Bibliographies thématiques / Upper limits

Littérature scientifique sur le sujet « Upper limits »

Auteur : Grafiati

Publié le 11 mars 2023

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Articles de revues sur le sujet "Upper limits"

O'Brien, William D., John G. Abbott, Mel E. Stratmeyer, Gerald R. Harris, Mark E. Schafer, Tariq A. Siddiqi, Christopher R. B. Merritt, Francis A. Duck et Phillip J. Bendick. « Acoustic Output Upper Limits Proposition ». Journal of Ultrasound in Medicine 21, n^o 12 (décembre 2002) : 1335–41. http://dx.doi.org/10.7863/jum.2002.21.12.1335.

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Alexander, Andrew M., Shane M. Hammer, Kaylin D. Didier, Dryden R. Baumfalk, Joshua R. Smith et Thomas J. Barstow. « Upper Limits Of Exercise Tolerance ». Medicine & ; Science in Sports & ; Exercise 49, n^o 5S (mai 2017) : 611–12. http://dx.doi.org/10.1249/01.mss.0000518603.34535.a8.

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Matthews, H. E., P. A. Feldman et P. F. Bernath. « Upper limits to interstellar PO ». Astrophysical Journal 312 (janvier 1987) : 358. http://dx.doi.org/10.1086/164881.

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Matejdes, Milan. « Graph and pointwise upper Kuratowski limits ». Colloquium Mathematicum 147, n^o 2 (2017) : 195–201. http://dx.doi.org/10.4064/cm6686-6-2016.

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Astone, P., et G. Pizzella. « On upper limits for gravitational radiation ». Astroparticle Physics 16, n^o 4 (février 2002) : 441–50. http://dx.doi.org/10.1016/s0927-6505(01)00166-9.

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Parker, Timothy W., et Ronald W. Humble. « Theoretical upper limits on enthalpy rocket performance ». Journal of Propulsion and Power 12, n^o 2 (mars 1996) : 445–48. http://dx.doi.org/10.2514/3.24055.

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Kabaila, Paul, et Chris J. Lloyd. « Profile upper Confidence Limits from Discrete Data ». Australian New Zealand Journal of Statistics 42, n^o 1 (mars 2000) : 67–79. http://dx.doi.org/10.1111/1467-842x.00108.

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Kabaila, Paul, et Chris J. Lloyd. « TIGHT UPPER CONFIDENCE LIMITS FROM DISCRETE DATA ». Australian Journal of Statistics 39, n^o 2 (juin 1997) : 193–204. http://dx.doi.org/10.1111/j.1467-842x.1997.tb00535.x.

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Kashyap, Vinay L., David A. van Dyk, Alanna Connors, Peter E. Freeman, Aneta Siemiginowska, Jin Xu et Andreas Zezas. « ON COMPUTING UPPER LIMITS TO SOURCE INTENSITIES ». Astrophysical Journal 719, n^o 1 (23 juillet 2010) : 900–914. http://dx.doi.org/10.1088/0004-637x/719/1/900.

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Elgarøy, Øystein. « Upper limits on neutrino masses from cosmology ». Nuclear Physics B - Proceedings Supplements 168 (juin 2007) : 51–53. http://dx.doi.org/10.1016/j.nuclphysbps.2007.02.005.

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Thèses sur le sujet "Upper limits"

Moretti, Elena. « Upper Limits on High Energy emissions from GRB ». Doctoral thesis, Università degli studi di Trieste, 2010. http://hdl.handle.net/10077/3721.

