TEI P5 and Special Characters Outside Unicode by Joel Fredell, Charles Borchers IV, Terri Ilgen

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Encoding Disappearing Characters: The Case of Twentieth-Century Japanese-Canadian Names by Stewart Arneil

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Alternative graphemics. Aztec writing system as a case study towards an integrated, digitalised model of non-typographic graphemics by Antonio Perri, Luciano Perondi, Daniele Capo, Roberto Arista, Giampiero Dalai

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ALMA Observations of Solar Spicules in a Polar Coronal Hole by T. S. Bastian, C. Alissandrakis, A. Nindos, M. Shimojo, S. M. White

“…\limits^{\unicode{x02033}}$ 5 × 0 $\mathop{.}\limits^{\unicode{x02033}}$ 7, respectively. …”
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Identifier syntax and mnemonics in programming languages by Mikas Grigaliūnas, Gintautas Grigas

“…Unicode itself provides syntax rules for identifiers, in order to ensure uniform treatment of identifiers. …”
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Testing the Flux Rope Paradigm for Coronal Mass Ejections Using a Three-spacecraft Encounter Event by Brian E. Wood, Phillip Hess

“…\limits^{\unicode{x000b0}}$ 7 east of Earth. The reconstruction assumes a magnetic flux rope (MFR) structure for the CME. …”
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Envejecimiento poblacional: actualidad y futuro by María Obdulia Benítez Pérez

“…<p class="western" style="margin-bottom: 0cm; font-weight: normal; line-height: 150%;" align="JUSTIFY"><span style="font-family: DejaVu Sans Condensed,Arial Unicode MS,sans-serif;"><br /></span></p>…”
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Orbit of a Possible Planet X by Amir Siraj, Christopher F. Chyba, Scott Tremaine

“…We find the best-fit unseen planet parameters to have mass m _p  = 4.4 ± 1.1 M _⊕ , semimajor axis a _p  = 290 ± 30 au, eccentricity e _p  = 0.29 ± 0.13, and inclination i _p  = 6 $\mathop{.}\limits^{\unicode{x000b0}}$ 8 ± 5 $\mathop{.}\limits^{\unicode{x000b0}}$ 0. …”
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First fluctuation measurements using an Imaging Neutral Particle Analyzer on DIII-D by K.R. Gage, X.D. Du, W.W. Heidbrink, J. Gonzalez-Martin, D. Liu, A.C. Brown

“…Simulated measurements in the range of pitches that the diagnostic is sensitive to ( $0.5\unicode{x2A7D} \left| \frac{v_{\parallel}}{v} \right| \unicode{x2A7D} 0.75$ ) show the signal is dominated by trapped orbits that pass through magnetic islands near the edge of the plasma. …”
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Wehrl entropy and entanglement complexity of quantum spin systems by Chen Xu, Yiqi Yu, Peng Zhang

“…Explicitly, we numerically calculate the Wehrl entropy of various N -particle ( $2\unicode{x2A7D} N\unicode{x2A7D} 20$ ) entangled pure states, with respect to the SU(2) $ ^{\otimes N}$ coherent states. …”
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Projet urbain et paysage littoral by Odile Jacquemin

“…The objective was to take the « landscape» out of the discourse relating to the « beauty», to develop a methodological frame renewing the local monograph in order to analyze the scale unicode2utf8(0x2018)from the local to the global». …”
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Search for Neutrino Signals Correlated with LHAASO Diffuse Galactic Emission by Wenlian Li, Tian-Qi Huang, Donglian Xu, Huihai He

“…In the Galactic plane scan search, the most significant location is found at l  = 63 $\mathop{.}\limits^{\unicode{x000B0}}$ 57 and b  = 0 $\mathop{.}\limits^{\unicode{x000B0}}$ 93 with a pretrial (posttrial) significance of 4.6 σ (1.8 σ ).…”
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Photospheric Swirls in a Quiet-Sun Region by Quan Xie, Jiajia Liu, Chris J. Nelson, Robert Erdélyi, Yuming Wang

“…All these results suggest that photospheric swirls at different scales and locations across the observational 56 $\mathop{.}\limits^{\unicode{x02033}}$ 5 × 57 $\mathop{.}\limits^{\unicode{x02033}}$ 5 field of view could share the same triggering mechanism at preferred spatial and energy scales. …”
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Probing Cosmic Isotropy with the FAST All Sky H i Survey by Yi-Wen Wu, Jun-Qing Xia

