The Detection of a Population of Submillimeter-Bright, Strongly-Lensed Galaxies

Abstract

Gravitational lensing is a powerful astrophysical and cosmological probe and is particularly valuable at submillimeter wavelengths for the study of the statistical and individual properties of dusty starforming galaxies. However the identification of gravitational lenses is often time-intensive, involving the sifting of large volumes of imaging or spectroscopic data to find few candidates. We used early data from the Herschel Astrophysical Terahertz Large Area Survey to demonstrate that wide-area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficiency.

arXiv commentThis is the author's version of the work. It is posted here by permission of the AAAS for personal use, not for redistribution. The definitive version was published in Science VOL 330, (Nov 5th, 2010), doi:10.1126/science.1193420

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• DESHIMA 2.0: Rapid redshift surveys and multi-line spectroscopy of dusty galaxies
• Milky Way-Like Gas Excitation in an Ultrabright Submillimeter Galaxy at $z=1.6$
• Extremely-bright submillimeter galaxies beyond the Lupus-I star-forming region
• Deep Submillimetre and Radio Observations in the SSA22 Field. II. Sub-millimetre source catalogue and number counts
• Probing General Relativity in galactic scales at z $\sim 0.3$
• PRUSSIC III -- ALMA and NOEMA survey of dense gas in high-redshift star-forming galaxies
• Interpreting the statistical properties of high-z extragalactic sources detected by the South Pole Telescope survey
• On rates of supernovae strongly lensed by galactic haloes in Millennium Simulation
• Detection of an ultra-bright submillimeter galaxy behind the Small Magellanic Cloud
• A Massive Molecular Gas Reservoir in the z=2.221 Type-2 Quasar Host Galaxy SMM J0939+8315 Lensed by the Radio Galaxy 3C220.3
• Predictions for surveys with the SPICA Mid-infrared Instrument
• The Einstein ring GAL-CLUS-022058s: a Lensed Ultrabright Submillimeter Galaxy at z=1.4796
• Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6
• Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy at z~3.3
• Multifrequency filter search for high redshift sources and lensing systems in Herschel-ATLAS
• Panchromatic radiation from galaxies as a probe of galaxy formation and evolution
• Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
• Multi-wavelength probes of distant lensed galaxies
• An upper limit to differential magnification effects in strongly gravitationally lensed galaxies
• The molecular-gas properties in the gravitationally lensed merger HATLAS J142935.3-002836
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• Cosmic Insights from Galaxy Clusters: Exploring Magnification Bias on Sub-millimeter Galaxies
• Resolved Neutral Outflow from a Lensed Dusty Star Forming Galaxy at z=2.09
• HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo
• Molecular gas in galaxies at all redshifts
• The ViSta method for stacking in the Fourier domain and its application to the dusty star-forming galaxies in the ALMA Science Archive
• Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration
• Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey
• The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at $z\sim 2$
• The Nature of Hyperluminous Infrared Galaxies