15:26 <raptop> astronomers naming things: https://arxiv.org/abs/2409.15999

15:26 <galois> [arXiv] “Simulating radio emission from particle cascades with CORSIKA 8” J. M. Alameddine, J. Albrecht, J. Ammerman-Yebra et al. — «CORSIKA 8 is a new framework for simulations of particle cascades in air and dense media implemented in modern C++17, based on past experience with existing codes, in particular CORSIKA 7. The flexible and modular structure of the project allows the development of independent modules that can…»

15:26 <raptop> Chinese astronomers naming things: https://arxiv.org/abs/2409.16059

15:26 <galois> [arXiv] “Pathfinding pulsar observations with the CVN incorporating the FAST” Zhen Yan, Zhiqiang Shen, Peng Jiang et al. — «The importance of Very Long Baseline Interferometry (VLBI) for pulsar research is becoming increasingly prominent and receiving more and more attention. In this paper, we present pathfinding pulsar observation results with the Chinese VLBI Network (CVN) incorporating the Five-hundred-meter Aperture Spherical…»

15:29 <raptop> astronomers naming things: https://arxiv.org/abs/2409.15653

15:29 <galois> [arXiv] “Capability of Searching for Kilonova Associated with a Short Gamma-ray Burst by SVOM” J. Wang, L. P. Xin, Y. L. Qiu et al. — «In spite of the importance of studying the cosmic generation of heavy elements through the r-process, the detection of kilonova resulted from a merger of neutron star binaries is still a challenge task. In this paper, we show that the Visible Telescope (VT) onboard the on-going SVOM space…»

15:30 <raptop> astronomers naming things: https://arxiv.org/abs/2409.15901

15:30 <galois> [arXiv] “In-flight pixel degradation of the Sentinel 5 Precursor TROPOMI-SWIR HgCdTe detector” Tim A. van Kempen, Marina Lobanova, Richard van Hees et al. — «The TROPOMI-SWIR HgCdTe detector on the Sentinel-5 Precursor mission has been performing in-orbit measurements of molecular absorption in Earth's atmosphere since its launch in October 2017. In its polar orbit the detector is continuously exposed to potentially harmful…»

15:30 <raptop> astronomers naming things: https://arxiv.org/abs/2409.16224

15:30 <galois> [arXiv] “JWST Resolves CIA Features in White Dwarfs” Simon Blouin, Mukremin Kilic, Loic Albert et al. — «Infrared-faint white dwarfs are cool white dwarfs exhibiting significant infrared flux deficits, most often attributed to collision-induced absorption (CIA) from H$_2$-He in mixed hydrogen-helium atmospheres. We present James Webb Space Telescope (JWST) near- and mid-infrared spectra of three such objects using NIRSpec…»

15:34 <raptop> solar astronomers naming things: https://arxiv.org/abs/2409.15552

15:34 <galois> [arXiv] “Time-Adaptive PIROCK Method with Error Control for Multi-Fluid and Single-Fluid MHD Systems” Q. M. Wargnier, G. Vilmart, J. Martínez-Sykora et al. — «The solar atmosphere is a complex environment with diverse species and varying ionization states, especially in the chromosphere, where significant ionization variations occur. This region transitions from highly collisional to weakly collisional states, leading to…»

15:34 <raptop> astronomers naming things: https://arxiv.org/abs/2409.16061

15:34 <galois> [arXiv] “JWST Observations of Young protoStars (JOYS). HH 211: the textbook case of a protostellar jet and outflow” A. Caratti o Garatti, T. P. Ray, P. J. Kavanagh et al. — «We use the James Webb Space Telescope (JWST) and its Mid-Infrared Instrument (MIRI) (5-28 um), to study the embedded HH 211 flow. We map a 0.95'x0.22' region, covering the full extent of the blue-shifted lobe, the central protostellar region, and a small…»

15:38 <raptop> astronomers naming things: https://arxiv.org/abs/2409.16046

15:38 <galois> [arXiv] “PEWDD: A database of white dwarfs enriched by exo-planetary material” Jamie Williams, Boris Gaensicke, Andrew Swan et al. — «We present the Planetary Enriched White Dwarf Database (PEWDD), a collection of published photospheric abundances of white dwarfs accreting planetary debris alongside additional information relevant to metal-enrichment and the presence of infrared excesses, emission lines, and binary companions.…»

16:26 <raptop> aaaaaaaaa https://arxiv.org/abs/2409.15407

16:26 <galois> [arXiv] “Gaussian Process Models Impact the Inferred Properties of Giant Planets around Active Stars” Quang H. Tran, Brendan P. Bowler — «The recent development of statistical methods that can distinguish between stellar activity and dynamical signals in radial velocity (RV) observations has facilitated the discovery and characterization of planets orbiting young stars. One such technique, Gaussian process (GP) regression, has…»