Isabel Sands
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isabel-sands.bsky.social
Isabel Sands
@isabel-sands.bsky.social
Physics PhD student at Caltech, interested in everything dark matter. Yale physics ‘21 (she/her)
🔭🧪 Paper day! I’m really excited about this one. We used simulations of Milky Way-like galaxies simulated with full cosmic ray spectra to model gamma-ray emission. The simulated galaxies form large gamma-ray bubbles with remarkable similarities to the Fermi bubbles observed in the Milky Way.
October 17, 2025 at 5:10 PM
🔭🧪
Paper day! We used MHD galaxy formation simulations with multi-species cosmic ray spectra to model diffuse gamma-ray emission in Milky Way analogs. This allows us to see how gamma-ray flux changes due to star formation, ISM structure, B fields, etc. over time. arxiv.org/pdf/2509.18351
September 25, 2025 at 1:51 AM
Reposted by Isabel Sands
This is what amounts to an ILLEGAL & indiscriminate funding cut for research centers everywhere. It will mean shuttering labs across the country, layoffs in red & blue states, and derailing lifesaving research on everything from cancer to opioid addiction.

We all need to speak out to save lives.
February 8, 2025 at 2:02 AM
Excited and honored to have the opportunity to share the recent work I led at #dwarfgalaxies2024 !
#dwarfgalaxies2024 using FIRE Isabel Sands suggests HI rotation curves are not a good representation of DM halo profiles due to time dependence and extra pressure terms, resulting in artificially diverse RCs. arxiv.org/abs/2404.16247
July 31, 2024 at 10:27 PM