5,512 research outputs found
Single-shot compressed ultrafast photography: a review
Compressed ultrafast photography (CUP) is a burgeoning single-shot computational imaging technique that provides an imaging speed as high as 10 trillion frames per second and a sequence depth of up to a few hundred frames. This technique synergizes compressed sensing and the streak camera technique to capture nonrepeatable ultrafast transient events with a single shot. With recent unprecedented technical developments and extensions of this methodology, it has been widely used in ultrafast optical imaging and metrology, ultrafast electron diffraction and microscopy, and information security protection. We review the basic principles of CUP, its recent advances in data acquisition and image reconstruction, its fusions with other modalities, and its unique applications in multiple research fields
Observation of laser pulse propagation in optical fibers with a SPAD camera
Recording processes and events that occur on sub-nanosecond timescales poses a difficult challenge. Conventional ultrafast imaging techniques often rely on long data collection times, which can be due to limited device sensitivity and/or the requirement of scanning the detection system to form an image. In this work, we use a single-photon avalanche detector array camera with pico-second timing accuracy to detect photons scattered by the cladding in optical fibers. We use this method to film supercontinuum generation and track a GHz pulse train in optical fibers. We also show how the limited spatial resolution of the array can be improved with computational imaging. The single-photon sensitivity of the camera and the absence of scanning the detection system results in short total acquisition times, as low as a few seconds depending on light levels. Our results allow us to calculate the group index of different wavelength bands within the supercontinuum generation process. This technology can be applied to a range of applications, e.g., the characterization of ultrafast processes, time-resolved fluorescence imaging, three-dimensional depth imaging, and tracking hidden objects around a corner. © The Author(s) 20171541sciescopu
The EBEX Balloon-borne Experiment—Gondola, Attitude Control, and Control Software
The E and B Experiment (EBEX) was a long-duration balloon-borne instrument designed to measure the polarization of the cosmic microwave background (CMB) radiation. EBEX was the first balloon-borne instrument to implement a kilopixel array of transition edge sensor (TES) bolometric detectors and the first CMB experiment to use the digital version of the frequency domain multiplexing system for readout of the TES array. The scan strategy relied on 40 s peak-to-peak constant-velocity azimuthal scans. We discuss the unique demands on the design and operation of the payload that resulted from these new technologies and the scan strategy. We describe the solutions implemented, including the development of a power system designed to provide a total of at least 2.3 kW, a cooling system to dissipate 590 W consumed by the detectors' readout system, software to manage and handle the data of the kilopixel array, and specialized attitude reconstruction software. We present flight performance data showing faultless management of the TES array, adequate powering and cooling of the readout electronics, and constraint of attitude reconstruction errors such that the spurious B-modes they induced were less than 10% of the CMB B-mode power spectrum with r = 0.05
Optical Synoptic Telescopes: New Science Frontiers
Over the past decade, sky surveys such as the Sloan Digital Sky Survey have
proven the power of large data sets for answering fundamental astrophysical
questions. This observational progress, based on a synergy of advances in
telescope construction, detectors, and information technology, has had a
dramatic impact on nearly all fields of astronomy, and areas of fundamental
physics. The next-generation instruments, and the surveys that will be made
with them, will maintain this revolutionary progress. The hardware and
computational technical challenges and the exciting science opportunities are
attracting scientists and engineers from astronomy, optics, low-light-level
detectors, high-energy physics, statistics, and computer science. The history
of astronomy has taught us repeatedly that there are surprises whenever we view
the sky in a new way. This will be particularly true of discoveries emerging
from a new generation of sky surveys. Imaging data from large ground-based
active optics telescopes with sufficient etendue can address many scientific
missions simultaneously. These new investigations will rely on the statistical
precision obtainable with billions of objects. For the first time, the full sky
will be surveyed deep and fast, opening a new window on a universe of faint
moving and distant exploding objects as well as unraveling the mystery of dark
energy.Comment: 12 pages, 7 figure
Imaging dynamics beneath turbid media via parallelized single-photon detection
Noninvasive optical imaging through dynamic scattering media has numerous
important biomedical applications but still remains a challenging task. While
standard methods aim to form images based upon optical absorption or
fluorescent emission, it is also well-established that the temporal correlation
of scattered coherent light diffuses through tissue much like optical
intensity. Few works to date, however, have aimed to experimentally measure and
process such data to demonstrate deep-tissue imaging of decorrelation dynamics.
In this work, we take advantage of a single-photon avalanche diode (SPAD) array
camera, with over one thousand detectors, to simultaneously detect speckle
fluctuations at the single-photon level from 12 different phantom tissue
surface locations delivered via a customized fiber bundle array. We then apply
a deep neural network to convert the acquired single-photon measurements into
video of scattering dynamics beneath rapidly decorrelating liquid tissue
phantoms. We demonstrate the ability to record video of dynamic events
occurring 5-8 mm beneath a decorrelating tissue phantom with mm-scale
resolution and at a 2.5-10 Hz frame rate
Instruments on large optical telescopes -- A case study
In the distant past, telescopes were known, first and foremost, for the sizes
of their apertures. Advances in technology are now enabling astronomers to
build extremely powerful instruments to the extent that instruments have now
achieved importance comparable or even exceeding the usual importance accorded
to the apertures of the telescopes. However, the cost of successive generations
of instruments has risen at a rate noticeably above that of the rate of
inflation. Here, given the vast sums of money now being expended on optical
telescopes and their instrumentation, I argue that astronomers must undertake
"cost-benefit" analysis for future planning. I use the scientific output of the
first two decades of the W. M. Keck Observatory as a laboratory for this
purpose. I find, in the absence of upgrades, that the time to reach peak paper
production for an instrument is about six years. The prime lifetime of
instruments (sans upgrades), as measured by citations returns, is about a
decade. Well thought out and timely upgrades increase and sometimes even double
the useful lifetime. I investigate how well instrument builders are rewarded. I
find acknowledgements ranging from almost 100% to as low as 60%. Next, given
the increasing cost of operating optical telescopes, the management of existing
observatories continue to seek new partnerships. This naturally raises the
question "What is the cost of a single night of telescope time". I provide a
rational basis to compute this quantity. I then end the paper with some
thoughts on the future of large ground-based optical telescopes, bearing in
mind the explosion of synoptic precision photometric, astrometric and imaging
surveys across the electromagnetic spectrum, the increasing cost of
instrumentation and the rise of mega instruments.Comment: Revised from previous submission (typos fixed, table 6 was garbled).
Submitted to PAS
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