13,571 results on '"Baker, John A."'
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52. Introduction
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Baker, John R. J., primary
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- 2023
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53. Macroautoradiography
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Baker, John R. J., primary
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- 2023
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54. Electron microscopic autoradiography—preparative methods
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Baker, John R. J., primary
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- 2023
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55. Light microscopic autoradiography—diffusible substances
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Baker, John R. J., primary
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- 2023
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56. Autoradiography in relation to other techniques
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Baker, John R. J., primary
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- 2023
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57. Quantification of EM autoradiographs
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Baker, John R. J., primary
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- 2023
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58. Light microscopic autoradiography—fixable substances
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Baker, John R. J., primary
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- 2023
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59. Resolution
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Baker, John R. J., primary
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- 2023
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60. Autoradiography of receptors
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Baker, John R. J., primary
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- 2023
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61. Components of autoradiographs
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Baker, John R. J., primary
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- 2023
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62. Efficiency
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Baker, John R. J., primary
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- 2023
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63. MarCO: Mars Cube One
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Krajewski, Joel, primary, Klesh, Andrew, primary, and Baker, John J., primary
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- 2023
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64. Building A Field: The Future of Astronomy with Gravitational Waves, A State of The Profession Consideration for Astro2020
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Holley-Bockelmann, Kelly, Key, Joey Shapiro, Kamai, Brittany, Caldwell, Robert, Brown, Warren, Gabella, Bill, Jani, Karan, Baghi, Quentin, Baker, John, Bellovary, Jillian, Bender, Pete, Berti, Emanuele, Brandt, T. J., Cutler, Curt, Conklin, John W., Eracleous, Michael, Ferrara, Elizabeth C., Kelly, Bernard J., Larson, Shane L., Livas, Jeff, McLaughlin, Maura, McWilliams, Sean T., Mueller, Guido, Natarajan, Priyamvada, Rioux, Norman, Schnittman, Jeremy, Shoemaker, David, Shoemaker, Deirdre, Stebbins, Robin, Thorpe, Ira, and Ziemer, John
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
Harnessing the sheer discovery potential of gravitational wave astronomy will require bold, deliberate, and sustained efforts to train and develop the requisite workforce. The next decade requires a strategic plan to build -- from the ground up -- a robust, open, and well-connected gravitational wave astronomy community with deep participation from traditional astronomers, physicists, data scientists, and instrumentalists. This basic infrastructure is sorely needed as an enabling foundation for research. We outline a set of recommendations for funding agencies, universities, and professional societies to help build a thriving, diverse, and inclusive new field.
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- 2019
65. A coupled equilibrium boundary layer model with stable water isotopes and its application to local water recycling
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Xiao, Ke, Griffis, Timothy J., Lee, Xuhui, Xiao, Wei, and Baker, John M.
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- 2023
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66. High angular resolution gravitational wave astronomy
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Baker, John, Baker, Tessa, Carbone, Carmelita, Congedo, Giuseppe, Contaldi, Carlo, Dvorkin, Irina, Gair, Jonathan, Haiman, Zoltan, Mota, David F., Renzini, Arianna, Buis, Ernst-Jan, Cusin, Giulia, Ezquiaga, Jose Maria, Mueller, Guido, Pieroni, Mauro, Quenby, John, Ricciardone, Angelo, Saltas, Ippocratis D., Shao, Lijing, Tamanini, Nicola, Tasinato, Gianmassimo, and Zumalacárregui, Miguel
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics ,General Relativity and Quantum Cosmology - Abstract
Since the very beginning of astronomy the location of objects on the sky has been a fundamental observational quantity that has been taken for granted. While precise two dimensional positional information is easy to obtain for observations in the electromagnetic spectrum, the positional accuracy of current and near future gravitational wave detectors is limited to between tens and hundreds of square degrees, which makes it extremely challenging to identify the host galaxies of gravitational wave events or to confidently detect any electromagnetic counterparts. Gravitational wave observations provide information on source properties and distances that is complementary to the information in any associated electromagnetic emission and that is very hard to obtain in any other way. Observing systems with multiple messengers thus has scientific potential much greater than the sum of its parts. A gravitational wave detector with higher angular resolution would significantly increase the prospects for finding the hosts of gravitational wave sources and triggering a multi-messenger follow-up campaign. An observatory with arcminute precision or better could be realised within the Voyage 2050 programme by creating a large baseline interferometer array in space and would have transformative scientific potential. Precise positional information of standard sirens would enable precision measurements of cosmological parameters and offer new insights on structure formation; a high angular resolution gravitational wave observatory would allow the detection of a stochastic background and resolution of the anisotropies within it; it would also allow the study of accretion processes around black holes; and it would have tremendous potential for tests of modified gravity and the discovery of physics beyond the Standard Model., Comment: 26 pages, 2 figures. White paper submitted to ESA's Voyage 2050 call on behalf of the LISA Consortium 2050 Task Force
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- 2019
67. Space Based Gravitational Wave Astronomy Beyond LISA
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Baker, John, Barke, Simon F., Bender, Peter L., Berti, Emanuele, Caldwell, Robert, Conklin, John W., Cornish, Neil, Ferrara, Elizabeth C., Holley-Bockelmann, Kelly, Kamai, Brittany, Larson, Shane L., Livas, Jeff, McWilliams, Sean T., Mueller, Guido, Natarajan, Priyamvada, Rioux, Norman, Sankar, Shannon R, Schnittman, Jeremy, Shoemaker, Deirdre, Slutsky, Jacob, Stebbins, Robin, Thorpe, Ira, and Ziemer, John
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
The Laser Interferometer Space Antenna (LISA) will open three decades of gravitational wave (GW) spectrum between 0.1 and 100 mHz, the mHz band. This band is expected to be the richest part of the GW spectrum, in types of sources, numbers of sources, signal-to-noise ratios and discovery potential. When LISA opens the low-frequency window of the gravitational wave spectrum, around 2034, the surge of gravitational-wave astronomy will strongly compel a subsequent mission to further explore the frequency bands of the GW spectrum that can only be accessed from space. The 2020s is the time to start developing technology and studying mission concepts for a large-scale mission to be launched in the 2040s. The mission concept would then be proposed to Astro2030. Only space based missions can access the GW spectrum between 10 nHz and 1 Hz because of the Earths seismic noise. This white paper surveys the science in this band and mission concepts that could accomplish that science. The proposed small scale activity is a technology development program that would support a range of concepts and a mission concept study to choose a specific mission concept for Astro2030. In this white paper, we will refer to a generic GW mission beyond LISA as bLISA., Comment: Astro2020 APC White Paper Primary Thematic Science Area: Multi-Messenger Astronomy and Astrophysics Secondary Areas: Cosmology and Fundamental Physics, Galaxy Evolution, Formation and Evolution of Compact Objects
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- 2019
68. Advanced Astrophysics Discovery Technology in the Era of Data Driven Astronomy
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Barry, Richard K., Babu, Jogesh G., Baker, John G., Feigelson, Eric D., Kaur, Amanpreet, Kogut, Alan J., Kraemer, Steven B., Mason, James P., Mehrotra, Piyush, Olmschenk, Gregory, Schnittman, Jeremy D., Stokholm, Amalie, Switzer, Eric R., Thomas, Brian A., and Walker, Raymond J.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Physics - Computational Physics - Abstract
