Liver abscess due to Salmonella enteritidis in a returned traveler with HIV infection: case report and review of the literature

Os pacientes com infecção pelo vírus da imunodeficiência humana (VIH) apresentam maior frequência de bacteremia associada a Salmonella não-typhi. Porém, complicações focais têm sido raramente descritas. Os autores relatam um caso de abscesso hepático devido a Salmonella enteritidis em paciente com infecção pelo VIH que retornou recentemente a São Paulo de uma viagem pelo Caribe. Após drenagem percutânea do abscesso e tratamento antimicrobiano, observou-se melhora clínica e radiológica. Segundo nossa revisão, este é o primeiro caso descrito de abscesso hepático por Salmonella não-typhi em paciente com infecção pelo VIH no Brasil.Bacteremia due to non-typhi Salmonella is more frequent in patients infected with the human immunodeficiency virus (HIV). However, focal complications have been rarely described. We report a case of liver abscess due to Salmonella enteritidis in an HIV-infected patient who recently returned to Sao Paulo, Brazil, from a trip in the Caribbean. A good clinical and radiological response was seen with both percutaneous catheter drainage and antibiotic treatment. To our knowledge, this is the first culture proven case of non-typhi Salmonellaliver abscess in an HIV-infected patient in Brazil

Search for muon-neutrino emission from GeV and TeV gamma-ray flaring blazars using five years of data of the ANTARES telescope

The ANTARES telescope is well-suited for detecting astrophysical transient neutrino sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. The background due to atmospheric particles can be drastically reduced, and the point-source sensitivity improved, by selecting a narrow time window around possible neutrino production periods. Blazars, being radio-loud active galactic nuclei with their jets pointing almost directly towards the observer, are particularly attractive potential neutrino point sources, since they are among the most likely sources of the very high-energy cosmic rays. Neutrinos and gamma rays may be produced in hadronic interactions with the surrounding medium. Moreover, blazars generally show high time variability in their light curves at different wavelengths and on various time scales. This paper presents a time-dependent analysis applied to a selection of flaring gamma-ray blazars observed by the FERMI/LAT experiment and by TeV Cherenkov telescopes using five years of ANTARES data taken from 2008 to 2012. The results are compatible with fluctuations of the background. Upper limits on the neutrino fluence have been produced and compared to the measured gamma-ray spectral energy distribution.Comment: 27 pages, 16 figure

Survey data on the impact of COVID-19 on parental engagement across 23 countries

This data article describes the dataset of the International COVID-19 Impact on Parental Engagement Study (ICIPES). ICIPES is a collaborative effort of more than 20 institutions to investigate the ways in which, parents and caregivers built capacity engaged with children's learning during the period of social distancing arising from global COVID-19 pandemic. A series of data were collected using an online survey conducted in 23 countries and had a total sample of 4,658 parents/caregivers. The description of the data contained in this article is divided into two main parts. The first part is a descriptive analysis of all the items included in the survey and was performed using tables and figures. The second part refers to the construction of scales. Three scales were constructed and included in the dataset: 'parental acceptance and confidence in the use of technology', 'parental engagement in children's learning' and 'socioeconomic status'. The scales were created using Confirmatory Factor Analysis (CFA) and Multi-Group Confirmatory Analysis (MG-CFA) and were adopted to evaluate their cross-cultural comparability (i.e., measurement invariance) across countries and within sub-groups. This dataset will be relevant for researchers in different fields, particularly for those interested in international comparative education

Physical constraints on a class of two-Higgs doublet models with FCNC at tree level

