183 results on '"Sina, R."'
Search Results
2. Advances in DBS Technology and Novel Applications: Focus on Movement Disorders
- Author
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Potel, Sina R., Marceglia, Sara, Meoni, Sara, Kalia, Suneil K., Cury, Rubens G., and Moro, Elena
- Published
- 2022
- Full Text
- View/download PDF
3. George Sword’s Warrior Narratives: Compositional Processes in Lakota Oral Tradition. By Delphine Red Shirt.
- Author
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Bear Eagle, Sina R.
- Published
- 2017
4. Cosmic-Ray Proton and Helium Spectra from the First CREAM Flight
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Yoon, Y. S., Ahn, H. S., Allison, P. S., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P. S., Minnick, S. A., Mognet, S. I., Nam, S., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Swordy, S., Wakely, S. P., Wu, J., Yang, J., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
Cosmic-ray proton and helium spectra have been measured with the balloon-borne Cosmic Ray Energetics And Mass experiment flown for 42 days in Antarctica in the 2004-2005 austral summer season. High-energy cosmic-ray data were collected at an average altitude of ~38.5 km with an average atmospheric overburden of ~3.9 g cm$^{-2}$. Individual elements are clearly separated with a charge resolution of ~0.15 e (in charge units) and ~0.2 e for protons and helium nuclei, respectively. The measured spectra at the top of the atmosphere are represented by power laws with a spectral index of -2.66 $\pm$ 0.02 for protons from 2.5 TeV to 250 TeV and -2.58 $\pm$ 0.02 for helium nuclei from 630 GeV/nucleon to 63 TeV/nucleon. They are harder than previous measurements at a few tens of GeV/nucleon. The helium flux is higher than that expected from the extrapolation of the power law fitted to the lower-energy data. The relative abundance of protons to helium nuclei is 9.1 $\pm$ 0.5 for the range from 2.5 TeV/nucleon to 63 TeV/nucleon. This ratio is considerably smaller than the previous measurements at a few tens of GeV/nucleon., Comment: 20 pages, 4 figures
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- 2011
- Full Text
- View/download PDF
5. Discrepant hardening observed in cosmic-ray elemental spectra
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Ahn, H. S., Allison, P., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Lutz, L., Maestro, P., Malinin, A., Marrocchesi, P. S., Minnick, S., Mognet, S. I., Nam, J., Nam, S., Nutter, S. L., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The balloon-borne Cosmic Ray Energetics And Mass (CREAM) experiment launched five times from Antarctica has achieved a cumulative flight duration of about 156 days above 99.5% of the atmosphere. The instrument is configured with complementary and redundant particle detectors designed to extend direct measurements of cosmic-ray composition to the highest energies practical with balloon flights. All elements from protons to iron nuclei are separated with excellent charge resolution. Here we report results from the first two flights of ~70 days, which indicate hardening of the elemental spectra above ~200 GeV/nucleon and a spectral difference between the two most abundant species, protons and helium nuclei. These results challenge the view that cosmic-ray spectra are simple power laws below the so-called knee at ~1015 eV. This discrepant hardening may result from a relatively nearby source, or it could represent spectral concavity caused by interactions of cosmic rays with the accelerating shock. Other possible explanations should also be investigated., Comment: 21 pages, 5 figures, published in ApJL (corresponding author: seo@umd.edu)
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- 2010
- Full Text
- View/download PDF
6. Measurements of cosmic-ray energy spectra with the 2nd CREAM flight
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Maestro, P., Ahn, H. S., Allison, P., Bagliesi, M. G., Barbier, L., Beatty, J. J., Bigongiari, G., Brandt, T. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Malinine, A., Marrocchesi, P. S., Minnick, S., Mognet, S. I., Nam, S. W., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Walpole, P., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
During its second Antarctic flight, the CREAM (Cosmic Ray Energetics And Mass) balloon experiment collected data for 28 days, measuring the charge and the energy of cosmic rays (CR) with a redundant system of particle identification and an imaging thin ionization calorimeter. Preliminary direct measurements of the absolute intensities of individual CR nuclei are reported in the elemental range from carbon to iron at very high energy., Comment: 4 pages, 3 figures, presented at XV International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2008)
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- 2010
- Full Text
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7. Elemental energy spectra of cosmic rays measured by CREAM-II
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Maestro, P., Ahn, H. S., Allison, P., Bagliesi, M. G., Barbier, L., Beatty, J. J., Bigongiari, G., Brandt, T. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Malinine, A., Marrocchesi, P. S., Minnick, S., Mognet, S. I., Nam, S. W., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Walpole, P., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present new measurements of the energy spectra of cosmic-ray (CR) nuclei from the second flight of the balloon-borne experiment CREAM (Cosmic Ray Energetics And Mass). The instrument (CREAM-II) was comprised of detectors based on different techniques (Cherenkov light, specific ionization in scintillators and silicon sensors) to provide a redundant charge identification and a thin ionization calorimeter capable of measuring the energy of cosmic rays up to several hundreds of TeV. The data analysis is described and the individual energy spectra of C, O, Ne, Mg, Si and Fe are reported up to ~ 10^14 eV. The spectral shape looks nearly the same for all the primary elements and can be expressed as a power law in energy E^{-2.66+/-0.04}. The nitrogen absolute intensity in the energy range 100-800 GeV/n is also measured., Comment: 4 pages, 3 figures, presented at ICRC 2009, Lodz, Poland
- Published
- 2010
8. Energy cross-calibration from the first CREAM flight: transition radiation detector versus calorimeter
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Maestro, P., Ahn, H. S., Allison, P. S., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P. J., Brandt, T. J., Childers, J. T., Conklin, N. B., Coutu, S., Duvernois, M. A., Ganel, O., Han, J. H., Hyun, H. J., Jeon, J. A., Kim, K. C., Lee, J. K., Lee, M. H., Lutz, L., Marrocchesi, P. S., Malinine, A., Minnick, S., Mognet, S. I., Nam, S., Nutter, S., Park, H., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Swordy, S., Wakely, S. P., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
The Cosmic Ray Energetics And Mass (CREAM) balloon experiment had two successful flights in 2004/05 and 2005/06. It was designed to perform energy measurements from a few GeV up to 1000 TeV, taking advantage of different detection techniques. The first instrument, CREAM-1, combined a transition radiation detector with a calorimeter to provide independent energy measurements of cosmicraynuclei. Each detector was calibrated with particle beams in a limited range of energies. In order to assess the absolute energy scale of the instrument and to investigate the systematic effects of each technique, a cross-calibration was performed by comparing the two independent energy estimates on selected samples of oxygen and carbon nuclei., Comment: 4 pages, 3 figures, presented at ICRC 2008
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- 2010
9. Elemental Spectra from the CREAM-I Flight
