The Astrophysical Journal (Jan 2024)

Galaxies Going Bananas: Inferring the 3D Geometry of High-redshift Galaxies with JWST-CEERS

  • Viraj Pandya,
  • Haowen Zhang,
  • Marc Huertas-Company,
  • Kartheik G. Iyer,
  • Elizabeth McGrath,
  • Guillermo Barro,
  • Steven L. Finkelstein,
  • Martin Kümmel,
  • William G. Hartley,
  • Henry C. Ferguson,
  • Jeyhan S. Kartaltepe,
  • Joel Primack,
  • Avishai Dekel,
  • Sandra M. Faber,
  • David C. Koo,
  • Greg L. Bryan,
  • Rachel S. Somerville,
  • Ricardo O. Amorín,
  • Pablo Arrabal Haro,
  • Micaela B. Bagley,
  • Eric F. Bell,
  • Emmanuel Bertin,
  • Luca Costantin,
  • Romeel Davé,
  • Mark Dickinson,
  • Robert Feldmann,
  • Adriano Fontana,
  • Raphael Gavazzi,
  • Mauro Giavalisco,
  • Andrea Grazian,
  • Norman A. Grogin,
  • Yuchen Guo,
  • ChangHoon Hahn,
  • Benne W. Holwerda,
  • Lisa J. Kewley,
  • Allison Kirkpatrick,
  • Dale D. Kocevski,
  • Anton M. Koekemoer,
  • Jennifer M. Lotz,
  • Ray A. Lucas,
  • Casey Papovich,
  • Laura Pentericci,
  • Pablo G. Pérez-González,
  • Nor Pirzkal,
  • Swara Ravindranath,
  • Caitlin Rose,
  • Marc Schefer,
  • Raymond C. Simons,
  • Amber N. Straughn,
  • Sandro Tacchella,
  • Jonathan R. Trump,
  • Alexander de la Vega,
  • Stephen M. Wilkins,
  • Stijn Wuyts,
  • Guang Yang,
  • L. Y. Aaron Yung

DOI
https://doi.org/10.3847/1538-4357/ad1a13
Journal volume & issue
Vol. 963, no. 1
p. 54

Abstract

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The 3D geometries of high-redshift galaxies remain poorly understood. We build a differentiable Bayesian model and use Hamiltonian Monte Carlo to efficiently and robustly infer the 3D shapes of star-forming galaxies in James Webb Space Telescope Cosmic Evolution Early Release Science observations with $\mathrm{log}{M}_{* }/{M}_{\odot }=9.0\mbox{--}10.5$ at z = 0.5–8.0. We reproduce previous results from the Hubble Space Telescope Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey in a fraction of the computing time and constrain the mean ellipticity, triaxiality, size, and covariances with samples as small as ∼50 galaxies. We find high 3D ellipticities for all mass–redshift bins, suggesting oblate (disky) or prolate (elongated) geometries. We break that degeneracy by constraining the mean triaxiality to be ∼1 for $\mathrm{log}{M}_{* }/{M}_{\odot }=9.0\mbox{--}9.5$ dwarfs at z > 1 (favoring the prolate scenario), with significantly lower triaxialities for higher masses and lower redshifts indicating the emergence of disks. The prolate population traces out a “banana” in the projected $b/a\mbox{--}\mathrm{log}a$ diagram with an excess of low- b / a , large- $\mathrm{log}a$ galaxies. The dwarf prolate fraction rises from ∼25% at z = 0.5–1.0 to ∼50%–80% at z = 3–8. Our results imply a second kind of disk settling from oval (triaxial) to more circular (axisymmetric) shapes with time. We simultaneously constrain the 3D size–mass relation and its dependence on 3D geometry. High-probability prolate and oblate candidates show remarkably similar Sérsic indices ( n ∼ 1), nonparametric morphological properties, and specific star formation rates. Both tend to be visually classified as disks or irregular, but edge-on oblate candidates show more dust attenuation. We discuss selection effects, follow-up prospects, and theoretical implications.

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