Academic literature on the topic 'J001x'

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Journal articles on the topic "J001x"

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PERIN, F., J. C. PITTET, D. HOFFSCHIR, F. DABURON, G. NORMIER, and A. LE PAPE. "201T1 and 99Tcm-J001X macrophage scintigraphy." Nuclear Medicine Communications 16, no. 7 (1995): 608–14. http://dx.doi.org/10.1097/00006231-199507000-00013.

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Diot, P., E. Diot, E. Lemarie, et al. "Imaging of pulmonary disease in scleroderma with J001X scintigraphy." Thorax 49, no. 5 (1994): 504–8. http://dx.doi.org/10.1136/thx.49.5.504.

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Goupille, Philippe, Patrice Diot, Jean Pierre Valat, et al. "Imaging of pulmonary disease in rheumatoid arthritis using J001X scintigraphy: Preliminary results." European Journal of Nuclear Medicine 22, no. 12 (1995): 1411–15. http://dx.doi.org/10.1007/bf01791150.

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Perin, F., J.-C. Pittet, D. Hoffschir, G. Normier, H. Binz, and A. Le Pape. "Scintigraphic potentials of J001X acylated poly-galactoside for imaging inflammatory lesions in pigs." Nuclear Medicine and Biology 20, no. 8 (1993): 963–71. http://dx.doi.org/10.1016/0969-8051(93)90097-e.

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Diot, P., A. Le Pape, D. Nolibe, et al. "Scintigraphy with J001X, a Klebsiella membrane glycolipid, for the early diagnosis of chronic berylliosis: results from an experimental model." Occupational and Environmental Medicine 49, no. 5 (1992): 359–64. http://dx.doi.org/10.1136/oem.49.5.359.

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Pittet, Jean Christophe, Michel Pepin, Ge´rard Normier, Hanz Binz, and Alain Le Pape. "Lymphoscintigraphy via the targeting of macrophages with 99mTc-J001X poly-galactoside in a model of pyogranulomas developed in sheep lymph nodes." Nuclear Medicine and Biology 22, no. 3 (1995): 355–65. http://dx.doi.org/10.1016/0969-8051(94)00100-x.

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Perin, Fabrice, Didier Hoffschir, Jean-Christophe Pittet, et al. "Evaluation of possible interference of anti-inflammatory drugs upon scintigraphic imaging with macrophage targeting 99mTc-J001X: Effects of methylprednisolone, dexamethasone, indomethacin and methotrexate." Nuclear Medicine and Biology 21, no. 8 (1994): 1093–100. http://dx.doi.org/10.1016/0969-8051(94)90181-3.

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Noterdaeme, P., S. Balashev, F. Combes, et al. "Remarkably high mass and velocity dispersion of molecular gas associated with a regular, absorption-selected type I quasar." Astronomy & Astrophysics 651 (July 2021): A17. http://dx.doi.org/10.1051/0004-6361/202140745.

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We present 3 mm observations of the quasar J0015+1842 at z = 2.63 with the NOrthern Extended Millimeter Array (NOEMA). Our data reveal molecular gas, traced with a Gaussian CO(3–2) line, with a remarkably high velocity dispersion (FWHM = 1010 ± 120 km s−1) that corresponds to a total molecular mass MH2 ≈ (3.4 − 17) × 1010 M⊙, depending on the adopted CO-to-H2 conversion factor αCO = (0.8 − 4.0) M⊙ (km s−1 pc2)−1. Assuming the 3 mm continuum emission is thermal, we derive a dust mass of about Mdust ∼ 5 × 108 M⊙. J0015+1842 is located in the molecular gas-rich region in the IR versus CO line luminosity diagram, in between the main locus of main-sequence and sub-millimetre galaxies and that of most other active galactic nuclei targeted so far for CO measurements. While the high velocity dispersion of the CO line suggests a merging system, J0015+1842 is observed to be a regular, only very moderately dust-reddened (AV ∼ 0.3 − 0.4) type I quasar from its UV-optical spectrum, from which we infer a mass of the super-massive black hole of about MBH ≈ 6 × 108 M⊙. We suggest that J0015+1842 is observed at a galaxy evolutionary stage where a massive merger has brought significant amounts of gas towards an actively accreting super-massive black hole (quasar). While the host still contains a large amount of dust and molecular gas with a high velocity dispersion, the quasar has already cleared the way towards the observer, likely through powerful outflows, as has recently been revealed by optical observations of the same object. High angular resolution observations of this and similar systems are expected to help us better determine the respective importance of evolution and orientation in the appearance of quasars and their host galaxies. These observations have the potential to investigate early feedback and star-formation processes in galaxies in their quasar phases.
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Hachisu, Izumi, and Mariko Kato. "A New Interpretation of the Low Radial Velocity Determined from the HeII Emission Line in the Galactic Supersoft X-Ray Source RX J0019.8+2156." International Astronomical Union Colloquium 194 (2004): 233. http://dx.doi.org/10.1017/s0252921100152789.

