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1. Sub-electron readout noise in a Skipper CCD fabricated on high resistivity silicon

Author: Fernández Moroni, Guillermo, Estrada, Juan, Cancelo, Gustavo, Holland, Stephen E., Paolini, Eduardo E., and Diehl, H. Thomas
Published: 2012
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2. Achieving sub electron noise in CCD systems by means of digital filtering techniques that lower 1/f pixel correlated noise

Author: Cancelo, Gustavo Indalecio, Estrada, Juan Cruz, Moroni, Guillermo Fernandez, Treptow, Ken, Zmuda, Ted, and Diehl, H. Thomas
Published: 2012
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3. Studies of $X(3872)$ and $\psi(2S)$ production in $p\bar{p}$ collisions at 1.96 TeV

Author: Abazov, Victor Mukhamedovich, Abbott, Braden Keim, Atkins, Scott, Edmunds, Daniel L., Ellison, John A., Elvira, V. Daniel, Enari, Yuji, Evans, Harold G., Evdokimov, Anatoly V., Evdokimov, Valeri N., Faure, Alexandre, Feng, Lei, Ferbel, Thomas, Augsten, Kamil, Fiedler, Frank, Filthaut, Frank, Fisher, Wade Cameron, Fisk, H. Eugene, Fortner, Michael R., Fox, Harald, Franc, Jiri, Fuess, Stuart C., Garbincius, Peter H., Garcia-Bellido, Aran, Aushev, Volodymyr, Garcia-Gonzalez, Jose Andres, Gavrilov, Vladimir B., Geng, Weigang, Gerber, Cecilia Elena, Gershtein, Yuri S., Ginther, George E., Gogota, Olga, Golovanov, Georgy Anatolievich, Grannis, Paul D., Greder, Sebastien, Aushev, Yegor, Greenlee, Herbert B., Grenier, Gerald Jean, Gris, Phillipe Luc, Grivaz, Jean-Francois, Grohsjean, Alexander, Gruenendahl, Stefan, Gruenewald, Martin Werner, Guillemin, Thibault, Gutierrez, Gaston R., Gutierrez, Phillip, Avila, Carlos A., Haley, Joseph Glenn Biddle, Han, Liang, Harder, Kristian, Harel, Amnon, Hauptman, John Michael, Hays, Jonathan M., Head, Tim, Hebbeker, Thomas, Hedin, David R., Hegab, Hatim, Badaud, Frederique, Heinson, Ann, Heintz, Ulrich, Hensel, Carsten, Heredia-de La Cruz, Ivan, Herner, Kenneth Richard, Hesketh, Gavin G., Hildreth, Michael D., Hirosky, Robert James, Hoang, Trang, Hobbs, John D., Bagby, Linda F., Hoeneisen, Bruce, Hogan, Julie, Hohlfeld, Mark, Holzbauer, Jenny Lyn, Howley, Ian James, Hubacek, Zdenek, Hynek, Vlastislav, Iashvili, Ia, Ilchenko, Yuriy, Illingworth, Robert A., Baldin, Boris, Ito, Albert S., Jabeen, Shabnam, Jaffre, Michel J., Jayasinghe, Ayesh, Jeong, Min-Soo, Jesik, Richard L., Jiang, Peng, Johns, Kenneth Arthur, Johnson, Emily, Johnson, Marvin E., Bandurin, Dmitry V., Jonckheere, Alan M., Jonsson, Per Martin, Joshi, Jyoti, Jung, Andreas Werner, Juste, Aurelio, Kajfasz, Eric, Karmanov, Dmitriy Y., Katsanos, Ioannis, Kaur, Manbir, Kehoe, Robert Leo Patrick, Banerjee, Sunanda, Kermiche, Smain, Khalatyan, Norayr, Khanov, Alexander, Kharchilava, Avto, Kharzheev, Yuri N., Kiselevich, Ivan Lvovich, Kohli, Jatinder M., Kozelov, Alexander V., Kraus, James Alexander, Kumar, Ashish, Acharya, Bannanje Sripath, Barberis, Emanuela, Kupco, Alexander, Kurca, Tibor, Kuzmin, Valentin Alexandrovich, Lammers, Sabine Wedam, Lebrun, Patrice, Lee, Hyeon-Seung, Lee, Seh-Wook, Lee, William M., Lei, Xiaowen, Lellouch, Jeremie, Baringer, Philip S., Li, Dikai, Li, Hengne, Li, Liang, Li, Qi-Zhong, Lim, Jeong Ku, Lincoln, Donald W., Linnemann, James Thomas, Lipaev, Vladimir V., Lipton, Ronald J., Liu, Huanzhao, Bartlett, J. Frederick, Liu, Yanwen, Lobodenko, Alexandre, Lokajicek, Milos, Lopes De Sá, Rafael, Luna-Garcia, Rene, Lyon, Adam Leonard, Maciel, Arthur K. A., Madar, Romain, Magana-Villalba, Ricardo, Malik, Sudhir, Bassler, Ursula Rita, Malyshev, Vladimir L., Mansour, Jason, Martínez-Ortega, Jorge, McCarthy, Robert L., Mcgivern, Carrie Lynne, Meijer, Melvin M., Melnitchouk, Alexander S., Menezes, Diego D., Mercadante, Pedro Galli, Merkin, Mikhail M., Bazterra, Victor, Meyer, Arnd, Meyer, Jorg Manfred, Miconi, Florian, Mondal, Naba K., Mulhearn, Michael James, Nagy, Elemer, Narain, Meenakshi, Nayyar, Ruchika, Neal, Homer A., Negret, Juan Pablo, Bean, Alice L., Neustroev, Petr V., Nguyen, Huong Thi, Nunnemann, Thomas P., Hernandez Orduna, Jose de Jesus, Osman, Nicolas Ahmed, Pal, Arnab, Parashar, Neeti, Parihar, Vivek, Park, Sung Keun, Partridge, Richard A., Begalli, Marcia, Parua, Nirmalya, Patwa, Abid, Penning, Bjoern, Perfilov, Maxim Anatolyevich, Peters, Reinhild Yvonne Fatima, Petridis, Konstantinos, Petrillo, Gianluca, Petroff, Pierre, Pleier, Marc-Andre, Podstavkov, Vladimir M., Bellantoni, Leo, Popov, Alexey V., Prewitt, Michelle, Price, Darren, Prokopenko, Nikolay N., Qian, Jianming, Quadt, Arnulf, Quinn, Gene Breese, Ratoff, Peter N., Razumov, Ivan A., Ripp-Baudot, Isabelle, Beri, Suman B., Rizatdinova, Flera, Rominsky, Mandy Kathleen, Ross, Anthony, Royon, Christophe, Rubinov, Paul Michael, Ruchti, Randal C., Sajot, Gerard, Sánchez Hernández, Alberto, Sanders, Michiel P., De Souza Santos, Angelo, Bernardi, Gregorio, Savage, David G., Savitskyi, Mykola, Sawyer, H. Lee, Scanlon, Timothy P., Schamberger, R. Dean, Scheglov, Yury A., Schellman, Heidi M., Schott, Matthias, Schwanenberger, Christian, Schwienhorst, Reinhard H., Adams, Mark Raymond, Bernhard, Ralf Patrick, Sekaric, Jadranka, Severini, Horst, Shabalina, Elizaveta K., Shary, Viacheslav V., Shaw, Savanna, Shchukin, Andrey A., Shkola, Oleg, Simak, Vladislav J., Skubic, Patrick Louis, Slattery, Paul F., Bertram, Iain A., Snow, Gregory R., Snow, Joel Mark, Snyder, Scott Stuart, Söldner-Rembold, Stefan, Sonnenschein, Lars, Soustruznik, Karel, Stark, Jan, Stefaniuk, Nazar, Stoyanova, Dina A., Strauss, Michael G., Besancon, Marc, Suter, Louise, Svoisky, Peter V., Titov, Maxim, Tokmenin, Valeriy V., Tsai, Yun-Tse, Tsybychev, Dmitri, Tuchming, Boris, Tully, Christopher George T., Uvarov, Lev, Uvarov, Sergey L., Beuselinck, Raymond, Uzunyan, Sergey A., Van Kooten, Richard J., van Leeuwen, Willem M., Varelas, Nikos, Varnes, Erich W., Vasilyev, Igor A., Verkheev, Alexander Yurievich, Vertogradov, Leonid S., Verzocchi, Marco, Vesterinen, Mika, Bhat, Pushpalatha C., Vilanova, Didier, Vokac, Petr, Wahl, Horst D., Wang, Chen, Wang, Michael H. L. S., Warchol, Jadwiga, Watts, Gordon Thomas, Wayne, Mitchell R., Weichert, Jonas, Welty-Rieger, Leah Christine, Bhatia, Sudeep, Williams, Mark Richard James, Wilson, Graham Wallace, Wobisch, Markus, Wood, Darien Robert, Wyatt, Terence R., Xie, Yunhe, Yamada, Ryuji, Yang, Siqi, Yasuda, Takahiro, Yatsunenko, Yuriy A., Bhatnagar, Vipin, Ye, Wanyu, Ye, Zhenyu, Yin, Hang, Yip, Kin, Youn, Sungwoo, Yu, Jiaming, Zennamo, Joseph, Zhao, Tianqi Gilbert, Zhou, Bing, Zhu, Junjie, Blazey, Gerald Charles, Zielinski, Marek, Zieminska, Daria, Zivkovic, Lidija, D0 Collaboration, Blessing, Susan K., Bloom, Kenneth A., Adams, Todd, Boehnlein, Amber S., Boline, Daniel Dooley, Boos, Edward E., Borissov, Guennadi, Borysova, Maryna, Brandt, Andrew, Brandt, Oleg, Brochmann, Michelle, Brock, Raymond L., Bross, Alan D., Agnew, James P., Brown, Duncan Paul, Bu, Xue-Bing, Buehler, Marc, Buescher, Volker, Bunichev, Viacheslav Yevgenyevich, Burdin, Sergey, Buszello, Claus Peter, Camacho-Perez, Enrique, Casey, Brendan Cameron Kieran, Castilla-Valdez, Heriberto, Alexeev, Guennadi D., Caughron, Seth Aaron, Chakrabarti, Subhendu, Chan, Kwok Ming Leo, Chandra, Avdhesh, Chapon, Emilien, Chen, Guo, Cho, Sung-Woong, Choi, Suyong, Choudhary, Brajesh C., Cihangir, Selcuk, Alkhazov, Georgiy D., Claes, Daniel R., Clutter, Justace Randall, Cooke, Michael P., Cooper, William Edward, Corcoran, Marjorie D., Couderc, Fabrice, Cousinou, Marie-Claude, Cuth, Jakub, Cutts, David, Das, Amitabha, Alton, Andrew K., Davies, Gavin John, de Jong, Sijbrand J., De La Cruz-Burelo, Eduard, Deliot, Frederic, Demina, Regina, Denisov, Dmitri S., Denisov, Sergei P., Desai, Satish Vijay, Deterre, Cecile, DeVaughan, Kayle Otis, Askew, Andrew Warren, Diehl, H. Thomas, Diesburg, Michael, Ding, Pengfei, Dominguez, D. Aaron M., Drutskoy, Alexey, Dubey, Abhinav Kumar, Dudko, Lev V., Duperrin, Arnaud, Dutt, Suneel, Eads, Michael T., Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Louis Pasteur - Strasbourg I, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), D0, Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département de Physique des Particules (ex SPP) (DPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: transverse momentum dependence, X(3872): hadroproduction, High Energy Physics - Experiment, anti-p p: colliding beams, energy dependence, bottom, hadroproduction [X(3872)], DZERO, anti-p p: scattering, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Particle Physics Experiments, ddc:530, Batavia TEVATRON Coll, enhancement, 1960 GeV-cms, scattering [anti-p p], energy: kinetic, hep-ex, hadroproduction [psi(3685)], psi(3685): hadroproduction, binding energy, kinetic [energy], direct production, High Energy Physics::Experiment, hadron, Particle Physics - Experiment, colliding beams [anti-p p], inclusive production, signature, experimental results
Abstract: Physical review / D 102(7), 072005 (1-14) (2020). doi:10.1103/PhysRevD.102.072005, We present various properties of the production of the $X(3872)$ and $ψ(2S)$ states based on $10.4 fb^{−1}$ collected by the D0 experiment in Tevatron $p\bar{p}$ collisions at $\sqrt{s}=1.96 TeV$. For both states, we measure the nonprompt fraction $f_{NP}$ of the inclusive production rate due to decays of $b$-flavored hadrons. We find the $f_{NP}$ values systematically below those obtained at the LHC. The fNP fraction for $ψ(2S)$ increases with transverse momentum, whereas for the $X(3872)$ it is constant within large uncertainties, in agreement with the LHC results. The ratio of prompt to nonprompt $ψ(2S)$ production, $(1−f_{NP})/f_{NP}$, decreases only slightly going from the Tevatron to the LHC, but for the $X(3872)$, this ratio decreases by a factor of about 3. We test the soft-pion signature of the $X(3872)$ modeled as a weakly bound charm-meson pair by studying the production of the $X(3872)$ as a function of the kinetic energy of the $X(3872)$ and the pion in the $X(3872)π$ center-of-mass frame. For a subsample consistent with prompt production, the results are incompatible with a strong enhancement in the production of the $X(3872)$ at the small kinetic energy of the $X(3872)$ and the π in the $X(3872)π$ center-of-mass frame expected for the $X$+soft-pion production mechanism. For events consistent with being due to decays of $b$ hadrons, there is no significant evidence for the soft-pion effect, but its presence at the level expected for the binding energy of 0.17 MeV and the momentum scale $Λ=M(π)$ is not ruled out., Published by Inst.302363, Melville, NY
Published: 2020
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4. Inclusive production of the $P_c$ resonances in $p \overline p $ collisions

