Search Results - "Unicode"
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VLT/ERIS Observations of the V960 Mon System: A Dust-embedded Substellar Object Formed by Gravitational Instability?
Published 2025-01-01“…The object is detected at a projected separation of 0 $\mathop{.}\limits^{\unicode{x02033}}$ 898 ± 0 $\mathop{.}\limits^{\unicode{x02033}}$ 01 with a contrast of (8.39 ± 0.07) × 10 ^−3 . …”
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22
Innamark: A Whitespace Replacement Information-Hiding Method
Published 2025-01-01“…By substituting conventional whitespace characters with visually similar Unicode whitespace characters, our proposed scheme preserves the semantics of the cover text without changing the number of characters. …”
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23
Trattamento delle risorse bibliografiche in alfabeti non latini e discoverability delle collezioni digitali: problemi e prospettive
Published 2025-04-01“…Su un piano più tecnico, l’implementazione dello standard Unicode nei software di gestione delle biblioteche si è rivelata una soluzione valida per la corretta codifica degli script nativi. …”
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24
In-depth Analysis of the 2022 March 28 3He-rich Solar Energetic Particle Event
Published 2025-01-01“…Near-Earth spacecraft (44 $\mathop{.}\limits^{\unicode{x000b0}}$ 8 from the flare site) observed abundance ratios closer to coronal values, and more uniform proton/heavy-ion spectra. …”
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25
Literary Analysis of Mufti Taqi Usmani's Ghazal
Published 2024-07-01“…<p class="MsoNormal" style="margin-bottom: 5.0pt; text-align: center; line-height: normal; mso-pagination: none; direction: rtl; unicode-bidi: embed;" align="center"><span style="font-size: 16.0pt; line-height: 115%; font-family: "Jameel Noori Nastaleeq"; mso-fareast-font-family: Calibri; mso-fareast-theme-font: minor-latin; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: ER;">:</span><span style="font-size: 16.0pt; line-height: 115%; font-family: "Calibri","sans-serif"; mso-ascii-theme-font: minor-latin; mso-fareast-font-family: Calibri; mso-fareast-theme-font: minor-latin; mso-hansi-theme-font: minor-latin; mso-bidi-font-family: Arial; mso-bidi-theme-font: minor-bidi; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA;"> </span><span style="font-size: 16.0pt; line-height: 115%; font-family: "Jameel Noori Nastaleeq"; mso-fareast-font-family: Calibri; mso-fareast-theme-font: minor-latin; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: ER;">Mufti Taqi is a major religious scholar of the sub-continent and a worldwide leading scholar of Islamic studies. …”
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26
Analytics of Some English Translations of Rashid’s Poem Saba Viraan
Published 2024-01-01“…<p class="MsoNormal" style="margin-bottom: 0cm; text-align: left; line-height: normal; direction: rtl; unicode-bidi: embed;" align="right"> </p> <p class="MsoNormal" style="margin-bottom: 0cm; text-align: justify; line-height: normal;"><strong><span style="font-size: 16.0pt; font-family: "Jameel Noori Nastaleeq";" lang="EN-US"> </span></strong><span style="font-family: "Jameel Noori Nastaleeq"; font-size: 14pt; text-indent: -1.2pt;">Abstract:</span></p> <p class="MsoNormal" style="margin-bottom: 0cm; text-align: justify; text-indent: -1.2pt; line-height: normal;"><span lang="EN-US"> </span><span style="font-size: 14.0pt; font-family: "Jameel Noori Nastaleeq"; mso-bidi-language: ER;" lang="EN-US">Nazr Muhammad Rashid is a reliable name in Urdu poetry. …”
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27
On the Extended Soft X-Ray and Fe Kα Emission in NGC 1068
Published 2025-01-01“…We fit the soft X-ray spectra from the core and two bright blobs (∼3 ^″ , S1 and ∼1 $\mathop{.}\limits^{\unicode{x02033}}$ 5, S2 from the nucleus) as a dual-temperature plasma with two APEC models. …”
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28
Tahzeeb-e-Niswan and Female Tareekh Goi
Published 2025-06-01“…<p class="MsoNormal" style="text-align: justify; direction: ltr; unicode-bidi: embed;"><em><span style="font-size: 14.0pt; line-height: 85%; font-family: "Cambria",serif;">Tareekhgoi</span></em><span style="font-size: 14pt; line-height: 85%; font-family: Cambria, serif;"> (chronogram), a revered art among classical Urdu poets, ingeniously encoded dates within poetic verses using Arabic numeral values of letters. …”
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29
Response of the LMC’s Bar to a Recent SMC Collision and Implications for the SMC’s Dark Matter Profile
Published 2025-01-01“…Post-collision, the simulated bar is offset (≈1.5 kpc) and tilted (≈8 $\mathop{.}\limits^{\unicode{x000b0}}$ 6). The simulated bar offset reduces with time, and comparing with the observed offset (≈0.8 kpc) suggests the timing of the true collision to be 150–200 Myr ago. …”
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30
Gyrokinetic simulation of full electromagnetic kinetic ballooning mode in tokamaks
