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  • 1
    Publication Date: 2009-04-11
    Description: Submillimetre surveys during the past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies. In the redshift range 1 〈or= z 〈or= 4, these massive submillimetre galaxies go through a phase characterized by optically obscured star formation at rates several hundred times that in the local Universe. Half of the starlight from this highly energetic process is absorbed and thermally re-radiated by clouds of dust at temperatures near 30 K with spectral energy distributions peaking at 100 microm in the rest frame. At 1 〈or= z 〈or= 4, the peak is redshifted to wavelengths between 200 and 500 microm. The cumulative effect of these galaxies is to yield extragalactic optical and far-infrared backgrounds with approximately equal energy densities. Since the initial detection of the far-infrared background (FIRB), higher-resolution experiments have sought to decompose this integrated radiation into the contributions from individual galaxies. Here we report the results of an extragalactic survey at 250, 350 and 500 microm. Combining our results at 500 microm with those at 24 microm, we determine that all of the FIRB comes from individual galaxies, with galaxies at z 〉or= 1.2 accounting for 70% of it. As expected, at the longest wavelengths the signal is dominated by ultraluminous galaxies at z 〉 1.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Devlin, Mark J -- Ade, Peter A R -- Aretxaga, Itziar -- Bock, James J -- Chapin, Edward L -- Griffin, Matthew -- Gundersen, Joshua O -- Halpern, Mark -- Hargrave, Peter C -- Hughes, David H -- Klein, Jeff -- Marsden, Gaelen -- Martin, Peter G -- Mauskopf, Philip -- Moncelsi, Lorenzo -- Netterfield, Calvin B -- Ngo, Henry -- Olmi, Luca -- Pascale, Enzo -- Patanchon, Guillaume -- Rex, Marie -- Scott, Douglas -- Semisch, Christopher -- Thomas, Nicholas -- Truch, Matthew D P -- Tucker, Carole -- Tucker, Gregory S -- Viero, Marco P -- Wiebe, Donald V -- England -- Nature. 2009 Apr 9;458(7239):737-9. doi: 10.1038/nature07918.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, Pennsylvania 19104, USA. devlin@physics.upenn.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19360081" target="_blank"〉PubMed〈/a〉
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  • 2
    Publication Date: 2013-04-20
    Description: Massive present-day early-type (elliptical and lenticular) galaxies probably gained the bulk of their stellar mass and heavy elements through intense, dust-enshrouded starbursts--that is, increased rates of star formation--in the most massive dark-matter haloes at early epochs. However, it remains unknown how soon after the Big Bang massive starburst progenitors exist. The measured redshift (z) distribution of dusty, massive starbursts has long been suspected to be biased low in z owing to selection effects, as confirmed by recent findings of systems with redshifts as high as ~5 (refs 2-4). Here we report the identification of a massive starburst galaxy at z = 6.34 through a submillimetre colour-selection technique. We unambiguously determined the redshift from a suite of molecular and atomic fine-structure cooling lines. These measurements reveal a hundred billion solar masses of highly excited, chemically evolved interstellar medium in this galaxy, which constitutes at least 40 per cent of the baryonic mass. A 'maximum starburst' converts the gas into stars at a rate more than 2,000 times that of the Milky Way, a rate among the highest observed at any epoch. Despite the overall downturn in cosmic star formation towards the highest redshifts, it seems that environments mature enough to form the most massive, intense starbursts existed at least as early as 880 million years after the Big Bang.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Riechers, Dominik A -- Bradford, C M -- Clements, D L -- Dowell, C D -- Perez-Fournon, I -- Ivison, R J -- Bridge, C -- Conley, A -- Fu, Hai -- Vieira, J D -- Wardlow, J -- Calanog, J -- Cooray, A -- Hurley, P -- Neri, R -- Kamenetzky, J -- Aguirre, J E -- Altieri, B -- Arumugam, V -- Benford, D J -- Bethermin, M -- Bock, J -- Burgarella, D -- Cabrera-Lavers, A -- Chapman, S C -- Cox, P -- Dunlop, J S -- Earle, L -- Farrah, D -- Ferrero, P -- Franceschini, A -- Gavazzi, R -- Glenn, J -- Solares, E A Gonzalez -- Gurwell, M A -- Halpern, M -- Hatziminaoglou, E -- Hyde, A -- Ibar, E -- Kovacs, A -- Krips, M -- Lupu, R E -- Maloney, P R -- Martinez-Navajas, P -- Matsuhara, H -- Murphy, E J -- Naylor, B J -- Nguyen, H T -- Oliver, S J -- Omont, A -- Page, M J -- Petitpas, G -- Rangwala, N -- Roseboom, I G -- Scott, D -- Smith, A J -- Staguhn, J G -- Streblyanska, A -- Thomson, A P -- Valtchanov, I -- Viero, M -- Wang, L -- Zemcov, M -- Zmuidzinas, J -- England -- Nature. 