Auswahl der wissenschaftlichen Literatur zum Thema „Fraction massique“

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Zeitschriftenartikel zum Thema "Fraction massique"

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Ousmane, Moctar, Dianda Boureima, Thierry Sikoudouin Maurice K.Y, et al. "ETUDE DES PERFORMANCES THERMIQUES DUN SECHOIR SOLAIRE." International Journal of Advanced Research 12, no. 01 (2024): 1062–72. http://dx.doi.org/10.21474/ijar01/18224.

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Les populations ouest africaines produisent de grandes quantites de recoltes. Malheureusement faute de moyens de conservation, ces produits pourrissent. Cest pour cette raison que nous nous sommes interesses au sechage solaire des produits agro-alimentaires avec comme produit la banana douce. Lobjectif de cette publication est letude des performances thermiques dun sechoir solaire à absorbeur à ailettes. Les materiels utilises sont : un sechoir complet constitue de cinq claies, des tranches de banane douce, dune balance de precision et dun enregistreur automatique de temperatures. Levolution d
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Davison, Thomas A., Mark A. Norris, Ryan Leaman, Harald Kuntschner, Alina Boecker, and Glenn van de Ven. "Mapping accreted stars in early-type galaxies across the mass–size plane." Monthly Notices of the Royal Astronomical Society 507, no. 2 (2021): 3089–112. http://dx.doi.org/10.1093/mnras/stab2362.

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ABSTRACT Galaxy mergers are instrumental in dictating the final mass, structure, stellar populations, and kinematics of galaxies. Cosmological galaxy simulations indicate that the most massive galaxies at z = 0 are dominated by high fractions of ‘ex-situ’ stars, which formed first in distinct independent galaxies, and then subsequently merged into the host galaxy. Using spatially resolved MUSE spectroscopy we quantify and map the ex-situ stars in thirteen massive early-type galaxies. We use full spectral fitting together with semi-analytic galaxy evolution models to isolate the signatures in t
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Sharma, Ray S., Alyson M. Brooks, Michael Tremmel, Jillian Bellovary, Angelo Ricarte, and Thomas R. Quinn. "A Hidden Population of Massive Black Holes in Simulated Dwarf Galaxies." Astrophysical Journal 936, no. 1 (2022): 82. http://dx.doi.org/10.3847/1538-4357/ac8664.

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Abstract We explore the characteristics of actively accreting massive black holes (MBHs) within dwarf galaxies in the Romulus25 cosmological hydrodynamic simulation. We examine the MBH occupation fraction, X-ray active fractions, and active galactic nucleus (AGN) scaling relations within dwarf galaxies of stellar mass 108 M ⊙ < M star < 1010 M ⊙ out to redshift z = 2. In the local universe, the MBH occupation fraction is consistent with observed constraints, dropping below unity at M star < 3 × 1010 M ⊙, M 200 < 3 × 1011 M ⊙. Local dwarf AGN in Romulus25 follow observed scaling rel
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Schootemeijer, Abel, Danny J. Lennon, Miriam Garcia, Norbert Langer, Ben Hastings, and Christoph Schürmann. "Massive stars in metal-poor dwarf galaxies are often extreme rotators." Proceedings of the International Astronomical Union 18, S361 (2022): 63–69. http://dx.doi.org/10.1017/s1743921322002538.

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AbstractWe probe how common extremely rapid rotation is among massive stars in the early universe by measuring the OBe star fraction in nearby metal-poor dwarf galaxies. We apply a new method that uses broad-band photometry to measure the galaxy-wide OBe star fractions in the Magellanic Clouds and three more distant, more metal-poor dwarf galaxies. We find OBe star fractions of ∼20% in the Large Magallanic Cloud (0.5Zȯ), and ∼30% in the Small Magellanic Cloud (0.2Zȯ) as well as in the so-far unexplored metallicity range 0.1 Z/Zȯ < 0.2 occupied by the other three dwarf galaxies. Our results
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Shenton, Robert G., René D. Oudmaijer, and Stuart L. Lumsden. "Binarity in Massive Young Stellar Objects." Proceedings of the International Astronomical Union 18, S361 (2022): 556–58. http://dx.doi.org/10.1017/s1743921322001909.

