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H-ATLAS : a candidate high redshift cluster/protocluster of star-forming galaxies

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Abstract
We investigate the region around the Planck-detected z = 3.26 gravitationally lensed galaxy HATLAS J114637.9-001132 (hereinafter HATLAS12-00) using both archival Herschel data from the H-ATLAS survey and using submm data obtained with both LABOCA and SCUBA2. The lensed source is found to be surrounded by a strong overdensity of both Herschel-SPIRE sources and submm sources. We detect 17 bright (S-870 > similar to 7 mJy) sources at >4 sigma closer than 5 arcmin to the lensed object at 850/870 mu m. 10 of these sources have good cross-identifications with objects detected by Herschel-SPIRE which have redder colours than other sources in the field, with 350 mu m flux > 250 mu m flux, suggesting that they lie at high redshift. Submillimeter Array (SMA) observations localise one of these companions to similar to 1 arcsec, allowing unambiguous cross identification with a 3.6 and 4.5 mu m Spitzer source. The optical/near-IR spectral energy distribution of this source is measured by further observations and found to be consistent with z > 2, but incompatible with lower redshifts. We conclude that this system may be a galaxy cluster/protocluster or larger scale structure that contains a number of galaxies undergoing starbursts at the same time.
Keywords
galaxies: high redshift, galaxies: starburst, submillimetre: galaxies, SPECTRAL ENERGY-DISTRIBUTIONS, SCIENCE DEMONSTRATION PHASE, HERSCHEL-ATLAS, SUBMILLIMETER GALAXIES, MOLECULAR GAS, SOURCE EXTRACTION, DUSTY STARBURSTS, LENSED GALAXIES, PROTO-CLUSTER, DEEP FIELD

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MLA
Clements, DL, et al. “H-ATLAS : A Candidate High Redshift Cluster/Protocluster of Star-Forming Galaxies.” MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol. 461, no. 2, 2016, pp. 1719–33, doi:10.1093/mnras/stw1224.
APA
Clements, D., Braglia, F., Petitpas, G., Greenslade, J., Cooray, A., Valiante, E., … van der Werf, P. (2016). H-ATLAS : a candidate high redshift cluster/protocluster of star-forming galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 461(2), 1719–1733. https://doi.org/10.1093/mnras/stw1224
Chicago author-date
Clements, DL, F Braglia, G Petitpas, J Greenslade, A Cooray, E Valiante, G De Zotti, et al. 2016. “H-ATLAS : A Candidate High Redshift Cluster/Protocluster of Star-Forming Galaxies.” MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 461 (2): 1719–33. https://doi.org/10.1093/mnras/stw1224.
Chicago author-date (all authors)
Clements, DL, F Braglia, G Petitpas, J Greenslade, A Cooray, E Valiante, G De Zotti, B O’Halloran, J Holdship, B Morris, I Pérez-Fournon, D Herranz, D Riechers, Maarten Baes, M Bremer, N Bourne, H Dannerbauer, A Dariush, L Dunne, S Eales, Jacopo Fritz, J Gonzalez-Nuevo, R Hopwood, E Ibar, RJ Ivison, LL Leeuw, S Maddox, MJ Michałowski, M Negrello, A Omont, I Oteo, S Serjeant, I Valtchanov, JD Vieira, J Wardlow, and P van der Werf. 2016. “H-ATLAS : A Candidate High Redshift Cluster/Protocluster of Star-Forming Galaxies.” MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 461 (2): 1719–1733. doi:10.1093/mnras/stw1224.
Vancouver
1.
Clements D, Braglia F, Petitpas G, Greenslade J, Cooray A, Valiante E, et al. H-ATLAS : a candidate high redshift cluster/protocluster of star-forming galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2016;461(2):1719–33.
IEEE
[1]
D. Clements et al., “H-ATLAS : a candidate high redshift cluster/protocluster of star-forming galaxies,” MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol. 461, no. 2, pp. 1719–1733, 2016.
@article{8503163,
  abstract     = {{We investigate the region around the Planck-detected z = 3.26 gravitationally lensed galaxy HATLAS J114637.9-001132 (hereinafter HATLAS12-00) using both archival Herschel data from the H-ATLAS survey and using submm data obtained with both LABOCA and SCUBA2. The lensed source is found to be surrounded by a strong overdensity of both Herschel-SPIRE sources and submm sources. We detect 17 bright (S-870 > similar to 7 mJy) sources at >4 sigma closer than 5 arcmin to the lensed object at 850/870 mu m. 10 of these sources have good cross-identifications with objects detected by Herschel-SPIRE which have redder colours than other sources in the field, with 350 mu m flux > 250 mu m flux, suggesting that they lie at high redshift. Submillimeter Array (SMA) observations localise one of these companions to similar to 1 arcsec, allowing unambiguous cross identification with a 3.6 and 4.5 mu m Spitzer source. The optical/near-IR spectral energy distribution of this source is measured by further observations and found to be consistent with z > 2, but incompatible with lower redshifts. We conclude that this system may be a galaxy cluster/protocluster or larger scale structure that contains a number of galaxies undergoing starbursts at the same time.}},
  author       = {{Clements, DL and Braglia, F and Petitpas, G and Greenslade, J and Cooray, A and Valiante, E and De Zotti, G and O'Halloran, B and Holdship, J and Morris, B and Pérez-Fournon, I and Herranz, D and Riechers, D and Baes, Maarten and Bremer, M and Bourne, N and Dannerbauer, H and Dariush, A and Dunne, L and Eales, S and Fritz, Jacopo and Gonzalez-Nuevo, J and Hopwood, R and Ibar, E and Ivison, RJ and Leeuw, LL and Maddox, S and Michałowski, MJ and Negrello, M and Omont, A and Oteo, I and Serjeant, S and Valtchanov, I and Vieira, JD and Wardlow, J and van der Werf, P}},
  issn         = {{0035-8711}},
  journal      = {{MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY}},
  keywords     = {{galaxies: high redshift,galaxies: starburst,submillimetre: galaxies,SPECTRAL ENERGY-DISTRIBUTIONS,SCIENCE DEMONSTRATION PHASE,HERSCHEL-ATLAS,SUBMILLIMETER GALAXIES,MOLECULAR GAS,SOURCE EXTRACTION,DUSTY STARBURSTS,LENSED GALAXIES,PROTO-CLUSTER,DEEP FIELD}},
  language     = {{eng}},
  number       = {{2}},
  pages        = {{1719--1733}},
  title        = {{H-ATLAS : a candidate high redshift cluster/protocluster of star-forming galaxies}},
  url          = {{http://doi.org/10.1093/mnras/stw1224}},
  volume       = {{461}},
  year         = {{2016}},
}

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