425 results on '"Marshall, Robert P."'
Search Results
2. Locating the Site of the Battle of Medina: A Research Note
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Marshall, Robert P.
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- 2016
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3. The Battle of the Alazán: First Texas Republic Victorious
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Marshall, Robert P.
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- 2015
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4. Locating the Battle of Rosillo: A Newly Discovered Map Indicates the Likely Site of the 1813 Battle where the First Republic of Texas Was Born
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Marshall, Robert P.
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- 2015
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5. Lightning-induced relativistic electron precipitation from the inner radiation belt
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Feinland, Max, Blum, Lauren W., Marshall, Robert A., Gan, Longzhi, Shumko, Mykhaylo, and Looper, Mark
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- 2024
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6. Echocardiographic assessment of left ventricular volumes: a comparison of different methods in athletes
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Kandels, Joscha, Denk, Verena, Pedersen, Maria Weinkouff, Kragholm, Kristian Hay, Søgaard, Peter, Tayal, Bhupendar, Marshall, Robert Percy, Denecke, Timm, Lindgren, Filip Lyng, Hagendorff, Andreas, and Stöbe, Stephan
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- 2024
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7. A Test of Energetic Particle Precipitation Models Using Simultaneous Incoherent Scatter Radar and Van Allen Probes Observations.
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Sanchez, Ennio R, Ma, Qianli, Xu, Wei, Marshall, Robert A, Bortnik, Jacob, Reyes, Pablo, Varney, Roger, and Kaeppler, Stephen
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Astronomical and Space Sciences ,Atmospheric Sciences - Abstract
Quantification of energetic electron precipitation caused by wave-particle interactions is fundamentally important to understand the cycle of particle energization and loss of the radiation belts. One important way to determine how well the wave-particle interaction models predict losses through pitch-angle scattering into the atmospheric loss cone is the direct comparison between the ionization altitude profiles expected in the atmosphere due to the precipitating fluxes and the ionization profiles actually measured with incoherent scatter radars. This paper reports such a comparison using a forward propagation of loss-cone electron fluxes, calculated with the electron pitch angle diffusion model applied to Van Allen Probes measurements, coupled with the Boulder Electron Radiation to Ionization model, which propagates the fluxes into the atmosphere. The density profiles measured with the Poker Flat Incoherent Scatter Radar operating in modes especially designed to optimize measurements in the D-region, show multiple instances of close quantitative agreement with predicted density profiles from precipitation of electrons caused by wave-particle interactions in the inner magnetosphere, alternated with intervals with large differences between observations and predictions. Several-minute long intervals of close prediction-observation approximation in the 65-93 km altitude range indicate that the whistler wave-electron interactions models are realistic and produce precipitation fluxes of electrons with energies between 10 keV and >100 keV that are consistent with observations. The alternation of close model-data agreement and poor agreement intervals indicates that the regions causing energetic electron precipitation are highly spatially localized.
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- 2022
8. Installation of the Dark Energy Spectroscopic Instrument at the Mayall 4-meter telescope
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Besuner, Robert, Allen, Lori, Baltay, Charles, Brooks, David, Carton, Pierre-Henri, Doel, Peter, Donaldson, John, Duan, Yutong, Dunlop, Patrick, Edelstein, Jerry, Evatt, Matt, Fagrelius, Parker, Gaztañaga, Enrique, Guenther, Derek, Gutierrez, Gaston, Hawes, Michael, Honscheid, Klaus, Jelinsky, Pat, Joyce, Richard, Karcher, Armin, Landriau, Martin, Levi, Michael, Magneville, Christophe, Marshall, Robert, Martini, Paul, Pappalardo, Daniel, Poppett, Claire, Prada, Francisco, Ross, Ashley J., Schubnell, Michael, Sharples, Ray, Shourt, William, Silber, Joseph, Sprayberry, David, Stupak, Bob, Tarle, Gregory, and Zhang, Kai
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The Dark Energy Spectroscopic Instrument (DESI) is a Stage IV ground-based dark energy experiment that will measure the expansion history of the Universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasars over 14000 square degrees will be measured during the life of the experiment. We describe the installation of the major elements of the instrument at the Mayall 4m telescope, completed in late 2019. The previous prime focus corrector, spider vanes, and upper rings were removed from the Mayall's Serrurier truss and replaced with the newly-constructed DESI ring, vanes, cage, hexapod, and optical corrector. The new corrector was optically aligned with the primary mirror using a laser tracker system. The DESI focal plane system was integrated to the corrector, with each of its ten 500-fiber-positioner petal segments installed using custom installation hardware and the laser tracker. Ten DESI spectrographs with 30 cryostats were installed in a newly assembled clean room in the Large Coude Room. The ten cables carrying 5000 optical fibers from the positioners in the focal plane were routed down the telescope through cable wraps at the declination and hour angle axes, and their integral slitheads were integrated with the ten spectrographs. The fiber view camera assembly was installed to the Mayall's primary mirror cell. Servers for the instrument control system replaced existing computer equipment. The fully integrated instrument has been commissioned and is ready to start its operations phase.