Author: Abazov, Victor Mukhamedovich, Abbott, Braden Keim, Acharya, Bannanje Sripath, Adams, Mark Raymond, Adams, Todd, Agnew, James P., Alexeev, Guennadi D., Alkhazov, Georgiy D., Alton, Andrew K., Askew, Andrew Warren, Atkins, Scott, Augsten, Kamil, Aushev, Volodymyr, Aushev, Yegor, Avila, Carlos A., Badaud, Frederique, Bagby, Linda F., Baldin, Boris, Bandurin, Dmitry V., Banerjee, Sunanda, Barberis, Emanuela, Baringer, Philip S., Bartlett, J. Frederick, Bassler, Ursula Rita, Bazterra, Victor, Bean, Alice L., Begalli, Marcia, Bellantoni, Leo, Beri, Suman B., Bernardi, Gregorio, Bernhard, Ralf Patrick, Bertram, Iain A., Besancon, Marc, Beuselinck, Raymond, Bhat, Pushpalatha C., Bhatia, Sudeep, Bhatnagar, Vipin, Blazey, Gerald Charles, Blessing, Susan K., Bloom, Kenneth A., Boehnlein, Amber S., Boline, Daniel Dooley, Boos, Edward E., Borissov, Guennadi, Borysova, Maryna, Brandt, Andrew, Brandt, Oleg, Michelle Brochmann, Brock, Raymond L., Bross, Alan D., Brown, Duncan Paul, Bu, Xue-Bing, Buehler, Marc, Buescher, Volker, Bunichev, Viacheslav Yevgenyevich, Burdin, Sergey, Buszello, Claus Peter, Camacho-Perez, Enrique, Casey, Brendan Cameron Kieran, Castilla-Valdez, Heriberto, Caughron, Seth Aaron, Chakrabarti, Subhendu, Chan, Kwok Ming Leo, Chandra, Avdhesh, Chapon, Emilien, Chen, Guo, Cho, Sung-Woong, Choi, Suyong, Choudhary, Brajesh C., Cihangir, Selcuk, Claes, Daniel R., Clutter, Justace Randall, Cooke, Michael P., Cooper, William Edward, Corcoran, Marjorie D., Couderc, Fabrice, Cousinou, Marie-Claude, Cuth, Jakub, Cutts, David, Das, Amitabha, Davies, Gavin John, Jong, Sijbrand Jan, La Cruz-Burelo, Eduard, Deliot, Frederic, Demina, Regina, Denisov, Dmitri S., Denisov, Sergei P., Desai, Satish Vijay, Deterre, Cecile, Devaughan, Kayle Otis, Diehl, H. Thomas, Diesburg, Michael, Ding, Pengfei, Dominguez, D. Aaronm, Drutskoy, Alexey, Dubey, Abhinav Kumar, Dudko, Lev V., Duperrin, Arnaud, Dutt, Suneel, Eads, Michael T., Edmunds, Daniel L., Ellison, John A., Elvira, V. Daniel, Enari, Yuji, Evans, Harold G., Evdokimov, Anatoly V., Evdokimov, Valeri N., Faure, Alexandre, Feng, Lei, Ferbel, Thomas, Fiedler, Frank, Filthaut, Frank, Fisher, Wade Cameron, Fisk, H. Eugene, Fortner, Michael R., Fox, Harald, Franc, Jiri, Fuess, Stuart C., Garbincius, Peter H., Garcia-Bellido, Aran, Garcia-Gonzalez, Jose Andres, Gavrilov, Vladimir B., Geng, Weigang, Gerber, Cecilia Elena, Gershtein, Yuri S., Ginther, George E., Gogota, Olga, Golovanov, Georgy Anatolievich, Grannis, Paul D., Greder, Sebastien, Greenlee, Herbert B., Grenier, Gerald Jean, Gris, Phillipe Luc, Grivaz, Jean-Francois, Grohsjean, Alexander, Gruenendahl, Stefan, Gruenewald, Martin Werner, Guillemin, Thibault, Gutierrez, Gaston R., Gutierrez, Phillip, Haley, Joseph Glenn Biddle, Han, Liang, Harder, Kristian, Harel, Amnon, Hauptman, John Michael, Hays, Jonathan M., Head, Tim, Hebbeker, Thomas, Hedin, David R., Hegab, Hatim, Heinson, Ann, Heintz, Ulrich, Hensel, Carsten, Heredia-De La Cruz, Ivan, Herner, Kenneth Richard, Hesketh, Gavin G., Hildreth, Michael D., Hirosky, Robert James, Hoang, Trang, Hobbs, John D., Hoeneisen, Bruce, Hogan, Julie, Hohlfeld, Mark, Holzbauer, Jenny Lyn, Howley, Ian James, Hubacek, Zdenek, Hynek, Vlastislav, Iashvili, Ia, Ilchenko, Yuriy, Illingworth, Robert A., Ito, Albert S., Shabnam Jabeen, Jaffre, Michel J., Jayasinghe, Ayesh, Jeong, Min-Soo, Jesik, Richard L., Jiang, Peng, Johns, Kenneth Arthur, Johnson, Emily, Johnson, Marvin E., Jonckheere, Alan M., Jonsson, Per Martin, Joshi, Jyoti, Jung, Andreas Werner, Juste, Aurelio, Kajfasz, Eric, Karmanov, Dmitriy Y., Katsanos, Ioannis, Kaur, Manbir, Kehoe, Robert Leo Patrick, Kermiche, Smain, Khalatyan, Norayr, Khanov, Alexander, Kharchilava, Avto, Kharzheev, Yuri N., Kiselevich, Ivan Lvovich, Kohli, Jatinder M., Kozelov, Alexander V., Kraus, James Alexander, Kumar, Ashish, Kupco, Alexander, Kurca, Tibor, Kuzmin, Valentin Alexandrovich, Lammers, Sabine Wedam, Lebrun, Patrice, Lee, Hyeon-Seung, Lee, Seh-Wook, Lee, William M., Lei, Xiaowen, Lellouch, Jeremie, Li, Dikai, Li, Hengne, Li, Liang, Li, Qi-Zhong, Lim, Jeong Ku, Lincoln, Donald W., Linnemann, James Thomas, Lipaev, Vladimir V., Lipton, Ronald J., Liu, Huanzhao, Liu, Yanwen, Lobodenko, Alexandre, Lokajicek, Milos, Lopes Sa, Rafael, Luna-Garcia, Rene, Lyon, Adam Leonard, Maciel, Arthur K. A., Madar, Romain, Magana-Villalba, Ricardo, Malik, Sudhir, Malyshev, Vladimir L., Mansour, Jason, Martinez-Ortega, Jorge, Mccarthy, Robert L., Mcgivern, Carrie Lynne, Meijer, Melvin M., Melnitchouk, Alexander S., Menezes, Diego D., Mercadante, Pedro Galli, Merkin, Mikhail M., Meyer, Arnd, Meyer, Jorg Manfred, Miconi, Florian, Mondal, Naba K., Mulhearn, Michael James, Nagy, Elemer, Narain, Meenakshi, Nayyar, Ruchika, Neal, Homer A., Negret, Juan Pablo, Neustroev, Petr V., Nguyen, Huong Thi, Nunnemann, Thomas P., Hernandez Orduna, Jose Jesus, Osman, Nicolas Ahmed, Pal, Arnab, Parashar, Neeti, Parihar, Vivek, Park, Sung Keun, Partridge, Richard A., Parua, Nirmalya, Patwa, Abid, Penning, Bjoern, Perfilov, Maxim Anatolyevich, Peters, Reinhild Yvonne Fatima, Petridis, Konstantinos, Petrillo, Gianluca, Petroff, Pierre, Pleier, Marc-Andre, Podstavkov, Vladimir M., Popov, Alexey V., Prewitt, Michelle, Price, Darren, Prokopenko, Nikolay N., Qian, Jianming, Quadt, Arnulf, Quinn, Gene Breese, Ratoff, Peter N., Razumov, Ivan A., Ripp-Baudot, Isabelle, Rizatdinova, Flera, Rominsky, Mandy Kathleen, Ross, Anthony, Royon, Christophe, Rubinov, Paul Michael, Ruchti, Randal C., Sajot, Gerard, Sanchez-Hernandez, Alberto, Sanders, Michiel P., Santos, Angelo Souza, Savage, David G., Savitskyi, Mykola, Sawyer, H. Lee, Scanlon, Timothy P., Schamberger, R. Dean, Scheglov, Yury A., Schellman, Heidi M., Schott, Matthias, Schwanenberger, Christian, Schwienhorst, Reinhard H., Sekaric, Jadranka, Severini, Horst, Shabalina, Elizaveta K., Shary, Viacheslav V., Shaw, Savanna, Shchukin, Andrey A., Shkola, Oleg, Simak, Vladislav J., Skubic, Patrick Louis, Slattery, Paul F., Snow, Gregory R., Snow, Joel Mark, Snyder, Scott Stuart, Soldner-Rembold, Stefan, Sonnenschein, Lars, Soustruznik, Karel, Stark, Jan, Stefaniuk, Nazar, Stoyanova, Dina A., Strauss, Michael G., Suter, Louise, Svoisky, Peter V., Titov, Maxim, Tokmenin, Valeriy V., Tsai, Yun-Tse, Tsybychev, Dmitri, Tuchming, Boris, Tully, Christopher George T., Uvarov, Lev, Uvarov, Sergey L., Uzunyan, Sergey A., Kooten, Richard J., Leeuwen, Willem M., Varelas, Nikos, Varnes, Erich W., Vasilyev, Igor A., Verkheev, Alexander Yurievich, Vertogradov, Leonid S., Verzocchi, Marco, Vesterinen, Mika, Vilanova, Didier, Vokac, Petr, Wahl, Horst D., Chen Wang, Wang, Michael H. L. S., Warchol, Jadwiga, Watts, Gordon Thomas, Wayne, Mitchell R., Weichert, Jonas, Welty-Rieger, Leah Christine, Williams, Mark Richard James, Wilson, Graham Wallace, Wobisch, Markus, Wood, Darien Robert, Wyatt, Terence R., Xie, Yunhe, Yamada, Ryuji, Yang, Siqi, Yasuda, Takahiro, Yatsunenko, Yuriy A., Ye, Wanyu, Ye, Zhenyu, Yin, Hang, Yip, Kin, Youn, Sungwoo, Yu, Jiaming, Zennamo, Joseph, Zhao, Tianqi Gilbert, Zhou, Bing, Zhu, Junjie, Zielinski, Marek, Zieminska, Daria, Zivkovic, Lidija, Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Louis Pasteur - Strasbourg I, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), D0, HEP, INSPIRE, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Université Louis Pasteur - Strasbourg 1 (ULP), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: 1960 GeV-cms, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], hep-ex, pentaquark: hadroproduction, pentaquark: charm, pentaquark: mass, FOS: Physical sciences, resonance: exotic, Breit-Wigner, High Energy Physics - Experiment, anti-p p: colliding beams, mass spectrum: (J/psi(3100) p), High Energy Physics - Experiment (hep-ex), pentaquark: width, mass: width, DZERO, anti-p p: scattering, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], structure, Batavia TEVATRON Coll, yield: ratio, enhancement, Particle Physics - Experiment, inclusive production, experimental results
Abstract: We present a study of the inclusive production in $p \overline p $ collisions of the pentaquark states $P_c(4440)$ and $P_c(4457)$ with the decay to the $J/\psi p$ final state previously observed by the LHCb experiment. Using a sample of candidates originating from decays of $b$-flavored hadrons, we find an enhancement in the $J/\psi p$ invariant mass distribution consistent with a sum of $P_c(4440)$ and $P_c(4457)$. The significance, with the input parameters set to the LHCb values, is $3.0\sigma$. This is the first confirmatory evidence for these pentaquark states. We measure the ratio $N_{\rm prompt}/N_{\rm nonprompt}=0.05 \pm 0.39$ and set an upper limit of 0.8 at the 95\% credibility level. The ratio of the yield of the $P_c(4312)$ to the sum of $P_c(4440)$ and $P_c(4457)$ is less than 0.6 at the 95\% credibility level. The study is based on $10.4~\rm{fb^{-1}}$ of data collected by the D0 experiment at the Fermilab Tevatron collider., Comment: 7 pages, 3 figures
Published: 2019

5. Properties of $Z_c^{\pm}(3900)$ Produced in $p \bar p$ Collision

Author: Abazov, Victor Mukhamedovich, Abbott, Braden Keim, Atkins, Scott, Edmunds, Daniel L., Ellison, John A., Elvira, V. Daniel, Enari, Yuji, Evans, Harold G., Evdokimov, Anatoly V., Evdokimov, Valeri N., Faure, Alexandre, Feng, Lei, Ferbel, Thomas, Augsten, Kamil, Fiedler, Frank, Filthaut, Frank, Fisher, Wade Cameron, Fisk, H. Eugene, Fortner, Michael R., Fox, Harald, Franc, Jiri, Fuess, Stuart C., Garbincius, Peter H., Garcia-Bellido, Aran, Aushev, Volodymyr, Garcia-Gonzalez, Jose Andres, Gavrilov, Vladimir B., Geng, Weigang, Gerber, Cecilia Elena, Gershtein, Yuri S., Ginther, George E., Gogota, Olga, Golovanov, Georgy Anatolievich, Grannis, Paul D., Greder, Sebastien, Aushev, Yegor, Greenlee, Herbert B., Grenier, Gerald Jean, Gris, Phillipe Luc, Grivaz, Jean-Francois, Grohsjean, Alexander, Gruenendahl, Stefan, Gruenewald, Martin Werner, Guillemin, Thibault, Gutierrez, Gaston R., Gutierrez, Phillip, Avila, Carlos A., Haley, Joseph Glenn Biddle, Han, Liang, Harder, Kristian, Harel, Amnon, Hauptman, John Michael, Hays, Jonathan M., Head, Tim, Hebbeker, Thomas, Hedin, David R., Hegab, Hatim, Badaud, Frederique, Heinson, Ann, Heintz, Ulrich, Hensel, Carsten, Heredia-de La Cruz, Ivan, Herner, Kenneth Richard, Hesketh, Gavin G., Hildreth, Michael D., Hirosky, Robert James, Hoang, Trang, Hobbs, John D., Bagby, Linda F., Hoeneisen, Bruce, Hogan, Julie, Hohlfeld, Mark, Holzbauer, Jenny Lyn, Howley, Ian James, Hubacek, Zdenek, Hynek, Vlastislav, Iashvili, Ia, Ilchenko, Yuriy, Illingworth, Robert A., Baldin, Boris, Ito, Albert S., Jabeen, Shabnam, Jaffre, Michel J., Jayasinghe, Ayesh, Jeong, Min-Soo, Jesik, Richard L., Jiang, Peng, Johns, Kenneth Arthur, Johnson, Emily, Johnson, Marvin E., Bandurin, Dmitry V., Jonckheere, Alan M., Jonsson, Per Martin, Joshi, Jyoti, Jung, Andreas Werner, Juste, Aurelio, Kajfasz, Eric, Karmanov, Dmitriy Y., Katsanos, Ioannis, Kaur, Manbir, Kehoe, Robert Leo Patrick, Banerjee, Sunanda, Kermiche, Smain, Khalatyan, Norayr, Khanov, Alexander, Kharchilava, Avto, Kharzheev, Yuri N., Kiselevich, Ivan Lvovich, Kohli, Jatinder M., Kozelov, Alexander V., Kraus, James Alexander, Kumar, Ashish, Acharya, Bannanje Sripath, Barberis, Emanuela, Kupco, Alexander, Kurca, Tibor, Kuzmin, Valentin Alexandrovich, Lammers, Sabine Wedam, Lebrun, Patrice, Lee, Hyeon-Seung, Lee, Seh-Wook, Lee, William M., Lei, Xiaowen, Lellouch, Jeremie, Baringer, Philip S., Li, Dikai, Li, Hengne, Li, Liang, Li, Qi-Zhong, Lim, Jeong Ku, Lincoln, Donald W., Linnemann, James Thomas, Lipaev, Vladimir V., Lipton, Ronald J., Liu, Huanzhao, Bartlett, J. Frederick, Liu, Yanwen, Lobodenko, Alexandre, Lokajicek, Milos, Lopes De Sá, Rafael, Luna-Garcia, Rene, Lyon, Adam Leonard, Maciel, Arthur K. A., Madar, Romain, Magana-Villalba, Ricardo, Malik, Sudhir, Bassler, Ursula Rita, Malyshev, Vladimir L., Mansour, Jason, Martínez-Ortega, Jorge, McCarthy, Robert L., Mcgivern, Carrie Lynne, Meijer, Melvin M., Melnitchouk, Alexander S., Menezes, Diego D., Mercadante, Pedro Galli, Merkin, Mikhail M., Bazterra, Victor, Meyer, Arnd, Meyer, Jorg Manfred, Miconi, Florian, Mondal, Naba K., Mulhearn, Michael James, Nagy, Elemer, Narain, Meenakshi, Nayyar, Ruchika, Neal, Homer A., Negret, Juan Pablo, Bean, Alice L., Neustroev, Petr V., Nguyen, Huong Thi, Nunnemann, Thomas P., Hernandez Orduna, Jose de Jesus, Osman, Nicolas Ahmed, Pal, Arnab, Parashar, Neeti, Parihar, Vivek, Park, Sung Keun, Partridge, Richard A., Begalli, Marcia, Parua, Nirmalya, Patwa, Abid, Penning, Bjoern, Perfilov, Maxim Anatolyevich, Peters, Reinhild Yvonne Fatima, Petridis, Konstantinos, Petrillo, Gianluca, Petroff, Pierre, Pleier, Marc-Andre, Podstavkov, Vladimir M., Bellantoni, Leo, Popov, Alexey V., Prewitt, Michelle, Price, Darren, Prokopenko, Nikolay N., Qian, Jianming, Quadt, Arnulf, Quinn, Gene Breese, Ratoff, Peter N., Razumov, Ivan A., Ripp-Baudot, Isabelle, Beri, Suman B., Rizatdinova, Flera, Rominsky, Mandy Kathleen, Ross, Anthony, Royon, Christophe, Rubinov, Paul Michael, Ruchti, Randal C., Sajot, Gerard, Sánchez Hernández, Alberto, Sanders, Michiel P., Santos, Angelo Souza, Bernardi, Gregorio, Savage, David G., Savitskyi, Mykola, Sawyer, H. Lee, Scanlon, Timothy P., Schamberger, R. Dean, Scheglov, Yury A., Schellman, Heidi M., Schott, Matthias, Schwanenberger, Christian, Schwienhorst, Reinhard H., Adams, Mark Raymond, Bernhard, Ralf Patrick, Sekaric, Jadranka, Severini, Horst, Shabalina, Elizaveta K., Shary, Viacheslav V., Shaw, Savanna, Shchukin, Andrey A., Shkola, Oleg, Simak, Vladislav J., Skubic, Patrick Louis, Slattery, Paul F., Bertram, Iain A., Snow, Gregory R., Snow, Joel Mark, Snyder, Scott Stuart, Söldner-Rembold, Stefan, Sonnenschein, Lars, Soustruznik, Karel, Stark, Jan, Stefaniuk, Nazar, Stoyanova, Dina A., Strauss, Michael G., Besancon, Marc, Suter, Louise, Svoisky, Peter V., Titov, Maxim, Tokmenin, Valeriy V., Tsai, Yun-Tse, Tsybychev, Dmitri, Tuchming, Boris, Tully, Christopher George T., Uvarov, Lev, Uvarov, Sergey L., Beuselinck, Raymond, Uzunyan, Sergey A., Van Kooten, Richard J., van Leeuwen, Willem M., Varelas, Nikos, Varnes, Erich W., Vasilyev, Igor A., Verkheev, Alexander Yurievich, Vertogradov, Leonid S., Verzocchi, Marco, Vesterinen, Mika, Bhat, Pushpalatha C., Vilanova, Didier, Vokac, Petr, Wahl, Horst D., Wang, Michael H. L. S., Warchol, Jadwiga, Watts, Gordon Thomas, Wayne, Mitchell R., Weichert, Jonas, Welty-Rieger, Leah Christine, Williams, Mark Richard James, Bhatia, Sudeep, Wilson, Graham Wallace, Wobisch, Markus, Wood, Darien Robert, Wyatt, Terence R., Xie, Yunhe, Yamada, Ryuji, Yang, Siqi, Yasuda, Takahiro, Yatsunenko, Yuriy A., Ye, Wanyu, Bhatnagar, Vipin, Ye, Zhenyu, Yin, Hang, Yip, Kin, Youn, Sungwoo, Yu, Jiaming, Zennamo, Joseph, Zhao, Tianqi Gilbert, Zhou, Bing, Zhu, Junjie, Zielinski, Marek, Blazey, Gerald Charles, Zieminska, Daria, Zivkovic, Lidija, D0 Collaboration, Blessing, Susan K., Bloom, Kenneth A., Adams, Todd, Boehnlein, Amber S., Boline, Daniel Dooley, Boos, Edward E., Borissov, Guennadi, Borysova, Maryna, Brandt, Andrew, Brandt, Oleg, Brochmann, Michelle, Brock, Raymond L., Bross, Alan D., Agnew, James P., Brown, Duncan Paul, Bu, Xue-Bing, Buehler, Marc, Buescher, Volker, Bunichev, Viacheslav Yevgenyevich, Burdin, Sergey, Buszello, Claus Peter, Camacho-Perez, Enrique, Casey, Brendan Cameron Kieran, Castilla-Valdez, Heriberto, Alexeev, Guennadi D., Caughron, Seth Aaron, Chakrabarti, Subhendu, Chan, Kwok Ming Leo, Chandra, Avdhesh, Chapon, Emilien, Chen, Guo, Cho, Sung-Woong, Choi, Suyong, Choudhary, Brajesh C., Cihangir, Selcuk, Alkhazov, Georgiy D., Claes, Daniel R., Clutter, Justace Randall, Cooke, Michael P., Cooper, William Edward, Corcoran, Marjorie D., Couderc, Fabrice, Cousinou, Marie-Claude, Cuth, Jakub, Cutts, David, Das, Amitabha, Alton, Andrew K., Davies, Gavin John, de Jong, Sijbrand J., De La Cruz-Burelo, Eduard, Deliot, Frederic, Demina, Regina, Denisov, Dmitri S., Denisov, Sergei P., Desai, Satish Vijay, Deterre, Cecile, DeVaughan, Kayle Otis, Askew, Andrew Warren, Diehl, H. Thomas, Diesburg, Michael, Ding, Pengfei, Dominguez, D. Aaron M., Drutskoy, Alexey, Dubey, Abhinav Kumar, Dudko, Lev V., Duperrin, Arnaud, Dutt, Suneel, Eads, Michael T., Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), D0, Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département de Physique des Particules (ex SPP) (DPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), and Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])
Subjects: mass: measured, +J%2Fpsi%283100%29+pi%22">Z/c(3900) --> J/psi(3100) pi, M210M, FOS: Physical sciences, measured [width], M210W, hadronic decay [Y(4260)], (J/psi(3100) pi-) [mass spectrum], M210:Desig=1, particle: exotic, High Energy Physics - Experiment, width [mass], anti-p p: colliding beams, High Energy Physics - Experiment (hep-ex), (J/psi(3100) pi+) [mass spectrum], mass: width, mass spectrum: (J/psi(3100) pi-), DZERO, +Z%2Fc%283900%29+pi%22">Y(4260) --> Z/c(3900) pi, anti-p p: scattering, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], ddc:530, Batavia TEVATRON Coll, Nuclear Experiment, weak interaction [decay], Z/c(3900): hadronic decay, scattering [anti-p p], measured [mass], 1960 GeV-cms, Y(4260): hadronic decay, hep-ex, M210.1, exotic [particle], mass spectrum: (J/psi(3100) pi+), semi-inclusive reaction, direct production, High Energy Physics::Experiment, decay: weak interaction, width: measured, Particle Physics - Experiment, hadronic decay [Z/c(3900)], colliding beams [anti-p p], experimental results
Abstract: We study the production of the exotic charged charmonium-like state $Z_c^{\pm}(3900)$ in $p \bar p$ collisions through the sequential process $\psi(4260) \rightarrow Z_c^{\pm}(3900) \pi^{\mp}$, $Z_c^{\pm}(3900) \rightarrow J/\psi \pi^{\pm}$. Using the subsample of candidates originating from semi-inclusive weak decays of $b$-flavored hadrons, we measure the invariant mass and natural width to be $M=3902.6^{+5.2}_{-5.0}{\rm \thinspace (stat)}^{+3.3}_{-1.4}{\rm \thinspace (syst)}$ MeV and $\Gamma=32 ^{+28}_{-21}{\rm \thinspace (stat)} ^{+26}_{-7}{\rm \thinspace (syst)}$ MeV, respectively. We search for prompt production of the $Z_c^{\pm}(3900)$ through the same sequential process. No significant signal is observed, and we set an upper limit of 0.66 at the 95\% credibility level on the ratio of prompt production to the production via $b$-hadron decays. The study is based on $10.4~\rm{fb^{-1}}$ of $p \overline p $ collision data collected by the D0 experiment at the Fermilab Tevatron collider., Comment: 10 pages, 5 figures. Accepted by Phys. Rev. D
Published: 2019
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6. Core or cusps:the central dark matter profile of a redshift one strong lensing cluster with a bright central image at Redshift 1

