16,625 results on '"Brown W."'
Search Results
2. Detection of the elusive dangling OH ice features at ~2.7 μm in Chamaeleon I with JWST NIRCam
- Author
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Noble, J. A., Fraser, H. J., Smith, Z. L., Dartois, E., Boogert, A. C. A., Cuppen, H. M., Dickinson, H. J., Dulieu, F., Egami, E., Erkal, J., Giuliano, B. M., Husquinet, B., Lamberts, T., Maté, B., McClure, M. K., Palumbo, M. E., Shimonishi, T., Sun, F., Bergner, J. B., Brown, W. A., Caselli, P., Congiu, E., Drozdovskaya, M. N., Herrero, V. J., Ioppolo, S., Jimenez-Serra, I., Linnartz, H., Melnick, G. J., McGuire, B. A., Oberg, K. I., Perotti, G., Qasim, D., Rocha, W. R. M., and Urso, R. G.
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- 2024
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3. Behaviour change techniques, barriers and facilitators for promoting self-managed physical activity in Australian defence force veterans: A mixed-methods study
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Papinczak, Zoe Elizabeth, Gilson, N, Mielke, G, Haslam, C, and Brown, W
- Published
- 2024
4. An Ice Age JWST inventory of dense molecular cloud ices
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McClure, M. K., Rocha, W. R. M., Pontoppidan, K. M., Crouzet, N., Chu, L. E. U., Dartois, E., Lamberts, T., Noble, J. A., Pendleton, Y. J., Perotti, G., Qasim, D., Rachid, M. G., Smith, Z. L., Sun, Fengwu, Beck, Tracy L, Boogert, A. C. A., Brown, W. A., Caselli, P., Charnley, S. B., Cuppen, Herma M., Dickinson, H., Drozdovskaya, M. N., Egami, E., Erkal, J., Fraser, H., Garrod, R. T., Harsono, D., Ioppolo, S., Jimenez-Serra, I., Jin, M., Jørgensen, J. K., Kristensen, L. E., Lis, D. C., McCoustra, M. R. S., McGuire, Brett A., Melnick, G. J., Oberg, Karin I., Palumbo, M. E., Shimonishi, T., Sturm, J. A., van Dishoeck, E. F., and Linnartz, H.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Icy grain mantles are the main reservoir of the volatile elements that link chemical processes in dark, interstellar clouds with the formation of planets and composition of their atmospheres. The initial ice composition is set in the cold, dense parts of molecular clouds, prior to the onset of star formation. With the exquisite sensitivity of JWST, this critical stage of ice evolution is now accessible for detailed study. Here we show the first results of the Early Release Science program "Ice Age" that reveal the rich composition of these dense cloud ices. Weak ices, including, $^{13}$CO$_2$, OCN$^-$, $^{13}$CO, OCS, and COMs functional groups are now detected along two pre-stellar lines of sight. The $^{12}$CO$_2$ ice profile indicates modest growth of the icy grains. Column densities of the major and minor ice species indicate that ices contribute between 2 and 19% of the bulk budgets of the key C, O, N, and S elements. Our results suggest that the formation of simple and complex molecules could begin early in a water-ice rich environment., Comment: To appear in Nature Astronomy on January 23rd, 2023. 33 pages, 16 figures, 3 tables; includes extended and supplemental data sections. Part of the JWST Ice Age Early Release Science program's science enabling products. Enhanced spectra downloadable on Zenodo at the following DOI: 10.5281/zenodo.7501239
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- 2023
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5. Four new deeply-eclipsing white dwarfs in ZTF
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Kosakowski, Alekzander, Kilic, M., Brown, W. R., Bergeron, P., and Kupfer, T.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We present the results of a search for deeply-eclipsing white dwarfs in the ZTF Data Release 4. We identify nine deeply-eclipsing white dwarf candidates, four of which we followed up with high-cadence photometry and spectroscopy. Three of these systems show total eclipses in the ZTF data and our follow-up APO 3.5-meter telescope observations. Even though the eclipse duration is consistent with sub-stellar companions, our analysis shows that all four systems contain a white dwarf with low-mass stellar companions of ~0.1 Msol. We provide mass and radius constraints for both stars in each system based on our photometric and spectroscopic fitting. Finally, we present a list of 41 additional eclipsing WD+M candidates identified in a preliminary search of ZTF DR7, including 12 previously studied systems. We identify two new candidate short-period, eclipsing, white dwarf-brown dwarf binaries within our sample of 41 WD+M candidates based on PanSTARRS colors., Comment: Accepted for publication with MNRAS. 12 pages, 15 figures, 3 tables
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- 2022
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6. Co3Ga2Ge5: Probing site mixing of the Ru3Sn7 structure type with elements difficult to distinguish by diffraction
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Brown, W. Kice, Oyekunle, Ifeoluwa P., Truong, Erica, Chen, Yudan, Ogbolu, Bright, Schundelmier, Benny, O’Donnell, Shaun, Smaha, Rebecca W., Hu, Yan-Yan, Wei, Kaya, McCandless, Gregory T., and Chan, Julia Y.
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- 2025
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7. Daily Living Skills in Adolescent and Young Adult Males With Fragile X Syndrome.
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Thurman, Angela John, Swinehart, Stephanie Summers, Klusek, Jessica, Roberts, Jane E, Bullard, Lauren, Marzan, Jocelyn Christina B, Brown, W Ted, and Abbeduto, Leonard
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Cognitive and Computational Psychology ,Psychology ,Rare Diseases ,Fragile X Syndrome ,Pediatric ,Mental Health ,Brain Disorders ,Autism ,Behavioral and Social Science ,Intellectual and Developmental Disabilities (IDD) ,Mental health ,Activities of Daily Living ,Adolescent ,Adult ,Autistic Disorder ,Humans ,Language ,Language Tests ,Male ,Young Adult ,fragile X syndrome ,daily living skills ,language ,autism spectrum disorder ,FMRP ,Medical and Health Sciences ,Education ,Psychology and Cognitive Sciences ,Rehabilitation ,Biomedical and clinical sciences - Abstract
By adulthood, most males with fragile X syndrome (FXS) require support to navigate day-to-day settings. The present study cross-sectionally: (1) characterized the profile of daily living skills in males with FXS and (2) examined associated participant characteristics (i.e., fragile X mental retardation protein [FMRP] expression, nonverbal cognition, language, autism symptomatology, and anxiety symptomatology) using the Waisman-Activities of Daily Living questionnaire. Males with FXS (n = 57, ages 15-23 years) needed more help/support in the areas of domestic and community daily livings skills, than in the area of personal daily living skills. Significant associations were observed between reduced daily living skills and lower nonverbal cognition, receptive language, expressive language, and increased autism symptomatology. Receptive language emerged as the strongest unique predictor of daily living skill performance.
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- 2022
8. Effects of mycobacterium cell wall fraction on embryo development following in vitro embryo production and pregnancy rates following embryo transfer in virgin dairy heifers
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Brown, W., Oliveira, M., Reis Silva, R., Woodruff, K., Bisha, B., Demetrio, D., and Block, J.
