APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields by Marc H. Pinsonneault, Joel C. Zinn, Jamie Tayar, Aldo Serenelli, Rafael A. García, Savita Mathur, Mathieu Vrard, Yvonne P. Elsworth, Benoit Mosser, Dennis Stello, Keaton J. Bell, Lisa Bugnet, Enrico Corsaro, Patrick Gaulme, Saskia Hekker, Marc Hon, Daniel Huber, Thomas Kallinger, Kaili Cao, Jennifer A. Johnson, Bastien Liagre, Rachel A. Patton, Ângela R. G. Santos, Sarbani Basu, Paul G. Beck, Timothy C. Beers, William J. Chaplin, Katia Cunha, Peter M. Frinchaboy, Léo Girardi, Diego Godoy-Rivera, Jon A. Holtzman, Henrik Jönsson, Szabolcs Mészáros, Claudia Reyes, Hans-Walter Rix, Matthew Shetrone, Verne V. Smith, Taylor Spoo, Keivan G. Stassun, Ji Wang

“…We provide evolutionary state, asteroseismic surface gravity, mass, radius, age, and the data used to derive them for 12,418 stars. …”
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Thermodynamic Relations for Kiselev and Dilaton Black Hole by Bushra Majeed, Mubasher Jamil, Parthapratim Pradhan

“…We have calculated the products relating the surface gravities, surface temperatures, Komar energies, areas, entropies, horizon radii, and the irreducible masses at the Cauchy and the event horizons. …”
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Nanofibre Electrospinning Poly(vinyl alcohol) and Cellulose Composite Mats Obtained by Use of a Cylindrical Electrode by Anna Sutka, Silvija Kukle, Janis Gravitis, Rimvydas Milašius, Jolanta Malašauskienė

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Research on Impact Process of Lander Footpad against Simulant Lunar Soils by Bo Huang, Zhujin Jiang, Peng Lin, Daosheng Ling

“…Described in this paper are model tests carried out using simulated lunar soils of different relative densities (called “simulant” lunar soils below), with a scale reduction factor of 1/6 to consider the relative gravities of the Earth and Moon. In the model tests, the lander was simplified as an impact column with a saucer-shaped footpad with various impact landing masses and velocities. …”
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Crater Dimensions on the Dwarf Planets by Veronica J. Bray, Michael F. Zeilnhofer, S. J. Robbins, P. M. Schenk, Kelsi M. Singer, O. L. White, S. A. Stern, S. D. Benecchi, K. A. Durfey, H. A. Weaver, C. B. Olkin, J. R. Spencer, the New Horizons Geology and Geophysics Investigation Team

“…The icy dwarf planets of Pluto, Charon, and Ceres provide important geologic comparisons for each other as they possess similar gravities and experience impacts of similar velocities compared to larger planets and moons. …”
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Investigation of the Thermal Improvement and the Kinetic Analysis of the Enriched Coal by Selma Duzyol, Cem Sensogut

“…Each fraction was, then, processed in the dense mediums with the specific gravities of 1.20, 1.30, 1.40, 1.50, and 1.60 g/cm3, respectively. …”
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