Published 2025-01-01“…For the case of $\eta_i\unicode{x2A7E} 1$ , the KBM is always unstable in almost the entire region of low shear $\hat {s}$ for a smaller pressure gradient, and the stability boundary in $\hat{s}-\alpha$ plane is much wider than that for the case of $\eta_i = 0$ . …”
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31
Activation of thermal states by coherently controlled thermalization processes
Published 2025-01-01“…Here we analyze this limitation, showing that it still holds true even when the medium interacts with $N\unicode{x2A7E} 2$ reservoirs in a coherently-controlled order. …”
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32
India through the Eyes of a Turkish Diplomat and Dukhter-i Hindu
Published 2025-01-01“…<p class="MsoNormal" style="margin-bottom: .0001pt; text-align: justify; text-indent: 35.4pt; line-height: 150%; direction: rtl; unicode-bidi: embed;"> </p><p class="MsoNormal" style="text-align: justify; text-indent: 35.45pt; line-height: 150%;"><span style="font-size: 12.0pt; line-height: 150%; font-family: "Book Antiqua",serif; mso-bidi-font-family: "Times New Roman"; mso-bidi-theme-font: major-bidi; mso-ansi-language: EN-GB;" lang="EN-GB">Abdulhak Hamit Tarhan, born on February 5, 1851, in Istanbul, was a Turkish poet, playwright, and diplomat. …”
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33
Size effect and phenomenological constitutive model of mechanical properties of ultra-thin 316L sheet
Published 2025-01-01“…The flow stress shows a decreasing trend with the decrease of ${\rm{d}}^{\unicode{x02212}1/2}$ . When t/d ≥ 2.59, the flow stress follows the traditional Hall-Petch relation, while when t/d < 2.59, the flow stress deviates from Hall-Petch relation curve, and the size effect of ‘smaller is weaker’ appears. …”
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34
Breaking the Mass Inclination Degeneracy of Radial Velocity Measurements via Monitoring von Zeipel–Lidov–Kozai Cycles: Implications in the HD 41004 System
Published 2025-01-01“…The von Zeipel–Lidov–Kozai (vZLK) mechanism becomes active when the mutual inclination is greater than 39 $\mathop{.}\limits^{\unicode{x000b0}}$ 2. High-inclination orbits exhibit coupled oscillations in eccentricity and inclination, along with apsidal precession. …”
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35
On-axis Polarization Calibration of the FAST L-band 19-beam Receiver
Published 2025-01-01“…The calibrated polarization percentage and polarization angle of a source with strong linear polarization emission are about 0.2% and 0 $\mathop{.}\limits^{\unicode{x000b0}}$ 5, respectively. Several parameters of the central-beam Mueller matrix show time variability from months to years, suggesting that relatively frequent polarization calibrations are needed. …”
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36
Recurrent Cometary Activity Discovered on Quasi-Hilda Jupiter Family Comet 362P/(457175) 2008 GO98
Published 2025-01-01“…We obtained observations with the Lowell Discovery Telescope, the Astrophysical Research Consortium telescope, and the Vatican Advanced Technology Telescope and identified a second activity epoch when 362P had a true anomaly ( ν ) as early as 318 $\mathop{.}\limits^{\unicode{x000b0}}$ 1. We conducted archival searches of six repositories and identified images obtained with Canada–France–Hawaii Telescope MegaCam, Dark Energy Camera, Pan-STARRS 1, SkyMapper, Zwicky Transient Facility, and Las Cumbres Observatory Global Telescope network data. …”
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37
Gas-poor Hosts and Gas-rich Companions of z ≈ 3.5 Radio Active Galactic Nuclei: ALMA Insights into Jet Triggering and Feedback
Published 2025-01-01“…With the assistance of [C ii ] at 0 $\mathop{.}\limits^{\unicode{x02033}}$ 2 resolution, we further confirm the gas-poor nature of the hosts by reanalyzing archival [C i ] (a tracer of H _2 ) at ∼2″ resolution. …”
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38
LiDO: Discovery of a 10:1 Resonator with a Novel Libration State
Published 2025-01-01“…This object has an inclination of 33 $\mathop{.}\limits^{\unicode{x000B0}}$ 4, and n -body integrations of orbital clones of 2020 VN _40 have revealed some unexpected evolutions. …”
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39
PROTOCALC, a W-band Polarized Calibrator for Cosmic Microwave Background Telescopes: Application to Simons Observatory and CLASS
Published 2025-01-01“…The data collected constrain the roll angle of the source with a statistical accuracy of 0 $\mathop{.}\limits^{\unicode{x000b0}}$ 045.…”
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40
Apache Point Observatory Follow-up of ACcelerating Candidate ExopLanet Host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
Published 2025-01-01“…We use Gaia DR3 and Hipparcos astrometry to identify 166 northern hemisphere stars with astrometric accelerations consistent with a substellar companion between 0 $\mathop{.}\limits^{\unicode{x02033}}$ 5 and 1″. For this accelerating sample we identify young stars using Apache Point Observatory/ARCES spectra and TESS light curves. …”
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