TY - JOUR
T1 - Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85
AU - Casey, Caitlin M.
AU - Zavala, Jorge A.
AU - Aravena, Manuel
AU - Béthermin, Matthieu
AU - Caputi, Karina I.
AU - Champagne, Jaclyn B.
AU - Clements, David L.
AU - Cunha, Elisabete Da
AU - Drew, Patrick
AU - Finkelstein, Steven L.
AU - Hayward, Christopher C.
AU - Kartaltepe, Jeyhan S.
AU - Knudsen, Kirsten
AU - Koekemoer, Anton M.
AU - Magdis, Georgios E.
AU - Man, Allison
AU - Manning, Sinclaire M.
AU - Scoville, Nick Z.
AU - Sheth, Kartik
AU - Spilker, Justin
AU - Staguhn, Johannes
AU - Talia, Margherita
AU - Taniguchi, Yoshiaki
AU - Toft, Sune
AU - Treister, Ezequiel
AU - Yun, Min
PY - 2019/12/10
Y1 - 2019/12/10
N2 - We present a physical characterization of MM J100026.36+021527.9 (a.k.a. "Mambo-9"), a dusty star-forming galaxy (DSFG) at z = 5.850 ± 0.001. This is the highest-redshift unlensed DSFG (and fourth most distant overall) found to date and is the first source identified in a new 2 mm blank-field map in the COSMOS field. Though identified in prior samples of DSFGs at 850 μm to 1.2 mm with unknown redshift, the detection at 2 mm prompted further follow-up as it indicated a much higher probability that the source was likely to sit at z > 4. Deep observations from the Atacama Large Millimeter and submillimeter Array (ALMA) presented here confirm the redshift through the secure detection of 12CO(J = 6→5) and p-H2O (21,1 → 20,2). Mambo-9 is composed of a pair of galaxies separated by 6 kpc with corresponding star formation rates of 590 M o˙ yr-1 and 220 M o˙ yr-1, total molecular hydrogen gas mass of (1.7 ± 0.4) × 1011 M o˙, dust mass of (1.3 ± 0.3) × 109 M o˙, and stellar mass of (3.2-1.5 +1.0) × 109 M o˙. The total halo mass, (3.3 ± 0.8) × 1012 M o˙, is predicted to exceed 1015 M o˙ by z = 0. The system is undergoing a merger-driven starburst that will increase the stellar mass of the system tenfold in τ depl = 40-80 Myr, converting its large molecular gas reservoir (gas fraction of 96-2 +1) into stars. Mambo-9 evaded firm spectroscopic identification for a decade, following a pattern that has emerged for some of the highest-redshift DSFGs found. And yet, the systematic identification of unlensed DSFGs like Mambo-9 is key to measuring the global contribution of obscured star formation to the star formation rate density at z ⪆ 4, the formation of the first massive galaxies, and the formation of interstellar dust at early times (≲1 Gyr).
AB - We present a physical characterization of MM J100026.36+021527.9 (a.k.a. "Mambo-9"), a dusty star-forming galaxy (DSFG) at z = 5.850 ± 0.001. This is the highest-redshift unlensed DSFG (and fourth most distant overall) found to date and is the first source identified in a new 2 mm blank-field map in the COSMOS field. Though identified in prior samples of DSFGs at 850 μm to 1.2 mm with unknown redshift, the detection at 2 mm prompted further follow-up as it indicated a much higher probability that the source was likely to sit at z > 4. Deep observations from the Atacama Large Millimeter and submillimeter Array (ALMA) presented here confirm the redshift through the secure detection of 12CO(J = 6→5) and p-H2O (21,1 → 20,2). Mambo-9 is composed of a pair of galaxies separated by 6 kpc with corresponding star formation rates of 590 M o˙ yr-1 and 220 M o˙ yr-1, total molecular hydrogen gas mass of (1.7 ± 0.4) × 1011 M o˙, dust mass of (1.3 ± 0.3) × 109 M o˙, and stellar mass of (3.2-1.5 +1.0) × 109 M o˙. The total halo mass, (3.3 ± 0.8) × 1012 M o˙, is predicted to exceed 1015 M o˙ by z = 0. The system is undergoing a merger-driven starburst that will increase the stellar mass of the system tenfold in τ depl = 40-80 Myr, converting its large molecular gas reservoir (gas fraction of 96-2 +1) into stars. Mambo-9 evaded firm spectroscopic identification for a decade, following a pattern that has emerged for some of the highest-redshift DSFGs found. And yet, the systematic identification of unlensed DSFGs like Mambo-9 is key to measuring the global contribution of obscured star formation to the star formation rate density at z ⪆ 4, the formation of the first massive galaxies, and the formation of interstellar dust at early times (≲1 Gyr).
UR - http://www.scopus.com/inward/record.url?scp=85077309336&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ab52ff
DO - 10.3847/1538-4357/ab52ff
M3 - Article
AN - SCOPUS:85077309336
SN - 0004-637X
VL - 887
JO - The Astrophysical Journal
JF - The Astrophysical Journal
IS - 1
M1 - 55
ER -