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AbstractMost massive stars (up to 100%) are thought to be in binary systems. The multiplicity of massive stars seems to be intrinsically linked to their formation and evolution, and so Massive Young Stellar Objects are key in observing this early stage of star formation. We have surveyed hundreds of MYSOs across the Galaxy from the RMS catalogue, using UKIDSS and VVV point source data. Preliminary results show binary fractions of 44±3% for the UKIDSS sample and 32±3% for the VVV sample. In addition we use the K-band magnitudes as a proxy for the companion mass, and find a significant fraction
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Contini, Emanuele, Seyoung Jeon, Jinsu Rhee, San Han, and Sukyoung K. Yi. "The Intracluster Light and Its Link with the Dynamical State of the Host Group/Cluster: The Role of the Halo Concentration." Astrophysical Journal 958, no. 1 (2023): 72. http://dx.doi.org/10.3847/1538-4357/acfd25.

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Abstract We investigate the role of halo concentration in the formation of intracluster light (ICL) in galaxy groups and clusters, as predicted by a state-of-the-art semianalytic model of galaxy formation, coupled with a set of high-resolution dark-matter-only simulations. The analysis focuses on how the fraction of ICL correlates with halo mass, concentration, and fraction of early-type galaxies (ETGs) in a large sample of groups and clusters with 13.0 ≤ log M halo ≤ 15.0 . The fraction of ICL follows a normal distribution, a consequence of the stochastic nature of the physical processes resp
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Mukherjee, Sampath, Léon V. E. Koopmans, Crescenzo Tortora, et al. "SEAGLE – III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations." Monthly Notices of the Royal Astronomical Society 509, no. 1 (2021): 1245–51. http://dx.doi.org/10.1093/mnras/stab3014.

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ABSTRACT The central dark-matter fraction of galaxies is sensitive to feedback processes during galaxy formation. Strong gravitational lensing has been effective in the precise measurement of the dark-matter fraction inside massive early-type galaxies. Here, we compare the projected dark-matter fraction of early-type galaxies inferred from the SLACS (Sloan Lens ACS Survey) strong-lens survey with those obtained from the Evolution and Assembly of GaLaxies and their Environment (EAGLE), Illustris, and IllustrisTNG hydrodynamical simulations. Previous comparisons with some simulations revealed a
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Grylls, Philip J., F. Shankar, and C. J. Conselice. "The significant effects of stellar mass estimation on galaxy pair fractions." Monthly Notices of the Royal Astronomical Society 499, no. 2 (2020): 2265–75. http://dx.doi.org/10.1093/mnras/staa2966.

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ABSTRACT Theoretical models suggest that galaxy mergers may have profoundly shaped galaxy morphologies through cosmic time. However, observational estimates of galaxy pair fractions, and implied galaxy mergers, still do not converge, suggesting different numbers and redshift evolution. This paper explores the connection between stellar mass estimation and the pair fraction of galaxies using $\rm {\small STEEL}$, the Statistical sEmi-Emprical modeL, in which galaxies are mapped on to host dark matter haloes via a stellar mass–halo mass (SMHM) relation. As haloes of different mass are predicted
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Yoo, Taehwa, Taysun Kimm, and Joakim Rosdahl. "On the origin of low escape fractions of ionizing radiation from massive star-forming galaxies at high redshift." Monthly Notices of the Royal Astronomical Society 499, no. 4 (2020): 5175–93. http://dx.doi.org/10.1093/mnras/staa3187.

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ABSTRACT The physical origin of low escape fractions of ionizing radiation derived from massive star-forming galaxies at z ∼ 3–4 is not well understood. We perform idealized disc galaxy simulations to understand how galactic properties such as metallicity and gas mass affect the escape of Lyman continuum (LyC) photons using radiation-hydrodynamic simulations with strong stellar feedback. We find that the luminosity-weighted escape fraction from a metal-poor (Z = 0.002) galaxy embedded in a halo of mass $M_{\rm h}\simeq 10^{11}\, \mathrm{M}_\odot$ is $\left\langle {f_{\rm esc}^{\rm 3D}}\right\r
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Liu, Shuang, Yizhou Gu, Qirong Yuan, et al. "Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 ≤ z ≤ 2.5 in 3D-HST/CANDELS." Astrophysical Journal 923, no. 1 (2021): 46. http://dx.doi.org/10.3847/1538-4357/ac2817.

