131 research outputs found
Playing Tag with ANN: Boosted Top Identification with Pattern Recognition
Many searches for physics beyond the Standard Model at the Large Hadron
Collider (LHC) rely on top tagging algorithms, which discriminate between
boosted hadronic top quarks and the much more common jets initiated by light
quarks and gluons. We note that the hadronic calorimeter (HCAL) effectively
takes a "digital image" of each jet, with pixel intensities given by energy
deposits in individual HCAL cells. Viewed in this way, top tagging becomes a
canonical pattern recognition problem. With this motivation, we present a novel
top tagging algorithm based on an Artificial Neural Network (ANN), one of the
most popular approaches to pattern recognition. The ANN is trained on a large
sample of boosted tops and light quark/gluon jets, and is then applied to
independent test samples. The ANN tagger demonstrated excellent performance in
a Monte Carlo study: for example, for jets with p_T in the 1100-1200 GeV range,
60% top-tag efficiency can be achieved with a 4% mis-tag rate. We discuss the
physical features of the jets identified by the ANN tagger as the most
important for classification, as well as correlations between the ANN tagger
and some of the familiar top-tagging observables and algorithms.Comment: 20 pages, 9 figure
Remote sensing research for development at IDRC
Meeting: International Symposium on Remote Sensing of Environment, 20-26 Oct. 1988, Abidjan, C
Local entanglement generation in the adiabatic regime
We study entanglement generation in a pair of qubits interacting with an
initially correlated system. Using time independent perturbation theory and the
adiabatic theorem, we show conditions under which the qubits become entangled
as the joint system evolves into the ground state of the interacting theory. We
then apply these results to the case of qubits interacting with a scalar
quantum field. We study three different variations of this setup; a quantum
field subject to Dirichlet boundary conditions, a quantum field interacting
with a classical potential and a quantum field that starts in a thermal state.Comment: 9 pages, 6 figures. v2: reference [14] adde
International cooperation in remote sensing : how can a project become a success?
Meeting: International Symposium on Remote Sensing of the Environment, 23d, 17-26 Apr. 1990, Bangkok, THIncludes abstract in FrenchPhotocop
Approche du CRDI dans la lutte contre la désertification en Afrique et l'apport de son programme en cartographie et télédétection
Réunion: Deuxièmes journées scientifiques du réseau thématique de l'UREF : télédétection, 21-24 nov. 1989, SNPhotocopi
New Shortwave Infrared Albedo Measurements for Snow Specific Surface Area Retrieval
Snow grain-size characterization, its vertical and temporal evolution is a key parameter for the improvement and validation of snow and radiative transfer models (optical and microwave) as well as for remote-sensing retrieval methods. We describe two optical methods, one active and one passive shortwave infrared, for field determination of the specific surface area (SSA) of snow grains. We present a new shortwave infrared (SWIR) camera approach. This new method is compared with a SWIR laser- based system measuring snow albedo with an integrating sphere (InfraRed Integrating Sphere (IRIS)). Good accuracy (10%) and reproducibility in SSA measurements are obtained using the IRIS system on snow samples having densities greater than 200 kg m-3, validated against X-ray microtomography measurements. The SWIRcam approach shows improved sensitivity to snow SSA when compared to a near-infrared camera, giving a better contrast of the snow stratigraphy in a snow pit
SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope
We describe the design of a new polarization sensitive receiver, SPT-3G, for
the 10-meter South Pole Telescope (SPT). The SPT-3G receiver will deliver a
factor of ~20 improvement in mapping speed over the current receiver, SPTpol.
The sensitivity of the SPT-3G receiver will enable the advance from statistical
detection of B-mode polarization anisotropy power to high signal-to-noise
measurements of the individual modes, i.e., maps. This will lead to precise
(~0.06 eV) constraints on the sum of neutrino masses with the potential to
directly address the neutrino mass hierarchy. It will allow a separation of the
lensing and inflationary B-mode power spectra, improving constraints on the
amplitude and shape of the primordial signal, either through SPT-3G data alone
or in combination with BICEP-2/KECK, which is observing the same area of sky.
The measurement of small-scale temperature anisotropy will provide new
constraints on the epoch of reionization. Additional science from the SPT-3G
survey will be significantly enhanced by the synergy with the ongoing optical
Dark Energy Survey (DES), including: a 1% constraint on the bias of optical
tracers of large-scale structure, a measurement of the differential Doppler
signal from pairs of galaxy clusters that will test General Relativity on ~200
Mpc scales, and improved cosmological constraints from the abundance of
clusters of galaxies.Comment: 21 pages, 9 figures. To be published in Proceedings of SPIE Volume
9153. Presented at SPIE Astronomical Telescopes + Instrumentation 2014,
conference 915
Design and Bolometer Characterization of the SPT-3G First-year Focal Plane
During the austral summer of 2016-17, the third-generation camera, SPT-3G,
was installed on the South Pole Telescope, increasing the detector count in the
focal plane by an order of magnitude relative to the previous generation.
Designed to map the polarization of the cosmic microwave background, SPT-3G
contains ten 6-in-hexagonal modules of detectors, each with 269 trichroic and
dual-polarization pixels, read out using 68x frequency-domain multiplexing.
Here we discuss design, assembly, and layout of the modules, as well as early
performance characterization of the first-year array, including yield and
detector properties.Comment: Conference proceeding for Low Temperature Detectors 2017. Accepted
for publication: 27 August 201
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