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Kev-Electron published presentations and documents on DocSlides.

RadInspector Radioisotope Identification and Measurement
RadInspector Radioisotope Identification and Measurement
by desha
Aman. . Kataria. (EE), Johnny . Klarenbeek. (EE),...
Investigation of a single plane Compton gamma camera as a radiation Imager
Investigation of a single plane Compton gamma camera as a radiation Imager
by isla
Om Prakash Dash*, Tomislav Bokulić, Damir Bosnar,...
Capillary Collimated XRF-imaging with
Capillary Collimated XRF-imaging with
by dorothy
Timepix. 3. Siwen . An. , David Krapohl, Börje N...
Status of the Astrosat
Status of the Astrosat
by madeline
mission. A R . Rao. Tata Institute of Fundamental ...
BINGO: B i- I sotope 0 ν
BINGO: B i- I sotope 0 ν
by delcy
2. β. . N. ext . G. eneration . O. bservatory. H...
Balraj Singh 50 years in Nuclear Science and Nuclear Data
Balraj Singh 50 years in Nuclear Science and Nuclear Data
by nicole
22nd Technical Meeting of the NSDD . Network, 22-2...
Image Reconstruction and Processing for Alpha Emitters
Image Reconstruction and Processing for Alpha Emitters
by skylar
Yong Du. Ph.D.. Department of Radiology, Johns Hop...
Radiation Protection 03.05.2017
Radiation Protection 03.05.2017
by genevieve
Lab coat → shields already approx. 80% of soft ...
RF Hobbs (Johns Hopkins University)
RF Hobbs (Johns Hopkins University)
by julia
Growth and Potential Isotope Needs in Medicine . ...
Gamma Ray Attenuation Properties of Common
Gamma Ray Attenuation Properties of Common
by wilson
Shielding Materials Daniel R. McAlister , Ph.D. PG...
Introduction to Bubble Chamber:
Introduction to Bubble Chamber:
by SkylineBabe
Ops Training. https://. wiki.jlab.org/ciswiki/inde...
PHYS389 : Semiconductor Applications
PHYS389 : Semiconductor Applications
by SimplySweet
L14. Lecture . 14: . Radiation detectors III. Germ...
eROSITA: Status & Scientific Prospects
eROSITA: Status & Scientific Prospects
by Dollface
t. o . extend the ROSAT all-sky survey up to . 10 ...
Radiation Protection in
Radiation Protection in
by LovableLatina
Laboratory. . work. Mats Isaksson, prof.. Departm...
Lively Accreting Black Holes in X-ray Binaries
Lively Accreting Black Holes in X-ray Binaries
by InLoveWithLife
Jeff McClintock. Harvard-Smithsonian Center for As...
Radio studies of mysterious Type
Radio studies of mysterious Type
by margaret
IIn. supernovae. Poonam Chandra. National Centre ...
Enhancement of Peak to Compton Ratio (P/C) using a New
Enhancement of Peak to Compton Ratio (P/C) using a New
by anastasia
Array. . Design for Safeguards . Applications. R....
Gd and Gd2O3 coatings as neutron converters
Gd and Gd2O3 coatings as neutron converters
by davies
Dorothea . Pfeiffer. 23. .09.2014. Content. 2. Ins...
AMEGO – A Wide Field Astrophysics Discovery Mission for the MeV Band
AMEGO – A Wide Field Astrophysics Discovery Mission for the MeV Band
by hanah
1. Julie . McEnery. (NASA/GSFC) on behalf of the ...
High Energy Solar Flares
High Energy Solar Flares
by morton
-. What Fermi Adds to the Picture. Brian R. Dennis...
When latest data differ from earlier ones: An example of
When latest data differ from earlier ones: An example of
by walsh
187. Hg. Shamsuzzoha. . Basunia. Lawrence Berkele...
57 Fe neutron inelastic scattering
57 Fe neutron inelastic scattering
by ida
The interplay between experiment and theory. . A....
DEPENDENCE OF THE MGA CODE PERFORMANCE ON DETECTOR ENERGY RESOLUTION C
DEPENDENCE OF THE MGA CODE PERFORMANCE ON DETECTOR ENERGY RESOLUTION C
by dandy
results during isotopic analysis Traditionally it ...
L Cosentino
L Cosentino
by helene
meeting EURISOL-NET CERN 28 June 2011L CosentinoIN...
BEGe projectBEGe project
BEGe projectBEGe project
by garcia
Results from detector operationsResults from detec...
Available
Available
by osullivan
performance 2013 Extended Performance (1) E ( Me...
Matthew Szydagis M. Szydagis, N
Matthew Szydagis M. Szydagis, N
by bikersnomercy
. Barry. , . K. . Kazkaz. , . J. Mock. , . D. . St...
The XENIA mission Cosmic chemical evolution of baryons
The XENIA mission Cosmic chemical evolution of baryons
by mjnt
. Luigi Piro. C. . Kouveliotou. , . J.W.. den . H...
Cooperation of Czech Republic and
Cooperation of Czech Republic and
by vamput
Laboratoire. . Soutterain. de . Modane. (LSM, F...
Alex Bogacz Optics for UITF
Alex Bogacz Optics for UITF
by fluental
-. ‘. keV. ’ and ‘MeV’ beam-lines. UITF M...
PHY582 ― Particle Physics II (Experiment)
PHY582 ― Particle Physics II (Experiment)
by vamput
Lecture 8: Dark Matter detectors. Ar. á. n Garc. ...
Direct Dark Matter (WIMPs) Searches and the XMASS Experiment
Direct Dark Matter (WIMPs) Searches and the XMASS Experiment
by envrrolex
S. earches and the XMASS Experiment. Y. Suzuki. Ka...
AX-PET Demonstrator 11 th
AX-PET Demonstrator 11 th
by welnews
ICATPP . 5-9 Oct, 2009, COMO, 2009. W. . Lusterman...
Colliding the Highest Brilliance Photon beam with the Highest Luminosity Hadron beam
Colliding the Highest Brilliance Photon beam with the Highest Luminosity Hadron beam
by onionchevrolet
⇒ phase space density (small emittance) vs. low ...
The XENIA mission Cosmic chemical evolution of baryons
The XENIA mission Cosmic chemical evolution of baryons
by titechas
. Dieter. H. . Hartmann. C. Kouveliotou, . M. . C...
β - decay, Collectivity and Shell Structure Evolution Around N=50:
β - decay, Collectivity and Shell Structure Evolution Around N=50:
by bagony
a Common Physics ?. Andrea Gottardo. OUTLINE. The ...
Searches for the Majorana neutrino in GERDA
Searches for the Majorana neutrino in GERDA
by slayrboot
Krzysztof Panas. Institute of Physics, . Jagiellon...
Proposer: Alex Obertelli, TU Darmstadt
Proposer: Alex Obertelli, TU Darmstadt
by shoffer
Review for the SPSC by Mike Tarbutt and Gerda Neye...
IS530: Properties of low-lying intruder states in
IS530: Properties of low-lying intruder states in
by syfarect
34. Al and . 34. Si. sequentially populated in bet...
Addendum to Proposal P-242 to the INTC
Addendum to Proposal P-242 to the INTC
by blackwidownissan
SEARCH FOR NEW CANDIDATES . FOR . THE NEUTRINO-ORI...