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Detection of the [O I] 63 µm emission line from the z = 6.04 quasar J2054-0005
DOI: 10.1093/pasj/psae105 Bibcode: 2025PASJ...77..139I

Fujimoto, Seiji; Inoue, Akio K.; Hashimoto, Takuya +23 more

We report the highest-redshift detection of [O I] 63 $\mu$m from a luminous quasar, J2054$-$0005, at $z=6.04$

2025 Publications of the Astronomical Society of Japan
ISO 4
Revisiting the Suzaku spectrum of the Galactic SNR W 49B: Non-detection of iron K-shell charge-exchange emission and refined ejecta-mass ratios of iron-group elements
DOI: 10.1093/pasj/psaf012 Bibcode: 2025PASJ...77..446S

Sato, Toshiki; Sawada, Makoto; Maeda, Keiichi +1 more

The origin of the recombining plasma in several Galactic SNRs has been debated. A plausible mechanism would be a rapid cooling in the past, by either an adiabatic or a conductive process. A recent spectral study of W 49B reported a possible charge-exchange emission due to collisions between the shock-heated ejecta and cold clouds, which could be d…

2025 Publications of the Astronomical Society of Japan
Suzaku 1
Smart Kanata: A framework for autonomous decision-making in rapid follow-up observations of cataclysmic variables
DOI: 10.1093/pasj/psae112 Bibcode: 2025PASJ...77..219U

Maehara, Hiroyuki; Nogami, Daisaku; Uemura, Makoto +11 more

Studying the early stages of transient events provides crucial information about the fundamental physical processes in cataclysmic variables (CVs). However, determining an appropriate observation mode immediately after the discovery of a new transient presents challenges due to significant uncertainties regarding its nature. We developed a framewo…

2025 Publications of the Astronomical Society of Japan
Gaia 0