2013 Apr 18;496(7445):329-33. doi: 10.1038/nature12050.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉California Institute of Technology, 1200 East California Boulevard, MC 249-17, Pasadena, California 91125, USA. dr@astro.cornell.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23598341" target="_blank"〉PubMed〈/a〉
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  • 3
    Publication Date: 2014-02-11
    Description: The reorganization of patterns of species diversity driven by anthropogenic climate change, and the consequences for humans, are not yet fully understood or appreciated. Nevertheless, changes in climate conditions are useful for predicting shifts in species distributions at global and local scales. Here we use the velocity of climate change to derive spatial trajectories for climatic niches from 1960 to 2009 (ref. 7) and from 2006 to 2100, and use the properties of these trajectories to infer changes in species distributions. Coastlines act as barriers and locally cooler areas act as attractors for trajectories, creating source and sink areas for local climatic conditions. Climate source areas indicate where locally novel conditions are not connected to areas where similar climates previously occurred, and are thereby inaccessible to climate migrants tracking isotherms: 16% of global surface area for 1960 to 2009, and 34% of ocean for the 'business as usual' climate scenario (representative concentration pathway (RCP) 8.5) representing continued use of fossil fuels without mitigation. Climate sink areas are where climate conditions locally disappear, potentially blocking the movement of climate migrants. Sink areas comprise 1.0% of ocean area and 3.6% of land and are prevalent on coasts and high ground. Using this approach to infer shifts in species distributions gives global and regional maps of the expected direction and rate of shifts of climate migrants, and suggests areas of potential loss of species richness.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Burrows, Michael T -- Schoeman, David S -- Richardson, Anthony J -- Molinos, Jorge Garcia -- Hoffmann, Ary -- Buckley, Lauren B -- Moore, Pippa J -- Brown, Christopher J -- Bruno, John F -- Duarte, Carlos M -- Halpern, Benjamin S -- Hoegh-Guldberg, Ove -- Kappel, Carrie V -- Kiessling, Wolfgang -- O'Connor, Mary I -- Pandolfi, John M -- Parmesan, Camille -- Sydeman, William J -- Ferrier, Simon -- Williams, Kristen J -- Poloczanska, Elvira S -- England -- Nature. 2014 Mar 27;507(7493):492-5. doi: 10.1038/nature12976. Epub 2014 Feb 9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Ecology, Scottish Association for Marine Science, Scottish Marine Institute, Oban, Argyll, PA37 1QA, Scotland, UK. ; School of Science and Engineering, University of the Sunshine Coast, Maroochydore, Queensland QLD 4558, Australia. ; 1] Climate Adaptation Flagship, CSIRO Marine and Atmospheric Research, Ecosciences Precinct, GPO Box 2583, Brisbane, Queensland 4001, Australia [2] Centre for Applications in Natural Resource Mathematics (CARM), School of Mathematics and Physics, The University of Queensland, St Lucia, Queensland 4072, Australia. ; Department of Genetics, University of Melbourne, 30 Flemington Road, Parkville, Victoria 3010, Australia. ; Department of Biology, The University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599-3280, USA. ; 1] Institute of Biological, Environmental and Rural Sciences, Aberystwyth University, Aberystwyth SY23 3DA, UK [2] Centre for Marine Ecosystems Research, Edith Cowan University, Perth 6027, Australia. ; The Global Change Institute, The University of Queensland, Brisbane, Queensland 4072, Australia. ; 1] The UWA Oceans Institute, University of Western Australia, 35 Stirling Highway, Crawley 6009, Australia [2] Department of Global Change Research, IMEDEA (UIB-CSIC), Instituto Mediterraneo de Estudios Avanzados, Esporles 07190, Spain [3] Department of Marine Biology, Faculty of Marine Sciences, King Abdulaziz University, PO Box 80207, Jeddah 21589, Saudi Arabia. ; 1] Bren School of Environmental Science and