Journal
ASTROPHYSICAL JOURNAL
Volume 833, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/833/1/71
Keywords
galaxies: evolution; galaxies: high-redshift; galaxies: ISM; galaxies: star formation; instrumentation:interferometers; submillimeter: galaxies
Categories
Funding
- FONDECYT [1140099]
- ERC grant COSMIC-DAWN
- ERC grant DUSTYGAL
- ERC grant COSMICISM
- Conicyt grant Basal-CATA [PFB-06/2007]
- Conicyt grant Anilo [ACT1417]
- FONDECYT Regular [1141218, 1151408]
- Ministry of Economy, Development, and Tourism's Millennium Science Initiative [IC120009]
- Future Fellowship [FT150100079]
- National Science Foundation [AST-1614213]
- STFC [ST/L00075X/1]
- Royal Society/Wolfson Merit award
- DFG priority program 1573 The physics of the interstellar medium.
- Collaborative Research Council 956, subproject A1 - Deutsche Forschungsgemeinschaft (DFG)
- German ARC
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1614213] Funding Source: National Science Foundation
- STFC [ST/L005042/1] Funding Source: UKRI
Ask authors/readers for more resources
We present a search for [C II] line and dust continuum emission from optical dropout galaxies at z > 6 using ASPECS, our Atacama Large Millimeter submillimeter Array Spectroscopic Survey in the Hubble Ultra-deep Field (UDF). Our observations, which cover the frequency range of 212-272 GHz, encompass approximately the range of 6 < z < 8 for [C II] line emission and reach a limiting luminosity of L-[C II] similar to (1.6-2.5) x 10(8) L-circle dot.We identify 14 [C II] line emitting candidates in this redshift range with significances > 4.5 sigma, two of which correspond to blind detections with no optical counterparts. At this significance level, our statistical analysis shows that about 60% of our candidates are expected to be spurious. For one of our blindly selected [C II] line candidates, we tentatively detect the CO(6-5) line in our parallel 3 mm line scan. None of the line candidates are individually detected in the 1.2 mm continuum. A stack of all [C II] candidates results in a tentative detection with S-1.2 (mm) = 14 +/- 5 mu Jy. This implies a dust-obscured star-formation rate (SFR) of (3 +/- 1) M-circle dot yr(-1). We find that the two highest-SFR objects have candidate [C II] lines with luminosities that are consistent with the low-redshift L-[C II] versus SFR relation. The other candidates have significantly higher [C II] luminosities than expected from their UV-based SFR. At the current sensitivity, it is unclear whether the majority of these sources are intrinsically bright [C II] emitters, or spurious sources. If only one of our line candidates was real (a scenario greatly favored by our statistical analysis), we find a source density for [C II] emitters at 6 < z < 8 that is significantly higher than predicted by current models and some extrapolations from galaxies in the local universe.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available