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Galaxies

The Galaxies Science Interest Group (Galaxies SIG) offers an opportunity for researchers across all career stages studying galaxies.

About Galaxies SIG

Exploring Galaxies Throughout the Universe

The Cosmic Origins program is forming a science interest group (SIG) that will help NASA understand and implement recommendations from the upcoming decadal survey in the area of galaxies. This group will also sponsor discussions, research seminars, and periodic meetings.

Participating in a science interest group is an opportunity to meet people and make professional connections. It is an opportunity to learn about NASA astrophysics and share in the joy of creative science. It is also an opportunity to help others and give back to the astronomical community.

distant galaxies appear as bright glowing spots in this Webb telescope image, with some smeared by gravitational lensing; foreground stars appear bright with six-pointed diffraction spikes, owing to the shape of Webb's mirrors
NASA's James Webb Space Telescope has produced the deepest and sharpest infrared image of the distant universe to date. Known as Webb's First Deep Field, this image of galaxy cluster SMACS 0723 is overflowing with detail. Thousands of galaxies - including the faintest objects ever observed in the infrared - have appeared in Webb's view for the first time.
NASA, ESA, CSA, and STScI

News & Events

Galaxies SIG Seminar 3 December 2025

Simulations Meet Space Telescopes to Understand AGN at Cosmic Dawn Speaker Sabrina Berger (University of Melbourne) Abstract For the first time, JWST lets us directly see the stellar light from galaxies hosting luminous quasars at z > 6. Early stellar…

Dec 3, 2025
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Galaxies SIG Seminar 5 November 2025

Disentangling Baryonic and Dark Matter Physics with the Smallest Galaxies Speaker Erin Kado-Fong (Stanford)  Abstract Low-mass “dwarf” galaxies, with masses less than around 10 percent that of the Milky Way, present both a puzzle and an opportunity for our understanding…

Nov 5, 2025
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Galaxies Science Interest Group (Galaxies SIG)

Leadership Council Name Affiliation & Email Lead: Benne Holwerda Email Co-Lead: Aaron Yung Email Caryl Gronwall Email Gregory Mosby Email David Sobral Email Shobita Satyapal Email Rupali Chandar Email

Aug 25, 2025
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Galaxies SIG Seminar June 18, 2025

Enhance! Spatially-Resolving Sub-kpc Physics Within High-z Galaxies Taylor Hutchison, NASA / GSFC With the advent of JWST, we have witnessed an explosion of science in the early Universe — with recent results unveiling the conditions for the earliest births and…

Jun 18, 2025
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Galaxies SIG Seminar June 4, 2025

Resolving Galaxy Evolution Across Space, Time, and Wavelength with HWO Kartheik Iyer, Columbia Univ., Hubble Fellow HWO’s exceptional angular resolution and wavelength coverage will enable detailed reconstruction of star formation histories (SFHs) for an unprecedented number of galaxies across cosmic…

Jun 4, 2025
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Galaxies SIG Seminar May 21, 2025

The Extreme Nature of Galaxies and Stellar Populations at Cosmic Dawn Harley Katz | University of Chicago The few years of JWST observations have revealed numerous anomalies at high-redshift such as an unexpected excess of bright galaxies at z>9, peculiar…

May 21, 2025
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Leadership Council

NameAffiliation & Email
Lead: Benne HolwerdaEmail
Co-Lead: Aaron YungEmail
Caryl GronwallEmail
Gregory MosbyEmail
David SobralEmail
Shobita SatyapalEmail
Rupali ChandarEmail

How to Participate

We invite participation from the community, particularly from early-career researchers and those from under represented backgrounds in astronomy. Please contact us for more information about our activities and mission, and how you can get involved.

Contact Us about How to Participate
Webb and Hubble�s Views of Spiral Galaxy NGC 628

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.