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Abstract To figure out the effect of stellar mass and local environment on morphological transformation and star formation quenching in galaxies, we use the massive (M * ≥ 1010 M ⊙) galaxies at 0.5 ≤ z ≤ 2.5 in five fields of 3D-HST/CANDELS. Based on the UVJ diagnosis and the possibility of possessing a spheroid, our sample of massive galaxies is classified into four populations: quiescent early-type galaxies (qEs), quiescent late-type galaxies (qLs), star-forming early-type galaxies (sEs), and star-forming late-type galaxies (sLs). It is found that the quiescent fraction is significantly elev
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Dissertationen zum Thema "Fraction massique"

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Rebillard-Soulie, Alex. "Etendre nοs cοnnaissances sur la matière nucléaire chaude dans la régiοn de faible densité". Electronic Thesis or Diss., Normandie, 2024. http://www.theses.fr/2024NORMC244.

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Les clusters légers dans la matière nucléaire apparaissent à des densités inférieures à la densité de saturation nucléaire. Ils peuvent jouer un rôle important dans des scénarios astrophysiques comme les supernovae à effondrement de cœur, où les propriétés de la matière nucléaire influence la propagation de l'onde de choc et le parcours des neutrinos émis. À de telles densités, des effets de milieu sont présents et modifient les propriétés des clusters formés, leur abondance et, par conséquent, la dynamique des supernovae. Nous avons utilisé un modèle champ moyen relativiste (RMF) avec des clu
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Hennig, C., J. J. Mohr, A. Zenteno, et al. "Galaxy Populations in Massive Galaxy Clusters to z = 1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/623801.

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We study the galaxy populations in 74 Sunyaev-Zeldovich effect selected clusters from the South Pole Telescope survey, which have been imaged in the science verification phase of the Dark Energy Survey. The sample extends up to z similar to 1.1 with 4 x 10(14)M(circle dot) <= M-200 <= 3 x 10(15)M(circle dot). Using the band containing the 4000 angstrom break and its redward neighbour, we study the colour-magnitude distributions of cluster galaxies to similar to m(*) + 2, finding that: (1) The intrinsic rest frame g - r colour width of the red sequence (RS) population is similar to 0.03 out to
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Parida, Priyabrata. "Stochastic Geometry Perspective of Massive MIMO Systems." Diss., Virginia Tech, 2021. http://hdl.handle.net/10919/105089.

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Owing to its ability to improve both spectral and energy efficiency of wireless networks, massive multiple-input multiple-output (mMIMO) has become one of the key enablers of the fifth-generation (5G) and beyond communication systems. For successful integration of this promising physical layer technique in the upcoming cellular standards, it is essential to have a comprehensive understanding of its network-level performance. Over the last decade, stochastic geometry has been instrumental in obtaining useful system design insights of wireless networks through accurate and tractable theoretical
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Bücher zum Thema "Fraction massique"

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Iliopoulos, John. A Brief History of Cosmology. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198805175.003.0002.

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We present the evolution of our ideas concerning the history of the Cosmos. They are based on Einstein’s theory of General Relativity in which E.P. Hubble and G. Lemaître brought two fundamental new concepts: the expansion of the Universe and the model of the Big Bang. They form the basic elements of the modern theory of Cosmology. We present very briefly the observational evidence which corroborates this picture based on a vast amount of data, among which the most recent ones come from the Planck mission with a detailed measurement of the cosmic microwave background (CMB) radiation. We show t
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Buchteile zum Thema "Fraction massique"

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Li, Chengyuan. "Binary Fraction in Young Massive Star Clusters." In Springer Theses. Springer Singapore, 2017. http://dx.doi.org/10.1007/978-981-10-5681-9_3.

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Le-Ngoc, Tho, and Ruikai Mai. "Nonlinear Hybrid Precoding for Massive MIMO with Fractional Frequency Reuse." In Hybrid Massive MIMO Precoding in Cloud-RAN. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-030-02158-0_5.

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Hwang, Dr Nian Chih, and Dr Michael Sinclair. "Induction of anaesthesia, peroperative preparation, and investigations." In Cardiac Anaesthesia. Oxford University PressNew York, NY, 1992. http://dx.doi.org/10.1093/oso/9780192628367.003.0014.

