6,279 results on '"Mohan, V."'
Search Results
302. Interview With Michelle Dunlap—Master Black Belt, Quality Champion
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Strodtbeck, George K., primary and Tatikonda, Mohan V., additional
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- 2019
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303. Interview With Tom Linebarger—Cummins CEO (2012+)
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Strodtbeck, George K., primary and Tatikonda, Mohan V., additional
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- 2019
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304. Special Situations
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Strodtbeck, George K., primary and Tatikonda, Mohan V., additional
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- 2019
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305. Six Sigma Pre-history
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Strodtbeck, George K., primary and Tatikonda, Mohan V., additional
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- 2019
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306. The Effect of Maturity on Organizational Communication
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Strodtbeck, George K., primary and Tatikonda, Mohan V., additional
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- 2019
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307. S-Curve 2—Launch and First Projects
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Strodtbeck, George K., primary and Tatikonda, Mohan V., additional
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- 2019
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308. Interview With Joe Loughrey—Cummins President & COO (2005–2008)
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Strodtbeck, George K., primary and Tatikonda, Mohan V., additional
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- 2019
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309. Fabrication of seed ball rolling machine.
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Arunraj, P. V., Ali, H. Mohammed, Praveen, G. S., Vignesh, D., Mohan, V. S. Vijay, and Mukil, R. V.
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FOOD supply ,AGRICULTURE ,SEEDS ,ECONOMIC equilibrium ,RESTORATION ecology - Abstract
The primary source of old is agriculture. Additionally, this industry contributes the country's economic stability and creates jobs. It is important to maintain a steady supply of food as the population grows. In order to do this, agricultural activities might be mechanized. Making and planting seed balls is one way to quickly and cheaply restore the earth's lost green cover for ecological restoration. However, manual seed ball manufacture and distribution are more time demanding and more expensive. Because of this, the goal is to develop a machine thatcan produce vast amounts of seed balls quickly and easily. [ABSTRACT FROM AUTHOR]
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- 2023
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310. Plasma Polymerization: Electronics and Biomedical Application
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Kumar, Avishek, Grant, Daniel, Alancherry, Surjith, Al-Jumaili, Ahmed, Bazaka, Kateryna, Jacob, Mohan V., and Rawat, Rajdeep Singh, editor
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- 2017
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311. Hurdles in Brown Rice Consumption
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Mohan, V., Ruchi, V., Gayathri, R., Ramya Bai, M., Shobana, S., Anjana, R. M., Unnikrishnan, R., Sudha, V., Manickavasagan, Annamalai, editor, Santhakumar, Chandini, editor, and Venkatachalapathy, N., editor
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- 2017
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312. Glycaemic Properties of Brown Rice
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Shobana, S., Jayanthan, M., Sudha, V., Unnikrishnan, R., Anjana, R. M., Mohan, V., Manickavasagan, Annamalai, editor, Santhakumar, Chandini, editor, and Venkatachalapathy, N., editor
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- 2017
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313. South Asian medical cohorts reveal strong founder effects and high rates of homozygosity
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Wall, Jeffrey D, Sathirapongsasuti, J Fah, Gupta, Ravi, Rasheed, Asif, Venkatesan, Radha, Belsare, Saurabh, Menon, Ramesh, Phalke, Sameer, Mittal, Anuradha, Fang, John, Tanneeru, Deepak, Deshmukh, Manjari, Bassi, Akshi, Robinson, Jacqueline, Chaudhary, Ruchi, Murugan, Sakthivel, Ul-Asar, Zameer, Saleem, Imran, Ishtiaq, Unzila, Fatima, Areej, Sheikh, Saqib Shafi, Hameed, Shahid, Ishaq, Mohammad, Rasheed, Syed Zahed, Memon, Fazal-Ur-Rehman, Jalal, Anjum, Abbas, Shahid, Frossard, Philippe, Fuchsberger, Christian, Forer, Lukas, Schoenherr, Sebastian, Bei, Qixin, Bhangale, Tushar, Tom, Jennifer, Gadde, Santosh Gopi Krishna, B V, Priya, Naik, Naveen Kumar, Wang, Minxian, Kwok, Pui-Yan, Khera, Amit V, Lakshmi, BR, Butterworth, Adam S, Chowdhury, Rajiv, Danesh, John, di Angelantonio, Emanuele, Naheed, Aliya, Goyal, Vinay, Kandadai, Rukmini M, Kumar, Hrishikesh, Borgohain, Rupam, Mukherjee, Adreesh, Wadia, Pettarusp M, Yadav, Ravi, Desai, Soaham, Kumar, Niraj, Biswas, Atanu, Pal, Pramod Kumar, Muthane, Uday B, Das, Shymal K, Ramprasad, Vedam L, Kukkle, Prashanth L, Seshagiri, Somasekar, Kathiresan, Sekar, Ghosh, Arkasubhra, Mohan, V, Saleheen, Danish, Stawiski, Eric W, Peterson, Andrew S, Wall, Jeffrey D [0000-0001-5066-1235], Venkatesan, Radha [0000-0002-4281-0250], Belsare, Saurabh [0000-0002-8148-1867], Fang, John [0000-0003-2372-0839], Bassi, Akshi [0000-0002-4443-1430], Robinson, Jacqueline [0000-0002-5556-815X], Forer, Lukas [0000-0003-2139-7329], Wang, Minxian [0000-0002-3753-508X], Kwok, Pui-Yan [0000-0002-5087-3059], Khera, Amit V [0000-0001-6535-5839], Butterworth, Adam S [0000-0002-6915-9015], Desai, Soaham [0000-0003-0378-1888], Kumar, Niraj [0000-0002-5863-2532], Kukkle, Prashanth L [0000-0002-4610-947X], Mohan, V [0000-0001-5038-6210], Saleheen, Danish [0000-0001-6193-020X], Stawiski, Eric W [0000-0002-9387-6719], and Apollo - University of Cambridge Repository
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Bangladesh ,Homozygote ,Human Genome ,India ,Founder Effect ,Good Health and Well Being ,Asian People ,South Asian People ,Clinical Research ,Genetics ,Humans ,Pakistan ,Generic health relevance ,Biotechnology - Abstract
The benefits of large-scale genetic studies for healthcare of the populations studied are well documented, but these genetic studies have traditionally ignored people from some parts of the world, such as South Asia. Here we describe whole genome sequence (WGS) data from 4806 individuals recruited from the healthcare delivery systems of Pakistan, India and Bangladesh, combined with WGS from 927 individuals from isolated South Asian populations. We characterize population structure in South Asia and describe a genotyping array (SARGAM) and imputation reference panel that are optimized for South Asian genomes. We find evidence for high rates of reproductive isolation, endogamy and consanguinity that vary across the subcontinent and that lead to levels of rare homozygotes that reach 100 times that seen in outbred populations. Founder effects increase the power to associate functional variants with disease processes and make South Asia a uniquely powerful place for population-scale genetic studies.
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- 2023
314. Multiband optical monitoring of the blazars S5 0716+714 and BL Lacertae
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Stalin, C. S., Gopal-Krishna, Sagar, Ram, Wiita, Paul J., Mohan, V., and Pandey, A. K.
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Astrophysics - Abstract
We report results of multiband optical monitoring of two well known blazars, S5 0716+714 and BL Lacertae, carried out in 1996 and 2000-01 with an aim to study optical variations on time scales from minutes to hours and longer.The light curves were derived relative to comparison stars present on the CCD frames. Night to night flux variations of >0.1 mag were observed in S5 0716+714 during a campaign of ~2 weeks in 1996.A good correlation between the lightcurves in different optical bands was found for both inter-night and intra-night observations. Two prominent events of intra-night optical variability were detected in S5 0716+714.Each of these rapidly varying segments of the lightcurves trace an exponential flux profile whose rate of variation is the same in both cases. Our long-term monitoring data of S5 0716+714 showed a distinct flare around JD 2451875 which can be identified in the BVRI bands.This flare coincides with the brightest phase recorded during 1994-2001 in the long-term lightcurves reported by Raiteri et al.(2003). No evidence for the bluer when brighter trend was noticed on inter-night and intra-night time scales. On the other hand, our nearly simultaneous multiband observations of BL Lacertae in October 2001 showed flux variations that were not achromatic. This blazar was found to become bluer when brighter on intra-night time scales and there is a hint of the same trend on inter-night time scales. Based on five nights of observations during a week, BL Lacertae showed a peak night-to-night variability of ~0.6 mag in B. Thus, we found that the present observations of the two blazars, reveal a contrasting behaviour in terms of the dependence of spectral hardening with increasing brightness, at least on intra-night, and possibly also on inter-night, time scales., Comment: 11 pages with 10 figures,uses mn2e.cls, Accepted for publication in MNRAS. Tables 4 and 5 in full will be available in the electronic version of the article
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- 2005
315. Biodegradable optically transparent terpinen-4-ol thin films for marine antifouling applications
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Kumar, Avishek, Mills, Scott, Bazaka, Kateryna, Bajema, Nigel, Atkinson, Ian, and Jacob, Mohan V.
