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19 results for “Bianchi”
Nicolò Bianchi (b3317)
<b>-- <a href="https://doi.org/10.5281/zenodo.11582199">Documentation</a> --</b><br><br><u>Name</u>: Nicolò Bianchi<br><u>musiXplora-ID</u>: b3317<br><u>musiXplora-URI</u>: <a href="https://musixplora.de/mxp/b3317">https://musixplora.de/mxp/b3317</a><br><u>Gender</u>: m<br><u>Date of Birth</u>: 29 May 1803<br><u>Place of Birth</u>: Albisola Superiore<br><u>Date of Death</u>: 04 January 1880<br><u>Place of Death</u>: Nizza<br><u>First Mentioned</u>: 1840<br><u>Sectors</u>: Instrumentenbau<br><u>Professions (Musical)</u>: Geigenbauer<br><u>Other Places of Activity</u>: Genua, Nizza, Paris<br><br><br><u>Portfolio:</u><br><table><tbody><tr><th>Group</th><th>Role</th><th>Name</th><th>mXp-ID</th></tr><tr><td>Sortimente</td><td>Sortiment</td><td>Geige</td><td><a href="https://musixplora.de/mxp/2001463">2001463</a></td></tr><tr><td>Sortimente</td><td>Sortiment</td><td>Bratsche</td><td><a href="https://musixplora.de/mxp/2001527">2001527</a></td></tr><tr><td>Sortimente</td><td>Sortiment</td><td>Violoncello</td><td><a href="https://musixplora.de/mxp/2001634">2001634</a></td></tr></tbody></table><br><br><u>Changelog</u>:<br> - v0.0.1: Initial Upload.<br>
The imprint on the cosmic microwave background (CMB) of Bianchi cosmologies
<p>These animations display the imprint that homogeneous but anisotropic Bianchi models induce in the cosmic microwave background (CMB).</p> <p> </p> <p> </p> <p>scalars_movie.mp4 : Bianchi VIIh/VII0 scalar modes, imprint on the CMB for varying morphology parameters (matter and dark-energy density, rotation scale of shear principal axes)</p> <p>vectors_movie.mp4: Bianchi VIIh/VII0 vector modes, imprint on the CMB for varying morphology parameters (matter and dark-energy density, rotation scale of shear principal axes)</p> <p>tensor_movie.mp4: Bianchi VIIh/VII0 regular tensor modes, imprint on the CMB for varying morphology parameters (matter and dark-energy density, rotation scale of shear principal axes)</p> <p>Additional fixed parameters for the three animations above:<br /> cold-dark-matter physical density: 0.112<br /> baryon physical density: 0.226<br /> Pattern orientation additionally fixed to put spiral in full view</p> <p>_____________________________</p> <p>SVTT_movie.mp4: combinations of Bianchi VIIh/VII0 scalar, vector, regular and irregular tensor modes for varying relative amplitudes of these degrees of freedom and phase angle.</p> <p>Additional fixed parameters:<br /> cold-dark-matter physical density: 0.112<br /> baryon physical density 0.0226<br /> matter density: 0.27<br /> dark energy density: 0.7<br /> rotation scale of shear principal axes: 0.5<br /> Pattern orientation additionally fixed to put spiral in full view</p>
Figures 2–7. Euchistus male genitalia. 2–4 in Description of the male of Euschistus (Euschistus) baranowskii Eger and Bianchi (Heteroptera: Pentatomidae: Pentatominae: Carpocorini)
Figures 2–7. Euchistus male genitalia. 2–4) E. (E.) baranowskii. 5–7) E. (E.) rugifer. 2, 5) pygophore, dorsal view. 3, 6) pygophore, posterior view. 5, 7) pygophore, ventral view (C = carina, IR = inferior ridge, Par = paramere, SR = superior ridge). Scale lines = 0.50 mm.
