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astro-ph.GA2024★ 9 cited
Halfway to the Peak: The JWST MIRI 5.6 micron number counts and source population
Leonid Sajkov, Anna Sajina, Alexandra Pope +9
We present an analysis of eight JWST Mid-Infrared Instrument (MIRI) 5.6 micron images with depths of ~0.1 uJy. We detect 2854 sources within our combined area of 18.4 square…
astro-ph.GA2024
Ground- and Space-Based Dust Observations of VV 191 Overlapping Galaxy Pair
C. Robertson, B. Holwerda, J. Young +12
The Balmer decrement (H/H) provides a constraint on attenuation, the cumulative effects of dust grains in the ISM. The ratio is a reliable spectroscopic tool for deriving the…