Management, University of California, Santa Barbara, California 93106, USA [2] Imperial College London, Silwood Park Campus, Buckhurst Road, Ascot SL5 7PY, UK. ; Bren School of Environmental Science and Management, University of California, Santa Barbara, California 93106, USA. ; 1] GeoZentrum Nordbayern, Palaoumwelt, Universitat Erlangen-Nurnberg, Loewenichstrasse 28, 91054 Erlangen, Germany [2] Museum fur Naturkunde, Invalidenstr asse 43, 10115 Berlin, Germany. ; Department of Zoology and Biodiversity Research Centre, University of British Columbia, Vancouver V6T 1Z4, Canada. ; School of Biological Sciences, Australian Research Council Centre of Excellence for Coral Reef Studies, The University of Queensland, Brisbane, Queensland 4072, Australia. ; 1] Integrative Biology, University of Texas, Austin, Texas 78712, USA [2] Marine Institute, Drake Circus, University of Plymouth, Devon PL4 8AA, UK. ; Farallon Institute for Advanced Ecosystem Research, 101 H Street, Suite Q, Petaluma, California 94952, USA. ; Climate Adaptation Flagship, CSIRO Ecosystem Sciences, GPO Box 1700, Canberra, Australian Capital Territory 2601, Australia. ; Climate Adaptation Flagship, CSIRO Marine and Atmospheric Research, Ecosciences Precinct, GPO Box 2583, Brisbane, Queensland 4001, Australia.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24509712" target="_blank"〉PubMed〈/a〉
    Keywords: *Animal Migration ; Animals ; Australia ; Biodiversity ; *Climate ; *Climate Change ; *Ecosystem ; *Geographic Mapping ; *Geography ; Models, Theoretical ; Population Dynamics ; Seawater ; Temperature ; Time Factors ; Uncertainty
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  • 4
    Publication Date: 2014-09-19
    Description: Non-caloric artificial sweeteners (NAS) are among the most widely used food additives worldwide, regularly consumed by lean and obese individuals alike. NAS consumption is considered safe and beneficial owing to their low caloric content, yet supporting scientific data remain sparse and controversial. Here we demonstrate that consumption of commonly used NAS formulations drives the development of glucose intolerance through induction of compositional and functional alterations to the intestinal microbiota. These NAS-mediated deleterious metabolic effects are abrogated by antibiotic treatment, and are fully transferrable to germ-free mice upon faecal transplantation of microbiota configurations from NAS-consuming mice, or of microbiota anaerobically incubated in the presence of NAS. We identify NAS-altered microbial metabolic pathways that are linked to host susceptibility to metabolic disease, and demonstrate similar NAS-induced dysbiosis and glucose intolerance in healthy human subjects. Collectively, our results link NAS consumption, dysbiosis and metabolic abnormalities, thereby calling for a reassessment of massive NAS usage.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Suez, Jotham -- Korem, Tal -- Zeevi, David -- Zilberman-Schapira, Gili -- Thaiss, Christoph A -- Maza, Ori -- Israeli, David -- Zmora, Niv -- Gilad, Shlomit -- Weinberger, Adina -- Kuperman, Yael -- Harmelin, Alon -- Kolodkin-Gal, Ilana -- Shapiro, Hagit -- Halpern, Zamir -- Segal, Eran -- Elinav, Eran -- England -- Nature. 2014 Oct 9;514(7521):181-6. doi: 10.1038/nature13793. Epub 2014 Sep 17.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Immunology, Weizmann Institute of Science, Rehovot 76100, Israel. ; 1] Department of Computer Science and Applied Mathematics, Weizmann Institute of Science, Rehovot 76100, Israel [2]. ; 1] Department of Immunology, Weizmann Institute of Science, Rehovot 76100, Israel [2]. ; Day Care Unit and the Laboratory of Imaging and Brain Stimulation, Kfar Shaul hospital, Jerusalem Center for Mental Health, Jerusalem 91060, Israel. ; 1] Internal Medicine Department, Tel Aviv Sourasky Medical Center, Tel Aviv 64239, Israel [2] Research Center for Digestive Tract and Liver Diseases, Tel Aviv Sourasky Medical Center, Sackler Faculty of Medicine, Tel Aviv University, Tel Aviv 69978, Israel [3] Digestive Center, Tel Aviv Sourasky Medical Center, Tel Aviv 64239, Israel. ; The Nancy and Stephen Grand Israel National Center for Personalized Medicine (INCPM), Weizmann Institute of Science, Rehovot 76100, Israel. ; Department of Computer Science and Applied Mathematics, Weizmann Institute of Science, Rehovot 76100, Israel. ; Department of Veterinary Resources, Weizmann Institute of Science, Rehovot 76100, Israel. ; Department of Molecular Genetics, Weizmann Institute of Science, Rehovot 76100, Israel. ; 1] Research Center for Digestive Tract and Liver Diseases, Tel Aviv Sourasky Medical Center, Sackler Faculty of Medicine, Tel Aviv University, Tel Aviv 69978, Israel [2] Digestive Center, Tel Aviv Sourasky Medical Center, Tel Aviv 64239, Israel.