We analyse the constraints and some of the phenomenological implications of a class of two Higgs doublet models where there are flavour-changing neutral currents (FCNC) at tree level but the potentially dangerous FCNC couplings are suppressed by small entries of the CKM matrix V. This class of models have the remarkable feature that, as a result of a discrete symmetry of the Lagrangian, the FCNC couplings are entirely fixed in the quark sector by V and the ratio v(2)/v(1) of the vevs of the neutral Higgs. The discrete symmetry is extended to the leptonic sector, so that there are FCNC in the leptonic sector with their flavour structure fixed by the leptonic mixing matrix. We analyse a large number of processes, including decays mediated by charged Higgs at tree level, processes involving FCNC at tree level, as well as loop induced processes. We show that in this class of models one has new physical scalars beyond the standard Higgs boson, with masses reachable at the next round of experiments

Search for muon-neutrino emission from GeV and TeV gamma-ray flaring blazars using five years of data of the ANTARES telescope

The ANTARES telescope is well-suited for detecting astrophysical transient neutrino sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. The background due to atmospheric particles can be drastically reduced, and the point-source sensitivity improved, by selecting a narrow time window around possible neutrino production periods. Blazars, being radio-loud active galactic nuclei with their jets pointing almost directly towards the observer, are particularly attractive potential neutrino point sources, since they are among the most likely sources of the very high-energy cosmic rays. Neutrinos and gamma rays may be produced in hadronic interactions with the surrounding medium. Moreover, blazars generally show high time variability in their light curves at different wavelengths and on various time scales. This paper presents a time-dependent analysis applied to a selection of flaring gamma-ray blazars observed by the FERMI/LAT experiment and by TeV Cherenkov telescopes using five years of ANTARES data taken from 2008 to 2012. The results are compatible with fluctuations of the background. Upper limits on the neutrino fluence have been produced and compared to the measured gamma-ray spectral energy distributionThe authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Region Ile-de-France (DIM-ACAV) Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINECO), Prometeo and Grisolia programs of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.Adrián Martínez, S.; Albert, A.; André, M.; Anton, G.; Ardid Ramírez, M.; Aubert, J.; Baret, B.... (2015). Search for muon-neutrino emission from GeV and TeV gamma-ray flaring blazars using five years of data of the ANTARES telescope. Journal of Cosmology and Astroparticle Physics. 12(14):1-26. https://doi.org/10.1088/1475-7516/2015/12/014S1261214Becker, J. K. (2008). High-energy neutrinos in the context of multimessenger astrophysics. Physics Reports, 458(4-5), 173-246. doi:10.1016/j.physrep.2007.10.006Bloom, S. D., & Marscher, A. P. (1996). An Analysis of the Synchrotron Self-Compton Model for the Multi--Wave Band Spectra of Blazars. The Astrophysical Journal, 461, 657. doi:10.1086/177092Maraschi, L., Ghisellini, G., & Celotti, A. (1992). A jet model for the gamma-ray emitting blazar 3C 279. The Astrophysical Journal, 397, L5. doi:10.1086/186531Dermer, C. D., & Schlickeiser, R. (1993). Model for the High-Energy Emission from Blazars. The Astrophysical Journal, 416, 458. doi:10.1086/173251Sikora, M., Begelman, M. C., & Rees, M. J. (1994). Comptonization of diffuse ambient radiation by a relativistic jet: The source of gamma rays from blazars? The Astrophysical Journal, 421, 153. doi:10.1086/173633Gaisser, T. K., Halzen, F., & Stanev, T. (1995). Particle astrophysics with high energy neutrinos. Physics Reports, 258(3), 173-236. doi:10.1016/0370-1573(95)00003-yLearned, J. G., & Mannheim, K. (2000). High-Energy Neutrino Astrophysics. Annual Review of Nuclear and Particle Science, 50(1), 679-749. doi:10.1146/annurev.nucl.50.1.679Urry, C. M., & Padovani, P. (1995). Unified Schemes for Radio-Loud Active Galactic Nuclei. Publications of the Astronomical Society of the Pacific, 107, 803. doi:10.1086/133630Halzen, F., & Hooper, D. (2002). High-energy neutrino astronomy: the cosmic ray connection. Reports on Progress in Physics, 65(7), 1025-1078. doi:10.1088/0034-4885/65/7/201Böttcher, M. (2007). Modeling the emission processes in