Research Notes

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Little Time for Oscillation: Fast Disruption of the Radcliffe Wave by Galactic Motions- ow.ly/BfUm50ULc9Q

An Exploration of Molecular Lines for Abundance Analysis in M-dwarf IR Spectra- ow.ly/P1Em50ULc8t

Pre-Outburst Observations of T CRB with a Smart Telescope- ow.ly/O3Ti50ULc5Y

HD 193182: A Bright Twin of the Unusual Be-shell Star HD 94509- ow.ly/mQaj50ULc2M

GHOST Reduced Data Products for the Gemini Observatory Community and Beyond- ow.ly/6l1q50ULbZ5

LOFAR Non-detections of SN 2023ixf in its First Year Post-explosion- ow.ly/EHKW50ULbWK

Gas Dynamics in 3 "Dippers": EPIC 203850058, EPIC 204638512, and EPIC 205151387 in 2017–2018- ow.ly/Zo6S50ULbUp

SNR 0519−69.0 as a Type Ia Explosion in a Planetary Nebula Cocoon- ow.ly/OIZb50ULbGC

The γ-Ray-emitting BL Lac 4FGL J1219.0+3653 in the Radio - ow.ly/NQZl50ULbtX

Zeeman Spectral Line Fitting- ow.ly/2r8N50ULbp6

The Symbiotic Star V694 Mon has Transitioned from the Accreting-only State to the Steady Burning Phase- ow.ly/SEtN50ULakE

Determination of the Abundance of Mercury from the Hg ii Line at 5677.10 Å in Late B-type Stars. XI. HD 11753 (ϕ Phe)- ow.ly/31Su50ULaif

Discovery of Raman-scattered C ii Lines in V366 Carinae with GHOST/Gemini South- ow.ly/L4Oy50ULafs

Mock JWST Colors of Two Different Star Formation Histories at z ~ 4- ow.ly/e5aB50ULa91

To Explode or Not Explode? An Analysis of the Explodability of Binary and Single Stars- ow.ly/5C1Z50ULa5l

The Multimodal Universe: 100 TB of Machine Learning Ready Astronomical Data- ow.ly/NOT850UBVj9

The Foundations of Multi-line Molecular Cloud Population Synthesis- ow.ly/MPbB50UBVhs

The Temperature versus Orbital Period Relation of AM CVns: Insights from Their Donors- ow.ly/ksTL50UBVfv

Reconstructing In-channel Processes from the Eberswalde Delta on Mars- ow.ly/ThZl50UBVbH

Spatially Resolved Stellar Populations of z = 3–6 Lyα-emitting Galaxies with CEERS JWST NIRCam Imaging- ow.ly/JarU50UBV92