Author: Collett, Thomas E., Buckley-Geer, Elizabeth J., Lin, Huan, Bacon, David, Nichol, Robert C., Nord, Brian, Morice-Atkinson, Xan, Amara, Adam, Birrer, Simon, Kuropatkin, Nikolay, More, Anupreeta, Papovich, Casey, Romer, A. Kathy, Tessore, Nicolas, Abbott, Tim M. C., Allam, Sahar S., Annis, James, Benoit-Lévy, Aurélien, Brooks, David, Burke, David L., Kind, Matias Carrasco, Castander, Francisco Javier, D'Andrea, Chris B., Costa, Luiz A. N. da, Desai, Shantanu, Diehl, H. Thomas, Doel, Peter, Eifler, Tim F., Flaugher, Brenna, Frieman, Josh, Gerdes, David W., Goldstein, Daniel A., Gruen, Daniel, Gschwend, Julia, Gutierrez, Gaston R., James, David J., Kuehn, Kyler, Kuhlmann, Steve, Lahav, Ofer, Li, Ting S., Lima, Marcos, Maia, Marcio Antonio Geimba, March, Marisa C., Marshall, Jennifer L., Martini, Paul, Melchior, Peter, Miquel, Ramon, Plazas, Andrés A., Rykoff, Eli S., Sanchez, Eusebio, Scarpine, Vic, Schindler, Rafe, Schubnell, Michael, Sevilla-Noarbe, Ignacio, Smith, Mathew, Sobreira, Flavia, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Tucker, Douglas L., and Walker, Alistair R.
Subjects: Cosmology and Gravitation, astro-ph.GA, astro-ph.CO, RCUK, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics, STFC
Abstract: We report on SPT-CLJ2011-5228, a giant system of arcs created by a cluster at z = 1.06. The arc system is notable for the presence of a bright central image. The source is a Lyman break galaxy at z s = 2.39 and the mass enclosed within the Einstein ring of radius 14 arcsec is ∼ 1014.2 MΘ. We perform a full reconstruction of the light profile of the lensed images to precisely infer the parameters of the mass distribution. The brightness of the central image demands that the central total density profile of the lens be shallow. By fitting the dark matter as a generalized Navarro–Frenk–White profile—with a free parameter for the inner density slope—we find that the break radius is 270∨{-76}^{+48} kpc, and that the inner density falls with radius to the power −0.38 ± 0.04 at 68% confidence. Such a shallow profile is in strong tension with our understanding of relaxed cold dark matter halos; dark matter-only simulations predict that the inner density should fall as r-1. The tension can be alleviated if this cluster is in fact a merger; a two-halo model can also reconstruct the data, with both clumps (density varying as r-0.8 and r-1.0) much more consistent with predictions from dark matter-only simulations. At the resolution of our Dark Energy Survey imaging, we are unable to choose between these two models, but we make predictions for forthcoming Hubble Space Telescope imaging that will decisively distinguish between them.
Published: 2017
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7. Dust Reverberation Mapping in Distant Quasars from Optical and Mid-infrared Imaging Surveys.

Author: Yang, Qian, Shen, Yue, Liu, Xin, Aguena, Michel, Annis, James, Avila, Santiago, Banerji, Manda, Bertin, Emmanuel, Brooks, David, Burke, David, Rosell, Aurelio Carnero, Kind, Matias Carrasco, da Costa, Luiz, De Vicente, Juan, Desai, Shantanu, Diehl, H. Thomas, Doel, Peter, Flaugher, Brenna, Fosalba, Pablo, and Frieman, Josh
Subjects: QUASARS, ACTIVE galactic nuclei, OPTICAL images, DUST, DISKS (Astrophysics), ACCRETION disks
Abstract: The size of the dust torus in active galactic nuclei (AGNs) and their high-luminosity counterparts, quasars, can be inferred from the time delay between UV/optical accretion disk continuum variability and the response in the mid-infrared (MIR) torus emission. This dust reverberation mapping (RM) technique has been successfully applied to ∼70 z ≲ 0.3 AGNs and quasars. Here we present first results of our dust RM program for distant quasars covered in the Sloan Digital Sky Survey Stripe 82 region combining ∼20 yr ground-based optical light curves with 10 yr MIR light curves from the WISE satellite. We measure a high-fidelity lag between W1 band (3.4 μm) and g band for 587 quasars over 0.3 ≲ z ≲ 2 () and two orders of magnitude in quasar luminosity. They tightly follow (intrinsic scatter ∼0.17 dex in lag) the IR lag–luminosity relation observed for z < 0.3 AGNs, revealing a remarkable size–luminosity relation for the dust torus over more than four decades in AGN luminosity, with little dependence on additional quasar properties such as Eddington ratio and variability amplitude. This study motivates further investigations in the utility of dust RM for cosmology and strongly endorses a compelling science case for the combined 10 yr Vera C. Rubin Observatory Legacy Survey of Space and Time (optical) and 5 yr Nancy Grace Roman Space Telescope 2 μm light curves in a deep survey for low-redshift AGN dust RM with much lower luminosities and shorter, measurable IR lags. The compiled optical and MIR light curves for 7384 quasars in our parent sample are made public with this work. [ABSTRACT FROM AUTHOR]
Published: 2020
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8. The DES Bright Arcs Survey : hundreds of candidate strongly lensed galaxy systems from the Dark Energy Survey Science Verification and Year 1 observations

Author: Diehl, H. Thomas, Santiago, Basilio Xavier, Walker, Alistair, and DES Collaboration
Subjects: high-redshift [Galaxies], Fotometria astronômica, Lentes gravitacionais, Matéria escura, Galáxias, strong [Gravitational lensing]
Abstract: We report the results of searches for strong gravitational lens systems in the Dark Energy Survey (DES) Science Verification and Year 1 observations. The Science Verification data span approximately 250 sq. deg. with a median i-band limiting magnitude for extended objects (10σ) of 23.0. The Year 1 data span approximately 2000 sq. deg. and have an i-band limiting magnitude for extended objects (10σ) of 22.9. As these data sets are both wide and deep, they are particularly useful for identifying strong gravitational lens candidates. Potential strong gravitational lens candidate systems were initially identified based on a color and magnitude selection in the DES object catalogs or because the system is at the location of a previously identified galaxy cluster. Cutout images of potential candidates were then visually scanned using an object viewer and numerically ranked according to whether or not we judged them to be likely strong gravitational lens systems. Having scanned nearly 400,000 cutouts, we present 374 candidate strong lens systems, of which 348 are identified for the first time. We provide the R.A. and decl., the magnitudes and photometric properties of the lens and source objects, and the distance (radius) of the source(s) from the lens center for each system.
Published: 2017

9. Galaxy populations in massive galaxy clusters to z = 1.1 : colour distribution, concentration, halo occupation number and red sequence fraction

Author: Hennig, C., Mohr, Joseph J., Zenteno, Alfredo, Desai, S., Dietrich, Jörg P., Bocquet, Sebastian, Strazzullo, Veronica, Saro, Alexandro, Abbott, Timothy M. C., Abdalla, Filipe B., Bayliss, Matthew B., Benoit-Lévy, Aurélien, Bernstein, Gary M., Bertin, Emmanuel, Brooks, D., Capasso, Raffaella, Capozzi, Diego, Carnero Rosell, Aurelio, Carrasco Kind, Matías, Carretero Palacios, Jorge, Chiu, I. Non Tim, D'Andrea, Christopher B., Costa, Luiz N. da, Diehl, H. Thomas, Doel, Peter, Eifler, Tim, Evrard, August E., Fausti Neto, Angelo, Fosalba Vela, Pablo, Frieman, Joshua A., Gangkofner, C., Gonzalez, Anthony, Gruen, Daniel, Gruendl, Robert A., Gupta, Nayantara, Gutierrez, Gaston R., Honscheid, K., Hlavacek-Larrondo, Julie, James, David J., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, March, Marisa Cristina, Marshall, Jennifer L., Martini, Paul, McDonald, Michael Kenneth, Melchior, Peter M., Miller, Christopher J., Miquel, Ramon, Neilsen, Eric H., Nord, Brian Dennis, Ogando, Ricardo L.C., Plazas Malagón, Andrés Alejandro, Reichardt, Christian L., Romer, Anita K., Rozo, Eduardo, Rykoff, Eli, Sanchez-Alvaro, Eusebio, Santiago, Basilio Xavier, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Stalder, Brian, Stanford, Spencer Adam, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Thomas, D., Vikram, Vinu, Walker, Alistair, and Zhang, Yuanyuan
Subjects: Galáxias ativas, Galaxies formation, Populacoes estelares, Galaxies evolution, Galaxies clusters individual, Galaxies mass function, Galaxies luminosity function, Aglomerados globulares, Galaxies clusters general
Abstract: We study the galaxy populations in 74 Sunyaev–Zeldovich effect selected clusters from the South Pole Telescope survey, which have been imaged in the science verification phase of the Dark Energy Survey. The sample extends up to z ∼ 1.1 with 4 × 1014M ≤ M200 ≤ 3 × 1015M . Using the band containing the 4000 Å break and its redward neighbour, we study the colour–magnitude distributions of cluster galaxies to ∼m∗ + 2, finding that: (1)The intrinsic rest frame g − r colour width of the red sequence (RS) population is ∼0.03 out to z ∼ 0.85 with a preference for an increase to ∼0.07 at z = 1, and (2) the prominence of the RS declines beyond z ∼ 0.6. The spatial distribution of cluster galaxies is well described by the NFW profile out to 4R200 with a concentration of cg = 3.59+0.20 −0.18, 5.37+0.27 −0.24 and 1.38+0.21 −0.19 for the full, the RS and the blue non-RS populations, respectively, but with ∼40 per cent to 55 per cent cluster to cluster variation and no statistically significant redshift or mass trends. The number of galaxies within the virial region N200 exhibits a mass trend indicating that the number of galaxies per unit total mass is lower in the most massive clusters, and shows no significant redshift trend. The RS fraction within R200 is (68 ± 3) per cent at z = 0.46, varies from ∼55 per cent at z = 1 to ∼80 per cent at z = 0.1 and exhibits intrinsic variation among clusters of ∼14 per cent. We discuss a model that suggests that the observed redshift trend in RS fraction favours a transformation time-scale for infalling field galaxies to become RS galaxies of 2–3 Gyr.
Published: 2017

10. Farthest neighbor : the distant Milky Way satellite Eridanus II

Author: Li, T. S., Simon, Josh D., Drlica-Wagner, Alex, Bechtol, Keith, Wang, M., García-Bellido, Juan, Frieman, Joshua A., Marshall, Jennifer L., James, David J., Strigari, Louis E., Pace, Andrew B., Balbinot, Eduardo, Zhang, Yuanyuan, Abbott, Timothy M. C., Allam, Sahar S., Benoit-Lévy, Aurélien, Bernstein, Gary M., Bertin, Emmanuel, Brooks, D., Burke, David Lyle, Carnero Rosell, Aurelio, Carrasco Kind, Matías, Carretero Palacios, Jorge, Cunha, Carlos Eduardo, D'Andrea, Christopher B., Costa, Luiz N. da, DePoy, Darren L., Desai, S., Diehl, H. Thomas, Eifler, Tim, Flaugher, Brenna, Goldstein, Daniel Abraham, Gruen, Daniel, Gruendl, Robert A., Gschwend, Julia de Figueiredo, Gutierrez, Gaston R., Krause, Elisabeth, Kuehn, Kyler, Lin, H., Maia, Marcio Antonio Geimba, March, Marisa Cristina, Menanteau, Felipe, Miquel, Ramon, Plazas Malagón, Andrés Alejandro, Romer, Anita K., Sanchez-Alvaro, Eusebio, Santiago, Basilio Xavier, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Sobreira, Flávia, Suchyta, Eric, Tarle, Gregory, Thomas, D., Tucker, Douglas L., Walker, Alistair, Wechsler, Risa H., Wester, William Carl, Yanny, Brian, and DES Collaboration
Subjects: dwarf [Galaxies], Populacoes estelares, Via láctea, abundances [Stars], Dark matter, Local group, Matéria escura, stellar content [Galaxies], individual (Eridanus II) [Galaxies], Composicao estelar, Metalicidade, Galáxias
Abstract: We present Magellan/IMACS spectroscopy of the recently discovered Milky Way satellite EridanusII (Eri II). We identify 28 member stars in EriII, from which we measure a systemic radial velocity of vhel = 75.6 1.3 (stat.) 2.0 (sys.) km s-1 and a velocity dispersion of - 6.9+0.9 1.2 km s-1. Assuming that EriII is a dispersion-supported system in dynamical equilibrium, we derive a mass within the half-light radius of - ´ 1.2+ 10 0.3 0.4 7 M, indicating a mass-tolight ratio of - 420+140 210 M/L and confirming that it is a dark matter-dominated dwarf galaxy. From the equivalent width measurements of the Ca triplet lines of 16 red giant member stars, we derive a mean metallicity of [Fe/ H]=−2.38±0.13 and a metallicity dispersion of s[ / ] = - 0.47+ Fe H 0.09 0.12. The velocity of EriII in the Galactic standard of rest frame is vGSR=−66.6 km s-1, indicating that either EriII is falling into the Milky Way potential for the first time or that it has passed the apocenter of its orbit on a subsequent passage. At a Galactocentric distance of 370 kpc, Eri II is one of the Milky Way’s most distant satellites known. Additionally, we show that the bright blue stars previously suggested to be a young stellar population are not associated with EriII. The lack of gas and recent star formation in EriII is surprising given its mass and distance from the Milky Way, and may place constraints on models of quenching in dwarf galaxies and on the distribution of hot gas in the Milky Way halo. Furthermore, the large velocity dispersion of Eri II can be combined with the existence of a central star cluster to constrain massive compact halo object dark matter with mass 10 M.
Published: 2017

11. Redshift distributions of galaxies in the Dark Energy Survey Science Verification shear catalogue and implications for weak lensing

