期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 268 (1)
We present the results of an unbiased (CO)-C-12/(CO)-C-13/(CO)-O-18 (J = 1-0) survey in a portion of the third Galactic quadrant (TGQ): 219.& DEG;......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 268 (2)
We developed a multiregion radiation model for the evolution of flux and spectral index with time. In this model, each perturbation component in the j......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 268 (2)
Timely solar flare forecasting is challenged by the delay of transmitting vast amounts of data from the satellite to the ground. To avoid this delay, ......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 269 (1)
Nearly 700 fast radio burst (FRB) sources have been detected so far, of which 29 are found to burst out repeatedly. Although a firm connection between......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 269 (2)
Regular, automated testing is a foundational principle of modern software development. Numerous widely used continuous integration systems exist, but ......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 264 (1)
Critical points represent a subset of special points tracing cosmological structures, carrying remarkable topological properties. They thus offer a ri......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 265 (2)
A complete map of the youngest stellar populations of the Milky Way in the era of all-sky surveys is one of the most challenging goals in modern astro......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 266 (2)
Double-line spectroscopic binaries (SB2s) are a vital class of spectroscopic binaries for studying star formation and evolution. Searching for SB2s ha......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 268 (1)
The minimum variation timescale (MVT) of soft gamma-ray repeaters can be an important probe to estimate the emission region in pulsar-like models, as ......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 268 (2)
We present the the new Swift/UVOT+MaNGA (SwiM) catalog (SwiM_v4.1). SwiM_v4.1 is designed to study star formation and dust attenuation within nearby g......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 268 (2)
We present an advanced light-scattering model to retrieve the optical constants of three Martian dust analogs: Johnson Space Center regolith simulant,......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 268 (2)
Intensity-mapping observations measure galaxy clustering fluctuations from spectral-spatial maps, requiring stable noise properties on large angular s......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 269 (1)
The Nancy Grace Roman Space Telescope (Roman) is NASA's next astrophysics flagship mission, expected to launch in late 2026. As one of Roman's core co......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 269 (1)
We analyze the X-ray spectra of the similar to 8000 sources detected in the Cygnus OB2 Chandra Legacy Survey (this focus issue), with the goals of cha......
期刊： ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2023; 264 (2)
Asteroseismology has become widely accepted as a benchmark for accurate and precise fundamental stellar properties. It can therefore be used to valida......
