TY - JOUR A1 - Abeysekara, A. U. A1 - Benbow, Wystan A1 - Bird, Ralph A1 - Brill, A. A1 - Brose, Robert A1 - Buckley, J. H. A1 - Chromey, A. J. A1 - Daniel, M. K. A1 - Falcone, A. A1 - Finley, J. P. A1 - Fortson, L. A1 - Furniss, Amy A1 - Gent, A. A1 - Gillanders, Gerald H. A1 - Hanna, David A1 - Hassan, T. A1 - Hervet, O. A1 - Holder, J. A1 - Hughes, G. A1 - Humensky, T. B. A1 - Kaaret, Philip A1 - Kar, P. A1 - Kertzman, M. A1 - Kieda, David A1 - Krause, Maria A1 - Krennrich, F. A1 - Kumar, S. A1 - Lang, M. J. A1 - Lin, T. T. Y. A1 - Maier, Gernot A1 - Moriarty, P. A1 - Mukherjee, Reshmi A1 - Ong, R. A. A1 - Otte, Adam Nepomuk A1 - Park, Nahee A1 - Petrashyk, A. A1 - Pohl, Martin A1 - Pueschel, Elisa A1 - Quinn, J. A1 - Ragan, K. A1 - Richards, Gregory T. A1 - Roache, E. A1 - Sadeh, I. A1 - Santander, Marcos A1 - Schlenstedt, S. A1 - Sembroski, G. H. A1 - Sushch, Iurii A1 - Tyler, J. A1 - Vassiliev, V. V. A1 - Wakely, S. P. A1 - Weinstein, A. A1 - Wells, R. M. A1 - Wilcox, P. A1 - Wilhelm, Alina A1 - Williams, David A. A1 - Williamson, T. J. A1 - Zitzer, B. A1 - Acciari, V. A. A1 - Ansoldi, S. A1 - Antonelli, L. A. A1 - Engels, A. Arbet A1 - Baack, D. A1 - Babic, A. A1 - Banerjee, B. A1 - de Almeida, U. Barres A1 - Barrio, J. A. A1 - Becerra Gonzalez, Josefa A1 - Bednarek, Wlodek A1 - Bernardini, Elisa A1 - Berti, A. A1 - Besenrieder, J. A1 - Bhattacharyya, W. A1 - Bigongiari, C. A1 - Biland, A. A1 - Blanch, O. A1 - Bonnoli, G. A1 - Busetto, G. A1 - Carosi, R. A1 - Ceribella, G. A1 - Cikota, S. A1 - Colak, S. M. A1 - Colin, P. A1 - Colombo, E. A1 - Contreras, J. L. A1 - Cortina, J. A1 - Covino, S. A1 - Da Vela, P. A1 - Dazzi, F. A1 - De Angelis, A. A1 - De Lotto, B. A1 - Delfino, M. A1 - Delgado, J. A1 - Di Pierro, F. A1 - Do Souto Espinera, E. A1 - Dominguez, A. A1 - Prester, D. Dominis A1 - Dorner, D. A1 - Doro, M. A1 - Einecke, S. A1 - Elsaesser, D. A1 - Ramazani, V. Fallah A1 - Fattorini, A. A1 - Fernandez-Barral, A. A1 - Ferrara, G. A1 - Fidalgo, D. A1 - Foffano, L. A1 - Fonseca, M. V. A1 - Font, L. A1 - Fruck, C. A1 - Galindo, D. A1 - Gallozzi, S. A1 - Lopez, R. J. Garcia A1 - Garczarczyk, M. A1 - Gasparyan, S. A1 - Gaug, Markus A1 - Giammaria, P. A1 - Godinovic, N. A1 - Guberman, D. A1 - Hadasch, D. A1 - Hahn, A. A1 - Herrera, J. A1 - Hoang, J. A1 - Hrupec, D. A1 - Inoue, S. A1 - Ishio, K. A1 - Iwamura, Y. A1 - Kubo, H. A1 - Kushida, J. A1 - Kuvezdic, D. A1 - Lamastra, A. A1 - Lelas, D. A1 - Leone, Francesco A1 - Lindfors, E. A1 - Lombardi, S. A1 - Longo, Francesco A1 - Lopez, M. A1 - Lopez-Oramas, A. A1 - Machado de Oliveira Fraga, B. A1 - Maggio, C. A1 - Majumdar, P. A1 - Makariev, M. A1 - Mallamaci, M. A1 - Maneva, G. A1 - Manganaro, M. A1 - Mannheim, K. A1 - Maraschi, L. A1 - Mariotti, M. A1 - Martinez, M. A1 - Masuda, S. A1 - Mazin, D. A1 - Minev, M. A1 - Miranda, J. M. A1 - Mirzoyan, R. A1 - Molina, E. A1 - Moralejo, A. A1 - Moreno, V. A1 - Moretti, E. A1 - Munar-Adrover, Pere A1 - Neustroev, V. A1 - Niedzwiecki, Andrzej