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We propose a new interpretation for the low radial velocity of He II emission line in the Galactic supersoft X-ray source RX J0019.8+2156 based on a 2-D numerical simulation of dynamical mass transfer in binary systems. A more massive main-sequence (MS) companion of ~ 2.0 M⊙ is derived for a ~ 0.6 M⊙ white dwarf (WD) primary.The Galactic supersoft X-ray source RX J0019.8+2156 (hereafter, RX J0019) with a 12.2 mag optical counterpart was discovered by ROSAT. The source is a binary with the period of 0.66 days and its X-ray luminosity is fairly constant, at least, for 7 yrs. Therefore RX J0019 seems to be a typical luminous supersoft X-ray source (SSS) with steady hydrogen shell-burning on a mass-accreting white dwarf (WD).
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Diot, Putrice, Etienne Lemarié, Jean Louis Banlieu, et al. "Scintigraphy with J001 Macrophage Targeting Glycolipopeptide." Chest 102, no. 3 (1992): 670–76. http://dx.doi.org/10.1378/chest.102.3.670.

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Dissertations / Theses on the topic "J001x"

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Diot, Patrice. "Le ciblage in vivo des macrophages : un nouveau concept pour l'imagerie du poumon inflammatoire et tumoral." Tours, 1994. http://www.theses.fr/1994TOUR3307.

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Pittet, Jean-Christophe. "Ciblage in vivo des macrophages par une sonde d'origine bactérienne, pour l'imagerie scintigraphique des foyers inflammatoires, infectieux et tumoraux du système lymphatique." Tours, 1994. http://www.theses.fr/1994TOUR3308.

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Perin, Fabrice. "Développement d'un agent de ciblage spécifique des macrophages, le J001, poly-1,3-galactoside acylé, pour l'imagerie scintigraphique fonctionnelle de foyers inflammatoires." Tours, 1994. http://www.theses.fr/1994TOUR3305.

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York, Brian A. "The search for diffuse interstellar bands in quasar absorption line systems". Thesis, 2008. http://hdl.handle.net/1828/1074.

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The diffuse interstellar bands (DIBs) probably arise from complex organic molecules whose strength in local galaxies correlates with neutral hydrogen column density, N(H I), and dust reddening, E(B−V). Because Damped Lyman-α systems are known to have high N(H I), and Ca II absorbers in quasar (QSO) spectra are posited to have high N(H I) and reddening, both represent promising sites for the detection of DIBs at cosmological distances. I present the results of a search for diffuse bands in seven DLAs and nine Ca II absorbers. I announce the detection of the first narrow DIBs at z>0 towards one DLA and one Ca II system. I further investigate the relative strengths of the DIBs as well as their correlations with N(H I) and E(B−V). Finally, I discuss the prospects for using DIBs to better understand the properties of quasar absorption systems, and for using DIB searches in absorption systems to better understand the properties of DIBs.
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Conference papers on the topic "J001x"

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Ekomadyo, Agus S., Fauzan A. Agirachman, and Diah F. Ardani. "Formalisasi Peer Learning untuk Pembelajaran Studio Desain Arsitektur." In Temu Ilmiah IPLBI 2018. Ikatan Peneliti Lingkungan Binaan Indonesia, 2018. http://dx.doi.org/10.32315/ti.7.j001.

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