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- 2018
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316. Inter- and Intraobserver Reliability of Pelvic Obliquity Measurement Methods in Patients With Cerebral Palsy
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Shrader, M. Wade, Andrisevic, Emily M., Belthur, Mohan V., White, Gregory R., Boan, Carla, and Wood, William
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- 2018
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317. Isotherms, kinetics and mechanism analysis of phosphorus recovery from aqueous solution by calcium-rich biochar produced from biosolids via microwave pyrolysis
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Antunes, Elsa, Jacob, Mohan V., Brodie, Graham, and Schneider, Philip A.
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- 2018
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318. Microwave pyrolysis of sewage biosolids: Dielectric properties, microwave susceptor role and its impact on biochar properties
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Antunes, Elsa, Jacob, Mohan V., Brodie, Graham, and Schneider, Philip A.
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- 2018
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319. Dark halo baryons not in ancient halo white dwarfs
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Creze, M., Mohan, V., Robin, A. C., Reyle, C., Cracken, H. J. Mc, Cuillandre, J. -C., Fevre, O. Le, and Mellier, Y.
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Astrophysics - Abstract
Having ruled out the possibility that stellar objects are the main contributor of the dark matter embedding galaxies, microlensing experiments cannot exclude the hypothesis that a significant fraction of the Milky Way dark halo might be made of MACHOs with masses in the range $0.5-0.8 \msun$. Ancient white dwarfs are generally considered the most plausible candidates for such MACHOs. We report the results of a search for such white dwarfs in a proper motion survey covering a 0.16 sqd field at three epochs at high galactic latitude, and 0.938 sqd at two epochs at intermediate galactic latitude (VIRMOS survey), using the CFH telescope. Both surveys are complete to I = 23, with detection efficiency fading to 0 at I = 24.2. Proper motion data are suitable to separate unambiguously halo white dwarfs identified by belonging to a non rotating system. No candidates were found within the colour-magnitude-proper motion volume where such objects can be safely discriminated from any standard population as well as from possible artefacts. In the same volume, we estimate the maximum white dwarf halo fraction compatible with this observation at different significance levels if the halo is at least 14 gigayears old and under different ad hoc initial mass functions. Our data alone rules out a halo fraction greater than 14% at 95% confidence level. Combined with two previous investigations exploring comparable volumes pushes the limit below 4 % (95% confidence level) or below 1.3% (64% confidence), this implies that if baryonic dark matter is present in galaxy halos, it is not, or it is only marginally in the form of faint hydrogen white dwarfs., Comment: accepted in Astronomy and Astrophysics (19-05-2004)
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- 2004
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320. Is Law Still Grappling with Groundwater?
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Katarki, Mohan V.
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- 2021
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321. Compact Device Models for FinFET and Beyond.
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Darsen D. Lu, Mohan V. Dunga, Ali M. Niknejad, Chenming Hu, Fu-Xiang Liang, Wei-Chen Hung, Jia-Wei Lee, Chun-Hsiang Hsu, and Meng-Hsueh Chiang
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- 2020
322. GRB 030227: the first multiwavelength afterglow of an INTEGRAL GRB
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Castro-Tirado, A. J., Gorosabel, J., Guziy, S., Reverte, D., Cerón, J. M. Castro, Postigo, A. de Ugarte, Tanvir, N., Mereghetti, S., Tiengo, A., Buckle, J., Sagar, R., Pandey, S. B., Mohan, V., Masetti, N., Mannucci, F., Feltzing, S., Lundstrom, I., Pedersen, H., Riess, C., Trushkin, S., Vilchez, J., Lund, N., Brandt, S., Nunez, S. Martinez, Reglero, V., Perez-Ramirez, M. D., Klose, S., Greiner, J., Hjorth, J., Kaper, L., Pian, E., Palazzi, E., Andersen, M. I., Fruchter, A., Fynbo, J. P. U., Jensen, B. L., Kouveliotou, C., Rhoads, J., Rol, E., Vreeswijk, P. M., Wijers, R. A. M. J., and Heuvel, E. van den
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Astrophysics - Abstract
We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ~1.7 days after the event. Here we report the discovery of a dim optical afterglow (OA) that would not have been detected by many previous searches due to its faintess (R~23). This OA was seen to decline following a power law decay with index Alpha_R= -0.95 +/- 0.16. The spectral index Beta_opt/NIR yielded -1.25 +/- 0.14. These values may be explained by a relativistic expansion of a fireball (with p = 2.0) in the cooling regime. We also find evidence for inverse Compton scattering in X-rays., Comment: 5 pages, 5 figures, accepted for publication in A&A
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- 2003
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323. Optical and near-infrared observations of the GRB020405 afterglow
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Masetti, N., Palazzi, E., Pian, E., Simoncelli, A., Hunt, L. K., Maiorano, E., Levan, A. J., Christensen, L., Rol, E., Savaglio, S., Falomo, R., Castro-Tirado, A. J., Hjorth, J., Delsanti, A., Pannella, M., Mohan, V., Pandey, S. B., Sagar, R., Amati, L., Burud, I., Cerón, J. M. Castro, Frontera, F., Fruchter, A., Fynbo, J. P. U., Gorosabel, J., Kaper, L., Klose, S., Kouveliotou, C., Nicastro, L., Pedersen, H., Rhoads, J. E., Salamanca, I., Tanvir, N. R., Vreeswijk, P. M., Wijers, R. A. M. J., and Heuvel, E. P. J. van den
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Astrophysics - Abstract
(Abridged) We report on observations of the optical and NIR afterglow of GRB020405. Ground-based optical observations started about 1 day after the GRB and spanned a period of ~10 days; archival HST data extended the coverage up to 70 days after the GRB. We report the first detection of the afterglow in NIR bands. The detection of emission lines in the optical spectrum indicates that the GRB is located at z = 0.691. Absorptions are also detected at z = 0.691 and at z = 0.472. The latter system is likely caused by clouds in a galaxy located 2 arcsec southwest of the GRB host. Hence, for the first time, the galaxy responsible for an intervening absorption system in the spectrum of a GRB afterglow is identified. Optical and NIR photometry indicates that the decay in all bands follows a single power law of index alpha = 1.54. The late-epoch VLT and HST points lie above the extrapolation of this power law, so that a plateau is apparent in the VRIJ light curves at 10-20 days after the GRB. The light curves at epochs later than day ~20 after the GRB are consistent with a power-law decay with index alphaprime = 1.85. We suggest that this deviation can be modeled with a SN having the same temporal profile as SN2002ap, but 1.3 mag brighter at peak, and located at the GRB redshift. Alternatively, a shock re-energization may be responsible for the rebrightening. A polarimetric R-band measurement shows that the afterglow is polarized, with P = 1.5 % and theta = 172 degrees. Optical-NIR spectral flux distributions show a change of slope across the J band which we interpret as due to the presence of nu_c. The analysis of the multiwavelength spectrum within the fireball model suggests that a population of relativistic electrons produces the optical-NIR emission via synchrotron in an adiabatically expanding blastwave, and the X-rays via IC., Comment: 17 pages, 10 figures, 4 tables, accepted for publication on A&A, main journal
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- 2003
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324. Design and implementation of digital fractional order PID controller using optimal pole-zero approximation method for magnetic levitation system.
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Amit S. Chopade, Swapnil W. Khubalkar, Anjali S. Junghare, Mohan V. Aware, and Shantanu Das 0002
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- 2018
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325. Accelerating Venture Milestone Achievement: Examining the Impact of Resource Acquisition Timing.