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Ahn, H. S., Allison, P., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P., Childers, J. T., Conklin, N. B., Coutu, S., Duvernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, J. K., Lee, M. H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P. S., Minnick, S., Mognet, S. I., Nam, S., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Swordy, S., Wakely, S., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ~ 10^15 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from Mc- Murdo Station, Antarctica, in December 2004 and December 2005. CREAM-I achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector and a Silicon Charge Detector (SCD) for particle identification, and a Transition Radiation Detector and a sampling tungsten/scintillating-fiber ionization calorimeter (CAL) for energy measurement. In this paper, preliminary energy spectra of various elements measured with CAL/SCD during the first 42-day flight are presented., Comment: Proc. 30th Int. Cosmic Ray Conf., Merida, 2, 63-66, 2007
- Published
- 2010
- Full Text
- View/download PDF
10. Performance of the CREAM calorimeter in accelerator beam test
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Yoon, Y. S., Ahn, H. S., Bagliesi, M. G., Bigongiari, G., Ganel, O., Han, J. H., Hyun, H. J., Jeon, J. A., Kang, T. G., Kim, H. J., Kim, K. C., Lee, J. K., Lee, M. H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P. S., Nam, S. W., Park, H., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Wu, J., Yang, J., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The CREAM calorimeter, designed to measure the spectra of cosmic-ray nuclei from under 1 TeV to 1000 TeV, is a 20 radiation length (X0) deep sampling calorimeter. The calorimeter is comprised of 20 layers of tungsten interleaved with 20 layers of scintillating fiber ribbons, and is preceded by a pair of graphite interaction targets providing about 0.42 proton interaction lengths (\lambda int). The calorimeter was placed in one of CERN's SPS accelerator beams for calibration and testing. Beams of 150 GeV electrons were used for calibration, and a variety of electron, proton, and nuclear fragment beams were used to test the simulation model of the detector. In this paper we discuss the performance of the calorimeter in the electron beam and compare electron beam data with simulation results., Comment: 29th International Cosmic Ray Conference Pune (2005) 8, 371-374
- Published
- 2010
11. Calibration of the CREAM-I calorimeter
- Author
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Yoon, Y. S., Ahn, H. S., Bagliesi, M. G., Bigongiari, G., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Lutz, L., Maestro, P., Malinin, A., Marrocchesi, P. S., Nam, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Wu, J., Yang, J., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The Cosmic Ray Energetics And Mass (CREAM) calorimeter is designed to measure the spectra of cosmic-ray particles over the energy range from ~10^11 eV to ~10^15 eV. Its first flight as part of the CREAM-I balloon-borne payload in Antarctica during the 2004/05 season resulted in a recordbreaking 42 days of exposure. Calorimeter calibration using various beam test data will be discussed in an attempt to assess the uncertainties of the energy measurements., Comment: Proc. 30th Int. Cosmic Ray Conf., Merida, 2, 421-424, 2007
- Published
- 2010
12. Beam test calibration of the balloon-borne imaging calorimeter for the CREAM experiment
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Marrocchesi, P. S., Ahn, H. S., Bagliesi, M. G., Basti, A., Bigongiari, G., Castellina, A., Ciocci, M. A., Di Virgilio, A., Lomtatze, T., Ganel, O., Kim, K. C., Lee, M. H., Ligabue, F., Lutz, L., Maestro, P., Malinine, A., Meucci, M., Millucci, V., Morsani, F., Seo, E. S., Sina, R., Wu, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
CREAM (Cosmic Ray Energetics And Mass) is a multi-flight balloon mission designed to collect direct data on the elemental composition and individual energy spectra of cosmic rays. Two instrument suites have been built to be flown alternately on a yearly base. The tungsten/Sci-Fi imaging calorimeter for the second flight, scheduled for December 2005, was calibrated with electron and proton beams at CERN. A calibration procedure based on the study of the longitudinal shower profile is described and preliminary results of the beam test are presented., Comment: This submission has been withdrawn by arXiv administrators because it is a duplicate of arXiv:physics/0507174
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- 2010
13. Energy spectra of cosmic-ray nuclei at high energies
- Author
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Ahn, H. S., Allison, P., Bagliesi, M. G., Barbier, L., Beatty, J. J., Bigongiari, G., Brandt, T. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Maestro, P., Malinine, A., Marrocchesi, P. S., Minnick, S., Mognet, S. I., Nam, S. W., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Walpole, P., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
We present new measurements of the energy spectra of cosmic-ray (CR) nuclei from the second flight of the balloon-borne experiment Cosmic Ray Energetics And Mass (CREAM). The instrument included different particle detectors to provide redundant charge identification and measure the energy of CRs up to several hundred TeV. The measured individual energy spectra of C, O, Ne, Mg, Si, and Fe are presented up to $\sim 10^{14}$ eV. The spectral shape looks nearly the same for these primary elements and it can be fitted to an $E^{-2.66 \pm 0.04}$ power law in energy. Moreover, a new measurement of the absolute intensity of nitrogen in the 100-800 GeV/$n$ energy range with smaller errors than previous observations, clearly indicates a hardening of the spectrum at high energy. The relative abundance of N/O at the top of the atmosphere is measured to be $0.080 \pm 0.025 $(stat.)$ \pm 0.025 $(sys.) at $\sim $800 GeV/$n$, in good agreement with a recent result from the first CREAM flight., Comment: 32 pages, 10 figures. Accepted for publication in Astrophysical Journal
- Published
- 2009
- Full Text
- View/download PDF
14. Changes in periapical status of root canal-treated teeth after head and neck IMRT: a retrospective study
- Author
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Steiner, Sina R., primary, Saccardin, Fabio, additional, Connert, Thomas, additional, and Filippi, Andreas, additional
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- 2023
- Full Text
- View/download PDF
15. Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment
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Ahn, H. S., Allison, P. S., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P. J., Brandt, T. J., Childers, J. T., Conklin, N. B., Coutu, S., Duvernois, M. A., Ganel, O., Han, J. H., Hyun, H. J., Jeon, J. A., Kim, K. C., Lee, J. K., Lee, M. H., Lutz, L., Maestro, P., Malinin, A., Marrocchesi, P. S., Minnick, S. A., Mognet, S. I., Nam, S., Nutter, S. L., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Swordy, S. P., Wakely, S. P., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
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Astrophysics - Abstract
We present new measurements of heavy cosmic-ray nuclei at high energies per- formed during the first flight of the balloon-borne cosmic-ray experiment CREAM (Cosmic-Ray Energetics And Mass). This instrument uses multiple charge detectors and a transition radiation detector to provide the first high accuracy measurements of the relative abundances of elements from boron to oxygen up to energies around 1 TeV/n. The data agree with previous measurements at lower energies and show a relatively steep decline (~E$^-0.6$ to E$^-0.5$) at high energies. They further show the source abundance of nitrogen relative to oxygen is ~10% in the TeV/n region., Comment: Accepted for publication in Astroparticle Physics
- Published
- 2008
- Full Text
- View/download PDF
16. Beam test calibration of the balloon-borne imaging calorimeter for the CREAM experiment
- Author
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Marrocchesi, P. S., Ahn, H. S., Bagliesi, M. G., Basti, A., Bigongiari, G., Castellina, A., Ciocci, M. A., Di Virgilio, A., Lomtatze, T., Ganel, O., Kim, K. C., Lee, M. H., Ligabue, F., Lutz, L., Maestro, P., Malinine, A., Meucci, M., Millucci, V., Morsani, F., Seo, E. S., Sina, R., Wu, J., Yoon, Y. S., Zei, R., and Zinn, S. -Y.
