Revisiting candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud

arXiv:2609.01011 · astro-ph.SR · Submitted 2026-09-01 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-01

Updated: 2026-09-07

Code: https://github.com/sncosmo/extinction

Terminology

• Abundance — 31× in this paper · explained in 1 episode
• Calibration — 26× in this paper · explained in 7 episodes
• Metallicity — 20× in this paper · explained in 3 episodes
• Large Magellanic Cloud — 5× in this paper
• Consistency — 3× in this paper · explained in 3 episodes
• Aperture — 1× in this paper · explained in 1 episode
• Degeneracy — 1× in this paper · explained in 3 episodes
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Grid Search in Stellar Parameters — 1× in this paper
• Magellan Inamori Kyocera Echelle — 1× in this paper
• SOAR Optical Imager — 1× in this paper
• Small Magellanic Cloud — 1× in this paper
• South African Astronomical Observatory — 1× in this paper
• VISTA Magellanic Clouds — 1× in this paper

Sources

• IAU 2015 Resolution B3 on Recommended Nominal Conversion Constants for Selected Solar and Planetary Properties
• Reddening maps of the Magellanic Clouds using spectral energy distribution fitting of red giants

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Constraining the origin of magnetic white dwarfs
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
• Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
• Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?