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Jennifer Bailey and Mohan V. Tatikonda
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- 2018
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326. Optical observations of the bright long duration peculiar GRB 021004 afterglow
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Pandey, S. B., Sahu, D. K., Resmi, L., Sagar, R., Anupama, G. C., Bhattacharya, D., Mohan, V., Prabhu, T. P., Bhatt, B. C., Pandey, J. C., Parihar, Padmaker, and Castro-Tirado, A. J.
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Astrophysics - Abstract
The CCD magnitudes in Johnson $B,V$ and Cousins $R$ and $I$ photometric passbands are determined for the bright long duration GRB 021004 afterglow from 2002 October 4 to 16 starting $\sim$ 3 hours after the $\gamma-$ray burst. Light curves of the afterglow emission in $B$,$V$,$R$ and $I$ passbands are obtained by combining these measurements with other published data. The earliest optical emission appears to originate in a revese shock. Flux decay of the afterglow shows a very uncommon variation relative to other well-observed GRBs. Rapid light variations, especially during early times ($\Delta t < 2$ days) is superposed on an underlying broken power law decay typical of a jetted afterglow. The flux decay constants at early and late times derived from least square fits to the light curve are $0.99\pm0.05$ and $2.0\pm0.2$ respectively, with a jet break at around 7 day. Comparison with a standard fireball model indicates a total extinction of $E(B-V)=0.20$ mag in the direction of the burst. Our low-resolution spectra corrected for this extinction provide a spectral slope $\beta = 0.6\pm0.02$. This value and the flux decay constants agree well with the electron energy index $p\sim 2.27$ used in the model. The derived jet opening angle of about $7^{\circ}$ implies a total emitted gamma-ray energy $E_{\gamma} = 3.5\times10^{50}$ erg at a cosmological distance of about 20 Gpc. Multiwavelength observations indicate association of this GRB with a star forming region, supporting the case for collapsar origin of long duration GRBs., Comment: 19 pages, 3 figures, BASI, 31, 19
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- 2002
327. Optical and Radio observations of the bright GRB010222 afterglow: evidence for rapid synchrotron cooling?
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Sagar, R., Stalin, C. S., Bhattacharya, D., Pandey, S. B., Mohan, V., Castro-Tirado, A. J., Rao, A. Pramesh, Trushkin, Sergei A., Nizhelskij, N. A., Bremer, M, and Cerón, J. M. Castro
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Astrophysics - Abstract
We report photometric observations of the optical afterglow of GRB010222 in V,R and I passbands carried out at UPSO, Naini Tal between 22-27 Feb 2001. We determine CCD Johnson BV and Cousins RI photometric magnitudes for 31 stars in the field of GRB010222 and use them to calibrate our measurements as well as other published BVRI photometric magnitudes of GRB010222 afterglow. We construct the light curve in V,R,I passbands and from a broken power-law fit determine the decay indices of 0.74+/-0.05 and 1.35+/-0.04 before and after the break at 0.7 days. Using reported X-ray flux measurements at 0.35 and 9.13 days after the burst we determine X-ray to opt/IR spectral index of 0.61+/-0.02 and 0.75+/-0.02 on these two days. We also report upper limits to the radio flux obtained from the RATAN-600 telescope and the GMRT, and millimeter-wave upper limits obtained from the Plateau de Bure Millimeter interferometer. We argue that the synchrotron cooling frequency is below the optical band for most of the observing period. We also estimate an initial jet opening angle of about 2.0n^(1/8) degrees, where n is the number density of the ambient medium., Comment: 16 pages, 4 postscript figures, minor revisions according to referee's comments, millimeter upper limit added, accepted for publication in Bulletin of the Astronomical Society of India
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- 2001
328. The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy
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Castro-Tirado, A. J., Sokolov, V. V., Gorosabel, J., Cerón, J. M. Castro, Greiner, J., Wijers, R. A. M. J., Jensen, B. L., Hjorth, J., Toft, S., Pedersen, H., Palazzi, E., Pian, E., Masetti, N., Sagar, R., Mohan, V., Pandey, A. K., Pandey, S. B., Dodonov, S. N., Fatkhullin, T. A., Afanasiev, V. L., Komarova, V. N., Moiseev, A. V., Hudec, R., Simon, V., Vreeswijk, P., Rol, E., Klose, S., Stecklum, B., Zapatero-Osorio, M. R., Caon, N., Blake, C., Wall, J., Heinlein, D., Henden, A., Benetti, S., Magazzu, A., Ghinassi, F., Tommasi, L., Bremer, M., Kouveliotou, C., Guziy, S., Shlyapnikov, A., Hopp, U., Feulner, G., Dreizler, S., Hartmann, D., Boehnhardt, H., Paredes, J. M., Marti, J., Xanthopoulos, E., Kristen, H. E., Smoker, J., and Hurley, H.
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Astrophysics - Abstract
Observations of the extraordinarily bright optical afterglow (OA) of GRB 991208 started 2.1 d after the event. The flux decay constant of the OA in the R-band is -2.30 +/- 0.07 up to 5 d, which is very likely due to the jet effect, and after that it is followed by a much steeper decay with constant -3.2 +/- 0.2, the fastest one ever seen in a GRB OA. A negative detection in several all-sky films taken simultaneously to the event implies either a previous additional break prior to 2 d after the occurrence of the GRB (as expected from the jet effect). The existence of a second break might indicate a steepening in the electron spectrum or the superposition of two events. Once the afterglow emission vanished, contribution of a bright underlying SN is found, but the light curve is not sufficiently well sampled to rule out a dust echo explanation. Our determination of z = 0.706 indicates that GRB 991208 is at 3.7 Gpc, implying an isotropic energy release of 1.15 x 10E53 erg which may be relaxed by beaming by a factor > 100. Precise astrometry indicates that the GRB coincides within 0.2" with the host galaxy, thus given support to a massive star origin. The absolute magnitude is M_B = -18.2, well below the knee of the galaxy luminosity function and we derive a star-forming rate of 11.5 +/- 7.1 Mo/yr. The quasi-simultaneous broad-band photometric spectral energy distribution of the afterglow is determined 3.5 day after the burst (Dec 12.0) implying a cooling frequency below the optical band, i.e. supporting a jet model with p = -2.30 as the index of the power-law electron distribution., Comment: Accepted for publication in Astronomy and Astrophysics, 9 pages, 6 figures (Fig. 3 and Fig. 4 have been updated)
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- 2001
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329. Investigation of electromagnetic torque production in induction motor during charging operation
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Sharma, Sohit, Aware, Mohan V, and Bhowate, Apekshit
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- 2020
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330. Silver removal from aqueous solution by biochar produced from biosolids via microwave pyrolysis
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Antunes, Elsa, Jacob, Mohan V., Brodie, Graham, and Schneider, Philip A.
