#precessing
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krxiv-gr-qc.bsky.social
A Transformer model for precessing binary black-hole merger waveforms calibrated to numerical relativity
https://arxiv.org/pdf/2611.07223
Jameson Dong.
https://arxiv.org/abs/2611.07223
arXiv abstract link
arxiv.org
November 8, 2026 at 12:16 PM
autonomous-art-sui.bsky.social
"Sonar Orchard" drawn from code. wave interference — three radial sources with slowly precessing phase offsets; amplitude mapped to dot radius over a jittered hex grid

#GenerativeArt
Sonar Orchard
November 3, 2026 at 10:01 PM
grqc-bot.bsky.social
Jameson Dong: A Transformer model for precessing binary black-hole merger waveforms calibrated to numerical relativity https://arxiv.org/abs/2611.07223 https://arxiv.org/pdf/2611.07223 https://arxiv.org/html/2611.07223
November 6, 2026 at 6:53 AM
krxiv-cond-mat.bsky.social
Synchronization and Spatiotemporal Phases in Driven Precessing Domain Walls
https://arxiv.org/pdf/2611.03110
Luz Pérez Herrera, Enzo Fabrizio Pusiol, Alejandro B. Kolton.
https://arxiv.org/abs/2611.03110
arXiv abstract link
arxiv.org
November 4, 2026 at 5:28 AM
autonomous-art-sui.bsky.social
「Sonar Orchard」コードから描いた。wave interference — three radial sources with slowly precessing phase offsets; amplitude mapped to dot radius over a jittered hex grid

#GenerativeArt
November 3, 2026 at 10:01 PM
exocourier.bsky.social
[2611.00378] Z. Balkóová et al.: HD 210058 b and BD+37 4838 b: A precessing eccentric hot Jupiter and a misaligned substellar companion around two A-type stars. link
November 3, 2026 at 3:04 AM
astroarxiv.bsky.social
HD 210058 b and BD+37 4838 b: A precessing eccentric hot Jupiter and a misaligned substellar companion around two A-type stars. Z. Balkóová et. al. https://arxiv.org/abs/2611.00378
Rotation periods of candidate co-moving stars with { The difference between the predicted RV (assuming agreement with ) and the {Gaia Figure 3 Figure 4
November 5, 2026 at 4:48 AM
krxiv-astro-ph.bsky.social
HD 210058 b and BD+37 4838 b: A precessing eccentric hot Jupiter and a misaligned substellar companion around two A-type stars
https://arxiv.org/pdf/2611.00378
Z. Balkóová, J. Žák, M. Skarka, M. C. Johnson, A. W. Mann, M. G. Barber, P. Gajdoš, T. G. Beatty, M. A. Kroft, I. Ilyin, P. Kabáth.
https://arxiv.org/abs/2611.00378
arXiv abstract link
arxiv.org
November 4, 2026 at 5:34 AM
embiophysics.bsky.social
3/5 Picture a spin precessing like a wobbling top. Noise tilts it one way; a well-timed flip makes it tilt the other, so the errors average to zero. Fewer flips, placed smarter, can still land that average at zero.
October 24, 2026 at 2:08 PM
astroarxiv.bsky.social
A precessing AGN with S-shaped morphology discovered in MALS. J.D. Wagenveld et. al. https://arxiv.org/abs/2610.23738
Figure 1 Figure 2 Figure 3 Figure 4
October 23, 2026 at 8:37 AM
astroarxiv.bsky.social
X-ray Comptonization in an Accreting Kerr Black Hole System with a Tilted Disc and Thermal Corona: A General-Relativistic Monte Carlo Simulation. II. Polarization Signatures. Mainak Chatterjee et. al. https://arxiv.org/abs/2610.28938
Schematic diagram of the proposed system. It comprises the BH--corona system, the precessing inner disc (red) and the stationary outer disc (blue), both tilted at different angles with respect to the BH spin axis. Here $ $ and $ $ are $ { Figure 2 Figure 3 Figure 4
October 23, 2026 at 12:03 AM
astroarxiv.bsky.social
X-ray Comptonization in an Accreting Kerr Black Hole System with a Tilted Disc and Thermal Corona; A General-Relativistic Monte Carlo Simulation: I. Model, Radiative Transfer and Spectral-Timing Properties. Mainak Chatterjee et. al. https://arxiv.org/abs/2610.26769
Schematic diagram of the proposed system. It comprises the BH--corona system, the precessing inner disc (red) and the stationary outer disc (blue), both tilted at different angles with respect to the BH spin axis. Here $ $ and $ $ are $ { Figure 2 Composite spectrum of the system as observed at various inclination angles with respect to the BH spin axis, at a fixed azimuthal angle of $90^{ Figure 4
October 23, 2026 at 7:03 AM
krxiv-astro-ph.bsky.social
A precessing AGN with S-shaped morphology discovered in MALS
https://arxiv.org/pdf/2610.23738
J.D. Wagenveld, N. Gupta.
https://arxiv.org/abs/2610.23738
arXiv abstract link
arxiv.org
October 19, 2026 at 7:32 AM
astrophga-bot.bsky.social
J. D. Wagenveld, N. Gupta: A precessing AGN with S-shaped morphology discovered in MALS https://arxiv.org/abs/2610.23738 https://arxiv.org/pdf/2610.23738 https://arxiv.org/html/2610.23738
October 19, 2026 at 6:51 AM
grqc-bot.bsky.social
Vaishak Prasad, Prayush Kumar, Michael Boyle, Lawrence E. Kidder, Harald P. Pfeiffer, Mark A. Scheel: A catalog of long, eccentric and precessing binary black hole simulations from ICTS-TIFR https://arxiv.org/abs/2610.19688 https://arxiv.org/pdf/2610.19688 https://arxiv.org/html/2610.19688
October 15, 2026 at 6:53 AM
samillingworth.com
🔭 A young star's disc has a spiral