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- 2024
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9. White dwarfs with planetary remnants in the era of Gaia I: six emission line systems
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Fusillo, N. P. Gentile, Manser, C. J., Gänsicke, Boris T., Toloza, O., Koester, D., Dennihy, E., Brown, W. R., Farihi, J., Hollands, M. A., Hoskin, M. J., Izquierdo, P., Kinnear, T., Marsh, T. R., Santamaria-Miranda, A., Pala, A. F., Redfield, S., Rodriguez-Gil, P., Schreiber, M. R., Veras, D., and Wilson, D. J.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
White dwarfs with emission lines from gaseous debris discs are among the rarest examples of planetary remnant hosts, but at the same time they are key objects for studying the final evolutionary stage of planetary systems. Making use of the large number of white dwarfs identified in Gaia DR2, we are conducting a survey of planetary remnants and here we present the first results of our search: six white dwarfs with gaseous debris discs. This first publication focuses on the main observational properties of these objects and highlights their most unique features. Three systems in particular stand out: WDJ084602.47+570328.64 displays an exceptionally strong infrared excess which defies the standard model of a geometrically-thin, optically-thick dusty debris disc; WDJ213350.72+242805.93 is the hottest gaseous debris disc host known with Teff=29282 K; and WDJ052914.32-340108.11, in which we identify a record number of 51 emission lines from five elements. These discoveries shed light on the underlying diversity in gaseous debris disc systems and bring the total number of these objects to 21. With these numbers we can now start looking at the properties of these systems as a class of objects rather than on a case-by-case basis., Comment: 20 pages, 11 figures, accepted for publication in MNRAS. V2 replaced Fig.10 and minor changes to sections 4 and 7
- Published
- 2020
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10. $\textit{Gaia}$ white dwarfs within 40 pc I: spectroscopic observations of new candidates
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Tremblay, P. -E., Hollands, M. A., Fusillo, N. P. Gentile, McCleery, J., Izquierdo, P., Gänsicke, B. T., Cukanovaite, E., Koester, D., Brown, W. R., Charpinet, S., Cunningham, T., Farihi, J., Giammichele, N., van Grootel, V., Hermes, J. J., Hoskin, M. J., Jordan, S., Kepler, S. O., Kleinman, S. J., Manser, C. J., Marsh, T. R., de Martino, D., Nitta, A., Parsons, S. G., Pelisoli, I., Raddi, R., Rebassa-Mansergas, A., Ren, J. -J., Schreiber, M. R., Silvotti, R., Toloza, O., Toonen, S., and Torres, S.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We present a spectroscopic survey of 230 white dwarf candidates within 40 pc of the Sun from the William Herschel Telescope and Gran Telescopio Canarias. All candidates were selected from $\textit{Gaia}$ Data Release 2 (DR2) and in almost all cases had no prior spectroscopic classifications. We find a total of 191 confirmed white dwarfs and 39 main-sequence star contaminants. The majority of stellar remnants in the sample are relatively cool ($\langle T_{\rm eff} \rangle$ = 6200 K), showing either hydrogen Balmer lines or a featureless spectrum, corresponding to 89 DA and 76 DC white dwarfs, respectively. We also recover two DBA white dwarfs and 9--10 magnetic remnants. We find two carbon-bearing DQ stars and 14 new metal-rich white dwarfs. This includes the possible detection of the first ultra-cool white dwarf with metal lines. We describe three DZ stars for which we find at least four different metal species, including one which is strongly Fe- and Ni-rich, indicative of the accretion of a planetesimal with core-Earth composition. We find one extremely massive (1.31 $\pm$ 0.01 M$_{\odot}$) DA white dwarf showing weak Balmer lines, possibly indicating stellar magnetism. Another white dwarf shows strong Balmer line emission but no infrared excess, suggesting a low-mass sub-stellar companion. High spectroscopic completeness ($>$99%) has now been reached for $\textit{Gaia}$ DR2 sources within 40 pc sample, in the northern hemisphere ($\delta >$ 0 deg) and located on the white dwarf cooling track in the Hertzsprung-Russell diagram. A statistical study of the full northern sample is presented in a companion paper., Comment: 37 pages, 25 figures. Accepted for publication in MNRAS
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- 2020
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11. Modeling community COVID-19 transmission risk associated with U.S. universities
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Uelmen, J. A., Kopsco, H., Mori, J., Brown, W. M., and Smith, R. L.
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- 2023
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12. Bedrock weathering contributes to subsurface reactive nitrogen and nitrous oxide emissions
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Wan, J, Tokunaga, TK, Brown, W, Newman, AW, Dong, W, Bill, M, Beutler, CA, Henderson, AN, Harvey-Costello, N, Conrad, ME, Bouskill, NJ, Hubbard, SS, and Williams, KH
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Meteorology & Atmospheric Sciences - Abstract
Atmospheric nitrous oxide contributes directly to global warming, yet models of the nitrogen cycle do not account for bedrock, the largest pool of terrestrial nitrogen, as a source of nitrous oxide. Although it is known that release rates of nitrogen from bedrock are large, there is an incomplete understanding of the connection between bedrock-hosted nitrogen and atmospheric nitrous oxide. Here, we quantify nitrogen fluxes and mass balances at a hillslope underlain by marine shale. We found that, at this site, bedrock weathering contributes 78% of the subsurface reactive nitrogen, while atmospheric sources (commonly regarded as the sole sources of reactive nitrogen in pristine environments) account for only the remaining 22%. About 56% of the total subsurface reactive nitrogen denitrifies, including 14% emitted as nitrous oxide. The remaining reactive nitrogen discharges in porewaters to a floodplain where additional denitrification probably occurs. We also found that the release of bedrock nitrogen occurs primarily within the zone of the seasonally fluctuating water table and suggest that the accumulation of nitrate in the vadose zone, often attributed to fertilization and soil leaching, may also include contributions from weathered nitrogen-rich bedrock. Our hillslope study suggests that, under oxygenated and moisture-rich conditions, weathering of deep, nitrogen-rich bedrock makes an important contribution to the nitrogen cycle.
- Published
- 2021
13. A data mining transmission switching heuristic for post-contingency AC power flow violation reduction in real-world, large-scale systems
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Brown, W. Eric and Moreno-Centeno, Erick
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- 2023
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14. Structural basis for antibody inhibition of flavivirus NS1–triggered endothelial dysfunction
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Biering, Scott B, Akey, David L, Wong, Marcus P, Brown, W Clay, Lo, Nicholas TN, Puerta-Guardo, Henry, Tramontini Gomes de Sousa, Francielle, Wang, Chunling, Konwerski, Jamie R, Espinosa, Diego A, Bockhaus, Nicholas J, Glasner, Dustin R, Li, Jeffrey, Blanc, Sophie F, Juan, Evan Y, Elledge, Stephen J, Mina, Michael J, Beatty, P Robert, Smith, Janet L, and Harris, Eva
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Vaccine Related ,Prevention ,Immunization ,Vector-Borne Diseases ,Rare Diseases ,Emerging Infectious Diseases ,Biodefense ,Infectious Diseases ,West Nile Virus ,Aetiology ,2.1 Biological and endogenous factors ,Infection ,Good Health and Well Being ,Animals ,Antibodies ,Monoclonal ,Antibodies ,Neutralizing ,Antibodies ,Viral ,Cross Reactions ,Crystallography ,X-Ray ,Dengue ,Dengue Virus ,Endothelium ,Glycocalyx ,Humans ,Mice ,Protein Conformation ,beta-Strand ,Protein Domains ,Viral Nonstructural Proteins ,West Nile Fever ,West Nile virus ,Zika Virus ,Zika Virus Infection ,General Science & Technology - Abstract
Medically important flaviviruses cause diverse disease pathologies and collectively are responsible for a major global disease burden. A contributing factor to pathogenesis is secreted flavivirus nonstructural protein 1 (NS1). Despite demonstrated protection by NS1-specific antibodies against lethal flavivirus challenge, the structural and mechanistic basis remains unknown. Here, we present three crystal structures of full-length dengue virus NS1 complexed with a flavivirus-cross-reactive, NS1-specific monoclonal antibody, 2B7, at resolutions between 2.89 and 3.96 angstroms. These structures reveal a protective mechanism by which two domains of NS1 are antagonized simultaneously. The NS1 wing domain mediates cell binding, whereas the β-ladder triggers downstream events, both of which are required for dengue, Zika, and West Nile virus NS1-mediated endothelial dysfunction. These observations provide a mechanistic explanation for 2B7 protection against NS1-induced pathology and demonstrate the potential of one antibody to treat infections by multiple flaviviruses.
- Published
- 2021
15. A study of young children's pull-apart strength (an addendum to NBSIR73-156-A study of the strength capabilities of children ages two through six)
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Brown, W. C.
- Published
- 1974
16. ESA Voyage 2050 white paper -- Faint objects in motion: the new frontier of high precision astrometry
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Malbet, F., Abbas, U., Alves, J., Boehm, C., Brown, W., Chemin, L., Correia, A., Courbin, F., Darling, J., Diaferio, A., Fortin, M., Fridlund, M., Gnedin, O., Holl, B., Krone-Martins, A., Léger, A., Labadie, L., Laskar, J., Mamon, G., McArthur, B., Michalik, D., Moitinho, A., Oertel, M., Ostorero, L., Schneider, J., Scott, P., Shao, M., Sozzetti, A., Tomsick, J., Valluri, M., and Wyse, R.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Sky survey telescopes and powerful targeted telescopes play complementary roles in astronomy. In order to investigate the nature and characteristics of the motions of very faint objects, a flexibly-pointed instrument capable of high astrometric accuracy is an ideal complement to current astrometric surveys and a unique tool for precision astrophysics. Such a space-based mission will push the frontier of precision astrometry from evidence of earth-massed habitable worlds around the nearest starts, and also into distant Milky way objects up to the Local Group of galaxies. As we enter the era of the James Webb Space Telescope and the new ground-based, adaptive-optics-enabled giant telescopes, by obtaining these high precision measurements on key objects that Gaia could not reach, a mission that focuses on high precision astrometry science can consolidate our theoretical understanding of the local universe, enable extrapolation of physical processes to remote redshifts, and derive a much more consistent picture of cosmological evolution and the likely fate of our cosmos. Already several missions have been proposed to address the science case of faint objects in motion using high precision astrometry ESA missions: NEAT for M3, micro-NEAT for S1 mission, and Theia for M4 and M5. Additional new mission configurations adapted with technological innovations could be envisioned to pursue accurate measurements of these extremely small motions. The goal of this white paper is to address the fundamental science questions that are at stake when we focus on the motions of faint sky objects and to briefly review quickly instrumentation and mission profiles., Comment: White paper for the Voyage 2050 long-term plan in the ESA Science Programme. arXiv admin note: substantial text overlap with arXiv:1707.01348
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- 2019
17. A study of the strength capabilities of children ages two through six
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Brown, W. C.