Experience suggests that structural issues in how institutional Astrophysics approaches data-driven science and the development of discovery technology may be hampering the community's ability to respond effectively to a rapidly changing environment in which increasingly complex, heterogeneous datasets are challenging our existing information infrastructure and traditional approaches to analysis. We stand at the confluence of a new epoch of multimessenger science, remote co-location of data and processing power and new observing strategies based on miniaturized spacecraft. Significant effort will be required by the community to adapt to this rapidly evolving range of possible discovery moduses. In the suggested creation of a new Astrophysics element, Advanced Astrophysics Discovery Technology, we offer an affirmative solution that places the visibility of discovery technologies at a level that we suggest is fully commensurate with their importance to the future of the field., Comment: White paper submitted to the ASTRO2020 decadal survey
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- 2019
69. The Laser Interferometer Space Antenna: Unveiling the Millihertz Gravitational Wave Sky
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Baker, John, Bellovary, Jillian, Bender, Peter L., Berti, Emanuele, Caldwell, Robert, Camp, Jordan, Conklin, John W., Cornish, Neil, Cutler, Curt, DeRosa, Ryan, Eracleous, Michael, Ferrara, Elizabeth C., Francis, Samuel, Hewitson, Martin, Holley-Bockelmann, Kelly, Hornschemeier, Ann, Hogan, Craig, Kamai, Brittany, Kelly, Bernard J., Key, Joey Shapiro, Larson, Shane L., Livas, Jeff, Manthripragada, Sridhar, McKenzie, Kirk, McWilliams, Sean T., Mueller, Guido, Natarajan, Priyamvada, Numata, Kenji, Rioux, Norman, Sankar, Shannon R., Schnittman, Jeremy, Shoemaker, David, Shoemaker, Deirdre, Slutsky, Jacob, Spero, Robert, Stebbins, Robin, Thorpe, Ira, Vallisneri, Michele, Ware, Brent, Wass, Peter, Yu, Anthony, and Ziemer, John
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,General Relativity and Quantum Cosmology - Abstract
The first terrestrial gravitational wave interferometers have dramatically underscored the scientific value of observing the Universe through an entirely different window, and of folding this new channel of information with traditional astronomical data for a multimessenger view. The Laser Interferometer Space Antenna (LISA) will broaden the reach of gravitational wave astronomy by conducting the first survey of the millihertz gravitational wave sky, detecting tens of thousands of individual astrophysical sources ranging from white-dwarf binaries in our own galaxy to mergers of massive black holes at redshifts extending beyond the epoch of reionization. These observations will inform - and transform - our understanding of the end state of stellar evolution, massive black hole birth, and the co-evolution of galaxies and black holes through cosmic time. LISA also has the potential to detect gravitational wave emission from elusive astrophysical sources such as intermediate-mass black holes as well as exotic cosmological sources such as inflationary fields and cosmic string cusps., Comment: White Paper submitted to Astro2020 (2020 Decadal Survey on Astronomy and Astrophysics). v2: fixed a reference
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- 2019
70. Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
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Baghi, Quentin, Thorpe, Ira, Slutsky, Jacob, Baker, John, Canton, Tito Dal, Korsakova, Natalia, and Karnesis, Nikos
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General Relativity and Quantum Cosmology ,Astrophysics - Instrumentation and Methods for Astrophysics ,83C35, 62-07 ,I.6 ,G.3 - Abstract
By listening to gravity in the low frequency band, between 0.1 mHz and 1 Hz, the future space-based gravitational-wave observatory LISA will be able to detect tens of thousands of astrophysical sources from cosmic dawn to the present. The detection and characterization of all resolvable sources is a challenge in itself, but LISA data analysis will be further complicated by interruptions occurring in the interferometric measurements. These interruptions will be due to various causes occurring at various rates, such as laser frequency switches, high-gain antenna re-pointing, orbit corrections, or even unplanned random events. Extracting long-lasting gravitational-wave signals from gapped data raises problems such as noise leakage and increased computational complexity. We address these issues by using Bayesian data augmentation, a method that reintroduces the missing data as auxiliary variables in the sampling of the posterior distribution of astrophysical parameters. This provides a statistically consistent way to handle gaps while improving the sampling efficiency and mitigating leakage effects. We apply the method to the estimation of galactic binaries parameters with different gap patterns, and we compare the results to the case of complete data., Comment: 18 pages, 7 figures, accepted for publication in Phys. Rev. D
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- 2019
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71. Kidney and Cardiovascular Effects of Canagliflozin According to Age and Sex: A Post Hoc Analysis of the CREDENCE Randomized Clinical Trial
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Perkovic, Vlado, Mahaffey, Kenneth W., Agarwal, Rajiv, Bakris, George, Brenner, Barry M., Cannon, Christopher P., Charytan, David M., de Zeeuw, Dick, Greene, Tom, Jardine, Meg J., Heerspink, Hiddo J.L., Levin, Adeera, Meininger, Gary, Neal, Bruce, Pollock, Carol, Wheeler, David C., Zhang, Hong, Zinman, Bernard, Jardine, Meg, Li, Nicole, Kolesnyk, Inna, Aizenberg, Diego, Pecoits-Filho, Roberto, Cherney, David, Obrador, Gregorio, Chertow, Glenn, Chang, Tara, Hawley, Carmel, Ji, Linong, Wada, Takashi, Jha, Vivekanand, Lim, Soo Kun, Lim-Abrahan, Mary Anne, Santos, Florence, Chae, Dong-Wan, Hwang, Shang-Jyh, Vazelov, Evgueniy, Rychlík, Ivan, Hadjadj, Samy, Krane, Vera, Rosivall, László, De Nicola, Luca, Dreval, Alexander, Nowicki, Michał, Schiller, Adalbert, Distiller, Larry, Górriz, Jose L., Kolesnyk, Mykola, David, Wheeler, C., Guerrero, Rodolfo Andres Ahuad, Albisu, Juan Pablo, Alvarisqueta, Andres, Bartolacci, Ines, Berli, Mario Alberto, Bordonava, Anselmo, Calella, Pedro, Cantero, Maria Cecilia, Cartasegna, Luis Rodolfo, Cercos, Esteban, Coloma, Gabriela Cecilia, Colombo, Hugo, Commendatore, Victor, Cuadrado, Jesus, Cuneo, Carlos Alberto, Cusumano, Ana Maria, Douthat, Walter Guillermo, Dran, Ricardo Dario, Farias, Eduardo, Fernandez, Maria Florencia, Finkelstein, Hernan, Fragale, Guillermo, Fretes, Jose Osvaldo, Garcia, Nestor Horacio, Gastaldi, Anibal, Gelersztein, Elizabeth, Glenny, Jorge Archibaldo, Gonzalez, Joaquin Pablo, Colaso, Patricia del Carmen Gonzalez, Goycoa, Claudia, Greloni, Gustavo Cristian, Guinsburg, Adrian, Hermida, Sonia, Juncos, Luis Isaias, Klyver, Maria Isabel, Kraft, Florencia, Krynski, Fernando, Lanchiotti, Paulina Virginia, Leon de la Fuente, Ricardo Alfonso, Marchetta, Nora, Mele, Pablo, Nicolai, Silvia, Novoa, Pablo Antonio, Orio, Silvia Ines, Otreras, Fabian, Oviedo, Alejandra, Raffaele, Pablo, Resk, Jorge Hector, Rista, Lucas, Papini, Nelson Rodriguez, Sala, Jorgelina, Santos, Juan Carlos, Schiavi, Lilia Beatriz, Sessa, Horacio, Casabella, Tomas Smith, Ulla, Maria Rosa, Valdez, Maria, Vallejos, Augusto, Villarino, Adriana, Visco, Virginia Esther, Wassermann, Alfredo, Zaidman, Cesar Javier, Cheung, Ngai Wah, Droste, Carolyn, Fraser, Ian, Johnson, David, Mah, Peak Mann, Nicholls, Kathy, Packham, David, Proietto, Joseph, Roberts, Anthony, Roger, Simon, Tsang, Venessa, Raduan, Roberto Abrão, Costa, Fernando Augusto Alves da, Amodeo, Celso, Turatti, Luiz Alberto Andreotti, Bregman, Rachel, Sanches, Fernanda Cristina Camelo, Canani, Luis Henrique, Chacra, Antônio Roberto, Borges, João Lindolfo Cunha, Vêncio, Sérgio Alberto Cunha, Franco, Roberto Jorge da Silva, d’Avila, Domingos, Portes, Evandro de Souza, de Souza, Pedro, Deboni, Luciane Mônica, Fraige Filho, Fadlo, Neto, Bruno Geloneze, Gomes, Marcus, Kohara, Suely Keiko, Keitel, Elizete, Saraiva, Jose Francisco Kerr, Lisboa, Hugo Roberto Kurtz, Contieri, Fabiana Loss de Carvalho, Milagres, Rosângela, Junior, Renan Montenegro, de Brito, Claudia Moreira, Hissa, Miguel Nasser, Sabbag, Ângela Regina Nazario, Noronha, Irene, Panarotto, Daniel, Filho, Roberto Pecoits, Pereira, Márcio Antônio, Saporito, Wladmir, Scotton, Antonio Scafuto, Schuch, Tiago, de Almeida, Roberto Simões, Ramos, Cássio Slompo, Felício, João Soares, Thomé, Fernando, Hachmann, Jean Carlo Tibes, Yamada, Sérgio, Hayashida, Cesar Yoiti, Petry, Tarissa Beatrice Zanata, Zanella, Maria Teresa, Andreeva, Viktoria, Angelova, Angelina, Dimitrov, Stefan, Genadieva, Veselka, Genova-Hristova, Gabriela, Hristozov, Kiril, Kamenov, Zdravko, Koundurdjiev, Atanas, Lozanov, Lachezar, Margaritov, Viktor, Nonchev, Boyan, Rangelov, Rangel, Shinkov, Alexander, Temelkova, Margarita, Velichkova, Ekaterina, Yakov, Andrian, Aggarwal, Naresh, Aronson, Ronnie, Bajaj, Harpreet, Chouinard, Guy, Conway, James, Cournoyer, Serge, DaRoza, Gerald, De Serres, Sacha, Dubé, François, Goldenberg, Ronald, Gupta, Anil, Gupta, Milan, Henein, Sam, Khandwala, Hasnain, Leiter, Lawrence, Madore, François, McMahon, Alan, Muirhead, Norman, Pichette, Vincent, Rabasa-Lhoret, Remi, Steele, Andrew, Tangri, Navdeep, Torshizi, Ali, Woo, Vincent, Zalunardo, Nadia, Montenegro, María Alicia Fernández, Gonzalo Godoy Jorquera, Juan, Fariña, Marcelo Medina, Gajardo, Victor Saavedra, Vejar, Margarita, Chen, Nan, Chen, Qinkai, Gan, Shenglian, Kong, Yaozhong, Li, Detian, Li, Wenge, Li, Xuemei, Lin, Hongli, Liu, Jian, Lu, Weiping, Mao, Hong, Ren, Yan, Song, Weihong, Sun, Jiao, Sun, Lin, Tu, Ping, Wang, Guixia, Yang, Jinkui, Yin, Aiping, Yu, Xueqing, Zhao, Minghui, Zheng, Hongguang, Mendoza, Jose Luis Accini, Arcos, Edgar, Avendano, Jorge, Diaz Ruiz, Jorge Ernesto Andres, Ortiz, Luis Hernando Garcia, Gonzalez, Alexander, Triana, Eric Hernandez, Higuera, Juan Diego, Malaver, Natalia, de Salazar, Dora Inés Molina, Rosero, Ricardo, Alexandra Terront Lozano, Monica, Cometa, Luis Valderrama, Valenzuela, Alex, Vargas Alonso, Ruben Dario, Villegas, Ivan, Yupanqui, Hernan, Bartaskova, Dagmar, Barton, Petr, Belobradkova, Jana, Dohnalova, Lenka, Drasnar, Tomas, Ferkl, Richard, Halciakova, Katarina, Klokocnikova, Vera, Kovar, Richard, Lastuvka, Jiri, Lukac, Martin, Pesickova, Satu, Peterka, Karel, Pumprla, Jiri, Rychlik, Ivan, Saudek, Frantisek, Tesar, Vladimir, Valis, Martin, Weiner, Pavel, Zemek, Stanislav, Alamartine, Eric, Borot, Sophie, Cariou, Bertrand, Dussol, Bertrand, Fauvel, Jean-Pierre, Gourdy, Pierre, Klein, Alexandre, Le Meur, Yannick, Penfornis, Alfred, Roussel, Ronan, Saulnier, Pierre-Jean, Thervet, Eric, Zaoui, Philippe, Burst, Volker, Faghih, Markus, Faulmann, Grit, Haller, Hermann, Jerwan-Keim, Reinhold, Maxeiner, Stephan, Paschen, Björn, Plassmann, Georg, Rose, Ludger, Gonzalez