A1 - Rosillo, Mireia Nievas A1 - Nigro, C. A1 - Nilsson, Kari A1 - Ninci, D. A1 - Nishijima, K. A1 - Noda, K. A1 - Nogues, L. A1 - Noethe, M. A1 - Paiano, Simona A1 - Palacio, J. A1 - Paneque, D. A1 - Paoletti, R. A1 - Paredes, J. M. A1 - Pedaletti, G. A1 - Penil, P. A1 - Peresano, M. A1 - Persic, M. A1 - Moroni, P. G. Prada A1 - Prandini, E. A1 - Puljak, I. A1 - Garcia, J. R. A1 - Rhode, W. A1 - Ribo, Marc A1 - Rico, J. A1 - Righi, C. A1 - Rugliancich, A. A1 - Saha, Lab A1 - Sahakyan, Narek A1 - Saito, T. A1 - Satalecka, K. A1 - Schweizer, T. A1 - Sitarek, J. A1 - Snidaric, I. A1 - Sobczynska, D. A1 - Somero, A. A1 - Stamerra, A. A1 - Strzys, M. A1 - Suric, T. A1 - Tavecchio, Fabrizio A1 - Temnikov, P. A1 - Terzic, T. A1 - Teshima, M. A1 - Torres-Alba, N. A1 - Tsujimoto, S. A1 - van Scherpenberg, J. A1 - Vanzo, G. A1 - Vazquez Acosta, M. A1 - Vovk, I. A1 - Will, M. A1 - Zaric, D. T1 - Periastron Observations of TeV Gamma-Ray Emission from a Binary System with a 50-year Period JF - The astrophysical journal : an international review of spectroscopy and astronomical physics ; Part 2, Letters N2 - We report on observations of the pulsar/Be star binary system PSR J2032+4127/MT91 213 in the energy range between 100 GeV and 20 TeV with the Very Energetic Radiation Imaging Telescope Array and Major Atmospheric Gamma Imaging Cherenkov telescope arrays. The binary orbit has a period of approximately 50 years, with the most recent periastron occurring on 2017 November 13. Our observations span from 18 months prior to periastron to one month after. A new point-like gamma-ray source is detected, coincident with the location of PSR J2032+4127/MT91 213. The gamma-ray light curve and spectrum are well characterized over the periastron passage. The flux is variable over at least an order of magnitude, peaking at periastron, thus providing a firm association of the TeV source with the pulsar/Be star system. Observations prior to periastron show a cutoff in the spectrum at an energy around 0.5 TeV. This result adds a new member to the small population of known TeV binaries, and it identifies only the second source of this class in which the nature and properties of the compact object are firmly established. We compare the gamma-ray results with the light curve measured with the X-ray Telescope on board the Neil Gehrels Swift Observatory and with the predictions of recent theoretical models of the system. We conclude that significant revision of the models is required to explain the details of the emission that we have observed, and we discuss the relationship between the binary system and the overlapping steady extended source, TeV J2032+4130. KW - gamma rays: general KW - pulsars: individual (PSR J2032+4127, VER J2032+414, MAGIC J2032+4127) KW - stars: individual (MT91 213) KW - X-rays: binaries Y1 - 2018 U6 - https://doi.org/10.3847/2041-8213/aae70e SN - 2041-8205 SN - 2041-8213 VL - 867 IS - 1 PB - IOP Publ. Ltd. CY - Bristol ER - TY - JOUR