The Red Radio Ring: a gravitationally lensed hyperluminous infrared radio galaxy at z=2.553 discovered through citizen science
J. E. Geach (Hertfordshire), A. More, A. Verma, P. J. Marshall, N., Jackson, P.-E. Belles, R. Beswick, E. Baeten, M. Chavez, C. Cornen, B. E., Cox, T. Erben, N. J. Erickson, S. Garrington, P. A. Harrison, K. Harrington,, D. H. Hughes, R. J. Ivison, C. Jordan, Y.-T. Lin

TL;DR
This paper reports the discovery of a gravitationally lensed hyperluminous infrared galaxy at z=2.553, identified through citizen science, with detailed multi-wavelength observations revealing its structure and lensing properties.
Contribution
It presents the first identification of such a galaxy via citizen science and provides detailed imaging and lens modeling of its structure and magnification.
Findings
Discovered a hyperluminous infrared galaxy with strong radio emission at z=2.553.
Resolved radio morphology shows a compact core and extended components.
Lens modeling indicates a magnification factor of approximately 10x.
Abstract
We report the discovery of a gravitationally lensed hyperluminous infrared galaxy (L_IR~10^13 L_sun) with strong radio emission (L_1.4GHz~10^25 W/Hz) at z=2.553. The source was identified in the citizen science project SpaceWarps through the visual inspection of tens of thousands of iJKs colour composite images of Luminous Red Galaxies (LRGs), groups and clusters of galaxies and quasars. Appearing as a partial Einstein ring (r_e~3") around an LRG at z=0.2, the galaxy is extremely bright in the sub-millimetre for a cosmological source, with the thermal dust emission approaching 1 Jy at peak. The redshift of the lensed galaxy is determined through the detection of the CO(3-2) molecular emission line with the Large Millimetre Telescope's Redshift Search Receiver and through [OIII] and H-alpha line detections in the near-infrared from Subaru/IRCS. We have resolved the radio emission with…
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