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- 2017
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331. Fruit, vegetable, and legume intake, and cardiovascular disease and deaths in 18 countries (PURE): a prospective cohort study
- Author
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Diaz, R, Orlandini, A, Linetsky, B, Toscanelli, S, Casaccia, G, Cuneo, JM Maini, Rahman, O, Yusuf, R, Azad, AK, Rabbani, KA, Cherry, HM, Mannan, A, Hassan, I, Talukdar, AT, Tooheen, RB, Khan, MU, Sintaha, M, Choudhury, T, Haque, R, Parvin, S, Avezum, A, Oliveira, GB, Marcilio, CS, Mattos, AC, Teo, K, Yusuf, S, Dejesus, J, Agapay, D, Tongana, T, Solano, R, Kay, I, Trottier, S, Rimac, J, Elsheikh, W, Heldman, L, Ramezani, E, Dagenais, G, Poirier, P, Turbide, G, Auger, D, De Bluts, A LeBlanc, Proulx, MC, Cayer, M, Bonneville, N, Lear, S, Gasevic, D, Corber, E, de Jong, V, Vukmirovich, I, Wielgosz, A, Fodor, G, Pipe, A, Shane, A, Lanas, F, Seron, P, Martinez, S, Valdebenito, A, Oliveros, M, Wei, Li, Lisheng, Liu, Chunming, Chen, Xingyu, Wang, Wenhua, Zhao, Hongye, Zhang, Xuan, Jia, Bo, Hu, Yi, Sun, Jian, Bo, Xiuwen, Zhao, Xiaohong, Chang, Tao, Chen, Hui, Chen, Qing, Deng, Xiaoru, Cheng, Xinye, He, Jian, Li, Juan, Li, Xu, Liu, Bing, Ren, Wei, Wang, Yang, Wang, Jun, Yang, Yi, Zhai, Manlu, Zhu, Fanghong, Lu, Jianfang, Wu, Yindong, Li, Yan, Hou, Liangqing, Zhang, Baoxia, Guo, Xiaoyang, Liao, Shiying, Zhang, Rongwen, Bian, Xiuzhen, Tian, Dong, Li, Di, Chen, Jianguo, Wu, Yize, Xiao, Tianlu, Liu, Peng, Zhang, Changlin, Dong, Ning, Li, Xiaolan, Ma, Yuqing, Yang, Rensheng, Lei, Minfan, Fu, Jing, He, Yu, Liu, Xiaojie, Xing, Qiang, Zhou, Lopez-Jaramillo, P, Lopez, PA Camacho, Garcia, R, Jurado, LJA, Gómez-Arbeláez, D, Arguello, JF, Dueñas, R, Silva, S, Pradilla, LP, Ramirez, F, Molina, DI, Cure-Cure, C, Perez, M, Hernandez, E, Arcos, E, Fernandez, S, Narvaez, C, Paez, J, Sotomayor, A, Garcia, H, Sanchez, G, David, T, Rico, A, Mony, P, Vaz, M, Bharathi, A V, Swaminathan, S, Kurpad, K Shankar AV, Jayachitra, KG, Kumar, N, Hospital, HAL, Mohan, V, Deepa, M, Parthiban, K, Anitha, M, Hemavathy, S, Rahulashankiruthiyayan, T, Anitha, D, Sridevi, K, Gupta, R, Panwar, RB, Mohan, I, Rastogi, P, Rastogi, S, Bhargava, R, Kumar, R, Thakur, J S, Patro, B, Lakshmi, PVM, Mahajan, R, Chaudary, P, Kutty, V Raman, Vijayakumar, K, Ajayan, K, Rajasree, G, Renjini, AR, Deepu, A, Sandhya, B, Asha, S, Soumya, HS, Kelishadi, R, Bahonar, A, Mohammadifard, N, Heidari, H, Yusoff, K, Ismail, TST, Ng, KK, Devi, A, Nasir, NM, Yasin, MM, Miskan, M, Rahman, EA, Arsad, MKM, Ariffin, F, Razak, SA, Majid, FA, Bakar, NA, Yacob, MY, Zainon, N, Salleh, R, Ramli, MKA, Halim, NA, Norlizan, SR, Ghazali, NM, Arshad, MN, Razali, R, Ali, S, Othman, HR, Hafar, CWJCW, Pit, A, Danuri, N, Basir, F, Zahari, SNA, Abdullah, H, Arippin, MA, Zakaria, NA, Noorhassim, I, Hasni, MJ, Azmi, MT, Zaleha, MI, Hazdi, KY, Rizam, AR, Sazman, W, Azman, A, Khatib, R, Khammash, U, Khatib, A, Giacaman, R, Iqbal, R, Afridi, A, Khawaja, R, Raza, A, Kazmi, K, Zatonski, W, Szuba, A, Zatonska, K, Ilow, R, Ferus, M, Regulska-Ilow, B, Rózanska, D, Wolyniec, M, Alkamel, Ali, M, Kruger, M A, Voster, H H, Schutte, A E, Wentzel-Viljoen, E, Eloff, FC, de Ridder, H, Moss, H, Potgieter, J, Roux, AA, Watson, M, de Wet, G, Olckers, A, Jerling, JC, Pieters, M, Hoekstra, T, Puoane, T, Igumbor, E, Tsolekile, L, Sanders, D, Naidoo, P, Steyn, N, Peer, N, Mayosi, B, Rayner, B, Lambert, V, Levitt, N, Kolbe-Alexander, T, Ntyintyane, L, Hughes, G, Swart, R, Fourie, J, Muzigaba, M, Xapa, S, Gobile, N, Ndayi, K, Jwili, B, Ndibaza, K, Egbujie, B, Rosengren, A, Boström, K Bengtsson, Gustavsson, A, Andreasson, M, Snällman, M, Wirdemann, L, Oguz, A, Imeryuz, N, Altuntas, Y, Gulec, S, Temizhan, A, Karsidag, K, Calik, KBT, Akalin, AAK, Caklili, OT, Keskinler, MV, Erbakan, AN, Yusufali, AM, Almahmeed, W, Swidan, H, Darwish, EA, Hashemi, ARA, Al-Khaja, N, Muscat-Baron, JM, Ahmed, SH, Mamdouh, TM, Darwish, WM, Abdelmotagali, MHS, Awed, SA Omer, Movahedi, GA, Hussain, F, Al Shaibani, H, Gharabou, RIM, Youssef, DF, Nawati, AZS, Salah, ZAR Abu, Abdalla, RFE, Al Shuwaihi, SM, Al Omairi, MA, Cadigal, OD, Alejandrino, R.S., Chifamba, J, Gwaunza, L, Terera, G, Mahachi, C, Murambiwa, P, Machiweni, T, Mapanga, R, Miller, Victoria, Mente, Andrew, Dehghan, Mahshid, Rangarajan, Sumathy, Zhang, Xiaohe, Swaminathan, Sumathi, Dagenais, Gilles, Gupta, Rajeev, Mohan, Viswanathan, Lear, Scott, Bangdiwala, Shrikant I, Schutte, Aletta E, Wentzel-Viljoen, Edelweiss, Avezum, Alvaro, Altuntas, Yuksel, Yusoff, Khalid, Ismail, Noorhassim, Peer, Nasheeta, Chifamba, Jephat, Diaz, Rafael, Rahman, Omar, Mohammadifard, Noushin, Lana, Fernando, Zatonska, Katarzyna, Wielgosz, Andreas, Yusufali, Afzalhussein, Iqbal, Romaina, Lopez-Jaramillo, Patricio, Khatib, Rasha, Rosengren, Annika, Li, Wei, Liu, Jiankang, Liu, Xiaoyun, Yin, Lu, Teo, Koon, Anand, Sonia, and Yusuf, Salim
- Published
- 2017
- Full Text
- View/download PDF
332. Associations of fats and carbohydrate intake with cardiovascular disease and mortality in 18 countries from five continents (PURE): a prospective cohort study
- Author
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Diaz, R, Orlandini, A, Linetsky, B, Toscanelli, S, Casaccia, G, Cuneo, JM Maini, Rahman, O, Yusuf, R, Azad, AK, Rabbani, KA, Cherry, HM, Mannan, A, Hassan, I, Talukdar, AT, Tooheen, RB, Khan, MU, Sintaha, M, Choudhury, T, Haque, R, Parvin, S, Avezum, A, Oliveira, GB, Marcilio, CS, Mattos, AC, Teo, K, Yusuf, S, Dejesus, J, Agapay, D, Tongana, T, Solano, R, Kay, I, Trottier, S, Rimac, J, Elsheikh, W, Heldman, L, Ramezani, E, Dagenais, G, Poirier, P, Turbide, G, Auger, D, De Bluts, A LeBlanc, Proulx, MC, Cayer, M, Bonneville, N, Lear, S, Gasevic, D, Corber, E, de