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- 1973
18. Depression, Perceived Risk of COVID-19, Loneliness, and Perceived Social Support from Friends Among University Students in Poland, UK, and India
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Bokszczanin A, Palace M, Brown W, Gladysh O, Tripathi R, and Shree D
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depression ,perceived risk of covid-19 ,loneliness ,perceived social support ,university students ,Psychology ,BF1-990 ,Industrial psychology ,HF5548.7-5548.85 - Abstract
Anna Bokszczanin,1 Marek Palace,2 William Brown,3 Olga Gladysh,4 Rakhi Tripathi,5 Divya Shree6 1Institute of Psychology, University of Opole, Opole, Poland; 2School of Psychology, Liverpool John Moores University, Liverpool, UK; 3School of Psychology, University of Bedfordshire, Luton, UK; 4Institute of Psychology, Polish Academy of Sciences, Warsaw, Poland; 5Information Technology Area, FORE School of Management, New Delhi, India; 6School of Criminology and Behavioural Sciences, Rashtriya Raksha University Lavad, Dahegam, IndiaCorrespondence: Anna Bokszczanin, University of Opole, Institute of Psychology, 45-052 Opole, Plac Staszica 1, Opole, Poland, Email abok@uni.opole.plBackground: The study examines the prevalence of depression among university students in Poland, the UK and India in the face of the second pandemic wave of COVID-19. The paper also examines the protective role of perceived social support, the hypothesis being that social support from friends would reduce depression. Methods: The data from university students (N=732) in Poland (N=335), UK (N= 198), and India (N=199) were collected online during of the fall/winter 2021. Participants completed measures of depression (CES-D), COVID-19 risk perception index, loneliness (DJGLS), and perceived social support (MSPSS).Results: Almost 52% of all participants (58.5% in Poland, 62.6% in the UK, and 29.1% in India) met the criteria for major depression. The higher levels of depression symptoms were associated with a higher perceived risk of COVID-19, greater loneliness, female gender, younger students’ age, and the lower levels of perceived social support. The greater family support predicted lower levels of depression symptoms in the Polish and Indian samples. Structural equation analyses (SEM) revealed the indirect effect of perceived social support from friends on the association between social loneliness and depression and between age and depression. This result shows that the support from friends significantly reduced depression, regardless of age, the level of social loneliness, and the perceived risk of COVID-19.Conclusion: Our conclusions link to university specialists’ enhancement of psychological help for students with depression. We also recommend information campaigns on depression and treatment options.Keywords: depression, perceived risk of COVID-19, loneliness, perceived social support, university students
- Published
- 2023
19. Structural and physical properties of R2M3X5 compounds
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Brown, W. Kice, primary, Plata, Mario A., additional, Raines, Morgan E., additional, and Chan, Julia Y., additional
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- 2023
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20. Outcomes of Medical Therapy Plus PCI for Multivessel or Left Main CAD Ineligible for Surgery
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Salisbury, Adam C., Grantham, J. Aaron, Brown, W. Morris, Ballard, William L., Allen, Keith B., Kirtane, Ajay J., Argenziano, Michael, Yeh, Robert W., Khabbaz, Kamal, Lasala, John, Kachroo, Puja, Karmpaliotis, Dimitri, Moses, Jeffrey, Lombardi, William L., Nugent, Karen, Ali, Ziad, Gosch, Kensey L., Spertus, John A., and Kandzari, David E.
- Published
- 2023
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21. Impact of Periprocedural Adverse Events After PCI and CABG on 5-Year Mortality: The EXCEL Trial
- Author
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Jain, Sneha S., Li, Ditian, Dressler, Ovidiu, Kotinkaduwa, Lak, Serruys, Patrick W., Kappetein, A. Pieter, Sabik, Joseph F., Morice, Marie-Claude, Puskas, John, Kandzari, David E., Karmpaliotis, Dimitri, Lembo, Nicholas J., Brown, W. Morris, III, Banning, Adrian P., and Stone, Gregg W.
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- 2023
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22. The McDonald Observatory search for pulsating sdA stars: asteroseismic support for multiple populations
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Bell, Keaton J., Pelisoli, Ingrid, Kepler, S. O., Brown, W. R., Winget, D. E., Winget, K. I., Vanderbosch, Z., Castanheira, B. G., Hermes, J. J., Montgomery, M. H., and Koester, D.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
Context. The nature of the recently identified "sdA" spectroscopic class of star is not well understood. The thousands of known sdAs have H-dominated spectra, spectroscopic surface gravities intermediate to main sequence stars and isolated white dwarfs, and effective temperatures below the lower limit for He-burning subdwarfs. Most are likely products of binary stellar evolution, whether extremely low-mass white dwarfs and their precursors, or blue stragglers in the halo. Aims. Stellar eigenfrequencies revealed through time series photometry of pulsating stars sensitively probe stellar structural properties. The properties of pulsations exhibited by any sdA stars would contribute importantly to our developing understanding of this class. Methods. We extend our photometric campaign to discover pulsating extremely low-mass white dwarfs from McDonald Observatory to target sdA stars classified from SDSS spectra. We also obtain follow-up time series spectroscopy to search for binary signatures from four new pulsators. Results. Out of 23 sdA stars observed, we clearly detect stellar pulsations in seven. Dominant pulsation periods range from 4.6 minutes to 12.3 hours, with most on ~hour timescales. We argue specific classifications for some of the new variables, identifying both compact and likely main sequence dwarf pulsators, along with a candidate low-mass RR Lyrae star. Conclusions. With dominant pulsation periods spanning orders of magnitude, the pulsational evidence supports the emerging narrative that the sdA class consists of multiple stellar populations. Since multiple types of sdA exhibit stellar pulsations, follow-up asteroseismic analysis can be used to probe the precise evolutionary natures and stellar structures of these individual subpopulations., Comment: 12 pages, 5 figures; accepted for publication in A&A; light curves of seven new pulsating sdA stars included as ancillary files
- Published
- 2018
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23. Fungal indole alkaloid biogenesis through evolution of a bifunctional reductase/Diels–Alderase
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Dan, Qingyun, Newmister, Sean A, Klas, Kimberly R, Fraley, Amy E, McAfoos, Timothy J, Somoza, Amber D, Sunderhaus, James D, Ye, Ying, Shende, Vikram V, Yu, Fengan, Sanders, Jacob N, Brown, W Clay, Zhao, Le, Paton, Robert S, Houk, KN, Smith, Janet L, Sherman, David H, and Williams, Robert M
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Biotechnology ,Emerging Infectious Diseases ,Vaccine Related ,Ascomycota ,Biocatalysis ,Cycloaddition Reaction ,Indole Alkaloids ,Models ,Molecular ,Molecular Structure ,Oxidoreductases ,Chemical Sciences ,Organic Chemistry - Abstract
Prenylated indole alkaloids such as the calmodulin-inhibitory malbrancheamides and anthelmintic paraherquamides possess great structural diversity and pharmaceutical utility. Here, we report complete elucidation of the malbrancheamide biosynthetic pathway accomplished through complementary approaches. These include a biomimetic total synthesis to access the natural alkaloid and biosynthetic intermediates in racemic form and in vitro enzymatic reconstitution to provide access to the natural antipode (+)-malbrancheamide. Reductive cleavage of an L-Pro-L-Trp dipeptide from the MalG non-ribosomal peptide synthetase (NRPS) followed by reverse prenylation and a cascade of post-NRPS reactions culminates in an intramolecular [4+2] hetero-Diels-Alder (IMDA) cyclization to furnish the bicyclo[2.2.2]diazaoctane scaffold. Enzymatic assembly of optically pure (+)-premalbrancheamide involves an unexpected zwitterionic intermediate where MalC catalyses enantioselective cycloaddition as a bifunctional NADPH-dependent reductase/Diels-Alderase. The crystal structures of substrate and product complexes together with site-directed mutagenesis and molecular dynamics simulations demonstrate how MalC and PhqE (its homologue from the paraherquamide pathway) catalyse diastereo- and enantioselective cyclization in the construction of this important class of secondary metabolites.