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2008/2009
The intense and unpredictable flashes of gamma rays in the energy band (10 keV – 1 MeV), called Gamma-Ray Bursts (GRB), were discovered in the late 60's. Since then several experiments were dedicated to detect and understand these phenomena. Up to now, we do not have yet a complete explanation for the GRB progenitors and their emission mechanism. In the first phase, the so-called prompt phase, lasting from few ms to tens of seconds, these bursts emit mainly in the band from hard-X to soft gamma. In a longer second phase, called afterglow, the GRB emission ranges from the radio frequencies to the X-ray band. The hard gamma band (>50 MeV), both in the prompt and in the afterglow phase, was poorly explored until the gamma-ray experiment EGRET flown on the Compton Gamma-ray Observatory (CGRO). Nevertheless EGRET detected only 5 GRBs in the band >200 MeV in 7 years of operation. Nowadays 2 gamma-ray experiments AGILE and Fermi/LAT are currently in operation. The number of detected burst with emitted energy >50 MeV is already more than duplicated by these two missions. The two experiments are based on the same high energy gamma-ray detection technique so these two experiments are similar: their core is made of a silicon tracker with tungsten conversion layers, surrounded by a plastic scintillator to veto cosmic-ray particles events. Below the tracker, a calorimeter provides the measure of the energy of the produced pairs. The main differences between the experiments are the larger effective area of the Fermi/LAT (~10 times larger) and its deeper calorimeter. On board of the satellites that host LAT and AGILE there are other 2 experiments respectively: the Fermi/GBM dedicated to the GRB science in the 8 keV-40 MeV band and the SuperAGILE that is a X-ray detector operational in the 18-60 keV band. Fermi/GBM, SuperAGILE and the Mini Calorimeter in the AGILE mission can independently trigger on a burst event respectively in the energy band (8 keV – 40 MeV), (18-60 keV) and (0.3-100 MeV). Their FoV is quite different however, ranging from 2 sr for SuperAGILE to almost 4 sr for MiniCalorimeter and 6 sr for FermiGBM. If the burst, triggered by these instruments or by other missions, is in the field of view of one of the two gamma-ray detectors a high energy signal is searched. In the AGILE pipeline the GRB signal is searched in the burst prompt time interval. During this time interval both background and signal are supposed to follow a Poisson distribution and the signal to be non-negative. The background average rate is computed before the burst trigger, in the same signal extraction region (15deg from the GRB position), with the same analysis cuts and in a time interval at least 10 times longer than the signal duration. Instead in the Fermi/LAT pipeline a map of the test statistic variable is computed. The test statistic distribution indicates how much the data differ from the background model used. In this thesis the non-detection cases are considered: a methodology for the computation of the upper limit on the signal is proposed. This method is based on the Bayesian statistics and was elaborated from Helene in 1984 (Helene, O. 1984, Nuclear Instruments and Methods 228, 120), it considers a Poisson fluctuation of the known background mean and of the estimated signal in the region of interest. The applications of this upper limit computing method to the AGILE and the Fermi/LAT data are also showed deriving upper limit on GRB flux. The AGILE energy coverage is smaller but starts from lower energy with respect the actual Fermi/LAT energy band. In the AGILE energy range above 30 MeV and till 2 GeV, the estimated GRB flux upper limits range between 1x10-3 and 1x10-2 ph s-1cm-2. Instead the Fermi/LAT flux upper limit is roughly 5x10-5 ph s-1cm-2 in the energy range from 100 MeV to 100 GeV. The studies of the upper limits help to understand the GRB emission mechanisms: most of these bursts are not detected in the highest energy band even if the extrapolation of their spectra from the low energy band predicts a detectable flux from those two instruments. On the other case there are some GRBs with low energy spectra predicting a non detectable H.E. flux but with high energy photons clearly detected. These photons indicate the existence of a new component above 100 MeV in the GRB photon spectrum extending up to the GeV region. This thesis gives a new contribution on the computation of the upper limits on the GRB flux in both the gamma-ray experiments operating nowadays. The thesis will concentrate in particular on the study of the upper limits in the interesting cases, when a high energy signal is predicted but not detected, giving some interesting hints on the GRB source physics.
1982

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Livas, Jeffrey C. (Jeffrey Clark). « Upper limits for gravitational radiation from some astrophysical sources ». Thesis, Massachusetts Institute of Technology, 1987. https://hdl.handle.net/1721.1/123082.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1987.
Title as it appeared in Massachusetts Institute of Technology Graduate List: Upper limits on gravitational radiation from some astrophysical sources.
Bibliography: leaves 155-159.
by Jeffrey Clark Livas.
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1987.

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Ceccotti, Emilio. « Upper limits on the 21 cm power spectrum from the epoch of reionization ». Master's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/20004/.

