Šarḥ al-Tashīl li-IBN MāLIK (Ğamāl al-dīn Muḥammad b. ʿAbd Allāh b. ʿAbd Allāh al-Ṭāʾī al-Ğayyānī al-ʾAndalusī) 600-672 taḥqīq al-Duktūr ʿAbd al-Raḥmān al-Sayyid [wa-] l-Duktūr Muḥammad al-MaḪtūn, HaĞrlil-Ṭibāʿa wa-l-našr wa-l-tawzīʿ wa-l-ʾiʿlān, 4 parties en 2 volumes, 70 p. + 11 planches   406 p. et 425 p.; 473 p. et 371 p., 1410H/1990.

Analysis of the Tore Supra ICRF antenna with TOPICA

“…For the sake of clarity, a poloidal section of the antenna system's final part is depicted in figure 2: it includes a single layer FS, the strap, two loading tuneable capacitors by COMET 5 with their own positioning units and a straight vacuum transmission line (VTL) connected to the feeder via a feedthrough. This arrangement of a centre-fed strap capacitively loaded at its top and bottom edges evidently forms two distinct loops, whence it is properly termed as a resonant double loop (RDL) circuit [15][16][17]. The RDL, which is a specificity of the Tore Supra ICRF antennas, is an internal matching device committed to dynamically matching the antenna to the VTL, while chasing the variable coupling of the radiated fields to the fast magnetosonic wave in the plasma.…”

Neutrophil Apoptosis Induction by Tick-Borne Encephalitis Virus

“…Their reactions with HIV, infl uenza virus, and EpsteinBarr virus and neutrophil apoptosis induction by these viruses have been described [8,9,14]. Tick-borne encephalitis (TBE) is a member of the Flaviviridae family and an agent of a severe disease of the nervous system.…”

JWST Photometric Time-delay and Magnification Measurements for the Triply Imaged Type Ia “SN H0pe” at z = 1.78

“…The spectroscopic analysis and updated lens modeling are described in companion papers, but the NIRSpec data unambiguously confirmed that the SN was of Type Ia at a refined spectroscopic redshift of z = 1.783 (Chen et al 2024;F24), whose value matches the redshift of the SN host galaxy of z = 1.7833 ± 0.0005 (F24; Polletta et al 2023). The two NIRCam imaging epochs occurred on 2023 April 22 (MJD 60056) and 2023 May 9 (MJD 60073).…”

“…In this way, our simulations should capture the intrinsic diversity of SN Ia color curves. The simulations include a range of values for the BayeSN light-curve shape (θ) and dust extinction (A V ) values based on independent constraints from the NIRSpec data (Chen et al 2024). The spectra show SN H0pe to be a normal SN Ia, and therefore we simulated SNe Ia over the reasonable population values for θ and A V of −2 θ 2 and 0 A V 1.5 given R V = 3.1 (Mandel et al 2022).…”

“…This work is part of a series of papers analyzing the SN H0pe system, which, together with M. Pascale et al (2024, in preparation), will provide the first measurement of H 0 with a multiply imaged SN Ia. The discovery of SN H0pe is described in F24, and time delays derived only from spectroscopy of the system are presented in Chen et al (2024). In this paper we focus on imaging of the SN itself, including the photometric time-delay measurement critical to that forthcoming H 0 inference.…”