- Published
- 2019
24. Depth- and Time-Resolved Distributions of Snowmelt-Driven Hillslope Subsurface Flow and Transport and Their Contributions to Surface Waters
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Tokunaga, TK, Wan, J, Williams, KH, Brown, W, Henderson, A, Kim, Y, Tran, AP, Conrad, ME, Bill, M, Carroll, RWH, Dong, W, Xu, Z, Lavy, A, Gilbert, B, Carrero, S, Christensen, JN, Faybishenko, B, Arora, B, Siirila-Woodburn, ER, Versteeg, R, Raberg, JH, Peterson, JE, and Hubbard, SS
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recharge ,hillslope ,transmissivity ,concentration-discharge ,groundwater ,snowmelt ,Environmental Engineering ,Physical Geography and Environmental Geoscience ,Civil Engineering - Abstract
Major components of hydrologic and elemental cycles reside underground, where their complex dynamics and linkages to surface waters are obscure. We delineated seasonal subsurface flow and transport dynamics along a hillslope in the Rocky Mountains (USA), where precipitation occurs primarily as winter snow and drainage discharges into the East River, a tributary of the Gunnison River. Hydraulic and geochemical measurements down to 10 m below ground surface supported application of transmissivity feedback of snowmelt to describe subsurface flow and transport through three zones: soil, weathering shale, and saturated fractured shale. Groundwater flow is predicted to depths of at least 176 m, although a shallower limit exists if hillslope-scale hydraulic conductivities are higher than our local measurements. Snowmelt during the high snowpack water year 2017 sustained flow along the weathering zone and downslope within the soil, while negligible downslope flow occurred along the soil during the low snowpack water year 2018. We introduce subsurface concentration-discharge (C-Q) relations for explaining hillslope contributions to C-Q observed in rivers and demonstrate their calculations based on transmissivity fluxes and measured pore water specific conductance and dissolved organic carbon. The specific conductance data show that major ions in the hillslope pore waters, primarily from the weathering and fractured shale, are about six times more concentrated than in the river, indicating hillslope solute loads are disproportionately high, while flow from this site and similar regions are relatively smaller. This methodology is applicable in different representative environments within snow-dominated watersheds for linking their subsurface exports to surface waters.
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- 2019
25. Distinct Source Water Chemistry Shapes Contrasting Concentration-Discharge Patterns
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Zhi, W, Li, L, Dong, W, Brown, W, Kaye, J, Steefel, C, and Williams, KH
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Civil Engineering ,Environmental Engineering ,Applied Economics ,Physical Geography and Environmental Geoscience - Abstract
Understanding concentration-discharge (C-Q) relationships are essential for predicting chemical weathering and biogeochemical cycling under changing climate and anthropogenic conditions. Contrasting C-Q relationships have been observed widely, yet a mechanistic framework that can interpret diverse patterns remains elusive. This work hypothesizes that seemingly disparate C-Q patterns are driven by switching dominance of end-member source waters and their chemical contrasts arising from subsurface biogeochemical heterogeneity. We use data from Coal Creek, a high-elevation mountainous catchment in Colorado, and a recently developed watershed reactive transport model (BioRT-Flux-PIHM). Sensitivity analysis and Monte-Carlo simulations (500 cases) show that reaction kinetics and thermodynamics and distribution of source materials across depths govern the chemistry gradients of shallow soil water and deeper groundwater entering the stream. The alternating dominance of organic-poor yet geo-solute-rich groundwater under dry conditions and organic-rich yet geo-solute-poor soil water during spring melt leads to the flushing pattern of dissolved organic carbon and the dilution pattern of geogenic solutes (e.g., Na, Ca, and Mg). In addition, the extent of concentration contrasts regulates the power law slopes (b) of C-Q patterns via a general equation (Formula presented.). At low ratios of soil water versus groundwater concentrations (Cratio = Csw/Cgw 1.8), flushing arises; chemostasis occurs in between. This equation quantitatively interprets b values of 11 solutes (dissolved organic carbon, dissolved P, NO3−, K, Si, Ca, Mg, Na, Al, Mn, and Fe) from three catchments (Coal Creek, Shale Hills, and Plynlimon) of differing climate, geologic, and land cover conditions. This indicates potentially broad regulation of subsurface biogeochemical heterogeneity in determining C-Q patterns and wide applications of this equation in quantifying b values, which can have broad implications for predicting chemical weathering and biogeochemical transformation at the watershed scale.
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- 2019
26. ASD Comorbidity in Fragile X Syndrome: Symptom Profile and Predictors of Symptom Severity in Adolescent and Young Adult Males
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Abbeduto, Leonard, Thurman, Angela John, McDuffie, Andrea, Klusek, Jessica, Feigles, Robyn Tempero, Ted Brown, W, Harvey, Danielle J, Adayev, Tatyana, LaFauci, Giuseppe, Dobkins, Carl, and Roberts, Jane E
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Biological Psychology ,Psychology ,Brain Disorders ,Intellectual and Developmental Disabilities (IDD) ,Mental Health ,Pediatric ,Rare Diseases ,Fragile X Syndrome ,Autism ,Behavioral and Social Science ,Aetiology ,2.1 Biological and endogenous factors ,Mental health ,Adolescent ,Autism Spectrum Disorder ,Comorbidity ,Humans ,Male ,Predictive Value of Tests ,Severity of Illness Index ,Young Adult ,Fragile X syndrome ,Autism spectrum disorder ,Language ,IQ ,Psychiatric symptoms ,FMRP ,Education ,Psychology and Cognitive Sciences ,Developmental & Child Psychology ,Health sciences - Abstract
Many males with FXS meet criteria for ASD. This study was designed to (1) describe ASD symptoms in adolescent and young adult males with FXS (n = 44) and (2) evaluate the contributions to ASD severity of cognitive, language, and psychiatric factors, as well as FMRP (the protein deficient in FXS). A few ASD symptoms on the ADOS-2 were universal in the sample. There was less impairment in restricted and repetitive behaviors (RRB) than in the social affective (SA) domain. The best predictor of overall ASD severity and SA severity was expressive syntactic ability. RRB severity was best predicted by the psychiatric factors. Implications for clinical practice and for understanding the ASD comorbidity in FXS are discussed.
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- 2019
27. Challenges in Building an End-to-End System for Acquisition, Management, and Integration of Diverse Data from Sensor Networks in Watersheds: Lessons from a Mountainous Community Observatory in East River, Colorado
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Varadharajan, C, Faybishenko, B, Henderson, A, Henderson, M, Hendrix, VC, Hubbard, SS, Kakalia, Z, Newman, A, Potter, B, Steltzer, H, Versteeg, R, Agarwal, DA, Williams, KH, Wilmer, C, Wu, Y, Brown, W, Burrus, M, Carroll, RWH, Christianson, DS, Dafflon, B, Dwivedi, D, and Enquist, BJ
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Rivers ,Data models ,Monitoring ,Temperature measurement ,Data collection ,Snow ,Biology ,Sensor systems and applications ,sensors ,geoscience ,water resources ,watershed ,data management ,data integration ,data processing ,co-design ,Information and Computing Sciences ,Engineering ,Technology - Abstract
The U.S. Department of Energy's Watershed Function Scientific Focus Area (SFA), centered in the East River, Colorado, generates diverse datasets including hydrological, geological, geochemical, geophysical, ecological, microbiological and remote sensing data. The project has deployed extensive field infrastructure involving hundreds of sensors that measure highly diverse phenomena (e.g. stream and groundwater hydrology, water quality, soil moisture, weather) across the watershed. Data from the sensor network are telemetered and automatically ingested into a queryable database. The data are subsequently quality checked, integrated with the United States Geological Survey's stream monitoring network using a custom data integration broker, and published to a portal with interactive visualizations. The resulting data products are used in a variety of scientific modeling and analytical efforts. This paper describes the SFA's end-to-end infrastructure and services that support the generation of integrated datasets from a watershed sensor network. The development and maintenance of this infrastructure, presents a suite of challenges from practical field logistics to complex data processing, which are addressed through various solutions. In particular, the SFA adopts a holistic view for data collection, assessment and integration, which dramatically improves the products generated, and enables a co-design approach wherein data collection is informed by model results and vice-versa.
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- 2019
28. The Outcomes of Percutaneous RevascularizaTIon for Management of SUrgically Ineligible Patients With Multivessel or Left Main Coronary Artery Disease (OPTIMUM) Registry: Rationale and Design
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Salisbury, Adam C., Kirtane, Ajay J., Ali, Ziad A., Grantham, J. Aaron, Lombardi, William L., Yeh, Robert W., Genereux, Philippe, Allen, Keith B., Brown, W. Morris, Nugent, Karen, Gosch, Kensey L., Karmpaliotis, Dimitri, Spertus, John A., and Kandzari, David E.