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Physics - Instrumentation and Detectors - Abstract
CREAM (Cosmic Ray Energetics And Mass) is a multi-flight balloon mission designed to collect direct data on the elemental composition and individual energy spectra of cosmic rays. Two instrument suites have been built to be flown alternately on a yearly base. The tungsten/Sci-Fi imaging calorimeter for the second flight, scheduled for December 2005, was calibrated with electron and proton beams at CERN. A calibration procedure based on the study of the longitudinal shower profile is described and preliminary results of the beam test are presented., Comment: 4 pages, 4 figures. To be published in the Proceedings of 29th International Cosmic Ray Conference (ICRC 2005), Pune, India, August 3-10, 2005
- Published
- 2005
17. Subacute cognitive impairment in B12 vitamin-deficiency neuromyelopathy secondary to nitrous oxide abuse
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Timour Vitte, Anna Castrioto, Emmanuelle Schmitt, Elena Moro, and Sina R. Potel
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Psychiatry and Mental health ,Neurology (clinical) ,Dermatology ,General Medicine - Published
- 2023
18. Advances in DBS Technology and Novel Applications: Focus on Movement Disorders
- Author
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Sina R, Potel, Sara, Marceglia, Sara, Meoni, Suneil K, Kalia, Rubens G, Cury, Elena, Moro, Potel, Sina R, Marceglia, Sara, Meoni, Sara, Kalia, Suneil K, Cury, Rubens G, and Moro, Elena
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Technology ,Neuromodulation ,General Neuroscience ,Parkinson Disease ,Technological advances ,Dystonia ,Tremor ,Basal ganglia ,Deep brain stimulation ,Movement disorders ,Parkinson’s disease ,Humans ,Neurology (clinical) ,Movement disorder - Abstract
Purpose of Review Deep brain stimulation (DBS) is an established treatment in several movement disorders, including Parkinson's disease, dystonia, tremor, and Tourette syndrome. In this review, we will review and discuss the most recent findings including but not limited to clinical evidence. Recent Findings New DBS technologies include novel hardware design (electrodes, cables, implanted pulse generators) enabling new stimulation patterns and adaptive DBS which delivers potential stimulation tailored to moment-to-moment changes in the patient's condition. Better understanding of movement disorders pathophysiology and functional anatomy has been pivotal for studying the effects of DBS on the mesencephalic locomotor region, the nucleus basalis of Meynert, the substantia nigra, and the spinal cord. Eventually, neurosurgical practice has improved with more accurate target visualization or combined targeting. A rising research domain emphasizes bridging neuromodulation and neuroprotection. Recent advances in DBS therapy bring more possibilities to effectively treat people with movement disorders. Future research would focus on improving adaptive DBS, leading more clinical trials on novel targets, and exploring neuromodulation effects on neuroprotection.
- Published
- 2022
19. METAFISICA CARTESIANA E TEOLOGIA NELL'EPISTOLARIO DI JEAN LE CLERC
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Sina, Mario and SINA, R.
- Published
- 2001
20. The Cosmic Ray Energetics and Mass (CREAM) timing charge detector
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Ahn, H.S., Allison, P.S., Bagliesi, M.G., Beatty, J.J., Bigongiari, G., Boyle, P., Childers, J.T., Conklin, N.B., Coutu, S., DuVernois, M.A., Ganel, O., Han, J.H., Jeon, J.A., Kim, K.C., Lee, J.K., Lee, M.H., Lutz, L., Maestro, P., Malinin, A., Marrocchesi, P.S., Minnick, S.A., Mognet, S.I., Nam, S.W., Nutter, S.L., Park, I.H., Park, N.H., Seo, E.S., Sina, R., Swordy, S.P., Wakely, S.P., Wu, J., Yang, J., Yoon, Y.S., Zei, R., and Zinn, S.Y.
- Published
- 2009
- Full Text
- View/download PDF
21. Estimating Blood Phenotype Probabilities and Their Products
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Greenwood, Sina R. and Seber, G. A. F.
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- 1992
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22. Approaching the Knee with Direct Measurements
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Seo, E.S., Ahn, H.S., Allison, P., Bagliesi, M.G., Barbier, L., Barrau, A., Bazer-Bachi, R., Beatty, J.J., Bigongiari, G., Boyle, P., Brandt, T.T., Buénerd, M., Childers, J.T., Conklin, N.B., Coutu, S., Derome, L., DuVernois, M.A., Ganel, O., Han, J.H., Jeon, J.A., Kim, K.C., Lee, M.H., Lutz, L., Malinin, A., Mangin-Brinet, M., Marrocchesi, P.S., Maestro, P., Menchaca-Rocha, A., Minnick, S., Mognet, S.I., Nam, S.W., Nutter, S., Park, I.H., Park, N.H., Putze, A., Sallaz-Damaz, Y., Sina, R., Swordy, S., Wakely, S., Walpole, P., Wu, J., Yang, J., Yoon, Y.S., Zei, R., and Zinn, S.Y.
