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  • Image# FN0416
  • FN
  • 05/08/2013

The Muon g-2 storage ring, in its current location at Brookhaven National Laboratory in New York. The ring, which will capture muons in a magnetic field, must be transported in one piece, and moved flat to avoid undue pressure on the superconducting cable inside. (Courtesy: Brookhaven National Laboratory)

  • Image# FN0413
  • FN
  • 05/02/2013

Image of one of the first bubbles seen in the COUPP-60 detector, located half a mile underground at SNOLAB in Ontario, Canada. The bubble appears as a black semi-circle on the lower left-hand side of the image. The white ovals in the center are reflections of LED lights. (Courtesy: SNOLAB)

  • Image# FN0414
  • FN
  • 05/02/2013

The COUPP-60 detector installed at the SNOLAB underground laboratory in Ontario, Canada. (Courtesy: SNOLAB)

  • Image# FN0415
  • FN
  • 05/02/2013

Scientists install the COUPP-60 detector a mile and a half underground at SNOLAB in Ontario, Canada. (Courtesy: Fermilab)

  • Image# FN0408
  • FN
  • 03/28/2013

When completed, the NOvA detector will comprise 28 detector blocks, each measuring about 50 feet tall, 50 feet wide and 6 feet deep. (Courtesy: Fermilab)

  • Image# FN0409
  • FN
  • 03/28/2013

Electronics that make up part of the data acquisition system are installed on the top and side of the detector. The NOvA experiment is a collaboration of 169 scientists from 19 universities and laboratories in the U.S and another 15 institutions around the world. The scientists are funded by the U.S. Department of Energy, the National Science Foundation and funding agencies in the Czech Republic, Greece, India, Russia and the United Kingdom. (Courtesy: Fermilab)

  • Image# FN0410
  • FN
  • 03/28/2013

Scientists and engineers at Fermi National Accelerator Laboratory developed the 750,000-pound pivoter machine that will put the blocks of the NOvA detector in place. (Courtesy: Fermilab)

  • Image# FN0411
  • FN
  • 03/28/2013

Technicians glue modules for the NOvA detector using a machine developed at Argonne National Laboratory. (Courtesy: William Miller, NOvA installation manager)

  • Image# FN0412
  • FN
  • 03/28/2013

This 3D image shows a cosmic-ray muon producing a large shower of energy as it passes through the NOvA far detector in Minnesota. (Courtesy: NOvA collaboration)

  • Image# CE0337
  • CE
  • 03/16/2013

Presentation of Large Hadron Collider (LHC) latest results at Moriond/QCD conference, Mar. 9-16, 2013 at La Thuile, Italy (Courtesy: CERN)

  • Image# CE0339
  • CE
  • 03/16/2013

Presentation of Large Hadron Collider (LHC) latest results at Moriond/QCD conference, Mar. 9-16, 2013 at La Thuile, Italy (Courtesy: CERN)

  • Image# CE0335
  • CE
  • 02/14/2013

LHC consolidations 2013-14 (Courtesy: CERN)

  • Image# SL0102
  • SL
  • 02/14/2013

When stars explode, the supernovas send off shock waves like the one shown in this artist's rendition, which accelerate protons to cosmic-ray energies through a process known as Fermi acceleration. (Credit: Greg Stewart / SLAC National Accelerator Laboratory)

  • Image# LB0054
  • LB
  • 08/07/2012

BOSS is capturing accurate spectra for millions of astronomical objects by using 2,000 plug plates that are placed at the Sloan Foundation Telescope's focal plane. Each of the 1,000 holes drilled in a single plug plate captures the light from a specific galaxy, quasar, or other target, and conveys its light to a sensitive spectrograph through an optical fiber. The plates are marked to indicate which holes belong to which bundles of the thousand optical fibers that carry the object's light. (Courtesy: Berkeley Lab)

  • Image# BN0045
  • BN
  • 07/19/2012

RHIC's two large experiments, STAR and PHENIX, have multiple detector components and complex electronics for tracking and identifying the particles that fly out after ions collide at nearly the speed of light. (Courtesy: BNL)

  • Image# BN0046
  • BN
  • 07/19/2012

The nuclear phase diagram: RHIC sits in the energy "sweet spot" for exploring the transition between ordinary matter made of hadrons and the early universe matter known as quark-gluon plasma. Courtesy: BNL)

  • Image# GN0017
  • GS
  • 07/18/2012

XENON100 (Courtesy: XENON Collaboration)

  • Image# CE0303
  • CE
  • 07/04/2012

Rolf Heuer at CERN Higgs Boson search update (Courtesy: Maximilien Brice, Laurent Egli)

  • Image# CE0302
  • CE
  • 07/04/2012

Higgs Boson search update - 4 July 2012 (Courtesy: Maximilien Brice, Laurent Egli)

  • Image# CE0305
  • CE
  • 07/04/2012

Joe Incandela, CERN spokesperson for Higgs Boson search update (Courtesy: Maximilien Brice, Laurent Egli)

  • Image# CE0306
  • CE
  • 07/04/2012

John Ellis, Higgs Boson search update at CERN (Courtesy: Maximilien Brice, Laurent Egli)

  • Image# CE0307
  • CE
  • 07/04/2012

Fabiola Gianotti, ATLAS experiment spokesperson, at Higgs Boson search update at CERN (Courtesy: Maximilien Brice, Laurent Egli)

  • Image# CE0308
  • CE
  • 07/04/2012

Peter Higgs, Higgs Boson search update at CERN (Courtesy: Maximilien Brice, Laurent Egli)

  • Image# CE0309
  • CE
  • 07/04/2012

A proton-proton collision event in the CMS experiment producing two high-energy photons (red towers). This is what we would expect to see from the decay of a Higgs boson but it is also consistent with background Standard Model physics processes. (Courtesy: CERN)

  • Image# CE0310
  • CE
  • 07/04/2012

Francois Englert, Higgs Boson search update at CERN (Courtesy: Maximilien Brice, Laurent Egli)

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