Sean Bryan
YOU?
Author Swipe
View article: Spaceflight KID Readout Electronics for PRIMA
Spaceflight KID Readout Electronics for PRIMA Open
We present the design and testing of a prototype multiplexing kinetic inductance detector (KID) readout electronics for the PRobe far-Infrared Mission for Astrophysics (PRIMA) space mission. PRIMA is a Probe-class astrophysics mission conc…
View article: The SPHEREx Sky Simulator: Science Data Modeling for the First All-sky Near-infrared Spectral Survey
The SPHEREx Sky Simulator: Science Data Modeling for the First All-sky Near-infrared Spectral Survey Open
We describe the SPHEREx Sky Simulator (henceforth the Simulator), a software tool designed to model science data for NASA’s SPHEREx mission that will carry out a series of all-sky spectrophotometric surveys at ∼6″ spatial resolution in 102…
View article: KID Detector Readout Electronics Development for Habitable Worlds Observatory
KID Detector Readout Electronics Development for Habitable Worlds Observatory Open
We present the status and goals of the readout electronics system we are developing to support the detector arrays in the coronagraph instrument on the NASA Habitable Worlds Observatory (HWO) mission currently in development. HWO aims to r…
View article: SPHEREx Discovery of Strong Water Ice Absorption and an Extended Carbon Dioxide Coma in 3I/ATLAS
SPHEREx Discovery of Strong Water Ice Absorption and an Extended Carbon Dioxide Coma in 3I/ATLAS Open
In mid-August 2025, 0.75–5.0 μ m SPHEREx imaging spectrophotometric and ancillary NASA-IRTF/SpeX 0.7–2.5 μ m low-resolution spectral observations of 3I/ATLAS were obtained. The combined spectrophotometry is dominated by features due to wat…
View article: The SPHEREx Sky Simulator: Science Data Modeling for the First All-Sky Near-Infrared Spectral Survey
The SPHEREx Sky Simulator: Science Data Modeling for the First All-Sky Near-Infrared Spectral Survey Open
We describe the SPHEREx Sky Simulator, a software tool designed to model science data for NASA's SPHEREx mission that will carry out a series of all-sky spectrophotometric surveys at $\sim$6'' spatial resolution in 102 spectral channels sp…
View article: The Relational Dynamics of Space-Time
The Relational Dynamics of Space-Time Open
The Relational Dynamics of Space-Time is a groundbreaking theory that redefines space-time as an emergent and discrete structure, arising from fundamental interactions between elementary entities. Rooted in the principle that “nothing is e…
View article: In-flight performance of SPIDER's 280 GHz receivers
In-flight performance of SPIDER's 280 GHz receivers Open
SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. Spider has mapped a large sky area in the Southern Hemisphere using more than 2000 trans…
View article: Robust Joint Estimation of Galaxy Redshift and Spectral Templates using Online Dictionary Learning
Robust Joint Estimation of Galaxy Redshift and Spectral Templates using Online Dictionary Learning Open
We present a novel approach to analyzing astronomical spectral survey data using our non-linear extension of an online dictionary learning algorithm. Current and upcoming surveys such as SPHEREx will use spectral data to build a 3D map of …
View article: BoloCalc: a sensitivity calculator for the design of Simons Observatory (Erratum)
BoloCalc: a sensitivity calculator for the design of Simons Observatory (Erratum) Open
Publisher's Note: This paper, originally published on, 9 July 2018, was replaced with a corrected/revised version on,12 September 2023. If you downloaded the original PDF but are unable to access the revision, please contact SPIE Digital L…
View article: In-Flight Gain Monitoring of SPIDER’s Transition-Edge Sensor Arrays
In-Flight Gain Monitoring of SPIDER’s Transition-Edge Sensor Arrays Open
View article: A Simulation-based Method for Correcting Mode Coupling in CMB Angular Power Spectra
A Simulation-based Method for Correcting Mode Coupling in CMB Angular Power Spectra Open
Modern cosmic microwave background (CMB) analysis pipelines regularly employ complex time-domain filters, beam models, masking, and other techniques during the production of sky maps and their corresponding angular power spectra. However, …
View article: Snowmass 2021 CMB-S4 White Paper
Snowmass 2021 CMB-S4 White Paper Open
This Snowmass 2021 White Paper describes the Cosmic Microwave Background Stage 4 project CMB-S4, which is designed to cross critical thresholds in our understanding of the origin and evolution of the Universe, from the highest energies at …
View article: Snowmass2021 CMB-HD White Paper
Snowmass2021 CMB-HD White Paper Open
CMB-HD is a proposed millimeter-wave survey over half the sky that would be ultra-deep (0.5 uK-arcmin) and have unprecedented resolution (15 arcseconds at 150 GHz). Such a survey would answer many outstanding questions about the fundamenta…
View article: A Constraint on Primordial B-modes from the First Flight of the Spider Balloon-borne Telescope
A Constraint on Primordial B-modes from the First Flight of the Spider Balloon-borne Telescope Open
We present the first linear polarization measurements from the 2015 long-duration balloon flight of Spider , which is an experiment that is designed to map the polarization of the cosmic microwave background (CMB) on degree angular scales.…
View article: CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
CMB-S4: Forecasting Constraints on Primordial Gravitational Waves Open
CMB-S4—the next-generation ground-based cosmic microwave background (CMB) experiment—is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the universe. Among the s…
View article: IEEE Transactions on Terahertz Science and Technology
IEEE Transactions on Terahertz Science and Technology Open
View article: The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps
The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps Open
We present the XFaster analysis package, a fast, iterative angular power spectrum estimator based on a diagonal approximation to the quadratic Fisher matrix estimator. It uses Monte Carlo simulations to compute noise biases and filter tran…
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: 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: IEEE Transactions on Terahertz Science and Technology
IEEE Transactions on Terahertz Science and Technology Open
View article: Design and pre-flight performance of SPIDER 280 GHz receivers
Design and pre-flight performance of SPIDER 280 GHz receivers Open
In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimized to search for a primordial B-mode polarization signature …
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: SPHEREx: NASA's near-infrared spectrophotometric all-sky survey
SPHEREx: NASA's near-infrared spectrophotometric all-sky survey Open
SPHEREx, the Spectro-Photometer for the History of the Universe, Epoch of\nReionization, and ices Explorer, is a NASA MIDEX mission planned for launch in\n2024. SPHEREx will carry out the first all-sky spectral survey at wavelengths\nbetwe…
View article: A millimeter-wave kinetic inductance detector camera for long-range imaging through optical obscurants
A millimeter-wave kinetic inductance detector camera for long-range imaging through optical obscurants Open
Millimeter-wave imaging provides a promising option for long-range target detection through optical obscurants such as fog, which often occur in marine environments. Given this motivation, we are currently developing a 150 GHz polarization…
View article: CMB-HD: Astro2020 RFI Response
CMB-HD: Astro2020 RFI Response Open
CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both fundamental physics of the Universe and astrophysics. This surve…
View article: CMB-S4 Decadal Survey APC White Paper
CMB-S4 Decadal Survey APC White Paper Open
We provide an overview of the science case, instrument configuration and project plan for the next-generation ground-based cosmic microwave background experiment CMB-S4, for consideration by the 2020 Decadal Survey.
View article: The Simons Observatory: Astro2020 Decadal Project Whitepaper
The Simons Observatory: Astro2020 Decadal Project Whitepaper Open
The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough discoveries in fundamental physics, cosmology, and astrophy…
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…