output
20042026
most citedHI4PI: A full-sky HI survey based on EBHIS and GASS

1.6k citations

364 papers

astro-ph.GA2026

First Trigonometric Parallax Measurements with the KVN and VERA Array (KaVA)

Nobuyuki Sakai, Daisuke Sakai, Noriyuki Kawaguchi +26

To demonstrate the astrometric capability of the combined Korean VLBI (Very Long Baseline Interferometry) Network (KVN) and VLBI Exploration of Radio Astrometry (VERA) Array (KaVA)…

math.DG2026

Michell-Prager type truss structures constructed from integrable discrete power function and discrete logarithmic function

Motoki Masada, Kentaro Hayakawa, Kazuki Hayashi +3

The Michell-Prager type truss structures are constructed from the integrable discrete power and logarithmic functions. It is demonstrated that specific sublattices, subject to suit…

astro-ph.GA2026

Molecular absorption lines toward the Galactic ISM detected at 89 GHz with VLBI

Keisuke Nakashima, Hiroshi Imai, Youngjoo Yun

As the first step to explore the Galactic foreground interstellar medium (ISM) with high angular resolution, we investigated the detectability of molecular absorption lines with ve…

astro-ph.EP2026

Interpreting ALMA Multiwavelength Continuum Observations of PDS 70 c: An Optically Thick Dust Ring in the Circumplanetary Disk

Yuhito Shibaike, Satoshi Okuzumi, Takahiro Ueda +2

Giant planets form small gas disks, called circumplanetary disks (CPDs), during gas accretion. The CPD of PDS 70 c has been detected by the Atacama Large Millimeter/submillimeter A…

astro-ph.GA2026

A differentiable hydrodynamical approach to the Milky Way bar pattern speed with CO longitude--velocity data

Junichi Baba, Kohei Hattori

We present a differentiable hydrodynamical framework for modeling barred gas flow in the Milky Way and constraining broad low-loss regions in bar-pattern-speed parameter space from…

astro-ph.GA2026

Axisymmetric Jeans modelling systematically overestimates the circular speed in the inner Milky Way

Tomoki Yamaguchi, Junichi Baba

We quantify systematic biases in rotation curves inferred from steady, axisymmetric Jeans modelling when the underlying stellar velocity field is non-axisymmetric. Using a high-res…