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Hungry Hungry Galaxies: How does the shape of a galaxy’s halo affect its appetite?

Hungry Hungry Galaxies: How does the shape of a galaxy’s halo affect its appetite?

by Ryan White | Jun 22, 2026 | Daily Paper Summaries

Stream in to today’s paper to understand how tearing apart dwarf galaxies can reveal the shape of the dark matter haloes of hungry galaxies.

Meet the AAS 248 Plenary Speakers: Dr. Cara Battersby

Meet the AAS 248 Plenary Speakers: Dr. Cara Battersby

by Niloofar Sharei | Jun 16, 2026 | Career Navigation, Current Events, Interviews, Personal Experiences

Today we interview Milky Way scientist and Central Molecular Zone expert, Prof. Cara Battersby from the University of Connecticut, for her Plenary Talk at #AAS248!

Meet the AAS 248 Plenary Speakers: Dr. George Helou

Meet the AAS 248 Plenary Speakers: Dr. George Helou

by Sowkhya Shanbhog | Jun 16, 2026 | Career Navigation, Current Events, Interviews, Personal Experiences

Meet Dr. George Helou: Caltech astronomer, infrared astronomy pioneer, and AAS plenary speaker reflecting on four decades of exploring the universe through infrared light.

[Guest post] Inviting dimmer cousins to the party

[Guest post] Inviting dimmer cousins to the party

by Guest | Jun 9, 2026 | Daily Paper Summaries

Are fainter galaxies really different than brighter ones? This study reveals that, despite being dimmer, low surface brightness galaxies obey the same fundamental laws of galaxy formation, offering new clues about how galaxies and dark matter halos evolve.

Surfing the (Cosmic) Web

Surfing the (Cosmic) Web

by Madison VanWyngarden | May 26, 2026 | Daily Paper Summaries

How astronomers used the largest JWST survey to build a new map of the Universe

Guest: Re‑envisioning Galaxy Morphology with Sparse Autoencoders

Guest: Re‑envisioning Galaxy Morphology with Sparse Autoencoders

by Guest | May 22, 2026 | Daily Paper Summaries

Euclid is delivering millions of galaxy images, far too many for humans to classify by hand. A new approach uses sparse autoencoders to uncover the hidden morphological features inside deep learning models, revealing both familiar structures and entirely new ones.

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