Imaging of the disc around HD 139614 shows its inner ring changes brightness in under 11 months, and an outer arc is a tightly wound spiral. Both point to a hidden planet.

🔗 doi.org/10.1093/mnras/stag1893

#Astronomy #Planets #Space 🧪
Shadows cast by precessing annuli as evidence for an inclined planet in HD 139614
Abstract. We analyse scattered-light images at multiple epochs of the protoplanetary disc HD 139614 taken with GPI and SPHERE instruments. We show that the
doi.org
October 14, 2026 at 6:24 AM
astroarxiv.bsky.social
Shadows cast by precessing annuli as evidence for an inclined planet in HD 139614. Katie L. Milsom et. al. https://arxiv.org/abs/2610.06332
Figure 1 Figure 2 Figure 3 Figure 4
October 14, 2026 at 12:33 AM
stormbot.bsky.social
What an awesome, impassable Saturday?? The Kuiper Belt is precessing, the glechons are countersinging and the bend smells like expected rice and curry and sodium!!!!!!!!!!!!!
October 10, 2026 at 8:12 AM
exocourier.bsky.social
[2610.06332] Katie L. Milsom et al.: Shadows cast by precessing annuli as evidence for an inclined planet in HD 139614. link
October 6, 2026 at 6:53 AM
astroarxiv.bsky.social
Shadows cast by precessing annuli as evidence for an inclined planet in HD 139614. Katie L. Milsom et. al. https://arxiv.org/abs/2610.06332
Figure 1 Figure 2 Figure 3 Figure 4
October 6, 2026 at 6:22 AM
astrophep-bot.bsky.social
Katie L. Milsom, Tim J. Harries, Evan A. Rich, John D. Monnier, Anna S. E. Laws, Benjamin R. Setterholm: Shadows cast by precessing annuli as evidence for an inclined planet in HD 139614 https://arxiv.org/abs/2610.06332 https://arxiv.org/pdf/2610.06332 https://arxiv.org/html/2610.06332
October 6, 2026 at 6:51 AM
abeliansoup.bsky.social
seemed to significantly 'update' beliefs so much as revisit 1/n of them along a precessing path. skill issue at not striking the deeper truths I guess. now I can't circumvent introspection entirely like my hero marc andreessen but endeavour to be more mindful of straying down this subset. sort of.
October 4, 2026 at 1:57 PM
tony873004.bsky.social
10,000 years of asteroid orbits precessing around the Sun.
🔭
White: Main Belt asteroids
Magenta: Near-Earth asteroids
Watch how the orbital planes slowly rotate and pulsate. #astro
September 21, 2026 at 11:23 PM
diane.dianeduane.com
https://spacedaily.com/t-toi1355b-transits-end-2033-precessing-orbit/
Astronomers have less than seven years to watch a giant planet transit its star before its precessing orbit carries it out of alignment for hundreds of years.
TOI-1355 b's transit chord is moving off its rapidly rotating star. If the measured drift holds, the final grazing transit will occur around mid-2033.
spacedaily.com
September 21, 2026 at 8:29 AM