resolution Fourier transform spectrometer dedicated to the study of star-forming galaxies and clusters of galaxies in the transparent millimeter windows from the gro…
View article: CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope Open
We present a detailed overview of the science goals and predictions for the Prime-Cam direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration for dedicated use on the Fred Young Submillimeter Telescope (FYST)…
View article: IEEE Transactions on Terahertz Science and Technology Publication Information
IEEE Transactions on Terahertz Science and Technology Publication Information Open
View article: IEEE Transactions on Terahertz Science and Technology Publication Information
IEEE Transactions on Terahertz Science and Technology Publication Information Open
View article: Gal/Xgal U/LDB Spectroscopic/Stratospheric THz Observatory: GUSTO
Gal/Xgal U/LDB Spectroscopic/Stratospheric THz Observatory: GUSTO Open
Gal/Xgal U/LDB Spectroscopic/ Stratospheric THz Observatory (GUSTO) is a NASA Explorers Mission of Opportunity that will make large scale maps of the Milky Way and Large Magellanic Cloud in three important interstellar lines: [CII], [OI], …
View article: CONCERTO: a breakthrough in wide field-of-view spectroscopy at millimeter wavelengths
CONCERTO: a breakthrough in wide field-of-view spectroscopy at millimeter wavelengths Open
International audience
View article: CCAT-prime: RFSoC Based Readout for Frequency Multiplexed Kinetic Inductance Detectors
CCAT-prime: RFSoC Based Readout for Frequency Multiplexed Kinetic Inductance Detectors Open
The Prime-Cam instrument on the Fred Young Submillimeter Telescope (FYST) is expected to be the largest deployment of millimeter and submillimeter sensitive kinetic inductance detectors to date. To read out these arrays efficiently, a micr…
View article: CCAT-prime: Design of the Mod-Cam receiver and 280 GHz MKID instrument module
CCAT-prime: Design of the Mod-Cam receiver and 280 GHz MKID instrument module Open
Mod-Cam is a first light and commissioning instrument for the CCAT-prime project's six-meter aperture Fred Young Submillimeter Telescope (FYST), currently under construction at 5600 m on Cerro Chajnantor in Chile's Atacama Desert. Prime-Ca…
View article: CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam
CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam Open
View article: Design and testing of kinetic inductance detector package for the Terahertz Intensity Mapper
Design and testing of kinetic inductance detector package for the Terahertz Intensity Mapper Open
The Terahertz Intensity Mapper (TIM) is designed to probe the star formation history in dust-obscured star-forming galaxies around the peak of cosmic star formation. This will be done via measurements of the redshifted 157.7 μm line of sin…
View article: IEEE Transactions on Terahertz Science and Technology
IEEE Transactions on Terahertz Science and Technology Open
View article: CONCERTO: a breakthrough in wide field-of-view spectroscopy at millimeter wavelengths
CONCERTO: a breakthrough in wide field-of-view spectroscopy at millimeter wavelengths Open
CarbON CII line in post-rEionization and ReionizaTiOn (CONCERTO) is a low-resolution spectrometer with an instantaneous field-of-view of 18.6 arcmin, operating in the 130-310 GHz transparent atmospheric window. It is installed on the 12-me…
View article: IEEE Transactions on Terahertz Science and Technology
IEEE Transactions on Terahertz Science and Technology Open
View article: IEEE Transactions on Terahertz Science and Technology
IEEE Transactions on Terahertz Science and Technology Open
View article: CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope Open
We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for dedicated use on the Fred Young Submillimeter Telescope (FYST)…
View article: 4.7 THz asymmetric beam multiplexer for GUSTO
4.7 THz asymmetric beam multiplexer for GUSTO Open
A full demonstration of the Fourier phase grating used as 4.7 THz local oscillator (LO) multiplexer for Galactic/Extragalactic ULDB Spectroscopic Terahertz Observatory (GUSTO) is presented in this paper, including its design, modeling, tol…
View article: Automated Noise-Parameter Measurements of Cryogenic LNAs
Automated Noise-Parameter Measurements of Cryogenic LNAs Open
This paper addresses the need for measured cryogenic noise parameters. The measurement process is discussed and an analysis of the measurement uncertainty is performed. To verify proper operation of the measurement system, measurements of …
View article: The Atacama large aperture submillimeter telescope (AtLAST) concept
The Atacama large aperture submillimeter telescope (AtLAST) concept Open
The coldest and densest structures of gas and dust in the Universe have unique spectral signatures across the (sub-)millimetre bands (υ ≈30 - 950 GHz). The current generation of single dish facilities has given a glimpse of the potential f…
View article: The Terahertz Intensity Mapper (TIM): a Next-Generation Experiment for Galaxy Evolution Studies
The Terahertz Intensity Mapper (TIM): a Next-Generation Experiment for Galaxy Evolution Studies Open
Understanding the formation and evolution of galaxies over cosmic time is one of the foremost goals of astrophysics and cosmology today. The cosmic star formation rate has undergone a dramatic evolution over the course of the last 14 billi…
View article: Multiple terahertz beams based on a Fourier grating and a quantum cascade laser
Multiple terahertz beams based on a Fourier grating and a quantum cascade laser Open
Large heterodyne receiver arrays (~100 pixel) allow astronomical instrumentations mapping more area within limited space mission lifetime. One challenge is to generate multiple local oscillator (LO) beams. Here, We succeeded in generating …
View article: 81 supra-THz beams generated by a Fourier grating and a quantum cascade laser
81 supra-THz beams generated by a Fourier grating and a quantum cascade laser Open
Large heterodyne receiver arrays (~100 pixel) allow astronomical instrumentations to map more area within limited space mission lifetime. One challenge is to generate multiple local oscillator (LO) beams. Here, we succeeded in generating 8…
View article: The Atacama Large Aperture Submillimeter Telescope (AtLAST)
The Atacama Large Aperture Submillimeter Telescope (AtLAST) Open
The sub-mm sky is a unique window for probing the architecture of the Universe and structures within it. From the discovery of dusty sub-mm galaxies, to the ringed nature of protostellar disks, our understanding of the formation, destructi…
View article: First Generation Heterodyne Instrumentation Concepts for the Atacama Large Aperture Submillimeter Telescope
First Generation Heterodyne Instrumentation Concepts for the Atacama Large Aperture Submillimeter Telescope Open
(abridged) The Atacama Large Aperture Submillimeter Telescope (AtLAST) project aims to build a 50-m-class submm telescope with $>1^\circ$ field of view, high in the Atacama Desert, providing fast and detailed mapping of the mm/submm sky. I…
View article: Complex Field Mapping of Large Direct Detector Focal Plane Arrays
Complex Field Mapping of Large Direct Detector Focal Plane Arrays Open
Complex field mapping is a powerful tool to characterize the optical performance of astronomical instruments, and has become the standard for characterizing heterodyne array cameras. Recently, an adaptation of the heterodyne beam mapping t…
View article: IF system design for the Galactic/Extragalactic ULDB Spectroscopic Terahertz Observatory (GUSTO)
IF system design for the Galactic/Extragalactic ULDB Spectroscopic Terahertz Observatory (GUSTO) Open
We present the design, and prototype phases of the intermediate frequency (IF) system for the upcoming balloon borne observatory, Galactic/Extragalactic Ultra-Long Duration Balloon (ULDB) Spectroscopic Terahertz Ob- servatory (GUSTO). GUST…