Dust is a fundamental component of the interstellar medium and provides a key tracer of the baryon cycle that regulates galaxy evolution. The dust-to-gas ratio links metals in the gas phase to those locked into dust grains, making it a sensitive diagnostic of dust production, grain growth, and destruction. We present m...
N. N. Geesink, G. Popping, L. Boogaard et al.· 0 citations
Dust plays a key role in galaxy evolution by influencing star formation and shaping the observed spectrum of galaxies. However, at z~2 (cosmic noon) our knowledge of the dust mass budget is currently limited to the most massive, metal-rich systems, which are not representative of the bulk galaxy population. Here, we pr...
M. Solimano, I. Shivaei, G. Popping et al.· 0 citations
The baryon cycle governs the exchange of gas, metals, and dust between galaxies and their environments, but simultaneous constraints on these constituents remain scarce beyond z~1. The ALMA Chemical Evolution (ACE) survey is a Cycle 11 ALMA Large Program designed to address this by studying the molecular gas, dust, and...
I. Shivaei, G. Popping, L. Boogaard et al.· 0 citations
Understanding how dust forms and evolves over cosmic time is a key open problem in extragalactic astrophysics. Galaxies in the early Universe were once thought to be mostly dust-poor, but recent discoveries of heavily dust-obscured galaxies near the Epoch of Reionization challenge models of early dust production and ra...
A. Faisst, Felix Martinez, J. Kartaltepe et al.· 0 citations
A deep-learning framework that performs 4.6x spatial super-resolution from WISE W1 toward Spitzer IRAC Ch1, and characterize its behavior on the COSMOS field suggests genuine resolution enhancement and source deblending, providing a path toward applying super-resolution across the all-sky area that Spitzer could not co...
S. Rezaee, S. Hemmati, B. Mobasher et al.· 0 citations
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