Jong, V, Vukmirovich, I, Wielgosz, A, Fodor, G, Pipe, A, Shane, A, Lanas, F, Seron, P, Martinez, S, Valdebenito, A, Oliveros, M, Wei, Li, Lisheng, Liu, Chunming, Chen, Xingyu, Wang, Wenhua, Zhao, Hongye, Zhang, Xuan, Jia, Bo, Hu, Yi, Sun, Jian, Bo, Xiuwen, Zhao, Xiaohong, Chang, Tao, Chen, Hui, Chen, Qing, Deng, Xiaoru, Cheng, Xinye, He, Jian, Li, Juan, Li, Xu, Liu, Bing, Ren, Wei, Wang, Yang, Wang, Jun, Yang, Yi, Zhai, Manlu, Zhu, Fanghong, Lu, Jianfang, Wu, Yindong, Li, Yan, Hou, Liangqing, Zhang, Baoxia, Guo, Xiaoyang, Liao, Shiying, Zhang, Rongwen, Bian, Xiuzhen, Tian, Dong, Li, Di, Chen, Jianguo, Wu, Yize, Xiao, Tianlu, Liu, Peng, Zhang, Changlin, Dong, Ning, Li, Xiaolan, Ma, Yuqing, Yang, Rensheng, Lei, Minfan, Fu, Jing, He, Yu, Liu, Xiaojie, Xing, Qiang, Zhou, Lopez-Jaramillo, P, Lopez, PA Camacho, Garcia, R, Jurado, LJA, Gómez-Arbeláez, D, Arguello, JF, Dueñas, R, Silva, S, Pradilla, LP, Ramirez, F, Molina, DI, Cure-Cure, C, Perez, M, Hernandez, E, Arcos, E, Fernandez, S, Narvaez, C, Paez, J, Sotomayor, A, Garcia, H, Sanchez, G, David, T, Rico, A, Mony, P, Vaz, M, Bharathi, A V, Swaminathan, S, Kurpad, K Shankar AV, Jayachitra, KG, Kumar, N, Hospital, HAL, Mohan, V, Deepa, M, Parthiban, K, Anitha, M, Hemavathy, S, Rahulashankiruthiyayan, T, Anitha, D, Sridevi, K, Gupta, R, Panwar, RB, Mohan, I, Rastogi, P, Rastogi, S, Bhargava, R, Kumar, R, Thakur, J S, Patro, B, Lakshmi, PVM, Mahajan, R, Chaudary, P, Kutty, V Raman, Vijayakumar, K, Ajayan, K, Rajasree, G, Renjini, AR, Deepu, A, Sandhya, B, Asha, S, Soumya, HS, Kelishadi, R, Bahonar, A, Mohammadifard, N, Heidari, H, Yusoff, K, Ismail, TST, Ng, KK, Devi, A, Nasir, NM, Yasin, MM, Miskan, M, Rahman, EA, Arsad, MKM, Ariffin, F, Razak, SA, Majid, FA, Bakar, NA, Yacob, MY, Zainon, N, Salleh, R, Ramli, MKA, Halim, NA, Norlizan, SR, Ghazali, NM, Arshad, MN, Razali, R, Ali, S, Othman, HR, Hafar, CWJCW, Pit, A, Danuri, N, Basir, F, Zahari, SNA, Abdullah, H, Arippin, MA, Zakaria, NA, Noorhassim, I, Hasni, MJ, Azmi, MT, Zaleha, MI, Hazdi, KY, Rizam, AR, Sazman, W, Azman, A, Khatib, R, Khammash, U, Khatib, A, Giacaman, R, Iqbal, R, Afridi, A, Khawaja, R, Raza, A, Kazmi, K, Zatonski, W, Szuba, A, Zatonska, K, Ilow, R, Ferus, M, Regulska-Ilow, B, Rózanska, D, Wolyniec, M, Alkamel, Ali, M, Kruger, M A, Voster, H H, Schutte, A E, Wentzel-Viljoen, E, Eloff, FC, de Ridder, H, Moss, H, Potgieter, J, Roux, AA, Watson, M, de Wet, G, Olckers, A, Jerling, JC, Pieters, M, Hoekstra, T, Puoane, T, Igumbor, E, Tsolekile, L, Sanders, D, Naidoo, P, Steyn, N, Peer, N, Mayosi, B, Rayner, B, Lambert, V, Levitt, N, Kolbe-Alexander, T, Ntyintyane, L, Hughes, G, Swart, R, Fourie, J, Muzigaba, M, Xapa, S, Gobile, N, Ndayi, K, Jwili, B, Ndibaza, K, Egbujie, B, Rosengren, A, Boström, K Bengtsson, Gustavsson, A, Andreasson, M, Snällman, M, Wirdemann, L, Oguz, A, Imeryuz, N, Altuntas, Y, Gulec, S, Temizhan, A, Karsidag, K, Calik, KBT, Akalin, AAK, Caklili, OT, Keskinler, MV, Erbakan, AN, Yusufali, AM, Almahmeed, W, Swidan, H, Darwish, EA, Hashemi, ARA, Al-Khaja, N, Muscat-Baron, JM, Ahmed, SH, Mamdouh, TM, Darwish, WM, Abdelmotagali, MHS, Awed, SA Omer, Movahedi, GA, Hussain, F, Al Shaibani, H, Gharabou, RIM, Youssef, DF, Nawati, AZS, Salah, ZAR Abu, Abdalla, RFE, Al Shuwaihi, SM, Al Omairi, MA, Cadigal, OD, Alejandrino, R.S., Chifamba, J, Gwaunza, L, Terera, G, Mahachi, C, Murambiwa, P, Machiweni, T, Mapanga, R, Dehghan, Mahshid, Mente, Andrew, Zhang, Xiaohe, Swaminathan, Sumathi, Li, Wei, Mohan, Viswanathan, Iqbal, Romaina, Kumar, Rajesh, Wentzel-Viljoen, Edelweiss, Rosengren, Annika, Amma, Leela Itty, Avezum, Alvaro, Chifamba, Jephat, Diaz, Rafael, Khatib, Rasha, Lear, Scott, Lopez-Jaramillo, Patricio, Liu, Xiaoyun, Gupta, Rajeev, Mohammadifard, Noushin, Gao, Nan, Oguz, Aytekin, Ramli, Anis Safura, Seron, Pamela, Sun, Yi, Szuba, Andrzej, Tsolekile, Lungiswa, Wielgosz, Andreas, Yusuf, Rita, Hussein Yusufali, Afzal, Teo, Koon K, Rangarajan, Sumathy, Dagenais, Gilles, Bangdiwala, Shrikant I, Islam, Shofiqul, Anand, Sonia S, and Yusuf, Salim
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- 2017
- Full Text
- View/download PDF
333. Association of dietary nutrients with blood lipids and blood pressure in 18 countries: a cross-sectional analysis from the PURE study
- Author
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Yusuf, S, Rangarajan, S, Teo, K K, Chow, C K, O'Donnell, M, Mente, A, Leong, D, Smyth, A, Joseph, P, Merchant, A, Islam, S, Zhang, M, Hu, W, Ramasundarahettige, C, Wong, G, Bangdiwala, S, Dyal, L, Casanova, A, Dehghan, M, Lewis, G, Aliberti, A, Arshad, A, Reyes, A, Zaki, A, Lewis, B, Zhang, B, Agapay, D, Hari, D, Milazzo, E, Ramezani, E, Hussain, F, Shifaly, F, McAlpine, G, Kay, I, Lindeman, J, Rimac, J, Swallow, J, Heldman, L, Mushtaha, M(a), Mushtaha, M(o), Trottier, M, Riggi, M, Aoucheva, N, Kandy, N, Mackie, P, Solano, R, Chin, S, Ramacham, S, Shahrook, S, Trottier, S, Tongana, T, ElSheikh, W, Iyengar, Y, McQueen, M, Hall, K, Keys, J, Wang, X, Keneth, J, Devanath, A, Diaz, R, Orlandini, A, Linetsky, B, Toscanelli, S, Casaccia, G, Cuneo, JM Maini, Rahman, O, Yusuf, R, Azad, AK, Rabbani, KA, Cherry, HM, Mannan, A, Hassan, I, Talukdar, AT, Tooheen, RB, Khan, MU, Sintaha, M, Choudhury, T, Haque, R, Parvin, S, Avezum, A, Oliveira, GB, Marcilio, CS, Mattos, AC, Teo, K, Dejesus, J, Elsheikh, W, Dagenais, G, Poirier, P, Turbide, G, Auger, D, De Bluts, A LeBlanc, Proulx, MC, Cayer, M, Bonneville, N, Lear, S, Gasevic, D, Corber, E, de Jong, V, Vukmirovich, I, Wielgosz, A, Fodor, G, Pipe, A, Shane, A, Lanas, F, Seron, P, Martinez, S, Valdebenito, A, Oliveros, M, Wei, Li, Lisheng, Liu, Chunming, Chen, Xingyu, Wang, Wenhua, Zhao, Hongye, Zhang, Xuan, Jia, Bo, Hu, Yi, Sun, Jian, Bo, Xiuwen, Zhao, Xiaohong, Chang, Tao, Chen, Hui, Chen, Qing, Deng, Xiaoru, Cheng, Xinye, He, Jian, Li, Juan, Li, Xu, Liu, Bing, Ren, Wei, Wang, Yang, Wang, Jun, Yang, Yi, Zhai, Manlu, Zhu, Fanghong, Lu, Jianfang, Wu, Yindong, Li, Yan, Hou, Liangqing, Zhang, Baoxia, Guo, Xiaoyang, Liao, Shiying, Zhang, Rongwen, Bian, Xiuzhen, Tian, Dong, Li, Di, Chen, Jianguo, Wu, Yize, Xiao, Tianlu, Liu, Peng, Zhang, Changlin, Dong, Ning, Li, Xiaolan, Ma, Yuqing, Yang, Rensheng, Lei, Minfan, Fu, Jing, He, Yu, Liu, Xiaojie, Xing, Qiang, Zhou, Lopez-Jaramillo, P, Lopez, PA Camacho, Garcia, R, Jurado, LJA, Gómez-Arbeláez, D, Arguello, JF, Dueñas, R, Silva, S, Pradilla, LP, Ramirez, F, Molina, DI, Cure-Cure, C, Perez, M, Hernandez, E, Arcos, E, Fernandez, S, Narvaez, C, Paez, J, Sotomayor, A, Garcia, H, Sanchez, G, David, T, Rico, A, Mony, P, Vaz, M, Bharathi, A