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In this Thesis work, we analyse 21cm line observations taken with the Precision Array to Probe the Epoch of Reionization (PAPER) in the 120-180MHz range (6

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Sellerholm, Alexander. « Cosmological dark matter and the isotropic gamma-ray background measurements and upper limits / ». Doctoral thesis, Stockholm : Department of Physics, Stockholm University, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-38900.

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Macdonald, Erin Patricia. « From upper limits to detection : continuous gravitational waves in the advanced detector era ». Thesis, University of Glasgow, 2012. http://theses.gla.ac.uk/3608/.

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This thesis concerns continuous gravitational wave signals from non-axisymmetric neutron stars and ground-based interferometric detectors. These detectors are currently being upgraded and this thesis explores relevant issues and methods to prepare for the advanced detector era. A study into sensitivity dependence on the addition of a southern hemisphere detector for a targeted continuous wave search is first presented. Next, we study the effect of close and/or high velocity neutron stars on the ability of a blind, all-sky search to make a detection. Initial results from a narrowband search for signals from the Crab Pulsar and a blind hardware injected signal are then presented. Finally, we describe the development and initial implementation of a large-scale mock data challenge designed to test current continuous wave algorithms to explore various issues before we enter the advanced detector era.

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Sylvestre, Julien 1976. « Upper limits for galactic transient sources of gravitational radiation from LIGO first observations ». Thesis, Massachusetts Institute of Technology, 2002. http://hdl.handle.net/1721.1/29933.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2002.
Includes bibliographical references (leaves 147-151).
A complete, scalable prototype analysis system for the observation of gravitational wave bursts with a network of interferometric detectors is designed and tested. This system detects localized transients in the gravitational wave data streams from two independent detectors using a time-frequency algorithm, applies veto conditions on these transients based on auxiliary channels, and looks for significant coincidences between the surviving transients from the two detectors. The analysis system was optimized for setting rate upper limits on three populations of astronomical sources, using preliminary data from the LIGO Project (the E7 Engineering Run data). The three classes of sources were core collapses, bar-mode instabilities in neutron stars, and equal-mass black hole binary coalescences, and a 95% confidence rate upper limit of 2 per hour was set, for sources uniformly distributed within a distance of 6 pc, 950 pc, and 3.2 kpc from the Earth, respectively. A detailed discussion of the character of the noise in the data used to derive these limits shows that a network of interferometers including the instruments of the GEO, LIGO and VIRGO Projects should attain a 50% detection efficiency for these sources out to distances of 40 kpc, 1 Mpc and 40 Mpc, respectively, for a false alarm rate giving expected upper limits of 6, 0.6, and 2. 10-4 per year per galaxy, respectively, for a full year of observation.
by Julien Sylvestre.
Ph.D.

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Burton, Ross E. « Upper Limits on the Ultra-High Energy Cosmic Ray Flux from Unresolved Sources ». Case Western Reserve University School of Graduate Studies / OhioLINK, 2012. http://rave.ohiolink.edu/etdc/view?acc_num=case1323452264.

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Joshi, Kanchan A. « Upper thermal limits differ among component species in a host-parasitoid-hyperparasitoid system ». VCU Scholars Compass, 2016. http://scholarscompass.vcu.edu/etd/4454.

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Among the predicted impacts associated with global climate change, warming is of special interest because the rates of physiological processes are temperature-dependent. Insects and other ectotherms are likely to be affected due to their limited ability to control body temperature. In this study, I measured the tolerance to extreme high temperatures, i.e., critical thermal maximum (CTmax), of component species in a tri-trophic system, including an herbivore (Manduca sexta), a primary larval parasitoid (Cotesia congregata) and a hyperparasitoid (genus Silochalcis). For wild insects, the parasitoid had the lowest CTmax, the hyperparasitoid had the highest, and the herbivore was intermediate. For laboratory insects, the parasitoid had a lower CTmax than the herbivore. Results suggest that laboratory colonies can be used to predict relative thermal performance of interacting species in the field. Variations in tolerance to high temperature among component species could disrupt the outcome of interactions in multi-trophic systems.