Figure 1 in Description of the male of Euschistus (Euschistus) baranowskii Eger and Bianchi (Heteroptera: Pentatomidae: Pentatominae: Carpocorini)
Figure 1. Euschistus (E.) baranowskii, habitus. Scale line = 1.0 mm.
Ipogeo di Torricchi - Tomba Bianchi
Source: Objaverse 1.0 / Sketchfab
FIGURES 22–23. 22 in Description of a new species of Chimarrhometra Bianchi, 1896 (Hemiptera: Heteroptera: Gerridae) from China
FIGURES 22–23. 22. Habitat of C. yunnanensis sp. n.; 23. adult C. yunnanensis sp. n. clinging to rock surface.
FIGURES 19–21 in Description of a new species of Chimarrhometra Bianchi, 1896 (Hemiptera: Heteroptera: Gerridae) from China
FIGURES 19–21. First gonocoxa (Gx1) and first gonopophysis (Go1) of Chimarrhometra spp. (females). 19. C. orientalis (Distant, 1879), Gx1+Go1; 20. C. orientalis (Distant, 1879), inner lobe of Go1; 21. C. yunnanensis sp. n., inner lobe of Go1.
FIGURES 13–18 in Description of a new species of Chimarrhometra Bianchi, 1896 (Hemiptera: Heteroptera: Gerridae) from China
FIGURES 13–18. Proctiger and paramere of Chimarrhometra spp. (males). 13–15. C. orientalis (Distant, 1879), 13. proctiger in dorsal view; 14. paramere in ventral view; 15. paramere in dorsal view. 16–18. C. yunnanensis sp. n.: 16. proctiger in dorsal view; 17. paramere in ventral view; 18. paramere in dorsal view. Scale = 0.2 mm.
FIGURES 9–12 in Description of a new species of Chimarrhometra Bianchi, 1896 (Hemiptera: Heteroptera: Gerridae) from China
FIGURES 9–12. Pygophore of Chimarrhometra spp. (males). 9. C. orientalis (Distant, 1879), ventral view; 10. C. orientalis (Distant, 1879), dorsal view; 11. C. yunnanensis sp. n., ventral view; 12. C. yunnanensis sp. n., dorsal view; Scale = 0.2 mm.
FIGURES 5–8 in Description of a new species of Chimarrhometra Bianchi, 1896 (Hemiptera: Heteroptera: Gerridae) from China
FIGURES 5–8. Abdominal segment VIII of Chimarrhometra spp. (males). 5. C. orientalis (Distant, 1879), dorsal view; 6. C. orientalis (Distant, 1879), lateral view; 7. C. yunnanensis sp. n., dorsal view; 8. C. yunnanensis sp. n., lateral view; Scale = 0.2 mm.
FIGURES 1–4 in Description of a new species of Chimarrhometra Bianchi, 1896 (Hemiptera: Heteroptera: Gerridae) from China
FIGURES 1–4. Habitus of Chimarrhometra spp. 1. C. orientalis (Distant, 1879), male; 2. C. orientalis (Distant, 1879), female; 3. C. yunnanensis sp. n., male (holotype); 4. C. yunnanensis sp. n., female (paratype); Scale = 4.0 mm.