V, Swaminathan, S, Kurpad, K Shankar AV, Jayachitra, KG, Kumar, N, Hospital, HAL, Mohan, V, Deepa, M, Parthiban, K, Anitha, M, Hemavathy, S, Rahulashankiruthiyayan, T, Anitha, D, Sridevi, K, Gupta, R, Panwar, RB, Mohan, I, Rastogi, P, Rastogi, S, Bhargava, R, Kumar, R, Thakur, J S, Patro, B, Lakshmi, PVM, Mahajan, R, Chaudary, P, Kutty, V Raman, Vijayakumar, K, Ajayan, K, Rajasree, G, Renjini, AR, Deepu, A, Sandhya, B, Asha, S, Soumya, HS, Kelishadi, R, Bahonar, A, Mohammadifard, N, Heidari, H, Yusoff, K, Ismail, TST, Ng, KK, Devi, A, Nasir, NM, Yasin, MM, Miskan, M, Rahman, EA, Arsad, MKM, Ariffin, F, Razak, SA, Majid, FA, Bakar, NA, Yacob, MY, Zainon, N, Salleh, R, Ramli, MKA, Halim, NA, Norlizan, SR, Ghazali, NM, Arshad, MN, Razali, R, Ali, S, Othman, HR, Hafar, CWJCW, Pit, A, Danuri, N, Basir, F, Zahari, SNA, Abdullah, H, Arippin, MA, Zakaria, NA, Noorhassim, I, Hasni, MJ, Azmi, MT, Zaleha, MI, Hazdi, KY, Rizam, AR, Sazman, W, Azman, A, Khatib, R, Khammash, U, Khatib, A, Giacaman, R, Iqbal, R, Afridi, A, Khawaja, R, Raza, A, Kazmi, K, Dans, A, Co, HU, Sanchez, JT, Pudol, L, Zamora-Pudol, C, Palileo-Villanueva, LAM, Aquino, MR, Abaquin, C, Pudol, SL, Cabral, ML, Zatonski, W, Szuba, A, Zatonska, K, Ilow, R, Ferus, M, Regulska-Ilow, B, Rózanska, D, Wolyniec, M, AlHabib, KF, Hersi, A, Kashour, T, Alfaleh, H, Alshamiri, M, Altaradi, HB, Alnobani, O, Bafart, A, Alkamel, N, Ali, M, Abdulrahman, M, Nouri, R, Kruger, A, Voster, H H, Schutte, A E, Wentzel-Viljoen, E, Eloff, FC, de Ridder, H, Moss, H, Potgieter, J, Roux, AA, Watson, M, de Wet, G, Olckers, A, Jerling, JC, Pieters, M, Hoekstra, T, Puoane, T, Igumbor, E, Tsolekile, L, Sanders, D, Naidoo, P, Steyn, N, Peer, N, Mayosi, B, Rayner, B, Lambert, V, Levitt, N, Kolbe-Alexander, T, Ntyintyane, L, Hughes, G, Swart, R, Fourie, J, Muzigaba, M, Xapa, S, Gobile, N, Ndayi, K, Jwili, B, Ndibaza, K, Egbujie, B, Rosengren, A, Bengtsson Boström, K, Gustavsson, A, Andreasson, M, Snällman, M, Wirdemann, L, Yeates, K, Sleeth, J, Kilonzo, K, Oguz, A, Imeryuz, N, Altuntas, Y, Gulec, S, Temizhan, A, Karsidag, K, Calik, KBT, Akalin, AAK, Caklili, OT, Keskinler, MV, Erbakan, AN, Yusufali, AM, Almahmeed, W, Swidan, H, Darwish, EA, Hashemi, ARA, Al-Khaja, N, Muscat-Baron, JM, Ahmed, SH, Mamdouh, TM, Darwish, WM, Abdelmotagali, MHS, Awed, SA Omer, Movahedi, GA, Al Shaibani, H, Gharabou, RIM, Youssef, DF, Nawati, AZS, Salah, ZAR Abu, Abdalla, RFE, Al Shuwaihi, SM, Al Omairi, MA, Cadigal, OD, Alejandrino, R.S., Chifamba, J, Gwaunza, L, Terera, G, Mahachi, C, Murambiwa, P, Machiweni, T, Mapanga, R, Mente, Andrew, Dehghan, Mahshid, Rangarajan, Sumathy, McQueen, Matthew, Dagenais, Gilles, Wielgosz, Andreas, Lear, Scott, Li, Wei, Chen, Hui, Wang, Yang, Diaz, Rafael, Avezum, Alvaro, Lopez-Jaramillo, Patricio, Seron, Pamela, Kumar, Rajesh, Gupta, Rajeev, Mohan, Viswanathan, Swaminathan, Sumathi, Kutty, Raman, Zatonska, Katarzyna, Iqbal, Romaina, Yusuf, Rita, Mohammadifard, Noushin, Khatib, Rasha, Nasir, Nafiza Mat, Ismail, Noorhassim, Oguz, Aytekin, Rosengren, Annika, Yusufali, Afzalhussein, Wentzel-Viljoen, Edelweiss, Puoane, Thandi, Chifamba, Jephat, Teo, Koon, Anand, Sonia S, and Yusuf, Salim
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- 2017
- Full Text
- View/download PDF
334. IDF23-0223 Targeting miR-122 and miR-4756 mitigates atherogenic events by upregulating Sestrin2 under high glucose condition
- Author
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Rajagopal, A., Venkatesan, S., Balasubramanyam, M., Anjana, R.M., Mohan, V., and Manickam, N.
- Published
- 2024
- Full Text
- View/download PDF
335. GRB 000926 and its optical afterglow: Another evidence for non-isotropic emission
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Sagar, R., Pandey, S. B., Mohan, V., Bhattacharya, D., and Castro-Tirado, A. J.
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Astrophysics - Abstract
CCD Johnsons BV and Cousins RI photometric magnitudes are determined for 20 stars in the field of GRB 000926. Using them as calibrators, B and R band light curves are constructed of the afterglow from ours and other published observations. They show a steepening of the flux decay, from a decay constant of 1.4+/-0.1 to 2.6+/-0.06 at about 1.7 days after the burst. Attributing this break to the onset of sideways expansion of a jet-like ejecta, we estimate an initial jet opening angle of ~0.14 radian, and a burst energy of ~10^51 erg. We construct the X-ray-optical-near infrared spectrum of the afterglow and derive a spectral index of ~ -0.9. From the spectrum we also estimate that the source has a rather large intrinsic extinction, amounting to E(B-V)=0.36+/-0.02., Comment: 13 pages, 3 figures, accepted for publication in Bull. Astr. Soc. India
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- 2000
336. A Three-Phase Reduced Switch Count Multilevel Inverter Topology
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SIVAMANI S and MOHAN V
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Article Subject ,Modeling and Simulation ,Energy Engineering and Power Technology ,Electrical and Electronic Engineering - Abstract
Multilevel inverters play a vital role in the industrial and renewable energy sectors due to their flexibility in synthesizing sinusoidal waveforms using a low-pass filter with a medium voltage range. It has several drawbacks, such as a higher number of power component requirements and voltage balancing problems. In this study, a new structure for multilevel inverters has been developed to offer good power quality with minimum number of switching devices and gate driver circuits. The proposed structure is configured to operate in symmetrical and asymmetrical configurations for single/three-phase versions. A simulation study using MATLAB/Simulink has been utilized to study the operating characteristics under both configurations. A laboratory prototype has been built to check the feasibility of the proposed structure for real-time applications.