Orellana, Ronaldo Arturo, Haase, Franklin Paul, Moreira Diaz, Juan Pablo, Ramirez Roca, Luis Alberto, Sánchez Arenales, Jose Antonio, Sanchez Polo, José Vicente, Juarez, Erick Turcios, Csecsei, Gyongyi, Csiky, Botond, Danos, Peter, Deak, Laszlo, Dudas, Mihaly, Harcsa, Eleonora, Keltai, Katalin, Keresztesi, Sandor, Kiss, Krisztian, Konyves, Laszlo, Major, Lajos, Mileder, Margit, Molnar, Marta, Mucsi, Janos, Oroszlan, Tamas, Ory, Ivan, Paragh, Gyorgy, Peterfai, Eva, Petro, Gizella, Revesz, Katalin, Takacs, Robert, Vangel, Sandor, Vasas, Szilard, Zsom, Marianna, Abraham, Oomman, Bhushan, Raju Sree, Deepak, Dewan, Edwin, Fernando M., Gopalakrishnan, Natarajan, Gracious, Noble, Hansraj, Alva, Jain, Dinesh, Keshavamurthy, C.B., Khullar, Dinesh, Manisha, Sahay, Peringat, Jayameena, Prasad, Narayan, Satyanarayana, Rao K., Sreedhar, Reddy, Sreelatha, Melemadathil, Sudhakar, Bhimavarapu, Chandra Vyasam, Ramesh, Bonadonna, Riccardo, Castellino, Pietro, Ceriello, Antonio, Chiovato, Luca, De Cosmo, Salvatore, Derosa, Giuseppe, Di Carlo, Alberto, Di Cianni, Graziano, Frascà, Giovanni, Fuiano, Giorgio, Gambaro, Giovanni, Garibotto, Giacomo, Giorda, Carlo, Malberti, Fabio, Mandreoli, Marcora, Mannucci, Edoardo, Orsi, Emanuela, Piatti, Piermarco, Santoro, Domenico, Sasso, Ferdinando Carlo, Serviddio, Gaetano, Stella, Andrea, Trevisan, Roberto, Veronelli, Anna Maria, Zanoli, Luca, Akiyama, Hitoshi, Aoki, Hiromi, Asano, Akimichi, Iitsuka, Tadashi, Kajiyama, Shizuo, Kashine, Susumu, Kawada, Toshio, Kodera, Takamoto, Kono, Hiroshi, Koyama, Kazunori, Kumeda, Yasuro, Miyauchi, Shozo, Mizuyama, Kazuyuki, Niiya, Tetsuji, Oishi, Hiroko, Ota, Satoshi, Sakakibara, Terue, Takai, Masahiko, Tomonaga, Osamu, Tsujimoto, Mitsuru, Wakasugi, Masakiyo, Wakida, Yasushi, Watanabe, Takayuki, Yamada, Masayo, Yanagida, Kazuhiro, Yanase, Toshihiko, Yumita, Wataru, Gaupsiene, Egle, Kozloviene, Dalia, Navickas, Antanas, Urbanaviciene, Egle, Abdul Ghani, Rohana, Kadir, Khalid Abdul, Ali, Norsiah, Che Yusof, Mohd Daud, Gan, Chye Lee, Ismail, Mastura, Kong, Wei Yen, Lam, Swee Win, Lee, Li Yuan, Loh, Chek Loong, Manocha, Anita Bhajan, Ng, Kee Sing, Ahmad, Nik Nur Fatnoon Nik, Ratnasingam, Vanassa, Shudim, Saiful Shahrizal Bin, Vengadasalam, Paranthaman, Abraira Munoz, Luis David, Salazar, Melchor Alpizar, Cruz, Juan Baas, Soto, Mario Burgos, Ramos, Jose Chevaile, Wong, Alfredo Chew, Correa Rotter, Jose Ricardo, Escalante, Tonatiu Diaz, Enriquez Sosa, Favio Edmundo, Lozano, Fernando Flores, Flota Cervera, Luis Fernando, Baron, Paul Frenk, Ballesteros, Cecilia Garcia, Gomez Rangel, Jose David, Herrera Jimenez, Luis Enrique, Irizar Santana, Sergio Saul, Flores, Fernando Jimenez, Molina, Hugo Laviada, Luna Ceballos, Rosa Isela, del Campo Blanco, Belia Martin, Franco, Guadalupe Morales, Moreno Loza, Oscar Tarsicio, Rocha, Cynthia Mustieles, Vera, Gregorio Obrador, Castellanos, Ricardo Orozco, Calcaneo, Juan Peralta, Reyes Rosano, Miguel Angel, Pattzi, Hiromi Rodriguez, Guzman, Juan Rosas, Rucker Joerg, Isabel Erika, Saavedra Sanchez, Sandra Berenice, Sanchez Mijangos, Jose Hector, Sanson, Pablo Serrano, Tamayo y Orozco, Juan Alfredo, Chavez, Eloisa Tellez, Cepeda, Alejandro Valdes, Carrillo, Luis Venegas, Mesa, Juan Villagordoa, Escobedo, Rolando Zamarripa, Baker, John, Noonan, Paul, Scott, Russell, Walker, Robert, Watson, Edward, Williams, Michael, Young, Simon, Abejuela, Zaynab, Agra, Jeimeen, Aquitania, Grace, Caringal, Clodoaido, Comia, Rhea Severina, Santos, Lalaine Delos, Gomez, Olivert, Jimeno, Cecilia, Tan, Gerry, Tolentino, Marsha, Yao, Christy, Yap, Yvette Ethel, Lallaine Ygpuara, Ma. Dovie, Bijata-Bronisz, Renata, Hotlos, Lucyna, Januszewicz, Andrzej, Kaczmarek, Barbara, Kaminska, Anna, Lazuka, Lech, Madej, Andrzej, Mazur, Stanislaw, Mlodawska-Choluj, Dorota, Nowicki, Michal, Orlowska-Kowalik, Grazyna, Popenda, Grazyna, Rewerska, Barbara, Sowinski, Dariusz, Angelescu, Liliana Monica, Anghel, Veronica, Avram, Rodica-Ioana, Busegeanu, Mihaela-Magdalena, Cif, Adriana, Cosma, Dana, Crisan, Carmen, Demian, Luiza Despina, Ferariu, Ioana Emilia, Halmagyi, Ildiko, Hancu, Nicolae, Munteanu, Mircea, Negru, Doru, Onaca, Adriana Gabriela, Petrica, Ligia, Popa, Amorin Remus, Ranetti, Aurelian-Emil, Serafinceanu, Cristian, Toarba, Cristina, Agafyina, Alina, Barbarash, Olga, Barysheva, Olga, Chizhov, Daniil, Dobronravov, Vladimir, Glinkina, Irina, Grineva, Elena, Khirmanov, Vladimir, Kolmakova, Elena, Koroleva, Tatiana, Kvitkova, Liudmila, Marasaev, Viacheslav, Mkrtumyan, Ashot, Morugova, Tatiana, Nagibovich, Galina, Nagibovich, Oleg, Nedogoda, Sergei, Osipova, Irina, Raskina, Tatiana, Samoylova, Yulia, Sazonova, Olga, Shamkhalova, Minara, Shutemova, Elena, Shwartz, Yuriy, Uriasyev, Oleg, Vorobyev, Sergey, Zateyshchikova, Anna, Zateyshshikov, Dmitry, Zykova, Tatyana, Antic, Slobodan, Djordjevic, Miodrag, Kendereski, Aleksandra, Lalic, Katarina, Lalic, Nebojsa, Popovic-Radinovic, Vesna, Babikova, Jana, Benusova, Olga, Buganova, Ingrid, Culak, Jan, Dzupina, Andrej, Dzuponova, Jana, Fulop, Peter, Ilavska, Adriana, Martinka, Emil, Ochodnicka, Zuzana, Pella, Daniel, Smatanova, Iveta, Ahmed, Fayzal, Badat, Aysha, Breedt, Johannes, Distiller, Lawrence, Govender, Vimladhevi, Govender, Ravendran, Joshi, Mukesh, Jurgens, Jaco, Latiff, Gulam, Lombard, Landman, Mookadam, Mohamed, Ngcakani, Nomangesi, Nortje, Hendrik, Oosthuizen, Helena, Pillay-Ramaya, Larisha, Prozesky, Hans, Reddy, Jeevren, Rheeder, Paul, Seeber, Mary, Cho, Young Min, Jeong, In-Kyung, Kim, Sin Gon, Kim, Yeong Hoon, Kwon, Hyuk-Sang, Kwon, Min Jeong, Lee, Byung-Wan, Lee, JungEun, Lee, Moon-Kyu, Nam, Moon-Suk, Oh, Kook-Hwan, Park, Cheol- Young, Park, Sun-Hee, Yoon, Kun Ho, Garcia, Pere Alvarez, Mercadal, Luis Asmarats, Barrios, Clara, Castro, Fernando Cereto, Guldris, Secundino Cigarran, Lopez, Marta Dominguez, Egido de los Rios, Jesus, Fresnedo, Gema Fernandez, Serrano, Antonio Galan, Garcia, Isabel, Gonzalez Martinez, Francisco Javier, Jodar Gimeno, Jose Esteban, Mendoza, Manuel Lopez, Marin, Tamara Malek, Portillo, Cristobal Morales, Munar Vila, Maria Antonia, Torres, Manuel Muñoz, Iglesias, Javier Nieto, Perez, Jonay Pantoja, Vera, Merce Perez, Portoles Perez, Jose M., Quesada Simón, María Angustias, Canonge, Rafael Simo, Gonzalez, Alfonso Soto, Riera, Manel Terns, Tinahones Madueno, Francisco Jose, Plaza, Mercedes Velo, Chang, Chwen-Tzuei, Chuang, Lee-Ming, Hsia, Te-Lin, Hsieh, Chang-Hsun, Lin, Chih-Ching, Lu, Yung- Chuan, Sheu, Wayne H-H, Barna, Olga, Bilyk, Svitlana D., Botsyurko, Volodymyr, Dudar, Iryna, Fushtey, Ivan, Godlevska, Olga, Golovchenko, Oleksandr, Gyrina, Olga, Kazmirchuk, Anatoliy, Komisarenko, Iuliia, Korzh, Oleksii, Kravchun, Nonna, Legun, Oleg, Mankovskyy, Borys, Martynyuk, Liliya, Mostovoy, Yuriy, Pashkovska, Nataliia, Pererva, Larysa, Pertseva, Tetyana, Samoylov, Oleksandr, Smirnov, Ivan, Svyshchenko, Yevgeniya, Tomashkevych, Halyna, Topchii, Ivan, Tryshchuk, Nadiya, Tseluyko, Vira, Vizir, Vadym, Vlasenko, Maryna, Zlova, Tetiana, Zub, Liliia, Abusnana, Salah, Railey, Mohamed, Abouglila, Kamal, Ainsworth, Paul, Ali, Zishan, Arutchelvam, Vijayaraman, Barnard, Maria, Bellary, Srikanth, Davies, Emyr, Davies, Mark, Davies, Simon, Dawson, Alison, El Kossi, Mohsen, English, Patrick, Fraser, Donald, Gnudi, Luigi, Gunstone, Anthony, Hall, Timothy, Hanif, Wasim, Jackson, Alan, Johnson, Andrew, Joseph, Franklin, Krishnan, Singhan, Kumwenda, Mick, MacDougall, Iain, Nixon, Paul, O'Hare, Joseph, Philip, Sam, Ramtoola, Shenaz, Saxena, Manish, Sennik, Davesh, Simon, Godwin, Singh, Baldev, Stephens, Jeffrey, Strzelecka, Anna, Symonds, Rehan, Turner, Wayne, Wahba, Mona, Wakeling, John, Wheeler, David, Winocour, Peter, Abdallah, Joseph, Abdullah, Raied, Abramowitz, Matthew, Acosta, Idalia, Aiello, Joseph, Akright, Laura, Akyea-Djamson, Ayim, Alappan, Rajendran, Alicic, Radica, Al-Karadsheh, Amer, Allison, Dale Crawford, Arauz-Pacheco, Carlos, Arfeen, Shahabul, Arif, Ahmed, Arvind, Moogali, Atray, Naveen, Awad, Ahmed, Barnhill, Peggy, Barranco, Elizabeth, Barrera, Carlos, Beacom, Matthew, Behara, Venkata, Belo, Diogo, Bentley-Lewis, Rhonda, Berenguer, Ramon, Bermudez, Lidia, Bernardo, Marializa, Biscoveanu, Mihaela, Bowman-Stroud, Cynthia, Brandon, Donald, Brusco, Osvaldo, Busch, Robert, Canaan, Yamil, Chilito, Alicia, Christensen, Tom, Christiano, Cynthia, Christofides, Elena, Chuateco, Caroucel, Cohen, Kenneth, Cohen, Robert, Cohen-Stein, Debbie, Cook, Charles, Coyne, Daniel, Daboul, Nizar, Darwish, Riad, Daswani, Adarsh, Deck, Kenneth, Desouza, Cyrus, Dev, Devasmita, Dhillon, Monika, Dua, Sohan, Eder, Frank, Elosegui, Ana Maria, El-Shahawy, Mohamed, Ervin, John, Esquenazi, Alberto, Evans, John, Fishbane, Steven, Frias, Juan, Galindo-Ramos, Eugenia, Galphin, Claude, Ghazi, Adline, Gonzalez, Enrique, Gorson, David, Gowda, Anupama, Greco, Barbara, Grubb, Stephen, Gulati, Rakesh, Hammoud, Jamal, Handelsman, Stuart, Hartman, Israel, Hershon, Kenneth, Hiser, Daniel, Hon, George, Jacob, Radu, Jaime, Maria, Jamal, Aamir, Kaupke, Charles, Keightley, Gerald, Kern, Elizabeth, Khanna, Rakhi, Khitan, Zeid, Kim, Sun, Kopyt, Nelson, Kovesdy, Csaba, Krishna, Gopal, Kropp, Jeffrey (Jay), Kumar, Amrendra, Kumar, Jayant, Kumar, Neil, Kusnir, Jorge, Lane, Wendy, Lawrence, Mary, Lehrner, Lawrence, Lentz, John, Levinson, Dennis, Lewis, Derek, Liss, Kenneth, Maddux, Andreas, Maheshwari, Hiralal, Mandayam, Sreedhar, Marar, Isam, Mehta, Bhasker, Middleton, John, Mordujovich, Jorge, Moreda, Ramon, Moustafa, Moustafa, Trenche, Samuel Mujica, Narayanan, Mohanram, Narvarte, Javier, Nassar, Tareq, Newman, George, Nichol, Brian, Nicol, Philip, Nisnisan, Josier, Nossuli, A. Kaldun, Obialo, Chamberlain, Olelewe, Sarah, Oliver, Michael, O'Shaughnessy, Andrew, Padron, John, Pankhaniya, Rohit, Parker, Reginald, Patel, Devesh, Patel, Gnyandev, Patel, Nina, Pavon, Humberto, Perez, Armando, Perez, Carlos, Perlman, Alan, Pettis, Karlton, Pharr, Walter, Phillips, Andrea, Purighalla, Raman, Quesada-Suarez, Luis, Ranjan, Rajiv, Rastogi, Sanjeev, Reddy, Jakkidi, Rendell, Marc, Rich, Lisa, Robinson, Michael, Rodriguez, Hector, Rosas, Sylvia, Saba, Fadi, Sankaram, Rallabhandi, Sarin, Ravi, Schreiman, Robert, Scott, David, Sekkarie, Mohamed, Sensenbrenner, John, Shakeel, Muhammad, Shanik, Michael, Shaw, Sylvia, Smith, Stephen, Solomon, Richard, Sprague, Amy, Spry, Leslie, Suchinda, Pusadee, Sultan, Senan, Surampudi, Prasanth, Sussman, Sherry, Tan, Anjanette, Terrelonge, Antonio, Thompson, Michael, Trespalacios, Fernando, Trippe, Bruce, Trueba, Pilar, Twahirwa, Marcel, Updegrove, John, Van Buren, Peter, Vannorsdall, Mark, Varghese, Freemu, Velasquez-Mieyer, Pedro, Ventrapragada, Sailaja, Vukotic, Goga, Wadud, Khurram, Warren, Mark, Watson, Henry, Watts, Ronald, Weiner, Daniel, Welker, James, Welsh, Jean, Williams, Shelley, Zaniewski-Singh, Michelle, Yi, Tae Won, Smyth, Brendan, Di Tanna, Gian Luca, Arnott, Clare, Cardoza, Kathryn, and Kang, Amy
