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  • American Association for the Advancement of Science (AAAS)
  • 2010-2014  (283)
  • 1
    Publication Date: 2013-11-23
    Description: We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to about 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the 28 events at the 4sigma level. These 28 events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected from the atmospheric muon and neutrino backgrounds. These properties are, however, consistent with generic predictions for an additional component of extraterrestrial origin.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉IceCube Collaboration -- Aartsen, M G -- Abbasi, R -- Abdou, Y -- Ackermann, M -- Adams, J -- Aguilar, J A -- Ahlers, M -- Altmann, D -- Auffenberg, J -- Bai, X -- Baker, M -- Barwick, S W -- Baum, V -- Bay, R -- Beatty, J J -- Bechet, S -- Becker Tjus, J -- Becker, K-H -- Benabderrahmane, M L -- BenZvi, S -- Berghaus, P -- Berley, D -- Bernardini, E -- Bernhard, A -- Bertrand, D -- Besson, D Z -- Binder, G -- Bindig, D -- Bissok, M -- Blaufuss, E -- Blumenthal, J -- Boersma, D J -- Bohaichuk, S -- Bohm, C -- Bose, D -- Boser, S -- Botner, O -- Brayeur, L -- Bretz, H-P -- Brown, A M -- Bruijn, R -- Brunner, J -- Carson, M -- Casey, J -- Casier, M -- Chirkin, D -- Christov, A -- Christy, B -- Clark, K -- Clevermann, F -- Coenders, S -- Cohen, S -- Cowen, D F -- Cruz Silva, A H -- Danninger, M -- Daughhetee, J -- Davis, J C -- Day, M -- De Clercq, C -- De Ridder, S -- Desiati, P -- de Vries, K D -- de With, M -- DeYoung, T -- Diaz-Velez, J C -- Dunkman, M -- Eagan, R -- Eberhardt, B -- Eichmann, B -- Eisch, J -- Ellsworth, R W -- Euler, S -- Evenson, P A -- Fadiran, O -- Fazely, A R -- Fedynitch, A -- Feintzeig, J -- Feusels, T -- Filimonov, K -- Finley, C -- Fischer-Wasels, T -- Flis, S -- Franckowiak, A -- Frantzen, K -- Fuchs, T -- Gaisser, T K -- Gallagher, J -- Gerhardt, L -- Gladstone, L -- Glusenkamp, T -- Goldschmidt, A -- Golup, G -- Gonzalez, J G -- Goodman, J A -- Gora, D -- Grandmont, D T -- Grant, D -- Gross, A -- Ha, C -- Haj Ismail, A -- Hallen, P -- Hallgren, A -- Halzen, F -- Hanson, K -- Heereman, D -- Heinen, D -- Helbing, K -- Hellauer, R -- Hickford, S -- Hill, G C -- Hoffman, K D -- Hoffmann, R -- Homeier, A -- Hoshina, K -- Huelsnitz, W -- Hulth, P O -- Hultqvist, K -- Hussain, S -- Ishihara, A -- Jacobi, E -- Jacobsen, J -- Jagielski, K -- Japaridze, G S -- Jero, K -- Jlelati, O -- Kaminsky, B -- Kappes, A -- Karg, T -- Karle, A -- Kelley, J L -- Kiryluk, J -- Klas, J -- Klein, S R -- Kohne, J-H -- Kohnen, G -- Kolanoski, H -- Kopke, L -- Kopper, C -- Kopper, S -- Koskinen, D J -- Kowalski, M -- Krasberg, M -- Krings, K -- Kroll, G -- Kunnen, J -- Kurahashi, N -- Kuwabara, T -- Labare, M -- Landsman, H -- Larson, M J -- Lesiak-Bzdak, M -- Leuermann, M -- Leute, J -- Lunemann, J -- Madsen, J -- Maggi, G -- Maruyama, R -- Mase, K -- Matis, H S -- McNally, F -- Meagher, K -- Merck, M -- Meures, T -- Miarecki, S -- Middell, E -- Milke, N -- Miller, J -- Mohrmann, L -- Montaruli, T -- Morse, R -- Nahnhauer, R -- Naumann, U -- Niederhausen, H -- Nowicki, S C -- Nygren, D R -- Obertacke, A -- Odrowski, S -- Olivas, A -- O'Murchadha, A -- Paul, L -- Pepper, J A -- Perez de los Heros, C -- Pfendner, C -- Pieloth, D -- Pinat, E -- Posselt, J -- Price, P B -- Przybylski, G T -- Radel, L -- Rameez, M -- Rawlins, K -- Redl, P -- Reimann, R -- Resconi, E -- Rhode, W -- Ribordy, M -- Richman, M -- Riedel, B -- Rodrigues, J P -- Rott, C -- Ruhe, T -- Ruzybayev, B -- Ryckbosch, D -- Saba, S M -- Salameh, T -- Sander, H-G -- Santander, M -- Sarkar, S -- Schatto, K -- Scheriau, F -- Schmidt, T -- Schmitz, M -- Schoenen, S -- Schoneberg, S -- Schonwald, A -- Schukraft, A -- Schulte, L -- Schulz, O -- Seckel, D -- Sestayo, Y -- Seunarine, S -- Shanidze, R -- Sheremata, C -- Smith, M W E -- Soldin, D -- Spiczak, G M -- Spiering, C -- Stamatikos, M -- Stanev, T -- Stasik, A -- Stezelberger, T -- Stokstad, R G -- Stossl, A -- Strahler, E A -- Strom, R -- Sullivan, G W -- Taavola, H -- Taboada, I -- Tamburro, A -- Tepe, A -- Ter-Antonyan, S -- Tesic, G -- Tilav, S -- Toale, P A -- Toscano, S -- Unger, E -- Usner, M -- van Eijndhoven, N -- Van Overloop, A -- van Santen, J -- Vehring, M -- Voge, M -- Vraeghe, M -- Walck, C -- Waldenmaier, T -- Wallraff, M -- Weaver, Ch -- Wellons, M -- Wendt, C -- Westerhoff, S -- Whitehorn, N -- Wiebe, K -- Wiebusch, C H -- Williams, D R -- Wissing, H -- Wolf, M -- Wood, T R -- Woschnagg, K -- Xu, D L -- Xu, X W -- Yanez, J P -- Yodh, G -- Yoshida, S -- Zarzhitsky, P -- Ziemann, J -- Zierke, S -- Zoll, M -- New York, N.Y. -- Science. 2013 Nov 22;342(6161):1242856. doi: 10.1126/science.1242856.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24264993" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2013-01-26
    Description: Pulsars emit from low-frequency radio waves up to high-energy gamma-rays, generated anywhere from the stellar surface out to the edge of the magnetosphere. Detecting correlated mode changes across the electromagnetic spectrum is therefore key to understanding the physical relationship among the emission sites. Through simultaneous observations, we detected synchronous switching in the radio and x-ray emission properties of PSR B0943+10. When the pulsar is in a sustained radio-"bright" mode, the x-rays show only an unpulsed, nonthermal component. Conversely, when the pulsar is in a radio-"quiet" mode, the x-ray luminosity more than doubles and a 100% pulsed thermal component is observed along with the nonthermal component. This indicates rapid, global changes to the conditions in the magnetosphere, which challenge all proposed pulsar emission theories.