blazars. Astrophysics and Space Science, 309(1-4), 95-104. doi:10.1007/s10509-007-9404-0Böttcher, M., Reimer, A., Sweeney, K., & Prakash, A. (2013). LEPTONIC AND HADRONIC MODELING OFFERMI-DETECTED BLAZARS. The Astrophysical Journal, 768(1), 54. doi:10.1088/0004-637x/768/1/54Reynoso, M. M., Romero, G. E., & Medina, M. C. (2012). A two-component model for the high-energy variability of blazars. Astronomy & Astrophysics, 545, A125. doi:10.1051/0004-6361/201219873Atoyan, A. ., & Dermer, C. . (2004). Neutrinos and γ-rays of hadronic origin from AGN jets. New Astronomy Reviews, 48(5-6), 381-386. doi:10.1016/j.newar.2003.12.046Neronov, A., & Ribordy, M. (2009). IceCube sensitivity for neutrino flux from Fermi blazars in quiescent states. Physical Review D, 80(8). doi:10.1103/physrevd.80.083008Mücke, A., & Protheroe, R. J. (2001). A proton synchrotron blazar model for flaring in Markarian 501. Astroparticle Physics, 15(1), 121-136. doi:10.1016/s0927-6505(00)00141-9Abdo, A. A., Ackermann, M., Ajello, M., Allafort, A., Antolini, E., Atwood, W. B., … Barbiellini, G. (2010). THE FIRST CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THEFERMILARGE AREA TELESCOPE. The Astrophysical Journal, 715(1), 429-457. doi:10.1088/0004-637x/715/1/429Ageron, M., Aguilar, J. A., Al Samarai, I., Albert, A., Ameli, F., André, M., … Ardid, M. (2011). ANTARES: The first undersea neutrino telescope. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 656(1), 11-38. doi:10.1016/j.nima.2011.06.103Aguilar, J. A., Samarai, I. A., Albert, A., André, M., Anghinolfi, M., Anton, G., … Astraatmadja, T. (2011). Search for a diffuse flux of high-energy νμ with the ANTARES neutrino telescope. Physics Letters B, 696(1-2), 16-22. doi:10.1016/j.physletb.2010.11.070Adrián-Martínez, S., Al Samarai, I., Albert, A., André, M., Anghinolfi, M., Anton, G., … Aubert, J.-J. (2012). SEARCH FOR COSMIC NEUTRINO POINT SOURCES WITH FOUR YEARS OF DATA FROM THE ANTARES TELESCOPE. The Astrophysical Journal, 760(1), 53. doi:10.1088/0004-637x/760/1/53Adrián-Martínez, S., Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., … Barrios, J. (2014). A search for time dependent neutrino emission from microquasars with the ANTARES telescope. Journal of High Energy Astrophysics, 3-4, 9-17. doi:10.1016/j.jheap.2014.06.002Adrián-Martínez, S., Albert, A., Al Samarai, I., André, M., Anghinolfi, M., Anton, G., … Aubert, J.-J. (2013). Search for muon neutrinos from gamma-ray bursts with the ANTARES neutrino telescope using 2008 to 2011 data. Astronomy & Astrophysics, 559, A9. doi:10.1051/0004-6361/201322169Abdo, A. A., Ackermann, M., Ajello, M., Antolini, E., Baldini, L., Ballet, J., … Bellazzini, R. (2010). GAMMA-RAY LIGHT CURVES AND VARIABILITY OF BRIGHTFERMI-DETECTED BLAZARS. The Astrophysical Journal, 722(1), 520-542. doi:10.1088/0004-637x/722/1/520Ackermann, M., Ajello, M., Allafort, A., Antolini, E., Atwood, W. B., Axelsson, M., … Bastieri, D. (2011). THE SECOND CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THEFERMILARGE AREA TELESCOPE. The Astrophysical Journal, 743(2), 171. doi:10.1088/0004-637x/743/2/171Hovatta, T., Pavlidou, V., King, O. G., Mahabal, A., Sesar, B., Dancikova, R., … Surace, J. (2014). Connection between optical and γ-ray variability in blazars. Monthly Notices of the Royal Astronomical Society, 439(1), 690-702. doi:10.1093/mnras/stt2494Adrián-Martínez, S., Al Samarai, I., Albert, A., André, M., Anghinolfi, M., Anton, G., … Aubert, J.-J. (2012). Search for neutrino emission from gamma-ray flaring blazars with the ANTARES telescope. Astroparticle Physics, 36(1), 204-210. doi:10.1016/j.astropartphys.2012.06.001Aguilar, J. A., Albert, A., Ameli, F., Amram, P., Anghinolfi, M., Anton, G., … Aubert, J.-J. (2005). Study of large hemispherical photomultiplier tubes for the ANTARES neutrino telescope. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 555(1-2), 132-141. doi:10.1016/j.nima.2005.09.035Amram, P., Anghinolfi, M., Anvar, S., Ardellier-Desages, F. ., Aslanides, E., Aubert, J.-J., … Battaglieri, M. (2002). The ANTARES optical module. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 484(1-3), 369-383. doi:10.1016/s0168-9002(01)02026-5Adrián-Martínez, S., Ageron, M., Aguilar, J. A., Samarai, I. A., Albert, A., André, M., … Ardid, M. (2012). The positioning system of the ANTARES Neutrino Telescope. Journal of Instrumentation, 7(08), T08002-T08002. doi:10.1088/1748-0221/7/08/t08002Aguilar, J. A., Albert, A., Ameli, F., Anghinolfi, M., Anton, G., Anvar, S., … Basa, S. (2007). The data acquisition system for the ANTARES neutrino telescope. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 570(1), 107-116. doi:10.1016/j.nima.2006.09.098Agrawal, V., Gaisser, T. K., Lipari, P., & Stanev, T. (1996). Atmospheric neutrino flux above 1 GeV. Physical Review D, 53(3), 1314-1323. doi:10.1103/physrevd.53.1314BECHERINI, Y., MARGIOTTA, A., SIOLI, M., & SPURIO, M. (2006). A parameterisation of single and multiple muons in the deep water or ice. Astroparticle Physics, 25(1), 1-13. doi:10.1016/j.astropartphys.2005.10.005Carminati, G., Bazzotti, M., Margiotta, A., & Spurio, M. (2008). Atmospheric MUons from PArametric formulas: a fast GEnerator for neutrino telescopes (MUPAGE). Computer Physics Communications, 179(12), 915-923. doi:10.1016/j.cpc.2008.07.014Margiotta, A. (2013). Common simulation tools for large volume neutrino detectors. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 725, 98-101. doi:10.1016/j.nima.2012.11.172Adrián-Martínez, S., Albert, A., Al Samarai, I., André, M., Anghinolfi, M., Anton, G., … Aubert, J.-J. (2013). Measurement of the atmospheric ν μ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope. The European Physical Journal C, 73(10). doi:10.1140/epjc/s10052-013-2606-4Abdo, A. A., Ajello, M., Allafort, A., Baldini, L., Ballet, J., Barbiellini, G., … Bellazzini, R. (2013). THE SECONDFERMILARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS. The Astrophysical Journal Supplement Series, 208(2), 17. doi:10.1088/0067-0049/208/2/17Scargle, J. D. (1981). Studies in astronomical time series analysis. I - Modeling random processes in the time domain. The Astrophysical Journal Supplement Series, 45, 1. doi:10.1086/190706Scargle, J. D. (1998). Studies in Astronomical Time Series Analysis. V. Bayesian Blocks, a New Method to Analyze Structure in Photon Counting Data. The Astrophysical Journal, 504(1), 405-418. doi:10.1086/306064Scargle, J. D., Norris, J. P., Jackson, B., & Chiang, J. (2013). STUDIES IN ASTRONOMICAL TIME SERIES ANALYSIS. VI. BAYESIAN BLOCK REPRESENTATIONS. The Astrophysical Journal, 764(2), 167. doi:10.1088/0004-637x/764/2/167Neyman, J. (1937). Outline of a Theory of Statistical Estimation Based on the Classical Theory of Probability. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 236(767), 333-380. doi:10.1098/rsta.1937.0005Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., … Arguelles, C. (2015). SEARCHES FOR TIME-DEPENDENT NEUTRINO SOURCES WITH ICECUBE DATA FROM 2008 TO 2012. The Astrophysical Journal, 807(1), 46. doi:10.1088/0004-637x/807/1/46Kelner, S. R., Aharonian, F. A., & Bugayov, V. V. (2006). Energy spectra of gamma rays, electrons, and neutrinos produced at proton-proton interactions in the very high energy regime. Physical Review D, 74(3). doi:10.1103/physrevd.74.034018Kelner, S. R., & Aharonian, F. A. (2010). Erratum: Energy spectra of gamma rays, electrons, and neutrinos produced at interactions of relativistic protons with low energy radiation [Phys. Rev. D78, 034013 (2008)]. Physical Review D, 82(9). doi:10.1103/physrevd.82.099901Tchernin, C., Aguilar, J. A., Neronov, A., & Montaruli, T. (2013). Neutrino signal from extended Galactic sources in IceCube. Astronomy & Astrophysics, 560, A67. doi:10.1051/0004-6361/201321801Padovani, P., & Resconi, E. (2014). Are both BL Lacs and pulsar wind nebulae the astrophysical counterparts of IceCube neutrino events? Monthly Notices of the Royal Astronomical Society, 443(1), 474-484. doi:10.1093/mnras/stu1166Aleksić, J., Antonelli, L. A., Antoranz, P., Backes, M., Barrio, J. A., Bastieri, D., … Berger, K. (2011). MAGIC Observations and multiwavelength properties of the quasar 3C 279 in 2007 and 2009. Astronomy & Astrophysics, 530, A4. doi:10.1051/0004-6361/201116497Aleksić, J., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., Bangale, P., … Bednarek, W. (2014). MAGIC observations and multifrequency properties of the flat spectrum radio quasar 3C 279 in 2011. Astronomy & Astrophysics, 567, A41. doi:10.1051/0004-6361/201323036Murase, K., Inoue, Y., & Dermer, C. D. (2014). Diffuse neutrino intensity from the inner jets of active galactic nuclei: Impacts of external photon fields and the blazar sequence. Physical Review D, 90(2). doi:10.1103/physrevd.90.023007Finke, J. D., & Becker, P. A. (2014). FOURIER ANALYSIS OF BLAZAR VARIABILITY. The Astrophysical Journal, 791(1), 21. doi:10.1088/0004-637x/791/1/21Tavecchio, F., Ghisellini, G., & Guetta, D. (2014). STRUCTURED JETS IN BL LAC OBJECTS: EFFICIENT PeV NEUTRINO FACTORIES? The Astrophysical Journal, 793(1), L18. doi:10.1088/2041-8205/793/1/l1