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- 2023
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72. Micrometeoroid Events in LISA Pathfinder
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Thorpe, James Ira, Slutsky, Jacob, Baker, John, Littenberg, Tyson, Hourihane, Sophie, Pagane, Nicole, Pokorny, Petr, Janches, Diego, Armano, Michele, Audley, Heather, Auger, G., Baird, Jonathan, Bassan, Massimo, Binetruy, Pierre, Born, Michael, Bortoluzzi, D., Brandt, N., Caleno, M., Cavalleri, A, Cesarini, A, Cruise, A. M., Danzmann, K., Silva, M. de Deus, De Rosa, R., Di Fiore, L., Diepholz, I., Dixon, G., Dolesi, R., Dunbar, N., Ferraioli, L., Ferroni, V., Fitzsimons, E., Flatscher, R., Freschi, M., Marirrodriga, C. Garcia, Gerndt, R., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grado, A., Grimani, C., Gryzmisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspe, H., Jennrich, O., Jetzer, P., Johlander, B., Karnesis, N., Kaune, B., Korsakova, N., Killow, C., Lobo, J. A., Lloro, I., Liu, L., Lopez-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martin, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Madden, S., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Nofarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Prat, P., Ragnit, U., Ramos-Castro, J., Reiche, J., Robertson, D., Rozemeijer, H., Rivas, F., Russano, G., Sarra, P., Schleicher, A., Shaul, D., Soperta, C., Stanga, R., Sumner, T., Texier, D., Trobs, M., Vetrungno, D., Vitale, S., Wanner, G., Ward, H., Wass, P., Wealthy, D., Weber, W. J., Wissel, L., Wittchen, A., Zambotti, A., Zanoni, C., Ziegler, T., and Zweifel, P.
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Astrophysics - Earth and Planetary Astrophysics - Abstract
The zodiacal dust complex, a population of dust and small particles that pervades the Solar System, provides important insight into the formation and dynamics of planets, comets, asteroids, and other bodies. Here we present a new set of data obtained using a novel technique: direct measurements of momentum transfer to a spacecraft from individual particle impacts. This technique is made possible by the extreme precision of the instruments flown on the LISA Pathfinder spacecraft, a technology demonstrator for a future space-based gravitational wave observatory that operated near the first Sun-Earth Lagrange point from early 2016 through Summer of 2017. Using a simple model of the impacts and knowledge of the control system, we show that it is possible to detect impacts and measure properties such as the transferred momentum (related to the particle's mass and velocity), direction of travel, and location of impact on the spacecraft. In this paper, we present the results of a systematic search for impacts during 4348 hours of Pathfinder data. We report a total of 54 candidates with momenta ranging from 0.2$\,\mu\textrm{Ns}$ to 230$\,\mu\textrm{Ns}$. We furthermore make a comparison of these candidates with models of micrometeoroid populations in the inner solar system including those resulting from Jupiter-family comets, Oort-cloud comets, Hailey-type comets, and Asteroids. We find that our measured population is consistent with a population dominated by Jupiter-family comets with some evidence for a smaller contribution from Hailey-type comets. This is in agreement with consensus models of the zodiacal dust complex in the momentum range sampled by LISA Pathfinder., Comment: 22 pages, 14 figures, accepted in ApJ
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- 2019
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73. The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project
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Porth, Oliver, Chatterjee, Koushik, Narayan, Ramesh, Gammie, Charles F., Mizuno, Yosuke, Anninos, Peter, Baker, John G., Bugli, Matteo, Chan, Chi-kwan, Davelaar, Jordy, Del Zanna, Luca, Etienne, Zachariah B., Fragile, P. Chris, Kelly, Bernard J., Liska, Matthew, Markoff, Sera, McKinney, Jonathan C., Mishra, Bhupendra, Noble, Scott C., Olivares, Héctor, Prather, Ben, Rezzolla, Luciano, Ryan, Benjamin R., Stone, James M., Tomei, Niccolò, White, Christopher J., Younsi, Ziri, and Collaboration, The Event Horizon Telescope
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Astrophysics - High Energy Astrophysical Phenomena ,General Relativity and Quantum Cosmology - Abstract
Recent developments in compact object astrophysics, especially the discovery of merging neutron stars by LIGO, the imaging of the black hole in M87 by the Event Horizon Telescope (EHT) and high precision astrometry of the Galactic Center at close to the event horizon scale by the GRAVITY experiment motivate the development of numerical source models that solve the equations of general relativistic magnetohydrodynamics (GRMHD). Here we compare GRMHD solutions for the evolution of a magnetized accretion flow where turbulence is promoted by the magnetorotational instability from a set of nine GRMHD codes: Athena++, BHAC, Cosmos++, ECHO, H-AMR, iharm3D, HARM-Noble, IllinoisGRMHD and KORAL. Agreement between the codes improves as resolution increases, as measured by a consistently applied, specially developed set of code performance metrics. We conclude that the community of GRMHD codes is mature, capable, and consistent on these test problems., Comment: Accepted version for publication in ApJS (May 28th, 2019)
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- 2019
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74. Multimessenger science opportunities with mHz gravitational waves
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Baker, John, Haiman, Zoltán, Rossi, Elena Maria, Berger, Edo, Brandt, Niel, Breedt, Elmé, Breivik, Katelyn, Charisi, Maria, Derdzinski, Andrea, D'Orazio, Daniel J., Ford, Saavik, Greene, Jenny E., Hill, J. Colin, Holley-Bockelmann, Kelly, Key, Joey Shapiro, Kocsis, Bence, Kupfer, Thomas, Larson, Shane, Madau, Piero, Marsh, Thomas, McKernan, Barry, McWilliams, Sean T., Natarajan, Priyamvada, Nissanke, Samaya, Noble, Scott, Phinney, E. Sterl, Ramsay, Gavin, Schnittman, Jeremy, Sesana, Alberto, Shoemaker, David, Stone, Nicholas, Toonen, Silvia, Trakhtenbrot, Benny, Vikhlinin, Alexey, and Volonteri, Marta
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
LISA will open the mHz band of gravitational waves (GWs) to the astronomy community. The strong gravity which powers the variety of GW sources in this band is also crucial in a number of important astrophysical processes at the current frontiers of astronomy. These range from the beginning of structure formation in the early universe, through the origin and cosmic evolution of massive black holes in concert with their galactic environments, to the evolution of stellar remnant binaries in the Milky Way and in nearby galaxies. These processes and their associated populations also drive current and future observations across the electromagnetic (EM) spectrum. We review opportunities for science breakthroughs, involving either direct coincident EM+GW observations, or indirect multimessenger studies. We argue that for the US community to fully capitalize on the opportunities from the LISA mission, the US efforts should be accompanied by a coordinated and sustained program of multi-disciplinary science investment, following the GW data through to its impact on broad areas of astrophysics. Support for LISA-related multimessenger observers and theorists should be sized appropriately for a flagship observatory and may be coordinated through a dedicated mHz GW research center., Comment: Submitted to the Astro2020 Decadal Survey call for science white papers
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- 2019
75. Irradiation of the kidneys causes pathologic remodeling in the nontargeted heart: A role for the immune system
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Lenarczyk, Marek, Laiakis, Evagelia C, Mattson, David L, Johnson, Bryon D, Kronenberg, Amy, North, Paula E, Komorowski, Richard, Mäder, Marylou, and Baker, John E
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Biological Sciences ,Cardiovascular ,Heart Disease ,Kidney Disease ,Cancer ,2.1 Biological and endogenous factors ,Aetiology ,Renal and urogenital ,Fibrosis ,T lymphocytes ,X‐rays ,cytokines ,heart diseases ,hypertension ,rats ,Biological sciences - Abstract
Cardiac disease is a frequent and significant adverse event associated with radiotherapy for cancer. Identifying the underlying mechanism responsible for radiation injury to the heart will allow interventions to be developed. In the present study, we tested if local kidney irradiation results in remodeling of the shielded, nontargeted heart. One kidney, two kidneys, or the total body of male WAG and Dahl SS rats were irradiated with 10 Gy of X-rays. Local kidney irradiation resulted in systemic hypertension, increased BUN, infiltration of T lymphocytes, natural killer cells, and macrophages into the renal cortex and medulla, and renal fibrosis. Local irradiation of kidneys in WAG rats resulted in remodeling in the nontargeted heart after 120 days, manifested by perivascular fibrosis and increased interventricular septal thickness, but was not seen in Dahl SS rats due to a high baseline level of fibrosis in the sham-irradiated animals. Genetic depletion of T cells mitigated the nephropathy after local kidney irradiation, indicating a role for the immune system in mediating this outcome. Local kidney irradiation resulted in a cascade of pro-inflammatory cytokines and low-molecular weight metabolites into the circulation associated with transmission of signals resulting in pathologic remodeling in the nontargeted heart. A new model is proposed whereby radiation-induced cardiac remodeling in susceptible animals is indirect, with lower hemi body organs such as the kidney exporting factors into the circulation that cause remodeling outside of the irradiated field in the shielded, nontargeted heart. This nontargeted effect appears to be mediated, in part, by the immune system.