Author: Bonnett, Christopher, Troxel, Michael, Hartley, William, Amara, Adam, Leistedt, Boris, Becker, Matthew R., Bernstein, Gary M., Bridle, Sarah Louise, Bruderer, Claudio, Busha, M. T., Carrasco Kind, Matías, Childress, Michael, Castander Serentill, Francisco Javier, Chang, Chihway, Crocce, Martin, Davis, Tamara M., Eifler, Tim, Frieman, Joshua A., Gangkofner, C., Gaztañaga, Enrique, Glazebrook, Karl, Gruen, Daniel, Kacprzak, Tomasz, King, Anthea L., Kwan, Juliana, Lahav, Ofer, Lewis, Geraint F., Lidman, Chris, Lin, H., MacCrann, Niall, Miquel, Ramon, O'Neill, C. R., Palmese, A., Peiris, Hiranya V., Refregier, Alexandre, Rozo, Eduardo, Rykoff, Eli, Sadeh, Iftach, Sánchez Alonso, Carles, Sheldon, Erin, Uddin, Syed, Wechsler, Risa H., Zuntz, J., Abbott, Timothy M. C., Abdalla, Filipe B., Allam, Sahar S., Armstrong, Robert, Banerji, M., Bauer, Anne Hollister, Benoit-Lévy, Aurélien, Bertin, Emmanuel, Brooks, D., Buckley-Geer, Elizabeth, Burke, David Lyle, Capozzi, Diego, Carnero Rosell, Aurelio, Carretero Palacios, Jorge, Cunha, Carlos Eduardo, D'Andrea, Christopher B., Costa, Luiz N. da, DePoy, Darren L., Desai, S., Diehl, H. Thomas, Dietrich, Jörg P., Doel, Peter, Fausti Neto, Angelo, Fernandez, Enrique, Flaugher, Brenna, Fosalba Vela, Pablo, Gerdes, David W., Gruendl, Robert A., Honscheid, K., Jain, Bhuvnesh, James, David J., Jarvis, Michael, Kim, A. G., Kuehn, Kyler, Kuropatkin, Nikolay P., Li, T. S., Lima, Marcos Vinicius Borges Teixeira, Maia, Marcio Antonio Geimba, March, Marisa Cristina, Marshall, Jennifer L., Martini, Paul, Melchior, Peter M., Miller, Christopher J., Neilsen, Eric H., Nichol, Robert C., Nord, Brian Dennis, Ogando, Ricardo L.C., Plazas Malagón, Andrés Alejandro, Reil, Kevin, Romer, Anita K., Roodman, Aaron, Sako, Masao, Sanchez-Alvaro, Eusebio, Santiago, Basilio Xavier, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Thaler, Jon J., Thomas, D., Vikram, Vinu, Walker, Alistair, and DES Collaboration
Subjects: Lentes gravitacionais, DATA RELEASE, SURVEY REQUIREMENTS, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, SHAPE MEASUREMENT, 01 natural sciences, Cosmology, Physics, Particles & Fields, PRECISION COSMOLOGY, LARGE-SCALE STRUCTURE, 0103 physical sciences, STAR-FORMING GALAXIES, PHOTO-Z PERFORMANCE, Deslocamento para o vermelho, Galáxias, PHOTOMETRIC REDSHIFTS, 010303 astronomy & astrophysics, Weak gravitational lensing, Astrophysics::Galaxy Astrophysics, QB, Photometric redshift, Physics, Science & Technology, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Sigma, VLT DEEP SURVEY, Redshift survey, Galaxy, Redshift, Fotometria astronômica, Physical Sciences, astro-ph.CO, Dark energy, NEURAL-NETWORKS
Abstract: We present photometric redshift estimates for galaxies used in the weak lensing analysis of the Dark Energy Survey Science Verification (DES SV) data. Four model-or machine learning-based photometric redshift methods-ANNZ2, BPZ calibrated against BCC-Ufig simulations, SKYNET, and TPZ-are analyzed. For training, calibration, and testing of these methods, we construct a catalogue of spectroscopically confirmed galaxies matched against DES SV data. The performance of the methods is evaluated against the matched spectroscopic catalogue, focusing on metrics relevant for weak lensing analyses, with additional validation against COSMOS photo-z's. From the galaxies in the DES SV shear catalogue, which have mean redshift 0.72 +/- 0.01 over the range 0.3 < z < 1.3, we construct three tomographic bins with means of z = {0.45;0.67;1.00}. These bins each have systematic uncertainties delta z
Published: 2016
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12. Measurement of spin correlation between top and antitop quarks produced in $p\bar{p}$ collisions at $\sqrt{s} = 1.96$ TeV

Author: D0 Collaboration, Abazov, Victor Mukhamedovich, Askew, Andrew Warren, Ellison, John A., Elvira, V. Daniel, Enari, Yuji, Evans, Harold G., Evdokimov, Anatoly V., Evdokimov, Valeri N., Faure, Alexandre, Feng, Lei, Ferbel, Thomas, Fiedler, Frank, Atkins, Scott, Filthaut, Frank, Fisher, Wade Cameron, Fisk, H. Eugene, Fortner, Michael R., Fox, Harald, Franc, Jiri, Fuess, Stuart C., Garbincius, Peter H., Garcia-Bellido, Aran, Garcia-González, J. A., Augsten, Kamil, Gavrilov, Vladimir B., Geng, Weigang, Gerber, Cecilia Elena, Gershtein, Yuri S., Ginther, George E., Gogota, Olga, Golovanov, Georgy Anatolievich, Grannis, Paul D., Greder, Sebastien, Greenlee, Herbert B., Aushev, Volodymyr, Grenier, Gerald Jean, Gris, Phillipe Luc, Grivaz, Jean-Francois, Grohsjean, Alexander, Gruenendahl, Stefan, Gruenewald, Martin Werner, Guillemin, Thibault, Gutierrez, Gaston R., Gutierrez, Phillip, Haley, Joseph Glenn Biddle, Aushev, Yegor, Han, Liang, Harder, Kristian, Harel, Amnon, Hauptman, John Michael, Hays, Jonathan M., Head, Tim, Hebbeker, Thomas, Hedin, David R., Hegab, Hatim, Heinson, Ann, Avila, Carlos A., Heintz, Ulrich, Hensel, Carsten, Heredia-de La Cruz, Ivan, Herner, Kenneth Richard, Hesketh, Gavin G., Hildreth, Michael D., Hirosky, Robert James, Hoang, Trang, Hobbs, John D., Hoeneisen, Bruce, Badaud, Frederique, Hogan, Julie, Hohlfeld, Mark, Holzbauer, Jenny Lyn, Howley, Ian James, Hubacek, Zdenek, Hynek, Vlastislav, Iashvili, Ia, Ilchenko, Yuriy, Illingworth, Robert A., Ito, Albert S., Bagby, Linda F., Jabeen, Shabnam, Jaffre, Michel J., Jayasinghe, Ayesh, Jeong, Min-Soo, Jesik, Richard L., Jiang, Peng, Johns, Kenneth Arthur, Johnson, Emily, Johnson, Marvin E., Jonckheere, Alan M., Baldin, Boris, Jonsson, Per Martin, Joshi, Jyoti, Jung, Andreas Werner, Juste, Aurelio, Kajfasz, Eric, Karacheban, Olena, Karmanov, Dmitriy Y., Katsanos, Ioannis, Kaur, Manbir, Kehoe, Robert Leo Patrick, Bandurin, Dmitry V., Kermiche, Smain, Khalatyan, Norayr, Khanov, Alexander, Kharchilava, Avto, Kharzheev, Yuri N., Kiselevich, Ivan Lvovich, Kohli, Jatinder M., Kozelov, Alexander V., Kraus, James Alexander, Kumar, Ashish, Abbott, Braden Keim, Banerjee, Sunanda, Kupco, Alexander, Kurca, Tibor, Kuzmin, Valentin Alexandrovich, Lammers, Sabine Wedam, Lebrun, Patrice, Lee, Hyeon-Seung, Lee, Seh-Wook, Lee, William M., Lei, Xiaowen, Lellouch, Jeremie, Barberis, Emanuela, Li, Dikai, Li, Hengne, Li, Liang, Li, Qi-Zhong, Lim, Jeong Ku, Lincoln, Donald W., Linnemann, James Thomas, Lipaev, Vladimir V., Lipton, Ronald J., Liu, Huanzhao, Baringer, Philip S., Liu, Yanwen, Lobodenko, Alexandre, Lokajicek, Milos, Lopes De Sá, Rafael, Luna-Garcia, R., Lyon, Adam Leonard, Maciel, Arthur K. A., Madar, Romain, Magana-Villalba, R., Malik, Sudhir, Bartlett, J. Frederick, Malyshev, Vladimir L., Mansour, Jason, Martínez-Ortega, J., McCarthy, Robert L., Mcgivern, Carrie Lynne, Meijer, Melvin M., Melnitchouk, Alexander S., Menezes, Diego D., Mercadante, Pedro Galli, Merkin, Mikhail M., Bassler, Ursula Rita, Meyer, Arnd, Meyer, Jorg Manfred, Miconi, Florian, Mondal, Naba K., Mulhearn, Michael James, Nagy, Elemer, Narain, Meenakshi, Nayyar, Ruchika, Neal, Homer A., Negret, Juan Pablo, Bazterra, Victor, Neustroev, Petr V., Nguyen, Huong Thi, Nunnemann, Thomas P., Hernandez Orduna, Jose de Jesus, Osman, Nicolas Ahmed, Osta, Jyotsna, Pal, Arnab, Parashar, Neeti, Parihar, Vivek, Park, Sung Keun, Bean, Alice L., Partridge, Richard A., Parua, Nirmalya, Patwa, Abid, Penning, Bjoern, Perfilov, Maxim Anatolyevich, Peters, Reinhild Yvonne Fatima, Petridis, Konstantinos, Petrillo, Gianluca, Petroff, Pierre, Pleier, Marc-Andre, Begalli, Marcia, Podstavkov, Vladimir M., Popov, Alexey V., Prewitt, Michelle, Price, Darren, Prokopenko, Nikolay N., Qian, Jianming, Quadt, Arnulf, Quinn, Gene Breese, Ratoff, Peter N., Razumov, Ivan A., Bellantoni, Leo, Ripp-Baudot, I., Rizatdinova, Flera, Rominsky, Mandy Kathleen, Ross, Anthony, Royon, Christophe, Rubinov, Paul Michael, Ruchti, Randal C., Sajot, Gerard, Sanchez-Hernandez, A., Sanders, Michiel P., Beri, Suman B., Santos, Angelo Souza, Savage, David G., Savitskyi, Mykola, Sawyer, H. Lee, Scanlon, Timothy P., Schamberger, R. Dean, Scheglov, Yury A., Schellman, Heidi M., Schott, Matthias, Schwanenberger, Christian, Acharya, Bannanje Sripath, Bernardi, Gregorio, Schwienhorst, Reinhard H., Sekaric, Jadranka, Severini, Horst, Shabalina, Elizaveta K., Shary, Viacheslav V., Shaw, Savanna, Shchukin, Andrey A., Simak, Vladislav J., Skubic, Patrick Louis, Slattery, Paul F., Bernhard, Ralf Patrick, Smirnov, Dmitri V., Snow, Gregory R., Snow, Joel Mark, Snyder, Scott Stuart, Söldner-Rembold, S., Sonnenschein, Lars, Soustruznik, Karel, Stark, Jan, Stefaniuk, Nazar, Stoyanova, Dina A., Bertram, Iain A., Strauss, Michael G., Suter, Louise, Svoisky, Peter V., Titov, Maxim, Tokmenin, Valeriy V., Tsai, Yun-Tse, Tsybychev, Dmitri, Tuchming, Boris, Tully, Christopher George T., Uvarov, Lev, Besancon, Marc, Uvarov, Sergey L., Uzunyan, Sergey A., Van Kooten, R. J., van Leeuwen, Willem M., Varelas, Nikos, Varnes, Erich W., Vasilyev, Igor A., Verkheev, Alexander Yurievich, Vertogradov, Leonid S., Verzocchi, Marco, Beuselinck, Raymond, Vesterinen, Mika, Vilanova, Didier, Vokac, Petr, Wahl, Horst D., Wang, Michael H. L. S., Warchol, Jadwiga, Watts, Gordon Thomas, Wayne, Mitchell R., Weichert, Jonas, Welty-Rieger, Leah Christine, Bhat, Pushpalatha C., Williams, Mark Richard James, Wilson, Graham Wallace, Wobisch, Markus, Wood, Darien Robert, Wyatt, Terence R., Xie, Yunhe, Yamada, Ryuji, Yang, Siqi, Yasuda, Takahiro, Yatsunenko, Yuriy A., Bhatia, Sudeep, Ye, Wanyu, Ye, Zhenyu, Yin, Hang, Yip, Kin, Youn, Sungwoo, Yu, Jiaming, Zennamo, Joseph, Zhao, Tianqi Gilbert, Zhou, Bing, Zhu, Junjie, Bhatnagar, Vipin, Zielinski, Marek, Zieminska, Daria, Zivkovic, Lidija, Blazey, Gerald Charles, Blessing, Susan K., Adams, Mark Raymond, Bloom, Kenneth A., Boehnlein, Amber S., Boline, Daniel Dooley, Boos, Edward E., Borissov, Guennadi, Borysova, Maryna, Brandt, Andrew, Brandt, Oleg, Brock, Raymond L., Bross, Alan D., Adams, Todd, Brown, Duncan Paul, Bu, Xue-Bing, Buehler, Marc, Buescher, Volker, Bunichev, Viacheslav Yevgenyevich, Burdin, Sergey, Buszello, Claus Peter, Camacho-Pérez, E., Casey, Brendan Cameron Kieran, Castilla-Valdez, Heriberto, Agnew, James P., Caughron, Seth Aaron, Chakrabarti, Subhendu, Chan, Kwok Ming Leo, Chandra, Avdhesh, Chapon, Emilien, Chen, Guo, Cho, Sung-Woong, Choi, Suyong, Choudhary, Brajesh C., Cihangir, Selcuk, Alexeev, Guennadi D., Claes, Daniel R., Clutter, Justace Randall, Cooke, Michael P., Cooper, William Edward, Corcoran, Marjorie D., Couderc, Fabrice, Cousinou, Marie-Claude, Cuth, Jakub, Cutts, David, Das, Amitabha, Alkhazov, Georgiy D., Davies, Gavin John, de Jong, Sijbrand J., De La Cruz-Burelo, Eduard, Deliot, Frederic, Demina, Regina, Denisov, Dmitri S., Denisov, Sergei P., Desai, Satish Vijay, Deterre, Cecile, DeVaughan, Kayle Otis, Alton, Andrew K., Diehl, H. Thomas, Diesburg, Michael, Ding, Pengfei, Dominguez, D. Aaron M., Dubey, Abhinav Kumar, Dudko, Lev V., Duperrin, Arnaud, Dutt, Suneel, Eads, Michael T., Edmunds, Daniel L., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), D0 Collaboration, Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: final state [jet], data analysis method, spin: correlation, ((n)jet dilepton) [final state], FOS: Physical sciences, final state: ((n)jet lepton), pair production [top], High Energy Physics - Experiment, anti-p p: colliding beams, top: spin, High Energy Physics - Experiment (hep-ex), correlation [spin], anti-p p: scattering, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], ddc:530, Batavia TEVATRON Coll, Nuclear Experiment, scattering [anti-p p], 1960 GeV-cms, final state: ((n)jet dilepton), High Energy Physics::Phenomenology, spin [top], High Energy Physics::Experiment, top: pair production, colliding beams [anti-p p], jet: final state, ((n)jet lepton) [final state], experimental results
Abstract: We present a measurement of the correlation between the spins of t and tbar quarks produced in proton-antiproton collisions at the Tevatron Collider at a center-of-mass energy of 1.96 TeV. We apply a matrix element technique to dilepton and single-lepton+jets final states in data accumulated with the D0 detector that correspond to an integrated luminosity of 9.7 fb$^{-1}$. The measured value of the correlation coefficient in the off-diagonal basis, $O_{off} = 0.89 \pm 0.22$ (stat + syst), is in agreement with the standard model prediction, and represents evidence for a top-antitop quark spin correlation difference from zero at a level of 4.2 standard deviations., Published version
Published: 2016
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13. The Phoenix stream : a cold stream in the southern hemisphere

Author: Balbinot, Eduardo, Yanny, Brian, Li, T. S., Santiago, Basilio Xavier, Marshall, Jennifer L., Finley, David A., Pieres, Adriano, Abbott, Timothy M. C., Abdalla, Filipe B., Allam, Sahar S., Benoit-Lévy, Aurélien, Bernstein, Gary M., Bertin, Emmanuel, Brooks, D., Burke, David Lyle, Carnero Rosell, Aurelio, Carrasco Kind, Matías, Carretero Palacios, Jorge, Cunha, Carlos Eduardo, Costa, Luiz N. da, DePoy, Darren L., Desai, S., Diehl, H. Thomas, Doel, Peter, Estrada, Juan, Flaugher, Brenna, Frieman, Joshua A., Gerdes, David W., Gruen, Daniel, Gruendl, Robert A., Honscheid, K., James, David J., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, March, Marisa Cristina, Martini, Paul, Miquel, Ramon, Nichol, Robert C., Ogando, Ricardo L.C., Romer, Anita K., Sanchez-Alvaro, Eusebio, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Tarle, Gregory, Thomas, D., Tucker, Douglas L., Walker, Alistair, and DES Collaboration
Subjects: Fotometria astronômica, Evolucao estelar, halo [Galaxy], Galaxia, structure [Galaxy]
Abstract: We report the discovery of a stellar stream in the Dark Energy Survey Year 1 (Y1A1) data. The discovery was made through simple color–magnitude filters and visual inspection of the Y1A1 data. We refer to this new object as the Phoenix stream, after its resident constellation. After subtraction of the background stellar population we detect a clear signal of a simple stellar population. By fitting the ridge line of the stream in color–magnitude space, we find that a stellar population with age τ=11.5±0.5 Gyr and [Fe/H]
Published: 2016

14. Digging deeper into the Southern skies : a compact Milky Way companion discovered in first-year Dark Energy Survey data

Author: Luque Canaza, Elmer Fidel, Queiroz, Anna Bárbara de Andrade, Santiago, Basilio Xavier, Pieres, Adriano, Balbinot, Eduardo, Bechtol, Keith, Drlica-Wagner, Alex, Fausti Neto, Angelo, Costa, Luiz N. da, Maia, Marcio Antonio Geimba, Yanny, Brian, Abbott, Timothy M. C., Allam, Sahar S., Benoit-Lévy, Aurélien, Bertin, Emmanuel, Brooks, D., Buckley-Geer, Elizabeth, Burke, David Lyle, Carnero Rosell, Aurelio, Carrasco Kind, Matías, Carretero Palacios, Jorge, Cunha, Carlos Eduardo, Desai, S., Diehl, H. Thomas, Dietrich, Jörg P., Eifler, Tim, Finley, David A., Flaugher, Brenna, Fosalba Vela, Pablo, Frieman, Joshua A., Gerdes, David W., Gruen, Daniel, Gutierrez, Gaston R., Honscheid, K., James, David J., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, Li, T. S., March, Marisa Cristina, Marshall, Jennifer L., Martini, Paul, Miquel, Ramon, Neilsen, Eric H., Nichol, Robert C., Nord, Brian Dennis, Ogando, Ricardo L.C., Plazas Malagón, Andrés Alejandro, Romer, Anita K., Roodman, Aaron, Sanchez-Alvaro, Eusebio, Scarpine, Victor Emanuel, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Thaler, Jon J., Tucker, Douglas L., Walker, Alistair, Zhang, Y., and DES Collaboration
Subjects: Mapeamentos astronômicos, dwarf [Galaxies], Energia escura, individual (DES 1) [Globular clusters], general [Globular clusters], Aglomerados globulares, Galáxias
Abstract: We use the first-year Dark Energy Survey (DES) data down to previously unprobed photometric depths to search for stellar systems in the Galactic halo, therefore complementing the previous analysis of the same data carried out by our group earlier this year. Our search is based on a matched filter algorithm that produces stellar density maps consistent with stellar population models of various ages, metallicities, and distances over the survey area. The most conspicuous density peaks in these maps have been identified automatically and ranked according to their significance and recurrence for different input models. We report the discovery of one additional stellar system besides those previously found by several authors using the same first-year DES data. The object is compact, and consistent with being dominated by an old and metal-poor population. DES 1 is found at high significance and appears in the DES images as a compact concentration of faint blue point sources. Assuming different spatial profile parameterizations, the best-fitting heliocentric distance and total absolute magnitude in the range of 77.6–87.1 kpc and −3.00 MV −2.21, respectively. The half-light radius of this object, rh ∼ 10 pc and total luminosity are consistent with it being a low-mass halo cluster. It is also found to have a very elongated shape ( ∼ 0.57). In addition, our deeper probe of DES first-year data confirms the recently reported satellite galaxy candidate Horologium II as a significant stellar overdensity. We also infer its structural properties and compare them to those reported in the literature.
Published: 2016