Astrosat/UVIT reduced images and HST/STIS merged spectra for the red-giant binary 2MASSJ05215658+4359220, published by Bianchi, L et al. 2024, ApJ ( DOI: 10.3847/1538-4357/ad712f ; arxiv:2409.06906)
<p>Reduced and calibrated datasets used in the paper: </p> <p>Bianchi, Luciana; Hutchings, John; Bohlin, Ralph; Thilker, David; and Berti, Emanuele 2024, ApJ, in press; DOI: 10.3847/1538-4357/ad712f ; <a href="https://arxiv.org/abs/2409.06906" target=" ">arxiv:2409.06906</a><br>Title:<em> Revealing the elusive companion of the red-giant binary 2MASSJ05215658+4359220 from UV HST and Astrosat/UVIT data.</em></p> <p>See<em> </em>the original paper for details on the data reduction. Please reference the original paper if using these datasets. </p> <p><em>1) </em>STIS_2mj05215.mrg</p> <p>The file includes the three-ranges spectra extracted and combined: G230L+G430L+G750L. Ascii file. Columns are: WAVELENGTH (˚A), COUNT-RATE (counts cm−2 s−1 pixel−1), FLUX (ergs cm−2 s−1 ˚A−1), STAT-ERROR (ergs cm−2 s−1 ˚A−1), SYS-ERROR (ergs cm−2 s−1 ˚A−1), NPTS (the number of co-added spectra for that pixel), TIME (total exposure time at that pixel in seconds), QUAL ( 1=good data, 0=possibly poor data quality). The DOI: 10.17909/tvvw-4e47 refers to the original HST data, not to te reduced and combined dataset.</p> <p>The file is also available from the author's website at : http:/dolomiti.pha.jhu.edu/uvsky/RGbinary_2MASSJ05215658+4359220/STISspectra/STIS_2mj05215.mrg</p> <p>2) UVITimages.tar. Tar file containing the UVIT images, reconstructed from the photon-counting archival data, calibrated accounting for dead-time corrections, in .fits format</p> <p>The tar file contains the following .fits files of the reconstructed images, where the “NORM EXPARRAY” files are the normalized relative response maps across the field, expressed as 0 to 1. So, the effective exposure time at a pixel position is RDCDTIME multiplied by this image. The ”NORMEXP IMAGE” is the science image, that must be divided by the product of RDCDTIME and the NORM EXPARRAY image on a pixel-by-pixel basis, to obtain counts s−1 pixel−1</p> <p>2MASSJ05215658+4359220_FUV_CaF2___MASTER_NORM_EXPARRAY_A10_093T01_9000004128.fits</p> <p>2MASSJ05215658+4359220_FUV_CaF2___MASTER_NORM_EXPARRAY_A10_093T01_9000004266.fits</p> <p>2MASSJ05215658+4359220_FUV_CaF2___MASTER_NORM_EXPARRAY_Merged.fits</p> <p>2MASSJ05215658+4359220_FUV_CaF2___MASTER_NORMEXP_IMAGE_A10_093T01_9000004128.fits</p> <p>2MASSJ05215658+4359220_FUV_CaF2___MASTER_NORMEXP_IMAGE_A10_093T01_9000004266.fits</p> <p>2MASSJ05215658+4359220_FUV_CaF2___MASTER_NORMEXP_IMAGE_Merged.fits</p> <p>2MASSJ05215658+4359220_FUV_Sapphire___MASTER_NORM_EXPARRAY_A10_093T01_9000004128.fits</p> <p>2MASSJ05215658+4359220_FUV_Sapphire___MASTER_NORM_EXPARRAY_A10_093T01_9000004266.fits</p> <p>2MASSJ05215658+4359220_FUV_Sapphire___MASTER_NORM_EXPARRAY_Merged.fits</p> <p>2MASSJ05215658+4359220_FUV_Sapphire___MASTER_NORMEXP_IMAGE_A10 093T01_9000004128.fits</p> <p>2MASSJ05215658+4359220_FUV_Sapphire___MASTER_NORMEXP_IMAGE_A10_093T01_9000004266.fits</p> <p>2MASSJ05215658+4359220_FUV_Sapphire___MASTER_NORMEXP_MAGE_Merged.fits</p> <p>The tar file is also available from the author's website at: http:/dolomiti.pha.jhu.edu/uvsky/RGbinary_2MASSJ05215658+4359220/UVITimages/UVITimages.tar</p>
FIGURE 1 in Grammatonotus bianchi, a new species of splendid perch (Percoidei: Callanthiidae) from Myanmar, northeastern Indian Ocean
FIGURE 1. Localities of Grammatonotus spp. within the Indian Ocean. Orange markers represents G. bianchi sp. nov.; white triangle G. lanceolatus; white square G. sp.1 (Mascarenes); and white star G. sp. 2 (Mozambique).
