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261 results for “217”
FIGURES 216–223. Pinodytes sequoia. 216. Male right antenna, dorsal. 217. Male right protibia and protarsus. 218. Male right mesotibia. 219. Male right metafemur and metatibia. 220. Aedeagus, lateral. 221. Aedeagus, dorsal. 222. Spermatheca. 223 in Systematics, distributions and bionomics of the Catopocerini (eyeless soil fungivore beetles) of North America (Coleoptera: Leiodidae: Catopocerinae) 3077
FIGURES 216–223. Pinodytes sequoia. 216. Male right antenna, dorsal. 217. Male right protibia and protarsus. 218. Male right mesotibia. 219. Male right metafemur and metatibia. 220. Aedeagus, lateral. 221. Aedeagus, dorsal. 222. Spermatheca. 223. Mesoventrite, lateral. Scale bar = 0.2 mm (Fig. 222), 0.3 mm (Fig. 223), 0.5 mm (Figs. 216–221).
FIGURES 209–217 in New species in the Neotropical genus Docalidia with a key to known species, notes on distribution, taxonomy and a synoptic catalogue of the genus (Hemiptera: Cicadellidae: Coelidiinae: Teruliini) 2952
FIGURES 209–217. Docalidia rondoniensis, sp. nov. (209) pygofer, lateral view; (210) segment X, lateral view; (211) right subgenital plate, ventral views; (212) right style, lateral view; (213) right style, dorsal view; (214) aedeagus and dorsal connective, lateral view; (215) aedeagus, ventral view; (216) connective, caudal view; (217) dorsal connective, dorsal view.
FIGURES 203–217 in <p><strong>A revision of Afrotropical Quasimodo flies (Diptera: Schizophora; Curtonotidae). Part IV—the continental Afrotropical species of <em>Curtonotum </em>Macquart, with descriptions of thirteen new species and a combined phylogenetic analysis of the Curtonotidae</strong></p>
FIGURES 203–217. Females of Afrotropical Curtonotum spp. 203–206. Postabdomen. 203. C. maculiventris (lateral) (N-T, Nigeria, River Bagel, NMWC) [not fully distended]. 204. Same (ventral). 205. C. striatifrons (lateral) (N-T, Sudan, Roseires, MNHN) [t7 distorted]. 206. Same (ventral). 207–209. Auxiliary sclerites in region of sternite 7. 207. C. herrero. 208. C. maculiventris. 209. C. striatifrons. 210–217. Spermatheca/e of Curtonotum spp. 210. C. herrero. 211. C. maculiventris. 212. C. striatifrons. 213. C. marriott sp. n. (PT, Cameroon, Kribi (beach), TAU). 214. C. moffatt sp. n. (PT, Uganda, Katona, HNHM). 215. C. platyphallum (N-T, Liberia, 8 mi. N.W. Zorzor, CAS). 216. C. helvum (N-T, [Canada], Sandbanks P.P., Picton, DEBU). 217. C. anus (lateral) (Israel, Park HaYarden, TAU). (Figs 207–212 from Tsacas (1977), figs 5e, 12e, 11e, 5d, 12f and 11d respectively; figs 12f and 12e as C. tigrinum). Scale bars: 203–206 = 1 mm; 207–212 = 0.2 mm; 213–217 = 50 µm.
FIGURES 217–224 in An annotated and illustrated Type Catalogue of the predacious Shieldbugs (Hemiptera: Heteroptera: Pentatomidae: Asopinae) in the Collection of the Natural History Museum, London
FIGURES 217–224. Type specimens deposited in NHMUK. 217–220, Platynopus turneri; 221, Supputius typicus; 222–224, Gilva varipes. Scale bars: 4 mm.
FIGURES 217–219 in A revision of the genus Photinopygus Chatzimanolis (Staphylinidae: Xanthopygina)
FIGURES 217–219. Aedeagus of Photinopygus tepidus (Erichson). 217. Lateral view. 218. Dorsal view. 219. Detail of paramere, ventral view.
Amplification of Zinc Finger Protein 217 Gene in Multiple Myeloma
ClinicalTrials.gov study NCT04212858. IPD Sharing: NO. Countries: 0. Publications: 0.
