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Dive into the research topics where Andrew S. Hoover is active.

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Featured researches published by Andrew S. Hoover.


The Astrophysical Journal | 2009

The Fermi gamma-ray burst monitor

Charles A. Meegan; Giselher G. Lichti; P. N. Bhat; E. Bissaldi; M. S. Briggs; V. Connaughton; R. Diehl; G. J. Fishman; J. Greiner; Andrew S. Hoover; Alexander Jonathan Van Der Horst; Andreas von Kienlin; R. Marc Kippen; C. Kouveliotou; Sheila McBreen; W. S. Paciesas; Robert B. Preece; H. Steinle; M. Wallace; Robert B. Wilson; C. Wilson-Hodge

The Gamma-Ray Burst Monitor (GBM) will significantly augment the science return from the Fermi Observatory in the study of gamma-ray bursts (GRBs). The primary objective of GBM is to extend the energy range over which bursts are observed downward from the energy range of the Large Area Telescope (LAT) on Fermi into the hard X-ray range where extensive previous data sets exist. A secondary objective is to compute burst locations onboard to allow re-orienting the spacecraft so that the LAT can observe delayed emission from bright bursts. GBM uses an array of 12 sodium iodide scintillators and two bismuth germanate scintillators to detect gamma rays from ~8 keV to ~40 MeV over the full unocculted sky. The onboard trigger threshold is ~0.7 photons cm–2 s–1 (50-300 keV, 1 s peak). GBM generates onboard triggers for ~250 GRBs per year.


Applied Physics Letters | 2007

14-pixel, multiplexed array of gamma-ray microcalorimeters with 47eV energy resolution at 103keV

W. B. Doriese; Joel N. Ullom; James A. Beall; W. D. Duncan; L. Ferreira; G. C. Hilton; Robert D. Horansky; K. D. Irwin; J. A. B. Mates; Carl D. Reintsema; Leila R. Vale; Y. Xu; Barry L. Zink; Michael W. Rabin; Andrew S. Hoover; C. R. Rudy; D. T. Vo

The authors present a prototype for a high-energy-resolution, high-count-rate, gamma-ray spectrometer intended for nuclear forensics and international nuclear safeguards. The prototype spectrometer is an array of 14 transition-edge-sensor microcalorimeters with an average energy resolution of 47eV (full width at half maximum) at 103keV. The resolution of the best pixel is 25eV. A cryogenic, time-division multiplexer reads out the array. Several important topics related to microcalorimeter arrays are discussed, including cross-talk, the uniformity of detector bias conditions, fabrication of the arrays, and the multiplexed readout. The measurements and calculations demonstrate that a kilopixel array of high-resolution microcalorimeters is feasible.


Review of Scientific Instruments | 2012

A high resolution gamma-ray spectrometer based on superconducting microcalorimeters

D. A. Bennett; Robert D. Horansky; Daniel R. Schmidt; Andrew S. Hoover; Ryan Winkler; Bradley K. Alpert; James A. Beall; W. B. Doriese; J. W. Fowler; C. P. Fitzgerald; G. C. Hilton; K. D. Irwin; V. Kotsubo; J. A. B. Mates; G. C. O’Neil; Michael W. Rabin; Carl D. Reintsema; F. J. Schima; Daniel S. Swetz; Leila R. Vale; Joel N. Ullom

Improvements in superconductor device fabrication, detector hybridization techniques, and superconducting quantum interference device readout have made square-centimeter-sized arrays of gamma-ray microcalorimeters, based on transition-edge sensors (TESs), possible. At these collecting areas, gamma microcalorimeters can utilize their unprecedented energy resolution to perform spectroscopy in a number of applications that are limited by closely-spaced spectral peaks, for example, the nondestructive analysis of nuclear materials. We have built a 256 pixel spectrometer with an average full-width-at-half-maximum energy resolution of 53 eV at 97 keV, a useable dynamic range above 400 keV, and a collecting area of 5 cm(2). We have demonstrated multiplexed readout of the full 256 pixel array with 236 of the pixels (91%) giving spectroscopic data. This is the largest multiplexed array of TES microcalorimeters to date. This paper will review the spectrometer, highlighting the instrument design, detector fabrication, readout, operation of the instrument, and data processing. Further, we describe the characterization and performance of the newest 256 pixel array.


