WISE J163940.83-684738.6: A Y Dwarf identified by Methane Imaging

We have used methane imaging techniques to identify the near-infrared counterpart of the bright WISE source WISEJ163940.83-684738.6. The large proper motion of this source (around 3.0arcsec/yr) has moved it, since its original WISE identification, very close to a much brighter background star -- it currently lies within 1.5" of the J=14.90+-0.04 star 2MASS16394085-6847446. Observations in good seeing conditions using methane sensitive filters in the near-infrared J-band with the FourStar instrument on the Magellan 6.5m Baade telescope, however, have enabled us to detect a near-infrared counterpart. We have defined a photometric system for use with the FourStar J2 and J3 filters, and this photometry indicates strong methane absorption, which unequivocally identifies it as the source of the WISE flux. Using these imaging observations we were then able to steer this object down the slit of the FIRE spectrograph on a night of 0.6" seeing, and so obtain near-infrared spectroscopy confirming a Y0-Y0.5 spectral type. This is in line with the object's near-infrared-to-WISE J3--W2 colour. Preliminary astrometry using both WISE and FourStar data indicates a distance of 5.0+-0.5pc and a substantial tangential velocity of 73+-8km/s. WISEJ163940.83-684738.6 is the brightest confirmed Y dwarf in the WISE W2 passband and its distance measurement places it amongst the lowest luminosity sources detected to date.Comment: Accepted for publication in The Astrophysical Journal, 20 September 201

Spectroscopy on two coupled flux qubits

We have performed spectroscopy measurements on two coupled flux qubits. The qubits are coupled inductively, which results in a $\sigma_1^z\sigma_2^z$ interaction. By applying microwave radiation, we observe resonances due to transitions from the ground state to the first two excited states. From the position of these resonances as a function of the magnetic field applied we observe the coupling of the qubits. The coupling strength agrees well with calculations of the mutual inductance

A Preliminary Report on Unique Hail and Tornadic Storm Observations in Central Illinois and Eastern Indiana on 3 April 1974

published or submitted for publicationis peer reviewedOpe

Derivation of tropospheric methane from TCCON CH₄ and HF total column observations

The Total Carbon Column Observing Network (TCCON) is a global ground-based network of Fourier transform spectrometers that produce precise measurements of column-averaged dry-air mole fractions of atmospheric methane (CH₄). Temporal variability in the total column of CH₄ due to stratospheric dynamics obscures fluctuations and trends driven by tropospheric transport and local surface fluxes that are critical for understanding CH₄ sources and sinks. We reduce the contribution of stratospheric variability from the total column average by subtracting an estimate of the stratospheric CH₄ derived from simultaneous measurements of hydrogen fluoride (HF). HF provides a proxy for stratospheric CH₄ because it is strongly correlated to CH₄ in the stratosphere, has an accurately known tropospheric abundance (of zero), and is measured at most TCCON stations. The stratospheric partial column of CH₄ is calculated as a function of the zonal and annual trends in the relationship between CH₄ and HF in the stratosphere, which we determine from ACE-FTS satellite data. We also explicitly take into account the CH₄ column averaging kernel to estimate the contribution of stratospheric CH₄ to the total column. The resulting tropospheric CH₄ columns are consistent with in situ aircraft measurements and augment existing observations in the troposphere

Spin-controlled Mott-Hubbard bands in LaMnO_3 probed by optical ellipsometry

Spectral ellipsometry has been used to determine the dielectric function of an untwinned crystal of LaMnO_3 in the spectral range 0.5-5.6 eV at temperatures 50 K < T < 300 K. A pronounced redistribution of spectral weight is found at the Neel temperature T_N = 140 K. The anisotropy of the spectral weight transfer matches the magnetic ordering pattern. A superexchange model quantitatively describes spectral weight transfer induced by spin correlations. This analysis implies that the lowest-energy transitions around 2 eV are intersite d-d transitions, and that LaMnO_3 is a Mott-Hubbard insulator.Comment: 4 pages, 4 figure

Total column CO_2 measurements at Darwin, Australia – site description and calibration against in situ aircraft profiles

An automated Fourier Transform Spectroscopic (FTS) solar observatory was established in Darwin, Australia in August 2005. The laboratory is part of the Total Carbon Column Observing Network, and measures atmospheric column abundances of CO_2 and O_2 and other gases. Measured CO_2 columns were calibrated against integrated aircraft profiles obtained during the TWP-ICE campaign in January–February 2006, and show good agreement with calibrations for a similar instrument in Park Falls, Wisconsin. A clear-sky low airmass relative precision of 0.1% is demonstrated in the CO2 and O2 retrieved column-averaged volume mixing ratios. The 1% negative bias in the FTS X_(CO_2) relative to the World Meteorological Organization (WMO) calibrated in situ scale is within the uncertainties of the NIR spectroscopy and analysis