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hermsen, W -- Hessels, J W T -- Kuiper, L -- van Leeuwen, J -- Mitra, D -- de Plaa, J -- Rankin, J M -- Stappers, B W -- Wright, G A E -- Basu, R -- Alexov, A -- Coenen, T -- Griessmeier, J-M -- Hassall, T E -- Karastergiou, A -- Keane, E -- Kondratiev, V I -- Kramer, M -- Kuniyoshi, M -- Noutsos, A -- Serylak, M -- Pilia, M -- Sobey, C -- Weltevrede, P -- Zagkouris, K -- Asgekar, A -- Avruch, I M -- Batejat, F -- Bell, M E -- Bell, M R -- Bentum, M J -- Bernardi, G -- Best, P -- Birzan, L -- Bonafede, A -- Breitling, F -- Broderick, J -- Bruggen, M -- Butcher, H R -- Ciardi, B -- Duscha, S -- Eisloffel, J -- Falcke, H -- Fender, R -- Ferrari, C -- Frieswijk, W -- Garrett, M A -- de Gasperin, F -- de Geus, E -- Gunst, A W -- Heald, G -- Hoeft, M -- Horneffer, A -- Iacobelli, M -- Kuper, G -- Maat, P -- Macario, G -- Markoff, S -- McKean, J P -- Mevius, M -- Miller-Jones, J C A -- Morganti, R -- Munk, H -- Orru, E -- Paas, H -- Pandey-Pommier, M -- Pandey, V N -- Pizzo, R -- Polatidis, A G -- Rawlings, S -- Reich, W -- Rottgering, H -- Scaife, A M M -- Schoenmakers, A -- Shulevski, A -- Sluman, J -- Steinmetz, M -- Tagger, M -- Tang, Y -- Tasse, C -- ter Veen, S -- Vermeulen, R -- van de Brink, R H -- van Weeren, R J -- Wijers, R A M J -- Wise, M W -- Wucknitz, O -- Yatawatta, S -- Zarka, P -- New York, N.Y. -- Science. 2013 Jan 25;339(6118):436-9. doi: 10.1126/science.1230960.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, Netherlands. w.hermsen@sron.nl〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23349288" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 3
    Publication Date: 2013-06-01
    Description: A genome-wide association study (GWAS) of educational attainment was conducted in a discovery sample of 101,069 individuals and a replication sample of 25,490. Three independent single-nucleotide polymorphisms (SNPs) are genome-wide significant (rs9320913, rs11584700, rs4851266), and all three replicate. Estimated effects sizes are small (coefficient of determination R(2) approximately 0.02%), approximately 1 month of schooling per allele. A linear polygenic score from all measured SNPs accounts for approximately 2% of the variance in both educational attainment and cognitive function. Genes in the region of the loci have previously been associated with health, cognitive, and central nervous system phenotypes, and bioinformatics analyses suggest the involvement of the anterior caudate nucleus. These findings provide promising candidate SNPs for follow-up work, and our effect size estimates can anchor power analyses in social-science genetics.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3751588/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3751588/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Rietveld, Cornelius A -- Medland, Sarah E -- Derringer, Jaime -- Yang, Jian -- Esko, Tonu -- Martin, Nicolas W -- Westra, Harm-Jan -- Shakhbazov, Konstantin -- Abdellaoui, Abdel -- Agrawal, Arpana -- Albrecht, Eva -- Alizadeh, Behrooz Z -- Amin, Najaf -- Barnard, John -- Baumeister, Sebastian E -- Benke, Kelly S -- Bielak, Lawrence F -- Boatman, Jeffrey A -- Boyle, Patricia A -- Davies, Gail -- de Leeuw, Christiaan -- Eklund, Niina -- Evans, Daniel S -- Ferhmann, Rudolf -- Fischer, Krista -- Gieger, Christian -- Gjessing, Hakon K -- Hagg, Sara -- Harris, Jennifer R -- Hayward, Caroline -- Holzapfel, Christina -- Ibrahim-Verbaas, Carla A -- Ingelsson, Erik -- Jacobsson, Bo -- Joshi, Peter K -- Jugessur, Astanand -- Kaakinen, Marika -- Kanoni, Stavroula -- Karjalainen, Juha -- Kolcic, Ivana -- Kristiansson, Kati -- Kutalik, Zoltan -- Lahti, Jari -- Lee, Sang H -- Lin, Peng -- Lind, Penelope A -- Liu, Yongmei -- Lohman, Kurt -- Loitfelder, Marisa -- McMahon, George -- Vidal, Pedro Marques -- Meirelles, Osorio -- Milani, Lili -- Myhre, Ronny -- Nuotio, Marja-Liisa -- Oldmeadow, Christopher J -- Petrovic, Katja E -- Peyrot, Wouter J -- Polasek, Ozren -- Quaye, Lydia -- Reinmaa, Eva -- Rice, John P -- Rizzi, Thais S -- Schmidt, Helena -- Schmidt, Reinhold -- Smith, Albert V -- Smith, Jennifer A -- Tanaka, Toshiko -- Terracciano, Antonio -- van der Loos, Matthijs J H M -- Vitart, Veronique -- Volzke, Henry -- Wellmann, Jurgen -- Yu, Lei -- Zhao, Wei -- Allik, Juri -- Attia, John R -- Bandinelli, Stefania -- Bastardot, Francois -- Beauchamp, Jonathan -- Bennett, David A -- Berger, Klaus -- Bierut, Laura J -- Boomsma, Dorret I -- Bultmann, Ute -- Campbell, Harry -- Chabris, Christopher F -- Cherkas, Lynn -- Chung, Mina K -- Cucca, Francesco -- de Andrade, Mariza -- De Jager, Philip L -- De Neve, Jan-Emmanuel -- Deary, Ian J -- Dedoussis, George V -- Deloukas, Panos -- Dimitriou, Maria -- Eiriksdottir, Guethny -- Elderson, Martin F -- Eriksson, Johan G -- Evans, David M -- Faul, Jessica D -- Ferrucci, Luigi -- Garcia, Melissa E -- Gronberg, Henrik -- Guethnason, Vilmundur -- Hall, Per -- Harris, Juliette M -- Harris, Tamara B -- Hastie, Nicholas D -- Heath, Andrew C -- Hernandez, Dena G -- Hoffmann, Wolfgang -- Hofman, Adriaan -- Holle, Rolf -- Holliday, Elizabeth G -- Hottenga, Jouke-Jan -- Iacono, William G -- Illig, Thomas -- Jarvelin, Marjo-Riitta -- Kahonen, Mika -- Kaprio, Jaakko -- Kirkpatrick, Robert M -- Kowgier, Matthew -- Latvala, Antti -- Launer, Lenore J -- Lawlor, Debbie A -- Lehtimaki, Terho -- Li, Jingmei -- Lichtenstein, Paul -- Lichtner, Peter -- Liewald, David C -- Madden, Pamela A -- Magnusson, Patrik K E -- Makinen, Tomi E -- Masala, Marco -- McGue, Matt -- Metspalu, Andres -- Mielck, Andreas -- Miller, Michael B -- Montgomery, Grant W -- Mukherjee, Sutapa -- Nyholt, Dale R -- Oostra, Ben A -- Palmer, Lyle J -- Palotie, Aarno -- Penninx, Brenda W J H -- Perola, Markus -- Peyser, Patricia A -- Preisig, Martin -- Raikkonen, Katri -- Raitakari, Olli T -- Realo, Anu -- Ring, Susan M -- Ripatti, Samuli -- Rivadeneira, Fernando -- Rudan, Igor -- Rustichini, Aldo -- Salomaa, Veikko -- Sarin, Antti-Pekka -- Schlessinger, David -- Scott, Rodney J -- Snieder, Harold -- St Pourcain, Beate -- Starr, John M -- Sul, Jae Hoon -- Surakka, Ida -- Svento, Rauli -- Teumer, Alexander -- LifeLines Cohort Study -- Tiemeier, Henning -- van Rooij, Frank J A -- Van Wagoner, David R -- Vartiainen, Erkki -- Viikari, Jorma -- Vollenweider, Peter -- Vonk, Judith M -- Waeber, Gerard -- Weir, David R -- Wichmann, H-Erich -- Widen, Elisabeth -- Willemsen, Gonneke -- Wilson, James