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- 2022
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29. Diagnostic accuracy of an automated artificial intelligence derived right ventricular to left ventricular diameter ratio tool on CT pulmonary angiography to predict pulmonary hypertension at right heart catheterisation
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Charters, P.F.P., Rossdale, J., Brown, W., Burnett, T.A., Komber, H.M.E.I., Thompson, C., Robinson, G., MacKenzie Ross, R., Suntharalingam, J., and Rodrigues, J.C.L.
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- 2022
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30. The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. III. Optical and UV Spectra of a Blue Kilonova From Fast Polar Ejecta
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Nicholl, M., Berger, E., Kasen, D., Metzger, B. D., Elias, J., Briceno, C., Alexander, K. D., Blanchard, P. K., Chornock, R., Cowperthwaite, P. S., Eftekhari, T., Fong, W., Margutti, R., Villar, V. A., Williams, P. K. G., Brown, W., Annis, J., Bahramian, A., Brout, D., Brown, D. A., Chen, H. -Y., Clemens, J. C., Dennihy, E., Dunlap, B., Holz, D. E., Marchesini, E., Massaro, F., Moskowitz, N., Pelisoli, I., Rest, A., Ricci, F., Sako, M., Soares-Santos, M., and Strader, J.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Solar and Stellar Astrophysics - Abstract
We present optical and ultraviolet spectra of the first electromagnetic counterpart to a gravitational wave (GW) source, the binary neutron star merger GW170817. Spectra were obtained nightly between 1.5 and 9.5 days post-merger, using the SOAR and Magellan telescopes; the UV spectrum was obtained with the \textit{Hubble Space Telescope} at 5.5 days. Our data reveal a rapidly-fading blue component ($T\approx5500$ K at 1.5 days) that quickly reddens; spectra later than $\gtrsim 4.5$ days peak beyond the optical regime. The spectra are mostly featureless, although we identify a possible weak emission line at $\sim 7900$ \AA\ at $t\lesssim 4.5$ days. The colours, rapid evolution and featureless spectrum are consistent with a "blue" kilonova from polar ejecta comprised mainly of light $r$-process nuclei with atomic mass number $A\lesssim 140$. This indicates a sight-line within $\theta_{\rm obs}\lesssim 45^{\circ}$ of the orbital axis. Comparison to models suggests $\sim0.03$ M$_\odot$ of blue ejecta, with a velocity of $\sim 0.3c$. The required lanthanide fraction is $\sim 10^{-4}$, but this drops to $<10^{-5}$ in the outermost ejecta. The large velocities point to a dynamical origin, rather than a disk wind, for this blue component, suggesting that both binary constituents are neutron stars (as opposed to a binary consisting of a neutron star and a black hole). For dynamical ejecta, the high mass favors a small neutron star radius of $\lesssim 12$ km. This mass also supports the idea that neutron star mergers are a major contributor to $r$-process nucleosynthesis., Comment: ApJL, in press (GW170817, LVC)
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- 2017
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31. Rural EMS STEMI Patients – Why the Delay to PCI?
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Stopyra, Jason P., Snavely, Anna C., Ashburn, Nicklaus P., Supples, Michael W., Brown, W. Mark, Miller, Chadwick D., and Mahler, Simon A.
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VITAL signs ,OXYGEN saturation ,RESEARCH funding ,ACADEMIC medical centers ,QUALITATIVE research ,CHEST pain ,HYPERTENSION ,SEX distribution ,LOGISTIC regression analysis ,KRUSKAL-Wallis Test ,TRAVEL ,EMERGENCY medical services ,TREATMENT effectiveness ,TERTIARY care ,CARDIOVASCULAR diseases risk factors ,DESCRIPTIVE statistics ,MULTIVARIATE analysis ,AGE distribution ,MYOCARDIAL reperfusion ,LONGITUDINAL method ,ELECTROCARDIOGRAPHY ,ODDS ratio ,RURAL population ,PERCUTANEOUS coronary intervention ,ELECTRONIC health records ,TREATMENT delay (Medicine) ,PULSE (Heart beat) ,HEALTH equity ,BLOOD pressure ,DATA analysis software ,CONFIDENCE intervals ,TUMORS ,ST elevation myocardial infarction ,TIME ,TRANSPORTATION of patients ,DIABETES ,CARDIAC catheterization - Abstract
Background: The objective of this study is to identify patient and EMS agency factors associated with timely reperfusion of patients with ST-elevation myocardial infarction (STEMI). Methods: We conducted a cohort study of adult patients (≥18 years old) with STEMI activations from 2016 to 2020. Data was obtained from a regional STEMI registry, which included eight rural county EMS agencies and three North Carolina percutaneous coronary intervention (PCI) centers. On each patient, prehospital and in-hospital time intervals were abstracted. The primary outcome was the ability to achieve the 90-minute EMS FMC to PCI time goal (yes vs. no). We used generalized estimating equations accounting for within-agency clustering to evaluate the association between patient and agency factors and meeting first medical contact (FMC) to PCI time goal while accounting for clustering within the agency. Results: Among 365 rural STEMI patients 30.1% were female (110/365) with a mean age of 62.5 ± 12.7 years. PCI was performed within the time goal in 60.5% (221/365) of encounters. The FMC to PCI time goal was met in 45.5% (50/110) of women vs 69.8% (178/255) of men (p < 0.001). The median PCI center activation time was 12 min (IQR 7–19) in the group that received PCI within the time goal compared to 21 min (IQR 10–37) in the cohort that did not. After adjusting for loaded mileage and other clinical variables (e.g., pulse rate, hypertension etc.), the male sex was associated with an improved chance of meeting the goal of FMC to PCI (aOR: 2.94; 95% CI 2.11–4.10) compared to the female sex. Conclusion: Nearly 40% of rural STEMI patients transported by EMS failed to receive FMC to PCI within 90 min. Women were less likely than men to receive reperfusion within the time goal, which represents an important health care disparity. [ABSTRACT FROM AUTHOR]
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- 2024
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32. US Traffic Sign Recognition Using CNNs
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Brown, W. Shannon, Roy, Kaushik, Yuan, Xiaohong, Kacprzyk, Janusz, Series Editor, Pal, Nikhil R., Advisory Editor, Bello Perez, Rafael, Advisory Editor, Corchado, Emilio S., Advisory Editor, Hagras, Hani, Advisory Editor, Kóczy, László T., Advisory Editor, Kreinovich, Vladik, Advisory Editor, Lin, Chin-Teng, Advisory Editor, Lu, Jie, Advisory Editor, Melin, Patricia, Advisory Editor, Nedjah, Nadia, Advisory Editor, Nguyen, Ngoc Thanh, Advisory Editor, Wang, Jun, Advisory Editor, Arai, Kohei, editor, Kapoor, Supriya, editor, and Bhatia, Rahul, editor
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- 2021
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33. LAMMPS - a flexible simulation tool for particle-based materials modeling at the atomic, meso, and continuum scales
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Thompson, Aidan P., Aktulga, H. Metin, Berger, Richard, Bolintineanu, Dan S., Brown, W. Michael, Crozier, Paul S., in 't Veld, Pieter J., Kohlmeyer, Axel, Moore, Stan G., Nguyen, Trung Dac, Shan, Ray, Stevens, Mark J., Tranchida, Julien, Trott, Christian, and Plimpton, Steven J.