- Published
- 2008
- Full Text
- View/download PDF
23. CREAM: 70 days of flight from 2 launches in Antarctica
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Seo, E.S., Ahn, H.S., Allison, P., Bagliesi, M.G., Barbier, L., Barrau, A., Bazer-Bachi, R., Beatty, J.J., Bigongiari, G., Boyle, P., Brandt, T.J., Buénerd, M., Childers, J.T., Conklin, N.B., Coutu, S., Derome, L., DuVernois, M.A., Ganel, O., Han, J.H., Jeon, J.A., Kim, K.C., Lee, M.H., Lutz, L., Malinin, A., Mangin-Brinet, M., Marrocchesi, P.S., Maestro, P., Menchaca-Rocha, A., Minnick, S., Mognet, S.I., Nam, S., Nutter, S., Park, I.H., Park, N.H., Putze, A., Sina, R., Swordy, S., Wakely, S., Walpole, P., Wu, J., Yang, J., Yoon, Y.S., Zei, R., and Zinn, S.Y.
- Published
- 2008
- Full Text
- View/download PDF
24. NMR resonance assignments of an engineered neomycin-sensing riboswitch RNA bound to ribostamycin and tobramycin
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Schmidtke, Sina R., Duchardt-Ferner, Elke, Weigand, Julia E., Suess, Beatrix, and Wöhnert, Jens
- Published
- 2010
- Full Text
- View/download PDF
25. CREAM-Pushing the high energy frontier of directly measured cosmic rays
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Ganel, O., Ahn, H. S., Allison, P., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P., Childers, J. T., Conklin, N. B., Coutu, S., Duvernois, M. A., Han, J. H., Hyun, H. J., Jeon, J. A., Kim, K. C., Lee, J. K., Lee, M. H., Lutz, L., Maestro, P., Malinin, A., Marrocchesi, P. S., Minnick, S., Mognet, S. I., Nam, S. W., Nutter, S., Park, H., Park, I. H., Park, N. H., Seo, E. S., Swordy, S., Sina, R., Wakely, S., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
- Published
- 2006
- Full Text
- View/download PDF
26. Performance of a dual layer silicon charge detector during CREAM balloon flight
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Nam, S., Ahn, H.S., Allison, P., Bagliesi, M.G., Barbier, L., Beatty, J.J., Bigongiari, G., Brandt, T.J., Jeon, J.A., Childers, J.T., Conklin, N.B., Coutu, S., DuVernois, M.A., Ganel, O., Han, J.H., Kim, K.C., Lee, M.H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P.S., Minnick, S., Zinn, S.Y., Mognet, S.I., Nutter, S., Park, I.H., Park, N.H., Seo, E.S., Sina, R., Walpole, P., Wu, J., Yang, J., Yoon, Y.S., and Zei, R.
- Subjects
Cosmic rays -- Properties ,Silicon compounds -- Properties ,Business ,Electronics ,Electronics and electrical industries - Abstract
The balloon-borne cosmic-ray experiment CREAM (Cosmic Ray Energetics And Mass) has completed two flights in Antarctica, with a combined duration of 70 days. One of the detectors in the payload is the SCD (Silicon Charge Detector) that measures the charge of high energy cosmic rays. The SCD was assembled with silicon sensors. A sensor is a 4 x 4 array of DC-coupled PIN diode pixels with the total active area of 21 x 16 [mm.sup.2]. The SCD used during the first flight (December 2004-January 2005) was a single layer device, then upgraded to a dual layer device for the second flight (December 2005-January 2006), covering the total sensitive area of 779 x 795 [mm.sup.2]. Flight data demonstrated that adding a second layer improved SCD performance, showing excellent particle charge resolution. With a total dissipation of 136 W for the dual layer system, special care was needed in designing thermal paths to keep the detector temperature within its operational range. As a consequence, flight temperatures of the SCD, even at diurnal maximum were kept below 38[degrees]C. The SCD mechanical structure was designed to minimize the possibility of damage to the sensors and electronics from the impacts of parachute deployment and landing. The detector was recovered successfully following the flight and is being refurbished for the next flight in 2007. Details of construction, operation, and performance are presented for the dual-layered SCD flown for the second CREAM flight. Index Terms--Balloon payload, charge measurement, cosmic rays, silicon sensors.
- Published
- 2007
27. The Cosmic Ray Energetics And Mass (CREAM) instrument
- Author
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Ahn, H.S., Allison, P., Bagliesi, M.G., Beatty, J.J., Bigongiari, G., Boyle, P., Childers, J.T., Conklin, N.B., Coutu, S., DuVernois, M.A., Ganel, O., Han, J.H., Jeon, J.A., Kim, K.C., Lee, J.K., Lee, M.H., Lutz, L., Maestro, P., Malinin, A., Marrocchesi, P.S., Minnick, S.A., Mognet, S.I., Nam, S.W., Nutter, S.L., Park, I.H., Park, N.H., Seo, E.S., Sina, R., Swordy, S.P., Wakely, S.P., Wu, J., Yang, J., Yoon, Y.S., Zei, R., and Zinn, S.Y.
- Published
- 2007
- Full Text
- View/download PDF
28. Design and performance in the first flight of the transition radiation detector and charge detector of the CREAM balloon instrument
- Author
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Coutu, S., Ahn, H.S., Allison, P., Bagliesi, M.G., Beatty, J.J., Bigongiari, G., Boyle, P., Brandt, T.J., Childers, J.T., Conklin, N.B., DuVernois, M.A., Ganel, O., Han, J.H., Hyun, H.J., Jeon, J.A., Kim, K., Lee, J.K., Lee, M.H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P.S., Minnick, S., Mognet, S.I., Nutter, S., Park, N.H., Park, H., Park, I.H., Seo, E.S., Sina, R., Swordy, S., Wakely, S.P., Wu, J., Yang, J., Yoon, Y.S., Zei, R., and Zinn, S.
