Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Gravitational Lens Models Based on Submillimeter Array Imaging of
  Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z>1.5   Strong gravitational lenses are now being routinely discovered in wide-field
surveys at (sub)millimeter wavelengths. We present Submillimeter Array (SMA)
high-spatial resolution imaging and Gemini-South and Multiple Mirror Telescope
optical spectroscopy of strong lens candidates discovered in the two widest
extragalactic surveys conducted by the Herschel Space Observatory: the
Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) and the Herschel
Multi-tiered Extragalactic Survey (HerMES). From a sample of 30 Herschel
sources with S_500>100 mJy, 21 are strongly lensed (multiply imaged), 4 are
moderately lensed (singly imaged), and the remainder require additional data to
determine their lensing status. We apply a visibility-plane lens modeling
technique to the SMA data to recover information about the masses of the lenses
as well as the intrinsic (i.e., unlensed) sizes (r_half) and far-infrared
luminosities (L_FIR) of the lensed submillimeter galaxies (SMGs). The sample of
lenses comprises primarily isolated massive galaxies, but includes some groups
and clusters as well. Several of the lenses are located at z_lens>0.7, a
redshift regime that is inaccessible to lens searches based on Sloan Digital
Sky Survey spectroscopy. The lensed SMGs are amplified by factors that are
significantly below statistical model predictions given the 500um flux
densities of our sample. We speculate that this may reflect a deficiency in our
understanding of the intrinsic sizes and luminosities of the brightest SMGs.
The lensed SMGs span nearly one decade in L_FIR (median L_FIR=7.9x10^12 L_sun)
and two decades in FIR luminosity surface density (median Sigma_FIR=6.0x10^11
L_sun kpc^-2). The strong lenses in this sample and others identified via
(sub-)mm surveys will provide a wealth of information regarding the
astrophysics of galaxy formation and evolution over a wide range in redshift.

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The categories of this paper are: acc-phys
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The categories of this paper are: patt-sol
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The categories of this paper are: hep-ex
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The categories of this paper are: gr-qc
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The categories of this paper are: stat
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The categories of this paper are: math-ph
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The categories of this paper are: quant-ph
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The categories of this paper are: hep-th
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The categories of this paper are: q-alg
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The categories of this paper are: atom-ph
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The categories of this paper are: cs
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The categories of this paper are: chem-ph
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The categories of this paper are: q-fin
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The categories of this paper are: eess
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The categories of this paper are: supr-con
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The categories of this paper are: q-bio