IEEE Transactions on Nuclear Science | 2009

Large-Area Microcalorimeter Detectors for Ultra-High-Resolution X-Ray and Gamma-Ray Spectroscopy

M. K. Bacrania; Andrew S. Hoover; P. J. Karpius; Michael W. Rabin; C. R. Rudy; Duc Vo; James A. Beall; D. A. Bennett; W. B. Doriese; G. C. Hilton; Robert D. Horansky; K. D. Irwin; N. Jethava; E. Sassi; Joel N. Ullom; Leila R. Vale

We discuss recent developments in using cryogenic microcalorimeter detectors for x- and gamma-ray spectroscopy. We are currently operating a detector array consisting of thirteen pixels with time-domain multiplexed readout. With a single pixel from this detector, we have measured 97.43-keV gamma rays from 153-Gd with 22-eV resolution (FWHM). We have also made the first multiplexed array measurements of plutonium x- and gamma-rays with 45-eV resolution. We are currently testing a 66-pixel next-generation detector chip. Preliminary measurements with the new detector indicate improved energy linearity and single-pixel energy resolution of 50-100 eV at 100 keV. We present preliminary calibration data from this chip, and a high-statistics multiplexed 21-pixel spectrum of the Pu x-ray region between 90 and 130 keV.


Structural Dynamics | 2015

Laser plasma x-ray source for ultrafast time-resolved x-ray absorption spectroscopy.

L. Miaja-Avila; Galen C. O'Neil; Jens Uhlig; Christopher L. Cromer; Marla L. Dowell; Ralph Jimenez; Andrew S. Hoover; Kevin L. Silverman; Joel N. Ullom

We describe a laser-driven x-ray plasma source designed for ultrafast x-ray absorption spectroscopy. The source is comprised of a 1 kHz, 20 W, femtosecond pulsed infrared laser and a water target. We present the x-ray spectra as a function of laser energy and pulse duration. Additionally, we investigate the plasma temperature and photon flux as we vary the laser energy. We obtain a 75 μm FWHM x-ray spot size, containing ∼106 photons/s, by focusing the produced x-rays with a polycapillary optic. Since the acquisition of x-ray absorption spectra requires the averaging of measurements from >107 laser pulses, we also present data on the source stability, including single pulse measurements of the x-ray yield and the x-ray spectral shape. In single pulse measurements, the x-ray flux has a measured standard deviation of 8%, where the laser pointing is the main cause of variability. Further, we show that the variability in x-ray spectral shape from single pulses is low, thus justifying the combining of x-rays obtained from different laser pulses into a single spectrum. Finally, we show a static x-ray absorption spectrum of a ferrioxalate solution as detected by a microcalorimeter array. Altogether, our results demonstrate that this water-jet based plasma source is a suitable candidate for laboratory-based time-resolved x-ray absorption spectroscopy experiments.


Review of Scientific Instruments | 2013

Note: Operation of gamma-ray microcalorimeters at elevated count rates using filters with constraints

Bradley K. Alpert; Robert D. Horansky; D. A. Bennett; W. B. Doriese; Joseph W. Fowler; Andrew S. Hoover; Michael W. Rabin; Joel N. Ullom

Microcalorimeter sensors operated near 0.1 K can measure the energy of individual x- and gamma-ray photons with significantly more precision than conventional semiconductor technologies. Both microcalorimeter arrays and higher per pixel count rates are desirable to increase the total throughput of spectrometers based on these devices. The millisecond recovery time of gamma-ray microcalorimeters and the resulting pulse pileup are significant obstacles to high per pixel count rates. Here, we demonstrate operation of a microcalorimeter detector at elevated count rates by use of convolution filters designed to be orthogonal to the exponential tail of a preceding pulse. These filters allow operation at 50% higher count rates than conventional filters while largely preserving sensor energy resolution.


IEEE Transactions on Nuclear Science | 2013

Determination of Plutonium Isotopic Content by Microcalorimeter Gamma-Ray Spectroscopy

Andrew S. Hoover; Ryan Winkler; Michael W. Rabin; Duc Vo; Joel N. Ullom; D. A. Bennett; W. B. Doriese; Joseph W. Fowler; Robert D. Horansky; Daniel R. Schmidt; Leila R. Vale; Kathryn Schaffer

Microcalorimeter detectors provide unprecedented energy resolution for gamma-ray spectroscopy. One application is measuring the isotopic composition of plutonium-bearing samples by non-destructive gamma-ray spectroscopy to support nuclear safeguards and nonproliferation efforts. When measured with conventional high-purity germanium (HPGe) detectors, data from these samples contain significant peak overlaps requiring spectral deconvolution for analysis. The improved energy resolution of the microcalorimeter detector reduces peak overlaps leading to improvement in the statistical error component of the total measurement uncertainty. In this paper, we describe analysis code that was developed for spectral peak fitting and isotopic content determination from microcalorimeter and HPGe data. We apply the code to data collected from several plutonium standards to quantify the improvement of the statistical error derived from the improved energy resolution.