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- 2020
76. Symmetrical Designs No. 2
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Baker, John L
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This music score was submitted for the Kaleidoscope 2020 Call for Scores, an open access collaboration with the UCLA Music Library.
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- 2020
77. Fantasy No. 4 on Mondrian’s “Composition in Red, Yellow, and Blue” (1939-42)
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Baker, John L
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This music score was submitted for the Kaleidoscope 2020 Call for Scores, an open access collaboration with the UCLA Music Library.
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- 2020
78. From a Sparrow Song
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Baker, John L
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This music score was submitted for the Kaleidoscope 2020 Call for Scores, an open access collaboration with the UCLA Music Library.
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- 2020
79. The mountaineer's farewell, or, My own native state.
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Baker, John C. and Baker, John C.
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- Broadsides 19th century. United States, Songs Texts. 19th century United States, Popular music Texts. 19th century United States, Nostalgia Songs and music Texts., Mountains Songs and music Texts., Musique populaire Textes. 19e siècle États-Unis, Broadsides., Mountains., Nostalgia., Popular music., Songs., New Hampshire Songs and music Texts., New Hampshire., United States.
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- 2024
80. Mountaineer's farewell, or, My own native state.
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Baker, John C. and Baker, John C.
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- Broadsides 19th century. United States, Songs Texts. 19th century United States, Popular music Texts. 19th century United States, Nostalgia Songs and music Texts., Mountains Songs and music Texts., Musique populaire Textes. 19e siècle États-Unis, Broadsides., Mountains., Nostalgia., Popular music., Songs., New Hampshire Songs and music Texts., New Hampshire., United States.
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- 2024
81. Adaptive Leadership
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Baker, John, primary and Seemiller, Corey, additional
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- 2023
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82. Spatiotemporal distribution of roots in a Maize-Kura clover living mulch system: Impact of tillage and fertilizer N source
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Alexander, Jonathan R., Baker, John M., Gamble, Joshua D., Venterea, Rodney T., and Spokas, Kurt A.
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- 2023
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83. Explanation of context, mechanisms and outcomes in adult community mental health crisis care: the MH-CREST realist evidence synthesis
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Clibbens Nicola, Baker John, Booth Andrew, Berzins Kathryn, Ashman Michael C, Sharda Leila, Thompson Jill, Kendal Sarah, and Weich Scott
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realist evidence synthesis ,mental health ,crisis care ,crisis services ,community ,patient participation ,stakeholders ,interagency ,compassionate leadership ,therapeutic crisis care ,Medicine (General) ,R5-920 ,Public aspects of medicine ,RA1-1270 - Abstract
Background Mental health crises cause significant disruption to individuals and families and can be life-threatening. The large number of community crisis services operating in an inter-agency landscape complicates access to help. It is unclear which underpinning mechanisms of crisis care work, for whom and in which circumstances. Aim The aim was to identify mechanisms to explain how, for whom and in what circumstances adult community crisis services work. Objectives The objectives were to develop, test and synthesise programme theories via (1) stakeholder expertise and current evidence; (2) a context, intervention, mechanism and outcome framework; (3) consultation with experts; (4) development of pen portraits; (5) synthesis and refinement of programme theories, including mid-range theory; and (6) identification and dissemination of mechanisms needed to trigger desired context-specific crisis outcomes. Design This study is a realist evidence synthesis, comprising (1) identification of initial programme theories; (2) prioritisation, testing and refinement of programme theories; (3) focused realist reviews of prioritised initial programme theories; and (4) synthesis to mid-range theory. Main outcome The main outcome was to explain context, mechanisms and outcomes in adult community mental health crisis care. Data sources Data were sourced via academic and grey literature searches, expert stakeholder group consultations and 20 individual realist interviews with experts. Review methods A realist evidence synthesis with primary data was conducted to test and refine three initial programme theories: (1) urgent and accessible crisis care, (2) compassionate and therapeutic crisis care and (3) inter-agency working. Results Community crisis services operate best within an inter-agency system. This requires compassionate leadership and shared values that enable staff to be supported; retain their compassion; and, in turn, facilitate compassionate interventions for people in crisis. The complex interface between agencies is best managed through greater clarity at the boundaries of services, making referral and transition seamless and timely. This would facilitate ease of access and guaranteed responses that are trusted by the communities they serve. Strengths and limitations Strengths include the identification of mechanisms for effective inter-agency community crisis care and meaningful stakeholder consultation that grounded the theories in real-life experience. Limitations include the evidence being heavily weighted towards England and the review scope excluding full analysis of ethnic and cultural diversity. Conclusions Multiple interpretations of crises and diverse population needs present challenges for improving the complex pathways to help in a crisis. Inter-agency working requires clear policy guidance with local commissioning. Seamless transitions between services generate trust through guaranteed responses and ease of navigation. This is best achieved where there is inter-agency affiliation that supports co-production. Compassionate leaders engender staff trust, and outcomes for people in crisis improve when staff are supported to retain their compassion. Future work Further work might explore inter-agency models of crisis delivery, particularly in rural communities. Future work could focus on evaluating outcomes across crisis care provider agencies and include evaluation of individual, as well as service-level, outcomes. The implementation and effect of mental health triage could be explored further, including via telehealth. Barriers to access for marginalised populations warrant a specific focus in future research. Study registration The study is registered as PROSPERO CRD42019141680. Funding This project was funded by the National Institute for Health and Care Research (NIHR) Health and Social Care Delivery Research programme and will be published in full in Health and Social Care Delivery Research; Vol. 11, No. 15. See the NIHR Journals Library website for further project information. Plain language summary The issue A mental health crisis can be traumatic for individuals and families. There are a lot of different agencies delivering crisis care. This can make getting the right help from services difficult, confusing and slow. It is not clear which services work best or who they work best for. What we did This research explored community mental health crisis services for adults. We focused on what is working, who it is working for and in what situations it is working. Service users, carers, mental health professionals and service managers formed an ‘expert stakeholder group’ to guide the project by helping the researchers make sense of what we learned. We gathered information from research reports, other documents and interviews with experts (i.e. service users, carers, professionals, managers). We focused on three questions: How can services make sure that people in crisis can get the right help, quickly? What makes crisis care compassionate? Does it help if different crisis services work together? What we learned Community crisis services are most compassionate and effective when staff from different organisations share information. When leaders of crisis care help staff to work together across services, they find better ways to help people. Close working across teams gives professionals a better understanding of what other services do and makes it easier for them to give people the right help at the right time. When leaders are kind and supportive to staff, they feel better at work and provide better crisis care. What future work can be done It would be useful to explore if the most effective crisis services are the same ones that service users like best. We need to know more about mental health triage, inter-agency working and telehealth. Our project did not explore diversity, but this is an important topic to investigate. Scientific summary Background Mental health crises cause significant disruption to the lives of individuals and families and can be life-threatening. The drive for community care alongside large reductions in hospital beds has led to a proliferation of community crisis services delivered by a diverse range of provider agencies, contributing to difficulties for people in navigating to timely crisis support. There is no single definition of a mental health crisis; people have diverse needs, resulting in a large variation in routes into and through mental health crisis care. Service users report unmet need. Services have diversified quickly in response to reported gaps and delayed responses, and continue to do so. Diversification has led to geographic differences in available crisis care and created a complex web of agencies with different values, referral processes, interventions and access thresholds. It is unclear, in this complex system, which underpinning mechanisms of crisis care are most effective, for whom and in which circumstances. Aim The aim was to identify mechanisms to explain how, for whom and in what circumstances mental health community crisis services for adults work to resolve crises, with a view to informing current and future intervention design and development. Objectives Use stakeholder expertise, current practice and research evidence to develop programme theories to explain how different crisis services work to produce the outcome of resolution of mental health crises. Use a context, intervention, mechanism and outcome (CIMO) framework to construct a sampling frame to identify subsets of literature within which to test programme theories. Iteratively consult, via an expert stakeholder group (ESG) and individual interviews, with diverse stakeholders to test and refine programme theories. Identify and describe pen portraits of UK crisis services that provide exemplars of the programme theories to explain how mental health crisis interventions work in order to explore and explain contextual variation. Synthesise, test and refine the programme theories, and, where possible, identify mid-range theory, to explain how crisis services work to produce the outcome of resolution of the crisis. Provide a framework for future empirical testing of theories in and for further intervention design and development. Produce dissemination materials that communicate the most important mechanisms needed to trigger desired context-specific crisis care outcomes, to inform current and future crisis care interventions and service designs. Design A four-phase realist evidence synthesis, reported in accordance with Realist And Meta-narrative Evidence Syntheses: Evolving Standards (RAMESES) reporting guidelines and comprising (1) identification of candidate programme theories from academic and grey literature; (2) iterative consultation with an ESG and individual interviews to prioritise, test and refine programme theories; (3) focused realist reviews of prioritised theory components; and (4) synthesis to mid-range theory. Main outcome measures The principal aim of the review was to generate and test programme theories, and then synthesise these with mid-range theory, to explain what works, for whom and in what circumstances in adult mental health community crisis care. Data sources The following were conducted: Google Scholar (Google Inc., Mountain View, CA, USA) searches to identify initial programme theories and logic models, focused searches of academic databases with backward citation searching, grey literature searches and hand-searches by the research team and expert stakeholders to test and refine three theory components. An ESG, with membership from lived experience, health professional, social care, policy expertise, health management and commissioning, was consulted on four occasions across the life of the research to test and refine theories and to connect them with real-world experience. Twenty individual realist interviews were conducted with 19 participants to further test, refine and sense-check theory components where there were gaps in topic expertise or theory; the 19 participants included service users; health, social care, ambulance and police professionals; and research and policy experts. Analysis A realist evidence synthesis with stakeholder primary data was used to test and refine three initial programme theories in adult mental health community crisis care: (1) urgent and accessible crisis care, (2) compassionate and therapeutic crisis care and (3) inter-agency working. Data analysis involved using realist logic to identify initial programme theories (objectives 1–3), and testing and refining the programme theories through a focused review of the literature, to extract and configure explanatory causal relationships between CIMO (objectives 3–5). Expert stakeholder consultations supported analysis through linking theories to real-world experience, enabling exploration and explanation of contextual variation as it related to putative mechanisms (objectives 3–5). Individual interviews with experts, who were purposively selected for their topic expertise related to the programme theory components, were deductively analysed according to the CIMO framework. An inductive process identified any new mechanisms not identified from other data sources (objective 3). Pen portraits were developed as illustrative exemplars of the link between CIMO and were refined in collaboration with expert stakeholders (objective 4). Findings from the focused review of the three theory components were synthesised with mid-range theories to produce a framework for any future empirical testing that may be developed (objective 5). Results The scope of the realist review was refined through an initial consultation and discussion between the ESG and the research team. A Diamond-9 prioritisation process was used to facilitate discussion between the ESG and the research team and to refine the scope of the review. This process resulted in three initial programme theories for testing, focused on (1) urgent and accessible crisis care, (2) compassionate and therapeutic crisis care and (3) inter-agency working. The findings from the three focused reviews were synthesised with mid-range theory. Mental health crisis care is provided by a complex array of agencies, each with different definitions of crises, different values about the nature of interventions and different