15. redMaGiC : selecting luminous red galaxies from the DES Science Verification data

Author: Rozo, Eduardo, Rykoff, Eli, Abate, Alexandra, Bonnet, Christopher Clive, Crocce, Martin, Davis, Christopher P., Hoyle, Ben, Leistedt, Boris, Peiris, Hiranya V., Wechsler, Risa H., Abbott, Timothy M. C., Abdalla, Filipe B., Banerji, M., Bauer, Anne Hollister, Benoit-Lévy, Aurélien, Bernstein, Gary M., Bertin, Emmanuel, Brooks, D., Buckley-Geer, Elizabeth, Burke, David Lyle, Capozzi, Diego, Carnero Rosell, Aurelio, Carollo, Daniela, Carrasco Kind, Matías, Carretero Palacios, Jorge, Castander Serentill, Francisco Javier, Childress, Michael, Cunha, Carlos Eduardo, D'Andrea, Christopher B., Davis, Tamara M., DePoy, Darren L., Desai, S., Diehl, H. Thomas, Dietrich, Jörg P., Doel, Peter, Eifler, Tim, Evrard, August E., Fausti Neto, Angelo, Flaugher, Brenna, Fosalba Vela, Pablo, Frieman, Joshua A., Gaztañaga, Enrique, Gerdes, David W., Glazebrook, Karl, Gruen, Daniel, Gruendl, Robert A., Honscheid, K., James, David J., Jarvis, Michael, Kim, A. G., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, Lewis, Geraint F., Lidman, Chris, Lima, Marcos Vinicius Borges Teixeira, Maia, Marcio Antonio Geimba, March, Marisa Cristina, Martini, Paul, Melchior, Peter M., Miller, Christopher J., Miquel, Ramon, Mohr, Joseph J., Nichol, Robert C., Nord, Brian Dennis, O'Neill, C. R., Ogando, Ricardo L.C., Plazas Malagón, Andrés Alejandro, Romer, Anita K., Roodman, Aaron, Sako, Masao, Sanchez-Alvaro, Eusebio, Santiago, Basilio Xavier, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Swanson, Molly E. C., Thaler, Jon J., Thomas, D., Uddin, Syed, Vikram, Vinu, Walker, Alistair, Wester, William Carl, Zhang, Yuanyuan, and Costa, Luiz N. da
Subjects: statistical [Methods], Fotometria astronômica, photometric [Techniques], general [Galaxies], Deslocamento para o vermelho, Galáxias
Abstract: We introduce redMaGiC, an automated algorithm for selecting luminous red galaxies (LRGs). The algorithm was specifically developed to minimize photometric redshift uncertainties in photometric large-scale structure studies. redMaGiC achieves this by self-training the colour cuts necessary to produce a luminosity-thresholded LRG sample of constant comoving density. We demonstrate that redMaGiC photo-zs are very nearly as accurate as the best machine learning-based methods, yet they require minimal spectroscopic training, do not suffer from extrapolation biases, and are very nearly Gaussian. We apply our algorithm to Dark Energy Survey (DES) Science Verification (SV) data to produce a redMaGiC catalogue sampling the redshift range z ∈ [0.2, 0.8]. Our fiducial sample has a comoving space density of 10−3 (h−1 Mpc)−3, and a median photo-z bias (zspec − zphoto) and scatter (σz/(1 + z)) of 0.005 and 0.017, respectively. The corresponding 5σ outlier fraction is 1.4 per cent.We also test our algorithm with Sloan Digital Sky Survey Data Release 8 and Stripe 82 data, and discuss how spectroscopic training can be used to control photo-z biases at the 0.1 per cent level.
Published: 2016

16. Stellar kinematics and metallicities in the ultra-faint dwarf galaxy Reticulum II

Author: Simon, Josh D., Drlica-Wagner, Alex, Li, T. S., Nord, Brian Dennis, Geha, Marla, Bechtol, Keith, Balbinot, Eduardo, Buckley-Geer, Elizabeth, Lin, H., Marshall, Jennifer L., Santiago, Basilio Xavier, Strigari, Louis E., Wang, M., Wechsler, Risa H., Yanny, Brian, Abbott, Timothy M. C., Bauer, Anne Hollister, Bernstein, Gary M., Bertin, Emmanuel, Brooks, D., Burke, David Lyle, Capozzi, Diego, Carnero Rosell, Aurelio, Carrasco Kind, Matías, D'Andrea, Christopher B., Costa, Luiz N. da, DePoy, Darren L., Desai, S., Diehl, H. Thomas, Dodelson, Scott, Cunha, Carlos Eduardo, Estrada, Juan, Evrard, August E., Fausti Neto, Angelo, Fernandez, Enrique, Finley, David A., Flaugher, Brenna, Frieman, Joshua A., Gaztañaga, Enrique, Gerdes, David W., Gruen, Daniel, Gruendl, Robert A., Honscheid, K., James, David J., Kent, Stephen M., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, Maia, Marcio Antonio Geimba, March, Marisa Cristina, Martini, Paul, Miller, Christopher J., Miquel, Ramon, Ogando, Ricardo L.C., Romer, Anita K., Roodman, Aaron, Sako, Masao, Sanchez-Alvaro, Eusebio, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Thaler, Jon J., Tucker, Douglas L., Vikram, Vinu, Walker, Alistair, Wester, William Carl, and DES Collaboration
Subjects: dwarf [Galaxies], abundances [Stars], Dark matter, individual (Reticulum II) [Galaxies], Local group, Matéria escura, stellar content [Galaxies], Galaxia, Composicao estelar, Dinamica estelar, Grande Nuvem de Magalhães, Espectros estelares, Pequena Nuvem de Magalhães
Abstract: We present Magellan/M2FS, Very Large Telescope/GIRAFFE, and Gemini South/GMOS spectroscopy of the newly discovered Milky Way satellite Reticulum II. Based on the spectra of 25 Ret II member stars selected from Dark Energy Survey imaging, we measure a mean heliocentric velocity of 62.8  0.5 km s-1 and a velocity dispersion of 3.3  0.7 km s-1. The mass-to-light ratio of Ret II within its half-light radius is 470  210 M L, demonstrating that it is a strongly dark matter-dominated system. Despite its spatial proximity to the Magellanic Clouds, the radial velocity of Ret II differs from that of the LMC and SMC by 199 and 83 km s-1, respectively, suggesting that it is not gravitationally bound to the Magellanic system. The likely member stars of Ret II span 1.3 dex in metallicity, with a dispersion of 0.28 ± 0.09 dex, and we identify several extremely metal-poor stars with [Fe/H] < -3. In combination with its luminosity, size, and ellipticity, these results confirm that Ret II is an ultra-faint dwarf galaxy. With a mean metallicity of [Fe/H] = -2.65  0.07, Ret II matches Segue 1 as the most metal-poor galaxy known. Although Ret II is the third-closest dwarf galaxy to the Milky Way, the line-of-sight integral of the dark matter density squared is log10 (J) 18.8 0.6 GeV cm =  2 -5 within 0 ◦. 2, indicating that the predicted gamma-ray flux from dark matter annihilation in Ret II is lower than that of several other dwarf galaxies.
Published: 2015

17. Search for gamma-ray emission from DES dwarf spheroidal galaxy candidates with Fermi-LAT data

Author: Drlica-Wagner, Alex, Albert, Andrea, Bechtol, Keith, Wood, Matthew Dunseth, Strigari, Louis E., Sánchez-Conde, Miguel A., Baldini, Luca, Essig, Rouven, Cohen-Tanugi, Johann, Anderson, Brandon, Bellazzini, Ronaldo, Bloom, Elliott D., Caputo, Regina, Cecchi, Claudia, Charles, Eric Andre, Chiang, James, De Angelis, Alessandro, Funk, Stefan, Fusco, Piergiorgio, Gargano, Fabio, Giglietto, Nico, Giordano, Francesco, Guiriec, Sylvain, Gustafsson, Michael, Kuss, Michael, Loparco, Francesco, Lubrano, Pasquale, Mirabal, N., Mizuno, Tsunefumi, Morselli, Aldo, Ohsugi, Takashi, Orlando, Elena, Persic, Massimo, Raino, Silvia, Spada, Francesca Romana, Suson, Daniel J., Zaharijas, Gabrijela, Zimmer, Stephan, Abbott, Timothy M. C., Allam, Sahar S., Balbinot, Eduardo, Bauer, Anne Hollister, Benoit-Lévy, Aurélien, Bernstein, Rebecca A., Bernstein, Gary M., Bertin, Emmanuel, Brooks, D., Buckley-Geer, Elizabeth, Burke, David Lyle, Carnero Rosell, Aurelio, Castander Serentill, Francisco Javier, Covarrubias, Ricardo A., D'Andrea, Christopher B., Costa, Luiz N. da, DePoy, Darren L., Desai, S., Diehl, H. Thomas, Cunha, Carlos Eduardo, Eifler, Tim, Estrada, Juan, Evrard, August E., Fausti Neto, Angelo, Fernandez, Enrique, Finley, David A., Flaugher, Brenna, Frieman, Joshua A., Gaztañaga, Enrique, Gerdes, David W., Gruen, Daniel, Gruendl, Robert A., Gutierrez, Gaston R., Honscheid, K., Jain, Bhuvnesh, James, David J., Jeltema, Tesla E., Kent, Stephen M., Kron, Richard G., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, Li, T. S., Luque Canaza, Elmer Fidel, Maia, Marcio Antonio Geimba, Makler, Martín, March, Marisa Cristina, Marshall, Jennifer L., Martini, Paul, Merritt, K. Wyatt, Miller, Christopher J., Miquel, Ramon, Mohr, Joseph J., Neilsen, Eric H., Nord, Brian Dennis, Ogando, Ricardo L.C., Peoples, John, Petravick, Donald L., Pieres, Adriano, Plazas Malagón, Andrés Alejandro, Queiroz, Anna Bárbara de Andrade, Romer, Anita K., Roodman, Aaron, Rykoff, Eli, Sako, Masao, Sanchez-Alvaro, Eusebio, Santiago, Basilio Xavier, Scarpine, Victor Emanuel, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Thaler, Jon J., Thomas, D., Tucker, Douglas L., Walker, Alistair, Wechsler, Risa H., Wester, William Carl, Williams, P., Yanny, Brian, Zuntz, J., Fermi LAT Collaboration, and DES Collaboration
Subjects: dwarf [Galaxies], galaxies [Gamma rays], Leptons pesados, Dark matter, Quarks, Local group, Matéria escura, Galaxia
Abstract: Due to their proximity, high dark-matter (DM) content, and apparent absence of non-thermal processes, Milky Way dwarf spheroidal satellite galaxies (dSphs) are excellent targets for the indirect detection of DM. Recently, eight new dSph candidates were discovered using the first year of data from the Dark Energy Survey (DES). We searched for gamma-ray emission coincident with the positions of these new objects in six years of Fermi Large Area Telescope data. We found no significant excesses of gamma-ray emission. Under the assumption that the DES candidates are dSphs with DM halo properties similar to the known dSphs, we computed individual and combined limits on the velocity-averaged DM annihilation cross section for these new targets. If the estimated DM content of these dSph candidates is confirmed, they will constrain the annihilation cross section to lie below the thermal relic cross section for DM particles with masses 20 GeV annihilating via the bb¯ or τ+τ− channels.
Published: 2015

18. Eight ultra-faint galaxy candidates discovered in year two the Dark Energy Survey

Author: Drlica-Wagner, Alex, Bechtol, Keith, Rykoff, Eli, Luque Canaza, Elmer Fidel, Queiroz, Anna Bárbara de Andrade, Mao, Yao-Yuan, Wechsler, Risa H., Simon, Josh D., Santiago, Basilio Xavier, Yanny, Brian, Balbinot, Eduardo, Dodelson, Scott, Fausti Neto, Angelo, James, David J., Li, T. S., Maia, Marcio Antonio Geimba, Marshall, Jennifer L., Pieres, Adriano, Stringer, Katelyn M., Walker, Alistair, Abbott, Timothy M. C., Abdalla, Filipe B., Allam, Sahar S., Benoit-Lévy, Aurélien, Bernstein, Rebecca A., Bernstein, Gary M., Bertin, Emmanuel, Brooks, D., Buckley-Geer, Elizabeth, Burke, David Lyle, Carnero Rosell, Aurelio, Carrasco Kind, Matías, Carretero Palacios, Jorge, Crocce, Martin, Costa, Luiz N. da, Desai, S., Diehl, H. Thomas, Dietrich, Jörg P., Doel, Peter, Eifler, Tim, Evrard, August E., Flaugher, Brenna, Fosalba Vela, Pablo, Frieman, Joshua A., Gaztañaga, Enrique, Gerdes, David W., Gruen, Daniel, Gruendl, Robert A., Gutierrez, Gaston R., Honscheid, K., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, Miquel, Ramon, Nord, Brian Dennis, Ogando, Ricardo L.C., Plazas Malagón, Andrés Alejandro, Reil, Kevin, Roodman, Aaron, Sako, Masao, Sanchez-Alvaro, Eusebio, Scarpine, Victor Emanuel, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Tucker, Douglas L., Vikram, Vinu, Wester, William Carl, Zhang, Yuanyuan, Zuntz, J., and DES Collaboration
Subjects: dwarf [Galaxies], Via láctea, Local group, Galáxias
Abstract: We report the discovery of eight new ultra-faint dwarf galaxy candidates in the second year of optical imaging data from the Dark Energy Survey (DES). Six of these candidates are detected at high confidence, while two lowerconfidence candidates are identified in regions of non-uniform survey coverage. The new stellar systems are found by three independent automated search techniques and are identified as overdensities of stars, consistent with the isochrone and luminosity function of an old and metal-poor simple stellar population. The new systems are faint (MV > −4.7mag) and span a range of physical sizes (17 pc < r1/2 < 181 pc) and heliocentric distances (25 kpc < De < 214 kpc). All of the new systems have central surface brightnesses consistent with known ultrafaint dwarf galaxies (μ  27.5mag arcsec−2). Roughly half of the DES candidates are more distant, less luminous, and/or have lower surface brightnesses than previously known Milky Way satellite galaxies. Most of the candidates are found in the southern part of the DES footprint close to the Magellanic Clouds. We find that the DES data alone exclude (p < 10−3) a spatially isotropic distribution of Milky Way satellites and that the observed distribution can be well, though not uniquely, described by an association between several of the DES satellites and the Magellanic system. Our model predicts that the full sky may hold ∼100 ultra-faint galaxies with physical properties comparable to the DES satellites and that 20%–30% of these would be spatially associated with the Magellanic Clouds.
Published: 2015

19. The LMC geometry and outer stellar populations from early DES data

Author: Balbinot, Eduardo, Santiago, Basilio Xavier, Girardi, Leo Alberto, Pieres, Adriano, Costa, Luiz N. da, Maia, Marcio Antonio Geimba, Gruendl, Robert A., Walker, Alistair, Yanny, Brian, Drlica-Wagner, Alex, Benoit-Lévy, Aurélien, Abbott, Timothy M. C., Allam, Sahar S., Annis, James T., Bernstein, Joseph P., Bernstein, Rebecca A., Bertin, Emmanuel, Brooks, D., Buckley-Geer, Elizabeth, Carnero Rosell, Aurelio, Cunha, Carlos Eduardo, DePoy, Darren L., Desai, S., Diehl, H. Thomas, Doel, Peter, Estrada, Juan, Evrard, August E., Fausti Neto, Angelo, Finley, David A., Flaugher, Brenna, Frieman, Joshua A., Gruen, Daniel, Honscheid, K., James, David J., Kuehn, Kyler, Kuropatkin, Nikolay P., Lahav, Ofer, March, Marisa Cristina, Marshall, Jennifer L., Miller, Christopher J., Miquel, Ramon, Ogando, Ricardo L.C., Peoples, John, Plazas Malagón, Andrés Alejandro, Scarpine, Victor Emanuel, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Tucker, Douglas L., Wechsler, Risa H., and Zuntz, J.
Subjects: Mapeamentos astronômicos, statistics [Stars], stellar content [Galaxies], Magellanic clouds, Grande Nuvem de Magalhães
Abstract: The Dark Energy Camera has captured a large set of images as part of Science Verification (SV) for the Dark Energy Survey (DES). The SV footprint covers a large portion of the outer LargeMagellanic Cloud (LMC), providing photometry 1.5 mag fainter than the main sequence turn-off of the oldest LMC stellar population.We derive geometrical and structural parameters for various stellar populations in the LMC disc. For the distribution of all LMC stars, we find an inclination of i = −38. ◦ 14 ± 0. ◦ 08 (near side in the north) and a position angle for the line of nodes of θ0 = 129. ◦ 51 ± 0. ◦ 17. We find that stars younger than ∼4 Gyr are more centrally concentrated than older stars. Fitting a projected exponential disc shows that the scale radius of the old populations is R>4 Gyr = 1.41 ± 0.01 kpc, while the younger population has R
Published: 2015

