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THE EARLIEST NEAR-INFRARED TIME-SERIES SPECTROSCOPY OF A TYPE Ia SUPERNOVA
Hsiao, E. Y.,Marion, G. H.,Phillips, M. M.,Burns, C. R.,Winge, C.,Morrell, N.,Contreras, C.,Freedman, W. L.,Kromer, M.,Gall, E. E. E.,Gerardy, C. L.,Hö,flich, P.,Im, M.,Jeon, Y.,Kirshner, R. P.,Nu IOP Publishing 2013 The Astrophysical journal Vol.766 No.2
<P>We present ten medium-resolution, high signal-to-noise ratio near-infrared (NIR) spectra of SN 2011fe from SpeX on the NASA Infrared Telescope Facility (IRTF) and Gemini Near-Infrared Spectrograph (GNIRS) on Gemini North, obtained as part of the Carnegie Supernova Project. This data set constitutes the earliest time-series NIR spectroscopy of a Type Ia supernova (SN Ia), with the first spectrum obtained at 2.58 days past the explosion and covering -14.6 to +17.3 days relative to B-band maximum. CI lambda 1.0693 mu m is detected in SN 2011fe with increasing strength up to maximum light. The delay in the onset of the NIR CI line demonstrates its potential to be an effective tracer of unprocessed material. For the first time in a SN Ia, the early rapid decline of the MgII lambda 1.0927 mu m velocity was observed, and the subsequent velocity is remarkably constant. The MgII velocity during this constant phase locates the inner edge of carbon burning and probes the conditions under which the transition from deflagration to detonation occurs. We show that the MgII velocity does not correlate with the optical light-curve decline rate Delta m(15)(B). The prominent break at similar to 1.5 mu m is the main source of concern for NIR k-correction calculations. We demonstrate here that the feature has a uniform time evolution among SNe Ia, with the flux ratio across the break strongly correlated with Delta m(15)(B). The predictability of the strength and the onset of this feature suggests that the associated k-correction uncertainties can be minimized with improved spectral templates.</P>
Jorge A. Gonzalez-y-Merchand,Ruben Zaragoza-Contreras,Rosalina Guadarrama-Medina,Addy C. Helguera-Repetto,Sandra Rivera-Gutierrez,Jorge F. Cerna-Cortes,Leopoldo Santos-Argumedo,Robert A. Cox 한국미생물학회 2012 The journal of microbiology Vol.50 No.3
The study of the in vitro cell growth of mycobacteria still remains a fastidious, difficult, and time-consuming procedure. In addition, assessing mycobacterial growth in the laboratory is often complicated by cell aggregation and slow growth-rate. We now report that the use of a stainless steel spring in the culture led to an absence of large cell clumps, to a decrease of dead cells in the exponential phase and to growth of a more homogeneous population of large cells. We also report that flow cytometry is a rapid, simple and reliable approach to monitor mycobacterial cell growth and viability. Here, we monitored Mycobacterium smegmatis cellular growth by optical density, dry cell mass, and colony forming units; in addition, viability, cell size and granularity profiles were analyzed by flow cytometry, and cell morphology by electron microscopy. Cultures monitored by flow cytometry may lead to a better understanding of the physiology of mycobacteria. Moreover, this methodology may aid in characterizing the cell growth of other fastidious species of microorganisms.
Surgical Management of a Type II Extracranial Internal Carotid Aneurysm near to the Skull Base
Miguel A. Mendez-Sosa,Emmanuel Contreras-Jimenez,Javier E. Anaya-Ayala,Montserrat W. Miranda-Ramirez,Gabriel Lopez-Pena,Luis H. Arzola,Santiago Mier y Teran-Ellis,Hugo Laparra-Escareno,Carlos A. Hinoj 대한혈관외과학회 2021 Vascular Specialist International Vol.37 No.3
True aneurysmal disease in the carotid arteries is very uncommon, but individuals with this pathology face the grave risk of thromboembolism, which may consequently lead to cerebrovascular accidents. Clinical knowledge remains relatively limited owing to its rarity. We present the case of a 41-year-old obese female with a type II right extracranial internal carotid artery aneurysm incidentally found during imaging work-up. She underwent open surgical reconstruction with an autologous interposition graft from the common carotid artery to the internal carotid artery at the base level of the skull. Her postoperative period was uneventful, and the patient was discharged on postoperative day five with aspirin. At 12 months of follow-up, the patient remained symptom-free without complications.
Knight, A.L.,Barros-Parada, W.,Bosch, D.,Escudero-Colomar, L.A.,Fuentes-Contreras, E.,Herná,ndez-Sá,nchez, J.,Yung, C.,Kim, Y.,Kovanci, O.B.,Levi, A.,Lo, P.,Molinari, F.,Valls, J.,Gemeno, Cambridge University Press 2015 Bulletin of entomological research Vol.105 No.1
<B>Abstract</B><P>The response of <I>Grapholita molesta</I> (Busck) males to three-component sex pheromone blends containing a 100% ratio of the major sex pheromone component, (<I>Z</I>)-8-dodecenyl acetate and a 10% ratio of (<I>Z</I>)-8-dodecenol, but with varying ratios of (<I>E</I>)-8-dodecenyl acetate (0.4, 5.4, 10.4, 30.4, and 100.1% <I>E</I>-blends) was tested with populations in eight stone and pome fruit orchards in Europe, Asia, and North and South America. Traps baited with the 5.4% <I>E</I>-blend caught significantly more males than traps with any other blend with all populations. Significantly more males were caught in traps baited with the 10.4% <I>E</I>-blend than in traps with the remaining blends, except with the 0.4% <I>E-</I>blend in Turkey. Significant differences in male moth catches occurred between the other blends with the 0.4>30.4% <I>E-</I>blend, and the 30.4>100.1% <I>E-</I>blend. Male moth catches with the 100.1% <I>E</I>-blend only differed from the hexane control in Chile. No apparent differences were noted to these blends in populations collected from pome or stone fruits. Flight tunnel assays to synthetic blends with a subset of populations were similar to the field results, but the breadth of the most attractive <I>E-</I>blends was wider. Flight tunnel assays also demonstrated a high level of male-female cross-attraction among field-collected populations. Female gland extracts from field-collected populations did not show any significant variation in their three-component blends. The only exceptions in these assays were that long-term laboratory populations were less responsive and attractive, and produced different blend ratios of the two minor components than recently collected field populations.</P>
Hoyer, S.,Ló,pez-Morales, M.,Rojo, P.,Nascimbeni, V.,Hidalgo, S.,Astudillo-Defru, N.,Concha, F.,Contreras, Y.,Servajean, E.,Hinse, T. C. Oxford University Press 2013 Monthly notices of the Royal Astronomical Society Vol.434 No.1
<P>We report 12 new transit observations of the exoplanet WASP-4b from the Transit Monitoring in the South (TraMoS) project. These transits are combined with all previously published transit data for this planet to provide an improved radius measurement of R-p = 1.395 +/- 0.022R(jup) and improved transit ephemerides. In a new homogeneous analysis in search for transit timing variations (TTVs) we find no evidence of those with rms amplitudes larger than 20 s over a 4-yr time span. This lack of TTVs rules out the presence of additional planets in the system with masses larger than about 2.5, 2.0 and 1.0 M-circle plus around the 1:2, 5:3 and 2:1 orbital resonances. Our search for the variation of other parameters, such as orbital inclination and transit depth, also yields negative results over the total time span of the transit observations. Finally, we perform a simple study of stellar spots configurations of the system and conclude that the star rotational period is about 34 d.</P>