Precision Study of Positronium: Testing Bound State QED Theory

As an unstable light pure leptonic system, positronium is a very specific probe atom to test bound state QED. In contrast to ordinary QED for free leptons, the bound state QED theory is not so well understood and bound state approaches deserve highly accurate tests. We present a brief overview of precision studies of positronium paying special attention to uncertainties of theory as well as comparison of theory and experiment. We also consider in detail advantages and disadvantages of positronium tests compared to other QED experiments.Comment: A talk presented at Workshop on Positronium Physics (ETH Zurich, May 30-31, 2003

Low Density Lipoprotein Metabolism by Human Macrophages Activated with Low Density Lipoprotein Immune Complexes: A Possible Mechanism of Foam Cell Formation

Human monocytes are known to be multifunctional cells that combine a variety of functions, including phagocytosis, antigen processing and presentation to immune cells, secretion of a large number of bioactive products with significant roles in the immune and inflammatory reactions, and the ability to kill tumor cells and other abnormal cells by a variety of mechanisms, including antibody-dependent cell-mediated cytotoxicity (1-5). Tissue macrophages are believed to derive from circulating monocytes, although the two types of cells differ by a variety of morphological and functional criteria (6-10). The role of macrophages is not always well understood, since it combines potentially useful properties related to its ability to ingest and process foreign and altered materials with the capacity to secrete large amounts of mediators having the potential to cause inflammatory changes and tissue damage in general (11-14). In atherosclerosis, substantial evidence has been gathered suggesting that the foam cells seen in early atherosclerotic plaques are derived from monocytes/macrophages (15-18). The formation and subendothelial accumulation of foam cells are believed to represent a critical event in the onset of atheromatous plaque formation (19). Some interesting correlations can be drawn between the involvement of macrophages in the pathogenesis of atherosclerosis and increasing evidence suggesting that immunologic mechanisms may influence the development or evolution of this pathologic process. In the early 1970s, it was postulated that immune mechanisms involving circulating immune complexes could contribute to the pathogenesis of atherosclerosis (20). The evidence supporting this role of immune complexes was both experimental (animals undergoing serum sickness and given a lipid-rich diet developed accelerated atherosclerosis [21]) and clinical (patients with IgA myelomas with anti-lipoprotein activity had massive hyperlipemia and accelerated atherosclerosis [22]). More recently, it was also shown that immune complexes (IC)1 involving low density lipoprotein (LDL) induce profound changes on cholesterol metabolism at the cellular level (23). Further support for the involvement of IC in the pathogenesis of atherosclerosis has been recently obtained by Szondy et al. (24), who demonstrated increased levels of IC and anti-LDL antibodies in patients with clinical manifestations of coronary heart disease. The possibility that IC interactions with macrophages may lead to their activation and, therefore, play a pathogenic role in the development of atherosclerosis is extremely challenging. Until recently, the mechanism proposed to explain how monocyte-derived macrophages could be transformed into foam cells has focused upon the interaction between macrophages and modified LDL or lipoproteins of abnormal composition, such as β-very low density lipoproteins (VLDL). Modified LDL can be taken up in a nonregulated fashion via the scavenger receptor, resulting in the intracellular accumulation of cholesteryl esters (CE) and in the formation of a foam cell. In contrast, it has been observed that cultured macrophages exposed to native LDL (NLDL) do not accumulate CE due to the stringent regulation of LDL receptors. However, it has been recently shown that in certain conditions, macrophages exposed to native LDL may accumulate CE. In our laboratory, we have shown that human macrophages stimulated with microbial or microbial-related products have an increased uptake of N-LDL and accumulated CE (25). Tabas et al. (26) observed increased uptake of N-LDL and concomitant CE accumulation in J774 cells, a mouse macrophage-like tumor cell line. They postulated that this was due to the enhanced metabolic activity of this tumor cell line (26). Klimov, et al. (27) had shown excessive CE accumulation in mouse peritoneal macrophages exposed to LDL immune complexes compared with control cells. A common denominator for all these observations is the known ability of microbial products and immune complexes to activate macrophages. Therefore, we decided to examine the effect of macrophage activation on N-LDL metabolism. More specifically, we wanted to investigate the effect of LDL-anti-LDL IC on N-LDL and cholesterol metabolism in human macrophages, and determine whether this type of IC can induce the transformation of human macrophages into foam cells contributing to the development of atherosclerosis

Ground-based NIR emission spectroscopy of HD189733b

We investigate the K and L band dayside emission of the hot-Jupiter HD 189733b with three nights of secondary eclipse data obtained with the SpeX instrument on the NASA IRTF. The observations for each of these three nights use equivalent instrument settings and the data from one of the nights has previously reported by Swain et al (2010). We describe an improved data analysis method that, in conjunction with the multi-night data set, allows increased spectral resolution (R~175) leading to high-confidence identification of spectral features. We confirm the previously reported strong emission at ~3.3 microns and, by assuming a 5% vibrational temperature excess for methane, we show that non-LTE emission from the methane nu3 branch is a physically plausible source of this emission. We consider two possible energy sources that could power non-LTE emission and additional modelling is needed to obtain a detailed understanding of the physics of the emission mechanism. The validity of the data analysis method and the presence of strong 3.3 microns emission is independently confirmed by simultaneous, long-slit, L band spectroscopy of HD 189733b and a comparison star.Comment: ApJ accepte