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25231862" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Anti-Bacterial Agents/pharmacology ; Aspartame/adverse effects ; Body Weight/drug effects ; Diet, High-Fat ; Dietary Fats/pharmacology ; Feces/microbiology ; Female ; Gastrointestinal Tract/*drug effects/*microbiology ; Germ-Free Life ; Glucose/metabolism ; Glucose Intolerance/*chemically induced/metabolism/*microbiology ; Humans ; Male ; Metabolic Syndrome X/chemically induced/metabolism/microbiology ; Mice ; Mice, Inbred C57BL ; Microbiota/*drug effects ; Saccharin/administration & dosage/adverse effects ; Sucrose/adverse effects/analogs & derivatives ; Sweetening Agents/*adverse effects ; Waist-Hip Ratio
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  • 5
    Publication Date: 2012-07-13
    Description: Recent advances in whole-genome sequencing have brought the vision of personal genomics and genomic medicine closer to reality. However, current methods lack clinical accuracy and the ability to describe the context (haplotypes) in which genome variants co-occur in a cost-effective manner. Here we describe a low-cost DNA sequencing and haplotyping process, long fragment read (LFR) technology, which is similar to sequencing long single DNA molecules without cloning or separation of metaphase chromosomes. In this study, ten LFR libraries were made using only approximately 100 picograms of human DNA per sample. Up to 97% of the heterozygous single nucleotide variants were assembled into long haplotype contigs. Removal of false positive single nucleotide variants not phased by multiple LFR haplotypes resulted in a final genome error rate of 1 in 10 megabases. Cost-effective and accurate genome sequencing and haplotyping from 10-20 human cells, as demonstrated here, will enable comprehensive genetic studies and diverse clinical applications.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3397394/" 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/PMC3397394/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Peters, Brock A -- Kermani, Bahram G -- Sparks, Andrew B -- Alferov, Oleg -- Hong, Peter -- Alexeev, Andrei -- Jiang, Yuan -- Dahl, Fredrik -- Tang, Y Tom -- Haas, Juergen -- Robasky, Kimberly -- Zaranek, Alexander Wait -- Lee, Je-Hyuk -- Ball, Madeleine Price -- Peterson, Joseph E -- Perazich, Helena -- Yeung, George -- Liu, Jia -- Chen, Linsu -- Kennemer, Michael I -- Pothuraju, Kaliprasad -- Konvicka, Karel -- Tsoupko-Sitnikov, Mike -- Pant, Krishna P -- Ebert, Jessica C -- Nilsen, Geoffrey B -- Baccash, Jonathan -- Halpern, Aaron L -- Church, George M -- Drmanac, Radoje -- P50 HG005550/HG/NHGRI NIH HHS/ -- P50HG005550/HG/NHGRI NIH HHS/ -- England -- Nature. 2012 Jul 11;487(7406):190-5. doi: 10.1038/nature11236.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Complete Genomics, Inc., 2071 Stierlin Court, Mountain View, California 94043, USA. bpeters@completegenomics.com〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22785314" target="_blank"〉PubMed〈/a〉
    Keywords: Alleles ; Cell Line ; Female ; Gene Silencing ; Genetic Variation ; *Genome, Human ; Genomics/*methods ; Haplotypes ; Humans ; Mutation ; Reproducibility of Results ; Sequence Analysis, DNA/economics/*methods/standards
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  • 6
    Publication Date: 2011-02-18
    Description: The extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star formation rates of a few hundred solar masses per year. These faint, submillimetre galaxies are challenging to study individually because of the relatively poor spatial resolution of far-infrared telescopes. Instead, their average properties can be studied using statistics such as the angular power spectrum of the background intensity variations. A previous attempt at measuring this power spectrum resulted in the suggestion that the clustering amplitude is below the level computed with a simple ansatz based on a halo model. Here we report excess clustering over the linear prediction at arcminute angular scales in the power spectrum of brightness fluctuations at 250, 350 and 500 mum. From this excess, we find that submillimetre galaxies are located in dark matter haloes with a minimum mass, M(min), such that log(10)[M(min)/M(middle dot in circle)] = 11.5(+0.7)(-0.2) at 350 mum, where M(middle dot in circle) is the solar mass. This minimum dark matter halo mass corresponds to the most efficient mass scale for star formation in the Universe, and is lower than that predicted by semi-analytical models for galaxy formation.