“…This refined subsample is divided into 10 distinct sky regions, for which we compute the two-point angular correlation functions (2PACF) over angular scales of 0 $\mathop{.}\limits^{\unicode{x000b0}}$ 5 <  θ  < 10°. We apply the Markov Chain Monte Carlo method to fit these 2PACFs with a power-law model and assess the statistical significance of the best-fit parameters for the 10 FASHI sky regions by comparing them against results from mock catalogs generated under the assumptions of homogeneity and isotropy. …”
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Elevated Rates of Tidal Disruption Events in Active Galactic Nuclei by Karamveer Kaur, Nicholas C. Stone

“…For M _• ~ 10 ^7 M _⊙ and M _d ~ 0.1 M _• , the rate enhancement can be up to a factor ${\dot{N}}_{{\rm{cl}}}/{\dot{N}}_{{\rm{2b}}}\unicode{x0007E}10$ . The orbits of collisionless TDEs sometimes have a preferred orientation in apses, carrying implications for observational signatures of resulting flares.…”
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Electrochemical performance of NiCo2O4 and NiCo2O4/Ti3AlC2 composite for supercapacitor applications by Shahid M Ramay, Mohammed H Aldosary

“…Structural analysis confirms the existence of the cubic spinel phase of NiCo _2 O _4 with the Fd $\mathop{3}\limits^{\unicode{773}}$ m space group. Surface morphological analysis reveals a distribution of well-defined particles with a decrease in particle size from 50–40 nm. …”
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Finding Lensed Radio Sources with the Very Large Array Sky Survey by Michael N. Martinez, Yjan A. Gordon, Keith Bechtol, Gillian Cartwright, Peter S. Ferguson, Miranda Gorsuch

“…We obtain high-resolution (0 $\mathop{.}\limits^{\unicode{x02033}}$ 2) VLA follow-up observations for 11 targets that we identify using three different techniques: (i) a search for compact radio sources offset from galaxies with high lensing potential, (ii) VLASS detections of known lensed galaxies, and (iii) VLASS detections of known lensed quasars. …”
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Pushing the Atacama Large Millimeter/submillimeter Array to the Limit: 140 pc Resolution Observations of a z = 6.6 Quasar–Galaxy Merger Resolve Strikingly Different Morphologies of... by Romain A. Meyer, Bram Venemans, Marcel Neeleman, Roberto Decarli, Fabian Walter

“…We find that dust continuum is emitted in regions of $\unicode{x0007E}0^{\prime\prime} \,.02-0^{\prime\prime} \,.04$ consistent with the size of photodissociation regions (PDRs), whereas 50% of the [C ii ] originates from larger physical scales ( θ ≳ 2″). …”
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Asymmetries and Circumstellar Interaction in the Type II SN 2024bch by Jennifer E. Andrews, Manisha Shrestha, K. Azalee Bostroem, Yize Dong, Jeniveve Pearson, M. M. Fausnaugh, David J. Sand, S. Valenti, Aravind P. Ravi, Emily Hoang, Griffin Hosseinzadeh, Ilya Ilyin, Daryl Janzen, M. J. Lundquist, Nicolás Meza, Nathan Smith, Saurabh W. Jha, Moira Andrews, Joseph Farah, Estefania Padilla Gonzalez, D. Andrew Howell, Curtis McCully, Megan Newsome, Craig Pellegrino, Giacomo Terreran, Patrick Wiggins, Brian Hsu, Collin T. Christy, Noah Franz, Xiaofeng Wang, Jialian Liu, Liyang Chen

“…Comparisons between models and the early spectra suggest a pre-SN mass-loss rate of $\dot{M}\,\unicode{x0007E}\,1{0}^{-3}\unicode{8210}1{0}^{-2}\,{M}_{\odot }\,{\mathrm{yr}}^{-1}$ , which is too high to be explained by quiescent mass loss from RSGs, but is consistent with some recent measurements of similar SNe. …”
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Detection of a New GeV Source in the Outer Region of the Coma Cluster: A Signature of External Accretion Shock? by Xiao-Bin Chen, Kai Wang, Yi-Yun Huang, Hai-Ming Zhang, Shao-Qiang Xi, Ruo-Yu Liu, Xiang-Yu Wang

“…Here, we report the detection of a new GeV source at a distance of about 2 $\mathop{.}\limits^{\unicode{x000b0}}$ 8 from the center of the Coma cluster through the analysis of 16.2 yr of Fermi-LAT data. …”
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