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Nominal values for selected solar and planetary quantities: iau 2015 resolution b3

TLDR
The IAU Working Group on Nominal Units for Stellar and Planetary Astronomy formed in 2011, uniting experts from the solar, stellar, planetary, exoplanetary, and fundamental astronomy, as well as from general standards as discussed by the authors.
Abstract
In this brief communication we provide the rationale for and the outcome of the International Astronomical Union (IAU) resolution vote at the XXIXth General Assembly in Honolulu, Hawaii, in 2015, on recommended nominal conversion constants for selected solar and planetary properties. The problem addressed by the resolution is a lack of established conversion constants between solar and planetary values and SI units: a missing standard has caused a proliferation of solar values (e.g., solar radius, solar irradiance, solar luminosity, solar effective temperature, and solar mass parameter) in the literature, with cited solar values typically based on best estimates at the time of paper writing. As precision of observations increases, a set of consistent values becomes increasingly important. To address this, an IAU Working Group on Nominal Units for Stellar and Planetary Astronomy formed in 2011, uniting experts from the solar, stellar, planetary, exoplanetary, and fundamental astronomy, as well as from general standards fields to converge on optimal values for nominal conversion constants. The effort resulted in the IAU 2015 Resolution B3, passed at the IAU General Assembly by a large majority. The resolution recommends the use of nominal solar and planetary values, which are by definition exact and are expressed in SI units. These nominal values should be understood as conversion factors only, not as the true solar/planetary properties or current best estimates. Authors and journal editors are urged to join in using the standard values set forth by this resolution in future work and publications to help minimize further confusion.

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The GALAH+ survey: Third data release

TL;DR: In this paper, the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1093/mnras/stab1242
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The Absolute Magnitude of the Sun in Several Filters

TL;DR: JWST/NIRCam [NAS5-02015], NASA/SAO ADS; NASA/IPAC Infrared Science Archive, Simbad; Mikulski Archive for Space Telescopes; European Community's Seventh Framework Programne (FP7 2012) [313188]
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Physics of eclipsing binaries. ii. toward the increased model fidelity

TL;DR: PHOEBE as discussed by the authors is an open source modeling code for computing theoretical light and radial velocity curves that addresses both problems by incorporating missing physics and by increasing the computational fidelity, including triangulation as a superior surface discretization algorithm, meshing of rotating single stars, light travel time effects, advanced phase computation, volume conservation in eccentric orbits, and improved computation of local intensity across the stellar surfaces.
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The chemical make-up of the Sun: A 2020 vision

TL;DR: In this article, a 3D radiative-hydrodynamical model of the solar surface convection and atmosphere is presented, which reproduces the full arsenal of key observational diagnostics, and the solar chemical composition more closely resembles that of the fine-grained matrix of CM chondrites with the expected exception of the highly volatile elements.
References
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Modules for Experiments in Stellar Astrophysics (MESA)

TL;DR: Modules for Experiments in Stellar Astrophysics (MESA) as mentioned in this paper is a suite of open source, robust, efficient, thread-safe libraries for a wide range of applications in computational stellar astrophysics.
Journal ArticleDOI

Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars

TL;DR: The Modules for Experiments in Stellar Astrophysics (MESA) project as discussed by the authors provides a one-dimensional stellar evolution module, MESA Star, which can model the evolution of giant planets down to masses as low as one-tenth that of Jupiter.
Journal ArticleDOI

Accurate masses and radii of normal stars: Modern results and applications

TL;DR: In this paper, the authors present a critical compilation of accurate, fundamental determinations of stellar masses and radii, including stellar luminosity, effective temperature, metal abundance, and apsidal motion determinations.
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