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Amblard, Alexandre -- Cooray, Asantha -- Serra, Paolo -- Altieri, B -- Arumugam, V -- Aussel, H -- Blain, A -- Bock, J -- Boselli, A -- Buat, V -- Castro-Rodriguez, N -- Cava, A -- Chanial, P -- Chapin, E -- Clements, D L -- Conley, A -- Conversi, L -- Dowell, C D -- Dwek, E -- Eales, S -- Elbaz, D -- Farrah, D -- Franceschini, A -- Gear, W -- Glenn, J -- Griffin, M -- Halpern, M -- Hatziminaoglou, E -- Ibar, E -- Isaak, K -- Ivison, R J -- Khostovan, A A -- Lagache, G -- Levenson, L -- Lu, N -- Madden, S -- Maffei, B -- Mainetti, G -- Marchetti, L -- Marsden, G -- Mitchell-Wynne, K -- Nguyen, H T -- O'Halloran, B -- Oliver, S J -- Omont, A -- Page, M J -- Panuzzo, P -- Papageorgiou, A -- Pearson, C P -- Perez-Fournon, I -- Pohlen, M -- Rangwala, N -- Roseboom, I G -- Rowan-Robinson, M -- Portal, M Sanchez -- Schulz, B -- Scott, Douglas -- Seymour, N -- Shupe, D L -- Smith, A J -- Stevens, J A -- Symeonidis, M -- Trichas, M -- Tugwell, K -- Vaccari, M -- Valiante, E -- Valtchanov, I -- Vieira, J D -- Vigroux, L -- Wang, L -- Ward, R -- Wright, G -- Xu, C K -- Zemcov, M -- England -- Nature. 2011 Feb 24;470(7335):510-2. doi: 10.1038/nature09771. Epub 2011 Feb 16.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics & Astronomy, University of California, Irvine, California 92697, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21326201" target="_blank"〉PubMed〈/a〉
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  • 7
    Publication Date: 2012-08-17
    Description: The ocean plays a critical role in supporting human well-being, from providing food, livelihoods and recreational opportunities to regulating the global climate. Sustainable management aimed at maintaining the flow of a broad range of benefits from the ocean requires a comprehensive and quantitative method to measure and monitor the health of coupled human-ocean systems. We created an index comprising ten diverse public goals for a healthy coupled human-ocean system and calculated the index for every coastal country. Globally, the overall index score was 60 out of 100 (range 36-86), with developed countries generally performing better than developing countries, but with notable exceptions. Only 5% of countries scored higher than 70, whereas 32% scored lower than 50. The index provides a powerful tool to raise public awareness, direct resource management, improve policy and prioritize scientific research.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Halpern, Benjamin S -- Longo, Catherine -- Hardy, Darren -- McLeod, Karen L -- Samhouri, Jameal F -- Katona, Steven K -- Kleisner, Kristin -- Lester, Sarah E -- O'Leary, Jennifer -- Ranelletti, Marla -- Rosenberg, Andrew A -- Scarborough, Courtney -- Selig, Elizabeth R -- Best, Benjamin D -- Brumbaugh, Daniel R -- Chapin, F Stuart -- Crowder, Larry B -- Daly, Kendra L -- Doney, Scott C -- Elfes, Cristiane -- Fogarty, Michael J -- Gaines, Steven D -- Jacobsen, Kelsey I -- Karrer, Leah Bunce -- Leslie, Heather M -- Neeley, Elizabeth -- Pauly, Daniel -- Polasky, Stephen -- Ris, Bud -- St Martin, Kevin -- Stone, Gregory S -- Sumaila, U Rashid -- Zeller, Dirk -- England -- Nature. 2012 Aug 30;488(7413):615-20. doi: 10.1038/nature11397.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉National Center for Ecological Analysis and Synthesis, 735 State St Suite 300, Santa Barbara, California 93101, USA. halpern@nceas.ucsb.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22895186" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Conservation of Natural Resources/*statistics & numerical data ; *Ecosystem ; Environmental Monitoring/*methods ; Environmental Policy ; Fisheries ; Geography ; Human Activities/standards/statistics & numerical data ; *Internationality ; Marine Biology/*methods ; Oceanography/*methods ; Oceans and Seas ; Recreation ; *Seawater ; Water Pollution/analysis
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  • 8
    Publication Date: 2012-05-12