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Abstract In the induction room, the patient receives ECG and pulse oximetry monitoring while breathing oxygen via a clear facemask. Under local anaesthesia, venous access is gained with a 14 G (2 mm diameter) cannula and invasive arterial blood pressure monitoring is obtained via a 20 G (1 mm diameter) arterial cannula inserted into an artery, usually the radial artery. Two 14 G venous cannulas are inserted for surgery which may require massive blood transfusion. Central venous catheterization is necessary for the monitoring of right atrial filling pressure and the infusion of inotropes and va
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Noble, Denis. "The Conductor: Downward Causation." In The Music of Life. Oxford University PressOxford, 2006. http://dx.doi.org/10.1093/oso/9780199295739.003.0004.

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Abstract The organist works from a very dififerent perspective to that of any of the individual pipes of his organ. Although in real organs the pipes themselves are often physically above the player, metaphorically speaking he surveys the keyboards and pedals from above, seeing patterns and musical forms that he constrains the instrument to follow. To play a piece on the organ is to call on many pipes simultaneously. In a complex piece, most of the pipes may at some point come into play. The organist must cause this massive apparatus to express its potential in an ordered way. These ordered pa
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"Herodotus: The History of the Persian Wars." In Schlager Anthology of Women’s History. Schlager Group Inc., 2023. https://doi.org/10.3735/9781961844025.book-part-005.

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Herodotus was a Greek historian who lived from approximately 484 to 420 BCE. Much of his life was overshadowed by the Greco-Persian Wars of approximately 499–449 BCE, a series of bitter conflicts pitting the massive Persian Empire against the disunited and fractious Greek city-states. Herodotus examined these conflicts using a unique approach. Earlier Greek historians narrated events from an unscientific perspective, citing the gods as the primary agents of historical development. Herodotus, in contrast, approached the Greco-Persian Wars from a rationalist perspective, attributing the outcome
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Bailyn, Charles D. "Supermassive Black Holes." In What Does a Black Hole Look Like? Princeton University Press, 2014. http://dx.doi.org/10.23943/princeton/9780691148823.003.0005.

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This chapter focuses on supermassive black holes, which are sometimes abbreviated “SMBHs.” Stellar-mass black holes are clearly common consequences of stellar evolution, but they are not the only kinds of black holes identified by astronomers. Much more massive black holes are located in the center of many, and perhaps all, galaxies. These black holes are referred to as supermassive black holes. They are responsible for a range of phenomena originating from objects described as active galactic nuclei (AGN), which were first observed in the form of quasi-stellar objects (QSOs) or quasars. AGN a
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Can, Taner. "Why Go Digital?" In Exploration of the Intersection of Corpus Linguistics and Language Science. IGI Global, 2025. https://doi.org/10.4018/979-8-3693-8146-5.ch003.

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Since the rise of New Criticism in the 1920s, literary studies has undergone various theoretical ‘turns'—linguistic, historicist, cultural, and others—that have transformed the field. Despite these innovations, the method of analysis has remained largely unchanged, with close reading still central to scholarly practice. However, the vast amount of data available through e-archives has rendered close reading obsolete as a sole method of literary analysis. Big data and computational technologies are revolutionizing the field, particularly through computational distant reading, which can analyze
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Templin, Christian, Jelena R. Templin-Ghadri, and Thomas F. Lüscher. "Takotsubo Syndrome." In Manual of Cardiovascular Medicine. Oxford University Press, 2021. http://dx.doi.org/10.1093/med/9780198850311.003.0015.

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Takotsubo syndrome is named after the octopus trap used by Japanese fisherman and reflects the shape of the left ventricle during systole in patients with this condition. Takotsubo is an acute cardiac syndrome (ACS), starting with chest pain, dyspnoea, ECG changes, sometimes presenting as STEMI or non-STEMI, and in some cases with hypotension, arrhythmias, pump failure, and sudden death. In most patients, the massive left ventricular dysfunction with a reduction in ejection fraction down to 35% is reversible over days, weeks, and months. However, around 4% of patients do not survive the acute
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Piantadosi, Claude A. "Weapons of Mass Destruction." In The Biology of Human Survival. Oxford University PressNew York, NY, 2003. http://dx.doi.org/10.1093/oso/9780195165012.003.0019.