FIGURE 3 in Grammatonotus bianchi, a new species of splendid perch (Percoidei: Callanthiidae) from Myanmar, northeastern Indian Ocean
FIGURE 3. Radiograph of Grammatonotus bianchi sp. nov. Holotype, SAIAB 208486, 68.7 mm SL (a–c); a: whole specimen in lateral view; b: close-up illustrating the configurations of supraneural bones (sn), anterior neural spines (ns), and anterior dorsal pterygiophore (pt); c: close-up of caudal skeleton where: (epu) epuralia, (hp) hypurals, (npu-2) neural process, (ph) parhypurale, (un) uroneurale (images by Mark Lisher & Nkosinathi Mazungula).
FIGURE 2 in Grammatonotus bianchi, a new species of splendid perch (Percoidei: Callanthiidae) from Myanmar, northeastern Indian Ocean
FIGURE 2. Fresh coloration of Grammatonotus bianchi sp. nov. shortly after collection: (a) Holotype, SAIAB 208486, 68.7 mm SL (photo by P.N. Psomadakis); (b) Specimen collected in 2015, 121 mm TL (photo by O. Alvheim) for which voucher is unavailable (specimen lost).
Supplementary material 1 from: Ravera S, Puglisi M, Vizzini A, Totti C, Barberis G, Bianchi E, Boemo A, Bonini I, Bouvet D, Cocozza C, Dagnino D, Di Nuzzo L, Fačkovcová Z, Gheza G, Gianfreda S, Giordani P, Hilpold A, Hurtado P, Köckinger H, Isocrono D, Loppi S, Malicek J, Matino C, Minuto L, Nascimbene J, Pandeli G, Paoli L, Puntillo D, Puntillo M, Rossi A, Sguazzin F, Spitale D, Stifter S, Turcato C, Vazzola S (2020) Notulae to the Italian flora of algae, bryophytes, fungi and lichens: 10. Italian Botanist 10: 83-99. https://doi.org/10.3897/italianbotanist.10.59352
Figure S1
FIGURE 24 in Description of a new species of Chimarrhometra Bianchi, 1896 (Hemiptera: Heteroptera: Gerridae) from China
FIGURE 24. Geographical distribution of species of Chimarrhometra.
Data set from Ranucci M, Bianchi P, Cotza M, Beccaris C, Silvetti S, Isgrò G, Giamberti A, Baryshnikova E. Fibrinogen levels and postoperative chest drain blood loss in low-weight (<10 kg) children undergoing cardiac surgery. Perfusion. 2019 Nov;34(8):629-636. doi: 10.1177/0267659119854246. Epub 2019 Jun 28. PMID: 31250738.
