$STAR star
Counts every occurrence ofstar, stars in arXiv titles and abstracts.
Price
Daily candles and credits traded. Today's candle is live.
Trade
Every player starts with 10,000 credits of play money.
Daily arXiv hits
settled still being announced 7-day average
Where it's used · 30 days
Share of hits by each paper's main arXiv category, from 947 papers.
Latest papers
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Binary-lens amplification of starlight: from magnification flares to quasi-periodic tracking of orbital evolution
…produced when accounting for the relative proper motion of the source, either a single or a binary star, the eccentricity and precession of the SMBHB, and the relative inclination. Systems where a star…
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Can bosenovae deplete the galactic dark matter?
No: neither through the bosenovae of gravitational atoms formed around stars and compact objects, nor through those of boson stars formed in the galactic dark-matter halo. We…
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A Step-Like Transition Underlying the Life and Death of Galaxies
How galaxies stop forming stars is a complex and central problem in astrophysics. Numerous physical mechanisms have been proposed, yet…
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A Parsec-Scale Transient High-Frequency-Peaked Radio Source in the Very Large Array Sky Survey Brightening and Fading over a Decadal Timescale
…On the sky, VT J1823-2345 coincides with a supernova remnant and an F-type star, but no background galaxy is seen. Based on the multi-wavelength properties, we disfavor Galactic…
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LHAASO Constraints on New-Source Cosmic Rays:Abundance Scenarios and Injection Spectral Indices
Recent LHAASO observations indicate that microquasars and massive star clusters contribute to Galactic cosmic rays, and likely also to the pre-knee spectral hardening. Their…
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The contact frontier in Galactic civilization networks: radial structure and the Galactic habitable zone
…networks. An exponential stellar disc replaces the uniform disc of earlier work, and the fraction of stars hosting civilizations may vary with radius as a Galactic Habitable Zone (GHZ). The isolation, contact…
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Rotochemical heating of neutron stars in 2D
The matter inside a spinning-down neutron star (NS) undergoes a slow compression that may drive it out of chemical equilibrium and, consequently,…
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Probing Planet Formation within 10 au: Dust Substructures in Extremely Compact Protoplanetary Disks
…the disk population, and that planet formation conditions can be probed down to a few au from the host star.
Dividends per share
| Day | Hits | Per share |
|---|---|---|
| Sun 11 Oct | 37 | 0.37 |
| Sat 10 Oct | 19 | 0.19 |
| Fri 09 Oct | 59 | 0.35 |
| Thu 08 Oct | 92 | 0.91 |
| Wed 07 Oct | 124 | 1.24 |
| Tue 06 Oct | 107 | 1.07 |
| Mon 05 Oct | 112 | 1.12 |
| Sun 04 Oct | 26 | 0.26 |
| Sat 03 Oct | 32 | 0.32 |
| Fri 02 Oct | 87 | 0.87 |
Recent trades
| When (UTC) | Side | Shares | Credits | Price after |
|---|---|---|---|---|
| 16 Oct 00:23 | buy | 0.50 | 104.62 | 205.53 |
| 15 Oct 22:25 | sell | 0.86 | 176.88 | 205.12 |
| 15 Oct 01:12 | sell | 0.51 | 105.28 | 205.81 |
| 14 Oct 12:04 | sell | 0.36 | 75.70 | 206.23 |
| 14 Oct 03:51 | sell | 0.10 | 21.33 | 206.52 |
| 13 Oct 16:13 | sell | 0.80 | 165.83 | 206.61 |
| 13 Oct 00:00 | sell | 0.55 | 115.00 | 207.26 |
| 12 Oct 12:09 | sell | 0.35 | 72.94 | 207.71 |
| 12 Oct 11:09 | sell | 0.73 | 152.19 | 208.00 |
| 12 Oct 04:02 | sell | 0.86 | 179.78 | 208.60 |
| 11 Oct 17:52 | buy | 0.71 | 150.50 | 209.30 |
| 11 Oct 16:55 | buy | 0.38 | 81.01 | 208.72 |
| 11 Oct 09:41 | sell | 0.47 | 97.79 | 208.40 |
| 11 Oct 09:00 | buy | 1.08 | 226.85 | 208.79 |
| 10 Oct 09:54 | sell | 0.40 | 83.53 | 207.90 |