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- 2021
9. Prähabilitation bei Verletzungen des vorderen Kreuzbandes
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Valle, Christina, Marshall, Robert, and Mengis, Natalie
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- 2023
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10. The DESI Instrument Control System: Status and Early Testing
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Honscheid, Klaus, Elliott, Ann, Buckley-Geer, Elizabeth, Abreshi, Bezhad, Castender, Francisco, daCosta, Luiz, Kent, Stephen, Kirkby, David, Marshall, Robert, Neilsen, Eric, Ogando, Riccardo, Rabinowitz, David, roodman, Aaron, Serrano, Santiago, Brooks, David, Levi, Michael, and Tarle, Greg
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The Dark Energy Spectroscopic Instrument (DESI) is a new instrument currently under construction for the Mayall 4-m telescope at Kitt Peak National Observatory. It will consist of a wide-field optical corrector with a 3.2 degree diameter field of view, a focal plane with 5,000 robotically controlled fiber positioners and 10 fiber-fed broad-band spectrographs. The DESI Instrument Control System (ICS) coordinates fiber positioner operations, interfaces to the Mayall telescope control system, monitors operating conditions, reads out the 30 spectrograph CCDs and provides observer support and data quality monitoring. In this article, we summarize the ICS design, review the current status of the project and present results from a multi-stage test plan that was developed to ensure the system is fully operational by the time the instrument arrives at the observatory in 2019., Comment: SPIE Astronomical Telescopes + Instrumentation, Austin, TX (2018)
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- 2018
11. Overview of the DESI Legacy Imaging Surveys
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Dey, Arjun, Schlegel, David J, Lang, Dustin, Blum, Robert, Burleigh, Kaylan, Fan, Xiaohui, Findlay, Joseph R, Finkbeiner, Doug, Herrera, David, Juneau, Stéphanie, Landriau, Martin, Levi, Michael, McGreer, Ian, Meisner, Aaron, Myers, Adam D, Moustakas, John, Nugent, Peter, Patej, Anna, Schlafly, Edward F, Walker, Alistair R, Valdes, Francisco, Weaver, Benjamin A, Yèche, Christophe, Zou, Hu, Zhou, Xu, Abareshi, Behzad, Abbott, TMC, Abolfathi, Bela, Aguilera, C, Alam, Shadab, Allen, Lori, Alvarez, A, Annis, James, Ansarinejad, Behzad, Aubert, Marie, Beechert, Jacqueline, Bell, Eric F, BenZvi, Segev Y, Beutler, Florian, Bielby, Richard M, Bolton, Adam S, Briceño, César, Buckley-Geer, Elizabeth J, Butler, Karen, Calamida, Annalisa, Carlberg, Raymond G, Carter, Paul, Casas, Ricard, Castander, Francisco J, Choi, Yumi, Comparat, Johan, Cukanovaite, Elena, Delubac, Timothée, DeVries, Kaitlin, Dey, Sharmila, Dhungana, Govinda, Dickinson, Mark, Ding, Zhejie, Donaldson, John B, Duan, Yutong, Duckworth, Christopher J, Eftekharzadeh, Sarah, Eisenstein, Daniel J, Etourneau, Thomas, Fagrelius, Parker A, Farihi, Jay, Fitzpatrick, Mike, Font-Ribera, Andreu, Fulmer, Leah, Gänsicke, Boris T, Gaztanaga, Enrique, George, Koshy, Gerdes, David W, Gontcho, Satya Gontcho A, Gorgoni, Claudio, Green, Gregory, Guy, Julien, Harmer, Diane, Hernandez, M, Honscheid, Klaus, Huang, Lijuan, James, David J, Jannuzi, Buell T, Jiang, Linhua, Joyce, Richard, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Jean-Paul, Kneib, Kueter-Young, Andrea, Lan, Ting-Wen, Lauer, Tod R, Le Guillou, Laurent, Le Van Suu, Auguste, Lee, Jae Hyeon, Lesser, Michael, Levasseur, Laurence Perreault, Li, Ting S, Mann, Justin L, and Marshall, Robert
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Space Sciences ,Physical Sciences ,catalogs ,surveys ,astro-ph.IM ,Astronomical and Space Sciences ,Astronomy & Astrophysics ,Astronomical sciences ,Particle and high energy physics - Abstract
The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ≈14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contiguous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. In addition to calibrated images, the project is delivering a catalog, constructed by using a probabilistic inference-based approach to estimate source shapes and brightnesses. The catalog includes photometry from the grz optical bands and from four mid-infrared bands (at 3.4, 4.6, 12, and 22 μm) observed by the Wide-field Infrared Survey Explorer satellite during its full operational lifetime. The project plans two public data releases each year. All the software used to generate the catalogs is also released with the data. This paper provides an overview of the Legacy Surveys project.
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- 2019
12. ProtoDESI: First On-Sky Technology Demonstration for the Dark Energy Spectroscopic Instrument
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Fagrelius, Parker, Abareshi, Behzad, Allen, Lori, Ballester, Otger, Baltay, Charles, Besuner, Robert, Buckley-Geer, Elizabeth, Butler, Karen, Cardiel, Laia, Dey, Arjun, Elliott, Ann, Emmet, William, Gershkovich, Irena, Honscheid, Klaus, Illa, Jose M., Jimenez, Jorge, Levi, Michael, Manser, Christopher, Marshall, Robert, Martini, Paul, Paat, Anthony, Probst, Ronald, Rabinowitz, David, Reil, Kevin, Robertson, Amy, Rockosi, Connie, Schlegel, David, Schubnell, Michael, Serrano, Santiago, Silber, Joseph, Soto, Christian, Sprayberry, David, Summers, David, Tarle, Greg, Weaver, Benjamin A., and Duan, Y. T.
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The Dark Energy Spectroscopic Instrument (DESI) is under construction to measure the expansion history of the universe using the baryon acoustic oscillations technique. The spectra of 35 million galaxies and quasars over 14,000 square degrees will be measured during a 5-year survey. A new prime focus corrector for the Mayall telescope at Kitt Peak National Observatory will deliver light to 5,000 individually targeted fiber-fed robotic positioners. The fibers in turn feed ten broadband multi-object spectrographs. We describe the ProtoDESI experiment, that was installed and commissioned on the 4-m Mayall telescope from August 14 to September 30, 2016. ProtoDESI was an on-sky technology demonstration with the goal to reduce technical risks associated with aligning optical fibers with targets using robotic fiber positioners and maintaining the stability required to operate DESI. The ProtoDESI prime focus instrument, consisting of three fiber positioners, illuminated fiducials, and a guide camera, was installed behind the existing Mosaic corrector on the Mayall telescope. A Fiber View Camera was mounted in the Cassegrain cage of the telescope and provided feedback metrology for positioning the fibers. ProtoDESI also provided a platform for early integration of hardware with the DESI Instrument Control System that controls the subsystems, provides communication with the Telescope Control System, and collects instrument telemetry data. Lacking a spectrograph, ProtoDESI monitored the output of the fibers using a Fiber Photometry Camera mounted on the prime focus instrument. ProtoDESI was successful in acquiring targets with the robotically positioned fibers and demonstrated that the DESI guiding requirements can be met., Comment: Accepted version