- Published
- 2007
- Full Text
- View/download PDF
29. Silicon charge detector for the CREAM experiment
- Author
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Park, I.H., Park, N.H., Nam, S.W., Ahn, H.S., Allison, P., Bagliesi, M.G., Baek, S.J., Beatty, J.J., Bigongiari, G., Boyle, P., Childers, J.T., Conkin, N.B., Coutu, S., DuVernois, M.A., Ganel, O., Han, J.H., Hyun, H.J., Jeon, J.A., Kim, K.C., Lee, M.H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P.S., Minnick, S., Mognet, S.I., Nutter, S., Park, J.H., Seo, E.S., Sina, R., Swordy, S., Wakely, S., Wu, J., Yang, J., Yoon, Y.S., Zei, R., and Zinn, S.Y.
- Published
- 2007
- Full Text
- View/download PDF
30. Performance of CREAM Calorimeter: Results of Beam Tests
- Author
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Ahn, H.S., Bagliesi, M.G., Beatty, J.J., Bigongiari, G., Castellina, A., Childers, J.T., Conklin, N.B., Coutu, S., DuVernois, M.A., Ganel, O., Han, J.H., Hyun, H.J., Kang, T.G., Kim, H.J., Kim, K.C., Kim, M.Y., Kim, T., Kim, Y.J., Lee, J.K., Lee, M.H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P.S., Mognet, S.I., Nam, S.W., Nutter, S., Park, N.H., Park, H., Park, I.H., Seo, E.S., Sina, R., Syed, S., Song, C., Swordy, S., Wu, J., Yang, J., Zhang, H.Q., Zei, R., and Zinn, S.Y.
- Published
- 2006
- Full Text
- View/download PDF
31. Beam tests of the balloon-borne ATIC experiment
- Author
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Ganel, O., Adams, J.H., Jr., Ahn, H.S., Ampe, J., Bashindzhagyan, G., Case, G., Chang, J., Ellison, S., Fazely, A., Gould, R., Granger, D., Gunasingha, R., Guzik, T.G., Han, Y.J., Isbert, J., Kim, H.J., Kim, K.C., Kim, S.K., Kwon, Y., Panasyuk, M., Panov, A., Price, B., Samsonov, G., Schmidt, W.K.H., Sen, M., Seo, E.S., Sina, R., Sokolskaya, N., Stewart, M., Voronin, A., Wagner, D., Wang, J.Z., Wefel, J.P., Wu, J., and Zatsepin, V.
- Published
- 2005
- Full Text
- View/download PDF
32. Cosmic-ray energetics and mass (CREAM) balloon project
- Author
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Seo, E.S., Ahn, H.S., Beatty, J.J., Coutu, S., Choi, M.J., DuVernois, M.A., Ganel, O., Kang, T.G., Kim, K.C., Lee, M.H., Lutz, L., Marrocchesi, P.S., Minnick, S., Min, K.W., Nutter, S., Park, H., Park, I.H., Schindhelm, E., Sina, R., Swordy, S., Wu, J., and Yang, J.
- Published
- 2004
- Full Text
- View/download PDF
33. The ATIC long duration balloon project
- Author
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Guzik, T.G., Adams, J.H., Ahn, H.S., Bashindzhagyan, G., Chang, J., Christl, M., Fazely, A.R., Ganel, O., Granger, D., Gunasingha, R., Han, Y.J., Isbert, J.B., Kim, H.J., Kim, K.C., Kim, S.K., Kouznetsov, E., Panasyuk, M., Panov, A., Price, B., Samsonov, G., Schmidt, W.K.H., Seo, E.S., Sina, R., Sokolskaya, N., Stewart, M., Voronin, A., Wang, J.Z., Wefel, J.P., Wu, J., and Zatsepin, V.
- Published
- 2004
- Full Text
- View/download PDF
34. Advanced Thin Ionization Calorimeter (ATIC) Update
- Author
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Ahn, H. S, Ganel, O, Kim, K. C, Seo, E. S, Sina, R, Wang, J. Z, Wu, J, Case, G, Ellison, S. B, Gould, R, and Six, N. Frank
- Subjects
Space Radiation - Abstract
The Advanced Thin Ionization Calorimeter (ATIC) experiment is designed to measure the composition and energy spectra of Z = 1 to 28 cosmic rays over the energy range of approximately 10 GeV - 100 TeV. ATIC is comprised of an eight-layer, 18 radiation length deep Bismuth Germanate (BGO) calorimeter, downstream of a 0.75 nuclear interaction length graphite target and an approximately 1 sq m finely segmented silicon charge detector. Interleaved with the graphite layers are three scintillator strip hodoscopes for pre-triggering and tracking. ATIC flew for the first time on a Long Duration Balloon (LDB) launched from McMurdo, Antarctica in January 2001. During its 16-day flight ATIC collected more than 30 million science events, along with housekeeping, calibration, and rate data. This presentation will describe the ATIC data processing, including calibration and efficiency corrections, and show results from analysis of this dataset. The next launch is planned for December 2002.
- Published
- 2002
35. What a Difference an OH Makes: Conformational Dynamics as the Basis for the Ligand Specificity of the Neomycin-Sensing Riboswitch
- Author
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Christian Hammann, Elke Duchardt-Ferner, Jens Wöhnert, Sina R. Gottstein-Schmidtke, Julia E. Weigand, Jan-Philip Wurm, Beatrix Suess, and Oliver Ohlenschläger
- Subjects
Models, Molecular ,0301 basic medicine ,Riboswitch ,Hydroxyl Radical ,Stereochemistry ,Ligand ,Chemistry ,Intermolecular force ,RNA ,Neomycin ,General Chemistry ,Ligands ,Catalysis ,03 medical and health sciences ,030104 developmental biology ,Structural biology ,Cobalamin riboswitch ,Intramolecular force ,medicine ,medicine.drug - Abstract
To ensure appropriate metabolic regulation, riboswitches must discriminate efficiently between their target ligands and chemically similar molecules that are also present in the cell. A remarkable example of efficient ligand discrimination is a synthetic neomycin-sensing riboswitch. Paromomycin, which differs from neomycin only by the substitution of a single amino group with a hydroxy group, also binds but does not flip the riboswitch. Interestingly, the solution structures of the two riboswitch-ligand complexes are virtually identical. In this work, we demonstrate that the local loss of key intermolecular interactions at the substitution site is translated through a defined network of intramolecular interactions into global changes in RNA conformational dynamics. The remarkable specificity of this riboswitch is thus based on structural dynamics rather than static structural differences. In this respect, the neomycin riboswitch is a model for many of its natural counterparts.