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Flodin, Mikael. « Determining upper limits on galactic ETI civilizations transmitting continuous beacon signals in the radio spectrum ». Thesis, KTH, Fysik, 2019. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-266824.

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Csigi, Kálmán K. XIV. « UPPER THERMAL LIMITS VARY AMONG AND WITHIN NATIVE BEE SPECIES IN RELATION TO SEASON, VOLTINISM, AND NEST TYPE ». VCU Scholars Compass, 2019. https://scholarscompass.vcu.edu/etd/5864.

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Native bees are only recently gaining attention for the extent to which they aid in pollination and ecosystem services. These services are threatened by predictions of warming temperatures if bees are not able to respond. Voltinism - the number of generations produced annually- can strongly influence thermal conditions experienced by both developing and adult bees based on emergence strategies for each voltinism type. Differences in experienced thermal conditions brought on by climate change could therefore affect upper thermal limits (UTL) in bees. This study observes UTLs across a foraging season within and among native bee species vi to elucidate the potential response by bees to a warming climate. Bees were collected across the field season in Central Virginia and subjected to dynamic ramping trials to determine the fatal knockdown point (FKP). Results show in both univoltine and multivoltine bees an increase in upper thermal tolerance as the foraging season progresses (in quadratic and linear fashions respectively). Within multivoltine bees, FKP was related to nest type; with stem-nesting bees having the highest FKP. All average FKPs were higher than historic air temperatures of the study region, but within several degrees of the highest recorded maximum temperature. The diversity of responses in native bees provides evidence for both genetic and plastic responses to extreme temperature. While bees still face a potential myriad of other issues brought on by climate change, the observed increases in FKP across warming temperatures offer tentatively hopeful predictions for limited physiological responses in native bees to a warming climate

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Livres sur le sujet "Upper limits"

Dicken, John E. Medicaid outpatient prescription drugs : Estimated changes in federal upper limits using the formula under the Patient Protection and Affordable Care Act. Washington, DC : U.S. Govt. Accountability Office, 2010.

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Assembly, Canada Legislature Legislative. Bill : An act to grant certain powers to township councils in Upper Canada, with respect to wharves within the limits of their municipalities. Quebec : Hunter, Rose & Lemieux, 2003.

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Medicaid prescription drugs : CMS should implement revised federal upper limits and monitor their relationship to retail pharmacy acquisition costs : report to congressional requesters. [Washington, D.C.] : United States Government Accountability Office, 2013.

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Wieser, Gerhard, et Michael Tausz, dir. Trees at their Upper Limit. Dordrecht : Springer Netherlands, 2007. http://dx.doi.org/10.1007/1-4020-5074-7.

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United States. Congress. Senate. Committee on Finance. Upper payment limits : Federal Medicaid spending for non-Medicaid purposes : hearing before the Committee on Finance, United States Senate, One Hundred Sixth Congress, second session, September 6, 2000. Washington : U.S. G.P.O., 2001.

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Assembly, Canada Legislature Legislative. Bill : An act for better defining the limits of the counties and districts in Upper Canada, for erecting certain new townships, for detaching townships from some counties and attaching them to others, and for other purposes relative to the division of Upper Canada into townships, counties and districts. [Montréal] : Lovell and Gibson, 2002.

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1940-, Muzumdar Ashok, dir. Powered upper limb prostheses. Berlin : Springer, 2004.

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NACRO. The upper age limit of the juvenile court. London : NACRO, 1989.

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Ahrens, John. Approximate upper limit of irregular wave runup on riprap. Vicksburg, Miss : U.S. Army Engineer Waterways Experiment Station, 1988.

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Ahrens, John. Approximate upper limit of irregular wave runup on riprap. [Vicksburg, Miss : U.S. Army Engineer Waterways Experiment Station, 1988.

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Chapitres de livres sur le sujet "Upper limits"

Lista, Luca. « Upper Limits ». Dans Statistical Methods for Data Analysis in Particle Physics, 137–72. Cham : Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-20176-4_8.

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Lista, Luca. « Discoveries and Upper Limits ». Dans Statistical Methods for Data Analysis in Particle Physics, 205–49. Cham : Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-62840-0_10.