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- 2017
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13. The DESI Experiment Part I: Science,Targeting, and Survey Design
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DESI Collaboration, Aghamousa, Amir, Aguilar, Jessica, Ahlen, Steve, Alam, Shadab, Allen, Lori E., Prieto, Carlos Allende, Annis, James, Bailey, Stephen, Balland, Christophe, Ballester, Otger, Baltay, Charles, Beaufore, Lucas, Bebek, Chris, Beers, Timothy C., Bell, Eric F., Bernal, José Luis, Besuner, Robert, Beutler, Florian, Blake, Chris, Bleuler, Hannes, Blomqvist, Michael, Blum, Robert, Bolton, Adam S., Briceno, Cesar, Brooks, David, Brownstein, Joel R., Buckley-Geer, Elizabeth, Burden, Angela, Burtin, Etienne, Busca, Nicolas G., Cahn, Robert N., Cai, Yan-Chuan, Cardiel-Sas, Laia, Carlberg, Raymond G., Carton, Pierre-Henri, Casas, Ricard, Castander, Francisco J., Cervantes-Cota, Jorge L., Claybaugh, Todd M., Close, Madeline, Coker, Carl T., Cole, Shaun, Comparat, Johan, Cooper, Andrew P., Cousinou, M. -C., Crocce, Martin, Cuby, Jean-Gabriel, Cunningham, Daniel P., Davis, Tamara M., Dawson, Kyle S., de la Macorra, Axel, De Vicente, Juan, Delubac, Timothée, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Ding, Zhejie, Doel, Peter, Duan, Yutong T., Ealet, Anne, Edelstein, Jerry, Eftekharzadeh, Sarah, Eisenstein, Daniel J., Elliott, Ann, Escoffier, Stéphanie, Evatt, Matthew, Fagrelius, Parker, Fan, Xiaohui, Fanning, Kevin, Farahi, Arya, Farihi, Jay, Favole, Ginevra, Feng, Yu, Fernandez, Enrique, Findlay, Joseph R., Finkbeiner, Douglas P., Fitzpatrick, Michael J., Flaugher, Brenna, Flender, Samuel, Font-Ribera, Andreu, Forero-Romero, Jaime E., Fosalba, Pablo, Frenk, Carlos S., Fumagalli, Michele, Gaensicke, Boris T., Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Fusillo, Nicola Pietro Gentile, Gerard, Terry, Gershkovich, Irena, Giannantonio, Tommaso, Gillet, Denis, Gonzalez-de-Rivera, Guillermo, Gonzalez-Perez, Violeta, Gott, Shelby, Graur, Or, Gutierrez, Gaston, Guy, Julien, Habib, Salman, Heetderks, Henry, Heetderks, Ian, Heitmann, Katrin, Hellwing, Wojciech A., Herrera, David A., Ho, Shirley, Holland, Stephen, Honscheid, Klaus, Huff, Eric, Hutchinson, Timothy A., Huterer, Dragan, Hwang, Ho Seong, Laguna, Joseph Maria Illa, Ishikawa, Yuzo, Jacobs, Dianna, Jeffrey, Niall, Jelinsky, Patrick, Jennings, Elise, Jiang, Linhua, Jimenez, Jorge, Johnson, Jennifer, Joyce, Richard, Jullo, Eric, Juneau, Stéphanie, Kama, Sami, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kennamer, Noble, Kent, Stephen, Kilbinger, Martin, Kim, Alex G., Kirkby, David, Kisner, Theodore, Kitanidis, Ellie, Kneib, Jean-Paul, Koposov, Sergey, Kovacs, Eve, Koyama, Kazuya, Kremin, Anthony, Kron, Richard, Kronig, Luzius, Kueter-Young, Andrea, Lacey, Cedric G., Lafever, Robin, Lahav, Ofer, Lambert, Andrew, Lampton, Michael, Landriau, Martin, Lang, Dustin, Lauer, Tod R., Goff, Jean-Marc Le, Guillou, Laurent Le, Van Suu, Auguste Le, Lee, Jae Hyeon, Lee, Su-Jeong, Leitner, Daniela, Lesser, Michael, Levi, Michael E., L'Huillier, Benjamin, Li, Baojiu, Liang, Ming, Lin, Huan, Linder, Eric, Loebman, Sarah R., Lukić, Zarija, Ma, Jun, MacCrann, Niall, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Manser, Christopher J., Marshall, Robert, Martini, Paul, Massey, Richard, Matheson, Thomas, McCauley, Jeremy, McDonald, Patrick, McGreer, Ian D., Meisner, Aaron, Metcalfe, Nigel, Miller, Timothy N., Miquel, Ramon, Moustakas, John, Myers, Adam, Naik, Milind, Newman, Jeffrey A., Nichol, Robert C., Nicola, Andrina, da Costa, Luiz Nicolati, Nie, Jundan, Niz, Gustavo, Norberg, Peder, Nord, Brian, Norman, Dara, Nugent, Peter, O'Brien, Thomas, Oh, Minji, Olsen, Knut A. G., Padilla, Cristobal, Padmanabhan, Hamsa, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Palmese, Antonella, Pappalardo, Daniel, Pâris, Isabelle, Park, Changbom, Patej, Anna, Peacock, John A., Peiris, Hiranya V., Peng, Xiyan, Percival, Will J., Perruchot, Sandrine, Pieri, Matthew M., Pogge, Richard, Pollack, Jennifer E., Poppett, Claire, Prada, Francisco, Prakash, Abhishek, Probst, Ronald G., Rabinowitz, David, Raichoor, Anand, Ree, Chang Hee, Refregier, Alexandre, Regal, Xavier, Reid, Beth, Reil, Kevin, Rezaie, Mehdi, Rockosi, Constance M., Roe, Natalie, Ronayette, Samuel, Roodman, Aaron, Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rozo, Eduardo, Ruhlmann-Kleider, Vanina, Rykoff, Eli S., Sabiu, Cristiano, Samushia, Lado, Sanchez, Eusebio, Sanchez, Javier, Schlegel, David J., Schneider, Michael, Schubnell, Michael, Secroun, Aurélia, Seljak, Uros, Seo, Hee-Jong, Serrano, Santiago, Shafieloo, Arman, Shan, Huanyuan, Sharples, Ray, Sholl, Michael J., Shourt, William V., Silber, Joseph H., Silva, David R., Sirk, Martin M., Slosar, Anze, Smith, Alex, Smoot, George F., Som, Debopam, Song, Yong-Seon, Sprayberry, David, Staten, Ryan, Stefanik, Andy, Tarle, Gregory, Tie, Suk Sien, Tinker, Jeremy L., Tojeiro, Rita, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Vargas-Magana, Mariana, Verde, Licia, Walker, Alistair R., Wang, Jiali, Wang, Yuting, Weaver, Benjamin A., Weaverdyck, Curtis, Wechsler, Risa H., Weinberg, David H., White, Martin, Yang, Qian, Yeche, Christophe, Zhang, Tianmeng, Zhao, Gong-Bo, Zheng, Yi, Zhou, Xu, Zhou, Zhimin, Zhu, Yaling, Zou, Hu, and Zu, Ying
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. To trace the underlying dark matter distribution, spectroscopic targets will be selected in four classes from imaging data. We will measure luminous red galaxies up to $z=1.0$. To probe the Universe out to even higher redshift, DESI will target bright [O II] emission line galaxies up to $z=1.7$. Quasars will be targeted both as direct tracers of the underlying dark matter distribution and, at higher redshifts ($ 2.1 < z < 3.5$), for the Ly-$\alpha$ forest absorption features in their spectra, which will be used to trace the distribution of neutral hydrogen. When moonlight prevents efficient observations of the faint targets of the baseline survey, DESI will conduct a magnitude-limited Bright Galaxy Survey comprising approximately 10 million galaxies with a median $z\approx 0.2$. In total, more than 30 million galaxy and quasar redshifts will be obtained to measure the BAO feature and determine the matter power spectrum, including redshift space distortions.