- Published
- 2022
337. Handover Approach for Heterogeneous Networks with Improved K-Partite Graph
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Jyothi Puligadda, Venkata Rama Rao Kolipaka, Murali Mohan V., and Vamsidhar Talasila
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Artificial Intelligence ,Software ,Information Systems - Published
- 2022
338. Improved dynamic performance with discrete sampling in digital ACM controlled DC‐DC boost converter with capacitor ESR inclusion
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Obulapathi Balapanuru, Makarand M. Lokhande, and Mohan. V. Aware
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Applied Mathematics ,Electrical and Electronic Engineering ,Computer Science Applications ,Electronic, Optical and Magnetic Materials - Published
- 2022
339. Hospital outcomes in pediatric patients with Prader–Willi syndrome (PWS) undergoing orthopedic surgery: A 12-year analysis of national trends in surgical management and inpatient hospital outcomes
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Joseph C. Brinkman, Kade S. McQuivey, Andrew S. Chung, Mohan V. Belthur, Justin L. Makovicka, Zachary K. Christopher, and Michael R. Jones
- Subjects
Pediatrics ,medicine.medical_specialty ,Acute blood loss anemia ,Urinary system ,medicine.medical_treatment ,Diabetes mellitus ,medicine ,Humans ,Orthopedics and Sports Medicine ,Musculoskeletal Diseases ,Child ,Retrospective Studies ,Inpatients ,business.industry ,Incidence (epidemiology) ,Retrospective cohort study ,medicine.disease ,medicine.icd_9_cm_classification ,Hospitals ,Spinal Fusion ,Spinal fusion ,Orthopedic surgery ,Surgery ,Orthopedic Procedures ,business ,Prader-Willi Syndrome - Abstract
Background The incidence of orthopedic disorders amongst patients with Prader–Willi Syndrome (PWS) is high when compared to the general pediatric population. The purpose of this retrospective study was to define the most commonly performed orthopedic procedures in pediatric patients with PWS and to characterize the peri-operative outcomes of these patients. Methods The Kids Inpatient Database (KID) was queried to collect data and identify all pediatric patients with PWS who underwent orthopedic procedures from 2001 to 2012. A total of 3684 patients with PWS were identified, 334 of who underwent an orthopedic procedure. Population demographics, comorbidities, and specific procedures undergone were defined. The incidences of postoperative complications and length of associated hospital stay were additionally evaluated. Results Mean age of patients in this sample was 10.33 years (SD 4.5). The most common comorbidities included obesity (18.1%), chronic pulmonary disease (14.1%), hypothyroidism (5.1%), hypertension (5.1%), and uncomplicated diabetes (4%). Common procedures were spinal fusion (165/334, 49%) and lower extremity procedures (50/334, 15%). Complications included acute blood loss anemia, device related complications, pneumonia, sepsis, and urinary tract infections. The overall complication rate was 35.6%. Average hospital lengths of stay for patients undergoing spinal fusion was 6.68 days (SD 4.13), lower extremity orthopedic procedure was 5.65 days (SD 7.4), and all other orthopedic procedures was 7.74 days (SD 16.3). Conclusions Orthopedic disorders are common in patients with PWS. Consequently, spinal fusions and lower extremity procedures are commonly performed in this patient population. Associated comorbid conditions may negatively impact surgical outcomes in these patients. This information should prove useful in the peri-operative management of patients with PWS undergoing orthopedic surgery and for shared decision making with families.
- Published
- 2022
340. Improved constant phase fractional order approximation method for induction motor FOPI speed controller
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Sudheer Adigintla and Mohan V. Aware
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Applied Mathematics ,Electrical and Electronic Engineering ,Computer Science Applications ,Electronic, Optical and Magnetic Materials - Published
- 2022
341. GRB000301C with peculiar afterglow emission
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Sagar, R., Mohan, V., Pandey, S. B., Pandey, A. K., Stalin, C. S., and Castro-Tirado, A. J.
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Astrophysics - Abstract
The CCD magnitudes in Johnson V and Cousins R and I photometric passbands are determined for GRB 000301C afterglow starting ~ 1.5 day after the gamma-ray burst. In fact we provide the earliest optical observations for this burst. Light curves of the afterglow emissions in U, B, V, R, I, J and K' passbands are obtained by combining the present measurements with the published data. Flux decay shows a very uncommon variation relative to other well observed GRBs. Overall, there is a steepening of the optical and near-infrared flux decay caused by a geometric and sideways expanding jet. This is superimposed by a short term variability especially during early time (Delta t < 8 days). The cause of variability is not well understood, though it has occurred simultaneously with similar amplitude in all the filters. We derive the early and late time flux decay constants using jet model. The late time flux decay is the steepest amongst the GRB OTs observed so far with alpha ~ 3. Steepening in the flux decay seems to have started simultaneously around Delta t ~ 7.6 day in all passbands. The value of spectral index in the optical-near IR region is ~ -1.0. Redshift determination with z=2.0335 indicates cosmological origin of the GRB having a luminosity distance of 16.6 Gpc. Thus it becomes the second farthest amongst the GRBs with known distances. An indirect estimate of the fluence > 20 keV indicates, if isotropic,> =10^53 ergs of release of energy. The enormous amount of released energy will be reduced, if the radiation is beamed which is the case for this event. Using a jet break time of 7.6 days, we infer a jet opening angle of ~ 0.15 radian. This means the energy released is reduced by a factor of ~ 90 relative to the isotropic value., Comment: LaTeX file, 11 pages including 4 figures, uses psfig.sty, Bull. Astron. Society of India(accepted, Sept, 2000 issue)
- Published
- 2000
342. Temporal behaviour of emissions from Gamma-ray bursts and optical/near-IR afterglows of GRB 991208 and GRB 991216
- Author
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Sagar, R., Mohan, V., Pandey, A. K., Pandey, S. B., and Castro-Tirado, A. J.
- Subjects
Astrophysics - Abstract
The CCD magnitudes in Cousins R and I photometric passbands are determined for GRB 991216 and GRB 991208 afterglows respectively about 1 and about 3 day after trigger of the corresponding gamma-ray bursts. Light curves of the afterglow emissions are obtained by combining the published data with the present measurements in R and I passbands for GRB 991208 and in R, Gunn I and J passbands for GRB 991216. They indicate that the flux decay constants of a GRB are almost the same in each passband with values about 2.2 for GRB 991208 and about 1.2 for GRB 991216 indicating very fast optical flux decay in the case of former which may be due to beaming effect. However, cause of steepening by 0.23 +/- 0.06 dex in the R light curve of GRB 991216 afterglow between 2 to 2.5 day after the burst, is presently not understood. Redshift determinations indicate that both GRBs are at cosmological distance with a value of 4.2 Gpc for GRB 991208 and 6.2 Gpc for GRB 991216. The observed fluence above 20 keV indicates, if isotropic, release of energy about 1.3 x 10^{53} erg for GRB 991208 and about 6.7 x 10^{53} erg for GRB 991216 by these bright gamma-ray flashes. The enormous amount of released energy will be reduced, if the radiation is beamed which seems to be case for GRB 991208 afterglow.The quasi-simultaneous broad-band photometric spectral energy distributions of the afterglows are determined about 8.5 day and about 35 hour after the bursts of GRB 991208 and GRB 991216 respectively.The flux decreases exponentially with frequency. The value of spectral index in the optical-near IR region is -0.75 +/- 0.03 for GRB 991208 and -1.0 +/- 0.12 for GRB 991216., Comment: 13 pages and 5 figures
- Published
- 2000
343. New surveys of UBV photometry and absolute proper motions at intermediate latitude
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Ojha, D. K., Bienayme, O., Mohan, V., and Robin, A. C.
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Astrophysics - Abstract
A photometric and proper motion survey has been obtained in 2 directions at intermediate latitude: ($l=167.5^\circ$, $b=47.4^\circ$; $\alpha_{2000}=9^h41^m26^s$,$\delta_{2000}=+49^\circ53'27''$) and ($l=278^\circ$, $b=47^\circ$; $\alpha_{2000}=11^h42^m56^s$, $\delta_{2000}=-12^\circ31'42''$). The survey covers 7.13 and 20.84 square degrees, respectively. The limiting magnitude is about 18.5 in V for both directions. We have derived the density laws for stars (M$_{V}$ $\ge$ 3.5) as a function of distance from the galactic plane. The density laws for stars follow a sum of two exponentials with scale heights of 240 pc (thin disk) and 790 pc (thick disk), respectively. The local density of thick disk is found to be 6.1$\pm$3 % relative to the thin disk. The kinematical distribution of stars has been probed to distances up to 3.5 kpc above the galactic plane. New estimates of the parameters of velocity ellipsoid have been derived for the thick disk of the Galaxy. A comparison of our data sets with the Besan\c con model star count predictions has been performed, giving a good agreement in the magnitude range V = 13 to 18., Comment: 13 pages, 8 PS figures, To appear in A&A
- Published
- 1999
344. BVRI CCD photometric standards in the field of GRB 990123
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Nilakshi, Yadav, R. K. S., Mohan, V., Pandey, A. K., and Sagar, R.
