Nuclear Instruments and Methods

By J. Salgado. 2003

730 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/c04d16a228b36874c5a36dd922e787573e3552d6

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Citations in the corpus

• X-Ray Imaging Spectrometer (XIS) on Board Suzaku (2007, methodology): “Details of the spectrometer system are described in Hashimotodani et al. (1998). In the high energy range, fluorescent X-rays from six materials (Al, Cl, Ti, Fe, Zn, and Se), and the radio isotope ((55)Fe) were used.”
• The LUVOIR Mission Concept Study Final Report (2019, background): “Most stars in the Galaxy, including our own, formed in rich clusters (e.g., Lada & Lada 2003; Adams 2010) that contain massive stars whose high-energy UV and X-ray photons contribute to disperse planet-forming material around young stars (e.”
• The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux (2016, methodology): “by past diffuse neutrino flux measurements (Abbasi et al. 2011; Aartsen et al. 2014a), for example the combined pp+pγ predictions in Mannheim (1995). More recent publications, on the other hand, differentiate between specific classes of blazars and are largely not constrained by experiment, yet. The”
• A side-by-side comparison of Daya Bay antineutrino detectors (2012, methodology): “All Gd-LS [7] and LS was produced in the LS Hall [8].”
• The gas electron multiplier (GEM): Operating principles and applications (2016, background): “Due to the large gas gain and the very low electrode capacitance, these devices have the potential to detect and image single ionization electrons, reaching the ultimate tracking precision of a gaseous counter [100,150].”
• THE INTERNAL-COLLISION-INDUCED MAGNETIC RECONNECTION AND TURBULENCE (ICMART) MODEL OF GAMMA-RAY BURSTS (2010, background): “At the extreme, even the outflow consists of cold (pressureless) matter accelerated exclusively by the magnetic field, the achievable σ is at most σc (Michel 1969).”
• Measurement of the Crab Nebula Spectrum Past 100 TeV with HAWC (2019, methodology): “As described in Abeysekara et al. (2017), the background estimate from direct integration is smoothed by an additional 0.”
• Milky Way Satellite Census. I. The Observational Selection Function for Milky Way Satellites in DES Y3 and Pan-STARRS DR1 (2019, methodology): “(deg) (deg) (′) (kpc) (pc) (mag) Horologium I DES 4 43.8813 -54.116 19.5 1.59 0.27 79 31 -3.55 3 Horologium II DES 3 49.1077 -50.0486 19.5 2.09 0.52 78 33 -2.6 15 Hydra II 3 185.4251 -31.9860 20.9 1.52 0.24 151 58 -4.60 3 Hydrus I 4 37.389 -79.3089 17.2 7.42 0.21 28 53 -4.71 16 Indus II DES 1 309.72”
• Electric dipole moments of atoms, molecules, nuclei, and particles (2017, background): “A quantitative test of light-shifts has been undertaken by Patton et al. (2014). The walls of the evacuated alkali metal vapor cells”
• Radioactive decays at limits of nuclear stability (2011, background): “The phase space factor can be approximated roughly by f = (1 +Q/mec2)5/30 in terms of the decay energy (Q-value) for β±-decays, more accurate determinations can be found through (Behrens and Büring, 1982; Wilkinson, 1995).”
• Angle-resolved photoemission studies of quantum materials (2020, unknown): “The hemispherical analyzer has been the workhorse of the ARPES community for the past two decades (FellnerFeldegg et al., 1974; Wannberg, 2009), as it is highly versatile (compatible with both pulsed and continuous radiation, at energies from eV to keV) and offers high angle and energy resolutions…”