The Herschel-ATLAS: a sample of 500 μm-selected lensed galaxies over 600 deg2

Negrello, M.; Amber, S.; Amvrosiadis, A.; Cai, Z.-Y.; Lapi, A.; Gonzalez-Nuevo, J.; De Zotti, G.; Furlanetto, C.; Maddox, S. J.; Allen, M.; Bakx, T.; Bussmann, R. S.; Cooray, A.; Covone, G.; Danese, L.; Dannerbauer, H.; Fu, H.; Greenslade, J.; Gurwell, M.; Hopwood, R.; Koopmans, L. V. E.; Napolitano, N.; Nayyeri, H.; Omont, A.; Petrillo, C. E.; Riechers, D. A.; Serjeant, S.; Tortora, C.; Valiante, E.; Verdoes Kleijn, G.; Vernardos, G.; Wardlow, J. L.; Baes, M.; Baker, A. J.; Bourne, N.; Clements, D.; Crawford, S. M.; Dye, S.; Dunne, L.; Eales, S.; Ivison, R. J.; Marchetti, L.; Michałowski, M. J.; Smith, M. W. L.; Vaccari, M. and van der Werf, P. (2016). The Herschel-ATLAS: a sample of 500 μm-selected lensed galaxies over 600 deg2. Monthly Notices of the Royal Astronomical Society, 465(3) pp. 3558–3580.

DOI: https://doi.org/10.1093/mnras/stw2911

Abstract

We present a sample of 80 candidate strongly lensed galaxies with flux density above 100mJy at 500{\mu}m extracted from the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), over an area of 600 square degrees. Available imaging and spectroscopic data allow us to confirm the strong lensing in 20 cases and to reject it in one case. For other 8 objects the lensing scenario is strongly supported by the presence of two sources along the same line of sight with distinct photometric redshifts. The remaining objects await more follow-up observations to confirm their nature. The lenses and the background sources have median redshifts z_L = 0.6 and z_S = 2.5, respectively, and are observed out to z_L = 1.2 and z_S = 4.2. We measure the number counts of candidate lensed galaxies at 500{\mu}m and compare them with theoretical predictions, finding a good agreement for a maximum magnification of the background sources in the range 10-20. These values are consistent with the magnification factors derived from the lens modelling of individual systems. The catalogue presented here provides sub- mm bright targets for follow-up observations aimed at exploiting gravitational lensing to study with un-precedented details the morphological and dynamical properties of dusty star forming regions in z >~ 1.5 galaxies.

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