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Astrophysics - Abstract
The CCD magnitudes in Johnson $BV$ and Cousins $RI$ photometric passbands are determined for 18 stars in the field of GRB 990123. These measurements can be used in carrying out precise CCD photometry of the optical transient of GRB 990123 using differential photometric techniques during non--photometric sky conditions. A comparison with previous photometry indicates that the present photmetry is more precise., Comment: Tex file, 5 pages with 1 figure. Bull. Astron. Society India, Vol. 27 (accepted)
- Published
- 1999
345. Optical follow up of the GRB 990123 source from UPSO, Nainital
- Author
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Sagar, R., Pandey, A. K., Mohan, V., Yadav, R. K. S., Nilakshi, Bhattacharya, D., and Castro-Tirado, A. J.
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Astrophysics - Abstract
The CCD magnitudes in Johnson $BV$ and Cousins $R$ photometric passbands are determined for the optical transient of GRB 990123. These observations have been taken approximately 12 hours after trigger of the gamma-ray burst. BVR photometric light curves are obtained by combining the published data with the present measurements. They indicate that the flux decay constants in $BV$ and $R$ passbands are almost the same. Its value is $1.1\pm 0.06$. Such decay is quite consistent with the fireball models for the optical transient., Comment: LaTex file, 5 pages with 1 figure. Bull. Astron. Society India, Vol. 27 (accepted)
- Published
- 1999
346. Correction to: Hospital outcomes of scoliosis surgery in children with Prader–Willi Syndrome: comparison with adolescent idiopathic scoliosis
- Author
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McQuivey, Kade S., Sheridan, Joseph R., Chung, Andrew, Mayfield, Cory, Gulbrandsen, Matthew, Brinkman, Joseph C., and Belthur, Mohan V.
- Published
- 2021
- Full Text
- View/download PDF
347. Decontamination-Induced Modification of Bioactivity in Essential Oil-Based Plasma Polymer Coatings
- Author
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Olha Bazaka, Karthika Prasad, Igor Levchenko, Mohan V. Jacob, Kateryna Bazaka, Peter Kingshott, Russell J. Crawford, and Elena P. Ivanova
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plasma polymer ,atmospheric pressure plasma ,antibacterial polymer coatings ,Organic chemistry ,QD241-441 - Abstract
Plasma polymer coatings fabricated from Melaleuca alternifolia essential oil and its derivatives have been previously shown to reduce the extent of microbial adhesion on titanium, polymers, and other implantable materials used in dentistry. Previous studies have shown these coatings to maintain their performance under standard operating conditions; however, when used in e.g., a dental implant, these coatings may inadvertently become subject to in situ cleaning treatments, such as those using an atmospheric pressure plasma jet, a promising tool for the effective in situ removal of biofilms from tissues and implant surfaces. Here, we investigated the effect of such an exposure on the antimicrobial performance of the Melaleuca alternifolia polymer coating. It was found that direct exposure of the polymer coating surface to the jet for periods less than 60 s was sufficient to induce changes in its surface chemistry and topography, affecting its ability to retard subsequent microbial attachment. The exact effect of the jet exposure depended on the chemistry of the polymer coating, the length of plasma treatment, cell type, and incubation conditions. The change in the antimicrobial activity for polymer coatings fabricated at powers of 20–30 W was not statistically significant due to their limited baseline bioactivity. Interestingly, the bioactivity of polymer coatings fabricated at 10 and 15 W against Staphylococcus aureus cells was temporarily improved after the treatment, which could be attributed to the generation of loosely attached bioactive fragments on the treated surface, resulting in an increase in the dose of the bioactive agents being eluted by the surface. Attachment and proliferation of Pseudomonas aeruginosa cells and mixed cultures were less affected by changes in the bioactivity profile of the surface. The sensitivity of the cells to the change imparted by the jet treatment was also found to be dependent on their origin culture, with mature biofilm-derived P. aeruginosa bacterial cells showing a greater ability to colonize the surface when compared to its planktonic broth-grown counterpart. The presence of plasma-generated reactive oxygen and nitrogen species in the culture media was also found to enhance the bioactivity of polymer coatings fabricated at power levels of 10 and 15 W, due to a synergistic effect arising from simultaneous exposure of cells to reactive oxygen and nitrogen species (RONS) and eluted bioactive fragments. These results suggest that it is important to consider the possible implications of inadvertent changes in the properties and performance of plasma polymer coatings as a result of exposure to in situ decontamination, to both prevent suboptimal performance and to exploit possible synergies that may arise for some polymer coating-surface treatment combinations.
- Published
- 2021
- Full Text
- View/download PDF
348. Single-Phase Grid-Connected Fault Tolerant Bi-directional Power Flow Converter for Electric Vehicle Charging System
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Kumar, Anup, primary, Aware, Mohan V., additional, Umre, B. S., additional, and Waghmare, Manoj A., additional
- Published
- 2023
- Full Text
- View/download PDF
349. Dual-Input High Gain DC-DC Converter with Two Energy Storage Systems for Light EV Applications
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Balapanuru, Obulapathi, primary, Lokhande, Makarand M., additional, and Aware, Mohan V., additional
- Published
- 2023
- Full Text
- View/download PDF
350. South Asian medical cohorts reveal strong founder effects and high rates of homozygosity
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Wall, Jeffrey D., primary, Sathirapongsasuti, J. Fah, additional, Gupta, Ravi, additional, Rasheed, Asif, additional, Venkatesan, Radha, additional, Belsare, Saurabh, additional, Menon, Ramesh, additional, Phalke, Sameer, additional, Mittal, Anuradha, additional, Fang, John, additional, Tanneeru, Deepak, additional, Deshmukh, Manjari, additional, Bassi, Akshi, additional, Robinson, Jacqueline, additional, Chaudhary, Ruchi, additional, Murugan, Sakthivel, additional, ul-Asar, Zameer, additional, Saleem, Imran, additional, Ishtiaq, Unzila, additional, Fatima, Areej, additional, Sheikh, Saqib Shafi, additional, Hameed, Shahid, additional, Ishaq, Mohammad, additional, Rasheed, Syed Zahed, additional, Memon, Fazal-ur-Rehman, additional, Jalal, Anjum, additional, Abbas, Shahid, additional, Frossard, Philippe, additional, Fuchsberger, Christian, additional, Forer, Lukas, additional, Schoenherr, Sebastian, additional, Bei, Qixin, additional, Bhangale, Tushar, additional, Tom, Jennifer, additional, Gadde, Santosh Gopi Krishna, additional, B V, Priya, additional, Naik, Naveen Kumar, additional, Wang, Minxian, additional, Kwok, Pui-Yan, additional, Khera, Amit V., additional, Lakshmi, B. R., additional, Butterworth, Adam S., additional, Chowdhury, Rajiv, additional, Danesh, John, additional, di Angelantonio, Emanuele, additional, Naheed, Aliya, additional, Goyal, Vinay, additional, Kandadai, Rukmini M., additional, Kumar, Hrishikesh, additional, Borgohain, Rupam, additional, Mukherjee, Adreesh, additional, Wadia, Pettarusp M., additional, Yadav, Ravi, additional, Desai, Soaham, additional, Kumar, Niraj, additional, Biswas, Atanu, additional, Pal, Pramod Kumar, additional, Muthane, Uday B., additional, Das, Shymal K., additional, Ramprasad, Vedam L., additional, Kukkle, Prashanth L., additional, Seshagiri, Somasekar, additional, Kathiresan, Sekar, additional, Ghosh, Arkasubhra, additional, Mohan, V., additional, Saleheen, Danish, additional, Stawiski, Eric W., additional, and Peterson, Andrew S., additional
- Published
- 2023
- Full Text
- View/download PDF
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