Searcharxiv⌕ Search

arXiv · 2610.41535

Demographics and growth of the astronomy and astrophysics community

Abstract

This paper presents the demographics and growth of the astronomy and astrophysics community over the past ~200 years based on data provided by the Astrophysics Data System. The analysis suggests that 59940 authors signed at least one paper in 2025, while about 40% of the community did not publish any papers, resulting in an estimated community size of roughly 100000 astronomers in 2025. About 38% of the community is hosted in Europe, followed by Asia (29%), North America (26%), South America (4%), Oceania (2%) and Africa (1%). Large variations exist among the countries in the number of astronomers, astronomers per capita of country population and astronomers per country gross domestic product (GDP). Overall, the community is dominated by early career scientists, with 50% of the authors publishing papers for seven years or less. This dominance is readily explained by a steady and exponential growth of the community of 4.3% per year over the last 50 years, implying that the community-size doubled every 16 years. The growth rate of the community exceeds that of the number of papers or paper pages, implying that the annual number of papers or pages published per astronomer is on decline. Over the last decade, the exponential growth of the community has accelerated to 5.1% per year, owing in particular to countries like China (13% per year) and India (10% per year). For almost all countries in the world, growth rates in authors, authors per capita and authors per GDP are positive. The growth in astronomy is not an exception, as the growth rates of the earth sciences and physics communities are even larger. If the past tendencies continue, Chinese and Indian astronomers will be first and second largest communities in the world by 2029 and 2043, respectively.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Jürgen Knödlseder. 2026-10-30. Demographics and growth of the astronomy and astrophysics community. https://arxiv.org/abs/2610.41535

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Geometrical and Optical Design of the GUEST Laser-Ranged Test Masses for the Detection of Gravitational Waves in the $μ$Hz range

The GUEST (Gravitational Universe Exploration with Satellite Tracking) mission aims at detecting gravitational waves in the yet almost unexplored $μ$Hz frequency range through high-precision orbital tracking. The unprecedented scientific objectives of this experiment demand equally advanced optical solutions: the highly eccentric orbit imposes dual measurement regimes; a low-velocity, long-range scenario at apogee and a high-velocity, short-range scenario at perigee. The substantial disparity between these conditions is addressed through a novel optical architecture incorporating two distinct types of Corner-Cube Retroreflectors (CCRs) with 1" and 2" apertures (CCR1 and CCR2, respectively). The proposed layout has been designed to ensure isotropy and homogeneity of the optical response while maintaining efficient packing over the spherical surface of the spacecraft. The resulting Optical Cross-Section (OCS) has been evaluated using a custom reduced-order model, which captures the behavior of individual CCRs under varying illumination conditions. This model has been calibrated by reconstructing the optical response of the LARES-2 satellite and has enabled a detailed assessment of the contributions of each CCR type along the GUEST orbit. Finally, sensitivity analyses have been conducted to investigate the impact of key design parameters, including the ratio between CCR types, laser wavelength, spacecraft diameter, Dihedral Angle Offsets (DAOs), and mechanical configurations.

astro-ph.IM↗

COSMIO: A Benchmark for Cross-Survey Modality Imputation

Large-scale astronomical surveys define a heterogeneous, partially observed multi-survey learning setting: each object is observed by only a subset of surveys, while survey observations differ in resolutions, wavelength coverage, noise characteristics, and footprints. This setting gives rise to a natural machine learning problem: given observations of an object in some surveys, how to infer its appearance in other surveys. We formalize this as the problem of cross-survey modality imputation and introduce COSMIO, a multi-survey benchmark of aligned observations obtained by forward-rendered shared astrophysical scenes across LSST, Euclid, and Roman under survey-specific instrument characteristics. The benchmark enables systematic evaluation of imputation across source-target survey combinations and missing-survey patterns. We evaluate a broad range of machine learning methods for imputation, which reveal a clear domain gap: methods developed for existing imputation settings transfer poorly to the survey setting. We identify rare-event imputation as a central challenge. This regime arises in the early stages of new surveys, when rare but scientifically valuable phenomena may be available only from prior surveys. We use strong gravitational lensing, where light from a background galaxy is gravitationally deflected by a foreground galaxy, as a representative rare-event setting. We evaluate model performance on zero-shot imputation of gravitational lenses and on downstream scientific tasks using the imputed lens observations. On our constructed evaluation set of galaxy-galaxy strong lenses, performance degrades under rare-event distribution shift, and this degradation further propagates to the downstream lens-detection task. Code: https://github.com/fw-ic/COSMIO.

astro-ph.IM↗

Photometric calibration of the 4m ILMT data

The International Liquid Mirror Telescope (ILMT) is a 4-meter survey telescope continuously observing towards the zenith in the SDSS g', r', and i' bands. This survey telescope is designed to detect various astrophysical transients (for example, supernovae) and very faint objects like multiply-imaged quasars and low surface brightness galaxies. Ensuring accurate and stable calibration of supernova (SN) and quasar measurements is essential for studying their intrinsic variability and long-term brightness evolution. In this work, we present a dedicated calibration approach tailored for ILMT point-like object observations obtained in Time Delayed Integration (TDI) mode. Using ZTF reference sources cross-matched with the Pan-STARRS1 catalog, we derive robust photometric zero-points along the ILMT scan. This calibration procedure enables the production of consistent, high-precision SN and quasar light curves, suitable for variability studies, structure-function analysis, and future reverberation-mapping applications.

astro-ph.IM↗