"Big Three Dragons": a z = 7.15 Lyman BreakGalaxy Detected in [OIII] 88 m, [CII] 158 m, and Dust Continuum with ALMA
arXiv:1806.00486 · doi:10.1093/pasj/psz049
Abstract
We present new ALMA observations and physical properties of a Lyman Break Galaxy at z=7.15. Our target, B14-65666, has a bright ultra-violet (UV) absolute magnitude, , and has been spectroscopically identified in Ly with a small rest-frame equivalent width of Å. Previous HST image has shown that the target is comprised of two spatially separated clumps in the rest-frame UV. With ALMA, we have newly detected spatially resolved [OIII] 88 m, [CII] 158 m, and their underlying dust continuum emission. In the whole system of B14-65666, the [OIII] and [CII] lines have consistent redshifts of , and the [OIII] luminosity, , is about three times higher than the [CII] luminosity, . With our two continuum flux densities, the dust temperature is constrained to be K under the assumption of the dust emissivity index of , leading to a large total infrared luminosity of . Owing to our high spatial resolution data, we show that the [OIII] and [CII] emission can be spatially decomposed into two clumps associated with the two rest-frame UV clumps whose spectra are kinematically separated by km s. We also find these two clumps have comparable UV, infrared, [OIII], and [CII] luminosities. Based on these results, we argue that B14-65666 is a starburst galaxy induced by a major-merger. The merger interpretation is also supported by the large specific star-formation rate (defined as the star-formation rate per unit stellar mass), sSFR Gyr, inferred from our SED fitting. Probably, a strong UV radiation field caused by intense star formation contributes to its high dust temperature and the [OIII]-to-[CII] luminosity ratio.
arXiv comment24 pages, 13 figures, 9 tables. Accepted for publication in PASJ. In addition to the dust continuum detection in ALMA Band 6 reported in the original manuscript, we newly report the dust continuum detection in ALMA Band 8 based on our new ALMA Cycle 5 observations
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- Constraining the physical properties of gas in high-z galaxies with far-infrared and submillimetre line ratios
- Spatially resolved H emission in B14-65666: compact starbursts, ionizing efficiency and gas kinematics in an advanced merger at the Epoch of Reionization
- Disentangling emission from star-forming regions in the Magellanic Clouds: Linking [OIII]88 micron and 24 micron
- Ly Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly detection
- Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
- A theoretical investigation of far-infrared fine structure lines at and of the origin of the [OIII]88/[CII]158 enhancement
- Development Status of Wideband Millimeter-Wave Receivers for LMT-FINER
- Tight correlation of star formation with [Ci] and CO lines across cosmic time
- Galaxy evolution and radiative properties in the early Universe: multi-wavelength analysis in cosmological simulations
- First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
- Measuring the HI content of individual galaxies out to the epoch of reionization with [CII]
- Early galaxy evolution: The complex interstellar medium distribution of the z~7 galaxy A1689-zD1
- The ALMA View of High-Redshift Galaxy Formation