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Abstract The reason to cover weapons of mass destruction in a book about extreme environments is because they have the potential to forever alter life on earth. The inconceivable destructive power of modern thermonuclear devices is antithetical to civilization, which requires a sophisticated infrastructure. The deaths from detonation of even one nuclear warhead over a population center would dwarf the September 11, 2001, World Trade Center disaster. The exploitation of fuel-loaded jets to attack the World Trade Center produced an unusual situation by trapping the victims inside the twin towers
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Bordo, Michael D. "The Lender of Last Resort: Alternative Views and Historical Experience." In Financial Crises, Contagion, and the Lender of Last Resort. Oxford University PressOxford, 2002. http://dx.doi.org/10.1093/oso/9780199247202.003.0006.

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Abstract Recent liquidity assistance to failing savings and loans and banks (some insolvent and some large) in the U.S. and similar rescues abroad have prompted renewed interest in the topic of the lender of last resort. Under the classical doctrine, the need for a lender of last resort arises in a fractional reserve banking system when a banking panic, defmed as a massive scramble for high-powered money, threatens the money stock and, hence, the level of economic activity. The lender of last resort can allay an incipient panic by timely assurance that it will provide whatever high-powered mon
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Konferenzberichte zum Thema "Fraction massique"

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Matoušek, Václav, Robert Visintainer, John Furlan, and Anders Sellgren. "Frictional Head Loss of Various Bimodal Settling Slurry Flows in Pipe." In ASME-JSME-KSME 2019 8th Joint Fluids Engineering Conference. American Society of Mechanical Engineers, 2019. http://dx.doi.org/10.1115/ajkfluids2019-5395.

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Abstract Pipe flows of bimodal settling slurries exhibit frictional head losses quite different from those determined simply as a sum of loss contributions by the individual fractions. Mechanisms governing flow friction and resulting from an interaction of grains of different fractions in transported slurry are not well understood. This makes a prediction of the frictional head loss in flows of bimodal slurries with Newtonian carrier uncertain. An extensive experimental campaign was conducted in GIW Hydraulic Laboratory in 2016 with slurries of four narrow graded fractions of the virtually sam
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Atzeni, Italo, Jesus Arnau, and Merouane Debbah. "Fractional pilot reuse in massive MIMO systems." In 2015 ICC - 2015 IEEE International Conference on Communications Workshops (ICC). IEEE, 2015. http://dx.doi.org/10.1109/iccw.2015.7247312.

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Zhou, Ruifeng, Youhua Fu, and Hairong Wang. "Uplink Asynchronous Fractional Pilots Scheduling in Massive MIMO System." In 2018 IEEE 18th International Conference on Communication Technology (ICCT). IEEE, 2018. http://dx.doi.org/10.1109/icct.2018.8600231.

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Su, Liyan, and Chenyang Yang. "Fractional Frequency Reuse Aided Pilot Decontamination for Massive MIMO Systems." In 2015 IEEE 81st Vehicular Technology Conference (VTC Spring). IEEE, 2015. http://dx.doi.org/10.1109/vtcspring.2015.7145845.

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Fan, Jiancun, and Weiqi Li. "Analysis and Optimization of Fractional Pilot Reusein Massive MIMO Systems." In 2017 IEEE 85th Vehicular Technology Conference (VTC Spring). IEEE, 2017. http://dx.doi.org/10.1109/vtcspring.2017.8108235.

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Fan, Jiancun, Weiqi Li, Ying Zhang, and Jianguo Deng. "Fractional Pilot Reuse with Vertical Sectorization in Massive MIMO Systems." In 2017 IEEE 85th Vehicular Technology Conference (VTC Spring). IEEE, 2017. http://dx.doi.org/10.1109/vtcspring.2017.8108331.

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Peng, Jingyi, and Yuhong Wang. "Fractional Fourier Transform Based Channel Estimation in Massive MIMO Systems." In 2023 IEEE 2nd International Conference on Electrical Engineering, Big Data and Algorithms (EEBDA). IEEE, 2023. http://dx.doi.org/10.1109/eebda56825.2023.10090634.