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Huo, Jiao, et Lishi Zhang. « Tolerable Upper Limits of Nutrients ». Dans Nutritional Toxicology, 205–41. Singapore : Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-0872-9_9.

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Chini, Rolf. « Upper Limits on the CMB Variation from 1300µm Observations ». Dans The Infrared and Submillimetre Sky after COBE, 385–90. Dordrecht : Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2448-5_21.

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Martinez-Gonzalez, E., J. I. Gonzalez-Serrano, J. L. Sanz, J. M. Martin-Mirones et L. Cayon. « Upper Limits on the LYα Emission aT Z = 3.4 ». Dans Examining the Big Bang and Diffuse Background Radiations, 497–98. Dordrecht : Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0145-2_59.

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Wyllie, Peter J. « Experimental Limits for Melting in the Earth's Crust and Upper Mantle ». Dans Geophysical Monograph Series, 279–301. Washington D. C. : American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm014p0279.

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Lago, M. T. V. T., M. V. Penston et R. M. Johnstone. « Upper limits to coronal emission from X-ray detected T Tauri stars ». Dans Nearby Molecular Clouds, 216–21. Berlin, Heidelberg : Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-15991-6_95.

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Ackermann, Markus. « Upper limits on neutrino fluxes from point-like sources with AMANDA-II ». Dans The Multi-Messenger Approach to High-Energy Gamma-Ray Sources, 421–27. Dordrecht : Springer Netherlands, 2007. http://dx.doi.org/10.1007/978-1-4020-6118-9_65.

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Beavis, Andrew D. « Upper and Lower Limits of Charge, Proton and ATP Stoichiometries of Oxidative Phosphorylation ». Dans Integration of Mitochondrial Function, 135–54. Boston, MA : Springer US, 1988. http://dx.doi.org/10.1007/978-1-4899-2551-0_13.

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Schreiber, Thomas, Ramona Eberhardt, Jens Limpert et Andreas Tünnermann. « High-Power Fiber Lasers and Amplifiers : Fundamentals and Enabling Technologies to Enter the Upper Limits ». Dans Fiber Lasers, 7–61. Weinheim, Germany : Wiley-VCH Verlag GmbH & Co. KGaA, 2012. http://dx.doi.org/10.1002/9783527648641.ch2.

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Actes de conférences sur le sujet "Upper limits"

Bojahr, H. « Upper limits on low redshift AGN ». Dans GeV-TeV gamma ray astrophysics workshop. AIP, 2000. http://dx.doi.org/10.1063/1.1291347.

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Maisack, M., W. Collmar, G. G. Lichti, V. Schönfelder, H. Steinle, H. Bloemen, W. Hermsen et al. « COMPTEL upper limits for Seyfert galaxies ». Dans The second Compton symposium. AIP, 1994. http://dx.doi.org/10.1063/1.45652.

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Parker, Timothy, et Ronald Humble. « Theoretical upper limits on enthalpy rocket performance ». Dans 30th Joint Propulsion Conference and Exhibit. Reston, Virigina : American Institute of Aeronautics and Astronautics, 1994. http://dx.doi.org/10.2514/6.1994-2872.

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Brainerd, J. J., et R. M. Kippen. « Upper limits on gamma-ray burst repetition ». Dans GAMMA-RAY BURSTS. ASCE, 1998. http://dx.doi.org/10.1063/1.55327.

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Sajjadi, Mahsa, et Hossein Seifi. « Governor Parameter Estimation Considering Upper/Lower Production Limits ». Dans 2019 IEEE Milan PowerTech. IEEE, 2019. http://dx.doi.org/10.1109/ptc.2019.8810572.

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Li, Ziyang, Di Qi, Mengwei Zhang et Yingyue Zhang. « Executive Pay-performance Sensitivity and Mandatory Upper Limits ». Dans 2020 6th International Conference on Information Management (ICIM). IEEE, 2020. http://dx.doi.org/10.1109/icim49319.2020.244686.

