Linda L. Ott
Lawrence Livermore National Laboratory
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Publication
Featured researches published by Linda L. Ott.
Journal of Bacteriology | 2004
Vladimir L. Motin; Anca Georgescu; Joseph P. Fitch; Pauline P. Gu; David O. Nelson; Shalini Mabery; Janine B. Garnham; Bahrad A. Sokhansanj; Linda L. Ott; Matthew A. Coleman; Jeffrey M. Elliott; Laura M. Kegelmeyer; Andrew J. Wyrobek; Thomas R. Slezak; Robert R. Brubaker; Emilio Garcia
DNA microarrays encompassing the entire genome of Yersinia pestis were used to characterize global regulatory changes during steady-state vegetative growth occurring after shift from 26 to 37 degrees C in the presence and absence of Ca2+. Transcriptional profiles revealed that 51, 4, and 13 respective genes and open reading frames (ORFs) on pCD, pPCP, and pMT were thermoinduced and that the majority of these genes carried by pCD were downregulated by Ca2+. In contrast, Ca2+ had little effect on chromosomal genes and ORFs, of which 235 were thermally upregulated and 274 were thermally downregulated. The primary consequence of these regulatory events is profligate catabolism of numerous metabolites available in the mammalian host.
Optical Engineering | 1990
Richard M. Bionta; E. Ables; Otis L. Clamp; Oliver Edwards; Peter C. Gabriele; Kirk Miller; Linda L. Ott; Kenneth M. Skulina; Ronald Tilley; T. Viada
We describe the implementation of an 8 keV microscope that operates with a conventional x-ray source in our lab. Samples are scanned pixel-by-pixel through a focused x-ray spot produced by a phase-modulating zone plate fabricated with the sputtered-sliced technique. The micro- focused x-ray source uses a Cu target and produces 8 keV photons that are detected with a Si(Li) spectroscopy system. The microscope currently achieves 10 µm resolution.
The Astrophysical Journal | 1997
H.-S. Park; E. Ables; David L. Band; S. D. Barthelmy; Richard M. Bionta; Paul Butterworth; T. L. Cline; D. H. Ferguson; G. J. Fishman; N. Gehrels; K. Hurley; C. Kouveliotou; B. C. Lee; Charles A. Meegan; Linda L. Ott; E. Parker
The Gamma-Ray Optical Counterpart Search Experiment presents new experimental upper limits on the optical flux from gamma-ray bursts (GRBs). Our experiment consisted of a fully automated very wide-field opto-electronic detection system that imaged locations of GRBs within a few seconds of receiving trigger signals provided by BATSEs real-time burst coordinate distribution network. The experiment acquired 3800 observing hours, recording 22 gamma-ray burst triggers within ~30 s of the start of the burst event. Some of these bursts were imaged while gamma-ray radiation was being detected by BATSE. We identified no optical counterparts associated with gamma-ray bursts among these events at the mV ~ 7.0-8.3 sensitivity level. We find the ratio of the upper limit to the V-band optical flux, Fν, to the gamma-ray fluence, Φγ, from these data to be 1 × 10-18 < Fν/Φγ < 2 × 10-16.
Fourth-Generation X-Ray Sources and Ultrafast X-Ray Detectors | 2004
Mark E. Lowry; Corey V. Bennett; Stephen P. Vernon; Tiziana C. Bond; Rebecca J. Welty; Elaine M. Behymer; Holly E. Petersen; Adam Krey; R. E. Stewart; Nobuhiko P. Kobayashi; Victor Sperry; Phillip L. Stephan; C. E. Reinhardt; Sean Simpson; Paul Stratton; Richard M. Bionta; Mark A. McKernan; E. Ables; Linda L. Ott; Steven W. Bond; J. Ayers; O. L. Landen; P. M. Bell
We present a new x-ray detection technique based on optical measurement of the effects of x-ray absorption and electron hole pair creation in a direct band-gap semiconductor. The electron-hole pairs create a frequency dependent shift in optical refractive index and absorption. This is sensed by simultaneously directing an optical carrier beam through the same volume of semiconducting medium that has experienced an xray induced modulation in the electron-hole population. If the operating wavelength of the optical carrier beam is chosen to be close to the semiconductor band-edge, the optical carrier will be modulated significantly in phase and amplitude. This approach should be simultaneously capable of very high sensitivity and excellent temporal response, even in the difficult high-energy xray regime. At xray photon energies near 10 keV and higher, we believe that sub-picosecond temporal responses are possible with near single xray photon sensitivity. The approach also allows for the convenient and EMI robust transport of high-bandwidth information via fiber optics. Furthermore, the technology can be scaled to imaging applications. The basic physics of the detector, implementation considerations, and preliminary experimental data are presented and discussed.