F -- Wright, Alan F -- Conley, Dalton -- Davey-Smith, George -- Franke, Lude -- Groenen, Patrick J F -- Hofman, Albert -- Johannesson, Magnus -- Kardia, Sharon L R -- Krueger, Robert F -- Laibson, David -- Martin, Nicholas G -- Meyer, Michelle N -- Posthuma, Danielle -- Thurik, A Roy -- Timpson, Nicholas J -- Uitterlinden, Andre G -- van Duijn, Cornelia M -- Visscher, Peter M -- Benjamin, Daniel J -- Cesarini, David -- Koellinger, Philipp D -- AA09367/AA/NIAAA NIH HHS/ -- AA11886/AA/NIAAA NIH HHS/ -- BB/F019394/1/Biotechnology and Biological Sciences Research Council/United Kingdom -- CZB/4/710/Chief Scientist Office/United Kingdom -- DA024417/DA/NIDA NIH HHS/ -- DA029377/DA/NIDA NIH HHS/ -- DA05147/DA/NIDA NIH HHS/ -- DA13240/DA/NIDA NIH HHS/ -- ETM/55/Chief Scientist Office/United Kingdom -- F31 DA029377/DA/NIDA NIH HHS/ -- G0600705/Medical Research Council/United Kingdom -- G0700704/Medical Research Council/United Kingdom -- G9815508/Medical Research Council/United Kingdom -- K05 AA017688/AA/NIAAA NIH HHS/ -- MC_PC_U127561128/Medical Research Council/United Kingdom -- MC_UU_12013/1/Medical Research Council/United Kingdom -- MC_UU_12013/3/Medical Research Council/United Kingdom -- MC_UU_12013/5/Medical Research Council/United Kingdom -- MH016880/MH/NIMH NIH HHS/ -- MH066140/MH/NIMH NIH HHS/ -- MR/K026992/1/Medical Research Council/United Kingdom -- P01 AG005842/AG/NIA NIH HHS/ -- P01 CA089392/CA/NCI NIH HHS/ -- P01 GM099568/GM/NIGMS NIH HHS/ -- P01-AG005842/AG/NIA NIH HHS/ -- P01-AG005842-20S2/AG/NIA NIH HHS/ -- P30 AG012810/AG/NIA NIH HHS/ -- P30-AG012810/AG/NIA NIH HHS/ -- R01 AA009367/AA/NIAAA NIH HHS/ -- R01 AA011886/AA/NIAAA NIH HHS/ -- R01 DA013240/DA/NIDA NIH HHS/ -- R01 HL090620/HL/NHLBI NIH HHS/ -- R01 HL105756/HL/NHLBI NIH HHS/ -- R01 HL111314/HL/NHLBI NIH HHS/ -- R01 MH066140/MH/NIMH NIH HHS/ -- R37 DA005147/DA/NIDA NIH HHS/ -- T32 AG000186/AG/NIA NIH HHS/ -- T32 MH016880/MH/NIMH NIH HHS/ -- T32-AG000186-23/AG/NIA NIH HHS/ -- U01 AG009740/AG/NIA NIH HHS/ -- U01 DA024417/DA/NIDA NIH HHS/ -- Z01 AG001050-01/Intramural NIH HHS/ -- ZIA AG000196-03/Intramural NIH HHS/ -- ZIA AG000196-04/Intramural NIH HHS/ -- New York, N.Y. -- Science. 2013 Jun 21;340(6139):1467-71. doi: 10.1126/science.1235488. Epub 2013 May 30.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Applied Economics, Erasmus School of Economics, Erasmus University Rotterdam, Rotterdam, Netherlands.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23722424" target="_blank"〉PubMed〈/a〉
    Keywords: Cognition ; *Educational Status ; Endophenotypes ; Female ; Genetic Loci ; *Genome-Wide Association Study ; Humans ; Male ; Multifactorial Inheritance ; *Polymorphism, Single Nucleotide
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 4
    Publication Date: 2014-11-08
    Description: Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescopes, revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20% of the gravitational radius of its central black hole. We suggest that the emission is associated with pulsar-like particle acceleration by the electric field across a magnetospheric gap at the base of the radio jet.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Aleksic, J -- Ansoldi, S -- Antonelli, L A -- Antoranz, P -- Babic, A -- Bangale, P -- Barrio, J A -- Becerra Gonzalez, J -- Bednarek, W -- Bernardini, E -- Biasuzzi, B -- Biland, A -- Blanch, O -- Bonnefoy, S -- Bonnoli, G -- Borracci, F -- Bretz, T -- Carmona, E -- Carosi, A -- Colin, P -- Colombo, E -- Contreras, J L -- Cortina, J -- Covino, S -- Da Vela, P -- Dazzi, F -- De Angelis, A -- De Caneva, G -- De Lotto, B -- de Ona Wilhelmi, E -- Delgado Mendez, C -- Dominis Prester, D -- Dorner, D -- Doro, M -- Einecke, S -- Eisenacher, D -- Elsaesser, D -- Fonseca, M V -- Font, L -- Frantzen, K -- Fruck, C -- Galindo, D -- Garcia Lopez, R J -- Garczarczyk, M -- Garrido Terrats, D -- Gaug, M -- Godinovic, N -- Gonzalez Munoz, A -- Gozzini, S R -- Hadasch, D -- Hanabata, Y -- Hayashida, M -- Herrera, J -- Hildebrand, D -- Hose, J -- Hrupec, D -- Idec, W -- Kadenius, V -- Kellermann, H -- Kodani, K -- Konno, Y -- Krause, J -- Kubo, H -- Kushida, J -- La Barbera, A -- Lelas, D -- Lewandowska, N -- Lindfors, E -- Lombardi, S -- Longo, F -- Lopez, M -- Lopez-Coto, R -- Lopez-Oramas, A -- Lorenz, E -- Lozano, I -- Makariev, M -- Mallot, K -- Maneva, G -- Mankuzhiyil, N -- Mannheim, K -- Maraschi, L -- Marcote, B -- Mariotti, M -- Martinez, M -- Mazin, D -- Menzel, U -- Miranda, J M -- Mirzoyan, R -- Moralejo, A -- Munar-Adrover, P -- Nakajima, D -- Niedzwiecki, A -- Nilsson, K -- Nishijima, K -- Noda, K -- Orito, R -- Overkemping, A -- Paiano, S -- Palatiello, M -- Paneque, D -- Paoletti, R -- Paredes, J M -- Paredes-Fortuny, X -- Persic, M -- Poutanen, J -- Prada Moroni, P G -- Prandini, E -- Puljak, I -- Reinthal, R -- Rhode, W -- Ribo, M -- Rico, J -- Rodriguez Garcia, J -- Rugamer, S -- Saito, T -- Saito, K -- Satalecka, K -- Scalzotto, V -- Scapin, V -- Schultz, C -- Schweizer, T -- Shore, S N -- Sillanpaa, A -- Sitarek, J -- Snidaric, I -- Sobczynska, D -- Spanier, F -- Stamatescu, V -- Stamerra, A -- Steinbring, T -- Storz, J -- Strzys, M -- Takalo, L -- Takami, H -- Tavecchio, F -- Temnikov, P -- Terzic, T -- Tescaro, D -- Teshima, M -- Thaele, J -- Tibolla, O -- Torres, D F -- Toyama, T -- Treves, A -- Uellenbeck, M -- Vogler, P -- Zanin, R -- Kadler, M -- Schulz, R -- Ros, E -- Bach, U -- Krauss, F -- Wilms, J -- New York, N.Y. -- Science. 2014 Nov 28;346(6213):1080-4. doi: 10.1126/science.1256183. Epub 2014 Nov 6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Institut de Fisica d'Altes Energies, Campus UAB, E-08193 Bellaterra, Spain. ; Universita di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy. ; INAF National Institute for Astrophysics, I-00136 Rome, Italy. ; Universita di Siena and INFN Pisa, I-53100 Siena, Italy. ; Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia. ; Max-Planck-Institut fur Physik, D-80805 Munchen, Germany. ; Universidad Complutense, E-28040 Madrid, Spain. ; Instituto de Astrofisica de Canarias, E-38200 La Laguna, Tenerife, Spain. Present address: NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA, and Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA. ; University of Lodz', PL-90236 Lodz, Poland. ; Deutsches Elektronen-Synchrotron, D-15738 Zeuthen, Germany. ; ETH Zurich, CH-8093 Zurich, Switzerland. ; Universitat Wurzburg, D-97074 Wurzburg, Germany. Present address: Ecole Polytechnique Federale de Lausanne (EPFL), Lausanne, Switzerland. ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas, E-28040 Madrid, Spain. ; Instituto de Astrofisica de Canarias, E-38200 La Laguna, Tenerife, Spain. ; Institute of Space Sciences, E-08193 Barcelona, Spain. ; Universitat Wurzburg, D-97074 Wurzburg, Germany. ; Universita di Padova and INFN, I-35131 Padova, Italy. ; Technische Universitat Dortmund, D-44221 Dortmund, Germany. ; Universitat Wurzburg, D-97074 Wurzburg, Germany. deisenacher@astro.uni-wuerzburg.de jsitarek@ifae.es mannheim@astro.uni-wuerzburg.de. ; Unitat de Fisica de les Radiacions, Departament de Fisica, and Centro de Estudios e Investigacion Espaciales-Institut d'Estudis Espacials de Catalunya, Universitat Autonoma de Barcelona, E-08193 Bellaterra, Spain. ; Universitat de Barcelona, Institut de Ciencies del Cosmos, Institut d'Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain. ; Institute of Space Sciences, E-08193 Barcelona, Spain. Present address: Institut fur Astro- und Teilchenphysik, Leopold-Franzens-Universitat Innsbruck, A-6020 Innsbruck, Austria. ; Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan. ; Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland. ; Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland. Present address: Finnish Centre for Astronomy with ESO (FINCA), Turku, Finland. ; Deceased. ; Institute for Nuclear Research and Nuclear Energy, BG-1784 Sofia, Bulgaria. ; Universita di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy. Present address: Astrophysics Science Division, Bhabha Atomic Research Centre, Mumbai 400085, India. ; Universita di Pisa and INFN Pisa, I-56126 Pisa, Italy. ; Institut de Fisica d'Altes Energies, Campus UAB, E-08193 Bellaterra, Spain. deisenacher@astro.uni-wuerzburg.de jsitarek@ifae.es mannheim@astro.uni-wuerzburg.de. ; Institut de Fisica d'Altes Energies, Campus UAB, E-08193 Bellaterra, Spain. Present address: School of Chemistry and Physics, University of Adelaide, Adelaide 5005, Australia. ; Max-Planck-Institut fur Physik, D-80805 Munchen, Germany. Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan. ; ICREA and Institute of Space Sciences, E-08193 Barcelona, Spain. ; Universita dell'Insubria and INFN Milano Bicocca, Como, I-22100 Como, Italy. ; Universitat Wurzburg, D-97074 Wurzburg, Germany. Dr. Remeis-Sternwarte Bamberg, Astronomisches Institut der Universitat Erlangen-Nurnberg, ECAP, D-96049 Bamberg, Germany. ; Max-Planck-Institut fur Radioastronomie, D-53121 Bonn, Germany. Observatori Astronomic, Universitat de Valencia, E-46980 Paterna, Valencia, Spain. Departament d'Astronomia i Astrofisica, Universitat de Valencia, E-46100 Burjassot, Valencia, Spain. ; Max-Planck-Institut fur Radioastronomie, D-53121 Bonn, Germany. ; Dr. Remeis-Sternwarte Bamberg, Astronomisches Institut der Universitat Erlangen-Nurnberg, ECAP, D-96049 Bamberg, Germany.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25378461" target="_blank"〉PubMed〈/a〉
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  • 5
    Publication Date: 2011-03-10
    Description: Protons and helium nuclei are the most abundant components of the cosmic radiation. Precise measurements of their fluxes are needed to understand the acceleration and subsequent propagation of cosmic rays in our Galaxy. We report precision measurements of the proton and helium spectra in the rigidity range 1 gigavolt to 1.2 teravolts performed by the satellite-borne experiment PAMELA (payload for antimatter matter exploration and light-nuclei astrophysics). We find that the spectral shapes of these two species are different and cannot be described well by a single power law. These data challenge the current paradigm of cosmic-ray acceleration in supernova remnants followed by diffusive propagation in the Galaxy. More complex processes of acceleration and propagation of cosmic rays are required to explain the spectral structures observed in our data.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Adriani, O -- Barbarino, G C -- Bazilevskaya, G A -- Bellotti, R -- Boezio, M -- Bogomolov, E A -- Bonechi, L -- Bongi, M -- Bonvicini, V -- Borisov, S -- Bottai, S -- Bruno, A -- Cafagna, F -- Campana, D -- Carbone, R -- Carlson, P -- Casolino, M -- Castellini, G -- Consiglio, L -- De Pascale, M P -- De Santis, C -- De Simone, N -- Di Felice, V -- Galper, A M -- Gillard, W -- Grishantseva, L -- Jerse, G -- Karelin, A V -- Koldashov, S V -- Krutkov, S Y -- Kvashnin, A N -- Leonov, A -- Malakhov, V -- Malvezzi, V -- Marcelli, L -- Mayorov, A G -- Menn, W -- Mikhailov, V V -- Mocchiutti, E -- Monaco, A -- Mori, N -- Nikonov, N -- Osteria, G -- Palma, F -- Papini, P -- Pearce, M -- Picozza, P -- Pizzolotto, C -- Ricci, M -- Ricciarini, S B -- Rossetto, L -- Sarkar, R -- Simon, M -- Sparvoli, R -- Spillantini, P -- Stozhkov, Y I -- Vacchi, A -- Vannuccini, E -- Vasilyev, G -- Voronov, S A -- Yurkin, Y T -- Wu, J -- Zampa, G -- Zampa, N -- Zverev, V G -- New York, N.Y. -- Science. 2011 Apr 1;332(6025):69-72. doi: 10.1126/science.1199172. Epub 2011 Mar 3.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics, University of Florence, I-50019 Sesto Fiorentino, Florence, Italy.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21385721" target="_blank"〉PubMed〈/a〉
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  • 6
    Publication Date: 2011-01-08