approaches to prioritisation. This is further complicated by multiple overlapping service boundaries. What is apparent is that these differences can only be accommodated within an inter-agency system in which information and decisions are shared from commissioning through to front-line delivery. Inter-agency working provides mechanisms that trigger seamless service delivery through improved communication and collaboration. For this system to work, representation from all agencies and stakeholders is needed. National co-ordination at policy level ensures that investment is appropriately targeted and that important strategic aspirations are met. National co-ordination should steer, but not dictate, local configurations of the agencies needed. Local crisis services should be configured to meet the crisis care needs of local populations within their geography, taking account of any marginalised individuals or communities they serve. Commissioning for inter-agency working needs a focus on managing complex boundaries and transitions across agencies to avoid gaps and disputes. Attention is also needed on how the inter-agency crisis system engages with wider systems important to resolution of crises, including, for example housing, police, local authority, safeguarding and the justice system. The ultimate aim of inter-agency system should be that there is no wrong door through which to access mental health crisis care, and, once in a service, navigation should be facilitated via a single trusted point of liaison. Evaluation is not restricted by organisational boundaries and aims to provide data that take account of how the whole inter-agency system is operating. Conceptualisations of crises as single events or as the sole responsibility of statutory secondary mental health systems are unhelpful and generate fragmentation, leading to gaps and delays for those seeking crisis care and frustration for leaders and front-line staff. The perception of whether or not a service and service providers are accessible carries more of an inhibitive effect than the way that the service is actually organised. People experiencing a crisis choose to access services they perceive as providing a guaranteed response, that are easy to navigate to and that fit with their definition of the crisis. Although the timing of responses in relation to outcomes remains unclear, what is clear is that people feel safer and have a reduced sense of urgency when they trust services. Trust is established through compassionate interactions and proactive management of transitions and waiting. Involvement of the person and their family or support network in decisions supports a sense of trust and relational safety, which may help meet a need for continuity for some. To sustain compassion, front-line staff need access to support for themselves, as well as resources to deliver crisis care that meets their personal and professional ideals. Training in the knowledge, skills and values required for compassion can build confidence among front-line staff in all agencies. System leaders must provide resources and communicate an expectation for compassionate engagement so that it becomes the norm for staff to seek support. This is achieved in an inter-agency context when there is interpersonal contact between all levels of worker, from commissioning through to front-line delivery, that facilitates learning, communication and appreciation of different roles. Furthermore, co-production of crisis care can be facilitated within the inter-agency system, enabling crisis care to be recognised and valued by the community it serves. Service users perceive a crisis when they feel overwhelmed and anxious and when they perceive that they lack a sense of control. Familiar contacts and a safe environment, coupled with reassurance, can help to shape their perception of the service, but, more importantly, can help to reduce distress, thereby mitigating risk and making it more likely that a service user is able to respond to suggested strategies. With an emphasis on rapport and compassion, professionals are encouraged to exhibit positive behaviours that mitigate against the dehumanisation and stigma that service users may perceive when they encounter a service, and which may precipitate or exacerbate a crisis. Compassion shown to front-line staff by leaders leads to compassionate care. A tension between exerting control and providing support was evident at all levels. As integrated care systems are introduced, there is an aspiration that strategic partnerships will reduce competing priorities, which appear debilitating to organisations. Alongside these strategic partnerships, there is a need for coherent local strategies for compassionate and psychologically safe crisis care cognisant of the fact that high-quality care can coexist alongside the worst examples of care in the same organisation. Strategies should include how compassionate and psychologically safe crisis care is provided. Different values and definitions of crisis are accommodated, allowing challenge and debate to become accepted as an opportunity to drive quality improvement. Strengths and limitations Much of the literature was descriptive; therefore, the evidence base was limited. The programme theories identified outline the mechanisms needed to facilitate the best inter-agency community crisis care. Meaningful consultation with expert stakeholders grounded the theories in the reality of community crisis care, although UK evidence is heavily weighted towards England. Project delivery was affected by the COVID-19 pandemic, reducing the number of individual interviews and delaying stakeholder consultations. Stakeholder consultation did not reach as wide a group as originally intended. Conclusion Community crisis care is likely to continue to be delivered by a complex array of agencies responding to a heterogeneous population that presents with different mental health concerns and perceptions of crisis. Inter-agency working provides a platform for seamless transitions between services and timely responses. To deliver desired outcomes, inter-agency working requires continual systems of engagement locally and nationally involving all providers of crisis care through compassionate leadership, sharing of values and shared understanding of systems. Compassion is central and begins with leaders who can influence the culture of crisis organisations. Compassionate leadership is focused on people over systems, enabling front-line staff to retain their compassion and hope, and to work collaboratively across agencies, and it provides a platform for shared decision-making and co-production. All of this helps people in crisis to recognise the service as designed for them and to have trust in community crisis services. The study achieved its objectives, despite unexpected difficulties resulting from the effects of the COVID-19 pandemic, owing to an agile and committed research team, flexible and accommodating stakeholders and support from the funders. Project milestones were adjusted to accommodate the changing context of the study. Future work A framework of programme theories synthesised with mid-range theory developed from this study can inform future research that seeks to develop better mental health crisis care systems. Further work might explore how inter-agency service configurations work, including how telehealth interventions are perceived by service users and how these interventions produce optimal outcomes. Evaluation of crisis care for marginalised groups is needed. The implementation and effect of mental health triage could be explored further. Meaningful engagement with expert stakeholders could be incorporated routinely into research design and delivery. Mental health triage appears to be a promising approach, but has a limited evidence base. Future research could explore and test the implementation and effect of mental health triage systems. This work could focus on different values about prioritisation and how these can be accommodated within an inter-agency system. Further exploration of models of crisis care to mitigate barriers to access for those with substance use or alcohol use problems, personality disorders, physical health conditions and autistic spectrum disorders is needed. Inter-agency models of crisis care are causally linked to optimal crisis outcomes. A focused realist evaluation is needed to explore in more depth the factors influencing access to, and transition through, crisis care for these populations. These outcomes are at times theoretical and have been subjected to limited testing in primary research. UK inter-agency crisis service models provide an opportunity for mixed-method case study approaches to evaluation. A neglected area of focus for this research is the efficacy of models for rural populations. Crisis interventions involving police and mental health services have a growing body of evidence; however, there is a lack of evidence for co-response models involving ambulance paramedic staff or emergency control rooms. There is a lack of focus on individual recovery outcomes. This review highlights the importance of mechanisms such as psychological and relational safety, compassion and trust in producing optimal crisis outcomes. Research is needed to develop evaluation approaches to measure the presence and impact of these mechanisms in crisis care. Data from the literature and from engagement with stakeholders (via the ESG and individual interviews) were combined to refine the realist programme theory/ies to identify key mechanisms that might operate across multiple interventions to ‘trigger’ an appropriate treatment response, and contexts related to these key mechanisms that might enhance or detract from intervention success. Meaningful co-production with service users and other expert stakeholders enhances the relevance of research and should be incorporated routinely into research design and delivery. Study registration The study is registered as PROSPERO CRD42019141680. Funding This project was funded by the National Institute for Health and Care Research (NIHR) Health and Social Care Delivery Research programme (NIHR127709) and will be published in full in Health and Social Care Delivery Research; Vol. 11, No. 15. See the NIHR Journals Library website for further project information.
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- 2023
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84. Fourier-domain modulations and delays of gravitational-wave signals
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Marsat, Sylvain and Baker, John G.
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General Relativity and Quantum Cosmology - Abstract
We present a Fourier-domain approach to modulations and delays of gravitational wave signals, a problem which arises in two different contexts. For space-based detectors like LISA, the orbital motion of the detector introduces a time-dependency in the response of the detector, consisting of both a modulation and a varying delay. In the context of signals from precessing spinning binary systems, a useful tool for building models of the waveform consists in representing the signal as a time-dependent rotation of a quasi-non-precessing waveform. In both cases, being able to compute transfer functions for these effects directly in the Fourier domain may enable performance gains for data analysis applications by using fast frequency-domain waveforms. Our results generalize previous approaches based on the stationary phase approximation for inspiral signals, extending them by including delays and computing corrections beyond the leading order, while being applicable to the broader class of inspiral-merger-ringdown signals. In the LISA case, we find that a leading-order treatment is accurate for high-mass and low-mass signals that are chirping fast enough, with errors consistently reduced by the corrections we derived. By contrast, low-mass binary black holes, if far away from merger and slowly-chirping, cannot be handled by this formalism and we develop another approach for these systems. In the case of precessing binaries, we explore the merger-ringdown range for a handful of cases, using a simple model for the post-merger precession. We find that deviations from leading order can give large fractional errors, while affecting mainly subdominant modes and giving rise to a limited unfaithfulness in the full waveform. Including higher-order corrections consistently reduces the unfaithfulness, and we further develop an alternative approach to accurately represent post-merger features., Comment: 41 pages, 21 figures
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- 2018
85. Horizontal and Vertical Consolidation of the United States into an Administrative State
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BAKER, JOHN S., primary
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- 2022
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86. A Sisyphean Task for Residents: Preparing Literature Reviews About Adverse Events Presented at Morbidity and Mortality Conferences
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Flaris, Alexandros N., Carnabatu, Christopher J., Smith, Alison, Simms, Eric R., Baker, John W., Schroll, Rebecca, Killackey, Mary, and Kandil, Emad
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- 2022
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87. Low- and Very Low-Dose Bevacizumab for Retinopathy of Prematurity: Reactivations, Additional Treatments, and 12-Month Outcomes
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Freedman, Sharon F., Prakalapakorn, Sasapin G., Wallace, David K., Jones, Sarah K., Barman, Navajyoti R., House, Robert J., Nasrazadani, David A., Crouch, Eric, Crouch, Earl R., Jr., Ventura, Gaylord G., Yang, Michael B., Dosunmu, Eniolami O., Gray, Michael E., Motley, William W., Castleberry, Katherine, Cobb, Patricia, Hirsch, Patricia, Reed, Melissa, Sandoval, Monica A., Vallabh, Neil, Rogers, David L., Bremer, Don.L., Golden, Richard P., Jordan, Catherine O., McGregor, Mary Lou, Reem, Rachel E., Schreckengost, Amanda N., Maletic, Sara A., Miller, Rachel T., Bhatt, Amit R., Coats, David K., Romany, Gihan, Demmy, Ann B., Kong, Lingkun X., Hartnett, Mary E., Dries, David C., Hoffman, Robert O., Allman, Susan, Farnsworth, Katie J., Hart, Barbara, Ordonez, Kelliann, Hutchinson, Amy K., Hubbard, George B., III, Rao, Prethy, Robinson, Joshua E., Brower, Judy L., Haider, Kathryn M., Boente, Charline S., Smith, Heather A., Hynes, Elizabeth A., Whitaker, Michele E., VanderVeen, Deborah K., Mantagos, Jason S., Wu, Carolyn, Goldstein, Samantha, Winter, Tamar, Yoon, Grace X., Siatkowski, R. Michael, Collinge, Janine E., Satnes, Kelli J., Blunt, Michelle H., Repka, Michael X., Kraus, Courtney, Shepard, Jennifer A., Kraker, Raymond T., Beck, Roy W., Austin, Darrell S., Boyle, Nicole M., Chandler, Danielle L., Connelly, Patricia L., Conner, Courtney L., Donahue, Quayleen, Fimbel, Brooke P., Henderson, Robert J., Hercinovic, Amra, Hoepner, James E., Kaplon, Joseph D., Li, Zhuokai, Melia, B. Michele, Ortiz, Gillaine, Robinson, Julianne L., Stutz, Kathleen M., Sutherland, Desirae R., Toro, David O., Woodard, Victoria C., Wu, Rui, Cotter, Susan A., Holmes, Jonathan M., Birch, Eileen E., Chen, Angela M., Christiansen, Stephen P., Crouch, Eric R., III, Enyedi, Laura B., Erzurum, S. Ayse, Everett, Donald F., Good, William V., Jenewein, Erin C., Lee, Katherine A., London, Richard, Manh, Vivian M., Manny, Ruth E., Morrell, Beth A., Morrison, David G., Petersen, David B., Pineles, Stacy L., Ranaivo, Hantamalala Ralay, Roberts, Tawna L., Ruark, Scott T., Schweinler, Bonita R., Silver, Jayne L., Suh, Donny W., Summers, Allison I., Verderber, Lisa C., Weise, Katherine K., Diener-West, Marie, Baker, John D., Davis, Barry, Phelps, Dale L., Poff, Stephen W., Saunders, Richard A., Tychsen, Lawrence, Crouch, Eric R., Hubbard, G. Baker, VanderVeen, Deborah, and Cheung, Nathan L.