The Astrophysical Journal | 1997
H.-S. Park; George Grant Williams; E. Ables; David L. Band; S. D. Barthelmy; Richard M. Bionta; Paul Butterworth; T. L. Cline; Donald H. Ferguson; G. J. Fishman; Neil Gehrels; Dieter H. Hartmann; K. Hurley; C. Kouveliotou; Charles A. Meegan; Linda L. Ott; E. Parker; Ron Wurtz
LOTIS is a gamma-ray burst optical counterpart search experiment located near Lawrence Livermore National Laboratory in California. Since operations began in 1996 October, LOTIS has responded to five triggers as of 1997 July 30, which occurred during good weather conditions. GRB 970223 (BATSE trigger 6100) was an exceptionally strong burst, lasting ~30 s with a peak at ~8 s. LOTIS began imaging the error box ~11 s after the burst began and achieved simultaneous optical coverage of 100% of the region enclosed by the BATSE 3 σ error circle and the interplanetary network annulus. No optical transients were observed brighter than the mV~11 completeness limit of the resulting images, providing a new upper limit on the ratio of simultaneous optical to gamma-ray fluence of RL<1.1×10−4 and on the ratio of simultaneous optical (at 700 nm) to gamma-ray (at 100 keV) flux density of RF<305 for a B-type spectrum and RF<475 for an M-type spectrum.
X-Ray/EUV Optics for Astronomy and Microscopy | 1989
Richard M. Bionta; E. Ables; O. Clamp; Oliver Edwards; P.C. Gabriele; D.M. Makowiecki; Linda L. Ott; Kenneth M. Skulina; N. Thomas
Sputtered-sliced transmissive x-ray zone plates consisting of concentric rings of Al and Cu have been fabricated and tested using the 8.04 keV k-a line from Cu. Due to the need for high aspect ratios for this 1.54 A radiation, magnetron sputtering onto a rotating opaque central wire was chosen as the fabrication method. Both the fabrication technology and initial results are presented.
Astrophysics and Space Science | 1995
C. Akerlof; E. Ables; S. D. Barthelmy; Richard M. Bionta; Thomas L. Cline; D. H. Ferguson; G. Fishman; Neil Gehrels; C. Kouveliotou; Brian J. Lee; Charles A. Meegan; Linda L. Ott; Hye-Sook Park; Everette Francis Parker
The GROCSE Collaboration (Gamma-Ray Optical Counterpart Search Experiment) has been operating a rapid response camera since January 1994 in an attempt to capture optical images of GRB events. This detector has a response time of 15 seconds and a limiting magnitude of 8. A second generation detector is now under construction which is expected to eventually reach mv ≃ 15 with a 5 second exposure.
Astronomical Telescopes and Instrumentation | 1998
Hye-Sook Park; E. Ables; S. D. Barthelmy; Richard M. Bionta; Linda L. Ott; E. Parker; George Grant Williams
LOTIS is a rapidly slewing wide-field-of-viewtelescope which was designed and constructed to search for simultaneous gamma- ray burst (GRB) optical counterparts. This experiment requires a rapidly slewing (less than 10 sec), wide-field-of-view (greater than 15 degrees celsius), automatic and dedicated telescope. LOTIS utilizes commercial tele-photo lenses and custom 2048 X 2048 CCD cameras to view a 17.6 X 17.6 degree field of view. It can point to any part of the sky within 5 sec and is fully automated. It is connected via Internet socket to the GRB coordinate distribution network which analyzes telemetry from the satellite and delivers GRB coordinate information in real-time. LOTIS started routine operation in Oct. 1996. In the idle time between GRB triggers, LOTIS systematically surveys the entire available sky every night for new optical transients. This paper will describe the system design and performance.
arXiv: Astrophysics | 1998
George Grant Williams; H.-S. Park; E. Ables; David L. Band; S. D. Barthelmy; Richard M. Bionta; Paul Butterworth; T. L. Cline; D. H. Ferguson; G. J. Fishman; Neil Gehrels; Dieter H. Hartmann; K. Hurley; C. Kouveliotou; Charles A. Meegan; Linda L. Ott; E. Parker; Ron Wurtz
LOTIS (Livermore Optical Transient Imaging System) is a gamma-ray burst optical couterpart search experiment located near Lawrence Livermore National Laboratory in California. The system is linked to the GCN (GRB Coordinates Network) real-time coordinate distribution network and can respond to a burst trigger in 6-15 seconds. LOTIS has a total field-of-view of 17.4 degrees x 17.4 degrees with a completeness sensitivity of mv {approximately} 11 for a 10 second integration time. Since operations began in October 1996, LOTIS has responded to over 30 GCN/BATSE GRB triggers. Seven of these triggers are considered good events subject to the criteria of clear weather conditions, {lt}60 S RESPONSE TIME, AND {gt}50% coverage of the final BATSE 3(sigma) error circle. We discuss results from the first year of LOTIS operations with an emphasis on the observations and analysis of GRB 971006 (BATSE trigger 6414).
X-Ray Multilayers in Diffractometers, Monochromators, and Spectrometers | 1988
Richard M. Bionta; E. Ables; K.J. Cook; Oliver Edwards; P.C. Gabriele; A.F. Jankowski; D.M. Makowiecki; Linda L. Ott; N. Thomas
We have made and tested several sliced multilayer structures that can function as transmissive x-ray optical elements (diffraction gratings, zone plates and phase gratings) at 8-keV. Both amplitude-modulating and phase-modulating devices have been produced. We show data taken in the beam of a 8 keV x-ray source that demonstrate diffraction and focusing. The diffraction patterns produced by the multilayer devices closely match theoretical predictions. Such transmissive optics have the potential for a wide application to high-resolution microscope and spectrometer systems.