Talk from Earl Bellinger describing black holes in the interior of stars, and observational consequences:
youtu.be/RW0GX36neKM?...
@gully.bsky.social
interpretable machine learning for atmospheric and astronomical data analysis, near-IR spectra, climate tech, stars & planets; bikes, Austin, diving off bridges into the ocean.
Talk from Earl Bellinger describing black holes in the interior of stars, and observational consequences:
youtu.be/RW0GX36neKM?...
I suppose this channel is rare enough that weβre not likely to see one on a nearby star in our lifetimes, but still itβd be cool. Also weβre not sure this channel exists.
26.02.2026 14:15 β π 0 π 0 π¬ 1 π 0The planets would still have IR, you could do direct imaging on them, even better if they were young, youβd probably want a high mass host star for the planets to be young enough. The BH removes the host star for you, no coronagraph needed
26.02.2026 14:10 β π 0 π 0 π¬ 1 π 0So thereβs the prospect of planets that previously had a host star suddenly orbiting a black hole, but without the destructive phase of traditional HR diagram stellar evolution. Dark Planet systems.
26.02.2026 14:01 β π 0 π 0 π¬ 1 π 0Assumes you have some precursor to predict the accretion event timing, probably wouldnβt work out, free fall time is at least comparable to light echo time, etc. but upside bonus if they were eclipsing before the event, resulting BH could lens the planets if geometry is perfect?
26.02.2026 13:59 β π 0 π 0 π¬ 1 π 0New planet detection technique:
Look for stars that disappear entirely (black holes in interior, cf Bellinger) then look for light echo plateaus from the reflected light of planets.
Apparently ~100 M dwarfs have disappeared consistent with this mechanism. Youβd have a few light minutes of signal.
Currently reading the Project Hail Mary book and thereβs a ton of astrophysics in itβno spoilers but early on thereβs infrared spectroscopy, ALMA, and more. Curious to hear what other astronomers think!
25.02.2026 14:44 β π 1 π 0 π¬ 1 π 0For astrometry, youβre right that better knowledge of the PSF yields benefits in the high SNR regime as well, since asymmetries in the PSF shape need to be understood to account for biases in the centroid. Chromatic effects mean the PSF fitting should help in all cases
25.02.2026 14:41 β π 0 π 0 π¬ 1 π 0Good point, I suppose it depends on the goalβ for photometry, aperture-based methods give you comparable results to PSF fitting in the high SNR regime. In the low SNR regime, the background noise dominates the aperture based methods, so PSF fitting boosts delivered SNR by weighting the pixels.
25.02.2026 14:31 β π 0 π 0 π¬ 2 π 0Well said
25.02.2026 14:24 β π 1 π 0 π¬ 0 π 0Neat work on precision PSF modeling of Gaia!
Little known fact: we captured Kepler driftscan PSFs during downtime in the K2 mission. PSF modeling is great boon for low SNR science, extended objects, etc.
Good band name, or maybe a softball team composed in part by punk rock astronomers with a fastball
20.02.2026 04:51 β π 1 π 0 π¬ 0 π 0Itβs me
12.02.2026 04:10 β π 4 π 0 π¬ 0 π 0Sans serif math in LaTeX is so satisfying. \mathsf{}
10.02.2026 16:44 β π 0 π 0 π¬ 0 π 0Above all itβs just great to hear Danβs voice, miss that guy
10.02.2026 15:52 β π 1 π 0 π¬ 0 π 0youtu.be/yUAZGR9RwPI?...
@benjaminpope.bsky.social itβs mostly live coding with examples of JAX-isms and some new goodies like context managers for float64
Very cool opportunity to make differentiable physics models for EPRV, work with Ben and co, and live in a cool place. Pretty much a dream job, apply!
10.02.2026 11:55 β π 1 π 0 π¬ 0 π 0Still want a JAX for science conference, where all my JAX scientists at
06.02.2026 18:05 β π 0 π 0 π¬ 0 π 0The sheer joy I felt just now discovering that there is a new Dan Foreman Mackey video about JAX.
06.02.2026 18:03 β π 11 π 2 π¬ 3 π 0standing room only for physics?
faith in humanity restored β¨π
I still feel like differentiable models are under appreciated, itβs like a magic super power for interpretability and extensibility. Maybe LLM-assisted coding can bring autodiff to more science teams? Still a mental leap to adoption.
04.02.2026 14:25 β π 0 π 0 π¬ 0 π 0Everything becomes so much easier when you can forward model your data
04.02.2026 14:16 β π 0 π 0 π¬ 0 π 0Looking back on this talk about autodiffable spectral models, there is still so much promise, Iβd love to see what folks have been up to in this space!
speakerdeck.com/gully/blase-...
New job opportunity at @stsci.edu: Senior Astronomical Data Scientist for data analysis tools, working closely with my team and me.
This role is very similar to mine. If you have questions, I'm happy to answer them. π§ͺπ
Currently 83% carbon-free energy in Texas right now:
- 40% wind
- 33% solar
- 10% nuclear
Wholesale prices are negative, and 3.5 GW of batteries are charging.
βοΈπ¨βοΈπ
Despite headwinds, over 20 new EVs are coming to the US market in 2026, including several more affordable vehicles. Can any thrive without federal tax credits? insideevs.com/news/782572/... ππ‘ ππ
04.01.2026 14:42 β π 66 π 8 π¬ 4 π 1Itβs wild that stellar limb effects start to matter at non-negligible fractions of a resolution element on the ELTs!
Challenge⦠or opportunity!?
The first batteries rolled off the production line at Toyotaβs new $14 billion battery plant in Liberty, North Carolina. The plant will produce batteries for hybrid, plug-in hybrid & electric models, which Toyota plans to make up 70% of its sales by 2030 electrek.co/2025/11/17/t... ππ‘ ππ
25.11.2025 16:11 β π 45 π 4 π¬ 0 π 1Get outside into a dark place if you can tonight - no guarantees, but a possible brilliant display of the northern lights.
12.11.2025 15:31 β π 208 π 64 π¬ 9 π 6Hat tip @wilsonar.bsky.social for this! π€£
06.11.2025 00:49 β π 100 π 28 π¬ 0 π 0