    Description: A young and energetic pulsar powers the well-known Crab Nebula. Here, we describe two separate gamma-ray (photon energy greater than 100 mega-electron volts) flares from this source detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope. The first flare occurred in February 2009 and lasted approximately 16 days. The second flare was detected in September 2010 and lasted approximately 4 days. During these outbursts, the gamma-ray flux from the nebula increased by factors of four and six, respectively. The brevity of the flares implies that the gamma rays were emitted via synchrotron radiation from peta-electron-volt (10(15) electron volts) electrons in a region smaller than 1.4 x 10(-2) parsecs. These are the highest-energy particles that can be associated with a discrete astronomical source, and they pose challenges to particle acceleration theory.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Abdo, A A -- Ackermann, M -- Ajello, M -- Allafort, A -- Baldini, L -- Ballet, J -- Barbiellini, G -- Bastieri, D -- Bechtol, K -- Bellazzini, R -- Berenji, B -- Blandford, R D -- Bloom, E D -- Bonamente, E -- Borgland, A W -- Bouvier, A -- Brandt, T J -- Bregeon, J -- Brez, A -- Brigida, M -- Bruel, P -- Buehler, R -- Buson, S -- Caliandro, G A -- Cameron, R A -- Cannon, A -- Caraveo, P A -- Casandjian, J M -- Celik, O -- Charles, E -- Chekhtman, A -- Cheung, C C -- Chiang, J -- Ciprini, S -- Claus, R -- Cohen-Tanugi, J -- Costamante, L -- Cutini, S -- D'Ammando, F -- Dermer, C D -- de Angelis, A -- de Luca, A -- de Palma, F -- Digel, S W -- do Couto e Silva, E -- Drell, P S -- Drlica-Wagner, A -- Dubois, R -- Dumora, D -- Favuzzi, C -- Fegan, S J -- Ferrara, E C -- Focke, W B -- Fortin, P -- Frailis, M -- Fukazawa, Y -- Funk, S -- Fusco, P -- Gargano, F -- Gasparrini, D -- Gehrels, N -- Germani, S -- Giglietto, N -- Giordano, F -- Giroletti, M -- Glanzman, T -- Godfrey, G -- Grenier, I A -- Grondin, M-H -- Grove, J E -- Guiriec, S -- Hadasch, D -- Hanabata, Y -- Harding, A K -- Hayashi, K -- Hayashida, M -- Hays, E -- Horan, D -- Itoh, R -- Johannesson, G -- Johnson, A S -- Johnson, T J -- Khangulyan, D -- Kamae, T -- Katagiri, H -- Kataoka, J -- Kerr, M -- Knodlseder, J -- Kuss, M -- Lande, J -- Latronico, L -- Lee, S-H -- Lemoine-Goumard, M -- Longo, F -- Loparco, F -- Lubrano, P -- Madejski, G M -- Makeev, A -- Marelli, M -- Mazziotta, M N -- McEnery, J E -- Michelson, P F -- Mitthumsiri, W -- Mizuno, T -- Moiseev, A A -- Monte, C -- Monzani, M E -- Morselli, A -- Moskalenko, I V -- Murgia, S -- Nakamori, T -- Naumann-Godo, M -- Nolan, P L -- Norris, J P -- Nuss, E -- Ohsugi, T -- Okumura, A -- Omodei, N -- Ormes, J F -- Ozaki, M -- Paneque, D -- Parent, D -- Pelassa, V -- Pepe, M -- Pesce-Rollins, M -- Pierbattista, M -- Piron, F -- Porter, T A -- Raino, S -- Rando, R -- Ray, P S -- Razzano, M -- Reimer, A -- Reimer, O -- Reposeur, T -- Ritz, S -- Romani, R W -- Sadrozinski, H F-W -- Sanchez, D -- Saz Parkinson, P M -- Scargle, J D -- Schalk, T L -- Sgro, C -- Siskind, E J -- Smith, P D -- Spandre, G -- Spinelli, P -- Strickman, M S -- Suson, D J -- Takahashi, H -- Takahashi, T -- Tanaka, T -- Thayer, J B -- Thompson, D J -- Tibaldo, L -- Torres, D F -- Tosti, G -- Tramacere, A -- Troja, E -- Uchiyama, Y -- Vandenbroucke, J -- Vasileiou, V -- Vianello, G -- Vitale, V -- Wang, P -- Wood, K S -- Yang, Z -- Ziegler, M -- New York, N.Y. -- Science. 2011 Feb 11;331(6018):739-42. doi: 10.1126/science.1199705. Epub 2011 Jan 6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21212321" target="_blank"〉PubMed〈/a〉
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  • 7
    Publication Date: 2010-03-06
    Description: Nuclear collisions recreate conditions in the universe microseconds after the Big Bang. Only a very small fraction of the emitted fragments are light nuclei, but these states are of fundamental interest. We report the observation of antihypertritons--comprising an antiproton, an antineutron, and an antilambda hyperon--produced by colliding gold nuclei at high energy. Our analysis yields 70 +/- 17 antihypertritons ((Lambda)(3)-H) and 157 +/- 30 hypertritons (Lambda3H). The measured yields of Lambda3H ((Lambda)(3)-H) and 3He (3He) are similar, suggesting an equilibrium in coordinate and momentum space populations of up, down, and strange quarks and antiquarks, unlike the pattern observed at lower collision energies. The production and properties of antinuclei, and of nuclei containing strange quarks, have implications spanning nuclear and particle physics, astrophysics, and cosmology.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉STAR Collaboration -- Abelev, B I -- Aggarwal, M M -- Ahammed, Z -- Alakhverdyants, A V -- Alekseev, I -- Anderson, B D -- Arkhipkin, D -- Averichev, G S -- Balewski, J -- Barnby, L S -- Baumgart, S -- Beavis, D R -- Bellwied, R -- Betancourt, M J -- Betts, R R -- Bhasin, A -- Bhati, A K -- Bichsel, H -- Bielcik, J -- Bielcikova, J -- Biritz, B -- Bland, L C -- Bonner, B E -- Bouchet, J -- Braidot, E -- Brandin, A V -- Bridgeman, A -- Bruna, E -- Bueltmann, S -- Bunzarov, I -- Burton, T P -- Cai, X Z -- Caines, H -- Calderon, M -- Catu, O -- Cebra, D -- Cendejas, R -- Cervantes, M C -- Chajecki, Z -- Chaloupka, P -- Chattopadhyay, S -- Chen, H F -- Chen, J H -- Chen, J Y -- Cheng, J -- Cherney, M -- Chikanian, A -- Choi, K E -- Christie, W -- Chung, P -- Clarke, R F -- Codrington, M J M -- Corliss, R -- Cramer, J G -- Crawford, H J -- Das, D -- Dash, S -- Davila Leyva, A -- De Silva, L C -- Debbe, R R -- Dedovich, T G -- DePhillips, M -- Derevschikov, A A -- Derradi de Souza, R -- Didenko, L -- Djawotho, P -- Dogra, S M -- Dong, X -- Drachenberg, J L -- Draper, J E -- Dunlop, J C -- Dutta Mazumdar, M R -- Efimov, L G -- Elhalhuli, E -- Elnimr, M -- Engelage, J -- Eppley, G -- Erazmus, B -- Estienne, M -- Eun, L -- Evdokimov, O -- Fachini, P -- Fatemi, R -- Fedorisin, J -- Fersch, R G -- Filip, P -- Finch, E -- Fine, V -- Fisyak, Y -- Gagliardi, C A -- Gangadharan, D R -- Ganti, M S -- Garcia-Solis, E J -- Geromitsos, A -- Geurts, F -- Ghazikhanian, V -- Ghosh, P -- Gorbunov, Y N -- Gordon, A -- Grebenyuk, O -- Grosnick, D -- Grube, B -- Guertin, S M -- Gupta, A -- Gupta, N -- Guryn, W -- Haag, B -- Hamed, A -- Han, L-X -- Harris, J W -- Hays-Wehle, J P -- Heinz, M -- Heppelmann, S -- Hirsch, A -- Hjort, E -- Hoffman, A M -- Hoffmann, G W -- Hofman, D J -- Hollis, R S -- Huang, B -- Huang, H Z -- Humanic, T J -- Huo, L -- Igo, G -- Iordanova, A -- Jacobs, P -- Jacobs, W W -- Jakl, P -- Jena, C -- Jin, F -- Jones, C L -- Jones, P G -- Joseph, J -- Judd, E G -- Kabana, S -- Kajimoto, K -- Kang, K -- Kapitan, J -- Kauder, K -- Keane, D -- Kechechyan, A -- Kettler, D -- Kikola, D P -- Kiryluk, J -- Kisiel, A -- Klein, S R -- Knospe, A G -- Kocoloski, A -- Koetke, D D -- Kollegger, T -- Konzer, J -- Kopytine, M -- Koralt, I -- Koroleva, L -- Korsch, W -- Kotchenda, L -- Kouchpil, V -- Kravtsov, P -- Krueger, K -- Krus, M -- Kumar, L -- Kurnadi, P -- Lamont, M A C -- Landgraf, J M -- LaPointe, S -- Lauret, J -- Lebedev, A -- Lednicky, R -- Lee, C-H -- Lee, J H -- Leight, W -- Levine, M J -- Li, C -- Li, L -- Li, N -- Li, W -- Li, X -- Li, Y -- Li, Z -- Lin, G -- Lindenbaum, S J -- Lisa, M A -- Liu, F -- Liu, H -- Liu, J -- Ljubicic, T -- Llope, W J -- Longacre, R S -- Love, W A -- Lu, Y -- Luo, X -- Ma, G L -- Ma, Y G -- Mahapatra, D P -- Majka, R -- Mal, O I -- Mangotra, L K -- Manweiler, R -- Margetis, S -- Markert, C -- Masui, H -- Matis, H S -- Matulenko, Yu A -- McDonald, D -- McShane, T S -- Meschanin, A -- Milner, R -- Minaev, N G -- Mioduszewski, S -- Mischke, A -- Mitrovski, M K -- Mohanty, B -- Mondal, M M -- Morozov, B -- Morozov, D A -- Munhoz, M G -- Nandi, B K -- Nattrass, C -- Nayak, T K -- Nelson, J M -- Netrakanti, P K -- Ng, M J -- Nogach, L V -- Nurushev, S B -- Odyniec, G -- Ogawa, A -- Okada, H -- Okorokov, V -- Olson, D -- Pachr, M -- Page, B S -- Pal, S K -- Pandit, Y -- Panebratsev, Y -- Pawlak, T -- Peitzmann, T -- Perevoztchikov, V -- Perkins, C -- Peryt, W -- Phatak, S C -- Pile, P -- Planinic, M -- Ploskon, M A -- Pluta, J -- Plyku, D -- Poljak, N -- Poskanzer, A M -- Potukuchi, B V K S -- Powell, C B -- Prindle, D -- Pruneau, C -- Pruthi, N K -- Pujahari, P R -- Putschke, J -- Qiu, H -- Raniwala, R -- Raniwala, S -- Ray, R L -- Redwine, R -- Reed, R -- Ritter, H G -- Roberts, J B -- Rogachevskiy, O V -- Romero, J L -- Rose, A -- Roy, C -- Ruan, L -- Sahoo, R -- Sakai, S -- Sakrejda, I -- Sakuma, T -- Salur, S -- Sandweiss, J -- Sangaline, E -- Schambach, J -- Scharenberg, R P -- Schmitz, N -- Schuster, T R -- Seele, J -- Seger, J -- Selyuzhenkov, I -- Seyboth, P -- Shahaliev, E -- Shao, M -- Sharma, M -- Shi, S S -- Sichtermann, E P -- Simon, F -- Singaraju, R N -- Skoby, M J -- Smirnov, N -- Sorensen, P -- Sowinski, J -- Spinka, H M -- Srivastava, B -- Stanislaus, T D S -- Staszak, D -- Stevens, J R -- Stock, R -- Strikhanov, M -- Stringfellow, B -- Suaide, A A P -- Suarez, M C -- Subba, N L -- Sumbera, M -- Sun, X M -- Sun, Y -- Sun, Z -- Surrow, B -- Svirida, D N -- Symons, T J M -- Szanto de Toledo, A -- Takahashi, J -- Tang, A H -- Tang, Z -- Tarini, L H -- Tarnowsky, T -- Thein, D -- Thomas, J H -- Tian, J -- Timmins, A R -- Timoshenko, S -- Tlusty, D -- Tokarev, M -- Trainor, T A -- Tram, V N -- Trentalange, S -- Tribble, R E -- Tsai, O D -- Ulery, J -- Ullrich, T -- Underwood, D G -- Van Buren, G -- van Leeuwen, M -- van Nieuwenhuizen, G -- Vanfossen, J A Jr -- Varma, R -- Vasconcelos, G M S -- Vasiliev, A N -- Videbaek, F -- Viyogi, Y P -- Vokal, S -- Voloshin, S A -- Wada, M -- Walker, M -- Wang, F -- Wang, G -- Wang, H -- Wang, J S -- Wang, Q -- Wang, X L -- Wang, Y -- Webb, G -- Webb, J C -- Westfall, G D -- Whitten, C Jr -- Wieman, H -- Wingfield, E -- Wissink, S W -- Witt, R -- Wu, Y -- Xie, W -- Xu, H -- Xu, N -- Xu, Q H -- Xu, W -- Xu, Y -- Xu, Z -- Xue, L -- Yang, Y -- Yepes, P -- Yip, K -- Yoo, I-K -- Yue, Q -- Zawisza, M -- Zbroszczyk, H -- Zhan, W -- Zhang, J -- Zhang, S -- Zhang, W M -- Zhang, X P -- Zhang, Y -- Zhang, Z P -- Zhao, J -- Zhong, C -- Zhou, J -- Zhou, W -- Zhu, X -- Zhu, Y H -- Zoulkarneev, R -- Zoulkarneeva, Y -- New York, N.Y. -- Science. 2010 Apr 2;328(5974):58-62. doi: 10.1126/science.1183980. Epub 2010 Mar 4.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20203011" target="_blank"〉PubMed〈/a〉
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  • 8
    Publication Date: 2014-07-06
    Description: Supermassive black holes in the nuclei of active galaxies expel large amounts of matter through powerful winds of ionized gas. The archetypal active galaxy NGC 5548 has been studied for decades, and high-resolution x-ray and ultraviolet (UV) observations have previously shown a persistent ionized outflow. An observing campaign in 2013 with six space observatories shows the nucleus to be obscured by a long-lasting, clumpy stream of ionized gas not seen before. It blocks 90% of the soft x-ray emission and causes simultaneous deep, broad UV absorption troughs. The outflow velocities of this gas are up to five times faster than those in the persistent outflow, and, at a distance of only a few light days from the nucleus, it may likely originate from the accretion disk.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kaastra, J S -- Kriss, G A -- Cappi, M -- Mehdipour, M -- Petrucci, P-O -- Steenbrugge, K C -- Arav, N -- Behar, E -- Bianchi, S -- Boissay, R -- Branduardi-Raymont, G -- Chamberlain, C -- Costantini, E -- Ely, J C -- Ebrero, J -- Di Gesu, L -- Harrison, F A -- Kaspi, S -- Malzac, J -- De Marco, B -- Matt, G -- Nandra, K -- Paltani, S -- Person, R -- Peterson, B M -- Pinto, C -- Ponti, G -- Pozo Nunez, F -- De Rosa, A -- Seta, H -- Ursini, F -- de Vries, C P -- Walton, D J -- Whewell, M -- New York, N.Y. -- Science. 2014 Jul 4;345(6192):64-8. doi: 10.1126/science.1253787. Epub 2014 Jun 19.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, Netherlands. Department of Physics and Astronomy, Universiteit Utrecht, Post Office Box 80000, 3508 TA Utrecht, Netherlands. Leiden Observatory, Leiden University, Post Office Box 9513, 2300 RA Leiden, Netherlands. j.kaastra@sron.nl. ; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA. ; Istituto Nazionale di Astrofisica (INAF)-Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF) Bologna, Via Gobetti 101, I-40129 Bologna, Italy. ; SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, Netherlands. Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK. ; Universite Grenoble Alpes, Institut de Planetologie et d'Astrophysique de Grenoble (IPAG), F-38000 Grenoble, France. CNRS, IPAG, F-38000 Grenoble, France. ; Instituto de Astronomia, Universidad Catolica del Norte, Avenida Angamos 0610, Casilla 1280, Antofagasta, Chile. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK. ; Department of Physics, Virginia Tech, Blacksburg, VA 24061, USA. ; Department of Physics, Technion-Israel Institute of Technology, 32000 Haifa, Israel. ; Dipartimento di Matematica e Fisica, Universita degli Studi Roma Tre, via della Vasca Navale 84, 00146 Roma, Italy. ; Department of Astronomy, University of Geneva, 16 Chemin d'Ecogia, 1290 Versoix, Switzerland. ; Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK. ; SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, Netherlands. ; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. ; SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, Netherlands. European Space Astronomy Centre, Post Office Box 78, E-28691 Villanueva de la Canada, Madrid, Spain. ; Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA. ; Universite de Toulouse, Universite Paul Sabatier (UPS)-Observatoire Midi-Pyrenees (OMP), Institut de Recherche en Astrophysique et Planelogie (IRAP), Toulouse, France. CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France. ; Max-Planck-Institut fur extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching, Germany. ; 22 Impasse du Bois Joli, 74410 St. Jorioz, France. ; Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA. Center for Cosmology and AstroParticle Physics, Ohio State University, 191 West Woodruff Avenue, Columbus, OH 43210, USA. ; Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK. ; Astronomisches Institut, Ruhr-Universitat Bochum, Universitatsstrasse 150, 44801, Bochum, Germany. ; INAF/Istituto di Astrofisica e Planetologia Spaziali, Via Fosso del Cavaliere 100, I-00133 Roma, Italy. ; Research Center for Measurement in Advanced Science, Faculty of Science, Rikkyo University 3-34-1 Nishi-Ikebukuro, Toshima-ku, Tokyo, Japan. Department of Physics, Saitama University, 255 Shimo-Okubo, Sakura-ku, Saitama 338-8570, Japan.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24994647" target="_blank"〉PubMed〈/a〉
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  • 9
    Publication Date: 2010-01-16
    Description: We report here genome sequences and comparative analyses of three closely related parasitoid wasps: Nasonia vitripennis, N. giraulti, and N. longicornis. Parasitoids are important regulators of arthropod populations, including major agricultural pests and disease vectors, and Nasonia is an emerging genetic model, particularly for evolutionary and developmental genetics. Key findings include the identification of a functional DNA methylation tool kit; hymenopteran-specific genes including diverse venoms; lateral gene transfers among Pox viruses, Wolbachia, and Nasonia; and the rapid evolution of genes involved in nuclear-mitochondrial interactions that are implicated in speciation. Newly developed genome resources advance Nasonia for genetic research, accelerate mapping and cloning of quantitative trait loci, and will ultimately provide tools and knowledge for further increasing the utility of parasitoids as pest insect-control agents.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2849982/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2849982/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Werren, John H -- Richards, Stephen -- Desjardins, Christopher A -- Niehuis, Oliver -- Gadau, Jurgen -- Colbourne, John K -- Nasonia Genome Working Group -- Beukeboom, Leo W -- Desplan, Claude -- Elsik, Christine G -- Grimmelikhuijzen, Cornelis J P -- Kitts, Paul -- Lynch, Jeremy A -- Murphy, Terence -- Oliveira, Deodoro C S G -- Smith, Christopher D -- van de Zande, Louis -- Worley, Kim C -- Zdobnov, Evgeny M -- Aerts, Maarten -- Albert, Stefan -- Anaya, Victor H -- Anzola, Juan M -- Barchuk, Angel R -- Behura, Susanta K -- Bera, Agata N -- Berenbaum, May R -- Bertossa, Rinaldo C -- Bitondi, Marcia M G -- Bordenstein, Seth R -- Bork, Peer -- Bornberg-Bauer, Erich -- Brunain, Marleen -- Cazzamali, Giuseppe -- Chaboub, Lesley -- Chacko, Joseph -- Chavez, Dean -- Childers, Christopher P -- Choi, Jeong-Hyeon -- Clark, Michael E -- Claudianos, Charles -- Clinton, Rochelle A -- Cree, Andrew G -- Cristino, Alexandre S -- Dang, Phat M -- Darby, Alistair C -- de Graaf, Dirk C -- Devreese, Bart -- Dinh, Huyen H -- Edwards, Rachel -- Elango, Navin -- Elhaik, Eran -- Ermolaeva, Olga -- Evans, Jay D -- Foret, Sylvain -- Fowler, Gerald R -- Gerlach, Daniel -- Gibson, Joshua D -- Gilbert, Donald G -- Graur, Dan -- Grunder, Stefan -- Hagen, Darren E -- Han, Yi -- Hauser, Frank -- Hultmark, Da -- Hunter, Henry C 4th -- Hurst, Gregory D D -- Jhangian, Shalini N -- Jiang, Huaiyang -- Johnson, Reed M -- Jones, Andrew K -- Junier, Thomas -- Kadowaki, Tatsuhiko -- Kamping, Albert -- Kapustin, Yuri -- Kechavarzi, Bobak -- Kim, Jaebum -- Kim, Jay -- Kiryutin, Boris -- Koevoets, Tosca -- Kovar, Christie L -- Kriventseva, Evgenia V -- Kucharski, Robert -- Lee, Heewook -- Lee, Sandra L -- Lees, Kristin -- Lewis, Lora R -- Loehlin, David W -- Logsdon, John M Jr -- Lopez, Jacqueline A -- Lozado, Ryan J -- Maglott, Donna -- Maleszka, Ryszard -- Mayampurath, Anoop -- Mazur, Danielle J -- McClure, Marcella A -- Moore, Andrew D -- Morgan, Margaret B -- Muller, Jean -- Munoz-Torres, Monica C -- Muzny, Donna M -- Nazareth, Lynne V -- Neupert, Susanne -- Nguyen, Ngoc B -- Nunes, Francis M F -- Oakeshott, John G -- Okwuonu, Geoffrey O -- Pannebakker, Bart A -- Pejaver, Vikas R -- Peng, Zuogang -- Pratt, Stephen C -- Predel, Reinhard -- Pu, Ling-Ling -- Ranson, Hilary -- Raychoudhury, Rhitoban -- Rechtsteiner, Andreas -- Reese, Justin T -- Reid, Jeffrey G -- Riddle, Megan -- Robertson, Hugh M -- Romero-Severson, Jeanne -- Rosenberg, Miriam -- Sackton, Timothy B -- Sattelle, David B -- Schluns, Helge -- Schmitt, Thomas -- Schneider, Martina -- Schuler, Andreas -- Schurko, Andrew