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- 2016
14. The DESI Experiment Part II: Instrument Design
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DESI Collaboration, Aghamousa, Amir, Aguilar, Jessica, Ahlen, Steve, Alam, Shadab, Allen, Lori E., Prieto, Carlos Allende, Annis, James, Bailey, Stephen, Balland, Christophe, Ballester, Otger, Baltay, Charles, Beaufore, Lucas, Bebek, Chris, Beers, Timothy C., Bell, Eric F., Bernal, José Luis, Besuner, Robert, Beutler, Florian, Blake, Chris, Bleuler, Hannes, Blomqvist, Michael, Blum, Robert, Bolton, Adam S., Briceno, Cesar, Brooks, David, Brownstein, Joel R., Buckley-Geer, Elizabeth, Burden, Angela, Burtin, Etienne, Busca, Nicolas G., Cahn, Robert N., Cai, Yan-Chuan, Cardiel-Sas, Laia, Carlberg, Raymond G., Carton, Pierre-Henri, Casas, Ricard, Castander, Francisco J., Cervantes-Cota, Jorge L., Claybaugh, Todd M., Close, Madeline, Coker, Carl T., Cole, Shaun, Comparat, Johan, Cooper, Andrew P., Cousinou, M. -C., Crocce, Martin, Cuby, Jean-Gabriel, Cunningham, Daniel P., Davis, Tamara M., Dawson, Kyle S., de la Macorra, Axel, De Vicente, Juan, Delubac, Timothée, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Ding, Zhejie, Doel, Peter, Duan, Yutong T., Ealet, Anne, Edelstein, Jerry, Eftekharzadeh, Sarah, Eisenstein, Daniel J., Elliott, Ann, Escoffier, Stéphanie, Evatt, Matthew, Fagrelius, Parker, Fan, Xiaohui, Fanning, Kevin, Farahi, Arya, Farihi, Jay, Favole, Ginevra, Feng, Yu, Fernandez, Enrique, Findlay, Joseph R., Finkbeiner, Douglas P., Fitzpatrick, Michael J., Flaugher, Brenna, Flender, Samuel, Font-Ribera, Andreu, Forero-Romero, Jaime E., Fosalba, Pablo, Frenk, Carlos S., Fumagalli, Michele, Gaensicke, Boris T., Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Fusillo, Nicola Pietro Gentile, Gerard, Terry, Gershkovich, Irena, Giannantonio, Tommaso, Gillet, Denis, Gonzalez-de-Rivera, Guillermo, Gonzalez-Perez, Violeta, Gott, Shelby, Graur, Or, Gutierrez, Gaston, Guy, Julien, Habib, Salman, Heetderks, Henry, Heetderks, Ian, Heitmann, Katrin, Hellwing, Wojciech A., Herrera, David A., Ho, Shirley, Holland, Stephen, Honscheid, Klaus, Huff, Eric, Hutchinson, Timothy A., Huterer, Dragan, Hwang, Ho Seong, Laguna, Joseph Maria Illa, Ishikawa, Yuzo, Jacobs, Dianna, Jeffrey, Niall, Jelinsky, Patrick, Jennings, Elise, Jiang, Linhua, Jimenez, Jorge, Johnson, Jennifer, Joyce, Richard, Jullo, Eric, Juneau, Stéphanie, Kama, Sami, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kennamer, Noble, Kent, Stephen, Kilbinger, Martin, Kim, Alex G., Kirkby, David, Kisner, Theodore, Kitanidis, Ellie, Kneib, Jean-Paul, Koposov, Sergey, Kovacs, Eve, Koyama, Kazuya, Kremin, Anthony, Kron, Richard, Kronig, Luzius, Kueter-Young, Andrea, Lacey, Cedric G., Lafever, Robin, Lahav, Ofer, Lambert, Andrew, Lampton, Michael, Landriau, Martin, Lang, Dustin, Lauer, Tod R., Goff, Jean-Marc Le, Guillou, Laurent Le, Van Suu, Auguste Le, Lee, Jae Hyeon, Lee, Su-Jeong, Leitner, Daniela, Lesser, Michael, Levi, Michael E., L'Huillier, Benjamin, Li, Baojiu, Liang, Ming, Lin, Huan, Linder, Eric, Loebman, Sarah R., Lukić, Zarija, Ma, Jun, MacCrann, Niall, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Manser, Christopher J., Marshall, Robert, Martini, Paul, Massey, Richard, Matheson, Thomas, McCauley, Jeremy, McDonald, Patrick, McGreer, Ian D., Meisner, Aaron, Metcalfe, Nigel, Miller, Timothy N., Miquel, Ramon, Moustakas, John, Myers, Adam, Naik, Milind, Newman, Jeffrey A., Nichol, Robert C., Nicola, Andrina, da Costa, Luiz Nicolati, Nie, Jundan, Niz, Gustavo, Norberg, Peder, Nord, Brian, Norman, Dara, Nugent, Peter, O'Brien, Thomas, Oh, Minji, Olsen, Knut A. G., Padilla, Cristobal, Padmanabhan, Hamsa, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Palmese, Antonella, Pappalardo, Daniel, Pâris, Isabelle, Park, Changbom, Patej, Anna, Peacock, John A., Peiris, Hiranya V., Peng, Xiyan, Percival, Will J., Perruchot, Sandrine, Pieri, Matthew M., Pogge, Richard, Pollack, Jennifer E., Poppett, Claire, Prada, Francisco, Prakash, Abhishek, Probst, Ronald G., Rabinowitz, David, Raichoor, Anand, Ree, Chang Hee, Refregier, Alexandre, Regal, Xavier, Reid, Beth, Reil, Kevin, Rezaie, Mehdi, Rockosi, Constance M., Roe, Natalie, Ronayette, Samuel, Roodman, Aaron, Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rozo, Eduardo, Ruhlmann-Kleider, Vanina, Rykoff, Eli S., Sabiu, Cristiano, Samushia, Lado, Sanchez, Eusebio, Sanchez, Javier, Schlegel, David J., Schneider, Michael, Schubnell, Michael, Secroun, Aurélia, Seljak, Uros, Seo, Hee-Jong, Serrano, Santiago, Shafieloo, Arman, Shan, Huanyuan, Sharples, Ray, Sholl, Michael J., Shourt, William V., Silber, Joseph H., Silva, David R., Sirk, Martin M., Slosar, Anze, Smith, Alex, Smoot, George F., Som, Debopam, Song, Yong-Seon, Sprayberry, David, Staten, Ryan, Stefanik, Andy, Tarle, Gregory, Tie, Suk Sien, Tinker, Jeremy L., Tojeiro, Rita, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Vargas-Magana, Mariana, Verde, Licia, Walker, Alistair R., Wang, Jiali, Wang, Yuting, Weaver, Benjamin A., Weaverdyck, Curtis, Wechsler, Risa H., Weinberg, David H., White, Martin, Yang, Qian, Yeche, Christophe, Zhang, Tianmeng, Zhao, Gong-Bo, Zheng, Yi, Zhou, Xu, Zhou, Zhimin, Zhu, Yaling, Zou, Hu, and Zu, Ying
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. The DESI instrument is a robotically-actuated, fiber-fed spectrograph capable of taking up to 5,000 simultaneous spectra over a wavelength range from 360 nm to 980 nm. The fibers feed ten three-arm spectrographs with resolution $R= \lambda/\Delta\lambda$ between 2000 and 5500, depending on wavelength. The DESI instrument will be used to conduct a five-year survey designed to cover 14,000 deg$^2$. This powerful instrument will be installed at prime focus on the 4-m Mayall telescope in Kitt Peak, Arizona, along with a new optical corrector, which will provide a three-degree diameter field of view. The DESI collaboration will also deliver a spectroscopic pipeline and data management system to reduce and archive all data for eventual public use.