A1 - Horikoshi, Momoko A1 - Yaghootkar, Hanieh A1 - Mook-Kanamori, Dennis O. A1 - Sovio, Ulla A1 - Taal, H. Rob A1 - Hennig, Branwen J. A1 - Bradfield, Jonathan P. A1 - St Pourcain, Beate A1 - Evans, David M. A1 - Charoen, Pimphen A1 - Kaakinen, Marika A1 - Cousminer, Diana L. A1 - Lehtimaki, Terho A1 - Kreiner-Moller, Eskil A1 - Warrington, Nicole M. A1 - Bustamante, Mariona A1 - Feenstra, Bjarke A1 - Berry, Diane J. A1 - Thiering, Elisabeth A1 - Pfab, Thiemo A1 - Barton, Sheila J. A1 - Shields, Beverley M. A1 - Kerkhof, Marjan A1 - van Leeuwen, Elisabeth M. A1 - Fulford, Anthony J. A1 - Kutalik, Zoltan A1 - Zhao, Jing Hua A1 - den Hoed, Marcel A1 - Mahajan, Anubha A1 - Lindi, Virpi A1 - Goh, Liang-Kee A1 - Hottenga, Jouke-Jan A1 - Wu, Ying A1 - Raitakari, Olli T. A1 - Harder, Marie N. A1 - Meirhaeghe, Aline A1 - Ntalla, Ioanna A1 - Salem, Rany M. A1 - Jameson, Karen A. A1 - Zhou, Kaixin A1 - Monies, Dorota M. A1 - Lagou, Vasiliki A1 - Kirin, Mirna A1 - Heikkinen, Jani A1 - Adair, Linda S. A1 - Alkuraya, Fowzan S. A1 - Al-Odaib, Ali A1 - Amouyel, Philippe A1 - Andersson, Ehm Astrid A1 - Bennett, Amanda J. A1 - Blakemore, Alexandra I. F. A1 - Buxton, Jessica L. A1 - Dallongeville, Jean A1 - Das, Shikta A1 - de Geus, Eco J. C. A1 - Estivill, Xavier A1 - Flexeder, Claudia A1 - Froguel, Philippe A1 - Geller, Frank A1 - Godfrey, Keith M. A1 - Gottrand, Frederic A1 - Groves, Christopher J. A1 - Hansen, Torben A1 - Hirschhorn, Joel N. A1 - Hofman, Albert A1 - Hollegaard, Mads V. A1 - Hougaard, David M. A1 - Hyppoenen, Elina A1 - Inskip, Hazel M. A1 - Isaacs, Aaron A1 - Jorgensen, Torben A1 - Kanaka-Gantenbein, Christina A1 - Kemp, John P. A1 - Kiess, Wieland A1 - Kilpelainen, Tuomas O. A1 - Klopp, Norman A1 - Knight, Bridget A. A1 - Kuzawa, Christopher W. A1 - McMahon, George A1 - Newnham, John P. A1 - Niinikoski, Harri A1 - Oostra, Ben A. A1 - Pedersen, Louise A1 - Postma, Dirkje S. A1 - Ring, Susan M. A1 - Rivadeneira, Fernando A1 - Robertson, Neil R. A1 - Sebert, Sylvain A1 - Simell, Olli A1 - Slowinski, Torsten A1 - Tiesler, Carla M. T. A1 - Toenjes, Anke A1 - Vaag, Allan A1 - Viikari, Jorma S. A1 - Vink, Jacqueline M. A1 - Vissing, Nadja Hawwa A1 - Wareham, Nicholas J. A1 - Willemsen, Gonneke A1 - Witte, Daniel R. A1 - Zhang, Haitao A1 - Zhao, Jianhua A1 - Wilson, James F. A1 - Stumvoll, Michael A1 - Prentice, Andrew M. A1 - Meyer, Brian F. A1 - Pearson, Ewan R. A1 - Boreham, Colin A. G. A1 - Cooper, Cyrus A1 - Gillman, Matthew W. A1 - Dedoussis, George V. A1 - Moreno, Luis A. A1 - Pedersen, Oluf A1 - Saarinen, Maiju A1 - Mohlke, Karen L. A1 - Boomsma, Dorret I. A1 - Saw, Seang-Mei A1 - Lakka, Timo A. A1 - Koerner, Antje A1 - Loos, Ruth J. F. A1 - Ong, Ken K. A1 - Vollenweider, Peter A1 - van Duijn, Cornelia M. A1 - Koppelman, Gerard H. A1 - Hattersley, Andrew T. A1 - Holloway, John W. A1 - Hocher, Berthold A1 - Heinrich, Joachim A1 - Power, Chris A1 - Melbye, Mads A1 - Guxens, Monica A1 - Pennell, Craig E. A1 - Bonnelykke, Klaus