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- 2022
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88. The Pediatric Optic Neuritis Prospective Outcomes Study: Two-Year Results
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Borchert, Mark S., Chang, Melinda Y., Contractor, Dilshad, Zolfaghari, Emily J., Vyas, Aarti, Yuen, Tiffany, Shah, Veeral S., Paysse, Evelyn A., Romany, Gihan, Peragallo, Jason H., Brower, Judy L., Raghuram, Aparna, Heidary, Gena, Al Wattar, Bilal, Chinn, Ryan, Kothari, Srishti, Siatkowski, R. Michael, Collinge, Janine E., Lim, Maria E., Brewer, Alisha N., Doughty, Annette M., Icks, Sonny W., Almeida, Shannon, de Alba Campomanes, Alejandra, Banwait, Premilla, Graves, Jennifer S., Hajkazemshirazi, Leila, Bastea-Forte, Yizhuo, Arjona, Jennifer K., Chen, Jeremy, Cooper, Karen, Ghadban, Rafif, Chung, Sophia M., Cruz, Oscar A., Khanna, Sangeeta, Christenson, Traci A., Breeding, Lisa L., Govreau, Dawn M., Wallis, Beth A., Geddie, Brooke E., Conley, Julie A., Wolinski, Elisabeth T., Davis, Patricia L., Rudaitis, Indre M., Twite, Jacqueline, Bloomquist, Carrie S., Laboy, Sarah R., Twite, Jackie M., Pineles, Stacy L., Doan, Michelle V., Bernardo, Marianne J., Brodsky, Michael C., Chen, John J., Holmes, Jonathan M., Wernimont, Suzanne M., Czaplewski, Lindsay L., Eastman, Stacy L., Keehn, Moriah A., Priebe, Debbie M., Bremer, Don L., Golden, Richard P., Jordan, Catherine O., McGregor, Mary Lou, Reem, Rachel E., Rogers, David L., Schreckengost, Amanda N., Maletic, Sara A., Dairi, Mays A., Enyedi, Laura B., Jones, Sarah K., Barman, Navajyoti R., House, Robert J., Nasrazadani, David A., Gratton, Sean M., Marsh, Justin D., Dent, Rebecca J., Bond, Lezlie L., Soske, Lori L., Sudhakar, Padmaja, Willen, Christi M., Taylor, Deborah, Moliterno, Nathaniel Q., Nsoesie, Michael, Vally, Shaista, Phillips, Paul H., Lowery, Robert S., Colon, Beth, Stotts, Nancy L., To, Kelly D., McClelland, Collin M., Areaux, Raymond G., Holleschau, Ann M., Merrill, Kim S., Ospina, Luis H., Superstein, Rosanne, Thibeault, Maryse, Gagnon, Helene, Donahue, Sean P., Ruark, Scott T., Fraine, Lisa A., Sprouse, Petrice A., Biernacki, Ronald J., Liu, Grant T., Avery, Robert A., Forbes, Brian J., Jivraj, Imran, Kohli, Anita A., Richter, Meg M., Baumritter, Agnieshka, Mitchell, Ellen B., Nischal, Ken K., Runkel, Lauren M., Blaha, Bianca, Churchfield, Whitney, Fulwylie, Christina, Ko, Melissa W., Mejico, Luis J., Iqbal, Muhammad, Attanasio, Catherine E., Deb, Lena F., Goodrich, Courtney B., Hartwell, Alisha M., Moore, Jennifer A., Bohra, Lisa, Apkarian, Alexandra O., Gianfermi, Elena M., Roarty, John D., Rotberg, Leemor B., Perzyk, Susan N., Kraker, Raymond T., Beck, Roy W., Austin, Darrell S., Boyle, Nicole M., Chandler, Danielle L., Connelly, Patricia L., Conner, Courtney L., Dean, Trevano W., Donahue, Quayleen, Fimbel, Brooke P., Henderson, Robert J., Hercinovic, Amra, Hoepner, James E., Kaplon, Joseph D., Li, Zhuokai, Ortiz, Gillaine, Robinson, Julianne L., Stutz, Kathleen M., Toro, David O., Woodard, Victoria C., Wu, Rui, Repka, Michael X., Balcer, Laura, Kupersmith, Mark, Lazar, Elizabeth L., Waldman, Amy, Wallace, David K., Cotter, Susan A., Birch, Eileen E., Chen, Angela M., Christiansen, Stephen P., Erzurum, S. Ayse, Everett, Donald F., Freedman, Sharon F., Good, William V., Lee, Katherine A., London, Richard, Manh, Vivian M., Manny, Ruth E., Morrison, David G., Schweinler, Bonita R., Silver, Jayne L., Verderber, Lisa C., Weise, Katherine K., Green, Ari, Diener-West, Marie, Baker, John D., Davis, Barry, Phelps, Dale L., Poff, Stephen W., Saunders, Richard A., Tychsen, Lawrence, and Waldman, Amy T.
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- 2022
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89. First report from the American Society of Metabolic and Bariatric Surgery closed-claims registry: prevalence, causes, and lessons learned from bariatric surgery medical malpractice claims
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Morton, John M., Khoury, Habib, Brethauer, Stacy A., Baker, John W., Sweet, William A., Mattar, Samer, Ponce, Jaime, Nguyen, Ninh T., Rosenthal, Raul J., and DeMaria, Eric J.
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- 2022
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90. Ethnic differences in metabolic achievement between Māori, Pacific, and European New Zealanders with type 2 diabetes
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Yu, Dahai, Cai, Yamei, Levi Osuagwu, Uchechukwu, Pickering, Karen, Baker, John, Cutfield, Richard, McKree Jansen, Rawiri, Orr-Walker, Brandon J., Sundborn, Gerhard, Zhao, Zhanzheng, and Simmons, David
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- 2022
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91. Evaluating carbon tax policy: A methodological reassessment of a natural experiment
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Arcila, Andres and Baker, John D.
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- 2022
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92. Minimizing the Impact of Parental Grief on Children: Parent and Family Interventions
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Baker, John E., primary
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- 2022
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93. Prompt Electromagnetic Transients from Binary Black Hole Mergers
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Kelly, Bernard J., Baker, John G., Etienne, Zachariah B., Giacomazzo, Bruno, and Schnittman, Jeremy
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Astrophysics - High Energy Astrophysical Phenomena ,General Relativity and Quantum Cosmology - Abstract
Binary black hole (BBH) mergers provide a prime source for current and future interferometric GW observatories. Massive BBH mergers may often take place in plasma-rich environments, leading to the exciting possibility of a concurrent electromagnetic (EM) signal observable by traditional astronomical facilities. However, many critical questions about the generation of such counterparts remain unanswered. We explore mechanisms that may drive EM counterparts with magnetohydrodynamic simulations treating a range of scenarios involving equal-mass black-hole binaries immersed in an initially homogeneous fluid with uniform, orbitally aligned magnetic fields. We find that the time development of Poynting luminosity, which may drive jet-like emissions, is relatively insensitive to aspects of the initial configuration. In particular, over a significant range of initial values, the central magnetic field strength is effectively regulated by the gas flow to yield a Poynting luminosity of $10^{45}-10^{46} \rho_{-13} M_8^2 \, {\rm erg}\,{\rm s}^{-1}$, with BBH mass scaled to $M_8 \equiv M/(10^8 M_{\odot})$ and ambient density $\rho_{-13} \equiv \rho/(10^{-13} \, {\rm g} \, {\rm cm}^{-3})$. We also calculate the direct plasma synchrotron emissions processed through geodesic ray-tracing. Despite lensing effects and dynamics, we find the observed synchrotron flux varies little leading up to merger., Comment: 22 pages, 21 figures; additional reference + clarifying text added to match published version
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- 2017
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94. Laser Interferometer Space Antenna
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Amaro-Seoane, Pau, Audley, Heather, Babak, Stanislav, Baker, John, Barausse, Enrico, Bender, Peter, Berti, Emanuele, Binetruy, Pierre, Born, Michael, Bortoluzzi, Daniele, Camp, Jordan, Caprini, Chiara, Cardoso, Vitor, Colpi, Monica, Conklin, John, Cornish, Neil, Cutler, Curt, Danzmann, Karsten, Dolesi, Rita, Ferraioli, Luigi, Ferroni, Valerio, Fitzsimons, Ewan, Gair, Jonathan, Bote, Lluis Gesa, Giardini, Domenico, Gibert, Ferran, Grimani, Catia, Halloin, Hubert, Heinzel, Gerhard, Hertog, Thomas, Hewitson, Martin, Holley-Bockelmann, Kelly, Hollington, Daniel, Hueller, Mauro, Inchauspe, Henri, Jetzer, Philippe, Karnesis, Nikos, Killow, Christian, Klein, Antoine, Klipstein, Bill, Korsakova, Natalia, Larson, Shane L, Livas, Jeffrey, Lloro, Ivan, Man, Nary, Mance, Davor, Martino, Joseph, Mateos, Ignacio, McKenzie, Kirk, McWilliams, Sean T, Miller, Cole, Mueller, Guido, Nardini, Germano, Nelemans, Gijs, Nofrarias, Miquel, Petiteau, Antoine, Pivato, Paolo, Plagnol, Eric, Porter, Ed, Reiche, Jens, Robertson, David, Robertson, Norna, Rossi, Elena, Russano, Giuliana, Schutz, Bernard, Sesana, Alberto, Shoemaker, David, Slutsky, Jacob, Sopuerta, Carlos F., Sumner, Tim, Tamanini, Nicola, Thorpe, Ira, Troebs, Michael, Vallisneri, Michele, Vecchio, Alberto, Vetrugno, Daniele, Vitale, Stefano, Volonteri, Marta, Wanner, Gudrun, Ward, Harry, Wass, Peter, Weber, William, Ziemer, John, and Zweifel, Peter
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
Following the selection of The Gravitational Universe by ESA, and the successful flight of LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's call for missions for L3. The observatory will be based on three arms with six active laser links, between three identical spacecraft in a triangular formation separated by 2.5 million km. LISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using Gravitational Waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the infant Universe at TeV energy scales, has known sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales near the horizons of black holes, all the way to cosmological scales. The LISA mission will scan the entire sky as it follows behind the Earth in its orbit, obtaining both polarisations of the Gravitational Waves simultaneously, and will measure source parameters with astrophysically relevant sensitivity in a band from below $10^{-4}\,$Hz to above $10^{-1}\,$Hz., Comment: Submitted to ESA on January 13th in response to the call for missions for the L3 slot in the Cosmic Vision Programme
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- 2017
95. 'Safer, Not Safe': Service Users' Experiences of Psychological Safety in Inpatient Mental Health Wards in the United Kingdom.