20. Discovery of two gravitationally lensed quasars in the Dark Energy Survey

Author: Agnello, Adriano, Treu, Tommaso, Ostrovski, F., Schechter, Paul L., Buckley-Geer, Elizabeth, Lin, H., Auger, Matthew W., Courbin, Frederic Y. M., Fassnacht, Christopher D., Frieman, Joshua A., Kuropatkin, Nikolay P., Marshall, Phillip J., McMahon, Richard G., Meylan, Georges, More, Andrew Mills, Suyu, Sherry, Rusu, Cristian Eduard, Finley, David A., Abbott, Timothy M. C., Abdalla, Filipe B., Allam, Sahar S., Annis, James T., Banerji, M., Benoit-Lévy, Aurélien, Bertin, Emmanuel, Brooks, D., Burke, David Lyle, Carnero Rosell, Aurelio, Carrasco Kind, Matías, Carretero Palacios, Jorge, Cunha, Carlos Eduardo, D'Andrea, Christopher B., Costa, Luiz N. da, Desai, S., Diehl, H. Thomas, Dietrich, Jörg P., Doel, Peter, Eifler, Tim, Estrada, Juan, Fausti Neto, Angelo, Flaugher, Brenna, Fosalba Vela, Pablo, Gerdes, David W., Gruen, Daniel, Gutierrez, Gaston R., Honscheid, K., James, David J., Kent, Stephen M., Kuehn, Kyler, Lahav, Ofer, Lima, Marcos Vinicius Borges Teixeira, Maia, Marcio Antonio Geimba, March, Marisa Cristina, Marshall, Jennifer L., Martini, Paul, Melchior, Peter M., Miller, Christopher J., Miquel, Ramon, Nichol, Robert C., Ogando, Ricardo L.C., Plazas Malagón, Andrés Alejandro, Reil, Kevin, Romer, Anita K., Roodman, Aaron, Sako, Masao, Sanchez-Alvaro, Eusebio, Santiago, Basilio Xavier, Scarpine, Victor Emanuel, Schubnell, Michael, Sevilla Noarbe, Ignacio, Smith, Robert Christopher, Soares-Santos, Marcelle, Sobreira, Flávia, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Thaler, Jon J., Tucker, Douglas L., Walker, Alistair, Wechsler, Risa H., and Zhang, Yuanyuan
Subjects: statistical [Methods], emission lines [Quasars], observational [Methods], Galáxias, strong [Gravitational lensing], Quasars
Abstract: We present spectroscopic confirmation of two new gravitationally lensed quasars, discovered in the Dark Energy Survey (DES) and Wide-field Infrared Survey Explorer (WISE) based on their multiband photometry and extended morphology in DES images. Images of DES J0115−5244 show a red galaxy with two blue point sources at either side, which are images of the same quasar at zs = 1.64 as obtained by our long-slit spectroscopic data. The Einstein radius estimated from the DES images is 0.51 arcsec. DES J2146−0047 is in the area of overlap between DES and the Sloan Digital Sky Survey (SDSS). Two blue components are visible in the DES and SDSS images. The SDSS fibre spectrum shows a quasar component at zs = 2.38 and absorption by Mg II and Fe II at zl = 0.799, which we tentatively associate with the foreground lens galaxy. Our long-slit spectra show that the blue components are resolved images of the same quasar. The Einstein radius is 0.68 arcsec, corresponding to an enclosed mass of 1.6 × 1011M . Three other candidates were observed and rejected, two being low-redshift pairs of starburst galaxies, and one being a quasar behind a blue star. These first confirmation results provide an important empirical validation of the data mining and model-based selection that is being applied to the entire DES data set.
Published: 2015

21. Measurement of the Differential $\gamma+2~b$-Jet Cross Section and the Ratio $\sigma$($\gamma+2~b$-jets)/$\sigma$($\gamma+b$-jet) in $p\bar{p}$ Collisions at $\sqrt{s}$ = 1.96 TeV

Author: D0 Collaboration, Abazov, Victor Mukhamedovich, Askew, Andrew Warren, Evans, Harold G., Evdokimov, Valeri N., Faure, Alexandre, Feng, Lei, Ferbel, Thomas, Fiedler, Frank, Filthaut, Frank, Fisher, Wade Cameron, Fisk, H. Eugene, Fortner, Michael R., Atkins, Scott, Fox, Harald, Fuess, Stuart C., Garbincius, Peter H., Garcia-Bellido, Aran, Garcia-Gonzalez, Jose Andres, Gavrilov, Vladimir B., Geng, Weigang, Gerber, Cecilia Elena, Gershtein, Yuri S., Ginther, George E., Augsten, Kamil, Gogota, Olga, Golovanov, Georgy Anatolievich, Grannis, Paul D., Greder, Sebastien, Greenlee, Herbert B., Grenier, Gerald Jean, Gris, Phillipe Luc, Grivaz, Jean-Francois, Grohsjean, Alexander, Gruenendahl, Stefan, Avila, Carlos A., Gruenewald, Martin Werner, Guillemin, Thibault, Gutierrez, Gaston R., Gutierrez, Phillip, Haley, Joseph Glenn Biddle, Han, Liang, Harder, Kristian, Harel, Amnon, Hauptman, John Michael, Hays, Jonathan M., Badaud, Frederique, Head, Tim, Hebbeker, Thomas, Hedin, David R., Hegab, Hatim, Heinson, Ann, Heintz, Ulrich, Hensel, Carsten, Heredia-de La Cruz, Ivan, Herner, Kenneth Richard, Hesketh, Gavin G., Bagby, Linda F., Hildreth, Michael D., Hirosky, Robert James, Hoang, Trang, Hobbs, John D., Hoeneisen, Bruce, Hogan, Julie, Hohlfeld, Mark, Holzbauer, Jenny Lyn, Howley, Ian James, Hubacek, Zdenek, Baldin, Boris, Hynek, Vlastislav, Iashvili, Ia, Ilchenko, Yuriy, Illingworth, Robert A., Ito, Albert S., Jabeen, Shabnam, Jaffre, Michel J., Jayasinghe, Ayesh, Jeong, Min-Soo, Jesik, Richard L., Bandurin, Dmitry V., Jiang, Peng, Johns, Kenneth Arthur, Johnson, Emily, Johnson, Marvin E., Jonckheere, Alan M., Jonsson, Per Martin, Joshi, Jyoti, Jung, Andreas Werner, Juste, Aurelio, Kajfasz, Eric, Banerjee, Sunanda, Karmanov, Dmitriy Y., Katsanos, Ioannis, Kaur, Manbir, Kehoe, Robert Leo Patrick, Kermiche, Smain, Khalatyan, Norayr, Khanov, Alexander, Kharchilava, Avto, Kharzheev, Yuri N., Kiselevich, Ivan Lvovich, Barberis, Emanuela, Kohli, Jatinder M., Kozelov, Alexander V., Kraus, James Alexander, Kumar, Ashish, Kupco, Alexander, Kurca, Tibor, Kuzmin, Valentin Alexandrovich, Lammers, Sabine Wedam, Lebrun, Patrice, Lee, Hyeon-Seung, Abbott, Braden Keim, Baringer, Philip S., Lee, Seh-Wook, Lee, William M., Lei, Xiaowen, Lellouch, Jeremie, Li, Dikai, Li, Hengne, Li, Liang, Li, Qi-Zhong, Lim, Jeong Ku, Lincoln, Donald W., Bartlett, J. Frederick, Linnemann, James Thomas, Lipaev, Vladimir V., Lipton, Ronald J., Liu, Huanzhao, Liu, Yanwen, Lobodenko, Alexandre, Lokajicek, Milos, Lopes de Sa, Rafael, Luna-Garcia, Rene, Lyon, Adam Leonard, Bassler, Ursula Rita, Maciel, Arthur K. A., Madar, Romain, Magana-Villalba, Ricardo, Malik, Sudhir, Malyshev, Vladimir L., Mansour, Jason, Martinez-Ortega, Jorge, McCarthy, Robert L., Mcgivern, Carrie Lynne, Meijer, Melvin M., Bazterra, Victor, Melnitchouk, Alexander S., Menezes, Diego D., Mercadante, Pedro Galli, Merkin, Mikhail M., Meyer, Arnd, Meyer, Jorg Manfred, Miconi, Florian, Mondal, Naba K., Mulhearn, Michael James, Nagy, Elemer, Bean, Alice L., Narain, Meenakshi, Nayyar, Ruchika, Neal, Homer A., Negret, Juan Pablo, Neustroev, Petr V., Nguyen, Huong Thi, Nunnemann, Thomas P., Hernandez Orduna, Jose de Jesus, Osman, Nicolas Ahmed, Osta, Jyotsna, Begalli, Marcia, Pal, Arnab, Parashar, Neeti, Parihar, Vivek, Park, Sung Keun, Partridge, Richard A., Parua, Nirmalya, Patwa, Abid, Penning, Bjoern, Perfilov, Maxim Anatolyevich, Peters, Reinhild Yvonne Fatima, Bellantoni, Leo, Petridis, Konstantinos, Petrillo, Gianluca, Petroff, Pierre, Pleier, Marc-Andre, Podstavkov, Vladimir M., Popov, Alexey V., Prewitt, Michelle, Price, Darren, Prokopenko, Nikolay N., Qian, Jianming, Beri, Suman B., Quadt, Arnulf, Quinn, Breese, Ratoff, Peter N., Razumov, Ivan A., Ripp-Baudot, Isabelle, Rizatdinova, Flera, Rominsky, Mandy Kathleen, Ross, Anthony, Royon, Christophe, Rubinov, Paul Michael, Bernardi, Gregorio, Ruchti, Randal C., Sajot, Gerard, Sanchez-Hernandez, Alberto, Sanders, Michiel P., Santos, Angelo Souza, Savage, David G., Savitskyi, Mykola, Sawyer, H. Lee, Scanlon, Timothy P., Schamberger, R. Dean, Bernhard, Ralf Patrick, Scheglov, Yury A., Schellman, Heidi M., Schwanenberger, Christian, Schwienhorst, Reinhard H., Sekaric, Jadranka, Severini, Horst, Shabalina, Elizaveta K., Shary, Viacheslav V., Shaw, Savanna, Shchukin, Andrey A., Acharya, Bannanje Sripath, Bertram, Iain A., Simak, Vladislav J., Skubic, Patrick Louis, Slattery, Paul F., Smirnov, Dmitri V., Snow, Gregory R., Snow, Joel Mark, Snyder, Scott Stuart, Soldner-Rembold, Stefan, Sonnenschein, Lars, Soustruznik, Karel, Besancon, Marc, Stark, Jan, Stoyanova, Dina A., Strauss, Michael G., Suter, Louise, Svoisky, Peter V., Titov, Maxim, Tokmenin, Valeriy V., Tsai, Yun-Tse, Tsybychev, Dmitri, Tuchming, Boris, Beuselinck, Raymond, Tully, Christopher George T., Uvarov, Lev, Uvarov, Sergey L., Uzunyan, Sergey A., Van Kooten, Richard J., van Leeuwen, Willem M., Varelas, Nikos, Varnes, Erich W., Vasilyev, Igor A., Verkheev, Alexander Yurievich, Bhat, Pushpalatha C., Vertogradov, Leonid S., Verzocchi, Marco, Vesterinen, Mika, Vilanova, Didier, Vokac, Petr, Wahl, Horst D., Wang, Michael H. L. S., Warchol, Jadwiga, Watts, Gordon Thomas, Wayne, Mitchell R., Bhatia, Sudeep, Weichert, Jonas, Welty-Rieger, Leah Christine, Williams, Mark Richard James, Wilson, Graham Wallace, Wobisch, Markus, Wood, Darien Robert, Wyatt, Terence R., Xie, Yunhe, Yamada, Ryuji, Yang, Siqi, Bhatnagar, Vipin, Yasuda, Takahiro, Yatsunenko, Yuriy A., Ye, Wanyu, Ye, Zhenyu, Yin, Hang, Yip, Kin, Youn, Sungwoo, Yu, Jiaming, Zennamo, Joseph, Zhao, Tianqi Gilbert, Blazey, Gerald Charles, Zhou, Bing, Zhu, Junjie, Zielinski, Marek, Zieminska, Daria, Zivkovic, Lidija, Blessing, Susan K., Bloom, Kenneth A., Boehnlein, Amber S., Adams, Mark Raymond, Boline, Daniel Dooley, Boos, Edward E., Borissov, Guennadi, Borysova, Maryna, Brandt, Andrew, Brandt, Oleg, Brock, Raymond L., Bross, Alan D., Brown, Duncan Paul, Bu, Xue-Bing, Adams, Todd, Buehler, Marc, Buescher, Volker, Bunichev, Viacheslav Yevgenyevich, Burdin, Sergey, Buszello, Claus Peter, Camacho-Perez, Enrique, Casey, Brendan Cameron Kieran, Castilla-Valdez, Heriberto, Caughron, Seth Aaron, Chakrabarti, Subhendu, Agnew, James P., Chan, Kwok Ming Leo, Chandra, Avdhesh, Chapon, Emilien, Chen, Guo, Cho, Sung-Woong, Choi, Suyong, Choudhary, Brajesh C., Cihangir, Selcuk, Claes, Daniel R., Clutter, Justace Randall, Alexeev, Guennadi D., Cooke, Michael P., Cooper, William Edward, Corcoran, Marjorie D., Couderc, Fabrice, Cousinou, Marie-Claude, Cutts, David, Das, Amitabha, Davies, Gavin John, de Jong, Sijbrand Jan, De La Cruz-Burelo, Eduard, Alkhazov, Georgiy D., Deliot, Frederic, Demina, Regina, Denisov, Dmitri S., Denisov, Sergei P., Desai, Satish Vijay, Deterre, Cecile, DeVaughan, Kayle Otis, Diehl, H. Thomas, Diesburg, Michael, Ding, Pengfei, Alton, Andrew K., Dominguez, D. Aaron M., Dubey, Abhinav Kumar, Dudko, Lev V., Duperrin, Arnaud, Dutt, Suneel, Eads, Michael T., Edmunds, Daniel L., Ellison, John A., Elvira, V. Daniel, and Enari, Yuji
Subjects: +bottom+photon+anything%22">p p --> bottom photon anything, perturbation theory [quantum chromodynamics], 1960 GeV-cms, scattering [anti-p p], hadroproduction [bottom], +2bottom+photon+anything%22">p p --> 2bottom photon anything, transverse momentum dependence, ratio [differential cross section], pair production [bottom], rapidity, factorization, measured [differential cross section], associated production [photon], PYTHIA, Batavia TEVATRON Coll, Monte Carlo, 1 [higher-order], experimental results
Published: 2014
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22. Characterization of DECam focal plane detectors.

Author: Diehl, H. Thomas, Angstadt, Robert, Campa, Julia, Cease, Herman, Derylo, Greg, Emes, John H., Estrada, Juan, Kubik, Donna, Flaugher, Brenna L., Holland, Steve E., Jonas, Michelle, Kolbe, William F., Krider, John, Kuhlmann, S., Kuk, Kevin, Maiorino, Marino, Palaio, Nick, Plazas, Andres, Roe, Natalie A., and Scarpine, Vic
Published: 2008
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23. 0.250mm-thick CCD packaging for the Dark Energy Survey Camera array.

Author: Derylo, Gregory, Diehl, H. Thomas, and Estrada, Juan
Published: 2006
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24. Search for anomalous couplings in WW and WZ measurements at the Tevatron (DO\ and CDF results).

Author: Diehl, H. Thomas
Published: 1996
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25. The 8 O’Clock Arc: A Serendipitous Discovery of a Strongly Lensed Lyman Break Galaxy in the SDSS DR4 Imaging Data.

Author: Allam, Sahar S., Tucker, Douglas L., Lin, Huan, Diehl, H. Thomas, Annis, James, Buckley-Geer, Elizabeth J., and Frieman, Joshua A.
Published: 2007
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26. Combined Forward-Backward Asymmetry Measurements in Top-Antitop Quark Production at the Tevatron