- Published
- 2015
36. Eine OH-Gruppe ändert alles: konformative Dynamik als Grundlage für die Ligandenspezifität des Neomycin-bindenden RNA-Schalters
- Author
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Beatrix Suess, Christian Hammann, Jan-Philip Wurm, Jens Wöhnert, Julia E. Weigand, Oliver Ohlenschläger, Sina R. Gottstein-Schmidtke, and Elke Duchardt-Ferner
- Subjects
0301 basic medicine ,03 medical and health sciences ,030104 developmental biology ,Chemistry ,General Medicine - Published
- 2015
37. First results from ATIC beam-test at CERN
- Author
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Ganel, O., Adams, J.H., Jr, Ahn, E.J., Ahn, H.S., Ampe, J., Bashindzhagyan, G., Case, G., Chang, J., Ellison, S., Fazely, A., Gould, R., Granger, D., Gunasingha, R., Guzik, T.G., Han, Y.J., Isbert, J., Kara, T., Kim, H.J., Kim, K.C., Kim, S.K., Kwon, Y., Lemczyk, T., Oubre, C., Panasyuk, M., Price, B., Samsonov, G., Schmidt, W.K.H., Sen, M., Seo, E.S., Sina, R., Sokolskaya, N., Stewart, M., Toptygin, A., Voronin, A., Wagner, D., Wang, J.Z., Wefel, J.P., Wu, J., Zatsepin, V., and Zigura, A.
- Published
- 2001
- Full Text
- View/download PDF
38. Antiproton spectrum in the galactic wind model
- Author
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Sina, R., Ptuskin, V.S., and Seo, E.S.
- Published
- 2001
- Full Text
- View/download PDF
39. Sequence Elements Distal to the Ligand Binding Pocket Modulate the Efficiency of a Synthetic Riboswitch
- Author
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Sina R. Gottstein-Schmidtke, Florian Groher, Elke Duchardt-Ferner, Jens Wöhnert, Beatrix Suess, Julia E. Weigand, and Shemsi Demolli
- Subjects
Models, Molecular ,Riboswitch ,Binding Sites ,Aptamer ,Organic Chemistry ,Mutant ,RNA ,Neomycin ,Aptamers, Nucleotide ,Biology ,Ligands ,Stem-loop ,Biochemistry ,Molecular biology ,Terminal loop ,Synthetic biology ,Cobalamin riboswitch ,Mutation ,Biophysics ,Molecular Medicine ,Molecular Biology - Abstract
Synthetic riboswitches can serve as sophisticated genetic control devices in synthetic biology, regulating gene expression through direct RNA-ligand interactions. We analyzed a synthetic neomycin riboswitch, which folds into a stem loop structure with an internal loop important for ligand binding and regulation. It is closed by a terminal hexaloop containing a U-turn and a looped-out adenine. We investigated the relationship between sequence, structure, and biological activity in the terminal loop by saturating mutagenesis, ITC, and NMR. Mutants corresponding to the canonical U-turn fold retained biological activity. An improvement of stacking interactions in the U-turn led to an RNA element with slightly enhanced regulatory activity. For the first position of the U-turn motif and the looped out base, sequence-activity relationships that could not initially be explained on the basis of the structure of the aptamer-ligand complex were observed. However, NMR studies of these mutants revealed subtle relationships between structure and dynamics of the aptamer in its free or bound state and biological activity.
- Published
- 2014
40. How well can a cosmic-ray spectral kink be measured?
- Author
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Sina, R. and Seo, E.S.
- Published
- 2000
- Full Text
- View/download PDF
41. Hochmodulare Struktur und Ligandenbindung durch 'Conformational Capture' in einem minimalistischen RNA-Schalter
- Author
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Oliver Ohlenschläger, Sina R. Schmidtke, Julia E. Weigand, Elke Duchardt-Ferner, Jens Wöhnert, and Beatrix Suess
- Subjects
Chemistry ,Aminoglycoside ,RNA ,General Medicine ,Molecular biology - Published
- 2010
42. Building a stable RNA U-turn with a protonated cytidine
- Author
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Julia E. Weigand, Beatrix Suess, Florian Groher, Daniel Gottstein, Sina R. Gottstein-Schmidtke, Elke Duchardt-Ferner, and Jens Wöhnert
- Subjects
Riboswitch ,Models, Molecular ,Stereochemistry ,Cytidine ,Biology ,Phosphates ,chemistry.chemical_compound ,Report ,ddc:570 ,Nucleotide ,Nucleic acid structure ,Nucleotide Motifs ,Structural motif ,Molecular Biology ,Nuclear Magnetic Resonance, Biomolecular ,Uridine ,chemistry.chemical_classification ,Base Sequence ,Hydrogen bond ,RNA ,Hydrogen Bonding ,chemistry ,Biochemistry ,Transfer RNA ,Nucleic Acid Conformation - Abstract
The U-turn is a classical three-dimensional RNA folding motif first identified in the anticodon and T-loops of tRNAs. It also occurs frequently as a building block in other functional RNA structures in many different sequence and structural contexts. U-turns induce sharp changes in the direction of the RNA backbone and often conform to the 3-nt consensus sequence 5′-UNR-3′ (N = any nucleotide, R = purine). The canonical U-turn motif is stabilized by a hydrogen bond between the N3 imino group of the U residue and the 3′ phosphate group of the R residue as well as a hydrogen bond between the 2′-hydroxyl group of the uridine and the N7 nitrogen of the R residue. Here, we demonstrate that a protonated cytidine can functionally and structurally replace the uridine at the first position of the canonical U-turn motif in the apical loop of the neomycin riboswitch. Using NMR spectroscopy, we directly show that the N3 imino group of the protonated cytidine forms a hydrogen bond with the backbone phosphate 3′ from the third nucleotide of the U-turn analogously to the imino group of the uridine in the canonical motif. In addition, we compare the stability of the hydrogen bonds in the mutant U-turn motif to the wild type and describe the NMR signature of the C+-phosphate interaction. Our results have implications for the prediction of RNA structural motifs and suggest simple approaches for the experimental identification of hydrogen bonds between protonated C-imino groups and the phosphate backbone.
