A detailed gravitational lens model based on Submillimeter Array and Keck adaptive optics imaging of a Herschel-atlas submillimeter galaxy at z = 4.243
Astrophysical Journal 756:2 (2012)
Abstract:
We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 μm and the Keck adaptive optics (AO) system at the K S-band of a gravitationally lensed submillimeter galaxy (SMG) at z = 4.243 discovered in the Herschel Astrophysical Terahertz Large Area Survey. The SMA data (angular resolution 06) resolve the dust emission into multiple lensed images, while the Keck AO K S-band data (angular resolution 01) resolve the lens into a pair of galaxies separated by 03. We present an optical spectrum of the foreground lens obtained with the Gemini-South telescope that provides a lens redshift of z lens = 0.595 ± 0.005. We develop and apply a new lens modeling technique in the visibility plane that shows that the SMG is magnified by a factor of μ = 4.1 ± 0.2 and has an intrinsic infrared (IR) luminosity of L IR = (2.1 ± 0.2) × 1013 L ⊙. We measure a half-light radius of the background source of r s = 4.4 ± 0.5kpc which implies an IR luminosity surface density of ΣIR = (3.4 ± 0.9) × 1011 L ⊙kpc-2, a value that is typical of z > 2 SMGs but significantly lower than IR luminous galaxies at z 0. The two lens galaxies are compact (r lens 0.9kpc) early-types with Einstein radii of θE1 = 0.57 ± 0.01 and θE2 = 0.40 ± 0.01 that imply masses of M lens1 = (7.4 ± 0.5) × 1010 M ⊙ and M lens2 = (3.7 ± 0.3) × 10 10 M ⊙. The two lensing galaxies are likely about to undergo a dissipationless merger, and the mass and size of the resultant system should be similar to other early-type galaxies at z 0.6. This work highlights the importance of high spatial resolution imaging in developing models of strongly lensed galaxies discovered by Herschel. © 2012. The American Astronomical Society. All rights reserved.SN 2010ay IS A LUMINOUS AND BROAD-LINED TYPE Ic SUPERNOVA WITHIN A LOW-METALLICITY HOST GALAXY
The Astrophysical Journal American Astronomical Society 756:2 (2012) 184
Search for the Standard Model Higgs Boson Decaying to a bb̄ Pair in Events with One Charged Lepton and Large Missing Transverse Energy Using the Full CDF Data Set
Physical Review Letters 109:11 (2012)
Abstract:
We present a search for the standard model Higgs boson produced in association with a W boson in √s=1.96TeV pp̄ collision data collected with the CDFA II detector at the Tevatron corresponding to an integrated luminosity of 9.45fb-1. In events consistent with the decay of the Higgs boson to a bottom-quark pair and the W boson to an electron or muon and a neutrino, we set 95% credibility level upper limits on the WH production cross section times the H→bb̄ branching ratio as a function of Higgs boson mass. At a Higgs boson mass of 125GeV/c2, we observe (expect) a limit of 4.9 (2.8) times the standard model value. © 2012 American Physical Society.Search for the standard model higgs boson decaying to a bb̄ pair in events with two oppositely charged leptons using the full CDF data set
Physical Review Letters 109:11 (2012)
Abstract:
We present a search for the standard model Higgs boson produced in association with a Z boson in data collected with the CDF II detector at the Tevatron, corresponding to an integrated luminosity of 9.45fb-1. In events consistent with the decay of the Higgs boson to a bottom-quark pair and the Z boson to electron or muon pairs, we set 95% credibility level upper limits on the ZH production cross section times the H→bb̄ branching ratio as a function of Higgs boson mass. At a Higgs boson mass of 125GeV/c2, we observe (expect) a limit of 7.1 (3.9) times the standard model value. © 2012 American Physical Society.Search for the standard model Higgs boson decaying to a bb̄ pair in events with no charged leptons and large missing transverse energy using the full CDF data set
Physical Review Letters 109:11 (2012)