IEEE Transactions on Applied Superconductivity | 2015

Integration of TES Microcalorimeters With Microwave SQUID Multiplexed Readout

D. A. Bennett; J. A. B. Mates; J. Gard; Andrew S. Hoover; Michael W. Rabin; Carl D. Reintsema; Daniel R. Schmidt; Leila R. Vale; Joel N. Ullom

The demonstration of a microwave superconducting quantum interference device (SQUID) multiplexed readout of transition-edge sensor (TES) microcalorimeters has the potential to dramatically expand the scale of arrays of TESs. In this paper, we discuss recent work to develop an instrument for high-resolution high-efficiency gamma-ray spectroscopy that integrates previously demonstrated high-resolution TES microcalorimeters with new lower noise microwave SQUID multiplexers. We will discuss the proposed instrument design and readout noise of the optimized microwave SQUID multiplexed readout. Finally, we will discuss the potential limits on the number of multiplexed TESs imposed by the analog-to-digital converter.


Applied Physics Letters | 2010

An analytical model for pulse shape and electrothermal stability in two-body transition-edge sensor microcalorimeters

D. A. Bennett; Robert D. Horansky; Andrew S. Hoover; Nathan J Hoteling; Michael W. Rabin; Daniel R. Schmidt; Daniel S. Swetz; Leila R. Vale; Joel N. Ullom

High-resolution superconducting gamma-ray sensors show potential for the more accurate analysis of nuclear material. These devices are part of a larger class of microcalorimeters and bolometers based on transition edge sensors (TESs) that have two distinct thermal bodies. We derive the time domain behavior of the current and temperature for compound TES devices in the small signal limit and demonstrate the utility of these equations for device design and characterization. In particular, we use the model to fit pulses from our gamma-ray microcalorimeters and demonstrate how critical damping and electrothermal stability can be predicted.


Proceedings of SPIE | 2004

The GLAST burst monitor

Andreas von Kienlin; Charles A. Meegan; Giselher G. Lichti; Narayana P. Bhat; M. S. Briggs; V. Connaughton; R. Diehl; G. J. Fishman; J. Greiner; Andrew S. Hoover; R. Marc Kippen; C. Kouveliotou; W. S. Paciesas; Robert D. Preece; V. Schönfelder; H. Steinle; Robert B. Wilson

The next large NASA mission in the field of gamma-ray astronomy, GLAST, is scheduled for launch in 2007. Aside from the main instrument LAT (Large-Area Telescope), a gamma-ray telescope for the energy range between 20 MeV and > 100GeV, a secondary instrument, the GLAST burst monitor (GBM), is foreseen. With this monitor one of the key scientific objectives of the mission, the determination of the high-energy behaviour of gamma-ray bursts and transients can be ensured. Its task is to increase the detection rate of gamma-ray bursts for the LAT and to extend the energy range to lower energies (from ~10 keV to ~30 MeV). It will provide real-time burst locations over a wide FoV with sufficient accuracy to allow repointing the GLAST spacecraft. Time-resolved spectra of many bursts recorded with LAT and the burst monitor will allow the investigation of the relation between the keV and the MeV-GeV emission from GRBs over unprecedented seven decades of energy. This will help to advance our understanding of the mechanisms by which gamma-rays are generated in gamma-ray bursts

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Michael W. Rabin

Los Alamos National Laboratory

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Joel N. Ullom

National Institute of Standards and Technology

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Robert D. Horansky

National Institute of Standards and Technology

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Leila R. Vale

National Institute of Standards and Technology

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D. A. Bennett

National Institute of Standards and Technology

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W. B. Doriese

National Institute of Standards and Technology

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James A. Beall

National Institute of Standards and Technology

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R. M. Kippen

Los Alamos National Laboratory

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Daniel R. Schmidt

National Institute of Standards and Technology

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