M -- Shuker, David M -- Simoes, Zila L P -- Sinha, Saurabh -- Smith, Zachary -- Solovyev, Victor -- Souvorov, Alexandre -- Springauf, Andreas -- Stafflinger, Elisabeth -- Stage, Deborah E -- Stanke, Mario -- Tanaka, Yoshiaki -- Telschow, Arndt -- Trent, Carol -- Vattathil, Selina -- Verhulst, Eveline C -- Viljakainen, Lumi -- Wanner, Kevin W -- Waterhouse, Robert M -- Whitfield, James B -- Wilkes, Timothy E -- Williamson, Michael -- Willis, Judith H -- Wolschin, Florian -- Wyder, Stefan -- Yamada, Takuji -- Yi, Soojin V -- Zecher, Courtney N -- Zhang, Lan -- Gibbs, Richard A -- 5R01GM070026-04/GM/NIGMS NIH HHS/ -- 5R01HG000747-14/HG/NHGRI NIH HHS/ -- 5R24GM084917-02/GM/NIGMS NIH HHS/ -- AI028309-13A2/AI/NIAID NIH HHS/ -- R01 AI055624/AI/NIAID NIH HHS/ -- R01 GM064864/GM/NIGMS NIH HHS/ -- R01 GM064864-04/GM/NIGMS NIH HHS/ -- R01 GM064864-05A2/GM/NIGMS NIH HHS/ -- R01 GM070026/GM/NIGMS NIH HHS/ -- R01 GM070026-04S1/GM/NIGMS NIH HHS/ -- R01 GM079484/GM/NIGMS NIH HHS/ -- R01 GM085163/GM/NIGMS NIH HHS/ -- R01 GM085163-01/GM/NIGMS NIH HHS/ -- R01 GM085233/GM/NIGMS NIH HHS/ -- R01 HG000747/HG/NHGRI NIH HHS/ -- R01 HG000747-14/HG/NHGRI NIH HHS/ -- R01GM064864/GM/NIGMS NIH HHS/ -- R24 GM084917/GM/NIGMS NIH HHS/ -- R24 GM084917-01/GM/NIGMS NIH HHS/ -- R24 GM084917-02/GM/NIGMS NIH HHS/ -- U54 HG003273/HG/NHGRI NIH HHS/ -- U54 HG003273-03/HG/NHGRI NIH HHS/ -- Intramural NIH HHS/ -- New York, N.Y. -- Science. 2010 Jan 15;327(5963):343-8. doi: 10.1126/science.1178028.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20075255" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Arthropods/parasitology ; *Biological Evolution ; DNA Methylation ; DNA Transposable Elements ; Female ; Gene Transfer, Horizontal ; Genes, Insect ; Genetic Speciation ; Genetic Variation ; *Genome, Insect ; Host-Parasite Interactions ; Insect Proteins/genetics/metabolism ; Insect Viruses/genetics ; Insects/genetics ; Male ; Molecular Sequence Data ; Quantitative Trait Loci ; Recombination, Genetic ; Sequence Analysis, DNA ; Wasp Venoms/chemistry/toxicity ; Wasps/*genetics/physiology ; Wolbachia/genetics
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 10
    Publication Date: 2010-04-03
    Description: The Fermi Gamma-ray Space Telescope has detected the gamma-ray glow emanating from the giant radio lobes of the radio galaxy Centaurus A. The resolved gamma-ray image shows the lobes clearly separated from the central active source. In contrast to all other active galaxies detected so far in high-energy gamma-rays, the lobe flux constitutes a considerable portion (greater than one-half) of the total source emission. The gamma-ray emission from the lobes is interpreted as inverse Compton-scattered relic radiation from the cosmic microwave background, with additional contribution at higher energies from the infrared-to-optical extragalactic background light. These measurements provide gamma-ray constraints on the magnetic field and particle energy content in radio galaxy lobes, as well as a promising method to probe the cosmic relic photon fields.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Fermi-LAT Collaboration -- Abdo, A A -- Ackermann, M -- Ajello, M -- Atwood, W B -- Baldini, L -- Ballet, J -- Barbiellini, G -- Bastieri, D -- Baughman, B M -- Bechtol, K -- Bellazzini, R -- Berenji, B -- Blandford, R D -- Bloom, E D -- Bonamente, E -- Borgland, A W -- Bregeon, J -- Brez, A -- Brigida, M -- Bruel, P -- Burnett, T H -- Buson, S -- Caliandro, G A -- Cameron, R A -- Caraveo, P A -- Casandjian, J M -- Cavazzuti, E -- Cecchi, C -- Celik, O -- Chekhtman, A -- Cheung, C C -- Chiang, J -- Ciprini, S -- Claus, R -- Cohen-Tanugi, J -- Colafrancesco, S -- Cominsky, L R -- Conrad, J -- Costamante, L -- Cutini, S -- Davis, D S -- Dermer, C D -- de Angelis, A -- de Palma, F -- Digel, S W -- do Couto e Silva, E -- Drell, P S -- Dubois, R -- Dumora, D -- Farnier, C -- Favuzzi, C -- Fegan, S J -- Finke, J -- Focke, W B -- Fortin, P -- Fukazawa, Y -- Funk, S -- Fusco, P -- Gargano, F -- Gasparrini, D -- Gehrels, N -- Georganopoulos, M -- Germani, S -- Giebels, B -- Giglietto, N -- Giordano, F -- Giroletti, M -- Glanzman, T -- Godfrey, G -- Grenier, I A -- Grove, J E -- Guillemot, L -- Guiriec, S -- Hanabata, Y -- Harding, A K -- Hayashida, M -- Hays, E -- Hughes, R E -- Jackson, M S -- Johannesson, G -- Johnson, A S -- Johnson, T J -- Johnson, W N -- Kamae, T -- Katagiri, H -- Kataoka, J -- Kawai, N -- Kerr, M -- Knodlseder, J -- Kocian, M L -- Kuss, M -- Lande, J -- Latronico, L -- Lemoine-Goumard, M -- Longo, F -- Loparco, F -- Lott, B -- Lovellette, M N -- Lubrano, P -- Madejski, G M -- Makeev, A -- Mazziotta, M N -- McConville, W -- McEnery, J E -- Meurer, C -- Michelson, P F -- Mitthumsiri, W -- Mizuno, T -- Moiseev, A A -- Monte, C -- Monzani, M E -- Morselli, A -- Moskalenko, I V -- Murgia, S -- Nolan, P L -- Norris, J P -- Nuss, E -- Ohsugi, T -- Omodei, N -- Orlando, E -- Ormes, J F -- Paneque, D -- Parent, D -- Pelassa, V -- Pepe, M -- Pesce-Rollins, M -- Piron, F -- Porter, T A -- Raino, S -- Rando, R -- Razzano, M -- Razzaque, S -- Reimer, A -- Reimer, O -- Reposeur, T -- Ritz, S -- Rochester, L S -- Rodriguez, A Y -- Romani, R W -- Roth, M -- Ryde, F -- Sadrozinski, H F-W -- Sambruna, R -- Sanchez, D -- Sander, A -- Saz Parkinson, P M -- Scargle, J D -- Sgro, C -- Siskind, E J -- Smith, D A -- Smith, P D -- Spandre, G -- Spinelli, P -- Starck, J-L -- Stawarz, L -- Strickman, M S -- Suson, D J -- Tajima, H -- Takahashi, H -- Takahashi, T -- Tanaka, T -- Thayer, J B -- Thayer, J G -- Thompson, D J -- Tibaldo, L -- Torres, D F -- Tosti, G -- Tramacere, A -- Uchiyama, Y -- Usher, T L -- Vasileiou, V -- Vilchez, N -- Vitale, V -- Waite, A P -- Wallace, E -- Wang, P -- Winer, B L -- Wood, K S -- Ylinen, T -- Ziegler, M -- Hardcastle, M J -- Kazanas, D -- New York, N.Y. -- Science. 2010 May 7;328(5979):725-9. doi: 10.1126/science.1184656. Epub 2010 Apr 1.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20360067" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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