    Description: The old, red stars that constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable rates and active galactic nuclei (AGN) shone brightly as a result of accretion onto black holes. It is widely suspected, but unproved, that the tight correlation between the mass of the black hole and the mass of the stellar bulge results from the AGN quenching the surrounding star formation as it approaches its peak luminosity. X-rays trace emission from AGN unambiguously, whereas powerful star-forming galaxies are usually dust-obscured and are brightest at infrared and submillimetre wavelengths. Here we report submillimetre and X-ray observations that show that rapid star formation was common in the host galaxies of AGN when the Universe was 2-6 billion years old, but that the most vigorous star formation is not observed around black holes above an X-ray luminosity of 10(44) ergs per second. This suppression of star formation in the host galaxy of a powerful AGN is a key prediction of models in which the AGN drives an outflow, expelling the interstellar medium of its host and transforming the galaxy's properties in a brief period of cosmic time.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Page, M J -- Symeonidis, M -- Vieira, J D -- Altieri, B -- Amblard, A -- Arumugam, V -- Aussel, H -- Babbedge, T -- Blain, A -- Bock, J -- Boselli, A -- Buat, V -- Castro-Rodriguez, N -- Cava, A -- Chanial, P -- Clements, D L -- Conley, A -- Conversi, L -- Cooray, A -- Dowell, C D -- Dubois, E N -- Dunlop, J S -- Dwek, E -- Dye, S -- Eales, S -- Elbaz, D -- Farrah, D -- Fox, M -- Franceschini, A -- Gear, W -- Glenn, J -- Griffin, M -- Halpern, M -- Hatziminaoglou, E -- Ibar, E -- Isaak, K -- Ivison, R J -- Lagache, G -- Levenson, L -- Lu, N -- Madden, S -- Maffei, B -- Mainetti, G -- Marchetti, L -- Nguyen, H T -- O'Halloran, B -- Oliver, S J -- Omont, A -- Panuzzo, P -- Papageorgiou, A -- Pearson, C P -- Perez-Fournon, I -- Pohlen, M -- Rawlings, J I -- Rigopoulou, D -- Riguccini, L -- Rizzo, D -- Rodighiero, G -- Roseboom, I G -- Rowan-Robinson, M -- Sanchez Portal, M -- Schulz, B -- Scott, D -- Seymour, N -- Shupe, D L -- Smith, A J -- Stevens, J A -- Trichas, M -- Tugwell, K E -- Vaccari, M -- Valtchanov, I -- Viero, M -- Vigroux, L -- Wang, L -- Ward, R -- Wright, G -- Xu, C K -- Zemcov, M -- England -- Nature. 2012 May 9;485(7397):213-6. doi: 10.1038/nature11096.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK. mjp@mssl.ucl.ac.uk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22575961" target="_blank"〉PubMed〈/a〉
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  • 9
    Publication Date: 2013-02-15
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Rochman, Chelsea M -- Browne, Mark Anthony -- Halpern, Benjamin S -- Hentschel, Brian T -- Hoh, Eunha -- Karapanagioti, Hrissi K -- Rios-Mendoza, Lorena M -- Takada, Hideshige -- Teh, Swee -- Thompson, Richard C -- England -- Nature. 2013 Feb 14;494(7436):169-71. doi: 10.1038/494169a.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉School of Veterinary Medicine, University of California, Davis, USA. cmrochman@ucdavis.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23407523" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Environmental Monitoring ; *Environmental Policy/economics ; Hazardous Waste/*adverse effects/analysis/classification/*prevention & control ; Humans ; Plastics/*adverse effects/analysis/chemistry/*classification ; Recycling/trends ; Refuse Disposal/economics/*legislation & jurisprudence/*statistics & numerical ; data
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    Publication Date: 2014-02-07
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Halpern, Benjamin S -- England -- Nature. 2014 Feb 13;506(7487):167-8. doi: 10.1038/nature13053. Epub 2014 Feb 5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Bren School of Environmental Science & Management, University of California, Santa Barbara, Santa Barbara, California 93106, USA, and in the Faculty of Natural Sciences, Imperial College London, UK.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24499821" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Conservation of Natural Resources/*statistics & numerical data ; Ecology/*statistics & numerical data ; *Ecosystem ; Fisheries/*statistics & numerical data ; Fishes/*physiology
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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