paper

JWST NIRSpec spectroscopy of the triply-lensed galaxy MACS0647JD

arXiv:2305.03042

Abstract

We present JWST/NIRSpec prism spectroscopy of MACS0647-JD, the triply-lensed candidate discovered in HST imaging and spatially resolved by JWST imaging into two components A and B. Spectroscopy of component A yields a spectroscopic redshift based on 7 detected emission lines: CIII] 1907,1909, [OII] 3727, [NeIII] 3869, [NeIII] 3968, H 4101, H 4340, and [OIII] 4363. These are the second-most distant detections of these emission lines to date, in a galaxy observed just 460 million years after the Big Bang. Based on observed and extrapolated line flux ratios we derive a gas-phase metallicity log(O/H) = , or , ionization parameter log() , and an ionizing photon production efficiency erg Hz. The spectrum has a softened Lyman- break, evidence for a strong Ly damping wing, suggesting that MACS0647-JD was unable to ionize its surroundings beyond its immediate vicinity ( pMpc). The Ly damping wing also suppresses the F150W photometry, explaining the slightly overestimated photometric redshift . MACS0647-JD has a stellar mass log() = , including 6 in component A, most of which formed recently (within 20 Myr) with a star formation rate / yr, all within an effective radius pc. The smaller component B () pc is likely older (100 Myr) with more dust ( mag), as found previously. Spectroscopy of a fainter companion galaxy C separated by a distance of \about\ 3kpc reveals a Lyman break consistent with . MACS0647-JD is likely the most distant galaxy merger known.

22 pages, 6 figures, accepted for publication in ApJ