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Thanh Tam, Nguyen, Matthias Weidlich, Duong Chi Thang, Hongzhi Yin, and Nguyen Quoc Viet Hung. "Retaining Data from Streams of Social Platforms with Minimal Regret." In Twenty-Sixth International Joint Conference on Artificial Intelligence. International Joint Conferences on Artificial Intelligence Organization, 2017. http://dx.doi.org/10.24963/ijcai.2017/397.

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Today's social platforms, such as Twitter and Facebook, continuously generate massive volumes of data. The resulting data streams exceed any reasonable limit for permanent storage, especially since data is often redundant, overlapping, sparse, and generally of low value. This calls for means to retain solely a small fraction of the data in an online manner. In this paper, we propose techniques to effectively decide which data to retain, such that the induced loss of information, the regret of neglecting certain data, is minimized. These techniques enable not only efficient processing of massiv
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Hburi, Ismail, and Hamed Al-Raweshidy. "Uplink performance of cellular massive MIMO with fractional power control: Asymptotic analysis." In IEEE EUROCON 2017 -17th International Conference on Smart Technologies. IEEE, 2017. http://dx.doi.org/10.1109/eurocon.2017.8011075.

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Ruperee, Amrita, and Shikha Nema. "Fractional frequency reuse to enhance down link performance in MU Massive MIMO." In 2016 International Conference on Wireless Communications, Signal Processing and Networking (WiSPNET). IEEE, 2016. http://dx.doi.org/10.1109/wispnet.2016.7566451.

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Berichte der Organisationen zum Thema "Fraction massique"

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Lougheed, H. D., M. B. McClenaghan, D. Layton-Matthews, and M. I. Leybourne. Indicator minerals in fine-fraction till heavy-mineral concentrates determined by automated mineral analysis: examples from two Canadian polymetallic base-metal deposits. Natural Resources Canada/CMSS/Information Management, 2022. http://dx.doi.org/10.4095/328011.

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Exploration under glacial sediment cover is a necessary part of modern mineral exploration in Canada. Traditional indicator methods use visual examination to identify mineral grains in the 250 to 2000 µm fraction of till heavy-mineral concentrates (HMC). This study tests automated mineralogical methods using scanning electron microscopy to identify indicator minerals in the fine (&amp;amp;lt;250 µm) HMC fraction of till. Automated mineralogy of polished grains from the fine HMC enables rapid data collection (10 000-300 000 grains/sample). Samples collected near two deposits were used to test t
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Perl, M. The search for fractional charge elemental particles and very massive particles in bulk matter. Office of Scientific and Technical Information (OSTI), 2000. http://dx.doi.org/10.2172/753254.

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Cawood, T. K., and J. M. Peter. The geology of critical battery metals: a spotlight on Co in VMS deposits and Li in pegmatites. Natural Resources Canada/CMSS/Information Management, 2024. http://dx.doi.org/10.4095/332348.

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As we move away from a fossil fuel-driven economy, the demand for metals used in energy-dense, rechargeable batteries is increasing; these include cobalt and lithium. Although cobalt is mostly obtained as a by-product from nickel and copper mining, significant amounts also occur in volcanogenic massive sulfide (VMS) deposits, of which Canada has many. However, the primary controls on cobalt distribution in VMS deposits are poorly understood, and may be affected by deformation and metamorphism. We show that cobalt can occur in pyrite, which retains its primary composition through greenschist fa
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Charusiri, Punya, Wasant Pongsapich, and Chakkaphan Sutthirat. Petrochemistry of probable gem-bearing basalts in Sop Prap-Ko Kha Area, Changwat Lampang : research report. Chulalongkorn University, 1996. https://doi.org/10.58837/chula.res.1996.17.

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The project area covers approximately 300 km[superscript 2] encompassing parts of Amphoe Sop Prap, Amphoe Ko Kha, and Amphoe Mae Tha of Changwat Lampang. The area is mainly occupied by sedimentary (and metamorphic) rocks of Permian, Triassic, Tertiary and Quaternary ages. The Triassic rocks include the Phra That, the Pha Kan, and the Hong Hoi Formations of the Lampang Group. Igneous rocks comprise Permo-Triassic volcanics, Triassic granodiorite, and Cenozoic basalts. Sapphires are frequently found in alluvial and residual deposits, particularly in the northern basaltic area. Sapphires in the s
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