Stephen Klein Wellness Center Patient Satisfaction Survey: Development and Preliminary Results

Study design: •Selected the CAHPS® with Patient Centered Medical Home question set to administer to patients receiving medical care at SKWC (52 questions) •Included 2 supplemental questions to assess patients’ likelihood to refer others to SKWC •Developed an additional survey for patients receiving behavioral health services (16 questions) Participant recruitment and data collection: •Calculated a target number of 130 participants based on CAHPS® guidelines of 50 surveys per Full Time Employee •Observed patient flow and developed recruitment strategy for a convenience sample •Eligibility criteria: patient ≥18 y/o and had a medical appointment in the last 12 months •Participants were invited to enter an optional raffle to win a $25 gift card to the Fresh Grocer Data analysis: •Responses were coded and entered into Microsoft Excel Database •Average scores and response frequencies for each survey question were calculatedhttps://jdc.jefferson.edu/cwicposters/1029/thumbnail.jp

Newsletter, Volume 27, Number 03, May - June 1982

UT MDAH Maintains High Cure Rate, Low Recurrence Rate for Rare Uterine Cancer UT MDAH Offers Oncology Lecture Series Biomathematicians Develop Software for Clinical Trial Design and Analysis Lectureship Honors Taylor Murray M. Copeland Dies Genetic Markers May Identify Chromosomal Deletion Associated with Retinoblastoma, Louise C. Strong, MD Noteworthyhttps://openworks.mdanderson.org/newsletter/1113/thumbnail.jp

Theory of Star Formation

We review current understanding of star formation, outlining an overall theoretical framework and the observations that motivate it. A conception of star formation has emerged in which turbulence plays a dual role, both creating overdensities to initiate gravitational contraction or collapse, and countering the effects of gravity in these overdense regions. The key dynamical processes involved in star formation -- turbulence, magnetic fields, and self-gravity -- are highly nonlinear and multidimensional. Physical arguments are used to identify and explain the features and scalings involved in star formation, and results from numerical simulations are used to quantify these effects. We divide star formation into large-scale and small-scale regimes and review each in turn. Large scales range from galaxies to giant molecular clouds (GMCs) and their substructures. Important problems include how GMCs form and evolve, what determines the star formation rate (SFR), and what determines the initial mass function (IMF). Small scales range from dense cores to the protostellar systems they beget. We discuss formation of both low- and high-mass stars, including ongoing accretion. The development of winds and outflows is increasingly well understood, as are the mechanisms governing angular momentum transport in disks. Although outstanding questions remain, the framework is now in place to build a comprehensive theory of star formation that will be tested by the next generation of telescopes.Comment: 120 pages, to appear in ARAA. No changes from v1 text; permission statement adde

Louise Connally Strong, MD, Oral History Interview, August 8, 2012

Major Topics Covered: Personal and educational background Overview and history of oncology genetics in the sixties and seventies Working with Alfred Knudson Research: longitudinal studies of inherited genetics patterns of neuroblastoma, aniridia, and Wilm’s tumor; discovery of the p53 tumor suppressor genes and link to Li-Fraumeni syndrome, survivorship Women at MD Anderson MD Anderson’s cancer screening program Ethics and genetic testing MD Anderson growth and cultural changehttps://openworks.mdanderson.org/mchv_interviewsessions/1179/thumbnail.jp

Louise Connally Strong, MD, Oral History Interview, August 10, 2012

Major Topics Covered: Personal and educational background Overview and history of oncology genetics in the sixties and seventies Working with Alfred Knudson Research: longitudinal studies of inherited genetics patterns of neuroblastoma, aniridia, and Wilm’s tumor; discovery of the p53 tumor suppressor genes and link to Li-Fraumeni syndrome, survivorship Women at MD Anderson MD Anderson’s cancer screening program Ethics and genetic testing MD Anderson growth and cultural changehttps://openworks.mdanderson.org/mchv_interviewsessions/1180/thumbnail.jp