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- 2016
15. ProtoDESI: First On-Sky Technology Demonstration for the Dark Energy Spectroscopic Instrument
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Fagrelius, Parker, Abareshi, Behzad, Allen, Lori, Ballester, Otger, Baltay, Charles, Besuner, Robert, Buckley-Geer, Elizabeth, Butler, Karen, Cardiel, Laia, Dey, Arjun, Duan, Yutong, Elliott, Ann, Emmet, William, Gershkovich, Irena, Honscheid, Klaus, Illa, Jose M, Jimenez, Jorge, Joyce, Richard, Karcher, Armin, Kent, Stephen, Lambert, Andrew, Lampton, Michael, Levi, Michael, Manser, Christopher, Marshall, Robert, Martini, Paul, Paat, Anthony, Probst, Ronald, Rabinowitz, David, Reil, Kevin, Robertson, Amy, Rockosi, Connie, Schlegel, David, Schubnell, Michael, Serrano, Santiago, Silber, Joseph, Soto, Christian, Sprayberry, David, Summers, David, Tarlé, Greg, and Weaver, Benjamin A
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Particle and High Energy Physics ,Astronomical Sciences ,Physical Sciences ,instrumentation: miscellaneous ,methods: observational ,telescopes ,(cosmology:) dark energy ,astro-ph.IM ,Astronomical and Space Sciences ,Astronomy & Astrophysics ,Astronomical sciences ,Particle and high energy physics - Abstract
The Dark Energy Spectroscopic Instrument (DESI) is under construction to measure the expansion history of the universe using the baryon acoustic oscillations technique. The spectra of 35 million galaxies and quasars over 14,000 square degrees will be measured during a 5-year survey. A new prime focus corrector for the Mayall telescope at Kitt Peak National Observatory will deliver light to 5,000 individually targeted fiber-fed robotic positioners. The fibers in turn feed ten broadband multi-object spectrographs. We describe the ProtoDESI experiment, that was installed and commissioned on the 4-m Mayall telescope from 2016 August 14 to September 30. ProtoDESI was an on-sky technology demonstration with the goal to reduce technical risks associated with aligning optical fibers with targets using robotic fiber positioners and maintaining the stability required to operate DESI. The ProtoDESI prime focus instrument, consisting of three fiber positioners, illuminated fiducials, and a guide camera, was installed behind the existing Mosaic corrector on the Mayall telescope. A fiber view camera was mounted in the Cassegrain cage of the telescope and provided feedback metrology for positioning the fibers. ProtoDESI also provided a platform for early integration of hardware with the DESI Instrument Control System that controls the subsystems, provides communication with the Telescope Control System, and collects instrument telemetry data. Lacking a spectrograph, ProtoDESI monitored the output of the fibers using a fiber photometry camera mounted on the prime focus instrument. ProtoDESI was successful in acquiring targets with the robotically positioned fibers and demonstrated that the DESI guiding requirements can be met.
- Published
- 2018
16. Analysis of left ventricular rotational deformation by 2D speckle tracking echocardiography: a feasibility study in athletes
- Author
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Hofrichter, Phillipp, Hagendorff, Andreas, Laufs, Ulrich, Fikenzer, Sven, Hepp, Pierre, Marshall, Robert Percy, Tayal, Bhupendar, and Stöbe, Stephan
- Published
- 2021
- Full Text
- View/download PDF
17. Possible new options and benefits to detect myocarditis, right ventricular remodeling and coronary anomalies by echocardiography in systematic preparticipation screening of athletes
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Döbel, Tom, Stöbe, Stephan, Marshall, Robert Percy, Hepp, Pierre, Fikenzer, Sven, Fikenzer, Kati, Tautenhahn, Sandra, Laufs, Ulrich, and Hagendorff, Andreas
- Published
- 2020
- Full Text
- View/download PDF
18. Alaska Wilderness : Exploring the Central Brooks Range, Second Edition
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MARSHALL, ROBERT, Marshall, George, Edited, with Introductions by, Leopold, A. Starker, Foreword by, MARSHALL, ROBERT, Marshall, George, and Leopold, A. Starker
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- 2023
- Full Text
- View/download PDF
19. Laparoscopic vs. open feeding jejunostomy insertion in oesophagogastric cancer
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Mastoridis, Sotiris, Bracalente, Giada, Hanganu, Christine-Bianca, Neccia, Michela, Giuliani, Antonio, Gillies, Richard, Marshall, Robert, Maynard, Nicholas, and Sgromo, Bruno
- Published
- 2021
- Full Text
- View/download PDF
20. Polish Post-Secondary Vocational Schools and Canadian Community Colleges: International Perspectives
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Butler, Norman L., Pachocinski, Ryszard, Davidson, Barry S., Marshall, Robert L., Kritsonis, Wiilliam Allan, Van Patten, James J., Borman, Kathryn M., Johanningmeier, Erwin, and Orlosfsky, Michael
- Abstract
The aim of this study was to compare Canadian community colleges with post-secondary vocational schools in Poland. The comparison concentrated upon programs in nursing, tourism and information technology delivered by the following three Polish schools Krakowska Szkola Medyczna, (Cracow, Poland), Policealne Studium Zawodowe, (Cracow, Poland), Cracow School of Information Technology and four Canadian community colleges Red Deer, (Red Deer, Alberta) Centennial (Scarborough, Ontario), Durham (Oshawa, Ontario) and Confederation (Thunder Bay, Ontario). Two research approaches were used in this study: qualitative and quantitative mixed research methodologies. Moreover, the theoretical framework was supplied by the general notion of the school as an organization and social institution. The investigators tried to answer the following research questions. (1) Are post-secondary vocational institutions meeting the requirements of the labor market as well as Canadian community colleges? The predicted answer was "no" because it is easier for colleges to form articulation agreements with schools of higher education than it is for their Polish counterparts. Community colleges in Canada are part of the same post- secondary system of schooling as schools of higher education whereas post-secondary vocational institutions are not--they are part of a secondary school scheme. Articulation agreements allow learners to begin their vocational or academic training in one institution and continue it in another. Labor market requirements are better addressed with comprehensive course transfer agreements. (2) Do Canadian college students have a higher perception of their programs than their Polish post-secondary vocational school counterparts? The predicted answer was "yes" because colleges are higher up in the school structure "pecking order" than post-secondary vocational schools in Poland: post-secondary as opposed to secondary. It was hypothesized that college learners ought to place more value on their programs than their Polish counterparts. The results of our investigation partially supported the predicted answer "no" for question 1--Centennial College's program in tourism has more articulation agreements than their Polish counterpart (Policealne Studium Zawodowe). The predicted answer "yes" was fully confirmed, with regard to question 2. (Contains 12 figures and 8 notes.)