- Published
- 2014
43. Eine OH-Gruppe ändert alles: konformative Dynamik als Grundlage für die Ligandenspezifität des Neomycin-bindenden RNA-Schalters
- Author
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Duchardt-Ferner, Elke, primary, Gottstein-Schmidtke, Sina R., additional, Weigand, Julia E., additional, Ohlenschläger, Oliver, additional, Wurm, Jan-Philip, additional, Hammann, Christian, additional, Suess, Beatrix, additional, and Wöhnert, Jens, additional
- Published
- 2015
- Full Text
- View/download PDF
44. What a Difference an OH Makes: Conformational Dynamics as the Basis for the Ligand Specificity of the Neomycin‐Sensing Riboswitch
- Author
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Duchardt‐Ferner, Elke, primary, Gottstein‐Schmidtke, Sina R., additional, Weigand, Julia E., additional, Ohlenschläger, Oliver, additional, Wurm, Jan‐Philip, additional, Hammann, Christian, additional, Suess, Beatrix, additional, and Wöhnert, Jens, additional
- Published
- 2015
- Full Text
- View/download PDF
45. Insights Into the Dynamic Personalities of Synthetic Riboswitches by NMR-Spectroscopy
- Author
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Elke Duchardt-Ferner, Julia E. Weigand, Jens Woehnert, Amir H. Nasiri, Sina R. Schmidtke, and Beatrix Suess
- Subjects
Riboswitch ,Novel gene ,Stereochemistry ,Biophysics ,Nuclear magnetic resonance spectroscopy ,Computational biology ,Biology ,Ligand (biochemistry) ,Small molecule ,Function (biology) ,Protein tertiary structure - Abstract
Riboswitches are novel gene regulatory elements found in the 5′- and 3′-untranslated regions of mRNAs. They regulate gene expression upon direct and specific interaction with small molecule ligands. In most riboswitches ligand binding triggers conformational changes on the secondary and/or tertiary structure level which result in changes in gene expression levels. While a lot is known about the structural basis for ligand recognition by riboswitch domains the conformational dynamics of riboswitches which are central to their function is less explored. NMR-spectroscopy in solution is well suited for investigating dynamical systems and for characterising conformational changes. We applied NMR-spectroscopy to two smaller synthetic riboswitches to characterize in detail their conformational dynamics in relation to their regulatory functions.
- Published
- 2011
- Full Text
- View/download PDF
46. Mechanistic insights into an engineered riboswitch: a switching element which confers riboswitch activity
- Author
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Tristan J. Will, Christian Hammann, Sina R. Schmidtke, Beatrix Suess, Jens Wöhnert, Elke Duchardt-Ferner, and Julia E. Weigand
- Subjects
chemistry.chemical_classification ,Riboswitch ,Aptamer ,RNA ,Neomycin ,Biology ,Aptamers, Nucleotide ,Ligand (biochemistry) ,Ligands ,Small molecule ,Biochemistry ,chemistry ,Cobalamin riboswitch ,ddc:570 ,Genetics ,Biophysics ,Molecule ,Thermodynamics ,Nucleotide ,Genetic Engineering - Abstract
While many different RNA aptamers have been identified that bind to a plethora of small molecules only very few are capable of acting as engineered riboswitches. Even for aptamers binding the same ligand large differences in their regulatory potential were observed. We address here the molecular basis for these differences by using a set of unrelated neomycin-binding aptamers. UV melting analyses showed that regulating aptamers are thermally stabilized to a significantly higher degree upon ligand binding than inactive ones. Regulating aptamers show high ligand-binding affinity in the low nanomolar range which is necessary but not sufficient for regulation. NMR data showed that a destabilized, open ground state accompanied by extensive structural changes upon ligand binding is important for regulation. In contrast, inactive aptamers are already pre-formed in the absence of the ligand. By a combination of genetic, biochemical and structural analyses, we identified a switching element responsible for destabilizing the ligand free state without compromising the bound form. Our results explain for the first time the molecular mechanism of an engineered riboswitch.
- Published
- 2010
47. Highly modular structure and ligand binding by conformational capture in a minimalistic riboswitch
- Author
-
Beatrix Suess, Jens Wöhnert, Sina R. Schmidtke, Julia E. Weigand, Elke Duchardt-Ferner, and Oliver Ohlenschläger
- Subjects
Riboswitch ,Ribostamycin ,Magnetic Resonance Spectroscopy ,Base pair ,Stereochemistry ,Chemistry ,Aptamer ,Temperature ,RNA ,General Chemistry ,Ligand (biochemistry) ,Ligands ,Catalysis ,Biochemistry ,Cobalamin riboswitch ,medicine ,Nucleic Acid Conformation ,Protein secondary structure ,medicine.drug - Abstract
Riboswitches are highly structured RNA motifs with gene regulatory activity located in the untranslated regions of mRNAs. They either modulate transcription termination or translation initiation through conformational changes triggered by direct interactions with small metabolite ligands. Many naturally occurring riboswitches are large and structurally very complex. In contrast, synthetic riboswitches—tailored gene regulatory elements for synthetic biology applications—are based on small in vitro selected RNA aptamers. Yet, despite a ligand affinity and specificity comparable to their natural counterparts only a few in vitro selected aptamers are regulatory active in vivo. Recently, Suess et al. engineered a riboswitch for the aminoglycoside antibiotic neomycin B by subjecting an in vitro SELEX-pool to an in vivo screening for gene regulatory activity in a yeastbased reporter gene assay. The resulting neomycin B and ribostamycin (Figure 1a) responsive RNA-element (N1) contains only 27 nucleotides in a bulged hairpin secondary structure (Figure 1b)—the smallest riboswitch functional in vivo identified to date. In sequence and secondary structure, N1 differs completely from an in vitro selected but regulatory inactive RNA-aptamer for the same ligand (R23). Instead it partially resembles the ribosomal A-site, the natural target for aminoglycoside antibiotics (Figure 1b). The NMR spectroscopic analysis of the N1 riboswitch complexed with ribostamycin identifies structural determinants for its regulatory activity and suggests a