Sperm whale long-range echolocation sounds revealed by ANTARES, a deep-sea neutrino telescope

[EN] Despite dedicated research has been carried out to adequately map the distribution of the sperm whale in the Mediterranean Sea, unlike other regions of the world, the species population status is still presently uncertain. The analysis of two years of continuous acoustic data provided by the ANTARES neutrino telescope revealed the year-round presence of sperm whales in the Ligurian Sea, probably associated with the availability of cephalopods in the region. The presence of the Ligurian Sea sperm whales was demonstrated through the real-time analysis of audio data streamed from a cabled-to- shore deep-sea observatory that allowed the hourly tracking of their long-range echolocation behaviour on the Internet. Interestingly, the same acoustic analysis indicated that the occurrence of surface shipping noise would apparently not condition the foraging behaviour of the sperm whale in the area, since shipping noise was almost always present when sperm whales were acoustically detected. The continuous presence of the sperm whale in the region confirms the ecological value of the Ligurian sea and the importance of ANTARES to help monitoring its ecosystemsThe authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a lenergie atomique et aux energies alternatives (CEA), la Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINECO), Prometeo and Grisolia programs of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilitiesAndre, M.; Caballé, A.; Van Der Schaar, M.; Solsona, A.; Houégnigan, L.; Zaugg, S.; Sanchez, AM.... (2017). Sperm whale long-range echolocation sounds revealed by ANTARES, a deep-sea neutrino telescope. Scientific Reports. 7:1-12. https://doi.org/10.1038/srep45517S1127Aguilar, J. A. et al. ANTARES: the first undersea neutrino telescope. Nucl Inst and Met Phys Res A. 656, 11–38 (2011a).Aguilar, J. A. et al. AMADEUS - The Acoustic Neutrino Detection Test System of the ANTARES Deep-Sea Neutrino Telescope -. Nucl Inst and Met Phys Res A. 626–627, 128–143 (2011b).Ruhl, H. et al. Societal need for improved understanding of climate change, anthropogenic impacts, and geo-hazard warning drive development of ocean observatories in European Seas. Prog Oceanog. 91, 1–33 (2011).Tamburini, C. et al. Deep-sea bioluminescence blooms after dense water formation at the ocean surface. PLoS One. 8(7), e67523. doi: 10.1371/journal.pone.0067523 (2013).Van Haren, H. et al. Acoustic and optical variations during rapid downward motion episodes in the deep North Western Mediterranean. Deep Sea Res I. 58, 875–884 (2011).Van der Graaf, A. J. et al. European Marine Strategy Framework Directive - Good Environmental Status (MSFD GES): Report of the Technical Subgroup on Underwater noise and other forms of energy (2012).Hatch, L. T., Clark, C. W., Van Parijs, S. M., Frankel, A. S. & Ponirakis, D. W. Quantifying Loss of Acoustic Communication Space for Right Whales in and around a U.S. National Marine Sanctuary. Conserv Biol. 26, 983–994 (2012).André, M. et al. Low-frequency sounds induce acoustic trauma in cephalopods. Front. Ecol. Environ. 9, 489–493 (2011).Solé, M. et al. Does exposure to noise from human activities compromise sensory information from cephalopod statocysts? Deep Sea Res. II. 95, 160–181 (2013).Solé, M. et al. Ultrastructural damage of Loligo vulgaris and Illex coindetii statocysts after low frequency sound exposure. PLoS One 8(10), e78825. doi: 10.1371/journal.pone.0078825 (2013).André, M. et al. Listening to the Deep: Live monitoring of ocean noise and cetacean acoustic signals. Mar Pollut Bull. 63, 18–26 (2011).Whitehead, H. Sperm whales: social evolution in the ocean(The University of Chicago Press, Chicaho, 2003).Mohl, B., Wahlberg, M., Madsen, P. T., Heerfordt, A. & Lund, A. The monopulsed nature of sperm whale clicks. J Acous Soc Am. 114, 1143–1154 (2003).André, M., Johansson, T., Delory, E. & van der Schaar, M. Foraging on squid: the sperm whale mid-range sonar. Jour Mar Biol Assoc. 