Work

A First Measurement of Circumgalactic Dust Reddening from Only 4.6 deg 2 of the Rubin Observatory’s Data Preview 1

Year: 2026
Type: article
Abstract: We present the first measurement of circumgalactic dust reddening from the Vera C. Rubin Observatory, using only 4.6 deg 2 of ComCam Data Preview 1—roughly 0.03% of the final LSST footprint. Using photometric redshifts, we stack background-galaxy colors around foreground-galaxy positions and detect a chromatic reddening profile from r ⊥ ≃ 10 kpc to 1 Mpc. Interpreting average E ( g − z ) with a Milky Way extinction curve, we find A V = ( 1.3 ± 0.4 ) × 1 0 − 1 ( r ⊥ / 20 kpc ) − 1.8 ± 0.4 within 120 kpc. The amplitude and radial dependence agree with earlier Sloan Digital Sky Survey, KiDS, and Dark Energy Survey results despite the ∼1000× smaller survey area and a foreground sample extending 3–6 mag fainter and 1–2 dex lower in stellar mass. The innermost 10–15 kpc bin reaches A V ≃ 0.3 mag, comparable to high-latitude extinction through the Milky Way disk near the solar circle; the steep power-law slope implies a dust distribution that does not simply trace the halo-gas profile. Splitting by rest-frame g − r shows stronger extinction around red foreground galaxies (rest-frame g − r > 0.5), although the blue subsample is too noisy to establish a significant color dependence. This red sample, with median halo mass 5 × 10 11 M ⊙ , shows substantially more reddening within 50 kpc than previously measured around more massive luminous red galaxies and implies a dust-to-stellar-mass ratio of ∼2%, nearly saturating the dust budget allowed by stellar metal yields. These pathfinder data demonstrate LSST’s promise for high-precision galaxy–dust measurements across galaxy mass, environment, and redshift.
Language: English
Open Access status: gold
Estimated APC paid: $2,400
OpenAlex ID: W7213459398
FWCI: 0.821
Cites: 100
Cited by: 1
Related to: 10