Peer Revenue Impact factor: volatile

$GAIA gaia

Counts every occurrence of gaia in arXiv titles and abstracts.
Price16.200.00% today
Hits8Fri 16 Oct · usual 8
Yield0.49%latest day
Dividends · 30d0.00per share

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Daily arXiv hits

settled still being announced 7-day average

Where it's used · 30 days

  1. Solar and Stellar Astrophysics astro-ph.SR 40%
  2. Astrophysics of Galaxies astro-ph.GA 35%
  3. Earth and Planetary Astrophysics astro-ph.EP 10%
  4. Artificial Intelligence cs.AI 6%
  5. High Energy Astrophysical Phenomena astro-ph.HE 4%
  6. Computational Physics physics.comp-ph 1%
  7. Everything else 3%

Share of hits by each paper's main arXiv category, from 115 papers.

Latest papers

  1. The Solar System through dust maps. Encounter statistics with interstellar gas astro-ph.GA · 19 Oct · 1 hit

    …motion and ISM stratification influence these statistics. We quantify gas influx and dust exposure. We use Gaia-based 3D dust maps of the Solar neighborhood, sampled by integrating the Solar System along its Galactic…

  2. A 36.34-day Sub-Neptune Candidate Transiting the Nearby K Dwarf TIC 402710280 astro-ph.EP · 19 Oct · 1 hit

    …\pm 0.004$. No high-resolution imaging exists, so companions within about $1''$ are constrained only by Gaia astrometry. The mid-times scatter about a linear ephemeris by 21.8 min (rms). Quick-Look Pipeline light…

  3. Kinematic structure and age of a Scorpius--Centaurus subcomponent: implications for PDS 70 planetary system astro-ph.SR · 19 Oct · 2 hits

    …(WiFeS) on the ANU 2.3~m telescope, reducing uncertainties by a factor of $\sim5.5$ compared to \textit{Gaia}. %We supplement these measurements with H$\alpha$ and lithium equivalent widths as youth diagnostics.…

  4. Gravity-mode main-sequence asteroseismology of 16 open clusters and associations astro-ph.SR · 19 Oct · 1 hit

    …Using light curves from the Kepler and TESS space missions, together with membership constraints based on Gaia astrometry, we identify g-mode period-spacing patterns in dozens of early-type ($T_{\rm eff} \gtrsim…

  5. Plate-YOLO: An End-to-End Object Detection Framework for Robust Astrometric Registration of Historical Plates astro-ph.IM · 19 Oct · 1 hit

    …attention, a high-resolution P2 head, and a Normalized Wasserstein Distance loss for small bounding boxes. A Gaia-guided fine-tuning procedure uses initially solved plates to construct labels for a new archive. On 150…

  6. IMF-aware N-body forward modelling of membership selection functions for young open clusters astro-ph.GA · 18 Oct · 1 hit

    …Our framework simulates clusters with IMF slopes $\alpha_2 = -2.7, -2.3, -1.9$, converts them into synthetic Gaia observations, adds mock field populations, and recovers members with HDBSCAN to mimic observational…

  7. Companions of Hot Jupiters: two decades of radial velocity monitoring with CORALIE astro-ph.EP · 18 Oct · 1 hit

    …mechanism shaping hot Jupiters with outer companions. Combining long-baseline radial velocities with future Gaia astrometry will further constrain companion masses, mutual inclinations, and dynamical histories.

  8. A Hectospec Spectroscopic Census of Kinematic Members in the Orion Nebula Cluster astro-ph.SR · 16 Oct · 1 hit

    …of pre-main-sequence stars. We combine these measurements with a kinematic membership analysis based on Gaia Data Release 3 astrometry to identify and confirm cluster members. Using these combined diagnostics, we…

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