<p>Data set from Ranucci M, Bianchi P, Cotza M, Beccaris C, Silvetti S, Isgrò G, Giamberti A, Baryshnikova E. Fibrinogen levels and postoperative chest drain blood loss in low-weight (<10 kg) children undergoing cardiac surgery. Perfusion. 2019 Nov;34(8):629-636. doi: 10.1177/0267659119854246. Epub 2019 Jun 28. PMID: 31250738.</p> <p> </p> <p>This is the abstract:</p> <p><strong>Introduction: </strong> Low-weight (<10 kg) children undergoing cardiac surgery with cardiopulmonary bypass are prone to dilution and consumption of soluble coagulation factors and fibrinogen. Low levels of fibrinogen may represent a possible cause of severe postoperative chest drain blood loss. The present study investigates the association between post-cardiopulmonary bypass fibrinogen levels and postoperative chest drain blood loss and severe bleeding, aiming to identify possible cut-off values to trigger specific interventions.</p> <p><strong>Methods: </strong> Prospective cohort study on 77 patients weighing <10 kg undergoing cardiac surgery with cardiopulmonary bypass. Haemostasis and coagulation data were collected before surgery (standard tests and thromboelastometry), after protamine (thromboelastometry) and at the arrival in the intensive care unit (standard tests). The primary outcome variable was severe bleeding (chest drain blood loss >30 ml kg<sup>-1</sup>/24h).</p> <p><strong>Results: </strong> Factors being independently associated with severe bleeding were the international normalized ratio and the fibrinogen levels at the arrival in the intensive care unit. Once corrected for other confounders, fibrinogen levels had an odds ratio of 0.2 (95% confidence interval = 0.011-0.54) per 1 gL<sup>-1</sup> for severe bleeding. The discrimination power was fair (area under the curve = 0.770). The best cut-off value was identified at a fibrinogen level of 150 mg dL<sup>-1</sup>, with a sensitivity of 52%, a specificity of 85% and a positive predictive value of 60% for severe bleeding.</p> <p><strong>Conclusion: </strong> Both a prolonged international normalized ratio and low fibrinogen levels were predictive for severe bleeding, underscoring the role of coagulation factors dilution and consumption in this specific patient population.</p> <p> </p>
Data set and 3d model from Emendi M, Sturla F, Ghosh RP, Bianchi M, Piatti F, Pluchinotta FR, Giese D, Lombardi M, Redaelli A, Bluestein D. Patient-Specific Bicuspid Aortic Valve Biomechanics: A Magnetic Resonance Imaging Integrated Fluid-Structure Interaction Approach. Ann Biomed Eng. 2020 Aug 17. doi: 10.1007/s10439-020-02571-4. Epub ahead of print. PMID: 32804291.
<p>Data set and 3d model from Emendi M, Sturla F, Ghosh RP, Bianchi M, Piatti F, Pluchinotta FR, Giese D, Lombardi M, Redaelli A, Bluestein D. Patient-Specific Bicuspid Aortic Valve Biomechanics: A Magnetic Resonance Imaging Integrated Fluid-Structure Interaction Approach. Ann Biomed Eng. 2020 Aug 17. doi: 10.1007/s10439-020-02571-4. Epub ahead of print. PMID: 32804291.</p> <p> </p> <p>This is the abstract:</p> <p>Congenital bicuspid aortic valve (BAV) consists of two fused cusps and represents a major risk factor for calcific valvular stenosis. Herein, a fully coupled fluid-structure interaction (FSI) BAV model was developed from patient-specific magnetic resonance imaging (MRI) and compared against in vivo 4-dimensional flow MRI (4D Flow). FSI simulation compared well with 4D Flow, confirming direction and magnitude of the flow jet impinging onto the aortic wall as well as location and extension of secondary flows and vortices developing at systole: the systolic flow jet originating from an elliptical 1.6 cm<sup>2</sup> orifice reached a peak velocity of 252.2 cm/s, 0.6% lower than 4D Flow, progressively impinging on the ascending aorta convexity. The FSI model predicted a peak flow rate of 22.4 L/min, 6.7% higher than 4D Flow, and provided BAV leaflets mechanical and flow-induced shear stresses, not directly attainable from MRI. At systole, the ventricular side of the non-fused leaflet revealed the highest wall shear stress (WSS) average magnitude, up to 14.6 Pa along the free margin, with WSS progressively decreasing towards the belly. During diastole, the aortic side of the fused leaflet exhibited the highest diastolic maximum principal stress, up to 322 kPa within the attachment region. Systematic comparison with ground-truth non-invasive MRI can improve the computational model ability to reproduce native BAV hemodynamics and biomechanical response more realistically, and shed light on their role in BAV patients' risk for developing complications; this approach may further contribute to the validation of advanced FSI simulations designed to assess BAV biomechanics.</p> <p> </p>
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