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- 2022
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34. Genetic and maternal predictors of cognitive and behavioral trajectories in females with fragile X syndrome
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del Hoyo Soriano, Laura, Thurman, Angela John, Harvey, Danielle Jenine, Ted Brown, W, and Abbeduto, Leonard
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Biomedical and Clinical Sciences ,Neurosciences ,Rare Diseases ,Fragile X Syndrome ,Pediatric ,Intellectual and Developmental Disabilities (IDD) ,Mind and Body ,Brain Disorders ,Behavioral and Social Science ,Basic Behavioral and Social Science ,Mental Health ,Mental health ,Adolescent ,Anxiety ,Female ,Gene-Environment Interaction ,Humans ,Intelligence ,Longitudinal Studies ,Phenotype ,Prospective Studies ,Females with FXS ,Ratio of affected to total chromosomes ,FMRP ,Maternal psychological distress ,Closeness in the mother-child relationship ,Fluid intelligence ,Crystallized intelligence ,Withdrawal ,Longitudinal ,Closeness in the mother–child relationship ,Psychology - Abstract
BackgroundFragile X syndrome (FXS) is caused by a mutation in the FMR1 gene on the X chromosome, leading to decreased levels of FMR1 protein (FMRP), which causes the array of neuropsychological impairments that define FXS. Because FXS is an X-linked condition, fewer females display FXS and females with FXS are more mildly affected than males, on average. However, there is a considerable variability in terms of severity of affectedness among females with FXS. The current study was designed to investigate potential genetic (FMRP level and ratio of affected to total chromosomes) and environmental factors (maternal psychological distress and closeness in the mother-child relationship) influencing the cognitive (fluid and crystallized intelligence) and behavioral (anxiety and withdrawal) phenotype of females with FXS.MethodsWe conducted a prospective 3-year longitudinal study of 16 females with FXS (with up to four assessments, each separated by a year) using an accelerated longitudinal design so that we had coverage of the age range of 10-15 years at study start and 13-18 at study end. We focused on both the level of functioning related to chronological age expectations (standard scores) and absolute change in skill (raw scores) over the 3-year period.ResultsAt a cross-sectional level, fluid intelligence and crystallized intelligence were both predicted by a closer mother-child relationship and lower maternal psychological distress. However, only fluid intelligence was predicted by a lower ratio of affected to total chromosomes. Anxiety and withdrawal were predicted by a higher ratio of affected to total chromosomes. Withdrawal was also predicted by lower closeness in the mother-child relationship and higher maternal distress. In terms of longitudinal change, gains were observed in fluid and crystallized intelligence, whereas anxious and withdrawn behaviors remained stable over visits. Gains in fluid intelligence were solely predicted by FXS biomarkers (higher FMRP level and lower ratio of affected to total chromosomes), while gains in crystallized intelligence were not predicted by any of the biological and environmental variables.ConclusionsOur results show that FXS biomarkers and maternal variables contribute differentially to the cognitive and behavioral features of the adolescent female with FXS. These findings can help in the design of treatment studies aimed at enhancing cognitive and behavioral abilities in the FXS population.
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- 2018
35. PKS-NRPS Enzymology and Structural Biology: Considerations in Protein Production.
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Skiba, Meredith, Maloney, Finn, Dan, Qingyun, Fraley, Amy, Aldrich, Courtney, Smith, Janet, and Brown, W
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Chaperones ,Coexpression ,Cyanobacteria ,Nonribosomal peptide synthetase ,Polyketide synthase ,Protein crystallization ,Protein folding ,Protein production ,Protein purification ,Protein solubility ,Acyl Carrier Protein ,Bacteria ,Bacterial Outer Membrane Proteins ,Cloning ,Molecular ,Codon ,Crystallization ,Culture Media ,Escherichia coli ,Escherichia coli Proteins ,Peptide Synthases ,Plasmids ,Polyketide Synthases ,Promoter Regions ,Genetic ,Protein Domains ,Protein Engineering ,Recombinant Proteins - Abstract
The structural diversity and complexity of marine natural products have made them a rich and productive source of new bioactive molecules for drug development. The identification of these new compounds has led to extensive study of the protein constituents of the biosynthetic pathways from the producing microbes. Essential processes in the dissection of biosynthesis have been the elucidation of catalytic functions and the determination of 3D structures for enzymes of the polyketide synthases and nonribosomal peptide synthetases that carry out individual reactions. The size and complexity of these proteins present numerous difficulties in the process of going from gene to structure. Here, we review the problems that may be encountered at the various steps of this process and discuss some of the solutions devised in our and other labs for the cloning, production, purification, and structure solution of complex proteins using Escherichia coli as a heterologous host.
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- 2018
36. Employment status at transplant influences ethnic disparities in outcomes after deceased donor kidney transplantation
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Divers, Jasmin, Mohan, Sumit, Brown, W. Mark, Pastan, Stephen O., Israni, Ajay K., Gaston, Robert S., Bray, Robert, Islam, Shahidul, Sakhovskaya, Natalia V., Mena-Gutierrez, Alejandra M., Reeves-Daniel, Amber M., Julian, Bruce A., and Freedman, Barry I.
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- 2022
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37. Challenges and potential solutions to enrollment in a clinical trial of AVF vs AVG vascular access strategy
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Goldman, Matthew P., primary, Patel, Dipal M., additional, Chang, Kevin Z., additional, Davis, Ross P., additional, Edwards, Matthew S., additional, Hurie, Justin B., additional, Sutsrim, Ashlee, additional, Velazquez-Ramirez, Gabriela, additional, Williams, Timothy K., additional, Grandas, Oscar H., additional, Freeman, Michael B., additional, McNally, Michael M., additional, Stevens, Scott L., additional, Bennett, Kyla M., additional, Woo, Karen, additional, Carsten, Christopher G., additional, Androes, Mark P., additional, Blas, Joseph-Vincent V., additional, Jones, Brian, additional, Patton, R. Michael, additional, Parr, Rachel, additional, Gandhi, Sagar S., additional, York, John W., additional, Young, Carlton J., additional, Rabbani, Muhammad U., additional, Gardezi, Ali I., additional, Abdelnour, Lama M., additional, Lee, Timmy, additional, Abusalah, Wala M., additional, Zayas, Carlos F., additional, Hicks, Caitlin W., additional, Geetha, Duvuru, additional, Brown, W. Mark, additional, Chen, Haiying, additional, Allon, Michael, additional, and Murea, Mariana, additional
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- 2024
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38. Going the distance : Estimating the effect of provincial borders on trade when geography (and everything else) matters
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Bemrose, Robby K., Brown, W. Mark, and Tweedle, Jesse
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- 2020
39. Mixing properties of stochastic quantum Hamiltonians
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Onorati, E., Buerschaper, O., Kliesch, M., Brown, W., Werner, A. H., and Eisert, J.
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Quantum Physics ,High Energy Physics - Theory ,Mathematical Physics - Abstract
Random quantum processes play a central role both in the study of fundamental mixing processes in quantum mechanics related to equilibration, thermalisation and fast scrambling by black holes, as well as in quantum process design and quantum information theory. In this work, we present a framework describing the mixing properties of continuous-time unitary evolutions originating from local Hamiltonians having time-fluctuating terms, reflecting a Brownian motion on the unitary group. The induced stochastic time evolution is shown to converge to a unitary design. As a first main result, we present bounds to the mixing time. By developing tools in representation theory, we analytically derive an expression for a local k-th moment operator that is entirely independent of k, giving rise to approximate unitary k-designs and quantum tensor product expanders. As a second main result, we introduce tools for proving bounds on the rate of decoupling from an environment with random quantum processes. By tying the mathematical description closely with the more established one of random quantum circuits, we present a unified picture for analysing local random quantum and classes of Markovian dissipative processes, for which we also discuss applications., Comment: 35 pages, 2 figures, replaced by final version for the Communications in Mathematical Physics
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- 2016
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40. The Pierre Auger Observatory Upgrade - Preliminary Design Report
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The Pierre Auger Collaboration, Aab, A., Abreu, P., Aglietta, M., Ahn, E. J., Samarai, I. Al, Albuquerque, I. F. M., Allekotte, I., Allison, P., Almela, A., Castillo, J. Alvarez, Alvarez-Muñiz, J., Batista, R. Alves, Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Aramo, C., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. M., Barber, K. B., Bäuml, J., Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Blaess, S. G., Blanco, A., Blanco, M., Blazek, J., Bleve, C., Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, B., Caccianiga, L., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. G., Chiavassa, A., Chinellato, J. A., Chudoba, J., Cilmo, M., Clay, R. W., Cocciolo, G., Colalillo, R., Coleman, A., Collica, L., Coluccia, M. R., Conceição, R., Contreras, F., Cooper, M. J., Cordier, A., Coutu, S., Covault, C. E., Cronin, J., Dallier, R., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., de Almeida, R. M., de Jong, S. J., De Mauro, G., Neto, J. R. T. de Mello, De Mitri, I., de Oliveira, J., de Souza, V., del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Di