- Published
- 2006
21. Kinetic analysis of 18F-fluorodihydrorotenone as a deposited myocardial flow tracer: Comparison to thallium-201.
- Author
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Marshall, Robert C., Powers-Risius, Patricia, Reutter, Bryan W., O'Neil, James P., La Belle, Michael, Huesman, Ronald H., and VanBrocklin, Henry F.
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Basic biological sciences ,myocardial perfusion fluorodihydrorotenone PET - Abstract
The goal of this investigation was to assess the accuracy of 18F-fluorodihydrorotenone (18F-FDHR) as a new deposited myocardial flow tracer and compare the results to those for 201Tl. Methods. The kinetics of these flow tracers were evaluated in 22 isolated, erythrocyte- and albumin-perfused rabbit hearts over a flow range encountered in patients. The two flow tracers plus a vascular reference tracer (131I-albumin) were introduced as a bolus through a port just above the aortic cannula. Myocardial extraction, retention, washout, and uptake parameters were computed from the venous outflow curves using the multiple indicator dilution technique and spectral analysis. Results. The mean initial extraction fractions of 18F-FDHR (0.85 +- 0.07) and 201Tl (0.87 +- 0.05) were not significantly different, although the initial extraction fraction for 18F-FDHR declined with flow (P < 0.0001), whereas the initial extraction fraction of 201Tl did not. Washout of 201Tl was faster (P < 0.001) and more affected by flow (P < 0.05) than 18F-FDHR washout. Except for initial extraction fraction, 18F-FDHR retention was greater (P < 0.001) and less affected by flow (P < 0.05) than 201Tl retention. Reflecting its superior retention, net uptake of 18F-FDHR was better correlated with flow than 201Tl uptake at both one and fifteen minutes after tracer introduction (P < 0.0001 for both comparisons). Conclusion. The superior correlation of 18F-FDHR uptake with flow indicates that it is a better flow tracer than 201Tl in the isolated rabbit heart. Compared to the other currently available positron-emitting flow tracers (82Rb, 13N-ammonia, and 15O-water), 18F-FDHR has the potential of providing excellent image resolution without the need for an on-site cyclotron.
- Published
- 2004
22. Ecosystem services of geoduck farming in South Puget Sound, USA: a modeling analysis
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Cubillo, Alhambra Martínez, Ferreira, João Gomes, Pearce, Christopher Michael, Marshall, Robert, Cheney, Dan, and Hudson, Bobbi
- Published
- 2018
- Full Text
- View/download PDF
23. Locating the Site of the Battle of Medina: A Research Note
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Marshall, Robert P.
- Published
- 2017
24. Spectral analysis for evaluation of myocardial tracers for medical imaging
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Huesman, Ronald H., Reutter, Bryan W., and Marshall, Robert C.
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Radiology and nuclear medicine - Abstract
Kinetic analysis of dynamic tracer data is performed with the goal of evaluating myocardial radiotracers for cardiac nuclear medicine imaging. Data from experiments utilizing the isolated rabbit heart model are acquired by sampling the venous blood after introduction of a tracer of interest and a reference tracer. We have taken the approach that the kinetics are properly characterized by an impulse response function which describes the difference between the reference molecule (which does not leave the vasculature) and the molecule of interest which is transported across the capillary boundary and is made available to the cell. Using this formalism we can model the appearance of the tracer of interest in the venous output of the heart as a convolution of the appearance of the reference tracer with the impulse response. In this work we parameterize the impulse response function as the sum of a large number of exponential functions whose predetermined decay constants form a spectrum, and each is required only to have a nonnegative coefficient. This approach, called spectral analysis, has the advantage that it allows conventional compartmental analysis without prior knowledge of the number of compartments which the physiology may require or which the data will support.
- Published
- 2000
25. Kinetic Analysis of Rubidium and Thallium as Deposited Myocardial Blood Flow Tracers in Isolated Rabbit Heart
- Author
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Marshall, Robert C.
- Published
- 1996
26. Slavery, Capitalism and the Industrial Revolution.
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Marshall, Robert
- Subjects
SLAVERY ,CAPITALISM ,INDUSTRIAL revolution ,INDUSTRIALISM ,TECHNOLOGICAL revolution - Published
- 2024
27. Collective Decision Making in Rural Japan
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Marshall, Robert C. and Marshall, Robert C.
- Published
- 2020
- Full Text
- View/download PDF
28. Teacher Flow and Its Relationship to School Mindfulness and Enabling School Structure
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Marshall, Robert Paul, III
- Abstract
Teacher flow experience is a phenomenon occurring when a teacher becomes totally absorbed into a given task at hand. The clearest indication of teacher flow is action-awareness merging; or, the degree in which an activity becomes so spontaneous and automatic that teachers lose conscious awareness of themselves as they perform their duties. This study focuses on teacher flow experience and its relationship to school mindfulness and enabling school structure while controlling for socio-economic status. Moreover, the study applies these constructs to 566 elementary, middle and high school faculty members including teachers and administrators from 51 public schools. The study is quantitative in nature. The three constructs are measured through surveys that have been designed for educators in school settings. The unit of analysis for this study is the school. [The dissertation citations contained here are published with the permission of ProQuest LLC. Further reproduction is prohibited without permission. Copies of dissertations may be obtained by Telephone (800) 1-800-521-0600. Web page: http://www.proquest.com/en-US/products/dissertations/individuals.shtml.]