Tripartite interactions between two phase qubits and a resonant cavity

The creation and manipulation of multipartite entangled states is important for advancements in quantum computation and communication, and for testing our fundamental understanding of quantum mechanics and precision measurements. Multipartite entanglement has been achieved by use of various forms of quantum bits (qubits), such as trapped ions, photons, and atoms passing through microwave cavities. Quantum systems based on superconducting circuits have been used to control pair-wise interactions of qubits, either directly, through a quantum bus, or via controllable coupling. Here, we describe the first demonstration of coherent interactions of three directly coupled superconducting quantum systems, two phase qubits and a resonant cavity. We introduce a simple Bloch-sphere-like representation to help one visualize the unitary evolution of this tripartite system as it shares a single microwave photon. With careful control and timing of the initial conditions, this leads to a protocol for creating a rich variety of entangled states. Experimentally, we provide evidence for the deterministic evolution from a simple product state, through a tripartite W-state, into a bipartite Bell-state. These experiments are another step towards deterministically generating multipartite entanglement in superconducting systems with more than two qubits

Measurement of the inclusive and dijet cross-sections of b-jets in pp collisions at sqrt(s) = 7 TeV with the ATLAS detector

The inclusive and dijet production cross-sections have been measured for jets containing b-hadrons (b-jets) in proton-proton collisions at a centre-of-mass energy of sqrt(s) = 7 TeV, using the ATLAS detector at the LHC. The measurements use data corresponding to an integrated luminosity of 34 pb^-1. The b-jets are identified using either a lifetime-based method, where secondary decay vertices of b-hadrons in jets are reconstructed using information from the tracking detectors, or a muon-based method where the presence of a muon is used to identify semileptonic decays of b-hadrons inside jets. The inclusive b-jet cross-section is measured as a function of transverse momentum in the range 20 < pT < 400 GeV and rapidity in the range |y| < 2.1. The bbbar-dijet cross-section is measured as a function of the dijet invariant mass in the range 110 < m_jj < 760 GeV, the azimuthal angle difference between the two jets and the angular variable chi in two dijet mass regions. The results are compared with next-to-leading-order QCD predictions. Good agreement is observed between the measured cross-sections and the predictions obtained using POWHEG + Pythia. MC@NLO + Herwig shows good agreement with the measured bbbar-dijet cross-section. However, it does not reproduce the measured inclusive cross-section well, particularly for central b-jets with large transverse momenta.Comment: 10 pages plus author list (21 pages total), 8 figures, 1 table, final version published in European Physical Journal

Observation of associated near-side and away-side long-range correlations in √sNN=5.02 TeV proton-lead collisions with the ATLAS detector

Two-particle correlations in relative azimuthal angle (Δϕ) and pseudorapidity (Δη) are measured in √sNN=5.02  TeV p+Pb collisions using the ATLAS detector at the LHC. The measurements are performed using approximately 1  μb-1 of data as a function of transverse momentum (pT) and the transverse energy (ΣETPb) summed over 3.1<η<4.9 in the direction of the Pb beam. The correlation function, constructed from charged particles, exhibits a long-range (2<|Δη|<5) “near-side” (Δϕ∼0) correlation that grows rapidly with increasing ΣETPb. A long-range “away-side” (Δϕ∼π) correlation, obtained by subtracting the expected contributions from recoiling dijets and other sources estimated using events with small ΣETPb, is found to match the near-side correlation in magnitude, shape (in Δη and Δϕ) and ΣETPb dependence. The resultant Δϕ correlation is approximately symmetric about π/2, and is consistent with a dominant cos⁡2Δϕ modulation for all ΣETPb ranges and particle pT

Structural and biochemical characterization of the exopolysaccharide deacetylase Agd3 required for Aspergillus fumigatus biofilm formation

The exopolysaccharide galactosaminogalactan (GAG) is an important virulence factor of the fungal pathogen Aspergillus fumigatus. Deletion of a gene encoding a putative deacetylase, Agd3, leads to defects in GAG deacetylation, biofilm formation, and virulence. Here, we show that Agd3 deacetylates GAG in a metal-dependent manner, and is the founding member of carbohydrate esterase family CE18. The active site is formed by four catalytic motifs that are essential for activity. The structure of Agd3 includes an elongated substrate-binding cleft formed by a carbohydrate binding module (CBM) that is the founding member of CBM family 87. Agd3 homologues are encoded in previously unidentified putative bacterial exopolysaccharide biosynthetic operons and in other fungal genomes. The exopolysaccharide galactosaminogalactan (GAG) is an important virulence factor of the fungal pathogen Aspergillus fumigatus. Here, the authors study an A. fumigatus enzyme that deacetylates GAG in a metal-dependent manner and constitutes a founding member of a new carbohydrate esterase family.Bio-organic Synthesi