87, 59–67 (2007).Madsen, P., Wahlberg, M. & Møhl, B. Male sperm whale (Physeter macrocephalus) acoustics in a high-latitude habitat: implications for echolocation and communication. Behav Ecol Sociobiol. 53, 31, doi: 10.1007/s00265-002-0548-1 (2002).Gannier, A., Drouot, V. & Goold, J. C. Distribution and relative abundance of sperm whales in the Mediterranean Sea . Mar Ecol Prog Ser. 243, 281–293 (2000).Drouot, V., Gannier, A. & Gould, J. C. Summer social distribution of sperm whales in the Mediterranean Sea. J Mar Biol Ass. 84, 675–680 (2004).Pavan, G. et al. G. Short Term and Long Term Bioacoustic Monitoring of the Marine Environment. Results from NEMO ONDE Experiment and Way Ahead in Computational bioacoustics for assessing biodiversity . Proceedings of the International Expert meeting on IT-based detection of bioacoustical patterns(ed. Frommolt, K. H., Rolf Bardeli, R. & Clausen, M. ) 7–14 (Federal Agency for Nature Conservation, Bonn, 2008).Frantzis, A. et al. Sperm whale presence off South-West Crete, Eastern Mediterranean Sea in Proc. 13th Ann. Conf. ECS. 214–217 (Eur Res Cet, Valencia, 1999).Notarbartolo-Di-Sciara, G. Sperm whales, Physeter macrocephalus, in the Mediterranean Sea: a summary of status, threats, and conservation recommendations. Aquatic Conserv. Mar. Freshw. Ecosyst. 24, 4–10. doi: 10.1002/aqc.2409 (2014).Pace, D. S., Mussi, B., Gordon, J. C. D. & Würtz, M. Ecology, Behaviour and Conservation of Sperm Whale in the Mediterranean Sea in Aquatic Conserv . Mar. Freshw. Ecosyst. 24 (ed. Wiley, J. ) 1–118 (Wiley Online library, 2014).Rendell, L. E. & Frantzis, A. Mediterranean sperm whales, Physeter macrocephalus: the precarious state of a lost tribe In Medit. Mar. Mam. Ecol. Cons. 75 (ed. Notarbartolo di Sciara, G., Podestà, M. P. & Curry, B. E. ) 37–74, doi: 10.1016/bs.amb.2016.08.001 (Advances in Marine Biology, Academic Press/Elsevier, 2016).Di Natale, A. & Notarbartolo di Sciara, G. A review of the passive fishing nets and trap fisheries in the Mediterranean Sea and of the cetacean bycatch In Gillnets and cetaceans(ed. Perrin, W. F., Donovan, G. P. & Barlow, J. ) 189–202 (Rep Int Whal Comm, 1994).Jaquet, N., Whitehead, H. & Lewis, M. Relationship between sperm whale distribution and primary productivity over large spatial scale in the Pacific ocean. Eur Res Cet. 9, 188–192 (1995).Millot, C. Circulation in the Western Mediterranean Sea. Oceanol Acta. 10, 143–150 (1987).Morel, A. & André, J. M. Pigment distribution and primary production in the Western Mediterranean as derived from coastal zone color scanner observations. J Geophy Res. 96, 2685–12698 (1991).Crépon, M., Wald, L. & Monget, J. M. Low-frequency waves in the Ligurian Sea during December 1977. J Geophys Res. 87, 595–600 (1982).Prieur, L. & Sathyendranath, S. An optical classification of coastal and oceanic waters based on the specific spectral absorption curves of phytoplankton pigments, dissolved organic matter, and other particulate materials. Limnol Oceanogr. 26, 671–89 (1981).Kawakami, T. A review of sperm whale food. Sci Rep Whales Res Inst. 32, 199–218 (1980).Roper, C. F. E. & Young, R. E. Vertical distribution of pelagic cephalopods. Smithson Contrib Zool. 209, 1–51 (1975).Matsushita, T. Daily rhythmic activity of the sperm whales in the Antarctic. Bull Jpn Soc Sci Fish. 20, 770–73 (1955).Zaugg, S. et al. Real-time acoustic classification of sperm whale clicks and shipping impulses from deep-sea observatories. Appl Acoust. 71(11), 1011–1019 (2010).Nelder, J. & Wedderburn, R. Generalized linear models. J R Stat Soc. 135, 370–384 (1972)

