(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - I. Multiwavelength identifications and redshift distribution
arXiv:1502.05854 · doi:10.1051/0004-6361/201425032
Abstract
We used the PdBI to map a sample of 15 SMGs in the COSMOS field at the wavelength of 1.3 mm. The target SMGs were originally discovered in the JCMT/AzTEC 1.1 mm continuum survey at S/N=4-4.5. This paper presents, for the first time, interferometric millimetre-wavelength observations of these sources. The angular resolution of our observations, 1.8", allowed us to accurately determine the positions of the target SMGs. Using a detection threshold of S/N>4.5 regardless of multiwavelength counterpart association, and 4<S/N<=4.5 if a multiwavelength counterpart within 1.5" is also present, the total number of detections in our survey is 22. Three of our detected SMGs (AzTEC21, 27, and 28; which corresponds to 20%) are marginally resolved at our angular resolution, and these sources are found to have elongated or clumpy morphologies and/or multiple components. Using optical to NIR photometric redshifts, available spectroscopic redshifts, and redshifts estimated from the radio-to-submm spectral index we infer a median redshift of for our sample. To study the overall multiplicity and redshift distribution of flux-limited samples of SMGs we combined these sources with the 15 brightest AzTEC SMGs detected at 1.1 mm, AzTEC1-15, and studied previously. This constitutes a complete, flux- and S/N-limited 1.1-mm selected sample. We find that the median redshift for the 15 brightest AzTEC SMGs () is consistent with that for AzTEC16-30. This conforms to recent observational findings that SMGs do not exhibit any significant trend between the redshift and (sub)mm flux density. For the combined AzTEC1-30 sample we derive a median redshift of , consistent with previous results based on mm-selected samples. We further infer that within the combined AzTEC1-30 sample of sources separate into multiple components.
31 pages (incl. 5 appendices with 3 figures and 1 table), 6 figures and 4 tables in the main text. Accepted for publication in A&A
References in corpus (40)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- The Cosmic Evolution Survey (COSMOS) -- Overview
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- Formation of Massive Galaxies at High Redshift: Cold Streams, Clumpy Disks and Compact Spheroids
- zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
- UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
- A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
- The Chandra COSMOS Survey, I: Overview and Point Source Catalog
- Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- SHARC-2 350 Micron Observations of Distant Submillimeter Selected Galaxies
- The VLA-COSMOS Survey: II. Source Catalog of the Large Project
- A massive proto-cluster of galaxies at a redshift of z {\approx} 5.3
- An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source counts
- AzTEC Millimetre Survey of the COSMOS Field: I. Data Reduction and Source Catalogue
- Star Formation at From the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH)
- Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
- ALMA Imaging of Gas and Dust in a Galaxy Protocluster at Redshift 5.3: [CII] Emission in "Typical" Galaxies and Dusty Starbursts ~1 Billion Years after the Big Bang
- Evidence for a Population of High-Redshift Submillimeter Galaxies from Interferometric Imaging
- A Massive Molecular Gas Reservoir in the z=5.3 Submillimeter Galaxy AzTEC-3
- Large Structures and Galaxy Evolution in COSMOS at z < 1.1
- The AzTEC mm-Wavelength Camera
- An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared morphologies and stellar sizes
- Spectroscopic Confirmation Of An Extreme Starburst At Redshift 4.547
- A submillimetre galaxy at z=4.76 in the LABOCA survey of the Extended Chandra Deep Field South
- Molecular Gas in a Submillimeter Galaxy at z=4.5: Evidence for a Major Merger at 1 Billion Years after the Big Bang
- The SCUBA HAlf Degree Extragalactic Survey (SHADES) - VII. Optical/IR photometry and stellar masses of sub-millimeter galaxies
- Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
- UV to IR SEDs of UV selected galaxies in the ELAIS fields: evolution of dust attenuation and star formation activity from z=0.7 to z=0.2
- The Cosmic Evolution Survey (COSMOS): a large-scale structure at z=0.73 and the relation of galaxy morphologies to local environment
- The evolution of submillimetre galaxies: two populations and a redshift cut-off
- Physical properties of z>4 submillimeter galaxies in the COSMOS field
- An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: radio properties and the far-infrared/radio correlation
- The growth of the nuclear black holes in submillimeter galaxies
- A Deep 1.2 mm Map of the Lockman Hole North Field
- Interferometric detections of GOODS 850-5 at 1 mm and 1.4 GHz
- An Evolutionary Model For Submillimeter Galaxies
- Clarifying the nature of the brightest submillimetre sources: interferometric imaging of LH850.02
- The redshift distribution of submillimetre galaxies at different wavelengths
Cited by in corpus (14)
- ALMA spectroscopic survey in the Hubble Ultra Deep Field: Continuum number counts, resolved 1.2-mm extragalactic background, and properties of the faintest dusty star forming galaxies
- ALMA Deep Field in SSA22: Source Catalog and Number Counts
- An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution
- The ALMA Frontier Fields survey I: 1.1 mm continuum detections in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
- An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
- The IRAM/GISMO two-millimeter survey in the COSMOS field
- The redshift and star formation mode of AzTEC2: a pair of massive galaxies at
- Unveiling the nature of 11 dusty star-forming galaxies at the peak of cosmic star formation history
- (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies IV. Physical properties derived from spectral energy distributions
- A photo-z cautionary tale: Redshift confirmation of COSBO-7 at z=2.625
- The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey
- On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
- A SCUBA-2 Selected Herschel-SPIRE Dropout and the Nature of this Population
- Tracing obscured galaxy build-up at high redshift using deep radio surveys