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Cibulka, Josef, et Jan Kynčl. « Better upper bounds on the Füredi-Hajnal limits of permutations ». Dans Proceedings of the Twenty-Eighth Annual ACM-SIAM Symposium on Discrete Algorithms. Philadelphia, PA : Society for Industrial and Applied Mathematics, 2017. http://dx.doi.org/10.1137/1.9781611974782.150.

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Williams, G. G. « LOTIS upper limits and the prompt OT from GRB 990123 ». Dans The fifth huntsville gamma-ray burst symposium. AIP, 2000. http://dx.doi.org/10.1063/1.1361544.

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KHRIPLOVICH, IOSIF, et ELENA PITJEVA. « UPPER LIMITS ON DENSITY OF DARK MATTER IN SOLAR SYSTEM ». Dans Proceedings of the MG11 Meeting on General Relativity. World Scientific Publishing Company, 2008. http://dx.doi.org/10.1142/9789812834300_0053.

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Cannady, Nicholas W. « CALET Upper Limits on GeV-energy Gamma-Ray Burst Emission ». Dans 36th International Cosmic Ray Conference. Trieste, Italy : Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0557.

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Rapports d'organisations sur le sujet "Upper limits"

Duk-Rodkin, A., F. Weber et R. W. Barendregt. Glacial limits map of upper Yukon River. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2002. http://dx.doi.org/10.4095/213393.

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Schroeder, P. C., M. P. Ulmer, S. M. Matz, D. A. Grabelsky, W. R. Purcell, J. E. Grove, W. N. Johnson et al. OSSE Upper Limits to Pulsar Gamma-Ray Emission. Fort Belvoir, VA : Defense Technical Information Center, septembre 1994. http://dx.doi.org/10.21236/ada464427.

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J.W. Pegram. Calculation of Upper Subcritical Limits for Nuclear Criticality in a Repository. Office of Scientific and Technical Information (OSTI), juillet 1998. http://dx.doi.org/10.2172/895333.

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Swartz, M. An Improved Method for Setting Upper Limits with Small Numbers of Events. Office of Scientific and Technical Information (OSTI), février 1990. http://dx.doi.org/10.2172/1449161.

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Rugari, S. L., R. H. III France, M. Gai, B. J. Lund, S. D. Smolen, Z. Zhao, S. E. Jones, J. E. Hack, K. W. Zilm et K. G. Lynn. Upper limits on neutron bursts emitted from Ti pressurized D sub 2 gas cells. Office of Scientific and Technical Information (OSTI), octobre 1989. http://dx.doi.org/10.2172/5175438.

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Alwin, Jennifer, Forrest Brown, Matthew Lazaric, Benjamin Murphy et Kristina Spencer. Comparison Study of Upper Subcritical Limits Derived Using Sensitivity/Uncertainty Tools Case Studies of Benchmarks and Applications. Office of Scientific and Technical Information (OSTI), octobre 2020. http://dx.doi.org/10.2172/1673352.

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Tournear, Derek M. X-ray Bursts in Neutron Star and Black Hole Binaries from USA Data : Detections and Upper Limits. Office of Scientific and Technical Information (OSTI), février 2003. http://dx.doi.org/10.2172/813180.

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Alwin, Jennifer Louise, Forest B. Brown et Michael Evan Rising. Excluding Benchmark Statistical Outliers in Nuclear Criticality Safety Validation : A Comparison Study of Upper Subcritical Limits for Plutonium Systems using Whisper-1.1. Office of Scientific and Technical Information (OSTI), août 2018. http://dx.doi.org/10.2172/1467235.

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Benjamin, Doug, Matt Herndon, Eric James, Tom Junk, Nils Krumnack, Weiming Yao, Gavin Davies et al. Combined CDF and D0 upper limits on MSSM Higgs boson production in tau-tau final states with up to 2.2 fb-1. Office of Scientific and Technical Information (OSTI), mars 2010. http://dx.doi.org/10.2172/975168.

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Wolinski, David Scott. Upper limits on rare decays of the top quark using jet flavor tagging in $p \bar{p}$ collisions at $\sqrt{s}$ = 1.8-TeV. Office of Scientific and Technical Information (OSTI), janvier 2001. http://dx.doi.org/10.2172/1421415.

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