Author: Aaltonen, Timo Antero, Abazov, Victor Mukhamedovich, Abbott, Braden Keim, Acharya, Bannanje Sripath, Adams, Mark Raymond, Adams, Todd, Agnew, James P., Alexeev, Guennadi D., Alkhazov, Georgiy D., Alton, Andrew K., Amerio, Silvia, Amidei, Dante E., Anastassov, Anton Iankov, Annovi, Alberto, Antos, Jaroslav, Apollinari, Giorgio, Appel, Jeffrey A., Arisawa, Tetsuo, Artikov, Akram Muzafarovich, Asaadi, Jonathan A., Ashmanskas, William Joseph, Askew, Andrew Warren, Atkins, Scott, Auerbach, Benjamin, Augsten, Kamil, Aurisano, Adam J., Aushev, Volodymyr, Aushev, Yegor, Avila, Carlos A., Azfar, Farrukh A., Badaud, Frederique, Badgett, William Farris, Bae, Taegil, Bagby, Linda F., Baldin, Boris, Bandurin, Dmitry V., Banerjee, Sunanda, Barbaro-Galtieri, Angela, Barberis, Emanuela, Baringer, Philip S., Barnes, Virgil E., Barnett, Bruce Arnold, Barria, Patrizia, Bartlett, J. Frederick, Bartos, Pavol, Bassler, Ursula Rita, Bauce, Matteo, Bazterra, Victor, Bean, Alice L., Bedeschi, Franco, Begalli, Marcia, Behari, Satyajit, Bellantoni, Leo, Bellettini, Giorgio, Bellinger, James Nugent, Benjamin, Douglas P., Beretvas, Andrew F., Beri, Suman B., Bernardi, Gregorio, Bernhard, Ralf Patrick, Bertram, Iain A., Besancon, Marc, Beuselinck, Raymond, Bhat, Pushpalatha C., Bhatia, Sudeep, Bhatnagar, Vipin, Bhatti, Anwar Ahmad, Bland, Karen Renee, Blazey, Gerald Charles, Blessing, Susan K., Bloom, Kenneth A., Blumenfeld, Barry J., Bocci, Andrea, Bodek, Arie, Boehnlein, Amber S., Boline, Daniel Dooley, Boos, Edward E., Borissov, Guennadi, Bortoletto, Daniela, Borysova, Maryna, Boudreau, Joseph Francis, Boveia, Antonio, Brandt, Andrew, Brandt, Oleg, Brigliadori, Luca, Brochmann, Michelle, Brock, Raymond L., Bromberg, Carl Michael, Bross, Alan D., Brown, Duncan Paul, Brucken, Erik, Bu, Xue-Bing, Budagov, Ioulian A., Budd, Howard Scott, Buehler, Marc, Buescher, Volker, Bunichev, Viacheslav Yevgenyevich, Burdin, Sergey, Burkett, Kevin Alan, Busetto, Giovanni, Bussey, Peter John, Buszello, Claus Peter, Butti, Pierfrancesco, Buzatu, Adrian, Calamba, Aristotle, Camacho-Perez, Enrique, Camarda, Stefano, Campanelli, Mario, Canelli, Florencia, Carls, Benjamin, Carlsmith, Duncan L., Carosi, Roberto, Carrillo Moreno, Salvador, Casal Larana, Bruno, Casarsa, Massimo, Casey, Brendan Cameron Kieran, Castilla-Valdez, Heriberto, Castro, Andrea, Catastini, Pierluigi, Caughron, Seth Aaron, Cauz, Diego, Cavaliere, Viviana, Cerri, Alessandro, Cerrito, Lucio, Chakrabarti, Subhendu, Chan, Kwok Ming Leo, Chandra, Avdhesh, Chapelain, Antoine, Chapon, Emilien, Chen, Guo, Chen, Yen-Chu, Chertok, Maxwell Benjamin, Chiarelli, Giorgio, Chlachidze, Gouram, Cho, Kihyeon, Cho, Sung-Woong, Choi, Suyong, Chokheli, Davit, Choudhary, Brajesh C., Cihangir, Selcuk, Claes, Daniel R., Clark, Allan Geoffrey, Clarke, Christopher Joseph, Clutter, Justace Randall, Convery, Mary Elizabeth, Conway, John Stephen, Cooke, Michael P., Cooper, William Edward, Corbo, Matteo, Corcoran, Marjorie D., Cordelli, Marco, Couderc, Fabrice, Cousinou, Marie-Claude, Cox, Charles Alexander, Cox, David Jeremy, Cremonesi, Matteo, Cruz Alonso, Daniel, Cuevas Maestro, Javier, Culbertson, Raymond Lloyd, Cuth, Jakub, Cutts, David, Das, Amitabha, D'Ascenzo, Nicola, Datta, Mousumi, Davies, Gavin John, De Barbaro, Pawel, De Jong, Sijbrand J., De La Cruz-Burelo, Eduard, Deliot, Frederic, Demina, Regina, Demortier, Luc M., Deninno, Maria Maddalena, Denisov, Dmitri S., Denisov, Sergei P., D'Errico, Maria, Desai, Satish Vijay, Deterre, Cecile, DeVaughan, Kayle Otis, Devoto, Francesco, Di Canto, Angelo, Di Ruzza, Benedetto, Diehl, H. Thomas, Diesburg, Michael, Ding, Pengfei, Dittmann, Jay Richard, Dominguez, D. Aaron M., Donati, Simone, D'Onofrio, Monica, Dorigo, Mirco, Driutti, Anna, Drutskoy, Alexey, Dubey, Abhinav Kumar, Dudko, Lev V., Duperrin, Arnaud, Dutt, Suneel, Eads, Michael T., Ebina, Koji, Edgar, Ryan Christopher, Edmunds, Daniel L., Elagin, Andrey Lvovich, Ellison, John A., Elvira, V. Daniel, Enari, Yuji, Erbacher, Robin D., Errede, Steven Michael, Esham, Benjamin, Evans, Harold G., Evdokimov, Anatoly V., Evdokimov, Valeri N., Farrington, Sinead Marie, Faure, Alexandre, Feng, Lei, Ferbel, Thomas, Fernández Ramos, Juan Pablo, Fiedler, Frank, Field, Richard D., Filthaut, Frank, Fisher, Wade Cameron, Fisk, H. Eugene, Flanagan, Gene U., Forrest, Robert David, Fortner, Michael R., Fox, Harald, Franc, Jiri, Franklin, Melissa E. B., Freeman, John Christian, Frisch, Henry J., Fuess, Stuart C., Funakoshi, Yujiro, Galloni, Camilla, Garbincius, Peter H., Garcia-Bellido, Aran, Garcia-Gonzalez, Jose Andres, Garfinkel, Arthur F., Garosi, Paola, Gavrilov, Vladimir B., Geng, Weigang, Gerber, Cecilia Elena, Gerberich, Heather Kay, Gerchtein, Elena A., Gershtein, Yuri S., Giagu, Stefano, Giakoumopoulou, Viktoria Athina, Gibson, Karen Ruth, Ginsburg, Camille Marie, Ginther, George E., Giokaris, Nikos D., Giromini, Paolo, Glagolev, Vladimir, Glenzinski, Douglas Andrew, Gogota, Olga, Gold, Michael S., Goldin, Daniel, Golossanov, Alexander, Golovanov, Georgy Anatolievich, Gomez, Gervasio, Gomez Ceballos, Guillelmo, Goncharov, Maxim T., Gonzalez Lopez, Oscar, Gorelov, Igor V., Goshaw, Alfred T., Goulianos, Konstantin A., Gramellini, Elena, Grannis, Paul D., Greder, Sebastien, Greenlee, Herbert B., Grenier, Gerald Jean, Gris, Phillipe Luc, Grivaz, Jean-Francois, Grohsjean, Alexander, Grosso-Pilcher, Carla, Gruenendahl, Stefan, Gruenewald, Martin Werner, Guillemin, Thibault, Guimaraes Da Costa, Joao, Gutierrez, Gaston R., Gutierrez, Phillip, Hahn, Stephen R., Haley, Joseph Glenn Biddle, Han, Ji-Yeon, Han, Liang, Happacher, Fabio, Hara, Kazuhiko, Harder, Kristian, Hare, Matthew Frederick, Harel, Amnon, Harr, Robert Francis, Harrington-Taber, Timothy, Hatakeyama, Kenichi, Hauptman, John Michael, Hays, Christopher Paul, Hays, Jonathan M., Head, Tim, Hebbeker, Thomas, Hedin, David R., Hegab, Hatim, Heinrich, Joel G., Heinson, Ann, Heintz, Ulrich, Hensel, Carsten, Heredia-De La Cruz, Ivan, Herndon, Matthew Fairbanks, Herner, Kenneth Richard, Hesketh, Gavin G., Hildreth, Michael D., Hirosky, Robert James, Hoang, Trang, Hobbs, John D., Hocker, James Andrew, Hoeneisen, Bruce, Hogan, Julie, Hohlfeld, Mark, Holzbauer, Jenny Lyn, Hong, Ziqing, Hopkins, Walter Howard, Hou, Suen Ray, Howley, Ian James, Hubacek, Zdenek, Hughes, Richard Edward, Husemann, Ulrich, Hussein, Mohammad, Huston, Joey Walter, Hynek, Vlastislav, Iashvili, Ia, Ilchenko, Yuriy, Illingworth, Robert A., Introzzi, Gianluca, Iori, Maurizio, Ito, Albert S., Ivanov, Andrew Gennadievich, Jabeen, Shabnam, Jaffre, Michel J., James, Eric B., Jang, Dongwook, Jayasinghe, Ayesh, Jayatilaka, Bodhitha Anjalike, Jeon, Eun-Ju, Jeong, Min-Soo, Jesik, Richard L., Jiang, Peng, Jindariani, Sergo Robert, Johns, Kenneth Arthur, Johnson, Emily, Johnson, Marvin E., Jonckheere, Alan M., Jones, Matthew T., Jonsson, Per Martin, Joo, Kyung Kwang, Joshi, Jyoti, Jun, Soon Yung, Jung, Andreas Werner, Junk, Thomas R., Juste, Aurelio, Kajfasz, Eric, Kambeitz, Manuel, Kamon, Teruki, Karchin, Paul Edmund, Karmanov, Dmitriy Y., Kasmi, Azeddine, Kato, Yukihiro, Katsanos, Ioannis, Kaur, Manbir, Kehoe, Robert Leo Patrick, Kermiche, Smain, Ketchum, Wesley Robert, Keung, Justin Kien, Khalatyan, Norayr, Khanov, Alexander, Kharchilava, Avto, Kharzheev, Yuri N., Kilminster, Benjamin John, Kim, DongHee, Kim, Hyunsoo, Kim, Jieun, Kim, Min Jeong, Kim, Shin-Hong, Kim, Soo Bong, Kim, Young-Jin, Kim, Young-Kee, Kimura, Naoki, Kirby, Michael H., Kiselevich, Ivan Lvovich, Kohli, Jatinder M., Kondo, Kunitaka, Kong, Dae Jung, Konigsberg, Jacobo, Kotwal, Ashutosh Vijay, Kozelov, Alexander V., Kraus, James Alexander, Kreps, Michal, Kroll, I. Joseph, Kruse, Mark Charles, Kuhr, Thomas, Kumar, Ashish, Kupco, Alexander, Kurata, Masakazu, Kurca, Tibor, Kuzmin, Valentin Alexandrovich, Laasanen, Alvin Toivo, Lammel, Stephan, Lammers, Sabine Wedam, Lancaster, Mark, Lannon, Kevin Patrick, Latino, Giuseppe, Lebrun, Patrice, Lee, Hyeon-Seung, Lee, Hyun Su, Lee, Jaison, Lee, Seh-Wook, Lee, William M., Lei, Xiaowen, Lellouch, Jeremie, Leo, Sabato, Leone, Sandra, Lewis, Jonathan D., Li, Dikai, Li, Hengne, Li, Liang, Li, Qi-Zhong, Lim, Jeong Ku, Limosani, Antonio, Lincoln, Donald W., Linnemann, James Thomas, Lipaev, Vladimir V., Lipeles, Elliot David, Lipton, Ronald J., Lister, Alison, Liu, Huanzhao, Liu, Qiuguang, Liu, Tiehui Ted, Liu, Yanwen, Lobodenko, Alexandre, Lockwitz, Sarah E., Loginov, Andrey Borisovich, Lokajicek, Milos, Lopes De Sá, Rafael, Lucchesi, Donatella, Lucà, Alessandra, Lueck, Jan, Lujan, Paul Joseph, Lukens, Patrick Thomas, Luna-Garcia, Rene, Lungu, Gheorghe, Lyon, Adam Leonard, Lys, Jeremy E., Lysak, Roman, Maciel, Arthur K. A., Madar, Romain, Madrak, Robyn Leigh, Maestro, Paolo, Magana-Villalba, Ricardo, Malik, Sarah Alam, Malik, Sudhir, Malyshev, Vladimir L., Manca, Giulia, Manousakis-Katsikakis, Arkadios, Mansour, Jason, Marchese, Luigi, Margaroli, Fabrizio, Marino, Christopher Phillip, Martínez-Ortega, Jorge, Matera, Keith, Mattson, Mark Edward, Mazzacane, Anna, Mazzanti, Paolo, McCarthy, Robert L., Mcgivern, Carrie Lynne, McNulty, Ronan, Mehta, Andrew, Mehtala, Petteri, Meijer, Melvin M., Melnitchouk, Alexander S., Menezes, Diego D., Mercadante, Pedro Galli, Merkin, Mikhail M., Mesropian, Christina, Meyer, Arnd, Meyer, Jorg Manfred, Miao, Ting, Miconi, Florian, Mietlicki, David John, Mitra, Ankush, Miyake, Hideki, Moed, Shulamit, Moggi, Niccolo, Mondal, Naba K., Moon, Chang-Seong, Moore, Ronald Scott, Morello, Michael Joseph, Mukherjee, Aseet, Mulhearn, Michael James, Muller, Thomas, Murat, Pavel A., Mussini, Manuel, Nachtman, Jane Marie, Nagai, Yoshikazu, Naganoma, Junji, Nagy, Elemer, Nakano, Itsuo, Napier, Austin, Narain, Meenakshi, Nayyar, Ruchika, Neal, Homer A., Negret, Juan Pablo, Nett, Jason Michael, Neustroev, Petr V., Nguyen, Huong Thi, Nigmanov, Turgun S., Nodulman, Lawrence J., Noh, Seoyoung, Norniella Francisco, Olga, Nunnemann, Thomas P., Oakes, Louise Beth, Oh, Seog Hwan, Oh, Young-Do, Okusawa, Toru, Orava, Risto Olavi, Hernandez Orduna, Jose De Jesus, Ortolan, Lorenzo, Osman, Nicolas Ahmed, Pagliarone, Carmine Elvezio, Pal, Arnab, Palencia Cortezon, Enrique, Palni, Prabhakar, Papadimitriou, Vaia, Parashar, Neeti, Parihar, Vivek, Park, Sung Keun, Parker, William Chesluk, Partridge, Richard A., Parua, Nirmalya, Patwa, Abid, Pauletta, Giovanni, Paulini, Manfred, Paus, Christoph Maria Ernst, Penning, Bjoern, Perfilov, Maxim Anatolyevich, Peters, Reinhild Yvonne Fatima, Petridis, Konstantinos, Petrillo, Gianluca, Petroff, Pierre, Phillips, Thomas J., Piacentino, Giovanni M., Pianori, Elisabetta, Pilot, Justin Robert, Pitts, Kevin T., Plager, Charles, Pleier, Marc-Andre, Podstavkov, Vladimir M., Pondrom, Lee G., Popov, Alexey V., Poprocki, Stephen, Potamianos, Karolos Jozef, Pranko, Aliaksandr Pavlovich, Prewitt, Michelle, Price, Darren, Prokopenko, Nikolay N., Prokoshin, Fedor, Ptohos, Fotios K., Punzi, Giovanni, Qian, Jianming, Quadt, Arnulf, Quinn, Gene Breese, Ratoff, Peter N., Razumov, Ivan A., Redondo Fernández, Ignacio, Renton, Peter B., Rescigno, Marco, Rimondi, Franco, Ripp-Baudot, Isabelle, Ristori, Luciano, Rizatdinova, Flera, Robson, Aidan, Rodriguez, Tatiana Isabel, Rolli, Simona, Rominsky, Mandy Kathleen, Ronzani, Manfredi, Roser, Robert Martin, Rosner, Jonathan L., Ross, Anthony, Royon, Christophe, Rubinov, Paul Michael, Ruchti, Randal C., Ruffini, Fabrizio, Ruiz-Jimeno, Alberto, Russ, James S., Rusu, Vadim Liviu, Sajot, Gerard, Sakumoto, Willis Kazuo, Sakurai, Yuki, Sánchez Hernández, Alberto, Sanders, Michiel P., Santi, Lorenzo, Santos, Angelo Souza, Sato, Koji, Savage, David G., Saveliev, Valeri, Savitskyi, Mykola, Savoy-Navarro, Aurore, Sawyer, H. 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Dean, Scheglov, Yury A., Schellman, Heidi M., Schlabach, Philip, Schmidt, Eugene E., Schott, Matthias, Schwanenberger, Christian, Schwarz, Thomas A., Schwienhorst, Reinhard H., Scodellaro, Luca, Scuri, Fabrizio, Seidel, Sally C., Seiya, Yoshihiro, Sekaric, Jadranka, Semenov, Alexei, Severini, Horst, Sforza, Federico, Shabalina, Elizaveta K., Shalhout, Shalhout Zaki, Shary, Viacheslav V., Shaw, Savanna, Shchukin, Andrey A., Shears, Tara G., Shepard, Paul F., Shimojima, Makoto, Shkola, Oleg, Shochet, Melvyn J., Shreyber-Tecker, Irina, Simak, Vladislav J., Simonenko, Alexander V., Skubic, Patrick Louis, Slattery, Paul F., Sliwa, Krzysztof Jan, Smith, John Rodgers, Snider, Frederick Douglas, Snow, Gregory R., Snow, Joel Mark, Snyder, Scott Stuart, Söldner-Rembold, Stefan, Song, Hao, Sonnenschein, Lars, Sorin, Maria Veronica, Soustruznik, Karel, St Denis, Richard Dante, Stancari, Michelle Dawn, Stark, Jan, Stefaniuk, Nazar, Stentz, Dale James, Stoyanova, Dina A., Strauss, Michael G., Strologas, John, Sudo, Yuji, Sukhanov, Alexander I., Suslov, Igor M., Suter, Louise, Svoisky, Peter V., Takemasa, Ken-Ichi, Takeuchi, Yuji, Tang, Jian, Tecchio, Monica, Teng, Ping-Kun, Thom, Julia, Thomson, Evelyn Jean, Thukral, Vaikunth, Titov, Maxim, Toback, David A., Tokar, Stanislav, Tokmenin, Valeriy V., Tollefson, Kirsten Anne, Tomura, Tomonobu, Tonelli, Diego, Torre, Stefano, Torretta, Donatella, Totaro, Pierluigi, Trovato, Marco, Tsai, Yun-Tse, Tsybychev, Dmitri, Tuchming, Boris, Tully, Christopher George T., Ukegawa, Fumihiko, Uozumi, Satoru, Uvarov, Lev, Uvarov, Sergey L., Uzunyan, Sergey A., Van Kooten, Richard J., Van Leeuwen, Willem M., Varelas, Nikos, Varnes, Erich W., Vasilyev, Igor A., Vázquez-Valencia, Elsa Fabiola, Velev, Gueorgui, Vellidis, Konstantinos, Verkheev, Alexander Yurievich, Vernieri, Caterina, Vertogradov, Leonid S., Verzocchi, Marco, Vesterinen, Mika, Vidal Marono, Miguel, Vilanova, Didier, Vilar Cortabitarte, Rocio, Vizan Garcia, Jesus Manuel, Vogel, Marcelo, Vokac, Petr, Volpi, Guido, Wagner, Peter, Wahl, Horst D., Wallny, Rainer S., Wang, Michael H. L. S., Wang, Song-Ming, Warchol, Jadwiga, Waters, David S., Watts, Gordon Thomas, Wayne, Mitchell R., Weichert, Jonas, Welty-Rieger, Leah Christine, Wester, William Carl, Whiteson, Daniel O., Wicklund, Arthur Barry, Wilbur, Scott, Williams, Hugh H., Williams, Mark Richard James, Wilson, Graham Wallace, Wilson, Jonathan Samuel, Wilson, Peter James, Winer, Brian L., Wittich, Peter, Wobisch, Markus, Wolbers, Stephen A., Wolfmeister, Homer, Wood, Darien Robert, Wright, Thomas Roland, Wu, Xin, Wu, Zhenbin, Wyatt, Terence R., Xie, Yunhe, Yamada, Ryuji, Yamamoto, Kazuhiro, Yamato, Daisuke, Yang, Siqi, Yang, Tingjun, Yang, Un-Ki, Yang, Yu Chul, Yao, Wei-Ming, Yasuda, Takahiro, Yatsunenko, Yuriy A., Ye, Wanyu, Ye, Zhenyu, Yeh, Gong Ping, Yi, Kai, Yin, Hang, Yip, Kin, Yoh, John, Yorita, Kohei, Yoshida, Takuo, Youn, Sungwoo, Yu, Geum Bong, Yu, Intae, Yu, Jiaming, Zanetti, Anna Maria, Zeng, Yu, Zennamo, Joseph, Zhao, Tianqi Gilbert, Zhou, Bing, Zhou, Chen, Zhu, Junjie, Zielinski, Marek, Zieminska, Daria, Zivkovic, Lidija, and Zucchelli, Stefano
Subjects: 1960 GeV-cms, angular distribution: asymmetry, rapidity: difference, kinematics, DZERO, anti-p p: scattering, CDF, Batavia TEVATRON Coll, top: pair production, 7. Clean energy, anti-p p: colliding beams, experimental results
Abstract: Physical review letters 120(4), 042001 (2018). doi:10.1103/PhysRevLett.120.042001, Published by APS, College Park, Md.

