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Found 4 papers, 1 papers with code
cecilia: A Machine Learning-Based Pipeline for Measuring Metal Abundances of Helium-rich Polluted White Dwarfs
Over the past several decades, conventional spectral analysis techniques of polluted white dwarfs have become powerful tools to learn about the geology and chemistry of extrasolar bodies.
Searching for the 1 mHz variability in the flickering of V4743 Sgr: a Cataclysmic Variable accreting at a high rate
Because we still have only small number statistics, we obtained a new observation to test whether this is a general characteristic of CVs, especially if mass transfer occurs at a high rate typical for dwarf nova in outbursts, in the so called "high state".
Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
K2-111: an old system with two planets in near-resonance
A global fit, performed by using PyORBIT shows that the transiting planet, K2-111b, orbits with a period $P_b=5. 3518\pm0. 0004$ d, and has a planet radius of $1. 82^{+0. 11}_{-0. 09}$ R$_\oplus$ and a mass of $5. 29^{+0. 76}_{-0. 77}$ M$_\oplus$, resulting in a bulk density slightly lower than that of the Earth.
Earth and Planetary Astrophysics
K2-106, a system containing a metal-rich planet and a planet of lower density
The period of the outer planet is 13. 3 days. Although the two planets have similar masses, their densities are very different.
Earth and Planetary Astrophysics