Impacts of the Tropical Pacific/Indian Oceans on the Seasonal Cycle of the West African Monsoon

The current consensus is that drought has developed in the Sahel during the second half of the twentieth century as a result of remote effects of oceanic anomalies amplified by local land–atmosphere interactions. This paper focuses on the impacts of oceanic anomalies upon West African climate and specifically aims to identify those from SST anomalies in the Pacific/Indian Oceans during spring and summer seasons, when they were significant. Idealized sensitivity experiments are performed with four atmospheric general circulation models (AGCMs). The prescribed SST patterns used in the AGCMs are based on the leading mode of covariability between SST anomalies over the Pacific/Indian Oceans and summer rainfall over West Africa. The results show that such oceanic anomalies in the Pacific/Indian Ocean lead to a northward shift of an anomalous dry belt from the Gulf of Guinea to the Sahel as the season advances. In the Sahel, the magnitude of rainfall anomalies is comparable to that obtained by other authors using SST anomalies confined to the proximity of the Atlantic Ocean. The mechanism connecting the Pacific/Indian SST anomalies with West African rainfall has a strong seasonal cycle. In spring (May and June), anomalous subsidence develops over both the Maritime Continent and the equatorial Atlantic in response to the enhanced equatorial heating. Precipitation increases over continental West Africa in association with stronger zonal convergence of moisture. In addition, precipitation decreases over the Gulf of Guinea. During the monsoon peak (July and August), the SST anomalies move westward over the equatorial Pacific and the two regions where subsidence occurred earlier in the seasons merge over West Africa. The monsoon weakens and rainfall decreases over the Sahel, especially in August.Peer reviewe