ligand binding mechanism based on conformational capture. Our results provide insights into the modularity of ligand binding sites in RNA and highlight structural and dynamic features N1 shares with the larger naturally occurring riboswitches as well as with other regulatory active aptamers. This knowledge may guide the future design of novel synthetic riboswitches for targeted in vivo applications. Structure of the N1–ligand complex—the “OFF”-state of the riboswitch: N1 represses gene expression upon binding to either neomycin B or the closely related but smaller ribostamycin. NMR spectra of N1 bound to either ligand (Supporting Information Figure S1) indicate that both complexes are formed with similarly high affinity and display a high degree of structural similarity suggesting that the contribution of ring IV of neomycin to the interaction is negligible. Thus, we determined the structure of the N1–ribostamycin complex, because of its superior spectral resolution for the ligand resonances, by NMR spectroscopy (see Table 1). Chemical shift assignments and coordinates have been deposited (BMRB code: 16609, pdb-code: 2kxm). The structure of ribostamycin-bound N1 consists of a continuous helical stem with canonical stacking interactions between the G5:C23 and the G9:C22 base pair despite the presence of a flexible three-nucleotide bulge (C6–U8) and a compactly folded apical hexaloop organized around a U-turn motif (U14–A16) closed by the U13:U18 base pair (Figure 1c–e). Ribostamycin rings I and II are sandwiched between the N1 major groove, in the region from G5:C23 to U13:U18 and A17 protruding from the apical loop (Figure 2). Ring III is located close to the backbone of the 3’-strand (U18 to G20). Simultaneous contacts of the ligand with the G5:C23 base pair below and G9:C22 above the bulge (Figure 2b) clamp together the lower and upper helical stem and thus enforce the uninterrupted coaxial helical stacking across the flexible C6–U8 internal bulge. The bulge itself is not interacting with the ligand. A detailed structural description of the N1– ribostamycin complex is given in the Supporting Information. A comparison of the N1–ribostamycin complex with other aminoglycoside binding RNAs reveals partial similarities to known aminoglycoside binding sub-motifs: The helical stem centered at the U10:U21 base pair is similar to the ribosomal [*] Dr. E. Duchardt-Ferner, S. R. Schmidtke, Prof. Dr. J. W hnert Institute for Molecular Biosciences, Center for Biomolecular Magnetic Resonance (BMRZ), Johann-Wolfgang-Goethe-University Frankfurt Max-von-Laue-Strasse 9, 60438 Frankfurt (Germany) Fax: (+49)69-798-29527 E-mail: woehnert@bio.uni-frankfurt.de
- Published
- 2010
48. NMR resonance assignments of an engineered neomycin-sensing riboswitch RNA bound to ribostamycin and tobramycin
- Author
-
Beatrix Suess, Julia E. Weigand, Jens Wöhnert, Elke Duchardt-Ferner, and Sina R. Schmidtke
- Subjects
Riboswitch ,Saccharomyces cerevisiae ,Biology ,Regulatory Sequences, Ribonucleic Acid ,Protein Engineering ,Biochemistry ,Ribostamycin ,Structural Biology ,Gene expression ,medicine ,Triple-resonance nuclear magnetic resonance spectroscopy ,RNA, Messenger ,Nuclear Magnetic Resonance, Biomolecular ,Carbon Isotopes ,Nitrogen Isotopes ,Aminoglycoside ,RNA ,Phosphorus Isotopes ,RNA, Fungal ,Neomycin ,Cobalamin riboswitch ,Tobramycin ,medicine.drug ,Hydrogen - Abstract
The neomycin-sensing riboswitch is an engineered riboswitch developed to regulate gene expression in vivo in the lower eukaryote Saccharomyces cerevisiae upon binding to neomycin B. With a size of only 27nt it is the smallest functional riboswitch element identified so far. It binds not only neomycin B but also related aminoglycosides of the 2'-deoxystreptamine class with high affinity. The regulatory activity, however, strongly depends on the identity of the aminoglycoside. As a prerequisite for the structure determination of riboswitch-ligand complexes we report here the (1)H, (15)N, (13)C and partial (31)P chemical shift assignments for the minimal functional 27nt neomycin sensing riboswitch RNA in complex with the 4,5-linked neomycin analog ribostamycin and the 4,6-linked aminoglycoside tobramycin.
- Published
- 2009
49. Measurements of cosmic-ray energy spectra with the second CREAM flight
- Author
-
Maestro, Paolo, Ahn, H. S., Allison, P., Bagliesi, MARIA GRAZIA, Barbier, L., Beatty, J. J., Bigongiari, Gabriele, Brandt, T. J., Childers, J. T., Conklin, N. B., Coutu, S., Duvernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Malinine, A., Marrocchesi, PIER SIMONE, Minnick, S., Mognet, S. I., Nam, S. W., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Walpole, P., Wu, J., Yang, J., Yoon, Y. S., Zei, Riccardo, and Zinn, S. Y.
- Subjects
Cosmic rays ,Direct detection - Published
- 2009
50. Elemental energy spectra of cosmic rays measured by CREAM-II
- Author
-
Maestro, P., Ahn, H. S., Allison, P., Bagliesi, M. G., Barbier, L., Beatty, J. J., Bigongiari, G., Brandt, T. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Malinine, A., Marrocchesi, P. S., Minnick, S., Mognet, S. I., Nam, S. W., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Walpole, P., Wu, J., Yang, J., Yoon, Y. S., Zei, R., and Zinn, S. Y.
- Subjects
High Energy Astrophysical Phenomena (astro-ph.HE) ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present new measurements of the energy spectra of cosmic-ray (CR) nuclei from the second flight of the balloon-borne experiment CREAM (Cosmic Ray Energetics And Mass). The instrument (CREAM-II) was comprised of detectors based on different techniques (Cherenkov light, specific ionization in scintillators and silicon sensors) to provide a redundant charge identification and a thin ionization calorimeter capable of measuring the energy of cosmic rays up to several hundreds of TeV. The data analysis is described and the individual energy spectra of C, O, Ne, Mg, Si and Fe are reported up to ~ 10^14 eV. The spectral shape looks nearly the same for all the primary elements and can be expressed as a power law in energy E^{-2.66+/-0.04}. The nitrogen absolute intensity in the energy range 100-800 GeV/n is also measured., Comment: 4 pages, 3 figures, presented at ICRC 2009, Lodz, Poland
- Published
- 2009
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