- Published
- 2013
29. Endoscopic mucosal resection of early oesophageal neoplasia in patients requiring anticoagulation: is it safe?
- Author
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Al-Mammari, Said, Owen, Richard, Findlay, John, Koutsoumpas, Andreas, Gillies, Richard, Marshall, Robert, Bailey, Adam A., Maynard, Nick, Sgromo, Bruno, and Braden, Barbara
- Published
- 2016
- Full Text
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30. Osteopetrosis, osteopetrorickets and hypophosphatemic rickets differentially affect dentin and enamel mineralization
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Koehne, Till, Marshall, Robert P., Jeschke, Anke, Kahl-Nieke, Bärbel, Schinke, Thorsten, and Amling, Michael
- Published
- 2013
- Full Text
- View/download PDF
31. Update on a Clinical Measure for the Assessment of Problem Solving
- Author
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Marshall, Robert C. and Karow, Colleen M.
- Abstract
Purpose: The Rapid Assessment of Problem Solving test (RAPS) is a clinical measure of problem solving based on the 20 Questions Test. This article updates clinicians on the RAPS, addresses questions raised about the test in an earlier article (R. C. Marshall, C. M. Karow, C. Morelli, K. Iden, & J. Dixon, 2003a), and discusses the clinical utility of the RAPS. Method: The RAPS was administered to 373 normal adults. Tests were analyzed to assess the impact of demographic, psychometric, and other factors on performance on the RAPS. To determine the effects of strategy selection on test scores, participants were assigned to novel, category-focused, or mixed strategy groups based on the types of first questions asked. Results: Normal participants exhibited a range of performance levels on the RAPS. Participants in the novel strategy group performed significantly better than the participants in 2 other strategy groups. Conclusions: The RAPS is a clinically useful tool to examine problem solving that is easy to administer and to score. Findings suggest clinicians can use the RAPS with greater confidence than was the case 4 years ago. The RAPS is now part of the public domain and may be used by clinicians to assess clients' problem-solving deficits. (Contains 7 tables, 2 figures and 1 footnote.)
- Published
- 2008
- Full Text
- View/download PDF
32. Using Semantic Feature Analysis to Improve Contextual Discourse in Adults with Aphasia
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Rider, Jill Davis, Wright, Heather Harris, and Marshall, Robert C.
- Abstract
Purpose: Semantic feature analysis (SFA) was used to determine whether training contextually related words would improve the discourse of individuals with nonfluent aphasia in preselected contexts. Method: A modified multiple-probes-across-behaviors design was used to train target words using SFA in 3 adults with nonfluent aphasia. Pretreatment, posttreatment, and follow-up sessions obtained language samples for the preselected contexts. Contexts included 4 story retellings and 4 procedure explanations. Results: All participants improved naming ability for treated words. No generalization to untrained items was found. Within discourse samples, participants increased number of target words produced from pretreatment to posttreatment sessions but did not increase lexical diversity across samples. Participants maintained performance on standardized measures from the beginning to the end of the study. Conclusions: Results support and extend previous research by indicating that SFA improves confrontational naming ability and may benefit word retrieval in discourse production of closed-set contexts. (Contains 5 tables and 3 figures.)
- Published
- 2008
- Full Text
- View/download PDF
33. Developing a Clinician-Friendly Aphasia Test
- Author
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Marshall, Robert C. and Wright, Heather Harris
- Abstract
Purpose: The Kentucky Aphasia Test (KAT) is an objective measure of language functioning for persons with aphasia. This article describes materials, administration, and scoring of the KAT; presents the rationale for development of test items; reports information from a pilot study; and discusses the role of the KAT in aphasia assessment. Method: The KAT has 3 parallel test batteries, KAT-1, KAT-2, and KAT-3. Each battery contains the same orientation test and 6 subtests, each with 10 items, assessing expressive and receptive language functions. Subtests for KAT-1, KAT-2, and KAT-3 systematically increase in difficulty so that it is possible to assess individuals with severe, moderate, and mild aphasia, respectively. The KAT was administered to 38 participants with aphasia and 31 non-brain-damaged (NBD) participants. Results: Results with the KAT clearly differentiated the language performance of individuals with and without aphasia. NBD participants made few errors, and overall scores on the test for individuals with aphasia were rarely within 1 "SD" of the NBD group. Performance of the participants with aphasia administered KAT-1, KAT-2, and KAT-3 suggested that the 3 versions of the test represent a hierarchy of difficulty. Conclusions: The KAT remains in its early stages of development. However, it does appear to meet the requirements for a "clinician-friendly" aphasia test and, as such, offers a rapid, convenient means of obtaining an objective score to determine changes in language functioning during the early postonset period. (Contains 4 tables, 1 figure and 1 footnote.)
- Published
- 2007
- Full Text
- View/download PDF
34. Bach and Mozart : Essays on the Enigma of Genius
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Marshall, Robert L. and Marshall, Robert L.
- Published
- 2019
- Full Text
- View/download PDF
35. The Personalized Cueing Method: From the Laboratory to the Clinic
- Author
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Marshall, Robert C. and Freed, Donald B.
- Abstract
Purpose: The personalized cueing method is a novel procedure for treating naming deficits of persons with aphasia that is relatively unfamiliar to most speech-language pathologists. The goal of this article is to introduce the personalized cueing method to clinicians so that it might be expanded and improved upon. It is also hoped that this article will promote further research in the treatment of naming deficits of clients with aphasia. Method: This clinical focus article (a) describes the origins of the personalized cueing method, the steps involved in creating personalized cues, and training and assessment procedures used with the personalized cueing method; (b) summarizes the published research supporting the use of the personalized cueing method; and (c) highlights some of the clinical advantages of this novel naming treatment for clients and clinicians. Results: Research with the personalized cueing method indicates that durability (long-term naming accuracy) for items trained with the personalized cueing method exceeds that for items trained with phonological cueing and other methods. It further shows that as the stimuli used to train naming in the personalized cueing experiments have become more realistic, durability of personalized cueing has increased. Conclusions: Personalized cueing is a parsimonious approach for treatment of naming deficits of persons with aphasia that has shown positive treatment effects in 8-12 training sessions.
- Published
- 2006
- Full Text
- View/download PDF
36. Having the Courage To Be Competent: Persons and Families Living with Aphasia.
- Author
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Marshall, Robert C.
- Abstract
This article provides examples and illustrations of how people with aphasia can and do demonstrate their competence in managing their lives despite chronic aphasia. It discusses a number of ways in which persons with aphasia and their families can learn to live fully despite the intrusion of aphasia. (Contains references.) (Author/CR)
- Published
- 2002
37. Dual-Credit Outcomes: A Second Visit.
- Author
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Marshall, Robert P. and Andrews, Hans A.