Optimasi Portofolio Resiko Menggunakan Model Markowitz MVO Dikaitkan dengan Keterbatasan Manusia dalam Memprediksi Masa Depan dalam Perspektif Al-Qur`an

Risk portfolio on modern finance has become increasingly technical, requiring the use of sophisticated mathematical tools in both research and practice. Since companies cannot insure themselves completely against risk, as human incompetence in predicting the future precisely that written in Al-Quran surah Luqman verse 34, they have to manage it to yield an optimal portfolio. The objective here is to minimize the variance among all portfolios, or alternatively, to maximize expected return among all portfolios that has at least a certain expected return. Furthermore, this study focuses on optimizing risk portfolio so called Markowitz MVO (Mean-Variance Optimization). Some theoretical frameworks for analysis are arithmetic mean, geometric mean, variance, covariance, linear programming, and quadratic programming. Moreover, finding a minimum variance portfolio produces a convex quadratic programming, that is minimizing the objective function ðð¥with constraintsð ð 𥠥 ðandð´ð¥ = ð. The outcome of this research is the solution of optimal risk portofolio in some investments that could be finished smoothly using MATLAB R2007b software together with its graphic analysis

Differential cross section measurements for the production of a W boson in association with jets in proton–proton collisions at √s = 7 TeV

Measurements are reported of differential cross sections for the production of a W boson, which decays into a muon and a neutrino, in association with jets, as a function of several variables, including the transverse momenta (pT) and pseudorapidities of the four leading jets, the scalar sum of jet transverse momenta (HT), and the difference in azimuthal angle between the directions of each jet and the muon. The data sample of pp collisions at a centre-of-mass energy of 7 TeV was collected with the CMS detector at the LHC and corresponds to an integrated luminosity of 5.0 fb[superscript −1]. The measured cross sections are compared to predictions from Monte Carlo generators, MadGraph + pythia and sherpa, and to next-to-leading-order calculations from BlackHat + sherpa. The differential cross sections are found to be in agreement with the predictions, apart from the pT distributions of the leading jets at high pT values, the distributions of the HT at high-HT and low jet multiplicity, and the distribution of the difference in azimuthal angle between the leading jet and the muon at low values.United States. Dept. of EnergyNational Science Foundation (U.S.)Alfred P. Sloan Foundatio