J. A. Shariff
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View article: Electrocardiogram sequences data analytics and classification using unsupervised and supervised machine learning algorithms
Electrocardiogram sequences data analytics and classification using unsupervised and supervised machine learning algorithms Open
This paper explores the prediction of cardiovascular disease (CVD) through the classification of electrocardiogram (ECG) sequences using both supervised and unsupervised machine learning (ML) algorithms. ECG 5000 dataset is considered to p…
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: Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER
Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER Open
Using data from the first flight of SPIDER and from Planck HFI, we probe the properties of polarized emission from interstellar dust in the SPIDER observing region. Component separation algorithms operating in both the spatial and harmonic…
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: 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: 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: 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: Submillimeter Polarization Spectrum of the Carina Nebula
Submillimeter Polarization Spectrum of the Carina Nebula Open
Linear polarization maps of the Carina Nebula were obtained at 250, 350, and 500 μm during the 2012 flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol). These measurements are combined with Planck …
View article: SPIDER: CMB Polarimetry from the Edge of Space
SPIDER: CMB Polarimetry from the Edge of Space Open
View article: The relation between the column density structures and the magnetic field orientation in the Vela C molecular complex
The relation between the column density structures and the magnetic field orientation in the Vela C molecular complex Open
We statistically evaluated the relative orientation between gas column density structures, inferred from Herschel submillimetre observations, and the magnetic field projected on the plane of sky, inferred from polarized thermal emission of…
View article: Optimization of Transition Edge Sensor Arrays for Cosmic Microwave Background Observations With the South Pole Telescope
Optimization of Transition Edge Sensor Arrays for Cosmic Microwave Background Observations With the South Pole Telescope Open
In this paper, we describe the optimization of transition-edge-sensor (TES) detector arrays for the third-generation camera for the South Pole Telescope. The camera, which contains ~16 000 detectors, will make high-angular-resolution maps …
View article: Large arrays of dual-polarized multichroic TES detectors for CMB measurements with the SPT-3G receiver
Large arrays of dual-polarized multichroic TES detectors for CMB measurements with the SPT-3G receiver Open
Detectors for cosmic microwave background (CMB) experiments are now essentially background limited, so a straightforward alternative to improve sensitivity is to increase the number of detectors. Large arrays of multichroic pixels constitu…
View article: SUBMILLIMETER POLARIZATION SPECTRUM IN THE VELA C MOLECULAR CLOUD
SUBMILLIMETER POLARIZATION SPECTRUM IN THE VELA C MOLECULAR CLOUD Open
Polarization maps of the Vela C molecular cloud were obtained at 250, 350, and 500 μ m during the 2012 flight of the balloon-borne telescope BLASTPol. These measurements are used in conjunction with 850 μ m data from Planck to study the su…
View article: Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud
Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud Open
We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight with polarized emission data at submillimeter (sub-mm) wavelengths for the Vela C molecular cloud. The near-IR data co…
View article: A cryogenic rotation stage with a large clear aperture for the half-wave plates in the Spider instrument
A cryogenic rotation stage with a large clear aperture for the half-wave plates in the Spider instrument Open
We describe the cryogenic half-wave plate rotation mechanisms built for and used in Spider, a polarization-sensitive balloon-borne telescope array that observed the cosmic microwave background at 95 GHz and 150 GHz during a stratospheric b…
View article: Polarimetry from the stratosphere with SPIDER and BLASTPol
Polarimetry from the stratosphere with SPIDER and BLASTPol Open
This thesis presents the hardware development and flight performance of two balloon-borne experiments. The Spider experiment is a millimetre-wavelength polarimeter designed to measure B-mode polarization in the Cosmic Microwave Background …
View article: A cryogenic rotation stage with a large clear aperture for a half-wave plate
A cryogenic rotation stage with a large clear aperture for a half-wave plate Open
We describe the cryogenic half-wave plate rotation mechanisms built for and used in Spider, a polarization-sensitive balloon-borne telescope array that observed the Cosmic Microwave Background at 95 GHz and 150 GHz during a stratospheric b…
View article: The thermal design, characterization, and performance of the S pider long-duration balloon cryostat
The thermal design, characterization, and performance of the S pider long-duration balloon cryostat Open