A1 - Bisgaard, Hans A1 - Eriksson, Johan G. A1 - Widen, Elisabeth A1 - Hakonarson, Hakon A1 - Uitterlinden, Andre G. A1 - Pouta, Anneli A1 - Lawlor, Debbie A. A1 - Smith, George Davey A1 - Frayling, Timothy M. A1 - McCarthy, Mark I. A1 - Grant, Struan F. A. A1 - Jaddoe, Vincent W. V. A1 - Jarvelin, Marjo-Riitta A1 - Timpson, Nicholas J. A1 - Prokopenko, Inga A1 - Freathy, Rachel M. T1 - New loci associated with birth weight identify genetic links between intrauterine growth and adult height and metabolism JF - Nature genetics N2 - Birth weight within the normal range is associated with a variety of adult-onset diseases, but the mechanisms behind these associations are poorly understood(1). Previous genome-wide association studies of birth weight identified a variant in the ADCY5 gene associated both with birth weight and type 2 diabetes and a second variant, near CCNL1, with no obvious link to adult traits(2). In an expanded genome-wide association metaanalysis and follow-up study of birth weight (of up to 69,308 individuals of European descent from 43 studies), we have now extended the number of loci associated at genome-wide significance to 7, accounting for a similar proportion of variance as maternal smoking. Five of the loci are known to be associated with other phenotypes: ADCY5 and CDKAL1 with type 2 diabetes, ADRB1 with adult blood pressure and HMGA2 and LCORL with adult height. Our findings highlight genetic links between fetal growth and postnatal growth and metabolism. Y1 - 2013 U6 - https://doi.org/10.1038/ng.2477 SN - 1061-4036 VL - 45 IS - 1 SP - 76 EP - U115 PB - Nature Publ. Group CY - New York ER - TY - JOUR A1 - Beaulieu, Jean-Philippe A1 - Bennett, David P. A1 - Fouqué, Pascal A1 - Williams, Andrew A1 - Dominik, Martin A1 - Jorgensen, Uffe Grae A1 - Kubas, Daniel A1 - Cassan, Arnaud A1 - Coutures, Christian A1 - Greenhill, John A1 - Hill, Kym A1 - Menzies, John A1 - Sackett, Penny D. A1 - Albrow, Michael D. A1 - Brillant, Stephane A1 - Caldwell, John A. R. A1 - Calitz, Johannes Jacobus A1 - Cook, Kem H. A1 - Corrales Cosmeli, Esperanza de Santa Cecilia A1 - Desort, Morgan A1 - Dieters, Stefan A1 - Dominis, Dijana A1 - Donatowicz, Jadzia A1 - Hoffman, Martie A1 - Kane, Stephen R. A1 - Marquette, Jean-Baptiste A1 - Martin, Ralph A1 - Meintjes, Pieter A1 - Pollard, Karen R. A1 - Sahu, Kailash C. A1 - Vinter, Christian A1 - Wambsganss, Joachim A1 - Woller, Kristian A1 - Horne, Keith A1 - Steele, Iain A1 - Bramich, Daniel M. A1 - Burgdorf, Martin A1 - Snodgrass, Colin A1 - Bode, Mike A1 - Udalski, Andr T1 - Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing N2 - In the favoured core-accretion model of formation of planetary systems, solid planetesimals accumulate to build up planetary cores, which then accrete nebular gas if they are sufficiently massive. Around M-dwarf stars ( the most common stars in our Galaxy), this model favours the formation of Earth-mass (M+) to Neptune-mass planets with orbital radii of 