Matteo, A., Diaz, J. C., Castro, M. L. Díaz, Diogo, F., Dobrigkeit, C., Docters, W., D'Olivo, J. C., Dorofeev, A., Hasankiadeh, Q. Dorosti, Dova, M. T., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Falcke, H., Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Ferguson, A. P., Fernandes, M., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fox, B. D., Fratu, O., Freire, M. M., Fuchs, B., Fujii, T., García, B., Garcia-Pinto, D., Gate, F., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glass, H., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, González, N., Gookin, B., Gordon, J., Gorgi, A., Gorham, P., Gouffon, P., Griffith, N., Grillo, A. F., Grubb, T. D., Guarino, F., Guedes, G. P., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Hartmann, S., Harton, J. L., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hemery, N., Herve, A. E., Hill, G. C., Hojvat, C., Hollon, N., Holt, E., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huber, D., Huege, T., Insolia, A., Isar, P. G., Jandt, I., Jansen, S., Jarne, C., Johnsen, J. A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. H., Kasper, P., Katkov, I., Kégl, B., Keilhauer, B., Keivani, A., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Krömer, O., Kuempel, D., Mezek, G. Kukec, Kunka, N., LaHurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, P., Coz, S. Le, Lebrun, D., Lebrun, P., de Oliveira, M. A. Leigui, Letessier-Selvon, A., Lhenry-Yvon, I., Link, K., Lopes, L., López, R., Casado, A. López, Louedec, K., Lu, L., Lucero, A., Malacari, M., Maldera, S., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. G., Marin, V., Mariş, I. C., Marsella, G., Martello, D., Martin, L., Martinez, H., Bravo, O. Martínez, Martraire, D., Meza, J. J. Masías, Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Maurizio, D., Mayotte, E., Mazur, P. O., Medina, C., Medina-Tanco, G., Meissner, R., Mello, V. B. B., Melo, D., Menshikov, A., Messina, S., Meyhandan, R., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Molina-Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Moura, C. A., Muller, M. A., Müller, G., Müller, S., Mussa, R., Navarra, G., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Ochilo, L., Oikonomou, F., Olinto, A., Pacheco, N., Selmi-Dei, D. Pakk, Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pȩkala, J., Pelayo, R., Pepe, I. M., Perrone, L., Petermann, E., Peters, C., Petrera, S., Petrov, Y., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porcelli, A., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Purrello, V., Quel, E. J., Querchfeld, S., Quinn, S., Rautenberg, J., Ravel, O., Ravignani, D., Reinert, D., Revenu, B., Ridky, J., Riggi, S., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigues, Fernandez, G. Rodriguez, Rojo, J. Rodriguez, Rodríguez-Frías, M. D., Rogozin, D., Rosado, J., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Greus, F. Salesa, Salina, G., Sánchez, F., Sanchez-Lucas, P., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sarmento, R., Sato, R., Scarso, C., Schauer, M., Scherini, V., Schieler, H., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schröder, F. G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. J., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. C., Sidelnik, I., Sigl, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. R., Sommers, P., Sorokin, J., Squartini, R., Srivastava, Y. N., Stanca, D., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A. D., Sutherland, M. S., Swain, J., Szadkowski, Z., Taborda, O. A., Tapia, A., Tepe, A., Theodoro, V. M., Timmermans, C., Peixoto, C. J. Todero, Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Elipe, G. Torralba, Machado, D. Torres, Travnicek, P., Trini, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdés, Valiño, I., Valore, L., van Aar, G., van Bodegom, P., Berg, A. M. van den, van Velzen, S., van Vliet, A., Varela, E., Cárdenas, B. Vargas, Varner, G., Vasquez, R., Vázquez, J. R., Vázquez, R. A., Veberič, D., Verzi, V., Vicha, J., Videla, M., Villaseñor, L., Vlcek, B., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Widom, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yapici, T., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zhu, Y., Zimmermann, B., Ziolkowski, M., Zong, Z., and Zuccarello, F.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
The Pierre Auger Observatory has begun a major Upgrade of its already impressive capabilities, with an emphasis on improved mass composition determination using the surface detectors of the Observatory. Known as AugerPrime, the upgrade will include new 4 m$^2$ plastic scintillator detectors on top of all 1660 water-Cherenkov detectors, updated and more flexible surface detector electronics, a large array of buried muon detectors, and an extended duty cycle for operations of the fluorescence detectors. This Preliminary Design Report was produced by the Collaboration in April 2015 as an internal document and information for funding agencies. It outlines the scientific and technical case for AugerPrime. We now release it to the public via the arXiv server. We invite you to review the large number of fundamental results already achieved by the Observatory and our plans for the future., Comment: 201 pages
- Published
- 2016
41. Experimentally accessible witnesses of many-body localisation
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Goihl, M., Friesdorf, M., Werner, A. H., Brown, W., and Eisert, J.
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Condensed Matter - Quantum Gases ,Condensed Matter - Statistical Mechanics ,Quantum Physics - Abstract
The phenomenon of many-body localised (MBL) systems has attracted significant interest in recent years, for its intriguing implications from a perspective of both condensed-matter and statistical physics: they are insulators even at non-zero temperature and fail to thermalise, violating expectations from quantum statistical mechanics. What is more, recent seminal experimental developments with ultra-cold atoms in optical lattices constituting analog quantum simulators have pushed many-body localised systems into the realm of physical systems that can be measured with high accuracy. In this work, we introduce experimentally accessible witnesses that directly probe distinct features of MBL, distinguishing it from its Anderson counterpart. We insist on building our toolbox from techniques available in the laboratory, including on-site addressing, super-lattices, and time-of-flight measurements, identifying witnesses based on fluctuations, density-density correlators, densities, and entanglement. We build upon the theory of out of equilibrium quantum systems, in conjunction with tensor network and exact simulations, showing the effectiveness of the tools for realistic models., Comment: 7 pages, 4 figures, small changes, references added, new Appendix on bosonic Hamiltonian with on-site interaction, detailed discussion of papers by the Greiner group added
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- 2016
42. Reduced vagal tone in women with the FMR1 premutation is associated with FMR1 mRNA but not depression or anxiety
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Klusek, Jessica, LaFauci, Giuseppe, Adayev, Tatyana, Brown, W Ted, Tassone, Flora, and Roberts, Jane E
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Biomedical and Clinical Sciences ,Neurosciences ,Mind and Body ,Clinical Research ,Depression ,Rare Diseases ,Fragile X Syndrome ,Intellectual and Developmental Disabilities (IDD) ,Behavioral and Social Science ,Mental Health ,Brain Disorders ,Genetics ,Mental health ,Fragile X carriers ,Vagal tone ,Heart rate ,Physiological arousal ,FMRP ,FMR1 mRNA ,Psychology - Abstract
BackgroundAutonomic dysfunction is implicated in a range of psychological conditions, including depression and anxiety. The fragile X mental retardation-1 (FMR1) premutation is a common genetic mutation that affects ~1:150 women and is associated with psychological vulnerability. This study examined cardiac indicators of autonomic function among women with the FMR1 premutation and control women as potential biomarkers for psychological risk that may be linked to FMR1.MethodsBaseline inter-beat interval and respiratory sinus arrhythmia (a measure of parasympathetic vagal tone) were measured in 35 women with the FMR1 premutation and 28 controls. The women completed anxiety and depression questionnaires. FMR1 genetic indices (i.e., CGG repeat, quantitative FMRP, FMR1 mRNA, activation ratio) were obtained for the premutation group.ResultsRespiratory sinus arrhythmia was reduced in the FMR1 premutation group relative to controls. While depression symptoms were associated with reduced respiratory sinus arrhythmia among control women, these variables were unrelated in the FMR1 premutation. Elevated FMR1 mRNA was associated with higher respiratory sinus arrhythmia.ConclusionsWomen with the FMR1 premutation demonstrated autonomic dysregulation characterized by reduced vagal tone. Unlike patterns observed in the general population and in study controls, vagal activity and depression symptoms were decoupled in women with the FMR1 premutation, suggesting independence between autonomic regulation and psychopathological symptoms that is atypical and potentially specific to the FMR1 premutation. The association between vagal tone and mRNA suggests that molecular variation associated with FMR1 plays a role in autonomic regulation.
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- 2017
43. Fragile X targeted pharmacotherapy: lessons learned and future directions
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Erickson, Craig A, Davenport, Matthew H, Schaefer, Tori L, Wink, Logan K, Pedapati, Ernest V, Sweeney, John A, Fitzpatrick, Sarah E, Brown, W Ted, Budimirovic, Dejan, Hagerman, Randi J, Hessl, David, Kaufmann, Walter E, and Berry-Kravis, Elizabeth
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Pharmacology and Pharmaceutical Sciences ,Biomedical and Clinical Sciences ,Fragile X Syndrome ,Intellectual and Developmental Disabilities (IDD) ,Pediatric ,Clinical Trials and Supportive Activities ,Neurosciences ,Brain Disorders ,Orphan Drug ,Clinical Research ,Rare Diseases ,Behavioral and Social Science ,Development of treatments and therapeutic interventions ,Evaluation of treatments and therapeutic interventions ,5.1 Pharmaceuticals ,6.1 Pharmaceuticals ,Fragile X syndrome ,Translational treatment ,Targeted treatments ,Drug development ,Genetic disorder ,Psychology - Abstract
Our understanding of fragile X syndrome (FXS) pathophysiology continues to improve and numerous potential drug targets have been identified. Yet, current prescribing practices are only symptom-based in order to manage difficult behaviors, as no drug to date is approved for the treatment of FXS. Drugs impacting a diversity of targets in the brain have been studied in recent FXS-specific clinical trials. While many drugs have focused on regulation of enhanced glutamatergic or deficient GABAergic neurotransmission, compounds studied have not been limited to these mechanisms. As a single-gene disorder, it was thought that FXS would have consistent drug targets that could be modulated with pharmacotherapy and lead to significant improvement. Unfortunately, despite promising results in FXS animal models, translational drug treatment development in FXS has largely failed. Future success in this field will depend on learning from past challenges to improve clinical trial design, choose appropriate outcome measures and age range choices, and find readily modulated drug targets. Even with many negative placebo-controlled study results, the field continues to move forward exploring both the new mechanistic drug approaches combined with ways to improve trial execution. This review summarizes the known phenotype and pathophysiology of FXS and past clinical trial rationale and results, and discusses current challenges facing the field and lessons from which to learn for future treatment development efforts.