27. Precise measurement of the top quark mass in dilepton decays using optimized neutrino weighting

Author: D0 Collaboration, Abazov, Victor Mukhamedovich, Abbott, Braden Keim, Acharya, Bannanje Sripath, Adams, Mark Raymond, Adams, Todd, Agnew, James P., Alexeev, Guennadi D., Alkhazov, Georgiy D., Alton, Andrew K., Askew, Andrew Warren, Atkins, Scott, Augsten, Kamil, Avila, Carlos A., Badaud, Frederique, Bagby, Linda F., Baldin, Boris, Bandurin, Dmitry V., Banerjee, Sunanda, Barberis, Emanuela, Baringer, Philip S., Bartlett, J. Frederick, Bassler, Ursula Rita, Bazterra, Victor, Bean, Alice L., Begalli, Marcia, Bellantoni, Leo, Beri, Suman B., Bernardi, Gregorio, Bernhard, Ralf Patrick, Bertram, Iain A., Besancon, Marc, Beuselinck, Raymond, Bhat, Pushpalatha C., Bhatia, Sudeep, Bhatnagar, Vipin, Blazey, Gerald Charles, Blessing, Susan K., Bloom, Kenneth A., Boehnlein, Amber S., Boline, Daniel Dooley, Boos, Edward E., Borissov, Guennadi, Borysova, Maryna, Brandt, Andrew, Brandt, Oleg, Brock, Raymond L., Bross, Alan D., Brown, Duncan Paul, Bu, Xue-Bing, Buehler, Marc, Buescher, Volker, Bunichev, Viacheslav Yevgenyevich, Burdin, Sergey, Buszello, Claus Peter, Camacho-Pérez, E., Casey, Brendan Cameron Kieran, Castilla-Valdez, Heriberto, Caughron, Seth Aaron, Chakrabarti, Subhendu, Chan, Kwok Ming Leo, Chandra, Avdhesh, Chapon, Emilien, Chen, Guo, Cho, Sung-Woong, Choi, Suyong, Choudhary, Brajesh C., Cihangir, Selcuk, Claes, Daniel R., Clutter, Justace Randall, Cooke, Michael P., Cooper, William Edward, Corcoran, Marjorie D., Couderc, Fabrice, Cousinou, Marie-Claude, Cuth, Jakub, Cutts, David, Das, Amitabha, Davies, Gavin John, De Jong, Sijbrand J., De La Cruz-Burelo, Eduard, Deliot, Frederic, Demina, Regina, Denisov, Dmitri S., Denisov, Sergei P., Desai, Satish Vijay, Deterre, Cecile, DeVaughan, Kayle Otis, Diehl, H. Thomas, Diesburg, Michael, Ding, Pengfei, Dominguez, D. Aaron M., Dubey, Abhinav Kumar, Dudko, Lev V., Duperrin, Arnaud, Dutt, Suneel, Eads, Michael T., Edmunds, Daniel L., Ellison, John A., Elvira, V. Daniel, Enari, Yuji, Evans, Harold G., Evdokimov, Anatoly V., Evdokimov, Valeri N., Faure, Alexandre, Feng, Lei, Ferbel, Thomas, Fiedler, Frank, Filthaut, Frank, Fisher, Wade Cameron, Fisk, H. Eugene, Fortner, Michael R., Fox, Harald, Fuess, Stuart C., Garbincius, Peter H., Garcia-Bellido, Aran, Garcia-Gonzalez, Jose Andres, Gavrilov, Vladimir B., Geng, Weigang, Gerber, Cecilia Elena, Gershtein, Yuri S., Ginther, George E., Gogota, Olga, Golovanov, Georgy Anatolievich, Grannis, Paul D., Greder, Sebastien, Greenlee, Herbert B., Grenier, Gerald Jean, Gris, Phillipe Luc, Grivaz, Jean-Francois, Grohsjean, Alexander, Gruenendahl, Stefan, Gruenewald, Martin Werner, Guillemin, Thibault, Gutierrez, Gaston R., Gutierrez, Phillip, Haley, Joseph Glenn Biddle, Han, Liang, Harder, Kristian, Harel, Amnon, Hauptman, John Michael, Hays, Jonathan M., Head, Tim, Hebbeker, Thomas, Hedin, David R., Hegab, Hatim, Heinson, Ann, Heintz, Ulrich, Hensel, Carsten, Heredia-De La Cruz, Ivan, Herner, Kenneth Richard, Hesketh, Gavin G., Hildreth, Michael D., Hirosky, Robert James, Hoang, Trang, Hobbs, John D., Hoeneisen, Bruce, Hogan, Julie, Hohlfeld, Mark, Holzbauer, Jenny Lyn, Howley, Ian James, Hubacek, Zdenek, Hynek, Vlastislav, Iashvili, Ia, Ilchenko, Yuriy, Illingworth, Robert A., Ito, Albert S., Jabeen, Shabnam, Jaffre, Michel J., Jayasinghe, Ayesh, Jeong, Min-Soo, Jesik, Richard L., Jiang, Peng, Johns, Kenneth Arthur, Johnson, Emily, Johnson, Marvin E., Jonckheere, Alan M., Jonsson, Per Martin, Joshi, Jyoti, Jung, Andreas Werner, Juste, Aurelio, Kajfasz, Eric, Karmanov, Dmitriy Y., Katsanos, Ioannis, Kaur, Manbir, Kehoe, Robert Leo Patrick, Kermiche, Smain, Khalatyan, Norayr, Khanov, Alexander, Kharchilava, Avto, Kharzheev, Yuri N., Kiselevich, Ivan Lvovich, Kohli, Jatinder M., Kozelov, Alexander V., Kraus, James Alexander, Kumar, Ashish, Kupco, Alexander, Kurca, Tibor, Kuzmin, Valentin Alexandrovich, Lammers, Sabine Wedam, Lebrun, Patrice, Lee, Hyeon-Seung, Lee, Seh-Wook, Lee, William M., Lei, Xiaowen, Lellouch, Jeremie, Li, Dikai, Li, Hengne, Li, Liang, Li, Qi-Zhong, Lim, Jeong Ku, Lincoln, Donald W., Linnemann, James Thomas, Lipaev, Vladimir V., Lipton, Ronald J., Liu, Huanzhao, Liu, Yanwen, Lobodenko, Alexandre, Lokajicek, Milos, Lopes De Sá, Rafael, Luna-Garcia, R., Lyon, Adam Leonard, Maciel, Arthur K. A., Madar, Romain, Magana-Villalba, R., Malik, Sudhir, Malyshev, Vladimir L., Mansour, Jason, Martínez-Ortega, J., McCarthy, Robert L., Mcgivern, Carrie Lynne, Meijer, Melvin M., Melnitchouk, Alexander S., Menezes, Diego D., Mercadante, Pedro Galli, Merkin, Mikhail M., Meyer, Arnd, Meyer, Jorg Manfred, Miconi, Florian, Mondal, Naba K., Mulhearn, Michael James, Nagy, Elemer, Narain, Meenakshi, Nayyar, Ruchika, Neal, Homer A., Negret, Juan Pablo, Neustroev, Petr V., Nguyen, Huong Thi, Nunnemann, Thomas P., Hernandez Orduna, Jose De Jesus, Osman, Nicolas Ahmed, Osta, Jyotsna, Pal, Arnab, Parashar, Neeti, Parihar, Vivek, Park, Sung Keun, Partridge, Richard A., Parua, Nirmalya, Patwa, Abid, Penning, Bjoern, Perfilov, Maxim Anatolyevich, Peters, Reinhild Yvonne Fatima, Petridis, Konstantinos, Petrillo, Gianluca, Petroff, Pierre, Pleier, Marc-Andre, Podstavkov, Vladimir M., Popov, Alexey V., Prewitt, Michelle, Price, Darren, Prokopenko, Nikolay N., Qian, Jianming, Quadt, Arnulf, Quinn, Gene Breese, Ratoff, Peter N., Razumov, Ivan A., Ripp-Baudot, I., Rizatdinova, Flera, Rominsky, Mandy Kathleen, Ross, Anthony, Royon, Christophe, Rubinov, Paul Michael, Ruchti, Randal C., Sajot, Gerard, Sanchez-Hernandez, A., Sanders, Michiel P., Santos, Angelo Souza, Savage, David G., Savitskyi, Mykola, Sawyer, H. Lee, Scanlon, Timothy P., Schamberger, R. Dean, Scheglov, Yury A., Schellman, Heidi M., Schott, Matthias, Schwanenberger, Christian, Schwienhorst, Reinhard H., Sekaric, Jadranka, Severini, Horst, Shabalina, Elizaveta K., Shary, Viacheslav V., Shaw, Savanna, Shchukin, Andrey A., Simak, Vladislav J., Skubic, Patrick Louis, Slattery, Paul F., Smirnov, Dmitri V., Snow, Gregory R., Snow, Joel Mark, Snyder, Scott Stuart, Söldner-Rembold, S., Sonnenschein, Lars, Soustruznik, Karel, Stark, Jan, Stoyanova, Dina A., Strauss, Michael G., Suter, Louise, Svoisky, Peter V., Titov, Maxim, Tokmenin, Valeriy V., Tsai, Yun-Tse, Tsybychev, Dmitri, Tuchming, Boris, Tully, Christopher George T., Uvarov, Lev, Uvarov, Sergey L., Uzunyan, Sergey A., Van Kooten, R. J., Van Leeuwen, W. M., Varelas, Nikos, Varnes, Erich W., Vasilyev, Igor A., Verkheev, Alexander Yurievich, Vertogradov, Leonid S., Verzocchi, Marco, Vesterinen, Mika, Vilanova, Didier, Vokac, Petr, Wahl, Horst D., Wang, Michael H. L. S., Warchol, Jadwiga, Watts, Gordon Thomas, Wayne, Mitchell R., Weichert, Jonas, Welty-Rieger, L., Williams, Mark Richard James, Wilson, Graham Wallace, Wobisch, Markus, Wood, Darien Robert, Wyatt, Terence R., Xie, Yunhe, Yamada, Ryuji, Yang, Siqi, Yasuda, Takahiro, Yatsunenko, Yuriy A., Ye, Wanyu, Ye, Zhenyu, Yin, Hang, Yip, Kin, Youn, Sungwoo, Yu, Jiaming, Zennamo, Joseph, Zhao, Tianqi Gilbert, Zhou, Bing, Zhu, Junjie, Zielinski, Marek, Zieminska, Daria, and Zivkovic, Lidija
Subjects: data analysis method, 1960 GeV-cms, top: mass: measured, quark: flavor, dilepton: final state, 7. Clean energy, anti-p p: colliding beams, flavor: dependence, DZERO, anti-p p: scattering, jet: energy, Batavia TEVATRON Coll, top: pair production, jet: calibration, statistical, experimental results
Abstract: Physics letters / B B752, 18-26 (2016). doi:10.1016/j.physletb.2015.10.086, Published by North-Holland Publ., Amsterdam

28. THE SLOAN BRIGHT ARCS SURVEY: TEN STRONG GRAVITATIONAL LENSING CLUSTERS AND EVIDENCE OF OVERCONCENTRATION.

Author: Wiesner, Matthew P., Lin, Huan, Allam, Sahar S., Annis, James, Buckley-Geer, Elizabeth J., Diehl, H. Thomas, Kubik, Donna, Kubo, Jeffrey M., and Tucker, Douglas
Subjects: OPEN clusters of stars, GALACTIC redshift, STAR clusters, GRAVITATIONAL lenses
Abstract: We describe 10 strong lensing galaxy clusters of redshift 0.26 ⩽ z ⩽ 0.56 that were found in the Sloan Digital Sky Survey. We present measurements of richness (N200), mass (M200), and velocity dispersion for the clusters. We find that in order to use the mass-richness relation from Johnston et al., which was established at mean redshift of 0.25, it is necessary to scale measured richness values up by 1.47. Using this scaling, we find richness values for these clusters to be in the range of 22 ⩽ N200 ⩽ 317 and mass values to be in the range of 1 × 1014h–1M☼ ⩽ M200 ⩽ 30 × 1014h–1M☼. We also present measurements of Einstein radius, mass, and velocity dispersion for the lensing systems. The Einstein radii (θE) are all relatively small, with 5.″4 ⩽ θE ⩽ 13″. Finally, we consider if there is evidence that our clusters are more concentrated than ΛCDM would predict. We find that six of our clusters do not show evidence of overconcentration, while four of our clusters do. We note a correlation between overconcentration and mass, as the four clusters showing evidence of overconcentration are all lower-mass clusters. For the four lowest mass clusters the average value of the concentration parameter c200 is 11.6, while for the six higher-mass clusters the average value of c200 is 4.4. ΛCDM would place c200 between 3.4 and 5.7. [ABSTRACT FROM AUTHOR]
Published: 2012
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29. THE SLOAN BRIGHT ARCS SURVEY: FOUR STRONGLY LENSED GALAXIES WITH REDSHIFT > 2.

Author: Diehl, H. Thomas, Allam, Sahar S., Annis, James, Buckley-Geer, Elizabeth J., Frieman, Joshua A., Kubik, Donna, Kubo, Jeffrey M., Lin, Huan, Tucker, Douglas, and West, Anderson
Published: 2009
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30. DISCOVERY OF A VERY BRIGHT, STRONGLY LENSED z = 2 GALAXY IN THE SDSS DR5.

Author: Lin, Huan, Buckley-Geer, Elizabeth, Allam, Sahar S., Tucker, Douglas L., Diehl, H. Thomas, Kubik, Donna, Kubo, Jeffrey M., Annis, James, Frieman, Joshua A., Oguri, Masamune, and Inada, Naohisa
Published: 2009
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31. THE SLOAN BRIGHT ARCS SURVEY: SIX STRONGLY LENSED GALAXIES AT z = 0.4-1.4.

Author: Kubo, Jeffrey M., Allam, Sahar S., Annis, James, Buckley-Geer, Elizabeth J., Diehl, H. Thomas, Kubik, Donna, Lin, Huan, and Tucker, Douglas
Published: 2009
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31 results on '"Diehl, H. Thomas"'

1. Sub-electron readout noise in a Skipper CCD fabricated on high resistivity silicon

2. Achieving sub electron noise in CCD systems by means of digital filtering techniques that lower 1/f pixel correlated noise

3. Studies of $X(3872)$ and $\psi(2S)$ production in $p\bar{p}$ collisions at 1.96 TeV

4. Inclusive production of the $P_c$ resonances in $p \overline p $ collisions

5. Properties of $Z_c^{\pm}(3900)$ Produced in $p \bar p$ Collision

6. Core or cusps:the central dark matter profile of a redshift one strong lensing cluster with a bright central image at Redshift 1

7. Dust Reverberation Mapping in Distant Quasars from Optical and Mid-infrared Imaging Surveys.

8. The DES Bright Arcs Survey : hundreds of candidate strongly lensed galaxy systems from the Dark Energy Survey Science Verification and Year 1 observations

9. Galaxy populations in massive galaxy clusters to z = 1.1 : colour distribution, concentration, halo occupation number and red sequence fraction

10. Farthest neighbor : the distant Milky Way satellite Eridanus II

11. Redshift distributions of galaxies in the Dark Energy Survey Science Verification shear catalogue and implications for weak lensing

12. Measurement of spin correlation between top and antitop quarks produced in $p\bar{p}$ collisions at $\sqrt{s} = 1.96$ TeV

13. The Phoenix stream : a cold stream in the southern hemisphere

14. Digging deeper into the Southern skies : a compact Milky Way companion discovered in first-year Dark Energy Survey data

15. redMaGiC : selecting luminous red galaxies from the DES Science Verification data

16. Stellar kinematics and metallicities in the ultra-faint dwarf galaxy Reticulum II

17. Search for gamma-ray emission from DES dwarf spheroidal galaxy candidates with Fermi-LAT data

18. Eight ultra-faint galaxy candidates discovered in year two the Dark Energy Survey

19. The LMC geometry and outer stellar populations from early DES data

20. Discovery of two gravitationally lensed quasars in the Dark Energy Survey

21. Measurement of the Differential $\gamma+2~b$-Jet Cross Section and the Ratio $\sigma$($\gamma+2~b$-jets)/$\sigma$($\gamma+b$-jet) in $p\bar{p}$ Collisions at $\sqrt{s}$ = 1.96 TeV

22. Characterization of DECam focal plane detectors.

23. 0.250mm-thick CCD packaging for the Dark Energy Survey Camera array.

24. Search for anomalous couplings in WW and WZ measurements at the Tevatron (DO\ and CDF results).

25. The 8 O’Clock Arc: A Serendipitous Discovery of a Strongly Lensed Lyman Break Galaxy in the SDSS DR4 Imaging Data.

26. Combined Forward-Backward Asymmetry Measurements in Top-Antitop Quark Production at the Tevatron

27. Precise measurement of the top quark mass in dilepton decays using optimized neutrino weighting

28. THE SLOAN BRIGHT ARCS SURVEY: TEN STRONG GRAVITATIONAL LENSING CLUSTERS AND EVIDENCE OF OVERCONCENTRATION.

29. THE SLOAN BRIGHT ARCS SURVEY: FOUR STRONGLY LENSED GALAXIES WITH REDSHIFT > 2.

30. DISCOVERY OF A VERY BRIGHT, STRONGLY LENSED z = 2 GALAXY IN THE SDSS DR5.

31. THE SLOAN BRIGHT ARCS SURVEY: SIX STRONGLY LENSED GALAXIES AT z = 0.4-1.4.

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31 results on '"Diehl, H. Thomas"'

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