Search Results for 'kev high'

kev high published presentations and documents on DocSlides.

keV HHG and Sub femtosecond K-shell excitation.

keV HHG and Sub femtosecond K-shell excitation.

by trish-goza

. ( . using IR (2.1. . m) Radiation Source. ...

The high mass accretion rate spectra of GX 339-4:

The high mass accretion rate spectra of GX 339-4:

by basidell

Black hole spin from reflection?. Mari Kolehmainen...

by myesha-ticknor

と. MAXI . で観測されている突発天体...

“X-ray Spectroscopy of the High-Mass X-ray Binary Pulsar

“X-ray Spectroscopy of the High-Mass X-ray Binary Pulsar

by marina-yarberry

Centaurus. X-3 Over its Binary Orbit”. -. Sach...

Improvement in scintillation

Improvement in scintillation

by sherrill-nordquist

counter. . energy. . resolution . with the . si...

Advance Gamma Tracking Array AGATA

Advance Gamma Tracking Array AGATA

by blondiental

Dino Bazzacco. INFN Padova. Part 1: Review of AGA...

High Resolution Spectroscopy in Nuclear Astrophysics

High Resolution Spectroscopy in Nuclear Astrophysics

by majerepr

Joachim Görres. University of Notre Dame & JI...

Accelerators in Homeland Security

Accelerators in Homeland Security

by eatfuzzy

William Bertozzi. Wilbur Franklin, Alexei Klimenko...

Filippo Frontera University of

Filippo Frontera University of

by alexa-scheidler

Ferrara. a. nd. INAF-IASF, Bologna. on . behalf o...

Collisional-Radiative Modeling of

Collisional-Radiative Modeling of

by karlyn-bohler

EBIT Spectra . of High-Z Ions . Yuri Ralchenko. N...

by tatyana-admore

a potentially background-free approach to the sea...

ATHENA: The Advanced Telescope for High Energy Astrophysics

ATHENA: The Advanced Telescope for High Energy Astrophysics

by celsa-spraggs

Nicholas E. White, NASA/GSFC. On behalf of the At...

by olivia-moreira

1.5 mm. 2 mm. 0.5 mm. 1.5 mm. ABSTRACT. Within. ...

X-ray Instruments for

X-ray Instruments for

by kittie-lecroy

MiniSatellites. High Resolution Spectroscopic Sur...

tandard lectrode Coaxial Ge Detectors SEGe Features Energy range from keV to MeV High resolution good peak shape Excellent timing resolution High energy rate capability Diode FET protection Warmup

tandard lectrode Coaxial Ge Detectors SEGe Features Energy range from keV to MeV High resolution good peak shape Excellent timing resolution High energy rate capability Diode FET protection Warmup

by jane-oiler

Regardless of the superlative used the detector i...

Status and Plans at LHD

Status and Plans at LHD

by trish-goza

. . Y. Takeiri. . for LHD Experiment Group. N...

APS Upgrade Brian Stephenson

APS Upgrade Brian Stephenson

by riley

Argonne National Lab. 7 December 2010. The APS Upg...

A New Proposal to the High Intensity Gamma-Ray Source (HI Sub-keV Nucl

A New Proposal to the High Intensity Gamma-Ray Source (HI Sub-keV Nucl

by giovanna-bartolotta

We propose to use the High Intensity Gamma-ray Sou...

Supernova Remnants in the ChASeM33 X-ray Survey of M33

Supernova Remnants in the ChASeM33 X-ray Survey of M33

by celsa-spraggs

Knox S. Long, William P. Blair, P. Frank Winkler,...

The Super-slow Pulsation X-ray Pulsars in High Mass X-ray

The Super-slow Pulsation X-ray Pulsars in High Mass X-ray

by phoebe-click

. Wei Wang. National Astronomical Observatories...

Solar flare hard X-ray spikes observed by

Solar flare hard X-ray spikes observed by

by tatiana-dople

RHESSI: a . statistical study. Jianxia. Cheng. ...

The REX-ISOLDE charge

The REX-ISOLDE charge

by trish-goza

state . breeder. Fredrik . Wenander. BE/ABP. ISO...

by karlyn-bohler

Studen. , . Karol . Brzezinski. , . Enrico. . Ch...

Measurement of formation cross-sections and

Measurement of formation cross-sections and

by marina-yarberry

decay properties for . short-lived isomers produc...

Development of a novel detector system for the

Development of a novel detector system for the

by luanne-stotts

keV. sterile neutrino search with KATRIN. Tobias...

PHY582 ― Particle Physics II (Experiment)

PHY582 ― Particle Physics II (Experiment)

by vamput

Lecture 8: Dark Matter detectors. Ar. á. n Garc. ...

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...

First Results of Deuterium Beam Operation on Neutral Beam Injectors in the Large Helical Device

First Results of Deuterium Beam Operation on Neutral Beam Injectors in the Large Helical Device

by gelbero

K. . Ikeda. 1). , . K. . . Tsumori. 1)2. ). , M. ....

High Energy Solar Flares

High Energy Solar Flares

by morton

-. What Fermi Adds to the Picture. Brian R. Dennis...

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 ...

Radio studies of mysterious Type

Radio studies of mysterious Type

by margaret

IIn. supernovae. Poonam Chandra. National Centre ...

Gamma Ray Attenuation Properties of Common

Gamma Ray Attenuation Properties of Common

by wilson

Shielding Materials Daniel R. McAlister , Ph.D. PG...

RadInspector Radioisotope Identification and Measurement

RadInspector Radioisotope Identification and Measurement

by desha

Aman. . Kataria. (EE), Johnny . Klarenbeek. (EE),...

2022-03-24 Development of high pixel density hard X-ray spectroscopic imagers for the direct imagin

2022-03-24 Development of high pixel density hard X-ray spectroscopic imagers for the direct imagin

by sylvia

keV. Elbereth. conference 2022. Hugo . Allaire. ,...

Terrestrial Gamma-ray

Terrestrial Gamma-ray

by gabriella

Flashes. Gamma Ray . Astronomy. . Beginning. star...