- Abstract
Discusses a study of 33 graduates from Marquette High School (Illinois) who participated in a dual-credit program with Illinois Valley Community College. Reports that students welcomed the opportunity to get a head start in college, and that it improved their perceptions of the college they attended. (NB)
- Published
- 2002
38. Short-term activation of liver X receptors inhibits osteoblasts but long-term activation does not have an impact on murine bone in vivo
- Author
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Prawitt, Janne, Beil, F. Timo, Marshall, Robert P., Bartelt, Alexander, Ruether, Wolfgang, Heeren, Joerg, Amling, Michael, Staels, Bart, and Niemeier, Andreas
- Published
- 2011
- Full Text
- View/download PDF
39. Guide to Databases Containing Data on Vocational and Adult Education Maintained by the U.S. Department of Education.
- Author
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Office of Vocational and Adult Education (ED), Washington, DC. and Marshall, Robert E.
- Abstract
This guide provides information on 22 databases maintained within the United States Department of Education in which information on vocational and/or adult education has been identified, including those housed in the Office of Vocational and Adult Education (OVAE). The guide was developed by conducting an in-house survey, and the information it contains has been reviewed by those listed as contact persons for their databases. Each one-page database profile consists of a description, design, survey type, how often data are collected, planned updates, and contact address. The databases included are the following: (1) Administrator and Teacher Survey of High School and Beyond Schools; (2) 1987 High School Transcript Study; (3) National Education Longitudinal Survey, 1988; (4) High School and Beyond Longitudinal Study; (5) National Longitudinal Survey, 1972; (6) Schools and Staffing Survey; (7) Beginning Postsecondary Students; (8) Integrated Postsecondary Education Data System; (9) National Postsecondary Student Aid Study; (10) Fast Response Survey System for National Assessment of Vocational Education; (11) Vocational-Technical Education Financial Database; (12) Vocational-Technical Education Program Performance Database; (13) Adult Education Financial Database; (14) Adult Education Program Performance Database; (15) Common Core of Data Part 4--Revenues and Current Expenditures for Public Elementary and Secondary Education FY 82-86; (16) Common Core of Data Public Education Agency Universe, 1987-88; (17) Inventory of Datasets Containing Data on OVAE-Administered Programs; (18) National Rural Education Data File; Expenditures for Public Elementary and Secondary Education FY 82-86; (19) Common Core of Data Public School Universe, 1986-87; (20) Common Core of Data Nonfiscal Report, 1987-88; (21) State Program Improvement Information in Vocational Education; and (22) GEPA 406A Data System. (KC)
- Published
- 1989
40. The phenotypic and molecular genetic spectrum of Alström syndrome in 44 Turkish kindreds and a literature review of Alström syndrome in Turkey
- Author
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Ozantürk, Ayşegül, Marshall, Jan D, Collin, Gayle B, Düzenli, Selma, Marshall, Robert P, Candan, Şükrü, Tos, Tülay, Esen, İhsan, Taşkesen, Mustafa, Çayır, Atilla, Öztürk, Şükrü, Üstün, İhsan, Ataman, Esra, Karaca, Emin, Özdemir, Taha Reşid, Erol, İlknur, Eroğlu, Fehime Kara, Torun, Deniz, Parıltay, Erhan, Yılmaz-Güleç, Elif, Karaca, Ender, Atabek, M Emre, Elçioğlu, Nursel, Satman, İlhan, Möller, Claes, Muller, Jean, Naggert, Jürgen K, and Özgül, Rıza Köksal
- Published
- 2015
- Full Text
- View/download PDF
41. Individual Risk Modelling for Esophagectomy: A Systematic Review
- Author
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Findlay, John M., Gillies, Richard S., Sgromo, Bruno, Marshall, Robert E. K., Middleton, Mark R., and Maynard, Nicholas D.
- Published
- 2014
- Full Text
- View/download PDF
42. Assessment of social marketing education, training, and application in public health settings
- Author
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Biroscak, Brian J., Lefebvre, R. Craig, Schneider, Tali, Marshall, Robert J., McDermott, Robert J., and Bryant, Carol A.
- Published
- 2014
- Full Text
- View/download PDF
43. Cartel issues in plain sight
- Author
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Kovacic, William E, Marshall, Robert C, and Meurer, Michael J
- Published
- 2023
- Full Text
- View/download PDF
44. Challenging High School Honor Students with Community College Courses.
- Author
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Andrews, Hans A. and Marshall, Robert P.
- Abstract
Describes a program whereby Illinois Valley Community College faculty offered courses for honors students at Marquette High School that were guaranteed to transfer to four-year colleges in Illinois. Considers the curriculum, course content, grading, student comments and impressions of the college, program institutionalization, and transfer outcomes. (DMM)
- Published
- 1991
45. Decreased bone formation and increased osteoclastogenesis cause bone loss in mucolipidosis II
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Kollmann, Katrin, Pestka, Jan Malte, Kühn, Sonja Christin, Schöne, Elisabeth, Schweizer, Michaela, Karkmann, Kathrin, Otomo, Takanobu, Catala‐Lehnen, Philip, Failla, Antonio Virgilio, Marshall, Robert Percy, Krause, Matthias, Santer, Rene, Amling, Michael, Braulke, Thomas, and Schinke, Thorsten
- Published
- 2013
- Full Text
- View/download PDF
46. Intramural haematoma of the oesophagus
- Author
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Arhi, Chanpreet, Marshall, Robert, Tang, Cheuk Bong, and Rotundo, Adriana
- Published
- 2013
- Full Text
- View/download PDF
47. The SERM raloxifene improves diaphyseal fracture healing in mice
- Author
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Spiro, Alexander S., Khadem, Shahram, Jeschke, Anke, Marshall, Robert Percy, Pogoda, Pia, Ignatius, Anita, Amling, Michael, and Beil, Frank Timo
- Published
- 2013
- Full Text
- View/download PDF
48. High bone mass in the STR/ort mouse results from increased bone formation and impaired bone resorption and is associated with extramedullary hematopoiesis
- Author
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Pasold, Juliane, Engelmann, Robby, Keller, Johannes, Joost, Sarah, Marshall, Robert P., Frerich, Bernhard, and Müller-Hilke, Brigitte
- Published
- 2013
- Full Text
- View/download PDF
49. Enhanced trabecular micro-architecture of the femoral neck in hip osteoarthritis vs. healthy controls: a micro-computer tomography study in postmenopausal women
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Djuric, Marija, Zagorac, Slavisa, Milovanovic, Petar, Djonic, Danijela, Nikolic, Slobodan, Hahn, Michael, Zivkovic, Vladimir, Bumbasirevic, Marko, Amling, Michael, and Marshall, Robert Percy
- Published
- 2013
- Full Text
- View/download PDF
50. Stress fractures in elderly patients
- Author
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Breer, Stefan, Krause, Matthias, Marshall, Robert P., Oheim, Ralf, Amling, Michael, and Barvencik, Florian
- Published
- 2012
- Full Text
- View/download PDF
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