Promote Sponsor
verified SJR 0,985 · Q2 • database Scopus / SJR & Web of Science indexed
Publication of the Astronomical Society of Japan
United Kingdom · Oxford University Press
workspace_premium Q2 — Astronomy and Astrophysics lock Subscription Unclaimed

Publication of the Astronomical Society of Japan

Publication of the Astronomical Society of Japan is a journal indexed in SJR in Astronomy and Astrophysics and Space and Planetary Science with an H index of 112. It has an SJR impact factor of 0,985 and it has a best quartile of Q2. It is published in English. It has an SJR impact factor of 0,985.

Publication of the Astronomical Society of Japan focuses its scope in these topics and keywords: gas, derived, ?, ly, z, dynamics, decomposition, emission, emitters, galactic, ...

ISSN: 0004-6264
Editorial: Oxford University Press
Category: Astronomy and Astrophysics
Indexation: verifiedScopus / SJR verifiedWeb of Science

Unclaimed profile — some fields may be incomplete.

open_in_new Portal NPD menu_book Guidelines NPD
schedule Datos CoP · solo campos en BD
SJR Impact Factor trending_up
0,985 Q2
H-index 112
Tasa de Aceptación pie_chart
24% Selectiva
Fuente Acceptance_Rate
Tiempo a publicación hourglass_top
NPD
Campo Sin dato
Coste de Publicación (APC) payments
NPD Subscription
Ruta Non-OA NPD

Metrics

Campos Scimago / CoP — sin series inventadas

Scopus / SJR Web of Science

SJR Impact

0,985

H-index

112

Docs (year)

106

Docs 3y

364

Total refs

7034

Cites 3y

877

Citable 3y

364

Cites/Doc 2y

2.64

Ref/Doc

66.36

Immediate OA

—

Embargoed OA

NPD

Non OA / Submission

—

shield Researcher voice

Name good journals. Call out predatory ones.

Share what peer review, fees, and timelines were really like. Praise fair editors. Flag APC traps, fake metrics, or spam solicitations — with facts from your submission.

Fair & fast peer review Clear APC / no surprise fees Suspected predatory Fake impact claims
rate_review Write an honest review

Researcher reviews

sentiment_dissatisfied No reviews yet — be the first to share an honest experience.
User
* Only to validate authenticity — identity is not shown publicly.

Best articles by citations

Constraining hot plasma in a non-flaring solar active region with FOXSI hard X-ray observations

View more

X-Ray View of the Shock Front in the Merging Cluster Abell 3376 with Suzaku

View more

Evolution of magnetic field inclination in a forming penumbra

View more

Escape conditions of radiative-driven strati from luminous accretion disks

View more

EOSDB: The database for nuclear equations of state

View more

Environmental impacts on molecular gas in protocluster galaxies at z ~ 2

View more

Eddington limit for a gaseous stratus with finite optical depth

View more

Dwarf nova EZLyncis second visit to instability strip

View more

Distribution and Kinematics of Molecular Gas in Barred Spiral Galaxies. II. NGC 253

View more

Distribution and Kinematics of Molecular Gas in Barred Spiral Galaxies. I. NGC 3504

View more

Distortion of magnetic fields in Barnard 68

View more

Discovery of a nearby early-phase major cluster merger CIZA J1358.9-4750

View more
SHOW MORE ARTICLES

Density Profile of a Cool Core of Galaxy Clusters

View more

"Huruhata's Variable" Revealed: The WZ Sge-Type Dwarf Nova EG Cancri

View more

CO Survey of Nearby Spiral Galaxies with the Nobeyama 45-m Telescope: I. The Data

View more

CO (J=3=>2) observations of the starburst galaxy NGC1808 with ASTE

View more

Chemical feature of Eu abundance in the Draco dwarf spheroidal galaxy

View more

Centre-to-limb spectro-polarimetric diagnostics of simulated solar photospheric magneto-convection: Signatures of photospheric Alfven waves

View more

Central Kinematics and Rotation Curve of the Sb Galaxy NGC 4527 in CO, Ha and [N II] Lines

View more

CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst

View more

Calibration of the AKARI far-infrared all-sky survey maps

View more

Are redshift-space distortions actually a probe of growth of structure?

View more

Appearance of the prolate and the toroidal magnetic field dominated stars: Analytic approach

View more

AKARI infrared camera observations of the 3.3 µm PAH feature in Swift/BAT AGNs

View more

FAQS