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- 2017
44. Noncomprehension Signaling in Males and Females With Fragile X Syndrome
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Thurman, Angela John, Kover, Sara T, Brown, W Ted, Harvey, Danielle J, and Abbeduto, Leonard
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Intellectual and Developmental Disabilities (IDD) ,Pediatric ,Clinical Research ,Rare Diseases ,Fragile X Syndrome ,Brain Disorders ,Adolescent ,Autistic Disorder ,Child ,Child ,Preschool ,Communication ,Comprehension ,Female ,Humans ,Intelligence ,Language ,Male ,Prospective Studies ,Psychological Tests ,Severity of Illness Index ,Sex Factors ,Speech Perception ,Superior Sagittal Sinus ,Clinical Sciences ,Cognitive Sciences ,Linguistics ,Speech-Language Pathology & Audiology - Abstract
PurposeThis study used a prospective longitudinal design to evaluate the trajectory and predictors of noncomprehension signaling in male and female youth with fragile X syndrome (FXS).MethodA direction-following task in which some of the directions were inadequate was administered. Participants were 52 youth (36 boys, 16 girls) with FXS. Upon study entry, participants ranged from 10 to 16 years. The average number of annual assessments per participant was 3.65 (range = 1-4), providing 198 data points for analysis.ResultsParticipants with FXS were less likely to signal noncomprehension than younger, typically developing, cognitively matched children. The average rate of change in noncomprehension signaling was not significantly different from 0 for either boys or girls, suggesting a plateau. Both FMRP and nonverbal IQ were significant independent predictors of noncomprehension signaling for boys. Variability in noncomprehension signaling among girls was not explained by any of the predictors, but trends similar to those observed for boys were observed.ConclusionsNoncomprehension signaling appears to be an area of weakness for individuals with FXS. Because the failure to signal noncomprehension can have negative, cumulative effects on comprehension, the results suggest a need for interventions targeting the requisite cognitive skills.
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- 2017
45. Analysis of Whole Exome Sequencing with Cardiometabolic Traits Using Family‐Based Linkage and Association in the IRAS Family Study
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Tabb, Keri L, Hellwege, Jacklyn N, Palmer, Nicholette D, Dimitrov, Latchezar, Sajuthi, Satria, Taylor, Kent D, Ng, Maggie CY, Hawkins, Gregory A, Chen, Yii‐der Ida, Brown, W Mark, McWilliams, David, Williams, Adrienne, Lorenzo, Carlos, Norris, Jill M, Long, Jirong, Rotter, Jerome I, Curran, Joanne E, Blangero, John, Wagenknecht, Lynne E, Langefeld, Carl D, and Bowden, Donald W
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Biological Sciences ,Genetics ,Human Genome ,Clinical Research ,Biotechnology ,Aetiology ,2.1 Biological and endogenous factors ,Good Health and Well Being ,Adiponectin ,Adolescent ,Adult ,Aged ,Aged ,80 and over ,Atherosclerosis ,Exome ,Female ,Gene Frequency ,Genetic Predisposition to Disease ,Genome-Wide Association Study ,Humans ,Insulin Resistance ,Lipids ,Lod Score ,Male ,Middle Aged ,Polymorphism ,Single Nucleotide ,Sequence Analysis ,DNA ,Young Adult ,Cohort study ,genetic variance ,Hispanic ,novel variants ,Clinical Sciences ,Genetics & Heredity - Abstract
Family-based methods are a potentially powerful tool to identify trait-defining genetic variants in extended families, particularly when used to complement conventional association analysis. We utilized two-point linkage analysis and single variant association analysis to evaluate whole exome sequencing (WES) data from 1205 Hispanic Americans (78 families) from the Insulin Resistance Atherosclerosis Family Study. WES identified 211,612 variants above the minor allele frequency threshold of ≥0.005. These variants were tested for linkage and/or association with 50 cardiometabolic traits after quality control checks. Two-point linkage analysis yielded 10,580,600 logarithm of the odds (LOD) scores with 1148 LOD scores ≥3, 183 LOD scores ≥4, and 29 LOD scores ≥5. The maximal novel LOD score was 5.50 for rs2289043:T>C, in UNC5C with subcutaneous adipose tissue volume. Association analysis identified 13 variants attaining genome-wide significance (P T in APOA5 and triglyceride levels (P = 3.67 × 10-10 ). Overall, there was a 5.2-fold increase in the number of informative variants detected by WES compared to exome chip analysis in this population, nearly 30% of which were novel variants relative to the Database of Single Nucleotide Polymorphisms (dbSNP) build 138. Thus, integration of results from two-point linkage and single-variant association analysis from WES data enabled identification of novel signals potentially contributing to cardiometabolic traits.
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- 2017
46. (Epi)genetic variants of the sarcomere-desmosome are associated with premature utero-contraction in spontaneous preterm labor
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Wang, Jie, Luo, Xiucui, Pan, Jing, Dong, Xiaoyan, Tian, Xiujuan, Tu, Zhihua, Ju, Weina, Zhang, Meijiao, Zhong, Mei, De Chen, Charles, Flory, Michael, Wang, Yong, Ted Brown, W., and Zhong, Nanbert
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- 2021
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47. Man in the Universe : Some Continuities in Indian Thought
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BROWN, W. NORMAN and BROWN, W. NORMAN
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- 2023
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48. SDSS J1152+0248: An eclipsing double white dwarf from the Kepler K2 campaign
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Hallakoun, N., Maoz, D., Kilic, M., Mazeh, T., Gianninas, A., Agol, E., Bell, K. J., Bloemen, S., Brown, W. R., Debes, J., Faigler, S., Kull, I., Kupfer, T., Loeb, A., Morris, B. M., and Mullally, F.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We report the discovery of the sixth known eclipsing double white dwarf (WD) system, SDSS J1152+0248, with a 2.3968 +/- 0.0003 h orbital period, in data from the Kepler Mission's K2 continuation. Analysing and modelling the K2 data together with ground-based fast photometry, spectroscopy, and radial-velocity measurements, we determine that the primary is a DA-type WD with mass M1 = 0.47 +/- 0.11 Msun, radius R1 = 0.0197 +/- 0.0035 Rsun, and cooling age t1 = 52 +/- 36 Myr. No lines are detected, to within our sensitivity, from the secondary WD, but it is likely also of type DA. Its central surface brightness, as measured from the secondary eclipse, is 0.31 of the primary's surface brightness. Its mass, radius, and cooling age, respectively, are M2 = 0.44 +/- 0.09 Msun, R2 = 0.0223 +0.0064 -0.0050 Rsun, and t2 = 230 +/- 100 Myr. SDSS J1152+0248 is a near twin of the double-lined eclipsing WD system CSS 41177., Comment: MNRAS, accepted
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- 2015
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49. Phase III Randomized, Placebo-Controlled Clinical Trial of Donepezil for Treatment of Cognitive Impairment in Breast Cancer Survivors After Adjuvant Chemotherapy (WF-97116).
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Rapp, Stephen R., Dressler, Emily V., Brown, W. Mark, Wade III, James L., Le-Lindqwister, Nguyet, King, David, Rowland, Kendrith M., Weaver, Kathryn E., Klepin, Heidi D., Shaw, Edward G., and Lesser, Glenn J.
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- 2024
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50. Safety, efficacy, and hemodynamic performance of a stented bovine pericardial aortic valve bioprosthesis: Two-year analysis
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Dagenais, François, Moront, Michael G., Brown, W. Morris, Reardon, Michael J., Chu, Michael W.A., Gearhart, Elizabeth, and Klautz, Robert J.M.
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- 2020
- Full Text
- View/download PDF
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