By Muhammad Akashi, Noam Soker. The study uses 3D simulations to explore core-collapse supernova explosions driven by jets, supporting the jittering jets explosion mechanism theory. The simulations explain observed circum-jet rings in supernova remnants.

By Serat M. Saad, Yuan-Sen Ting. A technique to measure differential radial velocities of wide-binary stars, improving precision and enabling better analysis of Modified Newtonian Dynamics (MOND), suggesting tension with current estimates of the acceleration scale.

By Ottavia Truttero, Maria Tsedrik & 5 more. This study presents a new analysis for LSST Y1 and Y10 data, exploring the effects of galaxy bias and baryonic feedback. The article also introduces a new open-source pipeline, MGL.

By Jessica Braudo, Noam Soker. The study suggests that jets shape the 'pipe' structures in core-collapse supernova remnants and jet-shaped planetary nebulae, based on comparisons with hydrodynamical numerical simulations.

By Nicholas S. Conroy, Michi Bauböck & 5 more. This study uses Event Horizon Telescope images to analyze black hole asymmetry, potentially providing insights into black hole mass, spin, and inclination.

By Florent Renaud, Katarina Kraljic & 11 more. This article explores the "starbursts in the main sequence" (SBMSs) that intermittently appear in galaxy evolution, attributing their existence to earlier stellar mass assembly and frequent mergers.

By Xiangchong Li. This study explores how galaxy model fitting responds to weak-lensing shear distortions using a new algebraic system, quintuple numbers, within the AnaCal framework, keeping multiplicative bias low.

By Cian Roche, Mark Vogelsberger & 10 more. This study presents a simulation-based method for generating strong-lensing images directly from particle data, considering all intervening objects. The method's effectiveness is demonstrated using IllustrisTNG data.

By Vaibhav Tiwari. Analysis of 256 binary black-hole (BBH) events, suggesting a hierarchical merger scenario to explain the structured mass distribution, and encouraging further investigation into hierarchical mergers' role in the BBH population

International MEGATRON project links space telescope observations of the infant Universe with the chemical fossil record of the Milky Way.

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By Harley Katz, Nicholas Choustikov & 8 more. This study uses radiation hydrodynamics simulations to explore the origin of extremely blue UV slopes in high-redshift galaxies, revealing that these slopes don't necessarily indicate high escape fractions.

By Martin Rey, Harley Katz & 24 more. The study uses MEGATRON simulations to examine the stellar mass-iron metallicity relation in dwarf galaxies, finding a correlation with Population III supernovae and predicting a subset of iron-deficient dwarf galaxies

By Luke Conaboy, James S. Bolton & 4 more. This study improves theoretical work on the connection between galaxies and the intergalactic medium, using an empirical model and James Webb Space Telescope surveys.

By G. Leidi, A. Holas & 13 more. PHLEGETHON is a magnetohydrodynamic code designed for multidimensional simulations in stellar astrophysics, capable of modeling a wide range of dynamical processes in stars. It's publicly accessible online.

By Ryan Brady, Xiang-Yu Huang & 8 more. The article "TDCOSMO XXVI: Uniform Lens Modeling of Eight Doubly Imaged Quasars" by Brady et al. contained some errors which have now been corrected

If the only reason you were not submitting papers to OJAp was that it wasn't a Q1 journal then you can start submitting them now!

By Jose Benavides, Laura V. Sales & 5 more. The paper " The Abundance of Thin Dwarf Galaxies: a Challenge for Cosmological Simulations" by Benavides et al. contained two errors which have now been corrected

By Pablo Penil, N. Torres−Albà & 6 more. The study examines the oscillation profiles of blazar PG~1553+113, finding that its 2.1-year periodicity is not strictly sinusoidal and varies across energy bands.

By Paul Rogozenski, Sankarshana Srinivasan & 16 more. This paper introduces the Augur tool, designed to provide Fisher forecasts for cosmological inference for the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST).

By Justin Clancy, Carlo Baccigalupi & 15 more. The study introduces a method for detecting fast, dynamic astrophysical transients using cosmic microwave background survey telescopes, demonstrating its effectiveness in the Simons Observatory time-domain pipeline.

By Hannah McCall, Irina Zhuravleva & 11 more. This study examines gas kinematics in the relaxed, AGN-feedback-free galaxy cluster A3571 using XRISM observations. Findings suggest sloshing motions may significantly contribute to the heating budget.

By Yuan-Sen Ting, Elliot M. Kim. The study introduces \paynezero, a tool that reorganizes stellar spectra calculations for GPU-native synthesis, significantly speeding up the process and enabling direct physical fitting and atomic-data calibration at survey scale.

By Sachi Weerasooriya, Mia Sauda Bovill & 7 more. Thi study investigates the lack of luminous satellite galaxies in Centaurus A's inner regions, suggesting that AGN-driven thermal feedback could suppress star formation, affecting the survival and evolution of satellites

By Diana Blanco, Alexie Leauthaud & 60 more. This study explores using the Dark Energy Spectroscopic Instrument (DESI) to calibrate photometric redshift distributions for gravitational lensing, which could improve understanding of dark energy and cosmic structure.

By Serat M. Saad, Yuan-Sen Ting. The study reanalyzes a dataset on gravitational anomalies, finding results consistent with Newtonian gravity, contrary to previous findings that suggested Modified Newtonian Dynamics.

By Jackson H. O'Donnell, Demetrius Y. Williams & 19 more. A spectroscopic survey of the Carousel lens galaxy cluster, identifying 12 lensed sources and 57 unlensed field galaxies. The findings could help constrain cosmological parameters and cluster properties.

By Anton D. Lazarev, Sergei B. Popov. This study analyzes the velocity kick of neutron stars, finding that 23% belong to the low-velocity mode. Differences in magnetic field distribution emerge, but no significant bimodality in physical parameters.

By Drake Deming, Andrew Lincowski & 7 more. The study proposes using color phase curves to detect and characterize the atmospheres of rocky exoplanets, including non-transiting ones, by observing their longitudinal heat transfer.

By Sergey Koposov, Ting S. Li & 66 more. The paper "DESI Data Release 1: Stellar Catalogue" by Koposov et al. contained a Figure that was incorrect. This has now been corrected.

By Raquel Forés-Toribio, C. S. Kochanek. The study re-analyzes images of potential failed supernova N6946-BH1, finding four unrelated near-infrared neighbors. It also compares the luminosity of failed supernova remnants to stellar merger remnants, noting significant differences.