Planck Catalog of 217-GHz Compact Sources (PCCS) Release 2
Planck was a European Space Agency (ESA) mission, with significant contributions from the National Aeronautics and Space Agency (NASA). It was the third generation of space-based cosmic microwave background experiments, after the Cosmic Background Explorer (COBE) and the Wilkinson Microwave Anisotropy Probe (WMAP). Planck was launched on 14 May 2009 on an Ariane 5 rocket from Kourou, French Guiana. Following a cruise to the Earth-Sun L2 Lagrange point, cooling and in orbit checkout, Planck initiated the First Light Survey on 12 August 2009. Planck then continuously measured the intensity of the sky over a range of frequencies from 30 to 857 GHz (wavelengths of 1 cm to 350 micron) with spatial resolutions ranging from about 33 to 5 arcminutes, respectively. The Low Frequency Instrument (LFI) on Planck provided temperature and polarization information using radiometers which operated between 30 and 70 GHz. The High Frequency Instrument (HFI) used pairs of polarization-sensitive bolometers at each of four frequencies between 100 and 353 GHz but did not measure polarization information in the two upper HFI bands at 545 and 857 GHz. The lowest Planck frequencies overlapped with WMAP, and the highest frequencies extended far into the submillimeter in order to improve separation between Galactic foregrounds and the cosmic microwave background (CMB). By extending to wavelengths longer than those at which the Infrared Astronomical Satellite (IRAS) operated, Planck provided an unprecedented window into dust emission at far-infrared and submillimeter wavelengths. The Second Planck Catalogue of Compact Sources is a list of discrete objects detected in single-frequency maps from the full duration of the Planck mission and supersedes previous versions. It consists of compact sources, both Galactic and extragalactic, detected over the entire sky. Compact sources detected in the lower frequency channels are assigned to the PCCS2, while at higher frequencies they are assigned to one of two subcatalogs, the PCCS2 or PCCS2E, depending on their location on the sky. The first of these (PCCS2) covers most of the sky and allows the user to produce subsamples at higher reliabilities than the target 80% integral reliability of the catalog. The second (PCCS2E) contains sources detected in sky regions where the diffuse emission makes it difficult to quantify the reliability of the detections. Both the PCCS2 and PCCS2E include polarization measurements, in the form of polarized flux densities, or upper limits, and orientation angles for all seven polarization-sensitive Planck channels. The improved data-processing of the full-mission maps and their reduced noise levels allow the authors to increase the number of objects in the catalog, improving its completeness for the target 80% reliability as compared with the previous versions, the PCCS and the Early Release Compact Source Catalogue (ERCSC). The Low Frequency Instrument (LFI) Data Processing Center (DPC) produced the 30, 44, and 70 GHz maps after the completion of eight full surveys (spanning the period from 12 August 2009 to 3 August 2013). In addition, special LFI maps covering the period 1 April 2013 to 30 June 2013 were produced in order to compare the Planck flux-density scales with those of the Very Large Array and the Australia Telescope Compact Array, by performing simultaneous observations of a sample of sources over that period. The High Frequency Instrument (HFI) DPC produced the 100-, 143-, 217-, 353-, 545-, and 857-GHz maps after five full surveys (from 2009 August 12 to 2012 January 11). As in the PCCS, the PCCS2 provides four different measures of the flux density for each source. They are determined by the source detection algorithm (DETFLUX), aperture photometry (APERFLUX), point spread function fitting (PSFFLUX), and Gaussian fitting (GAUFLUX). Only the first is obtained from the filtered maps; the other measures are estimated from the full-sky maps at the positions of the sources. The source detection algorithm photometry, the aperture photometry, and the point spread function (PSF) fitting use the Planck band-average effective beams, calculated with FEBeCoP (Fast Effective Beam Convolution in Pixel space). Note that only the PSF fitting algorithm takes into account the variation of the PSF with position on the sky. The PCCS2 has been produced from the Planck full-mission maps (eight sky surveys in the LFI and five sky surveys in the HFI), and therefore supersedes the previous catalogs (for the PCCS only 1.5 surveys were analyzed). It also includes the latest calibration and beam information, and the authors have improved some of the algorithms used to measure the photometry of the sources. This table contains the PCCS2 subsample of the PCCS Public Release 2 table of sources detected at 217 GHz. One of the primary differences of this release of the PCCS from previous releases is the division of the six highest frequency catalogs into two subcatalogs, the PCCS2 a
FIGURE 217 in Taxonomic revision of the Neotropical genus Telemiades Hübner, [1819] (Lepidoptera: Hesperiidae: Eudaminae), with descriptions of fourteen new species
FIGURE 217. Geographical distribution of Telemiades from the "trenda group".