1 to 10 astronomical units (AU), which is consistent with the small number of gas giant planets known to orbit M-dwarf host stars(1-4). More than 170 extrasolar planets have been discovered with a wide range of masses and orbital periods, but planets of Neptune's mass or less have not hitherto been detected at separations of more than 0.15 AU from normal stars. Here we report the discovery of a 5.5(-2.7)(+5.5)M(+) planetary companion at a separation of 2.6(- 0.6)(+1.5) AU from a 0.22(-0.11)(+0.21)M(.) M-dwarf star, where M-. refers to a solar mass. (We propose to name it OGLE- 2005-BLG-390Lb, indicating a planetary mass companion to the lens star of the microlensing event.) The mass is lower than that of GJ876d (ref. 5), although the error bars overlap. Our detection suggests that such cool, sub-Neptune-mass planets may be more common than gas giant planets, as predicted by the core accretion theory. Y1 - 2006 UR - http://www.nature.com/nature/ U6 - https://doi.org/10.1038/Nature04441 SN - 0028-0836 ER - TY - JOUR A1 - Steffen, Will A1 - Röckstrom, Johan A1 - Richardson, Katherine A1 - Lenton, Timothy M. A1 - Folke, Carl A1 - Liverman, Diana A1 - Summerhayes, Colin P. A1 - Barnosky, Anthony D. A1 - Cornell, Sarah E. A1 - Crucifix, Michel A1 - Donges, Jonathan A1 - Fetzer, Ingo A1 - Lade, Steven J. A1 - Scheffer, Marten A1 - Winkelmann, Ricarda A1 - Schellnhuber, Hans Joachim T1 - Trajectories of the Earth System in the Anthropocene JF - Proceedings of the National Academy of Sciences of the United States of America N2 - We explore the risk that self-reinforcing feedbacks could push the Earth System toward a planetary threshold that, if crossed, could prevent stabilization of the climate at intermediate temperature rises and cause continued warming on a "Hothouse Earth" pathway even as human emissions are reduced. Crossing the threshold would lead to a much higher global average temperature than any interglacial in the past 1.2 million years and to sea levels significantly higher than at any time in the Holocene. We examine the evidence that such a threshold might exist and where it might be. If the threshold is crossed, the resulting trajectory would likely cause serious disruptions to ecosystems, society, and economies. Collective human action is required to steer the Earth System away from a potential threshold and stabilize it in a habitable interglacial-like state. Such action entails stewardship of the entire Earth System-biosphere, climate, and societies-and could include decarbonization of the global economy, enhancement of biosphere carbon sinks, behavioral changes, technological innovations, new governance arrangements, and transformed social values. KW - Earth System trajectories KW - climate change KW - Anthropocene KW - biosphere feedbacks KW - tipping elements Y1 - 2018 U6 - https://doi.org/10.1073/pnas.1810141115 SN - 0027-8424 VL - 115 IS - 33 SP - 8252 EP - 8259 PB - National Acad. of Sciences CY - Washington ER -