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Vogt, Katharina Sophie, Baker, John, Kendal, Sarah, Griffin, Bethany Leigh, Mizen, Emily, Sharp, Hannah, and Johnson, Judith
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PATIENT safety , *QUALITATIVE research , *RESEARCH funding , *INTERVIEWING , *HOSPITAL patients , *PSYCHOLOGICAL safety , *DECISION making , *DESCRIPTIVE statistics , *THEMATIC analysis , *RESEARCH methodology , *ATTITUDES of medical personnel , *PSYCHIATRIC hospitals , *GROUNDED theory , *PATIENTS' attitudes - Abstract
Research on patient safety in mental health settings is limited compared to physical healthcare settings. Recent qualitative studies have highlighted that patient safety is more than just physical safety but includes psychological safety. Traditionally, psychological safety has been defined as the belief that it is safe to take interpersonal risks, such as speaking up, without a fear of negative consequences. However, to date, it is not clear what constitutes psychological safety for service users of inpatient mental health settings. To understand this, we conducted 12 interviews with former inpatient mental health service users. Interviews were analysed with Reflexive Thematic Analysis, and five themes were developed. All themes had subthemes. Overall, we found that participants were more readily able to draw on situations where they felt psychologically unsafe, rather than safe. Psychological safety in service users was influenced by (1) healthcare staff attitudes and behaviours towards them, (2) their relationships with other service users, (3) whether they felt they had any control over their environment and medical decision‐making regarding their care, (4) their experiences of physically safety, feeling listened to and believed and (5) access to meaningful occupation on the wards. These findings suggest that changes are needed to enhance inpatient mental health service users' general experiences of psychological safety. Further research will need to (1) further develop understanding of the concept of psychological safety for service users and (2) identify interventions, and such interventions should be co‐designed with service users. [ABSTRACT FROM AUTHOR]
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- 2024
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96. Mental health patients' preferences regarding restrictive interventions: An integrative review.
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Lindekilde, Camilla Rosendal, Pedersen, Martin Locht, Birkeland, Søren Fryd, Hvidhjelm, Jacob, Baker, John, and Gildberg, Frederik Alkier
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PSYCHOTHERAPY patients ,PATIENT autonomy ,MEDICAL information storage & retrieval systems ,PATIENTS ,RESEARCH funding ,CONTROL (Psychology) ,MENTAL health ,PSYCHIATRY ,HOSPITAL admission & discharge ,CINAHL database ,RESTRAINT of patients ,SECLUSION of psychiatric hospital patients ,TRANQUILIZING drugs ,DESCRIPTIVE statistics ,SYSTEMATIC reviews ,THEMATIC analysis ,MEDLINE ,COMMUNICATION ,PSYCHIATRIC hospitals ,PSYCHOSOCIAL factors ,PATIENTS' attitudes ,PSYCHOLOGY information storage & retrieval systems - Abstract
Accessible summary: What is known on the subject?: The use of restrictive interventions is described as a violation of patients' rights and autonomy. It must only be used as a last resort to manage dangerous behaviour, to prevent or reduce the risk of mental health patients harming themselves or others.International mental health policy and legislation agree that when restrictive interventions are applied, the least restrictive alternative should be chosen. What the paper adds to existing knowledge?: The results are ambiguous, as to which restrictive intervention is preferred over others, but there are tendencies towards the majority preferring observation, with mechanical restraint being the least preferred.To make the experience less intrusive and restrictive, certain factors are preferred, such as a more pleasant and humane seclusion room environment, staff communicating during the application and staff of same gender applying the intervention. What are the implications for practice?: When applying restrictive interventions, mental health professionals should consider environment, communication and duration factors that influence patient preferences, such as the opportunity to keep some personal items in the seclusion room, or, when using restraint, to communicate the reason and explain what is going to happen.More research is needed to clarify patients' preferences regarding restrictive interventions and their views on which are the least restrictive. Preferably, agreement is needed on standard measures, and global use of the same definition of restrictive interventions. Introduction: The use of restrictive interventions is a violation of patients' rights that causes physical and psychological harm and which is a well‐known challenge globally. Mental health law and legislative principles and experts agree that when restrictive interventions are applied, the least restrictive alternative should be used. However, there is no consensus on what is the least restrictive alternative, especially from the patient perspective. Aim: To investigate the literature on mental health patients' preferences regarding restrictive interventions applied during admission to a psychiatric hospital. Method: An integrative review informed by the PRISMA statement and thematic analysis were undertaken. Results: There were tendencies towards patients preferring observation and, for the majority, mechanical restraint was the least preferred restrictive intervention. Factors such as environment, communication and duration were found to influence patients' preferences. Discussion: There is a lack of agreement on how best to measure patients' preferences and this complicates the choice of the least restrictive alternative. Nonetheless, our findings show that staff should consider environment, communication and duration when applying restrictive interventions. Implications for Practice: More research on restrictive interventions and the least restrictive alternative is warranted, but agreement is needed on standard measures, and a standard global definition of restrictive interventions. [ABSTRACT FROM AUTHOR]
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- 2024
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97. Effects of 5-ion 6-beam sequential irradiation in the presence and absence of hindlimb or control hindlimb unloading on behavioral performances and plasma metabolic pathways of Fischer 344 rats.
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Raber, Jacob, Chaudhari, Mitali, De la Torre, Alexis, Holden, Sarah, Kessler, Kat, Glaeser, Breanna, Lenarczyk, Marek, Leonard, Scott Willem, Borg, Alexander, Kwok, Andy, Patel, Chirayu, Kronenberg, Amy, Olsen, Christopher M., Willey, Jeffrey S., Morré, Jeffrey, Choi, Jaewoo, Stevens, Jan Frederik, Bobe, Gerd, Minnier, Jessica, and Baker, John
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TOTAL body irradiation ,GALACTIC cosmic rays ,PHENYLALANINE ,GLUTAMINE ,GLUTAMIC acid - Abstract
Introduction: Effects and interactions between different spaceflight stressors are expected to be experienced by crew on missions when exposed to microgravity and galactic cosmic rays (GCRs). One of the limitations of previous studies on simulated weightlessness using hindlimb unloading (HU) is that a control HU condition was not included. Methods: We characterized the behavioral performance of male Fischer rats 2 months after sham or total body irradiation with a simplified 5-ion 6-mixed-beam exposure representative of GCRs in the absence or presence of HU. Six months later, the plasma, hippocampus, and cortex were processed to determine whether the behavioral effects were associated with long-term alterations in the metabolic pathways. Results: In the open field without and with objects, interactions were observed for radiation × HU. In the plasma of animals that were not under the HU or control HU condition, the riboflavin metabolic pathway was affected most for sham irradiation vs. 0.75 Gy exposure. Analysis of the effects of control HU on plasma in the sham-irradiated animals showed that the alanine, aspartate, glutamate, riboflavin, and glutamine metabolisms as well as arginine biosynthesis were affected. The effects of control HU on the hippocampus in the sham-irradiated animals showed that the phenylalanine, tyrosine, and tryptophan pathway was affected the most. Analysis of effects of 0.75 Gy irradiation on the cortex of control HU animals showed that the glutamine and glutamate metabolic pathway was affected similar to the hippocampus, while the riboflavin pathway was affected in animals that were not under the control HU condition. The effects of control HU on the cortex in sham-irradiated animals showed that the riboflavin metabolic pathway was affected. Animals receiving 0.75 Gy of irradiation showed impaired glutamine and glutamate metabolic pathway, whereas animals receiving 1.5 Gy of irradiation showed impaired riboflavin metabolic pathways. A total of 21 plasma metabolites were correlated with the behavioral measures, indicating that plasma and brain biomarkers associated with behavioral performance are dependent on the environmental conditions experienced. Discussion: Phenylalanine, tyrosine, and tryptophan metabolism as well as phenylalanine and tryptophan as plasma metabolites are biomarkers that can be considered for spaceflight as they were revealed in both Fischer and WAG/Rij rats exposed to simGCRsim and/or HU. [ABSTRACT FROM AUTHOR]
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- 2024
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98. The LTAR Integrated Common Experiment at Upper Mississippi River Basin‐Platteville.
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Busch, Dennis L., Mahmud, Kishan, Johnson, Jane M. F., Papanicolaou, Athanasios, Baker, John M., and Cartmill, Andrew D.
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- 2024
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99. The LTAR Cropland Common Experiment at Upper Mississippi River Basin–St. Paul.
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Dalzell, Brent J., Baker, John M., Venterea, Rodney T., Spokas, Kurt A., Feyereisen, Gary W., Rice, Pamela J., and Alexander, Jonathan R.
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- 2024
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100. Implementing and evaluating patient‐focused safety technology on adult acute mental health wards.
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Kendal, Sarah, Louch, Gemma, Walker, Lauren, Shafiq, Saba, Halligan, Daisy, Brierley‐Jones, Lyn, and Baker, John
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DIGITAL technology ,INTELLECT ,PATIENT safety ,RESEARCH funding ,DIFFUSION of innovations ,ETHNOLOGY research ,FIELD notes (Science) ,LEADERSHIP ,INTERVIEWING ,DESCRIPTIVE statistics ,SOUND recordings ,MOTIVATION (Psychology) ,INTENSIVE care units ,RESEARCH methodology ,COMMUNICATION ,PSYCHIATRIC hospitals ,DATA analysis software ,PATIENTS' attitudes ,CRITICAL care medicine ,COVID-19 pandemic - Abstract
Accessible Summary: What is known on the subject: Mental health wards can feel unsafe. We know that patients and staff have different ideas about what makes a hospital ward safe or unsafe.Patients are often the first to know when the atmosphere on a ward becomes tense, but often, no one asks them for their views.Patients and staff are experts and should be included in discussions about how to make wards safer. What this paper adds to existing knowledge: We got together with some service users and staff, and made an app that helps patients to tell staff when they are not feeling safe on a mental health ward. We tried it out on six wards and we asked patients and staff what they thought.The app was easy to use and most people liked the look of it.Patients said staff did not talk with them enough and so they liked using the app. However, some staff said they could tell how patients were feeling without an app and so they did not need it. Ward managers told us that staff were often very busy and did not always have time to use the app. What are the implications for practice: This app could help staff know straightaway when patients do not feel safe on the ward, so that they can act quickly to calm things down.To make the most of the app, staff need to get used to it and bring it into ward routines. Introduction: Safety improvement on mental health wards is of international concern. It should incorporate patient perspectives. Aim: Implementation and evaluation of 'WardSonar', a digital safety‐monitoring tool for adult acute mental health wards, developed with stakeholders to communicate patients' real‐time safety perceptions to staff. Method: Six acute adult mental health wards in England implemented the tool in 2022. Evaluation over 10 weeks involved qualitative interviews (34 patients, 33 staff), 39 focused ethnographic observations, and analysis of pen portraits. Results: Implementation and evaluation of the WardSonar tool was feasible despite challenging conditions. Most patients valued the opportunity to communicate their immediate safety concerns, stating that staff had a poor understanding of them. Some staff said the WardSonar tool could help enhanced ward safety but recognised a need to incorporate its use into daily routines. Others said they did not need the tool to understand patients' safety concerns. Discussion: Foreseeable challenges, including staff ambivalence and practical issues, appeared intensified by the post‐COVID‐19 context. Implications for Practice: The WardSonar tool could improve ward safety, especially from patients' perspectives. Future implementation could support staff to use the real‐time data to inform proactive safety interventions. [ABSTRACT FROM AUTHOR]
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- 2024
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