PROCRAFT_Form B_Dornier 217_B1
<p>Information and condition state of one part of Dornier 217 wreck. (related to PROCRAFT_Form A_Dornier 217_Sacoué)</p>
PROCRAFT_Form C_Dornier 217_B1C1
<p>Results of scientific analyses on a part collected from a Dornier 217 (See PROCRAFT_Form A_Dornier 217_Sacoué)</p>
PROCRAFT_Form C_Dornier 217_B2-12C1
<p>Results of scientific analyses on parts (stringer + plate + rivet) collected from a Dornier 217 (See PROCRAFT_Form A_Dornier 217_Sacoué)</p>
od_______217::9e5258195a8567a357dbe0a3376e5074
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od_______217::b1a9b09c2b101e3d58bdb0458ef693bf
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Data set from Adamo M, Grasso C, Capodanno D, Rubbio AP, Scandura S, Giannini C, Fiorelli F, Fiorina C, Branca L, Brambilla N, Bedogni F, Petronio AS, Curello S, Tamburino C. Five-year clinical outcomes after percutaneous edge-to-edge mitral valve repair: Insights from the multicenter GRASP-IT registry. Am Heart J. 2019 Nov;217:32-41. doi: 10.1016/j.ahj.2019.06.015. Epub 2019 Jul 3. PMID: 31473325.
<p>Data set from Adamo M, Grasso C, Capodanno D, Rubbio AP, Scandura S, Giannini C, Fiorelli F, Fiorina C, Branca L, Brambilla N, Bedogni F, Petronio AS, Curello S, Tamburino C. Five-year clinical outcomes after percutaneous edge-to-edge mitral valve repair: Insights from the multicenter GRASP-IT registry. Am Heart J. 2019 Nov;217:32-41. doi: 10.1016/j.ahj.2019.06.015. Epub 2019 Jul 3. PMID: 31473325.</p> <p> </p> <p>This is the abstract:</p> <p>Limited evidence is available on 5-year clinical outcomes after percutaneous edge-to-edge mitral valve repair.</p> <p><strong>Methods: </strong>The Getting Reduction of mitrAl inSufficiency by Percutaneous clip implantation in ITaly (GRASP-IT) is a multicenter registry including 304 consecutive patients undergoing Mitraclip between October 2008 and October 2013 at 4 Italian centers. Primary end point (all-cause mortality) and secondary end point (all-cause mortality or heart failure [HF] hospitalization) were evaluated up to 5 years and between 1 and 5 years.</p> <p><strong>Results: </strong>Cumulative incidence of the primary and secondary end points at 1, 2, 3, 4, and 5 years were 15.1%, 26.4%, 35.5%, 42.1%, and 47.3% and 29.1%, 41.7%, 49.8%, 56%, and 62.3%, respectively. Landmark analysis between 1 and 5 years showed an incidence of primary and secondary end point of 37.9% and 46.8%, respectively. Five-year event rates were significantly higher in patients with functional ischemic mitral regurgitation (MR) compared to other etiologies. MR recurrence and left ventricular ejection fraction <30% were associated with an increased risk of both primary and secondary end points. EuroSCORE II >5% was associated with an increased risk of 5-year mortality. Ischemic etiology of MR, baseline serum creatinine >1.5 mg/dL, chronic obstructive pulmonary disease, and previous HF hospitalizations were independent predictors of 5-year secondary end point.</p> <p><strong>Conclusions: </strong>At 5-year follow-up after Mitraclip, nearly half of patients died and almost two thirds died or were admitted for HF. MR recurrence, ischemic etiology, high comorbidity burden (ie, EuroSCORE II >5%, chronic obstructive pulmonary disease), and advanced cardiomyopathy (ie, left ventricular ejection fraction <30%, prior HF admission, creatinine >1.5 mg/dL) significantly increase the relative risk of 5-year clinical events.</p>
od_______217::3718531b1821302ec100469ef823a400
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od_______217::4b7471a71b4092598066b060fe6cd0e4
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od_______217::6afa6f2827d8f3b2d142d2ce29912a7d
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od_______217::923283557e9493ef6b9ca5491200daba
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od_______217::bdcfe61629ce111f84a49b44dbe6a2b1
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od_______217::cba34d714bac436b4c3a83cc307b0e45
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