The ALPINE-ALMA [C ii] survey: Investigation of 10 galaxies at z ∼ 4.5 with [O ii] and [C ii] line emission − ISM properties and [O ii]−SFR relation. Issue 1 (14th January 2022)

• Record Type: Journal Article
• Authors: Vanderhoof, Brittany N; Faisst, A L; Shen, L; Lemaux, B C; Béthermin, M; Capak, P L; Cassata, P; Le Fèvre, O; Schaerer, D; Silverman, J; Yan, L; Boquien, M; Gal, R; Kartaltepe, J; Lubin, L M; Dessauges-Zavadsky, M; Fudamoto, Y; Ginolfi, M; Hathi, N P; Jones, G C; Koekemoer, A M; Narayanan, D; Romano, M; Talia, M; Vergani, D; Zamorani, G
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 511:Issue 1(2022)
• Page Start: 1303
• Page End: 1316
• Publication Date: 2022-01-14
• Subjects: galaxies: evolution -- galaxies: high-redshift -- galaxies: ISM; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac071
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present 10 main-sequence ALPINE galaxies (log ( M / M ⊙ ) = 9.2−11.1 and ${\rm SFR}=23-190\, {\rm M_{\odot }\, yr^{-1}}$ ) at z ∼ 4.5 with optical [O ii ] measurements from Keck /MOSFIRE spectroscopy and Subaru /MOIRCS narrow-band imaging. This is the largest such multiwavelength sample at these redshifts, combining various measurements in the ultraviolet, optical, and far-infrared including [C ii ]158 $\mu$ m line emission and dust continuum from ALMA and H α emission from Spitzer photometry. For the first time, this unique sample allows us to analyse the relation between [O ii ] and total star-formation rate (SFR) and the interstellar medium (ISM) properties via [O ii ]/[C ii ] and [O ii ]/H α luminosity ratios at z ∼ 4.5. The [O ii ]−SFR relation at z ∼ 4.5 cannot be described using standard local descriptions, but is consistent with a metal-dependent relation assuming metallicities around $50{{\ \rm per\ cent}}$ solar. To explain the measured dust-corrected luminosity ratios of $\log (L_{\rm [OII]}/L_{\rm [CII]}) \sim 0.98^{+0.21}_{-0.22}$ and $\log (L_{\rm [OII]}/L_{\rm H\alpha }) \sim -0.22^{+0.13}_{-0.15}$ for our sample, ionization parameters log ( U ) < −2 and electron densities $\log (\rm n_e / {\rm [cm^{-3}]}) \sim 2.5-3$ are required. The former is consistent with galaxies at z ∼ 2−3, however lower than at z > 6. The latter may be slightly higher than expected given the galaxies' specific SFR. The analysis of this pilot sample suggests that typical log ( M /M⊙ ) > 9 galaxies at z ∼ 4.5 to have broadly similar ISM properties as their descendants at z ∼ 2 and suggest a strong evolution of ISM properties since the epoch of reionization at z > 6.