Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15
arXiv:2608.08015
Abstract
We present new Atacama Large Millimeter/submillimeter Array (ALMA) Band 9 () and 4 () observations towards the Big Three Dragons, a pair of merging Lyman-break galaxies (LBGs) at . The system was previously detected in ALMA Bands 6, 7 and 8 (), which, combined with our new observations, allows us to robustly constrain its dust temperature and obscured SFR. The unresolved Band 4 observations yield a detection, and the Band 9 observations detect the Eastern and Western LBGs at and , respectively. Through modified blackbody fitting, we infer a global dust temperature of for the system, which implies a high IR luminosity of . This makes the Big Three Dragons one of the most IR-luminous systems known at , with a total that is almost completely obscured (). Using resolved ALMA observations in Bands 6, 8 and 9, we confirm both LBGs have hot dust temperatures () and correspondingly high obscured fractions (). We find the Western LBG to fall above the canonical IRX- relation, suggesting patchy dust obscuration. The compact Eastern component, on the other hand, is consistent with a Calzetti- or SMC-like dust screen within the uncertainties. Together with the similarly hot dust temperature recently reported for the galaxy MACS0416-Y1, our results suggest a non-negligible fraction of star formation at the bright end of the UV luminosity function is highly dust-obscured, even at .
Submitted to MNRAS. Main text: 14 pages, 9 figures, 3 tables. Appendices: 2 pages, 4 figures, 2 tables